Spectral reflectivities of the Galilean satellites and Titan, 0.32 to 0.86 micrometers

Details Spectral reflectivities of the Galilean satellites and Titan, 0.32 to 0.86 micrometers Spectral reflectivities of the Galilean satellites and Titan, 0.32 to 0.86 micrometers

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978icar...36..304n&link_type=ejournal

Icarus, vol. 36, Dec. 1978, p. 304-329. NASA-supported research.

Astronomy and Astrophysics

Astronomy

24

Astronomical Spectroscopy, Galilean Satellites, Planetary Composition, Spectral Reflectance, Titan, Ultraviolet Astronomy, Hydrogen Sulfide, Lunar Albedo, Methane, Planetary Atmospheres, Planetary Surfaces, Spectrophotometry, Sulfur, Venus (Planet), Observations, Spectrophotometry, Wavelengths, Jupiter, Satellites, Titan, Micrometers, Spectrum, Io, Moon, Spectral Reflectivity, Absorption Spectra, Europa, Ganymede, Callisto, Atmosphere, Methane, Sulfur, Mixing, Irradiation, Outgassing, Comparisons

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