A satellite is revolving around the earth with speed v0If it is stopped suddenly, then with what velocity will the satellite hit the ground? (ve = escape velocity from the earth's surface)

1.  ve2 - v02

2.  ve2 - 2v02

3.  ve2 - 3v02

4.  ve2 - v022

Subtopic:  Orbital velocity |
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Two particles of mass \(m\) and \(4m\) are separated by a distance \(r.\) Their neutral point is at:
1. \(\frac{r}{2}~\text{from}~m\)
2. \(\frac{r}{3}~\text{from}~4m\)
3. \(\frac{r}{3}~\text{from}~m\)
4. \(\frac{r}{4}~\text{from}~4m\)

Subtopic:  Newton's Law of Gravitation |
 74%
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The potential energy of a satellite having mass \(m\) and rotating at a height of \(6.4\times 10^{6}~\text{m}\) from the Earth's surface is:
1. \(-0.5mg R_e\)
2. \(-mg R_e\)
3. \(-2mg R_e\)
4. \(4mg R_e\)

Subtopic:  Gravitational Potential Energy |
 63%
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A body of mass \(m\) is situated at a distance \(4R_e\) above the Earth's surface, where \(R_e\) is the radius of the Earth. What minimum energy should be given to the body so that it may escape? 
1. \(mgR_e\) 2. \(2mgR_e\)
3. \(\frac{mgR_e}{5}\) 4. \(\frac{mgR_e}{16}\)
Subtopic:  Gravitational Potential Energy |
 74%
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Two satellites \(S_1\) and \(S_2\) are revolving around a planet in coplanar and concentric circular orbits of radii \(R_1\) and \(R_2\) in the same direction respectively. Their respective periods of revolution are \(1\) hr and \(8\) hr. The radius of the orbit of satellite \(S_1\) is equal to \(10^4\) km. Find the relative speed when they are closest to each other. 
1. \(2\pi \times 10^4~\text{kmph}\)
2. \(\pi \times 10^4~\text{kmph}\)
3. \(\frac{\pi}{2} \times 10^4~\text{kmph}\)
4. \(\frac{\pi}{3} \times 10^4~\text{kmph}\)

Subtopic:  Kepler's Laws |
 56%
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The gravitational potential energy of an isolated system of three particles, each of mass \(m\) placed at three corners of an equilateral triangle of side \(l\) is: 
1. \(-Gm \over {l}^2\) 2. \(-Gm^2 \over 2{l}\)
3. \(-2Gm^2 \over {l}\) 4. \(-3Gm^2 \over {l}\)
Subtopic:  Gravitational Potential Energy |
 87%
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Three identical point masses, each of mass \(1\) kg lie at three points \((0,0)\), \((0,0.2~\text{m})\), \((0.2~\text{m}, 0)\). The net gravitational force on the mass at the origin is:
1. \(6.67\times 10^{-9}(\hat i +\hat j)~\text{N}\)
2. \(1.67\times 10^{-9}(\hat i +\hat j) ~\text{N}\)
3. \(1.67\times 10^{-9}(\hat i -\hat j) ~\text{N}\)
4. \(1.67\times 10^{-9}(-\hat i -\hat j) ~\text{N}\)

Subtopic:  Newton's Law of Gravitation |
 66%
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The figure shows a planet in an elliptical orbit around the sun (\(S\)). The ratio of the momentum of the planet at point \(A\) to that at point \(B\) is:

                              
1. \(\frac{r_1}{r_2}\)
2. \(\frac{r_{1}^{2}}{r_{2}^{2}}\)
3. \(\frac{r_2}{r_1}\)
4. \(\frac{r_{2}^{2}}{r_{1}^{2}}\)

Subtopic:  Kepler's Laws |
 59%
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If \(R\) is the radius of the orbit of a planet and \(T\) is the time period of the planet, then which of the following graphs correctly shows the motion of a planet revolving around the sun?

1.     2.
3. 4.  
Subtopic:  Kepler's Laws |
 79%
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If the speed of an artificial satellite revolving around the earth in a circular orbit be \(2 \over 3\) of the escape velocity from the surface of earth then its altitude above the surface of the earth is

1. \({4 \over 5 }R\) 2. \({2 \over 5 }R\)
3. \({1 \over 8 }R\) 4. \({3 \over 5 }R\)
Subtopic:  Satellite |
 54%
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