在碳状地铁的Ca,Al丰富含中含有康伦,鲁,环和CaO,含有碳状地铁
A Greshake1, A Bischoff, A Putnis
1Institut für Planetologie, Universität Münster, Germany.
概括
石中的微小的氧化物粒提供了早期太阳系过程的线索. 这些耐火氧化物可能是通过动力控制的凝聚形成的,而不是溶解,在太阳星云上发光.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 材料科学 材料科学 材料科学
背景情况:
- 碳状石是原始的石,保存了太阳系早期的材料.
- 富含和的含 (CAI) 是太阳星云中最早出现的固体凝聚物之一.
- 了解CAI矿物学可以了解星云状况.
研究的目的:
- 为了研究矿物学和氧化物的形成机制,在CAI内从各种碳状地铁.
- 为了限制在早期太阳星云中耐火性内含物形成过程中普遍存在的条件和过程.
主要方法:
- 使用传输电子显微镜 (TEM) 来分析氧化物颗粒的微观结构.
- 研究了来自阿伦德,Acfer 082,Acfer 086和Acfer 094的含量.
- 在CAI构成矿物中纳米级氧化物 (50-200nm) 的矿物学表征.
主要成果:
- 四个CAI含有至少两种氧化物:危氧化物 (MgO),鲁 (TiO2),氧化 (CaO) 和玉合金 (Al2O3).
- 这些氧化物在构成矿物和它们的谷物边界内都被观察到.
- 溶解被认为是这些氧化物的不太可能的形成机制.
结论:
- 观察到的氧化物组合表明通过动力控制的凝结形成.
- 这一发现支持早期太阳星云中异质凝聚的模型.
- 这项研究提供了关于里特体中耐火性含体的起源和演变的见解.
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