Difference between revisions of "October 31, 2010"

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=Lapping Lava=
 
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<em>WAC image M119591069ME processed by [mailto:revans_01420@yahoo.com" rel="nofollow Richard Evans]</em><br />
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<em>WAC image M119591069ME processed by [mailto:revans_01420@yahoo.com Richard Evans]</em><br />
 
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Bohnenberger looks like it was baked with too much yeast. Its floor is raised up and fractured just as bread sometimes is. The floor presumably formed with bulges of slumped wall debris and a small central peak, but that has been strongly modified. Spectral [http://www.lpi.usra.edu/meetings/lpsc97/pdf/1526.PDF" rel="nofollow studies] show that the floor material is highland rocks, so it is uplifted basement of the Nectaris basin, not convoluted volcanics. Interesting volcanics are just to the west, however. The dark basaltic lavas of Mare Nectaris lap up against the base of Bohnenberger. Seldom do we see such a sharp boundary between lava and pre-existing terrain, and it is fascinating how the lava flowed around minor elevations and filled small depressions. The mare-crater boundary is clear in a Clementine iron [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&amp;layers=moon_clem_feo_color&amp;west=33.63&amp;south=-18.83&amp;east=44.88&amp;north=-13.20&amp;center_lat=0&amp;center=39.255&amp;defaultcenter=on&amp;grid=none&amp;stretch=auto&amp;projection=SIMP&amp;advoption=NO&amp;info=NO&amp;resolution=64" rel="nofollow map], but is actually much more sharply defined that the Clementine view would suggest. <br />
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Bohnenberger looks like it was baked with too much yeast. Its floor is raised up and fractured just as bread sometimes is. The floor presumably formed with bulges of slumped wall debris and a small central peak, but that has been strongly modified. Spectral [http://www.lpi.usra.edu/meetings/lpsc97/pdf/1526.PDF studies] show that the floor material is highland rocks, so it is uplifted basement of the Nectaris basin, not convoluted volcanics. Interesting volcanics are just to the west, however. The dark basaltic lavas of Mare Nectaris lap up against the base of Bohnenberger. Seldom do we see such a sharp boundary between lava and pre-existing terrain, and it is fascinating how the lava flowed around minor elevations and filled small depressions. The mare-crater boundary is clear in a Clementine iron [http://www.mapaplanet.org/explorer-bin/explorer.cgi?map=Moon&amp;layers=moon_clem_feo_color&amp;west=33.63&amp;south=-18.83&amp;east=44.88&amp;north=-13.20&amp;center_lat=0&amp;center=39.255&amp;defaultcenter=on&amp;grid=none&amp;stretch=auto&amp;projection=SIMP&amp;advoption=NO&amp;info=NO&amp;resolution=64 map], but is actually much more sharply defined that the Clementine view would suggest. <br />
 
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br />
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+58 58]<br />
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Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_58 58]<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?===
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Click on this icon [[image:PostIcon.jpg]] at the upper right to post a comment.
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<p><b>Yesterday's LPOD:</b> [[October 30, 2010|Arm-Waving]] </p>
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<p><b>Tomorrow's LPOD:</b> [[November 1, 2010|Remnant Oldness]] </p>
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Latest revision as of 18:56, 13 October 2018

Lapping Lava

LPOD-Oct31-10.jpg
WAC image M119591069ME processed by Richard Evans

Bohnenberger looks like it was baked with too much yeast. Its floor is raised up and fractured just as bread sometimes is. The floor presumably formed with bulges of slumped wall debris and a small central peak, but that has been strongly modified. Spectral studies show that the floor material is highland rocks, so it is uplifted basement of the Nectaris basin, not convoluted volcanics. Interesting volcanics are just to the west, however. The dark basaltic lavas of Mare Nectaris lap up against the base of Bohnenberger. Seldom do we see such a sharp boundary between lava and pre-existing terrain, and it is fascinating how the lava flowed around minor elevations and filled small depressions. The mare-crater boundary is clear in a Clementine iron map, but is actually much more sharply defined that the Clementine view would suggest.

Chuck Wood

Related Links
Rükl plate 58


Yesterday's LPOD: Arm-Waving

Tomorrow's LPOD: Remnant Oldness


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