Three stars, each of mass m, are located at the vertices of an equilateral triangle of side a. They revolve in circular orbit under mutual gravitational force while preserving the equilateral triangle. Find the mechanical energy of the system.
A
+Gm22a
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B
−3Gm22a
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C
−Gm22a
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D
+3Gm22a
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Solution
The correct option is B−3Gm22a Let us consider all the stars move in a common circle of radius r about the centroid O as shown in the figure.
Let us calculate the net force on any one of the three particles.
From figure,
sin60∘=a2r
⇒r=a√3
Net force on the particle placed at point A: Fnet=2Fcos30∘=2F√32=√3F (along AO)
Substituting the value of gravitational force F,
⇒Fnet=√3G(m)(m)a2=√3Gm2a2
Since they revolve in circular orbit under mutual gravitational force, so we have