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A Toolkit to Enable Hydrocarbon Conversion in Aqueous Environments
Published on: October 2, 2012
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在火星的泥石中保存的长链基
Caroline Freissinet1, Daniel P Glavin2, P Douglas Archer3
1Laboratoire Atmosphères et Observations Spatiales, Université Versailles St Quentin Université Paris-Saclay, Sorbonne Université, CNRS, Guyancourt 78280, France.
概括
古老的火星岩石含有较大的有机分子,包括干,未干和十二干,由好奇号探测器探测到. 这些发现为火星提供了线索.
科学领域:
- 天体生物学和行星科学 天体生物学和行星科学
- 火星上的有机地质化学
背景情况:
- 火星岩石中的有机分子是了解过去可居住性和潜在生物特征的关键.
- 之前由好奇号上的火星样本分析 (SAM) 仪器进行的分析,在盖尔火山口中发现了较小的含和含硫有机物.
研究的目的:
- 在火星沉积岩中检测和识别超过六个碳的较大的有机分子.
- 调查这些较大的有机化合物的保存状态和潜在来源.
主要方法:
- 使用了经过修改的火星样本分析 (SAM) 分析程序,该分析程序针对更大的有机分子进行了优化.
- 分析了来自盖尔火山口的坎伯兰钻井泥石样本.
- 进行实验室实验以支持保存假设.
主要成果:
- 在泥石样本中检测到小分子级别的 (C10H22),未 (C11H24) 和十二 (C12H26).
- 实验室实验表明,这些基被保存为泥石中的长链碳酸.
- 这些检测到的分子的起源仍然未确定,非生物和生物来源都是合理的.
结论:
- 发现更大的基扩大了火星上已知的有机分子范围.
- 这些发现突出了在火星沉积环境中保存复杂有机物质的潜力.
- 需要进一步的研究来确定这些长链有机分子的非生物或生物起源.
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