Answer:
(a) T = 2.23h
(b) v = 6.78 km/s
(c) a = 5.31 m/s²
Step-by-step explanation:
(a) The period (T) of the orbit can be calculated using Kepler's Third Law equation:
(1)
where r: is the distance from the center of the Earth and the satellite, G: is the gravitational constant = 6.67x10⁻¹¹m³kg⁻¹s⁻² and M: is the Earth's mass = 5.97x10²⁴kg
Since
where
: is the Earth's radius and
: is the distance between the surface of the Earth and the satellite
Hence, by entering the radius calculated into equation (1) we can find the period of the orbit:

(b) The speed (v) of the satellite can be calculated using the following equation:
(c) The acceleration (a) of the satellite is:
I hope it helps you!