False Color Moon |
The visualizations depict spectral properties of the lunar surface known from
analysis of returned samples to be related to composition or weathering of
surface materials. The greenish-blue region at the upper right in the full
disk and the upper part of the right hand picture is Oceanus Procellarum. The
deeper blue mare regions here and elsewhere are relatively rich in titanium,
while the greens, yellows and light oranges indicate basalts low in titanium
but rich in iron and magnesium. The reds (deep orange in the right hand
picture) are typically cratered highlands relatively poor in titanium, iron
and magnesium. In the full disk picture on the left, the yellowish area to the
south is part of the newly confirmed South Pole Aitken basin, a large circular
depression some 1,200 miles across, perhaps rich in iron and magnesium.
Analysis of Apollo lunar samples provided the basis for calibration of this
spectral map; Galileo data, in turn, permit broad extrapolation of the Apollo
based composition information, reaching ultimately to the far side of the Moon.
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Galileo Solid State Imaging Team Leader: Dr. Michael J. S. Belton
The SSI Education and Public Outreach webpages were originally created and managed by Matthew Fishburn and Elizabeth Alvarez with significant assistance from Kelly Bender, Ross Beyer, Detrick Branston, Stephanie Lyons, Eileen Ryan, and Nalin Samarasinha.
Last updated: September 17, 1999, by Matthew Fishburn
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