Physics — Newtonian Gravitation
Universal gravitation, field strength and Kepler's third law.
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F = G\frac{m_1 m_2}{r^2}
g = \frac{GM}{r^2}
U = -\frac{GMm}{r}
T^2 = \frac{4\pi^2}{GM}\,r^3
Universal gravitation, field strength and Kepler's third law.
F = G\frac{m_1 m_2}{r^2}
g = \frac{GM}{r^2}
U = -\frac{GMm}{r}
T^2 = \frac{4\pi^2}{GM}\,r^3