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Gravitation Test - 26

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Gravitation Test - 26
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  • Question 1
    1 / -0
    The angular velocity of rotation of a star (mass M and radius R), such that the matter will start escaping from its equator is:
    Solution
    $$v_{esc} = \sqrt{ \dfrac{2GM}{R}}$$
    $$ \omega R = \sqrt{ \dfrac{2GM}{R}}$$
    $$ \therefore \omega = \sqrt{ \dfrac{2GM}{R^3}}$$
    $$\omega =\displaystyle \dfrac{1}{R}\sqrt{\dfrac{2GM}{R}}$$
  • Question 2
    1 / -0
    A body of mass $$m$$ is raised from the surface of the earth to a height $$nR$$ ($$R$$-radius of earth). Magnitude of the change in the gravitational potential energy of the body is ($$g$$- acceleration due to gravity on the surface of earth) :
    Solution
    Change in P.E.$$ = \dfrac {-GMm}{(n+1)R} - (\dfrac{-GMm}{R}) = (\dfrac {GMm}{(n+1)R}) ( -1 + (n+1)) $$
    $$= (\dfrac {GMm}{R}) \dfrac{(n)}{n+1}$$
    But $$ g = GM/R^2$$ or $$GM = g R^2$$
    Putting this value, we get Change in P.E. $$= mgR (\dfrac {n}{n+1})$$
  • Question 3
    1 / -0
    The work done to increase the radius of orbit of a satellite of mass $$m$$ revolving around a planet of mass $$M$$ from orbit of radius $$R$$ into another orbit of radius $$3R$$ is :
    Solution
    The gravitational force '$$F$$' on satellite of mass 'm' revolving around the planet in the orbit of radius '$$R$$' is
    $$F = -  \dfrac{GMm}{R^2} $$
    Where
    $$G$$ is gravitational constant
    $$M$$ is Mass of the planet.
    The work done in increasing the radius of orbit of the satellite through '$$dr$$' is
    $$W = F  dr $$
    but work done is equal to change in gravitational potential '$$-dV$$'
    therefore
    $$ -dV = F dr $$
    $$V = - \int_{R}^{3R}F  dr$$
    $$V = -\dfrac{GMm}{R^2}\int_{R}^{3R}-(F dr)$$
    $$V = GMm\int_{R}^{3R}\dfrac {1}{R^2}dr$$
    $$V = \dfrac{GMm}{R} - \dfrac{GMm}{3R}$$
    $$V = \dfrac{2GMm}{3R}$$
    Thus work done to increase the radius of orbit of satellite is $$ \dfrac{2GMm}{3R}$$
  • Question 4
    1 / -0
    If $$g$$ is 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
    Value of g is given by: $$g=\dfrac { { GM }_{ e } }{ { R }^{ 2 } } $$ 
     Initial Potential Energy: $${ U }_{ i }=-\dfrac { { GM }_{ e }m }{ { R } } =-MgR$$
    Final Potential Energy: $$U_f =-\dfrac { { GM }_{ e }m }{ { 2R } } =-MgR/2$$
    Therefore Gain in Potential Energy: $${ U }_{ f }-{ U }_{ i }=-MgR/2-(-MgR)=\dfrac{MgR}{2}$$ 
  • Question 5
    1 / -0
    Energy required to move a body of mass m from an orbit of radius 2R to 3R is:
    Solution
    $$\text{Energy required} =\text{(Final potential-Initial potential)m}$$
    $$\text{Energy required}=-\dfrac{GMm}{3R}-\dfrac{-GMm}{2R}=\dfrac{GMm}{6R}$$
  • Question 6
    1 / -0
    The change in the P.E., when a body of mass $$m$$ is displaced from Earth's surface to a vertical height equal to radius of earth (g $$=$$ acceleration due to gravity on earth surface) is:
    Solution
    $$\displaystyle \Delta PE=\frac{GMm}{R}\left \{ 1-\frac{1}{2} \right \}=
    \displaystyle \frac{GMm}{2R}$$
    $$gR=\displaystyle \frac{GM}{R}$$
    $$ \displaystyle \Delta PE=\frac{mgR}{2}$$
  • 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

    Gravitational potential energy on the earth surface, $$U_{r}=\displaystyle \dfrac{-GMm}{R}$$

    Gravitational potential energy at a height h above the earth's surface, $$U_{h}=\displaystyle \dfrac{-GMm}{R+h}$$

    $$ U_{h}=\displaystyle \dfrac{-GMm}{R+R}=\dfrac{-GMm}{2R}$$

    Gain in gravitational potential energy $$=U_{h}-U_{r}$$

    $$=\displaystyle \dfrac{-GMm}{2R}-(\dfrac{-GMm}{R})=\dfrac{GMm}{R}-\dfrac{GMm}{2R}$$

    $$=\displaystyle \dfrac{GMm}{2R}=\dfrac{1}{2}mgR$$

  • Question 8
    1 / -0
    A small body is initially at a distance $$r$$ from the centre of earth. $$r$$ is greater than the radius of the earth. If it takes $$W$$ joules of work to move the body from this position to another position at a distance $$2r$$ measured from the centre of earth, then how many joules would be required to move it from this position to a new position at a distance of $$3r$$ from the centre of the earth.
    Solution
    Work done to move the body in the gravitational field is equal to change in the potential energy of the body.
    i.e.
    $$W=-\dfrac {GMm}{2r}-\left(-\dfrac {GMm}{r}\right)$$

    $$\Rightarrow W = \dfrac {GMm}{2r}$$
    Now when the body is moved from $$2r$$ to $$3r$$, change in PE is
    $$W'=-\dfrac {GMm}{3r}-\left(-\dfrac {GMm}{2r}\right)=\dfrac {1}{3}\dfrac {GMm}{2r}=\dfrac {W}{3}$$
  • Question 9
    1 / -0
    A satellite of mass $$m$$ moves along an elliptical path around the earth. The areal velocity of the satellite is proportional to
    Solution
    The areal velocity $$ \dfrac{dA}{dt}$$ $$=$$constant
    $$\dfrac{dA}{dt}=\dfrac{L}{2 m}$$

    $$L=mvr \sin \theta$$ (angular momentum)

    $$\dfrac{dA}{dt}=\dfrac{mvr \sin \theta}{2m}$$$$= v r \sin \theta$$

    $$\therefore \dfrac{dA}{dt} \ \alpha\ m^0$$
  • Question 10
    1 / -0
    A person bring a mass of $$1 kg$$ from infinite to point $$A$$. Initially the mass was at rest but is moves a speed of $$2 m /s$$ as it reaches to $$A$$. The workdone by the person on mass is $$-3 J$$ the gravitational potential at $$A$$ is
    Solution
    $$K.E_{f}=1.2^2/2=2$$
    Work Energy Theorem,
    $$E_{f}-E_{i}=W$$
    $$2+P.E-0=-3$$
    $$P.E=mV=-5$$
    $$V=-5$$ since $$m=1$$
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