The Sierra Madera crater is a complex impact crater (astrobleme) in southwestern Pecos County, Texas, United States. The impact structure spans approximately in diameter and is centered south of Fort Stockton, roughly equidistant from Mexico and New Mexico and near the northeastern end of the Glass Mountains. The central peak of the rebound structure of the impact crater rises above the surrounding land. The peak is visible from U.S. Highway 385 between Fort Stockton, Texas and Marathon, Texas. The Sierra Madera crater is located on private property on the La Escalera Ranch.
The crater is mostly eroded but remains well exposed. At the center of the crater are the hilly remains of the central peak produced by the impact. Known as Sierra Madera or Madera Mountain, the uplift rises above sea level. The peak occupies most of the crater and is its most prominent feature, spanning about across. Strongly folded and faulted carbonate and siliciclastic rock layers from the upper Paleozoic to Cretaceous comprise the central structure, along with breccia fragments spanning as much as several meters across. The oldest Permian rocks in the structure lie above their typical position. The strata folded in the central uplift provide an indication of the impact's age. An alluvium-filled depression up to wide surrounds the central uplift, outlined by an outer concentric crater rim about wide. The crater rim consists of low hills that climb subtly above the surrounding land.
The first geological map of the Sierra Madera was published in 1930. The central peak was initially interpreted as a cryptovolcanic structure. However, no igneous rocks were detected within of the surface. The discovery of shatter cones, impact breccias, and shocked quartz in the 1960s, along with supporting gravity and magnetic surveys, lent credence to interpreting the structure as having impact origins. The shock-related features identified in rock samples suggest the impact produced pressures of at least 3 to 20 GPa, with erosion masking the record of more intense pressures.
The impact that produced the Sierra Madera likely occurred sometime between the late Cretaceous and early Paleogene (within 100 million years ago) in an area with thick sediment about in depth. The impact site, at the southern edge of the Val Verde Basin, may have been underwater at the time of impact. The surrounding area now is largely flat or rolling shrubland and grassland with sand and caliche. The apparent diameter of the crater is based on the diameter of the concentric outer hills interpreted as a crater rim. However, studies in the 2000s suggest the structure may be larger than initially thought; one 2006 study estimated a diameter with significant erosion. The entire bowl-shaped impact structure extends to below the surface.
In the 1960s, the Sierra Madera crater was the subject of various studies conducted by the Astrogeology Research Program at USGS as part of the Apollo program, providing an analogous setting to lunar craters. Apollo 17's Gene Cernan and Jack Schmitt did some of their geological training here in March 1972.