|Title||Toward a High-Resolution Age Model for the Deccan Traps by U-PB Zircon Geochronology|
|Publication Type||Conference Paper|
|Year of Publication||2017|
|Authors||Schoene, B, Samperton, KMichael, Eddy, MP, Keller, G, Adatte, T, Khadri, SFR|
|Conference Name||Geological Society of America Annual Meeting|
|Publisher||Geological Society of America|
|Conference Location||Seattle, Washington|
|Other Numbers||Session No. 197-9, Abstract #305419|
Both the Chicxulub bolide impact and the Deccan Traps large igneous province have been implicated as contributing to the end-Cretaceous mass extinction. However, linking these events to the stratigraphic record of biotic and climatic change around the extinction, and assessing their potential effects, requires precise temporal constraints.. To better constrain the timing and tempo of Deccan Traps volcanism, we apply CA-TIMS U-Pb zircon geochronology, which can yield eruption ages at the ±20 kyr level.
Our results are consistent with recently published U-Pb and 40Ar/39Ar geochronological data that demonstrate the majority of Deccan Traps basalt erupted in ~700 kyr, beginning near the C30n/C29r magnetic reversal, ~250 kyr before the main extinction event. We find that while our data can be used to resolve the tempo and duration of magmatic activity from individual stratigraphic sections, uncertainties in stratigraphic correlation present a challenge to quantifying eruption rates. Therefore, despite the extensive number of excellent geologic studies thus far undertaken in the Deccan Traps, additional mapping, stratigraphy, geochemistry, and geochronology may be required before calculating robust volumetric eruptions rates is tenable. Such data are essential to test models that address the effect of Deccan eruptions on the biosphere and carbon cycle on 100 kyr timescales, and to test proposed linkages between the Deccan Traps, the end-Cretaceous extinction, and Chicxulub impact.