The relative uncertainty in the period of a sateilite orbiting around the earth is $10^{-2}$. If the relative uncertainty in the radius of the orbit is negligible, the relative uncertainty in the mass of the earth is
$3\times 10^{-2}$
$10^{-2}$
$2\times 10^{-2}$
$6\times 10^{-2}$
Kepler discovered
According to Kepler, the period of revolution of a planet $(T)$ and its mean distance from the sun $(r)$ are related by the equation
A binary star system consists of two stars one of which has double the mass of the other. The stars rotate about their common centre of mass :-
A geostationary satellite is orbiting the earth at a height $5R$ above the surface of the earth , $R$ being the radius of the earth. The time period of another satellite in hours at a height of $2R$ from the surface of the earth is
If satellite is shifted towards the earth. Then time period of satellite will be