Logo image
No Cretaceous-Paleogene Boundary in Exposed Rajahmundry Traps: A Refined Chronology of the Longest Deccan Lava Flows From Ar-40/Ar-39 Dates, Magnetostratigraphy, and Biostratigraphy
Journal article   Open access

No Cretaceous-Paleogene Boundary in Exposed Rajahmundry Traps: A Refined Chronology of the Longest Deccan Lava Flows From Ar-40/Ar-39 Dates, Magnetostratigraphy, and Biostratigraphy

Isabel M. Fendley, Courtney J. Sprain, Paul R. Renne, Ignacio Arenillas, Jose A. Arz, Vicente Gilabert, Stephen Self, Loyc Vanderkluysen, Kanchan Pande, Jan Smit, …
Geochemistry, geophysics, geosystems : G3, v 21(9)
01 Sep 2020
url
https://doi.org/10.1029/2020gc009149View
Published, Version of Record (VoR)Maybe Open Access (Publisher Bronze) Open
url
https://doi.org/10.1029/2020GC009149View
Published, Version of Record (VoR) Open

Abstract

Geochemistry & Geophysics Physical Sciences Science & Technology
Deccan Traps flood basalt volcanism affected ecosystems spanning the end-Cretaceous mass extinction, with the most significant environmental effects hypothesized to be a consequence of the largest eruptions. The Rajahmundry Traps are the farthest exposures (similar to 1,000 km) of Deccan basalt from the putative eruptive centers in the Western Ghats and hence represent some of the largest volume Deccan eruptions. Although the three subaerial Rajahmundry lava flows have been geochemically correlated to the Wai Subgroup of the Deccan Traps, poor precision associated with previous radioisotopic age constraints has prevented detailed comparison with potential climate effects. In this study, we use new Ar-40/Ar-39 dates, paleomagnetic and volcanological analyses, and biostratigraphic constraints for the Rajahmundry lava flows to ascertain the timing and style of their emplacement. We find that the lower and middle flows (65.92 +/- 0.25 and 65.67 +/- 0.08 Ma, +/- 1 sigma systematic uncertainty) were erupted within magnetochron C29r and were a part of the Ambenali Formation of the Deccan Traps. By contrast, the uppermost flow (65.27 +/- 0.08 Ma) was erupted in C29n as part of the Mahabaleshwar Formation. Given these age constraints, the Rajahmundry flows were not involved in the end-Cretaceous extinction as previously hypothesized. To determine whether the emplacement of the Rajahmundry flows could have affected global climate, we estimated their eruptive CO2 release and corresponding climate change using scalings from the LOSCAR carbon cycle model. We find that the eruptive gas emissions of these flows were insufficient to directly cause multi-degree warming; hence, a causal relationship with significant climate warming requires additional Earth system feedbacks.

Metrics

19 Record Views
26 citations in Scopus

Details

UN Sustainable Development Goals (SDGs)

This publication has contributed to the advancement of the following goals:

#14 Life Below Water
#13 Climate Action

InCites Highlights

Data related to this publication, from InCites Benchmarking & Analytics tool:

Collaboration types
Domestic collaboration
International collaboration
Web of Science research areas
Geochemistry & Geophysics
Logo image