Science Physics Kepler's Third Law
Solve for planet mass.
G is the universal gravitational constant
G = 6.6726 x 10-11N-m2/kg2
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gravitational force exerted between two objects | |
mass of object 1 | |
mass of object 2 | |
distance between the objects |
satellite orbit period | |
satellite mean orbital radius | |
planet mass |
gravitational acceleration | |
planet mass | |
radius from the planet center |
escape or critical speed | |
planet mass | |
planet radius |
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