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CHEMISTRY NOTEBOOK

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Honors Chemistry<br />

Class Policies and Grading<br />

The students will receive a Unit Outline at the beginning of each Unit. It will<br />

have information about the assignments that they will do, what it’s grade<br />

classification will be, what action they will need to do to complete the<br />

assignment and when it is due.<br />

The students will receive a Weekly Memo of the activities they will be<br />

responsible for that week. It will serve to inform the students of the learning<br />

goal for the week. It will also give the students any special information<br />

about that week.<br />

The students will also receive daily lectures and assignments that are<br />

designed to teach and re-enforce information related to the learning goal.<br />

This will be time in which new material will be taught and reviewed and will<br />

give the students the opportunity to ask questions regarding the concepts<br />

being taught.<br />

The students will work with a Lab partner and also be in a Lab group, but it<br />

will be up to the individual student to do his or her part of all assignments<br />

and the individual student will ultimately be responsible for all information<br />

presented in the class.<br />

The students will be required to follow all District and School Policies and to<br />

follow all Lab Safety Procedures, which they will be given and will sign,<br />

while performing labs. Students should come to class on time and with the<br />

supplies needed for that class.<br />

The following grading policy will be used.<br />

Percent of Final Grade<br />

Notebook 40%<br />

Test/Projects 30%<br />

Labs/Quizzes 20%<br />

Work 10%<br />

The students will be given a teacher generated Mid Term and a District<br />

Final.<br />

0


Unit 1<br />

Measurement Lab<br />

Separation of Mixtures Lab with Lab Write Up<br />

Unit 2<br />

Flame Test Lab<br />

Nuclear Decay Lab<br />

Element Marketing Project<br />

Unit 3<br />

Golden Penny Lab with Lab Write Up<br />

Molecular Geometry<br />

Research Presentation on a Chemical<br />

Mid Term<br />

Unit 4<br />

Double Displacement Lab<br />

Stoichiometry Lab with Lab Write Up<br />

Mole Educational Demonstration Project<br />

Unit 5<br />

Gas Laws Lab with Lab Write Up<br />

States of Matter Lab<br />

Teach a Gas Law Project<br />

Unit 6<br />

Dilutions Lab<br />

Titration Lab<br />

District Final<br />

1


Unit 1 (22 days)<br />

Chapter 1 Introduction to Chemistry<br />

Honors Chemistry<br />

2016/2017 Syllabus<br />

3 days<br />

1.1 The Scope of Chemistry 1.3 Thinking Like a Scientist<br />

1.2 Chemistry and You 1.4 Problem Solving in Chemistry<br />

Chapter 2 Matter and Change<br />

2.1 Properties of Matter 2.3 Elements and Compounds<br />

2.2 Mixtures 2.4 Chemical Reactions<br />

Chapter 3 Scientific Measurement<br />

9 days<br />

10 days<br />

3.1 Using and Expressing Measurements 3.3 Solving Conversion Problems<br />

3.2 Units of Measurement<br />

Unit 2 (15 days)<br />

Chapter 4 Atomic Structure<br />

5 days<br />

4.1 Defining the Atom 4.3 Distinguishing Among Atoms<br />

4.2 Structure of the Nuclear Atom<br />

Chapter 5 Electrons in Atoms<br />

5 days<br />

5.1 Revising the Atomic Model 5.2 Electron Arrangement in Atoms<br />

5.3 Atomic Emission Spectrum and the Quantum Mechanical Model<br />

Chapter 6 The Periodic Table<br />

6.1 Organizing the Elements 6.3 Periodic Trends<br />

6.2 Classifying Elements<br />

Unit 3 (22 days)<br />

Chapter 25 Nuclear Chemistry<br />

25.1 Nuclear Radiation 25.3 Fission and Fusion<br />

25.2 Nuclear Transformations 25.4 Radiation in Your Life<br />

Chapter 7 Ionic and Metallic Bonding<br />

7.1 Ions 7.3 Bonding in Metals<br />

7.2 Ionic Bonds and Ionic Compounds<br />

Chapter 8 Covalent Bonding<br />

5 days<br />

6 days<br />

8 days<br />

8 days<br />

8.1 Molecular Compounds 8.3 Bonding Theories<br />

8.2 The Nature of Covalent Bonding 8.4 Polar Bonds and Molecules<br />

Unit 4 (14 days)<br />

Chapter 9 Chemical Names and Formulas<br />

6 days<br />

9.1 Naming Ions 9.3 Naming & Writing Formulas Molecular Compounds<br />

9.2 Naming and Writing Formulas for Ionic Compounds 9.4 Names for Acids and Bases<br />

Chapter 22 Hydrocarbons Compounds<br />

22.1 Hydrocarbons 22.4 Hydrocarbon Rings<br />

Chapter 23 Functional Groups<br />

4 days<br />

4 days<br />

23.1 Introduction to Functional Groups 23.4 Alcohols, Ethers, and Amines<br />

2


Unit 5 (28 days)<br />

Chapter 10 Chemical Quantities 8 days<br />

10.1 The Mole: A Measurement of Matter 10.3 % Composition & Chem. Formulas<br />

10.2 Mole-Mass and Mole-Volume Relationships<br />

Chapter 11 Chemical Reactions 8 days<br />

11.1 Describing Chemical Reactions 11.3 Reactions in Aqueous Solutions<br />

11.2 Types of Chemical Reactions<br />

Chapter 12 Stoichiometry 12 days<br />

12.1 The Arithmetic of Equations 12.3 Limiting Reagent and % Yield<br />

12.2 Chemical Calculations<br />

Unit 6 (22 days)<br />

Chapter 13 States of Matter 6 days<br />

13.1 The Nature of Gases 13.3 The Nature of Solids<br />

13.2 The Nature of Liquids 13.4 Changes in State<br />

Chapter 14 The Behavior of Gases 10 days<br />

14.1 Properties of Gases 14.3 Ideal Gases<br />

14.2 The Gas Laws 14.4 Gases: Mixtures and Movement<br />

Chapter 15 Water and Aqueous Systems 6 days<br />

15.1 Water and its Properties 15.3 Heterogeneous Aqueous Systems<br />

15.2 Homogeneous Aqueous Systems<br />

Unit 7 (18 days)<br />

Chapter 16 Solutions 8 days<br />

16.1 Properties of Solutions 16.3 Colligative Properties of Solutions<br />

16.2 Concentrations of Solutions 16.4 Calc. Involving Colligative Property<br />

Chapter 17 Thermochemistry 5 days<br />

17.1 The Flow of Energy 17.3 Heat in Changes of State<br />

17.2 Measuring and Expressing Enthalpy Change 17.4 Calculating Heats in Reactions<br />

Chapter 18 Reaction Rates and Equilibrium 5 days<br />

18.1 Rates of Reactions 18.3 Reversible Reaction & Equilibrium<br />

18.2 The Progress of Chemical Reactions 18.5 Free Energy and Entropy<br />

Unit 8 (14 days)<br />

Chapter 19 Acid and Bases 10 days<br />

19.1 Acid-Base Theories 19.4 Neutralization Reactions<br />

19.2 Hydrogen Ions and Acidity 19.5 Salts in Solutions<br />

19.3 Strengths of Acids and Bases<br />

Chapter 20 Oxidation-Reduction Reactions 4 days<br />

20.1 The Meaning of Oxidation and Reduction 20.3 Describing Redox Equations<br />

20.2 Oxidation Numbers<br />

3


Lorenzo Walker Technical High School<br />

MUSTANG LABORATORIES<br />

Chemistry Safety<br />

Safety in the MUSTANG LABORATORIES - Chemistry Laboratory<br />

Working in the chemistry laboratory is an interesting and rewarding experience. During your labs, you will be actively<br />

involved from beginning to end—from setting some change in motion to drawing some conclusion. In the laboratory, you<br />

will be working with equipment and materials that can cause injury if they are not handled properly.<br />

However, the laboratory is a safe place to work if you are careful. Accidents do not just happen; they are caused—by<br />

carelessness, haste, and disregard of safety rules and practices. Safety rules to be followed in the laboratory are listed<br />

below. Before beginning any lab work, read these rules, learn them, and follow them carefully.<br />

General<br />

1. Be prepared to work when you arrive at the lab. Familiarize yourself with the lab procedures before beginning the lab.<br />

2. Perform only those lab activities assigned by your teacher. Never do anything in the laboratory that is not called for in<br />

the laboratory procedure or by your teacher. Never work alone in the lab. Do not engage in any horseplay.<br />

3. Work areas should be kept clean and tidy at all times. Only lab manuals and notebooks should be brought to the work<br />

area. Other books, purses, brief cases, etc. should be left at your desk or placed in a designated storage area.<br />

4. Clothing should be appropriate for working in the lab. Jackets, ties, and other loose garments should be removed. Open<br />

shoes should not be worn.<br />

5. Long hair should be tied back or covered, especially in the vicinity of open flame.<br />

6. Jewelry that might present a safety hazard, such as dangling necklaces, chains, medallions, or bracelets should not be<br />

worn in the lab.<br />

7. Follow all instructions, both written and oral, carefully.<br />

8. Safety goggles and lab aprons should be worn at all times.<br />

9. Set up apparatus as described in the lab manual or by your teacher. Never use makeshift arrangements.<br />

10. Always use the prescribed instrument (tongs, test tube holder, forceps, etc.) for handling apparatus or equipment.<br />

11. Keep all combustible materials away from open flames.<br />

12. Never touch any substance in the lab unless specifically instructed to do so by your teacher.<br />

13. Never put your face near the mouth of a container that is holding chemicals.<br />

14. Never smell any chemicals unless instructed to do so by your teacher. When testing for odors, use a wafting motion to<br />

direct the odors to your nose.<br />

15. Any activity involving poisonous vapors should be conducted in the fume hood.<br />

16. Dispose of waste materials as instructed by your teacher.<br />

17. Clean up all spills immediately.<br />

18. Clean and wipe dry all work surfaces at the end of class. Wash your hands thoroughly.<br />

19. Know the location of emergency equipment (first aid kit, fire extinguisher, fire shower, fire blanket, etc.) and how to use them.<br />

20. Report all accidents to the teacher immediately.<br />

Handling Chemicals<br />

21. Read and double check labels on reagent bottles before removing any reagent. Take only as much reagent as you<br />

need.<br />

22. Do not return unused reagent to stock bottles.<br />

23. When transferring chemical reagents from one container to another, hold the containers out away from your body.<br />

24. When mixing an acid and water, always add the acid to the water.<br />

25. Avoid touching chemicals with your hands. If chemicals do come in contact with your hands, wash them immediately.<br />

26. Notify your teacher if you have any medical problems that might relate to lab work, such as allergies or asthma.<br />

27. If you will be working with chemicals in the lab, avoid wearing contact lenses. Change to glasses, if possible, or notify<br />

the teacher.<br />

Handling Glassware<br />

28. Glass tubing, especially long pieces, should be carried in a vertical position to minimize the likelihood of breakage and<br />

to avoid stabbing anyone.<br />

29. Never handle broken glass with your bare hands. Use a brush and dustpan to clean up broken glass. Dispose of the<br />

glass as directed by your teacher.<br />

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30. Always lubricate glassware (tubing, thistle tubes, thermometers, etc.) with water or glycerin before attempting to insert<br />

it into a rubber stopper.<br />

31. Never apply force when inserting or removing glassware from a stopper. Use a twisting motion. If a piece of glassware<br />

becomes "frozen" in a stopper, take it to your teacher.<br />

32. Do not place hot glassware directly on the lab table. Always use an insulating pad of some sort.<br />

33. Allow plenty of time for hot glass to cool before touching it. Hot glass can cause painful burns. (Hot glass looks cool.)<br />

Heating Substances<br />

34. Exercise extreme caution when using a gas burner. Keep your head and clothing away from the flame.<br />

35. Always turn the burner off when it is not in use.<br />

36. Do not bring any substance into contact with a flame unless instructed to do so.<br />

37. Never heat anything without being instructed to do so.<br />

38. Never look into a container that is being heated.<br />

39. When heating a substance in a test tube, make sure that the mouth of the tube is not pointed at yourself or anyone<br />

else.<br />

40. Never leave unattended anything that is being heated or is visibly reacting.<br />

First Aid in the MUSTANG LABORATORIES - Chemistry Laboratory<br />

Accidents do not often happen in well-equipped chemistry laboratories if students understand safe laboratory procedures<br />

and are careful in following them. When an occasional accident does occur, it is likely to be a minor one.<br />

The instructor will assist in treating injuries such as minor cuts and burns. However, for some types of injuries, you must<br />

take action immediately. The following information will be helpful to you if an accident occurs.<br />

1. Shock. People who are suffering from any severe injury (for example, a bad burn or major loss of blood) may be in a<br />

state of shock. A person in shock is usually pale and faint. The person may be sweating, with cold, moist skin and a weak,<br />

rapid pulse. Shock is a serious medical condition. Do not allow a person in shock to walk anywhere—even to the campus<br />

security office. While emergency help is being summoned, place the victim face up in a horizontal position, with the feet<br />

raised about 30 centimeters. Loosen any tightly fitting clothing and keep him or her warm.<br />

2. Chemicals in the Eyes. Getting any kind of a chemical into the eyes is undesirable, but certain chemicals are<br />

especially harmful. They can destroy eyesight in a matter of seconds. Because you will be wearing safety goggles at all<br />

times in the lab, the likelihood of this kind of accident is remote. However, if it does happen, flush your eyes with water<br />

immediately. Do NOT attempt to go to the campus office before flushing your eyes. It is important that flushing with water<br />

be continued for a prolonged time—about 15 minutes.<br />

3. Clothing or Hair on Fire. A person whose clothing or hair catches on fire will often run around hysterically in an<br />

unsuccessful effort to get away from the fire. This only provides the fire with more oxygen and makes it burn faster. For<br />

clothing fires, throw yourself to the ground and roll around to extinguish the flames. For hair fires, use a fire blanket to<br />

smother the flames. Notify campus security immediately.<br />

4. Bleeding from a Cut. Most cuts that occur in the chemistry laboratory are minor. For minor cuts, apply pressure to the<br />

wound with a sterile gauze. Notify campus security of all injuries in the lab. If the victim is bleeding badly, raise the<br />

bleeding part, if possible, and apply pressure to the wound with a piece of sterile gauze. While first aid is being given,<br />

someone else should notify the campus security officer.<br />

5. Chemicals in the Mouth. Many chemicals are poisonous to varying degrees. Any chemical taken into the mouth<br />

should be spat out and the mouth rinsed thoroughly with water. Note the name of the chemical and notify the campus<br />

office immediately. If the victim swallows a chemical, note the name of the chemical and notify campus security<br />

immediately.<br />

If necessary, the campus security officer or administrator will contact the Poison Control Center, a hospital emergency<br />

room, or a physician for instructions.<br />

6. Acid or Base Spilled on the Skin.<br />

Flush the skin with water for about 15 minutes. Take the victim to the campus office to report the injury.<br />

7. Breathing Smoke or Chemical Fumes.<br />

All experiments that give off smoke or noxious gases should be conducted in a well-ventilated fume hood. This will make<br />

an accident of this kind unlikely. If smoke or chemical fumes are present in the laboratory, all persons—even those who<br />

do not feel ill—should leave the laboratory immediately. Make certain that all doors to the laboratory are closed after the<br />

last person has left. Since smoke rises, stay low while evacuating a smoke-filled room. Notify campus security<br />

immediately.<br />

5


MUSTANG LABORATORIES<br />

COMMITMENT TO SAFETY IN THE LABORATORY<br />

As a student enrolled in Chemistry at Lorenzo Walker Technical High<br />

School, I agree to use good laboratory safety practices at all times. I<br />

also agree that I will:<br />

1. Conduct myself in a professional manner, respecting both my personal safety and the safety of<br />

others in the laboratory.<br />

2. Wear proper and approved safety glasses or goggles in the laboratory at all times.<br />

3. Wear sensible clothing and tie back long hair in the laboratory. Understand that open-toed shoes<br />

pose a hazard during laboratory classes and that contact lenses are an added safety risk.<br />

4. Keep my lab area free of clutter during an experiment.<br />

5. Never bring food or drink into the laboratory, nor apply makeup within the laboratory.<br />

6. Be aware of the location of safety equipment such as the fire extinguisher, eye wash station, fire<br />

blanket, first aid kit. Know the location of the nearest telephone and exits.<br />

7. Read the assigned lab prior to coming to the laboratory.<br />

8. Carefully read all labels on all chemical containers before using their contents, remove a small<br />

amount of reagent properly if needed, do not pour back the unused chemicals into the original<br />

container.<br />

9. Dispose of chemicals as directed by the instructor only. At no time will I pour anything down the<br />

sink without prior instruction.<br />

10. Never inhale fumes emitted during an experiment. Use the fume hood when instructed to do so.<br />

11. Report any accident immediately to the instructor, including chemical spills.<br />

12. Dispose of broken glass and sharps only in the designated containers.<br />

13. Clean my work area and all glassware before leaving the laboratory.<br />

14. Wash my hands before leaving the laboratory.<br />

NAME __________________________<br />

Britney Contreras<br />

PERIOD ________________________<br />

3<br />

PARENT NAME ____________________________<br />

Maria Benavides<br />

PARENT NUMBER _________________________<br />

(239)-692-1410<br />

SIGNATURE ____________________________<br />

DATE ____________________________________<br />

6


7


Chapter 1<br />

Unit 1<br />

Introduction to Chemistry<br />

The students will learn why and how to solve problems using<br />

chemistry.<br />

Identify what is science, what clearly is not science, and what superficially<br />

resembles science (but fails to meet the criteria for science).<br />

Students will identify a phenomenon as science or not science.<br />

Science<br />

Observation<br />

Inference<br />

Hypothesis<br />

Identify which questions can be answered through science and which<br />

questions are outside the boundaries of scientific investigation, such as<br />

questions addressed by other ways of knowing, such as art, philosophy, and<br />

religion.<br />

Students will differentiate between problems and/or phenomenon that can and<br />

those that cannot be explained or answered by science.<br />

Students will differentiate between problems and/or phenomenon that can and<br />

those that cannot be explained or answered by science.<br />

Observation<br />

Inference<br />

Hypothesis<br />

Theory<br />

Controlled experiment<br />

Describe how scientific inferences are drawn from scientific observations<br />

and provide examples from the content being studied.<br />

Students will conduct and record observations.<br />

Students will make inferences.<br />

Students will identify a statement as being either an observation or inference.<br />

Students will pose scientific questions and make predictions based on<br />

inferences.<br />

Inference<br />

Observation<br />

Hypothesis<br />

Controlled experiment<br />

Identify sources of information and assess their reliability according to the<br />

strict standards of scientific investigation.<br />

Students will compare and assess the validity of known scientific information<br />

from a variety of sources:<br />

8


Print vs. print<br />

Online vs. online<br />

Print vs. online<br />

Students will conduct an experiment using the scientific method and compare<br />

with other groups.<br />

Controlled experiment<br />

Investigation<br />

Peer Review<br />

Accuracy<br />

Precision<br />

Percentage Error<br />

Chapter 2<br />

Matter and Change<br />

The students will learn what properties are used to describe<br />

matter and how matter can change its form.<br />

Differentiate between physical and chemical properties and physical and<br />

chemical changes of matter.<br />

Students will be able to identify physical and chemical properties of various<br />

substances.<br />

Students will be able to identify indicators of physical and chemical changes.<br />

Students will be able to calculate density.<br />

mass<br />

physical property<br />

volume<br />

chemical property<br />

vapor<br />

extensive property<br />

Chapter 3<br />

mixture<br />

intensive property<br />

solution<br />

element<br />

compound<br />

Scientific Measurements<br />

The students will be able to solve conversion problems using<br />

measurements.<br />

Determine appropriate and consistent standards of measurement for the<br />

data to be collected in a survey or experiment.<br />

Students will participate in activities to collect data using standardized<br />

measurement.<br />

Students will be able to manipulate/convert data collected and apply the data<br />

to scientific situations.<br />

Scientific notation<br />

International System of Units (SI)<br />

Significant figures<br />

Accepted value<br />

Experimental value<br />

Percent error<br />

Dimensional analysis<br />

9


10


To use the Stair-Step method, find the prefix the original measurement starts with. (ex. milligram)<br />

If there is no prefix, then you are starting with a base unit.<br />

Find the step which you wish to make the conversion to. (ex. decigram)<br />

Count the number of steps you moved, and determine in which direction you moved (left or right).<br />

The decimal in your original measurement moves the same number of places as steps you moved and in the<br />

same direction. (ex. milligram to decigram is 2 steps to the left, so 40 milligrams = .40 decigrams)<br />

If the number of steps you move is larger than the number you have, you will have to add zeros to hold the<br />

places. (ex. kilometers to meters is three steps to the right, so 10 kilometers would be equal to 10,000 m)<br />

That’s all there is to it! You need to be able to count to 6, and know your left from your right!<br />

1) Write the equivalent<br />

a) 5 dm =_______m b) 4 mL = ______L c) 8 g = _______mg<br />

d) 9 mg =_______g e) 2 mL = ______L f) 6 kg = _____g<br />

g) 4 cm =_______m h) 12 mg = ______ g i) 6.5 cm 3 = _______L<br />

j) 7.02 mL =_____cm 3 k) .03 hg = _______ dg l) 6035 mm _____cm<br />

m) .32 m = _______cm n) 38.2 g = _____kg<br />

11


2. One cereal bar has a mass of 37 g. What is the mass of 6 cereal bars? Is that more than or less<br />

than 1 kg? Explain your answer.<br />

3. Wanda needs to move 110 kg of rocks. She can carry l0 hg each trip. How many trips must she<br />

make? Explain your answer.<br />

4. Dr. O is playing in her garden again She needs 1 kg of potting soil for her plants. She has 750 g.<br />

How much more does she need? Explain your answer.<br />

5. Weather satellites orbit Earth at an altitude of 1,400,000 meters. What is this altitude in kilometers?<br />

6. Which unit would you use to measure the capacity? Write milliliter or liter.<br />

a) a bucket __________<br />

b) a thimble __________<br />

c) a water storage tank__________<br />

d) a carton of juice__________<br />

7. Circle the more reasonable measure:<br />

a) length of an ant 5mm or 5cm<br />

b) length of an automobile 5 m or 50 m<br />

c) distance from NY to LA 450 km or 4,500 km<br />

d) height of a dining table 75 mm or 75 cm<br />

8. Will a tablecloth that is 155 cm long cover a table that is 1.6 m long? Explain your answer.<br />

9. A dollar bill is 15.6 cm long. If 200 dollar bills were laid end to end, how many meters long would<br />

the line be?<br />

10. The ceiling in Jan’s living room is 2.5 m high. She has a hanging lamp that hangs down 41 cm.<br />

Her husband is exactly 2 m tall. Will he hit his head on the hanging lamp? Why or why not?<br />

12


Using SI Units<br />

Match the terms in Column II with the descriptions in Column I. Write the letters of the correct term in<br />

the blank on the left.<br />

Column I Column II<br />

_____ 1. distance between two points<br />

a. time<br />

_____ 2. SI unit of length<br />

_____ 3. tool used to measure length<br />

_____ 4. units obtained by combining other units<br />

_____ 5. amount of space occupied by an object<br />

_____ 6. unit used to express volume<br />

_____ 7. SI unit of mass<br />

_____ 8. amount of matter in an object<br />

_____ 9. mass per unit of volume<br />

_____ 10. temperature scale of most laboratory thermometers<br />

_____ 11. instrument used to measure mass<br />

_____ 12. interval between two events<br />

_____ 13. SI unit of temperature<br />

_____ 14. SI unit of time<br />

_____ 15. instrument used to measure temperature<br />

b. volume<br />

c. mass<br />

d. density<br />

e. meter<br />

f. kilogram<br />

g. derived<br />

h. liter<br />

i. second<br />

j. Kelvin<br />

k. length<br />

1. balance<br />

m. meterstick<br />

n. thermometer<br />

o. Celsius<br />

Circle the two terms in each group that are related. Explain how the terms are related.<br />

16. Celsius degree, mass, Kelvin _____________________________________________________<br />

________________________________________________________________________________<br />

17. balance, second, mass __________________________________________________________<br />

________________________________________________________________________________<br />

18. kilogram, liter, cubic centimeter __________________________________________________<br />

________________________________________________________________________________<br />

19. time, second, distance __________________________________________________________<br />

________________________________________________________________________________<br />

20. decimeter, kilometer, Kelvin _____________________________________________________<br />

________________________________________________________________________________<br />

13


1. How many meters are in one kilometer? __________<br />

2. What part of a liter is one milliliter? __________<br />

3. How many grams are in two dekagrams? __________<br />

4. If one gram of water has a volume of one milliliter, what would the mass of one liter of water be in<br />

kilograms?__________<br />

5. What part of a meter is a decimeter? __________<br />

In the blank at the left, write the term that correctly completes each statement. Choose from the terms<br />

listed below.<br />

Metric SI standard ten<br />

prefixes ten tenth<br />

6. An exact quantity that people agree to use for comparison is a ______________ .<br />

7. The system of measurement used worldwide in science is _______________ .<br />

8. SI is based on units of _______________ .<br />

9. The system of measurement that was based on units of ten was the _______________ system.<br />

10. In SI, _______________ are used with the names of the base unit to indicate the multiple of ten<br />

that is being used with the base unit.<br />

11. The prefix deci- means _______________ .<br />

14


Standards of Measurement<br />

Fill in the missing information in the table below.<br />

S.I prefixes and their meanings<br />

Prefix<br />

Meaning<br />

0.001<br />

0.01<br />

deci- 0.1<br />

10<br />

hecto- 100<br />

1000<br />

Circle the larger unit in each pair of units.<br />

1. millimeter, kilometer 4. centimeter, millimeter<br />

2. decimeter, dekameter 5. hectogram, kilogram<br />

3. hectogram, decigram<br />

6. In SI, the base unit of length is the meter. Use this information to arrange the following units of<br />

measurement in the correct order from smallest to largest.<br />

Write the number 1 (smallest) through 7 - (largest) in the spaces provided.<br />

_____ a. kilometer<br />

_____ b. centimeter<br />

_____ c. meter<br />

_____ e. hectometer<br />

_____ f. millimeter<br />

_____ g. decimeter<br />

_____ d. dekameter<br />

Use your knowledge of the prefixes used in SI to answer the following questions in the spaces<br />

provided.<br />

7. One part of the Olympic games involves an activity called the decathlon. How many events do you<br />

think make up the decathlon?_____________________________________________________<br />

8. How many years make up a decade? _______________________________________________<br />

9. How many years make up a century? ______________________________________________<br />

10. What part of a second do you think a millisecond is? __________________________________<br />

15


The Learning Goal for this assignment is:<br />

etermine appropriate and consistent standards of measurement for the data to be collected in a survey<br />

r<br />

xperiment.<br />

Notes Section<br />

7.485 * 10E3 = 7.485 move deci =7485<br />

Positive exponents is move the decimal to the right and make the # (Exponent)bigger<br />

Negative exponent is when you move the decimal to the left and the # (exponent)gets<br />

smaller<br />

When the exponent is zero you don't move anything<br />

1. 7,485 6. 1.683<br />

2. 884.2 7. 3.622<br />

3. 0.00002887 8. 0.00001735<br />

4. 0.05893 9. 0.9736<br />

5. 0.006162 10. 0.08558<br />

11. 6.633 X 10−⁴ 16. 1.937 X 10⁴<br />

12. 4.445 X 10−⁴ 17. 3.457 X 10⁴<br />

13. 2.182 X 10−³ 18. 3.948 X 10−⁵<br />

14. 4.695 X 10² 19. 8.945 X 10⁵<br />

15. 7.274 X 10⁵ 20. 6.783 X 10²<br />

16


SCIENTIFIC NOTATION RULES<br />

How to Write Numbers in Scientific Notation<br />

Scientific notation is a standard way of writing very large and very small numbers so that they're<br />

easier to both compare and use in computations. To write in scientific notation, follow the form<br />

N X 10 ᴬ<br />

where N is a number between 1 and 10, but not 10 itself, and A is an integer (positive or negative<br />

number).<br />

RULE #1: Standard Scientific Notation is a number from 1 to 9 followed by a decimal and the<br />

remaining significant figures and an exponent of 10 to hold place value.<br />

Example:<br />

5.43 x 10 2 = 5.43 x 100 = 543<br />

8.65 x 10 – 3 = 8.65 x .001 = 0.00865<br />

****54.3 x 10 1 is not Standard Scientific Notation!!!<br />

RULE #2: When the decimal is moved to the Left the exponent gets Larger, but the value of the<br />

number stays the same. Each place the decimal moves Changes the exponent by one (1). If you<br />

move the decimal to the Right it makes the exponent smaller by one (1) for each place it is moved.<br />

Example:<br />

6000. x 10 0 = 600.0 x 10 1 = 60.00 x 10 2 = 6.000 x 10 3 = 6000<br />

(Note: 10 0 = 1)<br />

All the previous numbers are equal, but only 6.000 x 10 3 is in proper Scientific Notation.<br />

17


RULE #3: To add/subtract in scientific notation, the exponents must first be the same.<br />

Example:<br />

(3.0 x 10 2 ) + (6.4 x 10 3 ); since 6.4 x 10 3 is equal to 64. x 10 2 . Now add.<br />

(3.0 x 10 2 )<br />

+ (64. x 10 2 )<br />

67.0 x 10 2 = 6.70 x 10 3 = 6.7 x 10 3<br />

67.0 x 10 2 is mathematically correct, but a number in standard scientific notation can only<br />

have one number to the left of the decimal, so the decimal is moved to the left one place and<br />

one is added to the exponent.<br />

Following the rules for significant figures, the answer becomes 6.7 x 10 3 .<br />

RULE #4: To multiply, find the product of the numbers, then add the exponents.<br />

Example:<br />

(2.4 x 10 2 ) (5.5 x 10 –4 ) = ? [2.4 x 5.5 = 13.2]; [2 + -4 = -2], so<br />

(2.4 x 10 2 ) (5.5 x 10 –4 ) = 13.2 x 10 –2 = 1.3 x 10 – 1<br />

RULE #5: To divide, find the quotient of the number and subtract the exponents.<br />

Example:<br />

(3.3 x 10 – 6 ) / (9.1 x 10 – 8 ) = ? [3.3 / 9.1 = .36]; [-6 – (-8) = 2], so<br />

(3.3 x 10 – 6 ) / (9.1 x 10 – 8 ) = .36 x 10 2 = 3.6 x 10 1<br />

18


Convert each number from Scientific Notation to real numbers:<br />

1. 7.485 X 10³ 6. 1.683 X 10⁰<br />

7485<br />

1.683<br />

7,485<br />

1.683<br />

2. 8.842 X 10² 7. 3.622 10⁰<br />

884.2<br />

3.622<br />

884.2<br />

3.622<br />

3. 2.887 X 10−⁵ 8. 1.735 X 10−⁵<br />

.00002887 .00001735<br />

.00001735<br />

.00002887<br />

4. 5.893 X 10−² 9. 9.736 X 10−¹<br />

.005893<br />

.09736<br />

.05893<br />

.9736<br />

5. 6.162 X 10−³ 10. 8.558 X 10−²<br />

.006163<br />

.008558<br />

6.162<br />

.08558<br />

Convert each number from a real number to Scientific Notation:<br />

11. 0.0006633 16. 1,937,000<br />

6.633 * 10 -4<br />

1.937*10 6<br />

12. 0.0004445 17. 34,570<br />

4.445 * 10 -4 3.4570 * 10 -2<br />

13. 0.002182 18. 0.00003948<br />

2.184 * 10 -3<br />

3.948 * 10 5<br />

14. 469.5 19. 894,500 5<br />

469.5 * 10 2<br />

8.945 *10<br />

15. 727,400 20. 678.3<br />

6.783 * 10 2 19


The Learning Goal for this assignment is:<br />

Determine appropriate and consistent standards of measurement for the data to be collected in a survey<br />

or<br />

experiment.<br />

Notes Section:<br />

Increasing the # decreases the exponent<br />

Decreasing the # increases the exponent<br />

Question Sig Figs Question Add & Subtract Question Multiple & Divide<br />

1 4 1 55.36 1 20,000<br />

2 4 2 84.2 2 94<br />

3 3 3 115.4 3 300<br />

4 3 4 0.8 4 7<br />

5 4 5 245.53 5 62<br />

6 3 6 34.5 6 0.005<br />

7 3 7 74.0 7 4,000<br />

8 2 8 53.287 8 3,900,000<br />

9 2 9 54.876 9 2<br />

10 2 10 40.19 10 30,000,000<br />

11 3 11 7.7 11 1,200<br />

12 2 12 67.170 12 0.2<br />

13 3 13 81.0 13 0.87<br />

14 4 14 73.290 14 0.049<br />

15 4 15 29.789 15 2,000<br />

16 3 16 39.53 16 0.5<br />

17 4 17 70.58 17 1.9<br />

18 2 18 86.6 18 0.05<br />

19 2 19 64.990 19 230<br />

20 1 20 36.0 20 460,000<br />

20


Significant Figures Rules<br />

There are three rules on determining how many significant figures are in a<br />

number:<br />

1. Non-zero digits are always significant.<br />

2. Any zeros between two significant digits are significant.<br />

3. A final zero or trailing zeros in the DECIMAL PORTION ONLY are<br />

significant.<br />

Please remember that, in science, all numbers are based upon measurements (except for a very few<br />

that are defined). Since all measurements are uncertain, we must only use those numbers that are<br />

meaningful.<br />

Not all of the digits have meaning (significance) and, therefore, should not be written down. In<br />

science, only the numbers that have significance (derived from measurement) are written.<br />

Rule 1: Non-zero digits are always significant.<br />

If you measure something and the device you use (ruler, thermometer, triple-beam, balance, etc.)<br />

returns a number to you, then you have made a measurement decision and that ACT of measuring<br />

gives significance to that particular numeral (or digit) in the overall value you obtain.<br />

Hence a number like 46.78 would have four significant figures and 3.94 would have three.<br />

Rule 2: Any zeros between two significant digits are significant.<br />

Suppose you had a number like 409. By the first rule, the 4 and the 9 are significant. However, to<br />

make a measurement decision on the 4 (in the hundred's place) and the 9 (in the one's place), you<br />

HAD to have made a decision on the ten's place. The measurement scale for this number would have<br />

hundreds, tens, and ones marked.<br />

Like the following example:<br />

These are sometimes called "captured zeros."<br />

If a number has a decimal at the end (after the one’s place) then all digits (numbers) are significant<br />

and will be counted.<br />

In the following example the zeros are significant digits and highlighted in blue.<br />

