A Microbial Link to Weathering of Postglacial Rocks and Sediments, Mount Viso Area, Western Alps, Demonstrated through Analysis of a Soil/Paleosol Bio/Chronosequence

作者:Mahaney W C; Somelar Peeter; Dirszowsky Randy W; Kelleher Brian; Pentlavalli Prasanna; McLaughlin Shane; Kulakova Anna N; Jordan Sean; Pulleyblank Coren; West Allen; Allen Christopher C R
来源:Journal of Geology, 2016, 124(2): 149-169.
DOI:10.1086/684442

摘要

Understanding the mechanism associated with rates of weathering and evolution of rockssedimentsoilpaleosol in alpine environments raises questions related to the impact of microbial mediation versus various diverse abiotic chemical/physical processes, even including the overall effect of cosmic impact/airburst during the early stage of weathering in Late Glacial (LG) deposits. This study is of a chronosequence of soils/paleosols, with an age range that spans the post-Little Ice Age (post-LIA; <150 yr), the Little Ice Age (LIA; AD 1500-1850), the middle Neoglacial (approximate to 3 ka)-Younger Dryas (YD; <12.8 ka), and the LG (<15 ka). The goal is to elicit trends in weathering, soil morphogenesis, and related eubacterial population changes over the past 13-15 k.yr. The older LG/YD paleosols in the sequence represent soil morphogenesis that started during the closing stage of Pleistocene glaciation. These are compared with undated soils of mid- to late Neoglacial age, the youngest of LIA and post-LIA age. All profiles formed in a uniform parent material of metabasalt composition and in moraine, rockfall, protalus, and alluvial fan deposits. Elsewhere in Europe, North America, and Asia, the cosmic impact/airburst event at 12.8 ka often produced a distinctive, carbon-rich black mat layer that shows evidence of high-temperature melting. At this alpine site, older profiles of similar LG age contain scorched and melted surface sediments that are otherwise similar in composition to the youngest/thinnest profiles developing in the catchment today. Moreover, microbial analysis of the sediments offers new insight into the genesis of these sediments: the C and Cu (u = unweathered) horizons in LG profiles present at 12.8 ka (now Ah/Bw) show bacterial population structures that differ markedly from recent alluvial/protalus sample bacterial populations. We propose here that these differences are, in part, a direct consequence of the age/cosmic impact/weathering processes that have occurred in the chronosequence. Of the several questions that emerge from these sequences, perhaps the most important involve the interaction of biotic-mineral factors, which need to be understood if we are to generally fully appreciate the role played by microbes in rock weathering.

  • 出版日期2016-3