Special Session 59
    Central configurations, periodic solutions, variational method and beyond in celestial mechanics
   Organizer(s):
    Zhifu Xie
 Introduction:
  This special session will concentrate on the latest developments in the field of celestial mechanics. In classical celestial mechanics, the motion of the planets and stars is governed by universal gravity and it is mathematically formulated as a second-order system of differential equations, known as the N-body problem. One of the most important types of solutions to the N-body problem is periodic in nature. Among this class of solutions, analyzing the structure and stability of simple, rigidly rotating orbits known as relative equilibria (or central configurations) leads to a greater understanding of the complexities in the full problem. The study of the N-body problem continues to attract researchers in a wide range of fields including dynamical systems, topology, variational methods, algebraic geometry and numerical methods. Much progress has been made recently in the study of the finiteness and stability questions in the N-body problem. This special session provides a marketplace for ideas, and helps identify trends and areas of new opportunity in the field. The session brings established researchers and recent Ph. D graduates together, some of whom are women or from groups underrepresented in mathematics. Some specific topics to be covered include central configurations, discovery of new periodic solutions, variational methods, regularization of collisions, absence of collisions, stability of periodic solutions, spacecraft orbital design and applications of Morse index and Maslov index to the N-body problem. If the schedule permits, we anticipate ending the session with a discussion on open problems.

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