New spectral observations of Callisto and leading/trailing hemisphere distinctions

Details New spectral observations of Callisto and leading/trailing hemisphere distinctions New spectral observations of Callisto and leading/trailing hemisphere distinctions

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pggp.rept..294c&link_type=abstract

In NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990 p 294-295 (SEE N92-10728 01-91)

Physics

Geophysics

Atmospheric Composition, Callisto, Cometary Atmospheres, Infrared Telescopes, Spectra, Spectrometers, Spectrum Analysis, Ice, Leading Edges, Models, Signatures, Trailing Edges, Water

Scientific paper

In December 1989 and January 1990, new observations of the leading and trailing edges of Callisto were made from the NASA Infrared Telescope Facility on Mauna Kea in Hawaii. Using the Cool Grating Array Spectrometer, spectral coverage was obtained from 1.89 to 2.46 microns and from 2.8 to 4.2 microns for both the leading and trailing hemispheres. In addition, spectral coverage of the leading hemisphere was obtained from 1.30 to 2.55 microns and from 4.2 to 4.8 microns. Interpretations of the data are given.

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