960.<br />

70050.<br />

21


Rule 3: A final zero or trailing zeros in the decimal portion ONLY are<br />

significant.<br />

This rule causes the most confusion among students.<br />

In the following example the zeros are significant digits and highlighted in blue.<br />

0.07030<br />

0.00800<br />

Here are two more examples where the significant zeros are highlighted in blue.<br />

When Zeros are Not Significant Digits<br />

4.7 0 x 10−³<br />

6.5 0 0 x 10⁴<br />

Zero Type # 1 : Space holding zeros in numbers less than one.<br />

In the following example the zeros are NOT significant digits and highlighted in red.<br />

0.09060<br />

0.00400<br />

These zeros serve only as space holders. They are there to put the decimal point in its correct<br />

location.<br />

They DO NOT involve measurement decisions.<br />

Zero Type # 2 : Trailing zeros in a whole number.<br />

In the following example the zeros are NOT significant digits and highlighted in red.<br />

200<br />

25000<br />

For addition and subtraction, look at the decimal portion (i.e., to the right of the decimal point)<br />

of the numbers ONLY. Here is what to do:<br />

1) Count the number of significant figures in the decimal portion of each number in the problem. (The<br />

digits to the left of the decimal place are not used to determine the number of decimal places in the<br />

final answer.)<br />

2) Add or subtract in the normal fashion.<br />

3) Round the answer to the LEAST number of places in the decimal portion of any number in the<br />

problem<br />

The following rule applies for multiplication and division:<br />

The LEAST number of significant figures in any number of the problem determines the number of<br />

significant figures in the answer.<br />

This means you MUST know how to recognize significant figures in order to use this rule.<br />

22


How Many Significant Digits for Each Number?<br />

1) 2359 = ______<br />

4<br />

2) 2.445 x 10−⁵= ______ 4<br />

4<br />

2.445000 NOOO<br />

3) 2.93 x 10⁴= ______ 3<br />

4) 1.30 x 10−⁷= ______ 2<br />

5) 2604 = ______ 4<br />

6) 9160 = ______ 3<br />

7) 0.0800 = ______ 3<br />

8) 0.84 = ______ 2<br />

9) 0.0080 = ______ 2<br />

10) 0.00040 = ______ 2<br />

11) 0.0520 = ______ 3<br />

12) 0.060 = ______ 2<br />

13) 6.90 x 10−¹= ______ 3<br />

14) 7.200 x 10⁵= ______ 4<br />

15) 5.566 x 10−²= ______<br />

16) 3.88 x 10⁸= ______ 3<br />

17) 3004 = ______ 4<br />

18) 0.021 = ______ 2<br />

19) 240 = ______ 2<br />

20) 500 = ______ 1<br />

4<br />

23


For addition and subtraction, look at the decimal portion (i.e., to the right of the decimal point) of the<br />

numbers ONLY. Here is what to do:<br />

1) Count the number of significant figures in the decimal portion of each number in the problem. (The<br />

digits to the left of the decimal place are not used to determine the number of decimal places in the<br />

final answer.)<br />

2) Add or subtract in the normal fashion.<br />

3) Round the answer to the LEAST number of places in the decimal portion of any number in the<br />

problem.<br />

Solve the Problems and Round Accordingly...<br />

1) 43.287 + 5.79 + 6.284 = _______ 55.36<br />

2) 87.54 - 3.3 = _______ 84.2 84.24<br />

3) 99.1498 + 6.5397 + 9.7 = _______ 115.4<br />

115.3895<br />

4) 5.868 - 5.1 = _______ 0.8<br />

5) 59.9233 + 86.21 + 99.396 = _______ 245.53<br />

6) 7.7 + 26.756 = _______ 34.5<br />

7) 66.8 + 2.3 + 4.8516 = _______ 74.0<br />

8) 9.7419 + 43.545 = _______ 53.287<br />

9) 4.8976 + 48.4644 + 1.514 = _______ 54.876<br />

10) 4.335 + 35.85 = _______ 40.19<br />

11) 9.448 - 1.7 = _______ 7.7<br />

12) 75.826 - 8.6555 = _______ 67.170<br />

13) 57.2 + 23.814 = _______ 81.0<br />

14) 77.684 - 4.394 = _______ 73.290<br />

15) 26.4496 + 3.339 = _______ 29.789<br />

16) 9.6848 + 29.85 = _______ 39.53<br />

17) 63.11 + 2.5412 + 4.93 = _______ 70.58<br />

86.6<br />

18) 11.2471 + 75.4 = _______<br />

19) 73.745 - 8.755 = 64.990 _______<br />

20) 6.5238 + 1.7 + 27.79 = _______ 36.o<br />

24


The following rule applies for multiplication and division:<br />

The LEAST number of significant figures in any number of the problem determines the number of<br />

significant figures in the answer.<br />

This means you MUST know how to recognize significant figures in order to use this rule.<br />

Solve the Problems and Round Accordingly...<br />

1 2 3<br />

1) 0.6 x 65.0 x 602 = __________<br />

20,000<br />

2 2<br />

2) 720 ÷ 7.7 = __________<br />

3 1<br />

94<br />

300 278.7<br />

3) 929 x 0.3 = __________<br />

4) 300 ÷ 44.31 = __________<br />

7<br />

5) 608 ÷ 9.8 = __________<br />

62<br />

6) 0.06 x 0.079 = __________<br />

0.005<br />

7) 0.008 x 72.91 x 7000 = __________<br />

4,00<br />

8) 73.94 x 67 x 780 = __________<br />

3,900,000<br />

9) 0.62 x 0.097 x 40 = __________<br />

2<br />

10) 600 x 10 x 5030 = __________<br />

30,000,000<br />

11) 5200 ÷ 4.46 = __________<br />

1,200<br />

12) 0.0052 x 0.4 x 107 = __________<br />

0.2<br />

13) 0.099 x 8.8 = __________<br />

0.87<br />

14) 0.0095 x 5.2 = __________<br />

0.049<br />

15) 8000 ÷ 4.62 = __________<br />

2,000<br />

16) 0.6 x 0.8 = __________<br />

0.5<br />

17) 2.84 x 0.66 = __________<br />

1.9<br />

18) 0.5 x 0.09 = __________<br />

0.05<br />

19) 8100 ÷ 34.84 = 230 __________<br />

20) 8.24 x 6.9 x 8100 = __________<br />

460,000<br />

23478<br />

93.506493551<br />

25


Dimensional Analysis<br />

This is a way to convert from one unit of a given substance to<br />

another unit using ratios or conversion units. What this video<br />

www.youtube.com/watch?v=aZ3J60GYo6U<br />

Let’ look at a couple of examples:<br />

1. Convert 2.6 qt to mL.<br />

First we need a ratio or conversion unit so that we can go from quarts to milliliters. 1.00 qt = 946 mL<br />

Next write down what you are starting with<br />

2.6 qt<br />

Then make you conversion tree<br />

2.6 qt<br />

Then fill in the units in your ratio so that you can cancel out the original unit and will be left with the<br />

unit you need for the answer. Cross out units, one at a time that are paired, and one on top one on<br />

the bottom.<br />

2.6 qt mL<br />

qt<br />

Now fill in the values from the ratio.<br />

2.6 qt 946 mL<br />

1.00 qt<br />

Now multiply all numbers on the top and multiply all numbers on the bottom and write them as a<br />

fraction.<br />

2.6 qt 946 mL = 2,459.6 mL<br />

1.00 qt 1.00<br />

Now divide the top number by the bottom number and write that number with the unit that was not<br />

crossed out.<br />

26


1qt=32 oz 1gal = 4qts 1.00 qt = 946 mL 1L = 1000mL<br />

2. Convert 8135.6 mL to quarts<br />

8135.6mL 1qt<br />

946mL<br />

=<br />

8135.6<br />

946<br />

8.6qts<br />

3. Convert 115.2 oz to mL<br />

115.2oz 1qt<br />

946mL<br />

=<br />

108979.2<br />

32oz<br />

1qt<br />

32<br />

3405.6mL<br />

4. Convert 2.3 g to Liters<br />

2.3 4qts<br />

1g<br />

945mL<br />

1qt<br />

=<br />

1mL 108979.2 8.7L<br />

1000mL<br />

32<br />

5. Convert 8.42 L to oz<br />

8.42L<br />

1000mL<br />

1L<br />

1qt<br />

946mL<br />

Go to http://science.widener.edu/svb/tutorial/ chose #7 “Converting Volume” and do 5 more in the<br />

space provided.<br />

7.76L<br />

1. Convert _________ to _________ oz<br />

7.76L<br />

1000mL<br />

1qt<br />

1qt<br />

946mL<br />

1qt<br />

32oz<br />

1qt<br />

32oz<br />

=<br />

=<br />

269,440<br />

946<br />

249<br />

946<br />

284oz<br />

262.4<br />

2. Convert _________ 6.8qt to _________ oz<br />

6.8qt 946mL<br />

=<br />

6432 6432<br />

1qt<br />

1qt<br />

oz<br />

3. Convert _________ 7.1L to _________<br />

7.1L 1000mL 1qt<br />

1L<br />

945mL<br />

32oz<br />

1qt<br />

=<br />

227200<br />

946<br />

240.1<br />

4. Convert _________ 6.1qt to _________ mL<br />

1qt 946mL<br />

1qt<br />

=<br />

5770<br />

1<br />

5770<br />

5. Convert _________ 272oz to _________ mL<br />

272oz 1qt 945mL 8041<br />

32oz 1qt<br />

32<br />

=<br />

8041<br />

27


Chapter 4<br />

Unit 2<br />

Atomic Structure<br />

The students will learn what makes up atoms and how are<br />

atoms of one element different from atoms of another element.<br />

Explore the scientific theory of atoms (also known as atomic theory) by<br />

describing changes in the atomic model over time and why those changes<br />

were necessitated by experimental evidence.<br />

Students will be able to draw/identify each atomic model.<br />

Students will be able to compare/contrast the different atomic models.<br />

Students will be able to describe how results of experimental evidence caused<br />

the atomic model to change.<br />

proton<br />

electron<br />

neutron<br />

nucleus<br />

electron cloud<br />

Explore the scientific theory of atoms (also known as atomic theory) by<br />

describing the structure of atoms in terms of protons, neutrons and<br />

electrons, and differentiate among these particles in terms of their mass,<br />

electrical charges and locations within the atom.<br />

Students will compare/contrast the characteristics of subatomic particles.<br />

atomic number<br />

mass number<br />

isotope<br />

atomic mass unit (amu)<br />

atomic mass<br />

28


Chapter 5<br />

Electrons in Atoms<br />

The students will be able to describe the arrangement of<br />

electrons in atoms and predict what will happen when<br />

electrons in atoms absorb or release energy.<br />

Describe the quantization of energy at the atomic level.<br />

Students will participate in activities to view emission spectrums using a<br />

diffraction grating or a spectroscope.<br />

Students will be able to explain how the spectrum lines relate to electron motion.<br />

energy level<br />

atomic orbital<br />

quantum mechanical model<br />

Chapter 6<br />

The Periodic Table<br />

The student will learn what information the periodic table<br />

provides and how periodic trends can be explained.<br />

Relate properties of atoms and their position in the periodic table to the<br />

arrangement of their electrons.<br />

Students will be able to compare and contrast metals, nonmetals, and metalloids.<br />

Students will be able to describe the traits of various families on the periodic<br />

table.<br />

Students will be able to explain periodicity.<br />

Students will write/represent electron configuration of various elements.<br />

Students will be able to use a periodic table to calculate the number of p + , e - , and<br />

n 0 .<br />

Students will be able to calculate the average weight of mass.<br />

periodic law<br />

halogen<br />

metals<br />

noble gas<br />

nonmetals<br />

transition metal<br />

metalloid<br />

atomic radius<br />

alkali metal<br />

ionization energy<br />

alkaline earth metal<br />

electronegativity<br />

29


The Learning Goal for this assignment is:<br />

Relate properties of atoms and their position in the periodic table to the arrangement of their<br />

electrons.<br />

Notes Section<br />

Matter is composed of atoms<br />

Protons, neutrons, and elements mad up atoms<br />

120 known elements in the periodic table<br />

each has either a positive, negative or neutral charge<br />

Atomic # tell you the # of protons in an atom<br />

if you lose a electron you have a positive charge<br />

if you gain an electron then you have a negative<br />

when you gain or lose an electron you have to either subtract or add what you gain from your atomic #<br />

Electrovalence is something that has given up or taken electrons to become an ion<br />

Positive are cations<br />

Negative are antions<br />

In the periodic table elements on the left are usually positive and elements on the right are usually + &<br />

elements on the right are usually -<br />

Iconic bonds are Electrovalence bonds<br />

Iconic bonds are groups of charged ions held together be electric forces<br />

Iconic bonds are very strong but weak in water<br />

Iconic are atoms either missing or extra neutron<br />

Isotopes are atoms with a missing or extra neutron<br />

Atomic masses are calculated by figuring out the amounts of each type of atom and isotopes there are<br />

http://www.learner.org/interactives/periodic/basics_interactive.html<br />

30


Atoms Are Building Blocks<br />

Atoms are the basis of chemistry. They are the basis for everything in the Universe. You<br />

should start by remembering that matter is composed of atoms. Atoms and the study of<br />

atoms are a world unto themselves. We're going to cover basics like atomic structure<br />

and bonding between atoms.<br />

Smaller Than Atoms?<br />

Are there pieces of matter that are smaller than atoms?<br />

Sure there are. You'll soon be learning that atoms are<br />

composed of pieces like electrons, protons, and neutrons.<br />

But guess what? There are even smaller particles moving<br />

around in atoms. These super-small particles can be found<br />

inside the protons and neutrons. Scientists have many<br />

names for those pieces, but you may have heard of<br />

nucleons and quarks. Nuclear chemists and physicists<br />

work together at particle accelerators to discover the<br />

presence of these tiny, tiny, tiny pieces of matter.<br />

Even though super-tiny atomic particles exist, you only<br />

need to remember the three basic parts of an atom: electrons, protons, and neutrons.<br />

What are electrons, protons, and neutrons? A picture works best to show off the idea.<br />

You have a basic atom. There are three types of pieces in that atom: electrons, protons,<br />

and neutrons. That's all you have to remember. Three things! As you know, there are<br />

almost 120 known elements in the periodic table. Chemists and physicists haven't<br />

stopped there. They are trying to make new ones in labs every day. The thing that<br />

makes each of those elements different is the number of electrons, protons, and<br />

neutrons. The protons and neutrons are always in the center of the atom. Scientists call<br />

the center region of the atom the nucleus. The nucleus in<br />

a cell is a thing. The nucleus in an atom is a place where<br />

you find protons and neutrons. The electrons are always<br />

found whizzing around the center in areas called shells or<br />

orbitals.<br />

You can also see that each piece has either a "+", "-", or a<br />

"0." That symbol refers to the charge of the particle. Have<br />

you ever heard about getting a shock from a socket, static<br />

electricity, or lightning? Those are all different types of<br />

electric charges. Those charges are also found in tiny particles of matter. The electron<br />

always has a "-", or negative, charge. The proton always has a "+", or positive, charge. If<br />

the charge of an entire atom is "0", or neutral, there are equal numbers of positive and<br />

negative pieces. Neutral means there are equal numbers of electrons and protons. The<br />

third particle is the neutron. It has a neutral charge, also known as a charge of zero. All<br />

atoms have equal numbers of protons and electrons so that they are neutral. If there are<br />

more positive protons or negative electrons in an atom, you have a special atom called<br />

an ion.<br />

31


Looking at Ions<br />

We haven’t talked about ions before, so let’s get down to basics. The<br />

atomic number of an element, also called a proton number, tells you the<br />

number of protons or positive particles in an atom. A normal atom has a<br />

neutral charge with equal numbers of positive and negative particles.<br />

That means an atom with a neutral charge is one where the number of<br />

electrons is equal to the atomic number. Ions are atoms with extra<br />

electrons or missing electrons. When you are missing an electron or<br />

two, you have a positive charge. When you have an extra electron<br />

or two, you have a negative charge.<br />

What do you do if you are a sodium (Na) atom? You have eleven<br />

electrons — one too many to have an entire shell filled. You need to<br />

find another element that will take that electron away from you. When you lose that<br />

electron, you will you’ll have full shells. Whenever an atom has full shells, we say it is<br />

"happy." Let's look at chlorine (Cl). Chlorine has seventeen electrons and only needs<br />

one more to fill its third shell and be "happy." Chlorine will take your extra sodium<br />

electron and leave you with 10 electrons inside of two filled shells. You are now a happy<br />

atom too. You are also an ion and missing one electron. That missing electron gives you<br />

a positive charge. You are still the element sodium, but you are now a sodium ion (Na + ).<br />

You have one less electron than your atomic number.<br />

Ion Characteristics<br />

So now you've become a sodium ion. You have ten electrons.<br />

That's the same number of electrons as neon (Ne). But you<br />

aren't neon. Since you're missing an electron, you aren't really<br />

a complete sodium atom either. As an ion you are now<br />

something completely new. Your whole goal as an atom was<br />

to become a "happy atom" with completely filled electron<br />

shells. Now you have those filled shells. You have a lower<br />

energy. You lost an electron and you are "happy." So what<br />

makes you interesting to other atoms? Now that you have<br />

given up the electron, you are quite electrically attractive.<br />

Other electrically charged atoms (ions) of the opposite charge<br />

(negative) are now looking at you and seeing a good partner to<br />

bond with. That's where the chlorine comes in. It's not only chlorine. Almost any ion with<br />

a negative charge will be interested in bonding with you.<br />

32


Electrovalence<br />

Don't get worried about the big word. Electrovalence is just another word for something<br />

that has given up or taken electrons and become an ion. If you look at the periodic table,<br />

you might notice that elements on the left side usually become positively charged ions<br />

(cations) and elements on the right side get a negative charge (anions). That trend<br />

means that the left side has a positive valence and the right side has a negative<br />

valence. Valence is a measure of how much an atom wants to bond with other atoms. It<br />

is also a measure of how many electrons are excited about bonding with other atoms.<br />

There are two main types of bonding, covalent and electrovalent. You may have heard<br />

of the term "ionic bonds." Ionic bonds are electrovalent bonds. They are just groups of<br />

charged ions held together by electric forces. When in the presence of other ions, the<br />

electrovalent bonds are weaker because of outside electrical forces and attractions.<br />

Sodium and chlorine ions alone have a very strong bond, but as soon as you put those<br />

ions in a solution with H + (Hydrogen ion), OH - (Hydroxide), F - (Fluorine ion) or Mg ++<br />

(Magnesium ion), there are charged distractions that break the Na-Cl bond.<br />

Look at sodium chloride (NaCl) one more time. Salt is a very strong bond when it is<br />

sitting on your table. It would be nearly impossible to break those ionic/electrovalent<br />

bonds. However, if you put that salt into some water (H2O), the bonds break very<br />

quickly. It happens easily because of the electrical attraction of the water. Now you have<br />

sodium (Na + ) and chlorine (Cl - ) ions floating around the solution. You should remember<br />

that ionic bonds are normally strong, but they are very weak in water.<br />

33


Neutron Madness<br />

We have already learned that ions are atoms that are<br />

either missing or have extra electrons. Let's say an atom<br />

is missing a neutron or has an extra neutron. That type of<br />

atom is called an isotope. An atom is still the same<br />

element if it is missing an electron. The same goes for<br />

isotopes. They are still the same element. They are just a<br />

little different from every other atom of the same element.<br />

For example, there are a lot of carbon (C) atoms in the<br />

Universe. The normal ones are carbon-12. Those atoms have 6 neutrons. There are a<br />

few straggler atoms that don't have 6. Those odd ones may have 7 or even 8 neutrons.<br />

As you learn more about chemistry, you will probably hear about carbon-14. Carbon-14<br />

actually has 8 neutrons (2 extra). C-14 is considered an isotope of the element carbon.<br />

Messing with the Mass<br />

If you have looked at a periodic table, you may have noticed that the atomic mass of<br />

an element is rarely an even number. That happens because of the isotopes. If you are<br />

an atom with an extra electron, it's no big deal. Electrons don't have much of a mass<br />

when compared to a neutron or proton.<br />

Atomic masses are calculated by figuring out the<br />

amounts of each type of atom and isotope there are in<br />

the Universe. For carbon, there are a lot of C-12, a<br />

couple of C-13, and a few C-14 atoms. When you<br />

average out all of the masses, you get a number that is a<br />

little bit higher than 12 (the weight of a C-12 atom). The<br />

average atomic mass for the element is actually 12.011.<br />

Since you never really know which carbon atom you are<br />

using in calculations, you should use the average mass<br />

of an atom.<br />

Bromine (Br), at atomic number 35, has a greater variety of isotopes. The atomic mass<br />

of bromine (Br) is 79.90. There are two main isotopes at 79 and 81, which average out<br />

to the 79.90amu value. The 79 has 44 neutrons and the 81 has 46 neutrons. While it<br />

won't change the average atomic mass, scientists have made bromine isotopes with<br />

masses from 68 to 97. It's all about the number of neutrons. As you move to higher<br />

atomic numbers in the periodic table, you will probably find even more isotopes for<br />

each element.<br />

34


Summary<br />

Atoms are the basic building blocks of everything. In atoms there are smaller particles. These<br />

Particles are called nucleus, proton, electron. Protons positive and electrons negative. Atoms<br />

that have too many electrons or protons are called ions. To get these atoms they may bond with an<br />

other to become neutral again. That is called electrovalence and on the periodic table elements on<br />

the<br />

left are positive and are called cations, elements on the right are negative and are called anions.<br />

There are two kinds of bonds covalent and electrovalent. Electovanent (ionic bonds) are weaker<br />

because of their attractions and electronic forces. An atom without or extra nucleus is called an<br />

isotope. Same thing goes for isotopes if it were an atom with less or more electrons they are not that<br />

different than the original atom. Isotopes can be found on the higher part of the periodic table.<br />

35


36


Electron Configuration<br />

Color the sublevel:<br />

s = Red<br />

d = Green<br />

p = Blue<br />

f = Orange<br />

Write in sublevels<br />

Write period, sublevel and super scripts.<br />

Ctrl Shift =<br />

gives you super scripts<br />

37


The Learning Goal for this assignment is:<br />

Relate properties of atoms and their position in the periodic table to the arrangements of their<br />

electrons.<br />

www.youtube.com/watch?v=jtYzEzykFdg<br />

www.youtube.com/watch?<br />

annotation_id=annotation_2076&feature=iv&src_vid=jtYzEzykFdg&v=cOlac8ruD_0<br />

www.youtube.com/watch?<br />

annotation_id=annotation_570977&feature=iv&src_vid=cOlac8ruD_0&v=lR2vqHZWb5A<br />

Notes Section<br />

3p<br />

n=f-2<br />

n=d-1<br />

n=p<br />

n=s<br />

For abbreviated method start at a noble gas<br />

Poly rule says they have pairs and go opposite ways<br />

Huns rule says they fill the ones with the same spin first<br />

There cant be arrows facing the same way<br />

38


Electron Configuration<br />

In order to write the electron configuration for an atom you must know the 3 rules of<br />

electron configurations.<br />

1. Aufbau<br />

Notation<br />

nO e<br />

where<br />

n is the energy level<br />

O is the orbital type (s, p, d, or f)<br />

e is the number of electrons in that orbital shell<br />

Principle<br />

electrons will first occupy orbitals of the lowest energy level<br />

2. Hund rule<br />

when electrons occupy orbitals of equal energy, one electron enters each orbital until<br />

all the orbitals contain one electron with the same spin.<br />

3. Pauli exclusion principle<br />

an orbital contains a maximum of 2 electrons and<br />

paired electrons will have opposite spin<br />

39


In the space below, write the unabbreviated electron configurations of the following elements:<br />

1S 2 2S 2 2p 6<br />

3S 1<br />

1) sodium ________________________________________________<br />

2) iron ________________________________________________<br />

3) bromine ________________________________________________<br />

4) barium ________________________________________________<br />

5) neptunium ________________________________________________<br />

In the space below, write the abbreviated electron configurations of the following elements:<br />

6) cobalt ________________________________________________<br />

7) silver ________________________________________________<br />

8) tellurium ________________________________________________<br />

9) radium ________________________________________________<br />

10) lawrencium ________________________________________________<br />

Determine what elements are denoted by the following electron configurations:<br />

sulfur<br />

11) 1s²s²2p⁶3s²3p⁴ ____________________<br />

12) 1s²2s²2p⁶3s²3p⁶4s²3d¹⁰4p⁶5s¹ ____________________<br />

Antimony<br />

13) [Kr] 5s²4d¹⁰5p³ ____________________<br />

Osimius<br />

14) [Xe] 6s²4f¹⁴5d⁶ ____________________<br />

Einstein<br />

ium<br />

15) [Rn] 7s²5f¹¹ ____________________<br />

Identify the element or determine that it is not a valid electron configuration:<br />

16) 1s²2s²2p⁶3s²3p⁶4s²4d¹⁰4p⁵ ____________________<br />

17) 1s²2s²2p⁶3s³3d⁵ ____________________<br />

18) [Ra] 7s²5f⁸ ____________________<br />

19) [Kr] 5s²4d¹⁰5p⁵ ____________________<br />

20) [Xe] ____________________<br />

1S 2 2S 2 2p 6 3S 2 3p 6 4S 2 3D 6<br />

1S 2 2 6 2 6 2 14 6 2 10 6<br />

2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 2<br />

2<br />

{Ar} 4s<br />

{Kr} 5s 2<br />

3d<br />

7<br />

4d 9<br />

{Kr} 5s 2 4d 10 5p 6<br />

{Rn} 7s 2<br />

{Rn} 7s<br />

2<br />

5f 14 6d<br />

5<br />

not a noble gas<br />

Iodine<br />

not exsistent<br />

{xe is its own configuration}<br />

Rubidium<br />

4d makes it wrong<br />

1)sodium 1s 2 2s 2 2p 6 3s 1 2)iron 1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 6<br />

3)bromine 1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 10 4p 5 4)barium 1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 10 4p 6 5s 2 4d 10 5p 6 6s 2<br />

5)neptunium 1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 10 4p 6 5s 2 4d 10 5p 6 6s 2 4f 14 5d 10 6p 6 7s 2 5f 5 6)cobalt [Ar] 4s 2 3d 7<br />

7)silver [Kr] 5s 2 4d 9 8)tellurium[Kr] 5s 2 4d 10 5p 4<br />

9)radium [Rn] 7s 2 10)lawrencium[Rn] 7s 2 5f 14 6d 1<br />

1s 2 2s 2 2p 6 3s 2 3p 4 sulfur 1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 10 4p 6 5s 1 rubidium<br />

[Kr] 5s 2 4d 10 5p 3 antimony [Xe] 6s 2 4f 14 5d 6 osmium<br />

[Rn] 7s 2 5f 11 einsteinium 1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 4d 10 4p 5 not valid (take a look at “4d”)<br />

1s 2 2s 2 2p 6 3s 3 3d 5 not valid (3p comes after 3s) [Ra] 7s 2 5f 8 not valid (radium isn’t a noble gas)<br />

[Kr] 5s 2 4d 10 5p 5 valid iodine<br />

20)[Xe] not valid (an element can’t be its own electron configuration)<br />

40


{Sr} Stuontrum<br />

{Rh} Rohdium<br />

{Si} Silicon<br />

Krrypton<br />

{As} Atsente<br />

Radon<br />

There {Xe} areXenon<br />

two arrows going up in 2s<br />

{xo}<br />

{xo}{xo}{x} {x} {}<br />

{Ar}<br />

{xo}<br />

{Xe} [xo] [xo][xo][xo][xo][xo][xo][xo] [xo]<br />

{Rn} [xo] [x ][x ][x ][x ][x ][x ] [ ]<br />

[He] [xo] [xo][x ][x ]<br />

[Ar] [x ]<br />

41


Create groups for these Scientist and explain your groupings<br />

(use the information you got from your research)<br />

The scientist are sorted due to the importance of their discoveries that they had on the Atomic<br />

Theory.<br />

Radio Activity: Antonie Henri Becquerel, Glenn Seaborg, Marir & Pierri Curie<br />

Theories:<br />

Louis de Bargoilie, Democritus, John Dalton<br />

Periodic Table:<br />

Dmitri Mendeleev, J.W. Dobereiner, Lothar Meyer<br />

Models:<br />

Niels Bohr, Hantaro Nagaoka, Erwin Shodinger<br />

Electrons:<br />

Alpha Particle:<br />

J.J. Thomson, Eugene Goldstien, Robert Millikan<br />

James Chadwick, Ernst Rutherford<br />

42


Research the Scientist and summarize their contributions to the Atomic Theory<br />

Antoine Henri Becquerel<br />

Antoine discovered radio activity in his experiments with different substances as well as discovery the x-ray. Further contrubutions include the<br />

deflection<br />

of beta particles<br />

Niels Bohr<br />

Niels Bohr contributions to the understanding the structure of atoms and early development of quantum mechanics. He created the Bohr's model<br />

of the<br />

of the liquid drop model<br />

Louis de Barogilie<br />

Louis researched quantum theory and predicted the wave nature of<br />

electrons.<br />

Glenn Seaborg<br />

Gleen has isolated many radioactive elements and formulated the actin concept He also identified 8 elements one being named after<br />

him.<br />

Hantaro Nagaoka<br />

Contributed greatly to the Atomic model. He was the first to state that negatively charged electrons were located outside the atom<br />

and orbit<br />

around it. It was called the saturn model.<br />

Democritus<br />

Created the Atomic theory. The universe and all matter that obeyed the following principles. Everything is composed of atoms, which are<br />

physical<br />

but not geometrically invisible.<br />

Marie and Pierre Curie<br />

Marie and Pierre worked on radioactivity discovering 2 elements Radium and<br />

Polonium.<br />

Eugene Goldstein<br />

Eugene concluded that in addition to electrons or cathode rays, that travel from the negatively charged cathode towards the positively charged<br />

anode.<br />

Dmitri Mendeleev<br />

Dmitri contributed greatly to the periodic table by putting them into rows based on the atomic mass and columns based on chemical and<br />

physical<br />

properties.<br />

J.J. Thomson<br />

JJ discovered electrons by experimenting with a Crookes, or cathode ray, tube. He also demonstrated that cathode rays were negatively<br />

charged<br />

James Chadwick<br />

James discovered neutrons by hitting berylum atoms with alpha<br />

particles.<br />

Erwin Shrodinger<br />

Erwin contributed to the wave theory of matter and contributed to other fundamentals of quantum<br />

mechanics.<br />

John Dalton<br />

John contributed to the atomic theory. He proposed when atoms combined in a one ratio, it must be presumed to be a binary one,<br />

unless<br />

some cause to appear to the contray<br />

Lothar Meyer<br />

One of the first to creat the periodic<br />

table.<br />

Robert Millikan<br />

Robert Millikan did an oil drop experiment help to quantify the charge of an electron, which contributed to the understanding of the<br />

structure<br />

and atomic theory.<br />

J.W. Dobereiner<br />

J.W observation on the similarities between elements which contributed to the periodic system of<br />

elements.<br />

Ernest Rutherford<br />

Ernest discovered alpha and beta rays,set forth the law of radioactive decay, and alpha<br />

particles.<br />

43


The Learning Goal for this Assignment is<br />

Relate properties of atoms and their positions in the periodic table to the<br />

arrangement of their electrons<br />

Alkali Metals<br />

The elements in group 1A<br />

Alkali Earth Metals<br />

The elements in Group 2A<br />

Transitional Metals<br />

Are the Group B elements that are usually displayed in the main body of the<br />

Periodic Table.<br />

Inter Transitional Metals<br />

Elements appear below the main body of the Periodic Table.<br />

Metals<br />

Generally good conductor of heat and electric current<br />

Metalloids<br />

Generally has properties that are similar to those of metals and nonmetals.<br />

Non Metals<br />

Are poor conductors of heat and electric current.<br />

Noble Gases<br />

The Elements in the group 8A of the Periodic Table.<br />

44


Using Wikipedia, define the 8 categories of elements on the<br />

left page.<br />

Color your periodic table similar to the one on<br />

pages 168—169 of your book.<br />

alkali metals<br />

alkaline metals<br />

other metals<br />

transitional metals<br />

lanthanoids<br />

metalloids<br />

non metals<br />

halogens<br />

noble gases<br />

unknown elements<br />

actinoids<br />

45


46<br />

Atomic Size<br />

Define Atomic Size: The size of the atom determined by the size or mass of nucleus and number of energy of<br />

levels<br />

Explanation:<br />

As the nucelus gets bigger the mass gets bigger and atom gets<br />

smaller<br />

More energy levels<br />

the smaller it gets<br />

Electrons pull<br />

closer<br />

The larger the energy level the more the atom decreases. For example as I increase the nucleus I<br />

decrease the size of the atom.As we increase in mass we decrease in size. The size of the atom as we<br />

top to bottom we add energy levels. The size increases from right to left we increase the size of the mass<br />

making the gravitational pull stronger, keeping electrons closer.


