Two satellites A andB are revolving around the earth in circular orbits of radius r1 and r2 respectively with r1<r2. Plane of motion of the two are same. At position 1, A is given an impulse in the direction of velocity by firing a rocket so that it follows an elliptical path to meet B at position 2 as shown. Focal length of the elliptical path are r1 and r2 respectively. At position 2, A is given another impulse so that velocities of A and B at 2 become equal and the two move together.
For any elliptical path of the satellite time period of revolution is given by Kepler's planetary law as T2∝r3 where a is semi major axis of the ellipse which is r1+r22 in this case. Also angular momentum of any satellite revolving around the Earth will remain a constant about Earth's centre as force of gravity on the satellite which keeps it in elliptical path is along its position vector relative to the earth centre.
If the two bodies have same mass then,