PES Skill Sheets.book - Capital High School

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Skill Sheet 25.3: Refraction Part 1 answers: 1. The index of refraction will never be less than one because that would require the speed of light in a material to be faster than the speed of light in a vacuum. Nothing in the universe travels faster than that. 2. The index of refraction for air is less than that of glass because a gas like air is so much less dense than a solid like glass. The light rays are slowed each time they bump into an atom or molecule because they are absorbed and re-emitted by the particle. A light ray in a solid bumps into many more particles than a light ray traveling through a gas. 3. water: 2.26 × 10 8 ; glass: 2.0 × 10 8 ; diamond; 1.24 × 10 8 4. speed up Skill Sheet 25.3: Drawing Ray Diagrams 1. Diagram: The image is inverted as compared with the object. Skill Sheet 26.1: Astronomical Units 1. 9.53 AU 2. 0.72 AU 3. 58 million kilometers 4. 2.87 billion kilometers 5. Less. The moon is not nearly as far from Earth as the Sun. Page 53 of 57 5. slow down Part 2 answers: 1. The light ray is moving from low-n to high-n so it will bend toward the normal. 2. The light ray is moving from high-n to low-n so it will bend away from the normal. 3. The difference in n from diamond to water is 1.09 while the difference from sapphire to air is 0.770. The ray traveling from diamond to water experiences the greater change in n so it would bend more. 4. From left to right, material B is water, emerald, helium, cubic zirconia. 2. Diagram: 3. A lens acts like a magnifying glass if an object is placed to the left of a converging lens at a distance less than the focal length. The lens bends the rays so that they appear to be coming from a larger, more distant object than the real object. These rays you see form a virtual image. The image is virtual because the rays appear to come from an image, but don’t actually meet. 6. Uranus 7. Mercury 8. Saturn 9. Saturn 10. yes Skill Sheet 26.1: Gravity Problems Table 1 answers: 1. 9.5 pounds on Neptune Planet Force of gravity in Value compared to 2. 1,029 newtons on Saturn Newtons (N) Earth’s gravity 3. The baby weighs 44.1 Newtons on Earth which is equal to 9.8 Mercury Venus Earth 3.7 8.9 9.8 0.38 0.91 1 pounds. 4. Venus, Jupiter, Neptune, Pluto, then Saturn 5. Answer: Mars Jupiter Saturn 3.7 23.1 9.0 0.38 2.36 0.92 −11 2 24 26 ⎛6.67× 10 Nm i ⎞(6.4× 10 )(5.7× 10 ) Gravity = ⎜ 2 ⎟ 11 2 ⎝ kg ⎠ (6.52× 10 ) Uranus 8.7 0.89 17 = 5.72× 10 N Neptune 11.0 1.12 Pluto 0.6 0.06 Skill Sheet 26.1: Universal Gravitation 1. F =9.34× 10 –6 N. This is basically the force between you and your car when you are at the door. 2. 5.28 × 10 -10 N 3. 4.42 N 4. 7.33 × 10 22 kilograms 5. Answers are: a. 9.8 N/kg = 9.8 kg-m/sec 2 -kg = 9.8 m/sec 2 b. Acceleration due to the force of gravity of Earth. c. Earth’s mass and radius. 6. 1.99 ×10 20 N 7. 4,848 N 8. 3.52 × 10 22 N
Skill Sheet 26.1: Nicolaus Copernicus 1. Because he was from a privileged family, young Copernicus had the luxury of learning about art, literature, and science. When Copernicus was only 10 years old, his father died. Copernicus went to live his uncle who was generous with his money and provided Copernicus with an education from the best universities. Copernicus lived during the height of the Renaissance period when men from a higher social class were expected to receive well-rounded educations. 2. Copernicus’ uncle, Lucas Watzenrode, was a prominent Catholic Church official who became bishop of Varmia in 1489. After Copernicus finished four years of study at the University of Krakow, Watzenrode appointed Copernicus a church administrator. Copernicus used his church wages to help pay for additional education. While studying at the University of Bologna, Copernicus’ passion for astronomy grew under the influence of his mathematics professor, Domenico Maria de Novara. Copernicus lived in his professor’s home where they spent hours discussing astronomy. 3. Copernicus examined the sky from a tower in his uncle’s palace. He made his observations without any equipment. 