Chapter #3 Flashcards

1
Q

Which was a contribution to astronomy made by Copernicus?

A

He laid out the order and relative motion of the known solar system

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2
Q

Which of these was NOT a part of the original Copernican model?

A

Mercury speeds up at perihrlion, and slows down at aphelion

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3
Q

Kepler’s first law worked, where Copernicus’ original heliocentric model failed, because Kepler described the orbit as:

A

elliptical, not circular

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4
Q

Tycho Brahe’s contribution to Kepler’s Laws of Planetary Motion was

A

his detailed and accurate observations of the planet’s position

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5
Q

Upon which point do Copernicus and Kepler disagree?

A

the orbits of the planets are ellipses, with one focus at the Sun

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6
Q

Which concept was NOT a part of Kepler’s Laws of Planetary Motion?

A

epicycles are needed to explain the varying brightness of the planets.

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7
Q

According to Kelper’s third law, the square of the planet’s period in years is

A

proportional to the cube of its semimajor axis in A.U

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8
Q

The Ptolemaic model probably persisted for all these reasons EXCEPT

A

it accounted well for Galileo’s observations of the phase cycle of Venus.

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9
Q

A planet whose distance from the Sun is 3 A.U. would have an orbital period of how many Earth-years?

A

square root of 27

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10
Q

The place in a planet’s orbit that is closer to the Sun is called

A

perihelion

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11
Q

The Law of Universal Gravitation was developed by

A

Newton

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12
Q

The force of gravity between two objects

A

increase with the masses of the bodies, but decreases with the square of the distances between them

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13
Q

According to Newton’s Law of Universal Gravitation, if the Moon were three times further from Earth, the force by Earth on the Moon would:

A

decreases by a factor of 9

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14
Q

Which of these was a contribution of Newton to astronomy?

A

All of these were due to Newton’s work

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15
Q

How does Newton’s Universal Law of Gravitation explain Kepler’s laws

A
  • Universal gravitation implies that the planets further from the Sun will move more slowly than the planets closer to the Sun
  • Universal gravitation implies that when a planet is closer to the Sun in its orbit, it will move faster than when it is farther from the Sun
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