You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Chapter Two: Measurements<br />
Types of Measurements<br />
Suppose I ask the question:<br />
“How far is it from here to San Diego”<br />
Your answer must contain two pieces information<br />
A numerical value<br />
A unit<br />
Examples<br />
About 70 miles<br />
About 1.5 hours<br />
Length<br />
Distance from one location to another<br />
Distance between the “center” of one atom and one it is attached to<br />
Mass<br />
The quantity of matter in whatever it is we are measuring<br />
The more matter an object contains, the greater its mass<br />
Mass vs. Weight<br />
Weight measures the gravitational attraction between an object and the Earth (or moon,<br />
Jupiter, etc.)<br />
Weight is not the same as mass!<br />
Example: Consider a 1-ton (2,000 pound) rock on the surface of the Earth.<br />
How will its weight change if we move it to the moon To Jupiter<br />
How will its mass change<br />
Certain and Uncertain Digits<br />
In every measurement we take, digits we are sure of are said to be certain.<br />
A digit which must be estimated is said to be uncertain.<br />
In taking a measurement, first determine which digits you know without question.<br />
Then estimate exactly one uncertain digit.<br />
When & Where To Estimate<br />
Suppose you are taking a measurement with a ruler that has tenths (0.1) of a centimeter as<br />
its smallest markings.<br />
– You will estimate between the tenths mark, giving you an uncertain digit in the<br />
hundredths (0.01) place.<br />
Suppose you are using a thermometer which has whole degrees as its smallest markings.<br />
– You will estimate between each degree to the tenth of a degree.<br />
– Be careful not to drop the estimated digit!<br />
• If the thermometer is exactly at the 15 degree mark, report 15.0 degrees.<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Certain and Uncertain Digits<br />
In summary, in a given measurement, digits which are unambiguous are considered as<br />
certain.<br />
In any measurement there is always exactly one uncertain digit which results from estimation.<br />
It is always the right-most digit.<br />
In general, when taking a measurement on a device which measures to a given decimal<br />
place, estimate one digit to the right of this decimal place.<br />
– This would not apply for most electronic devices (like digital balances), which<br />
already estimate for you.<br />
Significant Figures<br />
Clearly, when we take measurements, there is a limit as to how accurate our data can be.<br />
For example, compare<br />
A bathroom scale<br />
A truck scale<br />
Significant figures are those values in a measurement which we can rely on for accuracy.<br />
The Rules for Determining Which Digits are Significant<br />
Non-zero digits<br />
– All non-zero digits (1-9) are always significant.<br />
– Example: How many significant digits are there in each value below<br />
48.9 7231.228<br />
Leading zeros are zeros to the left of the first non-zero digit.<br />
– Leading digits are not significant.<br />
– So, the zeros in 0.000825 and 0.0134 are not significant.<br />
– Why<br />
Enclosed zeros are zeros between other non-zero digits.<br />
– Enclosed zeros are always significant.<br />
– Examples of enclosed zeros:<br />
5,002 901.0802 101<br />
Trailing zeros are those zeros which come at the end (to the right) of a value.<br />
– Trailing zeros are significant if there is a decimal point in the value. If there is no<br />
decimal, the zeros are ambiguous and generally not considered significant.<br />
– Why<br />
Practice With “Sig Digs”<br />
How many significant digits do each of these values have<br />
462.0 1230 1230.<br />
0.030900 0.0005<br />
Calculations: Multiplication & Division<br />
When performing multiplication and division, count the number of significant digits in each<br />
part of the calculation.<br />
Determine which value has the least number of significant digits.<br />
Your answer will be rounded to that many significant digits.<br />
Examples<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Calculations: Addition and Subtraction<br />
When adding or subtracting, consider the value with the least precision. Your answer must<br />
extend to that level of precision.<br />
– For example, suppose you are adding 60.82 and 7.831<br />
• 60.82 goes to the hundredths place<br />
• 7.831 extends to the thousandths place<br />
• Therefore, your answer will round to the hundredths place.<br />
VERY IMPORTANT: Note that in adding and subtracting, the number of significant figures in<br />
the values does not matter!<br />
Example<br />
More Examples<br />
23.649 – 17.2 =<br />
8.75 + 9.414 + 105.32 =<br />
(6.834 × 8.32) – 3.45 =<br />
Scientific Notation<br />
Many measurements in chemistry involve numbers that are extremely large or small.<br />
Examples:<br />
• Number of atoms in a glass of water.<br />
• Distance between two atoms in a sugar molecule.<br />
• Scientific notation is a convenient mathematical notation which simplifies working with<br />
numbers of this magnitude.<br />
How it Works<br />
• Take the value under consideration, and move the decimal point after the first non-zero<br />
digit.<br />
Example: 582 5.82<br />
• Next, consider how many places the decimal was moved, and in what direction it was<br />
moved.<br />
The decimal moved 2 places to the left.<br />
Our new value is 10 2 , or 100 times, smaller than it was to begin with.<br />
• Undo this by multiplying by 10 to the power of how many places the decimal moved.<br />
This power is positive if the decimal moved to the left, negative if it moved to the right<br />
Our value is 5.82 × 10 2<br />
• Do not omit any significant digits!<br />
Examples<br />
Express these numbers in scientific notation.<br />
23,894. 0.004289<br />
20.000<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Calculations Involving Significant Digits<br />
• In calculations involving the multiplication and division of numbers expressed in scientific<br />
notation, it is helpful to remember the algebraic expressions:<br />
Examples<br />
Units of Measurement<br />
• Units are used in measurements to tell us<br />
– What type of measurement we are making<br />
• Distance<br />
• Time<br />
• Energy<br />
– The general magnitude of the measurement<br />
• Use feet to measure a person’s height<br />
• Use miles to measure distance between distant cities<br />
• Use light years to measure distance between distant galaxies.<br />
The English System<br />
• The English System of units includes many familiar units<br />
Inches, Feet, and Miles<br />
Liquid Ounces<br />
Pounds and Tons<br />
• Despite its popularity, the English System has a serious flaw<br />
SI Units<br />
• SI units (also called metric units) are based on powers of 10<br />
– There are 10 millimeters in a centimeter<br />
– There are 10 centimeters in a decimeter<br />
– There are 10 decimeters in a meter.<br />
• You only need to know what each prefix means to be able to easily convert from one unit<br />
to another.<br />
• These prefixes are used in all types of measurements, including distance, volume, time,<br />
and energy among many others.<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Converting Into Different Units<br />
• Consider the following well known equality:<br />
1 foot = 12 inches<br />
• Suppose we divide both sides by 12 inches:<br />
• Consider the following:<br />
“Convert 18.5 feet to inches.”<br />
• We need to get rid of feet, and end with inches.<br />
– Strategy: Divide by feet (in denominator), multiply by inches (in numerator)<br />
• Consider this example, using SI units:<br />
“How many centimeters are in 9.86 m”<br />
• Another example using the SI system.<br />
“How many nanoseconds (ns) are there in 2.83 milliseconds (ms)”<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Multiple Unit Conversions<br />
• In many measurements, such as in this problem, there are units in both the numerator<br />
and the denominator:<br />
“A car is traveling at 60. miles per hour. How fast is this in centimeters per<br />
second”<br />
A Side Note…<br />
• By now you have noticed that units can be factored (or divided out) just like numbers<br />
• You should also note that<br />
– Units also can be multiplied<br />
Ex. 2 ft × 2 ft = 4 (ft × ft) = 4 ft 2<br />
Ex. 3 ft. × 2 lbs. = 6 ft.·lbs. (read “foot pounds”)<br />
• You can only add and subtract measurements with the same units!<br />
– Before adding and subtracting, perform any unit conversions to make the<br />
measurements have the same units (of course, they must be the same type of<br />
measurement!).<br />
Area & Volume<br />
• Translating length to area involves squaring the units as well as the values which<br />
accompany them.<br />
• For example, what is the area of a square which is 5.0 cm on each side<br />
5.0 cm × 5.0 cm = 25 cm 2<br />
• Let’s convert that to square meters:<br />
• Common units of volume you should know<br />
Liter(L) – the SI unit of volume<br />
milliliter(mL) – another common unit<br />
Cubic centimeter (cm 3 or cc) – a unit equivalent to the milliliter<br />
1 mL = 1 cm 3 = 1 cc<br />
• Dealing with volumes involves a similar procedure to that of areas.<br />
A Volume Problem<br />
• A rectangular block is 14.6 in. by 7.2 in. by 6.8 in. What is its volume in cm 3 <br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
Density<br />
• Density (d) is the ratio between mass (m) and volume(V):<br />
density =<br />
mass<br />
volume<br />
• Units of density for liquids are usually g/mL.<br />
• For solids, we use the equivalent g/cm 3 .<br />
• If something has high density, then a small volume of it will have a large mass.<br />
– Ex. Which has greater mass, a liter of rocks or a liter of feathers<br />
Density Problems<br />
• The mass of an empty graduated cylinder is found to be 22.57 g. 7.25 mL of a liquid is<br />
added to it. The graduated cylinder and liquid have a combined mass of 30.79 g. What<br />
is the density of the liquid<br />
• A 73.43 g cube of gold is dropped into a graduated cylinder whose volume reads 27.8<br />
mL. After the cube sinks to the bottom, what volume reading will the graduated cylinder<br />
have Note that gold has density 19.3 g/cm 3 .<br />
Temperature<br />
• Temperature is a measurement of the average kinetic energy of a body.<br />
Kinetic Energy is the energy of motion, so the molecules in hot water are, on average,<br />
moving more rapidly than those in colder water.<br />
Note, temperature is not the same as heat!<br />
Units of Temperature<br />
• Fahrenheit (°F)<br />
– Commonly used to measure temperatures in the U.S., but not very practical for<br />
scientific use.<br />
• Celsius (°C)<br />
– Unit most commonly used in determining temperature in the laboratory.<br />
• Kelvin (K)<br />
7
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
– The SI unit of temperature.<br />
– 0 K is called “absolute zero.” It is impossible to for a system to have a temperature of<br />
0 K (or lower).<br />
The Temperature of the Freezing and Boiling Points of Water<br />
Temperature<br />
Scale<br />
Freezing Point<br />
Boiling Point<br />
°F 32 212<br />
°C 0 100<br />
K 273.15 373.15<br />
Converting Temperatures<br />
• To convert between Celsius and Kelvin, use the following relationship:<br />
T(in K) = T(in °C) + 273.15<br />
To convert between °C and °F, use the equation:<br />
°F = (1.8 × °C) + 32<br />
A Temperature Problem<br />
• The temperature in Paris is 23 °C. What is the equivalent temperature in Kelvin In<br />
Fahrenheit<br />
Accuracy & Precision in Measurements<br />
• If data is accurate, this means that the results obtained are close to the “true and correct”<br />
value(s).<br />
• If a group of measurements give data which are close in value, these measurements are<br />
said to be precise.<br />
8
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Two <strong>Notes</strong><br />
9
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Three <strong>Notes</strong><br />
Basic Concepts About Matter<br />
• <strong>Chemistry</strong> is the study of the properties and changes of matter<br />
• What exactly is matter<br />
◦ Matter is anything which has mass and takes up space (volume)<br />
◦ Examples of matter:<br />
• Sand (a solid)<br />
• Water (a liquid)<br />
• Air (a mixture of gases)<br />
How do we learn chemistry<br />
• <strong>Chemistry</strong> is an empirical science, meaning that it is based on the results of experiments.<br />
• In the lecture we will study theories and laws based on many years of observations and experiments.<br />
• In the laboratory we will verify many of these principles.<br />
A Conceptual Approach<br />
• During this course, we will focus on the fundamental concepts which define chemistry.<br />
• Specifically, we will often look at matter at the smallest level (the submicroscopic level) to try to<br />
reason why matter behaves the way it does on a larger, or macroscopic, scale.<br />
• This is an essential skill for the aspiring chemist; a good imagination is all you need to develop it!<br />
Atoms: A Brief Overview<br />
• Atoms are the most fundamental units of matter we consider in this course<br />
• All matter which we encounter in our daily lives contains an extremely large number of these tiny<br />
particles<br />
• There are many different types of atoms<br />
◦ Some common examples are hydrogen, oxygen, gold, and sodium<br />
• We will look closely at the structures of atoms at a later point in this course<br />
Molecules<br />
• Two or more atoms may join together to form a molecule<br />
• Molecules are held together by bonds<br />
◦ Specifically, these are called covalent bonds; more on these later!<br />
• A diatomic molecule is made up of exactly two atoms (which may be the same or different)<br />
Molecules<br />
Physical States of Matter<br />
• There are three common physical states of matter which we will consider in this class<br />
◦ Gases<br />
◦ Liquids<br />
◦ Solids<br />
• We compare the three states by asking two questions<br />
◦ Does the substance have a definite shape, or does it take the shape of its container<br />
◦ Does the substance have a definite volume<br />
Solids<br />
• Solids have a definite shape<br />
◦ They do not assume the shape of their container<br />
• Solids have a definite volume<br />
• The particles making up a solid<br />
◦ are close together<br />
◦ do not move about, but vibrate in place<br />
◦ tend to form organized patterns<br />
Page 1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Three <strong>Notes</strong><br />
Liquids<br />
• Liquids have an indefinite shape<br />
◦ They take the shape of their container<br />
• Liquids have a definite volume<br />
• The particles making up a liquid<br />
◦ are fairly close together, but not to the same extent as solids<br />
◦ move freely throughout the liquid<br />
◦ are not organized in any particular pattern<br />
Gases<br />
• Gases have an indefinite shape<br />
◦ Like liquids, they take the shape of their container<br />
• Gases have indefinite volume<br />
• The particles making up a gas<br />
◦ are generally far apart from one another<br />
◦ move freely throughout their container in a random fashion<br />
Classification of Matter<br />
• We classify matter as either a pure substance or a mixture<br />
• There are two types of pure substances<br />
◦ Elements<br />
◦ Compounds<br />
• There are two types of mixtures<br />
◦ Homogeneous mixtures<br />
◦ Heterogeneous mixtures<br />
Elements<br />
• A pure sample of an element contains only one type of atom<br />
◦ A sample of gold—an element—contains only gold atoms<br />
◦ Helium contains only helium atoms<br />
• There are over a hundred known elements<br />
• Each element is assigned a name and a symbol<br />
◦ Each symbol consists of one to three letters<br />
◦ The first letter of the symbol is always capitalized; any other letters are always written in lowercase<br />
• The symbols (and occasionally the names) are catalogued on the Periodic Table of the Elements<br />
Some Atomic Symbols<br />
H: Hydrogen O: Oxygen<br />
C: Carbon N: Nitrogen<br />
Na: Sodium<br />
Cl: Chlorine<br />
Cu: Copper<br />
K: Potassium<br />
• Note that some of these symbols are unusual!<br />
Elements<br />
• Some elements are generally only found as diatomic molecules<br />
• We will call these seven elements the diatomic elements<br />
H 2 N 2 O 2 F 2 Cl 2 Br 2 I 2<br />
Be sure you know these!<br />
Page 2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Three <strong>Notes</strong><br />
Compounds<br />
• Atoms come together in whole number ratios to form compounds.<br />
• The chemical formula lists the ratio of these elements in the compound.<br />
◦ Each unit of water contains two hydrogen atoms and one oxygen atom H 2 O<br />
◦ Other examples: NaCl, SiO 2 , C 6 H 12 O 6<br />
◦ This formula/ratio is always the same for a chemical compound<br />
◦ Different compounds may have the same formula.<br />
◦ The compound is said to have a definite composition<br />
Mixtures<br />
• The composition of a mixture is not fixed.<br />
◦ Consider salt water, a mixture of H 2 O and NaCl.<br />
• Is salt water always found in the same proportion The same atom-to-atom ratio<br />
• Mixtures can be classified into two types:<br />
◦ Homogeneous mixtures have all parts in the same state (gas, liquid or solid) and all parts must be<br />
mixed together.<br />
• If the parts of the mixture are visually inseparable, we will call the mixture homogeneous.<br />
◦ Heterogeneous mixtures are simply those which are not homogeneous.<br />
Separations<br />
• Mixtures can be separated by physical methods<br />
◦ A heterogeneous mixture of coffee grounds and water can be separated by filter paper<br />
◦ The water can be removed from a salt water solution (a homogeneous mixture) by boiling the<br />
water off. The salt will remain in the container.<br />
• Compounds can only be separated into their individual elements by chemical means (i.e. through the<br />
result of a chemical reaction)<br />
Mixtures<br />
• Ex. Are each of these mixtures homogeneous or heterogeneous Why<br />
◦ Vodka (a mixture of water and ethyl alcohol)<br />
◦ Cheerios in milk<br />
◦ A mixture of oil and water<br />
◦ A salt water solution<br />
• Note that the term solution is often used to refer to homogeneous mixtures, especially for<br />
compounds dissolved in water.<br />
Page 3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Three <strong>Notes</strong><br />
◦ Air<br />
◦ Dirty, dust-filled air<br />
Classification Problems<br />
• Classify each of these as an element, a compound, a homogeneous mixture, or a heterogeneous<br />
mixture.<br />
◦ Tap water<br />
◦ Steel (an alloy of several metals)<br />
• Note that alloys can be mixed in different proportions.<br />
◦ Helium<br />
◦ Mud<br />
◦ Carbon dioxide<br />
Properties of Matter<br />
• We can describe matter in two ways:<br />
◦ By its chemical properties, which describe how a type of matter interacts (or “reacts”) with another<br />
type of matter.<br />
• For example, hydrogen is able to react with oxygen to form water. Helium reacts with<br />
virtually nothing.<br />
◦ By its physical properties, which include all non-chemical properties.<br />
Page 4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Three <strong>Notes</strong><br />
