Step 1: State the formula for the orbital velocity of a satellite. The velocity (\(v\)) of a satellite in a circular orbit of radius \(r\) around a planet of mass \(M\) is given by equating the gravitational force to the centripetal force: \[ \frac{GMm}{r^2} = \frac{mv^2}{r} $\Rightarrow$ v = \sqrt{\frac{GM}{r}} \] This shows that the orbital velocity is inversely proportional to the square root of the orbital radius: \( v \propto \frac{1}{\sqrt{r}} \).
Step 2: Set up a ratio for the two satellites A and B. \[ \frac{v_B}{v_A} = \frac{\sqrt{GM/r_B}}{\sqrt{GM/r_A}} = \sqrt{\frac{r_A}{r_B}} \]
Step 3: Substitute the given values and solve for \(v_B\). - \( v_A = 3v \) - \( r_A = 4R \) - \( r_B = R \) \[ \frac{v_B}{3v} = \sqrt{\frac{4R}{R}} = \sqrt{4} = 2 \] \[ v_B = 2 \times (3v) = 6v \]
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:
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: 



