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Librations with Mass Transfer in the Sun-Jupiter System

Horedt, G. P. and Oproiu, T. (2005) Librations with Mass Transfer in the Sun-Jupiter System. Acta Astronomica, 55, pp. 321-329.

Full text not available from this repository.

Abstract

Trojan-type motion is analytically and numerically studied under mass transfer between the primaries with conservation of their total orbital angular momentum. We prove theoretically and numerically our new result that angular libration widths change as m^1/4, (m - Jupiter mass) if they are throughout smaller than about 60 arcd. Numerical examples show that for initial libration widths larger than about 60 arcd, the Trojan is ultimately driven out of the libration domain, becoming an ordinary asteroid, if Jupiter's transferred mass increases by a factor less than about two. Certain processes occurring in our solar system and in extrasolar planetary systems lead to a decrease of the Trojan's libration amplitude, while other processes lead to an increase, respectively.

Item URL in elib:https://elib.dlr.de/20193/
Document Type:Article
Additional Information: LIDO-Berichtsjahr=2003,
Title:Librations with Mass Transfer in the Sun-Jupiter System
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Horedt, G. P.UNSPECIFIEDUNSPECIFIED
Oproiu, T.Observatorul Astronomic, Cluj, RumänienUNSPECIFIED
Date:September 2005
Journal or Publication Title:Acta Astronomica
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:Yes
Volume:55
Page Range:pp. 321-329
Status:Published
Keywords:Celestial mechanics, Minor planets, asteroids
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W - no assignment
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - no assignment (old)
Location: Oberpfaffenhofen
Institutes and Institutions:Institute of Planetary Research
Deposited By: Pieth, Susanne
Deposited On:01 Feb 2006
Last Modified:27 Apr 2009 04:45

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