Fg=GMmr2F_g = \dfrac{GMm}{r^2}Fg=r2GMm
where;
FgF_gFg = Gravitational force acting on object mmm
MMM = Mass of massive body
mmm = mass of object
rrr = distance between the two masses
GGG = Gravitational constant (6.67×10−11)(6.67\times10^{-11})(6.67×10−11)
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