Hint: The gravitational force provides the required centripetal force for the satellite.
Consider the diagram, where a satellite of mass m is moving around the earth in a circular orbit of radius R.
Step 1: Find the kinetic energy of the satellite.
The orbital speed of the satellite orbiting the earth is given by, v0=√GMR
where M and R are the mass and radius of the earth.
(a) ∴ KE of a satellite of mass m,
EK=12mv20=12m×GMR
EK∝1R
lt means the KE decreases exponentially with radius.
The graph for KE versus orbital radius R is shown in the figure.
Step 2: Find the potential energy of the satellite.
(b) Potential energy of a satellite,
Ep=−GMmR
Ep∝−1R
The graph for PE versus orbital radius R is shown in the figure.
Step 3: Find the total energy of the satellite.
(c) Total energy of the satellite,
E=EK+Ep=GMm2R−GMmR=−GMm2R
The graph for total energy versus orbital radius R is shown in the figure.