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 Page 1


EXERCISES 
For JEE Main 
  Subjective Questions  
  Newton's Law of Gravitation 
Q 1.  Two particles of masses 1.0 kg and 2.0 kg are placed at a separation of 50 cm. 
Assuming that the only forces acting on the particles are their mutual gravitation, find 
the initial accelerations of the two particles. 
Q 2.  Three particles A, B and C, each of mass m, are placed in a line with AB = BC = d. 
Find the gravitational force on a fourth particle P of same mass, placed at a distance d 
from the particle B on the perpendicular bisector of the line AC. 
Q 3.  Four particles having masses m, 2m, 3m and 4m are placed at the four corners of a 
square of edge a. Find the gravitational force acting on a particle of mass m placed at 
the centre. 
Q 4.  Three uniform spheres each having a mass M and radius a are kept in such a way that 
each touches the other two. Find the magnitude of the gravitational force on any of the 
spheres due to the other two. 
Q 5.  The figure shows a uniform rod of length l whose mass per unit length is ? . What is 
the gravitational force of the rod on a particle of mass m located a distance d from one 
end of the rod? 
 
  Acceleration due to Gravity 
Q 6.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value on the surface of a planet 
whose mass and radius both are two times that of earth. 
Q 7.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value : 
  (a) at height h = R from the surface,  
  (b) at depth h = 
R
2
from the surface. (R = radius of earth) 
Q 8.  Calculate the distance from the surface of the earth at which the acceleration due to 
gravity is the  same below and above the surface of the earth. 
Q 9.  A body is weighed by a spring balance to be 1000 N at the north pole. How much will 
it weight at  the equator. Account for the earth's rotation only. 
Q 10.  At what rate should the earth rotate so that the apparent g at the equator becomes zero 
? What will be the length of the day in this situation ? 
Q 11.  Assuming earth to be spherical, at what height above the north pole, value of g is 
same as that on the earth's surface at equator ? 
  Gravitational Field Strength and Potential 
Page 2


EXERCISES 
For JEE Main 
  Subjective Questions  
  Newton's Law of Gravitation 
Q 1.  Two particles of masses 1.0 kg and 2.0 kg are placed at a separation of 50 cm. 
Assuming that the only forces acting on the particles are their mutual gravitation, find 
the initial accelerations of the two particles. 
Q 2.  Three particles A, B and C, each of mass m, are placed in a line with AB = BC = d. 
Find the gravitational force on a fourth particle P of same mass, placed at a distance d 
from the particle B on the perpendicular bisector of the line AC. 
Q 3.  Four particles having masses m, 2m, 3m and 4m are placed at the four corners of a 
square of edge a. Find the gravitational force acting on a particle of mass m placed at 
the centre. 
Q 4.  Three uniform spheres each having a mass M and radius a are kept in such a way that 
each touches the other two. Find the magnitude of the gravitational force on any of the 
spheres due to the other two. 
Q 5.  The figure shows a uniform rod of length l whose mass per unit length is ? . What is 
the gravitational force of the rod on a particle of mass m located a distance d from one 
end of the rod? 
 
  Acceleration due to Gravity 
Q 6.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value on the surface of a planet 
whose mass and radius both are two times that of earth. 
Q 7.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value : 
  (a) at height h = R from the surface,  
  (b) at depth h = 
R
2
from the surface. (R = radius of earth) 
Q 8.  Calculate the distance from the surface of the earth at which the acceleration due to 
gravity is the  same below and above the surface of the earth. 
Q 9.  A body is weighed by a spring balance to be 1000 N at the north pole. How much will 
it weight at  the equator. Account for the earth's rotation only. 
Q 10.  At what rate should the earth rotate so that the apparent g at the equator becomes zero 
? What will be the length of the day in this situation ? 
Q 11.  Assuming earth to be spherical, at what height above the north pole, value of g is 
same as that on the earth's surface at equator ? 
  Gravitational Field Strength and Potential 
Q 12.  Two concentric spherical shells have masses m 1 ,m2 and radii R1, R2 (R1 < R2). 
Calculate the force exerted by this system on a particle of mass m, if it is placed at a 
distance 
12
(R R )
2
?
from the centre. 
Q 13.  Two spheres one of mass M has radius R. Another sphere has mass 4M and radius 2R. 
The centre to centre distance between them is 12R. Find the distance from the centre 
of smaller sphere where :  
  (a) net gravitational field is zero, 
  (b) net gravitational potential is half the potential on the surface of larger sphere. 
Q 14.  A semicircular wire has a length L and mass M. Find the gravitational field at the 
centre of the circle. 
Q 15.  A uniform solid sphere of mass M and radius a is surrounded symmetrically by a 
uniform thin spherical shell of equal mass and radius 2a. Find the gravitational field at 
a distance  
  (a) 
3
a
2
from the centre,   (b) 
5
a
2
 