• For example, water is a liquid at room temperature, freezes at 0 °C, has a density of 1.0 g/mL,<br />
and is both clear (we can see through it) and colorless.<br />
Changes of Matter<br />
• Common changes of matter are described in essentially the same way as properties are<br />
• A chemical change is a change which involves a chemical reaction<br />
◦ Bonds are formed and/or broken in a chemical change<br />
◦ The chemical substances you end with are fundamentally different than what you began with<br />
• A physical change is a change which does not involve a chemical reaction<br />
◦ All changes of state of a given substance are physical changes<br />
• Examples include ice melting and liquid water boiling<br />
• Classify each change as either a physical change or a chemical change<br />
◦ Gasoline evaporates off of the ground<br />
◦ A glass vase is shattered<br />
◦ Sodium reacts with chlorine, forming sodium chloride<br />
◦ Dry grass burns in a large fire<br />
Page 5
<strong>Chemistry</strong> <strong>120</strong><br />
Elements and Symbols You Must Know<br />
Group<br />
1A<br />
H<br />
Hydrogen<br />
You must memorize the symbols and names (with the correct spelling) for each element<br />
listed on this periodic table. I recommend making flashcards to help you in this.<br />
2A 3A 4A 5A 6A 7A<br />
He<br />
Helium<br />
8A<br />
Li<br />
Lithium<br />
Be<br />
Beryllium<br />
B<br />
Boron<br />
C<br />
Carbon<br />
N<br />
Nitrogen<br />
O<br />
Oxygen<br />
F<br />
Fluorine<br />
Ne<br />
Neon<br />
Na<br />
Sodium<br />
Mg<br />
Magnesium<br />
3B 4B 5B 6B 7B 8B 1B 2B<br />
Al<br />
Aluminum<br />
Si<br />
Silicon<br />
P<br />
Phosphorus<br />
S<br />
Sulfur<br />
Cl<br />
Chlorine<br />
Ar<br />
Argon<br />
K<br />
Potassium<br />
Ca<br />
Calcium<br />
Sc<br />
Scandium<br />
Ti<br />
Titanium<br />
V<br />
Vanadium<br />
Cr<br />
Chromium<br />
Mn<br />
Manganese<br />
Fe<br />
Iron<br />
Co<br />
Cobalt<br />
Ni<br />
Nickel<br />
Cu<br />
Copper<br />
Zn<br />
Zinc<br />
Ga<br />
Gallium<br />
Ge<br />
Germanium<br />
As<br />
Arsenic<br />
Se<br />
Selenium<br />
Br<br />
Bromine<br />
Kr<br />
Krypton<br />
Rb<br />
Rubidium<br />
Sr<br />
Strontium<br />
Pd<br />
Palladium<br />
Ag<br />
Silver<br />
Cd<br />
Cadmium<br />
Sn<br />
Tin<br />
Sb<br />
Antimony<br />
I<br />
Iodine<br />
Xe<br />
Xenon<br />
Cs<br />
Cesium<br />
Ba<br />
Barium<br />
W<br />
Tungsten<br />
Pt<br />
Platinum<br />
Au<br />
Gold<br />
Hg<br />
Mercury<br />
Pb<br />
Lead<br />
Bi<br />
Bismuth<br />
U<br />
Uranium
<strong>Chemistry</strong> <strong>120</strong><br />
Standard States of the Elements<br />
Group<br />
1A<br />
H 2<br />
Hydrogen<br />
This periodic table shows you the state (gas, liquid, or solid) of many important elements at room<br />
temperature. Notice that all metals and metalloids except mercury are solids at room temperature.<br />
The only two elements which are found as liquids are bromine and mercury. All the elements in the<br />
last group (8A) are gases. The rest are fairly easy to memorize. On this periodic table I have<br />
indicated the diatomic elements with their formulas; you will not see this on a "normal" periodic<br />
table. I have left the boxes of the elements which are not important in this course blank.<br />
2A 3A 4A 5A 6A 7A<br />
He<br />
Helium<br />
8A<br />
Li<br />
Lithium<br />
Be<br />
Beryllium<br />
Key: solid liquid gas<br />
B<br />
Boron<br />
C<br />
Carbon<br />
N 2<br />
Nitrogen<br />
O 2<br />
Oxygen<br />
F 2<br />
Fluorine<br />
Ne<br />
Neon<br />
Na<br />
Sodium<br />
Mg<br />
Magnesium<br />
3B 4B 5B 6B 7B 8B 1B 2B<br />
Al<br />
Aluminum<br />
Si<br />
Silicon<br />
P<br />
Phosphorus<br />
S<br />
Sulfur<br />
Cl 2<br />
Chlorine<br />
Ar<br />
Argon<br />
K<br />
Potassium<br />
Ca<br />
Calcium<br />
Sc<br />
Scandium<br />
Ti<br />
Titanium<br />
V<br />
Vanadium<br />
Cr<br />
Chromium<br />
Mn<br />
Manganese<br />
Fe<br />
Iron<br />
Co<br />
Cobalt<br />
Ni<br />
Nickel<br />
Cu<br />
Copper<br />
Zn<br />
Zinc<br />
Ga<br />
Gallium<br />
Ge<br />
Germanium<br />
As<br />
Arsenic<br />
Se<br />
Selenium<br />
Br 2<br />
Bromine<br />
Kr<br />
Krypton<br />
Rb<br />
Rubidium<br />
Sr<br />
Strontium<br />
Pd<br />
Palladium<br />
Ag<br />
Silver<br />
Cd<br />
Cadmium<br />
Sn<br />
Tin<br />
Sb<br />
Antimony<br />
I 2<br />
Iodine<br />
Xe<br />
Xenon<br />
Cs<br />
Cesium<br />
Ba<br />
Barium<br />
W<br />
Tungsten<br />
Pt<br />
Platinum<br />
Au<br />
Gold<br />
Hg<br />
Mercury<br />
Pb<br />
Lead<br />
Bi<br />
Bismuth<br />
U<br />
Uranium
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Four <strong>Notes</strong><br />
Chapter Four: Matter and Energy<br />
Matter<br />
Recall that matter<br />
Has mass<br />
Takes up space (i.e. has volume)<br />
Matter also has one of four states<br />
Gas<br />
Liquid<br />
Solid<br />
Plasma (We will not be concerned with the plasma state in this course!)<br />
States of Matter<br />
The states of matter are classified by two parameters<br />
Does it take the shape of its container<br />
Does it completely fill its container<br />
Gases<br />
Take the shape of their container<br />
Completely fill their container<br />
Liquids<br />
Take the shape of their container<br />
Do not fill their container completely<br />
Solids<br />
Do not take the shape of their container<br />
Do not fill their container completely<br />
Which state a substance is in depends on two factors: Temperature and Pressure<br />
Gases are comprised of molecules which generally are far apart from one another, and travel in<br />
random paths.<br />
The particles in liquids and solids are much closer together than those of gases<br />
The particles of solids are generally “stuck in place”, but are able to vibrate<br />
Liquid particles freely move across one another<br />
Changes of State<br />
Special terms are associated when matter changes from one state to another.<br />
You may be familiar with the term “freezing,” which describes a change from liquid to solid.<br />
Solid<br />
Liquid<br />
Gas<br />
4-1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Four <strong>Notes</strong><br />
Properties of Matter<br />
We can describe matter in two ways:<br />
By its chemical properties, which describe how a type of matter interacts (or “reacts”) with<br />
another type of matter.<br />
For example, hydrogen is able to react with oxygen to form water. Helium reacts with<br />
virtually nothing.<br />
By its physical properties, which include all non-chemical properties.<br />
For example, water is a liquid at room temperature, freezes at 0 °C, has a density of 1.0<br />
g/mL, and is both clear (we can see through it) and colorless.<br />
Changes of Matter<br />
Similarly, changes can be classified in the same way as properties:<br />
Chemical changes involve a rearrangement of atoms, producing chemical compounds that were<br />
not there before.<br />
When iron (Fe) is exposed to oxygen on a wet day, rust (Fe 2 O 3 ) is formed.<br />
Physical changes are those which do not involve a chemical change.<br />
Boiling water (liquid H 2 O changes to gaseous H 2 O), glass shattering, a chemical<br />
evaporating.<br />
Metals<br />
The metals include many elements found on the left side of the periodic table.<br />
Many metals are known for having the following properties<br />
They are malleable (meaning they are soft and easily shaped)<br />
They are ductile (they can be twisted and drawn into a wire)<br />
They can conduct both electricity and heat.<br />
They tend to be lustrous (shiny).<br />
All metals are solids at room temperatures except for mercury, which is a liquid.<br />
Nonmetals<br />
Nonmetals are generally found on the right side of the periodic table (except hydrogen, which is<br />
placed on the left).<br />
Their properties are generally the opposite of the metals.<br />
Those which are solids tend to be brittle.<br />
Most are poor conductors of electricity at room temperature (insulators) and do not<br />
conduct heat well.<br />
Some are gases at room temperature; others are solids. Bromine is the only other<br />
element which is a liquid.<br />
Metalloids<br />
Metalloids are found between the metals and the nonmetals on the periodic table.<br />
They include B, Si, Ge, As, Sb, and Te.<br />
The properties of the metalloids are often a cross between those of the metals and the<br />
nonmetals.<br />
All the metalloids listed are solids at room temperature.<br />
(I do not include Po and At with the metalloids. They are rather unstable and unimportant<br />
to our studies at this point.)<br />
4-2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Four <strong>Notes</strong><br />
The Law of Conservation of Mass<br />
One of the most fundamental statements about matter is described by this law, which states:<br />
“Matter can neither be created nor destroyed in any chemical process”<br />
Another consequence of this law is that one type of atom cannot be changed into another through<br />
a chemical reaction.<br />
If you start a chemical process with 10 million hydrogen atoms and 10 million oxygen<br />
atoms, then you will end the process with 10 million hydrogen atoms and 10 million<br />
oxygen atoms. ALWAYS!<br />
Energy<br />
Energy is an important subject in chemistry, as chemical reactions either give off or take in<br />
energy.<br />
The Law of Conservation of Energy states that “Energy can neither be created nor destroyed in a<br />
process.”<br />
Energy can be transferred between two systems in two ways<br />
As work (w), which we will consider as energy put to some specific use, like making a<br />
motor run.<br />
As heat (q), which will be random energy(not directed to some useful purpose), like that<br />
given off by your car’s engine.<br />
Any change in energy is just the sum of the work and heat changes.<br />
The SI unit of energy is the Joule (J). Other units include the kJ, and the calorie (cal)<br />
1 calorie = 4.184 Joules<br />
For example, suppose that burning a certain amount of gasoline produces 50 kJ of energy. If<br />
only 20 kJ of it goes into doing work in a car engine, the remaining 30 kJ must be lost as heat.<br />
Remember, energy cannot be destroyed!<br />
An exothermic process is one which gives off more heat than it takes in.<br />
For an exothermic reaction, q < 0.<br />
For example, consider burning gasoline.<br />
An endothermic process is one which brings in more heat than it gives off.<br />
For an endothermic reaction, q > 0.<br />
Specific Heat<br />
Some substances require more energy to raise their temperatures than others.<br />
For example, it requires much less energy to raise the temperature of 50. g of aluminum<br />
by 10 °C than it would to raise 50. g of water by the same amount.<br />
This difference is represented by a constant called the specific heat, c.<br />
Its units are J/(g ·°C) or cal/(g ·°C) .<br />
Transferring Heat<br />
The amount of heat (q) absorbed or given off by a substance when it changes temperature can<br />
be found using the following equation:<br />
q = m × ΔT × c<br />
m is the mass of the substance<br />
ΔT is the change in the temperature; it equals (final T – starting T)<br />
c is the specific heat of the substance<br />
Note that heat always flows from an area of high temperature to one of lower temperature!<br />
4-3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Four <strong>Notes</strong><br />
Example<br />
How much heat is required to raised the temperature of 50.0 g of aluminum from 32 °C to 47 °C<br />
The specific heat of aluminum is 0.215 cal/(g ·°C).<br />
A More Difficult Example<br />
A 50.0 g aluminum block is heated to 75 °C, then dropped into a sealed container containing 350.<br />
g of water at 15 °C. What will be the temperature of the block when it is finished cooling<br />
More On Conservation<br />
Note that in the last problem, heat was transferred from the aluminum to the water, but never<br />
destroyed.<br />
Einstein is credited with the famous equation:<br />
E = mc 2<br />
Where E is energy, m is mass, and c is a constant (the speed of light, not the specific heat!)<br />
This shows that matter can be converted to energy.<br />
More on Conservation<br />
Note however, this will not apply to chemical reactions. We see this with nuclear reactions.<br />
In this class, mass is always conserved.<br />
4-4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Four <strong>Notes</strong><br />
We can now state the Law of Conservation of Mass-Energy:<br />
“Mass and energy can neither be created nor destroyed in a process, though they may<br />
be interchanged.”<br />
Kinetic and Potential Energy<br />
Kinetic Energy (K.E.) is the energy of motion.<br />
The amount of K.E. an object has is described by the formula<br />
K.E. = ½mv 2<br />
where m is the object’s mass, and v is its velocity.<br />
Potential Energy is the energy of position.<br />
Objects may be in a “high energy” position, and can convert this potential energy to kinetic energy<br />
while moving to a “lower energy” position.<br />
Examples:<br />
4-5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Five <strong>Notes</strong><br />
Chapter Five: Atomic Theory and Structure<br />
Evolution of Atomic Theory<br />
• The ancient Greek scientist Democritus is often credited with developing the idea of the atom<br />
• Democritus proposed that matter was, on the smallest scale, composed of particles described<br />
as atomos, meaning “indivisible”<br />
• While atoms can in fact be broken down into smaller particles, the atoms of each element are<br />
distinct from each other, making them the fundamental unit of matter.<br />
Dalton’s Atomic Theory<br />
• Compiling experimental information available during his lifetime, John Dalton described an<br />
accurate picture of atoms in 1803 with his atomic theory.<br />
• Dalton’s Atomic Theory maintains that<br />
◦ All elements are made up of tiny, indivisible particles called atoms, which can be neither<br />
created nor destroyed in reactions.<br />
◦ Atoms of the same type of element are the same; those of different elements are<br />
different.<br />
◦ Atoms of different elements form compounds by combining in fixed, whole number ratios.<br />
• This is also called “The Law of Definite Proportions”<br />
◦ If the same elements combine to make more than one compound, there can be a<br />
different, but definite, atom ratio for each compound.<br />
• This is also called “The Law of Multiple Proportions”<br />
• In actuality, atoms combining in the same ratio can make different compounds.<br />
◦ A chemical reaction does not involve a fundamental change of the atoms themselves, but<br />
of the way they are combined together.<br />
Probing Further into Atomic Structure: The Electron<br />
• One of the three particles which make up all atoms is the electron<br />
• Benjamin Franklin observed that, when a cloth was rubbed across a glass rod, a charge was<br />
developed on each.<br />
• The charges, called positive (+) and negative (-), show an attractive force between opposites<br />
and repulsion between identical charges.<br />
The Atom: A Complete Picture<br />
• Each atom contains at its core a nucleus, a region of positive charge.<br />
• Positively charged particles, called protons, are contained in the nucleus.<br />
• Electrons (negatively charged particles) “orbit” around the nucleus throughout the atom.<br />
• Later experiments also confirmed that all atoms except hydrogen must contain one or more<br />
neutral (non-charged) particles called neutrons.<br />
• Note that the protons and neutrons are each almost 2,000 times more massive than an<br />
electron; therefore, most of the mass of an atom is in the nucleus.<br />
• The protons and neutrons are called the nucleons.<br />
Characteristics of an Atom<br />
• The number of protons in an atom is called the elements atomic number, which is symbolized<br />
by Z.<br />
• The number Z indicates which type of element that atom represents.<br />
• These values are found in order on the periodic table.<br />
• Example: Which element contains 5 protons 10 34<br />
5-1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Five <strong>Notes</strong><br />
• Recall that the “Law of Conservation of Mass” indicated that atoms cannot be changed in<br />
different elements by chemical means.<br />
• So, protons are never “changed around” in a chemical reaction!<br />
Characteristics of an Atom<br />
• Atoms that have no charge must have the same amount of positive charge as negative<br />
charge.<br />
• Therefore, the number of electrons in an atom is equal to the number of protons in an atom<br />
(Z) for any neutral atom.<br />
• Atoms which contain more or less electrons than protons therefore must have a charge.<br />
These are called ions.<br />
Ions: A Lesson in Thinking Backwards<br />
• Suppose an ion has exactly one more electron than it does protons.<br />
◦ Will the ion be positively or negatively charged<br />
• What if an atom lost two electrons<br />
◦ Will the ion be positively or negatively charged<br />
• For each electron an ion has more than it does protons, we indicate it with a – as a<br />
superscript.<br />
• For each electron an ion has less than it does protons, we indicate it with a + as a<br />
superscript.<br />
Examples of Ions<br />
• A bromine atom normally has_______protons and________electrons.<br />
• Suppose we add exactly one electron; now we have________protons and_______electrons.<br />
• We symbolize this as Br - (or Br 1- ).<br />
• An aluminum atom normally has________protons and_________electrons.<br />
• Suppose the atom loses three electrons.<br />
• We symbolize this ion as Al 3+ .<br />
• Note that losing electrons is indicated with +, and gaining electrons is indicated with -.<br />
Neutrons and Isotopes<br />
• The number of neutrons in an atom cannot be easily predicted or found on the periodic table.<br />
• Atoms of the same element (i.e. have the same number of protons) can have different<br />
numbers of neutrons. They are called isotopes of one another.<br />
• Examples:<br />
◦ A carbon atom must contain 6 protons, but it may contain 6, 7, or 8 neutrons.<br />
◦ Almost all hydrogen atoms contain zero neutrons. The isotopes of hydrogen which<br />
contain one and two neutrons are called deuterium and tritium, respectively; they are<br />
symbolized as D and T, but do not appear on the periodic table.<br />
More on Isotopes<br />
• The sum of the number of protons and neutrons in an atom is called the mass number of that<br />
atom, and is symbolized by A.<br />
• Isotopes are named by stating the name of the element, followed by A.<br />
5-2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Five <strong>Notes</strong><br />
◦ Carbon (Z=6) with 6 neutrons is “carbon-12”<br />
◦ Carbon with 7 neutrons is “carbon-13”<br />
◦ Carbon with 8 neutrons is “carbon-14”<br />
More on Isotopes<br />
• Isotopes can be written in shorthand notation in two different ways,<br />
A<br />
Z<br />
X<br />
or<br />
A<br />
X<br />
Examples<br />
• For each of the following, indicate how many protons, electrons, and neutrons each atom or<br />
ion possesses.<br />
◦<br />
35 Cl<br />
◦<br />
81 Br -<br />
◦<br />
27 Al 3+<br />
The Mass of an Atom<br />
