Physics Gravitation Kepler’s laws

The relation between the time period (T) of a planet around the sun and the radius of the circular orbit (r) is:

1
\(T^2 \propto r^3\)
2
\(T^3 \propto r^2\)
3
\(T \propto r\)
4
\(T \propto T^4\)

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