Define Ionization Energy:<br />

Ionization Energy<br />

Ionization is how hard is is to take away electrons. The more energy it takes<br />

there is more electrons.<br />

Explanation:<br />

The bigger the mass the harder to take away electrons because the gravitational pull is<br />

much stronger.<br />

47


Define Electronegativity:<br />

The ability to attract electrons when an atoms<br />

is in a compound.<br />

Electronegativity<br />

The more mass more electronegativity<br />

Explanation:<br />

Its value decreases from top to bottom within each group. Values tend to increase from<br />

left to right across a period. Electromagnetically values due to transition to metals that aren't<br />

regular.<br />

48


Ion Size<br />

Define Ion Size:<br />

Electrically charged atoms. the size of the ion in comparison to the size of the element<br />

atom.<br />

Cation<br />

Anions<br />

Explanation:<br />

Ionic size tend to increase from top to bottom within a group. The size of the cations and<br />

anions decrease from left to right.across a period. During reactions between metals and<br />

non metals, metal atoms tend to lose electrons and nonmetals tend to gain electrons. Cations<br />

anions get larger.<br />

49


Unit 3<br />

Chapter 25 Nuclear Chemistry<br />

The students will learn what happens when an unstable<br />

nucleus decays and how nuclear chemistry affects their lives.<br />

Explore the theory of electromagnetism by comparing and contrasting the<br />

different parts of the electromagnetic spectrum in terms of wavelength,<br />

frequency, and energy, and relate them to phenomena and applications.<br />

Students will be able to compare and contrast the different parts of the<br />

electromagnetic spectrum.<br />

Students will be able to apply knowledge of the EMS to real world phenomena.<br />

Students will be able to quantitatively compare the relationship between energy,<br />

wavelength, and frequency of the EMS.<br />

amplitude<br />

wavelength<br />

frequency<br />

hertz<br />

electromagnetic radiation<br />

photon<br />

Planck’s constant<br />

Explain and compare nuclear reactions (radioactive decay, fission and<br />

fusion), the energy changes associated with them and their associated<br />

safety issues.<br />

Students will be able to compare and contrast fission and fusion reactions.<br />

Students will be able to complete nuclear decay equations to identify the type of<br />

decay.<br />

Students will participate in activities to calculate half-life.<br />

radioactivity<br />

nuclear radiation<br />

alpha particle<br />

beta particle<br />

gamma ray<br />

positron<br />

½ life<br />

transmutation<br />

fission<br />

fusion<br />

50


Chapter 7<br />

Ionic and Metallic Bonding<br />

The students will learn how ionic compounds form and how<br />

metallic bounding affects the properties of metals.<br />

Compare the magnitude and range of the four fundamental forces<br />

(gravitational, electromagnetic, weak nuclear, strong nuclear).<br />

Students will compare/contrast the characteristics of each fundamental force.<br />

gravity<br />

electromagnetic<br />

strong<br />

weak<br />

Distinguish between bonding forces holding compounds together and other<br />

attractive forces, including hydrogen bonding and van der Waals forces.<br />

Students will be able to compare/contrast traits of ionic and covalent bonds.<br />

Students will be able to compare/contrast basic attractive forces between<br />

molecules.<br />

Students will be able to predict the type of bond or attractive force between<br />

atoms or molecules.<br />

ionic bond<br />

covalent bond<br />

metallic bond<br />

polar covalent bond<br />

hydrogen bond<br />

van der Waals forces<br />

London dispersion forces<br />

Chapter 8<br />

Covalent Bonding<br />

The students will learn how molecular bonding is different<br />

than ionic bonding and electrons affect the shape of a<br />

molecule and its properties.<br />

Interpret formula representations of molecules and compounds in terms of<br />

composition and structure.<br />

Students will be able to interpret chemical formulas in terms of # of atoms.<br />

Students will be able to differentiate between ionic and molecular compounds.<br />

Students will be able to list various VSEPR shapes and identify examples of<br />

each.<br />

Students will be able to predict shapes of various compounds.<br />

Molecule<br />

empirical formula<br />

Atom<br />

Electron<br />

Element<br />

Compound<br />

51


Name ____________________<br />

Britney Contreras<br />

Go to the web site www.darvill.clara.net/emag<br />

1. Click on “How the waves fit into the spectrum” and fill in this table:<br />

>: look out for the<br />

RED words on the web site!<br />

Low __________, frequency Long wavelength<br />

High frequency, Short ______________<br />

wavelenght<br />

Radio Waves<br />

microwaves Infra wavs Visible light Ultra violest X-rays<br />

Gamma rays<br />

transmitter<br />

2. Click on “Radio waves”. They are used for _______________________<br />

Phones speed radar<br />

3. Click on “Microwaves”. They are used for cooking, mobile _________, _______ cameras and _________.<br />

4. Click on “Infra-red”. These waves are given off by _____ IR _________. waves They are used for remote controls,<br />

cameras in police ____________ heliocopters , and alarm systems.<br />

5. Click on “Visible Light”. This is used in DVD ___ players and _______ laser printers, and for seeing where we’re going.<br />

6. “UV” stands for “ ________ Ultra ___________”. Violet This can damage the _________ retnia in your eyes, and cause<br />

sunburn and even _______ skin cancer. Its uses include detecting forged ______ bank _______. notes<br />

7. X-rays are used to see inside people, and for _________ airport security.<br />

8. Gamma rays are given off by some ________________ radioactive substances. We can use them to kill ________ cancer cells,<br />

which is called R_______________ adiotherpay .<br />

9. My Quiz score is ____%. 100<br />

52


_____ Frequency _____ frequency,<br />

Short wavelength ______ Wavelength<br />

10. Name ________________________________<br />

Go to the web site www.darvill.clara.net/emag<br />

Name How they’re made Uses Dangers<br />

Gamma rays<br />

X-rays<br />

Ultra- violet<br />

Visible light<br />

Infra rays<br />

Given off by stars and<br />

radioactive<br />

substances.<br />

Given off by stars and X-ray<br />

machines by firing beams of<br />

electrons<br />

at a target.<br />

Given off by the sun and made<br />

by<br />

special lamps.<br />

Given off by anything that is hot<br />

enough to glow<br />

Infra Red waves are also given off by<br />

stars,lamps, flames and anything else<br />

that's warm - including you & lastly<br />

they're given off by hot objects<br />

use to kill cancer cells, sterilise<br />

food<br />

and sterilise medical equipment.<br />

Used to see inside people, airport<br />

security, and astronomer telescopes.<br />

Used for suntan, forged bank notes,<br />

kill microbes, sterilise (food &drug),<br />

and for the body to produce vitamin<br />

D<br />

We use light to see things & used in<br />

Compact Disc & DVD players<br />

Used for Remotes,<br />

weather forecasting<br />

helicopter cameras and<br />

alarm systems<br />

Cell damage and<br />

causes<br />

mutations in growing<br />

tissue.<br />

Can cause cell<br />

damage<br />

and give cancer.<br />

Can cause Damage to<br />

the<br />

retina, sun burn, and<br />

skin<br />

cancer.<br />

Too much light can damage<br />

the retina in your eye &<br />

large doses of UV cause<br />

sunburn and even skin<br />

cancer<br />

The danger to people<br />

from too much Infra-Red<br />

radiation is very simple -<br />

overheating.<br />

Microwaves<br />

made by various types of transmitter<br />

Cooks' many types of food,<br />

mobile phones, Wifi & used by<br />

fixed traffic speed camera, and for<br />

radar<br />

Prolonged exposure to<br />

significant levels of<br />

microwaves is known<br />

to cause "cataracts"<br />

Radio waves<br />

Radio waves are made by various<br />

types of transmitter<br />

Used mainly for communications<br />

Large doses of radio<br />

waves are believed to<br />

cause cancer, leukemia<br />

and other disorders<br />

53


Learning Goal for this section:<br />

Explain and compare nuclear reactions (radioactive decay, fission and fusion),<br />

the energy changes associated with them and their associated safety issues.<br />

Notes Section:<br />

An isotope is an element that has different variations of its mass. -Carbon 14 - Has a<br />

radio active isotope. Its total mass to determine if its radio active -Because the<br />

protons and neutrons are not the same, it is radioactive. -All living things have<br />

carbon, and most likley has carbon 14 -Carbonation is used to find out the age Alpha<br />

particles It can harm the germinal layer, but if consumed, it can become cancerous<br />

Goes down by 2 Beta Particles goes down by 1 e negative e- p6 n 8 14.6C --- 14/7 N<br />

7p 7n + e- positive e+ 8/5 Boron --- 8/4 Be + e+ Be is now neutral. Radition is high<br />

and can only be stopped with something like plastic Gamma Radiation Something<br />

densely packed, can be the only thing to stop gamma radiation (LEAD) Gamma is<br />

just energy, eating something with radiation can cause cancer and barium, can coat<br />

your stomach, and this can help diagnose what is your problem. -Half Life is the rate<br />

of what these things decay as it decays it is actually turning into something else.<br />

54


The Nucleus<br />

A typical model of the atom is called the Bohr Model, in<br />

honor of Niels Bohr who proposed the structure in 1913. The Bohr atom consists of a central nucleus<br />

composed of neutrons and protons, which is surrounded by electrons which “orbit” around the nucleus.<br />

Protons carry a positive charge of one and have a mass of about 1 atomic mass unit or amu (1 amu =1.7x10-<br />

27 kg, a very, very small number). Neutrons are electrically “neutral” and also have a mass of about 1 amu. In<br />

contrast electron carry a negative charge and have mass of only 0.00055 amu. The number of protons in a<br />

nucleus determines the element of the atom. For example, the number of protons in uranium is 92 and the<br />

number in neon is 10. The proton number is often referred to as Z.<br />

Atoms with different numbers of protons are called elements, and are arranged in the periodic table with<br />

increasing Z.<br />

Atoms in nature are electrically neutral so the number of electrons orbiting the nucleus equals the number of<br />

protons in the nucleus.<br />

Neutrons make up the remaining mass of the nucleus and provide a means to “glue” the protons in place.<br />

Without neutrons, the nucleus would split apart because the positive protons would repel each other. Elements<br />

can have nucleii with different numbers of neutrons in them. For example hydrogen, which normally only has<br />

one proton in the nucleus, can have a neutron added to its nucleus to from deuterium, ir have two neutrons<br />

added to create tritium, which is radioactive. Atoms of the same element which vary in neutron number are<br />

called isotopes. Some elements have many stable isotopes (tin has 10) while others have only one or two. We<br />

express isotopes with the nomenclature Neon-20 or 20 Ne 10, with twenty representing the total number of<br />

neutrons and protons in the atom, often referred to as A, and 10 representing the number of protons (Z).<br />

Alpha Particle<br />

Decay<br />

Alpha decay is a radioactive process in which a<br />

particle with two neutrons and two protons is<br />

ejected from the nucleus of a radioactive atom. The particle is identical to the nucleus of a helium atom.<br />

Alpha decay only occurs in very heavy elements such as uranium, thorium and radium. The nuclei of these<br />

atoms are very “neutron rich” (i.e. have a lot more neutrons in their nucleus than they do protons) which makes<br />

emission of the alpha particle possible.<br />

After an atom ejects an alpha particle, a new parent atom is formed which has two less neutrons and two less<br />

protons. Thus, when uranium-238 (which has a Z of 92) decays by alpha emission, thorium-234 is created<br />

(which has a Z of 90).<br />

Because alpha particles contain two protons, they have a positive charge of two. Further, alpha particles are<br />

very heavy and very energetic compared to other common types of radiation. These characteristics allow alpha<br />

particles to interact readily with materials they encounter, including air, causing many ionizations in a very short<br />

distance. Typical alpha particles will travel no more than a few centimeters in air and are stopped by a sheet of<br />

paper.<br />

55


Beta Particle Decay<br />

Beta decay is a radioactive process in which an electron is emitted from the nucleus of a radioactive<br />

atom Because this electron is from the nucleus of the atom, it is called a beta particle to distinguish it<br />

from the electrons which orbit the atom.<br />

Like alpha decay, beta decay occurs in isotopes which are “neutron rich” (i.e. have a lot more<br />

neutrons in their nucleus than they do protons). Atoms which undergo beta decay are located below<br />

the line of stable elements on the chart of the nuclides, and are typically produced in nuclear reactors.<br />

When a nucleus ejects a beta particle, one of the neutrons in the nucleus is transformed into a proton.<br />

Since the number of protons in the nucleus has changed, a new daughter atom is formed which has<br />

one less neutron but one more proton than the parent. For example, when rhenium-187 decays<br />

(which has a Z of 75) by beta decay, osmium-187 is created (which has a Z of 76). Beta particles<br />

have a single negative charge and weigh only a small fraction of a neutron or proton. As a result, beta<br />

particles interact less readily with material than alpha particles. Depending on the beta particles<br />

energy (which depends on the radioactive atom), beta particles will travel up to several meters in air,<br />

and are stopped by thin layers of metal or plastic.<br />

Positron emission or beta plus decay (β+ decay) is a subtype of radioactive decay called beta decay,<br />

in which a proton inside a radionuclide nucleus is converted into a neutron while releasing a positron<br />

and an electron neutrino (νe). Positron emission is mediated by the weak force.<br />

An example of positron emission (β+ decay) is shown with magnesium-23 decaying into sodium-23:<br />

23 Mg12 → 23 Na11 + e +<br />

Because positron emission decreases proton number relative to neutron number, positron decay<br />

happens typically in large "proton-rich" radionuclides. Positron decay results in nuclear transmutation,<br />

changing an atom of one chemical element into an atom of an element with an atomic number that is<br />

less by one unit.<br />

Positron emission should not be confused with electron emission or beta minus decay (β− decay),<br />

which occurs when a neutron turns into a proton and the nucleus emits an electron and an<br />

antineutrino.<br />

56


Gamma<br />

Radiation<br />

After a decay reaction, the nucleus is often in an<br />

“excited” state. This means that the decay has<br />

resulted in producing a nucleus which still has<br />

excess energy to get rid of. Rather than emitting another beta or alpha particle, this energy is lost by<br />

emitting a pulse of electromagnetic radiation called a gamma ray. The gamma ray is identical in<br />

nature to light or microwaves, but of very high energy.<br />

Like all forms of electromagnetic radiation, the gamma ray has no mass and no charge. Gamma rays<br />

interact with material by colliding with the electrons in the shells of atoms. They lose their energy<br />

slowly in material, being able to travel significant distances before stopping. Depending on their initial<br />

energy, gamma rays can travel from 1 to hundreds of meters in air and can easily go right through<br />

people.<br />

It is important to note that most alpha and beta emitters also emit gamma rays as part of their decay<br />

process. However, their is no such thing as a “pure” gamma emitter. Important gamma emitters<br />

including technetium-99m which is used in nuclear medicine, and cesium-137 which is used for<br />

calibration of nuclear instruments.<br />

Half Life<br />

Half-life is the time required for the quantity of a<br />

radioactive material to be reduced to one-half its<br />

original value.<br />

All radionuclides have a particular half-life, some<br />

of which a very long, while other are extremely<br />

short. For example, uranium-238 has such a<br />

long half life, 4.5x109 years, that only a small fraction has decayed since the earth was formed. In<br />

contrast, carbon-11 has a half-life of only 20 minutes. Since this nuclide has medical applications, it<br />

has to be created where it is being used so that enough will be present to conduct medical studies.<br />

57


The Learning Goal for this assignment is:<br />

Distinguish between bonding forces<br />

holding compounds together and<br />

other attractive forces , including<br />

hydrogen bonding and van der Waals<br />

forces.<br />

Introduction to Ionic Compounds<br />

Those molecules that consist of charged ions with opposite charges are called IONIC. These ionic<br />

compounds are generally solids with high melting points and conduct electrical current. Ionic<br />

compounds are generally formed from metal and a non-metal elements. See Ionic Bonding below.<br />

Ionic Compound Example<br />

For example, you are familiar with the fairly benign unspectacular behavior of common white<br />

crystalline table salt (NaCl). Salt consists of positive sodium ions (Na + ) & negative chloride ions (Cl - ).<br />

On the other hand the element sodium is a silvery gray metal composed of neutral atoms which react<br />

vigorously with water or air. Chlorine as an element is a neutral greenish-yellow, poisonous, diatomic<br />

gas (Cl2).<br />

The main principle to remember is that ions are completely different in physical and chemical<br />

properties from the neutral atoms of the elements.<br />

The notation of the + and - charges on ions is very important as it conveys a definite meaning.<br />

Whereas elements are neutral in charge, IONS have either a positive or negative charge depending<br />

upon whether there is an excess of protons (positive ion) or excess of electrons (negative ion).<br />

Formation of Positive Ions<br />

Metals usually have 1-4 electrons in the outer energy level. The electron arrangement of a rare gas is<br />

most easily achieved by losing the few electrons in the newly started energy level. The number of<br />

electrons lost must bring the electron number "down to" that of a prior rare gas.<br />

How will sodium complete its octet?<br />

First examine the electron arrangement of the atom. The atomic number is eleven, therefore, there<br />

are eleven electrons and eleven protons on the neutral sodium atom. Here is the Bohr diagram and<br />

Lewis symbol for sodium:<br />

58


This analysis shows that sodium has only one electron in its outer level. The nearest rare gas is neon<br />

with 8 electron in the outer energy level. Therefore, this electron is lost so that there are now eight<br />

electrons in the outer energy level, and the Bohr diagrams and Lewis symbols for sodium ion and<br />

neon are identical. The octet rule is satisfied.<br />

Ion Charge?<br />

What is the charge on sodium ion as a result of losing one electron? A comparison of the atom and<br />

the ion will yield this answer.<br />

Sodium Atom<br />

Sodium Ion<br />

11 p+ to revert to 11 p + Protons are identical in<br />

12 n an octet 12 n<br />

the atom and ion.<br />

Positive charge is<br />

11 e- lose 1 electron 10 e-<br />

caused by lack of<br />

0 charge + 1 charge<br />

electrons.<br />

Formation of Negative Ions<br />

How will fluorine complete its octet?<br />

First examine the electron arrangement of the atom. The atomic number is nine, therefore, there are<br />

nine electrons and nine protons on the neutral fluorine atom. Here is the Bohr diagram and Lewis<br />

symbol for fluorine:<br />

This analysis shows that fluorine already has seven electrons in its outer level. The nearest rare gas<br />

is neon with 8 electron in the outer energy level. Therefore only one additional electron is needed to<br />

complete the octet in the fluorine atom to make the fluoride ion. If the one electron is added, the Bohr<br />

diagrams and Lewis symbols for fluorine and neon are identical. The octet rule is satisfied.<br />

59


Ion Charge?<br />

What is the charge on fluorine as a result of adding one electron? A comparison of the atom and the<br />

ion will yield this answer.<br />

Fluorine Atom Fluoride Ion *<br />

9 p+ to complete 9 p + Protons are identical in<br />

10 n octet 10 n<br />

9 e- add 1 electron 10 e-<br />

0 charge - 1 charge<br />

the atom and ion.<br />

Negative charge is<br />

caused by excess<br />

electrons<br />

* The "ide" ending in the name signifies a simple negative ion.<br />

Summary Principle of Ionic Compounds<br />

An ionic compound is formed by the complete transfer of electrons from a metal to a nonmetal and<br />

the resulting ions have achieved an octet. The protons do not change. Metal atoms in Groups 1-3<br />

lose electrons to non-metal atoms with 5-7 electrons missing in the outer level. Non-metals gain 1-4<br />

electrons to complete an octet.<br />

Octet Rule<br />

Elemental atoms generally lose, gain, or share electrons with other atoms in order to achieve the<br />

same electron structure as the nearest rare gas with eight electrons in the outer level.<br />

The proper application of the Octet Rule provides valuable assistance in predicting and explaining<br />

various aspects of chemical formulas.<br />

Introduction to Ionic Bonding<br />

Ionic bonding is best treated using a simple<br />

electrostatic model. The electrostatic model<br />

is simply an application of the charge<br />

principles that opposite charges attract and<br />

similar charges repel. An ionic compound<br />

results from the interaction of a positive and<br />

negative ion, such as sodium and chloride in<br />

common salt.<br />

The IONIC BOND results as a balance<br />

between the force of attraction between<br />

opposite plus and minus charges of the ions<br />

and the force of repulsion between similar<br />

negative charges in the electron clouds. In<br />

crystalline compounds this net balance of<br />

forces is called the LATTICE ENERGY.<br />

Lattice energy is the energy released in the<br />

formation of an ionic compound.<br />

DEFINITION: The formation of an IONIC<br />

BOND is the result of the transfer of one or<br />

more electrons from a metal onto a nonmetal.<br />

60


Metals, with only a few electrons in the outer energy level, tend to lose electrons most readily. The<br />

energy required to remove an electron from a neutral atom is called the IONIZATION POTENTIAL.<br />

Energy + Metal Atom ---> Metal (+) ion + e-<br />

Non-metals, which lack only one or two electrons in the outer energy level have little tendency to lose<br />

electrons - the ionization potential would be very high. Instead non-metals have a tendency to gain<br />

electrons. The ELECTRON AFFINITY is the energy given off by an atom when it gains electrons.<br />

Non-metal Atom + e- --- Non-metal (-) ion + energy<br />

The energy required to produce positive ions (ionization potential) is roughly balanced by the energy<br />

given off to produce negative ions (electron affinity). The energy released by the net force of<br />

attraction by the ions provides the overall stabilizing energy of the compound.<br />

Notes Section:<br />

Na - Cl - Sodium - Chlorine Metal and Non Metal make an Ionic bond. Sodium is going to<br />

give up the 1 electron to chlorine making Na1+ and making Cl1- Ions are the 1+ and 2- All<br />

electron configurations looks like a noble gas To make an ionic bond, you need a metal and<br />

a non meta<br />

61


The Learning Goal for this assignment is:<br />

Introduction to Covalent Bonding:<br />

Bonding between non-metals consists of two electrons shared between two atoms. Using the Wave<br />

Theory, the covalent bond involves an overlap of the electron clouds from each atom. The electrons<br />

are concentrated in the region between the two atoms. In covalent bonding, the two electrons shared<br />

by the atoms are attracted to the nucleus of both atoms. Neither atom completely loses or gains<br />

electrons as in ionic bonding.<br />

There are two types of covalent bonding:<br />

1. Non-polar bonding with an equal sharing of electrons.<br />

The students will learn how molecular<br />

bonding is different than ionic bonding and<br />

electrons affect the shape of a molecule<br />

and its properties.<br />

2. Polar bonding with an unequal sharing of electrons. The number of shared electrons depends on<br />

the number of electrons needed to complete the octet.<br />

NON-POLAR BONDING results when two identical non-metals equally share electrons between<br />

them. One well known exception to the identical atom rule is the combination of carbon and hydrogen<br />

in all organic compounds.<br />

Hydrogen<br />

The simplest non-polar covalent molecule is hydrogen. Each hydrogen<br />

atom has one electron and needs two to complete its first energy level.<br />

Since both hydrogen atoms are identical, neither atom will be able to<br />

dominate in the control of the electrons. The electrons are therefore<br />

shared equally. The hydrogen covalent bond can be represented in a<br />

variety of ways as shown here:<br />

The "octet" for hydrogen is only 2 electrons since the nearest rare gas is<br />

He. The diatomic molecule is formed because individual hydrogen atoms<br />

containing only a single electron are unstable. Since both atoms are<br />

identical a complete transfer of electrons as in ionic bonding is<br />

impossible.<br />

Instead the two hydrogen atoms SHARE both electrons equally.<br />

Oxygen<br />

Molecules of oxygen, present in about 20% concentration in air are<br />

also covalent molecules. See the graphic on the left of the Lewis Dot<br />

Structure.<br />

There are 6 electrons in the outer shell, therefore, 2 electrons are<br />

needed to complete the octet. The two oxygen atoms share a total of<br />

four electrons in two separate bonds, called double bonds.<br />

The two oxygen atoms equally share the four electrons.<br />

62


POLAR BONDING results when two different non-metals unequally share electrons between them.<br />

One well known exception to the identical atom rule is the combination of carbon and hydrogen in all<br />

organic compounds.<br />

The non-metal closer to fluorine in the Periodic Table has a greater tendency to keep its own electron<br />

and also draw away the other atom's electron. It is NOT completely successful. As a result, only<br />

partial charges are established. One atom becomes partially positive since it has lost control of its<br />

electron some of the time. The other atom becomes partially negative since it gains electron some of<br />

the time.<br />

Hydrogen Chloride<br />

Hydrogen Chloride forms a polar covalent molecule. The graphic<br />

on the left shows that chlorine has 7 electrons in the outer shell.<br />

Hydrogen has one electron in its outer energy shell. Since 8<br />

electrons are needed for an octet, they share the electrons.<br />

However, chlorine gets an unequal share of the two electrons,<br />

although the electrons are still shared (not transferred as in ionic<br />

bonding), the sharing is unequal. The electrons spends more of the<br />

time closer to chlorine. As a result, the chlorine acquires a "partial"<br />

negative charge. At the same time, since hydrogen loses the<br />

electron most - but not all of the time, it acquires a "partial" charge.<br />

The partial charge is denoted with a small Greek symbol for delta.<br />

Water<br />

Water, the most universal compound on all of the earth, has the property of<br />

being a polar molecule. As a result of this property, the physical and<br />

chemical properties of the compound are fairly unique.<br />

Dihydrogen Oxide or water forms a polar covalent molecule. The graphic on<br />

the left shows that oxygen has 6 electrons in the outer shell. Hydrogen has<br />

one electron in its outer energy shell. Since 8 electrons are needed for an<br />

octet, they share the electrons.<br />

Notes Section:<br />

1.Count valence electrons<br />

2.Find the central atom and bond the other atoms to it .Subtract the number of electrons in the<br />

bonds from the total. Add Lone pairs to the terminal atoms. Add Lone Pair to the central atom or<br />

double or triple bonds.<br />

3.Find the formal Charges.Try to get the charges as close as possible by moving electrons and<br />

bonds.<br />

Na 1+ N2- Na:N:Na Na2N<br />

Not always making double bonds will work<br />

Hydrogen needs 2<br />

63


C 2 H 6 O Ethanol CH 3 CH 2 O<br />

Step 1<br />

Find valence e- for all atoms. Add them together.<br />

C: 4 x 2 = 8<br />

H: 1 x 6 = 6<br />

O: 6<br />

Total = 20<br />

Step 2<br />

Find octet e- for each atom and add them together.<br />

C: 8 x 2 = 16<br />

H: 2 x 6 = 12<br />

O: 8<br />

Total = 36<br />

Step 3<br />

Subtract Step 1 total from Step 2.<br />

Gives you bonding e-.<br />

36 – 20 = 16e-<br />

Step 4<br />

Find number of bonds by diving the number in step 3 by 2<br />

(because each bond is made of 2 e-)<br />

16e- / 2 = 8 bond pairs<br />

These can be single, double or triple bonds.<br />

Step 5<br />

Determine which is the central atom<br />

Find the one that is the least electronegative.<br />

Use the periodic table and find the one farthest<br />

away from Fluorine or<br />

The one that only has 1 atom.<br />

64


Step 6<br />

Put the atoms in the structure that you think it will<br />

have and bond them together.<br />

Put Single bonds between atoms.<br />

Step 7<br />

Find the number of nonbonding (lone pairs) e-.<br />

Subtract step 3 number from step 1.<br />

20 – 16 = 4e- = 2 lone pairs<br />

Step 8<br />

Complete the Octet Rule by adding the lone<br />

pairs.<br />

Then, if needed, use any lone pairs to make<br />

double and triple bonds so that all atoms meet<br />

the Octet Rule.<br />

See Step 4 for total number of bonds.<br />

65


Linear<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

sp AX 2 None 180<br />

BeCl 2<br />

Cl<br />

Be<br />

Cl<br />

element bond lone pair<br />

C<br />

66


Trigonal Planer<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

sp 2 AX3 none 120<br />

BF 3<br />

F<br />

B<br />

Triangle<br />

planer<br />

F<br />

F<br />

element bond lone pair<br />

C<br />

67


Bent<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

sp 2 AX 2 E 1 116<br />

O 3<br />

O<br />

O O<br />

Trioxogen<br />

trioxide<br />

element bond lone pair<br />

C<br />

68


Tetahedral<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 AX 4 None 109.5<br />

phosphate<br />

PO 4<br />

3-<br />

O<br />

O<br />

P<br />

O<br />

O<br />

element bond lone pair<br />

C<br />

69


Trigonal Pyramidal<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 Ax 3 E 1 107<br />

Phropherus<br />

Trihydride<br />

PH 3<br />

H<br />

P<br />

H<br />

H<br />

element bond lone pair<br />

C<br />

70


Bent<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 Ax 2 E 2 104.5<br />

Dihydrogenoxide<br />

H 2 O<br />

H<br />

O<br />

H<br />

element bond lone pair<br />

C<br />

71


Trigonal Bi Pyramidal<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 d Ax 5 None 120/90<br />

Phospherous<br />

pentachoride<br />

PCl 5<br />

C l<br />

C l<br />

P<br />

C l<br />

C l<br />

C l<br />

element bond lone pair<br />

C<br />

72


‘T’ Shaped<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 d Ax 3 E 2 2 90<br />

Chlorine Trifloride<br />

ClF 3<br />

F<br />

Cl<br />

F<br />

F<br />

element bond lone pair<br />

C<br />

73


Octahdral<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 d 2 AX6 None 90<br />

Sulfure Hexafloride<br />

SF 6<br />

C<br />

C<br />

F<br />

S<br />

F<br />

F<br />

F<br />

element bond lone pair<br />

C<br />

74


Square Planar<br />

Molecular Geometry<br />

Orbital Equation Lone Pairs Angle<br />

Sp 3 d 2 AX 4 E 2 2 90<br />

Iodne<br />

trechachloride<br />

ICl 4<br />

-<br />

Cl<br />

Cl<br />

I<br />

Cl<br />

Cl<br />

element bond lone pair<br />

C<br />

75


76<br />

Orbitals Equation Lone Pairs Angle<br />

Name<br />

sp Ax2 O 180 Linear<br />

sp2 AX3 0 120 Trigonal Planar<br />

sp2 AX2E 1 116 Bent<br />

sp3 AX4 0 109.5 Tetrahedral<br />

sp3 AX3E 1 107 Trigonal Pyramidal<br />

sp3 AX3E2 2 105 Bent<br />

sp3d AX3 0 120/90 Trigonal Bipyramid<br />

sp3d AX3E2 2 90 T-shaped<br />

sp3 AX6 0 90 Octahedral<br />

sp4d2 AX4E2 0 90 Square Planer


Name Formula Charge<br />

Dichromate Cr₂O₇ 2-<br />

Sulfate SO₄ 2-<br />

Hydrogen Carbonate HCO₃ 1-<br />

Hypochlorite ClO 1-<br />

Phosphate PO₄ 3-<br />

Nitrite NO₂ 1-<br />

Chlorite ClO₂ 1-<br />

Dihydrogen phosphate H₂PO₄ 1-<br />

Chromate CrO₄ 2-<br />

Carbonate CO₃ 2-<br />

Hydroxide OH 1-<br />

Hydrogen phosphate HPO₄ 2-<br />

Ammonium NH₄ 1+<br />

Acetate C₂H₃O₂ 1-<br />

Perchlorate ClO₄ 1-<br />

Permanganate MnO₄ 1-<br />

Chlorate ClO₃ 1-<br />

Hydrogen Sulfate HSO₄ 1-<br />

Phosphite PO₃ 3-<br />

Sulfite SO₃ 2-<br />

Silicate SiO₃ 2-<br />

Nitrate NO₃ 1-<br />

Hydrogen Sulfite HSO₃ 1-<br />

Oxalate C₂O₄ 2-<br />

Cyanide CN 1-<br />

Hydronium H₃O 1+<br />

Thiosulfate S₂O₃ 2-<br />

77


Chapter 9<br />

Unit 4<br />

Chemical Names and Formulas<br />

The students will learn how the periodic table helps them<br />

determine the names and formulas of ions and compounds.<br />

Chapter 22 Hydrocarbon Compounds<br />

The student will learn how Hydrocarbons are named and the<br />

general properties of Hydrocarbons.<br />

Describe how different natural resources are produced and how their rates<br />

of use and renewal limit availability.<br />

<br />

<br />

<br />

Students will explore local, national, and global renewable and nonrenewable<br />

resources.<br />

Students will explain the environmental costs of the use of renewable and<br />

nonrenewable resources.<br />

Students will explain the benefits of renewable and nonrenewable resources.<br />

Nuclear reactors<br />

Natural gas<br />

Petroleum<br />

Refining<br />

Coal<br />

78


Chapter 23 Functional Groups<br />

The student will learn what effects functional groups have on<br />

organic compounds and how chemical reactions are used in<br />

organic compounds.<br />

Describe the properties of the carbon atom that make the diversity of carbon<br />

compounds possible.<br />

Identify selected functional groups and relate how they contribute to<br />

properties of carbon compounds.<br />

<br />

<br />

Students will identify examples of important carbon based molecules.<br />

Students will create 2D or 3D models of carbon molecules and explain why this<br />

molecule is important to life.<br />

covalent bond<br />

single bond<br />

double bond<br />

triple bond<br />

monomer<br />

polymer<br />

79


The students will learn how the periodic table helps them determine the names and formulas of ions and<br />

compounds.<br />

The students will learn how Hydrocarbons are named and the general properties of Hydrocarbons.<br />

http://www.bbc.co.uk/education/guides/zm9hvcw/revision<br />

homologous series is a family of hydrocarbons with similar<br />

chemical properties who share the same general formula.<br />

1. Alkalnes-end in ane and have many uses<br />

2. Alkenes-all end in –ene-carbon to carbon double bond<br />

3. Cycloalkanes-all end in –ane and begin with cyclo-contain only<br />

single bonds<br />

methane – (natural gas) cooking, heating<br />

propane – used in gas cylinders for BBQ etc<br />

octane – used in petrol for cars<br />

The general formula of the alkanes is Equation: {C_n}{H_{2n +<br />

2}}.<br />

80


81


Unit 5<br />

Chapter 10 Chemical Quantities<br />

The student will learn why the mole is important and how the<br />

molecular formula of a compound can be determined<br />

experimentally.<br />

Chapter 11 Chemical Reactions<br />

The students will learn how chemical reactions obey the law of<br />

conservation of mass and how they can predict the products<br />

of a chemical reaction.<br />

Characterize types of chemical reactions, for example: redox, acid-base,<br />

synthesis, and single and double replacement reactions.<br />

Students will be able to identify the type of chemical reaction that occurs.<br />

Students will be able to compare/contrast reactants and products of various<br />

types of chemical reactions.<br />

Students will be able to predict the product of various reactants.<br />

Students will be able to write balanced chemical equations for each type of<br />

reaction.<br />

Decomposition<br />

Combustion<br />

Redox<br />

Acid-Base<br />

Synthesis<br />

single-replacement<br />

double-replacement<br />

Differentiate between chemical and nuclear reactions.<br />

Students will compare/contrast chemical and nuclear reactions.<br />

fission<br />

fusion<br />

82


Chapter 12 Stoichiometry<br />

The students will learn how balanced chemical equations are<br />

used in stoichiometric calculations and how to calculate<br />

amounts of reactants and products in a chemical equation.<br />

Apply the mole concept and the law of conservation of mass to calculate<br />

quantities of chemicals participating in reactions.<br />

Students will be able to use a balanced equation to determine mole ratios.<br />

Students will be able to apply law of conservation of mass to chemical equations.<br />

Students will be able to calculate empirical and molecular formulas.<br />

Students will be able to calculate the % composition of a compound.<br />

Students will be able to calculate theoretical yield.<br />

Students will be able to calculate % error.<br />

Students will be able to calculate molar mass.<br />

Students will be able to perform stoichiometric calculations, including limiting<br />

reagents.<br />

mole<br />

Avogadro’ s number<br />

molar mass<br />

gram formula mass<br />

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www.youtube.com/watch?v=AsqEkF7hcII<br />

www.youtube.com/watch?v=tEn0N4R2dqA<br />

www.youtube.com/watch?v=Pft2CASl0M0<br />

www.youtube.com/watch?v=rwhJklbK8R0<br />

The Mole<br />

Mole is the measurement in chemistry. It is used to express<br />

the amount of a chemical substance.<br />

One mole is defined as the amount of substance of a system<br />

which contains as many entities like, atoms, molecules and<br />

ions as there are atoms in 12 grams of carbon - 12".<br />

Avogadro number: The number of the particles present in<br />

one mole of any substance is equal to 6.022x1023. This is<br />

called avogadro’s number or avogadro’s constant.<br />

*1 mole of water molecules represents 6.022 × 1023 water<br />

molecules.<br />

Amedeo Avogadro was an Italian physics professor who proposed in 1811 that equal volumes<br />

of different gases at the same temperature contain equal numbers of molecules.<br />

