Deck 3: Motion of Astronomical Bodies

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Question
Retrograde motion is seen when ____________ due to the Earth's motion.

A) stars change their position in the sky with respect to background stars
B) stars rise in the west and set in the east
C) planets rise in the west and set in the east
D) planets change the direction in which they wander across the night sky
E) planets orbit the Sun in the opposite direction
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Question
Kepler's third law written as P2 =A3 holds true mathematically for our Solar System only if the period is expressed in years and the semimajor axis is expressed in AU.
Question
Newton's second law says that more massive objects are accelerated more than less massive objects when the same force is applied.
Question
How did Ptolemy "fix" the geocentric system?

A) He introduced retrograde motion.
B) He introduced prograde motion.
C) He moved the Sun to the center.
D) He introduced epicycles.
E) He introduced Earth's motion.
Question
When the geocentric model of the solar system did not match the observed positions of the planets:

A) Tycho Brahe made measurements of higher accuracy and showed the geocentric model was correct
B) Ptolemy added epicycles to the geocentric model to match the observed data
C) Galileo argued that the Sun revolved around the Earth
D) Kepler was inspired to create the theory of gravity
E) Copernicus proposed the heliocentric mode
Question
Based on his observations of the planets, Copernicus calculated the relative distance of the planets from the Sun using the heliocentric model, and these distances were:

A) 10 times too large
B) exactly correct
C) close to the correct values, with errors less than 0.5 AU
D) accurate, but not as accurate as Ptolemy's values
E) two times too small
Question
An inferior planet is one that is:

A) smaller than Earth
B) larger than Earth
C) closer to the Sun than Earth
D) farther from the Sun than Earth
E) made of lighter materials than Earth
Question
In the heliocentric system, retrograde motion is not an actual motion of the planet but appears to occur because of the Earth's movement.
Question
At the center of the geocentric model of the Solar System is the:

A) Sun
B) Moon
C) Earth
D) Venus
E) Jupiter
Question
Planets with circular orbits travel at the same speed at all points in their orbits, whereas planets with elliptical orbits change their speeds at different points in their orbits.
Question
Even though they move at faster average speeds, the outer planets in the Solar System have longer periods than the inner planets.
Question
Which of the following are the inferior planets?

A) Mercury
B) Mercury and Mars
C) Mercury and Venus
D) Mars
E) Mercury, Mars, and Pluto
Question
A planet travels fastest in its orbit when it is closest to the Sun.
Question
Planets orbit the Sun on circular orbits.
Question
Which of the following are superior planets?

A) Mars
B) Earth and Venus
C) Venus, Mars, Jupiter, and Saturn
D) Earth, Jupiter, and Saturn
E) Mars, Jupiter, and Saturn
Question
Who of the following was NOT a proponent of the heliocentric model of the solar system?

A) Galileo
B) Copernicus
C) Newton
D) Ptolemy
E) Aristarchus
Question
Nicolaus Copernicus was the first to propose that Earth revolved around the Sun.
Question
_________ was the first person to introduce a mathematical heliocentric model of the Solar System from which accurate predictions could be made of planets' positions.

A) Nicolaus Copernicus
B) Tycho Brahe
C) Johannes Kepler
D) Galileo Galilei
E) Isaac Newton
Question
Johannes Kepler obtained accurate data on the positions of the planets in the sky over time, which Galileo used to prove that planets revolved around the Sun.
Question
As we move farther from the Sun, the circumferences of planetary orbits are larger, and the speeds at which planets travel increase.
Question
In the ________ model of the Solar System, ________ motion is only an apparent, not a real, motion.

A) geocentric; retrograde
B) heliocentric; retrograde
C) geocentric; prograde
D) heliocentric; prograde
E) Galilean; prograde
Question
If the synodic period of Mars is observed from Earth to be 2.1 years, what is Mars's sidereal period?

A) 5.3 years
B) 0.47 years
C) 1.9 years
D) 3.4 years
E) 0.69 years
Question
Observations of what astronomical events allowed astronomers to definitively determine that the heliocentric model of the solar system was correct?

A) total eclipses of the Sun
B) the precise motions of planets across the celestial sphere
C) motion of bright stars on the celestial sphere
D) the timing of the equinoxes
E) the timing of the solstices
Question
The time it takes for a planet to come back to the same position relative to the Sun is called its _________ period.

A) synodic
B) sidereal
C) heliocentric
D) geocentric
E) prograde
Question
The fact that Kepler's heliocentric model of the Solar System predicted _________ more easily and accurately than the geocentric model is an illustration of how scientific theories evolve by the scientific method.

A) solar eclipses
B) lunar eclipses
C) retrograde motion of planets
D) prograde motion of planets
E) the duration of the seasons
Question
When the Sun, the Earth, and a planet all lie along a straight line, the planet is at:

A) quadrature
B) opposition
C) greatest elongation
D) conjunction
E) either opposition or conjunction
Question
If the synodic period of Venus is observed from Earth to be 1.6 years, Venus' sidereal period is _____ years.

