Alais meteorite

Alais or Allais is the first carbonaceous chondrite meteorite identified. It fell near Alès in 1806 in multiple fragments which together weighed 6 kg (13 lb 4 oz), although only 0.26 kg (9.2 oz) remains. The meteorite contains a number of elements in similar proportions to the Solar System in its primordial state. It also contains organic compounds and water. It has proved to be one of the most important meteorites discovered in France.

Alais
TypeChondrite
ClassCarbonaceous chondrite
GroupCI1
CountryFrance
RegionOccitanie
Coordinates44°7′N 4°5′E[1]
Observed fallYes
Fall date15 March 1806
TKW6 kg (13 lb 4 oz)
A fragment of the meteorite on display in 2018

History

At 17:00 on 15 March 1806, two detonations were heard near Alès in Gard, France.[2] Shortly afterwards, two soft black stones were discovered in the villages of Saint-Étienne-de-l'Olm and Castelnau-Valence, weighing 4 kg (8 lb 13 oz) and 2 kg (4 lb 7 oz) respectively. The fragments were collected by people who observed the impact and given to two scientists that lived locally.[1] The meteorite was analysed by Louis Jacques Thénard, who published a study in 1807, showing that it had a high carbon content.[2] It was initially doubted that the fragments were of non-terrestrial origins as their attributes were markedly different to existing meteorites.[3] However, it was increasingly realised that this was a new, albeit rare, type of meteorite.[4] The meteorite is also known as Valence.[1]

Curation and distribution

As an early fall (soon after the consensus that meteorites were real, extraterrestrial phenomenon), Alais has largely been dispersed. Few samples have been preserved, less than Orgueil, but more than Tonk and particularly Revelstoke.

OrgMassPlaceCountryRef
Mus. NdH45 gParisFrance[5]
Geol. Surv. Ind.5gKolkataIndia
Vat. Met. Coll.4.5gCastel GandolfoItaly
ASU3gTempeUSA
Field Mus.3.6gChicagoUSA
Uni. Tübingen1.9gTübingenGermany
Geol. Surv. Ca.1.9gOttawaCanada
Mus. fur Nat.1.7gBerlinGermany
Nat. Hist. Mus.1.7gWienAustria
Smithsonian0.7gWashingtonUSA[6]
Am. Mus. N.H.0.6gNew YorkUSA
IfP0.5gMunsterGermany
Ro. Akad. Nauk.<.5gMoscowRussia
West. Aus. Mus.<.5gPerthAustralia
DuPont Coll.0.2gPalatineUSA

Source: Grady, M. M. Catalogue of Meteorites, 5th Edition, Cambridge University Press

Description

Overview

The Alais meteorite is one of the most important meteorites in France.[7] It is black with loose friable textures with a low density of less than 1.7 g/cm3 (0.061 lb/cu in).[2] Originally consisting of fragments that together weighed 6 kg (13 lb 4 oz), it has been subject to substantial scientific examination and currently only 260 g (9.2 oz) remains.[8] A fragment, weighing 39.3 g (1.39 oz) is held by the National Museum of Natural History, France.[9]

Composition and classification

The meteorite is one of five known meteorites belonging to the CI chondrite group.[3] This group is remarkable for having an elemental distribution that has the strongest similarity to that of the solar nebula. Except for certain volatile elements, like carbon, hydrogen, oxygen, nitrogen and the noble gases, which are not present in the meteorites in the same proportions, the ratios of the elements are very similar.[10] The meteorite contains cubanite, dolomite, fosterite, pyrrhotite and zircon amongst other minerals.[11]

Origin of life controversy

The meteorite has been at the centre of controversial claims about an extraterrestrial origin of life since the discovery of organic matter on the meteorite by Jöns Jacob Berzelius.[12] Organic compounds, amino acids and water have been found in the meteorite. However, studies differentiate between organic and biological matter, the latter not being present.[4]

See also

References

Citations

  1. Meteoritical Bulletin Database: Alais
  2. Marvin 2006, p. 53.
  3. Mason 1963, p. 621.
  4. Marvin 2006, p. 54.
  5. "Sample of Alais". Muséum National d'Histoire Naturelle. Retrieved 15 Mar 2022.
  6. "Meteorites: Alais". Smithsonian: National Museum of Natural History. Retrieved 15 Mar 2022.
  7. McCall, Bowden & Howarth 2006, p. 5.
  8. Mason 1963, p. 622.
  9. Caillet Comorowski 2006, p. 192.
  10. Lauretta & McSween 2006, p. 40.
  11. Kerridge, Macdougall & Marti 1979, p. 360.
  12. Chyba 1990, p. 113.

Bibliography

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