Question
F = GM 1 M 2 /d 2 Where G is the gravitational constant, M1 and M2 are the two masses, and d is the
F = GM1M2/d2
Where G is the gravitational constant, M1 and M2 are the two masses, and d is the distance between them.
For the Earth and another body, Sun or Moon, the forces for the far side and near side of the Earth being attracted to that object look like this:
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Systems Analysis and Design
Authors: Scott Tilley, Harry J. Rosenblatt
11th Edition
1305494601, 9781305533936 , 978-1305494602
