Easiest way is to plug 2πR/T for v in the centripetal force equation: FC = mv2/R = 4π2Rm/T2
Equate the centripetal and gravitational force:
GMm/R2 = 4π2Rm/T2
Rearrange and cancel m, the mass of the satellite
T2 = (4π2/GM) R3 (which is how Kepler's Law connects to gravitation
Actually you are solving for R given T = 1day (you have to put T in seconds) R will be in meters
You can convert that to get miles.
In the second part, the total mechanical energy is EK + UG . You could just plug in 1/2 mv2 = EK and
-GMm/R for UG
but because mv2/R = GMm/R2 EK = 1/2 |UG| It is always true that ETot = 1/2 UG So, you only have to plug into the UG equation.
Please consider a tutor.
Bri S.
gotcha, thank you!11/12/21