Oxygen Isotopes in the Minerals of Unequilibrated Chondrites

不平衡球粒陨石矿物中的氧同位素

• 批准号: 9418520
• 负责人: John Wasson
• 金额: $ 6万
• 依托单位: University of California-Los Angeles
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1995
• 资助国家: 美国
• 起止时间: 1995-08-01 至 1998-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9418520&HistoricalAwards=false
• 关键词: Oxygen; Isotopes; Minerals; Unequilibrated; Chondrites

9418520 Wasson The P.I.s propose to use the UCLA Cameca 1270 ion-microprobe and petrographic techniques to determine the three O-isotopes in the conducting phase magnetite present in unequilibrated chondritic meteorites in order to obtain detailed compositional data that relate to: (1) the nebular processes that led to the formation of the chondrites; (2) the compositions of major O reservoirs that contributed to the solar nebula; and (3) low-grade metamorphic processes that occurred in parent bodies. During the next year the P.I.s will study the formation of the magnetite in unequilibrated carbonaceous (CV) and ordinary (H, L, LL) chondrites. The P.I.s examination of many thin sections of CV chondrites shows that magnetite is relatively common in chondrules. The P.I.s will use the ion microprobe to determine the compositions of these magnetites on the oxygen 3-isotope diagram relative to other CV minerals that describe a mixing line extending from 18O values -40% along a slope of 0.94 almost to the intersection of this line with the terrestrial fractionation line. A key question the P.I.s hope to answer is whether this magnetite formed in the solar nebula or during the oxidation of the CV parent body. The P.I.s' second project will be to examine the three O isotopes in magnetite present in magnetite-carbide assemblages in some unequilibrated ordinary chondrites. Krot discovered a number of these assemblages while at UCLA. The origin of these oxidized/reduced assemblages is not known; again, the possible locales are the solar nebula and the parent body. Precise O-isotope data will provide important constraints both on the locale and on the nature of the agent that oxidized the Fe of the magnetite.

9418520 Wasson PI.s建议使用UCLA Cameca1270离子微探针和岩石学技术来测定非平衡球粒陨石中存在的导电相磁铁矿中的三种氧同位素，以获得与以下相关的详细成分数据：(1)导致球粒陨石形成的星云过程；(2)对太阳星云做出贡献的主要氧水库的组成；以及(3)发生在母体中的低级别变质过程。在接下来的一年里，P.I.S将研究非平衡碳质(CV)和普通(H，L，LL)球粒陨石中磁铁矿的形成。对许多CV球粒陨石薄片的P.I.S分析表明，磁铁矿在球粒陨石中相对常见。P.I.将使用离子探针来确定相对于其他CV矿物的氧3同位素图上这些磁铁矿的组成，该图描述了一条从18O值-40%沿0.94的斜率延伸到这条线与陆地分馏线的交叉点的混合线。P.I.希望回答的一个关键问题是，这种磁铁矿是在太阳星云中形成的，还是在CV母体氧化期间形成的。P.I.S的第二个项目将是检查存在于一些不平衡的普通球粒陨石中的磁铁矿-碳化物组合中的磁铁矿中的三个氧同位素。克罗特在加州大学洛杉矶分校时发现了许多这样的组合。这些氧化/还原组合的起源尚不清楚；同样，可能的地点是太阳星云和母体。准确的氧同位素数据将对地点和氧化磁铁矿中铁的试剂的性质提供重要的约束。