小行星材料的氧气同位素组成由海亚布萨任务从伊托卡瓦返回
Hisayoshi Yurimoto1, Ken-ichi Abe, Masanao Abe
1Natural History Sciences, Hokkaido University, Sapporo 060-0810, Japan. yuri@ep.sci.hokudai.ac.jp
概括
研究人员发现,小行星伊托卡瓦的氧同位素组成与某些石相匹配. 这提供了直接的证据,将小行星与原始的地铁联系起来,进步了我们对太阳系形成的理解.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 地质地质地质地质地质地
背景情况:
- 太阳系天体具有独特的氧同位素组成.
- 石,原始的石,被认为起源于小行星.
- 小行星氧气同位素组成在很大程度上仍未确定.
研究的目的:
- 为了确定小行星25143 Itokawa的氧同位素组成.
- 为了在小行星和体石之间建立直接联系.
主要方法:
- 二次离子质谱法用于氧同位素分析.
- 分析是由海亚布萨航天器从小行星25143伊托卡瓦返回的岩石颗粒进行的.
主要成果:
- 测量了伊托卡瓦粒子的氧同位素组成.
- 与陆地材料相比,这些组合物在氧-16中耗尽.
- 伊托卡瓦的组成与LL或L组普通状体一致.
结论:
- 小行星25143伊托卡瓦是LL或L组普通体的潜在来源.
- 这项研究确立了母小行星和体之间的直接氧同位素联系.
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