Lightning-Driven Pyrite Oxidation Under Archean Atmosphere Conditions.

IF 3.5 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Astrobiology Pub Date : 2024-12-01 Epub Date: 2024-11-28 DOI:10.1089/ast.2024.0074
Annabel L S Long, Abu S Baidya, Eva E Stüeken
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Abstract

Oxidative weathering is a major source of bio-essential micronutrients on Earth today; however, this flux would have been muted on the early Earth or on Mars, where atmospheric O2(g) levels were very low. Here, we explore the hypothesis that nitrogen oxides generated by lightning in an anoxic atmosphere could have elevated pyrite oxidation levels under otherwise anoxic conditions. We performed spark discharge experiments in the presence of pyrite powder and three different gas mixtures, including 80% N2(g) with 20% CO2(g), 95% N2(g) with 5% CO2(g), and modern air. Experiments were run for 30 min, and we tracked the production of NO(g), dissolved nitrate and nitrite, pH, dissolved sulfate, and total dissolved iron. Our results reveal increasing production of nitrogen oxides with increasing CO2(g) and O2(g) levels, which is consistent with previous studies. Dissolved iron and sulfate also increase, indicating that the nitrogen oxides are able to oxidize pyrite abiotically. Extrapolating these data to global conditions suggests that this mechanism was probably insignificant on a global scale on the early Earth; however, in thunderstorm-prone areas, such as in the modern tropics where lightning rates may locally be over 10 times above the global average, lightning could have rivalled abiotic pyrite oxidation by Archean O2 levels. The lightning contribution would have been highest during time periods with elevated CO2(g), which makes it a potentially important contributor to local release of sulphur, iron, and bio-essential micronutrients on prebiotic land surfaces or on other planets with anoxic CO2-rich atmospheres.

阿基坦大气条件下雷电驱动的黄铁矿氧化。
氧化风化作用是当今地球上生物必需微量营养元素的一个主要来源;然而,在大气中氧气(g)水平非常低的早期地球或火星上,这种通量会被削弱。在这里,我们探讨了这样一个假设:在缺氧的大气中,闪电产生的氮氧化物可能会在其他缺氧条件下提高黄铁矿的氧化水平。我们在黄铁矿粉末和三种不同气体混合物(包括 80% N2(g) 与 20% CO2(g)、95% N2(g) 与 5% CO2(g)以及现代空气)的存在下进行了火花放电实验。实验进行了 30 分钟,我们跟踪了氮氧化物(g)、溶解硝酸盐和亚硝酸盐、pH 值、溶解硫酸盐和总溶解铁的产生情况。我们的结果表明,随着 CO2(g)和 O2(g)含量的增加,氮氧化物的生成量也在增加,这与之前的研究结果一致。溶解的铁和硫酸盐也在增加,这表明氮氧化物能够非生物地氧化黄铁矿。将这些数据推断到全球条件表明,在早期地球上,这种机制在全球范围内可能是微不足道的;然而,在雷暴多发地区,如现代热带地区,当地的闪电率可能比全球平均水平高出 10 倍以上,闪电对黄铁矿的非生物氧化作用可以与阿歇安时期的氧气水平相媲美。在二氧化碳(g)升高的时期,闪电的作用最大,这使得闪电可能成为前生物陆地表面或其他富含缺氧二氧化碳大气的行星上局部释放硫、铁和生物必需微量元素的重要因素。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Astrobiology
Astrobiology 生物-地球科学综合
CiteScore
7.70
自引率
11.90%
发文量
100
审稿时长
3 months
期刊介绍: Astrobiology is the most-cited peer-reviewed journal dedicated to the understanding of life''s origin, evolution, and distribution in the universe, with a focus on new findings and discoveries from interplanetary exploration and laboratory research. Astrobiology coverage includes: Astrophysics; Astropaleontology; Astroplanets; Bioastronomy; Cosmochemistry; Ecogenomics; Exobiology; Extremophiles; Geomicrobiology; Gravitational biology; Life detection technology; Meteoritics; Planetary geoscience; Planetary protection; Prebiotic chemistry; Space exploration technology; Terraforming
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