Difference between revisions of "October 19, 2010"

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=More Jackson=
 
=More Jackson=
 
 
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<em>LRO WAC image</em> processed <em>by [mailto:mauricejscollins@hotmail.com Maurice Collins], Palmerston, New Zealand</em><br />
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<em>LRO WAC image</em> processed <em>by [mailto:mauricejscollins@hotmail.com" rel="nofollow Maurice Collins], Palmerston, New Zealand</em><br />
 
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Jackson is a spectacular crater that would put Tycho to shame if it were on the nearside. Jackson's [http://www.lpod.org/coppermine/displayimage.php?pid=40&amp;fullsize=1 rays] strikingly define an oblique impact event, and the ejecta closer to the crater, and the crater interior also have stories to tell. The ejecta right outside the rim crest has a gritty look, as if were deposited as a pasty flow full of boulders. Just inside the rim the wall is full of narrow micro-terraces that each accommodated a small amount of the downslope slip. Flat areas on the floor are ponds of impact melt, but these also are dotted with smaller boulders. Apparently both the melted ejecta and the pasty stuff were entrained with boulders. I wonder why?<br />
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Jackson is a spectacular crater that would put Tycho to shame if it were on the nearside. Jackson's [http://www.lpod.org/coppermine/displayimage.php?pid=40&amp;fullsize=1" rel="nofollow rays] strikingly define an oblique impact event, and the ejecta closer to the crater, and the crater interior also have stories to tell. The ejecta right outside the rim crest has a gritty look, as if were deposited as a pasty flow full of boulders. Just inside the rim the wall is full of narrow micro-terraces that each accommodated a small amount of the downslope slip. Flat areas on the floor are ponds of impact melt, but these also are dotted with smaller boulders. Apparently both the melted ejecta and the pasty stuff were entrained with boulders. I wonder why?<br />
 
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><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 />
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<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 22:08, 4 January 2015

More Jackson

LPOD-Oct19-10.jpg
LRO WAC image processed by " rel="nofollow Maurice Collins, Palmerston, New Zealand

Jackson is a spectacular crater that would put Tycho to shame if it were on the nearside. Jackson's " rel="nofollow rays strikingly define an oblique impact event, and the ejecta closer to the crater, and the crater interior also have stories to tell. The ejecta right outside the rim crest has a gritty look, as if were deposited as a pasty flow full of boulders. Just inside the rim the wall is full of narrow micro-terraces that each accommodated a small amount of the downslope slip. Flat areas on the floor are ponds of impact melt, but these also are dotted with smaller boulders. Apparently both the melted ejecta and the pasty stuff were entrained with boulders. I wonder why?

" rel="nofollow Chuck Wood


You can support LPOD when you buy any book from Amazon thru " rel="nofollow LPOD!

COMMENTS?

Click on this icon File:PostIcon.jpg at the upper right to post a comment.