Gravitation PYQs - Last 10 Years
COMEDK / Physics / Mechanics / 29 recent questions
PhysicsMechanics2017-2026
Practice 29 COMEDK Physics questions from Gravitation. Use the year-wise and type-wise breakdown to prioritize recent PYQs, then continue into the question list below.
29
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Physics / Mechanics
2020-2026
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Based on indexed question metadata
25
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2022-2026
29
Last 10 Years
2017-2026
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MCQ100%
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25 in last 5 years29 in last 10 years
Last 10 Years Gravitation Questions
Showing 29 of 29 filtered questions.
1Gravitation
A body is projected vertically upwards from the surface of earth with a velocity ' $v$ ' to reach a height of $10 R$, where $R$ is the radius of the earth, then $v$ is
MCQ+1 / -02026
2Gravitation
Two spheres of masses $M_1$ and $M_2$ are in air separated by a distance of d m . The gravitational force of attraction between them is $F$. If the space around the masses is filled with a liquid of density $\rho$, the force between the mas...
MCQ+1 / -02026
3Gravitation
Two particles, one heavy and the other light, placed at 50 cm from each other, are under the influence of gravitational force of one another. If mass of the heavier particle is 4 kg and its acceleration under the influence of gravitational ...
MCQ+1 / -02026
4Gravitation
Two neutral bodies of masses $m_1$ and $m_2$ are kept at a distance of $r \mathrm{~cm}$ from one another in a vacuum medium. A gravitational force Fracts between the two bodies. The entire set-up is then transferred, as it is, to a water me...
MCQ+1 / -02026
5Gravitation
A planet is 121 times heavier than moon and has a diameter 9 times that of moon. If the escape velocity on the planet is $v$, then the escape velocity on the moon will be:
MCQ+1 / -02025
6Gravitation
The radius of earth is $R$ and acceleration due to gravity on its surface is $g$. The height at which the acceleration due to gravity becomes $\frac{g}{8}$ is:
MCQ+1 / -02025
7Gravitation
If the distance between the Sun and Earth is doubled, then the duration of the year on earth will be :
[Given actual duration of the year $=\mathbf{T}$ ]
[Given actual duration of the year $=\mathbf{T}$ ]
MCQ+1 / -02025
8Gravitation
The unit of universal gravitational constant is :
MCQ+1 / -02025
9Gravitation
Two spherical planets P and Q have the same uniform density $\rho$, and masses Mp and $\mathrm{MQ}_{\mathrm{Q}}$ and surface areas A and 4 A respectively. Another spherical planet $R$ also has the same uniform density $\rho$, and its mass i...
MCQ+1 / -02025
10Gravitation
The value of universal gravitational constant was first determined by
MCQ+1 / -02025
11Gravitation
If the radius of earth were to shrink by two percent, its mass remaining the same, the acceleration due to gravity on the earth's surface would
MCQ+1 / -02025
12Gravitation
If the earth has a mass nine times and radius four times that of planet X, the ratio of the maximum speed required by a rocket to pull out of the gravitational force of planet \(\mathrm{X}\) to that of the earth is
MCQ+1 / -02024
13Gravitation
If \(\mathrm{A}\) is the areal velocity of a planet of mass \(\mathrm{M}\), then its angular momentum is
MCQ+1 / -02024
14Gravitation
A satellite is revolving around the earth in a circular orbit with kinetic energy of \(1.69 \times 10^{10} \mathrm{~J}\). The additional kinetic energy required for just escaping into the outer space is
MCQ+1 / -02024
15Gravitation
The acceleration due to gravity at pole and equator can be related as
MCQ+1 / -02024
16Gravitation
Energy required for moving a body of mass \(\mathrm{m}\) from a circular orbit of radius 3R to a higher orbit of radius 4R around the earth is.
MCQ+1 / -02024
17Gravitation
A planet has double the mass of the earth and double the radius. The gravitational potential at the surface of the Earth is \(\mathrm{V}\) and the magnitude of the gravitational field strength is \(\mathrm{g}\). The gravitational potential ...
MCQ+1 / -02024
18Gravitation
An uniform sphere of mass \(M\) and radius \(R\) exerts a force of \(F\) on a small mass \(m\) placed at a distance of 3R from the centre of the sphere. A spherical portion of diameter \(R\) is cut from the sphere as shown in the fig. The f...
MCQ+1 / -02023
19Gravitation
The acceleration due to gravity at a height of \(7 \mathrm{~km}\) above the earth is the same as at a depth d below the surface of the earth. Then d is
MCQ+1 / -02023
20Gravitation
The height vertically above the earth's surface at which the acceleration due to gravity becomes \(1 \%\) of its value at the surface is
MCQ+1 / -02023
21Gravitation
If escape velocity on earth surface is \(11.1 \mathrm{~kmh}^{-1}\), then find the escape velocity on moon surface. If mass of moon is \(\frac{1}{81}\) times of mass of earth and radius of moon is \(\frac{1}{4}\) times radius of earth.
MCQ+1 / -02023
22Gravitation
Starting from the centre of the earth having radius \(R\), the variation of \(g\) (acceleration due to gravity) is shown by
MCQ+1 / -02023
23Gravitation
The escape velocity of a projectile on the earth's surface is 11.2 km/s. A body is projected out with thrice this speed. The speed of the body far away from the earth will be
MCQ+1 / -02022
24Gravitation
The height at which the acceleration due to gravity becomes \(\frac{g}{16}\) (where, g = acceleration due to gravity on the surface of the earth) in terms of R is, if R is the radius of earth.
MCQ+1 / -02022
25Gravitation
If the earth were to spin faster, acceleration due to gravity at the poles
MCQ+1 / -02022
26Gravitation
A constant potential energy of a satellite is given as
\(\mathrm{PE}=r(\mathrm{KE})\)
whee, PE = potential energy
and KE = kinetic energy.
The value of \(r\) will be
\(\mathrm{PE}=r(\mathrm{KE})\)
whee, PE = potential energy
and KE = kinetic energy.
The value of \(r\) will be
MCQ+1 / -02021
27Gravitation
Kepler's second law of planetary motion corresponds to
MCQ+1 / -02021
28Gravitation
Two spherical bodies of masses M and 5M and
radii R and 2R are released in free space with
initial separation between their centres equal to
12 R. If they attract each other due to
gravitational force only, then the distance
covered by the ...
radii R and 2R are released in free space with
initial separation between their centres equal to
12 R. If they attract each other due to
gravitational force only, then the distance
covered by the ...
MCQ+1 / -02020
29Gravitation
A satellite can be in a geostationary orbit around a planet if it is at a distance R from the centre of the planet. If the planet starts rotating about its axis with double the angular velocity, then to make the satellite geostationary, its...
MCQ+1 / -02020
