Here is the question:
A planet with mass $m$ and a second with mass $M$ are separated by a distance $d$. A third planet with mass $m_3$ happens to be midway between $M$ and $m$. Where could the third planet be positioned (distance from the larger planet $M$ in meters) so that the net gravitational force is zero?
My confusion lies with how to solve for the position of the third planet. I am given this equation to find the force between two planets at a given distance $r$: $$F = {GMm}/{r^2}$$ With this I can then set the sum of the two forces to zero: $$0 = {GMm_3}/r_1^2 + {Gmm_3}/r_2^2$$ My confusion lies in the fact that both $r_1$ and $r_2$ are unknown. However, we do know that $r_1 + r_2 = d$. But I am confused with how to solve for either $r_1$ or $r_2$.
