کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
4677322 1634797 2012 14 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Carbonate precipitation under bulk acidic conditions as a potential biosignature for searching life on Mars
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
پیش نمایش صفحه اول مقاله
Carbonate precipitation under bulk acidic conditions as a potential biosignature for searching life on Mars
چکیده انگلیسی

Recent observations of carbonate minerals in ancient Martian rocks have been interpreted as evidence for the former presence of circumneutral solutions optimal for carbonate precipitation. Sampling from surface and subsurface regions of the low-pH system of Río Tinto has shown, unexpectedly, that carbonates can form under diverse macroscopic physicochemical conditions ranging from very low to neutral pH (1.5–7.0). A multi-technique approach demonstrates that carbonate minerals are closely associated with microbial activity. Carbonates occur in the form of micron-size carbonate precipitates under bacterial biofilms, mineralization of subsurface colonies, and possible biogenic microstructures including globules, platelets and dumbbell morphologies. We propose that carbonate precipitation in the low-pH environment of Río Tinto is a process enabled by microbially-mediated neutralization driven by the reduction of ferric iron coupled to the oxidation of biomolecules in microbially-maintained circumneutral oases, where the local pH (at the scale of cells or cell colonies) can be much different than in the macroscopic environment. Acidic conditions were likely predominant in vast regions of Mars over the last four billion years of planetary evolution. Ancient Martian microbial life inhabiting low-pH environments could have precipitated carbonates similar to those observed at Río Tinto. Preservation of carbonates at Río Tinto over geologically significant timescales suggests that similarly-formed carbonate minerals could also be preserved on Mars. Such carbonates could soon be observed by the Mars Science Laboratory, and by future missions to the red planet.


► Micron-sized carbonates are found in an acidic environment.
► They associate to acidic sulfates.
► They form by microbially-maintained circumneutral oases.
► Acidic sulfates formed on Early Mars.
► We propose them as biosignatures to trace life in Mars paleoenvironments.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volumes 351–352, 15 October 2012, Pages 13–26
نویسندگان
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