Difference between revisions of "January 6, 2014"
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| − | <em>image by [mailto:tosi.philippe@wanadoo.fr Philippe Tosi] / E.Rousset / JL Dauvergne, Pic du Midi Observatory, France</em><br /> | + | <em>image by [mailto:tosi.philippe@wanadoo.fr" rel="nofollow Philippe Tosi] / E.Rousset / JL Dauvergne, Pic du Midi Observatory, France</em><br /> |
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| − | Remember the [http://lpod.wikispaces.com/January+3%2C+2014 rille segments] in front of the Apennine Mountains? This is what they may have looked like before inundation by lavas. In fact, just saying that points out a difference compared to these circumferential [http://the-moon.wikispaces.com/Rimae+Hippalus Hippalus Rilles] on the east side of the Humorum Basin. The Imbrium Basin circumferential rilles cut debris slumped from the basin's upraised rim, but mare lavas cover the rilles, so some volcanism occurred after basin subsidence. At Humorum, the main basin subsidence must have taken place after nearby lavas were emplaced and hardened because the subsidence-induced fracturing cut through the lavas. And here at the east side of Humorum, the fracturing created 3 or 4 rilles spread over a horizontal distance of about 50 km, whereas at Imbrium the exposure is less good but only 1 or 2 rilles are seen across about 10-20 km. I do not know the explanation for these differences, not to mention the very thin rilles on the west side of Tranquillitatis for a different variety. I need to dig out a 35 year old theoretical [http://planetary.brown.edu/pdfs/177.pdf study] of concentric rilles to look for reasons for the differences.<br /> | + | Remember the [http://lpod.wikispaces.com/January+3%2C+2014 rille segments] in front of the Apennine Mountains? This is what they may have looked like before inundation by lavas. In fact, just saying that points out a difference compared to these circumferential [http://the-moon.wikispaces.com/Rimae+Hippalus Hippalus Rilles] on the east side of the Humorum Basin. The Imbrium Basin circumferential rilles cut debris slumped from the basin's upraised rim, but mare lavas cover the rilles, so some volcanism occurred after basin subsidence. At Humorum, the main basin subsidence must have taken place after nearby lavas were emplaced and hardened because the subsidence-induced fracturing cut through the lavas. And here at the east side of Humorum, the fracturing created 3 or 4 rilles spread over a horizontal distance of about 50 km, whereas at Imbrium the exposure is less good but only 1 or 2 rilles are seen across about 10-20 km. I do not know the explanation for these differences, not to mention the very thin rilles on the west side of Tranquillitatis for a different variety. I need to dig out a 35 year old theoretical [http://planetary.brown.edu/pdfs/177.pdf" rel="nofollow study] of concentric rilles to look for reasons for the differences.<br /> |
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| − | <em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br /> | + | <em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br /> |
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<strong>Technical Details</strong><br /> | <strong>Technical Details</strong><br /> | ||
Revision as of 22:54, 4 January 2015
Hip-Hip-Hippalus
image by " rel="nofollow Philippe Tosi / E.Rousset / JL Dauvergne, Pic du Midi Observatory, France
Remember the rille segments in front of the Apennine Mountains? This is what they may have looked like before inundation by lavas. In fact, just saying that points out a difference compared to these circumferential Hippalus Rilles on the east side of the Humorum Basin. The Imbrium Basin circumferential rilles cut debris slumped from the basin's upraised rim, but mare lavas cover the rilles, so some volcanism occurred after basin subsidence. At Humorum, the main basin subsidence must have taken place after nearby lavas were emplaced and hardened because the subsidence-induced fracturing cut through the lavas. And here at the east side of Humorum, the fracturing created 3 or 4 rilles spread over a horizontal distance of about 50 km, whereas at Imbrium the exposure is less good but only 1 or 2 rilles are seen across about 10-20 km. I do not know the explanation for these differences, not to mention the very thin rilles on the west side of Tranquillitatis for a different variety. I need to dig out a 35 year old theoretical " rel="nofollow study of concentric rilles to look for reasons for the differences.
" rel="nofollow Chuck Wood
Technical Details
C.14 + skynyx 2.1 m + basler ACA 1300 + barlow 1.8x + red filter; process by AS2, CS5 and photomatix pro with tone mapping.
Related Links
21st Century Atlas chart 23.
