Kepler's third law of planetary motion when stated for circular orbits, has the form (v =…
Physics · NEET · NTA Exams — Gravitation
Kepler's third law of planetary motion when stated for circular orbits, has the form (v = orbital velocity of a planet and R = distance from the Sun)
- \(\text { væ R }\)
- \(\mathrm{v} \times 1 / \mathrm{R}\)
- \(\mathrm{v}^{2}=1 / \mathrm{R}\)
- none of the above
Answer
(C) v ^ 2 =1 / R
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