Question: Deduce from the orbit equation that a planet is closest to its sun when = 0 and show that r = r 0 at

Deduce from the orbit equationr = (1 + e)ro 1 + e cos 0


that a planet is closest to its sun when θ = 0 and show that r = r0 at that time.

r = (1 + e)ro 1 + e cos 0

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