A) 1.9 years
B) 0.45 years
C) 0.28 years
D) 1.6 years
E) 0.62 years
Question
The amount of time a planet takes to orbit the Sun is called its _________ period.

A) synodic
B) sidereal
C) prograde
D) retrograde
E) geocentric
Question
An empirical science is one that is based on:

A) assumptions
B) calculus
C) computer models
D) observed data
E) hypotheses
Question
You find a moon orbiting a planet and you measure the distance between the moon and the planet once a night over the course of a few weeks. Its behavior is shown in the figure below where the time shown is the time since your first observation. What is this moon's orbital period? <strong>You find a moon orbiting a planet and you measure the distance between the moon and the planet once a night over the course of a few weeks. Its behavior is shown in the figure below where the time shown is the time since your first observation. What is this moon's orbital period?  </strong> A) 22 days B) 20 days C) 18 days D) 11 days E) 6 days <div style=padding-top: 35px>

A) 22 days
B) 20 days
C) 18 days
D) 11 days
E) 6 days
Question
<strong>  Figure 1 Based on Figure 1, a superior planet at opposition:</strong> A) would rise at noon and set at midnight B) would rise at midnight and set at noon C) would rise at sunset and set at sunrise D) would rise at sunrise and set at sunrise E) would rise at 8 and set at 8 <div style=padding-top: 35px> Figure 1
Based on Figure 1, a superior planet at opposition:

A) would rise at noon and set at midnight
B) would rise at midnight and set at noon
C) would rise at sunset and set at sunrise
D) would rise at sunrise and set at sunrise
E) would rise at 8 and set at 8
Question
Which laws are based entirely on observational data without having any theoretical framework behind them?

A) physical laws
B) Galileo's laws of planetary motion
C) Newton's laws of motion
D) deductive laws
E) empirical laws
Question
<strong>  Figure 1 Based on Figure 1, a superior planet would be seen high overhead at midnight:</strong> A) when at opposition B) when at eastern quadrature C) when at conjunction D) when at western quadrature E) throughout its orbit <div style=padding-top: 35px> Figure 1
Based on Figure 1, a superior planet would be seen high overhead at midnight:

A) when at opposition
B) when at eastern quadrature
C) when at conjunction
D) when at western quadrature
E) throughout its orbit
Question
If a superior planet is observed from Earth to have a synodic period of 1.2 years, what is its sidereal period?

A) 0.54 years
B) 1.8 years
C) 2.3 years
D) 4.0 years
E) 6.0 years
Question
Based on the figure below, an inferior planet would be farthest from the Sun and therefore most easily visible at: <strong>Based on the figure below, an inferior planet would be farthest from the Sun and therefore most easily visible at:  </strong> A) inferior conjunction B) superior conjunction C) greatest eastern elongation D) greatest western elongation E) at either greatest eastern or western elongation <div style=padding-top: 35px>

A) inferior conjunction
B) superior conjunction
C) greatest eastern elongation
D) greatest western elongation
E) at either greatest eastern or western elongation
Question
If the sidereal period of Jupiter is 11.9 years, what is Jupiter's synodic period as observed from Earth?

A) 2.3 years
B) 0.84 years
C) 0.92 years
D) 1.09 years
E) 1.5 years
Question
A superior planet is one that is:

A) smaller than Earth
B) larger than Earth
C) closer to the Sun than Earth
D) farther from the Sun than Earth
E) made of heavier materials than Earth
Question
When the Earth catches up to a slower moving outer planet and passes it like a faster runner overtaking a slower runner in an outside lane, the planet:

A) exhibits retrograde motion
B) slows down because it feels the Earth's gravitational pull
C) decreases in brightness as it passes through the Earth's shadow
D) moves into a more elliptical orbit
E) exhibits prograde motion
Question
The time it takes a planet to complete one full orbital revolution is commonly known as its:

A) period
B) frequency
C) orbital domain
D) velocity
E) eccentricity
Question
Astronomers argued that the heliocentric model of the Solar System was simpler than the geocentric model, based on:

A) the observation that the planets do not move relative to the background stars
B) the fact that the Moon orbits the Earth
C) the fact that the Sun is more massive than the Earth
D) the observed retrograde motions of the planets
E) the observed timing of lunar and solar eclipses
Question
Kepler's third law is a relationship between an orbiting object's:

A) gravitational force and mass
B) acceleration and mass
C) velocity and period
D) period and semimajor axis
E) semimajor axis and velocity
Question
A circle has an eccentricity of _________ and a line has an eccentricity of _________.

