A satellite of mass m moving in a circular Earth orbit of radius r. It loses mechanical energy due to small air resistance at a constant rate C J s⁻¹. If the Earth's radius is Rₑ and the time to spiral down to the Earth is t = [GMm/(nC)](1/Rₑ - 1/r), find n.
Physics · Gravitation · Satellites, Orbital Motion & Kepler’s Laws
A satellite of mass m moving in a circular Earth orbit of radius r. It loses mechanical energy due to small air resistance at a constant rate C J s⁻¹. If the Earth's radius is Rₑ and the time to spiral down to the Earth is t = [GMm/(nC)](1/Rₑ - 1/r), find n.