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These two maps are derived
from images of asteroid 4 Vesta taken
between November 28 and December 1, 1994 with the Wide Field Planetary
Camera-2 (in PC mode) aboard NASA's Hubble Space Telescope.
This is about 500 Km in diameter. The top picture is a surface brightness map.
The surface markings may represent
ancient igneous activity such as lava flows and, in addition, regions
where major impacts have stripped away the crust revealing mantle
material below the crust.
The bottom map was produced from separate images in blue (439 nm), orange
(673 nm), red (953 nm), and near-infrared (1024 nm) light. It shows that Vesta has
two distinct hemispheres containing two
different types of solidified lava called basalts.
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