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dc.contributor.authorMacdonald, F. A.
dc.contributor.authorLahr, D. J. G.
dc.contributor.authorPruss, S. B.
dc.contributor.authorMoore, Kelsey Reed
dc.contributor.authorBosak, Tanja
dc.contributor.authorNewman, Sharon
dc.contributor.authorSettens, Charles M
dc.date.accessioned2018-12-18T15:15:24Z
dc.date.available2018-12-18T15:15:24Z
dc.date.issued2017-07
dc.identifier.issn14724677
dc.identifier.urihttp://hdl.handle.net/1721.1/119676
dc.description.abstractCryogenian cap carbonates that overlie Sturtian glacial deposits were formed during a post‐glacial transgression. Here, we describe microfossils from the Kakontwe Formation of Zambia and the Taishir Formation of Mongolia—both Cryogenian age, post‐Sturtian cap carbonates—and investigate processes involved in their formation and preservation. We compare microfossils from these two localities to an assemblage of well‐documented microfossils previously described in the post‐Sturtian Rasthof Formation of Namibia. Microfossils from both new localities have 10 ± 1 μm‐thick walls composed of carbonaceous matter and aluminosilicate minerals. Those found in the Kakontwe Formation are spherical or ovoid and 90 ± 5 μm to 200 ± 5 μm wide. Structures found in the Taishir Formation are mostly spherical, 50 ± 5 μm to 140 ± 5 μm wide, with distinct features such as blunt or concave edges. Chemical and mineralogical analyses show that the walled structures and the clay fraction extracted from the surrounding sediments are composed of clay minerals, especially muscovite and illite, as well as quartz, iron and titanium oxides, and some dolomite and feldspar. At each locality, the mineralogy of the microfossil walls matched that of the clay fractions of the surrounding sediment. The abundance of these minerals in the walled microfossils relative to the surrounding carbonate matrix and microbial laminae, and the presence of minerals that cannot precipitate from solution (titanium oxide and feldspar), suggests that the composition represents the original mineralogy of the structures. Furthermore, the consistency in mineralogy of both microfossils and sediments across the three basins, and the uniformity of size and shape among mineral grains in the fossil walls indicate that these organisms incorporated these minerals by primary biological agglutination. The discovery of new, mineral‐rich microfossil assemblages in microbially laminated and other fine‐grained facies of Cryogenian cap carbonates from multiple localities on different palaeocontinents demonstrates that agglutinating eukaryotes were widespread in carbonate‐dominated marine environments in the aftermath of the Sturtian glaciation. Keywords: microfossil, agglutinated, tests, Cryogenian, Sturtian, Kakontwe, Taishiren_US
dc.description.sponsorshipSmith College (Tomlinson Fund)en_US
dc.description.sponsorshipSmith College. Geosciences Departmenten_US
dc.description.sponsorshipNASA Astrobiology Instituteen_US
dc.language.isoen_US
dc.relation.isversionofhttps://doi.org/10.1111/gbi.12225en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourceProf. Bosak via Chris Sherratten_US
dc.titleBiologically agglutinated eukaryotic microfossil from Cryogenian cap carbonatesen_US
dc.typeArticleen_US
dc.identifier.citationMoore, K. R., T. Bosak, F. A. Macdonald, D. J. G. Lahr, S. Newman, C. Settens, and S. B. Pruss. “Biologically Agglutinated Eukaryotic Microfossil from Cryogenian Cap Carbonates.” Geobiology 15, no. 4 (January 6, 2017): 499–515.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Center for Materials Science and Engineeringen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.approverBosak, Tanjaen_US
dc.contributor.mitauthorMoore, Kelsey Reed
dc.contributor.mitauthorBosak, Tanja
dc.contributor.mitauthorNewman, Sharon
dc.contributor.mitauthorSettens, Charles M
dc.relation.journalGeobiologyen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsMoore, K. R.; Bosak, T.; Macdonald, F. A.; Lahr, D. J. G.; Newman, S.; Settens, C.; Pruss, S. B.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7332-4098
dc.identifier.orcidhttps://orcid.org/0000-0001-5179-5323
dc.identifier.orcidhttps://orcid.org/0000-0003-4664-308X
mit.licenseOPEN_ACCESS_POLICYen_US


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