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Question: The mass of the moon is \( \dfrac{1}{{81}} \) th of the earth but the gravitational pull is \( \dfra...

The mass of the moon is 181\dfrac{1}{{81}} th of the earth but the gravitational pull is 16\dfrac{1}{6} th of the earth.
(A) The radius of earth is 96\dfrac{9}{{\sqrt 6 }} of the moon.
(B) The radius of the moon is 816\dfrac{{81}}{6} of the earth.
(C) Moon is the satellite of the earth
(D) None of the above.

Explanation

Solution

Hint : The gravitational pull of the body is the acceleration due to gravitational force of the planet. From the law of gravitation, the gravitational pull is inversely proportional to the square of distance between two bodies.
The gravitational pull is expressed as,
g=Gmr2g = \dfrac{{Gm}}{{{r^2}}}
Here, mm is the mass of the body, rr is the radius distance and GG is the gravitational constant, which is equal to 6.67×1011  Nm2/kg26.67 \times {10^{ - 11}}\;{\rm{N}}{{\rm{m}}^{\rm{2}}}{\rm{/k}}{{\rm{g}}^{\rm{2}}} .

Complete Step By Step Answer:
From the given problem, the mass of the moon is 181\dfrac{1}{{81}} th of the earth, mm=181me{m_m} = \dfrac{1}{{81}}{m_e} and the gravitational pull of the mass of the moon is 16\dfrac{1}{6} th of the earth, gm=16ge{g_m} = \dfrac{1}{6}{g_e} .
We know that the gravitational pull is acceleration due to the gravitational force on the planet or satellite.
The gravitational pull of the planet earth,
ge=Gmere2{g_e} = \dfrac{{G{m_e}}}{{r_e^2}}
Rewrite the above equation,
re=Gmege{r_e} = \sqrt {\dfrac{{G{m_e}}}{{{g_e}}}} ... (I)
Similarly, the gravitational pull of the satellite moon,
gm=Gmmrm2{g_m} = \dfrac{{G{m_m}}}{{r_m^2}}
Rewrite the above equation,
rm=Gmmgm{r_m} = \sqrt {\dfrac{{G{m_m}}}{{{g_m}}}} ... (II)
Divide equation (I) and (II), we have,
rerm=GmegeGmmgm =me×gmge×mm \dfrac{{{r_e}}}{{{r_m}}} = \dfrac{{\sqrt {\dfrac{{G{m_e}}}{{{g_e}}}} }}{{\sqrt {\dfrac{{G{m_m}}}{{{g_m}}}} }}\\\ = \sqrt {\dfrac{{{m_e} \times {g_m}}}{{{g_e} \times {m_m}}}}
Now we substitute the given values in the above equation.
rerm=me×16gege×181me rerm=96 re=96rm \dfrac{{{r_e}}}{{{r_m}}} = \sqrt {\dfrac{{{m_e} \times \dfrac{1}{6}{g_e}}}{{{g_e} \times \dfrac{1}{{81}}{m_e}}}} \\\ \dfrac{{{r_e}}}{{{r_m}}} = \dfrac{9}{{\sqrt 6 }}\\\ {r_e} = \dfrac{9}{{\sqrt 6 }}{r_m}
Thus, the radius of earth is 96\dfrac{9}{{\sqrt 6 }} times the radius of the moon and option (a) is correct.

Note :
The value of acceleration due to the force of gravity of the planet or satellite is not depending on the mass of the planet, its size or its shape falling under the gravity. The universal law of gravitation holds everywhere. The value of acceleration due to gravity changes with the height and the depth. The angular velocity of rotation of earth affects the value of g.