Three body dynamics and its applications to exoplanets

This volume provides an overview of the gravitational orbital evolution of few-body systems, in particular those consisting of three bodies.

The authors present the historical context that begins with the origin of the problem as defined by Newton, which was followed up by Euler, Lagrange, Laplace, and many others.

Additionally, they consider the modern works from the 20th and 21st centuries that describe the development of powerful analytical methods by Poincare and others.