日本地球惑星科学連合2014年大会

講演情報

口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS25_2AM2] 隕石解剖学: 太陽系物質の総合的理解に向けて

2014年5月2日(金) 11:00 〜 12:45 213 (2F)

コンビーナ:*瀬戸 雄介(神戸大学大学院理学研究科)、臼井 寛裕(東京工業大学地球惑星科学科)、伊藤 正一(京都大学大学院理学研究科)、薮田 ひかる(大阪大学大学院理学研究科宇宙地球科学専攻)、三浦 均(名古屋市立大学大学院システム自然科学研究科)、座長:三浦 均(名古屋市立大学大学院システム自然科学研究科)、薮田 ひかる(大阪大学大学院理学研究科宇宙地球科学専攻)

12:30 〜 12:45

[PPS25-14] C-XANES analyses of carbonaceous solid inclusions from Monahans halite

*癸生川 陽子1Zolensky Michael2Kilcoyne David3Rahman Zia4Fries Marc2Cody George5 (1.北海道大学 大学院理学研究院 自然史科学専攻 地球惑星システム科学、2.NASA Johnson Space Center、3.Lawrence Berkeley National Laboratory、4.Jacobs-Sverdrup、5.Geophysical Laboratory, Carnegie Institution of Washington)

キーワード:C-XANES, Halite, Carbon, Chondrite, Organic matter

Monahans meteorite (H5) contains fluid inclusion-bearing halite (NaCl) crystals [1]. Microthermometry and Raman spectroscopy showed that the fluid in the inclusions is an aqueous brine and they were trapped near 25oC [1]. Their continued presence in the halite grains requires that their incorporation into the H chondrite asteroid was post metamorphism [2]. Abundant solid inclusions are also present in the halites. The solid inclusions include abundant and widely variable organics [2]. Analyses by Raman microprobe, SEM/EDX, synchrotron X-ray diffraction and TEM reveal that these grains include macromolecular carbon similar in structure to CV3 chondrite matrix carbon, aliphatic carbon compounds, olivine (Fo99-59), high- and low-Ca pyroxene, feldspars, magnetite, sulfides, lepidocrocite, carbonates, diamond, apatite and possibly the zeolite phillipsite [3]. Here we report organic analyses of these carbonaceous residues in Monahans halite using C-, N-, and O- X-ray absorption near edge structure (XANES). Approximately 100 nm-thick sections were extracted with a focused ion beam (FIB) at JSC from solid inclusions from Monahans halite. The sections were analyzed using the scanning transmission X-ray microscope (STXM) on beamline 5.3.2.2 at the Advanced Light Source, Lawrence Berkeley National Laboratory for XANES spectroscopy. C-XANES spectra of the solid inclusions show micrometer-scale heterogeneity, indicating that the macromolecular carbon in the inclusions have complex chemical variations. C-XANES features include 284.7 eV assigned to aromatic C=C, 288.4-288.8 eV assigned to carboxyl, and 290.6 eV assigned to carbonate. The carbonyl features obtained by C-XANES might have been caused by the FIB used in sample preparation. No specific N-XANES features are observed. Various degrees of 1s-σ* exciton shown in the C-XANES spectra indicate that the solid inclusions contain macromolecular carbon which experienced various degree of thermal processing. The natures of the macromolecular carbon in the solid inclusions observed by C-XANES are consistent with the previous studies showing that the solid inclusions have not originated from Monahans parent body [1-3].References: [1] Zolensky et al. 1999. Science 285: 1377-1379. [2] Fries et al. 2011. 74th MetSoc #5390. [3] Zolensky et al. 2013. 76th MetSoc #5200.