Moon Color Composite |
The concentric, circular Orientale basin, 600 miles across, is near the center; the near side is to the right, the far side to the left. At the upper right is the large, dark Oceanus Procellarum; below it is the smaller Mare Humorum. These, like the small dark Mare Orientale in the center of the basin, formed over 3 billion years ago as basaltic lava flows.
At the lower left, among the southern cratered highlands of the far side, is
the South-Pole-Aitken basin, similar to Orientale but twice as great in
diameter and much older and more degraded by cratering and weathering. The
cratered highlands of the near and far sides and the Maria are covered with
scattered bright, young ray craters.
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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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