Mottola, S. and Hoffmann, H. and Gonano-Beurer, M. and Neukum, G. and Di Martino, M.(1) (1993) Physical Propertiesand Color Variegation of 243 Ida. European Geophysical Society, Wiesbaden,3.-7.Mai 1993.
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The asteroid 243 Ida will be the second fly-by target of the Galileo space probe. During the 1990 and 1991 apparitions, we performed CCDphotometry and spectrophotometry of ths S-type asteroid in order to determine its physical and dynamical properties. The measurements were performed with the DLR CCD-cameraat the observa- tories of Loiano (Italy) and ESO (La Silla, Chile). During these observations we obtained composite lightcurves in V-Johnson band, which we used to derived the magnitude-phase and the amlpitude-phase relation-ships. Rotational lightcurves were also acquired with spectral filters at 700nm and 950nm, representing respectively wavelengths near the maximum of the Ida relfection spectrum and the olivine-pyroxene absorption band. These measurements have revealed a significant variation of the 1-mm absorption of about 4% at a detection level of 3s. The observed variegation indicates a heterogeneous surface of 243 Ida, and is similar to the variations we detected which our observations of 951 Gaspra, which have been successively confirmed by the images returned by Galileo. We will perform additional observations of 243 Ida during its next opposition in 1993. the new results will also be presented at the meeting.
|Document Type:||Conference or Workshop Item (Speech)|
|Title:||Physical Propertiesand Color Variegation of 243 Ida|
|Event Title:||European Geophysical Society, Wiesbaden,3.-7.Mai 1993|
|HGF - Research field:||UNSPECIFIED|
|HGF - Program:||Space (old)|
|HGF - Program Themes:||W EW - Erforschung des Weltraums|
|DLR - Research area:||UNSPECIFIED|
|DLR - Program:||W EW - Erforschung des Weltraums|
|DLR - Research theme (Project):||UNSPECIFIED|
|Institutes and Institutions:||Institute of Planetary Research > Institut für Planetenerkundung|
|Deposited By:||elib DLR-Beauftragter|
|Deposited On:||02 Apr 2006|
|Last Modified:||27 Apr 2009 09:44|
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