Which of the following quantities does not depend upon the orbital radius of the satellite
$\frac{T}{R}$
$\frac{{{T^2}}}{R}$
$\frac{{{T^2}}}{{{R^2}}}$
$\frac{{{T^2}}}{{{R^3}}}$
Kepler discovered
Kepler's third law states that square of period of revolution $(T)$ of a planet around the sun, is proportional to third power of average distance $r$ between sun and planet i.e.
$\therefore \;{T^2} = k{r^3}$
here $K$ is constant.
If the masses of sun and planet are $M$ and $m$ respectively then as per Newton's law of gravitation force of attraction between them is $F = \frac{{GMm}}{{{r^2}}}$ , here $G$ gravitational constant . The relation between $G$ and $K$ is described as
A planet has orbital radius twice as the earth's orbital radius then the time period of planet is .......... $years$
The mean radius of the earth's orbit round the sun is $1.5 \times 10^{11}.$ The mean radius of the orbit of mercury round the sun is $6 \times10^{10}\,m.$ The mercury will rotate around the sun in
During motion of a planet from perihelion to aphelion the work done by gravitational force of sun on it is ...........