Difference between revisions of "November 3, 2004"
Line 1: | Line 1: | ||
__NOTOC__ | __NOTOC__ | ||
=Looking Down the Chain= | =Looking Down the Chain= | ||
+ | <!-- Start of content --> | ||
<table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | <table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | ||
<tr> | <tr> | ||
Line 54: | Line 55: | ||
</table> | </table> | ||
<p> </p> | <p> </p> | ||
+ | <!-- End of content --> | ||
{{wiki/ArticleFooter}} | {{wiki/ArticleFooter}} |
Revision as of 18:28, 7 February 2015
Looking Down the Chain
Image Credit: Anthony Ayiomamitis |
Looking Down the Chain Radiating from Mare Nectaris are a number of linear features, most notably the Rheita and Snellius valleys. These are thought to be basin secondary crater chains resulting from large blocks of rock ejected almost like a ray during the Nectaris impact. Anthony's excellent image looking down the chain showcases a longtime peculiar feature of the Rheita Valley - it bends. And it also seems to change it character - the craters between Rheita and Mallet are about 25 lm wide, but those closer to the limb have average widths of only about 10 km. I wonder if these two different-sized and different angled crater chains were formed by the same event or by separate ones? Technical Details: Related Links: Yesterday's LPOD: Offset Moon Tomorrow's LPOD: Norwegian Ring |
Author & Editor: Technical Consultant: Contact Translator: A service of: |
COMMENTS?
Register, Log in, and join in the comments.