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Question: The gravitational force between two particles is F, if the objects are stationary and separated by a...

The gravitational force between two particles is F, if the objects are stationary and separated by a distance of 1m. If the object starts moving in opposite directions, from rest with uniform acceleration of a=1m/s2a = 1m/{s^2}, then the force between them after 3 seconds will be
A. 4F81\dfrac{{4F}}{{81}}
B. F100\dfrac{{F}}{{100}}
C. 4F121\dfrac{{4F}}{{121}}
D.F2\dfrac{{F}}{{2}}

Explanation

Solution

In the problem, two particles are given that are separated by certain distance. The gravitational force between two particles is attractive and can be given by Newton’s Law of Universal Gravitation. When these two particles move apart in opposite directions, the gravitational force between them will decrease as it inversely depends on the distance between two particles.

Formula Used:
Newton’s Law of Universal Gravitation is given as:
F=Gm1m2r2F = \dfrac{{G{m_1}{m_2}}}{{{r^2}}}
where, GG is the gravitational constant, FF is the gravitational force , m1{m_1} is the mass of particle 1, m2{m_2} is the mass of particle 2 and rr is the distance between two particles.
Distance between two particles (if travelling in uniform acceleration):
r=12at2r' = \dfrac{1}{2}a{t^2}
rr' is the distance between two particles (after uniform acceleration), aa is uniform acceleration and tt is the time period.

Complete step by step answer:
Two particles are given with a gravitational force FFacting between them. Let the mass of these two particles be m1{m_1}and m2{m_2}respectively. They are stationary and the distance between them is 1m1m. Let the distance be denoted as rr. Therefore, r=1mr = 1m.
By Newton’s Law of Universal Gravitation, every object having a mass attracts every other object by a force FF that is directly proportional to its masses m1{m_1} and m2{m_2}and inversely proportional to the square of the distance rrbetween them. Thus, Force FFis written as
F=Gm1m2r2F = \dfrac{{G{m_1}{m_2}}}{{{r^2}}}
where, GG is the gravitational constant.
Substituting the value r=1mr = 1m. Therefore,

\Rightarrow F = G{m_1}{m_2}$$ $$ \to (1)$$ Now, these particles start moving in opposite directions, from rest with uniform acceleration of $$a = 1m/{s^2}$$ . The distance between them after 3 seconds can be calculated by the following formula. Let $$t = 3s$$. Let $$r'$$ be the distance between these two particles. Then, $$r'$$is given as $$r' = \dfrac{1}{2}a{t^2}$$ where, $$a$$ is the acceleration and $$t$$ is the time. Thus, $$r' = \dfrac{1}{2}a{t^2} \\\ \Rightarrow r' = \dfrac{1}{2}\left( 1 \right){\left( 3 \right)^2} \\\ \Rightarrow r' = \dfrac{9}{2}$$ $$ \to (2)$$ Let the gravitational force after they move a distance apart in 3 seconds be $$F'$$. Then, $$F'$$ is given as $$F' = \dfrac{{G{m_1}{m_2}}}{{{{r'}^2}}}$$ Substituting the value of $$r'$$from equation (2) $$F' = \dfrac{{G{m_1}{m_2}}}{{{{\left( {\dfrac{9}{2}} \right)}^2}}} \\\ \Rightarrow F' = \dfrac{{G{m_1}{m_2}}}{{\left( {\dfrac{{81}}{4}} \right)}} \\\ \Rightarrow F' = \dfrac{{4G{m_1}{m_2}}}{{81}}$$ $$ \to (3)$$ Equation (2) can also be written as $$G{m_1}{m_2} = \dfrac{{81F'}}{4}$$ $$ \to (4)$$ Equating equations (1) and (3) $$F = \dfrac{{81F'}}{4} \\\ \therefore F' = \dfrac{{4F}}{{81}}$$ **Hence, option A is the correct answer.** **Note:** Consider equations (1) and (2). If the particles move apart, the force and the distance between them will change. Note that the values of $$G$$ (the gravitational constant), $${m_1}$$(mass of particle 1) and $${m_2}$$(mass of particle 2) will remain unchanged. Greater the distance between two particles, lesser is the gravitational force acting within them. The gravitational force is always attractive.