A) 1; 0
B) 1; 1
C) 0; infinity
D) 0; 1
E) infinity; 0
Question
Suppose an asteroid had an orbit with a semimajor axis of 4 AU. How long would it take for it to orbit once around the Sun?

A) 76 years
B) 45 years
C) 8 years
D) 16 years
E) 2 years
Question
Which of the following is TRUE about a comet that is on an elliptical orbit around the Sun?

A) The comet's speed is greatest when it is farthest from the Sun.
B) The comet's speed is greatest when it is nearest the Sun.
C) This comet's speed is zero.
D) The comet's speed is constant because its mass and the Sun's mass stay approximately the same.
E) The eccentricity is very low.
Question
The eccentricity of the majority of the planetary orbits in our Solar System is approximately:

A) 0
B) 1
C) 0.5
D) 0.2
E) infinity
Question
If Jupiter has an orbital period of 12 years, what value is closest to its average distance from the Sun?

A) 2 AU
B) 25 AU
C) 10 AU
D) 5 AU
E) 144 AU
Question
<strong>  Figure 2 In Figure 2, a planet orbits the Sun. During which of the three sections (A, B, or C) will the planet have the lowest average velocity?</strong> A) A B) B C) C D) The average velocity is the same for sections A, B, and C. E) The information given is insufficient to answer this question. <div style=padding-top: 35px> Figure 2
In Figure 2, a planet orbits the Sun. During which of the three sections (A, B, or C) will the planet have the lowest average velocity?

A) A
B) B
C) C
D) The average velocity is the same for sections A, B, and C.
E) The information given is insufficient to answer this question.
Question
A comet orbits the Sun with a semimajor axis of 90 AU. Using Kepler's third law, the comet's orbital period is approximately

A) 850 years
B) 630 years
C) 410 years
D) 180 years
E) 90 years
Question
During a certain comet's orbit around the Sun, its closest distance to the Sun is 0.6 AU, and its farthest distance from the Sun is 35 AU. At what distance will the comet's orbital velocity be the largest?

A) 35 AU
B) 17.8 AU
C) 1.2 AU
D) 0.6 AU
E) The comet's velocity is constant no matter what its distance is.
Question
Which equation represents the relationship of the planet's period to its semimajor axis in data shown in the figure below? <strong>Which equation represents the relationship of the planet's period to its semimajor axis in data shown in the figure below?  </strong> A) P = A B) P<sup>2</sup> = A<sup>2</sup> C) P<sup>3</sup> = A<sup>2</sup> D) P<sup>2</sup> = A<sup>3</sup> E) P= A<sup>3</sup> <div style=padding-top: 35px>

A) P = A
B) P2 = A2
C) P3 = A2
D) P2 = A3
E) P= A3
Question
Galileo's telescopic observations of _________ led him to conclude that the heliocentric model of the Solar System was correct.

A) motion of Jupiter and Saturn
B) motion of Venus
C) moons of Jupiter and phases of Venus
D) phases of the Moon
E) epicycles of Mars
Question
Kepler's third law for our Solar System can be expressed mathematically as:

A) P = A
B) P2 = A2
C) P2 = A3
D) P3= A2
E) P = A2
Question
If Neptune has a semimajor axis of 19 AU, its orbital period is:

A) 45 years
B) 83 years
C) 130 years
D) 220 years
E) 380 years
Question
Kepler's third law says that a comet with a period of 160 years will have a semimajor axis of:

A) 30 AU
B) 50 AU
C) 90 AU
D) 140 AU
E) 210 AU
Question
 <strong>  Figure 2  -In Figure 2, a planet orbits the Sun. The line connecting the planet and Sun sweeps out three areas labeled A, B, and C, during three different time intervals. If the duration of the time intervals are the same (meaning t<sub>2</sub> -t<sub>1</sub> = t<sub>4</sub> -t<sub>3</sub> = t<sub>6</sub> - t<sub>5</sub>), how are the sizes of these areas related?</strong> A) A   \gt  B   \gt  C B) C   \gt  B  \gt  A C) A   \gt  C   \gt  B D) B   \gt  A   \gt  C E) A, B, and C have the same size. <div style=padding-top: 35px>  Figure 2

-In Figure 2, a planet orbits the Sun. The line connecting the planet and Sun sweeps out three areas labeled A, B, and C, during three different time intervals. If the duration of the time intervals are the same (meaning t2 -t1 = t4 -t3 = t6 - t5), how are the sizes of these areas related?

A) A >\gt B >\gt C
B) C >\gt B >\gt A
C) A >\gt C >\gt B
D) B >\gt A >\gt C
E) A, B, and C have the same size.
Question
If the Sun is located at one focus of Earth's elliptical orbit, what is at the other focus?

A) Earth
B) the Moon
C) another planet
D) nothing
E) Jupiter
Question
If Mercury has an orbital period of about 88 days, what is its average distance from the Sun?

