4.4 Article

ACTIVE OOID GROWTH DRIVEN BY SEDIMENT TRANSPORT IN A HIGH-ENERGY SHOAL, LITTLE AMBERGRIS CAY, TURKS AND CAICOS ISLANDS

Journal

JOURNAL OF SEDIMENTARY RESEARCH
Volume 88, Issue 9, Pages 1132-1151

Publisher

SEPM-SOC SEDIMENTARY GEOLOGY
DOI: 10.2110/jsr.2018.59

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Funding

  1. Department of Environment and Coastal Resources (DECR), Ministry of Tourism, Environment, Heritage and Culture (MTEHC) of the Turks and Caicos Islands Government
  2. National Science Foundation (NSF) [OCE-1239667]
  3. Agouron Geobiology Postdoctoral Fellowship
  4. Marie Sklodowska-Curie Actions Programme
  5. Irish Research Council (ELEVATE Postdoctoral Fellowship) [ELEVATEPD/2014/47]
  6. National Aeronautics and Space Administration (NASA) Astrobiology Institute [NNA13AA90A]
  7. Agouron Institute
  8. American Chemical Society Petroleum Research Fund [56757-ND8]
  9. Irish Research Council (IRC) [ELEVATEPD/2014/47] Funding Source: Irish Research Council (IRC)

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Ooids are a common component of carbonate successions of all ages and present significant potential as paleoenvironmental proxies, if the mechanisms that control their formation and growth can be understood quantitatively. There are a number of hypotheses about the controls on ooid growth, each offering different ideas on where and how ooids accrete and what role, if any, sediment transport and abrasion might play. These hypotheses have not been well tested in the field, largely due to the inherent challenges of tracking individual grains over long timescales. This study presents a detailed field test of ooid-growth hypotheses on Little Ambergris Cay in the Turks and Caicos Islands, British Overseas Territories. This field site is characterized by westward net sediment transport from waves driven by persistent easterly trade winds. This configuration makes it possible to track changes in ooid properties along their transport path as a proxy for changes in time. Ooid size, shape, and radiocarbon age were compared along this path to determine in which environments ooids are growing or abrading. Ooid surface textures, petrographic fabrics, stable-isotope compositions (delta C-13, delta O-18, and delta S-34), lipid geochemistry, and genetic data were compared to characterize mechanisms of precipitation and degradation and to determine the relative contributions of abiotic (e.g., abiotic precipitation, physical abrasion) and biologically influenced processes (e.g., biologically mediated precipitation, fabric destruction through microbial microboring and micritization) to grain size and character. A convergence of evidence shows that active ooid growth occurs along the transport path in a high-energy shoal environment characterized by frequent suspended-load transport: median ooid size increases by more than 100 mu m and bulk radiocarbon ages decrease by 360 yr westward along the similar to 20 km length of the shoal crest. Lipid and 16S rRNA data highlight a spatial disconnect between the environments with the most extensive biofilm colonization and environments with active ooid growth. Stable-isotope compositions are indistinguishable among samples, and are consistent with abiotic precipitation of aragonite from seawater. Westward increases in ooid sphericity and the abundance of well-polished ooids illustrate that ooids experience subequal amounts of growth and abrasion-in favor of net growth-as they are transported along the shoal crest. Overall, these results demonstrate that, in the Ambergris system, the mechanism of ooid growth is dominantly abiotic and the loci of ooid growth is determined by both carbonate saturation and sediment transport mode. Microbes play a largely destructive, rather than constructive, role in ooid size and fabric.

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