How many grams of carbon dioxide is 0.2 moles of CO2?<br />

1. # of g per mol CO2= 12.01 + [2*16.00]<br />

2. # of g per mol CO2 = 12.01+ 32.00<br />

3. # of g per mol CO2 = 44.01 g/mol<br />

As you increase the volume of gas you increase the atoms.<br />

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www.youtube.com/watch?v=BTRm8PwcZ3U<br />

www.youtube.com/watch?v=F9NkYSKJifs<br />

www.youtube.com/watch?v=xPdqEX_WMjo<br />

Molar Mass<br />

we use relative atomic masses of atoms for calculating the molecular mass of 1 mole of any<br />

molecular or ionic substances.<br />

Example: Molecular mass of H2SO4<br />

Atomic mass of Hydrogen = 1<br />

Atomic mass of sulfur = 32<br />

Atomic mass of oxygen = 16<br />

Molecular mass of H2SO4 = 2(Atomic mass of Hydrogen) + 1 (Atomic mass of sulfur) + 4<br />

(Atomic mass of oxygen)<br />

= 2×1 + 32 + 4× 16 = 98 u.<br />

The molar mass M is a physical property defined as the mass of a given substance<br />

The base SI unit for molar mass is g/mol<br />

Molar mass steps<br />

1. Use the chemical formula to define the # of each type of atom present in the<br />

compound<br />

2. Multiply the atomic weight of each element by the number of atoms of that<br />

element present in the compound<br />

3.Add it all together and put units of g/mol after the number<br />

The precision to which a molar mass is known depends on the precision of the<br />

atomic masses from which it was calculated.<br />

Molar Mass serves as a bridge between the mass of a material and the number of<br />

mols since it is no possible to measure the number of mols directly<br />

the smallest quantity of a substance will contain billions of atoms so chemists<br />

generally use the mol as a unit for the amount of substance<br />

Molar mass can also be calculated by multiplying the atomic mass in amu by the<br />

molar<br />

85


Categories of Reactions<br />

All chemical reactions can be placed into one of six categories. Here they are, in no<br />

particular order:<br />

1) Synthesis: A synthesis reaction is when two or more simple compounds combine to form a<br />

more complicated one. These reactions come in the general form of: A+B --> AB<br />

EX: H2+O2-->H2O<br />

One example of a synthesis reaction is the combination of iron and sulfur to form iron (II) sulfide:<br />

8 Fe + S8 ---> 8 FeS<br />

If two elements or very simple molecules combine with each other, it’s probably a synthesis reaction.<br />

The products will probably be predictable using the octet rule to find charges.<br />

2) Decomposition: A decomposition reaction is the opposite of a synthesis reaction - a<br />

complex molecule breaks down to make simpler ones. These reactions come in the general form:<br />

AB--> A+B<br />

EX:H2O-->H2+O2<br />

One example of a decomposition reaction is the electrolysis of water to make oxygen and hydrogen<br />

gas:<br />

2 H2O ---> 2 H2 + O2<br />

If one compound has an arrow coming off of it, it’s probably a decomposition reaction. The products<br />

will either be a couple of very simple molecules, or some elements, or both.<br />

3) Single displacement: This is when one element trades places with another element in a<br />

compound. These reactions come in the general form of:<br />

Note: C=Nonmetal A=metal<br />

B=metal<br />

One example of A+BC-->AC+B<br />

a single displacement reaction is when magnesium replaces hydrogen in water to<br />

make magnesium hydroxide and hydrogen gas:<br />

Mg + 2 H2O ---> Mg(OH)2 + H2<br />

If a pure element reacts with another compound (usually, but not always, ionic), it’s probably a single<br />

displacement reaction. The products will be the compounds formed when the pure element switches<br />

places with another element in the other compound.<br />

Important note: these reactions will only occur if the pure element on the reactant side of the equation<br />

is higher on the activity series than the element it replaces.<br />

86


4) Double displacement: This is when the anions and cations of two different molecules<br />

switch places, forming two entirely different compounds. These reactions are in the general form:<br />

AB+CD=AD+CB<br />

WE ALWAYS PUT METAL BE FORE NONMETALS<br />

One example of a double displacement reaction is the reaction of lead (II) nitrate with potassium<br />

iodide to form lead (II) iodide and potassium nitrate:<br />

Pb(NO3)2 + 2 KI ---> PbI2 + 2 KNO3<br />

If two ionic compounds combine, it’s probably a double displacement reaction. Switch the cations<br />

and balance out the charges to figure out what will be made.<br />

Important note: These reactions will only occur if both reactants are soluble in water and only one<br />

product is soluble in water.<br />

5) Acid-base: This is a special kind of double displacement reaction that takes place when an<br />

acid and base react with each other. The H + ion in the acid reacts with the OH - ion in the base,<br />

causing the formation of water. Generally, the product of this reaction is some ionic salt and water:<br />

ALWAYS HAS AN ABUNDANCE OF OXYGEN HA+BOH-->AB(TYPE OF SALT)+H2O<br />

THE OXYGEN IS USUALLY CATION<br />

One example of an acid-base reaction is the reaction of hydrobromic acid (HBr) with sodium<br />

hydroxide:<br />

HBr + NaOH ---> NaBr + H2O<br />

If an acid and a base combine, it’s an acid-base reaction. The products will be an ionic compound<br />

and water.<br />

6) Combustion: A combustion reaction is when oxygen combines with another compound to<br />

form water and carbon dioxide. These reactions are exothermic, meaning they produce heat. An<br />

example of this kind of reaction is the burning of napthalene: CH+O2-->H2O+CO<br />

ORGANIC+OXYGEN<br />

C10H8 + 12 O2 ---> 10 CO2 + 4 H2O<br />

If something that has carbon and hydrogen reacts with oxygen, it’s probably a combustion reaction.<br />

The products will be CO2 and H2O.<br />

Follow this series of questions. When you can answer "yes" to a question, then<br />

stop!<br />

1) Does your reaction have two (or more) chemicals combining to form one chemical? If yes, then it's<br />

a synthesis reaction<br />

2) Does your reaction have one large molecule falling apart to make several small ones? If yes, then<br />

it's a decomposition reaction<br />

3) Does your reaction have any molecules that contain only one element? If yes, then it's a single<br />

displacement reaction<br />

4) Does your reaction have water as one of the products? If yes, then it's an acid-base reaction<br />

5) Does your reaction have oxygen as one of it's reactants and carbon dioxide and water as<br />

products? If yes, then it's a combustion reaction<br />

6) If you haven't answered "yes" to any of the questions above, then you've got a double<br />

displacement reaction.<br />

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List what type the following reactions are:<br />

1) NaOH + KNO3 --> NaNO3 + KOH Double displacement<br />

2) CH4 + 2 O2 --> CO2 + 2 H2O Combustion<br />

3) 2 Fe + 6 NaBr --> 2 FeBr3 + 6 Na<br />

Single displacement<br />

4) CaSO4 + Mg(OH)2 --> Ca(OH)2 + MgSO4<br />

Double displacement<br />

5) NH4OH + HBr --> H2O + NH4Br<br />

Acid base<br />

6) Pb + O2 --> PbO2<br />

Synthesis<br />

7) Na2CO3 --> Na2O + CO2<br />

Decomposition<br />

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Determine the Type of Reaction for each equation.<br />

Then predict the products of each of the following chemical reactions. If a reaction will not occur,<br />

explain why not.<br />

Then Balance the equation.<br />

1) __Ag2SO4 + __NaNO3 →<br />

Double displacment<br />

2) __NaI 2 + __CaSO4 →<br />

Double displacement<br />

3) __HNO3 + __Ca(OH)2 →<br />

Acid Base<br />

Ag 2<br />

S1<br />

O4<br />

Na1<br />

N1<br />

O3<br />

H1 H1<br />

N1 N1<br />

O3 O2<br />

Ca1 Ca1<br />

Ag1<br />

S1<br />

O3<br />

Na1<br />

N1<br />

O4<br />

Na1 Na2<br />

I1 I1<br />

Ca1 Ca<br />

S1 S1<br />

O4 O4<br />

4) __CaCO3 →<br />

decomposition<br />

Ca1<br />

C1<br />

O 3<br />

Ca1<br />

C1<br />

O3<br />

5) __AlCl3 + __(NH4)PO4 →<br />

Double Displacement<br />

6) __Pb + __Fe(NO3)3 →<br />

Al1<br />

Cl3<br />

N1<br />

H4<br />

P1<br />

O4<br />

Al1<br />

Cl3<br />

N1<br />

H3<br />

P1<br />

O4<br />

7) __C3H6 2 + 9 __O2 →<br />

Combustion<br />

C6<br />

H12<br />

O18<br />

C6<br />

H12<br />

H12<br />

8) __Na + __CaSO4 →<br />

Single Displacement<br />

Ca+Na2SO4<br />

Na1<br />

Ca1<br />

S1<br />

O4<br />

89


LG: The students will learn ho chemical reactions obey the ;aw of conservation of mass and how they can predict the products of a<br />

chemical reaction<br />

How to Balance Chemical Equations<br />

A chemical equation is a theoretical or written representation of what happens during a chemical<br />

reaction. The law of conservation of mass states that no atoms can be created or destroyed in a<br />

chemical reaction, so the number of atoms that are present in the reactants has to balance the<br />

number of atoms that are present in the products. Follow this guide to learn how to balance chemical<br />

equations.<br />

Step 1<br />

Write down your given equation. For this example, we will use:<br />

C3H8 + O2 --> H2O + CO2<br />

Step 2<br />

Write down the number of atoms that you have on each side of the equation. Look at the subscripts<br />

next to each atom to find the number of atoms in the equation.<br />

Left side: 3 carbon, 8 hydrogen and 2 oxygen<br />

Right side: 1 carbon, 2 hydrogen and 3 oxygen<br />

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Step 3<br />

Always leave hydrogen and oxygen for last. This means that you will need to balance the carbon<br />

atoms first.<br />

Step 4<br />

Add a coefficient to the single carbon atom on the right of the equation to balance it with the 3 carbon<br />

atoms on the left of the equation.<br />

C3H8 + O2 --> H2O + 3CO2<br />

The coefficient 3 in front of carbon on the right side indicates 3 carbon atoms just as the subscript 3<br />

on the left side indicates 3 carbon atoms.<br />

In a chemical equation, you can change coefficients, but you should never alter the subscripts.<br />

91


Step 5<br />

Balance the hydrogen atoms next. You have 8 on the left side, so you'll need 8 on the right side.<br />

C3H8 + O2 --> 4H2O + 3CO2<br />

On the right side, we added a 4 as the coefficient because the subscript showed that we already<br />

had 2 hydrogen atoms.<br />

When you multiply the coefficient 4 times the subscript 2, you end up with 8.<br />

Step 6<br />

Finish by balancing the oxygen atoms.<br />

Because we've added coefficients to the molecules on the right side of the equation, the number of<br />

oxygen atoms has changed. We now have 4 oxygen atoms in the water molecule and 6 oxygen<br />

atoms in the carbon dioxide molecule. That makes a total of 10 oxygen atoms.<br />

Add a coefficient of 5 to the oxygen molecule on the left side of the equation. You now have 10<br />

oxygen molecules on each side.<br />

C3H8 + 5O2 --> 4H2O + 3CO2.<br />

The carbon, hydrogen and oxygen atoms are balanced. Your equation is complete.<br />

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1) ___ NaNO3 + ___ PbO ___ Pb(NO3)2 + ___ Na2O<br />

2 2 7 1<br />

Na-1*2 Na-2<br />

N-1*2 ----> N-2<br />

O-4=7 O-7<br />

Pb-1 Pb-1<br />

2) ___ 6 AgI + ___ Fe2(CO3)3 ___ 2 FeI3 + ___ 3 Ag2CO3<br />

Ag1 (6)<br />

I1 (6)<br />

Fe2<br />

CO6<br />

Ag2(3)6<br />

I3(2)6<br />

Fe1(2)6<br />

CO3(3)6<br />

3) ___ 1 C2H4O2 + ___ 2 O2 ___ 2 CO2 + ___ 2 H2O<br />

C2<br />

H4<br />

O4(2)6<br />

C1(2)2<br />

H2(2)4<br />

O3(2)6<br />

4) ___ 1 ZnSO4 + ___ 1 Li2CO3 ___ 1 ZnCO3 + ___ 1 Li2SO4<br />

Zn1<br />

S1<br />

O7<br />

Li2<br />

C1<br />

Zn1<br />

S1<br />

O7<br />

Li2<br />

C1<br />

5) ___ 1 V2O5 + ___ 5 CaS ___ 5 CaO + ___ 1 V2S5<br />

V2<br />

O5<br />

Ca1(5)5<br />

S1(5)5<br />

V2<br />

O1(5)5<br />

Ca1(5)5<br />

S5<br />

93


6) ___ 1 Mn(NO2)2 + ___ 1 BeCl2 ___ 1 Be(NO2)2 + ___ 1 MnCl2<br />

Mn1<br />

NO4<br />

Be1<br />

CI2<br />

Mn1<br />

NO4<br />

Be1<br />

CI2<br />

7) ___ 3 AgBr + ___ 1 GaPO4 ___ 1 Ag3PO4 + ___ 1 GaBr3<br />

Ag1(3)<br />

Br1(3)<br />

Ga1<br />

PO4<br />

Ag3<br />

Br3<br />

Ga1<br />

PO4<br />

8) 3___ H2SO4 + ___ 2 B(OH)3 1__ B2(SO4)3 + ___ 6 H2O<br />

9) ___ 1 S8 + ___ 8 O2 ___ 8 SO2<br />

S8<br />

O2(8)16<br />

S1(8)8<br />

O2(8)16<br />

10) ___ 1 Fe + ___ AgNO3 ___ Fe(NO3)2 + ___ Ag<br />

Fe1<br />

Ag1(2)2<br />

NO3(2)6<br />

2 1 2<br />

Fe1<br />

Ag1(2)2<br />

NO6<br />

94


1) 2 NaNO3 + PbO Pb(NO3)2 + Na2O<br />

2) 6 AgI + Fe2(CO3)3 2 FeI3 + 3 Ag2CO3<br />

3) C2H4O2 + 2 O2 2 CO2 + 2 H2O<br />

4) ZnSO4 + Li2CO3 ZnCO3 + Li2SO4<br />

5) V2O5 + 5 CaS 5 CaO + V2S5<br />

6) Mn(NO2)2 + BeCl2 Be(NO2)2 + MnCl2<br />

7) 3 AgBr + GaPO4 Ag3PO4 + GaBr3<br />

8) 3 H2SO4 + 2 B(OH)3 B2(SO4)3 + 6 H2O<br />

9) S8 + 8 O2 8 SO2<br />

10) Fe + 2 AgNO3 Fe(NO3)2 + 2 Ag<br />

Additional Notes:<br />

Balance the equation.<br />

Convert units of a given substance to moles.<br />

Using the mole ratio, calculate the moles of substance yielded by the reaction.<br />

Convert moles of wanted substance to desired units<br />

Focus on the bigger parts of the equations being balanced<br />

There can be decimals<br />

Every equation can be balanced<br />

If you use fraction than time it by two to get rid of it<br />

Leave the parts of the equation with a single element for<br />

last<br />

NO MATTER CAN BE CREATED OR DESTROYED<br />

STEPS<br />

1. Determine the correct formulas for all the reactants and products in the reaction<br />

2. begin balancing with the most complicated looking group. A Polyatomic ion that appears unchanged on both sides of the equation<br />

can be counted as a single unit<br />

3. Save the elemental reactant and products for last. Exactly for hydrogen of oxygen. Keep you eye out for diatomic molecules such<br />

as oxygen, Hydrogen, and the halogens.<br />

4. If you get stuck double the most complicated looking group and try again.<br />

5. Finally make sure that all coefficients are in the lowest possible ratio<br />

6. None of the reactions you will encounter will be that difficult. If the coefficients are getting wild double check what you've done<br />

since you may have simple mistake<br />

95


The Learning Goal for this assignment is: Apply the mole concept and the law of conservation of mass<br />

to calculate quantities of chemicals participating in reactions.<br />

Stoichiometry and Balancing Reactions<br />

Stoichiometry is a section of chemistry that involves using relationships between reactants and/or<br />

products in a chemical reaction to determine desired quantitative data. In Greek, stoikhein means<br />

element and metron means measure, so stoichiometry literally translated means the measure of<br />

elements. In order to use stoichiometry to run calculations about chemical reactions, it is important to<br />

first understand the relationships that exist between products and reactants and why they exist, which<br />

require understanding how to balanced reactions.<br />

Balancing<br />

In chemistry, chemical reactions are frequently written as an equation, using chemical symbols. The<br />

reactants are displayed on the left side of the equation and the products are shown on the right, with<br />

the separation of either a single or double arrow that signifies the direction of the reaction. The<br />

significance of single and double arrow is important when discussing solubility constants, but we will<br />

not go into detail about it in this module. To balance an equation, it is necessary that there are the<br />

same number of atoms on the left side of the equation as the right. One can do this by raising the<br />

coefficients.<br />

Reactants to Products<br />

A chemical equation is like a recipe for a reaction so it displays all the ingredients or terms of a<br />

chemical reaction. It includes the elements, molecules, or ions in the reactants and in the products as<br />

well as their states, and the proportion for how much of each particle is create relative to one another,<br />

through the stoichiometric coefficient. The following equation demonstrates the typical format of a<br />

chemical equation:<br />

2Na(s) + 2HCl(aq) → 2NaCl(aq) + H2(g)<br />

In the above equation, the elements present in the reaction are represented by their chemical<br />

symbols. Based on the Law of Conservation of Mass, which states that matter is neither created nor<br />

destroyed in a chemical reaction, every chemical reaction has the same elements in its reactants and<br />

products, though the elements they are paired up with often change in a reaction. In this reaction,<br />

sodium (Na), hydrogen (H), and chloride (Cl) are the elements present in both reactants, so based on<br />

the law of conservation of mass, they are also present on the product side of the equations.<br />

Displaying each element is important when using the chemical equation to convert between<br />

elements.<br />

Stoichiometric Coefficients<br />

In a balanced reaction, both sides of the equation have the same number of elements. The<br />

stoichiometric coefficient is the number written in front of atoms, ion and molecules in a chemical<br />

reaction to balance the number of each element on both the reactant and product sides of the<br />

equation. These stoichiometric coefficients are useful since they establish the mole ratio between<br />

reactants and products. In the balanced equation:<br />

2Na(s)+2HCl(aq)→2NaCl(aq)+H2(g)<br />

96


we can determine that 2 moles of HCl will react with 2 moles of Na(s) to form 2 moles of NaCl(aq) and 1<br />

mole of H2(g). If we know how many moles of Na we start out with, we can use the ratio of 2 moles<br />

of NaCl to 2 moles of Na to determine how many moles of NaCl were produced or we can use the<br />

ration of 1 mole of H2 to 2 moles of Na to convert to NaCl. This is known as the coefficient factor. The<br />

balanced equation makes it possible to convert information about one reactant or product to<br />

quantitative data about another element. Understanding this is essential to solving stoichiometric<br />

problems.<br />

Example 1<br />

Lead (IV) hydroxide and sulfuric acid react as shown below. Balance the reaction.<br />

Solution<br />

___Pb(OH)4 +___H2SO4→___Pb(SO4)2 +___H2O<br />

Start by counting the number of atoms of each element.<br />

Unbalanced<br />

Pb 1 1 Pb<br />

O 8 9 O<br />

H 6 2 H<br />

S 1 2 S<br />

The reaction is not balanced; the reaction has 16 reactant atoms and only 14 product atoms and does<br />

not obey the conservation of mass principle. Stoichiometric coefficients must be added to make the<br />

equation balanced. In this example, there are only one sulfur atom present on the reactant side, so a<br />

coefficient of 2 should be added in front of H2SO4to have an equal number of sulfur on both sides of<br />

the equation. Since there are 12 oxygen on the reactant side and only 9 on the product side, a 4<br />

coefficient should be added in front of H2O where there is a deficiency of oxygen. Count the number<br />

of elements now present on either side of the equation. Since the numbers are the same, the<br />

equation is now balanced.<br />

Pb(OH)4 + 2H2SO4→ Pb(SO4)2 + 4H2O<br />

Balanced<br />

Pb 1 1 Pb<br />

O 8 12 12 9 O<br />

H 6 8 8 2 H<br />

S 1 2 2 2 S<br />

Balancing reactions involves finding least common multiples between numbers of elements present<br />

on both sides of the equation. In general, when applying coefficients, add coefficients to the<br />

molecules or unpaired elements last.<br />

A balanced equation ultimately has to satisfy two conditions.<br />

1. The numbers of each element on the left and right side of the equation must be equal.<br />

2. The charge on both sides of the equation must be equal. It is especially important to pay<br />

attention to charge when balancing redox reactions.<br />

97


Stoichiometry and Balanced Equations<br />

In stoichiometry, balanced equations make it possible to compare different elements through the<br />

stoichiometric factor discussed earlier. This is the mole ratio between two factors in a chemical<br />

reaction found through the ratio of stoichiometric coefficients. Here is a real world example to show<br />

how stoichiometric factors are useful.<br />

Example 2<br />

There are 12 party invitations and 20 stamps. Each party invitation needs 2 stamps to be sent. How<br />

many party invitations can be sent?<br />

Solution<br />

The equation for this can be written as<br />

I+2S→IS2<br />

where<br />

I represent invitations,<br />

S represents stamps, and<br />

IS 2 represents the sent party invitations consisting of one invitation and two stamps.<br />

<br />

Based on this, we have the ratio of 2 stamps for 1 sent invite, based on the balanced equation.<br />

Invitations Stamps Party Invitations Sent<br />

In this example are all the reactants (stamps and invitations) used up? No, and this is normally the<br />

case with chemical reactions. There is often excess of one of the reactants. The limiting reagent, the<br />

one that runs out first, prevents the reaction from continuing and determines the maximum amount of<br />

product that can be formed.<br />

Example 3<br />

What is the limiting reagent in this example?<br />

Solution<br />

Stamps, because there was only enough to send out invitations, whereas there were enough<br />

invitations for 12 complete party invitations. Aside from just looking at the problem, the problem can<br />

be solved using stoichiometric factors.<br />

12 I x 1IS2 = 12 IS2 possible<br />

1I<br />

20 S x 1IS2 = 10 IS2 possible<br />

2S<br />

98


When there is no limiting reagent because the ratio of all the reactants caused them to run out at the<br />

same time, it is known as stoichiometric proportions.<br />

Types of Reactions<br />

There are 6 basic types of reactions.<br />

Combustion: Combustion is the formation of CO2 and H2O from the reaction of a chemical<br />

and O2<br />

Combination (synthesis): Combination is the addition of 2 or more simple reactants to form a<br />

complex product.<br />

Decomposition: Decomposition is when complex reactants are broken down into simpler<br />

products.<br />

Single Displacement: Single displacement is when an element from on reactant switches with<br />

an element of the other to form two new reactants.<br />

Double Displacement: Double displacement is when two elements from on reactants<br />

switched with two elements of the other to form two new reactants.<br />

Acid-Base: Acid- base reactions are when two reactants form salts and water.<br />

Molar Mass<br />

Before applying stoichiometric factors to chemical equations, you need to understand molar mass.<br />

Molar mass is a useful chemical ratio between mass and moles. The atomic mass of each individual<br />

element as listed in the periodic table established this relationship for atoms or ions. For compounds<br />

or molecules, you have to take the sum of the atomic mass times the number of each atom in order to<br />

determine the molar mass.<br />

Example 4<br />

What is the molar mass of H2O?<br />

Solution<br />

Molar mass = 2 × (1.00g/mol) + 1×(16.0g/mol) = 18.0g/mol<br />

Using molar mass and coefficient factors, it is possible to convert mass of reactants to mass of<br />

products or vice versa.<br />

Example 5: Combustion of Propane<br />

Propane (C3H8) burns in this reaction:<br />

C3H8 + 5O2 → 4H2O + 3CO2<br />

If 200 g of propane is burned, how many g of H2Ois produced?<br />

Solution<br />

Steps to getting this answer: Since you cannot calculate from grams of reactant to grams of products<br />

you must convert from grams of C3H8 to moles of C3H8 then from moles of C3H8 to moles of H2O.<br />

Then convert from moles of H2O to grams of H2O.<br />

99


Step 1: 200g C3H8 is equal to 4.54 mol C3H8.<br />

Step 2: Since there is a ratio of 4:1 H2O to C3H8, for every 4.54 mol C3H8 there are 18.18 mol<br />

H2O.<br />

Step 3: Convert 18.18 mol H2O to g H2O 18.18 mol H2O is equal to 327.27 g H2O.<br />

Variation in Stoichiometric Equations<br />

Almost every quantitative relationship can be converted into a ratio that can be useful in data<br />

analysis.<br />

Density<br />

Density (ρ) is calculated as mass/volume. This ratio can be useful in determining the volume of a<br />

solution, given the mass or useful in finding the mass given the volume. In the latter case, the inverse<br />

relationship would be used.<br />

Volume x (Mass/Volume) = Mass<br />

Mass x (Volume/Mass) = Volume<br />

Percent Mass<br />

Percent establishes a relationship as well. A percent mass states how many grams of a mixture are of<br />

a certain element or molecule. The percent X% states that of every 100 grams of a mixture, X grams<br />

are of the stated element or compound. This is useful in determining mass of a desired substance in<br />

a molecule.<br />

Example 6<br />

A substance is 5% carbon by mass. If the total mass of the substance is 10.0 grams, what is the<br />

mass of carbon in the sample? How many moles of carbon are there?<br />

Solution<br />

10 g sample x 5 g carbon = 0.5 g carbon<br />

100 g sample<br />

0.5g carbon x 1 mol carbon = 0.0416 mol carbon<br />

12.0g carbon<br />

Molarity<br />

Molarity (moles/L) establishes a relationship between moles and liters. Given volume and molarity, it<br />

is possible to calculate mole or use moles and molarity to calculate volume. This is useful in chemical<br />

equations and dilutions.<br />

100


Example 7<br />

How much 5M stock solution is needed to prepare 100 mL of 2M solution?<br />

Solution<br />

100 mL of dilute solution (1 L/1000 mL) (2 mol/1L solution) (1 L stock solution/5 mol solution) (1000<br />

ml stock solution/1L stock solution) = 40 mL stock solution.<br />

These ratios of molarity, density, and mass percent are useful in complex examples ahead.<br />

Determining Empirical Formulas<br />

An empirical formula can be determined through chemical stoichiometry by determining which<br />

elements are present in the molecule and in what ratio. The ratio of elements is determined by<br />

comparing the number of moles of each element present.<br />

Example 8<br />

1. Find the molar mass of the empirical formula CH2O.<br />

12.0g C + (1.00g H) * (2H) + 16.0g O = 30.0 g/mol CH2O<br />

2. Determine the molecular mass experimentally. For our compound, it is 120.0 g/mol.<br />

3. Divide the experimentally determined molecular mass by the mass of the empirical formula.<br />

(120.0 g/mol) / (30.0 g/mol) = 3.9984<br />

4. Since 3.9984 is very close to four, it is possible to safely round up and assume that there was a<br />

slight error in the experimentally determined molecular mass. If the answer is not close to a whole<br />

number, there was either an error in the calculation of the empirical formula or a large error in the<br />

determination of the molecular mass.<br />

5. Multiply the ratio from step 4 by the subscripts of the empirical formula to get the molecular<br />

formula.<br />

CH2O * 4 =?<br />

C: 1 * 4 = 4<br />

H: 2 * 4 = 8<br />

O 1 * 4 = 4<br />

CH2O * 4 = C4H8O4<br />

6. Check your result by calculating the molar mass of the molecular formula and comparing it to the<br />

experimentally determined mass.<br />

molar mass of C4H8O4= 120.104 g/mol<br />

experimentally determined mass = 120.056 g/mol<br />

% error = | theoretical - experimental | / theoretical * 100%<br />

% error = | 120.104 g/mol - 120.056 g/mol | / 120.104 g/mol * 100%<br />

% error = 0.040 %<br />

101


Stoichiometry and balanced equations make it possible to use one piece of information to calculate<br />

another. There are countless ways stoichiometry can be used in chemistry and everyday life. Try and<br />

see if you can use what you learned to solve the following problems.<br />

Problem 1<br />

Why are the following equations not considered balanced?<br />

a.<br />

1. Not a balanced because there is a 1:2 ratio oxugen<br />

H2O(l)→H2(g)+O2(g)<br />

b. Zn(s)+Au + (aq) →Zn 2+ (aq) +Ag(s) 2. Not balanced because there are-unequal # of elements on both sides.<br />

Problem 2<br />

Hydrochloric acid reacts with a solid chunk of aluminum to produce hydrogen gas and aluminum ions.<br />

Write the balanced chemical equation for this reaction.<br />

2Al + 6HCl-> 2AlCl3 + 3H2<br />

2Al+6HCI-->3H6^2+CIAI6^3<br />

Problem 3<br />

Given a 10.1M stock solution, how many mL must be added to water to produce 200 mL of 5M<br />

solution?<br />

10.1M 1M 200mL 2020<br />

5M 1,000mL 5,000<br />

=.404mL<br />

Problem 4<br />

If 0.502g of methane gas react with 0.27g of oxygen to produce carbon dioxide and water, what is the<br />

limiting reagent and how many moles of water are produced? The unbalanced equation is provided<br />

below.<br />

CH4(g)+O2(g)→CO2(g)+H2O(l)<br />

.502gCH4 1MCH4 1MCO2 44gCO2<br />

16g CH4 1MCH4 1MCO2<br />

=1.38<br />

.27 1MO2 1MCO2 44gCO2<br />

32gO2 1MO2 1MCO2<br />

= .37125<br />

102


Theoretical and Actual Yields<br />

Key Terms<br />

<br />

<br />

<br />

(Excess reagent, limiting reagent)<br />

Theoretical and actual yields<br />

Percentage or actual yield<br />

Skills to Develop<br />

Use stoichiometric calculation to determine excess and limiting reagents in a chemical reaction<br />

<br />

<br />

and explain why.<br />

Calculate theoretical yields of products formed in reactions that involve limiting reagents.<br />

Evaluate percentage or actual yields from known amounts of reactants<br />

Theoretical and Actual Yields<br />

Reactants not completely used up are called excess reagents, and the reactant that completely<br />

reacts is called the limiting reagent. This concept has been illustrated for the reaction:<br />

2Na+Cl2 →2NaCl<br />

Amounts of products calculated from the complete reaction of the limiting reagent are called<br />

theoretical yields, whereas the amount actually produced of a product is the actual yield. The ratio of<br />

actual yield to theoretical yield expressed in percentage is called the percentage yield.<br />

percent yield = actual yield / theoretical yield ×100<br />

Chemical reaction equations give the ideal stoichiometric relationship among reactants and products.<br />

Thus, the theoretical yield can be calculated from reaction stoichiometry. For many chemical<br />

reactions, the actual yield is usually less than the theoretical yield, understandably due to loss in the<br />

process or inefficiency of the chemical reaction.<br />

Example 1<br />

Methyl alcohol can be produced in a high-pressure reaction<br />

CO(g) + 2H2(g) →CH3OH(l)<br />

If 6.1 metric tons of methyl alcohol is obtained from 1.2 metric tons of hydrogen reacting with excess<br />

amount of CO, estimate the theoretical and the percentage yield?<br />

Hint:<br />

To calculate the theoretical yield, consider the reaction<br />

CO(g) + 2H2(g) → CH3OH(l)<br />

28.0 + 4.0 = 32.0 (stoichiometric masses in, g, kg, or tons)<br />

1.2 tons H2 × 32.0 CH3OH = 9.6 tons CH3OH<br />

4.0 H2<br />

Thus, the theoretical yield from 1.2 metric tons (1.2x10 6 g) of hydrogen gas is 9.6 tons. The actual<br />

yield is stated in the problem, 6.1 metric tons. Thus, the percentage yield is<br />

103


%yield = 6.1 tons × 100 = 64%<br />

9.6tons<br />

Discussion<br />

Due to chemical equilibrium or the mass action law, the limiting reagent may not be completely<br />

consumed. Thus, a lower yield is expected in some cases. Losses during the recovery process of the<br />

product will cause an even lower actual yield.<br />

Example 2<br />

A solution containing silver ion, Ag + , has been treated with excess of chloride ions Cl − . When dried,<br />

0.1234 g of AgCl was recovered. Assuming the percentage yield to be 98.7%, how many grams of<br />

silver ions were present in the solution?<br />

Hint:<br />

The reaction and relative masses of reagents and product are:<br />

The calculation,<br />

Ag + (aq) + Cl − (aq) → AgCl(s)<br />

107.868 + 35.453 = 143.321<br />

0.1234 g AgCl ×107.868 g Ag + =0.09287 g Ag +<br />

143.321g AgCl<br />

shows that 0.1234 g dry AgCl comes from 0.09287g Ag + ions. Since the actual yield is only 98.7%,<br />

the actual amount of Ag + ions present is therefore<br />

0.09287 g Ag + = 0.09409 g Ag +<br />

0.987<br />

Discussion<br />

One can also calculate the theoretical yield of AgCl from the percentage yield of 98.7% to be<br />

