Ir al contenido (pulsa Retorno)

Universitat Politècnica de Catalunya

    • Català
    • Castellano
    • English
    • LoginRegisterLog in (no UPC users)
  • mailContact Us
  • world English 
    • Català
    • Castellano
    • English
  • userLogin   
      LoginRegisterLog in (no UPC users)

UPCommons. Global access to UPC knowledge

Banner header
61.608 UPC E-Prints
You are here:
View Item 
  •   DSpace Home
  • E-prints
  • Grups de recerca
  • MMAC - Models Matemàtics aplicats a les ciencies humanes i de la natura
  • Articles de revista
  • View Item
  •   DSpace Home
  • E-prints
  • Grups de recerca
  • MMAC - Models Matemàtics aplicats a les ciencies humanes i de la natura
  • Articles de revista
  • View Item
JavaScript is disabled for your browser. Some features of this site may not work without it.

Dynamical behavior of asteroids near resonance: the 4:1 gap and the 7:2 group

Thumbnail
View/Open
Article (163,7Kb) (Restricted access)   Request copy 

Què és aquest botó?

Aquest botó permet demanar una còpia d'un document restringit a l'autor. Es mostra quan:

  • Disposem del correu electrònic de l'autor
  • El document té una mida inferior a 20 Mb
  • Es tracta d'un document d'accés restringit per decisió de l'autor o d'un document d'accés restringit per política de l'editorial
  View Usage Statistics
  LA Referencia / Recolecta stats
Cita com:
hdl:2117/14731

Show full item record
Grau Sánchez, MiguelMés informacióMés informació
González Casado, GuillermoMés informacióMés informacióMés informació
Document typeArticle
Defense date1999-08
Rights accessRestricted access - publisher's policy
Attribution-NonCommercial-NoDerivs 3.0 Spain
Except where otherwise noted, content on this work is licensed under a Creative Commons license : Attribution-NonCommercial-NoDerivs 3.0 Spain
Abstract
A comparative study of the evolution of the Sun–Jupiter–Asteroid system near the 4:1 and 7:2 resonances is performed by means of two techniques that proceed differently from the Hamiltonian corresponding to the planar restricted elliptic three-body problem. One technique is based on the classical Schubart averaging while the other is based on a mapping method in which the perturbing part of the Hamiltonian is expanded and the resulting terms are ordered according to a weight function that depends on the powers of eccentricities and the coefficients of the terms. For the mapping method the effect of Saturn on the asteroidal evolution is introduced and the degree of chaos is estimated by means of the Lyapunov time. Both methods are shown to lead to similar results and can be considered a suitable tool for describing the evolution of asteroids in the Kirkwood gap and the group corresponding to the 4:1 and 7:2 Jovian resonances, respectively.
CitationGrau, M.; González, G. Dynamical behavior of asteroids near resonance: the 4:1 gap and the 7:2 group. "Celestial mechanics and dynamical astronomy", Agost 1999, vol. 72, núm. 3, p. 169-186. 
URIhttp://hdl.handle.net/2117/14731
ISSN0923-2958
Collections
  • MMAC - Models Matemàtics aplicats a les ciencies humanes i de la natura - Articles de revista [12]
  • Departament de Matemàtiques - Articles de revista [3.099]
  View Usage Statistics

Show full item record

FilesDescriptionSizeFormatView
fulltext.pdfBlockedArticle163,7KbPDFRestricted access

Browse

This CollectionBy Issue DateAuthorsOther contributionsTitlesSubjectsThis repositoryCommunities & CollectionsBy Issue DateAuthorsOther contributionsTitlesSubjects

© UPC Obrir en finestra nova . Servei de Biblioteques, Publicacions i Arxius

info.biblioteques@upc.edu

  • About This Repository
  • Contact Us
  • Send Feedback
  • Privacy Settings
  • Inici de la pàgina