Iridium and Spherules in Late Eocene Impact Deposits

Details Iridium and Spherules in Late Eocene Impact Deposits Iridium and Spherules in Late Eocene Impact Deposits

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1981k&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1981

Physics

2

Scientific paper

Global Ir in late Eocene impact deposits is about 9 ng/cm2,
sufficient to support a 6 km comet, capable of forming the Chesapeake
Bay or Popigai impact structures. The commonly collected impact
spherules (>63 microns) carry <1% of the total Ir.

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