According to Kepler’s law the time period of a satellite varies with its radius as
According to Kepler’s law the time period of a satellite varies with its radius as
- A
${T^2} \propto {R^3}$
- B
${T^3} \propto {R^2}$
- C
${T^2} \propto (\frac{1}{R^3})$
- D
${T^3} \propto (\frac{1}{R^2})$
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