第4章:地球早期生命起源的地质和化学背景
Laura E Rodriguez1,2, Thiago Altair3,4, Ninos Y Hermis1,5
1NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
Astrobiology
|March 18, 2024
概括
早期的地球通过地化学过程从不适合居住转变为支持生命. 了解这个早期的环境有助于寻找外星生命和新的生物化学.
科学领域:
- 地质化学 地质化学
- 天体生物学 天体生物学
- 行星科学 行星科学
背景情况:
- 哈代/欧阿纪时代见证了地球从一个敌对的行星转变为一个可居住的行星.
- 早期地球的关键组成部分,包括月球,地,海洋,大气和有机分子,对于理解生命起源至关重要.
- CHONPS元素 (碳,,氧,,,硫) 的非生物地化学循环在形成生命的基石中起到了至关重要的作用.
研究的目的:
- 审查当前关于早期地球地化学环境的知识.
- 探索非生物元素转化为生物学相关的分子和网络.
- 评估拟议的生物发生环境及其对可居住性和生物特征的影响.
主要方法:
- 对Hadean/Eoarchean地化学和地质数据的文献综述.
- 对地球月球,地,海洋和大气的起源模型的分析.
- 对有机分子和化学网络的非生物合成所提议的途径的评估.
主要成果:
- 早期地球的地化学环境是充满活力的,它在进化以支持生命.
- 无生物过程可以从基本元素中产生复杂的有机分子和化学网络.
- 已经提出了各种环境的生物发生,每个都有不同的含义.
结论:
- 了解早期地球的地质化学对于评估外星人的可居住性至关重要.
- 无生物化学可以实现显著的复杂性,为寻找生物标志提供信息.
- 研究早期地球可能会揭示非地球生物化学的可能性.
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