AP Physics Circular Motion, Centripetal Force and Planetary Motion Equations
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7 Terms
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geostationary
v=(4π^2r^2)/T^2
2
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Escape Velocity
Ve=sqr(GM)/r
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Period
(2πr)/T
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Centripetal Force
Fc=(mv^2)/r
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Orbital Period
T=2πsqrr^3/(Gm)
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Gravity
6.67x10^-11
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Orbital Speed
sqre(GM)/r