Gravitation PDF
Gravitation PDF
                                                                                          ab
                                                                                    (a)
                                                                                          m
                                    RI2
                                                                                          a2 +b2                           (d)
                                                                                                                                 a2+b2
                                 FIGURE 3.59                                        (c)
                                                                                                  m                                 m
      (a)
            GM                                 (b) 2GM2                                                  FIGURE 3.60
                42
                                                                                               G
                                                                                    (a)
            2GM2                                    3 GM2
   (C)A                                         (d)42                                                                      (d) Zero
33. Two astronauts have deserted their
                                            spaceship in a region of
    space far from the gravitational attraction of any other body.              39. Given that mass of the earth is M and its radius is R.
                                                                                                                                           A bodyis
    Each has a mass of 100 kg and they are 100 m                                    dropped from a height equal to the radius of the earth above
                                                     apart. They are
    initially at rest relative to one another. How long will it take                the surface of earth. When it reaches the
                                                                                    will be
                                                                                                                                ground its     velocity
    for the gravitional attraction to bring them closer by 1 cm
      (a) 2-52 days                            (b) 1.41 days
                                                                                    (a) GM                                       GM /2
      (c) 0-70 days
34. The
                                               (d) 141 s
            gravitational field in a region is given by
                                                                                              R
                                                                                                                       R
      & (5i+ 12j) N/kg. The magnitude of the gravitational
                                                                                                                           20M
                                                                                    (c2GM2
                                                                                                  GMm            11
                                                        4r                                  (c)
 41. A   particle of mass 10 kg is kept on the surface of a uniform                                            possible of     find the         required     work   as   the nature
                                                                                            (d) It is    not
      sphere of mass 100 kg and radius 10 cm. Find the work to be                                 of distribution of       mass      is   not    known.
      done against the gravitational force                                                                                                                                        the
                                           between them to take the                                                             M and 2 M,             respectively, having
      particle far away from the sphere. (G 6-67 x 10-1 Nm/kg)                    47. Two          rings having       masses
                                                                                                                                                                                3.62.
                                                    =
                                                                                            same   radius R     are   placed coaxially            as    shown in the     fig.
      (a) 6-67 x 109J                        (b) 6-67 x 10-7J
      (c) 13-34 x 10-10 J                    (d)3.33 x 10-10 J                                                                 3R
 42. A person      brings
                       a mass of 2
                                    kg from A to B. The increase in                                                               P
      kinetic energy of the mass is 4 J and the work done
                                                           by person
      on the mass is     10 J. The gravitational
                                                 potential difference
                         -
     R                                  R                                          3 GM                                   2 GM
50. A particle of mass mo is placed at the centre of a fixed, uniform
    semicircular ring of radius R and mass m as shown in the fig.
    3.64. The work required to displace the particle from centre
                                                                             (a)
                                                                                   4R                            6)3R
    of the ring to infinity is                                                     GM                            (
                                                                                                                          2 GM
                                                                                                                            R
                                                                              (c)2R
                                                                         56. A small body of super dense material, whose mass is twice
                                                                             the mass of the Earth but whose size is very small compared
                                                                             to the size of the Earth, starts from rest at a height H << R
                                       mo                                    above the Earth's surface. If it reaches the Earth's surface in
                                                                             time , then t is equal to?
(a)
                 R
     c)
                                                                                                                 R
52. A particle is projected vertically upward with velocity
                                                                                                   FIGURE 3.65
      2 GM        from the surface of earth. The height attained by it
     3 R                                                                      (a) G M                                      7 GM
     is (G, M and R have usual meanings)                                              7R
                                                                                                                 (6)
                                                                                                                            14R
     (a) 3 R                             (b) R/2
                                                                                    3 GM                                   9 GM
     (c) 2 R                             (d) R/3
53. Given that the gravitational potential on earth surface is Vo
                                                                               7R                                    d)
                                                                                                                            14R
                                                                          59. A small ball of mass m is released at a height R above the
    The potential at a point distant half the radius of earth from
                                                                              Earth surface, as shown in the fig. 3.66. The maximum depth
    the centre will be
                                                                              of the ball to which it goes is RI2 inside the Earth through a
                                                                              narrow groove before coming to rest
                                                                                                                    momentarily. If the groove
                                         (b2                                  contains an ideal spring of spring constant K and natural length
                                                                              R, the value of K is (R is radius of Earth and M mass of Earth)
    (c) 2 Vo                             ()
54. If the gravitational acceleration at surface of Earth is g, then
    increase in potential energy in lifting an object of mass m to a
                                                                                           m           www.
