(See description below)

Asteroid Gaspra
- This picture of asteroid 951 Gaspra is a mosaic of two
images taken by the Galileo spacecraft from a range of
5,300 kilometers (3,300 miles), some 10 minutes before
closest approach on October 29, 1991. The Sun is shining
from the right; phase angle is 50 degrees. The
resolution, about 54 meters/pixel, is the highest for the
Gaspra encounter and is about three times better than
that in the view released in November 1991.
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- 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. The north pole is
located at upper left; Gaspra rotates counterclockwise
every 7 hours. The large concavity on the lower right
limb is about 6 kilometers (3.7 miles) across, the
prominent crater on the terminator, center left, about
1.5 kilometers (1 mile).
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- A striking feature of Gaspra's surface is the abundance
of small craters. More than 600 craters, 100-500 meters
(330-1650 feet) in diameter are visible here. The number
of such small craters compared to larger ones is much
greater for Gaspra than for previously studied bodies of
comparable size such as the satellites of Mars. Gaspra's
very irregular shape suggests that the asteroid was
derived from a larger body by nearly catastrophic
collisions.
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- Consistent with such a history is the prominence of
groove-like linear features, believed to be related to
fractures. These linear depressions, 100-300 meters wide
and tens of meters deep, are in two crossing groups with
slightly different morphology, one group wider and more
pitted than the other. Grooves had previously been seen
only on Mars's moon Phobos, but were predicted for
asteroids as well. Gaspra also shows a variety of
enigmatic curved depressions and ridges in the terminator
region at left.
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- 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.
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- Source