0.1234 g AgCl =0.1250 g AgCl<br />

0.987<br />

From 0.1250 g AgCl, the amount of Ag + present is also 0.09409 g.<br />

Stoichiometry - A Review<br />

Skills Taught<br />

<br />

<br />

<br />

<br />

<br />

<br />

<br />

evaluate molecular weight for a given formula<br />

evaluate weight (mass) percentages of elements for a given formula<br />

evaluate amounts (in mass and mole units) produced in a chemical reaction from given<br />

conditions<br />

classify reactions by types: combination, combustion, displacement, formation, etc<br />

determine the chemical formula when weight percentages are given and then evaluate the<br />

mole percentages of elements in the formula<br />

determine the chemical formula when weight percentages are given and molecular weight is<br />

known<br />

determine the amount produced, the actual yield, and other stoichiometry quantities for a given<br />

reaction<br />

104


Review Purposes<br />

<br />

<br />

<br />

<br />

<br />

To get an overall view of stoichiometry.<br />

Apply skills learned to perform quantitative chemical analysis.<br />

Apply theories and rules of chemistry to solve problems.<br />

Assess areas of strength and weakness for review purposes.<br />

Improve problem solving strategy and learning efficiency.<br />

Stoichiometry<br />

STOICHIOMETRY is the quantitative relationship of reactants and products. This unit has been<br />

divided into the following objects. A brief review is given here so that you can get a birds'-eye or<br />

overall view of stoichiometry.<br />

1.Amounts of substances<br />

Express amounts of substance in mass units of g, kg, tons, and convert them to moles,<br />

kilomoles, or millimoles.<br />

2.Chemical formulas<br />

Represent a substance with a formula that reflects its chemical composition, structure, and<br />

bonding; evaluate weight and mole percentages of elements in a substance; and determine<br />

chemical formula by elemental analysis.<br />

3.Reaction features<br />

Define some common features of chemical reactions; classify chemical reactions by common<br />

features such as combination, combustion, decomposition, displacement, and redox reactions.<br />

4.Reaction equations<br />

Express quantitative relationships using chemical reaction equations; evaluate quantities of<br />

reactants and products in a chemical reaction; and solve reaction stoichiometry problems.<br />

5.Excess and limiting reagents<br />

Define excess and limiting reagents; determine excess and limiting reagents in a reaction<br />

mixture; and determine quantities produced in a chemical reaction.<br />

6.Yields<br />

Define theoretical and actual yields due to limiting reagent; apply the concept of limiting<br />

reagent to evaluate theoretical yield; convert actual yield to percentage yields.<br />

105


Use the space provided to write out the steps you take to solve different types of problems.<br />

Use any additional space for notes. These 2 pages should be full when you turn in your notebook.<br />

Steps to solve problems<br />

Mole to Mole:<br />

The disinfectant hydrogen peroxide, H2O2, decompose to form water and oxygen gas.<br />

How many moles of O2 will result from decomposition of 5 moles of hydrogen peroxide.<br />

5mol H2O2 1molO2<br />

NH3+O2---->NO+H2O is unbalanced<br />

2molH2O2<br />

5/2=2.5molO2<br />

round to 3<br />

2H2O2-->2H2O+O2<br />

H2-4 4H<br />

O20-4 4-3H<br />

4NH^3 +O^2--> 4NO+6H^2O<br />

is balanced<br />

We want NO =8/3<br />

2molO^2<br />

4molNO<br />

3molO^2<br />

we want H^2O=4molH2^O<br />

6molH^2O<br />

4molNO<br />

1.Balance the equation<br />

2. Convert units of a given substance to moles.<br />

3.Using the mole ratio, calculate the moles of substance yielded by the reaction.<br />

4.Convert moles of wanted substance to desired units<br />

Mol to grams<br />

2C+2H2O--> CH4+CO2<br />

1.Mke sure equation is balanced<br />

2.Find the # of mols in the reactant<br />

3.Find the # of grmas per mol for the reactant<br />

4.Multiply across the top and bottom<br />

5.Divide<br />

6.Find your Significant Figures<br />

2Mol<br />

12gC<br />

1mol<br />

24gC<br />

106


I have trouble remembering the types of reactants so I looked up more<br />

Synthesis- A compound that is made of simpler material A+B->AB C+O6^2-->CO2<br />

ecomposition-A compound broken into simpler compunds or all the way down to the elements that<br />

ake it up AB-->A+B<br />

2H2O--->O2+2H2<br />

Single Displacement-One element that starts out by itself replaces elements in a compound kicking it out<br />

AB+C-->AC+B 2CIMg---->MgCI2+H2<br />

ouble Displacement-The positive and negative ions in two compunds switchplaces AB+CD-->AC+BD<br />

OH+H2SO4---->K2SO4+H2O<br />

CumbustionA compund cotaining carbonand hydrogen (sometimes oxygen) combines with oxygen gas to<br />

produce carbondioxide and water Cx Hy O2--->CO2+H2O<br />

Mole to mass<br />

1.Determine how many mols are given in the prob<br />

2.Calculate the molar mass of the substance<br />

3.Multiply the mass by the mols given<br />

3MCO2<br />

44gCO2<br />

1MCO2<br />

132gCO2<br />

15CuCI 1MCuCI2<br />

Limiting Reagents<br />

33.5gCuCI2<br />

CuCI2+2NaNo3--> Cu(NO3)2+2NaCI<br />

Limiting reagent is CuCI2 with a product of 13.146<br />

1.Use the given amount of limiting reagent<br />

2.Convert the amount given in grams to mols<br />

3.Convert mols to mols to the product<br />

4.Convert back to grams<br />

5.repeat all these steps with the other limiting reagent<br />

6.Make sure to convert into the same product as the first one<br />

7.Evaluate both answers<br />

8.The lowest number will be the limiting reagent<br />

2MNaCI<br />

1MCuCI<br />

13.146<br />

The following reactiom is preformed with1.56g of BaCI2 which is the limiting reagent.<br />

We isp;ate 1.82g of our desired product AgCI<br />

BaCI2+2AgCI+Ba(NO)2<br />

Note: Percent yield= Actual yield/Theo yield*100%<br />

1.56<br />

1M BaCI2 2M AgCI 1435g AgCI<br />

Percent yield<br />

1.Find limiting reagent<br />

2.Use the limiting reagent and convert into mole<br />

3. Do a mol to mol conversion to find the product<br />

207g BaCI2 1M BaCI2 1M AgCI<br />

4. Make sure your finding the productthat is given th actual yield<br />

5.Take the product that is given the actual yield<br />

6.Divide and multiply by100%<br />

7.Round using significant figures<br />

1.82/2.16*100%=84.2%<br />

PY is 84.2%<br />

8.Percent yield should be found<br />

2.16289<br />

107


Unit 6<br />

Chapter 13 States of Matter<br />

The students will learn what are the factors that determine and<br />

characteristics that distinguish gases liquids and solids and<br />

how substances change from one state to another.<br />

Differentiate among the four states of matter.<br />

Students will measure the physical characteristics of matter such as temperature<br />

and density.<br />

Students will compare and contrast the physical characteristics of the 4 states of<br />

matter.<br />

solid<br />

liquid<br />

gas<br />

plasma<br />

Relate temperature to the average molecular kinetic energy.<br />

Students will be able to compare and contrast the motion of particles of a sample<br />

at various temperatures.<br />

Kinetic energy<br />

Kinetic theory<br />

Temperature<br />

Describe phase transitions in terms of kinetic molecular theory.<br />

Students will be able to identify and describe phase changes.<br />

Students will be able to compare and contrast the change in particle motion<br />

for phase changes.<br />

Students will be able to interpret heating/cooling curves and phase diagrams.<br />

melting point<br />

freezing point<br />

boiling point<br />

condensation<br />

sublimation<br />

phase diagram<br />

kinetic molecular theory<br />

108


Chapter 14 The Behavior of Gases<br />

The students will learn how gases respond to changes in<br />

pressure, volume, and temperature and why the ideal gas law<br />

is useful even though ideal gases do not exist.<br />

Interpret the behavior of ideal gases in terms of kinetic molecular theory.<br />

Students will be able to describe the behavior of an ideal gas.<br />

Students will participate in activities to apply the Ideal Gas Law and its<br />

component laws to predict gas behavior.<br />

Students will be able to perform temperature/pressure conversions.<br />

Compressibility<br />

Boyle’s Law<br />

Charles’s Law<br />

Gay-Lussac’s Law<br />

Combine Gas Law<br />

Ideal Gas Law<br />

Partial pressure<br />

Dalton’s Law of partial pressure<br />

Diffusion<br />

Effusion<br />

Graham’s Law of effusion<br />

Chapter 15 Water and Aqueous Systems<br />

The students will learn how the interactions between water<br />

molecules account for the unique properties of water and how<br />

aqueous solutions form.<br />

Discuss the special properties of water that contribute to Earth's suitability<br />

as an environment for life: cohesive behavior, ability to moderate<br />

temperature, expansion upon freezing, and versatility as a solvent.<br />

Students will be able to prepare a solution of known molarity<br />

Students will participate in activities to calculate molarity<br />

Surface tension<br />

Surfactant<br />

Aqueous solutionSolvent<br />

Solute<br />

109


The Learning Goal for this assignment is:<br />

The student will learn what are the factors that determine and characteristics that<br />

distinguish gases,liquids, and solids and how substances change from on state to<br />

another<br />

Take note over the following chapter. Use the Headings provided to organize your notes. Define and number all highlighted vocabulary (total 23 ) as well<br />

as summarize the sections. You may add pictures where needed. The pictures should be an appropriate size. Use Arial 12 for all text. This document<br />

should be 3 pages and should be saved as a pdf before you submit it into Angel.<br />

13.1 The Nature of Gases<br />

Chapter 13 States of Matter<br />

Pages 420 - 439<br />

Kinetic Theory and a Model for Gases<br />

Q: What are three assumptions of the kinetic theory as it applies to gases?<br />

(1) Kinetic energy is the energy in an object because it is in motion. There is also a (2)<br />

Kinetic Theory, all matter consists of tiny particles that are consistently in motion. The particles in a<br />

gas are small, hard spheres with an insignificant # of volume. The motions of particles in a gas are<br />

rapid, constant, and random. All collisions between a particle and a gas are perfectly elastic.<br />

Gas Pressure<br />

Q: How does Kinetic Theory explain gas pressure?<br />

(3) Gas pressure results from the force exerted by a gas per unit surface area of an object. Gas<br />

pressure is the result of billions of rapidly moving particles in a gas simultaneously colliding with an<br />

object. An empty space with no particles and no pressure is called a (4) vacuum. (5) Atmospheric<br />

pressure is the collisions of atoms and molecules in air with objects. (6) A barometer is a device that<br />

is used to measure atmospheric pressure. (7) The SI unit of pressure is the pascal (Pa). It represents<br />

a very small amount of pressure. One (8) standard atmosphere (atm) is the pressure required to<br />

support 760mm of mercury in a mercury barometer at 25 degrees. EX: 1atm=760mmHg=101.3kPa.<br />

Kinetic Energy and Temperature<br />

Q: What is the relationship between the temperature in kelvins and the average kinetic energy of<br />

particles?<br />

Temp does not rise when heated. The increase in kinetic energy results in an increase in tempted<br />

kelvin temp of a substance is directly proportional to the average kinetic energy of the particles of the<br />

substance.<br />

13.2 The Nature of Liquids<br />

A Model of Liquids<br />

Q: What factors determine the prop of a liquid?<br />

Interplay between the distributive motions of particles and the attractions among the particles<br />

determine the physical properties of liquid. Kinetic Theory states both particles in gases and liquids<br />

contain K.E it allows the flow against each other. There are no particles in gas, yet particles in liquid<br />

do keep each other close.<br />

Evaporation<br />

Q: What is the relationship between evaporation and Kinetic Energy?<br />

During evaporation, only molecules with certain minimum kinetic energy can escape from the surface<br />

of the liquid. (9) Vaporization is a liquid transformed into a gas. (10) Evaporation is when the surface<br />

of a liquid that is not boiling. Particles with the highest K.E tend to escape the first evaporation<br />

(cooling process).<br />

Vapor Pressure<br />

Q: When can, a dynamic equilibrium exists between a liquid and vapor?<br />

110


A system that is constant vapor pressure, a dynamic equilibrium exists between the vapor and liquid.<br />

The system is equilibrium because the rate of evaporation of liquid equals the condensation of vapor.<br />

(11) Vapor Pressure measure of force extorted by a gas above a liquid. In equilibrium particles in the<br />

system continue to evaporate and condense, but no change occurs in the air of particles in liquid or<br />

vapor. Increase of temp of contained liquid increases the vapor pressure equaling more particles in<br />

warm liquid increasing K.E to the surface of the liquid.<br />

Boiling Point<br />

Q: Under the conditions does boiling occur?<br />

(12) Boiling point (bp) is the temp at which the vapor of pressure of the liquid is just equal to the<br />

external pressure on the liquid. (13) Normal boiling point is defined as the boiling point of a liquid at<br />

the pressure of 101.3 kPa. Liquid is heated to a temp which particle throughout the liquid have<br />

enough kinetic energy to vaporize, liquid begins to boil. Heating allows greater ir if there are particles<br />

at the surface of a liquid to overcome the attraction forces that keep it in state. The remaining<br />

particles in the liquid move faster.<br />

13.3 The Nature of Solids<br />

A Model of Solids<br />

How are the structure and properties of solids related?<br />

The general properties of solids reflect the orderly arraignment of their particles and the fixed<br />

locations of their particles. The (14) melting point (mp) is the temp at which a solid change into a<br />

liquid. At this temp, the distributive vibration of the particles is strong enough to overcome the<br />

attractions that hold them in fixed positions. The (15) freezing point (fp) is the temp at which a liquid<br />

change into a solid. The melting and freezing points of a substance are at the same temp. Soli<br />

phases are in equilibrium.<br />

Crystal Structure and Unit Cell<br />

What determines the shape of a crystal?<br />

A (16) crystal are particles arranged in an<br />

order, repeating, three-dimensional pattern<br />

called a crystal lattice. These shapes of a<br />

crystal reflect the arrangement of the<br />

particles within the solid. The smallest<br />

group of particles within a crystal retains<br />

the geometric shape of the crystal lattice is<br />

known as a (17) unit cell. (18) Allotropes are<br />

two different molecular form of the same<br />

element in the same physical state, they<br />

have different properties due to their<br />

different structures. Non- Crystalline solids<br />

are (19) amorphous solids which lack and<br />

ordered internal structure. EX: rubber,<br />

plastic, and asphalt. (20) Glass is a<br />

transparent fusion product of inorganic<br />

substances that have cooled to a rigid state<br />

without crystallizing. They soften when<br />

heated.<br />

111


13.4 Changes of State<br />

Sublimation<br />

Q: When can sublimation occur?<br />

The change of a substance from a solid to a vapor without passing through the liquid state is called<br />

(21) sublimitation. Sublimitation occurs in solids with vapor pressures that exceed atmospheric<br />

pressure at or near room temp.<br />

Phase Diagrams<br />

How are the conditions at which phases are in equilibrium represented on a phase diagram?<br />

A Phase diagram gives the conditions of temp and pressure at which a substance exists as solid,<br />

liquid, or gas (vapor). The conditions of pressure and temp at which two phases exist in the<br />

equilibrium are indicated on a phase diagram by a line separating the two regions representing the<br />

phases. The (23) triple point describes the only sets of conditions at which all three phases can exist<br />

in equilibrium with one another. EX: triple point of water temp is 0.016C and pressure of .61 k Pa<br />

(0.0060 atm).<br />

112


Name:Britney Contreras<br />

Name:Jackie O<br />

Grade:<br />

States of Matter Project<br />

You and you lab partner are going to create a study aid in the form of a game for the<br />

information in Chapter 13 States of Matter.<br />

First, each of you, independently from each other, will summarize the chapter on 3<br />

pages of a pdf which will be submitted in Angel by the end of class on Wednesday Feb<br />

22.<br />

Second, you and you lab partner will be given a game platform which you will use for<br />

your questions and answers, either Jeopardy or Kahoot.<br />

Third, you will fill in the information at the bottom of this page with your username,<br />

passwords and/or websites so that you do not forget this and I have a copy in case<br />

anything gets misplaced. This page will be submitted into Angel as a Word Document<br />

on Wednesday February 22 during class.<br />

Fourth, you will use your notes to generate the questions and answers.<br />

Finally you will give me access to your game by putting the website or Game Number<br />

on this page adding this page to your 3 pages of notes and resubmitting it in Angel as<br />

a pdf by the end of the class on Friday Feb 24.<br />

This page is due by the end of class on Wednesday February 22.<br />

This Project is due by the end of class on Friday February 24.<br />

Jeopardy (https://jeopardylabs.com)<br />

Password:<br />

Edit Link:<br />

Play Link:<br />

Kahoot (https://getkahoot.com)<br />

Username: mlem2001<br />

Email: jaclyn.oksi@gmail.com<br />

Password: lordgabriel<br />

Game PIN: 883307<br />

113


Average Kinetic Energy/Temperature<br />

Gas Pressure<br />

Volume<br />

The Three Gas Laws: If we have one constant and we will see how the other two are effected and we<br />

could<br />

predict the outcome of the constant.<br />

114


Keeping these two constant<br />

Inverse realtionship/porportion<br />

vol of class + student = increased vol<br />

Pod+students= students move more Like pressure<br />

115


Balloon heated molecuals hitting each other more balloon<br />

expanded pressure stay same volume more vol<br />

Increase in temp Increase in volume<br />

3/3=9/9<br />

116


Increase temp increase pressure if container has the<br />

same volume<br />

when heated giving more energy and constant<br />

container<br />

pressure cooker + race = dead people<br />

117


118


119


C-> K = +273<br />

water freezes are 0c degrees<br />

C->K +273 273 in f<br />

K-> C -273 Absolute O K<br />

120


121


Combined Gas Law​: Is where all three gas laws: Charles, Boyle’s, and Gay Lussac’s are<br />

combined. Using pressure, volume, and temperature.<br />

​Formula:​ ​PV ​= ​PV<br />

z T T<br />

Ideal Gas Law: ​ ​a gas is compressed into a smaller volume, the number and velocity of<br />

molecular collisions increase, raising the gas's temperature and pressure.<br />

122


Formula: ​PV=nRT<br />

123


The Learning Goal for this assignment is:<br />

The students will learn how interactions between water molecules account for unique<br />

properties of water and how aqueous solutions form.<br />

Take note over the following chapter. Use the Headings provided to organize your notes. Define and number all highlighted vocabulary (total ​ 22​ ) as well<br />

as summarize and take notes over the sections. You may add pictures where needed. The pictures should be an appropriate size. Use Arial 12 for all<br />

text. This document should be 2 pages and should be saved as a pdf before you submit it into Angel.<br />

Chapter 15 Water and Aqueous Systems<br />

Pages 488 - 507<br />

15.1 Water and Its Properties<br />

Water in the Liquid State:<br />

Human beings cannot live without water. Water is a molecule (H2O). The molecule consists of<br />

oxygen and hydrogen; this bond is covalent. The O-H bond to a greater extent. Oxygen has a greater<br />

electronegativity than hydrogen, so the oxygen atom attracts the electron pair. Many unique and<br />

important properties of water including its high surface tension, low vapor pressure, and high boiling<br />

point result from hydrogen boiling. The bond angle in H2O is 150 degrees and that makes it a Bent<br />

shape. O and H do not cancel. Polar molecules are attracted to dipole interactions. As normal<br />

Negative attracts Positive. The inward force, or pull, that tends to minimize the surface area of a liquid<br />

is called (1) Surface tension. Water sometimes bead up not spread. GRAVITY! pulls everything down!<br />

(2) Surfactant is any substance that interferes with the hydrogen bonding between water molecules<br />

and there by reduces tension. To go from liquid to a vapor state a hydrogen bond has to be broken,<br />

evaporation is slow and molecules have a less chance to escape. It takes heat more time to separate<br />

attractions between water molecules than in ammonia.<br />

Water in the Solid State:<br />

Solid water has a lower density than liquid water. Density increases when he molecules are moving<br />

closer together and creating solid liquid. Below 4 degrees’ Celsius water is no longer formatted like a<br />

normal liquid. Ice forms at 0 degrees Celsius. Ice is the only few solutions that floats in its own liquid.<br />

Ice is less dense than as a liquid because the structure of ice is regular open framework of water<br />

molecules in a hexagonal arrangement. The ice on top of water like in the Artic keeps the water<br />

underneath it to keep it warmer. Ice melts at 0 degree Celsius.<br />

15.2 Homogeneous Aqueous Systems<br />

Solutions:<br />

You will not find chemically pure water in nature. (3) Aqueous solution is water that contains dissolved<br />

substances (such as tap water). In the solution, the dissolving medium is the (4) solvent. The<br />

dissolved particles in a solution are (5) solute. Solutions are homogeneous mixtures. Filtered solution<br />

can have solute and the solvent pass through the filter. Substances that dissolve more rapidly in<br />

water include ionic compounds and polar covalent compounds. Non covalent compounds (oil, grease,<br />

gasoline, and methane do not dissolve in water​.<br />

Electrolytes and Nonelectrolytes:<br />

124


All ionic compounds are electrolytes but not all electrolytes are ionic compounds. This is because to<br />

be an electrolyte it needs to be able to conduct electricity in an aqueous solution or at least in a<br />

molten state which can fit a broad range of substances which ionic compounds all fit into will room for<br />

other substances. The substances that do not fit requirements to be called an electrolyte are referred<br />

to as nonelectrolytes8 sadly most substances are nonelectrolytes like sugars and carbon. For the<br />

substances that are Electrolytes there are two groups of them Strong electrolytes9 and weak<br />

electrolytes10 which is basically a measure of how efficient an electrolyte is.<br />

Hydrates:<br />

When crystals form sometimes water is integrated into them become intertwined with the structure<br />

and becomes water of hydration​ 11​ , any compound that has WoH in it can appropriately be called a<br />

hydrate​ 12 ​ . If one was to write the chemical formula of a hydrate then in order to account for the water<br />

molecules in it then a simple dot and the number of water molecules in the appropriate ratios for<br />

example copper(II) sulfate pentahydrate can be written as CuSo​ 4​<br />

​<br />

⬝ 5H​ 2​<br />

0<br />

15.3 Heterogeneous Aqueous Systems<br />

Suspensions:<br />

A (#) suspension is a mixture from which particles settle out upon standing. A suspension differs from<br />

a solution because the particles of a suspension are much larger and do not stay suspended<br />

indefinitely.<br />

Colloids:<br />

A colloid is a heterogeneous mixture containing particles that range I size from 1nm to 1000. Colloids<br />

have particles smaller than those in suspension and larger than those in solutions. Colloids could be<br />

also defined as a Tyndall over time. Colloids are milky like suspension when they are concentrated.<br />

Colloids also look clear due almost like a solution when diluted.<br />

125


126<br />

Unit 7<br />

Chapter 16 Solutions<br />

The students will learn what properties are used to describe<br />

the nature of solutions and how to quantify the concentration<br />

of a solution.<br />

Chapter 17 Thermochemistry<br />

The student will learn how energy is converted in a chemical<br />

or physical process and how to determine the amount of<br />

energy is absorbed or released in that process.<br />

Differentiate among the various forms of energy and recognize that they can<br />

be transformed from one form to others.<br />

Students will participate in activities to investigate and describe the<br />

transformation of energy from one form to another (i.e. batteries, food, fuels,<br />

etc.)<br />

Explore the Law of Conservation of Energy by differentiating among open,<br />

closed, and isolated systems and explain that the total energy in an isolated<br />

system is a conserved quantity.<br />

Students will be able to calculate various energy changes:<br />

o q = mc∆t<br />

o ∆Hfus<br />

o ∆Hmelt<br />

Thermochemistry<br />

Heat<br />

System<br />

Surrounding<br />

Law of conservation of energy<br />

Bond Making is exothermic<br />

Bond Breaking is endothermic<br />

Heat capacity<br />

Specific heat<br />

Calorimetry<br />

Enthalpy<br />

Thermochemical equation<br />

Molar heat of (fusion, solidification,<br />

vaporization, condensation, solution)<br />

Distinguish between endothermic and exothermic chemical processes.<br />

Students will be able to recognize exothermic and endothermic reactions through<br />

experimentation.<br />

Students will participate in activities (Pasco) to create exothermic and<br />

endothermic graphs.<br />

Endothermic<br />

Exothermic


Create and interpret potential energy diagrams, for example: chemical<br />

reactions, orbits around a central body, motion of a pendulum<br />

Students will participate in activities (Pasco) to create exothermic and<br />

endothermic graphs.<br />

Students will be able to interpret exothermic and endothermic reaction graphs.<br />

Potential energy diagram<br />

Thermochemical equations<br />

Chapter 18 Reaction Rates and Equilibrium<br />

The student will learn how the rate of a chemical reaction can<br />

be controlled, what the role of energy is and why some<br />

reactions occur naturally and others do not.<br />

Explain how various factors, such as concentration, temperature, and<br />

presence of a catalyst affect the rate of a chemical reaction.<br />

Students will be able to describe how each factor may affect the rate of a<br />

chemical reaction.<br />

Students will be able to compare the relative effect of each factor on the rate of a<br />

chemical reaction.<br />

Rate<br />

Collision theory<br />

Activation energy<br />

Catalyst<br />

Activated complex<br />

Inhibitor<br />

Explain the concept of dynamic equilibrium in terms of reversible processes<br />

occurring at the same rates.<br />

Students will be able to describe a system in dynamic equilibrium.<br />

Students will be able to describe how factors may affect the equilibrium of a<br />

reaction.<br />

Reversible reaction<br />

Chemical equilibrium<br />

Le Chatelier principle<br />

Explain entropy’s role in determining the efficiency of processes that convert<br />

energy to work.<br />

Students will be able to describe the change in entropy of a reaction.<br />

Students will be able to determine if a reaction is spontaneous<br />

Entropy<br />

Law of disorder<br />

Spontaneous/nonspontaneous reaction<br />

127


The Learning Goal for this assignment is:<br />

The students will learn what properties are used to described the nature and how to quantify the<br />

concentration of a solution.<br />

Defining Concentration<br />

Measures of Concentration<br />

Concentration is defined as the amount of dissolved solute in a given amount of solvent or<br />

solution. There are several terms that describe concentration. Some of these terms are relative;<br />

that is, they can be used only to compare the concentration of one solution to another. Dilute and<br />

concentrated are two such terms. A dilute solution contains less dissolved solute than a<br />

concentrated solution (in equal volumes of solution).<br />

The terms saturated, unsaturated, and supersaturated are terms that describe concentration more<br />

precisely.<br />

Saturated: The maximum amount of solute is dissolved in a given amount of solvent at a<br />

particular temperature. Such solutions are stable.<br />

Unsaturated: Less than the maximum amount of solute is dissolved in a given amount of<br />

solvent at a particular temperature. Such solutions are stable.<br />

Supersaturated: More than the maximum amount of solute is dissolved in a given amount of<br />

solvent at a particular temperature. Such solutions are unstable.<br />

Look at the solubility curve shown below:<br />

The solubility of NaNO3 is 86.0 g/100 mL H2O (at 20 °C). If you<br />

prepare a solution of 50.0 g NaNO3 dissolved in 100 mL H2O, an unsaturated solution results<br />

(Point A on the graph).<br />

continue adding NaNO to the solution until 86.0 g are dissolved, a saturated solution results<br />

(Point B).<br />

heat the solution to 50 °C, 113 grams NaNO3 can be dissolved (Point C). When the solution<br />

cools back down to 20 °C, it will be supersaturated (Point D).<br />

Quantifying Concentration<br />

To describe the concentration of a solution even more precisely, various measures of concentration<br />

can be used. Some of the ways concentration can be quantified include calculating the<br />

Mass of solute per solution mass (expressed as a percent or parts per million)<br />

Moles of solute per kilogram solvent (molality)<br />

Mass of solute per liter of solution (grams/liter)<br />

Moles of solute per liter of solution (molarity)<br />

128


Part 1: Mass Percent<br />

Mass percent (also called percent by mass, weight percent, or percent by weight) compares the<br />

mass of the solute to the entire mass of the solution.<br />

Notes: 1. Determine the total mass of the sample 2. Determine the identity of each element in the<br />

sample 3.Determine the mass of each element in the sample 4. Calculate the present composition<br />

Part 2: Parts per Million<br />

Parts per million (ppm) is another measure of concentration. It is similar to mass percent. But<br />

mass percent indicates the number of grams of solute per 100 g solution. Parts per million<br />

indicates the number of grams of solute per 1,000,000 g solution. This measure of concentration is<br />

often used to express the concentrations of very dilute solutions.<br />

Notes:<br />

Parts per notations may be expressed in the terms of any units of the same measure. Parts per notation<br />

is often used describing dilute solutions in chemistry for instance, the relative abundance of dissolved<br />

minerals or pollutants in water.<br />

Part 3: Molality<br />

Molality (m) is the ratio of the moles of solute to the kilograms of solvent. Note: this is the first<br />

measure of concentration that is concerned with the mass of the solvent, not the mass of the<br />

solution as a whole.<br />

Notes:<br />

A measure of the concentration of a solut in a solution in terms of amount of substance in a specified<br />

amount of mass of the solvent, This contrasts with the definition of molarity which is based on a specified<br />

volume of solution.<br />

Part 4: Grams per Liter<br />

To express the concentration of a solution in grams per liter, you must know the mass of the solute<br />

and the volume of the solution, not just the volume of the solvent.<br />

Notes:<br />

Grams cannot be converted directly to liters so we have a ratio, 1 liter=1,000mL<br />

Suppose you wanted to know what the concentration would be before making the solution. Could that<br />

be done? In order to relate the volume or mass of solvent to the volume of solution, you would have<br />

to know the density of the solution. You will see how solution density can be used to calculate<br />

molarity in the next section.<br />

129


Part 5: Molarity<br />

Molarity (M) is the most common measure of concentration. The concentration of most solutions<br />

you see in the lab are expressed in terms of molarity. Just like g/L, molarity calculations require<br />

that you know either the volume or density of the resulting solution.<br />

Notes:<br />

Moles of solute divided by liters of solution, 1mL=.0001L , Change grams to moles.<br />

Using Density to Calculate Molarity<br />

If the volume of the resulting solution is not known, molarity is calculated as follows:<br />

Convert the volume of solvent to grams. (The simulation does this step for you.)<br />

Determine the total mass of the solution (mass of solute + mass of solvent).<br />

Convert the solution mass to volume in milliliters, using its density (volume = mass / density).<br />

Convert the solution volume to liters (divide by 1000).<br />

Convert solute grams to moles.<br />

Calculate the molarity (moles solute / L solution).<br />

Reinforcing What You've Learned<br />

1. 35.0 g potassium dichromate are dissolved in 354.0 g distilled water. What is the concentration<br />

of the resulting solution, expressed as percent by mass? 9.00%<br />

2. A chemist discovers that 2587.0 g distilled water are contaminated with 13.0 g NaNO3. What is<br />

the concentration of NaNO3, expressed in ppm? 5.00 X 10 3<br />

3. 175.00 g H2SO4 are added to 61.49 g distilled H2O. What is the molality of the resulting solution?<br />

29.04m<br />

4. 225 g NaBr are dissolved in 525 g distilled water. If the volume of the resulting solution is<br />

584 mL, what is its concentration when expressed in g/L? 385g/L<br />

5. 470.0 g Na2CO3 are dissolved in 4230.0 g distilled water. What is the molarity of the resulting<br />

solution (D = 1.1029 g/mL)?<br />

1.1561 M<br />

Applying What You've Learned<br />

6. Think about the equations for mass percent and parts/million. Consider how you might convert<br />

between these two measures of concentration.<br />

Mass percent = ppm ÷ 10,000 ppm = mass percent X .0001<br />

7. Think about the equations for grams/liter and molarity. Consider how you might convert<br />

between these two measures of concentration.<br />

grams / L = molarity X molar mass<br />

molarity = grams / L ÷ molar mass<br />

130


Glossary<br />

Concentration: Amount of dissolved solute in a given amount of solvent or solution.<br />

Density: Amount of matter per unit volume. Density is calculated by dividing an object's mass by<br />

its volume.<br />

Mass: Amount of matter an object contains or, more scientifically, the measure of an object's<br />

resistance to changes in motion. The SI (Systéme International) unit for mass is the kilogram. In<br />

the lab, mass is often measured in grams.<br />

Mass percent: Also referred to as percent by mass and, occasionally, weight percent or percent<br />

by weight. Mathematically, mass % = (mass of solute / mass of entire solution) x 100.<br />

Molar mass: Mass of a compound, calculated by adding up the individual masses for its component<br />

atoms, which are obtained from the periodic table of the elements. Molar mass is expressed in<br />

grams/mole and is sometimes referred to as molecular mass (for molecular compounds) or formula<br />

mass (for ionic compounds).<br />

Molality (m): Moles of solute per kilogram of solvent. Mathematically, m = moles of solute / kilogram of<br />

solvent.<br />

Molarity (M): Moles of solute per liter of solution. Mathematically, M = moles of solute / liter of<br />

solution.<br />

Mole (mol): Counting unit used to express the large numbers of particles, such as atoms or<br />

molecules, that are involved in chemical processes. One mole of particles contains 6.02 x 10<br />

particles. The mass of one mole of an element, in grams, is equivalent to the atomic mass for that<br />

element, as indicated on the periodic table.<br />

Parts per million (ppm): Measure of concentration often used for dilute solutions. Mathematically,<br />

ppm = (mass of solute / mass of solution) x 10.<br />

Solubility: Measure of the maximum amount of solute that can be dissolved in a given amount of<br />

solvent at a given temperature, forming a stable solution.<br />

Solute: Dissolved substance in a solution. The solute is generally the solution component present<br />

in the lesser amount.<br />

Solution: Homogeneous mixture in which one substance has been dissolved in another.<br />

Solvent: Substance in which a solute is dissolved to form a solution. The solvent is generally the<br />

solution component present in the greater amount.<br />

Volume: Amount of space an object occupies. The SI (Systéme International) unit for volume is<br />

the cubic meter. In the lab, volume is often measured in cubic centimeters, milliliters, or liters.<br />

SAS Curriculum Pathways VLab #866<br />

131


The Learning Goal for this assignment is:<br />

The students will be able to learn how energy is converted in a chemical or physical process & how<br />

to determine the amount of energy is absorbed or released in that process.<br />

The System and the Surroundings in Chemistry<br />

Thermochemistry<br />

The system is the part of the universe we wish to focus our attention on. In the world of chemistry, the<br />

system is the chemical reaction. For example:<br />

2H2 + O2 ---> 2H2O<br />

The system consists of those molecules which are reacting.<br />

The surroundings are everything else; the rest of the universe. For example, say the above reaction is<br />

happening in gas phase; then the walls of the container are part of the surroundings.<br />

There are two important issues:<br />

1. a great majority of our studies will focus on the change in the amount of energy, not the<br />

absolute amount of energy in the system or the surroundings.<br />

2. regarding the direction of energy flow, we have a "sign convention."<br />

Two possibilities exist concerning the flow of energy between system and surroundings:<br />

1. The system can have energy added to it, which increases its amount and lessens the energy<br />

amount in the surroundings.<br />

2. The system can have energy removed from it, thereby lowering its amount and increasing the<br />

amount in the surroundings.<br />

We will signify an increase in energy with a positive sign and a loss of energy with a negative sign.<br />

