The correct option is(A): \(\frac{4\pi^{2}}{GM_{S}}\).
Time period of a revolution of a planet,
\(T = \frac{2\pi r}{v} = \frac{2\pi r}{\sqrt{\frac{GM_{S}}{r}}} = \frac{2\pi r^{3/2}}{\sqrt{GM_{S}}}\)
where \(M_{S}\) is the mass of the sun
Squaring both sides, we get
\(T^{2} = \frac{4\pi^{2}r^{2}}{GM_{S}}\)
The graph between \(T^{2}\) and \(r^{3}\) is a straight line whose slope is \(\frac{4\pi^{2}}{GM_{S}}\)
A small point of mass \(m\) is placed at a distance \(2R\) from the center \(O\) of a big uniform solid sphere of mass \(M\) and radius \(R\). The gravitational force on \(m\) due to \(M\) is \(F_1\). A spherical part of radius \(R/3\) is removed from the big sphere as shown in the figure, and the gravitational force on \(m\) due to the remaining part of \(M\) is found to be \(F_2\). The value of the ratio \( F_1 : F_2 \) is: 
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:
In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.
According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,
On combining equations (1) and (2) we get,
F ∝ M1M2/r2
F = G × [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2
The dimension formula of G is [M-1L3T-2].