                                                                                                           RM
    height equal to the radius R of Earth will be
                                                                                                             K
           mgR                           (b) 2 mgR
    (a)
                                                gR                                                 FIGURE 3.66
    (c) mgR                              (4
    (a) GMm
    aR                                      (b) GMm
          9GMm
    (c)
                                            (d)
                                                      7GMm
              R3                                       R3                                                          FIGURE 3.68
60. A particle of mass m is
                             transferred from the centre of the base                       (a) increases continuously
    of a uniform solid
                         hemisphere of mass M and radius R to                              (b) decreases continuously
    infinity. The work performed in the process by the
    force exerted on the                               gravitational                       (c) first decreases, then
                                                                                                                     increases
                              particle by
                                       the        hemisphere      is
                                                                                                                             decreases
          3 GMm                                                                            d) first increases, then
                                                      3 GMm                                                        and M are placed at distance d apart.
   (a)2 R                                    (b) 4 R                                   66. Two bodies of masses m
                                                                                           The gravitational potential
                                                                                                                         V at the position where the
                                                                                                       field due to them is zero is
                                                                                           gravitational
    (c)            GMm                                 3 GMm
     R objects
61. Two                  of masses
                                            (d)- 4
                                         and 2
                                                           R                               (a) V=(m +M)                                        (b) V=-
                                     m            m    are at   rest at   infinite
     separation. They move towards each other under mutual
     gravitational   attraction. At the instant, when the              separation
                                                                                           (c) V-
                                                                                                          GM
                                                                                                          d
                                                                                                                                           V--m+
                                                                                                                                              d  M2
     between them is r, which of the following is true?                                                                                                    It has a uniform
                                                                                       67. Asphere of radius R has its centre at the origin.
     (a) The total energy of the system is zero                                            mass density Po except that there is a spherical
                                                                                                                                                             hole of radius
     (b) The force between them is not zero                                                r=     RI2 whose    centre   is   at   x   =   RI2 as shown in the fig. 3.69.
                                                                                           The magnitude of gravitational                 field at a point distant x on the
     (c) The centre of mass of the system is at rest
                                                                                           X-axis, where x > R is
     d) All are true
62. Two spherical bodies having masses M and 3 M, and radii r                                                                YA
     and 4 r respectively are released in free space from rest such
     that the initial separation between their centres is 13 r. If only
     force is gravitational attraction, the distance covered by the
     smaller body just before collision is
     (a) 6r                                  (b) 2 r
                                                      39
                                                                                                                   FIGURE 3.69
 63. Two spherical bodies of masses M and 5 M and radii R and12                                   4 GTR'PO
     R, respectively, are released in free space with initial separation                   (a)
     between their centres equal to 12 R. If they attract each other                                                    8(x-R/2)J
     due to gravitational force only, then the distance covered by
     the smaller body just before collision is                                             () 4GrR'P 2 -
                                                                                           (b)
      (a) 25 R                               (b) 4-5 R                                                  8 (r R/2)|
                                             (d) 15R
      (c) 75 R
                                                                                           (c)
                                                                                           (c)
                                                                                               2GTRPo1
 64. Find the distance between centre of gravity and centre of mass                                  3
     of a two particle system. Each particle has same mass.
                                                                                                                8(x-R/2)3 J
                                                                                                  oRRPOs-R/2*
                                                  other paticle is at
     One particle is on the surface of earth, the
     the centre of earth and R is the radius
                                             of Earth                                       (d)       3
        (a) V12:1
                                                                                               (a) Vo3
                                                                                                                                        6)o2
                                                    (b)24:1
                                                                                                                                                  Vo
       (c)1:12                         (d) 1:24                                                (c) v2
 74.   Two planets of masses M and
                                     M, are situated r distance apart.                   81.   Velocity of a point on the equator of a rotating spherical planet
       With what minimum velocity should a mass m be
       from the mid point of the two
                                                            projected                          is v. The angular velocity of the planet is such that, the value
                                     planets so that it escapes away                           of g at the equator is half of g at the pole. Determine the
       from the gravitational pull of both?
                                                                                               escape velocity for a polar particle on the planet as a function
                                                                                               of v.
       (a)        G(M+M2)                                     G(M+M,)
                                                    ()2                                        (a) 6 v
                                                                                               (c) 4 v
                                                                                                                                       (b) 2 v
                                                                                                                              (d) 3 v
       (c)       GM-M
                 N                                  (d 2GM-M                             82. Two satellites A and B go around the earth in circular
                                                                                                                                                    orbits               at
                                                                                               heights RA and Rg respectively, from the surface of earth.
75. The escape velocity from the earth is                                                      Assume the earth to be a uniform sphere of radius
                                          ve A body is projected                                                                                 RE. The
    with velocity v> v With what constant                                                      ratio of the     magnitudes of the velocity, v^hvg of the
                                            velocity will it move                                                                                              satellite is
    in the interplanetary
                          space?
