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7.Gravitation
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According to Kepler, the period of revolution of a planet $(T)$ and its mean distance from the sun $(r)$ are related by the equation
A
${T^3}{r^3} = $ constant
B
${T^2}{r^{ - 3}} = $ constant
C
$T{r^3} = $ constant
D
${T^2}r = $ constant
Solution
(b) $\frac{{{T^2}}}{{{r^3}}} = $ constant
$ \Rightarrow \,{T^2}{r^{ – 3}}$= constant
Standard 11
Physics
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