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Intro to Energy Types
10. Conservation of Energy / Intro to Energy Types / Problem 7

Consider three planets, P1P_1 , P2P_2 , and P3P_3 , each with masses m1m_1 , m2m_2 , and m3m_3, initially positioned infinitely far apart. The work required to bring them into a stable equilateral triangular configuration around their common center of mass, where each side of the triangle has the same distance r, is given by:


W=G(m1m2r+m1m3r+m2m3r)W=-G\left(\frac{m_1m_2}{r}+\frac{m_1m_3}{r}+\frac{m_2m_3}{r}\right)


Does this work W correspond to the gravitational binding energy of the planetary system? Explain.

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