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dc.contributor.authorNoffke, Nora-
dc.contributor.authorBeraldi-Campesi, Hugo-
dc.contributor.authorCallefo, Flavia-
dc.contributor.authorCarmona, Noelia Beatriz-
dc.contributor.authorCuadrado, Diana G.-
dc.contributor.authorHickman-Lewis, Keyron-
dc.contributor.authorHomann, Martin-
dc.contributor.authorMitchell, Ria-
dc.contributor.authorSheldon, Nathan-
dc.contributor.authorWestall, Francis-
dc.contributor.authorXiao, Shuhai-
dc.date.accessioned2022-09-08T14:53:16Z-
dc.date.available2022-09-08T14:53:16Z-
dc.date.issued2022-
dc.identifier.citationNoffke, N., Beraldi-Campesi, H., Callefo, F., Carmona, N., Cuadrado, D. G., Hickman- Lewis, K., Homann, M., Mitchell, R., Sheldon, N., Westall, F., & Xiao, S. (2022). Treatise Online no.162: Part B, Volume 2, Chapter 5: Microbially induced sedimentary structures (MISS). Treatise Online; 162; 1-29es_ES
dc.identifier.isbn2153-4012es_ES
dc.identifier.otherhttps://journals.ku.edu/treatiseonline/article/view/18111es_ES
dc.identifier.urihttp://rid.unrn.edu.ar/handle/20.500.12049/9065-
dc.format.extentp. 1-29es_ES
dc.language.isoenes_ES
dc.publisherPaleontological Institute- University of Kansases_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.titlePART B, VOLUME 2, CHAPTER 5: MICROBIALLY INDUCED SEDIMENTARY STRUCTURES (MISS)es_ES
dc.typeParte de libroes_ES
dc.rights.licenseCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-ND 4.0)-
dc.description.filiationNoffke, Nora. Old Dominion University, Department of Ocean, Earth and Atmospheric Sciences, Norfolk, Virginia 23529, USAes_ES
dc.description.filiationBeraldi-Campesi, Hugo. SOMA, Universidad Naciona l Autonoma de Mexico, Cuiadad Universitaria, 04510, CDMXes_ES
dc.description.filiationCallefo, Flavia. Brazilian Synchrotron Light Laboratory, Giuseppe Máximo Scolfaro Street, 10000, Campinas, 13083-100, Braziles_ES
dc.description.filiationCarmona, Noelia Beatriz. Universidad Nacional de Río Negro, Instituto de Investigación en Paleobiología y Geología, Río Negro, Argentina.es_ES
dc.description.filiationCuadrado, Diana. Instituto Argentino de Oceanografía (CONICET-UNS), Departamento de Geología (Universidad Nacional del Sur), Bahía Blanca B8000CPB, Buenos Aires, Argentinaes_ES
dc.description.filiationHickman-Lewis, Keyron. Department of Earth Sciences, The Natural History Museum, South Kensington, London, SW7 5BD, UKes_ES
dc.description.filiationHomann, Martin. University College London, Department of Earth Sciences, 5 Gower Place, London WC1E 6BS, UKes_ES
dc.description.filiationMitchell, Ria. 9 Sheffield Tomography Center, University of Sheffield, Sheffield, S3 7HQ, UKes_ES
dc.description.filiationSheldon, Nathan. Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109, USAes_ES
dc.description.filiationWestall, Francis. Centre de Biophysique Moleculaire, CNRS CBM, 45071 Orleans Cedex 2, Francees_ES
dc.description.filiationXiao, Shuhai. Virginia Tech, Department of Geosciences, Virginia Tech, Blacksburg, VA 24061, USAes_ES
dc.subject.keywordMicrobial Matses_ES
dc.subject.keywordSEDIMENTARY STRUCTURESes_ES
dc.type.versioninfo:eu-repo/semantics/publishedVersiones_ES
dc.subject.materiaCiencias Exactas y Naturaleses_ES
dc.origin.lugarDesarrolloUniversidad Nacional de Río Negroes_ES
dc.description.resumenTo date, microbialites include five groups: stromatolites, thrombolites, leiolites, and dendrolites. All these microbialites occur in carbonate or silica lithologies. However, research during the past 25 years has defined an additional group of microbialites that occurs predominantly in clastic deposits. These structures are called microbially induced sedimentary structures, commonly simply abbreviated to MISS. As outlined in this chapter, the morphologies of MISS do not resemble those of precipitated microbialites due to the much different formation and different location of these structural groups. The genesis of the main types of MISS has been elucidated in studies in modern environments. The results were key for the search of such structures in the fossil record. Systematic exploration from youngest to oldest stratigraphic successions has given rise to a data set that allows identification of MISS in respective paleoenvironments. MISS are biosignatures helpful to understanding aspects of prokaryote evolution and the search for life on other planets. This chapter first briefly focuses on the microbial communities that cause the structures, then discusses MISS formation, which is intimately related to the immediate setting. Next, the processes of their preservation is examined, and, finally, the chapter arrives at the classification of MISS.es_ES
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