U.S. DEPARTMENT OF THE INTERIOR GEOLOGIC INVESTIGATIONS SERIES U.S. GEOLOGICAL SURVEY 3 I–2631 105°37'30" 35' 32'30" 30' 105°27'30" 32°07'30" 32°07'30" Mountain and on Wind Mountain; two additional anticlines lacking exposed igneous rocks in their cores Psa Psa Cornudas are present north of Flat Top and southwest of Alamo Mountain. Between the anticlines are a series of Py Psa Psa Psa Mountain Ph subparallel to obliquely trending synclines or structural sags. The most pronounced syncline can be 11 ° 9 Qc traced along the west side of Wind Mountain where sedimentary rocks dip as much as 60 away from Py Psa 13 the peak. The complex, locally merging and commonly curvilinear patterns defined by the traces of the Ph Ti Black Qc 6 Qaf Qc North pၤ Qaf axial planes of folds in the Cornudas Mountains bears a strong similarity to folds associated with intru- Mountain Qaf Qaf Qa Psa 14 Qaf sive rocks so well described by Hunt (1953) in his study of the Henry Mountains, Utah. ၤ Qaf p Psa Psa To the north, Cornudas Mountain is within an anticline that can be traced for 12 mi (20 km) com- Ti Qfy 3000 Ku Psa pletely across the map area; the Hueco Formation is well exposed in that part of the fold that is cen- Py Py 11 Qa tered on the intrusive rocks. The anticlinal axis trends northwest on the east and folded Hueco lime- Ti Ph Psa Qa Qaf Unconformity 6 stones appear to extend beneath the east side of Cornudas Mountain. On the west, the fold deforms Ph East Qa Qaf Psa Qaf 7 Hueco limestones that overlie the intrusion; the fold axis trends west in this area but is displaced about 1 6 12 5 Wind pၤ mi (1.6 km) to the north where it merges with a north-trending structural sag or syncline before reach- pၤ Qc 5 Qc plift Mtn. ing the western map boundary. Spatial relations between the Cornudas Mountain intrusive and the brian lrocks u of Psa Psa 5000 adjacent folded rocks suggest that an elongate intrusive body underlies the entire anticlinal fold and that Ph 4 Qaf Psa PrecamPederna Flat Top Qc Psa Psa the exposed Cornudas intrusive is an irregular-shaped, sill-like body that plunges gently west, yet is bulg- Py Psa ingly discordant on the east (fig. 2); Hunt (1953) might have termed this apophysis of the underlying 3000 Ti 500 Ph Ph 0 Qc 13 intrusive a sphenolith. 5000 Py 6 13 pၤ 17 Qaf Psa Wind Mountain is the core of a dome in which dips of enclosing sedimentary rocks of the Hueco ၧၤu Qc 7 Qa pၤ 3000 Psa Formation are locally more than 60°. A structural sag appears to separate Deer Mountain on the west SEA ၤ 3000 LEVEL p ၤ from the main part of the dome; however, the Deer Mountain intrusive also intruded the Hueco and is p Qaf Alamo 12 structurally in the core of a west-trending anticlinal flexure that is a part of the Wind Mountain dome Mountain Psa SEA 5 Psa Ku LEVEL Qaf (fig. 2). The similarity in composition of the Wind and Deer Mountains intrusives suggests that they are SEA 0 6 7 petrologically related as well. The Wind Mountain dome cannot be traced east of the peak. The Wind LEVEL Ku 5000 FEET 13 5 Psa Psa 13 7 Mountain intrusive has been interpreted as a laccolithic intrusion (McLemore and others, 1996); howev- Ti Ph 1 South 3 Psa Ph Qaf 4 er, geologic and geophysical relations mapped during this and a previous study (Nutt and others, 1997) Ti 3000 4 Qaf argin 2 Qa 7 9 suggest that an alternative interpretation is justified. There is no