A planet revolves around the sum in an elliptical orbit of eccentricity e.If T is the time period of the planet, then the time spent by the planet between the ends of the planet between the ends of the minor axis close to the sun is

Question

$$(a)\;T\bigg [\frac{1}{4}-\frac{e}{2 \pi}\bigg] \quad (b)\;\frac{Te}{\pi} \quad (c)\;\bigg(\frac{e}{\pi}-1\bigg) T \quad (d)\;\frac{T \pi}{e}$$