A) 0.2 AU
B) 0.01 AU
C) 0.05 AU
D) 0.4 AU
E) 0.7 AU
Question
The dwarf planet named Eris orbits the Sun with a semimajor axis of 68 AU. Using Kepler's third law, Eris's orbital period is:

A) 26 years
B) 130 years
C) 72 years
D) 240 years
E) 560 years
Question
Kepler's second law says that if a planet is in an elliptical orbit around a star, then the planet moves fastest when the planet is:

A) farthest from the star
B) closest to the star
C) exceeding the escape velocity
D) experiencing zero acceleration
E) located at one of the foci
Question
The average distance between a planet and the Sun is given by the _________ of its elliptical orbit.

A) radius
B) semiminor axis
C) eccentricity
D) semimajor axis
E) distance between the foci
Question
Who was the first notable historical figure to argue that the Earth orbits the Sun? Name two other people that were instrumental in arguing for the heliocentric model.
Question
Assume that at sunset today, Jupiter appears to be 20 degrees away from the Sun. If the sidereal period of Jupiter is 12 years, when will it next appear exactly in this same position relative to the Sun?
Question
If you start from rest and accelerate at 10 mph/s and end up traveling at 60 mph, how long did it take?

A) 1 seconds
B) 6 seconds
C) 600 seconds
D) 0.6 seconds
E) 200 seconds
Question
Explain how the synodic and sidereal periods of a planet are defined. Why are they not the same? Explain how they are related to one another.
Question
If you travel 20 miles from home to school in 30 minutes, what is your average velocity?

A) 20 mph
B) 40 mph
C) 0.7 mph
D) 5 mph
E) 600 mph
Question
Explain how the Occam's razor argument influenced whether people believed in the heliocentric or the geocentric model of the Solar System.
Question
The natural tendency of an object to resist changes in motion is called:

A) inertia
B) weight
C) acceleration
D) mass
E) velocity
Question
If you apply a force of 10 N to a grocery cart and get an acceleration of 0.5 m/s2, then the mass of the grocery cart is:

A) 5 kg
B) 0.05 kg
C) 20 kg
D) 50 kg
E) 0.20 kg
Question
If a 100-kg astronaut pushes on a 5,000-kg satellite and the satellite experiences an acceleration of 0.1 m/s2, what is the acceleration experienced by the astronaut in the opposite direction?

A) 5 m/s2
B) 10 m/s2
C) 50 m/s2
D) 0.1 m/s2
E) 1000 m/s2
Question
Based on the figure shown below, explain why an inferior planet would not be able to be seen at all from Earth when it is in conjunction. Based on the figure shown below, explain why an inferior planet would not be able to be seen at all from Earth when it is in conjunction.  <div style=padding-top: 35px>
Question
  Figure 3 Based on Figure 3, explain why, when a superior planet is in opposition, it will be visible from Earth all night long.<div style=padding-top: 35px> Figure 3
Based on Figure 3, explain why, when a superior planet is in opposition, it will be visible from Earth all night long.
Question
If you travel at a velocity of 30 mph during a 15-mile trip from home to school, how long does the trip take?

A) 2 hours
B) 0.2 hours
C) 0.5 hours
D) 5 hours
E) 750 hours
Question
If you travel at a velocity of 60 mph for a 5-hour trip, how far did you travel?

A) 300 miles
B) 120 miles
C) 12 miles
D) 0.4 miles
E) 240 mph
Question
What is your acceleration if you go from 0 to 60 mph in 4 seconds?

A) 60 mph/s
B) 30 mph/s
C) 15 mph/s
D) 8.5 mph/s
E) 240 mph/s
Question
If you start from rest and accelerate at 15 mph/s for 5 seconds, how fast will you be traveling at the end?

A) 75 mph
B) 45 mph
C) 3 mph
D) 12 mph
E) 20 mph
Question
You apply a force of 10 N to a grocery cart in order to get an acceleration of 0.5 m/s2. If you apply a force of 20 N to the same grocery cart, its acceleration will be:

A) 10 m/s2
B) 1 m/s2
C) 0.5 m/s2
D) 0.25m/s2
E) 20 m/s2
Question
Newton's first law states that objects in motion:

A) eventually come to rest
B) experience an unbalanced force
C) experience a nonzero acceleration
D) stay in motion
E) must be subject to zero friction
Question
Why were epicycles used in the geocentric system? Who first introduced epicycles?
Question
Based on the figure shown below, explain why an inferior planet is most likely to be seen when it is at one of its greatest elongations. Based on the figure shown below, explain why an inferior planet is most likely to be seen when it is at one of its greatest elongations.  <div style=padding-top: 35px>
Question
  Figure 3 Based on Figure 3, explain why a superior planet, when it is at conjunction, will not be seen at all from Earth during the night.<div style=padding-top: 35px> Figure 3
Based on Figure 3, explain why a superior planet, when it is at conjunction, will not be seen at all from Earth during the night.
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Deck 3: Motion of Astronomical Bodies
1
Retrograde motion is seen when ____________ due to the Earth's motion.

