Q. 34 A star like the sun has several bodies moving around it at different distances. Consider that all of them are moving in circular orbits. Let r be the distance of a body from the centre of the star and let its linear velocity be v, angular velocity ω, kinetic energy K, gravitational potential energy U, total energy E & and angular momentum L. As the radius r of the orbit increases, determine which of the above quantities increases and which one decreases.

Hint: The kinetic energy, potential energy and angular momentum vary with the distance of the body from the star.
Step 1: Find the kinetic energy and the potential energy of the body.
The situation is shown in the diagram where a body of mass m is revolving around a star of mass M.
 
                                                    
 
The linear velocity of the body, v=GMr
                                           v1r
Therefore, when r increases, v decreases.
Angular velocity of the body, ω=2πkr3/2ω1r3/2                           ω=2πT
Therefore, when r increases, ω decreases.
The kinetic energy of the body, K=12mv2=12m×GMr=GMm2r
                                            K1r
Therefore, when r increases, KE decreases.
The gravitational potential energy of the body,
                    U=-GMmrU-1r
Therefore, when r increases, PE becomes less negative i.e., increases.
Step 2: Find the total energy of the body.
The total energy of the body, E=KE+PE=GMm2r+-GMmr=-GMm2r

Therefore, when r increases, the total energy becomes less negative i.e., increases.

Step 3: Find the angular momentum of the body.

Angular momentum of the body, L=mvr=mrGMr=mGMrLr

Therefore, when r increases, angular momentum L increases.