1. | \(\frac{\pi RG}{12g}\) | 2. | \(\frac{3\pi R}{4gG}\) |
3. | \(\frac{3g}{4\pi RG}\) | 4. | \(\frac{4\pi G}{3gR}\) |
1. | \(180 ~\text{N/kg}\) | 2. | \(0.05 ~\text{N/kg}\) |
3. | \(50 ~\text{N/kg}\) | 4. | \(20 ~\text{N/kg}\) |
Assuming the earth to be a sphere of uniform density, its acceleration due to gravity acting on a body:
1. | increases with increasing altitude. |
2. | increases with increasing depth. |
3. | is independent of the mass of the earth. |
4. | is independent of the mass of the body. |
Two planets are in a circular orbit of radius \(R\) and \(4R\) about a star. At a specific time, the two planets and the star are in a straight line. If the period of the closest planet is \(T,\) then the star and planets will again be in a straight line after a minimum time:
1. | \((4)^2T\) | 2. | \((4)^{\frac13}T\) |
3. | \(2T\) | 4. | \(8T\) |
The escape velocity from the Earth's surface is v. The escape velocity from the surface of another planet having a radius, four times that of Earth and same mass density is:
1. | 3v | 2. | 4v |
3. | v | 4. | 2v |
A particle of mass \(m\) is projected with a velocity, \(v=kV_{e} ~(k<1)\) from the surface of the earth. The maximum height, above the surface, reached by the particle is: (Where \(V_e=\) escape velocity, \(R=\) radius of the earth)
1. | \(\frac{R^{2}k}{1+k}\) | 2. | \(\frac{Rk^{2}}{1-k^{2}}\) |
3. | \(R\left ( \frac{k}{1-k} \right )^{2}\) | 4. | \(R\left ( \frac{k}{1+k} \right )^{2}\) |