A) stars change their position in the sky with respect to background stars
B) stars rise in the west and set in the east
C) planets rise in the west and set in the east
D) planets change the direction in which they wander across the night sky
E) planets orbit the Sun in the opposite direction
planets change the direction in which they wander across the night sky
2
Kepler's third law written as P2 =A3 holds true mathematically for our Solar System only if the period is expressed in years and the semimajor axis is expressed in AU.
True
3
Newton's second law says that more massive objects are accelerated more than less massive objects when the same force is applied.
False
4
How did Ptolemy "fix" the geocentric system?

A) He introduced retrograde motion.
B) He introduced prograde motion.
C) He moved the Sun to the center.
D) He introduced epicycles.
E) He introduced Earth's motion.
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5
When the geocentric model of the solar system did not match the observed positions of the planets:

A) Tycho Brahe made measurements of higher accuracy and showed the geocentric model was correct
B) Ptolemy added epicycles to the geocentric model to match the observed data
C) Galileo argued that the Sun revolved around the Earth
D) Kepler was inspired to create the theory of gravity
E) Copernicus proposed the heliocentric mode
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6
Based on his observations of the planets, Copernicus calculated the relative distance of the planets from the Sun using the heliocentric model, and these distances were:

A) 10 times too large
B) exactly correct
C) close to the correct values, with errors less than 0.5 AU
D) accurate, but not as accurate as Ptolemy's values
E) two times too small
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7
An inferior planet is one that is:

A) smaller than Earth
B) larger than Earth
C) closer to the Sun than Earth
D) farther from the Sun than Earth
E) made of lighter materials than Earth
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8
In the heliocentric system, retrograde motion is not an actual motion of the planet but appears to occur because of the Earth's movement.
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9
At the center of the geocentric model of the Solar System is the:

A) Sun
B) Moon
C) Earth
D) Venus
E) Jupiter
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10
Planets with circular orbits travel at the same speed at all points in their orbits, whereas planets with elliptical orbits change their speeds at different points in their orbits.
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11
Even though they move at faster average speeds, the outer planets in the Solar System have longer periods than the inner planets.
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12
Which of the following are the inferior planets?

A) Mercury
B) Mercury and Mars
C) Mercury and Venus
D) Mars
E) Mercury, Mars, and Pluto
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13
A planet travels fastest in its orbit when it is closest to the Sun.
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14
Planets orbit the Sun on circular orbits.
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15
Which of the following are superior planets?

A) Mars
B) Earth and Venus
C) Venus, Mars, Jupiter, and Saturn
D) Earth, Jupiter, and Saturn
E) Mars, Jupiter, and Saturn
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16
Who of the following was NOT a proponent of the heliocentric model of the solar system?

A) Galileo
B) Copernicus
C) Newton
D) Ptolemy
E) Aristarchus
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17
Nicolaus Copernicus was the first to propose that Earth revolved around the Sun.
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18
_________ was the first person to introduce a mathematical heliocentric model of the Solar System from which accurate predictions could be made of planets' positions.

A) Nicolaus Copernicus
B) Tycho Brahe
C) Johannes Kepler
D) Galileo Galilei
E) Isaac Newton
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19
Johannes Kepler obtained accurate data on the positions of the planets in the sky over time, which Galileo used to prove that planets revolved around the Sun.
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20
As we move farther from the Sun, the circumferences of planetary orbits are larger, and the speeds at which planets travel increase.
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21
In the ________ model of the Solar System, ________ motion is only an apparent, not a real, motion.

A) geocentric; retrograde
B) heliocentric; retrograde
C) geocentric; prograde
D) heliocentric; prograde
E) Galilean; prograde
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22
If the synodic period of Mars is observed from Earth to be 2.1 years, what is Mars's sidereal period?

A) 5.3 years
B) 0.47 years
C) 1.9 years
D) 3.4 years
E) 0.69 years
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23
Observations of what astronomical events allowed astronomers to definitively determine that the heliocentric model of the solar system was correct?

A) total eclipses of the Sun
B) the precise motions of planets across the celestial sphere
C) motion of bright stars on the celestial sphere
D) the timing of the equinoxes
E) the timing of the solstices
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24
The time it takes for a planet to come back to the same position relative to the Sun is called its _________ period.

A) synodic
B) sidereal
C) heliocentric
D) geocentric
E) prograde
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25
The fact that Kepler's heliocentric model of the Solar System predicted _________ more easily and accurately than the geocentric model is an illustration of how scientific theories evolve by the scientific method.

