Achondrite
From Wikipedia, the free encyclopedia
An achondrite is a stony meteorite that is made of material similar to terrestrial basalts or plutonic rocks. Compared to the chondrites, they have all been differentiated and reprocessed to a lesser or greater degree due to melting and recrystallization on or within meteorite parent bodies. As a result, achondrites have distinct textures and mineralogies indicative of igneous processes.
Achondrites account for about 8% of meteorites overall, and the majority (about two thirds) of them are HED meteorites, originating from the crust of asteroid 4 Vesta. Other types include Martian, Lunar, and several types thought to originate from other as-yet unidentified asteroids. These groups have been determined on the basis of e.g. the Fe/Mn chemical ratio and the 17O/18O oxygen isotope ratios, thought to be characteristic "fingerprints" for each parent body.
Achondrites are classified into the following groups:
- Primitive achondrites (PAC group)
- Acapulcoites
- Lodranites
- Brachinites
- Winonaites
- Ureilites
- HED (Vesta) meteorites
- Howardites
- Eucrites
- Diogenites
- Dunite diogenite
- Olivine diogenites
- Lunar meteorites
- Martian (SNC) meteorites
- Other evolved achondrites
- Angrites
- Aubrites
[edit] External links
- http://www.meteorite.fr/en/classification/stonymain.htm
- Achondrite Images from Meteorites Australia - Meteorites.com.au