The escape velocity for a planet is \[{{v}_{e}}\]. A particle starts from rest at a large distance from the planet, reaches the planet only under gravitational attraction, and passes through a smooth tunnel through its centre. Its speed at the centre of the planet will be?
A: \[\sqrt{1.5}{{v}_{e}}\]
B: \[\dfrac{{{v}_{e}}}{\sqrt{2}}\]
C: \[{{v}_{e}}\]
D: zero
Answer
585.9k+ views
Hint: This problem can be solved easily by using the concept of gravitational potential. The gravitational potential can be defined at a point in the gravitational field as the work done per unit mass that would have to be done by some competent external force to bring a massive object to that point from some defined position of zero potential which is taken to be infinity.
Complete step by step answer:
We know that the value of gravitational potential at some distance from the earth’s surface is given by: \[-GM[\dfrac{3{{R}^{2}}-{{r}^{2}}}{2{{R}^{2}}}]\]
Where G is the universal gravitational constant, r is the distance from the centre of the earth to the point where gravitational potential is to be found, \[\rho \]is the density of the earth and R is the radius of the earth.
If we go at the centre of the earth then r=0 and the above expression reduce to
\[\dfrac{-3GM}{2R}\]
Now using energy conservation,
$ \dfrac{m{{v}^{2}}}{2}=m[0-(\dfrac{-3GM}{2R})] \\
\Rightarrow {{v}^{2}}=\dfrac{3GM}{2R} \\
\because GM=g{{R}^{2}} \\
\Rightarrow {{v}^{2}}=\dfrac{3g{{R}^{2}}}{2R} \\
\Rightarrow {{v}^{2}}=1.5gR \\
v=\sqrt{1.5gR} \\
\because {{v}_{e}}=\sqrt{gR} \\
\therefore v=\sqrt{1.5}{{v}_{e}} \\ $
So, the correct answer is “Option A”.
Note:
Gravitational potential has its origin in gravitational potential energy and the value of gravitational potential at a point is always negative and it assumes its maximum value only at infinity.
The gravitational potential is measured in the units of J/kg and its dimensional formula is \[[{{M}^{0}}{{L}^{2}}{{T}^{-2}}]\]. Here we have written the velocity in terms of escape velocity on the earth.
Complete step by step answer:
We know that the value of gravitational potential at some distance from the earth’s surface is given by: \[-GM[\dfrac{3{{R}^{2}}-{{r}^{2}}}{2{{R}^{2}}}]\]
Where G is the universal gravitational constant, r is the distance from the centre of the earth to the point where gravitational potential is to be found, \[\rho \]is the density of the earth and R is the radius of the earth.
If we go at the centre of the earth then r=0 and the above expression reduce to
\[\dfrac{-3GM}{2R}\]
Now using energy conservation,
$ \dfrac{m{{v}^{2}}}{2}=m[0-(\dfrac{-3GM}{2R})] \\
\Rightarrow {{v}^{2}}=\dfrac{3GM}{2R} \\
\because GM=g{{R}^{2}} \\
\Rightarrow {{v}^{2}}=\dfrac{3g{{R}^{2}}}{2R} \\
\Rightarrow {{v}^{2}}=1.5gR \\
v=\sqrt{1.5gR} \\
\because {{v}_{e}}=\sqrt{gR} \\
\therefore v=\sqrt{1.5}{{v}_{e}} \\ $
So, the correct answer is “Option A”.
Note:
Gravitational potential has its origin in gravitational potential energy and the value of gravitational potential at a point is always negative and it assumes its maximum value only at infinity.
The gravitational potential is measured in the units of J/kg and its dimensional formula is \[[{{M}^{0}}{{L}^{2}}{{T}^{-2}}]\]. Here we have written the velocity in terms of escape velocity on the earth.
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