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来自星际冰的紫外线辐射的氨基酸类似于星际冰
G M Muñoz Caro1, U J Meierhenrich, W A Schutte
1Raymond and Beverly Sackler Laboratory for Astrophysics at Leiden Observatory, PO Box 9513, NL-2300 RA Leiden, The Netherlands.
Nature
|March 29, 2002
概括
对于生命至关重要的氨基酸可以在星际冰中形成. 这项研究表明,外星的氨基酸可能已经播种了早期的地球,支持从太空运送前生物分子.
科学领域:
- 天体生物学 天体生物学
- 有机化学 有机化学
- 行星科学 行星科学
背景情况:
- 氨基酸对地球上的生命至关重要.
- 现有的理论难以解释早期氨基酸的起源.
- 有机化合物的外星交付是一种拟议的替代方案.
研究的目的:
- 为了研究星际冰中氨基酸的形成.
- 为了确定前生物分子是否可以在太空中形成.
- 评估这些分子对早期地球的潜在输送.
主要方法:
- 模拟的星际冰模拟器.
- 在高真空中在低温度 (12 K) 的紫外线照射.
- 对氨基酸含量进行室温残留物的分析.
主要成果:
- 在被辐射的冰残留物中检测出16种不同的氨基酸.
- 在奇拉性氨基酸中鉴定异构分离.
- 检测到的氨基酸与石中发现的氨基酸之间的重叠.
结论:
- 在星际介质中,氨基酸的形成是可能的.
- 这支持了预微生物分子通过外星来源传送到地球的假设.
- 彗星尘埃,石和行星间尘埃颗粒是潜在的输送工具.
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