在CAI边缘的氧同位素变化记录了太阳星云内的循环
Justin I Simon1, Ian D Hutcheon, Steven B Simon
1Astromaterials Research Office KR111, NASA Johnson Space Center, Houston, TX 77058, USA. justin.i.simon@nasa.gov
概括
对富含和的含量 (CAI) 的分析显示了氧同位素的广泛变化. 这些发现表明CAI是由多个氧气储库形成的,这表明太阳星云早期的环境波动.
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:
- 富含和的包含物 (CAI) 是太阳星云中形成的最早的固体材料之一.
- 了解它们的同位素组成,可以了解太阳系早期的条件.
研究的目的:
- 为了研究特定的CAI及其周围矿物带的氧同位素组成.
- 确定观察到的同位素变异对CAI形成和早期太阳星云环境的影响.
主要方法:
- 对CAI及其矿物地幔的微米尺度分析.
- 测量氧同位素比率的测量.
主要成果:
- CAI的外部部分显示出各种各样的氧同位素组成.
- 氧同位素组成有系统地变化,向CAI边缘下降,然后在边缘变得非常富含16O.
- 观察到的变异性表明,由多个不同的氧气储形成.
结论:
- CAI很可能是从几个氧气储库中形成的.
- 这些数据支持太阳星云环境中的早期,短暂的波动.
- 这些波动可能是由于CAI运输或太阳星云气体组成的变化.
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