Noble gases in Dome C micrometeorites - An attempt to disentangle asteroidal and cometary sources
نویسندگان
چکیده
We have performed a comprehensive noble gas study, including the isotopes of krypton and xenon, on set micrometeorites (MMs) collected from surface snow at Dome C (DC) Antarctic plateau. He Ne are generally dominated by solar component, with lower 4He concentrations 4He/20Ne ratios in crystalline (Xtal) compared to fine-grained carbonaceous (FgC) MMs. Concentrations (surface-correlated) wind (SW) FgC MMs high end what has been seen earlier work, whereas abundances (volume-correlated) Kr Xe similar found previous studies In most samples, isotopic for usual range Q-Kr -Xe (the Q component is dominating primitive macroscopic meteorites) air. When quantifiable, cosmic ray exposure (CRE) ages based cosmogenic 21Ne 3He, combination Poynting-Robertson effect, broadly consistent an origin asteroid belt. An exception Xtal MM, which exhibits concentration agreement beyond Saturn, possible cometary origin. addition, data trapped gases three (out ten analyzed) DC provide hints that these may be related source. One sample, fragment particular interest. This composition, although large analytical uncertainties, deficient heavy 134Xe 136Xe. pattern, probably ice, measured Rosetta coma comet 67P/Churyumov-Gerasimenko. The same MM also unusually 36Ar/38Ar ratio, Rosetta's Ar measurement (in this case latter having uncertainty). other two MMs, type, show laboratory analysis refractory grains captured 81P/Wild 2 Stardust mission. Additionally, FgC/Xtal contain excess some cluster interplanetary dust particles (cluster IDPs).
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ژورنال
عنوان ژورنال: Icarus
سال: 2022
ISSN: ['0019-1035', '1090-2643']
DOI: https://doi.org/10.1016/j.icarus.2022.114884