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Published June 2017 | Supplemental Material + Published
Journal Article Open

Calibration of the B/Ca proxy in the planktic foraminifer Orbulina universa to Paleocene seawater conditions

Abstract

The B/Ca ratio of planktic foraminiferal calcite, a proxy for the surface ocean carbonate system, displays large negative excursions during the Paleocene-Eocene Thermal Maximum (PETM, 55.9 Ma), consistent with rapid ocean acidification at that time. However, the B/Ca excursion measured at the PETM exceeds a magnitude that modern pH calibrations can explain. Numerous other controls on the proxy have been suggested, including foraminiferal growth rate and the total concentration of dissolved inorganic carbon (DIC). Here we present new calibrations for B/Ca versus the combined effects of pH and DIC in the symbiont-bearing planktic foraminifer Orbulina universa, grown in culture solutions with simulated Paleocene seawater elemental composition (high [Ca], low [Mg], and low total boron concentration ([B]_T). We also investigate the isolated effects of low seawater [B]_T, high [Ca], reduced symbiont photosynthetic activity, and average shell growth rate on O. universa B/Ca in order to further understand the proxy systematics and to determine other possible influences on the PETM records. We find that average shell growth rate does not appear to determine B/Ca in high calcite saturation experiments. In addition, our "Paleocene" calibration shows higher sensitivity than the modern calibration at low [B(OH)_4−]/DIC. Given a large DIC pulse at the PETM, this amplification of the B/Ca response can more fully explain the PETM B/Ca excursion. However, further calibrations with other foraminifer species are needed to determine the range of foraminifer species-specific proxy sensitivities under these conditions for quantitative reconstruction of large carbon cycle perturbations.

Additional Information

© 2017 American Geophysical Union. Received 3 DEC 2016; Accepted 8 MAY 2017; Accepted article online 17 MAY 2017; Published online 17 JUN 2017. We thank Jordan Snyder, Alex Gagnon, Sam Phelps, Jennifer Fehrenbacher, Catherine Davis, and Ann Russell, who assisted in the collection of foraminifers, and Caroline Baptist and Nina Ruprecht for their laboratory assistance. Stella Woodard, Ryan Bu, and Paola Moffa-Sanchez provided assistance with ICP-MS analyses at Rutgers. We thank Richard Zeebe for access to LOSCAR model output. Special thanks to Bill Rosado, Govind Nadathur, and Orlando Espinosa for assistance in the lab and on the boat in Puerto Rico. We also thank Kat Allen, Jesse Farmer, Don Penman, and Sidney Hemming for their helpful discussion of the data. This manuscript was greatly improved by the constructive comments of Howie Spero, Michael Henehan, and one anonymous reviewer. This research is funded by NSF [OCE12-32987] to B.H. All data presented in this manuscript can be found in the main text and the supporting information.

Attached Files

Published - Haynes_et_al-2017-Paleoceanography.pdf

Supplemental Material - palo20418-sup-0001-Haynes_Supplement_S1.pdf

Supplemental Material - palo20418-sup-0002-Haynes_Supplemental_Table2.xlsx

Supplemental Material - palo20418-sup-0003-Haynes_Table_20S3_GrowthRate.xlsx

Supplemental Material - palo20418-sup-0004-Table_S6.xlsx

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Additional details

Created:
August 21, 2023
Modified:
October 26, 2023