The Puye Formation is a geologic formation exposed east of the Jemez Mountains of northern New Mexico. Radiometric dating constrains its age to between 5 and 2 million years, corresponding to the Pliocene epoch.
| Puye Formation | |
|---|---|
| Stratigraphic range: Miocene to Pliocene, | |
 Puye Formation at its type area, the Puye Escarpment, near San Ildefonso Pueblo, New Mexico | |
| Type | Formation |
| Unit of | Santa Fe Group |
| Sub-units | Totavi Lentil |
| Underlies | Tewa Group |
| Overlies | Chamita Formation |
| Area | 518 km2 |
| Thickness | 221 metres (725 feet) |
| Lithology | |
| Primary | Volcaniclastic |
| Other | Ignimbrite |
| Location | |
| Coordinates | 35°53′29″N 106°10′23″W / 35.8914°N 106.1730°W |
| Region |  New Mexico |
| Country |  United States |
| Type section | |
| Named for | Puye Escarpment |
| Named by | H.T.U. Smith |
| Year defined | 1938 |
  Puye Formation (the United States)  Puye Formation (New Mexico) | |
Description edit
The Puye Formation is a fanglomerate containing 25 pyroclastic 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 Tuff north and east of the city of Los Alamos, covering an area of 518 square kilometers (200 sq mi).[1] 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 (233 ft) thick at the type section but thickens westward towards the Sierra de los Valles, west of Los Alamos. Drilling has found that the formation is up to 221 meters (725 ft) thick.1964[2] 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 (~7 million years old) in the formation.[3][4]
The Totavi Lentil is the lowest part of the formation, some 24 meters (79 ft) 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.[2] This is separated by a significant unconformity from the underlying Chamita Formation.[4] The Totavi Lentil is raised to formation rank by some investigators.[1]
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.1964 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. The formation is remarkably well preserved for a volcanic fanglomerate, due to its deposition in an active graben associated with Rio Grande Rift.[5]
A notable feature of exposures of the formation is the presence of pedestal rocks.[6]
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Puye Formation exposures in Rendija Canyon -
Pedestal rocks in the Puye Formation -
Cliffs of the Puye Formation along the Puye Escarpment -
Road cut in Puye Formation, showing gravel beds of the Totavi Lentil near its type section.
Economic geology edit
The formation is a high-yield aquifer exploited in the Los Alamos area.[7] Use of potassium dichromate in a power plant created an unusually well-characterized source of chromium contamination in this aquifer, which has been studied to understand natural attenuation of such pollutants.[8]
History of investigation edit
The formation was first named the Puye Gravel by Harold T.U. Smith in his mapping of the Abiquiu quadrangle in 1938.[9] 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.[10]
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.[2]
Footnotes edit
- ^ a b Turbeville, Waresback & Self 1989.
- ^ a b c Bailey, Smith & Ross 1969, p. 12.
- ^ Heiken et al. 1990, p. 32.
- ^ a b Kelley et al. 2013.
- ^ Waresback & Turbeville 1990.
- ^ Nocita 1986.
- ^ Purtymun & Johansen 1974, p. 349.
- ^ Brown et al. 2014.
- ^ Smith 1938.
- ^ Griggs & Hem 1964, pp. 28–37.
References edit
- Bailey, R.A.; Smith, R.L.; Ross, C.S. (1969). "Stratigraphic Nomenclature of ' Volcanic Rocks in the Jemez Mountains, New Mexico" (PDF). Geological Survey Bulletin (1274-P). Retrieved 4 May 2020.
- Brown, D.B.; Ding, M.; WoldeGabriel, G.W.; Cheshire, M.; Rearick, M.; Conradson, S.; Kluk, E.; Katzman, D. (2014). "Natural Attenuation of Anthropogenic Chromium in Selected Puye Formation in Regional Aquifer System of Los Alamos, New Mexico". American Geophysical Union Fall Meeting Abstracts. H23J-1014. Bibcode:2014AGUFM.H23J1014B. Retrieved 1 July 2021.
- Griggs, R. L.; Hem, J.D. (1964). "Geology and ground-water resources of the Los Alamos area, New Mexico". U.S. Geological Survey Water Supply Paper. 1753. doi:10.3133/wsp1753.
- Heiken, G; Goff, F; Gardner, J N; Baldridge, W S; Hulen, J B; Nielson, D L; Vaniman, D (May 1990). "The Valles/Toledo Caldera Complex, Jemez Volcanic Field, New Mexico". Annual Review of Earth and Planetary Sciences. 18 (1): 27–53. Bibcode:1990AREPS..18...27H. doi:10.1146/annurev.ea.18.050190.000331.
- Kelley, Shari A.; McIntosh, William C.; Goff, Fraser; Kempter, Kirt A.; Wolff, John A.; Esser, Richard; Braschayko, Suzanne; Love, David; Gardner, Jamie N. (June 2013). "Spatial and temporal trends in pre-caldera Jemez Mountains volcanic and fault activity". Geosphere. 9 (3): 614–646. Bibcode:2013Geosp...9..614K. doi:10.1130/GES00897.1.
- Nocita, Bruce W. (October 1986). "Pedestal rocks in the Pliocene Puye Formation, New Mexico". Sedimentary Geology. 49 (3–4): 193–200. Bibcode:1986SedG...49..193N. doi:10.1016/0037-0738(86)90038-2.
- Purtymun, William D.; Johansen, Steven (1974). "General geohydrology of the Pajarito Plateau" (PDF). New Mexico Geological Society Field Conference Series. 25: 347–349. Retrieved 17 May 2020.
- Smith, H.T.U. (1938). "Tertiary geology of the Abiquiu quadrangle, New Mexico". Journal of Geology. 46 (7): 933–965. Bibcode:1938JG.....46..933S. doi:10.1086/624710. S2CID 140678910.
- Turbeville, B.N; Waresback, Damon B; Self, Stephen (February 1989). "Lava-dome growth and explosive volcanism in the Jemez Mountains, New Mexico: Evidence from the plio-pleistocene puye alluvial fan". Journal of Volcanology and Geothermal Research. 36 (4): 267–291. Bibcode:1989JVGR...36..267T. doi:10.1016/0377-0273(89)90074-7.
- Waresback, Damon B.; Turbeville, B. N. (March 1990). "Evolution of a Plio-Pleistocene volcanogenic-alluvial fan: The Puye Formation, Jemez Mountains, New Mexico". Geological Society of America Bulletin. 102 (3): 298–314. Bibcode:1990GSAB..102..298W. doi:10.1130/0016-7606(1990)102<0298:EOAPPV>2.3.CO;2.