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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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)|
|Title:||Long-term Orbital Evolution Study of (9969) 1992 KD|
|Event Title:||Annual Meeting of the DPS, Padua, Italy, Oct. 10-15, 1999|
|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|
|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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