
Sidney P. answered 12/17/21
Minored in physics in college, 2 years of recent teaching experience
a) Gravitational force Fg = G M m / r2. The distance r is from the center of Earth, so r = 6,380 + 450 km = 6.83 x 103 km • (1,000 m/1 km) = 6.83 x 106 m. Fg = (6.67 x 10-11) (5.98 x 1024) (800) / (6.83 x 106)2 = 6,840 N (on Earth's surface, the force would be mg = 7,850 N).
b) Orbital speed v = √[G ME / r] = √[(6.67 x 10-11) (5.98 x 1024) / (6.83 x 106)] = 7,640 m/s (17,100 mph).
c) The orbital speed v is circumference of the orbit, 2π r, divided by the time T to complete one orbit, so T = 2π r / v = 2π (6.83 x 106 m) / (7.64 x 103 m/s) = 5620 s • (1 hour /3600 s) = 1.56 hour.