P/Ca in Carbonates as a Proxy for Alkalinity and Phosphate Levels
Abstract
Understanding mechanisms, rates, and drivers of past carbonate formation provides insight into the chemical evolution of Earth's oceans and atmosphere. We paired geological observations with elemental and isotope geochemistry to test potential proxies for calcium‐to‐alkalinity ratios (Ca:ALK). Across diverse carbonate facies from Pleistocene closed‐basin lakes in Owens Valley, CA, we observed less δ^(44/40)Ca variation than theoretically predicted (>0.75‰) for the very low Ca:ALK in these systems. Carbonate clumped isotope disequilibria implied rapid carbonate growth—kinetic isotope effects, combined with the diverse carbonate minerals present, complicated the interpretation of δ^(44/40)Ca as a paleoalkalinity proxy. In contrast, we observed that the high phosphate concentrations are recorded by shoreline and lake bottom carbonates formed in 11 Pleistocene lakes at orders of magnitude greater concentrations than in marine carbonates. Because the maximum phosphate content of water depends on Ca:ALK, we propose that carbonate P/Ca can inform phosphate levels and thereby Ca:ALK of aqueous environments in the carbonate record.
Additional Information
© 2020 American Geophysical Union. Issue Online: 30 October 2020; Version of Record online: 30 October 2020; Accepted manuscript online: 19 October 2020; Manuscript accepted: 14 October 2020; Manuscript revised: 07 October 2020; Manuscript received: 09 May 2020. The authors would like to thank Christine Chen, Adam Hudson, Dan Ibarra, Max Lloyd, and Theodore Present for contributing sample material from other paleolakes and marine carbonates, two anonymous reviewers for greatly improving this manuscript, and the International Geobiology Course (supported by the Agouron Institute, Simons Foundation, NASA, and Caltech) for access to Mono Lake sediment cores. Funding for the work was provided by the Simons Foundation Collaboration on the Origins of Life (WWF) and Barr Foundation Postdoctoral Fellowship to M. I. Data Availability Statement: Supporting information detailing methods and all data may be found in the supporting information and were archived in the Open Science Framework (https://doi.org/10.17605/OSF.iO/N9Y3H). Samples collected as a part of this study were registered with IGSNs, listed in Table S1.Attached Files
Published - 2020GL088804.pdf
Submitted - essoar.10503082.1.pdf
Supplemental Material - grl61403-sup-0001-2020gl088804-si.docx
Supplemental Material - grl61403-sup-0002-2020gl088804-ts01.xlsx
Supplemental Material - grl61403-sup-0003-2020gl088804-ts02.xlsx
Supplemental Material - grl61403-sup-0004-2020gl088804-ts03.xlsx
Supplemental Material - grl61403-sup-0005-2020gl088804-ts04.xlsx
Supplemental Material - grl61403-sup-0006-2020gl088804-ds01.xlsx
Supplemental Material - grl61403-sup-0007-2020gl088804-ds02.xlsx
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Additional details
- Eprint ID
- 106182
- Resolver ID
- CaltechAUTHORS:20201021-084310520
- Agouron Institute
- Simons Foundation
- NASA
- Caltech
- Barr Foundation
- Created
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2020-10-21Created from EPrint's datestamp field
- Updated
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2023-06-01Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)