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在Ryugu小行星中发现的一种原始贵重气体成分及其含义
Alexander B Verchovsky1, Feargus A J Abernethy2, Mahesh Anand2
1The Open University, Milton Keynes, UK. sasha.verchovsky@open.ac.uk.
Nature communications
|September 14, 2024
概括
科学家们在Ryugu小行星样本中发现了一种新的原始贵重气体成分,称为P7. 这一发现,与显著更高的离子度,提供了洞察早期太阳系的组成和分成过程.
科学领域:
- 宇宙尘埃分析 太空尘埃分析
- 同位素地球化学 同位素地球化学
- 行星科学 行星科学
背景情况:
- 由Hayabusa2返回的Ryugu小行星样本含有贵重气体.
- 之前的分析表明,与碳状地质 (CIs) 相比,Ryugu样本中的太阳风和行星 (P1) 贵重气体度更高.
- 这表明瑞古样本可能比CI更原始.
研究的目的:
- 为了分析三个细粒度的Ryugu样本中的贵重气体含量.
- 为了研究具有异常高度的样品.
- 描述一个潜在的新原始贵重气体成分.
主要方法:
- 精细粒度的Ryugu样本的高贵气体分析.
- 对和的同位素分析.
- 与太阳风和已知的行星成分的同位素比率的比较.
主要成果:
- 一个样本与之前分析的Ryugu样本相比,异度增加了十倍.
- 这个样本中的同位素与行星 (P1) 成分相似,但显示出更大的分离率.
- 与P1.1相比,观察到明显较低的Ar/Xe比率.
- 确定了一种新的原始贵重气体成分,被指定为P7.
结论:
- P7组件代表了太阳系中以前未被识别的原始贵重气体储备.
- P7的同位素特性为了解太阳成分分成提供了关键数据.
- 这一发现完善了从最初的太阳星云中形成行星贵重气体成分的模型.
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