from the centre. 
Q 16.  The density inside a solid sphere of radius a is given by ? = ?0a/r, where ?0
 
is the 
density at the surface and r denotes the distance from the centre. Find the gravitational 
field due to this sphere at a distance 2a from its centre. 
Q 17.  A particle of mass m is placed at the centre of a uniform spherical shell of same mass 
and radius R. Find the gravitational potential at a distance 
R
2
from the centre. 
  Gravitational Potential Energy 
Q 18.  A rocket is accelerated to speed v 2 gR ?
 
near earth's surface (R =radius of earth). 
Show that very far from earth its speed will be v 2gR ? .
 
 
Q 19.  Two neutron stars are separated by a distance of 10
10
 m. They each have a mass of 
10
30
 kg and a radius of 10
5
 m. They are initially at rest with respect to each other. 
  As measured from the rest frame, how fast are they moving when : 
  (a) their separation has decreased to one-half its initial value, 
  (b) they are about to collide. 
Q 20.  A projectile is fired vertically from earth's surface with an initial speed of 10 km/s. 
Neglecting air drag, how far above the surface of earth will it go ? 
Q 21.  A mass m is taken to a height R from the surface of the earth and then is given a 
vertical velocity v. Find the minimum value of v, so that mass never returns to the 
surface of the earth. 
  (Radius of earth is R and mass of the earth M). 
Q 22.  In the figure masses 400 kg and 100 kg are fixed. 
Page 3


EXERCISES 
For JEE Main 
  Subjective Questions  
  Newton's Law of Gravitation 
Q 1.  Two particles of masses 1.0 kg and 2.0 kg are placed at a separation of 50 cm. 
Assuming that the only forces acting on the particles are their mutual gravitation, find 
the initial accelerations of the two particles. 
Q 2.  Three particles A, B and C, each of mass m, are placed in a line with AB = BC = d. 
Find the gravitational force on a fourth particle P of same mass, placed at a distance d 
from the particle B on the perpendicular bisector of the line AC. 
Q 3.  Four particles having masses m, 2m, 3m and 4m are placed at the four corners of a 
square of edge a. Find the gravitational force acting on a particle of mass m placed at 
the centre. 
Q 4.  Three uniform spheres each having a mass M and radius a are kept in such a way that 
each touches the other two. Find the magnitude of the gravitational force on any of the 
spheres due to the other two. 
Q 5.  The figure shows a uniform rod of length l whose mass per unit length is ? . What is 
the gravitational force of the rod on a particle of mass m located a distance d from one 
end of the rod? 
 
  Acceleration due to Gravity 
Q 6.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value on the surface of a planet 
whose mass and radius both are two times that of earth. 
Q 7.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value : 
  (a) at height h = R from the surface,  
  (b) at depth h = 
R
2
from the surface. (R = radius of earth) 
Q 8.  Calculate the distance from the surface of the earth at which the acceleration due to 
gravity is the  same below and above the surface of the earth. 
Q 9.  A body is weighed by a spring balance to be 1000 N at the north pole. How much will 
it weight at  the equator. Account for the earth's rotation only. 
Q 10.  At what rate should the earth rotate so that the apparent g at the equator becomes zero 
? What will be the length of the day in this situation ? 
Q 11.  Assuming earth to be spherical, at what height above the north pole, value of g is 
same as that on the earth's surface at equator ? 
  Gravitational Field Strength and Potential 
Q 12.  Two concentric spherical shells have masses m 1 ,m2 and radii R1, R2 (R1 < R2). 
Calculate the force exerted by this system on a particle of mass m, if it is placed at a 
distance 
12
(R R )
2
?
from the centre. 
Q 13.  Two spheres one of mass M has radius R. Another sphere has mass 4M and radius 2R. 
The centre to centre distance between them is 12R. Find the distance from the centre 
of smaller sphere where :  
  (a) net gravitational field is zero, 
  (b) net gravitational potential is half the potential on the surface of larger sphere. 
Q 14.  A semicircular wire has a length L and mass M. Find the gravitational field at the 
centre of the circle. 
Q 15.  A uniform solid sphere of mass M and radius a is surrounded symmetrically by a 
uniform thin spherical shell of equal mass and radius 2a. Find the gravitational field at 
a distance  
  (a) 
3
a
2
from the centre,   (b) 
5
a
2
 
