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Gravitation Test - 37

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Gravitation Test - 37
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  • Question 1
    1 / -0
    The ratio of the radii of the planets $${P}_{1}$$ and $${P}_{2}$$ is $$k$$. The ratio of gravitational field intensity at their surface is $$r$$ then the ratio of the escape velocities from them will be -
    Solution
    We are given that:
    $$\dfrac{\dfrac { G{ M }_{ 1 } }{ { R }_{ 1 }^{ 2 } }} {\dfrac { G{ M }_{ 2 } }{ { R }_{ 2 }^{ 2 } } }=r$$ 

    $$\\ \dfrac { { R }_{ 1 } }{ { R }_{ 2 } } =k$$.
    And the escape velocity is given by: $$v=\sqrt { \dfrac { 2GM }{ R }  }$$ where $$M$$ is the mass of the planet and $$R$$ is its radius.
    So, $$\dfrac { { v }_{ 1 } }{ { v }_{ 2 } } =\sqrt { \dfrac { { M }_{ 1 } }{ { M }_{ 2 } } /\dfrac { { R }_{ 1 } }{ { R }_{ 2 } }  } =\sqrt { \dfrac { r{ k }^{ 2 } }{ k }  } =\sqrt { rk } $$.
  • Question 2
    1 / -0
    Mass of a planet is $$5 \times  10^{24}$$ kg and radius is $$6.1 \times  10^6$$m. The energy needed to send a $$2$$ kg body into space from its surface, would be.
    Solution

     Energy required to send a body into the space from the surface of planet is equal to the negative of potential energy at surface.
    At surface $$P.E = -\dfrac{GMm}{R}$$
    Thus energy required $$E= \dfrac{GMm}{R}$$
    Given: $$M= 5 \times 10^{24}  kg                 m= 2  kg                       R= 6.1 \times 10^6  m                             G= 6.67 \times 10^{-11}  Nm^2/kg^2$$  
    $$\implies E=1.1 \times 10^{8}    Joule$$
  • Question 3
    1 / -0
    Gravitational potential difference between surface of a planet and a point situated at a height of $$20m$$ above its surface is $$2 joule/kg$$. If gravitational field is uniform, then the work done in taking a $$5kg$$ body of height $$4$$ meter above surface will be :-
    Solution
    The potential difference for a distance of $$20 m$$ is $$2  \  joule/kg$$.
    Now work done  $$=m \times$$ potential difference.
    Thus work done for a distance of $$4 m$$ for a mass $$5 kg$$,  $$W= \dfrac{4}{20} \times 2 \times 5$$
    $$\implies W= 2  J$$ 
  • Question 4
    1 / -0
    An object weighs $$10 N$$ at the north pole of theearth. In a geostationary satellite distance $$7R$$ from the centre of the earth (of radius $$R$$), the true weight and the apparent weight are.
    Solution
    Acceleration due to gravity at a height h from the surface ,  $$g'= g\bigg[1+\dfrac{h}{R}\bigg]^{-2}$$
    For radius of orbit $$= 7R    \implies h=6R$$
    $$mg'= mg\bigg[1+\dfrac{6R}{R}\bigg]^{-2}$$
    $$mg'= 10 \times  [7]^{-2}   N $$
    $$\implies W'= .2  N$$
    Also apparent weight of an object will bo zero.
  • Question 5
    1 / -0
    A body of mass $$m$$ is situated at distance $$4R_e$$ above the earth's surface, where $$R_e$$ is the radius of earth how much minimum energy be given to the body so that it may escape
    Solution
    Potential energy of the body at a distance 4$$R_e$$ from the surface of earth 
    $$U=-\dfrac{mgR_e}{1+n/R_e}$$

    $$=-\dfrac{mgR_e}{1+4}=-\dfrac{mgR_e}{5} $$  As  $$h=4R_e$$
    So, minimum energy required to escape the body will be $$\dfrac{mgR_e}{5}$$
  • Question 6
    1 / -0
    Read the assertion and reason carefully to mark the correct option out of the options given below :

