QUOTE (nprev @ Jan 20 2009, 07:58 AM)

Interesting analysis from Kelly Beatty over on Sky & Telescope.
Apparently there was water vapor associated with the emissions, and they were definitely transient. The plot thickens considerably.
....
Thank you, and excellent, just as I expected.
A photochemical process which produces methane which is catalyzed over a metal oxide dust or clays requires water. Water is the source of the hydrogen during the photoreduction of CO2. {note: Metal sulfide dusts or minerals could work too as photochemical catalysts, there are papers on this too.}
The detection of water vapor in a region of high solar irradiance are
exactly the localized conditions which I was hypothesizing would be required for the photochemical mechanism to produce methane, that I proposed several years earlier over at the SDC forums, and reposted some of the arguments into a UMSF thread here:
http://www.unmannedspaceflight.com/index.p...&hl=methane{p.s. The photochemical mechanism I have proposed on SDC and then on UMSF is quite different from that later published by Bar-Nun (thank you Alex Blackwell for a copy of his paper from Icarus back then) (and whose hypothesis is disputed in a subsequent letter). Bar-Nun's mechanism was direct high energy photolysis without a catalyst. It's problem is that the light at that wavelength may be highly absorbed, and not reach the surface with much intensity.}
If I wasn't so busy with my job, which is in a very different field, I would do some research and publish a paper on this. if anyone here is qualified to pursue this, I would be happy to collaborate.
Below are a few of the score(s?) of photochemistry papers on the photoreduction of CO2 with water with shorter wavelength light (250 nm - 450 nm). Light of these ultraviolet wavelengths should reach the martian surface in significant doses. There are at least 20 journal papers on the subject of photoreduction of CO2 to produce methane, of course none having anything to do with Mars:
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Photoreduction of carbon dioxide and water into formaldehyde and methanol on semiconductor materials. Aurian-Blajeni, B.; Halmann, M.; Manassen, J. Weizmann Inst. Sci., Rehovot, Israel. Solar Energy (1980), 25(2), 165-70. CODEN: SRENA4 ISSN: 0038-092X. Journal written in English. CAN 94:124490 AN 1981:124490 CAPLUS
Abstract
Heterogeneous photoassisted redn. of aq. CO2 to produce MeOH [67-56-1], HCHO [50-00-0], and CH4 [74-82-8] was achieved by using semiconductor powders with either high-pressure Hg lamps or sunlight. The reaction was carried out either as a gas-solid process, by passing CO2 and H2O vapor over illuminated semiconductor surfaces or as a liq.-solid reaction, by illuminating aq. suspensions of semiconductor powders through which CO2 was bubbled. Best results, under illumination by Hg lamps, were obtained with aq. suspensions of SrTiO3, WO3, and TiO2, resulting in absorbed energy conversion efficiencies of 6, 5.9, and 1.2%, resp.
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Reaction mechanism in the photoreduction of CO2 with CH4 over ZrO2. Kohno, Yoshiumi; Tanaka, Tsunehiro; Funabiki, Takuzo; Yoshida, Satohiro. Department of Molecular Engineering, Graduate School of Engineering, Kyoto University, Kyoto, Japan. Physical Chemistry Chemical Physics (2000), 2(22), 5302-5307. CODEN: PPCPFQ ISSN: 1463-9076. Journal written in English. CAN 134:185804 AN 2000:788525 CAPLUS
Abstract
The surface species produced during photoredn. of carbon dioxide with methane over zirconium oxide were obsd. by IR spectroscopy. One of them was a reaction intermediate and decompd. to CO at .apprx.623 K, and the other did not decompd. even at 673 K was called a carbonaceous residue. IR spectral features allowed to identify the latter as the surface acetate. Several properties of the former species were quite similar to those of the surface formate ion, which was a reaction intermediate in photoredn. of CO2 by H2 over ZrO2. The former species was assigned to the surface formate, which was also supposed to be an intermediate of photoreaction between CO2 and CH4. The existence of another carbonaceous residue different that the surface acetate was suggested. The EPR spectrum indicated the photoexcitation of adsorbed CO2 to the CO2- anion radical, and the interaction of the CO2- radical with CH4 in the dark. On the basis of these results, a possible reaction mechanism in this reaction was proposed.
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Titre du document / Document title
Photocatalytic production of methane and hydrogen through reduction of carbon dioxide with water using titania pellets
Auteur(s) / Author(s)
SENG SING TAN (1) ; ZOU Linda (2) ; HU Eric (1) ;
Affiliation(s) du ou des auteurs / Author(s) Affiliation(s)
(1) School of Engineering and Technology, Deakin University, AUSTRALIE
(2) Institute of Sustainability and Innovation, Victoria University, AUSTRALIE
Résumé / Abstract
This paper presents an experimental study on employing a pellet form of catalyst in photo-reduction of carbon dioxide with water. Water was first absorbed into titania pellets. Highly purified carbon dioxide gas was then discharged into a reactor containing the wet pellets, which were then illuminated continuously for 65 hours using UVC lamps. Analysing the products accumulated in the reactor confirmed that methane and hydrogen were produced through photo-reduction of carbon dioxide with water. No other hydrocarbons were detected. Increasing the temperature in the reactor has showed little change on the amount of methane produced.