According to Kepler's second law of planetary motion, the magnitude of areal velocity \(\left(\frac{\Delta A}{\Delta t}\right)\) of a planet of mass '\(m\)' revolving around the sun is constant and is equal to ('\(p\)' is the linear momentum and '\(L\)' is the angular momentum)
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The area swept per unit time equals half of the angular momentum divided by the mass.