超镁铁质岩
地质学
地球化学
硅酸盐
甲烷
硅酸盐矿物
天体生物学
早期地球
磁铁矿
地幔(地质学)
橄榄石
土(古典元素)
玄武岩
有机质
化学
古生物学
有机化学
物理
数学物理
作者
Norman H. Sleep,Anders Meibom,Thráinn Fridriksson,Robert G. Coleman,D. K. Bird
标识
DOI:10.1073/pnas.0405289101
摘要
Metamorphic hydration and oxidation of ultramafic rocks produces serpentinites, composed of serpentine group minerals and varying amounts of brucite, magnetite, and/or FeNi alloys. These minerals buffer metamorphic fluids to extremely reducing conditions that are capable of producing hydrogen gas. Awaruite, FeNi 3 , forms early in this process when the serpentinite minerals are Fe-rich. Olivine with the current mantle Fe/Mg ratio was oxidized during serpentinization after the Moon-forming impact. This process formed some of the ferric iron in the Earth's mantle. For the rest of Earth's history, serpentinites covered only a small fraction of the Earth's surface but were an important prebiotic and biotic environment. Extant methanogens react H 2 with CO 2 to form methane. This is a likely habitable environment on large silicate planets. The catalytic properties of FeNi 3 allow complex organic compounds to form within serpentinite and, when mixed with atmospherically produced complex organic matter and waters that circulated through basalts, constitutes an attractive prebiotic substrate. Conversely, inorganic catalysis of methane by FeNi 3 competes with nascent and extant life.
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