Geology of the Northeast Margin of the Salton Trough, Salton Sea, California

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Geology of the Northeast Margin of the Salton Trough, Salton Sea, California ELKANAH A. BABCOCK Department of Geology, University of Alberta, Edmonton 7, Alberta, Canada Geology of the Northeast Margin of the Salton Trough, Salton Sea, California ABSTRACT mately 6,100 m, about 35 km east-southeast of the Salton Sea. Sharp (1967) documented of Mexicali, Baja California (Biehler, 1964; about 24-km right-lateral separation on this The San Andreas fault zone, in the Biehler and others, 1964, p. 132). From the fault. Other important faults of the San Durmid area northeast of the Salton Sea, deepest part of the trough, the irregular Andreas system in the Salton trough are forms the northeast boundary of the Salton basement surface rises to crop out at San the Imperial, Cucapa, Superstition Moun- trough (the landward continuation of the Gorgonio Pass (Fig. 1; Biehler and others, tain, Superstition Hills, and Elsinore faults Gulf of California rift). The zone is 1964, Fig. 6). Recent work suggests that the (Fig- 1). characterized by subparallel faults having Gulf of California and the San Andreas fault The Mecca Hills lie immediately north of both right-lateral and vertical separations. are the result of sea-floor spreading and the Durmid area. Within the Mecca Hills, Stratigraphic offsets indicate at least 1,100 associated transform faulting (Menard, Cenozoic clastic rocks, tightly folded and m of vertical separation on the San Andreas 1960; Hamilton, 1961; Harrison and cut by numerous closely spaced faults of the fault, southwest side downthrown, and Mathur, 1964; Rusnak and Fisher, 1964; San Andreas system, form an anticlinorium. 850-m right-lateral strike-slip separation is Wilson, 1965; Larson and others, 1968). Crystalline basement rocks are exposed in indicated by offset drainage. The eastern margin of the Salton trough is Painted Canyon at the core of the An anticlinal structure southwest of the characterized by a complex of subparallel anticlinorium (Hays, 1957, PI. 2). This study San Andreas fault is probably caused by branches of the San Andreas fault. The zone indicates that the style of deformation in the drape folding over an upfaulted basement of faulting is about 8 to 16 km wide and Mecca Hills continues with little change block or a recently intruded pluton. Small extends from the north end of the Coachella southward into the Durmid area. folds on the southwest flank of the anticline Valley to the Durmid area northeast of the are caused by drag along the San Andreas Salton Sea (Fig. 1). Its trace southeast of the Previous Work fault and gravity sliding. An angular Durmid area is commonly hidden by Little has been published about the discordance of 18° between the Shavers Well Pleistocene lake silts and dune sand. geology of the Durmid area. Dibblee (1954) and Borrego Formations indicates that Evidence of active faulting can be seen, briefly described the sedimentary rocks and tilting adjacent to the San Andreas fault however, southeast of Niland, as offset structure. He assigned the older coarse began prior to Borrego deposition in cultural features and as lineaments on clastic rocks to the Palm Spring Formation Pleistocene time. Folding followed deposi- oblique infrared aerial photographs (Bab- and the younger lacustrine clay and silt to tion of the lacustrine Borrego Formation. cock, 1971). the Borrego lacustrine facies of the Palm Uplift halted, and the area was planed off by The two major faults lying along the Spring Formation and the unconformably erosion. Renewed uplift followed, probably northeast border of the Coachella Valley are overlying Brawley Formation. Dibblee's within the last few thousand years. Key the Banning and Mission Creek faults. data for the Durmid area are summarized on words: structural geology, stratigraphy, San Southward in the Indio Hills, they join to the Salton Sea sheet (see Rogers, 1967). Andreas fault, folds. become the principal fault of the San Andreas fault zone, which is parallel to the STRATIGRAPHY INTRODUCTION AND eastern shore of the Salton Sea (Fig. 1). Sedimentary rocks within the Salton GEOLOGIC Right-lateral displacements have been trough range in age from probable late SETTING measured on faults of the San Andreas zone Pliocene to Holocene. The sediments near The Durmid area (Fig. 1) is an excellent in the Indio Hills (Stotts, 1965) and Mecca the axis of the trough are deltaic sand, silt, location to study structural relations along Hills (Hays, 1957). The total right-lateral and clay deposited by the Colorado River the eastern margin of the Salton trough, a separation on the San Andreas fault in this (Merriam and Bandy, 1965; Muffler and landward continuation of the Gulf of area may be as much as 257 km (Crowell, Doe, 1968). At the margins of the trough California rift. The Salton trough (Fig. 1), an 1962). these fine-grained sediments interfinger with isostatically