The Capitan Reef is a fossil limestone reef of middle Permian age that is dramatically exposed along the southeast flank of the Guadalupe Mountains in Eddy County, New Mexico, reaching its maximum elevation in west Texas, in Guadalupe Mountains National Park. In New Mexico, the reef serves as the host rock for the Big Room in Carlsbad Cavern. A few miles northeast of Carlsbad Caverns National Park, the reef dips into the subsurface and passes beneath the city of Carlsbad, where it forms a karstic aquifer that is the principal source of fresh water for that community (Land and Burger, 2008). The Capitan Reef continues in the subsurface east and south into Lea County, then south for ~150 miles to its southeasternmost outcrop in the Glass Mountains of west Texas.
This study focused on the shallow aquifer that occurs in the dune field with depth-to-water ranging from 1 to 3 feet below interdunal surfaces. We used hydrologic and geochemical data to identify water sources that contribute to the shallow groundwater system in the dune field and to assess how this system responds to water level fluctuations in the adjacent regional basin-fill aquifer. Hydrologic modeling was used to assess the effects of projected additional groundwater pumping in Alamogordo on the shallow dune aquifer on the Monument.
The San Luis Basin is the northernmost and largest basin of the Rio Grande Rift system in New Mexico. Most of the basin is located in Colorado, where it merges to the north with the Upper Arkansas River graben (Grauch and Keller, 2004). The basin is ~150 miles long and 55 miles wide, and has the general form of an east-dipping half graben. Basin-fill material is composed of Tertiary-Quaternary sediments of the Santa Fe Group and late Cenozoic volcanics (Kelley et al., 1976). The basin is bounded to the west by the Tusas and San Juan Mountains and to the east by the Sangre de Cristo Mountains and the Sangre de Cristo fault zone. The deepest part of the basin is found in the Taos graben, a narrow zone 6 to 18 miles wide adjacent to the Sangre de Cristo mountain front (Grauch and Keller, 2004). The southern part of the basin is occupied by the Taos Plateau, which is composed of Pliocene basalt flows that overlie Santa Fe Group basin fill. The southeastern margin of the basin is defined by the Embudo fault zone, which separates the east-tilted San Luis Basin from the west-tilted Española Basin to the south (Bauer and Kelson, 2004).
At the forefront of cutting-edge research at New Mexico Tech, we have been utilizing Raman spectroscopy to unravel the mysteries locked within minerals. By harnessing the power of visible and ultraviolet lasers, we can unlock a plethora of information. So, you may be asking, what is Raman spectroscopy? In simple terms, it's a technique that uses laser light to interact with the atomic vibrations of a material, producing a unique "fingerprint" of its molecular composition. By analyzing the scattered light, we are able to identify and characterize minerals such as apatite, fluorite, and calcite.
Cosmogenic dating techniques have been successfully applied to dating of geomorphically-young surfaces, such as glacial moraines, beach terraces, and basaltic lava flows that have intact surface features, and hence have undergone little erosion (e.g. Phillips et al., 1997a and b; Phillips et al, in review, Dunbar and Phillips, 1996; Zreda et al., 1991, 1993; Zreda, 1994; Anthony and Poths, 1992, Laughlin et al., 1994). These techniques rely on measurement of cosmogenic nuclides that begin to build up as soon as a rock is exposed to cosmic rays. Therefore, cosmogenic techniques can be applied to dating of any surface that is composed of material that was not exposed to cosmic rays prior to formation of the surface, and has been exposed more-or-less continuously since. In the case of an extrusive volcanic rock, buildup of cosmogenic nuclides begins when the rock is erupted, so measurement of the ratio of a cosmogenic isotope to a non-cosmogenic isotope can provide an estimate of eruption age (Phillips et al., 1986).
In 2013, a team of New Mexico Tech researchers began a study of uranium transport, uranium source characteristics, and uranium legacy issues in New Mexico. The effort was funded by Energize New Mexico, a five-year NSF EPSCoR program that concluded in 2018 and that encompassed five research components focused on developing non-carbon emitting energy technologies. The uranium team, which included researchers from UNM, addressed uranium deposits and mine waste mainly in the Grants Mining District, including Laguna Pueblo, and on Navajo Nation lands. These uranium studies span a range of science and engineering disciplines, and not only provide new conclusions impacting remediation, hazard management, and uranium extraction, but hold implications for human health.
The main objective of this study is to examine hydrogeologic processes in Snowy River Passage by analysis of individual flood events. For a specific flood event, we will measure:
The volume of water that infiltrates downward through the Snowy River streambed
The volume of water that evaporates from the Snowy River stream
The volume of water that discharges at Government Spring
The San Agustin Basin is a closed intermontane basin on the northern edge of the Mogollon Plateau, and within the Datil-Mogollon volcanic field of southwestern New Mexico, extending across ~2,400 square miles in Catron and westernmost Socorro Counties. Myers et al. (1994) conducted an investigation of the hydrogeology of the basin, which is summarized here. The San Agustin Basin is bounded to the west and south by the Continental Divide, to the north by the Datil and Gallinas Mountains, and to the east by the San Mateo Mountains. The most recent structural activity in the region was late Tertiary Basin and Range faulting, which formed the San Agustin and Cuchillo Negro grabens. The Plains of San Agustin, which occupy the northeast-trending San Agustin graben, were covered by several large lakes during late Pleistocene time. Playas now occupy these former lake beds. There is no perennial streamflow in the basin.
The Mesilla Basin is one of the southernmost basins of the Rio Grande Rift system, extending from south-central New Mexico across state and international boundaries into west Texas and northern Chihuahua, Mexico. The hydrology of the Mesilla Basin region has been subject to extensive investigations for over a century (e.g., Slichter, 1905; Theis, 1938; Sayre and Livingston, 1945; Conover, 1954; Leggat et al., 1962; Hawley et al., 1969; King et al., 1971; Wilson and White, 1984; Hawley and Lozinsky, 1992; Nickerson and Myers, 1993; Kennedy et al., 2000), as summarized by Hawley et al. (2001), who is paraphrased here. The eastern margin of the Mesilla Basin is defined by the Organ-Franklin-Juarez mountain chain, and the western margin by fault block and volcanic uplands of the East Potrillo Mountains and West Potrillo basalt field. The Robledo and Doña Ana Mountains define the northern end of the Mesilla Basin. The northeast end of the basin is transitional with the Jornada del Muerto Basin. The southern basin boundary with the Bolson de los Muertos in northern Chihuahua state is less well-defined. The entrenched Mesilla Valley of the Rio Grande crosses the eastern margin of the Mesilla Basin, where the cities of Las Cruces, NM, El Paso, Texas, and Juarez, Mexico exploit groundwater resources from the basin aquifers. Regional groundwater and surface water flow is to the southeast toward El Paso, through a gap separating the Franklin Mountains from Sierra Juarez to the south.
