Page 343 - Carbonate Facies in Geologic History
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330       The Rise of Rudists; Middle Cretaceous Facies in Mexico and the Middle East

               such as Solenopora and Jania form  the nuclei. These coated, grainstone beds are  known  to
               overlie and flank caprinid mounds on the Cuesta EI Abra (SMF-11).
                  Bank interior facies of EI Abra (Standard Facies belt 8).
                  These strata are light-colored and well-bedded, varying from 30 cm to 3 m thick. They are
               commonly cyclic; repetitions of strata progress upward in a shoaling sequence. Lowest beds
               are burrowed  micrite  with  Toucasia  or miliolid  grainstones.  These  pass  upward  through
               laminated micrite to a cap of dolomite crust or intraformational pebble conglomerate. Eight
               common bank interior-restricted marine microfacies are recognized  in  the  various  studies
               noted above.
               1.  Miliolid grainstone: Thick-bedded (1 m) to massive strata, burrows in upper parts of bed,
                 some  peloid  grains  but  mostly  tests  of  miliolid  foraminifera  (SMF-18)  (Plate XXX C).
               2.  Peloidal grainstone to wackestone with some grapestone: Sparry cement, generally 75%
                 grains,  less  than  10%  miliolids,  5%  bioclasts.  This  sediment  is  derived  from  organic
                 pelleting of lime muds in an environment where lime precipitation continuously hardens
                 the grains and where gentle current partly winnows remaining lime mud (SMF-16).
               3.  Miliolid wackestone-packstone: Burrowed sediment which includes a few  rudists (SMF-
                 19).
               4.  Molluscan wackestone:  Toucasia  and monopleurid rudists,  oysters,  and scattered milio-
                 lids. In places the oysters or rudists form biostromes (Plate VB).
               5.  Dolomite-lime mudstone laminated crusts: Formed by evaporation causing mineral pre-
                 cipitation and replacement. By analogy with Holocene sediments, lamination is probably
                 algal in origin. Disruption of the crust by drying and curling-up of the fragments results in
                 the construction of intraformational breccia which ftlls channels and is a common lateral
                 facies to the crusts (SMF-24).
               6.  Bulbous algal laminites with fenestral fabric: Mostly peloidal lime mudstone or homoge-
                 neous mudstone. Represent desiccated algal  mats with scattered miliolids  and ostracods
                 (SMF-20).
               7.  Planar fine  mm laminites, nonfenestral, often pure dolomite, containing scattered miliol-
                 ids. Probably also induced by algal trapping of seasonal increments of lime mud.
               8.  Homogeneous lime mudstone or dolomite (SMF-23).
                  The outcrop areas of the platforms studied in  Mexico all  show strong facies
               differentiation displaying the above standard rock  types  and illustrating clearly
               their interpreted environments. The interiors of the platforms and large offshore
               banks are wide  expanses  of the  well-bedded  EI  Abra  Formation.  The  margins
               contain  knolls  of  caprinid-radiolitid  rudist  buildups  and  much  biogenic  lime
               sand. These facies are reasonably well understood. The foreslopes of the banks, on
               the other hand, provide problems in interpretation in almost all places where they
               have been studied. Is the common faulting at the edge of the massive carbonate of
               the  banks  contemporaneous with deposition, or later? Just how  steep  was  the
               original slope? How much  original relief was  there  on  anyone bank-tens  of
               meters or hundreds of meters? To what extent can sedimentologic study of the
               basinal sediments provide some estimate of depth? Clear answers to these ques-
               tions are important in developing exploration models  and  in  comparing Creta-
               ceous shelf margins with others in the geologic record.
                  One of the best areas for display of shelf margin facies lies along the Tampico
               highway about 10-12 km east of the city of Valles, San Luis Potosi (Figs. XI-3, XI-
               6).  Here extensive  quarries  have  been  cut  into  the  eastern  edge  of the  Valles
               platform which has been uplifted along a faulted  anticline in front  of the  Sierra
               Madre for  a distance  of more  than  100 km.  The  frontal,  east-facing  scarp,  the
               Cuesta  EI  Abra,  exposes  knoll  reefs  close  to  the  shelf  margin  at  the  railway
               loading station, Taninu!.  Large  springs  and  caverns  along  the  escarpment  are
               present, making additional exposures possible. Detailed studies have been made
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