AP Physics Circular Motion, Centripetal Force and Planetary Motion Equations

geostationary

v=(4π^2r^2)/T^2

Escape Velocity

Ve=sqr(GM)/r

Period

(2πr)/T

Centripetal Force

Fc=(mv^2)/r

Orbital Period

T=2πsqrr^3/(Gm)

Gravity

6.67x10^-11

Orbital Speed

sqre(GM)/r