Arturo O. answered 09/27/19
Experienced Physics Teacher for Physics Tutoring
I will set this up for you, but YOU do the math.
R = radius of planet in meters (given)
H = height of orbit in meters (given)
G = constant of gravitation (look it up in your book in units of Nm2/kg2)
M = mass of planet in kg (given)
Assuming the satellite is in a circular orbit, get the speed v in m/s by setting the gravitational force equal to the centripetal force, and solve for v. Note you do not need to know the mass of the satellite, since it cancels out.
GM / (R + H)2 = v2 / (R + H) ⇒
v = √[GM / (R + H)]
Get period P in seconds from
v = 2π(R + H) / P ⇒
P = 2π(R + H) / v
Now plug in R, H, and v to get P in seconds, convert seconds to days, and you are done.