Chassigny (meteorite)
| Chassigny meteorite | |
|---|---|
Chassignite | |
| Parent body | Mars |
| Country | France |
| Region | Chassigny, Haute-Marne |
| Coordinates | 47°43′N 5°23′E / 47.717°N 5.383°E[1] |
| Fall date | 1815-10-03 |
 Related media on Wikimedia Commons | |
Chassigny is a
SNC group of meteorites. Chassigny is an olivine cumulate rock (dunite). It consists almost entirely of olivine with intercumulus pyroxene, feldspar, and oxides. It was the only known chassignite until NWA2737 was found in the Moroccan Sahara in northwest Africa.[4]
Chassigny is particularly important because, unlike most SNCs, its noble gas composition differs from that in the current Martian atmosphere. These differences are presumably due to its cumulate (mantle-derived) nature.[5]
See also
- Glossary of meteoritics
- Meteorite falls
References
- ^ Meteoritical Bulletin Database: Chassigny
- ^ Pistollet (1816) The circumstances of the Chassigny meteorite shower. Ann. Chim. Phys. (Paris) v. 1, pg 45-48.
- ^ "The Chassigny Meteorite" - From NASA's Jet Propulsion Laboratory, stating it is the only example. URL accessed September 6, 2006.
- ^ Beck P., Barret J. A., Gillet P., Franchi I.A., Greenwood R. C., Van De Moortele B., Reyard B., Bohn M. and Cotton J. (2005) The Diderot Meteorite, the second chassignite.Lunar and Planet. Sci. XXXVI, Abstract #1326.
- ^ Mars Meteorite Compendium: Chassigny, Compiled by Charles Meyer.
