Question:

In a planetary motion, the areal velocity of position vector of a planet depends on angular velocity ($ω$) and distance ($r$) of the planet from the sun. The correct relation for areal velocity $\fracdAdt$ is

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Kepler's second law: Areal velocity is constant for a planet, $\fracdAdt = \frac12 r² ω$.
Updated On: Apr 16, 2026
  • $\fracdAdt \propto ω r$
  • $\fracdAdt \propto ω r²$
  • $\fracdAdt \propto \frac\omegar²$
  • $\fracdAdt \propto \frac\omegar$
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The Correct Option is B

Solution and Explanation


Step 1:
Areal velocity $\fracdAdt = \frac12 r² ω$ (from $dA = \frac12 r² dθ$, $ω = dθ/dt$).

Step 2:
So $\fracdAdt \propto ω r²$.
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