Coordinated U-Pb and microtexture characterization of zircon and reidite in Chicxulub ejecta deposits, Raton Basin, USA

1Jennifer R. Davis, 1Carolyn A. Crow, 2Timmons M. Erickson, 1Jeffrey Benowitz
Earth and Planetary Science Letters, 698, 120443
Open Source Link to Article [DOI: 10.1016/j.epsl.2026.120443]

1Department of Earth Science, University of Colorado Boulder, 2200 Colorado Ave, Boulder, CO 80309, USA
2Amentum-JETS II, NASA Johnson Space Center, Houston, TX 77058, USA
Copyright Elsevier

Dating meteorite impact structures is confounded by shock-temperature heterogeneity and potential long-lived (>106 years) post-event hydrothermal systems. Meteorite-impact airfall ejecta may provide independent material for corroborating an impact age or establishing a primary impact event age. However, dating ejecta deposits may be complicated by the presence of detrital and/or unreset target-rock material. Post-depositional heating and fluid flow may further disturb isotopic systems. To further our ability to date ejecta material, here we present the results of a test-of-concept, coordinated microstructural (using electron backscatter diffraction [EBSD]; Nzircon=217) and in-situ U-Pb geochronology (via secondary ion mass spectrometry [SIMS]; Nspots=116 on 92 zircons) survey of ZrSiO4 from Chicxulub ejecta in the Raton Basin of southern Colorado and northern New Mexico (USA). Seventy-three ZrSiO₄ grains were identified as Chicxulub-derived based on the presence of mechanical microtwins, reidite, granular recrystallization, and/or FRIGN (former reidite in granular neoblastic) zircon microtextures, of which 42 were selected for geochronology. U-Pb spots (N = 12) on only partially granular grains were generally older (>230 Ma) than spots on fully granular grains (N = 38). ∼75% of the Chicxulub grains that experienced ≥90% Pb loss contained FRIGN zircon domains. Our results suggest that a microstructural survey of zircons and targeted in-situ geochronology of fully granular zircons with FRIGN domains is a viable method for determining the age of an impact event from distal ejecta materials. Furthermore, a compilation of paired ejecta-crater (N = 11) dates demonstrates overlap, and such dual dating should be considered best practice for dating meteorite impact events when both materials are present.

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