M. De Craen et al., Petrography and geochemistry of septarian carbonate concretions from the Boom Clay Formation (Oligocene, Belgium), GEOL MIJNB, 77(1), 1998, pp. 63-76
The septarian carbonate concretions from the Boom Clay (Belgium) consist ma
inly of authigenic minerals such as micrite (less than or equal to 70% bulk
volume) and pyrite framboids (similar to 3%). These mineral phases occur b
etween detrital grains and fossils. The septarian cracks are lined with cal
cite, which is sometimes covered with pyrite. The preservation of delicate
sedimentological features in the concretion matrix (hardly compacted faecal
pellets, burrows and uncrushed shells) points to an early origin of the co
ncretions. Systematic geochemical variations from concretion centre to edge
suggest that growth continued during shallow burial. The delta(13)C values
(-17.5 to -20.5%) of the concretionary carbonate show that bacterial sulph
ate-reduction processes were dominant. Sulphate-reduction-derived HCO3- was
diluted by marine-related HCO3-, derived from dissolved bioclasts. A sligh
t enrichment in delta(13)C during growth is caused by the decreasing influe
nce of sulphate reduction because of the progressive closure of the diagene
tic system due to shallow-burial compaction. The delta(18)O values (-0.5 to
+1.0%) of the concretionary carbonate point to a marine origin. The slight
ly O-18-depleted signature with respect to time-equivalent marine-derived c
arbonate relates to the incorporation of an O-18-depleted component, origin
ating from sulphate and organic matter. The slight decrease in delta(18)O d
uring growth relates to an increasing influence of this component and to a
decreasing influence of seawater-derived oxygen during early diagenesis.