Possibilities for Methanogenic and Acetogenic Life in Molecular Clouds

被引:0
|
作者
Feng, Lei [1 ,2 ,3 ]
机构
[1] Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210023, Peoples R China
[2] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China
[3] Nanjing Univ, Joint Ctr Particle Nucl Phys & Cosmol, Purple Mt Observ, Nanjing 210093, Peoples R China
来源
LIFE-BASEL | 2024年 / 14卷 / 11期
基金
中国国家自然科学基金;
关键词
origin of life; LUCA; molecular cloud; CARBON-MONOXIDE; AMINO-ACIDS; METHANE; TEMPERATURE; ATMOSPHERE; DISCOVERY; ABUNDANCE; DIOXIDE; MARS;
D O I
10.3390/life14111364
中图分类号
Q [生物科学];
学科分类号
07 ; 0710 ; 09 ;
摘要
According to panspermia, life on Earth may have originated from life forms transported through space from elsewhere. These life forms could have passed through molecular clouds, where the process of methanogenesis could have provided enough energy to sustain living organisms. In this study, we calculate the Gibbs free energy released from synthesizing hydrocarbons for methanogenic (acetogenic) life in a molecular cloud, with methane (acetic acid) as the final metabolic product. Our calculations demonstrate that the chemical reactions during methanogenesis can release enough free energy to support living organisms. The methanogenic life may have served as the predecessor of life on Earth, and there is some preliminary evidence from various molecular biology studies to support this idea. Furthermore, we propose a potential distinguishing signal to test our model.
引用
收藏
页数:9
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