A planet of mass `m` revolves in elliptical orbit around the sun of mass `M` so that its maximum and minimum distance from the sun equal to `r_(a)` and `r_(p)` respectively. Find the angular momentum of this planet relative to the sun.
A. `L=msqrt((GMr_(p)r_(a))/((r_(p)+r_(a))))`
B. `L=msqrt((2GMr_(p)r_(a))/((r_(p)+r_(a))))`
C. `L=Msqrt((GMr_(p)r_(a))/((r_(p)+r_(a))))`
D. `L=Msqrt(((r_(p)+r_(a)))/(GMr_(p)r_(a)))`