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Kepler's second law of planetary motion corresponds to
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The correct answer is:
conservation of angular momentum
From Kepler's second law of planetary motion,
$$
\frac{d L}{d t}=\frac{L}{2 m}
$$
Thus, angular monentum remains conserved.
$$
\frac{d L}{d t}=\frac{L}{2 m}
$$
Thus, angular monentum remains conserved.
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