Gravitation


  1. The ratio of escape velocity at earth (ve) to the escape velocity at a planet (vp) whose radius and mean density are twice as that of earth is :









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    As we know, escape velocity,

    Vc
    =
    Rc
    ρc / 2ρc
    Vp2Rc

    ∴ Ratio
    Vc
    = 1 : 2 √2
    Vp

    Correct Option: B

    As we know, escape velocity,

    Vc
    =
    Rc
    ρc / 2ρc
    Vp2Rc

    ∴ Ratio
    Vc
    = 1 : 2 √2
    Vp


  1. With what velocity should a particle be projected so that its height becomes equal to radius of earth?​​​









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    From conservation of energy

    1
    mu2 -
    GMm
    =
    1
    m × (0)2 -
    GMm
    2R2R + R

    ⇒ u2 =
    2GM
    -
    2GM
    =
    GM
    R2RR


    Correct Option: A

    From conservation of energy

    1
    mu2 -
    GMm
    =
    1
    m × (0)2 -
    GMm
    2R2R + R

    ⇒ u2 =
    2GM
    -
    2GM
    =
    GM
    R2RR




  1. ​The potential energy of a satellite, having mass m and rotating at a height of 6.4 × 106 m from the earth surface, is​​​









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    Mass of the satellite = m and height of satellite from earth (h) = 6.4 × 106 m. ​
    We know that gravitational potential energy of the satellite at height

    h = -
    G Me m
    = -
    gRe2 m
    (Re + h)2Re

    = -
    gRem
    = -0.5 mgRe
    2

    (where, GMe = gRe2 and h = Re)

    Correct Option: C

    Mass of the satellite = m and height of satellite from earth (h) = 6.4 × 106 m. ​
    We know that gravitational potential energy of the satellite at height

    h = -
    G Me m
    = -
    gRe2 m
    (Re + h)2Re

    = -
    gRem
    = -0.5 mgRe
    2

    (where, GMe = gRe2 and h = Re)


  1. Assuming the radius of the earth as R, the change in gravitational potential energy of a body of mass m, when it is taken from the earth's surface to a height 3R above its surface, is









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    Gravitational potential energy (GPE) on the surface of earth,

    E1 = -
    G M m
    R

    GPE at 3R, E2 = -
    G M m
    = -
    G M m
    (R + 3R)4R

    ∴ Change in GPE = E2 - E1 = -
    GMm
    +
    GMm
    =
    3GMm
    4RR4R

    =
    3g R2m
    ∵ g =
    GM
    4RR2

    =
    3
    mg R
    4

    Correct Option: B

    Gravitational potential energy (GPE) on the surface of earth,

    E1 = -
    G M m
    R

    GPE at 3R, E2 = -
    G M m
    = -
    G M m
    (R + 3R)4R

    ∴ Change in GPE = E2 - E1 = -
    GMm
    +
    GMm
    =
    3GMm
    4RR4R

    =
    3g R2m
    ∵ g =
    GM
    4RR2

    =
    3
    mg R
    4