(d) From Kepler’s third law of planetary motion, $\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ T^{2} \propto R^{3}$ $\Longrightarrow \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \frac{T^{2}}{R^{3}} = constant\ $
Physics Educator & NEET/JEE Specialist
Ph.D. in Physics with 19+ years of teaching experience.