Difference between revisions of "March 20, 2010"

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=Another Ina?=
 
=Another Ina?=
 
 
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<em>LROC Observation M104476560L from [http://wms.lroc.asu.edu/lroc#damoon LROC WMS Image Map] (illumination from the left)</em><br />
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<em>LROC Observation M104476560L from [http://wms.lroc.asu.edu/lroc#damoon" rel="nofollow LROC WMS Image Map] (illumination from the left)</em><br />
 
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The peculiar depression [http://the-moon.wikispaces.com/Ina Ina] has a bizarre floor of [http://lpod.armoredpenguin.com/wiki/February+3%2C+2010 rubbly hills and islands of smooth terrain]. Sorting through the LRO images released on March 15 I found this image of part of the floor of Hyginus crater that looks similar. The largest roughly circular feature is 350-400 m wide, but it is not clear what the feature is. Smaller circular to irregular depressions are across the scene. The arcuate depression on the left looks like it continues as a circular feature covered by the darker material. But if Hyginus is like Ina, the dark smooth material is as old as maria outside Hyginus, suggesting that it is not a younger deposit. Thus, it seems that something is removing the terrain under the original mare surface. Like Ina, Hyginus is thought to be a volcanic collapse depression. Perhaps volcanic gases dissolve the regolith in volcanic craters causing this characteristic pattern. But what gas would do this? Comparison with the 43 year old Orbiter V [http://www.lpi.usra.edu/resources/lunarorbiter/frame/?5095 image] reveals no obvious changes so the process does not appear to be active on a human timescale.<br />
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The peculiar depression [http://the-moon.wikispaces.com/Ina Ina] has a bizarre floor of [/February+3%2C+2010 rubbly hills and islands of smooth terrain]. Sorting through the LRO images released on March 15 I found this image of part of the floor of Hyginus crater that looks similar. The largest roughly circular feature is 350-400 m wide, but it is not clear what the feature is. Smaller circular to irregular depressions are across the scene. The arcuate depression on the left looks like it continues as a circular feature covered by the darker material. But if Hyginus is like Ina, the dark smooth material is as old as maria outside Hyginus, suggesting that it is not a younger deposit. Thus, it seems that something is removing the terrain under the original mare surface. Like Ina, Hyginus is thought to be a volcanic collapse depression. Perhaps volcanic gases dissolve the regolith in volcanic craters causing this characteristic pattern. But what gas would do this? Comparison with the 43 year old Orbiter V [http://www.lpi.usra.edu/resources/lunarorbiter/frame/?5095" rel="nofollow image] reveals no obvious changes so the process does not appear to be active on a human timescale.<br />
 
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<br />
<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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<strong>Related Links</strong><br />
 
<strong>Related Links</strong><br />
 
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+34 34]<br />
 
Rükl plate [http://the-moon.wikispaces.com/R%C3%BCkl+34 34]<br />
Note that Pete Schultz and colleagues included Hyginus as an Ina-like object in their 2006 [http://adsabs.harvard.edu/abs/2006Natur.444..184S paper].<br />
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Note that Pete Schultz and colleagues included Hyginus as an Ina-like object in their 2006 [http://adsabs.harvard.edu/abs/2006Natur.444..184S" rel="nofollow paper].<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 19:20, 4 January 2015

Another Ina?

LPOD-Mar20-10.jpg
LROC Observation M104476560L from " rel="nofollow LROC WMS Image Map (illumination from the left)

The peculiar depression Ina has a bizarre floor of [/February+3%2C+2010 rubbly hills and islands of smooth terrain]. Sorting through the LRO images released on March 15 I found this image of part of the floor of Hyginus crater that looks similar. The largest roughly circular feature is 350-400 m wide, but it is not clear what the feature is. Smaller circular to irregular depressions are across the scene. The arcuate depression on the left looks like it continues as a circular feature covered by the darker material. But if Hyginus is like Ina, the dark smooth material is as old as maria outside Hyginus, suggesting that it is not a younger deposit. Thus, it seems that something is removing the terrain under the original mare surface. Like Ina, Hyginus is thought to be a volcanic collapse depression. Perhaps volcanic gases dissolve the regolith in volcanic craters causing this characteristic pattern. But what gas would do this? Comparison with the 43 year old Orbiter V " rel="nofollow image reveals no obvious changes so the process does not appear to be active on a human timescale.

" rel="nofollow Chuck Wood

Related Links
Rükl plate 34
Note that Pete Schultz and colleagues included Hyginus as an Ina-like object in their 2006 " rel="nofollow paper.


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.