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A Study of Cybele asteroids II. Spectral properties of Cybele asteroids

Lagerkvist, C.-I. and Moroz, L. and Nathues, A. and Erikson, A. and Lahulla, F. and Karlsson, O. and Dahlgren, M. (2005) A Study of Cybele asteroids II. Spectral properties of Cybele asteroids. Astronomy and Astrophysics, 432, pp. 349-354.

Full text not available from this repository.

Abstract

We have used the 3.5 m New Technology Telescope at ESO, La Silla, to obtain spectra of 18 asteroids belonging to the Cybele group. One additional Cybele asteroid was observed with the ESO 3.6 m telescope. From the spectra we have derived spectral slopes and taxonomy classifications. Our observations show that spectrally red D-type Cybeles tend to be smaller than more spectrally neutral P- and C-type objects from this group. Similar colour-diameter trends have previously been reported for other outer belt low albedo asteroids (Hildas and Trojans). We discuss possible reasons for this trend. In particular, the observed dominance of red objects for small diameters is consistent with a space weathering scenario, where irradiation of asteroid regoliths with solar wind plasma neutralizes their surface colours due to carbonization of originally reddish organic components. Collisional disruption of such large greyish "aged" P-type objects would produce a number of redder D-type fragments lacking mature regoliths. In addition, the observed colour-diameter trend may be due to compositional differences between D-, P- and C-type asteroids. P- and C-types may be lacking at small diameters, since their materials are less susceptible to collisional break-up than spectrally red D-type material. A simultaneous contribution of both factors (compositional differences and space weathering) to the observed trend is possible as well.

Document Type:Article
Additional Information: LIDO-Berichtsjahr=2005,
Title:A Study of Cybele asteroids II. Spectral properties of Cybele asteroids
Authors:
AuthorsInstitution or Email of Authors
Lagerkvist, C.-I.Astronomical Observatory, Uppsala, Sweden
Moroz, L.UNSPECIFIED
Nathues, A.Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau
Erikson, A.UNSPECIFIED
Lahulla, F.Observatorio Astronomico, Madrid, Spain
Karlsson, O.Astronomical Observatory, Uppsala, Sweden
Dahlgren, M.Astronomical Observatory, Uppsala, Sweden
Date:2005
Journal or Publication Title:Astronomy and Astrophysics
Refereed publication:Yes
In ISI Web of Science:Yes
Volume:432
Page Range:pp. 349-354
Status:Published
Keywords:minor planets, asteroids
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:Institute of Planetary Research
Optical Information Systems
Deposited By: Susanne Pieth
Deposited On:09 Oct 2005
Last Modified:14 Jan 2010 19:54

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