The force of attraction between two masses, especially that between the Earth and another body.This force is proportional to the masses of the two bodies and inversely proportional to the distance between them.
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\begin
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[F_
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= \frac{GM_
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M_{2}}r_{1,2
^{2}} ]\end
Here M1 and M2 are the masses, r1,2 is their separation, and G is the constant of proportionality, called the Gravitational Constant.
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\begin
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[ G = (6.67428 \pm 0.00067) \times 10^{-8} \frac{cm^{3}}{g \; sec^{2}} ]\end