LIP GAS EMISSION RATES: NEW METHODS USING HG CHEMOSTRATIGRAPHY AND IMPLICATIONS FOR ENVIRONMENTAL EFFECTS
Here, we use mercury (Hg) chemostratigraphy in sedimentary records along with Hg cycle box model scaling factors to understand the tempo of LIP gas emissions. We examine a few key Hg records per LIP which have good geochronological constraints and determine peak Hg enrichment factors, defined as multiples of background Hg values (explicitly considering co-variation with other geochemical parameters, e.g., TOC). As Hg reservoir timescales are short (<10 kyr between emission and deposition), these values likely reflect emissions from individual or closely spaced LIP eruptions. We compare these enrichment factors with scalings from a modern Hg cycle box model to estimate Hg emission fluxes, and then use volcanic Hg/C ratios to estimate CO2 fluxes. We ensure that all estimates are volcanologically reasonable: consistent with volcanological properties of LIP lavas, e.g., texture (as peak eruption rate cap), approximate total equivalent volume and geochronology.
We find that peak and average LIP CO2 emission rates significantly vary between LIPs: e.g., peak CO2 fluxes are 1 Pg/yr (Siberian Traps), 0.5 Pg/yr (Karoo/Ferrar), and 0.4ā0.5 Pg/yr (Deccan Traps). However, our average CO2 emissions are generally lower than those estimated by reproducing paleoenvironmental proxy records using carbon cycle models, suggesting a potentially key role for carbon cycle feedback processes. Our results highlight the differences in tempo of volatile release between different LIPs and consequently have strong implications for their potential environmental impacts.