A) solar eclipses
B) lunar eclipses
C) retrograde motion of planets
D) prograde motion of planets
E) the duration of the seasons
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26
When the Sun, the Earth, and a planet all lie along a straight line, the planet is at:

A) quadrature
B) opposition
C) greatest elongation
D) conjunction
E) either opposition or conjunction
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27
If the synodic period of Venus is observed from Earth to be 1.6 years, Venus' sidereal period is _____ years.

A) 1.9 years
B) 0.45 years
C) 0.28 years
D) 1.6 years
E) 0.62 years
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28
The amount of time a planet takes to orbit the Sun is called its _________ period.

A) synodic
B) sidereal
C) prograde
D) retrograde
E) geocentric
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29
An empirical science is one that is based on:

A) assumptions
B) calculus
C) computer models
D) observed data
E) hypotheses
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30
You find a moon orbiting a planet and you measure the distance between the moon and the planet once a night over the course of a few weeks. Its behavior is shown in the figure below where the time shown is the time since your first observation. What is this moon's orbital period? <strong>You find a moon orbiting a planet and you measure the distance between the moon and the planet once a night over the course of a few weeks. Its behavior is shown in the figure below where the time shown is the time since your first observation. What is this moon's orbital period?  </strong> A) 22 days B) 20 days C) 18 days D) 11 days E) 6 days

A) 22 days
B) 20 days
C) 18 days
D) 11 days
E) 6 days
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31
<strong>  Figure 1 Based on Figure 1, a superior planet at opposition:</strong> A) would rise at noon and set at midnight B) would rise at midnight and set at noon C) would rise at sunset and set at sunrise D) would rise at sunrise and set at sunrise E) would rise at 8 and set at 8 Figure 1
Based on Figure 1, a superior planet at opposition:

A) would rise at noon and set at midnight
B) would rise at midnight and set at noon
C) would rise at sunset and set at sunrise
D) would rise at sunrise and set at sunrise
E) would rise at 8 and set at 8
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32
Which laws are based entirely on observational data without having any theoretical framework behind them?

A) physical laws
B) Galileo's laws of planetary motion
C) Newton's laws of motion
D) deductive laws
E) empirical laws
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33
<strong>  Figure 1 Based on Figure 1, a superior planet would be seen high overhead at midnight:</strong> A) when at opposition B) when at eastern quadrature C) when at conjunction D) when at western quadrature E) throughout its orbit Figure 1
Based on Figure 1, a superior planet would be seen high overhead at midnight:

A) when at opposition
B) when at eastern quadrature
C) when at conjunction
D) when at western quadrature
E) throughout its orbit
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34
If a superior planet is observed from Earth to have a synodic period of 1.2 years, what is its sidereal period?

A) 0.54 years
B) 1.8 years
C) 2.3 years
D) 4.0 years
E) 6.0 years
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35
Based on the figure below, an inferior planet would be farthest from the Sun and therefore most easily visible at: <strong>Based on the figure below, an inferior planet would be farthest from the Sun and therefore most easily visible at:  </strong> A) inferior conjunction B) superior conjunction C) greatest eastern elongation D) greatest western elongation E) at either greatest eastern or western elongation

A) inferior conjunction
B) superior conjunction
C) greatest eastern elongation
D) greatest western elongation
E) at either greatest eastern or western elongation
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36
If the sidereal period of Jupiter is 11.9 years, what is Jupiter's synodic period as observed from Earth?

A) 2.3 years
B) 0.84 years
C) 0.92 years
D) 1.09 years
E) 1.5 years
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37
A superior planet is one that is:

A) smaller than Earth
B) larger than Earth
C) closer to the Sun than Earth
D) farther from the Sun than Earth
E) made of heavier materials than Earth
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38
When the Earth catches up to a slower moving outer planet and passes it like a faster runner overtaking a slower runner in an outside lane, the planet:

A) exhibits retrograde motion
B) slows down because it feels the Earth's gravitational pull
C) decreases in brightness as it passes through the Earth's shadow
D) moves into a more elliptical orbit
E) exhibits prograde motion
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39
The time it takes a planet to complete one full orbital revolution is commonly known as its:

A) period
B) frequency
C) orbital domain
D) velocity
E) eccentricity
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40
Astronomers argued that the heliocentric model of the Solar System was simpler than the geocentric model, based on:

A) the observation that the planets do not move relative to the background stars
B) the fact that the Moon orbits the Earth
C) the fact that the Sun is more massive than the Earth
D) the observed retrograde motions of the planets
E) the observed timing of lunar and solar eclipses
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41
Kepler's third law is a relationship between an orbiting object's:

A) gravitational force and mass
B) acceleration and mass
C) velocity and period
D) period and semimajor axis
E) semimajor axis and velocity
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42
A circle has an eccentricity of _________ and a line has an eccentricity of _________.