Also, we will take the point-of-view from the system. Consequently:<br />

1. When energy (heat or work) flow out of the system, the system decreases in its amount. This<br />

is assigned a negative sign and is called exothermic.<br />

2. When energy (heat or work) flows into the system, the system increases its energy amount.<br />

This is assigned a positive sign and is called endothermic.<br />

We do not discuss chemical reactions from the surrounding's point-of-view. Only from the system's.<br />

132<br />

Notes:<br />

If the heat is going out of the system it is an exothermic reaction, If the heats is going into the system it is<br />

an endothermic reaction, For EX: an ice pac would be an endothermic reaction because it is taking heat in<br />

from the persons body


Specific Heat<br />

Here is the definition of specific heat:<br />

the amount of heat necessary for 1.00 gram of a substance to change 1.00 °C<br />

Note the two important factors:<br />

1. It's 1.00 gram of a substance<br />

2. and it changes 1.00 °C<br />

Keep in mind the fact that this is a very specific value. It is only for one gram going one degree. The<br />

specific heat is an important part of energy calculations since it tells you how much energy is needed<br />

to move each gram of the substance one degree.<br />

Every substance has its own specific heat and each phase has its own distinct value. In fact, the<br />

specific heat value of a substance changes from degree to degree, but we will ignore that.<br />

The units are often Joules per gram-degree Celsius (J/g*°C). Sometimes the unit J/kg K is also used.<br />

This last unit is technically the most correct unit to use, but since the first one is quite common, you<br />

will need to know both.<br />

I will ignore calorie-based units almost entirely.<br />

Here are the specific heat values for water:<br />

Phase J g¯1 °C¯1 J kg¯1<br />

K¯1<br />

Gas 2.02 2.02 x 10 3<br />

Liquid 4.184 4.184 x 10 3<br />

Solid 2.06 2.06 x 10 3<br />

Notice that one set of values is simply 1000 times bigger than the other. That's to offset the influence<br />

of going from grams to kilograms in the denominator of the unit.<br />

Notice that the change from Celsius to Kelvin does not affect the value. That is because the specific<br />

heat is measured on the basis of one degree. In both scales (Celsius and Kelvin) the jump from one<br />

degree to the next are the same "distance." Sometimes a student will think that 273 must be involved<br />

somewhere. Not in this case.<br />

Specific heat values can be looked up in reference books. Typically, in the classroom, you will not be<br />

asked to memorize any specific heat values. However, you may be asked to memorize the values for<br />

the three phases of water.<br />

As you go about the Internet, you will find different values cited for specific heats of a given<br />

substance. For example, I have seen 4.186 and 4.187 used in place of 4.184 for liquid water. None of<br />

the values are wrong, it's just that specific heat values literally change from degree to degree. What<br />

happens is that an author will settle on one particular value and use it. Often, the one particular value<br />

used is what the author used as a student.<br />

Hence, 4.184.<br />

133


The Time-Temperature Graph<br />

We are going to heat a container that has 72.0 grams of ice (no liquid water yet!) in it. To make the<br />

illustration simple, please consider that 100% of the heat applied goes into the water. There is no loss<br />

of heat into heating the container and no heat is lost to the air.<br />

Let us suppose the ice starts at -10.0 °C and that the pressure is always one atmosphere. We will<br />

end the example with steam at 120.0 °C.<br />

There are five major steps to discuss in turn before this problem is completely solved. Here they are:<br />

1. the ice rises in temperature from -10.0 to 0.00 °C.<br />

2. the ice melts at 0.00 °C.<br />

3. the liquid water then rises in temperature from zero to 100.0 °C.<br />

4. the liquid water then boils at 100.0 °C.<br />

5. the steam then rises in temperature from 100.0 to 120.0 °C<br />

Each one of these steps will have a calculation associated with it. WARNING: many homework and<br />

test questions can be written which use less than the five steps. For example, suppose the water in<br />

the problem above started at 10.0 °C. Then, only steps 3, 4, and 5 would be required for solution.<br />

To the right is the type of graph which is typically used to<br />

show this process over time.<br />

You can figure out that the five numbered sections on the<br />

graph relate to the five numbered parts of the list just above<br />

the graph.<br />

Also, note that numbers 2 and 4 are phases changes: solid<br />

to liquid in #2 and liquid to gas in #4.<br />

Q=mcΔT<br />

where ΔT is (Tf – Ti)<br />

Here are some symbols that will be used, A LOT!!<br />

Δt = the change in temperature from start to finish in degrees Celsius (°C)<br />

m = mass of substance in grams<br />

c = the specific heat. Its unit is Joules per gram X degree Celsius (J / g °C is one way to write<br />

the unit; J g¯1 °C¯1 is another)<br />

q = the amount of heat involved, measured in Joules or kilojoules (symbols = J and kJ)<br />

mol = moles of substance.<br />

ΔH is the symbol for the molar heat of fusion and ΔH is the symbol for the molar heat of<br />

vaporization.<br />

We will also require the molar mass of the substance. In this example it is water, so the molar mass is<br />

18.0 g/mol.<br />

Notes:<br />

the system consist of molecules reacting & to calculate things such as the final temp enthalpy, or the amount<br />

of energy needed we need to view the process as a chart. When is remains at a flat line we use the MHv<br />

or MHf equation, When it's a steady increase we use the equation MCΔt, for the c the # is given based on<br />

it's state, and for Hf or Hv it is also given based on it's state.<br />

134


Step One: solid ice rises in temperature<br />

As we apply heat, the ice will rise in temperature until it<br />

arrives at its normal melting point of zero Celsius.<br />

Once it arrives at zero, the Δt equals 10.0 °C.<br />

Here is an important point: THE ICE HAS NOT MELTED<br />

YET.<br />

At the end of this step we have SOLID ice at zero<br />

degrees. It has not melted yet. That's an important point.<br />

Each gram of water requires a constant amount of energy<br />

to go up each degree Celsius. This amount of energy is<br />

called specific heat and has the symbol c.<br />

72.0 grams of ice (no liquid water yet!) has changed 10.0 °C. We need to calculate the energy<br />

needed to do this.<br />

This summarizes the information needed:<br />

Δt = 10 °C<br />

The mass = 72.0 g<br />

c = 2.06 Joules per gram-degree Celsius<br />

The calculation needed, using words & symbols is:<br />

q = (mass) (Δt) (c)<br />

Why is this equation the way it is?<br />

Think about one gram going one degree. The ice needs 2.06 J for that. Now go the second degree.<br />

Another 2.06 J. Go the third degree and use another 2.06 J. So one gram going 10 degrees needs<br />

2.06 x 10 = 20.6 J. Now we have 72 grams, so gram #2 also needs 20.6, gram #3 needs 20.6 and so<br />

on until 72 grams.<br />

With the numbers in place, we have:<br />

q = (72.0 g) (10 °C) (2.06 J/g °C)<br />

So we calculate and get 1483.2 J. We won't bother to round off right now since there are four more<br />

calculations to go. Maybe you can see that we will have to do five calculations and then sum them all<br />

up.<br />

One warning before going on: three of the calculations will yield J as the unit on the answer and two<br />

will give kJ. When you add the five values together, you MUST have them all be the same unit.<br />

In the context of this problem, kJ is the preferred unit. You might want to think about what 1483.2 J is<br />

in kJ.<br />

Notes:<br />

FFor this step we need to focus on the equation MCΔt, For the C we need to use the given 2.1, In this<br />

calculation we must find the final temp and - the final temp to find the temp change.<br />

135


Step Two: solid ice melts<br />

Now, we continue to add energy and the ice begins to<br />

melt.<br />

However, the temperature DOES NOT CHANGE. It<br />

remains at zero during the time the ice melts.<br />

Each mole of water will require a constant amount of<br />

energy to melt. That amount is named the molar heat of<br />

fusion and its symbol is ΔHf. The molar heat of fusion is<br />

the energy required to melt one mole of a substance at its<br />

normal melting point. One mole of solid water, one mole<br />

of solid benzene, one mole of solid lead. It does not<br />

matter. Each substance has its own value.<br />

During this time, the energy is being used to overcome water molecules' attraction for each other,<br />

destroying the three-dimensional structure of the ice.<br />

The unit for this is kJ/mol. Sometimes you see older references that use kcal/mol. The conversion<br />

between calories and Joules is 4.184 J = 1.000 cal.<br />

Sometimes you also see this number expressed "per gram" rather than "per mole." For example,<br />

water's molar heat of fusion is 6.02 kJ/mol. Expressed per gram, it is 334.16 J/g.<br />

Typically, the term "heat of fusion" is used with the "per gram" value.<br />

72.0 grams of solid water is 0.0 °C. It is going to melt AND stay at zero degrees. This is an important<br />

point. While the ice melts, its temperature will remain the same. We need to calculate the energy<br />

needed to do this.<br />

This summarizes the information needed:<br />

ΔHf = 6.02 kJ/mol<br />

The mass = 72.0 g<br />

The molar mass of H2O = 18.0 gram/mol<br />

The calculation needed, using words & symbols is:<br />

q = (moles of water) (ΔHf)<br />

We can rewrite the moles of water portion and make the equation like this:<br />

q = (grams water / molar mass of water) (ΔHf)<br />

Why is this equation the way it is?<br />

Think about one mole of ice. That amount of ice (one mole or 18.0 grams) needs 6.02 kilojoules of<br />

energy to melt. Each mole of ice needs 6.02 kilojoules. So the (grams water / molar mass of water) in<br />

the above equation calculates the amount of moles.<br />

With the numbers in place, we have:<br />

q = (72.0 g / 18.0 g mol¯1 ) (6.02 kJ / mol)<br />

So we calculate and get 24.08 kJ. We won't bother to round off right now since there are three more<br />

calculations to go. We're doing the second step now. When all five are done, we'll sum them all up.<br />

136


Step Three: liquid water rises in temperature<br />

Once the ice is totally melted, the temperature can now<br />

begin to rise again.<br />

It continues to go up until it reaches its normal boiling<br />

point of 100.0 °C.<br />

Since the temperature went from zero to 100, the Δt is<br />

100.<br />

Here is an important point: THE LIQUID HAS NOT<br />

BOILED YET.<br />

At the end of this step we have liquid water at 100 degrees. It has not turned to steam yet.<br />

Each gram of water requires a constant amount of energy to go up each degree Celsius. This amount<br />

of energy is called specific heat and has the symbol c. There will be a different value needed,<br />

depending on the substance being in the solid, liquid or gas phase.<br />

72.0 grams of liquid water is 0.0 °C. It is going to warm up to 100.0 °C, but at that temperature, the<br />

water WILL NOT BOIL. We need to calculate the energy needed to do this.<br />

This summarizes the information needed:<br />

Δt = 100.0 °C (100.0 °C – 0.0 °C)<br />

The mass = 72.0 g<br />

c = 4.184 Joules per gram-degree Celsius<br />

The calculation needed, using words & symbols is:<br />

q = (mass) (Δt) (c)<br />

Why is this equation the way it is?<br />

Think about one gram going one degree. The liquid water needs 4.184 J for that. Now go the second<br />

degree. Another 4.184 J. Go the third degree and use another 4.184 J. So one gram going 100<br />

degrees needs 4.184 x 100 = 418.4 J. Now we have 72 grams, so gram #2 also needs 418.4, gram<br />

#3 needs 418.4 and so on until 72 grams.<br />

With the numbers in place, we have:<br />

q = (72.0 g) (100.0 °C) (4.184 J/g °C)<br />

So we calculate and get 30124.8 J. We won't bother to round off right now since there are two more<br />

calculations to go. We will have to do five calculations and then sum them all up.<br />

Notes:<br />

For this step we need to take in account the equation MQΔt, In this sate C= 4.18 for water, The two most<br />

important parts to this equation is finding the temp change and C, which is given.<br />

137


Step Four: liquid water boils<br />

Now, we continue to add energy and the water begins to<br />

boil.<br />

However, the temperature DOES NOT CHANGE. It<br />

remains at 100 during the time the water boils.<br />

Each mole of water will require a constant amount of<br />

energy to boil. That amount is named the molar heat of<br />

vaporization and its symbol is ΔH. The molar heat of<br />

vaporization is the energy required to boil one mole of a<br />

substance at its normal boiling point. One mole of liquid water, one mole of liquid benzene, one mole<br />

of liquid lead. It does not matter. Each substance has its own value.<br />

During this time, the energy is being used to overcome water molecules' attraction for each other,<br />

allowing them to move from close together (liquid) to quite far apart (the gas state).<br />

The unit for this is kJ/mol. Sometimes you see older references that use kcal/mol. The conversion<br />

between calories and Joules is 4.184 J = 1.000 cal.<br />

Typically, the term "heat of vaporization" is used with the "per gram" value.<br />

72.0 grams of liquid water is at 100.0 °C. It is going to boil AND stay at 100 degrees. This is an<br />

important point. While the water boils, its temperature will remain the same. We need to calculate the<br />

energy needed to do this.<br />

This summarizes the information needed:<br />

ΔH = 40.7 kJ/mol<br />

The mass = 72.0 g<br />

The molar mass of H2O = 18.0 gram/mol<br />

The calculation needed, using words & symbols is:<br />

q = (moles of water) (ΔH)<br />

We can rewrite the moles of water portion and make the equation like this:<br />

q = (grams water / molar mass of water) (ΔH)<br />

Why is this equation the way it is?<br />

Think about one mole of liquid water. That amount of water (one mole or 18.0 grams) needs 40.7<br />

kilojoules of energy to boil. Each mole of liquid water needs 40.7 kilojoules to boil. So the (grams<br />

water / molar mass of water) in the above equation calculates the amount of moles.<br />

With the numbers in place, we have:<br />

q = (72.0 g / 18.0 g mol¯1 ) (40.7 kJ / mol)<br />

So we calculate and get 162.8 kJ. We won't bother to round off right now since there is one more<br />

calculation to go. We're doing the fourth step now. When all five are done, we'll sum them all up.<br />

138


Step Five: steam rises in temperature<br />

Once the water is completely changed to steam, the<br />

temperature can now begin to rise again.<br />

It continues to go up until we stop adding energy. In this<br />

case, let the temperature rise to 120 °C.<br />

Since the temperature went from 100 °C to 120°C, the Δt<br />

is 20°C.<br />

Each gram of water requires a constant amount of energy<br />

to go up each degree Celsius. This amount of energy is called specific heat and has the symbol c.<br />

There will be a different value needed, depending on the substance being in the solid, liquid or gas<br />

phase.<br />

72.0 grams of steam is 100.0 °C. It is going to warm up to 120.0 °C. We need to calculate the energy<br />

needed to do this.<br />

This summarizes the information needed:<br />

Δt = 20 °C<br />

The mass = 72.0 g<br />

c = 2.02 Joules per gram-degree Celsius<br />

The calculation needed, using words & symbols is:<br />

q = (mass) (Δt) (c)<br />

Why is this equation the way it is?<br />

Think about one gram going one degree. The liquid water needs 2.02 J for that. Now go the second<br />

degree. Another 2.02 J. Go the third degree and use another 2.02 J. So one gram going 20 degress<br />

needs 2.02 x 20 = 44 J. Now we have 72 grams, so gram #2 also needs 44, gram #3 needs 44 and<br />

so on until 72 grams.<br />

I hope that helped.<br />

With the numbers in place, we have:<br />

q = (72.0 g) (20 °C) (2.02 J/g °C)<br />

So we calculate and get 2908.8 J. We won't bother to round off right now since we still need to sum<br />

up all five values.<br />

Notes:<br />

WHen it is a constant level we use the equation MHv, Vis this case will equal 2256, When we are on the<br />

steady increase MCΔt C=2.01, when we are going up to steam we must look at each individual<br />

step to get there.<br />

139


The following table summarizes the five steps and their results. Each step number is a link back to<br />

the explanation of the calculation.<br />

Converting to kJ gives us this:<br />

1.4832 kJ<br />

24.08 kJ<br />

30.1248 kJ<br />

162.8 kJ<br />

2.9088 kJ<br />

Step q 72.0 g of H2O<br />

1 1483.2 J Δt = 10 (solid)<br />

2 24.08 kJ melting<br />

3 30124.8 J Δt = 100 (liquid)<br />

4 162.8 kJ boiling<br />

5 2908.8 J Δt = 20 (gas)<br />

Summing up gives 221.3968 kJ and proper significant digits gives us 221.4 kJ for the answer.<br />

Notice how all units were converted to kJ before continuing on. Joules is a perfectly fine unit; it's just<br />

that 221,396.8 J is an awkward number to work with. Usually Joules is used for values under 1000,<br />

otherwise kJ is used.<br />

By the way, on other sites you may see kj used for kilojoules. I've also seen Kj used. Both of these<br />

are wrong symbols. kJ is the only correct symbol.<br />

Enthalpy<br />

When a process occurs at constant pressure, the heat evolved (either released or absorbed) is equal<br />

to the change in enthalpy. Enthalpy (H) is the sum of the internal energy (U) and the product of<br />

pressure and volume (PV) given by the equation:<br />

H=U+PV<br />

When a process occurs at constant pressure, the heat evolved (either released or absorbed) is equal<br />

to the change in enthalpy. Enthalpy is a state function which depends entirely on the state<br />

functions T, P and U. Enthalpy is usually expressed as the change in enthalpy (ΔH) for a process<br />

between initial and final states:<br />

ΔH=ΔU+ΔPVΔ<br />

If temperature and pressure remain constant through the process and the work is limited to pressurevolume<br />

work, then the enthalpy change is given by the equation:<br />

ΔH=ΔU+PΔV<br />

Also at constant pressure the heat flow (q) for the process is equal to the change in enthalpy defined<br />

by the equation:<br />

ΔH=q<br />

By looking at whether q is exothermic or endothermic we can determine a relationship between ΔH<br />

and q. If the reaction absorbs heat it is endothermic meaning the reaction consumes heat from the<br />

surroundings so q>0 (positive). Therefore, at constant temperature and pressure, by the equation<br />

above, if q is positive then ΔH is also positive. And the same goes for if the reaction releases heat,<br />

140


then it is exothermic, meaning the system gives off heat to its surroundings, so q


The Learning Goal for this section is: Explain how the various factors such as concentration,<br />

temperature, and presence of a catalyst affect the rate of a chemical reaction.<br />

You are going to answer these 15 questions first in the order they are given to you. This will be a quiz grade. You are then going to explain the<br />

chemical concepts that are used in each question. You can do this in the order given or group them by concepts. You can use your book or information<br />

found on the internet but all information must be written in your own word. The font needs to be Arial 12. This is due on Monday April 24 by midnight in<br />

the drop box. This document should be a 6-page pdf.<br />

1. B 6.B 11.A<br />

2. C 7.B 12.D<br />

3. C 8.D 13.C<br />

4. D 9.A 14.A<br />

5. D 10.B 15.D<br />

1 This graph represents the change in energy for two laboratory trials of the same reaction.<br />

Which factor could explain the energy difference between the trials?<br />

A Heat was added to trial #2.<br />

B A catalyst was added to trial #2.<br />

C Trial #1 was stirred.<br />

D Trial #1 was cooled.<br />

Explanation:<br />

The answer is B, A catalyst was added to trial #2 because if we look at the trials in the graph we can<br />

see that trial A requires way more energy than trail 2 to achieve its pathway to reaction. If we look at<br />

the two different pathways we could assume that the factor that changed the energy pathway in trial 2<br />

was a catalyst. A catalyst is, “a substance that enables a chemical reaction to proceed at a usually<br />

faster rate or under different conditions (as at a lower temperature) than otherwise possible” (Merriam<br />

Webster). In addition to this by looking at answer A, which states, Heat was added to trial #2, we can<br />

see that this would help the reaction, but not as much as what happened when the catalyst was<br />

added. In addition, answer C and D are wrong because if trial 2 was stirred or cooled it would not<br />

have the same effect of which occurred in trial 2.<br />

2 Consider this balanced chemical equation:<br />

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Which will increase the rate of the reaction?<br />

A increasing pressure on the reaction<br />

B decreasing concentration of the reactants<br />

C adding a catalyst to the reaction<br />

D decreasing the temperature of the reaction<br />

2H2O2 (aq) → 2H2O(l) + O2 (g)<br />

Explanation:<br />

The answer is C adding a catalyst to the reaction because in any chemical reaction adding a catalyst<br />

will help decrease the amount of energy need for the reaction. So, if our goal is trying to increase the<br />

rate at which the reaction will occur, it would be best to add a catalyst. In addition to this the reason<br />

it’s not A, B, or D is because if we were to add pressure to the chemical reaction it wouldn’t speed it<br />

up, either would decreasing the temperature because by doing so it would only decrease the rate of<br />

the reaction. In addition to this by decreasing the concentration it would only increase the solubility<br />

rather than increase the reaction process.<br />

3 For the reaction<br />

A + (aq) + B — (aq) → AB (s)<br />

increasing the temperature increases the rate of the reaction. Which is the best explanation for this<br />

happening?<br />

A The pressure increases, which in turn increases the production of products.<br />

B The concentration of reactants increases with an increase in temperature.<br />

C The average kinetic energy increases, so the likelihood of more effective collisions between ions<br />

increases.<br />

D Systems are more stable at high temperatures.<br />

Explanation:<br />

The answer is C, the average kinetic energy increases, so the likelihood of more effective collisions<br />

between ions increases, because this best defines how increasing the temperature increases the rate<br />

of the reaction. If we were to look at the other answers we would see that the rate of temperature<br />

does not affect the amount of concentrations, pressure, or the stability of systems at higher<br />

temperatures. C is correct because is best and correctly explains how the increase of temperatures<br />

increase the rate of the reaction.<br />

4 Which statement explains why the speed of some reactions is increased when the surface area of<br />

one or all the reactants is increased?<br />

A increasing surface area changes the electronegativity of the reactant particles<br />

B increasing surface area changes the concentration of the reactant particles<br />

C increasing surface area changes the conductivity of reactant particles<br />

D increasing surface area enables more reactant particles to collide<br />

Explanation:<br />

The answer is D, D increasing surface area enables more reactant particles to collide, because if it<br />

could increase the size at which a reaction occurs it would have allowed there to be more particles<br />

143


collide and more space for the concentrate to dissolve or disperse within. If we look at B and C we<br />

can tell those answers are insufficient to the question asked because by changing the surface area, it<br />

has no effect to the electro negativity of particles nor the concentration of reaction particles. Lastly, it<br />

also has no effect to the conductivity of reactant particles because by increasing the surface are you<br />

are only allowing the ability for more particles to collide.<br />

catalyst<br />

C6H6 + Br2 → C6H5Br + HBr<br />

5 Which of the following changes will cause an increase in the rate of the above reaction?<br />

A increasing the concentration of Br2<br />

B decreasing the concentration of C6H6<br />

C increasing the concentration of HBr<br />

D decreasing the temperature<br />

Explanation:<br />

The answer is D, decreasing the temperature, because in the chemical reaction shown above a<br />

catalyst is shown already being added to the reaction. So, by decreasing the temperature with the<br />

already added catalyst we would be increasing the rate of the reaction further. We can also see the<br />

credibility to answer D by looking at the other answers. If we look at A, b, C we can see that<br />

increasing the concentration of Br2, decreasing the concentration of C6H6, or increasing the<br />

concentration of HBr would not help speed up the reaction, but slow it down.<br />

2CO + O2 → 2CO2<br />

6 If the above reaction takes place inside a sealed reaction chamber, then which of these procedures<br />

will cause a decrease in the rate of reaction?<br />

A raising the temperature of the reaction chamber<br />

B increasing the volume inside the reaction chamber<br />

C removing the CO2 as it is formed<br />

D adding more CO to the reaction chamber<br />

Explanation:<br />

The answer is B, increasing the volume inside the reaction chamber will decrease the rate of the<br />

reaction because it will take a longer time for the particles to collide with one another. Ina addition to<br />

this the answer is not A, B, or D because removing the CO2 as it is formed, or adding more CO to the<br />

reaction chamber will not affect the particle that have collided or are still colliding, so the rate will<br />

neither decrease or increase. In addition, the other answer is wrong because by increasing the<br />

temperature, it will increase the rate of the reaction rather than decreasing it.<br />

7 A catalyst can speed up the rate of a given chemical reaction by<br />

A increasing the equilibrium constant in favor of products.<br />

B lowering the activation energy required for the reaction to occur.<br />

C raising the temperature at which the reaction occurs.<br />

D increasing the pressure of reactants, thus favoring products.<br />

Explanation:<br />

144


B lowering the activation energy required the reaction to occur, because the exact definition of a<br />

catalyst is, “a substance that enables a chemical reaction to proceed at a usually faster rate or under<br />

different conditions (as at a lower temperature) than otherwise possible.” In addition to this, it is not<br />

the other answers because it does not increase the temperature or pressure for the reaction and it<br />

does not bring the equilibrium.<br />

8 Which reaction diagram shows the effect of using the appropriate catalyst in a chemical reaction?<br />

A<br />

C<br />

B<br />

D<br />

Explanation:<br />

The answer is D because if we look at all the graphs and analyze them we can see that the one that<br />

correctly displays the use of a catalyst is graph D. It shows the difference between the two trials and<br />

how the energy needed to activate the reaction is lowered. If we look at the other graphs we could tell<br />

that they are wrong based on the increase than decrease than increase that the graph shows of a<br />

catalyst, and the graph that shows the slope of the catalyst being higher than without one.<br />

9 H2O2, hydrogen peroxide, naturally breaks down into H2O and O2 over time. MnO2, manganese<br />

dioxide, can be used to lower the energy of activation needed for this reaction to take place and, thus,<br />

increase the rate of reaction. What type of substance is MnO2?<br />

A a catalyst<br />

B an enhancer<br />

C an inhibitor<br />

D a reactant<br />

Explanation:<br />

The answer is A because the substance MnO2 as described by the question is breaking manganese<br />

dioxide, can be used to lower the energy of activation. If a substance is lowering the level of energy<br />

need for the reaction than it is the definition of a catalyst. In addition to this the other answers are<br />

wrong because an enhancer would be making the substance quality better not the process to achieve<br />

it. In addition, a reactant would not cause the result described in the question like a catalyst would.<br />

10 When a reaction is at equilibrium and more reactant is added, which of the following changes is<br />

the immediate result?<br />

145


Unit 8<br />

Chapter 19 Acid and Bases<br />

The student will learn what are the different ways chemists<br />

define aids and bases, what the pH of a solution means and<br />

how chemist use acid-base reactions.<br />

Relate acidity and basicity to hydronium and hydroxyl ion concentration and<br />

pH.<br />

Students will be able to use a pH scale to identify substances as acids or bases.<br />

Students will be able to use various equipment (probeware, universal pH, etc.) to<br />

identify the pH of substances.<br />

Students will be able to calculate H3O+ and OH- concentration of various<br />

substances.<br />

pH scale<br />

Hydronium ion<br />

Arrhenius acid/base<br />

Lewis acid/base<br />

Bronsted-Lowry acid/base<br />

Strong acid/base<br />

Weak acid/base<br />

Neutralization reaction<br />

Titration<br />

Chapter 20 Oxidation-Reduction Reactions<br />

The student will learn what happens during oxidation and<br />

reduction and how to balance redox equations.<br />

Describe oxidation-reduction reactions in living and non-living systems.<br />

Students will be able to compare and contrast redox reactions.<br />

Students will be able to assign oxidation numbers to redox reactions.<br />

Students will be able to write half reactions<br />

Oxidation<br />

148


Reduction<br />

Oxidation reduction reaction<br />

Oxidation number<br />

Half reaction<br />

Electrochemical process<br />

Battery<br />

Cathode<br />

Anode<br />

Electrolysis<br />

149


The Learning Goal for this section is:<br />

Th student will learn what are the different ways chemicals define acids an bases, what the pH of<br />

solutions means and how chemist use acids- base reaction.<br />

Acids and Bases<br />

150<br />

The Observable Properties of Acids and Bases<br />

The words acid and alkaline (an older word for base) are derived from direct sensory experience.<br />

Acid Property #1:<br />

The word acid comes from the Latin word acere, which means "sour." All acids taste sour. Well<br />

known from ancient times were vinegar, sour milk and lemon juice. Aspirin (scientific name:<br />

acetylsalicylic acid) tastes sour if you don't swallow it fast enough. Other languages derive their word<br />

for acid from the meaning of sour. So, in France, we have acide. In Germany, we have säure from<br />

saure and in Russia, kislota from kisly.<br />

Base Property #1:<br />

The word "base" has a more complex history (see below) and its name is not related to taste. All<br />

bases taste bitter. For example, mustard is a base. It tastes bitter. Many medicines, because they are<br />

bases, taste bitter. This is the reason cough syrups are advertised as having a "great grape taste."<br />

The taste is added in order to cover the bitterness of the active ingredient in cough syrup.<br />

Acid Property #2:<br />

Acids make a blue vegetable dye called litmus turn red.<br />

Base Property #2:<br />

Bases are substances which will restore the original blue color of litmus after having been reddened<br />

by an acid.<br />

Acid Property #3:<br />

Acids destroy the chemical properties of bases.<br />

Base Property #3:<br />

Bases destroy the chemical properties of acids.<br />

Neutralization is the name for this type of reaction.<br />

Acid Property #4:<br />

Acids conduct an electric current.<br />

Base Property #4:<br />

Bases conduct an electric current.<br />

This is a common property shared with salts. Acids, bases and salts are grouped together into a<br />

category called electrolytes, meaning that a water solution of the given substance will conduct an<br />

electric current.<br />

Non-electrolyte solutions cannot conduct a current. The most common example of this is sugar<br />

dissolved in water.


