Titan Atmospheric & Surface Chemistry |
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Titan Atmospheric & Surface Chemistry |
May 16 2012, 12:07 AM
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#16
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![]() Senior Member ![]() ![]() ![]() ![]() Group: Moderator Posts: 2605 Joined: 10-November 06 From: Pasadena, CA Member No.: 1345 |
Well, if the ice was really fractured and porous (IIRC, Janssen et al had it at organics + fractured, so if it is ice it would need to be REALLY porous), and it was coated with some organic gunk, then it might fit the data.
The coating could happen during erosional tumbling. Kinda like breaded chicken. So the coating could be thin, which gives the IR signature. The high porosity ices gives the low dielectric constant. That's one possibility. As to actual compounds for such a coating, probably difficult to identify from just the limited IR. It could be a realy complex mixture. If I had to guess functional groups, I'd wave my arms and guess aromatcs, alkenes, alkynes, nitriles, (guanidines? Amidines?), imines, amines, and hydrocarbons, and polymerized things. I'd exclude carboxylic acids, amides, ketones, aldehydes, ethers, and alcohols. -------------------- Some higher resolution images available at my photostream: http://www.flickr.com/photos/31678681@N07/
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Nov 29 2012, 01:04 AM
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#17
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Member ![]() ![]() ![]() Group: Members Posts: 474 Joined: 1-April 08 From: Minnesota ! Member No.: 4081 |
An interesting paper was published in Nature today by the CIRCS (composite infrared spectrometer) team members concerning suprisingly rapid (for Titan) seasonal changes in the South Polar upper atmosphere infrared spectra. Link to the paper found here http://www.nature.com/nature/journal/v491/...ature11611.html
JPL summary article found here http://www.jpl.nasa.gov/news/news.php?release=2012-374 |
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Dec 2 2012, 10:21 PM
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#18
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Member ![]() ![]() ![]() Group: Members Posts: 138 Joined: 1-October 06 Member No.: 1206 |
Many wont have access, but the Icarus abstract really says it all:
Does Ice Float in Titan’s Lakes and Seas? Jason D. Hofgartner, Jonathan I. Lunine Department of Astronomy and Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA Abstract We model Titan’s lakes and seas as methane-ethane-nitrogen systems and model the buoyancy of solids in these systems assuming thermodynamic equilibrium. We find that ice will float in methane–rich lakes for all temperatures below the freezing point of pure methane and that ice will also float in ethane–rich seas provided the ice has an air porosity of greater than 5% by volume. Keywords: Titan, Titan, Surface P |
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