Answer:
To estimate the mass of the Sun, we require, the time
period of revolution T of one of its planets (say the Earth). Let be the
masses of Sun and Earth respectively and r be the mean orbital radius of the Earth
around the Sun. The gravitational force acting on Earth due to Sun is Let, the
Earth be moving in circular orbit around the Sun, with a uniform angular
velocity , the
centripetal force acting on Earth is As this
centripetal force is provided by the gravitational pull of Sun on Earth, so
Knowing
r and T, mass My of the Sun can be estimated.
In this question, we are given,
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