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Please explain how to answer this question? Use the following data for Saturn to calculate the mass of the sun. The period of Saturn is 9.3*10^8 s and the mean orbital radius is 1.43*10^12 m. Thank you!
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Assuming a circular orbit at the mean radius The centripetal force to keep the body in that orbit is \[mr \omega ^{2}\] The force of gravity between the two bodies is \[\frac{ GM _{sun}m _{Saturn} }{ r ^{2} }\] These two forces are equal So using G (universal gravitational constant) Omega (= 2pi/period) r = given radius you can calculate M
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