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A planet has a period of revolution about the Sun equal to and a mean distance from the Sun equal to R .T^2 varies directly as __________.
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A planet has a period of revolution about the Sun equal to and a mean distance from the Sun equal to R .T^2 varies directly as __________.

User Sharry
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T² caries directly as R³ .

This is Kepler's 3rd law of planetary motion .
User Champer Wu
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