(a) [tex]2.09\cdot 10^6 m[/tex] above Earth's surface
The orbital speed of a satellite orbiting the Earth can be found using the equation
[tex]v=\sqrt{\frac{GM}{r}}[/tex]
where
G is the gravitational constant
[tex]M=5.98\cdot 10^{24} kg[/tex] is the Earth's mass
r is the radius of the satellite's orbit
The orbital speed can also be rewritten as the ratio between the circumference of the orbit and the orbital period, T:
[tex]\frac{2\pi r}{T}[/tex]
where
T = 129 min = 7740 s is the period
Combining the two equations,
[tex]\frac{2\pi r}{T}=\sqrt{\frac{GM}{r}}[/tex]
And solving for r,
[tex]\frac{(2\pi)^2 r^2}{T^2}=\frac{GM}{r}\\r=\sqrt[3]{\frac{GMT^2}{(2\pi)^2}}=\sqrt[3]{\frac{(6.67\cdot 10^{-11})(5.98\cdot 10^{24})(7740)^2}{(2\pi)^2}}=8.46\cdot 10^6 m[/tex]
This is, however, the orbital radius: this means we have to subtract the Earth's radius to find the altitude of the satellite, which is
[tex]R=6.37\cdot 10^6 m[/tex]
therefore, the altitude of the satellite is
[tex]h=r-R=8.46\cdot 10^6 - 6.37\cdot 10^6 =2.09\cdot 10^6 m[/tex]
b) [tex]5.57 m/s^2[/tex]
The value of g at the location of the satellite is given by
[tex]g=\frac{GM}{r^2}[/tex]
where:
G is the gravitational constant
[tex]M=5.98\cdot 10^{24} kg[/tex] is the Earth's mass
[tex]r=8.46 \cdot 10^6 m[/tex] is the radius of the satellite's orbit
Substituting into the equation, we find
[tex]g=\frac{(6.67\cdot 10^{-11})(5.98\cdot 10^{24})}{(8.46\cdot 10^6)^2}=5.57 m/s^2[/tex]