Encyclopedia of Astrobiology

Living Edition
| Editors: Muriel Gargaud, William M. Irvine, Ricardo Amils, Henderson James Cleaves, Daniele Pinti, José Cernicharo Quintanilla, Michel Viso

Meteorite, Orgueil

Living reference work entry
DOI: https://doi.org/10.1007/978-3-642-27833-4_976-3

Definition

The Orgueil meteorite fell on May 14, 1864, near the village of the same name, in the south of France. With a mass of 14 kg, it is the biggest sample of the C I carbonaceous chondrite group, which represents the most primitive bodies of the solar system. Its composition is identical to that of the Solar photosphere, except for the lightest elements hydrogen and helium. An important discovery was the detection of a high abundance of isotopically anomalous xenon which could be the signature of presolar material. The Orgueil meteorite also contains many amino acids. Recent studies suggest that Orgueil has a cometary origin.

See Also

Keywords

Bioorganic Chemistry High Abundance Solar System Light Element Carbonaceous Chondrite 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer-Verlag Berlin Heidelberg 2014

Authors and Affiliations

  1. 1.LESIA – Bâtiment ISO (n°17)Observatoire de Paris – Section de MeudonMeudonFrance