A thin rod of length \(L\) is bent to form a circle. Its mass is \(M\). What force will act on the mass \(m\) placed at the centre of the circle?
1. \(\frac{4\pi^2 GMm}{L^2}\)
2. \(\frac{GMm}{4\pi^2 L^2}\)
3. \(\frac{2\pi GMm}{L^2}\)
4. zero
View Answer
Due to the symmetrical distribution of mass in a circular ring, the gravitational field at the center is zero. Therefore, the force on any mass placed at the center is zero.
Two bodies of masses \(m\) and \(M\) are placed at distance \(d\) apart. What is the gravitational potential (\(V\)) at the position where the gravitational field due to them is zero is \(V\) :
1. \(V = -\frac{G}{d}(m+M)\)
2. \(V = -\frac{G}{d} m\)
3. \(V = -\frac{GM}{d}\)
4. \(V = -\frac{G}{d}(\sqrt{m}+\sqrt{M})^2\)
View Answer
Let the point of zero field be at distance \(r_1\) from \(m\) and \(r_2\) from \(M\). Then \(\frac{\sqrt{m}}{r_1} = \frac{\sqrt{M}}{r_2}\), with \(r_1 + r_2 = d\). Solving gives \(r_1 = \frac{\sqrt{m}d}{\sqrt{m}+\sqrt{M}}\) and \(r_2 = \frac{\sqrt{M}d}{\sqrt{m}+\sqrt{M}}\). Thus, \(V = -\frac{Gm}{r_1} - \frac{GM}{r_2} = -\frac{G}{d}(\sqrt{m}+\sqrt{M})^2\).
Two identical particles of combined mass \(M\), placed in space with certain separation, are released. Interaction between the particles is only of gravitational in nature and there is no external force present. Acceleration of one particle with respect to the other when separation between them is \(R\), has a magnitude :
1. \(\frac{GM}{2R^2}\)
2. \(\frac{GM}{R^2}\)
3. \(\frac{2GM}{R^2}\)
4. not possible to calculate due to lack of information
View Answer
Each particle has mass \(m = M/2\). The force is \(F = \frac{G m^2}{R^2} = \frac{GM^2}{4R^2}\). Acceleration of each is \(a = \frac{F}{m} = \frac{GM}{2R^2}\). Relative acceleration is \(a_{\text{rel}} = 2a = \frac{GM}{R^2}\).
Two concentric shells have mass \(M\) and \(m\) and their radii are \(R\) and \(r\) respectively, where \(R > r\). What is the gravitational potential at their common centre ?
1. \(-\frac{GM}{R}\)
2. \(-\frac{GM}{r}\)
3. \(-G\left[\frac{M}{R} - \frac{m}{r}\right]\)
4. \(-G\left[\frac{M}{R} + \frac{m}{r}\right]\)
View Answer
The potential at the center of a shell of mass \(M\) and radius \(R\) is \(-\frac{GM}{R}\). By superposition, the total potential at the common center is \(V = -\frac{GM}{R} - \frac{Gm}{r} = -G\left[\frac{M}{R} + \frac{m}{r}\right]\).
If three uniform spheres, each having mass \(M\) and radius \(R\), are kept in such a way that each touches the other two, the magnitude of the gravitational force on any sphere due to the other two is
1. \(\frac{GM^2}{4r^2}\)
2. \(\frac{2GM^2}{r^2}\)
3. \(\frac{2GM^2}{4r^2}\)
4. \(\frac{\sqrt{3}GM^2}{4r^2}\)
View Answer
The distance between the centers of any two touching spheres is \(2R\). The gravitational force between any two is \(F = \frac{GM^2}{(2R)^2} = \frac{GM^2}{4R^2}\). The angle between the two forces acting on one sphere is \(60^\circ\). Net force is \(F_{\text{net}} = \sqrt{3}F = \frac{\sqrt{3}GM^2}{4R^2}\).