4. Prior to the 1500s, most astronomers believed that Earth was motionless and the center of the universe. They also thought that all celestial bodies moved around Earth in complicated patterns. The Greek astronomer Ptolomy proposed this geocentric theory more than 1000 years earlier. Skill Sheet 26.1: Galileo Galilei 1. “On Motion” described how a pendulum’s long and short swings take the same amount of time. 2. Galileo’s many inventions include the thermometer, water pump, military compass, microscope, telescope, and pendulum clock. Information and illustrations of the inventions can be found using the Internet or library. 3. Galileo observed the motion of Jupiter’s moons and realized that despite what Ptolemy said, heavenly bodies do not revolve exclusively around Earth. He also realized that his observation of the phases of Venus showed that Venus was revolving around the sun, not around Earth. Galileo therefore Skill Sheet 26.1: Johannes Kepler 1. Copernicus’ idea that the sun was at the center of the solar system was revolutionary because people believed Earth was the center of the universe. 2. Brahe helped Kepler make his important discoveries in several ways. Brahe invited Kepler to come and work with him. He asked Kepler to solve the problem of Mars’ orbit. When Brahe died, Kepler gained all of his observational records. Kepler also got Brahe’s job. 3. Kepler used mathematics to solve problems in astronomy. For this reason, Kepler is considered a theoretical positional astronomer. Brahe was an observational astronomer. He made and recorded the motion of planets and the stars in the night sky without a telescope. Galileo was also an observational astronomer. He used and improved the telescope, but he was not a mathematician. 4. Kepler’s discovery that Mars traveled in an elliptical orbit was different than Copernicus’ theory which said planets traveled in circular orbits. 5. Kepler’s three laws of planetary motion are: Planets orbit the sun in an elliptical orbit with the sun in one of the foci. Page 54 of 57 5. Copernicus believed that the universe was heliocentric (suncentered), with all of the planets revolving around the sun. He explained that Earth rotates daily on its axis and revolves yearly around the sun. He also suggested that Earth wobbles like a top as it rotates. Copernicus’ theory led to a new ordering of the planets. In addition, it explained why the planets farther from the sun sometimes appear to move backward (retrograde motion), while the planets closest to the sun always seem to move in one direction. This retrograde motion is due to Earth moving faster around the sun than the planets farther away. 6. At the time, Church law held great influence over science and dictated a geocentric universe. 7. The Copernicus Satellite, or Orbiting Astronomical Observatory 3 (OAO-3) was a collaborative project of both the United States’ National Aeronautics and Space Administration (NASA) and the United Kingdom’s Science and Engineering Research Council (SERC). The satellite operated from August 1972 to February 1981. The main experiment on the satellite was a Princeton University ultraviolet (UV) telescope. An x-ray astronomy experiment created by the University College London/Mullard Space Science Laboratory was also onboard. The Copernicus Satellite gathered a series of high-resolution ultraviolet spectral scans of over 500 objects, most of them being bright stars. concluded that Copernicus’ assertion that the sun, not Earth, was at the center must be correct. 4. Answers will vary. Students might suggest that Galileo use a less abrasive approach to convince people that the Copernican view is correct. 5. Galileo’s telescope is the most likely student response, because it so profoundly changed our understanding of the solar system. However, students may choose another invention as long as they provide valid reasons for their decision. The law of areas says that planets speed up as they travel in their orbit closer to the sun and they slow down as they travel in their orbit farther away from the sun. The harmonic law says that a planet’s distance from the sun is mathematically related to the amount of time it takes the planet to revolve around the sun. 6. Three examples of a paradigm shift: Copernicus’ theory that the sun and not Earth was the center of the solar system. Kepler’s discovery that planets orbit the sun in an elliptical and not a circular path. Newton’s laws of gravitational attraction.