evidence that sedimentary rocks floor ၧၤu Qaf 10 Qfy 21 Qfy the intrusion; all sedimentary host rocks are strongly deformed adjacent to the intrusion and dip steeply Py ၧၤ 3 4 7 Qaf u pၤ Qaf away from the peak. Foliation within the Wind Mountain intrusive defines a circular pattern that is SCALE IN MILES SEA Psa 23 LEVEL 10 4 6 Qfy mimicked by the enclosing sedimentary rocks. The aeromagnetic signature at Wind Mountain is the 5000 Psa 4 est-facing,of Pedernal faulted uplift m 5 8 strongest, most prominent magnetic anomaly in the Cornudas Mountains (Nutt and others, 1997) even W 14 Psa EXPLANATION 4 though topographically similar peaks are present; all other peaks are clearly floored by sedimentary 3000 Qc 12 13 rocks and, based on the magnetic signature, lack the lithologic mass of Wind Mountain. The Wind Ti Tertiary intrusive rock Ph Permian Hueco Fm. Qaf Qaf Mountain intrusive appears to be a steep-sided plug that extends downward to its intersection with a Ku Cretaceous sedimentary rock ၧၤu Pennsylvanian to Cambrian rock parent intrusive body that underlies the combined Wind-Deer Mountains anticlinal flexure. Hunt (1953) 16 Qa Psa Qaf SEA 7 described intrusive forms similar to Wind Mountain as bysmaliths. Psa Permian San Andres Fm. pၤ Precambrian rock 5 6 9 3 4 LEVEL An anticlinal, convex-northward upwarp is present north of Flat Top. The fold plunges west and Tqs Qa Qa Py Permian Yeso Fm. 12 Qfy 3 terminates near Alamo Mountain; on the east it appears to merge with and become a part of the Wind- West Qa Qfo 14 Qfy 15 Psa Deer Mountains anticline. A second anticlinal flexure is mapped southwest of Alamo Mountain; the fold Figure 2. Schematic fence diagram showing stratigraphic, structural, and intrusive relationships discussed in text. 10 Qaf can be traced southeast at least 7 mi (11 km) into Texas. Based on the direct correlation of anticlinal Qfy Qfo 21 Ti 2 Qaf Qaf 10 flexures and doming with known intrusive rocks, we suggest that these two additional upwarps are also 17 6 23 10 14 12 33 7 cored by igneous rocks. 15 4 Qaf Qaf Ph Synclines mapped in the Cornudas Mountains appear to be related to igneous intrusions as well. 4 Psa Qa 10 Tqs They occur as partial ring structures around Wind Mountain, as structural sags above and between bur- 10 11 ied intrusive bodies, and as paired anticline-syncline accommodation folds formed in response to dilation 16 25 Qfy Ph 13 8 of intruded sedimentary rocks. 106°00' 105°00' Qc Peaks in the map area other than Cornudas Mountain and Wind Mountain do not appear to be 7 48 Qfy 7 Psa
0 associated with strongly deformed sedimentary rocks. Alamo Mountain, San Antonio Mountain, Chatt- ° –992 3500 21 4 32 30' Qfy field Mountain, Black Mountain, and Flat Top are similar to one another in that they are concordant Qaf 9 Qa 16 –2500 22 4 Tqs Qaf and clearly sills or laccoliths, and, unlike Wind and Cornudas Mountains, they were injected into sedi- –1500 Qc T 6 mentary host rocks at or above the Permian-Cretaceous unconformity (fig. 2). San Antonio Mountain,
