4.7 Article

Phosphorus mineral evolution and prebiotic chemistry: From minerals to microbes

期刊

EARTH-SCIENCE REVIEWS
卷 221, 期 -, 页码 -

出版社

ELSEVIER
DOI: 10.1016/j.earscirev.2021.103806

关键词

Prebiotic; Chemistry; Origin; Life; Early Earth; Geology; Minerals; Phosphorus; Phosphate; Meteorite

资金

  1. NERC [NE/M000303/1, NE/L002507/1]
  2. Sloan, Deep Carbon Observatory, Keck, Templeton, NASA Astrobiology Institute
  3. NERC 'Deep Volatiles' consortium grant [NE/M000427/1]
  4. ERC [306655]
  5. NASA Exobiology grant [80NSSCC18K1288]
  6. European Research Council (ERC) [306655] Funding Source: European Research Council (ERC)
  7. NERC [NE/M000427/1, NE/M000303/1] Funding Source: UKRI

向作者/读者索取更多资源

The availability of phosphorus is crucial for the origin of life, and understanding the diversity of P-bearing phases on Earth's surface during the emergence of life is important for evaluating prebiotic scenarios. Differentiating between exogenous and endogenous phases, as well as considering the formation conditions and temporal distributions of P-bearing minerals, helps in determining the relevance of these phases for prebiotic chemistry. Connecting mineral-chemical scenarios to the environmental conditions and tectonic state of early Earth allows for a better assessment of the plausibility of these scenarios, bridging the fields of geoscience and prebiotic chemistry.
Phosphorus availability is considered a limiting factor in many scenarios for the origin of life. The concentration of P in environments of prebiotic interest will have been governed by the available mineral sources of P on the early Earth. A knowledge of early Earth P mineralogy and prevailing global and local environmental conditions is therefore needed to understand which scenarios for prebiotic chemistry are most plausible. Here, we review the plausible diversity of P-bearing phases at Earth's surface during the emergence of life. We consider phases that were delivered by meteorites (exogenous phases), as well as those that developed solely as a result of Earth system processes (endogenous phases). We take into account the known formation conditions of individual phases, as well as the observed temporal distributions of P-bearing minerals found at Earth's surface today. Our approach allows us to leverage what is known about changes in the Earth system in order to rule out the prebiotic relevance of many P-bearing phases. Meanwhile, we highlight a small number of phases that are of possible prebiotic relevance; specifically, exogenous schreibersite, merrillite, and apatite, and endogenous apatite, olivine, and glass. Prebiotic mineral-chemical scenarios can be formulated for each phase, with distinct requirements for the environmental and tectonic state of early Earth. We can therefore relate the plausibility of mineral-chemical scenarios to the nature of early Earth, bridging the fields of geoscience and prebiotic chemistry.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据