For a planet around the sun in an elliptical orbit of semi - major and semi - minor axes a and b, respectively and period T.
Keplers law of area
Areal velocity = Area swept Time =12r(rdθ)dt =12r2dθdt= constant
Hence, 12r2ω= constant
or mr2ω= constant
where mr2=M of the planet relative to Sun=I
Iω= constant or →L= constant
Hence, The angular momentum of the planet about the sun is constant