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.2021 Apr 6;118(14):e2007797118.
doi: 10.1073/pnas.2007797118.

Reconciling early Deccan Traps CO2 outgassing and pre-KPB global climate

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Reconciling early Deccan Traps CO2 outgassing and pre-KPB global climate

Andres Hernandez Nava et al. Proc Natl Acad Sci U S A..

Abstract

A 2 to 4 °C warming episode, known as the Latest Maastrichtian warming event (LMWE), preceded the Cretaceous-Paleogene boundary (KPB) mass extinction at 66.05 ± 0.08 Ma and has been linked with the onset of voluminous Deccan Traps volcanism. Here, we use direct measurements of melt-inclusion CO2 concentrations and trace-element proxies for CO2 to test the hypothesis that early Deccan magmatism triggered this warming interval. We report CO2 concentrations from NanoSIMS and Raman spectroscopic analyses of melt-inclusion glass and vapor bubbles hosted in magnesian olivines from pre-KPB Deccan primitive basalts. Reconstructed melt-inclusion CO2 concentrations range up to 0.23 to 1.2 wt% CO2 for lavas from the Saurashtra Peninsula and the Thakurvadi Formation in the Western Ghats region. Trace-element proxies for CO2 concentration (Ba and Nb) yield estimates of initial melt concentrations of 0.4 to 1.3 wt% CO2 prior to degassing. Our data imply carbon saturation and degassing of Deccan magmas initiated at high pressures near the Moho or in the lower crust. Furthermore, we find that the earliest Deccan magmas were more CO2 rich, which we hypothesize facilitated more efficient flushing and outgassing from intrusive magmas. Based on carbon cycle modeling and estimates of preserved lava volumes for pre-KPB lavas, we find that volcanic CO2 outgassing alone remains insufficient to account for the magnitude of the observed latest Maastrichtian warming. However, accounting for intrusive outgassing can reconcile early carbon-rich Deccan Traps outgassing with observed changes in climate and atmospheric pCO2.

Keywords: Deccan Traps; carbon release; end-Cretaceous; magmatic outgassing; paleoclimate.

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Conflict of interest statement

The authors declare no competing interest.

Figures

Fig. 1.
Fig. 1.
Map showing the location and extent of Deccan Traps volcanism, including the Saurashtra region. The stratigraphic column shows Deccan formations and the position of melt inclusion samples in this study. The stratigraphic relationship between the Saurashtra region and the Main Deccan Traps section is uncertain, but the earliest Saurashtra lavas are thought to predate the main Deccan Basalt Group (21).
Fig. 2.
Fig. 2.
Representative Raman spectrum for CO2 showing the Fermi diad peaks that are located at 1,284.62 and 1,387.78 cm−1 in this example. The spacing between the two CO2 peaks,Δ, is used to calculate the density of CO2 in the bubble (68). The complete Raman spectrum of a melt inclusion (B4_SB_g9_MI11) along with the Ne lines that are used to calibrate the CO2 peak positions (A), and the corresponding glassy, bubble-bearing melt inclusion is shown in inset (B).
Fig. 3.
Fig. 3.
CO2 degassing trends for Deccan melt inclusions. The CO2 lost to degassing at the time of melt inclusion entrapment is calculated as the difference between initial CO2 based on Ba concentrations in each inclusion versus the reconstructed CO2 concentration. Some melt inclusions lack trace-element data. For these inclusions, we used the mean Ba concentration in melt inclusions from that unit. We used VolatileCalc (47) to determine the saturation pressure of each melt inclusion (see text for details). (A) Melt inclusion data from the Thakurvadi Formation in the Western Ghats region. (B) Melt inclusion data from the Saurashtra region. (C) Saurashtra and Thakurvadi CO2 versus Ba and (D) CO2 versus Nb, compared with CO2/Ba and CO2/Nb ratios from refs. , , , .
Fig. 4.
Fig. 4.
Evolving CO2 budgets for early Deccan Traps magmas and implications for latest Cretaceous climate. (A) CO2 concentrations of Deccan melt inclusions and initial CO2 concentrations based on trace element proxies from melt inclusion and whole-rock data, assuming CO2/Ba = 48.3 and CO2/Nb = 391 (38). Whole-rock trace element data from the Western Ghats region are from ref. . (B) Magnetostratigraphy from ref. . (C) The mean extrusive flux for each formation, calculated using the volumes estimated by ref. and the age model of ref. . The duration of volcanism in the Saurashtra region is uncertain. (D) A comparison of observed changes in latest Maastrichtian climate with changes modeled with LOSCAR. Ocean temperatures are from a benthicδ18O record from Integrated Ocean Drilling Program site 1262 on Walvis Ridge (18). LOSCAR results are shown for an I:E ratio of 0:1 (white) or 5:1 (blue shading), where the range reflects a climate sensitivity from 3 to 6 °C per doubling of CO2 (75). Results are shown for lower and higher CO2/Ba ratios (37, 38). SeeMaterials and Methods andSI Appendix for details of LOSCAR modeling.
Fig. 5.
Fig. 5.
A schematic showing CO2 evolution from early (Left) to late (Right) Deccan based on initial CO2 from trace elements and CO2 saturation pressures. We hypothesize that declining initial CO2 contents result from an expanding melting column and that higher initial CO2 in the earliest Deccan magmas facilitated more efficient flushing and thus degassing of intrusive magmas. Adapted from ref. , with permission from Elsevier.
Fig. 6.
Fig. 6.
Cumulative Deccan carbon release for a range of I:E magma-emplacement ratios. (A) Cumulative carbon contribution based on mean melt inclusion Ba concentrations from Saurashtra and Thakurvadi lavas, melt inclusions from the Wai subgroup from ref. , and whole-rock Ba data from the remaining formations from ref. . These calculations assume CO2/Ba = 48.3 (38). Increasing the assumed CO2/Ba ratio would increase carbon release estimates proportionally. SeeSI Appendix, Table S1 for details of calculations. Estimates of (B) extrusive carbon release and (C) intrusive plus extrusive carbon release from the Deccan Traps from this study compared with estimates from the Siberian Traps (55), the North Atlantic Igneous Province (55), and the Central Atlantic Magmatic Province (33). (D) The estimated carbon release per cubic kilometer of magma, assuming CO2/Ba = 48.3 (38).
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