• Recall that virtually all of the mass of an atom comes from its nucleus.<br />
• Knowing the mass of protons and neutrons allows us to calculate the mass of one atom of a<br />
particular isotope.<br />
• Since most elements have more than one isotope, and these isotopes are mixed in nature, it<br />
is not possible to provide an exact mass for the element.<br />
• Instead, we consider a weighted average mass, based on the weight of each individual<br />
isotope and its abundance in nature.<br />
• The periodic table provides the atomic weight of each element, which corresponds to this<br />
weighted average mass.<br />
• These values are in atomic mass units (amu), a very small unit of mass.<br />
◦ 1 amu = 1.66 × 10 -24 g<br />
• For example, the mass of a single helium atom is 4.003 amu.<br />
Calculating Atomic Weights<br />
• The atomic weight of an element can be calculated if we know:<br />
◦ The atomic weight of each isotope of that element, and<br />
◦ The percent abundance of that element in nature.<br />
• For example, suppose that 2 isotopes exist for an element X, and that the isotopes have<br />
atomic weights of 64. amu and 66. amu. If there are 50.% of each in nature, what is the<br />
atomic weight of X<br />
5-3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Five <strong>Notes</strong><br />
Examples<br />
There are three isotopes of potassium, as the data in the table below indicates. Calculate the<br />
atomic weight of potassium from this data.<br />
Isotope Mass(amu) % Abundance<br />
39 K 38.963707 93.2581<br />
40 K 39.963999 0.001171<br />
41 K 40.961826 6.7302<br />
Chlorine has only two naturally occurring isotopes. The atomic weight of 35 Cl is 34.96885 amu,<br />
and its % abundance is 75.53%. What is the atomic weight of the other isotope, 37 Cl<br />
Percent Composition<br />
• The percent composition of a compound indicates the percentage of each element in the<br />
compound by mass<br />
• For example, suppose that a compound containing only nitrogen and oxygen is 36.85%<br />
nitrogen<br />
• From this, we see that, for every 100. grams of the compound, 36.85 grams of it comes from<br />
the nitrogen in the compound<br />
• What about oxygen<br />
5-4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Five <strong>Notes</strong><br />
Suppose a compound is analyzed and is found to contain 6.00 grams of carbon, 2.00 grams of<br />
hydrogen, and 8.00 grams of oxygen. What is the percent composition of the compound<br />
What mass of hydrogen is in a 1.450 kg sample of this compound<br />
5-5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Ten <strong>Notes</strong><br />
Chapter Ten:<br />
Modern Atomic Theory<br />
Light and Energy<br />
• Electromagnetic radiation(EM) is an especially important form of energy for scientific study.<br />
◦ Many types of “radiant” energy are included under this description, including visible light,<br />
X-rays, and radio waves.<br />
◦ EM can be described as waves, which can be characterized by their wavelengths (λ), the<br />
distance between the peaks of each wave.<br />
◦ We also may describe light as a particle, called a photon<br />
Wavelength and Frequency<br />
• The frequency (ν) of waves is measured as the number of waves which occur in a period of<br />
time, usually a second.<br />
◦ For example, there are 445 peaks in a second, we would indicate this as 445 s -1 .<br />
◦ Alternatively, the Hertz(Hz) may be used<br />
• 1 Hz = 1 s -1<br />
• The frequency and the wavelength are inversely proportional<br />
◦ That is, as the wavelength increases, the frequency decreases, and vice versa.<br />
The Mathematical Relationship Between Wavelength and Frequency<br />
c<br />
ν =<br />
λ<br />
Where c is the speed of light<br />
c = 3.00 ×10 8 m/s<br />
Energy of EM Radiation<br />
• The total energy of a single photon depends on the frequency (or wavelength) which that<br />
photon is associated with.<br />
• This is described by the equation<br />
E = hν<br />
where E is the energy (in J), νis the frequency (in s -1 ), and h is<br />
Planck’s Constant (6.626 ×10 -34 J·s).<br />
• Greater frequency (and shorter wavelengths) indicate higher energy photons.<br />
• Provide a formula relating energy to wavelength rather than frequency:<br />
The Electromagnetic Spectrum<br />
• EM radiation can be classified into different regions based on its wavelength or its frequency.<br />
◦ The longest wavelenths (smallest frequencies) correspond to radio waves.<br />
◦ The shortest wavelengths (greatest frequencies) correspond to gamma rays.<br />
10-1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Ten <strong>Notes</strong><br />
Electrons & Energy Levels<br />
• Evidence suggested to scientists studying atomic structure that electrons “orbit” around the<br />
nucleus in specific energy levels (also called shells).<br />
◦ The farther the energy level is from the nucleus, the higher the energy of its electrons.<br />
• Normally, electrons “fill up” the lower energy levels first, and as new electrons are added they<br />
go into higher and higher energy levels.<br />
◦ An atom is said to be in the ground state when this is true.<br />
• An energy source, such as light or heat, can give electrons the energy necessary to “jump”<br />
from its energy level to a higher one.<br />
◦ In this situation, the atom is said to be in an excited state.<br />
Emission of Light<br />
• An atom in the excited state is unstable and must release the energy it gained in the first<br />
place to return to the ground state.<br />
◦ According to the Law of Conservation of Energy, this extra energy cannot simply<br />
disappear<br />
• One way in which this is accomplished is for the atom to give off this energy as light. This<br />
process is called emission.<br />
◦ The released light is called a quanta (energy packet) or a photon.<br />
• Excited electrons return to lower energy levels.<br />
◦ Depending on the atom itself and which energy levels are involved, EM radiation of<br />
different wavelengths are given off.<br />
Example<br />
Suppose that a photon has 2.45 × 10 -19 J of energy.<br />
(a) What is its wavelength in meters<br />
(b) What is its frequency in s -1 <br />
(c) What type of EM radiation is this<br />
So What is Light, Really<br />
• The answer to this is not as simple as you might think<br />
• Light (EM in general) is correctly described as both<br />
◦ Particles (photons)<br />
◦ Waves<br />
• Light is not one or the other; it is both simultaneously!<br />
10-2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Ten <strong>Notes</strong><br />
Quantization<br />
• Notice that, for a given atom, electrons are only allowed to jump to discrete energy levels.<br />
◦ In other words, an electron in the third level may fall to the first or second level, but not “in<br />
between” the levels.<br />
• As a result, only specific energy changes are allowed and can be observed for each atom.<br />
◦ We say that these energy changes are “quantized” since only specific quantities of<br />
energy can be emitted,<br />
• As an analogy, compare a ball moving down a set of stairs (step-by-step) to one moving<br />
down a ramp.<br />
◦ Which corresponds to “quantized” energy values<br />
Orbitals & Subshells<br />
• In truth, electrons do not simply rotate about the nucleus in simple patterns.<br />
• Instead, electrons are mostly contained in orbitals, which are shapes which describe the<br />
regions where an electron is likely to be found.<br />
• We will call a complete “set” of orbitals in a given energy level a subshell.<br />
• Four orbital types are commonly encountered in modern chemistry.<br />
◦ These are designated s, p, d, and f, and are listed here from lowest energy orbital type to<br />
highest.<br />
• Each individual orbital can hold, at most, two electrons in its ground state.<br />
The s Orbital<br />
• The s orbital is the least energetic of the orbitals, and, as a sphere, is also the most simplelooking.<br />
• All energy levels have exactly one s orbital.<br />
◦ Since any orbital can only hold two electrons, each s orbital is limited to this.<br />
The p Orbital<br />
• Starting with the 2 nd energy level, each level possesses three “sets” of p orbitals.<br />
◦ There are three 2p orbitals, three 3p orbitals, etc.<br />
• Recall that each orbital can hold up to two electrons, so the three orbitals combined will hold<br />
up to six electrons.<br />
• The p orbitals are more complex in shape than the s orbital, and electrons residing in them<br />
typically have greater energy than those in an s orbital.<br />
10-3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Ten <strong>Notes</strong><br />
d and f Orbitals<br />
• Energy levels three and higher have a total of 5 sets of d orbitals.<br />
◦ A full set of d orbitals can therefore hold up to_____electrons.<br />
• Energy levels four and higher have a total of 7 sets of f orbitals.<br />
◦ A full set of f orbitals can therefore hold up to_____electrons.<br />
Electron Configurations<br />
• Each element has its own unique electron configuration which describes which orbitals have<br />
electrons in them and how many.<br />
◦ For example, the electron configuration of boron is 1s 2 2s 2 2p 1 , which means that there are<br />
• 2 electrons in an s orbital on the first energy level (called the 1s subshell)<br />
• 2 electrons in the 2s orbital (the 2s subshell)<br />
• 1 electron in a 2p orbital (the three p orbitals collectively make up the 2p subshell)<br />
• Atoms always fill their lowest energy orbitals first, and successively higher ones as more<br />
electrons are added.<br />
◦ This is known as the Aufbau principle; aufbau is German for “building up”<br />
• The order in which the electrons fill can be found on the periodic table.<br />
◦ Notice that the periodic table is broken up into 4 distinct “blocks,” each of which indicates<br />
where the highest energy electrons are.<br />
Examples<br />
Determine the electron configuration for each of the following atoms/ions:<br />
Be<br />
N<br />
Na<br />
V<br />
10-4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Ten <strong>Notes</strong><br />
Shorthand Notation for Electron Configurations<br />
• You can abbreviate the electron configuration with a special notation<br />
◦ Consider V for example.<br />
◦ The last noble gas before V was Ar (element 18)<br />
◦ So, we can write [Ar]4s 2 3d 3 as vanadium’s electron configuration.<br />
◦ What is the electron configuration of antimony in shorthand notation<br />
Unusual Electron Configurations<br />
• Unfortunately, the electron configurations we predict are not always correct<br />
• For example, predict the electron configuration of copper<br />
• The actual electron configuration is:<br />
There are several other elements which do not “follow the rules”; however, at this point in your<br />
study of chemistry, you do not need to be concerned with these exceptions<br />
Spin<br />
• Each electron is able to rotate about its central axis, a process we call spin<br />
• Electrons may spin in one of two possible directions<br />
• We refer to these directions as “spin up” and “spin down”<br />
The Pauli Exclusion Principle & Hund’s Rule<br />
• In a ground state atom, two electrons in the same orbital must have opposite spins; this is a<br />
simplified version of a rule called the Pauli Exclusion Principle<br />
• Another important principle, Hund’s Rule, states that, for ground state atoms, electrons will fill<br />
unoccupied orbitals within a subshell before filling singularly-occupied ones<br />
• For example, in a nitrogen atom, with electron configuration 1s 2 2s 2 2p 3 , the three<br />
electrons in the 2p subshell reside in different orbitals (i.e. they do not pair up)<br />
Energy Level Diagrams<br />
• Energy level diagrams are a graphical form of the electron configuration, representing<br />
electrons as arrows (up arrow for spin-up, down for spin-down)<br />
and orbitals as lines<br />
• The lines are listed from lowest energy at the bottom (i.e. the 1s orbital) to highest<br />
10-5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Ten <strong>Notes</strong><br />
Example<br />
• Draw the energy level diagrams for<br />
a. titanium b. S 2- 10-6
<strong>Chemistry</strong> <strong>120</strong><br />
Orbital Blocks<br />
Group<br />
1A<br />
Here you see the periodic table separated into blocks, which should assist you in your study<br />
of electron configurations. Note that helium belongs in the s block.<br />
8A<br />
2A 3A 4A 5A 6A 7A<br />
He<br />
Helium<br />
s<br />
block<br />
3B 4B 5B 6B 7B 8B 1B 2B<br />
d<br />
block<br />
p<br />
block<br />
f<br />
block
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Chapter Eleven<br />
Chemical Bonding<br />
Valence Electrons<br />
• The electrons occupying the outermost energy level of an atom are called the valence<br />
electrons; all other electrons are called the core electrons.<br />
• The valence electrons, as we will see, are responsible for chemical bonding.<br />
◦ Knowing the number of valence electrons an atom has is the single most important<br />
information you can have in predicting how an atom will react chemically.<br />
• Note that the valence electrons are not always the electrons with the highest energy, as we<br />
will see with the transition metals<br />
• For elements in group IA through VIIIA, the number of valence electrons an atom has is<br />
simply its group number.<br />
◦ So phosphorus, in group VA, has five valence electrons.<br />
• Helium is the only significant exception; it has 2 valence electrons, even though it is in group<br />
VIIIA<br />
Lewis Dot Diagrams<br />
• Lewis dot diagrams are simple symbols which show the symbol of an element surrounded by<br />
as many dots as that atom has valence electrons.<br />
• The first four electrons are drawn (in any order) on each of the four “sides” of the symbol.<br />
• The next four electrons are “paired up” with the other four atoms (again, in any order).<br />
• These symbols will be used to model chemical bonding.<br />
Examples<br />
• Draw the Lewis dot diagrams for selenium, rubidium, and manganese atoms.<br />
The Octet Rule<br />
• The Octet Rule states that atoms react in such a way as to give them eight electrons in their<br />
outermost energy level (their valence shell).<br />
• The Noble Gases, those elements in the period on the far right of the Periodic Table,<br />
generally do not react with other atoms, as their valence shell is filled with eight electrons (or<br />
two in the case of helium).<br />
• By gaining or losing enough electrons to give an atom eight electrons in its valence shell, the<br />
atom gains the stable features of a noble gas.<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Getting an Octet<br />
• Atoms usually achieve an octet in the following way:<br />
◦ Metals lose their valence electrons, giving them an empty outer shell.<br />
• Note that the ion now has the electron configuration of a noble gas.<br />
◦ Nonmetals gain or share enough electrons to give themselves eight electrons in their<br />
outer shell.<br />
• Nonmetals generally share with other nonmetal atoms, or take electrons away from<br />
metal atoms.<br />
Example<br />
• How many electrons will usually be gained or lost by each of the following atoms<br />
◦ Bromine<br />
◦ Barium<br />
◦ Potassium<br />
◦ Aluminum<br />
◦ Oxygen<br />
◦ Neon<br />
The Duet Rule<br />
• Hydrogen atoms attempt to pick up another electron, giving them the same electron<br />
configuration as the noble gas helium; this is called The Duet Rule.<br />
• Likewise, when lithium loses an electron to become Li + , it has the same electron configuration<br />
as helium.<br />
A Cautionary Note<br />
• Gaining and losing electrons does not occur unless there are other atoms around to<br />
encourage this.<br />
◦ A sodium atom cannot just toss its valence electron away; it must give it to another atom<br />
which wants to take it, like chlorine.<br />
• Considering this, be sure that you do not confuse an atom of an element (which has its usual<br />
number of electrons) with an ion (which has gained or lost electrons).<br />
What is Bonding<br />
• Bonding describes how atoms interact with each other in an attractive sense.<br />
• There are three types of bonding:<br />
◦ Ionic bonding<br />
◦ Covalent bonding<br />
◦ Metallic bonding<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Ionic Bonding<br />
• Ionic bonding occurs between ions of different charges.<br />
• Often, but not always, ionic bonding occurs between the ion of metal with the ion of a<br />
nonmetal.<br />
◦ Sometimes, one of these ions is a polyatomic ion, such as sulfate (SO 4 2- ).<br />
• Ionic bonding is generally the strongest of the bonding types.<br />
◦ It requires a great amount of energy to separate the ions from each other, resulting in<br />
high melting points.<br />
Examples of Ionic Compounds<br />
NaCl CaO CuBr 2 LiF<br />
Formulas of Ionic Compounds<br />
• An ionic compound should have no total charge in its formula.<br />
• Ions of opposite charge are paired in such a way as to cancel out charges.<br />
◦ Positively charged ions are called cations.<br />
◦ Negatively charged ions are called anions.<br />
• Example:<br />
One Na + combines with one Cl - to give the neutral ionic compound NaCl.<br />
Two Na + combine with one O 2- to give the neutral ionic compound Na 2 O.<br />
• Notice that the cation is always listed first in the formula.<br />
Formulas of Ionic Compounds<br />
• Further examples<br />
◦ Note that the formula of an ionic compound shows the smallest whole number ratio<br />
between the ions.<br />
◦ So, when Ca 2+ and O 2- combine, the formula of the product is CaO, not Ca 2 O 2 .<br />
◦ Sometimes, the ratio between ions is more complex, like with Al 3+ and O 2- .<br />
Example<br />
• What is the formula of the ionic compound which contains ions of each of the two elements<br />
below<br />
sodium and sulfur<br />
barium and nitrogen<br />
selenium and calcium<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Covalent Bonding<br />
• Covalent bonds result from the sharing of electrons between two atoms.<br />
• Recall that covalent bonding is usually found between nonmetal atoms.<br />
◦ This is a bit oversimplified, but will work well for our purposes in this class.<br />
• In following the octet rule, atoms share enough electrons with each other to give each eight<br />
valence electrons (or two in the case of hydrogen).<br />
• Covalent bonds are generally not as strong as ionic bonds; still, many are relatively strong.<br />
◦ Example: Compare heating salt (ionic) and sugar (covalent).<br />
Molecules<br />
• Compounds which are held together by covalent bonds are called molecules<br />
• This term is not appropriate for ionic compounds, which are made up of repeating unit cells<br />
• For example an H 2 O molecule contains exactly three elements, but there is no “NaCl<br />
molecule” consisting of only two atoms<br />
Examples of Covalent Compounds<br />
H 2 O<br />
C 6 H 12 O 6<br />
Cl 2 (an element)<br />
C 6 H 6<br />
CO 2<br />
H 2 S<br />
SO 3<br />
Diatomic Elements<br />
• Seven elements are essentially always found in nature as diatomic molecules, which are<br />
molecules which contain exactly two atoms<br />
• The formulas of these seven elements are:<br />
