EGU23-16700
https://doi.org/10.5194/egusphere-egu23-16700
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Linking enstatite meteorites to a unique source.

Chrysa Avdellidou1, Marco Delbo1, Alessandro Morbidelli1, Kevin Walsh2, Edhah Munaibari1,3, Jules Bourdelle de Micas4, Maxime Devogele5, Sonia Fornasier4,6, Matthieu Gounelle7, and Gerard van Belle8
Chrysa Avdellidou et al.
  • 1Observatoire de la Cote dAzur, Laboratoire Lagrange, Nice, France (chrysa.avdellidou@oca.eu)
  • 2Southwest Research Institute, 1050 Walnut St. Suite 300, Boulder, CO, 80302, USA
  • 3Université Côte d'Azur, CNRS-Geóazur, Observatoire de la Côte d'Azur, 250 rue Albert Einstein, Sophia Antipolis, 06560, Valbonne, France
  • 4LESIA, Université Paris Cité, Observatoire de Paris, Université PSL, Sorbonne Université, CNRS, F-92190 MEUDON, France
  • 5Arecibo Observatory, University of Central Florida, HC-3 Box 53995, Arecibo, PR 00612, USA

  • 6Institut Universitaire de France (IUF), 1 rue Descartes, 75231 Paris Cedex 05)
  • 7Muséum National d'Histoire Naturelle, Sorbonne Universités, CNRS, IMPMC - UMR CNRS 7590 57 rue Cuvier 75005 Paris, France
  • 8Lowell Observatory, Flagstaff, 1400 West Mars Hill Road, AZ, 86001, USA

The identification of meteorite parent bodies provides the context for understanding planetesimal formation and evolution as well as the key Solar System events they have witnessed. However, identifying such links has proven challenging and some appear ambiguous. Here, we identify that the family of asteroid fragments whose largest member is (161) Athor is the unique source of the rare EL enstatite chondrite meteorites, the closest meteorites to Earth in terms of their isotopic ratios. The Athor family was created by the collisional fragmentation of a parent body 3 Gyr ago in the inner main belt. We calculate that the diameter of the Athor family progenitor was 64 km in diameter, much smaller than the putative size of the EL original planetesimal. Therefore, we deduce that the EL planetesimal that accreted in the terrestrial planet region underwent a first catastrophic collision in that region, and one of its fragments suffered a more recent catastrophic collision in the main belt, generating the current source of the EL meteorites. 

How to cite: Avdellidou, C., Delbo, M., Morbidelli, A., Walsh, K., Munaibari, E., Bourdelle de Micas, J., Devogele, M., Fornasier, S., Gounelle, M., and van Belle, G.: Linking enstatite meteorites to a unique source., EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-16700, https://doi.org/10.5194/egusphere-egu23-16700, 2023.