The minimum and maximum distances of a planet revolving around the Sun are \( x_1 \) and \( x_2 \). If the minimum speed of the planet on its trajectory is \( v_0 \) then its maximum speed will be
\( \dfrac{v_0 x_1^2}{x_2^2} \)
\( \dfrac{v_0 x_1}{x_2} \)
\( \dfrac{v_0 x_2}{x_1} \)
\( \dfrac{v_0 x_2^2}{x_1^2} \)