H 2 , N 2 , O 2 , F 2 , Cl 2 , Br 2 , and I 2<br />
• When we refer to oxygen gas for example, we mean O 2 , not individual oxygen atoms.<br />
• These seven formulas will appear frequently throughout the course and must be learned!<br />
Phosphorus, Sulfur, and Ozone<br />
• The most stable form of phosphorus is a molecule containing four P atoms, which is given the<br />
formula P 4 .<br />
• Similarly, sulfur forms molecules which contain eight sulfur atoms each, and has the formula<br />
S 8 .<br />
◦ Unlike for the diatomic elements, chemists do not consistently use these formulas when<br />
writing chemical reactions<br />
• Oxygen also forms the molecule known as ozone, O 3 .<br />
◦ Although both O 2 and O 3 contain only oxygen atoms, they have entirely different chemical<br />
properties<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Electronegativity<br />
• The electronegativity of an atom indicates how strong its attraction for electrons is.<br />
◦ The greater an atom’s electronegativity, the more strongly it pulls electrons toward it.<br />
• Like the atomic radius and the ionization energy, electronegativity has a periodic trend:<br />
◦ Electronegativity increases up a group and from left to right across a period.<br />
• Fluorine is the most electronegative atom; in general, the closer a main group element is<br />
to fluorine on the periodic table, the more electronegative it is.<br />
• The noble gases have virtually no electronegativity.<br />
Lewis Structures<br />
• Lewis Structures are simple drawings that show the covalent bonds between atoms.<br />
• As in Lewis dot diagrams, electrons are represented by dots.<br />
◦ Since two electrons are required to make a bond, a pair of electrons between two atoms<br />
indicates a bond.<br />
Multiple Bonds<br />
• Remember, atoms bond in order to gain an octet (or duet for hydrogen).<br />
• In order to do this, atoms can also share more than one pair of electrons, up to a maximum of<br />
three pairs.<br />
◦ Sharing one pair of electrons forms a single bond.<br />
◦ Sharing two pairs forms a double bond.<br />
◦ Sharing three pairs forms a triple bond.<br />
◦ There are not quadruple bonds!<br />
Examples of Multiple Bonds<br />
More on Lewis Structures<br />
• It is much simpler when drawing Lewis structures to represent electron pairs as lines rather<br />
than dots.<br />
◦ However, always keep in mind that the lines stand for electron pairs!<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Drawing Lewis Structures<br />
• There are several steps involved in taking a formula and converting it to a Lewis structure;<br />
just keep in mind the goals set out by the octet and duet rules.<br />
1. Add up the total number of valence electrons in the formula.<br />
Ex. NH 3 has 5 + (3×1)=8 v.e.<br />
Note that if the molecule is an ion, each negative charge adds one electron to this count, and<br />
each positive charge takes one away.<br />
2. Draw a simple “skeleton” of the molecule, showing which atoms are connected to which. If<br />
there is one “central” atom (the one surrounded by the others) it is usually the least<br />
electronegative.<br />
Note: Hydrogen is never a central atom!<br />
3. Figure out how many electrons you have left. Remember that each bond stands for two<br />
electrons, so subtract two from the total number of valence electrons for every bond you drew<br />
in the previous step.<br />
8 – 6 = 2 electrons left<br />
4. Give enough electron pairs to each atom in the structure to give each atom (except<br />
hydrogen) an octet, using the following guidelines:<br />
-Electrons go to the most electronegative atoms first.<br />
-You must stop adding electron pairs when you run out of electrons (from the original number<br />
you started with in step 1).<br />
5. This step is not always necessary:<br />
If you have run out of electrons, and some atoms still need octets, change a lone pair on the<br />
least electronegative adjacent atom (except hydrogen) to a double bond between the two<br />
atoms. If necessary, you may need to make a triple bond by taking away another lone pair.<br />
Note that fluorine will not share its lone pairs.<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Examples<br />
Draw Lewis Structures for each of the following molecules:<br />
•<br />
CH 4<br />
H 2 O<br />
HCN<br />
NO 3<br />
-<br />
N 2 H 2<br />
C 2 H 2<br />
7
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eleven <strong>Notes</strong><br />
Exceptions to the Octet Rule<br />
• Boron and beryllium often will not be able to gain a complete octet.<br />
◦ For example, consider BH 3 and BF 3<br />
• Atoms in period 3 and below only may exceed the octet rule for reasons we will not consider<br />
here. You will often see this in cases where the central atom is P, S, Cl, Br, or I; others exist<br />
as well.<br />
◦ For example, consider PCl 5, SF 6 ,and SO 3 .<br />
8
Additional Chapter 11 Topics<br />
Periodic Trends<br />
• By comparing the position of one element to another on the periodic table, it is often possible<br />
to make comparisons between the properties of those elements; these are a result of periodic<br />
trends.<br />
• In this class we consider three of these trends:<br />
◦ Electronegativity<br />
◦ Atomic radius<br />
◦ Ionization Energy<br />
Atomic Radius<br />
• The radius of an atom tends to increase as you move down a group in the periodic table.<br />
◦ Explanation: Elements in lower groups of the periodic table have electrons in outer<br />
energy levels. These electrons are not held as tightly by the nucleus, so they can travel<br />
further away from it.<br />
• The radius of an atom tends to decrease from left to right across a period.<br />
◦ Explanation: The valence electrons of atoms in the same period fill the same energy<br />
levels. However, the positive charge in the nucleus is increasing as we move from left to<br />
right on the periodic table as the number of protons is likewise increasing. This pulls the<br />
electrons in closer, making the radius smaller.<br />
Atomic Radius: Ions<br />
• Recall that when an ion is formed, an atom gains or loses electrons, while the number of<br />
protons remains the same<br />
• When an atom loses an electron to form a cation, the positive charge of the nucleus pulls the<br />
remaining electrons closer towards the nucleus<br />
• A monatomic cation is smaller than the corresponding neutral atom<br />
◦ Na + has a smaller atomic radius than Na<br />
◦ Mg 2+ has a smaller atomic radius that Mg<br />
• When an atom gains an electron to form an anion, the increased repulsion of the additional<br />
electrons results in electrons moving farther from the nucleus<br />
◦ Cl - has a larger atomic radius than Cl<br />
◦ O 2- has a larger atomic radius than O<br />
• When comparing atoms and ions with the same number of electrons, the largest ions are<br />
those with the most negative charge<br />
Atomic Radius: Ions<br />
Rank each of the following atoms/ions in order from largest to smallest<br />
I. Ne Al 3+ O 2- F - Na + Mg 2+<br />
II. Li K N Ne Cs
Ionization Energy<br />
• The ionization energy is the amount of energy required to remove an electron from a mole of<br />
atoms in their gas state of a particular element.<br />
X (g) X + (g) + e -<br />
◦ The first ionization energy is the amount of energy required to remove the first electron.<br />
◦ The second ionization energy is the amount of energy required to remove the second<br />
electron. Etc.<br />
• Ionization energy tends to decrease down a group.<br />
◦ Explanation: Electrons in the outer shells are further from the nucleus and feel its pull less<br />
than the core electrons do. Less energy is required to remove them.<br />
• Ionization energy tends to increase from left to right across a period.<br />
◦ Explanation: Protons are added to the nucleus from left to right across the table, and<br />
these protons exert a greater pull on the electrons, requiring more energy to remove<br />
them.<br />
◦ Why is the first ionization energy of oxygen less than that of nitrogen<br />
Comparing Ionization Energies<br />
• Generally, the first ionization energy is less than the second, which is less than the third, etc.<br />
• If an atom has lost enough electrons to give it an octet in its outer shell, it requires a<br />
tremendous amount of energy to remove any electrons beyond this.<br />
Covalent Bonds<br />
• Recall that<br />
◦ Covalent bonds result from the sharing of electrons between atoms.<br />
◦ Nonmetals bond with other nonmetal atoms through covalent bonding.<br />
◦ The strength of a covalent bond is generally less than that of an ionic bond.<br />
• A question:<br />
◦ Do atoms involved in covalent bonding share electrons equally<br />
Polarity and Dipole Moment<br />
• If two atoms which are covalently bonded have substantially different electronegativity values,<br />
then the bond is said to be polar covalent.<br />
◦ The electrons are not shared equally in the bond.<br />
◦ The electrons will tend to stay closer to the more electronegative atom.<br />
• The molecule might have a dipole moment, which is shown by drawing a special arrow<br />
pointing towards the more electronegative atom. More on this later…
Shapes of Molecules<br />
• From Lewis structures we can usually figure out the three-dimensional structure of simple<br />
molecules.<br />
• VSEPR theory (stands for Valence Shell Electron Pair Repulsion) helps us to understand the<br />
shapes that molecules take.<br />
• According to VSEPR, electron pairs move as far away from each other (in three dimensions)<br />
as possible.<br />
◦ Remember that electrons all have negative charge, so they repel one another.<br />
The Basic Geometries of Molecules<br />
• Depending on the number of attached atoms and lone pairs, a basic geometry can be<br />
described for an atom in a molecule.<br />
◦ Linear: 2 attached groups<br />
◦ Trigonal Planar: 3 attached groups<br />
◦ Tetrahedral: 4 attached groups<br />
◦ Trigonal Bipyramidal: 5 attached groups<br />
◦ Octahedral: 6 attached groups<br />
Assigning Shapes to Molecules<br />
• A shape is assigned to each central atom in a molecule.<br />
◦ To be a central atom, an atom must have two or more atoms bonded to it.<br />
• The number of atoms bonded to the central atom is added up. Call this m.<br />
◦ Careful! Add the number of atoms, not the number of bonds!<br />
• The number of lone pairs on the central atoms is added up. Call this n.<br />
Assigning Shapes to Molecules<br />
• Take these numbers and put them in the following formula:<br />
AX m E n<br />
• The A in this formula stands for the central atom, the X for the attached atoms, and the E for<br />
the lone pairs.<br />
• From this code we can name the shape of the molecule.<br />
Linear<br />
• AX 2 is called the linear shape.<br />
• The bond angle (atoms between the three bonds) in this shape is 180°.<br />
Trigonal Planar and<br />
Bent/V-Shaped<br />
• The shape associated with AX 3 is trigonal planar because it resembles a flat triangle.<br />
• The shape associated with AX 2 E 1 is called bent/V-shaped.<br />
◦ When naming a shape we pretend to only “see” the atoms, not the lone pairs. That is<br />
why we have two different shape names for the same geometry.<br />
• Both of these shapes have bond angles of approximately <strong>120</strong>°, which may vary slightly in<br />
some molecules.
Tetrahedral Geometries<br />
• The shape associated with AX 4 is called tetrahedral, with all atoms at the four points of a<br />
pyramid.<br />
• Replacing an atom with an electron pair gives AX 3 E 1 , which is called trigonal pyramidal.<br />
• Changing another atom to a lone pair gives the the AX 2 E 2 code, which is called the bent/Vshaped<br />
shape.<br />
◦ This is the same shape name as we saw earlier, but it has a different geometry and<br />
different bond angles.<br />
• The bond angles associated with these three are approximately 109.5°.<br />
Trigonal Bipyramidal and Octahedral Shapes<br />
• The AX 5 shape is called trigonal bipyramidal, and resembles two pyramids sharing a common<br />
face.<br />
◦ The bond angles associated with this shape are both 90° and <strong>120</strong>°, depending on where<br />
you look.<br />
• The AX 6 shape is called octahedral.<br />
◦ The bond angles for this shape are 90°.<br />
• Other shapes within these geometries are not included in this course, but they do exist.<br />
Dipole Moments<br />
• Molecules which have fairly electronegative atoms may have a dipole moment.<br />
• Since electrons are drawn towards more electronegative atoms, a “partial negative charge”<br />
(δ-)develops in this region of the molecule, and a partial positive charge (δ+)develops on the<br />
other side.<br />
• Consider CH 3F. .
Dipole Moments<br />
• In thinking about dipole moments, we have to consider the three-dimensional structure of the<br />
molecule.<br />
• Dipoles can cancel each other out, if the same type of bonds are oriented in opposite<br />
directions.<br />
Example<br />
• Example: Which of these molecules have dipole moments Which, if any, have polar bonds<br />
but no dipole moment<br />
CCl 4 NH 3 H 2 O CO 2
<strong>Chemistry</strong> <strong>120</strong> Molecular Geometry<br />
Molecular Geometry<br />
AX m E n<br />
Code<br />
Approximate Bond<br />
Angles (degrees)<br />
Hybridization<br />
of Central Atom*<br />
2-dimensional<br />
Representation<br />
3-dimensional<br />
Representation<br />
Linear AX 2 180 sp X A X X A<br />
X<br />
X<br />
X<br />
Trigonal Planar AX 3 <strong>120</strong> sp 2 A<br />
X<br />
X<br />
X<br />
A<br />
X<br />
Bent/V-shaped AX 2 E 1
<strong>Chemistry</strong> <strong>120</strong> Molecular Geometry<br />
Molecular Geometry<br />
AX m E n<br />
Code<br />
Approximate Bond<br />
Angles (degrees)<br />
Hybridization<br />
of Central Atom<br />
2-dimensional<br />
Representation<br />
3-dimensional<br />
Representation<br />
X<br />
X<br />
Trigonal Bipyramid AX 5 90 & <strong>120</strong> dsp 3 X<br />
A<br />
X X<br />
X<br />
X<br />
A<br />
X<br />
X<br />
X<br />
X<br />
See-saw AX 4 E 1 90 &<strong>120</strong> dsp 3 X A<br />
X X<br />
X<br />
A<br />
X<br />
X<br />
X<br />
X<br />
X A<br />
T-shaped AX 3 E 2 90 dsp 3<br />
X<br />
X<br />
A<br />
X<br />
X<br />
X<br />
Linear AX 2 E 3 180 dsp 3 X A X A<br />
X<br />
Note: None of the shapes on pages 2 or 3 of this handout will be tested in CHEM <strong>120</strong>, as they all have central atoms which exceed an octet.<br />
These are included to assist you in your later studies in General <strong>Chemistry</strong>.<br />
Page 2
<strong>Chemistry</strong> <strong>120</strong> Molecular Geometry<br />
Molecular Geometry<br />
AX m E n<br />
Code<br />
Approximate Bond<br />
Angles (degrees)<br />
Hybridization<br />
of Central Atom<br />
2-dimensional<br />
Representation<br />
Octahedral AX 6 90 d 2 sp 3 A<br />
Square Pyramid AX 5 E 1 90 d 2 sp 3 X<br />
A<br />
X<br />
X<br />
X<br />
X<br />
X<br />
X<br />
X<br />
X<br />
X<br />
X<br />
3-dimensional<br />
Representation<br />
X<br />
X<br />
X<br />
X<br />
X<br />
A<br />
X<br />
X<br />
A<br />
X<br />
X<br />
X<br />
X<br />
Square Planar AX 4 E 2 90 d 2 sp 3 A<br />
X<br />
X<br />
X<br />
X<br />
X<br />
X<br />
A<br />
X<br />
X<br />
Note: None of the shapes on pages 2 or 3 of this handout will be tested in CHEM <strong>120</strong>, as they all have central atoms which exceed an octet.<br />
These are included to assist you in your later studies in General <strong>Chemistry</strong>.<br />
Page 3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
Chapter Six:<br />
Nomenclature—The Names of Chemical Compounds<br />
Types of Ions<br />
• Ions are classified according to how many atoms they contain<br />
◦ If an ion is derived from a single atom, it is called a monatomic ion.<br />
• Examples include Na + , O 2- , and Pb 4+ .<br />
◦ Ions which are derived from two or more atoms are called polyatomic ions.<br />
Polyatomic Ions<br />
• Polyatomic ions can be described as molecules which have collectively gained or lost<br />
electrons to become an ion.<br />
• Being molecules, the ions themselves are held together by covalent bonds.<br />
• From this, you would expect the atoms in a polyatomic ion to all be nonmetals.<br />
◦ Examples: NO 3 - , ClO 4 - , NH 4<br />
+<br />
• However, some polyatomic ions contain metals which are able to covalently bond.<br />
◦ Examples: Cr 2 O 7 2- , MnO 4<br />
-<br />
• All but one of the more common polyatomic ions are anions.<br />
• The ammonium ion, NH 4 + , is the only common polyatomic cation.<br />
• The common polyatomic ions must be memorized, and you must learn to recognize them in a<br />
formula on sight.<br />
1- anions<br />
OH - hydroxide<br />
-<br />
NO 3<br />
CN - cyanide<br />
-<br />
ClO 3<br />
OCN - cyanate<br />
-<br />
BrO 3<br />
SCN - thiocyanate<br />
-<br />
IO 3<br />
-<br />
MnO 4 permanganate<br />
-<br />
C 2 H 3 O 2<br />
2- anions<br />
2-<br />
CO 3 carbonate<br />
2-<br />
SO 4<br />
2-<br />
CrO 4 chromate<br />
2-<br />
Cr 2 O 7<br />
2-<br />
C 2 O 4 oxalate<br />
2-<br />
SiO 3<br />
2-<br />
S 2 O 3 thiosulfate<br />
2-<br />
O 2<br />
3- anions<br />
3-<br />
PO 4 phosphate<br />
3-<br />
BO 3<br />
nitrate<br />
chlorate<br />
bromate<br />
iodate<br />
acetate<br />
sulfate<br />
dichromate<br />
silicate<br />
peroxide<br />
borate<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
Classifications of Compounds<br />
• When naming inorganic compounds, two different naming systems are used, depending on<br />
the type of compound you are considering.<br />
• Binary nonmetals (sometimes called molecular compounds) contain atoms from exactly two<br />
different nonmetals.<br />
◦ Examples: NO, CO 2 , CO, SO 2 , H 2 S.<br />
• Ionic compounds are composed of a cation and an anion.<br />
◦ For the purposes of this course, if a compound is not a binary nonmetal, it is an ionic<br />
compound.<br />
◦ The ions may be monatomic and/or polyatomic.<br />
◦ Examples: NaCl, CaCl 2 , NH 4 Cl, CaCO 3 , Na 3 PO 4 .<br />
Examples<br />
• Classify each of these compounds as binary nonmetals or as ionic compounds.<br />
◦ KBr<br />
◦ Na 2 CO 3<br />
◦ NaCN<br />
◦ N 2 O 4<br />
◦ NaH 2 PO 4<br />
◦ P 2 O 5<br />
◦ NH 4 NO 3<br />
Naming Binary Nonmetals<br />
• Nonmetals can bond with one another in many possible combinations.<br />
◦ For example, nitrogen and oxygen make compounds such as NO, NO 2 , and N 2 O.<br />
• Although these compounds contain the same elements (and may even contain them in the<br />
same ratio), these chemicals have considerably different chemical and physical properties.<br />
• Therefore, each must be given its own distinct name to distinguish it.<br />
• The compound is named by putting prefixes before the name of the element to indicate how<br />
many atoms of each type are in the molecule.<br />
• The ending of the name of the second element is changed to “-ide”.<br />
prefix[1 st element] prefix[2 nd element]<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
Naming Binary Nonmetals<br />
The first ten prefixes must be memorized:<br />
Number of Atoms<br />
in Molecule Prefix<br />
1 mono-<br />
2 di-<br />
3 tri-<br />
4 tetra-<br />
5 penta-<br />
6 hexa-<br />
7 hepta-<br />
8 octa-<br />
9 nona-<br />
10 deca-<br />
• For example, a compound with formula S 2 O 3 would be named disulfur trioxide.<br />
