The distribution and stable isotopic composition of nitrogen released at lo
w temperatures from the ALH 84001 Martian meteorite have been appraised. Th
e results demonstrate an apparently complex geochemistry of the element, wi
th at least three, and possibly four, separate components present. While th
e isotopic composition of most of the nitrogen is within the range of typic
al terrestrial materials (and thus is probably contamination), nitrogen in
the balance of the material has a very different delta(15)N value. Isotopic
ally light nitrogen (component N2; 2.2 ppm with delta(15)N similar to -30 p
arts per thousand and C/N similar to 6) is released when a carbonaceous pha
se combusts below 300 degrees C. Since amino acids and nucleic acid bases h
ave C/N similar to 2-3, the host phase of N2 could be from a mixture of suc
h compounds. The associated nitrogen isotopic composition is very different
from terrestrial contaminants; while this is suggestive of a Martian origi
n for the components, it is difficult to reconcile without advocating forma
tion under special conditions.