Daniel B. answered 12/18/22
A retired computer professional to teach math, physics
Let
T = 0.7 days = 0.7×24×3600 s = 60480 s be the satellite's period,
M = 5.97×1024 kg be the mass of the Earth,
R = 6.37×106 m be the Earth's radius,
m be the mass of the satellite (unknown),
r be the distance of the satellite from the center of the Earth (to be computed),
G = 6.6743×10-11 m³/kgs² be the gravitational constant.
The length of the satellites orbit is 2πr, and therefore its velocity is
v = 2πr/T
The only force acting on the satellite is gravity, and it is of magnitude
F = GMm/r²
The setellite is experiencing centripetal acceleration
a = v²/r = (2πr/T)²/r = 4π²r/T²
By Newton's Second Law
F = ma
Substitute the above quantities
GMm/r² = 4mπ²r/T²
Simplify into
r = (GMT²/4π²)1/3
Substitute actual numbers
r = (6.6743×10-11 × 5.97×1024 × 60480²/(4π²))1/3 ≈ 33.3 × 106 m
(a) The satellite is about 33300 km from the center of the Earth.
(b) The average altitude is r - R = 33.3×106 - 6.37×106 ≈ 27×106 m
The average altitude is about 27000 km.
That is a little lower that geostationary.