    Assertion : Radius of circular orbit of a satellite is made two times, then it areal velocity will also become two times.
    Reason : Areal velocity is given as $$\dfrac {dA}{dt}=\dfrac {L}{2m}=\dfrac {mvr}{2m}$$
    Solution
    Areal velocity     $$\dfrac{dA}{dt}= \dfrac{L}{2m}=\dfrac{mvr}{2m}$$
    As there is no external torque, thus $$L=constant$$
    Now if radius of orbit increases by 2 times then the velocity of satellite will get reduced by 2 times so as to make $$L$$ to be constant.
    Hence overall, increasing $$r$$ has no effect on areal velocity.
    So the assertion is false.
  • Question 7
    1 / -0
    If 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 it. When both $$d$$ and $$h$$ are much smaller than the radius of earth, then
    Solution
    the value of 'g' at a height $$h$$ above the surface of the earth, $$g_h=g(1-\dfrac{2h}{R})$$
    the value of 'g' at a depth d, $$g_d=g(1-\dfrac{d}{R})$$
    But, $$g_h=g_d$$
    $$\therefore$$ $$1-\dfrac{2h}{R}=1-\cfrac{d}{R}$$
    or,  $$d=2h$$




  • Question 8
    1 / -0
    The weight of an object would be minimum when it is placed :
    Solution
    $$Answer:-$$ D
    Value of g at any point on  surface of earth is given by:-
    $${ g }^{ \prime  }=g-{ \omega  }^{ 2 }R\cos { \varphi  }$$
    At equator $$cos\varphi =1\ so\ { g }^{ \prime  }=g-{ \omega  }^{ 2 }R $$
    Value of $$\cos { \varphi  } <1$$ at every point other than equator.
    So, $$ { g }^{ \prime  }$$ will be more at any point other than equator relative to equator.
    Variation of $$g$$ with depth is given by:
    $$g_d=g(1-\dfrac{d}{R})$$
    So, when depth d is maximum g is minimum. So, weight (mg) will also be minimum.
  • Question 9
    1 / -0
    If $$A$$ is the areal velocity of planet of mass $$M$$. its angular momentum is
    Solution

    $$\textbf{Hint: First calculate $\omega$ and Moment of inertia of planet is, $I=M{R}^{2}$.}$$

    $$\textbf{Step 1: Calculating the angular velocity.}$$

    Given that the planet has an aerial velocity of A, Aerial velocity is given by,

    $$A=\dfrac{Area swept by radius vector}{Time taken}$$

    $$\Rightarrow A=\dfrac{\pi {{R}^{2}}}{T}$$ (Where R is the radius of the planet)

    We know that, $$T=\dfrac{2\pi }{\omega }$$

    $$\Rightarrow A=\dfrac{\omega {{R}^{2}}}{2}$$

    $$\Rightarrow \omega =\dfrac{2A}{{{R}^{2}}}$$

    $$\textbf{Step 2: Calculating the angular momentum.}$$

    Angular momentum of the planet will be, $$L=I\omega =M{{R}^{2}}\times \dfrac{2A}{{{R}^{2}}}$$

    $$\Rightarrow L=2MA$$

    $$\textbf{Thus, option (B) is correct.}$$
  • Question 10
    1 / -0
    The velocity of a planet revolving around the sun at three different times of a year is shown in the figure. Which among the following alternatives is correct ?

    Solution
    Kepler's law states that angular momentum is conserved.
    $$L  = constant$$
    $$v_{1} r_{1} = v_{2}r_{2} = v_{3}r_{3}$$
    r is the position vector from one point to the sun.
    As we can see from the ellipse:
    $$r_{3} > r_{2} > r_{1}$$
    Hence,
    $$v_{1} > v_{2} > v_{3}$$
    Option C is correct.
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