日本地球惑星科学連合2016年大会

講演情報

ポスター発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS12] 太陽系における惑星物質の形成と進化

2016年5月24日(火) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*宮原 正明(広島大学理学研究科地球惑星システム学専攻)、山口 亮(国立極地研究所)、臼井 寛裕(東京工業大学地球惑星科学科)、癸生川 陽子(横浜国立大学 大学院工学研究院 機能の創生部門)、藤谷 渉(茨城大学 理学部)、瀬戸 雄介(神戸大学大学院理学研究科)、伊藤 正一(京都大学大学院理学研究科)

17:15 〜 18:30

[PPS12-P03] Nogoya CMコンドライトに含まれるカルサイトの酸素・炭素同位体比

*藤谷 渉1福田 航平2小池 みずほ3石田 章純3佐野 有司3 (1.茨城大学、2.東京大学、3.東京大学 大気海洋研究所)

キーワード:カルサイト、酸素同位体、炭素同位体、CMコンドライト

CM chondrites exhibit evidence for aqueous alteration to variable degrees. Carbonate is a secondary mineral of aqueous alteration. Detailed petrological and mineralogical observations along with O-isotope measurements have been carried out by previous studies. These studies have suggested that carbonates in CM chondrites did not form in a single event but formed intermittently (Tyra et al., 2012; Lee et al., 2013). In this study, we conducted in-situ O- and C-isotope measurements on calcite grains in the Nogoya CM 2.2-2.3 chondrite. Isotope measurement on carbonates in multiple “generations” could shed light on the evolution of O and C isotopic compositions during aqueous alteration.
We found many calcite grains by SEM observation. As reported in the previous studies (e.g., Lee et al., 2014), two types of calcite grains with distinct mineralogical characteristics were found. Following the definition by Lee et al. (2014), we describe these calcite grains as type 1 and 2 grains. Most type 1 grains are single crystals and have serpentine/tochilinite rims. On the other hand, type 2 grains are polycrystalline and microporous, and do not have rims.
Oxygen isotopic compositions are highly different between type 1 and 2 grains, but similar within each type (d18O = 34.7 ‰ (type 1) and 19.3 ‰ (type 2) on average). The average D17O values are -2.5 ‰ (type 1) and -5.4 ‰ (type 2). The d18O and D17O values indicate that type 2 calcite formed later than type 1 calcite, because progressive alteration led to O-isotope exchange between water and anhydrous silicate with lower d18O and D17O values than water. Carbon isotopic ratios of type 1 grains are similar (d13C = 31.8 ‰ on average), whereas type 2 grains have variable d13C values ranging from 28.8 to 61.2 ‰. These observations indicate an increase in d13C values in later stages of aqueous alteration.
It has been suggested that the Rayleigh-type isotopic fractionation driven by the escape of 13C-poor CH4 could have led to 13C enrichments of the dissolved inorganic C (Guo and Eiler, 2007). The observed d13C increase of ~30 ‰ can be explained if ~28 % of the dissolved C was reduced to produce CH4 and was lost at 28 oC. If true, aqueous alteration in CM chondrites would have occurred in an open system at least in later stages.