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Gravitation Test - 56

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Gravitation Test - 56
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  • Question 1
    1 / -0
    The mass of the moon is $$\left(\dfrac{1}{8}\right)$$ of the earth but the gravitational pull is $$\left(\dfrac{1}{6}\right)$$ of the earth. It is due to the fact that:
    Solution
    We know that,  $$g = \dfrac{GM}{R^2}$$

    $$\dfrac{g_{M}}{g_{E}}=\dfrac{\dfrac{G\left({M_{E}}/{8}\right)}{R_{M}^{2}}}{\dfrac{GM_{E}}{R_{E}^{2}}}=\dfrac{R_{E}^{2}}{8R_{M}^{2}}$$              ....(i)
    where the sunscripts M and E are for the moon and the earth respectively.
    Given, $$\dfrac{g_{M}}{g_{E}}=\dfrac{1}{6}$$                             .....(ii)
    From (i) and (ii), we get
    $$\dfrac{R_{E}^{2}}{8R_{M}^{2}}=\dfrac{1}{6}$$ or 
    $${R}_{E}=\sqrt{\dfrac{8}{6}}R_{M}$$
  • Question 2
    1 / -0
    If density of a planet is double that of the earth and the radius 1.5 times that of the earth, the acceleration due to gravity on the surface of the planet is: 
    Solution
    The correct option is B

    We have,

    The density of the planet is double of the earth

    So, $$D_p=2D_e$$

    The radius of  the planet is equal to 1.5 times the radius of the earth

    So, $$R_p=1.5R_e$$

    Since$$ D_p=2D_e$$

    $$\dfrac{M_p}{\dfrac{4}{3}\pi R_p^3}=2\times\dfrac{M_e}{\dfrac{4}{3}4R_e^3}$$

    $$M_p=2\times(1.5)^3M_e$$

    So,

    $$\dfrac{g_p}{g_e}=\dfrac{\dfrac{GM_p}{R_P^2}}{\dfrac{GM_e}{R_e}^2}$$

    $$g_P=3g_e$$
  • Question 3
    1 / -0
    If the radius of the earth is made three times, keeping the mass constant, then the weight of a body on the earth's surface will be as compared to its previous value is 
    Solution
    Weight is nothing but mass multiplied by the acceleration due to gravity
                         ie    $$W=mg$$ ............(1)
    If Mass of earth is $$M$$ and radius is $$r$$ then gravitational acceleration,  $$g=GM/r^2$$

    According to question, radius is increased by three times 
     ie   $$r'=3r$$
        $$g'=GM/(3r)^2=GM/9r^2=\dfrac{g}{9}$$
         $$g'=\dfrac{g}{9}$$
    As gravity became one-ninth so from equation (1) the weight will also become one-ninth because mass of the body remain same.
  • Question 4
    1 / -0
    Two spheres of radius $$r=0.5 \ m$$ and mass $$ m = 1 \ kg$$ are placed in contact with each other, what will be the gravitational force between them:
    Solution
    The centre of mass of each sphere lies at the centre of the sphere. Thus, the spheres can be considered to be equal to point masses and they are separated by a distance equal to $$R=2 \times r=1 \ m$$

    The gravitational force of attraction is given by $$F = \dfrac{Gm_1m_2}{R^2}$$

    Hence,
    The force of attraction between them is $$F=\dfrac{Gm^2}{R^2}= \dfrac{G1^2}{1^2} = 6.67 \times 10^{-11}N$$

    The correct option is (B)

  • Question 5
    1 / -0
    A body of weight $$W_1$$ is suspended from the ceiling of a room through a chain of weight $$W_2$$. The ceiling pulls the chain by a force equal to:
    Solution
    The ceiling pulls the chain with a force equal to the sum of weights of chain and the body.  So the pulling force = (w1 + w2)
  • Question 6
    1 / -0
    The ratio between masses of two planets is 2 : 3 and the ratio between their radii is 3 : 2. The ratio between acceleration due to gravity on these two planets is:
    Solution
    Hint:Use the formula of acceleration due to gravity.

    Step 1:Writing the acceleration due to gravity on both the planet,
    Acceleration due to gravity on the first planet,
    $${g_1} = \dfrac{GM_1}{R_1^2}$$ ..................(i)
    Acceleration due to gravity on the second planet 
    $${g_1} = \dfrac{GM_2}{R_2^2}$$ ....................(ii)

    Step 2:Dividing equation (i) by equation (ii),
    $$\dfrac{g_1}{g_2} = \dfrac{M_1}{M_2} \times \dfrac{R_2^2}{R_1^2}$$
    $$ = \dfrac{2}{3} \times {\left( {\dfrac{2}{3}} \right)^2}$$
    $$ = \dfrac{8}{27}$$
    $$\textbf{Option B is correct.}$$
  • Question 7
    1 / -0
    A cricket ball is thrown up with a speed of $$19.6\ ms^{-1}$$. The maximum height it can reach is
    Solution
    Given,
    $$u=19.6m/s$$
    $$v=0m/s$$
    $$g=9.8m/s^2$$
    From 3rd equation of motion,
    $$2gh=v^2-u^2$$
    $$-2\times 9.8\times h=0^2-19.6\times 19.6$$
    $$h=\dfrac{19.6\times 19.6}{2\times 9.8}=19.6m$$
    The correct option is B.

  • Question 8
    1 / -0
    The SI unit of the universal gravitational constant G:
    Solution
    Force $$=\dfrac{G\ M_{1}\ M_{2}}{R^{2}}$$

    $$[G]=\dfrac{[Force][R]^{2}}{[M_{1}][M_{2}]}$$

    $$=\dfrac{N\ m^{2}}{(kg)^{2}}$$

    $$=N\ m^{2}\ kg^{-2}$$

    Option $$B$$.
  • Question 9
    1 / -0
    $$F = G\dfrac{m_1m_2}{R^2}$$ is the formula to prove ______. 
    Solution
    According to Newton's Law of Gravitation, every body attracts every other body with a constant force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
    $$F=G\dfrac{m_1m_2}{R^2}$$
  • Question 10
    1 / -0
    The gravitational force $$F_{g}$$ between two objects does not depend on
    Solution

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