盐是彗星核和一些小行星上的储物
Olivier Poch1, Istiqomah Istiqomah2, Eric Quirico2
1Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), 38000 Grenoble, France. olivier.poch@univ-grenoble-alpes.fr.
概括
彗星67P/Churyumov-Gerasimenko以盐的形式含有大量的气,解决了气与碳的比例差异. 这些盐是主要的储物, 连接彗星和小行星组成.
科学领域:
- 星球科学
- 天体化学
- 彗星科学
背景情况:
- 彗星中与碳 (N/C) 的比率低于太阳,这表明缺少储备.
- 彗星67P/Churyumov-Gerasimenko在其核中显示了一个独特的光谱特征.
研究的目的:
- 确定67P/Churyumov-Gerasimenko彗星上未知的光谱特征的来源.
- 确定这个特征作为彗星中潜在的储库的作用.
主要方法:
- 模拟彗星表面条件的实验室实验.
- 对67P/Churyumov-Gerasimenko彗星的光谱反射率数据进行分析.
- 彗星光谱特征与小行星光谱的比较.
主要成果:
- 3,2微米的吸收范围归因于与尘埃混合的盐.
- 盐在67P彗星中占有大量的储量,可能超过其他含化合物.
- 在一些小行星中观察到类似的光谱特征.
结论:
- 盐被确定为67P/Churyumov-Gerasimenko彗星上的重要储物.
- 这一发现有助于协调彗星中观察到的N/C比率差异.
- 氨盐的存在表明彗星,小行星和星际介质之间的组成联系.
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