太阳的氧同位素组成是由捕获的太阳风推断出来的
K D McKeegan1, A P A Kallio, V S Heber
1Department of Earth and Space Sciences, University of California-Los Angeles (UCLA), Los Angeles, CA 90095-1567, USA. mckeegan@ess.ucla.edu
概括
太阳的氧气-16 (16O) 含量比太阳系内部的岩石材料要高. 这表明早期的非质量依赖化学在更重的氧同位素中丰富了陆地行星.
科学领域:
- 宇宙化学 宇宙化学
- 行星科学 行星科学
- 天体生物学 天体生物学
背景情况:
- 太阳系材料的氧同位素组成显示出显著的差异.
- 一个明确的原始太阳系氧同位素组成尚未确定.
- 太阳的光球被认为是太阳系中比更重元素的平均同位素组成的代表.
研究的目的:
- 为了确定太阳的氧同位素组成.
- 为了将太阳的氧同位素与太阳系内部行星材料的氧同位素进行比较.
- 调查太阳系内部同位素变化的起源.
主要方法:
- 分析太阳风样本由美国宇航局的创世纪任务返回地球.
- 在太阳风中测量氧同位素比率 ((16) O, (17) O, (18) O).
- 太阳风同位素数据与地球,月球,火星和石的现有数据进行比较.
主要成果:
- 与地球,月球,火星和散装石相比,太阳在氧气-16 (16O) 中表现出显著的丰富.
- 内部太阳系的岩石体相对于太阳的16O是耗尽的.
- 这些发现表明,岩石材料在较重的氧同位素 ((17) O和 (18) O) 中相对于16O的比例大约为7%.
结论:
- 太阳的同位素组成反映了早期太阳系的平均值.
- 太阳系内部的岩石材料可能经历了17O和18O的丰富.
- 这种丰富可能是行星积累之前发生的非质量依赖化学过程的结果.
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