Meteorite Flux to Earth in the Early Cretaceous As Reconstructed from Sediment-Dispersed Extraterrestrial Spinels
Meteorite flux to Earth in the Early Cretaceous as reconstructed from sediment-dispersed extraterrestrial spinels Birger Schmitz1,2*, Philipp R. Heck2, Walter Alvarez3,4, Noriko T. Kita5, Surya S. Rout2, Anders Cronholm1, Céline Defouilloy5, Ellinor Martin1, Jan Smit4,6, and Fredrik Terfelt1 1Astrogeobiology Laboratory, Department of Physics, Lund University, SE-22100 Lund, Sweden 2Robert A. Pritzker Center for Meteoritics and Polar Studies, The Field Museum of Natural History, Chicago, Illinois 60605, USA 3Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA 4Osservatorio Geologico di Coldigioco, Contrada Coldigioco 4, 62021 Apiro, Italy 5WiscSIMS, Department of Geoscience, University of Wisconsin–Madison, Madison, Wisconsin 53706, USA 6Department of Sedimentary Geology, Vrije Universiteit, 1081 HV Amsterdam, Netherlands ABSTRACT to 470 ± 6 Ma (Korochantseva et al., 2007), but the most precise relative We show that Earth’s sedimentary strata can provide a record of date is given by an abrupt two-orders-of magnitude increase worldwide the collisional evolution of the asteroid belt. From 1652 kg of pelagic in sand-sized L-chondritic chromite grains in mid-Ordovician sediments Maiolica limestone of Berriasian–Hauterivian age from Italy, we (Schmitz et al., 2003; Heck et al., 2016). recovered 108 extraterrestrial spinel grains (32–250 μm) represent- By dissolving 100-kg-sized samples of condensed sediments from ing relict minerals from coarse micrometeorites. Elemental and three different time periods in various acids, the highly refractory extraterres- oxygen isotope analyses were used to characterize the grains, provid- trial spinel minerals can be concentrated. The recovered grains typically ing a first-order estimate of the major types of asteroids delivering contain high concentrations of solar-wind noble gases, indicating that material at the time.
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