
Sidney P. answered 03/25/21
Astronomy, Physics, Chemistry, and Math Tutor
From setting centripetal force = gravitational force, v2 = GM/r. The orbital speed is also circumference divided by period T, so v2 = (2π r / T)2 = 4π2 r2 / T2. Note that r = 9.405 x 103 km or 9.405 x 106 m. Then T2 = 4π2 r3 /GM = 4π2 (9.405 x 106 m)3 / [(6.67 x 10-11)(6.42 x 1023)] = 7.67 x 108 and T = 2.77 x 104 seconds = 462 minutes.