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粗粒硅质碎屑沉积物中形成席状的蓝细菌的实验石化作用。

Experimental fossilization of mat-forming cyanobacteria in coarse-grained siliciclastic sediments.

作者信息

Newman S A, Klepac-Ceraj V, Mariotti G, Pruss S B, Watson N, Bosak T

机构信息

Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA.

Department of Biological Sciences, Wellesley College, Wellesley, MA, USA.

出版信息

Geobiology. 2017 Jul;15(4):484-498. doi: 10.1111/gbi.12229. Epub 2017 Feb 11.

Abstract

Microbial fossils and textures are commonly preserved in Ediacaran and early Cambrian coarse-grained siliciclastic sediments that were deposited in tidal and intertidal marine settings. In contrast, the fossilization of micro-organisms in similar marine environments of post-Cambrian age is less frequently reported. Thus, temporal discrepancies in microbial preservation may have resulted from the opening and closing of a unique taphonomic window during the terminal Proterozoic and early Phanerozoic, respectively. Here, we expand upon previous work to identify environmental factors which may have facilitated the preservation of cyanobacteria growing on siliciclastic sand, by experimentally determining the ability of microbial mats to trap small, suspended mineral grains, and precipitate minerals from ions in solution. We show that (i) fine grains coat the sheaths of filamentous cyanobacteria (e.g., Nodosilinea sp.) residing within the mat, after less than 1 week of cell growth under aerobic conditions, (ii) clay minerals do not coat sterile cellulose fibers and rarely coat unsheathed cyanobacterial cells (e.g., Nostoc sp.), (iii) stronger disturbances (where culture jars were agitated at 170 rpm; 3 mm orbital diameter) produce the smoothest and most extensive mineral veneers around cells, compared with those agitated at slower rotational speeds (150 and 0 rpm), and (iv) mineral veneers coating cyanobacterial cells are ~1 μm in width. These new findings suggest that sheathed filamentous cyanobacteria may be preferentially preserved under conditions of high fluid energy. We integrate these results into a mechanistic model that explains the preservation of microbial fossils and textures in Ediacaran sandstones and siltstones, and in fine-grained siliciclastic deposits that contain exceptionally preserved microbial mats.

摘要

微生物化石和纹理通常保存在埃迪卡拉纪和寒武纪早期的粗粒硅质碎屑沉积物中,这些沉积物沉积于潮汐和潮间带海洋环境。相比之下,寒武纪之后类似海洋环境中微生物的化石记录较少。因此,微生物保存的时间差异可能分别是由于元古宙末期和显生宙早期独特的埋藏学窗口的开启和关闭所致。在这里,我们在之前工作的基础上进行拓展,通过实验测定微生物垫捕获小的悬浮矿物颗粒以及从溶液中的离子沉淀矿物的能力,来确定可能促进硅质碎屑砂上生长的蓝细菌保存的环境因素。我们发现:(i)在有氧条件下细胞生长不到1周后,细颗粒覆盖了位于微生物垫内的丝状蓝细菌(如Nodosilinea属)的鞘;(ii)粘土矿物不会覆盖无菌纤维素纤维,也很少覆盖无鞘蓝细菌细胞(如念珠藻属);(iii)与以较慢转速(150和0转/分钟)搅拌的培养瓶相比,更强的扰动(培养瓶以170转/分钟搅拌;轨道直径3毫米)会在细胞周围产生最光滑、最广泛的矿物覆盖层;(iv)覆盖蓝细菌细胞的矿物覆盖层宽度约为1微米。这些新发现表明,有鞘丝状蓝细菌可能在高流体能量条件下被优先保存。我们将这些结果整合到一个机制模型中,该模型解释了埃迪卡拉纪砂岩和粉砂岩以及含有保存异常完好的微生物垫的细粒硅质碎屑沉积物中微生物化石和纹理的保存情况。

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