The chemical states of iron in sixteen Antarctic meteorites belonging
to H-group chondrites were studied by means of Mossbauer spectroscopy.
An Fe-Ni alloy, troilite, paramagnetic Fe(III), and two kinds of para
magnetic Fe(II) were observed in each meteorite. The Mossbauer paramet
ers indicated that the Fe(II) components can be assigned to olivine an
d some pyroxenes. The relative area intensities of Fe(III) in the chon
drites correlated positively with iodine content, which was determined
by radiochemical neutron activation analysis, and those of two Fe(II)
-species correlated negatively with the content. On the basis of the d
ata on the halogen and the Mossbauer spectroscopy, the terrestrial con
tamination on Antarctic meteorites is discussed.