–500 9 235 IF 3000 –1000 500 2500 8 Qa Psa perhaps the only true laccolith of the Cornudas Mountains and only partly exposed in the south-central –2000 L Psa 19 2000 14 1000 8 Qao part of the map area, is floored by basal Cretaceous rocks (Kues and Lucas, 1993). Chattfield Moun- –3000 500 1500 Qfy 14 1 UP Qaf tain, at least on the north where exposed in the map area, also is underlain by flat-lying Cretaceous stra- –3500 Qaf 19 Ph 2000 5' Qfy 5' ta. Black Mountain, a multiple sill complex east of Wind Mountain, was emplaced in part directly above 2500 1000 15 Ph 6 850 3000 10 6 10 Ph the unconformity as well as higher in the Cretaceous section. The Flat Top sill is underlain by the San 12 10 8 Qc Py Qc Andres Formation; no Cretaceous rocks were observed on this peak. The stratigraphic position of the L Qaf 4 8 17 3 unconformity east of Flat Top (north of Wind Mountain) as well as on the west (beneath Alamo Moun- A Psa Qc Qaf tain) relative to the statigraphy at Flat Top suggests that the Flat Top sill was intruded along or very near 1664 N Psa Qfo Qa R Qfy the Permian-Cretaceous unconformity. E 5 Qc 8 Qfy The Alamo intrusion is perhaps the most complex of the stratigraphically higher intrusions (fig. 2). 1214 1935 D Qfy E 10 11 The intrusive body is discordant on the north where it probably intruded gently west-dipping limestones P 24 7 Qaf Qa 3 of the San Andres. Along the south and west base of the peak, Cretaceous rocks are exposed. Flow 481 1560 10 9 foliation within the intrusive is complex. On the north flank, foliation dips steeply north; midway Qaf between the north flank and the crest of the peak, foliation is gently inclined to the north. Directly Ph 5 Qa beneath the crest of the peak, the foliation steepens whereas at the crest the attitude of the foliation 5 Qa Qa Psa 4 NEW MEXICO Psa 13 again becomes nearly flat lying. The contemporary morphology of the peak, as viewed from the north- 32°00' Qa –2933 Qfy west, reflects the abrupt changes of foliation attitude. Hornfelsed Cretaceous rocks rest on the intrusion TEXAS 3 Py Psa 0 20 MILES Qao on its north side (shown as Km) suggesting that the present exposed upper surface of the igneous rocks 5 probably represents the exhumed upper contact of the intrusion. As such, Alamo Mountain appears to 2280 1232 Psa 16 Qfy 18 Qaf 0 20 KILOMETERS 14 represent a steeply inclined, thick, east-trending dike on the north where it intruded Permian strata. When the dike encountered the Permian-Cretaceous unconformity, it spread laterally to the south as a Qa 12 Qa Ph Figure 3. Structure contour map drawn on top of Precambrian basement showing location of buried Pedernal uplift concordant intrusion before it bulged, thickened, and folded overlying Cretaceous rocks; it then con- Qfy Qaf with respect to Cornudas Mountains (pink). Contour interval 500 ft; datum is mean sea level. Solid dot, well, Psa 8 21 18 cordantly invaded Cretaceous strata farther to the south before abruptly terminating at its present loca- Qaf showing depth. Dashed line, fault; bar and ball on downthrown side. Modified from King and Harder (1985). Qfy 8 tion. In a crude way, Alamo Mountain appears to represent an incompletely formed laccolith with its 4 Qc Psa 7 northern half undeveloped (fig. 2). Hunt (1953) did not describe an intrusive form quite like Alamo 12 Qa Qc 9 Mountain although he did suggest, following Daly (1914), that such an intrusive form could be called a Qc Qa Psa 9 Qao Qfy Qa chonolith. 105°40' 25 17 17
