posted on 2015-03-05, 16:51authored byS. R. Taylor
Norian and Rhaetian (Upper Triassic) sediments from the
Mercia Mudstone Group of the East Midlands are described. Four
facies are recognized; (1) sheet flood, (2) red-bed saline
mudflat, (3) lacustrine and (4) marginal. Sedimentation occurred
on an extensive peneplain which had areas of minor relief.
Interstitial sulphate precipitation from hypersaline brines formed
widespread evaporitic gypsum and anhydrite horizons. Dolomitization
of carbonate material and possibly extensive interstitial halite
growth also occurred. Displacive sulphate masses in Fauld Mine are
recognized to be diapiric structures associated with an identifiable
source bed. Fault movement triggered flowage of water-saturated,
source bed gypsum.
A new approach to correlating fine-grained, unfossiliferous
red-beds utilizes variations in clay mineralogy and δ18o dolomite.
The Trent Formation is subdivided by this method into the Fauld
Member and overlying Hawton Member. An isotopic study of the Trent
Formation sulphates (S, Sr) and dolomites (C, 0) indicates that
during deposition of the Fauld Member, grabens and adjacent areas
had a marine brine regime with minor continental input (up to 20%
sulphate derived from continental sulphides). The morst area was
strongly influenced by continental brines which derived sulphate
from the exposed Carboniferous Hathern Anhydrite Series. The
Hawton member brine regime was predominantly continental with
periodic marine influxes.
Two distinct clay suites are recognized. The first is
characterized by a predominance of detrital illite and chlorite
( = Hawton Member); the second is characterized by the presence of
either Mg-rich smectite/chlorite and/or palygorskite and/or
sepiolite with minor illite and chlorite (=Fauld Member).
Sepiolite and palygorskite were neoformed, whilst smectite/chlorite
was transformed from degraded detrital illite. Both processes
occurred in an alkaline brine regime rich in Mg[superscript 2+] and amorphous
silica. The distribution of Mg-rich clays reflects availability
of [superscript 2+], Al[superscript 3+] and Si within the brines.