Difference between revisions of "February 10, 2011"

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=A Basin Quest=
 
=A Basin Quest=
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<em>image by [mailto:tosi.philippe@wanadoo.fr Philippe Tosi], FRANCE-Nîmes</em><br />
 
<em>image by [mailto:tosi.philippe@wanadoo.fr Philippe Tosi], FRANCE-Nîmes</em><br />
 
<br />
 
<br />
Near the middle of this scene is an ill-formed smooth area, not as dark as the Lacus Spei mare material at upper right. <br />
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Near the middle of this scene is an ill-formed smooth area, not as dark as the Lacus Spei mare material at upper right.  
The light-hued material has a name, Lacus Temporis, and occupies the central area of a 350 km wide depression. At <br />
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The light-hued material has a name, Lacus Temporis, and occupies the central area of a 350 km wide depression. At  
least that is what LPOD [http://www.lpod.org/archive/LPOD-2004-08-08.htm reported] in 2004, and there have been little additional analyses of this putative small impact <br />
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least that is what LPOD [[August_8,_2004|reported]] in 2004, and there have been little additional analyses of this putative small impact  
basin. But Harry Hiesinger and his crater-counting colleagues have [http://planetary.brown.edu/pdfs/3740.pdf estimated] that the lavas of Lacus Temporis erupted <br />
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basin. But Harry Hiesinger and his crater-counting colleagues have [http://planetary.brown.edu/pdfs/3740.pdf estimated] that the lavas of Lacus Temporis erupted  
between 3.62 and 3.74 b.y. ago. I imagine that the new LRO topographic data can much better define the size and depth<br />
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between 3.62 and 3.74 b.y. ago. I imagine that the new LRO topographic data can much better define the size and depth
of the supposed basin that in 2006 was defined by the relatively coarse Clementine data. I imagine that by tomorrow <br />
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of the supposed basin that in 2006 was defined by the relatively coarse Clementine data. I imagine that by tomorrow  
LPOD readers/contributers will have derived new information about this possible depression. Is there a Temporis Basin? <br />
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LPOD readers/contributers will have derived new information about this possible depression. Is there a Temporis Basin?  
 
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
<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+15 15]<br />
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Rükl plate [https://the-moon.us/wiki/R%C3%BCkl_15 15]<br />
 
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<br />
 
<hr />
 
<hr />
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<p><b>Yesterday's LPOD:</b> [[February 9, 2011|Lightening the Shadows]] </p>
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<p><b>Tomorrow's LPOD:</b> [[February 11, 2011|How Old is That Mare?]] </p>
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Latest revision as of 18:46, 13 October 2018

A Basin Quest

LPOD-Feb10-11.jpg
image by Philippe Tosi, FRANCE-Nîmes

Near the middle of this scene is an ill-formed smooth area, not as dark as the Lacus Spei mare material at upper right. The light-hued material has a name, Lacus Temporis, and occupies the central area of a 350 km wide depression. At least that is what LPOD reported in 2004, and there have been little additional analyses of this putative small impact basin. But Harry Hiesinger and his crater-counting colleagues have estimated that the lavas of Lacus Temporis erupted between 3.62 and 3.74 b.y. ago. I imagine that the new LRO topographic data can much better define the size and depth of the supposed basin that in 2006 was defined by the relatively coarse Clementine data. I imagine that by tomorrow LPOD readers/contributers will have derived new information about this possible depression. Is there a Temporis Basin?
Chuck Wood

Technical Details
9 Feb, 2011. C.14 + DMK camera/7.5 img/s + registax 5 + CS2

Related Links
Rükl plate 15


Yesterday's LPOD: Lightening the Shadows

Tomorrow's LPOD: How Old is That Mare?


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