相关实验视频
Updated: Jun 15, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
来自NASA星尘任务彗星物质形成年龄的限制
J E P Matzel1, H A Ishii, D Joswiak
1Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, CA 94550, USA. matzel2@llnl.gov
概括
像科基这样的彗星包含在太阳系早期固体后超过170万年形成. 这表明,太阳系内部形成的物质后来被纳入彗星中.
科学领域:
- 宇宙化学 宇宙化学
- 行星科学 行星科学
- 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,为其形成提供了洞察力.
- 了解彗星包含形成的时间是太阳系进化模型的关键.
研究的目的:
- 通过分析它们的同位素组成来确定彗星内含物形成的时间表.
- 将彗星材料的形成时间与石对应物进行比较,例如富含和的含 (CAI).
主要方法:
- 在来自彗星81P/Wild 2的耐火粒子 (Coki) 中测量26Al-26Mg同位素的系统性.
- 使用质谱法分析同位素丰度并限制26Al的存在.
主要成果:
- 在Coki粒子中没有发现放射性26Mg的证据.
- 粒子形成时的26Al丰度的上限被确定为:26Al/27Al < 1 x 10(-5).
- 缺少26Al表明Coki是在CAI形成后的170多万年形成的.
结论:
- 科基比最早的太阳系固体 (CAI) 形成的时间要晚得多.
- 这意味着来自内太阳系的高温物质被加工并运送到外太阳系.
- 彗星内含物代表了在太阳系形成的最初阶段数百万年后融入彗星的物质.
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