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The Embudo Fault between Pilar and Arroyo Hondo, New Mexico ...

The Embudo Fault between Pilar and Arroyo Hondo, New Mexico ...

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EMBUDO FAULT BETWEEN PI LAR AND ARROYO HONDO 79interpreted to be s<strong>and</strong>-dune, playa-type lacustrine <strong>and</strong> alluvialf<strong>and</strong>eposits.<strong>The</strong> s<strong>and</strong>-dune facies consists of buff s<strong>and</strong> in large crossbeddedunits with an easterly paleo-wind direction. <strong>The</strong>se bedsare identical to the typical Ojo Caliente S<strong>and</strong>stone exposed 15mi (24 km) to the west along the Ojo Caliente River. <strong>The</strong>intervening strip is covered by basalts of Black Mesa <strong>and</strong> itsflanking l<strong>and</strong>slide apron so that direct correlation is impossible.<strong>The</strong> playa-type lacustrine facies consists of brownish silt <strong>and</strong>s<strong>and</strong> that is parallel-bedded (vertically accreted windblowns<strong>and</strong>) <strong>and</strong> which contains small carbonate nodules <strong>and</strong> fossilsoil zones.<strong>The</strong> alluvial-fan facies forms ribbed outcrops <strong>and</strong> consists ofgray pebbly gravel that is subangular to subrounded. All clastsare schist <strong>and</strong> quartzite derived from the Precambrian rocksexposed immediately to the south in the Picuris Mountains.<strong>The</strong> gray color is due to the abundance of s<strong>and</strong> <strong>and</strong> smallpebble-sized fragments of black slate <strong>and</strong> phyllite. Placers ofgarnet crystals also are present. <strong>The</strong> average size of the conglomerateclasts is slightly larger in the higher exposed layers.Total exposed section is estimated to be about 1500 ft (460m) thick. <strong>The</strong> base is not exposed <strong>and</strong> the top is an angularunconformity under the Servilleta Formation (Unit D).nating with bluish-gray pebbly s<strong>and</strong>stone. Unit B is dominatedby gravelly s<strong>and</strong>s that have gray or reddish matrices separatedby meter-thick red mudstones. In both units, the gravellylayers are cemented better <strong>and</strong> tend to hold up low ridges. <strong>The</strong>generally uncemented, easily eroded nature of these units isshown by the wide amphitheater (fig. 3) that is eroded intothese units as compared with the usual narrow V-shapedcanyon of <strong>Arroyo</strong> <strong>Hondo</strong>. <strong>The</strong>se units have been recognizedonly in <strong>Arroyo</strong> <strong>Hondo</strong> <strong>and</strong> in the unnamed arroyo immediatelyto the east.Unit C (Ojo Caliente S<strong>and</strong>stone Member of theTesuque Formation)This unit is exposed well on the southward-facing bluffs ofRito Cieneguilla from <strong>Pilar</strong> northeastward. <strong>New</strong> <strong>Mexico</strong> Highway68 parallels this Rito <strong>and</strong> its roadcuts provide many convenientexposures until it tops out on the Taos Plateau. <strong>The</strong>oldest exposed part of Unit C is in the bluffs near <strong>Pilar</strong>, <strong>and</strong>because of consistent west to north dips, progressively youngerbeds are traversed northeastward along Highway 68 until itpasses out of Rito Cieneguilla <strong>and</strong> onto the Taos Plateau.Unit C consists of three distinctive facies that are interbeddedin units 40 to 50 ft (12 to 15 m) thick, <strong>and</strong> which areUnit D (Servilleta Formation)This unit will be described in three segments, in stratigraphicorder from oldest to youngest: the conglomeratesnorth of the <strong>Embudo</strong> fault scarp along the Rio Gr<strong>and</strong>e, theiroverlying basalts, <strong>and</strong> the single basalt <strong>and</strong> associated conglomeratessouth of the <strong>Embudo</strong> fault scarp.<strong>The</strong> canyon of the Rio Gr<strong>and</strong>e north of <strong>Pilar</strong> is carved intothe Servilleta Formation. Near <strong>Pilar</strong>, extensive l<strong>and</strong>slide covermasks the underlying sedimentary rocks except for those bedsimmediately underlying the capping basalts <strong>and</strong> exposures incanyons on the east wall 2.5 mi (4 km) north of <strong>Pilar</strong>. Here,about 500 ft (150 m) of gray pebble-cobble conglomerate thatis subrounded to subangular <strong>and</strong> which coarsens upward areexposed in a steep-walled arroyo. All clasts are of rock typesexposed in the Picuris Mountains to the southeast. Pebble imbrication<strong>and</strong> crossbed transport directions lie in the northwestquadrant. None of the units is of mudflow origin, but insteadis characteristic of braided-stream alluvial-fan types. Presumably,these lie on the Santa Fe Group, but if present aboveriver level, they are covered. <strong>The</strong> widening of the canyon inthis reach might be a result of erosion through the lightlycemented Servilleta sedimentary rocks into the eolian s<strong>and</strong>facies of the Ojo Caliente Member of the Tesuque Formation.<strong>The</strong>se beds dip only a few degrees north <strong>and</strong> west (initial dip?)<strong>and</strong> appear to underlie conformably the capping basalts of theRio Gr<strong>and</strong>e Canyon.<strong>The</strong> basalts exposed along the Rio Gr<strong>and</strong>e Gorge are in distinctpackages of 3-5 flows each separated by sedimentaryinterbeds of varying thickness. <strong>The</strong> lowest exposed basaltpackage terminates a few kilometers north of the confluenceof the Rio Pueblo de Taos <strong>and</strong> the Rio Gr<strong>and</strong>e; the visibleresult is the change in shape of the gorge from a steep V-shaped canyon southward to the wider slump-block-coated U-shaped canyon. Continuing southward, successively higherbasalt packages step farther southward over the northward-

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