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Long-term Orbital Evolution Study of (9969) 1992 KD

Hahn, G. and Lagerkvist, C.-I. and Oberst, J. (1999) Long-term Orbital Evolution Study of (9969) 1992 KD. Annual Meeting of the DPS, Padua, Italy, Oct. 10-15, 1999.

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Abstract

The orbital evolution of this asteroid has been studied by numerical integration methods, taking into account the pertubations by all major planets (Mercury through Neptune, Earth and Moon were treated as a single body). An interval of +/- 1 million year into the future and past is covered by these calculations. The latest osculating orbital elements were used, together with nine variational orbits in order to study the long-term dynamical evolution in a statistical sense. Conclusions about the dynamical lifetime of the orbit, and its implication for the age of the asteroid's surface will be discussed.

Document Type:Conference or Workshop Item (Speech)
Additional Information: LIDO-Berichtsjahr=1999,
Title:Long-term Orbital Evolution Study of (9969) 1992 KD
Authors:
AuthorsInstitution or Email of Authors
Hahn, G.UNSPECIFIED
Lagerkvist, C.-I.Astronomical Observatory, Uppsala, Sweden
Oberst, J.UNSPECIFIED
Date:1999
Status:Published
Event Title:Annual Meeting of the DPS, Padua, Italy, Oct. 10-15, 1999
Organizer:AAS-DPS
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):UNSPECIFIED
Location: Berlin-Adlershof
Institutes and Institutions:Institut für Weltraumsensorik und Planetenerkundung
Deposited By: Susanne Pieth
Deposited On:16 Sep 2005
Last Modified:14 Jan 2010 18:21

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