3 Faults 15 Qfy Ph Qaf Qa 12 11 40 Qc Qaf Qfy The Cornudas Mountains are near the western edge of the Salt Basin graben (fig. 1), which is the easternmost structure related to Basin and Range tectonism and shows evidence of Quaternary fault Qa Qaf 12 Psa Qaf Qc Qa movement (Goetz, 1980). In contrast, the Cornudas Mountains are cut by rare faults in which the offset 16 7 Qaf is typically 15 ft or less (4.6 m). Apparently the Cornudas Mountains are within a stable block bounded 12 Qfy 12 75 11 by segments of the late Cenozoic Rio Grande Rift to the west and east. Several of the small faults are Qa 24 18 Psa 12 3 6 Qao Qfy Qao 8 Qa intruded by dikes related to the larger intrusions of the area. We interpret the faults to have formed Psa Qaf 14 mainly in response to deformation of host sedimentary rocks during intrusion of alkaline rocks. Psa 9 5 13 5 Psa Qfy 17 5 10 17 Td PRE-PERMIAN FAULTING 6 4 Qaf Qaf Ph In Pennsylvanian time, New Mexico and adjacent Texas and Colorado were the sites of numerous Qaf Psa 3 59Qc 14 uplifted intracratonic basement blocks of the ancestral Rocky Mountains (Kluth and Coney, 1981). Py 25 Td Most of these uplifts and adjacent basins in New Mexico trended north; one of the larger crustal blocks, 17 44 3 18 10 9 Qaf Qc 15 16 9 3 the Pedernal uplift, can be traced on the surface from central New Mexico southward into the Sacramento Mountains in eastern Otero County (fig. 1). From the Sacramento Mountains southward, Qfy 9 Qc Td Qa 16 the uplift is buried beneath Permian rocks that now underlie the Otero platform. Basement faulting, Psa 78 Psa Qaf Qaf 80 11 9 Psa stratigraphic pinchouts, and syntectonic sedimentary deposits associated with the uplift are best exposed 5 Qfy Psa Qc in the Sacramento Mountains near Alamogordo, N. Mex. (Pray, 1959; Kottlowski, 1963; Bauer and Lozinsky, 1991). To the south, similar geologic features associated with the uplift have been detected in 12Qfy 13 Qaf 20 6 10 exploratory oil wells drilled on the Otero platform (Black, 1975). 18 Qfy Psa 12 Qaf Structure contours drawn on the top of the buried Precambrian of the Otero platform indicate that Qfy Tas Qaf 5 Qaf 12 Qa Psa the Cornudas Mountains are located near the western edge of the buried Pedernal uplift (Woodward and 4 16 others, 1975; Foster, 1978; King and Harder, 1985). Geologic cross sections drawn across the Otero 12 11 Tp 14 16 platform by Black (1975), particularly his section C–C’ drawn through the northern part of the Cornu- Psa Td 16 Tas das Mountains, show the beveled top of the buried pre-Permian uplift. In section C–C’, the well drilled Psa 2 Qc Qaf Qfo Ti 13 east of the Cornudas bottomed in Permian strata resting directly on Precambrian rocks at 2,280 ft (684 20 12 Py Qfy Psa 11 Kc Qaf Qt m) above sea level; the well on the west penetrated Permian as well as older Paleozoic rocks and Qfo Tas Qfy encountered Precambrian basement nearly 2,000 ft (600 m) lower, at an elevation of 481 ft (145 m) Qt Kma Qt Qa Qaf (King and Harder, 1985). The faulted, western edge of the Pedernal uplift, as shown by Black, is locat- 7 15 Qc ed between these two wells; in this cross section the Cornudas Mountains are shown as laccolithic intru- Td 2'30" 8 Psa Qa 6 Tps 2'30" sions localized along a minor fault located about 2 mi (3.5 km) west of the faulted edge of the uplift. Qa Tps Qfy Ti Qao Qa Geologic mapping and geophysical investigations conducted by Nutt and others (1997) suggest Tp 4 Kc Kc that the western, faulted edge of the Pedernal uplift lies beneath or west of the Cornudas Mountains. Qls 3 Qa 25 Qao Psa 43 Qfy Kc Kma 8 Geologic evidence for the location of the