Answer :
The second satellite will orbit at a larger distance, as the satellite's distance from the planet's core is inversely proportional to the square of that distance.
The centripetal force, which is comparable to the gravitational attraction of the Earth to a satellite, causes it to orbit the planet, allowing us to write
GMm/[tex]r^{2}[/tex] = m[tex]v^{2}[/tex]/r
where
G stands for gravity constant.
The Earth's mass is M.
The mass of the satellite is m.
R is the satellite's separation from the planet's center.
The satellite's speed is v.
We can modify the formula to read as:
r = Gm/[tex]v^{2}[/tex]
As a result, we can see that the satellite's distance from the planet's core is inversely proportional to the square of that distance. This implies that the second satellite, which moves slower, will be farther out from the planet's center.
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