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Geology Section 26.2 Homework: Observing the Solar System: A History: Due Friday, 2/3/12
Read Section 26.2, pages 577-581. Answer the questions that follow.
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Last Name, First Name
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Your answer
Period (Do not put nd, rd, or th after the number!)
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Your answer
Explain the retrograde motion of Mars and how the motion of Mars led early scientists and theologians to believe that the Universe was Earth-centered.
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Your answer
Who proposed the idea of epicycles in a geocentric system?
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Copernicus
Galileo
Ptolemy
Newton
Kepler
Planets sweep out equal areas in equal times. This is a statement of
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Kepler's 1st Law
Kepler's 2nd Law
Kepler's 3rd Law
Newton's 2nd Law
Newton's 1st Law
To find the period of orbit of a planet (time in years it takes to go around the Sun), you would
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Take the cube root of the distance of the planet from the Sun in Astronomical Units squared
Take the square root of the distance of the planet from the Sun in Astronomical Units cubed
Use the formula F = ma
Square the planet's distance from the Sun in Astronomical Units
Mars is 1.5 astronomical units from the Sun. How long will it take Mars to go around the Sun in Earth years?
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Around 1/2 an Earth year
Around 1 Earth years
Around 4 Earth years
Around 2 Earth years
Define an astronomical unit. What is it and why is it an easier unit to use when measuring distances in the solar system?
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Your answer
What law describes the reason that planets continue to travel around the Sun without any apparent propulsion?
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Newton's 1st Law
Newton's 2nd Law
Newton's 3rd Law
Newton's 4th Law
Kepler's 1st Law
Read the article on page 581 about Galileo. Summarize Galileo's major contributions to science in a short paragraph. You must cite at least 3 contributions to be worthy of an A on this one.
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