Grigoriy S. answered 12/17/21
AP Physics / Math Expert Teacher With 40 Years of Proven Success
Because only one force acts on the satellite - gravitational force of attraction from the Earth
ac = g
Centripetal acceleration
ac = v2 / r
For velocity we can use the formula
v = 2πr / T (1)
Hence,
ac = 4π2r / T2 (2)
At any height acceleration due to gravity
g = G M / r 2 ,
where
r = R + h - radius of the satellite orbit with respect to the center of Earth.
On the Earth surface h = 0
g0 = GM / R2 = 9.8 m/s2
From here
GM = g0R2
Then for g I have
g = g0R2 / r2
Combining with (2), we get
4π2r / T2 = g0R2 / r2
Then
r3 = g0R2T2 / 4π2
But numerical value of π2 and g0 the same and I can write
π2 ≡ g0
So,
r3 = R2T2 / 4
Then to find r we need to take cubic root from both parts
r = (R2T2 / 4) 1/3
If we put the values, we will obtain
r = ( (6.38 x 10 6)2∙(8.64 x 104)2) / 4 ) 1/3 = 42.4 x 106 (m)
Or
r = 42, 400 km.
Subtracting the the radius of the Earth, we will have
h = 3.6 x 10 7 m
The speed of the satellite we find by substituting all known values to (1)
v = 2∙3.14∙42.4 x 106 m / 8.64 x 104 s = 3.1x103 m/s
Or v = 3.1 km/s