3. Deduce from the orbit equation (1 + e)ro 1 + e cos 0 that a planet is closest to its sun when 0 = 0 and show that r = r at that time.

Algebra & Trigonometry with Analytic Geometry
13th Edition
ISBN:9781133382119
Author:Swokowski
Publisher:Swokowski
Chapter7: Analytic Trigonometry
Section7.6: The Inverse Trigonometric Functions
Problem 37E
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3. Deduce from the orbit equation
(1 + e)ro
1 + e cos 0
that a planet is closest to its sun when 0
= 0 and show that r = r
at that time.
Transcribed Image Text:3. Deduce from the orbit equation (1 + e)ro 1 + e cos 0 that a planet is closest to its sun when 0 = 0 and show that r = r at that time.
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