METEORIC DIAGENESIS BELOW A SUBMERGED PLATFORM - IMPLICATIONS FOR DELTA-C-13 COMPOSITIONS PRIOR TO PRE-VASCULAR PLANT EVOLUTION, MIDDLE ORDOVICIAN, ALABAMA, USA
Kj. Tobin et Kr. Walker, METEORIC DIAGENESIS BELOW A SUBMERGED PLATFORM - IMPLICATIONS FOR DELTA-C-13 COMPOSITIONS PRIOR TO PRE-VASCULAR PLANT EVOLUTION, MIDDLE ORDOVICIAN, ALABAMA, USA, Sedimentary geology, 90(1-2), 1994, pp. 95-111
The Middle Ordovician ''Chickamauga'' Formation at Red Mountain Expres
sway (RME) and Tidwell Hollow (TWH) sections in Alabama (U.S.A) has a
complex early diagenetic history. Early diagenetic history of the buil
dup facies consisted of two phases of marine cementation separated by
two generations of meteoric, equant calcite with moldic dissolution se
parating equant calcite generations. A third generation of meteoric, e
quant (drusy) calcite is present after secondary marine diagenesis. Eq
uant (drusy) calcite is interpreted as meteoric because its stable iso
topic composition (deltaC-13 = -0.1 to -1.6 parts per thousand, deltaO
-18 = -4.8 to -7.3 parts per thousand) is too variable to be accounted
for by marine or mixing zone precipitation. Equant (drusy) calcite fr
om buildup facies is mostly non-luminescent and non-ferroan. This is u
nlike early, ferroan equant calcite (dull to bright luminescent) from
below the unconformity that overlies the ''Chickamauga'' Formation at
RME. Meteoric diagenesis below the unconformity is unrelated to early
diagenesis in the underlying buildup facies. Equant (drusy) calcite fr
om the buildup facies at RME has a covariation of deltaC-13 and deltaO
-18 values that forms a truncated inverted ''J'' and has elevated Mg v
alues. These geochemical signatures indicate precipitation at a site t
hat was distal from the recharge zone. Meteoric diagenesis at RME occu
rred during rising relative sea level and flow of meteoric fluids unde
r a submerged platform is the only mechanism able to reconcile availab
le stratigraphic, petrologic, and geochemical data. Ordovician meteori
c deltaC-13 values (from TWH and other formations) are slightly deplet
ed (2-4 parts per thousand) relative to coeval marine carbonate, espec
ially when compared with post-Silurian meteoric carbonate. Minor deple
tion of Ordovician carbonate is the result of limited generation of li
ght soil-gas CO2 before the development of vascular plants.