The meteorite flux of the past 2 m.y. recorded in the atacama desert
- Others:
- Centre européen de recherche et d'enseignement des géosciences de l'environnement (CEREGE) ; Institut de Recherche pour le Développement (IRD)-Institut National de la Recherche Agronomique (INRA)-Aix Marseille Université (AMU)-Collège de France (CdF (institution))-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Laboratoire d'Astrophysique de Marseille (LAM) ; Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
- Lunar and Planetary Institute [Houston] (LPI)
- Sorbonne Universités (COMUE)
- COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)
- Université libre de Bruxelles (ULB)
- Geological Survey of Belgium
- SERNAGEOMIN ; Partenaires INRAE
- Millennium Institute of Astrophysics
- Museo del Meteorito ; Partenaires INRAE
- Programme National de Planetologie (PNP, Institut National des Sciences de l'Univers/Centre National des Etudes Spatiales [INSU/CNES]); Agence Nationale de la Recherche (project FRIPON) [ANR13-BS05-0009]; program "program "Investissements d'Avenir" [ANR-10-EQPX-20]; Chilean scientific agency Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT; FONDECYT) [3140562, 11171090]; European Research Council (ERC) Starting Grant (StG); Fund for Scientific Research (FRS-FNRS), BelgiumFonds de la Recherche Scientifique - FNRS
Description
The evolution of the meteorite flux to Earth can be studied by determining the terrestrial ages of meteorites collected in hot deserts. We measured the terrestrial ages of 54 stony meteorites from the El Medano area, in the Atacama Desert, Chile, using the cosmogenic nuclide Cl-36. With an average age of 710 ka, this collection is the oldest collection of nonfossil meteorites at Earth's surface. This allows both determination of the average meteorite flux intensity over the past 2 m.y. (222 meteorites larger than 10 g per km(2) per m.y.) and discussion of its possible compositional variability over the Quaternary Period. A change in the flux composition, with more abundant H chondrites, occurred between 1 and 0.5 Ma, possibly due to the direct delivery to Earth of a meteoroid swarm from the asteroid belt.
Abstract
International audience
Additional details
- URL
- https://hal.inrae.fr/hal-02627708
- URN
- urn:oai:HAL:hal-02627708v1
- Origin repository
- UNICA