在太阳星云中存在一个富含16O的气体储
Alexander N Krot1, Kevin D McKeegan, Laurie A Leshin
1Hawaii Institute of Geophysics and Planetology, School of Ocean and Earth Science and Technology, University of Hawaii, Honolulu, HI 96822, USA. sasha@higp.hawaii.edu
概括
石中的橄粒显示富含氧-16 (16O),这表明早期太阳星云中的气体富含16O. 这表明,富含和的含有物 (CAI) 和阿米类橄类聚合物 (AOA) 形成在一个独特的局部区域.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 碳状地质含有在早期太阳星云中形成的橄粒.
- 氧同位素组成为早期太阳系材料的条件和位置提供了洞察力.
- 富含和的含有物 (CAI) 和阿米波酸橄聚合物 (AOA) 是最早的固体凝结物之一.
研究的目的:
- 为了研究来自CAI增积边缘和AOA的橄素粒的氧气同位素组成.
- 确定这些原始物体形成的气体库的氧同位素特征.
- 了解早期太阳星云中的同位素储库的空间分布.
主要方法:
- 使用二次离子质谱法 (SIMS) 对橄素粒的现场氧同位素分析.
- 碳化石样本的石化检查,以确定目标颗粒.
- 同位素数据与CAI和chondrules的现有数据集的比较.
主要成果:
- 来自CAI轮和AOA的橄素颗粒显示出显著的氧-16 (16O) 丰富.
- 这种16O丰富度与CAI中观察到的相似.
- 它的同位素成分与构造体区域的16O贫乏特征形成鲜明对比.
结论:
- 数据表明,CAI和AOA形成的特定星云区域的气体具有高度的16O含量.
- 这表明16O丰富气体的空间有限的储备,与构成体的环境不同.
- 富含16O气体的可能来源包括质量独立的同位素分离或年轻太阳附近的局部蒸发过程.
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