The discussion centers on the challenges of solving the three-body problem in Newtonian physics, highlighting that while equations can be defined for three interacting bodies under gravity, they lack closed-form solutions and must be approached numerically. The equations become nonlinear due to the dependence of gravitational force on the inverse square of the distance between bodies. Most nonlinear differential equations do not yield closed-form solutions, with the two-body problem being a notable exception that can be simplified. The terminology distinction between "many-body problem" and "N-body problem" is also emphasized, as the former typically refers to complex interactions in condensed matter physics. The conversation underscores the importance of understanding these concepts for further study in celestial mechanics.