1) Step 1: Find the orbital velocity of the satellite.
Given:
Mass of earth = M
Radius of orbite of satellite = R
Mass of satellite = m
Let's denote the orbital velocity of the satellite as
v∘.
Now as we know, in equilibrium, the gravitational pull provides the necessary centripetal force i.e., force of gravity
(Fg) is equal to the centripetal force
(Fc).
Therefore,
Centripetal Force
(Fc)=mv20r ....(i)
Force of gravity
(Fg)=GMmr2 ....(ii)
From equation
(i) & (ii)
Fg=Fc
We have,
mv20r=GMmr2
Therefore, orbital velocity of the body
(satellite) is given by,
v∘=√GMr=√GMR
Step 2: Find the kinetic Energy of the satellite.
As we know,
K.E=12mv20
By putting the values of
v∘ in K.E,
we get,
K.E=12m.GMR
K.E=GMm2R
Therefore, as per the equation, kinetic energy is inversely proportional to
R.
K.E∝1R
Step 3: Draw KE vs orbital radius (R) graph.
2) Step 1: Find the relation between potential energy and orbital radius.
As we know,
Gravitational potential energy of the body,
U=−GMmr
U∝−1r
Therefore, when
r invreases,
PE becomes less negative i.e., increases.
Step 2: Draw P.E vs. orbital radius R graph.
3) Step 1: Find the equation of total Energy.
As we know,
T.E.=K.E.+P.E.
Therefore,
T.E=GMm2R+(−GMmR)
T.E=−GMm2R
This shows,
T.E∝1R
Step 2: Draw T.E vs orbital radius R graph.