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Gravitation Test - 23

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Gravitation Test - 23
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Weekly Quiz Competition
  • Question 1
    1 / -0
    The energy required to remove a body of mass 'm' from earths surface is/are equal to:
    Solution
    Potential energy required to remove a body of mass $$m$$ from earth's surface is $$mgR$$
  • Question 2
    1 / -0
     The escape velocity of projection from the earth is approximately ($$R = 6400 km$$).
    Solution
    $$V_{escape}=\sqrt{\cfrac{2GM}{R}}$$
    $$=\sqrt{\cfrac{2(6.67\times 10^{-11}\times 5.98\times 10^{24})}{6.38\times 10^{6}}}ms^{-1}$$
    $$=\sqrt{1.251\times 10^8} ms^{-1}$$
    $$=11184 ms^{-1}$$
    $$\approx 11.2 Kms^{-1}$$
  • Question 3
    1 / -0
    The earth retains its atmosphere because
    Solution
    The earth have atmosphere because earths escape velocity is move than mean speed of gaseous molecules, due to this reason gas can't escape.
  • Question 4
    1 / -0
    Two identical spherical masses are kept at some distance. Potential energy when a mass $$m$$ is taken from the surface of one sphere to the other
    Solution
    Centre point is unstable equilibrium position where potential energy is maximum.
    (c) first increases then decreases
  • Question 5
    1 / -0
    The weight of a body of mass $$3kg$$ at a height of $$12.8 \times 10^6m$$ from the surface of the earth is _______.
    Solution
    Given,
    $$Mass=3kg$$
    $$,h=128\times10^8=12.8\times10^7 \ m $$
    $$R=6.4\times10^6 \ m$$
    So, $$ h  = 12.8\times10^6=2R$$
    $$g'=g_m(\dfrac{R}{R+h})^2=9.8(\dfrac{R}{R+2R})^2=9.8(\dfrac{1}{3})^2=\dfrac{9.8}{9}$$
    Thus the weight,
    $$W=mg'=3\times \dfrac{9.8}{9}=3.26N$$
  • Question 6
    1 / -0
    Gravitational potential energy is negative. This implies 
    Solution
    Negative gravitational potential energy implies the particle is being bounded by the potential

    The correct option is (b)
  • Question 7
    1 / -0
    The weight of an astronaut in outer space is
    Solution

  • Question 8
    1 / -0
    The value of $$'g'$$ will be $$1$$% of its value at the surface of the earth at a height of $$(R_e = 6400km)$$ -
    Solution

    $${g^1} = g\left( {1 - {h \over R}} \right)$$

    $$g = g\left( {1 - {h \over R}} \right)$$

     $$1 = {h \over R},h = R$$

  • Question 9
    1 / -0
    If $$R$$ is the radius of the earth, then the value of acceleration due to gravity at a height $$h$$ from the surface of the earth will become half its value on the surface of the earth if
    Solution
    $$ g^{1} = \dfrac{Gm}{(R+h)^{2}} ...(1) $$ & at surface $$ g = \dfrac{Gm}{R^{2}} ...(2) $$
    given that $$ g^{1} = g/2 $$
    (1)/(2) we get $$ \dfrac{g^{1}}{g} = \dfrac{R^{2}}{(R+h)^{2}} $$
    Put $$ g^{1} = g/2 $$ we get $$ \dfrac{1}{2} = \dfrac{R^{2}}{(R+h)^{2}} $$
    $$ \Rightarrow \sqrt{2} = \dfrac{R+h}{R} = 1+\dfrac{h}{R} $$
    $$ \Rightarrow \dfrac{h}{R} = \sqrt{2}-1 \Rightarrow h = R(\sqrt{2}-1) $$

  • Question 10
    1 / -0
    If the distance between the earth and sun were to be doubled from its present value, the number of days in a year would be :
    Solution

    Given,

    Radius of rotation become double, $${{a}_{2}}=2{{a}_{1}}$$

    By Kepler’s law, $$T ^ { 2 }$$$$\alpha \,\,{{a}^{3}}$$

    $$\dfrac { T _ { 1 } ^ { 2 } } { a _ { 1 } ^ { 3 } }$$$$= \dfrac { T _ { 2 } ^ { 2 } } { a _ { 2 } ^ { 3 } }$$

    $$T _ { 2 } ^ { 2 }$$$$= \left( \dfrac { a _ { 2 } } { a _ { 1 } } \right) ^ { 3 } \times T _ { 1 } ^ { 2 }$$

    $$T _ { 2 } ^ { 2 }$$ $$={{\left( \dfrac{2}{1} \right)}^{3}}\times T_{1}^{2}$$

    $$T _ { 2 } ^ { 2 }$$ $$=8\times T_{1}^{2}$$

    $$T _ { 2 } ^ { 2 }$$ $$=\sqrt{8}\times 365\text{ days }$$

    $${{T}_{2}}=1032.37\text{ days }$$

    Hence, $$1032$$ days in year.

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