A planet moving along an elliptical orbit is closest to the Sun at distance `r_(1)` and farthest away at a distance of `r_(2)`. If `v_(1)` and `v_(2)` are linear speeds at these points respectively. Then the ratio `(v_1)/(v_2)` is

A plenet moving along an elliptical orbit is closest to the sun at a distance r_(1) and farthest away at a distance of r_(2) . If v_(1) and v_(2) are the linear velocities at these points respectively, then the ratio (v_(1))/(v_(2)) is

A plenet moving along an elliptical orbit is closest to the sun at a distance r_(1) and farthest away at a distance of r_(2) . If v_(1) and v_(2) are the linear velocities at these points respectively, then the ratio (v_(1))/(v_(2)) is

A plenet moving along an elliptical orbit is closest to the sun at a distance r_(1) and farthest away at a distance of r_(2) . If v_(1) and v_(2) are the linear velocities at these points respectively, then the ratio (v_(1))/(v_(2)) is

A planet moves around the sun. It is closest to sun to sun at a distance d_(1) and have velocity v_(1) At farthest distance d_(2) its speed will be

A planet moves around the sun. It is closest to sun to sun at a distance d_(1) and have velocity v_(1) At farthest distance d_(2) its speed will be

A planet moves around the Sun. It is closest to Sun at a distant d_(1) and has velocity v_(1) and farthest with distance d_(2) , its speed at this point will be: