Class 11 Physics: Gravitation Mock Test | Exam Style Test
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Gravitation Mock Test – Class 11 Physics

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Gravitation – Progressive Test

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1. The table compares horizontal launch speeds from the same high point above Earth, with air resistance neglected.

Case Speed condition Likely ideal result
P Too small for orbit Projectile returns to Earth
Q Suitable circular orbital speed Projectile keeps falling around Earth
R At least escape speed Projectile can escape Earth’s gravity well

The table is

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2. A body of mass is moved slowly from distance to distance from a planet’s centre. The work done by gravity is

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3. At a distance from Earth’s centre, the escape speed is related to Earth’s surface escape speed by

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4. Assertion: A mass placed at the centre of a square experiences zero net gravitational force if equal masses are placed at all four vertices. Reason: Forces due to opposite vertices are equal in magnitude and opposite in direction.

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5. The orbital speed of a geostationary satellite of orbital radius may be written as

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6. Assertion: A planet in an elliptical orbit moves faster when it is nearer the Sun. Reason: The line joining the planet and the Sun sweeps equal areas in equal time intervals.

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7. A graph is drawn with on the horizontal axis and surface gravity on the vertical axis for planets having the same radius . The expected graph is

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8. For a uniform solid sphere of radius , the gravitational field magnitude inside the sphere varies with distance from the centre as

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9. A student applies to a mountain height above Earth’s surface. The mistake is that the formula is meant for

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10. The following table compares two roles of mass.

Role Meaning Example relation
P. Inertial role Resistance to acceleration
Q. Gravitational role Participation in gravitational attraction

The table is

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11. A feather and a metal ball are dropped in a long vacuum tube near Earth. Their accelerations are equal mainly because

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12. The Moon produces noticeable tides on Earth mainly because

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13. Two planets move around the same star in nearly circular orbits. Planet has orbital radius , and planet has orbital radius . The ratio is

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14. The gravitational potential at the surface of a planet is , where . The escape speed from the surface is

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15. The table lists common errors and corrections.

Error Correction
P. Using altitude as orbital radius Use
Q. Treating and as the same quantity is universal; is local field or acceleration
R. Saying weightlessness means no gravity Apparent weight is zero in free fall, but gravity acts
S. Applying outside point-mass field inside uniform Earth Use the interior model and its condition

The table is

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16. A pair of masses is moved slowly from separation to separation . The work done by gravitational force during this motion is

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17. Two ideas are compared for an orbiting satellite: “free fall” and “no gravity.” The correct comparison is that

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18. Using , Earth’s escape speed can also be written as

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19. Gravitation is best described as the interaction by which

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20. A satellite in a circular orbit of radius has its speed increased to , where is the circular speed at that radius. Its speed at infinity, if it escapes, is

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21. A person of mass stands on a weighing machine inside a lift falling freely with acceleration . The reading of the weighing machine is

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22. A satellite in circular orbit is moved to a higher circular orbit. During this change, the final circular orbital speed is smaller, but external energy must be supplied. This is because the higher orbit has

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23. A satellite is moving in a circular orbit. The gravitational force on it does no work over one complete revolution because

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24. A graph is drawn for a fixed arrangement of several source masses. The horizontal axis is the test mass , and the vertical axis is the net gravitational force magnitude on it. If the source masses and distances are unchanged, the graph should be

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25. A planet has radius and uniform density . The escape speed from its surface is proportional to

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26. A thin uniform spherical shell has mass and radius . A small body is placed at a distance from the shell’s centre. The shell’s gravitational effect on the body is equivalent to

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27. A planet has times Earth’s mass and times Earth’s radius. If Earth’s escape speed is , the planet’s escape speed is

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28. A satellite is in a circular orbit of radius . Its kinetic energy is . If the satellite is shifted to a circular orbit of radius , its new kinetic energy is

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29. A astronaut is in a satellite where the local gravitational field is . If the astronaut is freely orbiting with the satellite, the gravitational force and apparent weight are respectively

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30. A satellite is in a circular orbit of radius . The engine supplies energy equal to half the satellite’s binding energy while the satellite is still at the same radius. Its total mechanical energy becomes

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31. Two masses and are separated by . Taking , their gravitational potential energy is closest to

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32. Four point masses are placed at the corners of a square of side . In cyclic order, the masses are , , , and . The gravitational potential at the centre of the square is

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33. In a uniform solid Earth model, the gravitational potential is most negative at

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34. The value of is very small. This explains why

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35. A satellite is shifted from a circular orbit of radius to a circular orbit of radius around the same planet. Its total mechanical energy changes from to

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36. The following table compares two causes of latitude variation in .

Cause Effect at equator Effect at poles
P. Rotation Maximum reduction in effective No rotational reduction
Q. Oblate shape Larger radius gives smaller Smaller radius gives larger

The table is

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37. A satellite’s orbital radius is doubled. The ratio of its new orbital speed, escape speed from that radius, and period to their original values is

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38. A planet has density and radius . Planet has density and radius . The ratio of their escape speeds is

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39. The conservation idea most closely linked with Kepler’s second law is conservation of

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40. A graph-like description says: the vertical axis represents area swept by the Sun-planet line, and the horizontal axis represents time. For one planet in its orbit, Kepler’s second law predicts a graph that is

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41. For two spherical bodies separated by a gap, the distance in the gravitational force formula is measured

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42. Assertion: The gravitational field inside a thin uniform spherical shell is zero everywhere. Reason: At an interior point, vector contributions from different parts of the shell cancel due to spherical symmetry.

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43. At a height above Earth’s surface, the distance from Earth’s centre to a body is

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44. A body is fired from Earth’s surface with speed , and at infinity its speed is , where is Earth’s escape speed. The launch speed is

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45. A satellite moves in a circular orbit of radius with total energy . If its radius is decreased to , its new total energy is

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46. A satellite formula uses , while a height description gives . For a satellite at height above Earth’s surface, the correct substitution in is

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47. A point has two gravitational field contributions, east and north. The resultant field magnitude is

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48. The SI unit of gravitational field intensity can be written as

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49. A line graph of against for satellites around a planet has a smaller slope than the same type of graph for satellites around another planet. The first planet must have

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50. Use the arrangement described below. The Moon is to the right of Earth. Point P is on Earth’s surface nearest the Moon, Point Q is at Earth’s centre, and Point R is on the far side. The Moon’s gravitational pull is strongest at

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