McKay D S, Gibson E K, Thomas-Keprta K L, Vali H, Romanek C S, Clemett S J, Chillier X D, Maechling C R, Zare R N
NASA Lyndon B. Johnson Space Center (JSC), Houston, TX 77058, USA.
Science. 1996 Aug 16;273(5277):924-30. doi: 10.1126/science.273.5277.924.
Fresh fracture surfaces of the martian meteorite ALH84001 contain abundant polycyclic aromatic hydrocarbons (PAHs). These fresh fracture surfaces also display carbonate globules. Contamination studies suggest that the PAHs are indigenous to the meteorite. High-resolution scanning and transmission electron microscopy study of surface textures and internal structures of selected carbonate globules show that the globules contain fine-grained, secondary phases of single-domain magnetite and Fe-sulfides. The carbonate globules are similar in texture and size to some terrestrial bacterially induced carbonate precipitates. Although inorganic formation is possible, formation of the globules by biogenic processes could explain many of the observed features, including the PAHs. The PAHs, the carbonate globules, and their associated secondary mineral phases and textures could thus be fossil remains of a past martian biota.
火星陨石ALH84001的新鲜断面上含有大量多环芳烃(PAHs)。这些新鲜断面还呈现出碳酸盐小球。污染研究表明,这些多环芳烃是陨石所固有的。对选定碳酸盐小球的表面纹理和内部结构进行的高分辨率扫描和透射电子显微镜研究表明,这些小球含有细粒的单畴磁铁矿和铁硫化物次生相。这些碳酸盐小球在纹理和大小上与一些地球上由细菌诱导形成的碳酸盐沉淀相似。尽管有可能是无机形成,但这些小球由生物过程形成可以解释许多观察到的特征,包括多环芳烃。因此,多环芳烃、碳酸盐小球及其相关的次生矿物相和纹理可能是过去火星生物群的化石遗迹。