QUOTE (JRehling @ Jul 18 2008, 05:21 PM)
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Also D:H ratios, which are hugely interesting -- they may match the atmospheric D:H perfectly, or be significantly different, which would tell us whether there is significant interchange over long spans of time.
In the last press conference (just a distant memory now) they reported having successfully baked the first sample:
QUOTE
Scientists on Thursday also discussed the preliminary results of another experiment, in which a soil sample was baked to 1,800 degrees Fahrenheit. The sample contained carbon dioxide gas as well as water vapor, said William Boynton, a lead scientist on the Thermal and Evolved Gas Analyzer, or TEGA.
So should they not have a D:H and C13:C12 measurement already?
QUOTE
What else it might find is up to Mars. Salts, etc., will not become gaseous when heated, but anything else that does will be of interest.
According to Wright and Pillinger,
Mars, Modulus and MAGIC:
QUOTE
Apart from H2O and CO2 other trapped volatiles could be studied [with evolved gas analysis], e.g. simple organic molecules (hydrocarbons, for instance), and clathrates containing CO, CH4, NH3, etc. These entities may not always be simply trapped atmospheric constituents; rather they may have been synthesized within the regolith. This could be the result of fluid interactions with other minerals, the input of extramartian materials, free-radical chemistry, or possibly by biological reactions.
In a
TEGA test run on shale:
QUOTE
As would be expected, there are significant differences in the evolved gas behaviors for samples run under combustion and pyrolysis conditions (Figs. 1 & 2). In combustion experiments, organic C in the form of CO2 and H2 evolved between 300-600ºC (Fig. 1); whereas, CO2 and H2 evolved between 450-600ºC in pyrolysis experiments (Fig. 2). CO2 that evolved between 650-750ºC is primarily due to the thermal decomposition of dolomite, although, some of the CO2 evolved in this range for the pyrolysis experiment may be due to decomposition of the kerogen (see below). Nearly all of the kerogen was “cracked” into CO2, H2, and H2O in the combustion experiments with the exception of a mass 41 fragment that we have assigned to C3H5 and mass 15 that we assigned to methane.
So even with the ice subliming away before they had a chance to bake this first sample, ought there not be some significant results from the analysis regarding other substances (including adsorbed water that came off at high temperature)? I believe the analysis equipment was reported as working to specs.