Difference between revisions of "November 3, 2004"
Line 8: | Line 8: | ||
<table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | <table width="85%" border="0" align="center" cellpadding="6" cellspacing="2"> | ||
<tr><td colspan="2" valign="top"><div align="center"> | <tr><td colspan="2" valign="top"><div align="center"> | ||
− | + | [[File:LPOD-2004-11-03.jpeg|LPOD-2004-11-03.jpeg]] | |
</div></td> | </div></td> | ||
</tr> | </tr> |
Revision as of 13:57, 17 January 2015
Looking Down the Chain
<nobr>Looking Down the Chain</nobr> |
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: Tomorrow's LPOD: Norwegian Ring |
Author & Editor: Technical Consultant: Contact Translator: A service of: |
COMMENTS?
Register, and click on the Discussion tab at the top of the page.