Asteroid 951 Gaspra
This picture of asteroid 951 Gaspra is a combination of the
highest-resolution morphology and color information obtained by the Galileo
spacecraft during its approach to the asteroid on October 29, 1991. The Sun is
shining from the right; phase angle is 50 degrees. The base image is the best
black-and-white view of Gaspra (resolution 54 meters/pixel) on which are
superimposed the subtle color variations constructed from violet, green, and
near-infrared (1000 nanometers) images taken in an earlier sequence at a
resolution about 164 meters/pixel.
The very subtle color variations on Gaspra's surface have been artificially
exaggerated here; to first order Gaspra's color is fairly homogeneous over the
surface. However, subtle albedo and color variations do occur and are correlated
with surface topography in a significant way. In this false-color view, the
bluish areas represent regions of slightly higher albedo, which are also regions
of slightly stronger spectral absorption near 1000 nanometers, probably due to
the mineral olivine. These bluish areas tend to be associated with some of the
crisper craters and with ridges. The slightly reddish areas, apparently
concentrated in topographic lows, represent regions of somewhat lower albedo and
weaker absorption near 1000 nanometers. In general, such patterns can be
explained in terms of greater exposure of fresher rock in the brighter bluish
areas and the accumulation of some regolith materials in the darker reddish
areas.
Gaspra is an irregular body with dimensions about 19 x 12 x 11 kilometers (12
x 7.5 x 7 miles). The portion illuminated in this view is about 18 kilometers
(11 miles) from lower left to upper right.
This color picture results from a joint effort by image processing groups
at the U. S. Geological Survey in Flagstaff, Arizona, Cornell University in
Ithaca, New York, and JPL. The Galileo project, whose primary mission is the
exploration of the Jupiter system in 1995-97, is managed for NASA's Office of
Space Science and Applications by the Jet Propulsion Laboratory.

Last Update: 2005-Nov-29