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      The meteorite flux of the last 2 Myr recorded in the Atacama desert

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          Abstract

          The evolution of the meteorite flux to the Earth can be studied by determining the terrestrial ages of meteorite collected in hot deserts. We have measured the terrestrial ages of 54 stony meteorites from the El M\'edano area, in the Atacama Desert, using the cosmogenic nuclide chlorine 36. With an average age of 710 ka, this collection is the oldest collection of non fossil meteorites at the Earth's surface. This allows both determining the average meteorite flux intensity over the last 2 Myr (222 meteorites larger than 10 g per km2 per Myr) and discussing its possible compositional variability over the Quaternary period. A change in the flux composition, with more abundant H chondrites, occurred between 0.5 and 1 Ma, possibly due to the direct delivery to Earth of a meteoroid swarm from the asteroid belt.

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          Most cited references10

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          Catch a Falling Star: Meteorites and Old Ice

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            Dynamical Evolution of Main Belt Meteoroids: Numerical Simulations Incorporating Planetary Perturbations and Yarkovsky Thermal Forces

            W Bottke (2000)
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              Climate and rock weathering: a study of terrestrial age dated ordinary chondritic meteorites from hot desert regions

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                Author and article information

                Journal
                29 April 2019
                Article
                1904.12644
                4c2b4908-c8de-4927-a432-9c8cb2aadd06

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                accepted in Geology
                astro-ph.EP

                Planetary astrophysics
                Planetary astrophysics

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