Difference between revisions of "October 7, 2010"
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=Cone Pits= | =Cone Pits= | ||
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| − | <em>top LRO NAC image [http://wms.lroc.asu.edu/lroc/view_lroc/LRO-L-LROC-3-CDR-V1.0/M127247376RC M127247376RC] processed by [mailto:revans_01420@yahoo.com Rick Evans], and two smaller LRO WAC images ([http://wms.lroc.asu.edu/lroc/view_lroc/LRO-L-LROC-3-CDR-V1.0/M117807235MC M117807235MC] and [http://wms.lroc.asu.edu/lroc/view_lroc/LRO-L-LROC-3-CDR-V1.0/M109554979CE M109554979CE]) processed by [mailto:mauricejscollins@hotmail.com Maurice Collins] All images courtesy of NASA/GSFC/ASU.</em><br /> | + | <em>top LRO NAC image [http://wms.lroc.asu.edu/lroc/view_lroc/LRO-L-LROC-3-CDR-V1.0/M127247376RC" rel="nofollow M127247376RC] processed by [mailto:revans_01420@yahoo.com" rel="nofollow Rick Evans], and two smaller LRO WAC images ([http://wms.lroc.asu.edu/lroc/view_lroc/LRO-L-LROC-3-CDR-V1.0/M117807235MC" rel="nofollow M117807235MC] and [http://wms.lroc.asu.edu/lroc/view_lroc/LRO-L-LROC-3-CDR-V1.0/M109554979CE" rel="nofollow M109554979CE]) processed by [mailto:mauricejscollins@hotmail.com" rel="nofollow Maurice Collins] All images courtesy of NASA/GSFC/ASU.</em><br /> |
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| − | There are few volcanic cones on the Moon and all are small. One of the largest is Mairan T, a steep-sided, multiply-pitted little volcano just [ | + | There are few volcanic cones on the Moon and all are small. One of the largest is Mairan T, a steep-sided, multiply-pitted little volcano just [/October+3%2C+2010 west] of the Sinus Iridum crater ejecta. WIth a low Sun (bottom left), the central depression has an odd tri-corner look. With higher illumination (bottom right), it is clear that the depression is formed of 3 or 4 overlapping pits. Higher resolution provided by the LRO Narrow Angle Camera (top) shows that the pits are highly softened by erosion and no original layering is visible in their rims. The steep conical walls suggest that Mairan T is composed of more viscous lavas than those making maria and their gentle-sided domes. Perhaps Mairan T is made of the same material as the nearby steep-sided Gruithuisen domes.<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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<strong>Related Links</strong><br /> | <strong>Related Links</strong><br /> | ||
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| − | <div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591 LPOD!]<br /> | + | <div>You can support LPOD when you buy any book from Amazon thru [http://www.lpod.org/?page_id=591" rel="nofollow LPOD!]<br /> |
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===COMMENTS?=== | ===COMMENTS?=== | ||
Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment. | ||
Revision as of 22:07, 4 January 2015
Cone Pits
top LRO NAC image " rel="nofollow M127247376RC processed by " rel="nofollow Rick Evans, and two smaller LRO WAC images (" rel="nofollow M117807235MC and " rel="nofollow M109554979CE) processed by " rel="nofollow Maurice Collins All images courtesy of NASA/GSFC/ASU.
There are few volcanic cones on the Moon and all are small. One of the largest is Mairan T, a steep-sided, multiply-pitted little volcano just [/October+3%2C+2010 west] of the Sinus Iridum crater ejecta. WIth a low Sun (bottom left), the central depression has an odd tri-corner look. With higher illumination (bottom right), it is clear that the depression is formed of 3 or 4 overlapping pits. Higher resolution provided by the LRO Narrow Angle Camera (top) shows that the pits are highly softened by erosion and no original layering is visible in their rims. The steep conical walls suggest that Mairan T is composed of more viscous lavas than those making maria and their gentle-sided domes. Perhaps Mairan T is made of the same material as the nearby steep-sided Gruithuisen domes.
" rel="nofollow Chuck Wood
Related Links
Rükl plate 3
COMMENTS?
Click on this icon File:PostIcon.jpg at the upper right to post a comment.
