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Discovery of enigmatic toroidal carbonate concretions on the Rio Grande Rise (Southwestern Atlantic Ocean)

Millo, Christian; Vieira do Nascimento e Silva, Matheus H.; de Mello, Renata Moura; Leckie, R. Mark; Benites, Mariana; Fonseca Giannini, Paulo C.; Boggiani, Paulo C.; Bosence, Dan; Lusty, Paul A.J.; Murton, Bramley J. ORCID: https://orcid.org/0000-0003-1522-1191; Jovane, Luigi. 2022 Discovery of enigmatic toroidal carbonate concretions on the Rio Grande Rise (Southwestern Atlantic Ocean). Marine Geology, 443, 106665. 10.1016/j.margeo.2021.106665

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Abstract/Summary

We present enigmatic toroidal carbonate concretions retrieved from 700 m water depth from two sites in the upper plateau of the Rio Grande Rise. The concretions have a diameter of ~15 cm and a central hole of ~5 cm, and were observed on top of loose bioclastic sand over an area of ~30 m2 at 0.5–1.5 m from one another. They consist of brown, porous, bioclastic grainstone, lacking internal structures. Grains consist of sand (< 3% coarse, 30% medium, 35% fine, 25% very fine), composed mainly by planktonic foraminiferal tests, and < 10% lime mud. The observed foraminiferal species indicate initial deposition of the sand in an open ocean setting. Biostratigraphy suggests an age no older than Pleistocene. Petrographic thin sections and SEM reveal that the fossiliferous grainstone contains intraclastic micritic cement and isopachous rim cement made of bladed magnesian calcite. δ18O values range from +1.5 to +3.3‰ (V-PDB) and increase with the degree of cementation, while δ13C ranges from +0.5 to +2.3‰ irrespective of cementation. The cementation of the grainstones is likely to have taken place in the marine phreatic environment. Carbonate precipitation induced by methane oxidation or (subaerial) meteoric diagenesis are ruled out based on both cement fabric and isotopic composition. Plausible causes for the toroidal shape of these structures could be: 1) sediment excavation by organisms, or 2) cementation within biofilms around burrows, followed by selective seafloor erosion. However, unveiling the actual formation mechanisms warrants further investigation.

Item Type: Publication - Article
Digital Object Identifier (DOI): 10.1016/j.margeo.2021.106665
ISSN: 00253227
Date made live: 17 Jan 2022 15:11 +0 (UTC)
URI: https://nora.nerc.ac.uk/id/eprint/531768

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