A) 1; 0
B) 1; 1
C) 0; infinity
D) 0; 1
E) infinity; 0
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43
Suppose an asteroid had an orbit with a semimajor axis of 4 AU. How long would it take for it to orbit once around the Sun?

A) 76 years
B) 45 years
C) 8 years
D) 16 years
E) 2 years
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44
Which of the following is TRUE about a comet that is on an elliptical orbit around the Sun?

A) The comet's speed is greatest when it is farthest from the Sun.
B) The comet's speed is greatest when it is nearest the Sun.
C) This comet's speed is zero.
D) The comet's speed is constant because its mass and the Sun's mass stay approximately the same.
E) The eccentricity is very low.
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45
The eccentricity of the majority of the planetary orbits in our Solar System is approximately:

A) 0
B) 1
C) 0.5
D) 0.2
E) infinity
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46
If Jupiter has an orbital period of 12 years, what value is closest to its average distance from the Sun?

A) 2 AU
B) 25 AU
C) 10 AU
D) 5 AU
E) 144 AU
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47
<strong>  Figure 2 In Figure 2, a planet orbits the Sun. During which of the three sections (A, B, or C) will the planet have the lowest average velocity?</strong> A) A B) B C) C D) The average velocity is the same for sections A, B, and C. E) The information given is insufficient to answer this question. Figure 2
In Figure 2, a planet orbits the Sun. During which of the three sections (A, B, or C) will the planet have the lowest average velocity?

A) A
B) B
C) C
D) The average velocity is the same for sections A, B, and C.
E) The information given is insufficient to answer this question.
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48
A comet orbits the Sun with a semimajor axis of 90 AU. Using Kepler's third law, the comet's orbital period is approximately

A) 850 years
B) 630 years
C) 410 years
D) 180 years
E) 90 years
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49
During a certain comet's orbit around the Sun, its closest distance to the Sun is 0.6 AU, and its farthest distance from the Sun is 35 AU. At what distance will the comet's orbital velocity be the largest?

A) 35 AU
B) 17.8 AU
C) 1.2 AU
D) 0.6 AU
E) The comet's velocity is constant no matter what its distance is.
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50
Which equation represents the relationship of the planet's period to its semimajor axis in data shown in the figure below? <strong>Which equation represents the relationship of the planet's period to its semimajor axis in data shown in the figure below?  </strong> A) P = A B) P<sup>2</sup> = A<sup>2</sup> C) P<sup>3</sup> = A<sup>2</sup> D) P<sup>2</sup> = A<sup>3</sup> E) P= A<sup>3</sup>

A) P = A
B) P2 = A2
C) P3 = A2
D) P2 = A3
E) P= A3
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51
Galileo's telescopic observations of _________ led him to conclude that the heliocentric model of the Solar System was correct.

A) motion of Jupiter and Saturn
B) motion of Venus
C) moons of Jupiter and phases of Venus
D) phases of the Moon
E) epicycles of Mars
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52
Kepler's third law for our Solar System can be expressed mathematically as:

A) P = A
B) P2 = A2
C) P2 = A3
D) P3= A2
E) P = A2
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53
If Neptune has a semimajor axis of 19 AU, its orbital period is:

A) 45 years
B) 83 years
C) 130 years
D) 220 years
E) 380 years
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54
Kepler's third law says that a comet with a period of 160 years will have a semimajor axis of:

A) 30 AU
B) 50 AU
C) 90 AU
D) 140 AU
E) 210 AU
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55
 <strong>  Figure 2  -In Figure 2, a planet orbits the Sun. The line connecting the planet and Sun sweeps out three areas labeled A, B, and C, during three different time intervals. If the duration of the time intervals are the same (meaning t<sub>2</sub> -t<sub>1</sub> = t<sub>4</sub> -t<sub>3</sub> = t<sub>6</sub> - t<sub>5</sub>), how are the sizes of these areas related?</strong> A) A   \gt  B   \gt  C B) C   \gt  B  \gt  A C) A   \gt  C   \gt  B D) B   \gt  A   \gt  C E) A, B, and C have the same size.  Figure 2

-In Figure 2, a planet orbits the Sun. The line connecting the planet and Sun sweeps out three areas labeled A, B, and C, during three different time intervals. If the duration of the time intervals are the same (meaning t2 -t1 = t4 -t3 = t6 - t5), how are the sizes of these areas related?

A) A >\gt B >\gt C
B) C >\gt B >\gt A
C) A >\gt C >\gt B
D) B >\gt A >\gt C
E) A, B, and C have the same size.
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56
If the Sun is located at one focus of Earth's elliptical orbit, what is at the other focus?

A) Earth
B) the Moon
C) another planet
D) nothing
E) Jupiter
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57
If Mercury has an orbital period of about 88 days, what is its average distance from the Sun?