buried uplift margin is derived from regional variations in the Qls thickness of the Permian Yeso Formation. In the Cornudas Mountains, the Yeso is only 100 ft (30.5 8 Qt Qt Tas 3 Ph Psa QTp Qt Kma Qc Qa m) thick. In cross sections constructed by Black (1975, C–C’), exploratory oil wells drilled 10 mi (16 12 Qt Qa QTp Qa QTp 8 4 km) east and 5 mi (8 km) northwest of the Cornudas encountered a much thicker Yeso: about 850 ft QTp Kc 3 7 Qt Qfy 14 Qfo (255 m) thick on the east and nearly 900 ft (270 m) thick on the west (King and Harder, 1985). The 12 4 Ph Tps Qt Qfy Qt explanation for this anomalously thin Yeso section is speculative. The Yeso is exposed only as upturned Qls Qfy Kc 6 Py Psa Qfo QTp strata between the Hueco and San Andres around the Wind and Deer Mountains and Cornudas Moun- 12 Qfy Psa 24 28 Kma Qaf 7 Psa 15 Psa tain intrusive centers. Given that gypsum flows at the slightest provocation and is also quite soluble, it is Tp 3 Qaf 7 7 52 9 Qt 37 3 7 12 Qls possible that the thinness of the formation is the result of deformation related to intrusion and (or) disso- Tp lution due to magmatic fluids. Arguing against such an interpretation is the noticeable lack of strong Km Qt Qfy 9 Ph 50 Ph 9 Qfo 8 folding, contorted bedding, and brecciation of the Yeso and the overlying San Andres and the paucity of 27 Td 16 Py Td 10 28 13 Qt evidence of magmatic fluids. Alternatively, thinning of the Yeso to about 100 ft (30.5 m) in the Cornu- Td Qls 8 Tp das Mountains may likely be due to abrupt gradation and intertonguing with the overlying San Andres 11 Qc Qa Qt 15 8 14 16 4 (see Black, 1975, p. 328–329); equally likely is the possibility that the formation pinches out against, 16 4 24 7 3 Td Ph QTp over, and across an elevated Precambrian high—the uplifted Pedernal massif. Abrupt thickening of the
20 6 65 Qt Kma Yeso to the west, and the fact that the entire Cambrian through Pennsylvanian section (encountered in Kc 4 Ph the wildcat well) rests directly on Precambrian rocks that are nearly 2,000 ft (600 m) deeper than to the Qfy 12 26 5 23 Ph 62 east of the Cornudas Mountains, suggest that the major west-bounding fault of the Pedernal uplift is Qca Qca Psa 6 Psa Kc more correctly interpreted to be located west of or beneath the Cornudas Mountains. Tns 23 Tns1 QTp 10 Qfy Qfy 9 Geophysical evidence for an abrupt change in the character of the subsurface rocks lies in aero- 7 Psa Qls 65 Tns2 Ts Qt magnetic anomalies and audio-magnetotelluric (AMT) soundings conducted across the Cornudas Moun- Qls Qaf Ph 50 23 46 5 tains (Nutt and others, 1997). The intrusive rocks in the subsurface of the Cornudas Mountains appear Qfy 11 29 Psa 18 3 Qa Ph 11 4 to be concentrated at or near the unconformity between the sedimentary rocks and the underlying Pre- Qfy Psa 26 Py 7 Qao 74 65 Qao cambrian crystalline basement. That unconformity is interpreted from the aeromagnetic data to be 12 about 2,200 ft (660 m) beneath the surface and at an elevation of about 3,000 ft (900 m) above sea Qls 33 11 Qfo 15 Py Qc 42 level. Similarly, ATM soundings detected highly resistive rocks directly east of the Cornudas Mountains 4 52 Qaf 11 10 Qao that contrast markedly with a layered rock sequence detected on the west. The interpretation offered Qc Psa 17 Tns 14Qc 3 36 here is that the Precambrian basement is much nearer the surface directly east of the Cornudas Moun-