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Question: Four particles of masses m, 2m, 3m and 4m are placed at the corners of a square of side of length ‘a...

Four particles of masses m, 2m, 3m and 4m are placed at the corners of a square of side of length ‘a’. The gravitational force on a particle of mass m placed at the centre of the square is
A) 42Gm2a24\sqrt 2 \dfrac{{G{m^2}}}{{{a^2}}}
B) 32Gm2a23\sqrt 2 \dfrac{{G{m^2}}}{{{a^2}}}
C) 22Gm2a22\sqrt 2 \dfrac{{G{m^2}}}{{{a^2}}}
D) 2Gm2a2\sqrt 2 \dfrac{{G{m^2}}}{{{a^2}}}

Explanation

Solution

Recall Newton’s law of universal gravitation. According to this law, every object attracts other objects in the universe. The force of attraction points in a straight line between the centre of both the objects. It is directly proportional to the mass of the objects and inversely proportional to the square of distance between them.

Complete step by step solution:
The formula for gravitational force is given by
F=Gm1m2r2F = \dfrac{{G{m_1}{m_2}}}{{{r^2}}}
Where G is the gravitational force
m1{m_1} is the mass of the first object
m2{m_2} is the mass of the second object
And ‘r’ is the distance between them
Given that the length of each side of the square is = a
The distance of each corner from the centre will be =a2 = \dfrac{a}{{\sqrt 2 }}

The gravitational force on point O due to point A is given by
F1=Gmm(a2)2=2Gm2a2\Rightarrow {F_1} = \dfrac{{Gmm}}{{{{(\dfrac{a}{{\sqrt 2 }})}^2}}} = \dfrac{{2G{m^2}}}{{{a^2}}}
Similarly, the gravitational force on point O due to point B is written as
F2=G(2m)(m)(a2)2=4Gm2a2\Rightarrow {F_2} = \dfrac{{G(2m)(m)}}{{{{(\dfrac{a}{{\sqrt 2 }})}^2}}} = \dfrac{{4G{m^2}}}{{{a^2}}}
The gravitational force on point O due to point C will be
F3=G(3m)(m)(a2)2=6Gm2a2\Rightarrow {F_3} = \dfrac{{G(3m)(m)}}{{{{(\dfrac{a}{{\sqrt 2 }})}^2}}} = \dfrac{{6G{m^2}}}{{{a^2}}}
The gravitational force on point O due to point D will be
F4=G(4m)(m)(a2)2=8Gm2a2\Rightarrow {F_4} = \dfrac{{G(4m)(m)}}{{{{(\dfrac{a}{{\sqrt 2 }})}^2}}} = \dfrac{{8G{m^2}}}{{{a^2}}}
The net force of F1{F_1}and F3{F_3}on point O is given by
F13=F3F1\Rightarrow {F_{13}} = {F_3} - {F_1}
F13=6Gm2a22Gm2a2=4Gm2a2\Rightarrow {F_{13}} = \dfrac{{6G{m^2}}}{{{a^2}}} - \dfrac{{2G{m^2}}}{{{a^2}}} = \dfrac{{4G{m^2}}}{{{a^2}}}
Similarly, the force of F2{F_2}andF4{F_4}on point O is given by
F24=F4F2\Rightarrow {F_{24}} = {F_4} - {F_2}
F24=8Gm2a24Gm2a2=4Gm2a2\Rightarrow {F_{24}} = \dfrac{{8G{m^2}}}{{{a^2}}} - \dfrac{{4G{m^2}}}{{{a^2}}} = \dfrac{{4G{m^2}}}{{{a^2}}}
The magnitude of net force on point O is given by
F=(F13)2+(F24)2\Rightarrow F = \sqrt {{{({F_{13}})}^2} + {{({F_{24}})}^2}}
F=(4Gm2a2)2+(4Gm2a2)2\Rightarrow F = \sqrt {{{(\dfrac{{4G{m^2}}}{{{a^2}}})}^2} + {{(\dfrac{{4G{m^2}}}{{{a^2}}})}^2}}
F=2.4G2m4a4\Rightarrow F = \sqrt {2.\dfrac{{4{G^2}{m^4}}}{{{a^4}}}}
F=22Gm2a2\Rightarrow F = 2\sqrt 2 \dfrac{{G{m^2}}}{{{a^2}}}

Option C is the right answer.

Note: It is important to note that since the force of gravitation is directly proportional to the mass of the object, so an object with more mass will have a large force of gravitation. But it varies inversely with the square of distance, so if the distance is doubled the force of gravitation will decrease by 4 times and so on.