Madrigal-Trejo David, Baldes Matthew J, Tamura Nobumichi, Klepac-Ceraj Vanja, Bosak Tanja
Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA.
Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, California, USA.
Geobiology. 2025 May-Jun;23(3):e70024. doi: 10.1111/gbi.70024.
Carbonaceous particles that concentrate arsenic in microbialites as old as ~3.5 Ga are similar to As-rich organic globules in modern microbialites. The former particles have been interpreted as tracers of As cycling by early microbial metabolisms. However, it is unclear if arsenic accumulation is a consequence of biological activity or passive postmortem binding of arsenic by organic matter during diagenesis in volcanically influenced, As-rich environments. Here, we address this uncertainty by evaluating the concentrations, speciation, and detectability of As in active or heat-killed biofilms formed by cyanobacteria or anoxygenic photosynthetic microbes exposed to environmentally relevant concentrations of As(III) or As(V) (50 μM to 3 mM). The genomes or metagenomes of these biofilms contain genes involved in detoxifying or energy-yielding As metabolisms. Biomass accumulates As from the solution in a concentration-dependent manner and with a preference for oxidized As(V) over As(III). Autoclaved biomass accumulates As even more strongly than active biomass, likely because living biofilms actively detoxify As. Active biofilms oxidize and reduce As and accumulate both As(III) and As(V), whereas a small fraction of As(V) can be reduced in inactive biofilms that bind As during diagenesis. Arsenic enrichments in the biomass are detectable by X-ray based spectroscopy techniques (XRF, EPMA-WDS) that are commonly used to analyze geological materials. These findings enable the reconstruction of past active and passive interactions of microbial biomass with arsenic in fossilized microbial biofilms and microbialites from the early Earth.
在年龄达35亿年的微生物岩中富集砷的碳质颗粒,与现代微生物岩中富含砷的有机小球类似。前者颗粒被解释为早期微生物代谢过程中砷循环的追踪物。然而,尚不清楚砷的积累是生物活动的结果,还是在受火山影响、富含砷的环境中,成岩过程中砷被有机物被动地死后结合的结果。在这里,我们通过评估暴露于环境相关浓度的As(III)或As(V)(50 μM至3 mM)的蓝细菌或厌氧光合微生物形成的活性或热灭活生物膜中砷的浓度、形态和可检测性,来解决这一不确定性。这些生物膜的基因组或宏基因组包含参与砷解毒或产能量代谢的基因。生物量以浓度依赖的方式从溶液中积累砷,并且优先积累氧化态的As(V)而非As(III)。高压灭菌的生物量比活性生物量积累砷的能力更强,这可能是因为活的生物膜能主动解毒砷。活性生物膜能氧化和还原砷,并积累As(III)和As(V),而在成岩过程中结合砷的非活性生物膜中,一小部分As(V)可以被还原。通过常用于分析地质材料的基于X射线的光谱技术(XRF、EPMA-WDS)可以检测到生物量中的砷富集。这些发现有助于重建早期地球化石微生物生物膜和微生物岩中微生物生物量与砷过去的主动和被动相互作用。