Three equal masses \(m\) are placed at the three vertices of an equilateral triangle of sides \(r.\) The work required to double the separation between masses will be:

                      

1. \(Gm^2\over r\) 2. \(3Gm^2\over r\)
3. \({3 \over 2}{Gm^2\over r}\) 4. None of the above

Subtopic:  Gravitational Potential Energy |
 74%
Level 2: 60%+
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If the radius of a planet is \(R\) and its density is \(\rho,\) the escape velocity from its surface will be:
1. \(v_e\propto \rho R\)
2. \(v_e\propto \sqrt{\rho} R\)
3. \(v_e\propto \frac{\sqrt{\rho}}{R}\)
4. \(v_e\propto \frac{1}{\sqrt{\rho} R}\)

Subtopic:  Escape velocity |
 89%
Level 1: 80%+
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An artificial satellite moving in a circular orbit around the earth has a total (kinetic + potential) energy \(E_0.\) Its potential energy is:
1. \(-E_0\)
2. \(1.5E_0\)
3. \(2E_0\)
4. \(E_0\)
Subtopic:  Gravitational Potential Energy |
 82%
Level 1: 80%+
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A body weighs \(200\) N on the surface of the earth. How much will it weigh halfway down the centre of the earth?

1. \(100\) N 2. \(150\) N
3. \(200\) N 4. \(250\) N
Subtopic:  Acceleration due to Gravity |
 82%
Level 1: 80%+
NEET - 2019
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Radii and densities of two planets are \(R_1, R_2\) and \(\rho_1, \rho_2\) respectively. The ratio of accelerations due to gravity on their surfaces is:
1. \(\frac{\rho_1}{R_1}:\frac{\rho_2}{R_2}\)
2. \(\frac{\rho_1}{R^2_1}: \frac{\rho_2}{R^2_2}\)
3. \(\rho_1 R_1 : \rho_2R_2\)
4. \(\frac{1}{\rho_1R_1}:\frac{1}{\rho_2R_2}\)

Subtopic:  Acceleration due to Gravity |
 84%
Level 1: 80%+
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\(1\) kg of sugar has maximum weight:
1. at the pole.
2. at the equator.

3. at a latitude of \(45^{\circ}.\)
4. in India.

Subtopic:  Acceleration due to Gravity |
 81%
Level 1: 80%+
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A particle is located midway between two point masses each of mass \(M\) kept at a separation \(2d.\) The escape speed of the particle is:
(neglecting the effect of any other gravitational effect)

1. \(\sqrt{\frac{2 GM}{d}}\)
2. \(2 \sqrt{\frac{GM}{d}}\)
3. \(\sqrt{\frac{3 GM}{d}}\)
4. \(\sqrt{\frac{GM}{2 d}}\)

Subtopic:  Escape velocity |
 61%
Level 2: 60%+
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A planet is revolving around a massive star in a circular orbit of radius \(R\). If the gravitational force of attraction between the planet and the star is inversely proportional to \(R^3,\) then the time period of revolution \(T\) is proportional to:
1. \(R^5\)
2. \(R^3\)
3. \(R^2\)
4. \(R\)

Subtopic:  Satellite |
 67%
Level 2: 60%+
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Two satellites of Earth, \(S_1\), and \(S_2\), are moving in the same orbit. The mass of \(S_1\) is four times the mass of \(S_2\). Which one of the following statements is true?

1. The time period of \(S_1\) is four times that of \(S_2\).
2. The potential energies of the earth and satellite
in the two cases are equal.
3. \(S_1\) and \(S_2\) are moving at the same speed.
4. The kinetic energies of the two satellites are equal.

Subtopic:  Satellite |
 69%
Level 2: 60%+
AIPMT - 2007
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The figure shows the elliptical orbit of a planet \(m\) about the sun \({S}.\) The shaded area \(SCD\) is twice the shaded area \(SAB.\) If \(t_1\) is the time for the planet to move from \(C\) to \(D\) and \(t_2\) is the time to move from \(A\) to \(B,\) then:
                     

1. \(t_1=3t_2\) 2. \(t_1=4t_2\)
3. \(t_1=2t_2\) 4. \(t_1=t_2\)


Subtopic:  Kepler's Laws |
 73%
Level 2: 60%+
AIPMT - 2009
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