A. Use the definition of the center of mass to determine the maximum “wobble” velocity of a star of mass M caused by a planet of mass m orbiting at a distance r from the star with a period T. B. Thanks to Kepler, we know that the mass, period, and distance of an orbiting object are actually related. Use Newton’s version of Kepler’s Third Law to determine the maximum “wobble” velocity in terms of M, m, and r.
A. Use the definition of the center of mass to determine the maximum “wobble” velocity of a star of mass M caused by a planet of mass m orbiting at a distance r from the star with a period T. B. Thanks to Kepler, we know that the mass, period, and distance of an orbiting object are actually related. Use Newton’s version of Kepler’s Third Law to determine the maximum “wobble” velocity in terms of M, m, and r.
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A. Use the definition of the center of mass to determine the maximum “wobble” velocity
of a star of mass M caused by a planet of mass m orbiting at a distance r from the star
with a period T.
B. Thanks to Kepler, we know that the mass, period, and distance of an orbiting object
are actually related. Use Newton’s version of Kepler’s Third Law to determine the
maximum “wobble” velocity in terms of M, m, and r.
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