Saturn's moon mimas has an orbital period of 82,800 s at a distance of 1.87x10^8m from saturn. using m central m= (4n^2d^3/gt^2) 1 determine saturn's mass. determine saturn's mass by rearranging newton's version of kepler's third law.

Explanation:

From Kepler's third law: Mass of the planet is given by:

where, T is the time period of satellite revolving about the planet at a distance d. G is the gravitational constant = 6.67 × 10⁻¹¹ Nm²/kg²

Given, d = 1.87 × 10⁸ m

T = 82800 s

⇒

number of electrons for neutral cl