So far, the properties have an obvious relationship: taste, color change, mutual destruction, and<br />

response to electric current. This last property is related, but in a less obvious way. The property<br />

below identifies a unique chemical reaction that acids and bases engage in.<br />

Acid Property #5:<br />

Upon chemically reacting with an active metal, acids will evolve hydrogen gas (H2). The key word, of<br />

course, is active. Some metals, like gold, silver or platinum, are rather unreactive and it takes rather<br />

extreme conditions to get these "unreactive" metals to react. Not so with the metals in this property.<br />

They include the alkali metals (Group I, Li to Rb), the alkaline earth metals (Group II, Be to Ra), as<br />

well as zinc and aluminum. Just bring the acid and the metal together at anything close to room<br />

temperature and you get a reaction. Here's a sample reaction:<br />

Zn + 2 HCl(aq) ---> ZnCl2 + H2<br />

Another common acid reaction some sources mention is that acids react with carbonates (and<br />

bicarbonates) to give carbon dioxide gas:<br />

HCl + NaCO3 ---> CO2 + H2O + NaCl<br />

Base Property #5:<br />

Bases feel slippery, sometimes people say soapy. This is because they dissolve the fatty acids and<br />

oils from your skin and this cuts down on the friction between your fingers as you rub them together.<br />

In essence, the base is making soap out of you. Yes, bases are involved in the production of soap! In<br />

the early years of soap making, the soaps were very harsh on the skin and clothes due to the high<br />

base content. Even today, people with very sensitive skin must sometimes use a non-soap-based<br />

product for bathing.<br />

It was not until more modern times that the chemical nature (as opposed to observable properties) of<br />

acids and bases began to be explored. That leads to this property that is not directly observable by<br />

the senses.<br />

Acid Property #6:<br />

Acids produce hydrogen ion (H + ) in solution. A more correct formula for what is produced is that of the<br />

hydronium ion, H3O + . Both formulas are used interchangeably.<br />

Acid base theories: Svante Arrhenius<br />

I. Introduction<br />

The basic idea is that certain substances remain ionized in solution all the time. Today, everyone<br />

accepts this without question, but it was the subject of much dissention and disagreement in 1884,<br />

when a twenty-five-year-old Arrhenius presented and defended his dissertation.<br />

II. The Acid Base Theory<br />

Acid - any substance which delivers hydrogen ion (H + ) to the solution.<br />

Base - any substance which delivers hydroxide ion (OH¯) to the solution.<br />

Here is a generic acid dissociating, according to Arrhenius:<br />

HA ---> H + + A¯<br />

151


This would be a generic base:<br />

XOH ---> X + + OH¯<br />

When acids and bases react according to this theory, they neutralize each other, forming water and a<br />

salt:<br />

HA + XOH ---> H2O + XA<br />

Keeping in mind that the acid, the base and the salt all ionize, we can write this:<br />

Finally, we can drop all spectator ions, to get this:<br />

H + + A¯ + X + + OH¯ ---> H2O + X + + A¯<br />

H + + OH¯ ---> H2O<br />

These ideas covered all of the known acids at the time (the usual suspects like hydrochloric acid,<br />

acetic acid, and so on) and most of the bases (sodium hydroxide, potassium hydroxide, calcium<br />

hydroxide and so on). HOWEVER, and it is a big however, the theory did not explain why ammonia<br />

(NH3) was a base. There are other problems with the theory also.<br />

III. Problems with Arrhenius' Theory<br />

1. The solvent has no role to play in Arrhenius' theory. An acid is expected to be an acid in any<br />

solvent. This was found to not be the case. For example, HCl is an acid in water, behaving in<br />

the manner Arrhenius expected. However, if HCl is dissolved in benzene, there is no<br />

dissociation, the HCl remaining as un-dissociated molecules. The nature of the solvent plays a<br />

critical role in acid-base properties of substances.<br />

2. All salts in Arrhenius' theory should produce solutions that are neither acidic or basic. This is<br />

not the case. If equal amounts of HCl and ammonia react, the solution is slightly acidic. If equal<br />

amounts of acetic acid and sodium hydroxide are reacted, the resulting solution is basic.<br />

Arrhenius had no explanation for this.<br />

3. The need for hydroxide as the base led Arrhenius to propose the formula NH4OH as the<br />

formula for ammonia in water. This led to the misconception that NH4OH is the actual base,<br />

not NH3.<br />

In fact, by 1896, several years before Arrhenius announced his theory, it had been recognized that<br />

characteristic base properties where just as evident in such solvents as aniline, where no hydroxide<br />

ions were possible.<br />

4. H + , a bare proton, does not exist for very long in water. The proton affinity of H2O is about 799<br />

kJ/mol. Consequently, this reaction:<br />

H2O + H + ---> H3O +<br />

happens to a very great degree. The "concentration" of free protons in water has been estimated to<br />

be 10¯130 M. A rather preposterous value, indeed.<br />

The Arrhenius theory of acids and bases will be fully supplanted by the theory proposed<br />

independently by Johannes and Thomas Lowry in 1923.<br />

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The acid base theory of Brønsted and Lowry<br />

I. Introduction<br />

In 1923, within several months of each other, Johannes Nicolaus Brønsted (Denmark) and Thomas<br />

Martin Lowry (England) published essentially the same theory about how acids and bases behave.<br />

Since they came to their conclusions independently of each other, both names have been used for<br />

the theory name.<br />

II. The Acid Base Theory<br />

Using the words of Brønsted:<br />

". . . acids and bases are substances that are capable of splitting off or taking up hydrogen ions,<br />

respectively."<br />

Or an acid-base reaction consists of the transfer of a proton from an acid to a base. KEEP THIS<br />

THOUGHT IN MIND!!<br />

Here is a more recent way to say the same thing:<br />

An acid is a substance from which a proton can be removed.<br />

A base is a substance that can remove a proton from an acid.<br />

Remember: proton, hydrogen ion and H + all mean the same thing<br />

Very common in the chemistry world is this definition set:<br />

An acid is a "proton donor."<br />

A base is a "proton acceptor."<br />

In an acid, the hydrogen ion is bonded to the rest of the molecule. It takes energy (sometimes a little,<br />

sometimes a lot) to break that bond. So the acid molecule does not "give" or "donate" the proton, it<br />

has it taken away. In the same sense, you do not donate your wallet to the pickpocket, you have it<br />

removed from you.<br />

The base is a molecule with a built-in "drive" to collect protons. As soon as the base approaches the<br />

acid, it will (if it is strong enough) rip the proton off the acid molecule and add it to itself.<br />

Now this is where all the fun stuff comes in that you get to learn. You see, some bases are stronger<br />

than others, meaning some have a large "desire" for protons, while other bases have a weaker drive.<br />

It's the same way with acids, some have very weak bonds and the proton is easy to pick off, while<br />

other acids have stronger bonds, making it harder to "get the proton."<br />

One important contribution coming from Lowry has to do with the state of the hydrogen ion in solution.<br />

In Brønsted's announcement of the theory, he used H + . Lowry, in his paper (actually a long letter to<br />

the editor) used the H3O + that is commonly used today.<br />

III. Sample Equations written in the Brønsted-Lowry Style<br />

A. Reactions that proceed to a large extent:<br />

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HCl + H2O ⇌ H3O + + Cl¯<br />

HCl - this is an acid, because it has a proton available to be transferred.<br />

H2O - this is a base, since it gets the proton that the acid lost.<br />

Now, here comes an interesting idea:<br />

H3O + - this is an acid, because it can give a proton.<br />

Cl¯ - this is a base, since it has the capacity to receive a proton.<br />

Notice that each pair (HCl and Cl¯ as well as H2O and H3O + differ by one proton (symbol = H + ). These<br />

pairs are called conjugate pairs.<br />

HNO3 + H2O ⇌ H3O + + NO3¯<br />

The acids are HNO3 and H3O + and the bases are H2O and NO3¯.<br />

Remember that an acid-base reaction is a competition between two bases (think about it!) for a<br />

proton. If the stronger of the two acids and the stronger of the two bases are reactants (appear on the<br />

left side of the equation), the reaction is said to proceed to a large extent.<br />

Here are some more conjugate acid-base pairs to look for:<br />

H2O and OH¯<br />

HCO3¯ and CO3 2¯<br />

H2PO4¯ and HPO4 2¯<br />

HSO4¯ and SO4 2¯<br />

NH4 + and NH3<br />

CH3NH3 + and CH3NH2<br />

HC2H3O2 and C2H3O2¯<br />

B. Reactions that proceed to a small extent:<br />

If the weaker of the two acids and the weaker of the two bases are reactants (appear on the left side<br />

of the equation), the reaction is said to proceed to only a small extent:<br />

HC2H3O2 + H2O ⇌ H3O + + C2H3O2¯<br />

NH3 + H2O ⇌ NH4 + + OH¯<br />

Identify the conjugate acid base pairs in each reaction.<br />

HC 2H 3O 2 and C 2H 3O 2¯<br />

is one conjugate pair.<br />

H 2O and H 3O + is the other.<br />

NH 3 and NH 4<br />

+<br />

is one pair.<br />

H 2O and OH¯ is the other.<br />

Notice that H 2O in the first equation is acting as a base and in the second equation is acting as an acid.<br />

154


IV. Problems with the Theory<br />

This theory works very nicely in all protic solvents (water, ammonia, acetic acid, etc.), but fails to<br />

explain acid base behavior in aprotic solvents such as benzene and dioxane. That job will be left for a<br />

more general theory, such as the Lewis Theory of Acids and Bases.<br />

The Lewis theory of acids and bases<br />

I. Introduction<br />

Lewis gives his definition of an acid and a base:<br />

"We are inclined to think of substances as possessing acid or basic properties, without having a<br />

particular solvent in mind. It seems to me that with complete generality we may say that a basic<br />

substance is one which has a lone pair of electrons which may be used to complete the stable group<br />

of another atom, and that an acid is one which can employ a lone pair from another molecule in<br />

completing the stable group of one of its own atoms."<br />

"In other words, the basic substance furnishes a pair of electrons for a chemical bond, the acid<br />

substance accepts such a pair."<br />

It is important to make two points here:<br />

1. NO hydrogen ion need be involved.<br />

2. NO solvent need be involved.<br />

The Lewis theory of acids and bases is more general than the "one sided" nature of the Bronsted-<br />

Lowry theory. Keep in mind that Bronsted-Lowry, which defines an acid as a proton donor and a base<br />

as a proton acceptor, REQUIRES the presence of a solvent, specifically a protic solvent, of which<br />

water is the usual example. Since almost all chemistry is done in water, the fact that this limits the<br />

Bronsted-Lowry definition is of little practical consequence.<br />

The Lewis definitions of acid and base do not have the constraints that the Bronsted-Lowry theory<br />

does and, as we shall see, many more reactions were seen to be acid base in nature using the Lewis<br />

definition than when using the Bronsted-Lowry definitions.<br />

II. The Acid Base Theory<br />

The modern way to define a Lewis acid and base is a bit more concise than above:<br />

Acid: an electron acceptor.<br />

Base: an electron donor.<br />

A "Lewis acid" is any atom, ion, or molecule which can accept electrons and a "Lewis base" is any<br />

atom, ion, or molecule capable of donating electrons. However, a warning: many textbooks will say<br />

"electron pair" where I have only written "electron." The truth is that it sometimes is an electron pair<br />

and sometimes it is not.<br />

It turns out that it may be more accurate to say that "Lewis acids" are substances which are electrondeficient<br />

(or low electron density) and "Lewis bases" are substances which are electron-rich (or high<br />

electron density).<br />

155


Several categories of substances can be considered Lewis acids:<br />

1. positive ions<br />

2. having less than a full octet in the valence shell<br />

3. polar double bonds (one end)<br />

4. expandable valence shells<br />

Several categories of substances can be considered Lewis bases:<br />

1. negative ions<br />

2. one of more unshared pairs in the valence shell<br />

3. polar double bonds (the other end)<br />

4. the presence of a double bond<br />

Sören Sörenson and the pH scale<br />

I. Short Historical Introduction<br />

In the late 1880's, Svante Arrhenius proposed that acids were substances that delivered hydrogen ion<br />

to the solution. He has also pointed out that the law of mass action could be applied to ionic<br />

reactions, such as an acid dissociating into hydrogen ion and a negatively charged anion.<br />

This idea was followed up by Wilhelm Ostwald, who calculated the dissociation constants (the<br />

modern symbol is Ka) of many weak acids. Ostwald also showed that the size of the constant is a<br />

measure of an acid's strength.<br />

By 1894, the dissociation constant of water (today called Kw) was measured to the modern value of<br />

1 x 10¯14 .<br />

In 1904, H. Friedenthal recommended that the hydrogen ion concentration be used to characterize<br />

solutions. He also pointed out that alkaline (modern word = basic) solutions could also be<br />

characterized this way since the hydroxyl concentration was always 1 x 10¯14 ÷ the hydrogen ion<br />

concentration. Many consider this to be the real introduction of the pH scale.<br />

III. The Introduction of pH<br />

Sörenson defined pH as the negative logarithm of the hydrogen ion concentration.<br />

pH = - log [H + ]<br />

Remember that sometimes H3O + is written, so<br />

pH = - log [H3O + ]<br />

means the same thing.<br />

So let's try a simple problem: The [H + ] in a solution is measured to be 0.010 M. What is the pH?<br />

The solution is pretty straightforward. Plug the [H + ] into the pH definition:<br />

pH = - log 0.010<br />

An alternate way to write this is:<br />

pH = - log 10¯2<br />

Since the log of 10¯2 is -2, we have:<br />

pH = - (- 2)<br />

Which, of course, is 2.<br />

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Let's discuss significant figures and pH.<br />

Another sample problem: Calculate the pH of a solution in which the [H3O + ] is 1.20 x 10¯3 M.<br />

For the solution, we have:<br />

pH = - log 1.20 x 10¯3<br />

This problem can be done very easily using your calculator. However, be warned about putting<br />

numbers into the calculator.<br />

So you enter (-), log, 1.20, X10 n , (-), 3, enter.<br />

The answer, to the proper number of significant digits is: 2.921.<br />

III. Significant Figures in pH<br />

Here is the example problem: Calculate the pH of a solution where the [H + ] is 0.00100 M. (This could<br />

also be a pOH problem. The point being made is the same.)<br />

OK, you say, that's pretty easy, the answer is 3. After all, 0.00100 is 10¯3 and the negative log of 10¯3<br />

is 3.<br />

You would be graded wrong!! Why? Because the pH is not written to reflect the number of significant<br />

figures in the concentration.<br />

Notice that there are three sig figs in 0.00100. (Hopefully you remember significant figures, since you<br />

probably studied them months ago before getting to acid base stuff. THEY ARE STILL IMPORTANT!)<br />

So, our pH value should also reflect three significant figures.<br />

However, there is a special rule to remember with pH (and pOH) values. The whole number portion<br />

DOES NOT COUNT when figuring out how many digits to write down.<br />

Let's phrase that another way: in a pH (and a pOH), the only place where significant figures are<br />

contained is in the decimal portion.<br />

So, the correct answer to the above problem is 3.000. Three sig figs and they are all in the decimal<br />

portion, NOT (I repeat NOT) in the whole number portion.<br />

Practice Problems<br />

Convert each hydrogen ion concentration into a pH. Identify each as an acidic pH or a basic pH.<br />

1. 0.0015<br />

2.82<br />

2. 5.0 x 10¯9<br />

8.30<br />

3. 1.0<br />

0.00<br />

4. 3.27 x 10¯4 3.485<br />

5. 1.00 x 10¯12 12.000<br />

6. 0.00010 4.00<br />

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1. 2.82<br />

2. 8.30<br />

3. 0.00<br />

4. 3.485<br />

5. 12.000<br />

6. 4.00<br />

Sörenson also just mentions the reverse direction. That is, suppose you know the pH and you want to<br />

get to the hydrogen ion concentration ([H + ])?<br />

Here is the equation for that:<br />

[H + ] = 10¯pH<br />

That's right, ten to the minus pH gets you back to the [H + ] (called the hydrogen ion concentration).<br />

This is actually pretty easy to do with the calculator. Here's the sample problem: calculate the [H + ]<br />

from a pH of 2.45.<br />

This problem can be done very easily using your calculator. However, be warned about putting<br />

numbers into the calculator.<br />

So you enter 2nd, 10 x , (-), 2.45, enter.<br />

The answer, to the proper number of significant digits is: .00355.<br />

The pH of an acidic pond is 5. What is the hydrogen ion concentration (moles per liter)?<br />

The answer is:<br />

pH = -log (hydrogen ion concentration)<br />

The answer was .00001. Thus, 5 = -log (.00001).<br />

We'll take the formula that you started with (pH = -log([H+])) and work to the answer (solve for [H+]).<br />

pH = - log ([H+]) Given.<br />

pH = log ([H+] (-1) ) Since logarithms are like exponents, when you multiply a log by<br />

something, you can just move it to the inside of log as an exponent.<br />

10 pH = 10 log ([H+] (-1)) Take each side to tenth power.<br />

10 pH = [H+] (-1) Since "log" is just another notation for "log base 10", when you<br />

raise a log to the tenth power, the log cancels out.<br />

[H+] = 10 (-pH)<br />

Take the reciprocal of both sides.<br />

That is the general form. To answer the specific question,<br />

5 = - log ([H+])<br />

5 = log ([H+] (-1) )<br />

10 5 = [H+] (-1)<br />

10 (-5) = [H+]<br />

[H+] = .00001 mol/L<br />

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On your calculator you would input 10, ^, (-), 5 and you would get 0.00001.<br />

This is also the way to find the amount of OH + that are present in a base.<br />

To find the pH: -log(concentration)<br />

To find the concentration: 10 -pH<br />

Define these terms:<br />

pH scale<br />

pH is a numeric scale used to specify the acidity or bascity of an aqueous solution. It is roughly the negative<br />

of the logarithm to base 10 of the concentration, measured in units of m;es per liter of hydrogen ions.<br />

More precisely the negative of the logarithm to base 10 of the activity of the hydrogen ion.<br />

Hydronium ion<br />

Hydromium, ion is water molecule with an extra hydrogen ion attached to it. (H2O+H+ -> H3O) It is used<br />

to determine the acidity of a chemical compound. When a compound is put into water solution, the more the<br />

hydronium ion is produced, the higher the acidity is.<br />

Arrhenius acid/base<br />

The arrhenius acid-base concept classies a substance as an acid if it produces hydrogen ions h(+) or<br />

hydronium ions in water. A substance is classified as a base if it produces hydroxide ions OH(-) in<br />

water.<br />

Lewis acid/base<br />

Lewis Acid is a chemical species that reacts with a lewis base to form a Lewis adduct. A Lewis base<br />

then, is any species that donates a pair of electrons to a Lewis Acid to form a adduct. For EX: OH- & NH3<br />

are Lewis bases, because they can donate a lone pair of electrons.<br />

Bronsted-Lowry acid/base<br />

A Bronsted- Lowry acid is a substance that donates a proton in the form of a hydrogen ion. The Bronsted<br />

Lowry base, in turn accepts this proton, and the resulting products are a conjugate acid and a conjugate<br />

bas. the conjugate acid is the result of the base accepting the proton, so the charge increases by+1.<br />

Strong acid/base<br />

Sulfuric acid, as its name suggests, is not a base. Sulfuric acid is a strong acid as it dissociates readily.<br />

to give H+ ions. The dissociation of sulfuric acid in water in complete and all H+ ions are dissociated when<br />

dissolved in water.<br />

Weak acid/base<br />

The ionization of weak acids and bases are chemical equilibrium phenomenon. The equilibrium principles<br />

are essential for the understanding of equilibria of weak acids and weak bases. The conjugate acid- base<br />

pairs have been discussed in acids and bases<br />

Neutralization reaction<br />

In chemistry, neutralization or neuralisation, is a chemical reaction in which an acid and a base react<br />

quantitatively with each other. In a reaction in water, neutralization results in there being no excess<br />

of hydrogen or hydroxide ions present in solution.<br />

Titration<br />

Tiration, also known as titrimetry, is common laboratory method of quantitative chemical analysis that<br />

is used t determine the unknown concentration of an identified analyte. Since volume measurement<br />

play a key role in tiration, it is also known as volumetric analysis. A reagent. called the titrant or titrator<br />

is prepared as a standard solution.<br />

159


The Learning Goal for this assignment is:<br />

The students will learn what happens during oxidation and reduction and how to balance redox equations.<br />

1. Oxidation Numbers<br />

Redox Reactions<br />

Oxidation and reduction<br />

Every atom, ion or polyatomic ion has a formal oxidation number associated with it. This value<br />

compares the number of protons in an atom (positive charge) and the number of electrons assigned<br />

to that atom (negative charge).<br />

In many cases, the oxidation number reflects the actual charge on the atom, but there are many<br />

cases where it does not. Think of oxidation numbers as a bookkeeping exercise simply to keep track<br />

of where electrons go.<br />

2. Reduction<br />

Reduction means what it says: the oxidation number is reduced in reduction.<br />

This is accomplished by adding electrons. The electrons, being negative, reduce the overall oxidation<br />

number of the atom receiving the electrons.<br />

3. Oxidation<br />

Oxidation is the reverse process: the oxidation number of an atom is increased during oxidation.<br />

This is done by removing electrons. The electrons, being negative, make the atom that lost them<br />

more positive.<br />

I use this mnemonic to help me remember which is which: LEO the lion says GER.<br />

LEO = Loss of Electrons is Oxidation<br />

GER = Gain of Electrons is Reduction<br />

Another well-known mnemonic is this: OIL RIG<br />

OIL = Oxidation Is Loss (of Electrons)<br />

RIG = Reduction Is Gain (of Electrons)<br />

Another way is to simply remember that reduction is to reduce the oxidation number. Therefore,<br />

oxidation must increase the value.<br />

4. Reduction-Oxidation Reactions<br />

There are many chemical reactions in which one substance gets reduced in oxidation number<br />

(reduction) while another participating substance gets increased in oxidation number (oxidation).<br />

Such a reaction is called called a REDOX reaction. The RED, of course, comes from REDuction and<br />

OX from OXidation. However, it is pronounced re-dox and not red-ox.<br />

Here is a simple example of a redox reaction:<br />

160


Ag+ + Cu ---> Ag + Cu2+<br />

I have deliberately not balanced it and I have also written it in net ionic form. I have found that kids<br />

studying redox get confused by net ionic form and how to change a full equation into net ionic form.<br />

Redox equations need to be balanced but, except for the simplest ones, it cannot be done by<br />

inspection (also called trial and error). I take that back, complex ones can be done by trial and error. It<br />

typically takes quite a bit of work, especially when compared to how long it takes when the proper<br />

technique is used.<br />

There is a technique used to balance redox reactions. It is called "balancing by half-reactions." The<br />

basic plan will be to split the full equation into two simpler parts (called half-reactions), balance them<br />

following several standard steps, then recombine the balanced half-reactions into the final answer.<br />

This is another technique called the "ion-electron method." I plan to ignore it.<br />

Notes:<br />

Trial & error is useful for complex equations & look at one part at a time.<br />

5. Some Definitions<br />

Oxidizing Agent - that substance which oxidizes somebody else. It is reduced in the process.<br />

Reducing Agent - that substance which reduces somebody else. It is oxidized in the process.<br />

It helps me to remember these definitions by the opposite nature of what happens. By that, I mean<br />

the oxidizing agent gets reduced and the reducing agent gets oxidized.<br />

6. Rules for Assigning Oxidation Numbers<br />

The Oxidation Number of an element corresponds to the number of electrons, e - , that an atom loses,<br />

gains, or appears to use when joining with other atoms in compounds. In determining the Oxidation<br />

Number of an atom, there are seven guidelines to follow:<br />

1. The Oxidation Number of an individual atom is 0. This includes diatomic elements such as<br />

O2 or others like P4 and S8<br />

2. The total Oxidation Number of all atoms in: a neutral species is 0 and in an ion is equal to the<br />

ion charge.<br />

3. Group 1 metals have an Oxidation Number of +1 and Group 2 an Oxidation Number of +2<br />

4. The Oxidation Number of fluorine is -1 in compounds<br />

5. Hydrogen generally has an Oxidation Number of +1 in compounds, except hydrides<br />

6. Oxygen generally has an Oxidation Number of -2 in compounds, except peroxides<br />

7. In binary metal compounds, Group 17 elements have an Oxidation Number of -1, Group 16 of -<br />

2, and Group 15 of -3.<br />

Note: The sum of the Oxidation Number s is equal to zero for neutral compounds and equal to the<br />

charge for polyatomic ion species.<br />

Now, some examples:<br />

1. What is the oxidation number of Cl in HCl?<br />

Since H = +1, the Cl must be -1 (minus one).<br />

161


2. What is the oxidation number of Na in Na2O?<br />

Since O = -2, the two Na must each be +1.<br />

3. What is the oxidation number of Cl in ClO¯?<br />

The O is -2, but since a -1 must be left over, then the Cl is +1.<br />

4. What is the oxidation number for each element in KMnO4?<br />

K = +1 because KCl exists. We know the Cl = -1 because HCl exists.<br />

O = -2 by definition<br />

Mn = +7. There are 4 oxygens for a total of -8, K is +1, so Mn must be the rest.<br />

5. What is the oxidation number of S in SO4 2¯<br />

O = -2. There are four oxygens for -8 total. Since -2 must be left over, the S must = +6.<br />

Please note that, if there is no charge indicated on a formula, the total charge is taken to be zero.<br />

Practice Problems<br />

Find oxidation numbers<br />

1. N in NO3¯<br />

5+<br />

2. C in CO3 2¯<br />

3. Cr in CrO4 2¯<br />

4. Cr in Cr2O7 2¯<br />

5. Fe in Fe2O3<br />

6. Pb in PbOH +<br />

7. V in VO2 +<br />

8. V in VO 2+<br />

4+<br />

6+<br />

+12<br />

+3<br />

2+<br />

5+<br />

4+<br />

9. Mn in MnO4¯<br />

7+<br />

10. Mn in MnO4 2¯<br />

Notes:<br />

6+<br />

in almost all cases the oxidation # foe O2 is always 2-. We can find the oxidation # by using the periodic<br />

table. If it is a metal and gas we must make sure that they balance each other out. If it is an element<br />

by itself it will be 0.<br />

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7. Half Reactions<br />

A half-reaction is simply one which shows either reduction OR oxidation, but not both. Here is the<br />

example redox reaction used in a different file:<br />

Ag + + Cu → Ag + Cu 2+<br />

It has BOTH a reduction and an oxidation in it. That is why we call it a redox reaction, from REDuction<br />

and OXidation.<br />

What you must be able to do is look at a redox reaction and separate out the two half-reactions in it.<br />

To do that, identify the atoms which get reduced and get oxidized. Here are the two half-reactions<br />

from the above example:<br />

Ag+ → Ag<br />

Cu → Cu 2+<br />

The silver is being reduced, its oxidation number going from +1 to zero. The copper's oxidation<br />

number went from zero to +2, so it was oxidized in the reaction. In order to figure out the halfreactions,<br />

you MUST be able to calculate the oxidation number of an atom.<br />

Keep in mind that a half-reaction shows only one of the two behaviors we are studying. A single halfreaction<br />

will show ONLY reduction or ONLY oxidation, never both in the same equation.<br />

Also, notice that the reaction is read from left to right to determine if it is reduction or oxidation. If you<br />

read the reaction in the opposite direction (from right to left) it then becomes the other of our two<br />

choices (reduction or oxidation). For example, the silver half-reaction above is a reduction, but in the<br />

reverse direction it is an oxidation, going from zero on the right to +1 on the left.<br />

There will be times when you want to switch a half-reaction from one of the two types to the other. In<br />

that case, rewrite the entire equation and swap sides for everything involved. If I needed the silver<br />

half-reaction to be oxidation, I'd write Ag → Ag+ rather than just doing it mentally.<br />

The next step is that both half-reactions must be balanced. However, there is a twist. When you<br />

learned about balancing equation, you made equal the number of atoms of each element on each<br />

side of the arrow. That still applies, but there is one more thing: the total amount of charge on each<br />

side of the half-reaction MUST be the same.<br />

When you look at the two half-reactions above, you will see they are already balanced for atoms with<br />

one Ag on each side and one Cu on each side. So, all we need to do is balance the charge. To do<br />

this you add electrons to the more positive side. You add enough to make the total charge on each<br />

side become EQUAL.<br />

To the silver half-reaction, we add one electron:<br />

To the copper half-reaction, we add two electrons:<br />

Ag+ + e¯ ---> Ag<br />

Cu ---> Cu 2+ + 2e¯<br />

163


164<br />

One point of concern: notice that each half-reaction wound up with a total charge of zero on each<br />

side. This is not always the case. You need to strive to get the total charge on each side EQUAL, not<br />

zero.<br />

One more point to make before wrapping this up. A half-reaction is a "fake" chemical reaction. It's just<br />

a bookkeeping exercise. Half-reactions NEVER occur alone. If a reduction half-reaction is actually<br />

happening (say in a beaker in front of you), then an oxidation reaction is also occurring. The two halfreactions<br />

can be in separate containers, but they do have to have some type of "chemical<br />

connection" between them.<br />

Half-Reaction Practice Problems<br />

Balance each half-reaction for atoms and charge:<br />

1) Cl2 → Cl¯<br />

2) Sn → Sn 2+<br />

3) Fe 2+ → Fe 3+<br />

4) I3¯ → I¯<br />

Cl2+2-e->2Cl<br />

Sn->Sn2+ +2e<br />

Fe2+ ->Fe3+ +e-<br />

I3->3I + 2e-<br />

5) ICl2¯ → I¯ (I'm being mean on this one. Hint: the iodine is the only thing reduced or oxidized.)<br />

ICI2-+2e-->I-+2CI-<br />

Separate each of these redox reactions into their two half-reactions (but do not balance):<br />

6) Sn + NO3¯ →SnO2 + NO2<br />

7) HClO + Co →Cl2 + Co 2+<br />

8) NO2 →NO3¯ + NO<br />

Sn->SnO2 & NO3-->NO2<br />

HCIO->CL2 & Co-> Co2+<br />

NO2->NO3- & NO2->NO<br />

Here are the two half-reactions to be combined:<br />

Here is the rule to follow:<br />

Ag+ + e¯ → Ag<br />

Cu → Cu 2+ + 2e¯<br />

the total electrons MUST cancel when the two half-reactions are added.<br />

Another way to say it:<br />

the number of electrons in each half-reaction MUST be equal when the two half-reactions are<br />

added.<br />

What that means is that one (or both) equations must be multiplied through by a factor. The value of<br />

the factor is selected so as to make the number of electrons equal.<br />

In our example problem, the top reaction (the one with silver) must be multiplied by two, like this:<br />

2Ag+ + 2e¯ → 2Ag


Notice that each separate substance is increased by the factor amount. Occasionally, a student will<br />

multiply ONLY the electrons by the factor. That is incorrect.<br />

When the two half-reactions are added, we get:<br />

2Ag+ + 2e¯ + Cu → 2Ag + Cu 2+ + 2e¯<br />

With two electrons on each side, they may be canceled, resulting in:<br />

2Ag+ + Cu → 2Ag + Cu 2+<br />

This is the correct answer. Notice that there are two silvers on each side and one copper. Notice also<br />

that the total charge on each side is +2. It is balanced for both atoms and charge. Sometimes, I am<br />

asked if the order matters, if the Cu could be first on the left-hand side. The answer is that the order<br />

does not matter. There happen to be certain styles about where particular substances are put in the<br />

final answer, but these are only styles. They do not affect the chemical correctness of the answer.<br />

Notes:<br />

The equation must always be balanced to find the correct oxidation #'s and they must cancel an other<br />

Practice Problems<br />

Separate into half-reactions, balance them and then recombine.<br />

1) Sn + Cl2 ---> Sn 2+ + Cl¯<br />

2) Fe 2+ + I3¯ ---> Fe 3+ + I¯<br />

1. N in NO 3¯<br />

The O is -2 and three of them makes -6. Since -1 is left over, the N must be +5<br />

2. C in CO 3<br />

2¯<br />

The O is -2 and three of them makes -6. Since -2 is left over, the C must be +4<br />

3. Cr in CrO 4<br />

2¯<br />

The O is -2 and four of them makes -8. Since -2 is left over, the Cr must be +6<br />

4. Cr in Cr 2 O 7<br />

2¯<br />

The O is -2 and seven of them makes -14. Since -2 is left over, the two Cr must be +12<br />

What follows is an important point. Each Cr is +6. Each one. We do not speak of Cr 2 being +12. Each Cr atom is considered individually.<br />

5. Fe in Fe 2 O 3<br />

The O is -2 and three of them makes -6. Each Fe must then be +3<br />

6. +2 9. +7<br />

7. +5 10. +6<br />

8. +4<br />

1) Cl 2 + 2e¯ →2Cl¯ 5) ICl 2¯<br />

+ 2e¯ →I¯ + 2Cl¯<br />

2) Sn →Sn 2+ + 2e¯ 6) Sn →SnO 2 and NO 3¯<br />

→NO 2<br />

3) Fe 2+ →Fe 3+ + e¯ 7) HClO →Cl 2 and Co ---> Co 2+<br />

4) I 3¯ → 3I¯ + 2e¯ 8) NO 2 →NO 3¯<br />

and NO 2 →NO<br />

Note that in this last redox equation the NO 2 (actually just the N) is both being reduced AND being oxidized. In the first half-reaction, the N goes from +4<br />

to +5 (oxidation) and in the second, the N goes from +4 to +2 (reduction).<br />

By the way, we could flip the reaction so that NO 3¯<br />

and NO are reacting together to produce only one product, the NO 2 . In that case, the two halfreactions<br />

