Physics Circular Motion Equations

Get a hint

hint

gravitational period (T)

gravitational period (T)

(2π/√GM)r^3/2

gravitational velocity (v)

√(GM/r)

Gravity on another planet (g)

(GM/r^2)

centripetal force

(mv^2/r)

centripetal acceleration

(v^2)/r

velocity

(2πr)/T

In √(GM/r) , what does the M represent?

mass of the object being orbited

Newton's Law of Universal Gravitation (F)

G((m1 * m2)/r^2)