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Gravitation Test - 34

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Gravitation Test - 34
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  • Question 1
    1 / -0
    A man weighs $$80 kg$$ on the surface of earth of radius $$R$$. At what height above the surface of earth his weight will be $$40 kg$$?
    Solution
    Let $$r$$ be the distance from center of earth where it weighs 40 kg.
    $$W_{surface}=\dfrac{GMm}{R^2}$$
    $$W_{r}=\dfrac{GMm}{r^2}$$
    Since $$W_{r}=\dfrac{1}{2}W_{p}$$,
    $$r=\sqrt{2}R$$.
    Hence the height of this point$$=r-R=\sqrt{2}R-R=(\sqrt{2}-1)R$$
  • Question 2
    1 / -0
    Let $$V$$ and $$E$$ denote the gravitational potential and gravitational field at a point. It is possible to have
    Solution
    A) At $$\infty$$ both V and E are zero.
    B) Let, $$V_ \infty = \dfrac{GM}{R}$$ for an unit mass. 
    So, $$V_R = 0$$ i.e. at the radius $$R$$ of solid sphere(mass $$M$$) and $$ E_R = \dfrac{GM}{R^2} $$
    C) Inside a spherical shell V =$$\dfrac{-GM}{R}$$ and E =0
    Thus, all the above(D) is correct.
  • Question 3
    1 / -0
    The escape velocity of a projectile from the earth is approximately
    Solution
    The escape velocity of projectile from earth is
    $$\displaystyle v_{e}=\sqrt {2g{R_e}}$$, where $$\displaystyle R_{e}$$ is radius of earth
    since $$\displaystyle g=9.8m/sec^2, R_{e}=6.4\times10^6$$ metre
    $$\displaystyle \Rightarrow v_{e}=11.2km/sec$$
  • Question 4
    1 / -0
    The escape velocity of an object projected from the surface of a given planet is independent of
    Solution
    The escape velocity of an object from any planet is
    $$\displaystyle v_{escape}=\sqrt {2gR} = \sqrt {2GM/R}$$
    Where $$R$$ & $$M$$ are the radius & mass of the planet
  • Question 5
    1 / -0
    There is no atmosphere on the moon because.
    Solution
    There is no atmosphere at moon because escape velocity is less than the root mean square velocity of the molecules at moon. Hence all molecules escape.
  • Question 6
    1 / -0
    The weight of an object in the coal mine, sea level and at the top of the mountain, are respectively $$W_1$$, $$W_2$$ and $$W_3$$ then
    Solution
    At the surface of earth, the value of $$g=9.8m/sec^2$$. If we go towards the centre of earth or we go above the surface of earth, then in both the cases the value of $$g$$ decreases.
    Hence $$\displaystyle W_1=mg_{mine}, W_2=mg_{sea level}, W_3=mg_{mountain}$$
    So $$\displaystyle W_1<W_2>W_3$$     ($$g$$ at the sea  level $$=g$$ at the surface of earth)
  • Question 7
    1 / -0
    If $$g$$ is the acceleration due to gravity on the earth's surface, the gain in the potential energy of an object of mass $$m$$ raised from the surface of the earth to a height equal to the radius $$R$$ of the earth is
    Solution
    Gain in potential energy
    $$=(-\dfrac{GMm}{2R})-(-\dfrac{GMm}{R})$$
    $$=\dfrac{GMm}{R}-\dfrac{GMm}{2R}$$
    $$=\dfrac{GMm}{2R}$$
    $$=\dfrac{mgR^2}{2R}            As,  GM=gR^2$$
    $$=\dfrac{1}{2}mgR$$

  • Question 8
    1 / -0
    The weight of a body at the centre of the earth is
    Solution

    Hint:
    The magnitude of the gravitational force on a body equals the weight of the body.

    Solution:
    Step 1:
    Concept used:
    The force that pulls a body towards the center of the earth is its weight.
    $$W =mg$$ .......(1)
     
    where 'g' is the acceleration due to gravity, 
    W is the weight of a body of mass 'm'.

    Step2:
    A test mass always experiences an acceleration towards the center of the earth so it always tries to go towards the center of the earth. therefore, if the test mas is placed at the center of the earth then it will not feel any acceleration towards any other point, therefore the acceleration at the center of the earth is zero. 

    Calculating the weight of a body at the center of the earth:
    The force exerted by any portion of the Earth at its center will be neutralized by the force exerted by the opposite portion. When the value of g is substituted in equation (1) as zero, the total weight will be zero.

  • Question 9
    1 / -0
    The largest and the shortest distance of the earth from the sun is $$r_1$$ and $$r_2$$. Its distance from the sun when it is at perpendicular to the major axis of the orbit drawn from the sun:
    Solution
    Using the ellipse property is :
    $$2/R=1/r_1 + 1/r_2$$
    $$R=2r_1r_2/(r_1+r_2)$$
  • Question 10
    1 / -0
    Taking the gravitational potential at a point infinte distance away as zero, the gravitational potential at a point $$A$$ is $$-5$$ unit. If the gravitational potential at a point infinite distance away is taken as $$+10$$ units, the potential at a point $$A$$ is
    Solution
    The gravitational potential $$V$$ at a point distance $$'r'$$ from a body a mass $$m$$ is equal to the amount of work done in moving a unit mass from infinity to that point
    $$\displaystyle V_r-V_\infty =-\int_{\infty}^{r} \bar{E}.d \bar{r}=-GM (1/r-1/ \infty)$$
    $$\displaystyle = \frac {-GM}{r} \left [ As \bar{E}= \frac {-dV}{dr} \right ]$$

    $$(i)$$   In the first case
        when $$\displaystyle V_{\infty}=0, V_{r}=\frac {-GM}{r}= -5$$ unit
    $$(ii)$$   In the second case $$V_{\infty}=+10$$ unit
         $$\displaystyle V_{r}-10=-5$$
    or  $$\displaystyle V_{r}=+5$$ unit
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