Growing spherulitic calcite grains in saline, hyperalkaline lakes: Experimental evaluation of the effects of Mg-clays and organic acids

R. Mercedes-Martin, M. R. Rogerson, A. T. Brasier, H. B. Vonhof, T. J. Prior, S. M. Fellows, J. J. G. Reijmer, I. Billing, H. M. Pedley

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Abstract

The origin of spherical-radial calcite bodies – spherulites – in sublacustrine, hyperalkaline and saline systems is unclear, and therefore their palaeoenvironmental significance as allochems is disputed. Here, we experimentally investigate two hypotheses concerning the origin of spherulites. The first is that spherulites precipitate from solutions super-saturated with respect to magnesium-silicate clays, such as stevensite. The second is that spherulite precipitation happens in the presence of dissolved, organic acid molecules. In both cases, experiments were performed under sterile conditions using large batches of a synthetic and cell-free solution replicating waters found in hyperalkaline, saline lakes (such as Mono Lake, California). Our experimental results show that a highly alkaline and highly saline solution supersaturated with respect to calcite (control solution) will precipitate euhedral to subhedral rhombic and trigonal bladed calcite crystals. The same solution supersaturated with respect to stevensite precipitates sheet-like stevensite crystals rather than a gel, and calcite precipitation is reduced by ~ 50% compared to the control solution, producing a mixture of patchy prismatic subhedral to euhedral, and minor needle-like, calcite crystals. Enhanced magnesium concentration in solution is the likely cause of decreased volumes of calcite precipitation, as this raised equilibrium ion activity ratio in the solution. On the other hand, when alginic acid was present then the result was widespread development of micron-size calcium carbonate spherulite bodies. With further growth time, but falling supersaturation, these spherules fused into botryoidal-topped crusts made of micron-size fibro-radial calcite crystals. We conclude that the simplest tested mechanism to deposit significant spherical-radial calcite bodies is to begin with a strongly supersaturated solution that contains specific but environmentally-common organic acids. Furthermore, we found that this morphology is not a universal consequence of having organic acids dissolved in the solution, but rather spherulite development requires specific binding behaviour. Finally, we found that the location of calcite precipitation was altered from the air: water interface to the surface of the glassware when organic acids were present, implying that attached calcite precipitates reflect precipitation via metal–organic intermediaries, rather than direct forcing via gas exchange.
Original languageEnglish
Pages (from-to)93-102
Number of pages10
JournalSedimentary Geology
Volume335
Early online date15 Feb 2016
DOIs
Publication statusPublished - 15 Apr 2016

Bibliographical note

Acknowledgements
BP Exploration Co. is thanked for funding, and particularly the Carbonate Team (Anna Matthews, Teresa Sabato Ceraldi, and Darryl G. Green) for supporting this research and for fruitful discussions. Mark Anderson, Kim Rosewell, and Tony Sinclair (University of Hull) are thanked for laboratory assistance, and for SEM sample preparation and set-up respectively. The technical and human support from Prof. Jörg Hardege and Maggy A. Harley (University of Hull) was key to perform these experiments. We would like to acknowledge an anonymous reviewer for the detailed and constructive comments, and Brian Jones's editorial handling of the manuscript which is greatly appreciated.

Keywords

  • spherulite
  • hyperalkaline
  • stevensite
  • Mg-clays
  • organic acid
  • lacustrine

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