• Exceptions:<br />
◦ Do not use the prefix “mono-” with the first element in the formula; just stating the name of<br />
the element implies that there is only one of it in the formula.<br />
• For example, CO 2 is carbon dioxide, not monocarbon dioxide.<br />
• What is the name of SO 3 <br />
◦ If the last letter of the prefix is an “a” or an “o”, and the first letter of the element after the<br />
prefix is an “o”, drop the last letter of the prefix; it looks and sounds awkward.<br />
• Example: CO is carbon monoxide, not carbon monooxide.<br />
• P 2 O 5 should be named diphosphorus pentoxide, which is preferable to diphosphorus<br />
pentaoxide (which is technically acceptable).<br />
Common Names<br />
• In three cases, the naming rules are totally ignored, and the common name is used.<br />
• These three are<br />
◦ H 2 O, which is always called water.<br />
◦ NH 3 , which is always called ammonia.<br />
◦ PH 3 , commonly known as phosphine.<br />
• Other common names do exist, but are omitted here (they are less common).<br />
Hydrogen-Containing Formulas<br />
• When hydrogen appears first in the formula of a binary nonmetal, do not use prefixes at all.<br />
Simply name the compound without them.<br />
◦ There will be as many hydrogens bonded to the other nonmetal as are necessary to give<br />
it a complete octet.<br />
◦ So, H 2 S (g) is named hydrogen sulfide, and HCl (g) is named hydrogen chloride.<br />
◦ Note that the (g) means “gas”, an important fact which must be specified in the formula<br />
for these types of compounds.<br />
• If the hydrogen-containing binary nonmetal is dissolved in water, a different name is used.<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
• In the formula, the notation (aq) is used, meaning aqueous, to indicate that it is dissolved in<br />
water.<br />
• These compounds are named as acids.<br />
◦ These are not to be confused with oxyacids, which will have a different naming system.<br />
Naming Acids of Binary Nonmetals<br />
• The prefix “hydro-” is put before the name of the element.<br />
• The ending of the name of the element is changed to “-ic”, followed by the word “acid”.<br />
◦ Examples:<br />
HCl (aq) is hydrochloric acid<br />
HBr (aq) is hydrobromic acid<br />
HI (aq) is hydroiodic acid<br />
H 2 S (aq) is hydrosulfuric acid<br />
CAUTION: Do not confuse this with sulfuric acid, which is H 2 SO 4 !<br />
Examples<br />
Name each of the following:<br />
N 2 O 5<br />
H 2 Se (aq)<br />
SO 2<br />
NH 3<br />
HF (aq)<br />
XeF 4<br />
HF (g)<br />
H 2 S (aq)<br />
Naming Ionic Compounds<br />
• The naming system for ionic compounds is different than that for binary nonmetals.<br />
• Most importantly: The prefixes used for binary nonmetals (mono, di, tri, etc.) are never used<br />
to name ionic compounds.<br />
◦ This is, by far, the most common mistake made by students in naming compounds.<br />
Naming Individual Ions: Cations<br />
• Some cations always have the same charge in virtually all compounds.<br />
• These include<br />
◦ Group I cations, which only form 1+ ions<br />
•<br />
Ex.: Li + , Na + , K + , Rb + , Cs +<br />
◦ Group II cations, which only form 2+ ions<br />
• Ex.: Mg 2+ , Ca 2+ , Sr 2+ , Ba 2+<br />
◦ Group III cations, which only form 3+ ions<br />
• Al 3+ , (Ga 3+ if it is forming an ionic compound)<br />
• Note that this is not true for elements below Ga<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
• Three additional common metals also only form one ion.<br />
• These must be memorized. They are<br />
◦ Zinc: Zn 2+<br />
◦ Cadmium: Cd 2+<br />
◦ Silver: Ag +<br />
• For all other metals, the charge must be specified in naming the cation.<br />
• The name of the individual cation is stated by simply stating the name of the metal, followed<br />
by the word “ion”.<br />
• Examples:<br />
◦ Na + is the sodium ion.<br />
◦ Ba 2+ is the barium ion.<br />
◦ Zn 2+ is the zinc ion.<br />
• The new method for naming all other cations places the charge of ion in Roman numerals in<br />
parenthesis after the name of the metal.<br />
◦ Cu 2+ is the copper (II) ion.<br />
◦ Cu + is the copper (I) ion.<br />
◦ Pb 4+ is the lead (IV) ion.<br />
◦ Pb 2+ is the lead (II) ion.<br />
• Remember, you only use Roman numerals for those ions that form multiple charges.<br />
• The old names for many ions are still in use and must be learned.<br />
• The names of the ions must be memorized, noting the following:<br />
◦ The ion possessing the higher charge ends in “-ic”<br />
◦ That possessing the lower charge ends in<br />
“-ous”<br />
◦ Ex.: Fe 3+ is the ferric ion, Fe 2+ is the ferrous ion.<br />
Ion Common Name Ion Common Name<br />
Cu 2+ cupric ion Cu + cuprous ion<br />
Fe 3+ ferric ion Fe 2+ ferrous ion<br />
Pb 4+ plumbic ion Pb 2+ plumbous ion<br />
Sn 4+ stannic ion Sn 2+ stannous ion<br />
Hg 2+ 2+<br />
mercuric ion Hg 2 mercurous ion<br />
Cr 3+ chromic ion Cr 2+ chromous ion<br />
Co 3+ cobaltic ion Co 2+ cobaltous ion<br />
Mn 3+ manganic ion Mn 2+ manganous ion<br />
Examples<br />
Name the following cations:<br />
Rb +<br />
Hg 2<br />
2+<br />
Fe 3+<br />
Cd 2+<br />
Hg 2 +<br />
Ca 2+<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
Naming Individual Ions: Anions<br />
• The charge on a monatomic anion is simply 8 minus the group number of the element.<br />
◦ For example, nitrogen is in group 5, so it will only make a N 3- ion. (8-5=3)<br />
• Monatomic anions are named by simply changing the ending of the element’s name to “ide”.<br />
• Examples:<br />
◦ S 2- is the sulfide ion<br />
◦ O 2- is oxide ion<br />
◦ P 3- is the phosphide ion<br />
• CAUTION: Do not confuse these monatomic ions (nitride, sulfide, phosphide, etc.) with the<br />
similar-sounding oxoanions (nitrate, sulfate, phosphate, etc.)<br />
Naming Ionic Compounds<br />
• To name the ionic compound, simply state the cation, followed by the anion. Do not use the<br />
word “ion” in the name of a neutral compound.<br />
• Examples:<br />
◦ NaCl is sodium chloride<br />
◦ CaBr 2 is calcium bromide<br />
◦ CuO is copper (II) oxide, or cupric oxide<br />
◦ Cu 2 O is copper (I) oxide, or cuprous oxide<br />
• Again, notice that we never use the prefixes used for binary nonmetals<br />
(mono-, di-, tri-, etc.) when naming ionic compounds!<br />
• This is because ionic compounds always form predictable ratios, as we have already seen.<br />
◦ Na + and Cl - can only come together as NaCl.<br />
◦ Cu 2+ and O 2- come together as CuO.<br />
◦ Cu + and O 2- come together as Cu 2 O.<br />
• Recall that the total charges of the cations and anions must neutralize.<br />
Examples<br />
Name each of the following ionic compounds:<br />
AgCl<br />
NH 4 NO 3<br />
KNO 3<br />
Hg(ClO 3 ) 2<br />
PbCl 2<br />
CdSO 4<br />
ZnBr 2<br />
SnCl 4<br />
Oxoanions<br />
• The oxoanions include many polyatomic anions which contain oxygen.<br />
◦ OH - and O 2 2- are not considered oxoanions.<br />
• So far, we have only encountered those oxoanions whose names end in “-ate.”<br />
• Related oxoanions have different numbers of oxygen atoms but the same charge.<br />
• Examples:<br />
◦ SO 4 2- is the sulfate anion, SO 3 2- is the sulfite anion.<br />
◦ ClO 3 - is the chlorate anion, ClO 4 - is the perchlorate anion.<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
• Let us consider the chlorate ion, which we know has formula ClO 3 - .<br />
• It is very important that we know how many oxygen atoms are in the “-ate” ion.<br />
• If the ion has one more oxygen in its formula than that of the “-ate” ion, add the prefix “per-” to<br />
its name.<br />
• So ClO 4 - is perchlorate, SO 5 2- would be persulfate, etc.<br />
• Again, consider the chlorate ion, ClO 3 - .<br />
• Taking away one oxygen from the “-ate” anion changes its ending from “-ate” to<br />
“-ite.”<br />
◦ Therefore, ClO 2 - is the chlorite ion, and SO 3 2- is the sulfite ion.<br />
• Taking away two oxygens from the “-ate” anion changes its ending from “-ate” to<br />
“-ite,” and you must add the prefix “hypo-”<br />
◦ So, ClO - is the hypochlorite ion, and SO 2 2- is the hyposulfite ion.<br />
Oxoanions Containing Hydrogen<br />
• Some common polyatomic anions have an H + “within” their formula.<br />
◦ In these ions, the H is always listed first, and the normal charge of the ion is changed by<br />
+1.<br />
◦ The name of the ion is changed by adding one of the following:<br />
• The prefix “bi-”, or<br />
• The word “hydrogen” before the name of the anion (sometimes you might see<br />
“monohydrogen” instead.)<br />
◦ For example, HCO 3 - is commonly called the “bicarbonate ion” or the “hydrogen carbonate<br />
ion.”<br />
◦ What would HSO 3 - be called<br />
• Occasionally you may also see two hydrogen atoms added to the ion. This is rare, except in<br />
the case of phosphate.<br />
• This would increase the charge of the original anion by +2.<br />
• The word “dihydrogen” is added to the name of the anion.<br />
• So H 2 PO - 4 is the “dihydrogen phosphate” ion.<br />
• KH 2 PO 4 is called “potassium dihydrogen phosphate.”<br />
• NOTE: In all these examples, H + is not the cation; we should consider it an “attachment” of<br />
the anion for naming purposes.<br />
Examples<br />
Name each of the following compounds:<br />
KIO 4<br />
LiH 2 PO 4<br />
NaHCO 3<br />
NaClO<br />
Al 2 (SO 3 ) 3<br />
Co(NO 2 ) 3<br />
CuHPO 3<br />
7
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
Oxoacids<br />
• Oxoacids are compounds which contain exactly as many H + ions as are necessary to cancel<br />
out the negative charge of an oxoanion.<br />
◦ For example, SO 4 2- would need two H + ions to balance out the 2- charge of sulfate; the<br />
oxoacid has the formula H 2 SO 4 .<br />
◦ Note that the H + ions are<br />
• the only cations in the formula, and<br />
• always listed first in the formula.<br />
Naming Oxoacids<br />
• The naming rules for oxoacids are similar to those for oxoanions.<br />
◦ The name of the oxyacid depends on how many oxygen atoms are in the corresponding<br />
oxoanion.<br />
• For those oxoanions which end in “-ate”, change the ending to “-ic acid.”<br />
◦ So, CO 3<br />
2-<br />
is the carbonate ion<br />
◦ H 2 CO 3 is carbonic acid<br />
◦ HNO 3 is named _________________________________<br />
◦ Slightly “weird” cases: H 2 SO 4 is sulfuric acid, and H 3 PO 4 is phosphoric acid.<br />
• An oxoanion that begins with “per-” follows the same rules.<br />
• Simply change the ending to “-ic acid.”<br />
◦ HClO 4 is called perchloric acid.<br />
◦ HIO 4 is called periodic acid.<br />
• Any oxoanion that ends in “-ite” has its ending changed to “-ous acid”<br />
◦ H 2 SO 3 is called sulfurous acid.<br />
◦ HClO 2 is called chlorous acid.<br />
• The acids of oxoanions which begin with “hypo-” likewise have their ending changed to “-ous<br />
acid”.<br />
◦ HBrO would be called hypobromous acid.<br />
◦ HNO would be called hyponitrous acid.<br />
Examples<br />
Name the following oxoacids:<br />
H 3 PO 4<br />
HIO 2<br />
HNO 3<br />
H 2 CO 3<br />
HNO 2 HIO<br />
8
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Six <strong>Notes</strong><br />
The Cyanide Ion<br />
• One last random bit of information…<br />
• The cyanide ion (CN - ) often behaves like a halogen, so naming rules for it are similar to those<br />
of F - , Cl - , etc.<br />
• HCN (g) is called “hydrogen cyanide.”<br />
• HCN (aq) is called hydrocyanic acid.<br />
Hydrates<br />
• A hydrate is an ionic compound which has “trapped” a fixed number of water molecules within<br />
its structure<br />
• For example, the following compound is called copper (II) sulfate pentahydrate:<br />
CuSO 4 · 5 H 2 O<br />
◦ The formula tells us that there are five water molecules in the structure for every unit of<br />
copper (II) sulfate<br />
• The naming of other hydrates is similar:<br />
◦ State the name of the salt<br />
◦ End with a prefix indicating how many water molecules are present, followed by the word<br />
“hydrate”<br />
Name each of the following hydrates:<br />
BaCl 2 · 2 H 2 O<br />
MgSO 4 · 7 H 2 O<br />
Final Examples<br />
Name each of the following compounds.<br />
BrO 4<br />
NH 3<br />
Cu(ClO 4 ) 2<br />
N 2 O<br />
H 2 SO 3<br />
F 2<br />
HF (aq)<br />
HIO 3<br />
LiHCO 3<br />
9
<strong>Chemistry</strong> <strong>120</strong><br />
Monatomic Ions I<br />
This periodic table contains the formulas of what I consider to be the most important ions<br />
which only form one charge. You'll notice a few important details:<br />
(1) The charge on almost all of the metal ions on this list is the same as the group number.<br />
Group<br />
1A<br />
(2) The charge on a nonmetal is simply its group number minus eight (i.e. oxide is<br />
derived from oxygen, which is in group 6; 6 - 8= -2 )<br />
(3) Zinc, cadmium, and silver ions are generally only encountered with the charge indicated.<br />
(4) As a cation, hydrogen makes a 1+ ion; when hydrogen makes an ionic bond with a metal<br />
H + /H - 2A the result is a "hydride" ion, which has charge 1-.<br />
3A 4A 5A 6A 7A<br />
(5) Boron and beryllium are excluded, as they generally form only covalent bonds.<br />
(6) Many other elements form ions with two or more different charges; they have also been<br />
Li + excluded.<br />
C 4-<br />
N 3- O 2-<br />
carbide<br />
nitride oxide<br />
(rare)<br />
Na + Mg 2+ 3B 4B 5B 6B 7B 8B 1B 2B Al 3+ P 3- S 2-<br />
phosphide sulfide<br />
K + Ca 2+ Zn 2+ Ga 3+ Se 2-<br />
selenide<br />
Rb + Sr 2+ Ag + Cd 2+ I -<br />
F -<br />
fluoride<br />
Cl -<br />
chloride<br />
Br -<br />
bromide<br />
iodide<br />
8A
<strong>Chemistry</strong> <strong>120</strong><br />
Monatomic Ions II<br />
Group<br />
1A<br />
This sheet lists the possible charges of many common elements which have more than one stable charge sta<br />
You should know both the new name and old name for each (i.e. copper (I) ion and cuprous ion). Note that<br />
the mercury (I) ion is a strange case; it is always found as a pair of atoms with a net charge of 2+ shared<br />
between each atom in the pair.<br />
8A<br />
2A 3A 4A 5A 6A 7A<br />
3B 4B 5B 6B 7B 8B 1B 2B<br />
Cr 3+<br />
Fe 3+ Co 3+<br />
Cr 2+ Fe 2+<br />
Co 2+ Cu 2+<br />
Cu + Sn 4+<br />
Sn 2+<br />
Hg 2+<br />
Hg 2<br />
2+<br />
Pb 4+<br />
Pb 2+
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Seven <strong>Notes</strong><br />
Chapter Seven<br />
Formula Calculations<br />
Introducing the Mole<br />
• The dozen is a unit of quanity<br />
◦ If I have a dozen atoms, I have 12 atoms by definition.<br />
• The mole(mol) is a very important unit of quantity in chemistry. It is used to count large<br />
numbers of atoms, molecules, and other submicroscopic pieces of matter.<br />
• If you have 1 mole of something, you have 6.02 × 10 23 of it.<br />
Examples<br />
• How many eggs are in 5.5 dozen eggs<br />
• How many atoms are in 5.5 mole of atoms<br />
• How many hydrogen atoms are in one molecule of water How many oxygen atoms<br />
• How many hydrogen atoms are in one mole of water How many oxygen atoms How many<br />
atoms total <br />
Practice<br />
• If you have 18.45 mol of oxygen gas, how many individual molecules do you have How<br />
many individual atoms<br />
• If a sample of methane contains 7.35 × 10 25 atoms, how many moles of methane do you<br />
have<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Seven <strong>Notes</strong><br />
Atomic Weights and The Mole<br />
• The atomic weights provided on the periodic table can be used in much more convenient<br />
units than amu.<br />
• The values on the periodic table can be interpreted as grams per mole of the atom.<br />
◦ For example, 1 mol of calcium atoms has a mass of 40.08 g; 1 mol of neon atoms has a<br />
mass of 20.18 g.<br />
• Note that atomic weights are often also called molar masses.<br />
Molecular Weights<br />
• The mass of molecules can be calculated by adding up the atomic weights of the individual<br />
atoms making up the molecule.<br />
• For example, suppose we wanted to know the atomic weight of CO 2 .<br />
◦ Every 1 mol of CO 2 contains_____mole of C atoms and_____moles of O atoms.<br />
◦ Calculate the total mass of all of these atoms and add them up to get the molecular<br />
weight of CO 2 .<br />
◦ Aside: what is the mass of a single molecule of CO 2 in amu<br />
• Note that the term formula weight is applied for those compounds which do not form true<br />
molecules (ionic compounds like NaCl and CaO).<br />
Examples<br />
Determine the molecular weights of glucose (C 6 H 12 O 6 ) and acetic acid (CH 3 CO 2 H).<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Seven <strong>Notes</strong><br />
Percent Composition<br />
• One common technique used in specialized chemical laboratories is elemental analysis,<br />
which can be used to determine the percent each element in a compound contributes to its<br />
mass.<br />
• Since this type of data is very common, it is important that we know how to interpret it and put<br />
it to practical use.<br />
• The percent composition is the percent of the total mass percent of each element in a<br />
compound.<br />
• To determine its value, we use the following formula for each element in the compound:<br />
total mass of element<br />
% composition =<br />
× 100%<br />
molar mass<br />
Examples<br />
What is the percent composition of each element in acetic acid<br />
A 19.82 g chunk of an ore is analyzed and found to have a percent composition of 5.75% silver,<br />
64.33% iron, and the remainder is silicon. What mass of each element is contained in a 4.87 kg<br />
sample of this ore<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Seven <strong>Notes</strong><br />
Percent compositions can also be determined for mixtures, such as alloys.<br />
Suppose that 5.50 mols each of copper and zinc are blended with 2.43 mols of tin to make an<br />
alloy. What is the percent composition of the alloy<br />
A student determines the mass of a hydrate sample to be 6.873 g. After severely heating the<br />
sample for 20 minutes to remove water, he reweighs the sample, finding the mass to be<br />
5.276 g. What percent of the mass of the original hydrate is water<br />
Molecular and Empirical Formulas<br />
• The molecular formula of a compound tells us exactly how many atoms of each element are<br />
contained in a compound.<br />
• In contrast, the empirical formula only tells us the lowest whole-number ratio between each<br />
element<br />
• For example, glucose has molecular formula C 6 H 12 O 6 (each molecule of glucose contains 6<br />
carbon atoms, 12 hydrogen atoms, and 6 oxygen atoms)<br />
• Glucose then has empirical formula CH 2 O (1 C to 2 H to 1 O is the lowest whole-number<br />
ratio).<br />
Empirical Formulas<br />
• While the molecular formula ultimately is more useful for most applications, it is often more<br />
difficult to determine than the empirical formula.<br />
• When a sample is analyzed we can easily determine the percent composition, and from here<br />
find the ratio of the number of atoms of each element.<br />
• Information on the exact number of atoms in each molecule cannot be found in this way.<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Seven <strong>Notes</strong><br />
Determining the Emprical Formula<br />
• A simple series of steps can be used to determine the empirical formula of a compound:<br />
◦ Find the mass of each element in the compound<br />
