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Rock Varnish As A Habitat For Extant Life On Mars

机译:岩石清漆作为现存在火星上的生命的栖息地

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Many of the rocks on the surface of Mars that have been imaged by the Viking and Mars Pathfinder Landers display dark shiny surface coatings resembling Mn-rich terrestrial rock varnish. On our planet, these thin (5 um - 1 mm) coatings can be the result of a combination of various weathering processes combined with microbial precipitation of mineral oxides over a wide variety of geographical locations but most commonly in those with arid and semi-arid conditions. Terrestrial Mn-rich rock varnish is produced by a wide variety of microorganisms including epilithic and edolithic cyanobacteria, bacteria and microcolonial fungi. As these microorganisms absorb trace amounts of Mn and Fe from atmospheric dust, rain and fog, they slowly precipitate "reddish" iron and "brown to black" manganese oxides as well as magnetite particles. These microbial communities then produce secretions that cement the Mn/Fe mix together with clay particles in a process involving time periods of perhaps thousands of years for a thin 5 um layer. Mn-rich rock varnish has been found to form on the surfaces of undisturbed desert fragments and even sand grains. Both Mn and Fe would serve as a UV shield for any microflora residing beneath and within the layers of varnish thus protecting against high UV irradiation, dissication, an widely varying temperature extremes. Recent research on rock varnish has led to the discovery that some microbial communities that produce dark ferromanganese varnishes also precipitate biogenic magnetite. In view recent independent evidence put forth by D. McKay and E.I. Friedmann et al for indigenous biogenic magnetite-chains in ALH 84001 along with meteorological models showing the possibility for small quantities of liquid water on the surface of Mars in combination with data obtained from the Viking LR experiment 27 years ago, recommendations are made to elucidate on whether or not the shiny dark-coatings covering some Martian rocks have been produced by living or extinct microbial communities.
机译:MARS表面上的许多岩石已经被Viking和Mars Pathfinder登陆器展示了类似MN Rich的陆地岩石清漆的深色闪亮的表面涂料。在我们的星球上,这些薄(5 um-1 mm)涂层可以是各种风化过程的组合,所述耐风化工艺结合在各种地理位置上,但最常见于有干旱和半干旱的矿物质中的微生物沉淀状况。富有的富有的岩石清漆是由各种微生物生产的,包括脱岩和亚摩奇菌,细菌和微菌菌真菌。由于这些微生物吸收痕量的Mn和Fe来自大气粉尘,雨水和雾,它们慢慢沉淀“Reddish”铁和“棕色至黑色”锰氧化物以及磁铁矿颗粒。然后,这些微生物群落产生分泌物,使得将Mn / Fe与粘土颗粒一起混合在涉及薄5um层的几千年的时间段的过程中。已发现富含富岩石清漆的岩石清漆在未受干扰的沙漠碎片和均匀的砂粒的表面上形成。 Mn和Fe都是UV屏蔽,用于驻留下方的任何微氟氯虫,在清漆层内,从而保护抗高紫外线照射,筛选,广泛变化的温度极端。最近对岩石清漆的研究导致了发现产生深色铁锰干法的一些微生物群落也沉淀生物磁铁矿。在查看D. McKay和E.I的最近独立证据。 Friedmann等人在ALH 84001中的本土生物磁铁矿链以及气象模型以及27年前从Viking LR实验中获得的数据的少量液体水的可能性,建议阐明无论是覆盖着一些火星岩石的闪亮的黑色涂层是由生物或灭绝的微生物社区生产的。

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