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Journal of Geophysical Research | 1995

Galileo multispectral imaging of Earth

P. E. Geissler; W. Reid Thompson; Richard Greenberg; Jeff Moersch; Alfred S. McEwen; C. Sagan

Nearly 6000 multispectral images of Earth were acquired by the Galileo spacecraft during its two flybys. The Galileo images offer a unique perspective on our home planet through the spectral capability made possible by four narrowband near-infrared filters, intended for observations of methane in Jupiters atmosphere, which are not incorporated in any of the currently operating Earth orbital remote sensing systems. Spectral variations due to mineralogy, vegetative cover, and condensed water are effectively mapped by the visible and near-infrared multispectral imagery, showing a wide variety of biological, meteorological, and geological phenomena. Global tectonic and volcanic processes are clearly illustrated by these images, providing a useful basis for comparative planetary geology. Differences between plant species are detected through the narrowband IR filters on Galileo, allowing regional measurements of variation in the red edge of chlorophyll and the depth of the 1-micrometer water band, which is diagnostic of leaf moisture content. Although evidence of life is widespread in the Galileo data set, only a single image (at approximately 2 km/pixel) shows geometrization plausibly attributable to our technical civilization. Water vapor can be uniquely imaged in the Galileo 0.73-micrometer band, permitting spectral discrimination of moist and dry clouds with otherwise similar albedo. Surface snow and ice can be readily distinguished from cloud cover by narrowband imaging within the sensitivity range of Galileos silicon CCD camera. Ice grain size variations can be mapped using the weak H2O absorption at 1 micrometer, a technique which may find important applications in the exploration of the moons of Jupiter. The Galileo images have the potential to make unique contributions to Earth science in the areas of geological, meteorological and biological remote sensing, due to the inclusion of previously untried narrowband IR filters. The vast scale and near global coverage of the Galileo data set complements the higher-resolution data from Earth orbiting systems and may provide a valuable reference point for future studies of global change.


Archive | 1992

Organic chemistry on Titan: Surface interactions

W. Reid Thompson; C. Sagan


Archive | 1994

Optical Constants of Triton Tholin: Preliminary Results

B. N. Khare; C. Sagan; M. N. Heinrich; William R. Thompson; E. T. Arakawa; P. S. Tuminello; Matthew D. H. Clark


Archive | 1983

Reflection Spectra of Model Titan Atmospheres and Aerosols

C. Sagan; William R. Thompson; B. N. Khare


Archive | 1992

Impact-Mediated Chemical Evolution on Titan

William R. Thompson; C. Sagan; David B. Stephenson; Matthew Wing


Archive | 1986

Radiation Darkening of CH4-clathrate: Implications for the Uranian Satellites

C. Sagan; William R. Thompson; B. N. Khare; B. G. J. P. T. Murray


Archive | 1992

Titan's organic chemistry: Results of simulation experiments

C. Sagan; W. Reid Thompson; B. N. Khare


Archive | 1989

Depth to Unoxidized Material in the Martian Regolith

Christopher Frank Chyba; Steven W. Squyres; C. Sagan


Archive | 1985

Photometry, Multiple Light Scattering, and Lab Simulations: Constraints on the Structure of Titan's Haze/Cloud.

C. Sagan; William R. Thompson; Steven W. Squyres; B. N. Khare


Archive | 1984

Time-Evolution of Infrared Absorption Features in an Oxygen-Free Titan Organic Synthesis Experiment

B. N. Khare; William R. Thompson; C. Sagan; Maren Leyla Cooke; Joseph A. Dimauro; B. G. J. P. T. Murray; E. T. Arakawa

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B. N. Khare

Smithsonian Astrophysical Observatory

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E. T. Arakawa

Oak Ridge National Laboratory

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