Difference between revisions of "March 12, 2010"

From LPOD
Jump to: navigation, search
Line 1: Line 1:
 
__NOTOC__
 
__NOTOC__
 
=Wiggly Lines=
 
=Wiggly Lines=
 
 
<!-- ws:start:WikiTextHeadingRule:1:&lt;h1&gt; -->
 
<!-- ws:start:WikiTextHeadingRule:1:&lt;h1&gt; -->
 
<!-- ws:start:WikiTextLocalImageRule:16:&lt;img src=&quot;/file/view/LPOD-Mar12-10.jpg/127009957/LPOD-Mar12-10.jpg&quot; alt=&quot;&quot; title=&quot;&quot; /&gt; -->[[File:LPOD-Mar12-10.jpg|LPOD-Mar12-10.jpg]]<!-- ws:end:WikiTextLocalImageRule:16 --><br />
 
<!-- ws:start:WikiTextLocalImageRule:16:&lt;img src=&quot;/file/view/LPOD-Mar12-10.jpg/127009957/LPOD-Mar12-10.jpg&quot; alt=&quot;&quot; title=&quot;&quot; /&gt; -->[[File:LPOD-Mar12-10.jpg|LPOD-Mar12-10.jpg]]<!-- ws:end:WikiTextLocalImageRule:16 --><br />
<em>image by [http://www.agu.org/pubs/crossref/2009/2009GL039835.shtml Oshigami and others (2009), ]Geophysics Research Letters</em><br />
+
<em>image by [http://www.agu.org/pubs/crossref/2009/2009GL039835.shtml" rel="nofollow Oshigami and others (2009), ]Geophysics Research Letters</em><br />
 
<br />
 
<br />
Apollo 17 included a radar sounder that pumped pulses of energy into the lunar surface and detected reflections within the upper part of two maria. Kaguya carried an improved Lunar Radar Sounder (LSR) that covered much more of the lunar surface. The Kaguya images here show cross-sectional views of layering within Mare Imbrium (a) and Oceanus Procellarum (b), with the second and fourth images including white lines that mark strong reflections. The [http://www.agu.org/pubs/crossref/2009/2009GL039835.shtml LSR science team] interprets these reflections as regolith layers that formed on temporary top layers of earlier lava flows, which were later covered by more recent lava flows. This layering confirms that each mare was not emplaced all at once - which no one advocates - but that each is a thick pile of many separate lava flows. The distances between the regolith layers - apparently 100 to 500 m - is much greater than the few flows visible on the the surfaces of mare (average about 35 m) so that the spaces between regolith layers include multiple flow units that erupted on top of each other quickly enough that no appreciable regolith built up. Surprisingly, the LSR detected buried regolith layers in only about 10% of the western maria. This suggests that the lavas erupted onto the surface in nearly continuous outpourings, without long enough gaps for significant regoliths to form. But we know this can not be true because there are as much as 2 billion years difference in [http://www.lpod.org/?m=20070407 ages] of the youngest and oldest lavas in these areas. Two explanations are offered by the LSR team. Younger lavas may have scoured away the built-up regolith, making in undetectable. Additionally, regolith layers have only been detected under areas were surface lavas are at least 3.2 b.y. old. Because the rate of accumulation of regolith depends on the impact cratering rate, deep regolith layers were more like to have formed on older lavas than younger ones, because the cratering rate declined greatly after about 3.8 b.y. ago. This explanation can't be completely true because all of the young lavas cover older ones. This Kaguya result is wonderful because it provides new data that answers some questions but leaves more for future astronauts and scientists to investigaate.<br />
+
Apollo 17 included a radar sounder that pumped pulses of energy into the lunar surface and detected reflections within the upper part of two maria. Kaguya carried an improved Lunar Radar Sounder (LSR) that covered much more of the lunar surface. The Kaguya images here show cross-sectional views of layering within Mare Imbrium (a) and Oceanus Procellarum (b), with the second and fourth images including white lines that mark strong reflections. The [http://www.agu.org/pubs/crossref/2009/2009GL039835.shtml" rel="nofollow LSR science team] interprets these reflections as regolith layers that formed on temporary top layers of earlier lava flows, which were later covered by more recent lava flows. This layering confirms that each mare was not emplaced all at once - which no one advocates - but that each is a thick pile of many separate lava flows. The distances between the regolith layers - apparently 100 to 500 m - is much greater than the few flows visible on the the surfaces of mare (average about 35 m) so that the spaces between regolith layers include multiple flow units that erupted on top of each other quickly enough that no appreciable regolith built up. Surprisingly, the LSR detected buried regolith layers in only about 10% of the western maria. This suggests that the lavas erupted onto the surface in nearly continuous outpourings, without long enough gaps for significant regoliths to form. But we know this can not be true because there are as much as 2 billion years difference in [http://www.lpod.org/?m=20070407" rel="nofollow ages] of the youngest and oldest lavas in these areas. Two explanations are offered by the LSR team. Younger lavas may have scoured away the built-up regolith, making in undetectable. Additionally, regolith layers have only been detected under areas were surface lavas are at least 3.2 b.y. old. Because the rate of accumulation of regolith depends on the impact cratering rate, deep regolith layers were more like to have formed on older lavas than younger ones, because the cratering rate declined greatly after about 3.8 b.y. ago. This explanation can't be completely true because all of the young lavas cover older ones. This Kaguya result is wonderful because it provides new data that answers some questions but leaves more for future astronauts and scientists to investigaate.<br />
 
<br />
 
<br />
<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
+
<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br />
 
<br />
 
<br />
 
<br />
 
<br />
 
<hr />
 
<hr />
<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 />
 
</div>
 
</div>
 
 
----
 
----
 
===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 19:20, 4 January 2015

Wiggly Lines

LPOD-Mar12-10.jpg
image by " rel="nofollow Oshigami and others (2009), Geophysics Research Letters

Apollo 17 included a radar sounder that pumped pulses of energy into the lunar surface and detected reflections within the upper part of two maria. Kaguya carried an improved Lunar Radar Sounder (LSR) that covered much more of the lunar surface. The Kaguya images here show cross-sectional views of layering within Mare Imbrium (a) and Oceanus Procellarum (b), with the second and fourth images including white lines that mark strong reflections. The " rel="nofollow LSR science team interprets these reflections as regolith layers that formed on temporary top layers of earlier lava flows, which were later covered by more recent lava flows. This layering confirms that each mare was not emplaced all at once - which no one advocates - but that each is a thick pile of many separate lava flows. The distances between the regolith layers - apparently 100 to 500 m - is much greater than the few flows visible on the the surfaces of mare (average about 35 m) so that the spaces between regolith layers include multiple flow units that erupted on top of each other quickly enough that no appreciable regolith built up. Surprisingly, the LSR detected buried regolith layers in only about 10% of the western maria. This suggests that the lavas erupted onto the surface in nearly continuous outpourings, without long enough gaps for significant regoliths to form. But we know this can not be true because there are as much as 2 billion years difference in " rel="nofollow ages of the youngest and oldest lavas in these areas. Two explanations are offered by the LSR team. Younger lavas may have scoured away the built-up regolith, making in undetectable. Additionally, regolith layers have only been detected under areas were surface lavas are at least 3.2 b.y. old. Because the rate of accumulation of regolith depends on the impact cratering rate, deep regolith layers were more like to have formed on older lavas than younger ones, because the cratering rate declined greatly after about 3.8 b.y. ago. This explanation can't be completely true because all of the young lavas cover older ones. This Kaguya result is wonderful because it provides new data that answers some questions but leaves more for future astronauts and scientists to investigaate.

" 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.