       (a) v- Ve                                    (b) v+e                                    (a)      RB
                                                                                                       RA
76. A        particle   is thrown
                              vertically upwards from the surface of
                                                                                                                                          Rg+RE
       earth and it reaches to a maximum height
       of earth. The ratio of the velocity of
                                                   equal to the radius
                                              projection to the escape
                                                                                                       RA+R
                                                                                         83. The orbital velocity of an
                                                                                                                                       (dRA  Rg
       velocity on the surface of earth is                                                                               artificial satellite in a circular orbit
                                                                                             just above the earth's surface is v. For a satellite
                                                                                             altitude of half of the earth's radius, the           orbiting at an
   (                                                ()
                                                                                               (a) 3 v/2
                                                                                                                                           orbital velocity is
                                                                                                                                       (b) 3/2v
       (c)                                                                                   c)2/3v                            d) 2 v/3
                                                                                         84. Select the correct alternative
77. A projectile is fired from the surface of earth of radius R with
    a velocity kv, (where v, is the escape velocity from surface of                          (a) The gravitational field inside   a
                                                                                                   spherical planet must be non-zerospherical cavity, within              a
    earth and k< 1). Neglecting air resistance, the maximum height                                                                      and uniform
    of rise from the centre of earth is                                                        (b) When a body is projected
                                                                                                                            horizontally at an appreciable
                                                                                                   height above the Earth, with a velocity less than for a large
                                                                                                       orbit,
                                                                                                         it will fall to the                              circular
                                                    (b)R                                                                     Earth along a
                                                                                               (c) A body of zero total                    parabolic path
                                                                                                                              mechanical        energy       placed
                                                                                                                                                              in a
                                                    (d) k R
                                                                                                       gravitational field   will escape the field
                                                                                               (d) Earth's satellite      must be in
                                                                                                                                       equatorial plane
85. Two satellites A and B
                           go around        a
                                               planet P in circular orbit
      having  radii 4 R and R
                              respectively.   If the speed of the satellite                                            (d)R
      A is 3 V, the speed of the
                                  satellite B will be
                                                                                  (c)R 2                                that the force of attraction
                                                                                                               be such
      (a) 12 V                                                                 93. If the law of gravitation                                 of their
                                          b) 6 V                                   between two particles vary   inversely as the 5/2th power
      (c) (4/3) V                                                                                                  orbital velocity vo plotted against
                                         (d) (3/2) V                               separation, then the graph of
86. If an artificial satellite is                                                                                from the earth's center on a log-log
                                  moving in a circular orbit around the            the distance r of a satellite
    earth with a speed equal to half                                                                                       is
                                         the magnitude of the escape               scale is shown. The slope of graph
    velocity from the surface of earth, the      height of the satellite                             In Vo
    above the surface of the earth is
                                         (Radius of earth is R)
      (a) 2 R
                                              (b) R/2
      (c)R
                                              (d)R/4
87. Let G be the universal           gravitational    constant and p be the                                                   Inr
      uniform density    of   a
                                  spherical planet.   Then shortest possible                             FIGURE 3.70
      period of rotation around a planet can be
                                                                                                                        (b) -       5/2
                                                                                   (a)    -    5/4
      km above the earth's surface (Rearth = 6400 km) will approxi-            96. A satellite is launched in the equatorial plane in such a way
      mately be                                                                    that it can transmit signals upto 60° latitude on the earth. The
                                              (b) 1 hr                             angular velocity of the   satellite is
      (a) 1/2 hr
    (c) 2 hr                          (d) 4 hr                                                GM                                    GM
90. A projectile after deviating from its path, starts moving round
    the Earth in a circular path of radius equal to nine times the
                                                                                  @2R
    radius of Earth R. Its time period will be                                                GM                                    33 GM
                R                            (b) 27x 2m,
                                                                                    4R                                                      8R3
      (a) 21                                                                   97. The radius of a planet is R. A satellite revolves around it in a
                                                                                   circular orbit of radius r with angular speed o. The acceleration
               centripetal force m   where v is speed of planet and r                         circular path of radius R under the mutual interaction of each
                                                                                              other. The velocity of each particle is
          is distance between sun
                                     and planet
116. A point P is on the axis of a fixed                                                                                                  GM
                                         ring of mass M and radius R,
     at a distance 2 R from the
     from P and reaches O under the
                                    centre O. A small
                                                        particle starts
                                                                                              () R
                                                                                                                                     b)3R
     Its speed at O will be              gravitational attraction only.
     (a) zero                                     2 GM
                                                                                              () 3R
                                                                                                                                    3          R
                                                                                         121. Four particles of equal mass M move along a circle of radius
                                                        R
                                                                                              R under the action of their mutual gravitational attraction. The
     (c)        2GM
                 R (5-1)
                     -                      (d
                                                                                              speed of each particle is
               Gm                                  Gm
     R                                      b4R
               Gm                             Gm
     c)3R                                   (2R                                                ()             GPo                     )    2GPo
                                          ASSIGNMENT-1