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Chapter and Section Chapter 1: Meas
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Chapter and Section Chapter 5: Forc
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Chapter and Section Chapter 9: Heat
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Chapter and Section Chapter 14: Cha
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Chapter and Section Chapter 18: Ear
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Chapter and Section Chapter 24: Wav
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Name: Date: 1.1 Lab Safety What can
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Name: Date: 1.1 Using Your Textbook
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Page 2 of 3 The following prefixes
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Name: Date: 1.1 Scientific Notation
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Name: Date: 1.2 Reading Strategies
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Name: Date: 1.2 Stopwatch Math What
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Name: Date: 1.2 Understanding Light
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Name: Date: 1.2 Indirect Measuremen
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Name: Date: 1.3 Dimensional Analysi
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Name: Date: Skill Builder Fractions
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Page 3 of 4 Solving fraction proble
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Name: Date: 1.3 Significant Digits
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Page 3 of 4 Follow these steps for
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Name: Date: 1.3 Study Notes This sk
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Name: Date: 1.3 Science Vocabulary
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Page 3 of 3 Using the table of pref
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Name: Date: 1.4 Creating Scatterplo
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Name: Date: 1.4 Recognizing Pattern
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Page 2 of 2 4. Measurements: List a
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Page 2 of 4 Recording valid observa
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Name: Date: 2.2 Using Computer Spre
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Name: Date: 3.1 Latitude and Longit
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Name: Date: 3.1 Map Scales Mapmaker
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Page 2 of 5 It’s time to go! 3.1
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Name: Date: 4.1 Vectors on a Map Yo
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Page 2 of 3 1. Draw a profile map o
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Name: Date: 3.3 Bathymetric Maps Im
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Page 1 of 2 3.3 Tanya Atwater Tanya
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Name: Date: 4.1 Solving Equations w
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Page 3 of 4 Use the formula V = l
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Name: Date: 4.1 Problem Solving Box
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Name: Date: 4.1 Percent Error When
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Page 3 of 3 1. The lab group conduc
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Page 2 of 3 1. A bicyclist travels
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Name: Date: 4.1 Velocity Speed and
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Name: Date: 4.2 Calculating Slope f
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Name: Date: 4.2 Analyzing Graphs of
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Name: Date: 4.2 Analyzing Graphs of
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Name: Date: 4.3 Acceleration Accele
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Name: Date: 4.3 Acceleration and Sp
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Page 3 of 3 3. Graph 3: 4. Find acc
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Page 2 of 3 Example 1: How fast wil
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Name: Date: 5.1 Ratios and Proporti
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Name: Date: 5.1 Internet Research S
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Name: Date: 5.1 Preparing a Bibliog
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Name: Date: 5.1 Mass vs. Weight Wha
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Page 2 of 2 1. A physical science t
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Page 2 of 2 How much does it weigh
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Name: Date: 5.3 Equilibrium When al
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Name: Date: 6.1 Net Force and Newto
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Page 2 of 2 Reading reflection 1. I
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Name: Date: 6.3 Applying Newton’s
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Name: Date: 6.3 Momentum Conservati
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Name: Date: 6.3 Collisions and Cons
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Name: Date: 6.3 Rate of Change of M
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Page 3 of 3 6. A 50.-g (0.050-kg) e
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Page 2 of 2 1. A machine uses an in
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Page 2 of 2 Example 3: A 500-newton
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Page 2 of 2 The relationship betwee
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Page 2 of 2 6. Use the gear ratio f
