1.) 7382 m/s
The gravitational attraction between the satellite and the Earth provides the centripetal force that keeps the satellite in circular motion, so we can write

where
G is the gravitational constant
is the Earth's mass
m is the satellite's mass
is the Earth's radius
is the altitude of the satellite above the Earth's surface
v is the orbital speed
Solving the formula for v, we find

2) 1.73 hours
The period of the orbit is the time taken to complete one revolution around the Earth, therefore:

where the numerator is the circumference of the orbit and v the orbital speed, therefore we find

Converting into hours,
