One of Kepler's laws suggests that for moons that have circular orbits around a…

PHYSICS · Multi-part · A Level · Physics · Fields and their consequences · Fields and their consequences

Problem

One of Kepler's laws suggests that for moons that have circular orbits around a planet: T24πr3=k\frac{T^2}{4\pi r^3} = k where TT is the orbital period of the moon, rr is the radius of its circular orbit about the planet, and kk is a constant. The table gives data relating to the two moons of Mars.
MoonTT / hourrr / Mm
Phobos7.669.38
Deimos30.4-
(1) Show that k=1GMk = \frac{1}{GM}. (2) Determine rr for Deimos.

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