from the centre. 
Q 16.  The density inside a solid sphere of radius a is given by ? = ?0a/r, where ?0
 
is the 
density at the surface and r denotes the distance from the centre. Find the gravitational 
field due to this sphere at a distance 2a from its centre. 
Q 17.  A particle of mass m is placed at the centre of a uniform spherical shell of same mass 
and radius R. Find the gravitational potential at a distance 
R
2
from the centre. 
  Gravitational Potential Energy 
Q 18.  A rocket is accelerated to speed v 2 gR ?
 
near earth's surface (R =radius of earth). 
Show that very far from earth its speed will be v 2gR ? .
 
 
Q 19.  Two neutron stars are separated by a distance of 10
10
 m. They each have a mass of 
10
30
 kg and a radius of 10
5
 m. They are initially at rest with respect to each other. 
  As measured from the rest frame, how fast are they moving when : 
  (a) their separation has decreased to one-half its initial value, 
  (b) they are about to collide. 
Q 20.  A projectile is fired vertically from earth's surface with an initial speed of 10 km/s. 
Neglecting air drag, how far above the surface of earth will it go ? 
Q 21.  A mass m is taken to a height R from the surface of the earth and then is given a 
vertical velocity v. Find the minimum value of v, so that mass never returns to the 
surface of the earth. 
  (Radius of earth is R and mass of the earth M). 
Q 22.  In the figure masses 400 kg and 100 kg are fixed. 
 
  (a) How much work must be done to move a 1 kg mass from point A to point B ? 
(b) What is the minimum kinetic energy with which the 1 kg mass must be projected 
from A to the right to reach the point B ? 
  Planets and Satellites : Kepler's Law 
Q 23.  A sky lab of mass 2 x 10
3
 kg is first launched from the surface of earth in a circular 
orbit of radius 2R and then it is shifted from this circular orbit to another circular orbit 
of radius 3R. Calculate the energy required: 
  (a) to place the lab in the first orbit, 
  (b) to shift the lab from first orbit to the second orbit. (R = 6400 km, g = 10m/s
2
) 
Q 24.  Two identical stars of mass M orbit around their centre of mass. Each orbit is circular 
and has radius R, so that the two stars are always on opposite sides of the circle. 
  (a) Find the gravitational force of one star on the other. 
  (b) Find the orbital speed of each star and the period of the orbit. 
  (c) What minimum energy would be required to separate the two stars to infinity ? 
Q 25.  Consider two satellites A and B of equal mass, moving in the same circular orbit of 
radius r around the earth but in the opposite sense and therefore a collision occurs. 
  (a) Find the total mechanical energy EA+EB of the two satellite-plus-earth system 
before collision. 
(b) If the collision is completely inelastic, find the total mechanical energy 
immediately after collision. Describe the subsequent motion of the combined satellite. 
Q 26.  Two satellites A and B revolve around a planet in two coplanar circular orbits in the 
same sense with radii 10
4
 km and 2 x 10
4
 km respectively. Time period of A is 28 
hours. What is time period of another satellite. 
Q 27.  A satellite of mass 1000 kg is supposed to orbit the earth at a height of 2000 km above 
the earth's surface. Find (a) its speed in the orbit, (b) its kinetic energy, (c) the 
potential energy of the earth-satellite system and (d) its time period. Mass of the earth 
= 6 x 10
24
 kg. 
Q 28.  In a certain binary star system, each star has the same mass as our sun. They revolve 
about their centre of mass. The distance between them is the same as the distance 
between earth and the sun. What is their period of revolution in years ? 
Q 29.  (a) Does it take more energy to get a satellite upto 1500 km above earth than to put it 
in circular orbit once it is there. 
  (b) What about 3185 km?  (c) What about 4500 km? (Take Re = 6370 km) 
Solutions 
1.  
Page 4


