The Puye Formation is a fanglomerate containing 25 pyroclasic flows, including pumicious ignimbrites and block-and-ash flows, erupted by vents of the Tschicoma Formation. It is exposed from the mouth of Ancho Canyon in White Rock Canyon north to Santa Clara Peak, and generally underlies the Bandelier Tuffnorth and east of the city of Los Alamos, covering an area of 518 square kilometers. It is best exposed in Guaje Canyon and on the southern end of the Puye Escarpment where it is a cliff-forming formation. It is 71 meters thick at the type section but thickens westward towards the Sierra de los Valles. Drilling has found that the formation is up to 221 meters thick.The formation was deposited between 7 and 4 million years ago, based on radiometric dating of an ash bed in the upper part of the formation and the absence of Bearhead Rhyolite ash in the formation. The Totavi Lentil is the lowest part of the formation, some 24 meters thick, which consists of pebbles, cobbles, and small boulders of quartzite and granite with only limited volcanic debris, contrasting with the remainder of the formation. This is separated by a significant unconformity from the underlying Chamita Formation. The main body of the Puye Formation consists of fanglomerates in which most of the detritus is volcanic rock of dacitic composition. There are also dacitic tephra beds and some basalt. The formation shows cyclicity on the scale of 5 to 30 meters representing individual eruptive pulses in the northeastern Jemez highlands. Each sequence shows marked facies changes with increased distance from the eruptive center. Deposition ceased with reduction in Tschicoma volcanism and basinwide pedimentation due to downcutting of the Rio Grande. It is remarkably well preserved for an alluvial fan, due to its deposition in an active graben associated with Rio Grande Rift. A notable feature of exposures of the formation is the presence of pedestal rocks.
Economic geology
The formation is a high-yield aquifer exploited in the Los Alamos area.
The formation was first named the Puye Gravel by H.T.U. Smith in his mapping of the Abiquiu quadrangle in 1938. The name was changed to Puye Conglomerate by Roy Griggs in 1964, since the exposures he studied were consolidated enough to stand as cliffs. Griggs also designated a type section and divided the unit into an upper unnamed fanglomerate and a lower Totavi Lentil, named for a nearby settlement. Griggs assigned the formation to the Santa Fe Group. Because of its diverse lithology, the formation was renamed the Puye Formation by Bailey, Smith, and Ross in 1969 as part of their work establishing the stratigraphy of the Jemez Mountains.
