Chapter 2: The Copernican Revolution: The Birth of Modern Science Review Sheet Flashcards

1
Q

The principal culture that transferred Greek astronomical knowledge to Renaissance Europe was:

A

Islamic

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2
Q

The most accurate Greek attempt to explain planetary motion was the model of:

A

Ptolemy

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3
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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4
Q

The greatest contribution of the Greeks to modern thought was:

A

the development of scientific inquiry and model building

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5
Q

On which of these assumptions do Ptolemy and Copernicus agree?

A

All orbits must be perfect circles

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6
Q

The heliocentric model was actually first proposed by:

A

Aristarchus

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7
Q

According to Copernicus, the retrograde motion for Mars must occur:

A

At opposition, when the Earth overtakes Mars and passes between Mars and the Sun.

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8
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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9
Q

Which of these was NOT seen telescopically by Galileo?

A

Stellar parallax

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10
Q

Which of the following is a contribution to astronomy made by Galileo?

A

All of the above

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11
Q

Which of these observations of Galileo refuted Ptolemy’s epicycles?

A

The complete cycle of Venus’ phases

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12
Q

A fatal flaw with Ptolemy’s model is its inability to predict the observed phases of:

A

Mercury and Venus

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13
Q

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

A

elliptical, not circular

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14
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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15
Q

The most famous prehistoric astronomical observatory is:

A

Stonehenge

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16
Q

What contribution to astronomy was made by Tycho Brahe?

A

His observations of planetary motion with great accuracy proved circular orbits could not work

17
Q

According to Kepler’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.

18
Q

What does Kepler’s third law imply about planetary motion?

A

Planets further from the Sun orbit at a slower speed than planets closer to the Sun

19
Q

Today we rely largely on what technique to precisely measure distances in the solar system?

A

Radar echo timings

20
Q

The Law of Universal Gravitation was developed by

A

Newton

21
Q

The force of gravity between two objects:

A

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

22
Q

Which of these was a contribution of Newton to astronomy?

A

All of these were due to Newton’s work

23
Q

Kepler’s second law implies what about planetary motion?

A

A planet moves faster when it is closer to the Sun

24
Q

SHORT ANSWER: What did Galileo discover about Jupiter that supported Copernicus?

A

Its four moons were a model solar system, orbiting a larger central body just as the smaller planets orbit the Sun

25
Q

Explain how Kepler’s laws allow us to use the motion of an asteroid to find its average distance from the Sun

A

By watching it long enough to find its period of revolution around the Sun, we can use Kepler’s third law to get the average distance by squaring the period in years, then finding the cube root of this value for the average distance of the asteroid from the Sun in astronomical units.