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
Correct Answer:
Verified
Q1: Retrograde motion is seen when _ due
Q2: Kepler's third law written as P2 =A3
Q3: Newton's second law says that more massive
Q4: How did Ptolemy "fix" the geocentric system?
A)
Q5: When the geocentric model of the solar
Q8: In the heliocentric system, retrograde motion is
Q9: At the center of the geocentric model
Q10: Planets with circular orbits travel at the
Q11: Even though they move at faster average
Q20: An inferior planet is one that is
A)
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