在162173 Ryugu中大量的微型控制器表明,原始小行星的起源是动荡的
Matthew J Genge1,2, Natasha V Almeida3, Matthias van Ginneken4
1Department of Earth Science and Engineering, Imperial College London, London, UK. m.genge@imperial.ac.uk.
Nature communications
|July 23, 2025
概括
研究人员在小行星Ryugu样本中发现了丰富的微粒体,这表明了太阳系早期尘埃形成的新模型. 这些发现挑战了关于原始小行星形成的传统观念.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 太阳系的演变 太阳系的演变
背景情况:
- 圆柱体是原始太阳系材料的关键组成部分,为原行星盘过程提供了洞察力.
- 它们的形成与太阳星云内的能量事件有关,但较小变体的起源仍在争论中.
研究的目的:
- 为了研究C型小行星Ryugu的样本中微粒体的存在和特征.
- 提出一个新的形成和运输机制,在早期的太阳系内微型控制器.
主要方法:
- 来自小行星Ryugu.180的A0180样本的分析.
- 描述微粒规则的丰富性,大小和形状分布.
主要成果:
- 发现了大量的改变的微粒 (超过350ppm),其尺寸为6-8μm.
- 微粒体表现出类似于较大粒体的日志-正常大小和形状分布.
- 证据表明,形成在太阳系外层的"圆柱体工厂"和随后通过流和流动的集中.
结论:
- 微粒体可能是在木星的压力突起区域中形成的,并因流和流而集中.
- 这挑战了原始小行星必须在最大的日中心距离形成的观念.
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