Exam 10: Dynamics of Rotational Motion
Exam 2: Motion Along a Straight Line55 Questions
Exam 3: Motion in Two or Three Dimensions59 Questions
Exam 4: Newtons Laws of Motion50 Questions
Exam 5: Applying Newtons Laws139 Questions
Exam 6: Work and Kinetic Energy109 Questions
Exam 7: Potential Energy and Energy Conservation50 Questions
Exam 8: Momentum, Impulse, and Collisions99 Questions
Exam 9: Rotation of Rigid Bodies26 Questions
Exam 10: Dynamics of Rotational Motion49 Questions
Exam 11: Equilibrium and Elasticity50 Questions
Exam 12: Fluid Mechanics54 Questions
Exam 13: Gravitation52 Questions
Exam 14: Periodic Motion109 Questions
Exam 15: Mechanical Waves50 Questions
Exam 16: Sound and Hearing121 Questions
Exam 17: Temperature and Heat60 Questions
Exam 18: Thermal Properties of Matter41 Questions
Exam 19: The First Law of Thermodynamics55 Questions
Exam 20: The Second Law of Thermodynamics52 Questions
Exam 21: Electric Charge and Electric Field54 Questions
Exam 22: Gausss Law54 Questions
Exam 23: Electric Potential88 Questions
Exam 24: Capacitance and Dielectrics70 Questions
Exam 25: Current, Resistance, and Electromotive Force44 Questions
Exam 26: Direct-Current Circuits51 Questions
Exam 27: Magnetic Field and Magnetic Forces105 Questions
Exam 28: Sources of Magnetic Field82 Questions
Exam 29: Electromagnetic Induction51 Questions
Exam 30: Inductance88 Questions
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Exam 32: Electromagnetic Waves Optics53 Questions
Exam 33: The Nature and Propagation of Light31 Questions
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Exam 35: Interference59 Questions
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Escape speed: A satellite is in circular orbit at an altitude of 1500 km above the surface of a nonrotating planet with an orbital speed of 9.2 km/s. The minimum speed needed to escape from the surface of the planet is 14.9 km/s, and G = 6.67 × 10-11 N ∙ m2/kg2. The orbital period of the satellite is closest to
(Multiple Choice)
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Gravitational potential energy: Sputnik I was launched into orbit around Earth in 1957. It had a perigee (the closest approach to Earth, measured from Earth's center) of 6.81 × 106 m and an apogee (the furthest point from Earth's center) of 7.53 × 106 m. What was its speed when it was at its perigee? The mass of Earth is 5.97 × 1024 kg and G = 6.67 × 10-11 N ∙ m2/kg2.
(Multiple Choice)
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Gravitational force: A small-sized 155-kg mass is located 1.50 m from a small-sized 275-kg mass, with both masses fixed in place. Where should you place a third small-sized mass so that the net gravitational force on it due to the original two masses is zero?
(Essay)
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Weight and g: The weight of spaceman Speff at the surface of planet X, solely due to its gravitational pull, is 389 N. If he moves to a distance of 1.86 × 104 km above the planet's surface, his weight changes to 24.31 N. What is the mass of planet X, if Speff's mass is 75.0 kg? (G = 6.67 × 10-11 N ∙ m2/kg2)
(Multiple Choice)
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Weight and g: From what height above the surface of the earth should an object be dropped to initially experience an acceleration of 0.9200g? The radius of the earth is 6.38 × 106 m.
(Multiple Choice)
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Kepler's laws: Two moons orbit a planet in nearly circular orbits. Moon A has orbital radius r, and moon B has orbital radius 4r. Moon A takes 20 days to complete one orbit. How long does it take moon B to complete an orbit?
(Multiple Choice)
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Gravitational potential energy: Beings on spherical asteroid Π have observed that a large rock is approaching their asteroid in a collision course. At
from the center of the asteroid, the rock has a speed of
and later at
it has a speed of
Use energy conservation to find the mass of asteroid Π. You can neglect any effects due to the parent star of the asteroid. (G = 6.67 × 10-11 N ∙ m2/kg2)




(Multiple Choice)
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Satellites: What is the period (in hours) of a satellite circling Mars 100 km above the planet's surface? The mass of Mars is 6.42 × 1023 kg, its radius is 3.40 × 106 m, and G = 6.67 × 10-11 N ∙ m2/kg2.
(Multiple Choice)
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Satellites: You are the science officer on a visit to a distant solar system. Prior to landing on a planet you measure its diameter to be 1.8 × 107 m and its rotation period to be 22.3 hours. You have previously determined that the planet orbits 1.8 × 1011 m from its star with a period of 402 earth days. Once on the surface you find that the acceleration due to gravity is 59.7 m/s2. What are the mass of (a) the planet and (b) the star? (G = 6.67 × 10-11 N ∙ m2/kg2.)
(Multiple Choice)
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Weight and g: Ekapluto is an unknown planet that has two spherical moons in circular orbits. The table summarizes the hypothetical data about the moons. Both moons have low axial spin rates. (G = 6.67 × 10-11 N ∙ m2/kg2)
The acceleration due to gravity at the surface of Moon B is

(Multiple Choice)
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Escape speed: A certain planet has an escape speed V. If another planet has twice size and twice the mass of the first planet, its escape speed will be
(Multiple Choice)
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Gravitational potential energy: Two planets having equal masses are in circular orbit around a star. Planet A has a smaller orbital radius than planet B. Which statement is true?
(Multiple Choice)
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Escape speed: A certain spherical asteroid has a mass of 3.5 × 1016 kg and a radius of 8.8 km. What is the minimum speed needed to escape from the surface of this asteroid? (G = 6.67 × 10-11 N ∙ m2/kg2)
(Multiple Choice)
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Weight and g: The gravitational acceleration on a planet's surface is 16.0 m/s2. What is the gravitational acceleration at an altitude of one planet diameter above the SURFACE of the planet?
(Multiple Choice)
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Gravitational force: A baseball is located at the surface of the earth. Which statements about it are correct? (There may be more than one correct choice.)
(Multiple Choice)
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Satellites: A man-made satellite of mass 6105 kg is in orbit around the earth, making one revolution in 430 minutes. What is the magnitude of the gravitational force exerted on the satellite by the earth? (The mass of the earth is 6.0 × 1024 kg and G = 6.67 × 10-11 N ∙ m2/kg2)
(Short Answer)
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Gravitational force: Three identical very small 50-kg masses are held at the corners of an equilateral triangle, 0.30 m on each side. If one of the masses is released, what is its initial acceleration if the only forces acting on it are the gravitational forces due to the other two masses? (G = 6.67 × 10-11 N ∙ m2/kg2)
(Multiple Choice)
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Kepler's laws: Neptune circles the Sun at a distance of 4.50 × 1012 m once every 164 years. Saturn circles the Sun at a distance of 1.43 × 1012 m. What is the orbital period of Saturn?
(Multiple Choice)
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Satellites: Ekapluto is an unknown planet that has two moons in circular orbits. The table summarizes the hypothetical data about the moons. (G = 6.67 × 10-11 N ∙ m2/kg2)
The mass of Ekapluto is closest to

(Multiple Choice)
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Kepler's laws: A planet has two small satellites in circular orbits around the planet. The first satellite has a period 18.0 hours and an orbital radius 2.00 × 107 m. The second planet has an orbital radius 3.00 × 107 m. What is the period of the second satellite?
(Multiple Choice)
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