An analysis of the three body problem
Abstract (Summary)
In this paper we will be presenting my approach to generating two possible
solutions to the three-body problem. We will first discuss the theory of reducing the
dimension of the dynamical system through the use of symmetry and constants of
motion. However, we can reduce no farther than to 5 degrees of freedom, which is
still too high to solve and therefore we must change our attack from trying to find
a general solution, to simply finding a specific solution.
We will then make use of the program Maple, which will allow me to create a
simulation of this system. Through the simulations we will try and find the stable
figure eight solution as well as a solution having a light satellite coming in from
infinity and being captured in a stable orbit around a tight binary. We can adjust
the initial conditions of the three bodies until we have generated a simulation that
has the potential to be a stable periodic orbit. Unfortunately Maple will not prove
that any solution found is stable, and we are therefore left with only a conjecture as
to the stability of the system.
Index words: Celestial Mechanics, n-Body Problem, Three-Body Problem,
3-Body Problem
An Analysis of the Three Body Problem
by
Mark E. Hannah
B.S., Oglethorpe University 1996
A Thesis Submitted to the Graduate Faculty
of The University of Georgia in Partial Fulfillment
of the
Requirements for the Degree
Master of Arts
Athens, Georgia
2002
c? 2002
Mark E. Hannah
All Rights Reserved
An Analysis of the Three Body Problem
by
Mark E. Hannah
Approved:
Major Professor: Dr. Malcolm Adams
Committee: Dr. Thomas Gard
Dr. Robert Varley
Electronic Version Approved:
Gordhan L. Patel
Dean of the Graduate School
The University of Georgia
Bibliographical Information:
Advisor:
School:The University of Georgia
School Location:USA - Georgia
Source Type:Master's Thesis
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