کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
4677579 1634810 2012 13 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Sulfur species and biosignatures in Sulphur Springs, Valles Caldera, New Mexico—Implications for Mars astrobiology
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم زمین و سیاره ای (عمومی)
پیش نمایش صفحه اول مقاله
Sulfur species and biosignatures in Sulphur Springs, Valles Caldera, New Mexico—Implications for Mars astrobiology
چکیده انگلیسی

A biogeochemical SO42 − cycle was investigated in the acid-hot springs of Valles Caldera, New Mexico using S isotopes and distribution of amino acids. In 2007, a major contribution of SO42 − in this modern volcanic setting came from oxidation of H2S from hydrothermal sources, which largely increased SO42 − concentrations (up to 2550 mg L− 1) and decreased pH (down to 2.27) in surface water. A relatively small variation of δ34S among the analyzed S-bearing minerals (2.1 to 4.0‰), fumarole H2S (1.7 to 4.6‰) and dissolved SO42 − in modern surface and groundwater (2.5 to 7.9‰) indicates poor evidence of S isotope biosignatures related to microbial disproportionation of elemental S to H2S and SO42 − which, in turn, are not effectively captured in the hydrothermal minerals of the studied volcanic setting. This is mainly due to prevailing contribution of reduced S forms from magmatic/hydrothermal sources and considerably smaller microbial activity in acid-hot spring areas. Although hydrothermal gypsum and elemental S effectively trap amino acids, their preservation lifetimes in S-bearing hydrothermal minerals appear to be small. The minimal lifetimes are inferred to be the result of increased temperatures and rapid recycling time of S materials in hydrothermal settings.Landed missions to the Martian surface at sites inferred to have experienced active hydrothermal activity similar to the one studied in Valles Caldera (e.g., elevated volcanic S flux), may provide valuable insight into geological and geochemical processes that have influenced the Martian surface, but may provide minimal potential for recording either amino acid or S isotopic biosignatures of an extinct Martian ecosystem.


► Hydrothermal settings minimize preservation of S isotope and amino acid biosignatures.
► Abiotic oxidation of magmatic H2S overprints the biotic S isotope fractionation.
► Amino acid decarboxylation and racemization rates are rapid in hydrothermal deposits.
► Martian hydrothermal sites may provide minimal preservation of similar biosignatures.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Earth and Planetary Science Letters - Volumes 321–322, 1 March 2012, Pages 1–13
نویسندگان
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