A planet moving along an elliptical orbit is closest to the sun at a distance r1 and farthest away at a distance of r2. If v1 and v2 are the linear velocities at these points respectively, then the ratio v1v2 is :
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a planet moving along an elliptical orbit is closest to the sun at a distance r1 and farthest away at a distance of r2. If V1 and V2 are the linear velocity of the points respectively then ratio V1V2 is:
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