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火星陨石ALH84001中的亚微米级磁铁矿颗粒与碳化合物:通过冲击和热变质作用形成的无机、非生物成因。

Submicron magnetite grains and carbon compounds in Martian meteorite ALH84001: inorganic, abiotic formation by shock and thermal metamorphism.

作者信息

Treiman Allan H

机构信息

Lunar and Planetary Institute, Houston, Texas 77058, USA.

出版信息

Astrobiology. 2003 Summer;3(2):369-92. doi: 10.1089/153110703769016451.

Abstract

Purported biogenic features of the ALH84001 Martian meteorite (the carbonate globules, their submicron magnetite grains, and organic matter) have reasonable inorganic origins, and a comprehensive hypothesis is offered here. The carbonate globules were deposited from hydrothermal water, without biological mediation. Thereafter, ALH84001 was affected by an impact shock event, which raised its temperature nearly instantaneously to 500-700K, and induced iron-rich carbonate in the globules to decompose to magnetite and other minerals. The rapidity of the temperature increase caused magnetite grains to nucleate in abundance; hence individual crystals were very small. Nucleation and growth of magnetite crystals were fastest along edges and faces of the precursor carbonate grains, forcing the magnetite grains to be platy or elongated, including the "truncated hexa-octahedra" shape. ALH84001 had formed at some depth within Mars where the lithostatic pressure was significantly above that of Mars' surface. Also, because the rock was at depth, the impact heat dissipated slowly. During this interval, magnetite crystals approached chemical equilibria with surrounding minerals and gas. Their composition, nearly pure Fe(3)O(4), reflects those of equilibria; elements that substitute into magnetite are either absent from iron-rich carbonate (e.g., Ti, Al, Cr), or partitioned into other minerals during magnetite formation (Mg, Mn). Many microstructural imperfections in the magnetite grains would have annealed out as the rock cooled. In this post-shock thermal regime, carbon-bearing gas from the decomposition of iron carbonates reacted with water in the rock (or from its surroundings) to produce organic matter via Fischer-Tropschlike reactions. Formation of such organic compounds like polycyclic aromatic hydrocarbons would have been catalyzed by the magnetite (formation of graphite, the thermochemically stable phase, would be kinetically hindered).

摘要

ALH84001火星陨石所谓的生物成因特征(碳酸盐小球、其亚微米级磁铁矿颗粒和有机物)具有合理的无机成因,本文提出了一个全面的假说。碳酸盐小球是由热液水沉淀形成的,没有生物介导。此后,ALH84001受到一次撞击冲击事件的影响,其温度几乎瞬间升至500-700K,并促使小球中富含铁的碳酸盐分解为磁铁矿和其他矿物。温度升高的速度导致磁铁矿颗粒大量成核;因此单个晶体非常小。磁铁矿晶体的成核和生长在前体碳酸盐颗粒的边缘和表面最快,迫使磁铁矿颗粒呈片状或拉长状,包括“截顶六八面体”形状。ALH84001在火星内部的某个深度形成,那里的岩石静压力明显高于火星表面。此外,由于岩石处于深处,撞击热消散缓慢。在此期间,磁铁矿晶体与周围的矿物和气体接近化学平衡。它们的成分几乎是纯Fe(3)O(4),反映了这些平衡;替代进入磁铁矿的元素要么在富含铁的碳酸盐中不存在(如Ti、Al、Cr),要么在磁铁矿形成过程中分配到其他矿物中(Mg、Mn)。随着岩石冷却,磁铁矿颗粒中的许多微观结构缺陷会退火消除。在这种冲击后热状态下,铁碳酸盐分解产生的含碳气体与岩石(或其周围环境)中的水反应,通过费托类反应产生有机物。磁铁矿会催化多环芳烃等有机化合物的形成(石墨这种热化学稳定相的形成在动力学上会受到阻碍)。

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