We report Cl-36 (301-kyr half-life) data obtained by accelerator mass
spectrometry allowing nominal terrestrial ages to be determined for 39
Antarctic H4-6 chondrites for which contents of volatile trace elemen
ts are known. The compositional difference between these Antarctic met
eorites and 58 non-Antarctic falls increases with terrestrial age and,
using multivariate statistical techniques, becomes highly significant
for Antarctic samples with ages >50 kyr. The compositional difference
is inconsistent with trivial causes such as weathering and seems to r
eflect differences in thermal histories of parent sources. Temporal so
urce variations for the H chondrite flux on Earth thus exist not only
on a short-term, 40 years, basis (Dodd et al., 1993) but also on a lon
g-term, >50 kyr, basis.