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Page 2 of 2 The three classes of le
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Page 2 of 2 3. Now, calculate the g
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Page 2 of 2 To do this calculation,
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Name: Date: 7.2 Energy Transformati
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Name: Date: 7.2 Conservation of Ene
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Page 2 of 2 Reading reflection 1. W
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Name: Date: 7.3 Power In science, w
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Name: Date: 7.3 Power in Flowing En
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Name: Date: 7.3 Efficiency and Ener
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Page 2 of 2 Reading the temperature
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Page 2 of 4 1. For each of the prob
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Page 4 of 4 1. Surface temperatures
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Page 2 of 2 The graph below shows a
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Name: Date: 9.1 Using the Heat Equa
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Name: Date: 10.1 Measuring Mass wit
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Page 3 of 3 Reading the balance cor
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Page 2 of 2 d. Explain how the disp
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Page 2 of 3 Calculating volume of a
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Name: Date: 10.1 Density The densit
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Name: Date: 10.3 Pressure in Fluids
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Name: Date: 10.3 Boyle’s Law The
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Name: Date: 10.4 Charles’s Law Ch
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Name: Date: 10.4 Archimedes 10.4 Ar
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Name: Date: 10.4 Narcís Monturiol
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Name: Date: 10.4 Archimedes’ Prin
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Name: Date: 11.1 Layers of the Atmo
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Page 2 of 2 Reading reflection 1. H
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Page 2 of 3 Using temperature data
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Page 1 of 2 11.3 Joanne Simpson 11.
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Name: Date: 11.3 Weather Maps You h
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Name: Date: 11.3 Tracking a Hurrica
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Page 3 of 4 Hurricane Andrew crosse
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Name: Date: 12.1 Structure of the A
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Name: Date: 12.1 Atoms and Isotopes
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Name: Date: 12.1 Ernest Rutherford
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Name: Date: 12.2 Electrons and Ener
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Page 2 of 2 Periodic Table Groups T
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Page 2 of 2 Using dot diagrams to r
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Page 2 of 2 13.2 Important note: If
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Page 2 of 2 Example 2: Aluminum and
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Page 2 of 2 13.2 Predict the name o
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Page 2 of 2 Using the information i
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Page 2 of 3 Conservation of atoms T
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Name: Date: 14.1 The Avogadro Numbe
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Page 3 of 4 Substance Elements in s
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Name: Date: 14.1 Formula Mass A che
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Name: Date: 14.2 Classifying Reacti
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Name: Date: 14.2 Predicting Chemica
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Name: Date: 14.2 Percent Yield You
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Name: Date: 14.4 Lise Meitner Lise
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Name: Date: 14.4 Marie and Pierre C
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Page 2 of 2 Reading reflection 1. R
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Page 2 of 2 1. The decay series for
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. Page 2 of 3 i. Switches 2, 3, and
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Name: Date: 16.1 Benjamin Franklin
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Name: Date: 16.2 Using an Electric
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Page 3 of 4 Build a series circuit
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Name: Date: 16.3 Voltage, Current,
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Page 3 of 3 Now you will have the o
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Page 2 of 2 7. How much voltage wou
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Page 2 of 2 5. Use the series circu
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Page 2 of 2 In part (d) of problems
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Page 2 of 2 Reading reflection 1. N
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Page 2 of 2 6. Repeat step 5 to for
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Page 2 of 2 4. Calculate the power
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Page 2 of 4 Determining the relativ
