Answer:
v = 1630 m/s
T = 5.78 x 10^5 s
Explanation:
The tangential speed of the satellite can be found by requiring that the gravitational force on the satellite is equal to the centripetal force:
[tex]G\frac{Mm}{(R+h)^2}=m\frac{v^2}{R+h}[/tex]
where
G is the gravitational constant
M=5.97 x 1024kg is the Earth's mass
m is the satellite's mass
[tex]R=6.38 \cdot 10^6 m[/tex] is the Earth's radius
[tex]h=1.44\cdot 10^8 m[/tex] is the altitude of the satellite
v is the speed of the satellite
Solving for v,
[tex]v=\sqrt{\frac{GM}{R+h}}=\sqrt{\frac{(6.67\cdot 10^{-11})(5.97\cdot 10^{24}kg)}{6.38\cdot 10^6 m+1.44\cdot 10^8 m}}=1627 m/s \sim 1630 m/s[/tex]
And the period of the orbit is equal to the ratio between the distance covered during one revolution (the circumference of the orbit) and the speed:
[tex]T=\frac{2 \pi (R+h)}{v}=\frac{2\pi (6.38\cdot 10^6 m+1.44\cdot 10^8 m)}{1630 m/s}=5.79\cdot 10^5 s[/tex]
So the correct answer is
v = 1630 m/s
T = 5.78 x 10^5 s