Daniel B. answered 12/29/20
A retired computer professional to teach math, physics
Let
T = 43200 s be the satellite's period,
M = 5.98×1024 kg be the mass of the Earth,
G = 6.674×10-11 m3kg-1s-2 be the gravitational constant,
R (to be calculated) be the radius of the satellite's orbit,
v (unknown) be the satellite's velocity.
The satellite's centripetal acceleration
v²/R
must equal its gravitational acceleration
GM/R²
The reason is that the centripetal acceleration is caused by gravity.
The velocity, v, is distance divided by time, i.e.,
v = 2πR/T
By setting the two accelerations equal we get
(2πR)²/T²R = GM/R²
R = (GMT²/4π²)1/3
Before substituting numbers into the above, let's calculate the dimensions:
(m3kg-1s-2 kg s²/4π²)1/3 = m
So we will get the final answer in meters.
Now substitute actual numbers
R = (6.674×10-11 × 5.98 × 1024 × 43200² / 4π²)1/3 = 26.62 x 106 m
So the radius of the satellite's orbit is about 26,620 km,
which approximately 20,000 km above the surface of the Earth.