Answer:
v = 1630 m/s
T = 5.78 x 10^5 s
Step-by-step 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:
![G(Mm)/((R+h)^2)=m(v^2)/(R+h)](https://img.qammunity.org/2020/formulas/physics/high-school/ugrnqts3gxg8wivljf5xlx0nkr19b1heoi.png)
where
G is the gravitational constant
M=5.97 x 1024kg is the Earth's mass
m is the satellite's mass
is the Earth's radius
is the altitude of the satellite
v is the speed of the satellite
Solving for v,
![v=\sqrt{(GM)/(R+h)}=\sqrt{((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](https://img.qammunity.org/2020/formulas/physics/middle-school/2o0irmovvn6mfhlibvpu543ad1divp0z03.png)
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:
![T=(2 \pi (R+h))/(v)=(2\pi (6.38\cdot 10^6 m+1.44\cdot 10^8 m))/(1630 m/s)=5.79\cdot 10^5 s](https://img.qammunity.org/2020/formulas/physics/middle-school/pw6thojwlq8wgeau7ciqcjbz8v0o34dg47.png)
So the correct answer is
v = 1630 m/s
T = 5.78 x 10^5 s