Us Kepler's 3rd Law to calculate the mass of a star which has a planet orbiting at 2.35 A.U. and takes 4.56 Earth years to complete one full orbit. a. 0.600-0.610 b. 0.623-0.625 c. 0.653-0.675 d. 0.733-0.775
Us Kepler's 3rd Law to calculate the mass of a star which has a planet orbiting at 2.35 A.U. and takes 4.56 Earth years to complete one full orbit. a. 0.600-0.610 b. 0.623-0.625 c. 0.653-0.675 d. 0.733-0.775
College Physics
1st Edition
ISBN:9781938168000
Author:Paul Peter Urone, Roger Hinrichs
Publisher:Paul Peter Urone, Roger Hinrichs
Chapter2: Kinematics
Section: Chapter Questions
Problem 10PE: Tidal friction is slowing the rotation of the Earth. As a result, the orbit of the Moon is...
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Us Kepler's 3rd Law to calculate the mass of a star which has a planet orbiting at 2.35 A.U. and takes 4.56 Earth years to complete one full orbit.
a. 0.600-0.610
b. 0.623-0.625
c. 0.653-0.675
d. 0.733-0.775
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