Orgueil is one of five known meteorites belonging to the
CI chondrite group (see
meteorites classification), and is the largest (). This group has a composition that is essentially identical to that of the sun, excluding gaseous elements like
hydrogen and
helium. Notably though, the Orgueil meteor is highly enriched in (volatile) mercury - undetectable in the solar photosphere, and this is a major driver of the "mercury paradox" that mercury abundances in meteors do not follow its volatile nature and isotopic ratios based expected behaviour in the solar nebula. Because of its extraordinarily primitive composition and relatively large mass, Orgueil is one of the most-studied meteorites. One notable discovery in Orgueil was a high concentration of
isotopically anomalous
xenon called "xenon-HL". The carrier of this gas is extremely fine-grained
diamond dust that is older than the
Solar System itself, known as
presolar grains. In 1962, Nagy et al. announced the discovery of 'organised elements' embedded in the Orgueil meteorite that were purportedly biological structures of extraterrestrial origin. These elements were subsequently shown to be either
pollen (including that of ragwort) and fungal
spores (Fitch & Anders, 1963) that had contaminated the sample, or crystals of the mineral
olivine. ==Seed capsule hoax==