Presentation is loading. Please wait.

Presentation is loading. Please wait.

 Angelique Northcutt, Garrett Owen, Chris Perdue, Bo Price, Tory Rogers Geology of the Precambrian Sangre De Cristo Range and Picuris Mountains of New.

Similar presentations


Presentation on theme: " Angelique Northcutt, Garrett Owen, Chris Perdue, Bo Price, Tory Rogers Geology of the Precambrian Sangre De Cristo Range and Picuris Mountains of New."— Presentation transcript:

1  Angelique Northcutt, Garrett Owen, Chris Perdue, Bo Price, Tory Rogers Geology of the Precambrian Sangre De Cristo Range and Picuris Mountains of New Mexico

2 Where are we going?

3 -The Sangre de Cristo fault is a west dipping fault in New Mexico -It forms the border between the Sangre de Cristo Mountains and the San Luis Basin. -The Sangre de Cristo fault extends from poncho Pass, Colorado to near where we’ll be in Taos, NM. Background

4 - -The section we will be focused on extends from the San Pedro Mesa creek south to the intersection with the Embudo Fault at Rio del Rancho which is about 8 km south of Taos. -The Sangre de Cristo is part of the more recent Rio Grande Rift. -It is a normal fault that moves less than 0.2 mm/year. Background

5 -The Basement rocks in this location are Precambrian in age. -The rocks of Colorado and Northern New Mexico are juvenile Volcanic- Plutonic, Ocean Arc rocks that are approximately 1.78 to 1.65 billion years old. -In New Mexico these rocks have been assigned to the Yavapi and Mazatzal provinces. - These Rocks were deformed during 2 major Proterozoic orogenies. History

6 -First the Colorado Orogeny has a U-Pb date that goes through Ga. -It was a prolonged thermotectonic episode resulting from collision, subduction, and continued convergence. -This occurred along the paleosuture known as the Cheyenne Belt along the Archean Wyoming Province. History

7 -Second the Berthoud Orogeny has a U-Pb date that started 1.45 Ga and went through 1.40 Ga. -This was a thermo tectonic episode that produced NE trending ductile shear zones and related folds. -The mechanism powering this Orogeny was granitic plutonism. -This Orogeny also formed many high grade metamorphic rocks through generally pervasive metamorphism. History

8 -Isoclinal folding -East-west strike -Southward dips (60-70 degrees) Pre-Cambrian rocks

9 -2 major anticlines and 2 major synclines -Wave lengths 1 to 2 miles -Doubly plunging (~20-30 degrees) Folds

10 Pilar Anticline -Widely displaced by the Pilar-Vadito tear fault -Widely displaced by the Pilar-Vadito tear fault -Slightly overturned to the north -Slightly overturned to the north -Axial plane dipping south (60 degrees) -Axial plane dipping south (60 degrees) Hondo Syncline Hondo Syncline -Overturned -Overturned -Axial plane dips south (60-70 degrees) -Axial plane dips south (60-70 degrees) -Eastern segment plunges 30-40W -Eastern segment plunges 30-40W -Western segment plunges 10-20E -Western segment plunges 10-20E Folds

11 Copper Hill Anticline -Axial plane plunges 30-35W -Axial plane plunges 30-35W -N85W, 50W -N85W, 50W -Can be traced 9 miles east of Copper Hill -Can be traced 9 miles east of Copper Hill Harding Syncline -Structural detail is obscure -Structural detail is obscure -Strikes E-W -Strikes E-W -Plunge ranges 25-17NE -Plunge ranges 25-17NE Folds

12 -Abundant/wide variability in pre-Cambrian rocks -3 predominant sets -N10W to N10E (almost vertical) -N10W to N10E (almost vertical) -N50W to N70W (dipping steeply NE) -N50W to N70W (dipping steeply NE) -N20E to N40E (dipping steeply SE) -N20E to N40E (dipping steeply SE) Jointing

13 -N-S joints followed almost exclusively by copper ore-bearing quartz veins -Mineralization after granitic intrusion intrusion -Harding pegmatite estimated 800myo -Indicates time of jointing Jointing

