Difference between revisions of "August 13, 2012"
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| − | <em>LRO QuickMap images from [http://target.lroc.asu.edu/da/qmap.html NASA/ASU]</em><br /> | + | <em>LRO QuickMap images from [http://target.lroc.asu.edu/da/qmap.html" rel="nofollow NASA/ASU]</em><br /> |
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Crater chains excavated by lines of ejecta spewed out during the formation of impact basins are sparely seen on the nearside.<br /> | Crater chains excavated by lines of ejecta spewed out during the formation of impact basins are sparely seen on the nearside.<br /> | ||
The Snellius and Rheita valleys are the most visible, while the Baade and Bouvard valleys are hard to appreciate. Remnants of<br /> | The Snellius and Rheita valleys are the most visible, while the Baade and Bouvard valleys are hard to appreciate. Remnants of<br /> | ||
| − | possible other basin secondary chains are sometimes [http://lpod.wikispaces.com/message/view/August+12%2C+2012/55746794 proposed] but proof is difficult. The little-degraded secondary chains of<br /> | + | possible other basin secondary chains are sometimes [http://lpod.wikispaces.com/message/view/August+12%2C+2012/55746794" rel="nofollow proposed] but proof is difficult. The little-degraded secondary chains of<br /> |
the Orientale Basin provide clues to what might have originally existed around other basins. A broad swath of chains radiates<br /> | the Orientale Basin provide clues to what might have originally existed around other basins. A broad swath of chains radiates<br /> | ||
to the northwest of Orientale, stretching at least 2000 km from the basin center. Near the basin rim the terrain is covered with<br /> | to the northwest of Orientale, stretching at least 2000 km from the basin center. Near the basin rim the terrain is covered with<br /> | ||
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modify nearly all of them, but the rate drastically declined after Orientale, leaving its chains in nearly pristine condition. <br /> | modify nearly all of them, but the rate drastically declined after Orientale, leaving its chains in nearly pristine condition. <br /> | ||
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| − | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | + | <em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br /> |
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Revision as of 22:34, 4 January 2015
Chains
LRO QuickMap images from " rel="nofollow NASA/ASU
Crater chains excavated by lines of ejecta spewed out during the formation of impact basins are sparely seen on the nearside.
The Snellius and Rheita valleys are the most visible, while the Baade and Bouvard valleys are hard to appreciate. Remnants of
possible other basin secondary chains are sometimes " rel="nofollow proposed but proof is difficult. The little-degraded secondary chains of
the Orientale Basin provide clues to what might have originally existed around other basins. A broad swath of chains radiates
to the northwest of Orientale, stretching at least 2000 km from the basin center. Near the basin rim the terrain is covered with
thick and swirly textured debris with the chains becoming more prominent further out. Individual chains - like the Leuschner
Chain and an unnamed one next to it (image above right) - are made up of lines of 10-30 km wide craters, surrounded by tongues
of material that flowed - probably like a hurricane - across the surface. Surprisingly, there are few Orientale secondary chains
in other radial directions. A concentration does occur to the basin's south, southeast (beyond this image) but only occassional
chains are seen elsewhere. This may be consistent with an oblique impact for Orientale or another unknown factor may be
responsible. The paucity of readily seen nearside chains implies that the rate of bombardment was high enough to severely
modify nearly all of them, but the rate drastically declined after Orientale, leaving its chains in nearly pristine condition.
" rel="nofollow Chuck Wood