compensated depression caused Relatively high seismicity characterizes locally derived coarse-grained detritus. by thinning of the crust, contains a the San Jacinto fault zone which enters the Formations recognized within the Dur- maximum sediment thickness of approxi- Salton trough through Borrego Valley west mid area by the author include the lacustrine Geological Society of America Bulletin, v. 85, p. 321—332, 9 figs., March 1974 321 Downloaded from http://pubs.geoscienceworld.org/gsa/gsabulletin/article-pdf/85/3/321/3432965/i0016-7606-85-3-321.pdf by guest on 02 October 2021 Figure 1. Index map of the Saltón trough, California Downloaded from http://pubs.geoscienceworld.org/gsa/gsabulletin/article-pdf/85/3/321/3432965/i0016-7606-85-3-321.pdf by guest on 02 October 2021 SALTON TROUGH, SALTON SEA, CALIFORNIA 323 Fault „»^ Fault located approximately " Fault existance uncertain Approximate axial trace of Durmid Anticline Generalized strike and dip of bedding linilllllll Generalized outline of Durmid Hill Scale in kilometers J 2 3 Figure 2. Sketch map of tectonic elements in the Durmid area. Borrego Formation named by Tarbet and is predominantly coarse-grained arkose and Borrego Formation Holman (1944, p. 1781) and the coarse- arkosic conglomerate, containing cobbles of grained Shavers Well Formation, defined by coarse-grained plutonic rock derived from The Borrego Formation crops out in the Hays (1957). the eastern side of the Chocolate Mountains Durmid area between the San Andreas fault or from ranges east of the Orocopia and the Salton Sea and on the plain Shavers Well Formation Mountains (Fig. 1), where similar rocks are northeast of Durmid Hill (Figs. 2 and 5). exposed today. Coarse-grained sandstone Exposed in the Durmid area is a The Shavers Well Formation, of late with interbeds of pebble conglomerate and 1,475-m-thick section which has been Pliocene or early Pleistocene age, crops out siltstone make up the upper 330 m of the Sea divided into six informal units (Fig. 4). Units northeast of the San Andreas fault at the Bat View Member. 1 and 2, the lowermost, crop out near Salt Caves Buttes (Figs. 2 and 5). The section Finer grained than the Sea View Member, Creek, northeast of the San Andreas fault; exposed at the Bat Caves Buttes is the Skeleton Canyon Member consists of and units 3, 4, 5, and 6 crop out at the south approximately 765 m thick (Fig. 3); but the medium- to coarse-grained sandstone in the end of Durmid Hill (Figs. 2 and 5). The base of the formation is not exposed, and the lower half and mostly fine-grained sand- complete Borrego section is not exposed in upper surface is eroded. On the basis of stone and siltstone in the upper half of the the Durmid area because the contact lithologic similarities, the lower 550 m of the member. Conglomerate beds in the top 15 m between units 2 and 3 is covered. formation was assigned to the Sea View of the Shavers Well Formation contain Based on faunal evidence, the Borrego Member and the upper 215 m was assigned pebbles of Orocopia schist which indicates Formation is a brackish water lacustrine to the Skeleton Canyon Member of Hays uplift of the Orocopia Mountains, and deposit of Pleistocene age (Tarbet and (1957). possibly the Chocolate Mountains, when Holman, 1944, p. 1782). Mineralogical The lower 220 m of the Sea View Member these sediments were being deposited. analyses of samples of the Borrego Forma- Downloaded from http://pubs.geoscienceworld.org/gsa/gsabulletin/article-pdf/85/3/321/3432965/i0016-7606-85-3-321.pdf by guest on 02 October 2021 324 E. A. BABCOCK sand and coarse, bouldery alluvium on the alluvial fans near the mountains. -5 E Description Depositional History unconformify meters- Depositional events in the Durmid area are summa rized below. During late Pliocene or early Pleistocene time, sediments carried Tan, medium-to fine-grained quartz into the area were mostly coarse clastics sandstones, which contain lenses of derived from ranges east of the Chocolate 220+3 granitic conglomerate, interbedded with grey end olive-cobred laminated and Orocopia Mountains, indicating that siltstones. these areas were exposed and shedding coarse detritus at: that time. Near the end of Shavers Well deposition, uplift of :he - -600 Orocopia Mountains is indicated by :he presence of clasts of Orocopia schist in the Shavers Well Formation. Prior to deposition of the Borrego Formation, beds of the LU Shavers Well Formation were tilted and eroded, creating an erosional surface upon Tan, medium-to coarse-grained sandstones. which the Borrego lacustrine sediments were u Granitic pebble conglomerate in lenses. deposited. During deposition of the Borrego OC o Beds '5-25-meters thick. Extensively trough Formation, the Salton trough probably had < I— 330+3 cross bedded. Coarse - grained sandstones a configuration similar to that of today. The oo II® - -400 are arkosic M edium-grained sandstones trough underwent repeated periods of I— are quartzose.
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