The figure shows elliptical orbit of a planet m about the sun S. The shaded area SCD is twice the shaded area SAB. If t1 is the time for the planet to move from C to D and t2 is the time to move from A to B, then
Key Concept: Kepler’s 2nd Law of planetary motion - A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time. |