Cameron Vyllinniskii, Vance Derek, Archer Corey, House Christopher H
Department of Geosciences and Penn State Astrobiology Research Center, The Pennsylvania State University, University Park, PA 16802, USA.
Proc Natl Acad Sci U S A. 2009 Jul 7;106(27):10944-8. doi: 10.1073/pnas.0900726106. Epub 2009 Jun 24.
The new stable isotope systems of transition metals are increasingly used to understand and quantify the impact of primitive microbial metabolisms on the modern and ancient Earth. To date, little effort has been expended on nickel (Ni) isotopes but there are good reasons to believe that this system may be more straightforward, and useful in this respect, than some others. Here, we present Ni stable isotope data for abiotic terrestrial samples and pure cultures of methanogens. The dataset for rocks reveals little isotopic variability and provides a lithologic baseline for terrestrial Ni isotope studies. In contrast, methanogens assimilate the light isotopes, yielding residual media with a complementary heavy isotopic enrichment. Methanogenesis may have evolved during or before the Archean, when methane could have been key to Earth's early systems. Our data suggest significant potential in Ni stable isotopes for identifying and quantifying methanogenesis on the early planet. Additionally, Ni stable isotope fractionation may well prove to be the fundamental unambiguous trace metal biomarker for methanogens.
新的过渡金属稳定同位素体系越来越多地被用于理解和量化原始微生物代谢对现代和古代地球的影响。迄今为止,在镍(Ni)同位素方面投入的精力很少,但有充分理由相信,在这方面该体系可能比其他一些体系更直接、更有用。在此,我们展示了非生物陆地样品和产甲烷菌纯培养物的镍稳定同位素数据。岩石数据集显示出很少的同位素变化,并为陆地镍同位素研究提供了岩性基线。相比之下,产甲烷菌吸收轻同位素,产生具有互补重同位素富集的残余介质。甲烷生成可能在太古代期间或之前就已演化,当时甲烷可能是地球早期系统的关键。我们的数据表明镍稳定同位素在识别和量化早期行星上的甲烷生成方面具有巨大潜力。此外,镍稳定同位素分馏很可能被证明是产甲烷菌的基本明确的痕量金属生物标志物。