Please, find the speed of a satellite in orbit 265 km above the surface and the period of the satellite.
The second Newton's law for satellite:
M a = G M e M ( R + h ) 2 M a = G \frac {M _ {e} M}{(R + h) ^ {2}} M a = G ( R + h ) 2 M e M a = G M e ( R + h ) 2 a = G \frac {M _ {e}}{(R + h) ^ {2}} a = G ( R + h ) 2 M e
Where a a a is the centripetal acceleration:
v 2 R + h = G M e ( R + h ) 2 \frac {v ^ {2}}{R + h} = G \frac {M _ {e}}{(R + h) ^ {2}} R + h v 2 = G ( R + h ) 2 M e
So, satellite's speed:
v = G M e R + h v = \sqrt {G \frac {M _ {e}}{R + h}} v = G R + h M e
Using g = G M e R 2 → G M e = g R 2 g = G\frac{M_e}{R^2} \rightarrow GM_e = gR^2 g = G R 2 M e → G M e = g R 2
v = R g R + h v = R \sqrt {\frac {g}{R + h}} v = R R + h g v = 6.4 ∗ 1 0 6 m 10 m / s 2 6.4 ∗ 1 0 6 m + 0.265 ∗ 1 0 6 m = 7.84 ∗ 1 0 3 m / s v = 6.4 * 10^{6} m \sqrt {\frac {10 m / s ^ {2}}{6 . 4 * 1 0 ^ {6} m + 0 . 2 6 5 * 1 0 ^ {6} m}} = 7. 8 4 * 1 0 ^ {3} m / s v = 6.4 ∗ 1 0 6 m 6.4 ∗ 1 0 6 m + 0.265 ∗ 1 0 6 m 10 m / s 2 = 7.84 ∗ 1 0 3 m / s
Satellite's period:
T = 2 π ( R + h ) v T = \frac {2 \pi (R + h)}{v} T = v 2 π ( R + h ) T = 2 ∗ 3.14 ∗ ( 6.4 ∗ 1 0 6 m + 0.265 ∗ 1 0 6 m ) 7.84 ∗ 1 0 3 m / s = 5.34 ∗ 1 0 3 s T = \frac {2 * 3 . 1 4 * (6 . 4 * 1 0 ^ {6} m + 0 . 2 6 5 * 1 0 ^ {6} m)}{7 . 8 4 * 1 0 ^ {3} m / s} = 5. 3 4 * 1 0 ^ {3} s T = 7.84 ∗ 1 0 3 m / s 2 ∗ 3.14 ∗ ( 6.4 ∗ 1 0 6 m + 0.265 ∗ 1 0 6 m ) = 5.34 ∗ 1 0 3 s
Answer: v = 7.84 ∗ 1 0 3 m/s , T = 5.34 ∗ 1 0 3 s v = 7.84 * 10^{3} \, \text{m/s}, T = 5.34 * 10^{3} \, \text{s} v = 7.84 ∗ 1 0 3 m/s , T = 5.34 ∗ 1 0 3 s