MCQOPTIONS
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| 1. |
According to Kepler, the period of revolution of a planet (T) and its mean distance from the sun (r) are related by the equation [EAMCET (Med.) 1995; MH CET 2000; Pb. PET 2001] |
| A. | \[{{T}^{3}}{{r}^{3}}=\] constant |
| B. | \[{{T}^{2}}{{r}^{-3}}=\]constant |
| C. | \[T{{r}^{3}}=\] constant |
| D. | \[{{T}^{2}}r=\] constant |
| Answer» C. \[T{{r}^{3}}=\] constant | |