Laboratory reflection spectra for the determination of chemical composition of ice bodies

Details Laboratory reflection spectra for the determination of chemical composition of ice bodies Laboratory reflection spectra for the determination of chemical composition of ice bodies

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976icar...28..379l&link_type=abstract

Icarus, vol. 28, July 1976, p. 379-387.

Computer Science

12

Chemical Composition, Ice, Jupiter (Planet), Natural Satellites, Saturn (Planet), Saturn Rings, Spectral Reflectance, Gas Mixtures, Infrared Spectra, Planetary Composition

Scientific paper

The visible (0.3 to 1.03 microns) spectral reflectances of N2O, NH3,
H2S, and NH4HS frosts and mixtures of these frosts as well as their
UV-irradiated products have been measured. These spectra are compared
with the spectra of the Galilean satellites of Jupiter, Saturn's rings,
and Saturn's satellites to place limits on their surface compositions.

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