would be reversed.<br />

165


Reference Tables for Physical Setting/<strong>CHEMISTRY</strong><br />

Table A<br />

Standard Temperature and Pressure<br />

Name Value Unit<br />

Standard Pressure 101.3 kPa kilopascal<br />

1 atm atmosphere<br />

Standard Temperature 273 K kelvin<br />

0°C degree Celsius<br />

Table D<br />

Selected Units<br />

Symbol Name Quantity<br />

m meter length<br />

g gram mass<br />

Pa pascal pressure<br />

K kelvin temperature<br />

Table B<br />

Physical Constants for Water<br />

mol<br />

J<br />

mole<br />

joule<br />

amount of<br />

substance<br />

energy, work,<br />

quantity of heat<br />

Heat of Fusion<br />

Heat of Vaporization<br />

Specific Heat Capacity of H 2<br />

O()<br />

Specific Heat Capacity of H 2<br />

O(s)<br />

Specific Heat Capacity of H 2<br />

O(g)<br />

Table C<br />

Selected Prefixes<br />

Factor Prefix Symbol<br />

10 3 kilo- k<br />

334 J/g<br />

2260 J/g<br />

4.18 J/g•K<br />

2.10 J/g•K<br />

2.01 J/g•K<br />

s second time<br />

min minute time<br />

h hour time<br />

d day time<br />

y year time<br />

L liter volume<br />

ppm parts per million concentration<br />

M<br />

molarity<br />

solution<br />

concentration<br />

u atomic mass unit atomic mass<br />

10 –1 deci- d<br />

10 –2 centi- c<br />

10 –3 milli- m<br />

10 –6 micro- μ<br />

10 –9 nano- n<br />

10 –12 pico- p<br />

R1


Table E<br />

Selected Polyatomic Ions<br />

Formula Name Formula Name<br />

H 3<br />

O +<br />

hydronium<br />

CrO 4<br />

2–<br />

chromate<br />

Hg 2<br />

2+<br />

mercury(I)<br />

Cr 2<br />

O 7<br />

2–<br />

dichromate<br />

NH 4<br />

+<br />

C 2<br />

H 3<br />

O<br />

–<br />

2 –}<br />

CH 3<br />

COO<br />

CN –<br />

CO 3<br />

2–<br />

HCO<br />

–<br />

3<br />

C 2<br />

O<br />

2–<br />

4<br />

ClO –<br />

ammonium<br />

acetate<br />

cyanide<br />

carbonate<br />

hydrogen<br />

carbonate<br />

oxalate<br />

hypochlorite<br />

MnO 4<br />

–<br />

NO<br />

–<br />

2<br />

NO<br />

–<br />

3<br />

O<br />

2–<br />

2<br />

OH –<br />

PO 4<br />

3–<br />

SCN –<br />

SO 3<br />

2–<br />

permanganate<br />

nitrite<br />

nitrate<br />

peroxide<br />

hydroxide<br />

phosphate<br />

thiocyanate<br />

sulfite<br />

ClO 2<br />

–<br />

chlorite<br />

SO 4<br />

2–<br />

sulfate<br />

ClO 3<br />

–<br />

chlorate<br />

HSO 4<br />

–<br />

hydrogen sulfate<br />

ClO 4<br />

–<br />

perchlorate<br />

S 2<br />

O 3<br />

2–<br />

thiosulfate<br />

Table F<br />

Solubility Guidelines for Aqueous Solutions<br />

Ions That Form<br />

Soluble Compounds<br />

Group 1 ions<br />

(Li + , Na + , etc.)<br />

ammonium (NH 4 + )<br />

nitrate (NO 3 – )<br />

acetate (C 2<br />

H 3<br />

O 2 – or<br />

CH 3<br />

COO – )<br />

hydrogen carbonate<br />

(HCO 3 – )<br />

chlorate (ClO 3 – )<br />

halides (Cl – , Br – , I – )<br />

Exceptions<br />

when combined with<br />

Ag + , Pb 2+ , or Hg 2<br />

2+<br />

sulfates (SO 4 2– ) when combined with Ag + ,<br />

Ca 2+ , Sr 2+ , Ba 2+ , or Pb 2+<br />

Ions That Form<br />

Insoluble Compounds*<br />

Exceptions<br />

carbonate (CO 3 2– ) when combined with Group 1<br />

ions or ammonium (NH 4 + )<br />

chromate (CrO 4 2– ) when combined with Group 1<br />

ions, Ca 2+ , Mg 2+ , or<br />

ammonium (NH 4 + )<br />

phosphate (PO 4 3– ) when combined with Group 1<br />

ions or ammonium (NH 4 + )<br />

sulfide (S 2– ) when combined with Group 1<br />

ions or ammonium (NH 4 + )<br />

hydroxide (OH – ) when combined with Group 1<br />

ions, Ca 2+ , Ba 2+ , Sr 2+ , or<br />

ammonium (NH 4 + )<br />

*compounds having very low solubility in H 2 O<br />

R2


150.<br />

140.<br />

Table G<br />

Solubility Curves at Standard Pressure<br />

KI<br />

NaNO 3<br />

130.<br />

120.<br />

KNO 3<br />

110.<br />

100.<br />

Solubility (g solute/100. g H 2<br />

O)<br />

90.<br />

80.<br />

70.<br />

60.<br />

HCl<br />

NH 4<br />

Cl<br />

KCl<br />

50.<br />

40.<br />

30.<br />

NaCl<br />

KClO 3<br />

NH 3<br />

20.<br />

10.<br />

SO 2<br />

0<br />

0 10. 20. 30. 40. 50. 60. 70. 80. 90. 100.<br />

Temperature (°C)<br />

R3


Table H<br />

Vapor Pressure of Four Liquids<br />

200.<br />

propanone<br />

ethanol<br />

150.<br />

water<br />

Vapor Pressure (kPa)<br />

100.<br />

101.3 kPa<br />

ethanoic<br />

acid<br />

50.<br />

0<br />

0 25 50. 75 100. 125<br />

R4


Table I<br />

Heats of Reaction at 101.3 kPa and 298 K<br />

Reaction<br />

ΔH (kJ)*<br />

CH 4<br />

(g) + 2O 2<br />

(g) CO 2<br />

(g) + 2H 2<br />

O() –890.4<br />

C 3<br />

H 8<br />

(g) + 5O 2<br />

(g) 3CO 2<br />

(g) + 4H 2<br />

O() –2219.2<br />

2C 8<br />

H 18<br />

() + 25O 2<br />

(g) 16CO 2<br />

(g) + 18H 2<br />

O() –10943<br />

2CH 3<br />

OH() + 3O 2<br />

(g) 2CO 2<br />

(g) + 4H 2<br />

O() –1452<br />

C 2<br />

H 5<br />

OH() + 3O 2<br />

(g) 2CO 2<br />

(g) + 3H 2<br />

O() –1367<br />

C 6<br />

H 12<br />

O 6<br />

(s) + 6O 2<br />

(g) 6CO 2<br />

(g) + 6H 2<br />

O() –2804<br />

2CO(g) + O 2<br />

(g) 2CO 2<br />

(g) –566.0<br />

C(s) + O 2<br />

(g) CO 2<br />

(g) –393.5<br />

4Al(s) + 3O 2<br />

(g) 2Al 2<br />

O 3<br />

(s) –3351<br />

N 2<br />

(g) + O 2<br />

(g) 2NO(g) +182.6<br />

N 2<br />

(g) + 2O 2<br />

(g) 2NO 2<br />

(g) +66.4<br />

2H 2<br />

(g) + O 2<br />

(g) 2H 2<br />

O(g) –483.6<br />

2H 2<br />

(g) + O 2<br />

(g) 2H 2<br />

O() –571.6<br />

N 2<br />

(g) + 3H 2<br />

(g) 2NH 3<br />

(g) –91.8<br />

2C(s) + 3H 2<br />

(g) C 2<br />

H 6<br />

(g) –84.0<br />

2C(s) + 2H 2<br />

(g) C 2<br />

H 4<br />

(g) +52.4<br />

2C(s) + H 2<br />

(g) C 2<br />

H 2<br />

(g) +227.4<br />

H 2<br />

(g) + I 2<br />

(g) 2HI(g) +53.0<br />

KNO 3<br />

(s) H 2 O K + (aq) + NO 3 – (aq) +34.89<br />

NaOH(s) H 2 O Na + (aq) + OH – (aq) –44.51<br />

NH 4<br />

Cl(s) H 2 O NH 4 + (aq) + Cl – (aq) +14.78<br />

NH 4<br />

NO 3<br />

(s) H 2 O NH 4 + (aq) + NO 3 – (aq) +25.69<br />

NaCl(s) H 2 O Na + (aq) + Cl – (aq) +3.88<br />

LiBr(s) H 2 O Li + (aq) + Br – (aq) –48.83<br />

H + (aq) + OH – (aq) H 2<br />

O() –55.8<br />

*The ΔH values are based on molar quantities represented in the equations.<br />

A minus sign indicates an exothermic reaction.<br />

Most<br />

Active<br />

Least<br />

Active<br />

Table J<br />

Activity Series**<br />

Metals Nonmetals Most<br />

Active<br />

Li<br />

Rb<br />

K<br />

Cs<br />

Ba<br />

Sr<br />

Ca<br />

Na<br />

Mg<br />

Al<br />

Ti<br />

Mn<br />

Zn<br />

Cr<br />

Fe<br />

Co<br />

Ni<br />

Sn<br />

Pb<br />

H 2<br />

Cu<br />

Ag<br />

Au<br />

F 2<br />

Cl 2<br />

Br 2<br />

I 2<br />

**Activity Series is based on the hydrogen<br />

standard. H 2 is not a metal.<br />

Least<br />

Active<br />

R5


Table K<br />

Common Acids<br />

Table N<br />

Selected Radioisotopes<br />

HCl(aq)<br />

Formula<br />

HNO 2<br />

(aq)<br />

HNO 3<br />

(aq)<br />

H 2<br />

SO 3<br />

(aq)<br />

H 2<br />

SO 4<br />

(aq)<br />

H 3<br />

PO 4<br />

(aq)<br />

H 2<br />

CO 3<br />

(aq)<br />

or<br />

CO 2<br />

(aq)<br />

CH 3<br />

COOH(aq)<br />

or<br />

HC 2<br />

H 3<br />

O 2<br />

(aq)<br />

Name<br />

hydrochloric acid<br />

nitrous acid<br />

nitric acid<br />

sulfurous acid<br />

sulfuric acid<br />

phosphoric acid<br />

carbonic acid<br />

ethanoic acid<br />

(acetic acid)<br />

Nuclide Half-Life Decay<br />

Mode<br />

Nuclide<br />

Name<br />

198 Au 2.695 d β – gold-198<br />

14 C 5715 y β – carbon-14<br />

37 Ca 182 ms β + calcium-37<br />

60 Co 5.271 y β – cobalt-60<br />

137 Cs 30.2 y β – cesium-137<br />

53 Fe 8.51 min β + iron-53<br />

220 Fr 27.4 s α francium-220<br />

3 H 12.31 y β – hydrogen-3<br />

131 I 8.021 d β – iodine-131<br />

37 K 1.23 s β + potassium-37<br />

42 K 12.36 h β – potassium-42<br />

Table L<br />

Common Bases<br />

85 Kr 10.73 y β – krypton-85<br />

16 N 7.13 s β – nitrogen-16<br />

Formula<br />

NaOH(aq)<br />

KOH(aq)<br />

Ca(OH) 2<br />

(aq)<br />

NH 3<br />

(aq)<br />

Name<br />

sodium hydroxide<br />

potassium hydroxide<br />

calcium hydroxide<br />

aqueous ammonia<br />

19 Ne 17.22 s β + neon-19<br />

32 P 14.28 d β – phosphorus-32<br />

239 Pu 2.410 × 10 4 y α plutonium-239<br />

226 Ra 1599 y α radium-226<br />

222 Rn 3.823 d α radon-222<br />

90 Sr 29.1 y β – strontium-90<br />

Table M<br />

Common Acid–Base Indicators<br />

Approximate<br />

Indicator pH Range Color<br />

for Color Change<br />

Change<br />

methyl orange 3.1–4.4 red to yellow<br />

bromthymol blue 6.0–7.6 yellow to blue<br />

phenolphthalein 8–9 colorless to pink<br />

litmus 4.5–8.3 red to blue<br />

bromcresol green 3.8–5.4 yellow to blue<br />

thymol blue 8.0–9.6 yellow to blue<br />

99 Tc 2.13 × 10 5 y β – technetium-99<br />

232 Th 1.40 × 10 10 y α thorium-232<br />

233 U 1.592 × 10 5 y α uranium-233<br />

235 U 7.04 × 10 8 y α uranium-235<br />

238 U 4.47 × 10 9 y α uranium-238<br />

Source: CRC Handbook of Chemistry and Physics, 91 st ed., 2010–2011,<br />

CRC Press<br />

Source: The Merck Index, 14 th ed., 2006, Merck Publishing Group<br />

R6


Table O<br />

Symbols Used in Nuclear Chemistry<br />

Name Notation Symbol<br />

alpha particle<br />

4<br />

2<br />

He or 4 2 α α<br />

beta particle<br />

0<br />

–1<br />

e or 0<br />

–1 β β–<br />

gamma radiation<br />

0<br />

0<br />

γ γ<br />

neutron<br />

1<br />

0<br />

n n<br />

proton<br />

1<br />

1<br />

H or 1 1 p p<br />

positron<br />

0<br />

+1<br />

e or 0<br />

+1 β β+<br />

Table P<br />

Organic Prefixes<br />

Prefix<br />

meth- 1<br />

eth- 2<br />

prop- 3<br />

but- 4<br />

pent- 5<br />

hex- 6<br />

hept- 7<br />

oct- 8<br />

non- 9<br />

dec- 10<br />

Number of<br />

Carbon Atoms<br />

Table Q<br />

Homologous Series of Hydrocarbons<br />

Name General Examples<br />

Formula Name Structural Formula<br />

R7<br />

alkanes C n<br />

H 2n+2<br />

ethane<br />

alkenes C n<br />

H 2n<br />

ethene<br />

alkynes C n<br />

H 2n–2<br />

ethyne<br />

Note: n = number of carbon atoms<br />

H H<br />

H C C H<br />

H H<br />

H<br />

H<br />

C C<br />

H<br />

H<br />

H C C H


Table R<br />

Organic Functional Groups<br />

Class of<br />

Compound<br />

Functional<br />

Group<br />

General<br />

Formula<br />

Example<br />

halide<br />

(halocarbon)<br />

F (fluoro-)<br />

Cl (chloro-)<br />

Br (bromo-)<br />

I (iodo-)<br />

R X<br />

(X represents<br />

any halogen)<br />

CH 3<br />

CHClCH 3<br />

2-chloropropane<br />

alcohol<br />

OH<br />

R<br />

OH<br />

CH 3<br />

CH 2<br />

CH 2<br />

OH<br />

1-propanol<br />

ether<br />

O<br />

R O R′<br />

CH 3<br />

OCH 2<br />

CH 3<br />

methyl ethyl ether<br />

aldehyde<br />

O<br />

C H<br />

R<br />

O<br />

C H<br />

O<br />

CH 3<br />

CH 2<br />

C H<br />

propanal<br />

ketone<br />

O<br />

C<br />

O<br />

R C R′<br />

O<br />

CH 3<br />

CCH 2<br />

CH 2<br />

CH 3<br />

2-pentanone<br />

organic acid<br />

O<br />

C OH<br />

R<br />

O<br />

C OH<br />

O<br />

CH 3<br />

CH 2<br />

C OH<br />

propanoic acid<br />

ester<br />

O<br />

C O<br />

O<br />

R C O R′<br />

O<br />

CH 3<br />

CH 2<br />

COCH 3<br />

methyl propanoate<br />

amine<br />

N<br />

R<br />

R′<br />

N R′′<br />

CH 3<br />

CH 2<br />

CH 2<br />

NH 2<br />

1-propanamine<br />

amide<br />

O<br />

C NH<br />

R<br />

O R′<br />

C NH<br />

O<br />

CH 3<br />

CH 2<br />

C NH 2<br />

propanamide<br />

Note: R represents a bonded atom or group of atoms.<br />

R8


0<br />

6.941<br />

+1<br />

Li<br />

3<br />

2-1<br />

Na<br />

39.0983<br />

K +1<br />

19<br />

2-8-8-1<br />

85.4678 +1<br />

Rb<br />

Cs<br />

(223)<br />

Fr<br />

87<br />

-18-32-18-8-1<br />

+1<br />

Ra<br />

88<br />

-18-32-18-8-2<br />

39<br />

138.9055<br />

La<br />

57<br />

2-8-18-18-9-2<br />

+2 (227)<br />

Ac<br />

89<br />

-18-32-18-9-2<br />

47.867<br />

Ti<br />

22<br />

2-8-10-2<br />

91.224<br />

Zr<br />

40<br />

2-8-18-10-2<br />

+3 178.49<br />

Hf<br />

72<br />

*18-32-10-2<br />

+3 (261)<br />

Rf<br />

104<br />

+2<br />

+3<br />

+4<br />

+4<br />

+4<br />

50.9415<br />

V<br />

23<br />

2-8-11-2<br />

+2<br />

+3<br />

+4<br />

+5<br />

51.996<br />

Cr<br />

24<br />

2-8-13-1<br />

95.94<br />

Mo<br />

42<br />

2-8-18-13-1<br />

183.84<br />

W<br />

74<br />

-18-32-12-2<br />

+2<br />

+3<br />

+6<br />

+6<br />

+6<br />

54.9380<br />

Mn<br />

25<br />

2-8-13-2<br />

+2<br />

+3<br />

+4<br />

+7<br />

55.845<br />

Fe<br />

26<br />

2-8-14-2<br />

+2<br />

+3 58.9332<br />

Co<br />

27<br />

2-8-15-2<br />

+2<br />

+3<br />

58.693<br />

Ni<br />

28<br />

2-8-16-2<br />

+2<br />

+3 63.546 Cu<br />

2-8-18-1<br />

107.868<br />

Ag<br />

47<br />

2-8-18-18-1<br />

79<br />

+1<br />

+2<br />

+1<br />

65.409<br />

Zn<br />

30<br />

2-8-18-2<br />

10.81<br />

+3 12.011<br />

B<br />

5<br />

2-3<br />

26.98154<br />

Al<br />

13<br />

2-8-3<br />

+2 69.723<br />

Ga<br />

31<br />

2-8-18-3<br />

+3<br />

+3<br />

–4<br />

+2<br />

+4<br />

C<br />

6<br />

2-4<br />

28.0855<br />

Si<br />

14<br />

2-8-4<br />

72.64<br />

Ge<br />

32<br />

2-8-18-4<br />

Pb<br />

–4<br />

+2<br />

+4<br />

+2<br />

+4<br />

74.9216<br />

As<br />

33<br />

2-8-18-5<br />

Sb<br />

–3<br />

+3<br />

15.9994 O<br />

–2 18.9984<br />

8<br />

2-6 2-7<br />

78.96<br />

Se<br />

34<br />

2-8-18-6<br />

127.60<br />

Te<br />

52<br />

2-8-18-18-6<br />

(209)<br />

Po<br />

84<br />

-18-32-18-6<br />

–2<br />

+4<br />

+6<br />

–2<br />

+4<br />

+6<br />

+2<br />

+4<br />

F<br />

79.904<br />

Br<br />

35<br />

2-8-18-7<br />

126.904<br />

l<br />

53<br />

2-8-18-18-7<br />

(210)<br />

At<br />

85<br />

-18-32-18-7<br />

( ? )<br />

Uus<br />

117<br />

4.00260 0<br />

He<br />

2<br />

2<br />

–1 20.180<br />

Ne<br />

10<br />

2-8<br />

0<br />

22.98977<br />

11<br />

2-8-1<br />

1<br />

1.00794 +1<br />

–1<br />

H<br />

1<br />

1<br />

1<br />

37<br />

2-8-18-8-1<br />

–1<br />

+1<br />

+5<br />

–1<br />

+1<br />

+5<br />

+7<br />

83.798<br />

Kr<br />

36<br />

2-8-18-8<br />

131.29<br />

Xe<br />

54<br />

2-8-18-18-8<br />

(222)<br />

Rn<br />

86<br />

-18-32-18-8<br />

0<br />

+2<br />

0<br />

+2<br />

+4<br />

+6<br />

0<br />

132.905<br />

55<br />

2-8-18-18-8-1<br />

Symbol<br />

Relative atomic masses are based<br />

Group on 12 C = 12 (exact)<br />

Group<br />

2<br />

13 14 15 16 17 18<br />

Atomic Number<br />

+1<br />

+1<br />

9.01218 +2<br />

Be<br />

4<br />

2-2<br />

24.305<br />

Mg<br />

12<br />

2-8-2<br />

40.08<br />

Ca<br />

20<br />

2-8-8-2<br />

87.62<br />

Sr<br />

38<br />

2-8-18-8-2<br />

137.33<br />

Ba<br />

56<br />

2-8-18-18-8-2<br />

(226)<br />

+2<br />

+2<br />

+2<br />

+2<br />

3<br />

44.9559<br />

Sc<br />

21<br />

2-8-9-2<br />

88.9059<br />

Y<br />

2-8-18-9-2<br />

+3<br />

+3<br />

4<br />

KEY<br />

92.9064<br />

Nb +3<br />

+5<br />

41<br />

2-8-18-12-1<br />

180.948<br />

Ta<br />

73<br />

-18-32-11-2<br />

(262)<br />

105<br />

5<br />

Periodic Table of the Elements<br />

Atomic Mass<br />

Electron Configuration<br />

+4<br />

Db<br />

+5<br />

6<br />

(266)<br />

Sg<br />

106<br />

12.011 2-4<br />

–4<br />

6<br />

C<br />

+2<br />

+4<br />

(98)<br />

Tc<br />

43<br />

2-8-18-13-2<br />

186.207<br />

Re<br />

75<br />

-18-32-13-2<br />

(272)<br />

Bh<br />

107<br />

7<br />

Group<br />

+4<br />

+6<br />

+7<br />

+4<br />

+6<br />

+7<br />

8<br />

101.07<br />

Ru<br />

44<br />

2-8-18-15-1<br />

190.23<br />

Os<br />

76<br />

-18-32-14-2<br />

(277)<br />

Hs<br />

108<br />

+3<br />

+3<br />

+4<br />

Selected Oxidation States<br />

Note: Numbers in parentheses<br />

are mass numbers of the most<br />

stable or common isotope.<br />

9<br />

102.906<br />

Rh<br />

45<br />

2-8-18-16-1<br />

192.217<br />

Ir<br />

77<br />

-18-32-15-2<br />

(276)<br />

Mt<br />

109<br />

+3<br />

+3<br />

+4<br />

106.42<br />

Pd<br />

46<br />

2-8-18-18<br />

195.08<br />

Pt<br />

78<br />

-18-32-17-1<br />

+2<br />

+4<br />

+2<br />

+4<br />

196.967<br />

Au<br />

-18-32-18-1<br />

(281)<br />

Ds (280) Rg<br />

110<br />

10<br />

29<br />

111<br />

11 12<br />

+1<br />

+3<br />

112.41<br />

Cd<br />

48<br />

2-8-18-18-2<br />

200.59<br />

Hg<br />

80<br />

-18-32-18-2<br />

(285)<br />

Cn<br />

112<br />

+2 114.818<br />

In<br />

+1<br />

+2<br />

49<br />

2-8-18-18-3<br />

204.383<br />

Tl<br />

81<br />

-18-32-18-3<br />

(284)<br />

Uut<br />

113**<br />

+3<br />

+1<br />

+3<br />

118.71<br />

Sn<br />

50<br />

2-8-18-18-4<br />

207.2<br />

82<br />

-18-32-18-4<br />

(289)<br />

Uuq<br />

114<br />

+2<br />

+4<br />

+2<br />

+4<br />

14.0067 –3<br />

–2<br />

N<br />

–1<br />

7<br />

2-5<br />

30.97376<br />

P<br />

15<br />

2-8-5<br />

121.760<br />

51<br />

2-8-18-18-5<br />

208.980<br />

Bi<br />

83<br />

-18-32-18-5<br />

(288)<br />

Uup<br />

115<br />

+1<br />

+2<br />

+3<br />

+4<br />

+5<br />

–3<br />

+3<br />

+5<br />

+5<br />

–3<br />

+3<br />

+5<br />

+3<br />

+5<br />

32.065<br />

S<br />

16<br />

2-8-6<br />

(292)<br />

Uuh<br />

116<br />

–2<br />

+4<br />

+6<br />

35.453<br />

Cl<br />

17<br />

2-8-7<br />

–1<br />

+1<br />

+5<br />

+7<br />

39.948<br />

Ar<br />

18<br />

2-8-8<br />

18<br />

(294)<br />

Uuo<br />

118<br />

140.116<br />

Ce<br />

58<br />

232.038<br />

Th<br />

90<br />

+3<br />

+4<br />

140.908<br />

Pr +3<br />

59<br />

144.24<br />

Nd<br />

60<br />

+4 231.036<br />

Pa +4 238.029 +5<br />

U +3<br />

+4<br />

+5<br />

+6<br />

91<br />

92<br />

+3<br />

(145)<br />

Pm<br />

61<br />

+3<br />

150.36<br />

Sm<br />

62<br />

+2<br />

+3<br />

151.964<br />

Eu<br />

63<br />

+2<br />

+3<br />

157.25<br />

Gd<br />

64<br />

+3<br />

158.925<br />

(237)Np (244) Pu (243) Am (247) Cm +3 (247) Bk +3<br />

+3<br />

+4<br />

+5<br />

+6<br />

93 94<br />

+3<br />

+4<br />

+5<br />

+6<br />

65<br />

+3<br />

+4<br />

+5<br />

+6<br />

95 96 97<br />

Tb<br />

+3<br />

+4<br />

162.500<br />

Dy<br />

66<br />

(251)<br />

+3<br />

164.930<br />

Ho<br />

67<br />

+3<br />

167.259<br />

Er<br />

68<br />

Cf +3 (252) Es (257) Fm<br />

100<br />

98 99<br />

+3<br />

+3<br />

+3<br />

168.934<br />

Tm +3<br />

69<br />

(258)<br />

Md<br />

101<br />

+2<br />

+3<br />

173.04<br />

Yb<br />

70<br />

(259)<br />

No<br />

102<br />

+2<br />

+3<br />

+2<br />

+3<br />

174.9668<br />

Lu<br />

71<br />

(262)<br />

Lr<br />

103<br />

+3<br />

+3<br />

*denotes the presence of (2-8-) for elements 72 and above<br />

**The systematic names and symbols for elements of atomic numbers 113 and above<br />

will be used until the approval of trivial names by IUPAC.<br />

Source: CRC Handbook of Chemistry and Physics, 91 st ed., 2010–2011, CRC Press<br />

9<br />

R9<br />

Period<br />

1<br />

2<br />

3<br />

4<br />

5<br />

6<br />

7


Table S<br />

Properties of Selected Elements<br />

First<br />

Atomic Symbol Name Ionization<br />

Electro- Melting Boiling* Density** Atomic<br />

Number Energy negativity Point Point (g/cm 3 ) Radius<br />

(kJ/mol) (K) (K) (pm)<br />

1 H hydrogen 1312 2.2 14 20. 0.000082 32<br />

2 He helium 2372 — — 4 0.000164 37<br />

3 Li lithium 520. 1.0 454 1615 0.534 130.<br />

4 Be beryllium 900. 1.6 1560. 2744 1.85 99<br />

5 B boron 801 2.0 2348 4273 2.34 84<br />

6 C carbon 1086 2.6 — — .— 75<br />

7 N nitrogen 1402 3.0 63 77 0.001145 71<br />

8 O oxygen 1314 3.4 54 90. 0.001308 64<br />

9 F fluorine 1681 4.0 53 85 0.001553 60.<br />

10 Ne neon 2081 — 24 27 0.000825 62<br />

11 Na sodium 496 0.9 371 1156 0.97 160.<br />

12 Mg magnesium 738 1.3 923 1363 1.74 140.<br />

13 Al aluminum 578 1.6 933 2792 2.70 124<br />

14 Si silicon 787 1.9 1687 3538 2.3296 114<br />

15 P phosphorus (white) 1012 2.2 317 554 1.823 109<br />

16 S sulfur (monoclinic) 1000. 2.6 388 718 2.00 104<br />

17 Cl chlorine 1251 3.2 172 239 0.002898 100.<br />

18 Ar argon 1521 — 84 87 0.001633 101<br />

19 K potassium 419 0.8 337 1032 0.89 200.<br />

20 Ca calcium 590. 1.0 1115 1757 1.54 174<br />

21 Sc scandium 633 1.4 1814 3109 2.99 159<br />

22 Ti titanium 659 1.5 1941 3560. 4.506 148<br />

23 V vanadium 651 1.6 2183 3680. 6.0 144<br />

24 Cr chromium 653 1.7 2180. 2944 7.15 130.<br />

25 Mn manganese 717 1.6 1519 2334 7.3 129<br />

26 Fe iron 762 1.8 1811 3134 7.87 124<br />

27 Co cobalt 760. 1.9 1768 3200. 8.86 118<br />

28 Ni nickel 737 1.9 1728 3186 8.90 117<br />

29 Cu copper 745 1.9 1358 2835 8.96 122<br />

30 Zn zinc 906 1.7 693 1180. 7.134 120.<br />

31 Ga gallium 579 1.8 303 2477 5.91 123<br />

32 Ge germanium 762 2.0 1211 3106 5.3234 120.<br />

33 As arsenic (gray) 944 2.2 1090. — 5.75 120.<br />

34 Se selenium (gray) 941 2.6 494 958 4.809 118<br />

35 Br bromine 1140. 3.0 266 332 3.1028 117<br />

36 Kr krypton 1351 — 116 120. 0.003425 116<br />

37 Rb rubidium 403 0.8 312 961 1.53 215<br />

38 Sr strontium 549 1.0 1050. 1655 2.64 190.<br />

39 Y yttrium 600. 1.2 1795 3618 4.47 176<br />

40 Zr zirconium 640. 1.3 2128 4682 6.52 164<br />

R10


First<br />

Atomic Symbol Name Ionization<br />

Electro- Melting Boiling* Density** Atomic<br />

Number Energy negativity Point Point (g/cm 3 ) Radius<br />

(kJ/mol) (K) (K) (pm)<br />

41 Nb niobium 652 1.6 2750. 5017 8.57 156<br />

42 Mo molybdenum 684 2.2 2896 4912 10.2 146<br />

43 Tc technetium 702 2.1 2430. 4538 11 138<br />

44 Ru ruthenium 710. 2.2 2606 4423 12.1 136<br />

45 Rh rhodium 720. 2.3 2237 3968 12.4 134<br />

46 Pd palladium 804 2.2 1828 3236 12.0 130.<br />

47 Ag silver 731 1.9 1235 2435 10.5 136<br />

48 Cd cadmium 868 1.7 594 1040. 8.69 140.<br />

49 In indium 558 1.8 430. 2345 7.31 142<br />

50 Sn tin (white) 709 2.0 505 2875 7.287 140.<br />

51 Sb antimony (gray) 831 2.1 904 1860. 6.68 140.<br />

52 Te tellurium 869 2.1 723 1261 6.232 137<br />

53 I iodine 1008 2.7 387 457 4.933 136<br />

54 Xe xenon 1170. 2.6 161 165 0.005366 136<br />

55 Cs cesium 376 0.8 302 944 1.873 238<br />

56 Ba barium 503 0.9 1000. 2170. 3.62 206<br />

57 La lanthanum 538 1.1 1193 3737 6.15 194<br />

Elements 58–71 have been omitted.<br />

72 Hf hafnium 659 1.3 2506 4876 13.3 164<br />

73 Ta tantalum 728 1.5 3290. 5731 16.4 158<br />

74 W tungsten 759 1.7 3695 5828 19.3 150.<br />

75 Re rhenium 756 1.9 3458 5869 20.8 141<br />

76 Os osmium 814 2.2 3306 5285 22.587 136<br />

77 Ir iridium 865 2.2 2719 4701 22.562 132<br />

78 Pt platinum 864 2.2 2041 4098 21.5 130.<br />

79 Au gold 890. 2.4 1337 3129 19.3 130.<br />

80 Hg mercury 1007 1.9 234 630. 13.5336 132<br />

81 Tl thallium 589 1.8 577 1746 11.8 144<br />

82 Pb lead 716 1.8 600. 2022 11.3 145<br />

83 Bi bismuth 703 1.9 544 1837 9.79 150.<br />

84 Po polonium 812 2.0 527 1235 9.20 142<br />

85 At astatine — 2.2 575 — — 148<br />

86 Rn radon 1037 — 202 211 0.009074 146<br />

87 Fr francium 393 0.7 300. — — 242<br />

88 Ra radium 509 0.9 969 — 5 211<br />

89 Ac actinium 499 1.1 1323 3471 10. 201<br />

Elements 90 and above have been omitted.<br />

*boiling point at standard pressure<br />

**density of solids and liquids at room temperature and density of gases at 298 K and 101.3 kPa<br />

— no data available<br />

Source: CRC Handbook for Chemistry and Physics, 91 st ed., 2010–2011, CRC Press<br />

R11


Table T<br />

Important Formulas and Equations<br />

d = density<br />

m<br />

Density d = m = mass<br />

V<br />

V = volume<br />

Mole Calculations number of moles =<br />

given mass<br />

gram-formula mass<br />

measured value – accepted value<br />

Percent Error % error = × 100<br />

accepted value<br />

mass of part<br />

Percent Composition % composition by mass = × 100<br />

mass of whole<br />

mass of solute<br />

parts per million = × 1000000<br />

mass of solution<br />

Concentration<br />

molarity =<br />

moles of solute<br />

liter of solution<br />

Combined Gas Law<br />

P<br />

P = pressure<br />

1<br />

V 1<br />

P<br />

= 2<br />

V 2<br />

V = volume<br />

T 1<br />

T 2 T = temperature<br />

M A<br />

= molarity of H + M B<br />

= molarity of OH –<br />

Titration M A<br />

V A<br />

= M B<br />

V B<br />

V A<br />

= volume of acid V B<br />

= volume of base<br />

q = mCΔT q = heat H f<br />

= heat of fusion<br />

Heat q = mH f<br />

m = mass H v<br />

= heat of vaporization<br />

q = mH v<br />

C=specific heat capacity<br />

ΔT = change in temperature<br />

Temperature<br />

K = °C + 273<br />

K = kelvin<br />

°C = degree Celsius<br />

R12


Collier County <strong>CHEMISTRY</strong> EXAM FORMULA AND RESOURCE PACKET<br />

GENERAL<br />

D m V<br />

[ ExperimentalValue AcceptedVa lue]<br />

% error <br />

x100<br />

AcceptedVa lue<br />

% yield <br />

ExperimentalYield<br />

TheoreticalYield<br />

x100<br />

CONCENTRATIONS<br />

moles of solute<br />

M = Molarity <br />

liters of solution<br />

KEY<br />

P = pressure<br />

V = volume<br />

T = temperature<br />

n = number of moles<br />

m = mass<br />

M = molar mass (grams/mole)<br />

D = density<br />

KE = kinetic energy<br />

Avogadro’s Number = 6.02 x 10 23<br />

GASES, LIQUIDS, SOLUTIONS<br />

m = Molality <br />

M1V1 M2V2<br />

S1<br />

P1<br />

S 2<br />

P 2<br />

ACID/BASE<br />

pH = - log[H + ]<br />

[H + ]=10 -pH<br />

moles of solute<br />

kilograms of solvent<br />

<br />

Gas constant<br />

R 8.314 L kPa L atm L mmHg<br />

0.0821 62.4<br />

K mol K mol K mol<br />

1 atm = 760 mmHg = 760 torr = 101.3 kPa<br />

K = o C + 273<br />

o C = K - 273<br />

STP = Standard Temperature and Pressure = 0 o C<br />

and 1 atm<br />

P V<br />

1 1<br />

<br />

P2V<br />

2<br />

pOH = - log [OH - ]<br />

[OH - ]= 10 -pOH<br />

pH + pOH = 14<br />

Kw = [H + ] x [OH - ] = 1.0 x 10 -14 M 2<br />

V<br />

T<br />

1<br />

1<br />

P<br />

T<br />

1<br />

1<br />

V<br />

<br />

T<br />

P<br />

<br />

T<br />

2<br />

2<br />

2<br />

2<br />

Or V1T2 = V2T1<br />

Or P1T2 = P2T1<br />

THERMO<strong>CHEMISTRY</strong><br />

ΔH= mCΔT, where ΔT = T f - T<br />

P1V<br />

1<br />

T<br />

1<br />

<br />

P2V<br />

2<br />

T<br />

2<br />

Or<br />

P1V1T2=P2V2T1<br />

q = mCΔT<br />

PV<br />

nRT<br />

Specific Heat of Water = 4.18 J/g*˚C or 1.0 cal/g*˚C<br />

Specific Heat of Ice = 2.1 J/g*˚C or 0.5 cal/g*˚C<br />

Specific Heat of Steam = 2.0 J/g*˚C or 0.4 cal/g*˚C<br />

P<br />

Total<br />

P<br />

1<br />

P<br />

2<br />

Rate A<br />

Rate B<br />

...<br />

<br />

Molar MassB<br />

Molar MassA<br />

R13


<strong>CHEMISTRY</strong> EXAM FORMULA AND RESOURCE PACKET<br />

Solubility of Compounds at 25 o C and 1 atm<br />

acetate<br />

bromide<br />

carbonate<br />

chlorate<br />

chloride<br />

hydroxide<br />

iodide<br />

nitrate<br />

oxide<br />

perchlorate<br />

phosphate<br />

sulfate<br />

sulfide<br />

aluminum S S - S S I S S I S I S d<br />

ammonium S S S S S S S S - S S S S<br />

barium S S I S S S S S sS S I I d<br />

calcium S S I S S S S S sS S I sS I<br />

copper(II) S S - S S I S S I S I S I<br />

iron(II) S S I S S I S S I S I S I<br />

iron(III) S S - S S I S S I S I sS d<br />

lithium S S sS S S S S S S S sS S S<br />

magnesium S S I S S I S S I S I S d<br />

potassium S S S S S S S S S S S S S<br />

silver sS I I S I - I S I S I sS I<br />

sodium S S S S S S S S S S S S S<br />

strontium S S I S S S S S S S I I I<br />

zinc S S I S S I S S I S I S I<br />

S=soluble<br />

sS = slightly soluble in water<br />

I = insoluble in water<br />

d = decomposes in water<br />

- = no such compound<br />

R14


<strong>CHEMISTRY</strong> EXAM FORMULA AND RESOURCE PACKET<br />

Common Polyatomic Ions<br />

1- Charge 2- Charge 3- Charge<br />

Formula Name Formula Name Formula Name<br />

Dihydrogen<br />

Phosphate<br />

Hydrogen<br />

phosphate<br />

Phosphite<br />

Acetate Oxalate Phosphate<br />

Hydrogen<br />

sulfite<br />

Sulfite<br />

Hydrogen<br />

sulfate<br />

Sulfate<br />

Hydrogen<br />

carbonate<br />

Carbonate<br />

Nitrite Chromate 1+ Charge<br />

Nitrate Dichromate Formula Name<br />

Cyanide Silicate Ammonium<br />

Hydroxide<br />

Permanganate<br />

Hypochlorite<br />

Chlorite<br />

Chlorate<br />

Perchlorate<br />

R15


Activity Series of Metals<br />

Name<br />

Symbol<br />

D<br />

Lithium<br />

Li<br />

e<br />

Potassium<br />

K<br />

c<br />

r<br />

Barium<br />

Ba<br />

e<br />

Calcium<br />

Ca<br />

a<br />

Sodium<br />

Na<br />

s<br />

i<br />

Magnesium<br />

Mg<br />

n<br />

Aluminum<br />

Al<br />

g<br />

Zinc<br />

Zn<br />

Iron<br />

Fe<br />

A<br />

c<br />

Nickel<br />

Ni<br />

t<br />

Tin<br />

Sn<br />

i<br />

v<br />

Lead<br />

Pb<br />

i<br />

(Hydrogen)<br />

(H)*<br />

t<br />

Copper<br />

Cu<br />

y<br />

Mercury<br />

Hg<br />

Silver<br />

Ag<br />

Gold<br />

Au<br />

*Metals from Li to Na will replace H from acids and water; from Mg to<br />

Pb they will replace H from acids only.<br />

Decreasing<br />

Activity<br />

Activity Series of Nonmetal (Halogens)<br />

Name<br />

Symbol<br />

Fluorine F 2<br />

Chlorine Cl 2<br />

Bromine Br 2<br />

Iodine I 2<br />

R16

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