An anclent stratlgraphic trap for petroleum exists in continental deposits at Rangely oil field, about 24 km south of Dinosaur National Monument, where the eol Ian Weber Sandstone (pennsy lvanlan-permian) intertongues with the Maroon Formation of fluvlal origin. The stratigraphic trap developed as a result of the progradation of eolian dunes toward the ancient Uncompahgre uplift. Fine silt and conglomeratic material brought into the dunes along the margins of the dunefield became impermeable layers--due to postdepositional diagenetic cementation and intrinsic textural properties. The conditions which created the stratlgraphic trap at Rangely may have developed ' in other areas along the margins of ancient Pennsylvanian uplifts in Colorado, Wyoming, and Utah. Analysis of cores from Rangely oil field indicates that porosity and permeability within the oil-productive sandstone Is affected by primary and secondary diagenetic processes. Reduction of porosity and permeability in the reservoir sandstones Is due to burrowing and contortlon of laminations, which destroyed or ~dified previously well-sorted laminations of sandstone units. Cementation is most complete in the burrowed and contorted Intervals. Evidence for eol Ian origin of the Weber Sandstone near Dinosaur National Honument includes: (a) large scale tabular-planar cross-stratified u nits with few horizontal symmetric ripples, but many low-relief, asymnetric ripples oriented up and down slipface deposits; (b) raindrop imprints on slipface deposits at Deerlodge Park, Colorado; (c) characteristics of contorted stratification, lamination style, and burrowing that e xactly match those of modern eolian deposits and some inferred ancient eolian deposits, and which can be interpreted in the l ight of known eol Ian processes; (d) interbedding of we1 I-sorted quartz sandstones and poor1 y sorted, mica-r ich siltstones and conglomerates at Rangely oil field, which Is interpreted to be interbedded eolian dune and fluvial sediments; (e) consistent southward transport directions In the Weber Sandstone are more compatible with a wind- driven depositional system than a marine depositional system, since steady ocean currents flowing south to south- east would be forced to flow upslope toward the anclent Uncompahgre and Front Range up1 ifts; (f) absence of appre- ciable clay or chert In the Weber Sandstone in the study area, in contrast to the occurrence of these minerals in marine rocks of the Weber Sandstone farther west; (g) thin, lentlcular carbonates (usually only .31-.61 m thick) restricted to extensive dlastems In the Weber Sandstone In the study area which indicate t hat the carbonates were deposited in non-marine ponds associated with interdune areas; (h) striking dl fferences between the lenticular, brecciated, unfossiliferous dolomites In the Weber Sandstone and the t hick, fossiliferous cherty limestones of approximately the same age in marine deposfts within the Weber Sandstone, and the older underlying Morgan Forma- tion. Shortly after deposition. the eollan deposlts of the Weber Sandstone became saturated with water and were then subjected to penecontemporaneous deformation that produced complex folding and breaking of laminations.
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