Comparison of the Surface Composition on Different Regions of Saturn's Satellites
Denk, T. and Jaumann, R. and Neukum, G. (1993) Comparison of the Surface Composition on Different Regions of Saturn's Satellites. In: BAAS, 3, p. 1114. 25th Annual Meeting of the AAS, Division for Planetary Sciences, Boulder, Colorado, 18-22 October 1993.
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Voyager 1 nad 2 images of the six Saturnian satellites Mimas, Enceladus, Tethys, Dione, Rhea and Iapetus have been investigated in the orange (OR), grren (GR), and violet (VI) spectral range. The objective of our study was to examine and compare spectra differences of surface features in order to obtain information about compositional trends. After several steps of data reduction, the OR, GR, and VI reflectances of 324 selected points have been measured. Additionally,the six satellite surfaces have been subdivided into 50 spectral or photogeological homogenious regions. The "spectra" of these 50 regions, which have been made out from the 324 measured spectra, are the basis of our interpretation.
|Document Type:||Conference or Workshop Item (Speech)|
|Additional Information:||LIDO-Berichtsjahr=1993, pages=1,|
|Title:||Comparison of the Surface Composition on Different Regions of Saturn's Satellites|
|Journal or Publication Title:||BAAS|
|Page Range:||p. 1114|
|Keywords:||Composition, Saturnian Satellites, Voyager images, End-members, Spectra|
|Event Title:||25th Annual Meeting of the AAS, Division for Planetary Sciences, Boulder, Colorado, 18-22 October 1993|
|HGF - Research field:||UNSPECIFIED|
|HGF - Program:||no assignment|
|HGF - Program Themes:||no assignment|
|DLR - Research area:||UNSPECIFIED|
|DLR - Program:||no assignment|
|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 09:45|
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