
William W. answered 10/25/19
Experienced Tutor and Retired Engineer
- F = ma but the centripetal acceleration = v2/r so F = (mv2)/r
- F = Gm1m2/d2 where G = 6.674 x 10-11 m3/kg/s2.
- Using F = Gm1m2/d2 and solving for d and equating m1 = m2 = m, we get d2 = Gm2/F so d = √(Gm2/F) or d = m√(G/F)
- Using F = Gm1m2/d2 and replacing m1 with mT (mass of Tom) and m2 with mS (mass of Sally) and solving for mS, we get: F = GmTmS/d2 or (Fd2)/(GmT) = mS
- Let gP be the gravitational acceleration of the planet. Using F = Gm1m2/d2, we can also say that F = ma, or in this case F = mgP. We can replace m1 with MP (mass of the planet) and m2 can be replaced with just m which represents the mass of some random object on the surface of the planet. So, GMPm/d2 = mgP. Since the mass of a planet acts as if all the mass was concentrated at the center, the distance from MP to m is the radius of the planet (r), so GMPm/r2 = mgP. Dividing both sides by m, the m's just cancel out making the equation: GMP/r2 = gP