◦ Convert the masses into moles of each element<br />
◦ Express the moles of atoms as the smallest possible whole-number ratio<br />
◦ Use the numbers from these ratios in the empirical formula for each element.<br />
Examples<br />
A sample of a compound is analyzed, and found to contain 1.61 g of phosphorus and 2.98 g of<br />
fluorine. What is the empirical formula of this compound<br />
The mass of a piece of iron is 1.62 g. The iron is exposed to oxygen and reacts to form a pure<br />
oxide of iron, now with mass of 2.31 g. What is the empirical formula of this oxide<br />
A compound is found to contain 20.0% carbon, 2.2% hydrogen, with the remainder of the mass<br />
derived from chlorine. What is the empirical formula of this compound<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Seven <strong>Notes</strong><br />
Molecular Formula<br />
• Given the empirical formula and the molecular weight of a compound, it is possible to<br />
determine the molecular formula.<br />
• For example, suppose we have a compound with empirical formula CH.<br />
◦ Its molecular formula could be CH, C 2 H 2 , C 3 H 3 , etc.<br />
• Now, let’s see what the formula weight would be for each:<br />
◦ CH = 13.02 g/mol<br />
◦ C 2 H 2 = 26.04 g/mol<br />
◦ C 3 H 3 = 39.06 g/mol<br />
◦ Notice that each is a multiple of 13.02!<br />
• To determine the molecular formula from this information<br />
◦ Find the formula weight of the empirical formula<br />
◦ Divide the molecular weight by this value (you should get a whole number).<br />
◦ Multiply the subscripts in your empirical formula by this whole number.<br />
• You now have your molecular formula.<br />
Example<br />
An unknown compound is determined to be 91.8% silicon and 8.2% hydrogen. The molar mass<br />
of this compound is found to be 122 g/mol. Determine the molecular formula of the<br />
compound.<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Chapter Eight<br />
Chemical Reactions<br />
What is a Chemical Reaction<br />
• A chemical reaction involves the conversion of one or more substances into one or more<br />
different substances.<br />
• The substance(s) which we begin with are called the reactant(s)<br />
• The substance(s) which we end with are called the product(s)<br />
Writing Chemical Reactions<br />
• Chemical reactions are written with the reactants to the left, the products to the right, and an<br />
arrow between them to indicate the change.<br />
◦ Occasionally symbols or values may be written over or under the arrow to indicate the<br />
reaction conditions.<br />
• An Example:<br />
H 2 + O 2 H 2 O<br />
Balancing Chemical Equations<br />
• Consider the last reaction:<br />
H 2 + O 2 H 2 O<br />
• There is a problem with this equation!<br />
• It indicates that we started with two oxygen atoms, but ended with one.<br />
• What does this contradict<br />
• We must balance chemical equations, which is to say that there must be equal numbers of<br />
each type of atom on either side of a chemical reaction.<br />
• To accomplish this, we put coefficients in front of the chemical formulas whose atom numbers<br />
we wish to increase.<br />
• Note that you may never change the subscripts already in place in a chemical formula!<br />
◦ Why<br />
• To balance chemical equations first count the number of each type of atom you have on both<br />
sides of the reaction.<br />
• Identify any lone elements (as opposed to compounds) in the formulas; you will balance<br />
these last.<br />
• From here, each equation requires its own logic; by trial and error, you should be able to<br />
balance the equation.<br />
• The only other real “tip” I can give you on this subject is that practice makes perfect!<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Examples<br />
Balance each of the following chemical reactions:<br />
Mg + O 2 MgO<br />
HgO Hg + O 2<br />
Na + MgCl 2 Mg + NaCl<br />
Na 3 PO 4 + BaCl 2 Ba 3 (PO 4 ) 2 + NaCl<br />
C 6 H 12 O 6 + O 2 CO 2 + H 2 O<br />
• Write the balanced equation that corresponds to each statement<br />
◦ When methane reacts with oxygen gas, carbon dioxide and water vapor are produced.<br />
◦ Calcium metal reacts with ferric oxide, yielding calcium oxide and iron metal.<br />
◦ Treatment of carbon monoxide gas with oxygen gas produces carbon dioxide.<br />
Types of Chemical Reactions<br />
• There are five main classification types of chemical reactions.<br />
• Knowing how each of these reaction types “works” gives you the ability to predict what<br />
chemical products will be formed in a given reaction in most cases.<br />
• Types of Chemical Reactions<br />
◦ Combustion<br />
◦ Single Substitution (Displacement)<br />
◦ Double Substitution (Displacement)<br />
◦ Combination (or Synthesis)<br />
◦ Decomposition<br />
• Within these five classification types, even more specific reaction types can be identified;<br />
these will be described as we come to them.<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Combustion Reactions<br />
• In a combustion reaction, a chemical reacts with oxygen gas, forming various products.<br />
• In this class, we will only consider the combustion of organic compounds containing C, H, and<br />
sometimes O.<br />
• In these reactions, the compound reacts with oxygen gas, producing carbon dioxide and<br />
water vapor.<br />
[organic compound] + O 2(g) CO 2(g) + H 2 O (g)<br />
Examples of Combustion<br />
• Combustion of benzene<br />
2C 6 H 6(l) + 15O 2(g) 12CO 2(g) + 6H 2 O (g)<br />
Combustion of formaldehyde<br />
•<br />
CH 2 O (l) + O 2(g) CO 2(g) + H 2 O (g)<br />
• What is the balanced equation for the combustion of glycerol (C 3 H 8 O 3(l) )<br />
Single Substitution Reactions<br />
• In a single substitution reaction, an element replaces another element which is present as an<br />
ion in a compound.<br />
• There are two types of substitutions we should be aware of:<br />
◦ substitution of one metal with another<br />
◦ substitution of one halogen with another<br />
• Format of the first type of single substitution reactions:<br />
A + BX AX + B<br />
Where A and B are metals/metal ions, and X is an anion.<br />
• Here are some examples:<br />
Mg + ZnCl 2 MgCl 2 + Zn<br />
Zn + 2AgNO 3 Zn(NO 3 ) 2 + 2Ag<br />
2Na + 2H 2 O 2NaOH + H 2<br />
Activities of Metals<br />
• We can use the activity of a metal to describe how readily it loses electron(s) in a reaction.<br />
◦ The more active the metal, the more readily it loses its electrons.<br />
• A more active metal will displace a less active metal in a single substitution reaction; the<br />
reverse will not occur.<br />
◦ In other words, an active metal will force the cation of a less active metal to take its<br />
electrons away from it.<br />
• We look to the activity series to see the relative activities of the metals.<br />
◦ The activity series should not be memorized, but you should become familiar with trends<br />
within it.<br />
Displacing Hydrogen<br />
• Notice that many metals can displace the H + from acids, changing it into H 2 .<br />
◦ Notice that the charged hydrogen ion is transformed into the neutral hydrogen molecule.<br />
• Some very active metals can even displace H + from water, leaving OH - behind.<br />
◦ In these cases, think of water as HOH.<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
When Does the Reaction “Go”<br />
• So let’s consider one single substitution that works well…<br />
Zn + 2AgNO 3 Zn(NO 3 ) 2 + 2Ag<br />
• Since zinc is more active than silver (higher on the activity series), zinc will displace silver.<br />
• Consider the reverse reaction…<br />
Ag + Zn(NO 3 ) 2 no reaction<br />
• Since silver is less active than zinc, it cannot displace it; therefore, no reaction can occur.<br />
Oxidation & Reduction:<br />
An Introduction<br />
• Single substitution reactions involve an oxidation and a reduction.<br />
◦ When a metal atom or ion is oxidized, it loses one or more electrons, resulting in an<br />
increase in its charge.<br />
• Example: Zn Zn 2+ + 2e -<br />
◦ When a metal ion is reduced, it gains one or more electrons, causing its charge to<br />
decrease.<br />
• Example: Ag + + e - Ag<br />
• An oxidation reaction is always accompanied by a reduction reaction.<br />
• Redox is the common term for these reactions.<br />
A Look at Some Redox Reactions<br />
• Consider the following single substitution reaction:<br />
3Mg + 2FeCl 3 3MgCl 2 + 2Fe<br />
◦ What is being oxidized<br />
◦ What is being reduced<br />
• Try this reaction:<br />
2Na + 2H 2 O 2NaOH + H 2<br />
◦ What is being oxidized<br />
◦ What is being reduced<br />
Single Substitution Reactions:<br />
Substitution of Halogens<br />
• Anions derived from halogens (Group VII) can be displaced by a more active halogen.<br />
• Activity of the halogens decreases down the group:<br />
F 2 > Cl 2 > Br 2 > I 2<br />
most active least active<br />
• An example:<br />
Cl 2 + 2NaI 2NaCl + I 2<br />
• Will the reverse reaction proceed<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Examples<br />
Predict the products of the following reactions. Write “no rxn.” if none is expected to occur.<br />
Ba + CoBr 3 <br />
Ni + NaCl <br />
I 2 + KF <br />
Li + H 2 O <br />
Ni + HNO 3 <br />
Double Substitution Reactions<br />
• The general format for a double substitution reaction involves two ionic compounds trading<br />
their anions:<br />
AX + BY AY + BX<br />
• AX and BY are both aqueous solutions, meaning both ionic compounds are dissolved in<br />
water.<br />
• These reactions will proceed only if at least one of the following is true:<br />
◦ A solid precipitate is produced<br />
◦ A covalent (molecular) compound is produced, such as H 2 O, H 2 , CO 2 , SO 3 , etc.<br />
Examples of Double Substitution Reactions<br />
AgNO 3(aq) + NaCl (aq) AgCl (s) + NaNO 3(aq)<br />
3Ba(OH) 2(aq) + 2FeCl 3(aq) 3BaCl 2(aq) + 2Fe(OH) 3(s)<br />
HCl (aq) + NaOH (aq) H 2 O (l) + NaCl (aq)<br />
Solubility of Compounds<br />
• Solubility is best described as the degree to which a compound will dissolve in a solvent<br />
(usually water).<br />
◦ A compound that is soluble will dissolve to a significant extent.<br />
◦ Compounds that are insoluble will not dissolve, remaining solid in solution.<br />
• A reaction which produces an insoluble product can be described as a precipitation reaction;<br />
the product “falls out” of the solution like rain precipitates.<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Solubility<br />
• It is important to know whether or not some common chemicals are soluble or not in order to<br />
predict how a reaction will proceed.<br />
• You should know the following solubility rules (in water) by memory:<br />
◦ All nitrates and acetates are soluble.<br />
◦ All salts of Group I cations (Li + , Na + , etc.) and ammonium are soluble.<br />
◦ All chlorides, bromides, and iodides are soluble, except those of Ag + , Pb 2+ , and Hg 2 2+ .<br />
◦ All hydroxides are insoluble except those of Group I, NH 4 + , Ba 2+ , Sr 2+ , and Ca 2+ .<br />
• Ca(OH) 2 is only slightly soluble.<br />
Unstable Products of Reactions<br />
• When produced in a reaction, some compounds will immediately decompose into other<br />
products.<br />
◦ Carbonic acid (H 2 CO 3 ) will decompose into CO 2(g) and H 2 O (l) .<br />
◦ Ammonium hydroxide (NH 4 OH) will decompose into NH 3(aq) and H 2 O (l) .<br />
◦ Sulfurous acid (H 2 SO 3 ) will decompose into SO 2(g) and H 2 O (l) .<br />
• Notice that each produces water and a compound formed by the atoms left after water has<br />
been removed from the starting formula.<br />
• If you produce any of these three compounds in a reaction, cancel it out and replace it with<br />
the decomposition products.<br />
Electrolytes<br />
• When an ionic compound dissolves in water, it dissociates (separates) into ions.<br />
• A solution containing ions is capable of conducting an electric current.<br />
• The term electrolytes is applied to these ions.<br />
• A solution formed from a soluble ionic compound conducts the current very strongly; the<br />
compound is called a strong electrolyte.<br />
• A solution formed from an only slightly soluble ionic compound conducts the current weakly;<br />
the compound is called a weak electrolyte.<br />
• A solution derived from a non-ionic (i.e. covalent) compound will not conduct an electric<br />
current; the compound is called a nonelectrolyte.<br />
Acids and Bases<br />
• You have heard the term acid applied to several compounds.<br />
◦ All of these compounds mentioned so far contain the H + , called a proton.<br />
• We will look more in depth at the definitions of acids and bases later, but for now we will use<br />
the following:<br />
◦ Acids are compounds which give up H + ions.<br />
◦ Bases are compounds which accept H + ions.<br />
• For now, we will limit our study of bases to some hydroxide-containing compounds<br />
and NH 3 .<br />
Strong Acids<br />
• Strong acids are strong electrolytes, meaning they completely break up into ions in solution.<br />
◦ So, HCl, which is a strong acid, breaks up into H + ions and Cl - ions in solution.<br />
There are six strong acids you must know:<br />
•<br />
HCl HBr HI<br />
HNO 3 H 2 SO 4 HClO 4<br />
• Note that H 2 SO 4 dissociates into H + and HSO - 4 .<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Example: If you were to “look” into a beaker of the following solutions, what ions, solids, or<br />
molecules would you expect to see (besides water)<br />
a. HNO 3<br />
b. HBr<br />
c. HClO 4<br />
Weak Acids<br />
• Weak acids are weak electrolytes, meaning that relatively few acid molecules will break up<br />
into separate ions.<br />
• Some samples of weak acids are<br />
H 3 PO 4 H 2 CO 3<br />
HCH 3 CO 2<br />
Strong and Weak Bases<br />
• Similar definitions apply to strong bases.<br />
• The strong bases are the Group I hydroxides (LiOH, NaOH, KOH, etc.) and some Group II<br />
hydroxides: Ba(OH) 2 , Sr(OH) 2 , and Ca(OH) 2 .<br />
• The weak bases include Mg(OH) 2 and NH 3(aq) (which can be treated as<br />
NH 4 OH (aq) for now).<br />
Neutralization Reactions<br />
• Neutralization reactions are a subclass of double substitution reactions.<br />
• The general form of this reaction is<br />
acid + base water + salt<br />
where the salt is any ionic compound.<br />
• This can be further simplified as follows:<br />
H + + OH - H 2 O<br />
• Strong acids and strong bases completely neutralize each other.<br />
• A strong acid will neutralize a weak base, and a strong base will neutralize a weak acid.<br />
• The reactions of weak acids with weak bases is somewhat more complicated and will not be<br />
considered in this class.<br />
Examples<br />
HBr (aq) + KOH (aq) H 2 O (l) + KBr (aq)<br />
2HNO 3(aq) + Ba(OH) 2(aq) 2H 2 O (l) + Ba(NO 3 ) 2(aq)<br />
7
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Write the balanced equations showing:<br />
a) the neutralization of lithium hydroxide by perchloric acid.<br />
b) the reaction of sulfuric acid with strontium hydroxide.<br />
c) an ammonia solution is treated with hydrobromic acid.<br />
Combination Reactions<br />
• In a combination (or synthesis) reaction, two chemicals combine into one new chemical.<br />
• These reactions have the general form<br />
A + B C<br />
• It will not always be possible to predict the products of combination reactions at this level of<br />
preparation, so we will study a few general cases.<br />
Oxide Formation<br />
• Metals often react with oxygen to form a metal oxide.<br />
Ex. 4Na + O 2 2Na 2 O<br />
• Nonmetals often react with oxygen to form a nonmetal oxide.<br />
Ex. C + O 2 CO 2<br />
◦ It is often difficult to predict the products in this case, as CO was another possible oxide<br />
you might have considered.<br />
Reactions of Oxides<br />
• Metal oxides often react with water to form metal hydroxides.<br />
Ex. Na 2 O + H 2 O 2NaOH<br />
• Nonmetal oxides often react with water to form oxyacids.<br />
Ex. CO 2 + H 2 O H 2 CO 3<br />
P 4 O 10 + 6H 2 O 4H 3 PO 4<br />
SO 3 + H 2 O H 2 SO 4<br />
N 2 O 5 + H 2 O 2HNO 3<br />
• Metal oxides and nonmetal oxides often combine to form a salt.<br />
Na 2 O + CO 2 Na 2 CO 3<br />
CaO + SO 3 CaSO 4<br />
Decomposition Reactions<br />
• Decomposition reactions are simply the reverse of combination reactions.<br />
• Their general form is<br />
Z X + Y<br />
• Like combination reactions, predicting the products of these reactions is often difficult.<br />
• For now, simply decompose a given compound into two products which could have produced<br />
it from a method we discussed earlier.<br />
◦ This is very oversimplified, and not always correct, but it is the best we can do at this<br />
level.<br />
8
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Eight <strong>Notes</strong><br />
Examples<br />
2HgO 2Hg + O 2<br />
Na 2 CO 3 Na 2 O + CO 2<br />
Li 2 SO 4 Li 2 O + SO 3<br />
Heat in Chemical Reactions<br />
•Virtually every chemical reaction results in either a gain or loss of heat to the reaction system<br />
•A reaction which produces more heat than it consumes is called an exothermic reaction<br />
•A reaction which consumes more heat than it produces is called an endothermic reaction<br />
•The chemical reaction written below describes an exothermic reaction:<br />
CH 4(g) + 2 O 2(g) CO 2(g) + 2 H 2 O (g) + 890 Kj<br />
•For an endothermic reaction, the heat would appear with the reactants in the chemical<br />
equation:<br />
PCl 5 + 92.9 kJ PCl 3 + Cl 2<br />
•Although this method is convenient for indicating heat changes, it often leads to confusion in<br />
balancing equations<br />
◦A better method for indicating energy changes will be presented in Chem 130<br />
Heat and Chemical Bonds<br />
•Energy is always consumed in the breaking of chemical bonds.<br />
•The opposite is also true: energy is always released when new chemical bonds are formed.<br />
•Ultimately, whether a reaction is exothermic or endothermic therefore depends on the number and type of<br />
bonds being broken and formed in a chemical reaction<br />
Activation Energy and Energy Diagrams<br />
•In order for a chemical reaction to begin, some amount of energy specific to that reaction must be<br />
supplied to start the reaction process<br />
•The amount of this initial investment of energy is called the activation energy<br />
•The activation energy, as well as the energy changes in chemical reactions, may be illustrated by energy<br />
diagrams<br />
9
Activity Series of Metals<br />
Most Li Displaces hydrogen from<br />
Active Rb cold water, steam, and acids<br />
K<br />
Cs<br />
Ba<br />
Sr<br />
Ca<br />
Na<br />
Mg Displaces hydrogen from<br />
Al steam and acids<br />
Mn<br />
Zn<br />
Cr<br />
Fe<br />
Cd Displaces hydrogen from<br />
Co acids<br />
Ni<br />
Sn<br />
Pb<br />
H 2<br />
Cu Cannot displace hydrogen from<br />
Hg cold water, steam, or acids<br />
Ag<br />
Least Pt<br />
Active Au<br />
Solubilities of Selected Ionic Compounds in Water<br />
In general, all ionic compounds containing ammonium (NH 4 + ) and Group IA cations (Li + , Na + , K + , etc.) are<br />
soluble.<br />
nitrates<br />
acetates<br />
chlorates<br />
chlorides<br />
bromides<br />
iodides<br />
sulfates<br />
chromates<br />
oxides<br />
hydroxides<br />
sulfides<br />
carbonates<br />
phosphates<br />
sulfites<br />
all are soluble<br />
all are soluble except Ag + , Pb 2+ , & Hg 2<br />
