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Spin vector evolution for inner solar system asteroids
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory. Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Faculty of Science and Technology, Astronomical observatory.
1999 (English)In: PLANETARY AND SPACE SCIENCE, ISSN 0032-0633, Vol. 47, no 1-2, 11-22 p.Article in journal (Refereed) Published
Abstract [en]

The spin vector evolution of 30 asteroids in the inner solar system is investigated using 10 different orbital integrations for each object, since the orbital evolutions are chaotic for all the objects examined. Close encounters with major planets and res

Place, publisher, year, edition, pages
PERGAMON-ELSEVIER SCIENCE LTD , 1999. Vol. 47, no 1-2, 11-22 p.
Keyword [en]
NEAR-EARTH ASTEROIDS; SECULAR RESONANCES; CHAOTIC OBLIQUITY; DYNAMICS; MOTION; BEHAVIOR; POLE; MARS
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-85282OAI: oai:DiVA.org:uu-85282DiVA: diva2:113190
Note
Addresses: Skoglov Erik, Astron Observ, Box 515, S-75120 Uppsala, Sweden. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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