年轻的chondrules在CB的chondrites从太阳系早期的巨大撞击
Alexander N Krot1, Yuri Amelin, Patrick Cassen
1Hawai'i Institute of Geophysics & Planetology, School of Ocean & Earth Science & Technology, University of Hawai'i at Manoa, 2525 Correa Rd, Honolulu, Hawaii 96822, USA. sasha@higp.hawaii.edu
Nature
|August 19, 2005
概括
石中的原始孔德鲁尔是由早期太阳系尘埃形成的. 关于CB地质的新研究表明,它们是由巨型撞击形成的,这表明小行星带的早期行星形成.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 太阳系早期的进化过程
背景情况:
- 圆柱体是圆柱体石的主要组成部分,是由太阳系早期的粉尘融化形成的.
- 它们的形成年龄与原行星盘消散时间尺度一致.
- 以前的模型表明,形成是通过原行星盘中的冲击波.
研究的目的:
- 为了确定金属丰富的CB碳酸地里特中流体的形成年龄和机制.
- 调查这些发现对早期太阳系形成模型的影响.
主要方法:
- 使用207Pb-206Pb同位素系统进行放射测年.
- 对古吉巴和哈马达哈姆拉237颗石的孔德鲁尔年龄的分析.
主要成果:
- 来自Gujba和Hammadah al Hamra 237的CB孔德鲁的年龄分别为4,562.7 +/- 0.5 Myr和4,562.8 +/- 0.9 Myr.
- 这些圆柱体是在单一的,高能量的事件中形成的.
- 年龄和形成特征与星云冲击波起源不一致.
结论:
- CB孔德鲁和相关的金属粒很可能是由行星胚胎之间巨大的撞击产生的蒸汽融化羽毛形成的.
- 这次撞击发生在原行星盘中大量尘埃消散后.
- 这些发现提供了早期小行星带中行星大小物体的证据,支持目前的行星形成模拟.
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