Just use the formula
F = GMm/r^2
Disregard the data about the sizes of the bodies. You have their masses and the separation, and G.
So, plug in the numbers.
Find the gravitational force acting on the Sun by the Earth.
Given: Mass of the Sun = 1.99 * 1030 kg
Mass of the Earth = 5.98 * 1024 kg
Radius of the Sun = 6.96 * 108 m
Radius of the Earth = 6.37 * 106 m
Distance between the Sun and the Earth = 1.50 * 1011 m
G = 6.67 * 10–11 N m2 kg–2
2 answers
use the formula g=Gm1m2/r^2
G=6.67 x 10^-11 N
G=6.67 x 10^-11 N
0 answers