A satellite is moving  in a low nearly circular orbit around the earth. Its radius is roughly equal to that of the earth's radius \(R_e\). By firing rockets attached to it, its speed is instantaneously increased in the direction of its motion so that is become \(\sqrt{\frac{3}{2}}\) times larger. Due to this the farthest distance from the centre of the earth that the satellite reaches is \(R\). Value  of \(R\) is ? 
1. \( 2 R_e \)
2. \( 2.5 R_e \)
3. \( 3 R_e \)
4. \( 4 R_e\)

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A satellite is in an elliptical orbit around a planet \(P\). It is observed that the velocity of the satellite when it is farthest from the planet is \(6\) times less than that when it is closest to the planet. The ratio of distances between the satellite and the planet at closest and farthest points is:
1. \(1:3\)
2. \(1:2\)
3. \(3:4\)
4. \(1:6\)

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Consider two satellites, \(S_1\) and \(S_2,\) with periods of revolution \(1~\text{hr}\) and \(8~\text{hr},\) respectively revolving around a planet in circular orbits. The ratio of the angular velocity of the satellite \(S_1\) to the angular velocity of the satellite \(S_2\) is:
1. \(8:1\)
2. \(1:4\)
3. \(2:1\)
4. \(1:8\)

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Two satellites A and B of masses \(200\) kg and \(400\) kg are revolving round the earth at height of \(600\) km and \(1600\) km respectively. If \(T_A\) and \(T_B\) are the time periods of \(A\) and \(B\) respectively then the value of \(T_B-T_A\) is: 

  

[Given : radius of earth = \(6400\) km, mass of earth = \(6\times 10^{24}\)]
1. \( 1.33 \times 10^3 \mathrm{~s} \)
2. \( 3.33 \times 10^2 \mathrm{~s} \)
3. \( 4.24 \times 10^3 \mathrm{~s} \)
4. \( 4.24 \times 10^2 \mathrm{~s}\)

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Two satellites, \(A\) and \(B,\) have masses in the ratio of \(4:3\) and are revolving in circular orbits with radii \(3r\) and \(4r\) respectively around the Earth. The ratio of the total mechanical energy of the satellite \(A\) to that of the satellite \(B\) is:
1. \(9:16\)
2. \(16:9\)
3. \(1:1\)
4. \(4:3\)
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Given below are two statements:
Statement I: If total energy of a satellite revolving around earth in circular path is \(E\), then potential energy of satellite is \(2E.\)
Statement II: Kinetic energy is also twice of total energy.
 
1. Statement I is incorrect and Statement II is correct.
2. Both Statement I and Statement II are correct.
3. Both Statement I and Statement II are incorrect.
4. Statement I is correct and Statement II is incorrect.
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If the time period for one revolution by satellite near the Earth’s surface is \(T,\) then, the time period of revolution of the satellite at a height equal to the radius of the Earth will be:
1. \(\sqrt 8 ~T\) 2. \(\sqrt 2 ~T\)
3. \(\sqrt 4 ~T\) 4. \(\sqrt 3 ~T\)
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Suppose a situation in which two planet orbits around the sun in same orbit. If the mass of planet 1 is twice the mass of planet 2, then what do they have same? 
1. Potential energy 
2. Kinetic energy 
3. Total energy 
4. Velocity 
Subtopic:  Satellite |
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Correct formula for height of a satellite from earths surface is -
1. \(\left(\frac{\mathrm{T}^2 \mathrm{R}^2 \mathrm{~g}}{4 \pi^2}\right)^{1 / 3}-\mathrm{R}\)
2. \(\left(\frac{T^2 R^2 g}{4 \pi}\right)^{1 / 2}-R\)
3. \(\left(\frac{\mathrm{T}^2 \mathrm{R}^2}{4 \pi^2 \mathrm{~g}}\right)^{1 / 3}-{R}\)
4. \(\left(\frac{\mathrm{T}^2 {R}^2 \mathrm{~g}}{4 \pi}\right)^{-1 / 3}+{R}\)
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An astronaut takes a ball of mass m from earth to space. He throws the ball into a circular orbit about earth at an altitude of \(318.5\) km. From earth's surface to the orbit, the change in total mechanical energy of the ball is \(x \frac{\mathrm{GM}_{\mathrm{e}} \mathrm{~m}}{21 \mathrm{R}_{\mathrm{e}}}\). The value of \(x\) is (take \(R_e\text { = } 6370\) km) :
1. \(11\)
2. \(10\)
3. \(9\)
4. \(12\)
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