14 -Conglomerate of the Vadito -Pebbles have average axial ratio of 1:2:3 -Pebbles have average axial ratio of 1:2:3 -Shortest axis perpendicular to foliation -Some wedge-like shaped with apex oriented down the lineation -Pebbles in close contact have greater impacted shape Stretched Pebbles

15 Three Major Fault Systems Picuris-Pecos fault system Picuris-Pecos fault system Embudo transfer fault Embudo transfer fault Sangre de Cristo fault zone Sangre de Cristo fault zone

16 Picuris-Pecos Fault System 84 km long fault system consisting of five parallel fault zones: Picuris-Pecos - Major crustal boundary juxtaposing two Proterozoic rock sequences: the Hondo Group and the Miranda Granite Picuris-Pecos - Major crustal boundary juxtaposing two Proterozoic rock sequences: the Hondo Group and the Miranda Granite La Serna La Serna -East-down fault separating Miranda Granite and Picuris Formation Miranda Miranda -North-striking strike slip fault McGaffey McGaffey -West-down branching fault splay Rio Grande del Rancho Rio Grande del Rancho -Kilometer-wide, west-down fault zone

17 Embudo Fault Zone Sinistral, antithetic transfer zone which forms border between the Española Basin and the San Luis Basin Sinistral, antithetic transfer zone which forms border between the Española Basin and the San Luis Basin 64 km long fault thought to be part of Jemez lineament 64 km long fault thought to be part of Jemez lineament Fault consists of two sections based on reversal of throw Fault consists of two sections based on reversal of throw Strike of N60E Strike of N60E Sinistral net slip rate of.15 mm/year Sinistral net slip rate of.15 mm/year

18 Sangre de Cristo Fault Zone West-dipping normal fault that forms border between the Sangre de Cristo Mountains and the San Luis Basin West-dipping normal fault that forms border between the Sangre de Cristo Mountains and the San Luis Basin Beginning of Sangre de Cristo Fault forms the terminus of the Embudo fault Beginning of Sangre de Cristo Fault forms the terminus of the Embudo fault The southern area of the fault is divided into five sections. From north to south, the sections are: - San Pedro Mesa - Urraca - Questa The southern area of the fault is divided into five sections. From north to south, the sections are: - San Pedro Mesa - Urraca - Questa  The northern three strike north-south - Hondo - Hondo  Strikes N30W - Cañon - Cañon  Strikes N20E

19 Aerial View of Faults in Taos Region

20 The Hondo Group -The Pilar Formation -The Riconada Formation -The Ortega Formation The Vadito Formation Pre-Cambrian Formations:

21 The Ortega Formation Estimated 2,500 ft. thick Gray to very light gray in color Mostly Quartzite Thin beds of sillmanite - kyanite gneiss Bands of schistose with muscovite Tourmaline

22 Riconada Formation -Richly micaceous foliated rocks -Consists of four distinct beds: Andalusite-biotite Hornfels bed- Muscovite and quartz matrix that contains biotite, nodular masses of quartz and andalusite Staurolite Schist and Gneiss Bed- Soft and light gray in color micaceous matrix speckled with biotite, contains staurolite crystals Staurolite Andalusite

23 The Riconada Formation Quartzite bed – Grayish white in color, contains glassy- white and translucent quartzite Muscovite-quartz-biotite-garnet Phyllite bed- Muscovite rich phyllite containing garnet crystals and biotite, sheen that ranges from pearly gray to greenish

24 Pilar Phyllite Formation Estimated 2,300 ft. thick Black to gray-black in color with a gray sheen Contains muscovite flakes Quartz veins Limonite masses

25 Occupies the southern 1/3 of the Picuris Range Occupies the southern 1/3 of the Picuris Range -Named after the village of Vadito -Named after the village of Vadito Best outcrops come from within a one-mile radius of the Harding Mine Best outcrops come from within a one-mile radius of the Harding Mine -Total thickness: 4,500 feet -Total thickness: 4,500 feet Comprised of a Lower Conglomerate Member and an Upper Schist Member Comprised of a Lower Conglomerate Member and an Upper Schist Member Vadito Formation

