月球形成的冲击和生命的自食起源
Natalia Mrnjavac1, Jessica L E Wimmer1, Max Brabender1
1Department of Biology, Institute for Molecular Evolution, Heinrich Heine University Duesseldorf, Universitaetsstr. 1, 40225, Düsseldorf, Germany.
ChemPlusChem
|October 9, 2023
概括
月球形成的撞击造成了地球的岩海洋,释放出二氧化碳. 这种二氧化碳溶解在海洋中,使有机化合物合成和早期生命的起源通过自身养过程.
科学领域:
- *行星科学 *行星科学
- * 星际生物学 星际生物学
- * 地质化学 * 地质化学
背景情况:
- * 形成月球的撞击事件显著改变了地球早期的地幔,形成了岩海洋.
- *二氧化碳 (CO2) 从这种岩海洋中脱气进入大气层.
- * 大气中的二氧化碳后来溶解成新形成的海洋.
研究的目的:
- * 解释月球形成撞击在创造有利于生命起源的条件中的作用.
- *阐明大气中的二氧化碳到微生物新陈代谢必不可少的有机化合物的途径.
- *将早期地球的碳循环与自营生命的出现联系起来.
主要方法:
- * 分析月球形成撞击后的地球化学过程.
- *研究过渡金属催化剂在有机合成中的作用.
- * 对生命自身养的起源理论的综述.
主要成果:
- *撞击事件使碳均质化,使其成为有机合成的可访问基质.
- *海洋中溶解的二氧化碳与催化剂反应形成有机化合物.
- * 这一过程在早期富含二氧化碳的大气和第一个微生物之间建立了直接联系.
结论:
- * 形成月球的撞击对于建立地球产生生命的能力至关重要.
- *早期的生态系统依赖于初级生产者的二氧化碳固定,它们的起源可以追溯到这种影响.
- * 化学性自营性古生物和细菌,起源于这个过程,仍然居住在地球地.
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