Experimental evidence that ooid size reflects a dynamic equilibrium between rapid precipitation and abrasion rates
Abstract
Ooids are enigmatic concentrically coated carbonate sand grains that reflect a fundamental mode of carbonate sedimentation and inorganic product of the carbon cycle—trends in their composition and size are thought to record changes in seawater chemistry over Earth history. Substantial debate persists concerning the roles of physical, chemical, and microbial processes in their growth, including whether carbonate precipitation on ooid surfaces is driven by seawater chemistry or microbial activity, and what role—if any—sediment transport and abrasion play. To test these ideas, we developed an approach to study ooids in the laboratory employing sediment transport stages and seawater chemistry similar to natural environments. Ooid abrasion and precipitation rates in the experiments were four orders of magnitude faster than radiocarbon net growth rates of natural ooids, implying that ooids approach a stable size representing a dynamic equilibrium between precipitation and abrasion. Results demonstrate that the physical environment is as important as seawater chemistry in controlling ooid growth and, more generally, that sediment transport plays a significant role in chemical sedimentary systems.
Additional Information
© 2017 Elsevier B.V. Received 16 January 2017, Revised 31 March 2017, Accepted 1 April 2017, Available online 20 April 2017. We thank Brian Fuller and Joel Scheingross for assistance with the abrasion mills. Particle size analysis was made in collaboration with Brandon McElroy, who also provided fantastic feedback. We thank John Grotzinger and Frank Corsetti for helpful discussions on this work. EJT acknowledges support from an Agouron Geobiology Postdoctoral Fellowship. This work was also supported by the Agouron Institute and an American Chemical Society Petroleum Research Fund Grant #56757-ND8 (to WWF). The data used are listed in the references, tables, and supplements.Attached Files
Supplemental Material - mmc1.pdf
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Additional details
- Eprint ID
- 76745
- DOI
- 10.1016/j.epsl.2017.04.004
- Resolver ID
- CaltechAUTHORS:20170420-073602236
- Agouron Institute
- 56757-ND8
- American Chemical Society Petroleum Research Fund
- Created
-
2017-04-27Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences