Sphaerosiderite, a morphologically distinct millimeter-scale spherulit
ic siderite (FeCO3), forms predominantly in wetland soils and sediment
s, and is common in the geologic record. Ancient sphaerosiderites are
found in paleosol horizons within coal-bearing stratigraphic intervals
and, like their modern counterparts, are interpreted as having formed
in water-saturated environments. Here we report on sphaerosiderites f
rom four different stratigraphic units, each of which has highly varia
ble C-13 and relatively stable O-18 compositions. The unique isotopic
trends are analogous to well-documented meteoric calcite lines, which
we define here as meteoric sphaerosiderite lines. Meteoric sphaeroside
rite lines provide a new means of constraining ground-water delta(18)O
and thus allow evaluation of paleohydrology and paleoclimate in humid
continental settings.