Disk-resolved Spectral Characteristics of Ganymede and Callisto
Abstract
Three different kinds of spectral signatures for ice and nonice components found on Ganymede and Callisto are discussed. The reasons for this, possibly material differences or grain size effects, are addressed.
- Publication:
-
Lunar and Planetary Science Conference
- Pub Date:
- March 1997
- Bibcode:
- 1997LPI....28..293D
- Keywords:
-
- Ganymede;
- Callisto;
- Spectral Signatures;
- Satellite Surfaces;
- Planetary Composition;
- Grain Size;
- Minerals;
- Spectrum Analysis;
- Spectral Resolution;
- Lunar and Planetary Exploration;
- CALLISTO;
- GANYMEDE;
- SATELLITES: GALILEAN;
- SPECTRAL ANALYSIS