TY - JOUR
T1 - Disentangling global geochemical signals from local diagenetic alteration in shallow-water marine carbonates during OAE1a
AU - Nadeau, Matthew D.
AU - Murphy, Jack G.
AU - Hagen, Cedric J.
AU - Wu, Ziman
AU - Akhtar, Alliya A.
AU - Ahm, Anne Sofie
AU - Stolper, Daniel A.
AU - Maloof, Adam C.
AU - Higgins, John Andrew
N1 - Publisher Copyright:
© 2025
PY - 2025/9/15
Y1 - 2025/9/15
N2 - Shallow-water marine carbonates are widely used to reconstruct short-lived (∼ million years) perturbations to global geochemical cycles (e.g., carbon, calcium, strontium, and lithium). However, local environmental phenomena like meteoric and marine diagenetic alteration or changes in carbonate facies often decouple carbonate geochemistry from open-ocean seawater chemistry. To accurately reconstruct global geochemical cycles using shallow-water carbonates, it is therefor crucial to separate signals of local environmental phenomena from genuine changes in open-ocean seawater chemistry. The well-documented shallow-water carbonate succession from Ocean Drilling Program Site 866A (Resolution Guyot, Mid-Pacific Mountains) offers an opportunity to disentangle global and local signals recorded in shallow-water carbonates during the Early Cretaceous oceanic anoxic event 1a (OAE1a), a brief, globally correlative perturbation to the carbon cycle. Recent studies at this site have documented a δ13C excursion, a modest decline in 87Sr/86Sr, and large stratigraphic variability in δ7Li and δ44Ca values, all of which have been interpreted as reflecting temporal changes in the chemical composition of open-ocean seawater associated with OAE1a. However, other work at this site demonstrates clear evidence of meteoric and marine diagenesis as well as changes in carbonate facies across the OAE1a interval. Here, we aim to disentagle signals that reflect global geochemical cycling from those that reflect local environmental phenomena by employing a suite of carbonate-bound geochemical proxies (δ7Li, δ13C, δ18Ocarb, δ26Mg, δ44Ca, Δ47, [Mg], [Ca], [Sr], [Li]) and a numerical model of carbonate diagenesis. We show that while changes in 87Sr/86Sr ratios at this site reflect changes in primary seawater composition, stratigraphic variability in other geochemical systems (e.g., δ7Li, δ26Mg and δ44Ca values and trace element concentrations) arises primarily from early marine and meteoric diagenesis, with some contamination of Li from co-occurring clays. With much of the chemostratigraphic variability preserved today conceivably owing its origin to carbonate diagenesis and in recognition of the residence times for these elements in seawater (>1 million years) being longer than the short-lived OAE1a event, we make a case that our model-derived “snapshot” estimate for the calcium, magnesium, and lithium isotope composition of the marine diagenetic fluid reflects a stable open-ocean Early Cretaceous seawater signature. Although a global δ13C signal may still be present, our findings show how the stratigraphic record of δ13C values across the OAE1a at this site is a complex function of marine and meteoric diagenesis and changes in carbonate facies.
AB - Shallow-water marine carbonates are widely used to reconstruct short-lived (∼ million years) perturbations to global geochemical cycles (e.g., carbon, calcium, strontium, and lithium). However, local environmental phenomena like meteoric and marine diagenetic alteration or changes in carbonate facies often decouple carbonate geochemistry from open-ocean seawater chemistry. To accurately reconstruct global geochemical cycles using shallow-water carbonates, it is therefor crucial to separate signals of local environmental phenomena from genuine changes in open-ocean seawater chemistry. The well-documented shallow-water carbonate succession from Ocean Drilling Program Site 866A (Resolution Guyot, Mid-Pacific Mountains) offers an opportunity to disentangle global and local signals recorded in shallow-water carbonates during the Early Cretaceous oceanic anoxic event 1a (OAE1a), a brief, globally correlative perturbation to the carbon cycle. Recent studies at this site have documented a δ13C excursion, a modest decline in 87Sr/86Sr, and large stratigraphic variability in δ7Li and δ44Ca values, all of which have been interpreted as reflecting temporal changes in the chemical composition of open-ocean seawater associated with OAE1a. However, other work at this site demonstrates clear evidence of meteoric and marine diagenesis as well as changes in carbonate facies across the OAE1a interval. Here, we aim to disentagle signals that reflect global geochemical cycling from those that reflect local environmental phenomena by employing a suite of carbonate-bound geochemical proxies (δ7Li, δ13C, δ18Ocarb, δ26Mg, δ44Ca, Δ47, [Mg], [Ca], [Sr], [Li]) and a numerical model of carbonate diagenesis. We show that while changes in 87Sr/86Sr ratios at this site reflect changes in primary seawater composition, stratigraphic variability in other geochemical systems (e.g., δ7Li, δ26Mg and δ44Ca values and trace element concentrations) arises primarily from early marine and meteoric diagenesis, with some contamination of Li from co-occurring clays. With much of the chemostratigraphic variability preserved today conceivably owing its origin to carbonate diagenesis and in recognition of the residence times for these elements in seawater (>1 million years) being longer than the short-lived OAE1a event, we make a case that our model-derived “snapshot” estimate for the calcium, magnesium, and lithium isotope composition of the marine diagenetic fluid reflects a stable open-ocean Early Cretaceous seawater signature. Although a global δ13C signal may still be present, our findings show how the stratigraphic record of δ13C values across the OAE1a at this site is a complex function of marine and meteoric diagenesis and changes in carbonate facies.
KW - Diagenesis
KW - Dolomite
KW - Geochemistry
KW - Limestone
KW - Oae1a
KW - Paleoclimate
KW - Seawater chemistry
KW - Stable isotopes
UR - https://www.scopus.com/pages/publications/105008441067
UR - https://www.scopus.com/inward/citedby.url?scp=105008441067&partnerID=8YFLogxK
U2 - 10.1016/j.epsl.2025.119513
DO - 10.1016/j.epsl.2025.119513
M3 - Article
AN - SCOPUS:105008441067
SN - 0012-821X
VL - 666
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
M1 - 119513
ER -