A) 0.2 AU
B) 0.01 AU
C) 0.05 AU
D) 0.4 AU
E) 0.7 AU
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58
The dwarf planet named Eris orbits the Sun with a semimajor axis of 68 AU. Using Kepler's third law, Eris's orbital period is:

A) 26 years
B) 130 years
C) 72 years
D) 240 years
E) 560 years
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59
Kepler's second law says that if a planet is in an elliptical orbit around a star, then the planet moves fastest when the planet is:

A) farthest from the star
B) closest to the star
C) exceeding the escape velocity
D) experiencing zero acceleration
E) located at one of the foci
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60
The average distance between a planet and the Sun is given by the _________ of its elliptical orbit.

A) radius
B) semiminor axis
C) eccentricity
D) semimajor axis
E) distance between the foci
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61
Who was the first notable historical figure to argue that the Earth orbits the Sun? Name two other people that were instrumental in arguing for the heliocentric model.
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62
Assume that at sunset today, Jupiter appears to be 20 degrees away from the Sun. If the sidereal period of Jupiter is 12 years, when will it next appear exactly in this same position relative to the Sun?
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63
If you start from rest and accelerate at 10 mph/s and end up traveling at 60 mph, how long did it take?

A) 1 seconds
B) 6 seconds
C) 600 seconds
D) 0.6 seconds
E) 200 seconds
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64
Explain how the synodic and sidereal periods of a planet are defined. Why are they not the same? Explain how they are related to one another.
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65
If you travel 20 miles from home to school in 30 minutes, what is your average velocity?

A) 20 mph
B) 40 mph
C) 0.7 mph
D) 5 mph
E) 600 mph
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66
Explain how the Occam's razor argument influenced whether people believed in the heliocentric or the geocentric model of the Solar System.
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67
The natural tendency of an object to resist changes in motion is called:

A) inertia
B) weight
C) acceleration
D) mass
E) velocity
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68
If you apply a force of 10 N to a grocery cart and get an acceleration of 0.5 m/s2, then the mass of the grocery cart is:

A) 5 kg
B) 0.05 kg
C) 20 kg
D) 50 kg
E) 0.20 kg
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69
If a 100-kg astronaut pushes on a 5,000-kg satellite and the satellite experiences an acceleration of 0.1 m/s2, what is the acceleration experienced by the astronaut in the opposite direction?

A) 5 m/s2
B) 10 m/s2
C) 50 m/s2
D) 0.1 m/s2
E) 1000 m/s2
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70
Based on the figure shown below, explain why an inferior planet would not be able to be seen at all from Earth when it is in conjunction. Based on the figure shown below, explain why an inferior planet would not be able to be seen at all from Earth when it is in conjunction.
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71
  Figure 3 Based on Figure 3, explain why, when a superior planet is in opposition, it will be visible from Earth all night long. Figure 3
Based on Figure 3, explain why, when a superior planet is in opposition, it will be visible from Earth all night long.
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72
If you travel at a velocity of 30 mph during a 15-mile trip from home to school, how long does the trip take?

A) 2 hours
B) 0.2 hours
C) 0.5 hours
D) 5 hours
E) 750 hours
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73
If you travel at a velocity of 60 mph for a 5-hour trip, how far did you travel?

A) 300 miles
B) 120 miles
C) 12 miles
D) 0.4 miles
E) 240 mph
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74
What is your acceleration if you go from 0 to 60 mph in 4 seconds?

A) 60 mph/s
B) 30 mph/s
C) 15 mph/s
D) 8.5 mph/s
E) 240 mph/s
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75
If you start from rest and accelerate at 15 mph/s for 5 seconds, how fast will you be traveling at the end?

A) 75 mph
B) 45 mph
C) 3 mph
D) 12 mph
E) 20 mph
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76
You apply a force of 10 N to a grocery cart in order to get an acceleration of 0.5 m/s2. If you apply a force of 20 N to the same grocery cart, its acceleration will be:

A) 10 m/s2
B) 1 m/s2
C) 0.5 m/s2
D) 0.25m/s2
E) 20 m/s2
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77
Newton's first law states that objects in motion:

A) eventually come to rest
B) experience an unbalanced force
C) experience a nonzero acceleration
D) stay in motion
E) must be subject to zero friction
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78
Why were epicycles used in the geocentric system? Who first introduced epicycles?
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79
Based on the figure shown below, explain why an inferior planet is most likely to be seen when it is at one of its greatest elongations. Based on the figure shown below, explain why an inferior planet is most likely to be seen when it is at one of its greatest elongations.
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80
  Figure 3 Based on Figure 3, explain why a superior planet, when it is at conjunction, will not be seen at all from Earth during the night. Figure 3
Based on Figure 3, explain why a superior planet, when it is at conjunction, will not be seen at all from Earth during the night.
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