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Asteroid Models from Disk-Integrated Data

Kaasalainen, M. and Mottola, S. and Fulchignoni, M. (2002) Asteroid Models from Disk-Integrated Data. In: Asteroids III University of Arizona Press. pp. 139-150. ISBN 0-8165-2281-2.

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Abstract

Photometric observations are the primary source of information on the bulk of the asteroid population. The macroscopic shapes, rotational states, and scattering parameters of asteroids ca be deduced from photometric measurements of total brightness in different viewing/illumination geometries. Shape classes include convex, nonconvex, and binary objects, while rotational states include relaxed rotation, precessing motion, and mutually orbiting configurations. We discuss the role of lightcurve inversion in light of results from other sources.

Document Type:Book Section
Additional Information: LIDO-Berichtsjahr=2003,
Title:Asteroid Models from Disk-Integrated Data
Authors:
AuthorsInstitution or Email of Authors
Kaasalainen, M.University of Helsinki
Mottola, S.UNSPECIFIED
Fulchignoni, M.Observatoire de Paris
Date:2002
Journal or Publication Title:Asteroids III
Refereed publication:Yes
In ISI Web of Science:No
Page Range:pp. 139-150
Editors:
EditorsEmail
Bottke, W.F.UNSPECIFIED
Cellino, A.UNSPECIFIED
Paolicchi, P.UNSPECIFIED
Binzel, R.P.UNSPECIFIED
Publisher:University of Arizona Press
ISBN:0-8165-2281-2
Status:Published
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 19:17

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