2+<br />
all are soluble except Ag + , Pb 2+ , & Hg 2 2+ , Hg 2+ ,<br />
Ba 2+ , Sr 2+ , & Ca 2+<br />
note: CaCrO 4 is soluble, CuCrO 4 is not<br />
none soluble except Group IA, NH 4 + ,<br />
Ba 2+ , Sr 2+ , & Ca 2+<br />
none soluble except Group IA, NH 4 + , and<br />
Group IIA<br />
none soluble except Group IA & NH 4<br />
+
Activity Series of Metals—Test Version<br />
Most Li Displaces hydrogen from<br />
Active Rb cold water, steam, and acids<br />
K<br />
Cs<br />
Ba<br />
Sr<br />
Ca<br />
Na<br />
Mg Displaces hydrogen from<br />
Al steam and acids<br />
Mn<br />
Zn<br />
Cr<br />
Fe<br />
Cd Displaces hydrogen from<br />
Co acids<br />
Ni<br />
Sn<br />
Pb<br />
H 2<br />
Cu Cannot displace hydrogen from<br />
Hg cold water, steam, or acids<br />
Ag<br />
Least Pt<br />
Active Au<br />
Solubilities of Selected Ionic Compounds in Water<br />
Note that the solubility rules for those compounds which you were to have memorized have been deleted<br />
from the table.<br />
chlorates<br />
sulfates<br />
chromates<br />
sulfides<br />
carbonates<br />
phosphates<br />
sulfites<br />
all are soluble<br />
all are soluble except Ag + , Pb 2+ , & Hg 2 2+ , Hg 2+ ,<br />
Ba 2+ , Sr 2+ , & Ca 2+<br />
note: CaCrO 4 is soluble, CuCrO 4 is not<br />
none soluble except Group IA, NH 4 + , and<br />
Group IIA<br />
none soluble except Group IA & NH 4<br />
+
'{rB u} paEmq s1 '@1ItC'se5 auelng '61<br />
az-rpuo<br />
lt1a1a1duo sI ppe apaE pfnbq arnd 'IT<br />
'r:fs uT peumq q TfC<br />
'se5 anBdcrd '0I<br />
'sasoduoap 1r IFFrn psleeq z(ltuoqs sI ppu cr.mrms pFbII amd -6<br />
'PatBeq sr apporpzfq rrnrrBg 'g<br />
'peleaq sr s+B.roFIc urrgpob 'L<br />
'Pe4Baq q sl"uoqrBc urmclBc 'g<br />
'eulurorq qlIA slcBar umuumlg 'g<br />
'pepear are errrrolqr pue uatorpdg ',<br />
'r€ylB.s, cr+q polqqnq s! epFrolJr n!flns 'g<br />
'rslBA 01 PeppE sI aPFEo umuBg<br />
'z<br />
t<br />
'aPDr@ap sruroqdsoqde.4al pIlos Eurcnpo.rd {rE uI paErnq sr sruroqdsoq4 'I<br />
'suonccar 1ecpeqa tuurogog aWJo rpea rq[ suonenbe paruaqa s;1r/U\<br />
€sUoTlcBar<br />
$ro!+tlrbglc'[Eerlc
<strong>Chemistry</strong> <strong>120</strong><br />
Net Ionic Equation <strong>Notes</strong><br />
Net Ionic Equations<br />
Revisiting “aqueous”<br />
• The term aqueous is mainly a visual one; when you add a chemical to water and it appears to<br />
dissolve, we say an aqueous solution has been formed.<br />
• However, we must be more specific:<br />
◦ For ionic compounds, including strong acids, aqueous means that the compound has<br />
dissociated into ions.<br />
◦ For weak acids and other covalent compounds, aqueous means that the compound has<br />
dissolved, but not been broken down into smaller parts. It is merely “surrounded” by<br />
water molecules.<br />
Looking Back<br />
• Consider the following reaction:<br />
NaCl (aq) +KNO 3(aq) <br />
• Since both the products of this reaction are aqueous, and since no molecular compound is<br />
formed, we say that there is no reaction.<br />
• However, since we did bring these two solutions together, why is it incorrect to say that the<br />
products are KCl (aq) and NaNO 3(aq) <br />
• Earlier, we defined a chemical change as one that involves transforming one or more<br />
chemical compounds into one or more different products.<br />
• By combining two solutions which do not make an insoluble product or a molecular<br />
compound, we fail to create a new product, as we shall now prove.<br />
Total Ionic Equations<br />
• Total molecular equations show all species in solution for a given reaction.<br />
◦ The term species refers to the specific ions and/or compounds in the solution.<br />
• Examples of species:<br />
For NaCl (aq) , Na + (aq) and Cl - (aq).<br />
For HNO 3(aq) , H + (aq) and NO 3<br />
-(aq).<br />
For H 3 PO 4(aq) , it remains H 3 PO 4(aq) .<br />
• Some simple guidelines for writing down the species.<br />
◦ Strong electrolytes, including strong acids and bases, dissociate into their ions.<br />
◦ Weak electrolytes, including weak acids and bases, generally do not dissociate, so the<br />
species is just the original compound.<br />
◦ Nonelectrolytes do not dissociate, so the species is again the same as the original<br />
compound.<br />
Total Ionic Equations<br />
Example:<br />
NaCl (aq) + AgNO 3(aq) AgCl (s) + NaNO 3(aq)<br />
Total Molecular Equation:<br />
Na + (aq) + Cl - (aq) + Ag + (aq) + NO 3<br />
-<br />
(aq) AgCl (s) + Na + (aq) + NO 3<br />
-<br />
(aq)<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Net Ionic Equation <strong>Notes</strong><br />
Spectator Ions<br />
• A spectator of sports is someone who watches the game from the sidelines, but does not<br />
participate.<br />
• Similarly, in chemical reactions, spectator ions “hang out” in a solution but do not actively<br />
participate in the reaction itself.<br />
◦ In other words, any ion which is both on the reactants and products side of a reaction is a<br />
spectator ion, for it has not undergone a chemical change.<br />
• The ions’ main purpose is to maintain constant charge in the solution.<br />
Net Ionic Equations<br />
• Net ionic equations only show those chemicals which participate in the reaction. Spectator<br />
ions are not included.<br />
• To write a net ionic equation, first write down the total ionic equation.<br />
• Then, cancel anything which appears identically on both sides of the reaction.<br />
• Consider the total ionic equation<br />
Na + (aq) + Cl - (aq) + Ag + (aq) + NO 3<br />
-<br />
(aq) AgCl (s) + Na + (aq) + NO 3<br />
-(aq)<br />
Now, factor out the spectator ions<br />
•<br />
Na + (aq) + Cl - (aq) + Ag + (aq) + NO 3<br />
-<br />
(aq) AgCl (s) + Na + (aq) + NO 3<br />
-(aq)<br />
• The net ionic equation is left over.<br />
Ag + (aq) + Cl - (aq) AgCl (s)<br />
Examples<br />
Write chemical equations, total ionic equations, and net ionic equations for the following:<br />
a. a solution of barium chloride reacts with a sodium sulfate solution.<br />
b. sodium hydroxide is neutralized by hydrochloric acid.<br />
c. phosphoric acid is reacted with potassium hydroxide.<br />
d. solutions of sodium nitrate and ammonium chloride are brought together.<br />
e. a piece of sodium metal is dropped into cold water.<br />
2
Type of Substance Type of Electrolyte Ionizes in Water Examples<br />
How to Write in Net<br />
Ionic Equations<br />
NaCl (aq)<br />
Na + (aq) + Cl - (aq)<br />
soluble ionic<br />
compounds<br />
strong<br />
completely<br />
KNO 3(aq)<br />
K + (aq) + NO 3<br />
-<br />
(aq)<br />
(NH 4 ) 2 SO 4(aq)<br />
2 NH 4<br />
+<br />
(aq) + SO 4<br />
2-<br />
(aq)<br />
AgCl (s)<br />
AgCl (s)<br />
insoluble ionic<br />
compounds<br />
nonelectrolyte<br />
PbI 2(s)<br />
PbI 2(s)<br />
covalent/molecular<br />
compounds<br />
(not all compounds in these<br />
categories are nonelectrolytes,<br />
but you should<br />
not worry about exceptions)<br />
not at all<br />
BaSO 4(s)<br />
H 2 O (l)<br />
C 6 H 12 O 6(aq)<br />
BaSO 4(s)<br />
H 2 O (l)<br />
C 6 H 12 O 6(aq)<br />
H 2(g)<br />
H 2(g)<br />
strong acids<br />
and<br />
strong bases<br />
strong<br />
completely<br />
HCl (aq)<br />
HNO 3(aq)<br />
NaOH (aq)<br />
H + (aq) + Cl - (aq)<br />
H + (aq) + NO 3<br />
-<br />
(aq)<br />
Na + (aq) + OH - (aq)<br />
weak acids<br />
and<br />
weak bases<br />
weak<br />
only slightly<br />
H 3 PO 4(aq)<br />
HC 2 H 3 O 2(aq)<br />
Mg(OH) 2(s)<br />
H 3 PO 4(aq)<br />
HC 2 H 3 O 2(aq)<br />
Mg(OH) 2(s)
Net Ionic Equations<br />
Write (1) full formula, (2) total ionic, and (3) net ionic equations for each of the following chemical<br />
combinations. Write “no rxn.” To the right of the arrow if you expect no reaction to occur.<br />
1. A piece of potassium is dropped in water.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
2. Aqueous solutions of iron (III) sulfate and ammonia are mixed.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
3. Silver is added to a cupric bromide solution.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
4. A sodium fluoride solution is mixed with nitric acid.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic
5. Aqueous solutions of potassium phosphate and cobalt (II) chloride are mixed.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
6. Aqueous ammonia is mixed with hydoiodic acid.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
7. Phosphoric acid is mixed with an aqueous solution of lithium hydroxide.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
8. Carbon dioxide is passed into aqueous barium hydroxide.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
9. Hydrobromic acid is mixed with a sodium carbonate solution.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic
10. Nitric acid is mixed with aqueous potassium bicarbonate.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
11. Rubidium oxide is added to water.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
12. Aqueous solutions of lithium acetate and tin (II) chloride are mixed.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic<br />
13. Hydrochloric acid is added to a lithium sulfite solution.<br />
(1) Full:<br />
(2) Total<br />
(3) Net Ionic
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
Chapter Nine: Stoichiometry<br />
Conservation<br />
• Recall that, in any chemical reaction, that matter is always conserved.<br />
• Consider the reaction of zinc with sulfur:<br />
Zn (s) + S (s) ZnS (s)<br />
• From this reaction we can imply that, assuming the reaction works perfectly, every one atom<br />
of zinc reacts with one atom of sulfur to produce one unit of zinc sulfide.<br />
• More conveniently, we can say that one mole of zinc atoms (1 mol Zn) reacts with one mole<br />
of sulfur atoms (1 mol S), producing one mole of zinc sulfide (1 mol ZnS)<br />
Common Misconceptions<br />
• Is it true that if I start a reaction with 5.0 g of zinc and 5.0 g of sulfur that I will end the reaction<br />
with 10.0 g of matter<br />
• Is it true that if I start a reaction with 5.0 g of zinc and 5.0 g of sulfur that I will end the reaction<br />
with 10.0 g of zinc sulfide<br />
• In predicting the quantities of products created during a reaction, it is ultimately the number of<br />
atoms/molecules reacting that we must consider, not the mass.<br />
• The most convenient way to do this is to consider the moles of reactants participating in a<br />
reaction.<br />
Coefficients of Reactions<br />
• The coefficients in chemical equations are useful in this context because they tell us how<br />
many moles of reactants are required to produce a certain number of moles of products.<br />
• We can say that one mole of zinc reacts with one mole of sulfur, producing 1 mole of zinc<br />
sulfide. The three are equivalent for the purpose of this reaction.<br />
1 mol Zn1mol S1 mol ZnS<br />
• We can convert between moles of reactants and products using dimensional analysis, the<br />
same technique we used for unit conversions.<br />
• To convert between moles of zinc and moles of zinc sulfide, we use the following ratio:<br />
Basic Problems<br />
Let’s consider the following reaction:<br />
2H 2(g) + O 2(g) 2H 2 O (l)<br />
To produce 2 mol of water we need to combine_____mol H 2 with_____mol O 2 .<br />
How many moles of each reactant are required to produce 10 moles of water<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
How many moles of water can be produced at most from 13 moles of hydrogen How many<br />
moles of oxygen would I need to accomplish this<br />
In the reaction of aqueous solutions of hydrochloric acid and barium hydroxide:<br />
a. How many moles of each reactant do you need to produce 5.75 mol water<br />
b. What is the maximum number of moles of water you can produce with 18.0 mol HCl How<br />
many moles of barium hydroxide would you need to accomplish this<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
Using the Mass-Mole Relationship<br />
• Recall that the molar mass relates the mass of a compound (or element) to the number of<br />
moles.<br />
• Therefore, if we know the mass of a given reactant, we can easily determine the number of<br />
moles of the reactant, and from there the number of moles of product produced.<br />
• Remember, you must use the mole-mole relationship to carry out a conversion; the mass<br />
alone is not sufficient!<br />
Mass-Mole Problems<br />
Consider the reaction of sodium metal with chlorine to make sodium chloride.<br />
a. How many moles of sodium are contained in 15.50 g of sodium<br />
b. Assuming we have excess (that is, more than enough) chlorine, how many moles of<br />
sodium chloride could be produced<br />
c. How many grams of sodium chloride is this<br />
When 39.75 g of sodium is reacted with excess chlorine, how many grams of sodium chloride can<br />
be produced<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
When 146.7 g of chlorine is reacted with excess sodium, how many grams of sodium chloride can<br />
be produced<br />
How many grams of each reactant do you need to produce 100.00 g of sodium chloride<br />
Another Example:<br />
Ethanol has molecular formula CH 3 CH 2 OH.<br />
a. How many grams of carbon dioxide and water can be produced if 55.0 mL of ethanol is<br />
combusted<br />
Note: The density of ethanol is 0.789 g/mL.<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
b. How many oxygen molecules are required to react with this amount of ethanol<br />
The Ice Cream Sundae Problem<br />
• Suppose we are going to make ice cream sundaes.<br />
• We decide that each of our sundaes must contain<br />
◦ 2 scoops of ice cream<br />
◦ 50 mL of chocolate syrup<br />
◦ 1 cherry<br />
• How many sundaes can I make if I have 8 scoops of ice cream, 13 cherries, and 300 mL of<br />
chocolate syrup available<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
Limiting Reactants<br />
• The problem we had with our ice cream sundaes is the same type of problem we face in<br />
chemical reactions.<br />
• In virtually all reactions, we will have a disproportionate amount of reactants.<br />
• The reactant which will produce less product is called the limiting reactant; in all cases, it<br />
predicts the amount of product formed.<br />
• The other reactants are said to be in excess, meaning there is more than enough of it.<br />
• The key to identifying a limiting reagent problem is that it will give you the amounts being<br />
reacted of more than one reactant.<br />
• Suppose you with to synthesize zinc sulfide.<br />
You combine 50. grams of zinc with 50. grams of sulfur.<br />
• What mass of zinc sulfide is predicted to be produced from the zinc<br />
• What mass of zinc sulfide is predicted to be produced from the sulfur<br />
• Which reactant is the limiting reactant<br />
What mass of zinc sulfide is produced by the reaction of 75.8 g of zinc with 60.5 g of sulfur<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
Using the Tabulation Method<br />
• The tabulation method is an alternative method for solving some stoichiometry problems<br />
• While most problems do not require using this method, it is essential for more complex<br />
problems, especially those involving equilibrium calculations<br />
• This method is most helpful when you need to know the amounts of each chemical present at<br />
the end of the reaction<br />
Use the tabulation method to solve this problem:<br />
3.0 mols of N 2(g) react with 8.0 mols of H 2(g) to produce NH 3(g) . If the reaction goes to<br />
completion (that is, until you run out of the limiting reactant), how many moles of each<br />
substance will be present in the flask at the end of the reaction<br />
Consider the hydrogenation of propene(C 3 H 6 ):<br />
C 3 H 6 + H 2 C 3 H 8<br />
78.24 g of propene is treated with 25.0 g of hydrogen.<br />
a. What mass of propane (C 3 H 8 ) is produced<br />
7
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
b. Which reactant was in excess, and what mass of it remains after the reaction is<br />
completed<br />
Percent Yield<br />
• So far, we have assumed that all reactions will produce exactly the amount of products that<br />
our calculations will predict.<br />
• The theoretical yield is the amount of a product you expect to get at the end of a reaction.<br />
• In reality, we never actually get 100% of this amount.<br />
◦ Why might this be so<br />
• The amount of a product that is really produced at the end of a reaction is called the actual<br />
yield.<br />
• The percent yield gives us an idea of how much of a product we actually produced compared<br />
to the amount that should have been produced.<br />
actual yield<br />
% yield =<br />
× 100%<br />
theoretical yield<br />
• In general, the closer the percent yield is to 100% percent, the better the reaction<br />
Example<br />
• 8.0 g of hydrogen is combined with excess oxygen, producing 58.5 g of water. What is the<br />
percent yield of this reaction<br />
8
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
Example<br />
Suppose that you wish to produce 15.00 grams of barium sulfate by reacting excess sulfuric acid<br />
with barium hydroxide. If this reaction is known to usually give an 87.5% yield, how many<br />
grams of barium hydroxide should you use<br />
Stoichiometry and Net Ionic Equations<br />
• It is often more practical to use net ionic equations in stoichiometry calculations, especially for<br />
problems dealing with solutions<br />
• There is no significant difference in solving problems using these equations than with the<br />
methods used so far<br />
9
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Nine <strong>Notes</strong><br />
Example<br />
12.0 grams of strontium chloride is dissolved in approximately 500 mL of water. To this is added<br />
5.00 grams of silver nitrate. Determine<br />
a. The total ionic equation and net ionic equation describing this process.<br />
b. The mass of solid precipitate theoretically produced, and<br />
c. The moles of each ion remaining in solution at the end of the reaction.<br />
10
<strong>Chemistry</strong> <strong>120</strong><br />
Molarity <strong>Notes</strong><br />
Molarity<br />
Concentration and Molarity<br />
• The concentration of a solution is a measurement of how much of a solute it contains (the<br />
solute is the substance dissolved within it.)<br />
• The most useful term for concentration relates the number of moles of solute in a liter of<br />
solution; it is called the molarity, and abbreviated “M”:<br />
mol solute<br />
molarity(M ) =<br />
L solution<br />
• We often use square brackets around a compound or ion to indicate molarity<br />
• For example [Na + ] means “molarity of sodium ion”<br />
• For example, to prepare a 1.0 M NaCl solution, we take 1.0 mol of NaCl (58.44 g) and add<br />
enough water to it to bring the total volume of the solution to 1.0 L.<br />
• We cannot simply say “add 1.0 L of water,” because the presence of the salt will effect the<br />
final volume of the solution.<br />
Example<br />
Explain how to prepare 2.00 L of a 0.550 M solution of potassium chloride.<br />
Mole-Volume Problems<br />
• Since the molarity of a solution relates the volume to the number of moles of a solute, we can<br />
use it to help us calculate the amount of product formed in a reaction.<br />
• First, we must convert the volume of a solution to moles of solute, using the molarity.<br />
• From there, we can use the mole ratios of the chemical equation to figure out how much<br />
