Accorrding to Kepler, the period of revolution of a planet (T) and its mean distance from the Sun ® related by the equation.

Accorrding to Kepler, the period of revolution of a planet (T) and its

1.	Accorrding to Kepler, the period of revolution of a planet (T) and its mean distance from the Sun ® related by the equation.
Answer» `T^(3)a^(3)` = CONSTANT `T^(2)a^(-3)`=constant `TA^(3)`=constant `T^(2)a`=constant Solution :`(T^(2))/(a^(3))` = constant , `T^(2) a^(-3)` = constant