Exam 5: Gravity

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One of the first tests of the general theory of relativity was the ____.

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The circular velocity of a satellite orbiting Earth is given by ve=GMrv _ { e } = \sqrt { \frac { G M } { r } } .  In this equation, M represents the ____.

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According to Aristotle, an object with no forces acting on it will ____.

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Describe two experiments that provide evidence of space-time curvature by the presence of a mass.

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According to Aristotle, which scenario illustrates violent motion?

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The radius of Earth is 6,378 km. The force of gravity on a 1 kg ball at Earth's surface is 9.8 kg m/s2.  What is the force of gravity on this same ball when the ball is located 12,756 km from Earth's center? Hint: G = 6.67  10-11 m3/s2/kg

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Newton's first law of motion was very similar to descriptions of motion proposed by _______________.

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The second postulate of special relativity states that the speed of light, when measured in a vacuum, is constant for all observers.

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The escape velocity at a given distance from a planet is less than the circular velocity of an orbit around that planet at the same distance.

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The M oon pulls more strongly on Earth's near and far side than on its center.

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Gravity obeys the inverse square law, which implies that the gravitational force of one body on another will be ____ times stronger at two meters than at six meters apart.

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When two objects of unequal mass orbit each other, the center of mass is ____.

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How can tidal forces affect the rotation of celestial bodies and their orbital motion?

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Newtonian gravity is often called universal mutual gravitation because every particle with mass in the Universe must attract every other particle.

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The equivalence principle can be best illustrated by ____.

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A comet near the Sun whose orbit is ____ would never be near the Sun again.

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