EXERCISES 
For JEE Main 
  Subjective Questions  
  Newton's Law of Gravitation 
Q 1.  Two particles of masses 1.0 kg and 2.0 kg are placed at a separation of 50 cm. 
Assuming that the only forces acting on the particles are their mutual gravitation, find 
the initial accelerations of the two particles. 
Q 2.  Three particles A, B and C, each of mass m, are placed in a line with AB = BC = d. 
Find the gravitational force on a fourth particle P of same mass, placed at a distance d 
from the particle B on the perpendicular bisector of the line AC. 
Q 3.  Four particles having masses m, 2m, 3m and 4m are placed at the four corners of a 
square of edge a. Find the gravitational force acting on a particle of mass m placed at 
the centre. 
Q 4.  Three uniform spheres each having a mass M and radius a are kept in such a way that 
each touches the other two. Find the magnitude of the gravitational force on any of the 
spheres due to the other two. 
Q 5.  The figure shows a uniform rod of length l whose mass per unit length is ? . What is 
the gravitational force of the rod on a particle of mass m located a distance d from one 
end of the rod? 
 
  Acceleration due to Gravity 
Q 6.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value on the surface of a planet 
whose mass and radius both are two times that of earth. 
Q 7.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value : 
  (a) at height h = R from the surface,  
  (b) at depth h = 
R
2
from the surface. (R = radius of earth) 
Q 8.  Calculate the distance from the surface of the earth at which the acceleration due to 
gravity is the  same below and above the surface of the earth. 
Q 9.  A body is weighed by a spring balance to be 1000 N at the north pole. How much will 
it weight at  the equator. Account for the earth's rotation only. 
Q 10.  At what rate should the earth rotate so that the apparent g at the equator becomes zero 
? What will be the length of the day in this situation ? 
Q 11.  Assuming earth to be spherical, at what height above the north pole, value of g is 
same as that on the earth's surface at equator ? 
  Gravitational Field Strength and Potential 
Q 12.  Two concentric spherical shells have masses m 1 ,m2 and radii R1, R2 (R1 < R2). 
Calculate the force exerted by this system on a particle of mass m, if it is placed at a 
distance 
12
(R R )
2
?
from the centre. 
Q 13.  Two spheres one of mass M has radius R. Another sphere has mass 4M and radius 2R. 
The centre to centre distance between them is 12R. Find the distance from the centre 
of smaller sphere where :  
  (a) net gravitational field is zero, 
  (b) net gravitational potential is half the potential on the surface of larger sphere. 
Q 14.  A semicircular wire has a length L and mass M. Find the gravitational field at the 
centre of the circle. 
Q 15.  A uniform solid sphere of mass M and radius a is surrounded symmetrically by a 
uniform thin spherical shell of equal mass and radius 2a. Find the gravitational field at 
a distance  
  (a) 
3
a
2
from the centre,   (b) 
5
a
2
 
from the centre. 
Q 16.  The density inside a solid sphere of radius a is given by ? = ?0a/r, where ?0
 
is the 
density at the surface and r denotes the distance from the centre. Find the gravitational 
field due to this sphere at a distance 2a from its centre. 
Q 17.  A particle of mass m is placed at the centre of a uniform spherical shell of same mass 
and radius R. Find the gravitational potential at a distance 
R
2
from the centre. 
  Gravitational Potential Energy 
Q 18.  A rocket is accelerated to speed v 2 gR ?
 
near earth's surface (R =radius of earth). 
Show that very far from earth its speed will be v 2gR ? .
 
