How do three celestial bodies move under their mutual gravitational attraction? This problem has been studied by Isaac Newton and leading mathematicians over the last two centuries. PoincarΓ©'s conclusion, that the problem represents an example of chaos in nature, opens the new possibility of using a
The Three-Body Problem
β Scribed by CHRISTIAN MARCHAL (Eds.)
- Publisher
- Elsevier Science
- Year
- 1990
- Tongue
- English
- Leaves
- 583
- Series
- Studies in Astronautics 4
- Category
- Library
No coin nor oath required. For personal study only.
β¦ Synopsis
Recent research on the theory of perturbations, the analytical approach and the quantitative analysis of the three-body problem have reached a high degree of perfection. The use of electronics has aided developments in quantitative analysis and has helped to disclose the extreme complexity of the set of solutions. This accelerated progress has given new orientation and impetus to the qualitative analysis that is so complementary to the quantitative analysis.
The book begins with the various formulations of the three-body problem, the main classical results and the important questions and conjectures involved in this subject. The main part of the book describes the remarkable progress achieved in qualitative analysis which has shed new light on the three-body problem. It deals with questions such as escapes, captures, periodic orbits, stability, chaotic motions, Arnold diffusion, etc. The most recent tests of escape have yielded very impressive results and border very close on the true limits of escape, showing the domain of bounded motions to be much smaller than was expected. An entirely new picture of the three-body problem is emerging, and the book reports on this recent progress.
The structure of the solutions for the three-body problem lead to a general conjecture governing the picture of solutions for all Hamiltonian problems. The periodic, quasi-periodic and almost-periodic solutions form the basis for the set of solutions and separate the chaotic solutions from the open solutions
β¦ Table of Contents
Content:
Studies in Astronautics
Page ii
Front Matter
Page iii
Copyright page
Page iv
Foreword
Pages v-vi
Victor SZEBEHELY
Dedication
Page vii
Acknowledgments
Page viii
Chapter 1 - Summaries
Pages 1-11
Chapter 2 - History
Pages 12-13
Chapter 3 - The Law of Universal Attraction
Page 14
Chapter 4 - Exact Formulations of the Three-Body Problem
Pages 15-20
Chapter 5 - The Invariants in the Three-Body Problem
Pages 21-29
Chapter 6 - Existence and Uniqueness of Solutions. Binary and Triple Collisions. Regularization of Singularities
Pages 30-35
Chapter 7 - Final Simplifications, the Elimination of Nodes, the Elimination of Time
Pages 36-40
Chapter 8 - Simple Solutions of the Three-Body Problem
Pages 41-57
Chapter 9 - The Restricted Three-Body Problem
Pages 58-78
Chapter 10 - The General Three-Body Problem. Quantitative Analysis
Pages 79-300
Chapter 11 - The General Three-Body Problem. Qualitative Analysis and Qualitative Methods
Pages 301-518
Chapter 12 - Main Conjectures and Further Investigations
Pages 519-522
Conclusions
Pages 523-526
Chapter APPENDIX I - Some Asymptotic Motions in a Very Particular Case of Integrability of the Three-Body Problem
Pages 527-530
Chapter APPENDIX II - The Halo Orbits Complements the Michalodimitrakis Family of Halo Orbits
Pages 531-537
Chapter APPENDIX III - Full Demonstration of the Near-Resonance Theorem
Pages 538-546
References
Pages 547-562
Bibliography
Pages 563-565
Subject Index
Pages 566-569
Author Index
Pages 570-576
π SIMILAR VOLUMES
How do three celestial bodies move under their mutual gravitational attraction? This problem has been studied by Isaac Newton and leading mathematicians over the last two centuries. PoincarΓ©'s conclusion, that the problem represents an example of chaos in nature, opens the new possibility of using a
Recent research on the theory of perturbations, the analytical approach and the quantitative analysis of the three-body problem have reached a high degree of perfection. The use of electronics has aided developments in quantitative analysis and has helped to disclose the extreme complexity of the se