从小行星伊托卡瓦瓦返回的一颗粒子的中子激活分析
M Ebihara1, S Sekimoto, N Shirai
1Department of Chemistry, Tokyo Metropolitan University, Hachioji, Tokyo 192-0397, Japan. ebihara-mitsuru@tmu.ac.jp
概括
对海亚布萨航天器颗粒的分析揭示了外星起源和原始组成. 它的化学构成与地铁类似,尽管其金属成分中的含量较低.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 天文地质学 天文地质学
背景情况:
- 小行星伊托卡瓦的样本由海亚布萨任务返回地球.
- 了解小行星样本的组成,可以了解太阳系早期的材料.
- 中子激活分析是一种敏感的技术,用于确定元素组成.
研究的目的:
- 为了确定返回的伊托卡瓦小行星颗粒的化学成分和来源.
- 为了将伊托卡瓦样本的化学特性与已知的石类别进行比较.
- 调查样品成分对星云凝结过程的影响.
主要方法:
- 从海亚布萨任务的伊托卡瓦样本中分析了一粒3微克的颗粒.
- 使用中子激活分析来确定谷物的元素组成.
- 计算和比较了主要元素的比率 (例如Fe/Sc,Ni/Co,Ir/Ni,Ir/Co).
主要成果:
- 谷物主要由橄素组成,少量有青酸盐,酸盐和金属.
- 伊托卡瓦样本的化学特征 (Fe/Sc,Ni/Co比率) 类似于混凝土,证实了外星起源和原始组成.
- 伊托卡瓦样本中的金属显示/和/的比率大约是CI碳状地铁的五倍,类似于普通地铁金属.
结论:
- 伊托卡瓦谷物是外星人,具有原始的化学成分.
- 伊托卡瓦样本金属中的枯竭表明,它来自雾状环境的凝结,在那里,耐火的 siderophile 元素已经分离出来.
- 这一发现有助于理解太阳星云的化学演变和行星形状的形成.
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