G * m1 * m2 F = ------------- r*rwhere G is the gravitational constant, m1 and m2 are the masses of the bodies, and r is the separation between them.
G * M(earth) * m G * M(earth) F = ----------------- = -------------- * m R(earth)^2 R(earth)^2 = g * mwhere g, the gravitational acceleration at the surface of the earth, has a value of about 9.8 meters per second squared, downwards.
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Copyright © Michael Richmond. This work is licensed under a Creative Commons License.