 
Q 19.  Two neutron stars are separated by a distance of 10
10
 m. They each have a mass of 
10
30
 kg and a radius of 10
5
 m. They are initially at rest with respect to each other. 
  As measured from the rest frame, how fast are they moving when : 
  (a) their separation has decreased to one-half its initial value, 
  (b) they are about to collide. 
Q 20.  A projectile is fired vertically from earth's surface with an initial speed of 10 km/s. 
Neglecting air drag, how far above the surface of earth will it go ? 
Q 21.  A mass m is taken to a height R from the surface of the earth and then is given a 
vertical velocity v. Find the minimum value of v, so that mass never returns to the 
surface of the earth. 
  (Radius of earth is R and mass of the earth M). 
Q 22.  In the figure masses 400 kg and 100 kg are fixed. 
 
  (a) How much work must be done to move a 1 kg mass from point A to point B ? 
(b) What is the minimum kinetic energy with which the 1 kg mass must be projected 
from A to the right to reach the point B ? 
  Planets and Satellites : Kepler's Law 
Q 23.  A sky lab of mass 2 x 10
3
 kg is first launched from the surface of earth in a circular 
orbit of radius 2R and then it is shifted from this circular orbit to another circular orbit 
of radius 3R. Calculate the energy required: 
  (a) to place the lab in the first orbit, 
  (b) to shift the lab from first orbit to the second orbit. (R = 6400 km, g = 10m/s
2
) 
Q 24.  Two identical stars of mass M orbit around their centre of mass. Each orbit is circular 
and has radius R, so that the two stars are always on opposite sides of the circle. 
  (a) Find the gravitational force of one star on the other. 
  (b) Find the orbital speed of each star and the period of the orbit. 
  (c) What minimum energy would be required to separate the two stars to infinity ? 
Q 25.  Consider two satellites A and B of equal mass, moving in the same circular orbit of 
radius r around the earth but in the opposite sense and therefore a collision occurs. 
  (a) Find the total mechanical energy EA+EB of the two satellite-plus-earth system 
before collision. 
(b) If the collision is completely inelastic, find the total mechanical energy 
immediately after collision. Describe the subsequent motion of the combined satellite. 
Q 26.  Two satellites A and B revolve around a planet in two coplanar circular orbits in the 
same sense with radii 10
4
 km and 2 x 10
4
 km respectively. Time period of A is 28 
hours. What is time period of another satellite. 
Q 27.  A satellite of mass 1000 kg is supposed to orbit the earth at a height of 2000 km above 
the earth's surface. Find (a) its speed in the orbit, (b) its kinetic energy, (c) the 
potential energy of the earth-satellite system and (d) its time period. Mass of the earth 
= 6 x 10
24
 kg. 
Q 28.  In a certain binary star system, each star has the same mass as our sun. They revolve 
about their centre of mass. The distance between them is the same as the distance 
between earth and the sun. What is their period of revolution in years ? 
Q 29.  (a) Does it take more energy to get a satellite upto 1500 km above earth than to put it 
in circular orbit once it is there. 
  (b) What about 3185 km?  (c) What about 4500 km? (Take Re = 6370 km) 
Solutions 
1.  
    
   = 5.3 × 10
-10
 m/s
2
 
   
   = 2.65 × 10
-10 
m/s
2
 
2.  
   
  And the net force is directed along PB. 
3.  
   
4.  
   
5.  
 
6.  
    
Page 5


EXERCISES 
For JEE Main 
  Subjective Questions  
  Newton's Law of Gravitation 
Q 1.  Two particles of masses 1.0 kg and 2.0 kg are placed at a separation of 50 cm. 
Assuming that the only forces acting on the particles are their mutual gravitation, find 
the initial accelerations of the two particles. 
Q 2.  Three particles A, B and C, each of mass m, are placed in a line with AB = BC = d. 
Find the gravitational force on a fourth particle P of same mass, placed at a distance d 
from the particle B on the perpendicular bisector of the line AC. 
Q 3.  Four particles having masses m, 2m, 3m and 4m are placed at the four corners of a 
square of edge a. Find the gravitational force acting on a particle of mass m placed at 
the centre. 
Q 4.  Three uniform spheres each having a mass M and radius a are kept in such a way that 
each touches the other two. Find the magnitude of the gravitational force on any of the 
spheres due to the other two. 
Q 5.  The figure shows a uniform rod of length l whose mass per unit length is ? . What is 
the gravitational force of the rod on a particle of mass m located a distance d from one 
end of the rod? 
 
