March 27, 2011
Geology Lesson
north to the left image by Michael Wirths, Baja Dark Skies Inn, Baja California, Mexico
The three geologic processes responsible for forming most of the Moon's surface are visible in this patch of southern Mare Imbrium. Impact craters, both primaries and secondaries, are scattered across the scene; volcanism appears as massive mare lava flows and small craters and rilles; and tectonism threw up the mare ridges that cut across the surface. The most prominent feature is the chain of overlapping secondary craters at right center. These must have formed by chunks of rocks excavated during the Copernicus impact event that did not separate much during their short ballistic trajectory from the crater. Across the bottom of the frame is another type of secondary cratering where the separation of ejecta was great enough that individual small packets of debris typically made one large crater and a few small ones. In both cases vee-shaped patterns of ejecta roughness show that there was a strong horizontal component of velocity away from Copernicus. The lower secondary trail is typical of cratering along a ray, whose brightness is just hinted at in this low Sun view. Although there are no volcanic flow fronts preserved here - as they are Chuck Wood
Technical Details
18" Starmaster dob + Lumerera 2-2 camera + 2.5X's Powermate + R/IR filter + Registax 5
Related Links
Rükl plate 20
Mike's new website, observatory and home
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