26 Marquenas Formation Total thickness: ~ 2,000 feet Total thickness: ~ 2,000 feet Composed of Quartz Conglomerate and Quartzite, Felsites and Meta-andesites Composed of Quartz Conglomerate and Quartzite, Felsites and Meta-andesites Quartz conglomerate outcrops in a quarter-mile wide east-west belt near Picuris Canyon but grow sparser farther east Quartz conglomerate outcrops in a quarter-mile wide east-west belt near Picuris Canyon but grow sparser farther east Composed of gray coarse to pebbly Quartzite with fine-grained micaceous quartzite matrix Composed of gray coarse to pebbly Quartzite with fine-grained micaceous quartzite matrix Thickness of the Quartz Conglomerate: ,000 feet Thickness of the Quartz Conglomerate: ,000 feet

27 Marquenas Formation Felsites occur to the east and west of the canyon but appear to pinch out to the west along the Ortega-Vadito contact Felsites occur to the east and west of the canyon but appear to pinch out to the west along the Ortega-Vadito contact Composed of meta-rhyolite that grades into coarser granite representing partial replacement by granite Composed of meta-rhyolite that grades into coarser granite representing partial replacement by granite Gray-white to pink-white and has a dense felsitic texture with micas and feldspars present Gray-white to pink-white and has a dense felsitic texture with micas and feldspars present Thickness of the Felsites: feet Thickness of the Felsites: feet

28 Marquenas Formation Meta-andesites occur abundantly to the south and east of the Harding mine Meta-andesites occur abundantly to the south and east of the Harding mine Greenish-gray to gray-black in color Greenish-gray to gray-black in color Hornblende occurs in all of these rocks as prisms and give the variable darkness in color to them Hornblende occurs in all of these rocks as prisms and give the variable darkness in color to them Rocks show strong pleochroism in thin-section. Rocks show strong pleochroism in thin-section. Represent thin-layered volcanic material of dacitic and andesitic composition Represent thin-layered volcanic material of dacitic and andesitic composition

29 Schist Member Consists of a schist and phyllite composed of quartz-muscovite and a quartz-biotite granulite Consists of a schist and phyllite composed of quartz-muscovite and a quartz-biotite granulite The schist is similar to the underlying conglomerate quartzite with more densely disseminated flakes of muscovite The schist is similar to the underlying conglomerate quartzite with more densely disseminated flakes of muscovite Phyllite is a lustrous, silvery-gray rock with stubby biotite porphyroblasts Phyllite is a lustrous, silvery-gray rock with stubby biotite porphyroblasts Granulite is fine-grained, sandy, and crudely foliated with micaceous surfaces with flakes of biotite Granulite is fine-grained, sandy, and crudely foliated with micaceous surfaces with flakes of biotite Thickness: At least 1,250 feet and no more than 2,500 feet Thickness: At least 1,250 feet and no more than 2,500 feet

30 Amphibolites The amphibolites found in the Vadito Formation are split into two zones based on lithology: The amphibolites found in the Vadito Formation are split into two zones based on lithology: -One of the zones occurs in the Lower Conglomerate and one occurs in the Upper Schist -One of the zones occurs in the Lower Conglomerate and one occurs in the Upper Schist These amphibolites show effects of intrusion by granitic and pegmatitic magma These amphibolites show effects of intrusion by granitic and pegmatitic magma Thickness: 750 feet in Lower Conglomerate, and 1,250 feet in Upper Schist Thickness: 750 feet in Lower Conglomerate, and 1,250 feet in Upper Schist

31 Questions?


Download ppt " Angelique Northcutt, Garrett Owen, Chris Perdue, Bo Price, Tory Rogers Geology of the Precambrian Sangre De Cristo Range and Picuris Mountains of New."

Similar presentations


Ads by Google