  Acceleration due to Gravity 
Q 6.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value on the surface of a planet 
whose mass and radius both are two times that of earth. 
Q 7.  Value of g on the surface of earth is 9.8 m/s
2
. Find its value : 
  (a) at height h = R from the surface,  
  (b) at depth h = 
R
2
from the surface. (R = radius of earth) 
Q 8.  Calculate the distance from the surface of the earth at which the acceleration due to 
gravity is the  same below and above the surface of the earth. 
Q 9.  A body is weighed by a spring balance to be 1000 N at the north pole. How much will 
it weight at  the equator. Account for the earth's rotation only. 
Q 10.  At what rate should the earth rotate so that the apparent g at the equator becomes zero 
? What will be the length of the day in this situation ? 
Q 11.  Assuming earth to be spherical, at what height above the north pole, value of g is 
same as that on the earth's surface at equator ? 
  Gravitational Field Strength and Potential 
Q 12.  Two concentric spherical shells have masses m 1 ,m2 and radii R1, R2 (R1 < R2). 
Calculate the force exerted by this system on a particle of mass m, if it is placed at a 
distance 
12
(R R )
2
?
from the centre. 
Q 13.  Two spheres one of mass M has radius R. Another sphere has mass 4M and radius 2R. 
The centre to centre distance between them is 12R. Find the distance from the centre 
of smaller sphere where :  
  (a) net gravitational field is zero, 
  (b) net gravitational potential is half the potential on the surface of larger sphere. 
Q 14.  A semicircular wire has a length L and mass M. Find the gravitational field at the 
centre of the circle. 
Q 15.  A uniform solid sphere of mass M and radius a is surrounded symmetrically by a 
uniform thin spherical shell of equal mass and radius 2a. Find the gravitational field at 
a distance  
  (a) 
3
a
2
from the centre,   (b) 
5
a
2
 
from the centre. 
Q 16.  The density inside a solid sphere of radius a is given by ? = ?0a/r, where ?0
 
is the 
density at the surface and r denotes the distance from the centre. Find the gravitational 
field due to this sphere at a distance 2a from its centre. 
Q 17.  A particle of mass m is placed at the centre of a uniform spherical shell of same mass 
and radius R. Find the gravitational potential at a distance 
R
2
from the centre. 
  Gravitational Potential Energy 
Q 18.  A rocket is accelerated to speed v 2 gR ?
 
near earth's surface (R =radius of earth). 
Show that very far from earth its speed will be v 2gR ? .
 
 
Q 19.  Two neutron stars are separated by a distance of 10
10
 m. They each have a mass of 
10
30
 kg and a radius of 10
5
 m. They are initially at rest with respect to each other. 
  As measured from the rest frame, how fast are they moving when : 
  (a) their separation has decreased to one-half its initial value, 
  (b) they are about to collide. 
Q 20.  A projectile is fired vertically from earth's surface with an initial speed of 10 km/s. 
Neglecting air drag, how far above the surface of earth will it go ? 
Q 21.  A mass m is taken to a height R from the surface of the earth and then is given a 
vertical velocity v. Find the minimum value of v, so that mass never returns to the 
surface of the earth. 
  (Radius of earth is R and mass of the earth M). 
Q 22.  In the figure masses 400 kg and 100 kg are fixed. 
 
