在星际介质中形成的Ryugu样本中的多环芳
Sarah S Zeichner1, José C Aponte2, Surjyendu Bhattacharjee1
1Geological and Planetary Science Division, California Institute of Technology, Pasadena, CA 91125, USA.
概括
石中的多环芳 (PAH) 表明它们的星际起源. 同位素分析显示PAHs是在寒冷的星际云中形成的,而不仅仅是热的环恒星环境.
科学领域:
- 天体化学
- 宇宙化学
- 同位素地化学
背景情况:
- 多环芳 (PAH) 是星际介质中的重要碳载体.
- PAHs可能在不同的环境中形成,包括环恒星外,星际云或通过尘埃颗粒处理.
研究的目的:
- 通过在外星样本中分析它们的同位素特性来调查PAHs的起源.
- 根据它们的同位素组成区分PAH的形成途径.
主要方法:
- 从小行星Ryugu和Murchison石样本中提取PAHs.
- 测量特定PAH的双重13C替代成分 (Δ2×13C值).
主要成果:
- 纳夫他,和的 Δ2×13C值明显高于随机分布的预期值.
- 这些高值表明形成在寒冷的星际介质中,而不是高温的星际环境中.
- 在Ryugu样本中,氨酸和氨酸的 Δ2×13C 值与高温形成一致.
结论:
- 同位素数据支持在石中发现的某些PAH的星际形成.
- 证据表明PAHs的双重起源,其中一些在寒冷的星际环境中形成,而另一些则在更热的环境中形成.
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