Generating Families in the Restricted Three-Body Problem: Lecture Notes in Physics Monographs, cartea 52
Autor Michel Henonen Limba Engleză Hardback – 27 noi 1997
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Specificații
ISBN-13: 9783540638025
ISBN-10: 3540638024
Pagini: 296
Ilustrații: XI, 280 p.
Dimensiuni: 155 x 235 x 22 mm
Greutate: 0.59 kg
Ediția:1997
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria Lecture Notes in Physics Monographs
Locul publicării:Berlin, Heidelberg, Germany
ISBN-10: 3540638024
Pagini: 296
Ilustrații: XI, 280 p.
Dimensiuni: 155 x 235 x 22 mm
Greutate: 0.59 kg
Ediția:1997
Editura: Springer Berlin, Heidelberg
Colecția Springer
Seria Lecture Notes in Physics Monographs
Locul publicării:Berlin, Heidelberg, Germany
Public țintă
ResearchCuprins
Definitions and Properties.- Generating Orbits of the First Species.- Generating Orbits of the Second Species.- Generating Orbits of the Third Species.- Bifurcation Orbits.- Junctions: Symmetry.- Junctions: Broucke’s Principle.- Fragments.- Generating Families.
Recenzii
From the reviews
"The book is an excellent overview of the state-of-the-art of the restricted three-body problem."
Zentralblatt für Mathematik, 1998
"The book is an excellent overview of the state-of-the-art of the restricted three-body problem."
Zentralblatt für Mathematik, 1998
Textul de pe ultima copertă
The classical restricted problem of three bodies is of fundamental importance for its applications to astronomy and space navigation, and also as a simple model of a non-integrable Hamiltonian dynamical system. A central role is played by periodic orbits, of which a large number have been computed numerically. In this book an attempt is made to explain and organize this material through a systematic study of generating families, which are the limits of families of periodic orbits when the mass ratio of the two main bodies becomes vanishingly small. The most critical part is the study of bifurcations, where several families come together and it is necessary to determine how individual branches are joined. Many different cases must be distinguished and studied separately. Detailed recipes are given. Their use is illustrated by determining a number of generating families, associated with natural families of the restricted problem, and comparing them with numerical computations in the Earth-Moon and Sun-Jupiter case.
Caracteristici
The first classification of the orbit structure of a seemingly non-integrable system in every detail