Answer:
a) v = 5.59x10³ m/s
b) T = 4 h
c) F = 1.92x10³ N
Step-by-step explanation:
a) We can find the satellite's orbital speed by equating the centripetal force and the gravitation force as follows:


Where:
g is the gravity = 9.81 m/s²
r: is the Earth's radius = 6371 km
h: is the satellite's height = r = 6371 km
b) The period of its revolution is:
c) The gravitational force acting on it is given by:

Where:
M is the Earth's mass = 5.97x10²⁴ kg
m is the satellite's mass = 782 kg
G is the gravitational constant = 6.67x10⁻¹¹ Nm²kg⁻²

I hope it helps you!