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Page 4 of 4 Extension—Creating cl
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Name: Date: 19.1 Earth’s Interior
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Name: Date: 19.4 Continental United
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Page 3 of 4 When a mountain is form
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Name: Date: 20.1 Averaging The most
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Page 2 of 5 Locating the epicenter
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Page 4 of 5 20.1 For each of the pr
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Name: Date: 20.2 Volcano Parts 20.2
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Name: Date: 21.2 Calculating Concen
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Name: Date: 21.2 Solubility In this
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Page 3 of 3 The influence of temper
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Page 2 of 3 Work through these exam
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Name: Date: 21.3 Calculating pH The
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Name: Date: 22.1 Groundwater and We
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Page 3 of 3 Testing the model: 1. W
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Name: Date: 24.1 Period and Frequen
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Page 2 of 2 2. Use the grids below
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Page 2 of 2 2. Use the grids below
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Page 2 of 3 x-axis (blocks) Height
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Name: Date: 24.3 Decibel Scale The
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Page 2 of 2 a. ____________________
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Page 2 of 2 2. Two students want to
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Name: Date: 24.3 Palm Pipes Project
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Page 3 of 3 6. Challenge: You can f
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Page 2 of 2 Answer the following pr
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Page 2 of 2 4. You see a chair that
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Page 2 of 2 a. ____________________
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Name: Date: 25.3 Using Ray Diagrams
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Page 2 of 2 2. Light strikes a mirr
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Page 2 of 2 Which way does the ligh
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Page 2 of 2 25.3 1. A lens has a fo
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Name: Date: 26.1 Gravity Problems I
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Name: Date: 26.1 Universal Gravitat
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Page 1 of 2 26.1 Nicolaus Copernicu
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Page 1 of 2 26.1 Galileo Galilei Ga
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Page 1 of 2 26.1 Johannes Kepler 26
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Name: Date: 26.1 Measuring the Moon
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Page 3 of 3 Semi-Circle Card: 26.1
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Page 2 of 2 Reading reflection 1. B
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Page 2 of 2 Part 2: Provisions for
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Page 1 of 2 27.1 Arthur Walker 27.1
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Name: Date: 27.2 The Inverse Square
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Page 2 of 3 1. Fill in the missing
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Name: Date: 28.1 Understanding Ligh
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Name: Date: 28.1 Parsecs You have a
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Page 1 of 2 28.1 Edwin Hubble Edwin
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Name: Date: 28.2 Light Intensity Pr
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Page 2 of 2 If we know the brightne
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Page 2 of 2 Solving Doppler Shift P
Page 443 and 444: 13. A decimeter is 100 times larger
Page 445 and 446: Skill Sheet 1.3: Significant Digits
Page 447 and 448: 7. Yes, there is a relationship bet
Page 449 and 450: 6. The slope is the same (2.0) unti
Page 451 and 452: 13. S Sh—Sand and shells on the b
Page 453 and 454: 10. 410 miles 11. 6.6 miles -------
Page 455 and 456: Skill Sheet 4.2: Analyzing Graphs o
Page 457 and 458: Skill Sheet 5.1: Mass, Weight, and
Page 459 and 460: Skill Sheet 6.3: Applying Newton’
Page 461 and 462: Skill Sheet 7.1: Mechanical Advanta
Page 463 and 464: 8. The middle gear turns left. The
Page 465 and 466: Skill Sheet 7.3: Power in Flowing E
Page 467 and 468: Skill Sheet 10.1: Calculating volum
Page 469 and 470: 3. Answers are: a. 100 cm 3 b. 13 N
Page 471 and 472: Skill Sheet 11.3: Weather Maps Samp
Page 473 and 474: a. b. c. d. e f. Skill Sheet 12.2:
Page 475 and 476: Skill Sheet 14.1: Chemical Equation
Page 477 and 478: must be blocking their insulin’s
Page 479 and 480: 8. The current is approximately the
Page 481 and 482: 7. Students can find information ab
Page 483 and 484: Skill Sheet 17.4: Electrical Power
Page 485 and 486: Skill Sheet 19.1: Charles Richter 1
Page 487 and 488: Practice 2: 1. First problem is don
Page 489 and 490: Skill Sheet 21.3: Calculating pH 1.
Page 491 and 492: Question 8 (con’t) 9. The new wav
Page 493: Skill Sheet 25.2: The Human Eye a.
Page 497 and 498: Skill Sheet 27.1: Arthur Walker 1.
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