product is produced.<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Molarity <strong>Notes</strong><br />
Examples<br />
25.00 mL of a 0.45 M AgNO 3 solution is treated with excess NaCl solution. What solid precipitate<br />
is formed, and what should its mass be in grams<br />
What volume of 0.224 M Ba(OH) 2 solution is required to completely neutralize 15.00 mL of a<br />
0.855 M HNO 3 solution<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Molarity <strong>Notes</strong><br />
25.00 mL of a 0.425 M potassium iodide solution is added to about 90 mL of water. To this is<br />
added 25.00 mL of a 0.724 M lead(II) nitrate solution. What precipitate is formed, and what is<br />
its mass<br />
Millimoles<br />
• Since we often carry out volume measurements in the lab in milliliters, it is often convenient to<br />
use millimoles (mmol) rather than moles in calculations<br />
• A millimole is defined in the same way other metric units are<br />
◦ 1 mmol = 10 -3 mol, or equivalently<br />
◦ 1000 mmol = 1 mol<br />
• We can define molarity as<br />
mol solute mmol solute<br />
molarity(M ) =<br />
=<br />
L solution mL solution<br />
and use the form which is most convenient<br />
Example<br />
Let’s redo an earlier problem, using millimoles instead of moles in the calculation:<br />
What volume of 0.224 M Ba(OH) 2 solution is required to completely neutralize 15.00 mL of a<br />
0.855 M HNO 3 solution<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Molarity <strong>Notes</strong><br />
Titrations<br />
• A titration is usually carried out to determine the molarity of an unknown solution.<br />
• A specific amount of a compound whose concentration is well known, called the primary<br />
standard is measured out.<br />
• An indicator, a compound with a different color under different chemical environments, is<br />
added to the primary standard.<br />
• The unknown solution is added until the indicator changes color, signaling the end of the<br />
titration (called the end point).<br />
• From the collected data it is possible to determine the molarity of the unknown solution.<br />
• At the end point, we assume that there are “equivalent” amounts of each chemical present<br />
◦ This is not precisely true, but this definition is adequate for now<br />
• By equivalent, we mean that the ratio of the moles of each reactant added equals the ratio in<br />
the balanced equation<br />
Examples<br />
HCl + NaOH H 2 O + NaCl<br />
Ratio of acid to base: 1 to 1, so we need 1<br />
equivalent of acid for every 1<br />
equivalent of base<br />
H 2 SO 4 + 2 NaOH 2 H 2 O + Na 2 SO 4<br />
Ratio of acid to base: 1 to 2, so we need 1 equivalent of acid for every 2<br />
equivalents of base<br />
Examples<br />
10.00 mL of an HCl solution is pipetted into a beaker containing about 25 mL of deionized water.<br />
This solution is then titrated with 0.4575 M NaOH. It is found that 17.85 mL of base is<br />
required to reach the end point. What is the molarity of the acid solution<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Molarity <strong>Notes</strong><br />
4.2554 grams of solid oxalic acid (H 2 C 2 O 4 ) is dissolved in about 50 mL of deionized water. It is<br />
found that 37.55 mL of a KOH solution is required to titrate this acid to the end point. What is<br />
the concentration of the base solution<br />
Ion Concentration<br />
• For many chemical calculations, it is essential that we know the concentration of each ion in<br />
the solution<br />
• For example, consider a 1.00 M CuCl 2 solution<br />
• What is the molarity of Cu 2+ in this solution<br />
• What is the molarity of Cl - <br />
Examples<br />
10.00 mL of 2.45 M NaCl solution is combined with 10.00 mL of 1.50 M BaCl 2 solution. What is<br />
the concentration of each ion in solution after the two have been combined<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Molarity <strong>Notes</strong><br />
How could we prepare 500. mL of a solution with [Ni 2+ ] = 0.100 M We will use nickel (II) nitrate<br />
as the source of the nickel ion. (Why is it not possible to add only Ni 2+ ion to the solution<br />
without adding any other ion)<br />
15.00 mL of a 0.1555 M HCl solution is combined with 10.00 mL of a 0.1250 M Sr(OH) 2 solution.<br />
What is the concentration of each ion in solution after the reaction has occured<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Chapter Twelve: Gases<br />
Pressure<br />
• An important parameter which must be taken into account when studying gases is pressure.<br />
• Pressure is the amount of force applied to an area:<br />
force<br />
pressure =<br />
area<br />
• Consider laying on a bed of nails. Do you want there to be many nails or few nails in the<br />
bed<br />
Pressures of Gases<br />
• The pressure exerted by a gas in a sealed container results from collisions of many individual<br />
gas particles with the walls of its container.<br />
◦ When we say a gas is at high pressure, its individual particles are colliding frequently with<br />
the sides of its container.<br />
• Later we will see that many other parameters can have an effect on the pressure of a gas<br />
sample, such as the volume of the enclosing container.<br />
Air Pressure<br />
• The air in the atmosphere exerts a substantial amount of pressure on everything on the<br />
surface of the earth.<br />
• Since air is composed of matter (nitrogen, oxygen, etc.), it has mass.<br />
• Air reaches up to at least 20 miles above the surface of Earth.<br />
• The weight of the air pushes down on everything on the surface, including us.<br />
• In a similar fashion, the weight of ocean water exerts tremendous pressures at the lower<br />
depths of the oceans.<br />
Measuring Pressure<br />
• A device used for measuring pressure is called a manometer; a device specifically designed<br />
to measure air pressure is called a barometer.<br />
• To build a simple barometer, we completely fill a thin cylinder with mercury<br />
◦ Mercury is very dense and is therefore ideal for this application<br />
• Then, we partially fill a deep dish with mercury and invert the mercury tube in this pool of<br />
mercury.<br />
• Some of the mercury will descend out of the tube as gravity pulls it down.<br />
• However, some of the mercury will stay in the tube, as the air pressure keeps this mercury<br />
supported.<br />
◦ The weight of the air on the surface of the mercury pool opposes the force of gravity as it<br />
tries to pull the mercury down out of the column.<br />
• On an “average” day, the height of the mercury column will be close to 760 mm.<br />
• What would the height of the column be on average at a higher altitude: greater than 760<br />
mm, or less<br />
• The “standard” air pressure is set at this value of 760 mm, as we shall shortly see.<br />
1
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Measuring Pressure<br />
• Measuring the pressure of the gas in a container involves a similar principal.<br />
• One method of measuring this pressure involves attaching the sample to a manometer, which<br />
has a U-shaped tube partially filled with mercury.<br />
• The gas exerts pressure on its side of the U-tube, and the atmosphere exerts pressure on the<br />
other open end.<br />
• The difference in the heights of the columns can tell use the difference in the pressures of the<br />
gases.<br />
• The side of the U-tube with the lower height indicates that that side is at a higher pressure,<br />
since it is ultimately pushing back the force of the other gas.<br />
• To determine the pressure of the gas, the difference in the height is measured and<br />
◦ added to the atmospheric pressure value if the height is lower on the gas sample side.<br />
◦ subtracted from the atmospheric pressure value if the height is higher on the gas sample<br />
side.<br />
Units of Pressure<br />
• Unfortunately, many different units are used to measure pressure.<br />
• The units we will employ most often include<br />
◦ Atmospheres (atm)<br />
• Though not the SI unit of pressure, this is a very common unit. The value of the air<br />
pressure at sea level on an average day is close to 1 atm.<br />
◦ Millimeters of Mercury (mm Hg)<br />
• This unit is derived from the way one takes a measurement with a barometer or<br />
manometer. Recall that on an average day, the height of a mercury column in a<br />
barometer is about 760 mm Hg.<br />
• 1 atm = 760 mm Hg (approximately, though treat this as exact).<br />
◦ Torr (torr)<br />
• This unit is essentially the same as the mm Hg, so<br />
1 atm = 760 torr (exactly).<br />
• You must know these units and conversions.<br />
• Other units of pressure you may encounter, but need not memorize the conversion for,<br />
include<br />
◦ Pascals (Pa) (the SI unit of pressure) and kilopascals (kPa)<br />
◦ Pounds per square inch (psi)<br />
◦ Bars (bar) and millibars (mbar)<br />
1 atm = 101,325 Pa = 14.7 psi = 1013 mbar<br />
2
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Kinetic-Molecular Theory<br />
• Recall that our only previous description of gases stated that gases completely fill and take<br />
the shape of their containers.<br />
• The Kinetic-Molecular Theory goes much farther in describing how gases ideally behave.<br />
• There are five principle statements that comprise it, which should be understood thoroughly<br />
as well as memorized.<br />
◦ Note that some textbooks give slight modifications of these<br />
The Statements of the Kinetic-Molecular Theory<br />
• The particles of a gas are so small compared to the distances between them that the volume<br />
of the individual gas particles is considered negligible (zero).<br />
• Gas particles are in constant, rapid, and random motion.<br />
• Gas particles exert neither attractive nor repulsive forces on each other.<br />
• The average kinetic energy of a collection of gas particles is directly proportional to the<br />
temperature (in Kelvin) of the gas.<br />
◦ From this we can state that all gases at the same temperature have the same average<br />
kinetic energy.<br />
• Collisions between gas particles are perfectly elastic<br />
◦ By this, we mean that the gas molecules do not lose energy when they collide<br />
The Gas Laws<br />
• In considering gases, there are three important measured values which we will often<br />
consider.<br />
◦ Pressure (P)<br />
◦ Volume (V)<br />
◦ Temperature (T)<br />
• Note that the units of temperature will always be expressed in Kelvin in the gas laws.<br />
• The gas laws describe the mathematical relationship between these parameters<br />
Boyle’s Law<br />
• Suppose we have a gas in a sealed piston (a container whose volume can change), and we<br />
know its pressure, volume, and temperature.<br />
• Keeping the temperature the same, we decrease the volume of the container.<br />
• What will happen to the pressure<br />
◦ Hint: Will the gas molecules collide with the sides of the container more or less<br />
frequently<br />
• Pressure and volume are inversely proportional.<br />
◦ That is, if one increases, the other must decrease.<br />
◦ Remember that the temperature must remain constant for this to be true.<br />
• We can use this fact to derive Boyle’s Law:<br />
P 1 V 1 = P 2 V 2 (at constant T)<br />
where the 1 stands for the beginning values and the 2 the final values.<br />
• Derivation:<br />
3
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Example<br />
A gas occupies 29.5 L, and exerts a pressure of 640. mm Hg. If the container’s volume is<br />
expanded to 40.0 L (keeping the temperature constant), what will be the pressure of the gas<br />
in mm Hg and in atm<br />
Charles’ Law<br />
• Suppose we have a gas in an expandable container, and, without changing its pressure, we<br />
raise its temperature.<br />
• How will the behavior of the gas molecules change<br />
• In order to keep the pressure constant, what will happen to the volume of the gas<br />
• Volume and temperature are directly proportional.<br />
◦ That is, if one increases the other increases.<br />
◦ Pressure must remain constant for the process.<br />
• Mathematically, this is stated as<br />
V<br />
1 =<br />
T<br />
1<br />
V<br />
T<br />
2<br />
2<br />
(constant P)<br />
Example<br />
A gas occupies 35.8 L at 1.13 atm and 42.3 °C. What would be the temperature of this gas, in<br />
Celcius, if the volume were decreased to 25.0 L and the pressure was left unchanged<br />
4
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Gay-Lussac’s Law<br />
• Suppose a gas is kept in a rigid container whose volume cannot change.<br />
• If the gas is heated, how will the pressure be effected<br />
• Pressure and temperature are directly proportional, assuming the volume remains<br />
unchanged. Mathematically, this is stated:<br />
T<br />
1<br />
1<br />
P<br />
T<br />
2<br />
2<br />
(constant V)<br />
P =<br />
2<br />
The Combined Gas Law<br />
• The three previous laws can all be combined into one convenient form, the combined gas<br />
law.<br />
P1<br />
V<br />
T<br />
1<br />
1<br />
P2<br />
V<br />
=<br />
T<br />
2<br />
• You may use this law in place of the other three if you wish, since the constant values will<br />
always divide out.<br />
Example<br />
72.6 L of a gas at 35.7 °C and 0.872 atm is heated to 50.0 °C and allowed to expand to 87.5 L.<br />
What is the pressure of the gas under these new conditions<br />
Avogadro’s Hypothesis<br />
• Amadeo Avogadro is credited with stating one of the most fundamental statements describing<br />
gases:<br />
“Equal amounts (moles) of gases occupy equal volumes under the same conditions”<br />
• This greatly simplifies our treatment of gases, as we can conclude that, regardless of what<br />
composes the gas, if we know how many moles of it we have and its conditions, we can find<br />
its volume.<br />
5
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Avogadro’s Law<br />
• Mathematically we can use Avogadro’s hypothesis to derive the mathematical relationship<br />
V<br />
1 =<br />
n1<br />
V<br />
n<br />
2<br />
2<br />
(constant P, T)<br />
• n is the number of moles of the gas, regardless of what the gas actually is.<br />
The Ideal Gas Law<br />
• All the previous laws allow us to compare a gas under one set of conditions with its values<br />
under other conditions.<br />
• The Ideal Gas Law summarizes the previous laws in a fundamentally different way: its power<br />
is that it shows how the four parameters (P, V, T, and n) can be used to determine one<br />
another.<br />
• The Ideal Gas Law is, mathematically,<br />
PV = nRT<br />
where R is a constant, called the universal gas constant.<br />
L ⋅atm<br />
R = 0.0821<br />
mol⋅K<br />
• If you know any three parameters from the ideal gas law, the fourth can be determined by<br />
substitution into this equation.<br />
Examples<br />
What volume is one mole of a gas expected to occupy at exactly 1 atm and exactly 0 °C<br />
Note: These pressures and temperatures are called STP (standard temperature and<br />
pressure).<br />
If a balloon containing methane has a volume of 7.25 L at 754 mm Hg and 296.4 K, then how<br />
many moles of methane does the balloon contain How many grams is this<br />
6
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
A 1.45 g piece of dry ice (solid CO 2 ) is put in a balloon and warmed to 298 K, causing all the CO 2<br />
to sublimate (turn to gas). The volume of the balloon after the sublimation is completed is<br />
measured to be 3.29 L. What is the pressure exerted by the gas inside the balloon<br />
What is the density of pure carbon dioxide gas at 1.05 atm and 300.0 K Report your answer in<br />
grams per liter.<br />
Dalton’s Law of Partial Pressures<br />
• In a mixture of gases (like air) each substance in the mixture exerts its own indivual pressure,<br />
called the partial pressure of that gas.<br />
• The total pressure of the mixture of these gases is simply the sum of these partial pressures.<br />
◦ So, air pressure is derived from the partial pressures of all the gases making up the air,<br />
including N 2 , O 2 , Ar, H 2 O, CO 2 , and others.<br />
• Mathematically, this is stated as<br />
P total = P gas a + P gas b + P gas c + …<br />
◦ There are as many terms on the right side of the equation as there are gases in the<br />
mixture.<br />
7
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Example<br />
Argon, neon, and helium gases are all combined in a 40.0 L container. The total pressure of the<br />
three gases is measured to be 1.45 atm. Argon and neon each exert a partial pressure of<br />
0.65 atm. What is the partial pressure of helium in this mixture<br />
Collecting a Gas Over Water<br />
• One common way to collect a gas produced by an experiment is over water.<br />
• From the reaction vessel, the gas enters a hose which leads to a container filled with water.<br />
• The gas then bubbles up through the water into a tube filled with water that penetrates the<br />
waters surface.<br />
• The gas displaces the water in the tube, and is collected there.<br />
• However the gas is “wet”, meaning it contains some water vapor.<br />
• To find the pressure of the “dry” (i.e. without water) sample, we must subtract out the<br />
pressure of the water vapor mixed with it.<br />
◦ The pressure exerted by the water pressure can be found in a table, so long as we know<br />
the temperature of the water.<br />
• If the level of the water in the tube is the same as the level of the water in the container the<br />
tube is in, the following relationship exists:<br />
P air = P gas + P water vapor<br />
Example<br />
A sample of argon is collected over water at 23 °C. After collecting the gas, the height of the gas<br />
in the collecting tube is lowered to that of the water container. According to a barometer, the<br />
air pressure is 763 mm Hg. What is the pressure exerted by argon in atmospheres<br />
8
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
Gas Stoichiometry<br />
• The Ideal Gas Law aids us in predicting the quantity relationships when reactants or products<br />
are gases.<br />
• An important value to keep in mind is that 1 mole of a gas at STP will occupy 22.4 liters.<br />
• We will use the Ideal Gas Law for similar calculations under different conditions.<br />
Examples<br />
54.8 L of hydrogen gas is combined with excess oxygen at STP. What mass of water should be<br />
produced<br />
72.9 L of hydrogen (at STP) is reacted with 28.0 L of nitrogen (at STP), producing ammonia.<br />
What volume will the ammonia produced occupy at 1.25 atm and 325 K<br />
9
<strong>Chemistry</strong> <strong>120</strong><br />
Chapter Twelve <strong>Notes</strong><br />
65.0 grams of nitrogen gas and 15.0 grams of hydrogen gas are combined in a 10.0 L container.<br />
The gases react, producing ammonia gas. Assume that the reaction goes to completion.<br />
a. What is the partial pressure of each gas in the container at the end of the reaction,<br />
assuming the total pressure in the container is 2.50 atm<br />
b. What is the temperature of the gas sample in the flask under the conditions in part a<br />
c. Suppose that all the ammonia produced in this reaction is dissolved into water to make 555<br />
mL of solution. How many milliliters of 3.00 M H 2 SO 4 solution would be required to<br />
completely neutralize the ammonia solution<br />
10