As with other ureilites, Almahata Sitta falls on the carbonaceous chondrite anhydrous mineral line. Although complex organic compounds commonly occur in many other carbonaceous chondrites groups, Glavin et al. (2010) conducted the first such analysis on a ureiliteAlmahata Sitta. Compared to over 80 amino acids identified in some CM chondrites, only 19 amino acids and their enantiomers were identified in Almahata Sitta, along with 4 amines (produced by thermal decomposition of amino acids), plus other unidentified amino acids belonging to the 5-carbon group.
Because these organic compounds rapidly decompose at temperatures of 500600°C, and it is generally accepted that ureilites experienced temperatures twice that, conditions for the formation of organics are tightly constrained. The amino acids could have been introduced by collisions with carbon-rich asteroids, or peak temperatures might not have been high enough to destroy them all; however, it is thought most likely that the organics were formed by catalytic reactions after asteroid 2008 TC3 had cooled.
As in all groups, these organic compounds have a non-biogenic origin. The following organic compounds have been isolated from Almahata Sitta (Glavin et al., 2010):
ORGANIC COMPOUNDS IDENTIFIED IN THE UREILITE ALMAHATA SITTA