Huygens Probe aerosol collector pyrolyser experiment

被引:30
作者
Israel, G [1 ]
Cabane, M
Brun, JF
Niemann, H
Way, S
Riedler, W
Steller, M
Raulin, F
Coscia, D
机构
[1] CNRS, Serv Aeron, F-91371 Verrieres Les Buissons, France
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Space Res Inst, A-8010 Graz, Austria
[4] Univ Paris 07, LISA, Creteil, France
[5] Univ Paris 12, LISA, Creteil, France
基金
美国国家航空航天局;
关键词
D O I
10.1023/A:1023640723915
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
ACP's main objective is the chemical analysis of the aerosols in Titan's atmosphere. For this purpose, it will sample the aerosols during descent and prepare the collected matter (by evaporation, pyrolysis and gas products transfer) for analysis by the Huygens Gas Chromatograph Mass Spectrometer (GCMS). A sampling system is required for sampling the aerosols in the 135-32 km and 22-17 km altitude regions of Titan's atmosphere. A pump unit is used to force the gas flow through a filter. In its sampling position, the filter front face extends a few mm beyond the inlet tube. The oven is a pyrolysis furnace where a heating element can heat the filter and hence the sampled aerosols to 250degreesC or 600degreesC. The oven contains the filter, which has a thimble-like shape (height 28 mm). For transferring effluent gas and pyrolysis products to GCMS, the carrier gas is a labeled nitrogen N-15(2), to avoid unwanted secondary reactions with Titan's atmospheric nitrogen. Aeraulic tests under cold temperature conditions were conducted by using a cold gas test system developed by ONERA. The objective of the test was to demonstrate the functional ability of the instrument during the descent of the probe and to understand its thermal behavior, that is to test the performance of all its components, pump unit and mechanisms. In order to validate ACP's scientific performance, pyrolysis tests were conducted at LISA on solid phase material synthesized from experimental simulation. The chromatogram obtained by GCMS analysis shows many organic compounds. Some GC peaks appear clearly from the total mass spectra, with specific ions well identified thanks to the very high sensitivity of the mass spectrometer. The program selected for calibrating the flight model is directly linked to the GCMS calibration plan. In order not to pollute the two flight models with products of solid samples such as tholins, we excluded any direct pyrolysis tests through the ACP oven during the first phase of the calibration. Post probe descent simulation of flight results are planned, using the much representative GCMS and ACP spare models.
引用
收藏
页码:433 / 468
页数:36
相关论文
共 23 条
[1]   FRACTAL AGGREGATES IN TITAN ATMOSPHERE [J].
CABANE, M ;
RANNOU, P ;
CHASSEFIERE, E ;
ISRAEL, G .
PLANETARY AND SPACE SCIENCE, 1993, 41 (04) :257-267
[2]   FORMATION AND GROWTH OF PHOTOCHEMICAL AEROSOLS IN TITANS ATMOSPHERE [J].
CABANE, M ;
CHASSEFIERE, E ;
ISRAEL, G .
ICARUS, 1992, 96 (02) :176-189
[3]   2 FORMATION REGIONS FOR TITANS HAZES - INDIRECT CLUES AND POSSIBLE SYNTHESIS MECHANISMS [J].
CHASSEFIERE, E ;
CABANE, M .
PLANETARY AND SPACE SCIENCE, 1995, 43 (1-2) :91-103
[4]   Chemical evolution on Titan: Comparisons to the prebiotic earth [J].
Clarke, DW ;
Ferris, JP .
ORIGINS OF LIFE AND EVOLUTION OF BIOSPHERES, 1997, 27 (1-3) :225-248
[5]   Review and latest results of laboratory investigations of Titan's aerosols [J].
Coll, P ;
Coscia, D ;
Gazeau, MC ;
Guez, L ;
Raulin, F .
ORIGINS OF LIFE AND EVOLUTION OF THE BIOSPHERE, 1998, 28 (02) :195-213
[6]   New planetary atmosphere simulations: Application to the organic aerosols of Titan [J].
Coll, P ;
Cosia, D ;
Gazeau, MC ;
Raulin, F .
LIFE SCIENCES: COMPLEX ORGANICS IN SPACE, 1997, 19 (07) :1113-1119
[7]  
COLL P, 1997, THESIS U PARIS 12
[8]  
Davies C.N., 1952, P I MECH ENG, VB1, P185, DOI [DOI 10.1177/002034835316701B13, DOI 10.1177/095440545300100113]
[9]  
Davies CharlesNorman., 1973, Air filtration
[10]  
Ehrenfreund P, 1995, Adv Space Res, V15, P335, DOI 10.1016/S0273-1177(99)80105-7