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Gravitation Test - 16

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Gravitation Test - 16
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  • Question 1
    1 / -0
    The dependence of acceleration due to gravity $$g$$ on the distance $$r $$ from the centre of the earth, assumed to be a sphere of radius $$R$$ of uniform density is as shown in figures below. The correct figure is
    Solution
    The acceleration due to gravity at a depth d below surface of earth is
    $$\displaystyle g' = \frac{GM}{R^2} \left( 1 - \frac{d}{R} \right) = g \left(  1 - \frac{d}{R} \right)$$
    $$g' = 0$$ at $$d = R$$
    i.e., acceleration due to gravity is zero at the centre of earth.
    Thus, the variation in value $$g$$ with $$r$$ is for, $$r > R$$,
    $$\displaystyle g' = \frac{g}{ \left( \displaystyle 1 + \frac{h}{R} \right)^2} = \frac{gR^2}{r^2}    \Rightarrow g' \propto \frac{1}{r^2}$$
    Here, $$R + h = r$$
    For           $$\displaystyle r < R, g' = g \left( 1 - \frac{d}{R} \right) = \frac{gr}{R}$$
    Here, $$R - d = r$$   $$\Rightarrow g' \propto r$$
    Therefore, the variation of $$g$$ with distance from centre of the earth will be as shown in the figure.

  • Question 2
    1 / -0
    The acceleration due to gravity at a height 1 km above the earth is the same as at a depth d below the surface of earth. Then:
    Solution
    Acceteration due to gravity at height h, 
    $$g_n=g_0 (1-\dfrac{2h}{R})$$  $$ h=1km$$
    Acceleration due to gravity at depth d,
    $$d_d = g_0\left(1-\dfrac{d}{R}\right)$$
    $$g_h=g_d$$
    $$g_0(1-\dfrac{2h}{R})=g_0(1-\dfrac{d}{R})$$
    $$\rightarrow d=2h$$
    $$= 2\times 1 km$$
    $$d=2km$$
  • Question 3
    1 / -0
    If $${v}_{e}$$ is escape velocity and $${v}_{o}$$ is orbital velocity of a satellite for orbit close to the earth's surface, then these are related by :
    Solution
    $${v}_{escape}=\sqrt {\cfrac{2GM}{R}}$$
    $${v}_{orbital}=\sqrt {\cfrac{GM}{R}}$$
    $${v}_{escape}=\sqrt {2}{v}_{o}$$
  • Question 4
    1 / -0
    A particle of mass $$m$$ is thrown upwards from the surface of the earth, with a velocity $$u$$. The mass and the radius of the earth are, respectively, $$M$$ and $$R$$. $$G$$ is gravitational constant and $$g$$ is acceleration due to gravity on the surface of the earth. The minimum value of $$u$$ so that the particle does not return back to earth is
    Solution
    $$GM = g{R}^{2}$$
    $${V}_{e} = \sqrt{2gR} = \sqrt{2\displaystyle\frac{GM}{{R}^{2}}}R = \sqrt{\displaystyle\frac{2GM}{R}}$$.
  • Question 5
    1 / -0
    Starting from the centre of the earth having radius R, the variation of g (acceleration due to gravity) is shown by which of the following options ?
    Solution
    Acceleration due to gravity,         $$g = \dfrac{GMr}{R^3}$$         for  $$0\leq r\leq R$$
    $$\implies$$    $$g \propto  r$$         for  $$0\leq r\leq R$$

    Acceleration due to gravity,         $$g = \dfrac{GM}{r^2}$$         for  $$ r\geq R$$
    $$\implies$$    $$g \propto \dfrac{1}{r^2} $$         for  $$ r\geq R$$
    Hence option C is correct.
  • Question 6
    1 / -0
    A body of mass m is taken from the earth's surface to the height equal to twice the radius (R) of the earth. The change in potential energy of body will be
    Solution

  • Question 7
    1 / -0
    The change in the gravitational potential energy when a body of mass $$m$$ is raised to a height $$nR$$ above the surface of the earth is (here $$R$$ is the radius of the earth).
    Solution
    Gravitational potential energy of mass $$m$$ at any point at a distance $$r$$ from the centre of earth is
    $$U = -\dfrac {GMm}{r}$$
    At the surface of earth $$r = R$$,
    $$\therefore U_{s} = -\dfrac {GMm}{R} = -mgR \left (\because g = \dfrac {GM}{R^{2}}\right )$$
    At the height $$h= nR$$ from the surface of earth
    $$r = R + h = R + nR = R (1 + n)$$
    $$\therefore U_{h} = -\dfrac {GMm}{R(1 + n)} = -\dfrac {mgR}{(1 + n)}$$
    Change in gravitational potential energy is
    $$\triangle U = U_{h} - U_{s} = -\dfrac {mgR}{(1 + n)} - (-mgR)$$
    $$=-\dfrac {mgR}{1 + n} + mgR$$
    $$= mgR\left (1 - \dfrac {1}{1 - n}\right ) = mgR\left (\dfrac {n}{1 + n}\right )$$.
  • Question 8
    1 / -0
    The value of $$g$$ at a height of $$100km$$ from the surface of the Earth is nearly (Radius of the Earth $$=$$ 6400km) ($$g$$ on the surface of the Earth $$=$$ $$9.8m/s^{2}$$)
    Solution
    Acceleration due to gravity changes with the height from Earth's surface as:
    $$g^{'} = g(1-\dfrac {2h}{R})$$
    $$\Rightarrow g^{'} = 9.8 (1-\dfrac {2\times 100}{6400})$$
    $$\Rightarrow g^{'} = 9.8(1-\dfrac {1}{32})=9.49 m/s^2$$
  • Question 9
    1 / -0
    The escape velocity for a body projected vertically upwards from the surface of earth is $$11$$ km/s. If the body is projected at an angle of $$45^{0}$$ with the vertical, the escape velocity will be
    Solution
    Escape speed of a body from Earth's surface is given by: $$v_{min}= \sqrt {2gR}$$
    This expression is obtained by conservation of energy and doesn't involve in which direction the body is thrown/projected.
    So, irrespective of the angle of projection, escape speed of the body from Earth's surface remains constant i.e. $$\approx 11$$ km/s
  • Question 10
    1 / -0
    If $$g$$ on the surface of the Earth is $$9.8\  ms^{-2}$$, its value at a height of $$6400 km$$ is: (Radius of the Earth $$= 6400km$$)
    Solution
    The expression for $$g$$ is given by:
    $$g_R =\dfrac {GM}{R^2}$$
    The value of $$g$$ changes according to
    $$g_h=\dfrac {GM}{(R+h)^2}$$
    Therefore, $$\displaystyle \dfrac{g_{h}}{g_R} = \dfrac{R^{2}}{(R+h)^{2}}$$
    Here, $$h = R$$
    So, $$\dfrac {g_h}{g_R}=(\dfrac {R}{R+h})^2$$
    $$\Rightarrow \dfrac {g_h}{g_R}=(\dfrac {R}{R+R})^2$$
    $$\Rightarrow g_h=g_R\times\dfrac {1}{4} = 9.8\times 0.25=2.45\ m/s^2$$
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