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A planet moving along an elliptical orbit is closest to the Sun at distance r1 and farthest away at a distance of r2 If V1 and V2 are linear speeds at these points respectively. Then the ratio \(\frac {v_1}{v_2}\) is ……

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(a) \(\frac{r_1}{r_2}\)

According to the Law of conservation of angular momentum

mv1r1 = mv2r2; v1r1 = v2r2

\(\frac{v_1}{v_2}\) = \((\frac{r_2}{r_1})\)

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