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Gravitation Test - 30

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Gravitation Test - 30
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  • Question 1
    1 / -0
    A spherical uniform planet is rotating about its axis. The velocity of a point on its equator is $$V$$. Due to the rotation of planet about its axis the acceleration due to gravity $$g$$ at equator is  $$\dfrac{1}{2}$$ of $$g$$ at poles. The escape velocity of a particle on the pole of planet in terms of  $$V$$.
    Solution

  • Question 2
    1 / -0
    At what height over the earth's pole does the freefall acceleration decreases by 1% ?
    Solution
    $$mg'=\dfrac{GMm}{R^2+h^2}$$

    $$mg=\dfrac{GMm}{R^2}$$

    $$\dfrac{g'}{g}=\dfrac{R^2}{R^2+h^2}$$
    $$\dfrac{g'}{g}=(R^2)(R^2+h^2)^{-2}$$
    $$\dfrac{g'}{g}=(1+\dfrac{h^2}{r^2})^{-2}$$

    Expanding using binomial expansion and neglecting higher terms,
    $$\dfrac{g'} {g}=  \displaystyle \left ( 1 - \dfrac{2h}{R} \right )  = \dfrac{99}{100}    or    h = 32 km$$
  • Question 3
    1 / -0
    The condition for a uniform spherical mass $$m$$ of radius $$r$$ to be a black hole is [$$G= $$gravitational constant, $$g=$$ acceleration due to gravity].
    Solution
    For a uniform spherical mass to be a black hole, total energy of the "particle + spherical mass" system  $$\leq 0$$
    Let the mass of particle be  $$m_1$$ moving with its maximum speed  $$c$$.
    $$\therefore$$   $$\dfrac{1}{2}m_1 c^2 + (-\dfrac{Gmm_1}{r}) \leq 0$$
    $$\implies \ c\leq\bigg[\dfrac{2Gm}{r}\bigg]$$
  • Question 4
    1 / -0
    A body is projected up with a velocity $$2$$ times the escape velocity $$v_{e}$$  from the surface of the earth. The velocity of the body at a point  far away the earth's attraction is
    Solution
    $$v_e = (\dfrac{2GM}{R})^{0.5}$$
    now, $$V = 2v_e = 2(\dfrac{2GM}{R})^{0.5} = (\dfrac{8GM}{R})^{0.5}$$

    By conservation of energy, $$ \dfrac{-GMm}{R} +\dfrac{8GMm}{2R} = 0 + \dfrac{mv^2}{2}$$

    solving this, we get $$v = (\dfrac{3 \times 2GM}{R})^{0.5} = 3^{0.5}v_e$$
  • Question 5
    1 / -0
    A particle of mass $$10 g$$ is kept on the surface of a uniform sphere of mass $$100 kg$$ and radius $$10 cm$$. Find the work to be done against the gravitational force between them to take the particle far away from the sphere 
    Solution
    $$W=\Delta PE=\left ( \dfrac{-GMm}{\infty } \right )-\left ( \dfrac{-GMm}{R} \right )=\dfrac{6.67\times10^-11 \times 100\times 10\times 10^{-3}}{1}= 6.67\times10^{-10} J$$
  • Question 6
    1 / -0
    The change in the value of $$g$$ at a height $$h$$ above the surface of the earth is the same as at a depth d below the surface of the earth.When both $$h$$ and d are much smaller than the radius of earth,then which one of the following is true?
    Solution
    $$\displaystyle{{g}'=g \left ( 1-\frac{2h}{R} \right )=g \left ( 1-\frac{d}{R}\right )\therefore d=2h}$$
  • Question 7
    1 / -0
    A $$75 kg$$ astronaut is repairing Hubble telescope at a height of $$600 km$$ above the surface of the earth. Find his weight there.
    Solution
    $$\displaystyle mg' = mg \left ( 1 - \dfrac{2h}{R} \right )$$
    $$= 75 \times 10 (1 - 0.185) = 610 N$$
  • Question 8
    1 / -0
    If the orbital speed of moon is increased by $$41.4\%$$ then moon will
    Solution

    Velocity of the planet is $$v=\sqrt{\dfrac{GM}{a}}$$

    Kinetic Energy  is $$K=\dfrac{1}{2}m{v}^{2}=\dfrac{GMm}{2a}$$

    Potential Energy is $$U=-{\dfrac{GMm}{a}}$$

    $$Total\  energy= K+U= -{\dfrac{GMm}{2a}}$$

    $${v}= \sqrt{\dfrac{GM}{a}}$$

    So if$$,\quad v=1+0.414 v=1.414v= \sqrt{2} v= \sqrt{\dfrac{2GM}{a}}$$

    Escape  Velocity is  $$v_e=\sqrt{\dfrac{2GM}{a}}$$

    So the moon will escape.

  • Question 9
    1 / -0
    A spaceship is released in a circular orbit near the Earth's surface. How much additional velocity will have to be given to the spaceship in order to escape out of this orbit?
    Solution
    Here, orbital velocity and escape velocity are
    $$v_0 = \sqrt{gR}$$
    $$v_e = \sqrt{2gR}$$
    Hence, required additional velocity will be,
    $$v = v_e - v_o$$
    $$v = \sqrt{2gR} - \sqrt{gR}$$
    $$v = (\sqrt 2 - 1) \sqrt{gR}$$
    $$v = (1.414 - 1)\sqrt{(10)(6400 \times 10^3)}$$..........$$($$since, $$g = 10 ms^{-2}$$ and $$R = 6400 \times 10^3 m)$$
    $$v = (0.414)(8) \times 10^3$$
    $$v = 3.3 \times 10^3 ms^{-1}$$
  • Question 10
    1 / -0
    Find the work done to take a particle of mass m from surface of the earth to a height equal to $$2R$$.
    Solution
    $$Work\quad Done\quad =\quad \Delta \quad PE\\ PE=\quad \dfrac { GMm }{ r } \\ \Delta PE=GMm(\dfrac { 1 }{ R } -\dfrac { 1 }{ 3R } )=\dfrac { 2GMm }{ 3R } =\dfrac { 2 }{ 3 } mgR$$
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