The angular momentum of a planet of mass \( M \) moving around the sun in an elliptical orbit is \( \vec{L} \). The magnitude of the areal velocity of the planet is:
\( \dfrac{4L}{M} \)
\( \dfrac{2L}{M} \)
\( \dfrac{L}{2M} \)
\( \dfrac{L}{M} \)