彗星物质的同位素组成由星尘返回
Kevin D McKeegan1, Jerome Aléon, John Bradley
1Department of Earth and Space Sciences, University of California Los Angeles, Los Angeles, CA 90095-1567, USA. mckeegan@ess.ucla.edu
概括
彗星81P/Wild 2包含来自内外太阳系的物质,而不仅仅是原始的太阳前物质. 同位素分析揭示了起源的混合,挑战了纯粹原始彗星的想法.
科学领域:
- 宇宙尘埃分析 太空尘埃分析
- 彗星科学 彗星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 彗星是太阳系早期的残余物,为其形成提供了线索.
- 彗星81P/Wild 2因其独特的组成而受到研究,它有可能保留原始材料.
研究的目的:
- 为了研究彗星81P/Wild 2粒子碎片的同位素组成.
- 为了确定彗星内部材料的起源,并评估它的原始性质.
主要方法:
- 在彗星碎片中分析,碳,和氧同位素组成.
- 检查单个颗粒的矿物学和同位素特征.
主要成果:
- 观察到同位素异质性,但极端异常是罕见的,表明有限的前太阳物质.
- 非地球上的和同位素表明土著有机和挥发性物质的存在.
- 大多数酸盐和氧化物都显示出太阳系的同位素起源,其中一个耐火粒显示出 (16) O 丰富,表明太阳系内部的形成.
结论:
- 彗星81P/Wild 2不是一个原始的前太阳物质聚合物.
- 彗星中含有来自内外太阳系的物质混合物.
- 有证据表明,高温的太阳系内部物质在彗星积聚之前被运送到柯伊伯带.
相关概念视频
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