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Two particles of equal mass m go around a circle of radius R under the action of their mutual gravitational attraction. The speed of each particle with respect to their centre of

1) \(\begin{array}{l}\sqrt{\frac{Gm}{R}}\end{array} \) 2) \(\begin{array}{l}\sqrt{\frac{Gm}{4R}}\end{array} \) 3) \(\begin{array}{l}\sqrt{\frac{Gm}{3R}}\end{array} \) 4) \(\begin{array}{l}\sqrt{\frac{Gm}{2R}}\end{array} \) Answer: 2) \(\begin{array}{l}\sqrt{\frac{Gm}{4R}}\end{array} \) Solution: \(\begin{array}{l}\frac{Gm^{2}}{(2R)^{2}}=m\omega^{2}R\end{array} \)   \(\begin{array}{l}\frac{Gm^{2}}{4R^{3}}= \omega^{2}\end{array} \)   \(\begin{array}{l}\omega=\sqrt{\frac{Gm}{4R^{3}}}\end{array} \)... View Article

Two stars of masses m1 and m2 are in mutual interaction and revolving in orbits of radii r1 and r2 respectively. The time period of revolution for this system will be?

a. \(\begin{array}{l}2\pi \sqrt{\frac{(r_{1}-r_{2})^{3}}{G(m_{1}+m_{2})}}\end{array} \) b. \(\begin{array}{l}2\pi \sqrt{\frac{(r_{1}+r_{2})^{3}}{G(m_{1}+m_{2})}}\end{array} \) c. \(\begin{array}{l}2\pi \sqrt{\frac{(r_{1}-r_{2})^{3}}{G(m_{1}-m_{2})}}\end{array} \) d. \(\begin{array}{l}2\pi \sqrt{\frac{(r_{1}+r_{2})^{3}}{G(m_{1}-m_{2})}}\end{array} \) Solution: Answer: (b) Let... View Article