Difference between revisions of "March 8, 2010"
Line 19: | Line 19: | ||
<table class="wiki_table"> | <table class="wiki_table"> | ||
<tr> | <tr> | ||
− | <td><!-- | + | <td> <!-- RemoveRevolverMaps --> |
− | + | <!-- RemoveRevolverMaps --> | |
+ | </td> | ||
<p><b>Yesterday's LPOD:</b> [[March 7, 2010|Improved Gravity Eyes]] </p> | <p><b>Yesterday's LPOD:</b> [[March 7, 2010|Improved Gravity Eyes]] </p> | ||
<p><b>Tomorrow's LPOD:</b> [[March 9, 2010|Alpine Moonrise]] </p> | <p><b>Tomorrow's LPOD:</b> [[March 9, 2010|Alpine Moonrise]] </p> | ||
− | |||
<!-- End of content --> | <!-- End of content --> | ||
{{wiki/ArticleFooter}} | {{wiki/ArticleFooter}} |
Revision as of 19:48, 8 February 2015
A Matter of Time
image by Nick Smith, La Palma, Canary Islands.
How many events do you see? The rim of Archimedes is partly draped over the hilly and rilled terrain in the foreground, which must be older. Sometime after Archimedes formed, Imbrium mare lavas flooded the outside of the crater and lavas somehow rose up under it to cover the floor. As the mare lava cooled and subsided, sinking into a smaller volume of the basin, low angle faulting made the circular ridges. Since the time of mare flows, small impacts have continued to occur, pitting the floor of Archimedes and everywhere else.
Chuck Wood
Technical Details
August 13, 2009. C14, Infinity 2-1M camera
Related Links
Rükl plate 22
Yesterday's LPOD: Improved Gravity Eyes
Tomorrow's LPOD: Alpine Moonrise
COMMENTS?
Register, Log in, and join in the comments.