Arturo O. answered 05/03/18
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I will explain how to solve this, but YOU do the calculations.
r = radius of Saturn's orbit (given)
M = mass of sun (given)
m = mass of Saturn (you will see in a few lines that we really do not need this)
G = constant of universal gravitation (look it up in your physics book)
T = period = ?
Equate the gravitational attraction of the sun to the centripetal force on Saturn.
GMm/r2 = mv2/r ⇒
GM/r = v2
v = 2πr/T ⇒
GM/r = 4π2r2/T2
Solve for T and get
T = 2π [r3/(GM)]1/2
Plug in the numbers in appropriate units and get T. This is actually Kepler's 3rd law of planetary motion.