Nearly 6000 multispectral images of Earth were acquired by the Galileo
spacecraft during its two flybys. The Galileo images offer a unique p
erspective on our home planet through the spectral capability made pos
sible by four narrowband near-infrared filters, intended for observati
ons of methane in Jupiter's atmosphere, which are not incorporated in
any of the currently operating Earth orbital remote sensing systems. S
pectral variations due to mineralogy, vegetative cover, and condensed
water are effectively mapped by the visible and near-infrared multispe
ctral imagery, showing a wide variety of biological, meteorological, a
nd geological phenomena. Global tectonic and volcanic processes are cl
early illustrated by these images, providing a useful basis for compar
ative planetary geology. Differences between plant species are detecte
d through the narrowband IR filters on Galileo, allowing regional meas
urements of variation in the ''red edge'' of chlorophyll and the depth
of the 1-mu m water band, which is diagnostic of leaf moisture conten
t. Although evidence of life is widespread in the Galileo data set, on
ly a single image (at similar to 2 km/pixel) shows geometrization plau
sibly attributable to our technical civilization Water vapor can be un
iquely imaged in the Galileo 0.73-mu m band, permitting spectral discr
imination of moist and dry clouds with otherwise similar albedo. Surfa
ce snow and ice can be readily distinguished from cloud cover by narro
wband imaging within the sensitivity range of Galileo's silicon CCD ca
mera. Ice grain size variations can be mapped using the weak H2O absor
ption at 1 mu m, a technique which may find important applications in
the exploration of the moons of Jupiter. The Galileo images have the p
otential 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 highe
r-resolution data from Earth orbiting systems and may provide a valuab
le reference point for future studies of global change.