Initially:
Star A has mass \( M_A \), and star B has mass \( M_B = 2M_A \), both having the same radius \( R \).
Due to an interaction process, star A loses some of its mass and radius becomes smaller. Let the new mass of star A be \( M_A' \). The density of star A remains the same in both cases.
Initially, the density of star A is: \[ \rho_A = \frac{M_A}{\frac{4}{3} \pi R^3} \]
Finally, the density of star A is: \[ \rho_A = \frac{M_A'}{\frac{4}{3} \pi (R')^3} \]
Since density remains the same: \[ \frac{M_A}{\frac{4}{3} \pi R^3} = \frac{M_A'}{\frac{4}{3} \pi (R')^3} \Rightarrow 8M_A' = M_A \]
Therefore, the lost mass by star A is: \[ A = M_A - M_A' = M_A - \frac{M_A}{8} = \frac{7M_A}{8} \] This lost mass is attached to star B, and the radius of star B changes to \( R_2 \).
Finally:
The density of the removed part from star A is: \[ \rho_A = \frac{\frac{7M_A}{8}}{\frac{4}{3} \pi (R^3 - (R_2)^3)} \]
The density of the added part in star B remains the same as \( \rho_A \), so we get: \[ \frac{\frac{7M_A}{8}}{\frac{4}{3} \pi (R^3 - (R_2)^3)} = \frac{\frac{7M_A}{8}}{\frac{4}{3} \pi (R_2^3 - R^3)} \]
Solving for \( R_2 \): \[ R_2 = 15^{1/3} R \]
Escape Velocity:
Escape velocity from star A after interaction is: \[ V_A = \sqrt{\frac{2GM_A}{R/2}} \]
Escape velocity from star B after interaction is: \[ V_B = \sqrt{\frac{2G(23M_A/8)}{15^{1/3} R}} \]
The ratio of escape velocities is: \[ \frac{V_B}{V_A} = \sqrt{\frac{23}{15}} \times \frac{M_A}{8} \Rightarrow \frac{V_B}{V_A} = 10n \quad \text{(where n = 2.3)} \]
Final Answer:
The value of \( n \) is \( \boxed{2.3} \).
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 

Let $ P(x_1, y_1) $ and $ Q(x_2, y_2) $ be two distinct points on the ellipse $$ \frac{x^2}{9} + \frac{y^2}{4} = 1 $$ such that $ y_1 > 0 $, and $ y_2 > 0 $. Let $ C $ denote the circle $ x^2 + y^2 = 9 $, and $ M $ be the point $ (3, 0) $. Suppose the line $ x = x_1 $ intersects $ C $ at $ R $, and the line $ x = x_2 $ intersects $ C $ at $ S $, such that the $ y $-coordinates of $ R $ and $ S $ are positive. Let $ \angle ROM = \frac{\pi}{6} $ and $ \angle SOM = \frac{\pi}{3} $, where $ O $ denotes the origin $ (0, 0) $. Let $ |XY| $ denote the length of the line segment $ XY $. Then which of the following statements is (are) TRUE?
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].