  (a) How much work must be done to move a 1 kg mass from point A to point B ? 
(b) What is the minimum kinetic energy with which the 1 kg mass must be projected 
from A to the right to reach the point B ? 
  Planets and Satellites : Kepler's Law 
Q 23.  A sky lab of mass 2 x 10
3
 kg is first launched from the surface of earth in a circular 
orbit of radius 2R and then it is shifted from this circular orbit to another circular orbit 
of radius 3R. Calculate the energy required: 
  (a) to place the lab in the first orbit, 
  (b) to shift the lab from first orbit to the second orbit. (R = 6400 km, g = 10m/s
2
) 
Q 24.  Two identical stars of mass M orbit around their centre of mass. Each orbit is circular 
and has radius R, so that the two stars are always on opposite sides of the circle. 
  (a) Find the gravitational force of one star on the other. 
  (b) Find the orbital speed of each star and the period of the orbit. 
  (c) What minimum energy would be required to separate the two stars to infinity ? 
Q 25.  Consider two satellites A and B of equal mass, moving in the same circular orbit of 
radius r around the earth but in the opposite sense and therefore a collision occurs. 
  (a) Find the total mechanical energy EA+EB of the two satellite-plus-earth system 
before collision. 
(b) If the collision is completely inelastic, find the total mechanical energy 
immediately after collision. Describe the subsequent motion of the combined satellite. 
Q 26.  Two satellites A and B revolve around a planet in two coplanar circular orbits in the 
same sense with radii 10
4
 km and 2 x 10
4
 km respectively. Time period of A is 28 
hours. What is time period of another satellite. 
Q 27.  A satellite of mass 1000 kg is supposed to orbit the earth at a height of 2000 km above 
the earth's surface. Find (a) its speed in the orbit, (b) its kinetic energy, (c) the 
potential energy of the earth-satellite system and (d) its time period. Mass of the earth 
= 6 x 10
24
 kg. 
Q 28.  In a certain binary star system, each star has the same mass as our sun. They revolve 
about their centre of mass. The distance between them is the same as the distance 
between earth and the sun. What is their period of revolution in years ? 
Q 29.  (a) Does it take more energy to get a satellite upto 1500 km above earth than to put it 
in circular orbit once it is there. 
  (b) What about 3185 km?  (c) What about 4500 km? (Take Re = 6370 km) 
Solutions 
1.  
    
   = 5.3 × 10
-10
 m/s
2
 
   
   = 2.65 × 10
-10 
m/s
2
 
2.  
   
  And the net force is directed along PB. 
3.  
   
4.  
   
5.  
 
6.  
    
7.  (a) 
    
  (b) 
    
8.  
  ? (R-x)(R + x)
2
 = R
3  
  ? 
(R
2
 -x
2
)(R + x)=R
3
 
  or  R
3
+R
2
x - x
2
R-x
3
=R
3  
  
or  x
3
 + x
2
 R - xR
2
 = 0  
  or  x
2
 +Rx - R
2
 = 0 
   
9.  wp = mg and we = mg - m ?
2
R 
   
   = 1000 × 0397 = 997 N 
10.  gapparent = g - ?
2
 
R = 0 
   
   = 16 ? × 10
2
 
   = 5026.5 s = 1.4 h 
   
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FAQs on DC Pandey Solutions (JEE Main): Gravitation - DC Pandey Solutions for JEE Physics

1. What are the important topics in the Gravitation chapter for JEE Main Physics?
Ans. The important topics in the Gravitation chapter for JEE Main Physics include Newton's law of gravitation, gravitational potential energy, escape velocity, gravitational field, Kepler's laws of planetary motion, and orbital motion.
2. How can I prepare for the Gravitation chapter in JEE Main Physics?
Ans. To prepare for the Gravitation chapter in JEE Main Physics, you should start by understanding the basic concepts and laws related to gravitation. Practice solving numerical problems based on these concepts and also solve previous years' question papers. It is also helpful to refer to a reliable study material such as DC Pandey's book on Physics for JEE Main.
3. How can I improve my understanding of the gravitational field concept for JEE Main Physics?
Ans. To improve your understanding of the gravitational field concept in JEE Main Physics, you can start by learning the definition and properties of the gravitational field. Practice solving problems related to the calculation of gravitational field intensity and potential at different points. You can also visualize the concept by studying the field lines and their properties.
4. What is the significance of Kepler's laws of planetary motion in the Gravitation chapter for JEE Main Physics?
Ans. Kepler's laws of planetary motion are significant in the Gravitation chapter for JEE Main Physics as they provide a mathematical description of the motion of planets around the Sun. These laws help in understanding the elliptical nature of planetary orbits, the equal area law, and the relation between the period and radius of the orbit. Questions based on Kepler's laws are frequently asked in JEE Main Physics.
5. How can I solve numerical problems related to escape velocity in the Gravitation chapter for JEE Main Physics?
Ans. To solve numerical problems related to escape velocity in the Gravitation chapter for JEE Main Physics, you should first understand the concept of escape velocity and its formula. Practice solving problems where you need to calculate the escape velocity of an object from a given planet or satellite. Pay attention to the units and make sure to use the correct formula for the calculation.
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