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Physical Properties of Near-Earth Asteroids from Thermal Infrared Observations and Thermal Modeling

Delbo, M. and Harris, A.W. (2002) Physical Properties of Near-Earth Asteroids from Thermal Infrared Observations and Thermal Modeling. Meteoritics and Planetary Science, 37 (12), pp. 1929-1936.

Full text not available from this repository.

Abstract

We review the physical principles on which asteroid thermal models are based and their application in the derivation of asteroid sizes and albedos. In particular, the use of simple thermal models to derive reliable diameters and albedos of near-Earth asteroids is discussed.

Document Type:Article
Additional Information: LIDO-Berichtsjahr=2003,
Title:Physical Properties of Near-Earth Asteroids from Thermal Infrared Observations and Thermal Modeling
Authors:
AuthorsInstitution or Email of Authors
Delbo, M.UNSPECIFIED
Harris, A.W.UNSPECIFIED
Date:2002
Journal or Publication Title:Meteoritics and Planetary Science
Refereed publication:Yes
In ISI Web of Science:Yes
Volume:37
Page Range:pp. 1929-1936
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 19:15

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