Mathematics – Logic
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....13453c&link_type=abstract
EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #13453
Mathematics
Logic
Scientific paper
The technique of GCMS analysis, which has been used with a great success on several past planetary missions, is not adapted for precise measurements of the isotopic composition of planetary atmospheres (noble gases, stable isotopes), and volatile outgassed products from solid sample pyrolysis. Static mass spectrometry, coupled with gas separation by cryo-separation, and chemical trapping, is commonly used in the laboratory to study volatiles extracted from terrestrial and meteoritic samples. This technique allows to reach a precision on isotopic ratios of the order of a few 0.1 ppm for a typical amount of gas of a few micromoles. We are presently studying an instrument based on the same principle for space exploration applications. The PALOMA instrument (PAyload for Local Observation of Mars Atmosphere) will be proposed in response to the AO for the instrumentation of the NASA Mars Smart Lander mission, planned to be launched in 2009. It might be part as well of the EXOMARS mission presently studied at ESA in the frame of the Aurora program. The miniaturization of major key elements, like the cryogenic device, the mass spectrometer, the line and its ensemble of valves, is presently led in our laboratories under CNES funding. The instrument consists of : (i) a gas purification and separation line, using techniques of cryogenic and chemical trapping, and possibly membrane permeation for molecular hydrogen analysis, (ii) a mass spectrometer working in static mode, without carrier gas (both time-of-flight and magnetic solutions are studied), (iii) a turbo-molecular pump that provides the required level of vacuum in the separation line and in the spectrometer. In the specific case of Mars, it is designed to work during typically 2 years (about 1000 measurement cycles), in order to perform accurate measurements of molecular, elemental and isotopic composition and of their diurnal/seasonal variations. The gas is sampled directly from the ambient atmosphere, without need for an external sample distribution system. The general characteristics of the instrument are as following . The mass is 6 kg, for a size of 30 x 30 x 20 cm. The required power, averaged over a complete measurement cycle, is 20 W (peak value : 30 W). The total energy required for one sequence is 100 Wh. This number must be considered as an upper limit, and corresponds to the most complex sequence (noble gas isotope analysis). Sequences used for stable isotopes measurement, and atmospheric molecular composition (trace gases of geological and/or astrobiological interest), are expected to be simpler, and less power-consuming. The anticipated volume of data produced by one observation sequence is estimated to be in the 3-6 kb range. The gas is sampled directly from the ambient atmosphere.
Agrinier Pierre
Berthelier Jean-Jacques
Chassefiere Eric
Jambon Albert
Sarda Ph.
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