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 \(v_B\). - \( v_A = 3v \) - \( r_A = 4R \) - \( r_B = R \) \[ \frac{v_B}{3v} = \sqrt{\frac{4R}{R}} = \sqrt{4} = 2 \] \[ v_B = 2 \times (3v) = 6v \]
Net gravitational force at the center of a square is found to be \( F_1 \) when four particles having masses \( M, 2M, 3M \) and \( 4M \) are placed at the four corners of the square as shown in figure, and it is \( F_2 \) when the positions of \( 3M \) and \( 4M \) are interchanged. The ratio \( \dfrac{F_1}{F_2} = \dfrac{\alpha}{\sqrt{5}} \). The value of \( \alpha \) is 
