Difference between revisions of "November 3, 2004"
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=Looking Down the Chain= | =Looking Down the Chain= | ||
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| − | <tr><td><div align="center" class="main_sm">Image Credit: [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> | + | <tr><td><div align="center" class="main_sm"><p>Image Credit: [mailto:anthony@perseus.gr Anthony Ayiomamitis]</p> |
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<br>Rukl <i>Atlas of the Moon,</i> Sheet 68 | <br>Rukl <i>Atlas of the Moon,</i> Sheet 68 | ||
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| − | <p | + | <p><b>Yesterday's LPOD:</b> [[November 2, 2004|Offset Moon]] </p> |
| + | <p><b>Tomorrow's LPOD:</b> [[November 4, 2004|Norwegian Ring]] </p> | ||
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<p align="center" class="main_titles"><b>Author & Editor:</b><br> | <p align="center" class="main_titles"><b>Author & Editor:</b><br> | ||
[mailto:tychocrater@yahoo.com Charles A. Wood]</p> | [mailto:tychocrater@yahoo.com Charles A. Wood]</p> | ||
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Latest revision as of 15:03, 15 March 2015
Looking Down the Chain
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Image Credit: Anthony Ayiomamitis |
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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 |
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