A Method to Determine the End of Impact-related Sedimentation at Marine-Target Craters: Geochemistry and Micropaleontology of the Transition from Resurge to Secular Deposits at the Lockne, Tvären, and Chesapeake Bay Impact Structures

Details A Method to Determine the End of Impact-related Sedimentation at Marine-Target Craters: Geochemistry and Micropaleontology of the Transition from Resurge to Secular Deposits at the Lockne, Tvären, and Chesapeake Bay Impact Structures A Method to Determine the End of Impact-related Sedimentation at Marine-Target Craters: Geochemistry and Micropaleontology of the Transition from Resurge to Secular Deposits at the Lockne, Tvären, and Chesapeake Bay Impact Structures

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1318o&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Computer Science

Scientific paper

Stable isotope and major element analysis is proving to be a necessary
complement to inadequate visual inspection for distinguishing the end of
impact-related sedimentation at marine-target craters.

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