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Gravitation Test - 35

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Gravitation Test - 35
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  • Question 1
    1 / -0
    The mass of the moon is $$1/81$$ of earth's mass and its radius $$1/4$$ that of the earth. If the escape velocity from the earth's surface is $$11.2$$ km/sec. its value from the surface of the moon will be
    Solution
    $$\displaystyle v_e = \sqrt {\frac{2GM_e}{R_e}}$$
    $$v_m = \sqrt {\dfrac{2G \dfrac{M_e}{81}}{\dfrac {R_e}{4}}}= \dfrac {2}{9}v_e$$
    $$\displaystyle =2/9 \times 11.2 kms^{-1}=2.5 kms^{-1}$$
  • Question 2
    1 / -0
    The gravitational potential difference between the surface of a planet and a point $$20 m$$ above the surface is $$2$$ joule/kgs. If the gravitational field is uniform, then the work done in carrying a $$5$$ kg body to a height of $$4 m$$ above the surface is
    Solution
    For uniform gravitational field,
    $$\displaystyle g =-\dfrac {V}{r}= - \frac {-2}{20}=\frac {1}{10}ms^{-2}$$

    Now, $$\displaystyle W= mgh = 5 \times \frac {1}{10}\times 4 = 2J$$
  • Question 3
    1 / -0
    In the region of only gravitational fields of mass '$$M$$' a particle is shifted from $$A$$ to $$B$$ via three different paths of length 5m, 10m and 25m. The work done in different paths is $$W_1, W_2, W_3$$ respectively then:
    Solution
    The gravitational field is a conservative field i.e. work done by gravitational field to displace a body is independent of its path. In other words, work done is determined by difference in potential energy at initial and final positions of body.
    Therefore, $$ W = P_f - P_i $$.($$ P_f $$ =final potential energy, $$ P_i $$ = Initial potential energy )
    So, $$ W_1 = P_B - P_A $$ and similarly
    $$ W_2 = P_B - P_A $$
    $$ W_3 = P_B - P_A $$
    Thus $$ W_1 = W_2 = W_3 $$
  • Question 4
    1 / -0
    The radius of a planet is $$1/4^{th}$$ of $$R_e$$ and its acc, due to gravity is $$2g$$. What would be the value of escape velocity on the planet, if escape velocity on earth is $$v_e$$
    Solution
    The escape velocity on the earth is defined as
    $$\displaystyle v_e = \sqrt {2g_eR_e}$$
    Where $$R_e$$ & $$g_e$$ are the radius & acceleration due to gravity of earth
    Now for planet $$\displaystyle g_p=2g_e, R_p=R_e/4$$
    So $$\displaystyle v_p =\sqrt {2g_pR_p}=\sqrt {2 \times 2g_e \times R_e/4}=\frac {v_e}{\sqrt {2}}$$
  • Question 5
    1 / -0
    A satellite of mass '$$m$$', moving around the earth in a circular orbit of radius $$R$$, has angular momentum $$L$$. The areal velocity of satellite is :
    Solution
    According to kepler's second law, areal velocity is constant .
    i.e. $$ A_v = \dfrac{rv}{2} = \dfrac{\omega r^2}{2} = \dfrac{L}{2m}$$
  • Question 6
    1 / -0
    Consider earth to be a homogeneous sphere. Scientist $$A$$ goes deep down in a mine and scientist $$B$$ goes high up in a balloon. The gravitational field measured by
    Solution
    $$Consider\quad Earth\quad to\quad be\quad a\quad uniform\quad solid\quad sphere.\\ Inside\quad the\quad sphere\quad g\quad \propto \quad R,\quad while\\ outside\quad the\quad sphere\quad g\propto \quad \dfrac { 1 }{ { R }^{ 2 } } \\ Hence,\quad the\quad observatvion\quad of\quad each\quad scientist\quad will\quad differ.$$
  • Question 7
    1 / -0
    The amount of work done in lifting a mass '$$m$$' from the surface of the earth to height $$2R$$ is
    Solution
    Work done $$\displaystyle = U_f-U_i$$

    $$\displaystyle =-\dfrac {GMm}{2R+R}-\left ( -\dfrac {Gmm}{R} \right )=\dfrac {2}{3}\dfrac {GmM}{R}=\dfrac {2}{3}mgR$$
  • Question 8
    1 / -0
    At what height from the surface of earth will the value of g be reduced by $$36$$% from the value at the surface? $$R = 6400km$$.
    Solution
    $${g}'=0.64g=\displaystyle\dfrac{g}{\left ( 1+\dfrac{h}{R} \right )}^{2}$$

    $$\Rightarrow  1+\dfrac{h}{R}=\dfrac{5}{4}$$

    $$h=\dfrac{R}{4}=1600\ km$$
  • Question 9
    1 / -0
    The total mechanical energy E possessed by a body of mass 'm',  moving with a velocity 'v' at a height 'h' is given by : $$E\, =\, \displaystyle \frac{1}{2}\, mv^{2}\, +\, mgh.$$ Make 'm' the subject of formula.
    Solution
    $$E= \frac{1}{2}mv^{2}+mgh$$

    Multiply both side 2:
    $$2E= mv^{2}+2mgh$$
    Or $$2E= m\left ( v^{2}+2gh \right )$$
    Or $$m= \dfrac{2E}{v^{2}+2gh}$$
  • Question 10
    1 / -0
    The change in potential energy, when a body of mass $$m$$ is raised to a height $$nR$$ from the earth's surface is $$(R=$$ radius of earth$$)$$
    Solution
    $$\displaystyle \bigtriangleup U=U_f-U_i=-\dfrac {GMm}{nR+h}-\left (-\dfrac {GMm}{R}\right )$$

    $$\displaystyle =\dfrac {n}{n+1}.\dfrac {GMm}{R}=\dfrac {n}{n+1}mgR$$
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