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Tectonic Style and Deformational Environment in the Eagle ...

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TECTONIC STYLE AND DEFORMATIONAL ENVIRONMENT 125<br />

Many of <strong>the</strong> relatively small imbricate thrust slices <strong>in</strong> <strong>the</strong> Indio<br />

Mounta<strong>in</strong>s appear to have moved southwestward as counterthrusts.<br />

This should not be surpris<strong>in</strong>g. A homogeneous mass<br />

undergo<strong>in</strong>g nor<strong>the</strong>ast-southwest compression might be expected<br />

to fail equally along southwest dipp<strong>in</strong>g or nor<strong>the</strong>ast dipp<strong>in</strong>g fractures<br />

(DeFord, 1958). That most of <strong>the</strong> faults orig<strong>in</strong>ally dipped<br />

southwest may be <strong>the</strong> result of <strong>in</strong>homogeneities <strong>in</strong> <strong>the</strong> rocks, irregularities<br />

<strong>in</strong> <strong>the</strong> underly<strong>in</strong>g basement, <strong>and</strong>/or marked th<strong>in</strong>n<strong>in</strong>g of<br />

<strong>the</strong> late Paleozoic <strong>and</strong> Mesozoic rocks from southwest to nor<strong>the</strong>ast.<br />

Because of later fold<strong>in</strong>g, dips of <strong>the</strong> fault planes are now<br />

nor<strong>the</strong>ast to east-nor<strong>the</strong>ast.<br />

Folds, for <strong>the</strong> most part, are open <strong>and</strong> symmetrical (Horse Peak<br />

anticl<strong>in</strong>e <strong>and</strong> Lost Valley syncl<strong>in</strong>e), but <strong>the</strong> vertical- to near-vertical<br />

rocks <strong>in</strong> Bramblett Ridge are <strong>the</strong> strik<strong>in</strong>gly exposed steep southwest<br />

limb of a north-northwest-trend<strong>in</strong>g syncl<strong>in</strong>e (fig. 2).<br />

Thus, <strong>the</strong> Indios are characterized by complex thrust faults <strong>and</strong><br />

mostly open, symmetrical folds. Impr<strong>in</strong>ted on <strong>the</strong>se are major normal<br />

faults: <strong>the</strong> Indio fault along <strong>the</strong> axis of <strong>the</strong> mounta<strong>in</strong>s <strong>and</strong> <strong>the</strong><br />

unnamed bound<strong>in</strong>g fault along <strong>the</strong> west marg<strong>in</strong> of <strong>the</strong> Indio Mounta<strong>in</strong>s<br />

(fig. 3).<br />

The Mesozoic rocks of <strong>the</strong> <strong>Eagle</strong> Mounta<strong>in</strong>s are largely covered<br />

by a thick sequence of volcanic rock which masks many of <strong>the</strong><br />

details of folds <strong>and</strong> thrust faults of Laramide age. The Devil Ridge<br />

thrust fault, for example, cannot be traced with certa<strong>in</strong>ty through<br />

<strong>the</strong> <strong>Eagle</strong>s, although a number of thrust faults have been mapped<br />

<strong>the</strong>re<strong>in</strong> (Underwood, 1963). The ma<strong>in</strong> part of <strong>the</strong> mounta<strong>in</strong>s appears<br />

to be rest<strong>in</strong>g <strong>in</strong> <strong>the</strong> trough of a large syncl<strong>in</strong>e (Gillerman,<br />

1953), which may be <strong>the</strong> result of subsidence follow<strong>in</strong>g extrusion<br />

of a vast quantity of volcanic rock.<br />

The east- to east-nor<strong>the</strong>ast-strik<strong>in</strong>g faults are significant structural<br />

features of <strong>the</strong> <strong>Eagle</strong> Mounta<strong>in</strong>s (Underwood, 1963). These faults<br />

may well have developed dur<strong>in</strong>g <strong>the</strong> period of Laramide compression<br />

as one of a possible set of conjugate shear fractures, with<br />

dom<strong>in</strong>ant strike-slip motion. Reorientation of <strong>the</strong> stress field produced<br />

vertical movement dur<strong>in</strong>g <strong>the</strong> late Tertiary episode of Bas<strong>in</strong><br />

<strong>and</strong> Range block fault<strong>in</strong>g when some of <strong>the</strong> early to mid-Tertiary<br />

igneous rocks were offset. A similar history of movement is<br />

recognized along <strong>the</strong> Red Bull fault zone <strong>in</strong> <strong>the</strong> sou<strong>the</strong>rn Quitman<br />

Mounta<strong>in</strong>s (Jones <strong>and</strong> Reaser, 1970).<br />

The Speck Ridge-Black Butte area (fig. 4), on <strong>the</strong> northwest flank<br />

of <strong>the</strong> <strong>Eagle</strong>s, is a complexly folded <strong>and</strong> faulted area from which<br />

once-cover<strong>in</strong>g volcanic rocks have been eroded. The folds are<br />

Figure 2. Nor<strong>the</strong>rn Indio Mounta<strong>in</strong>s; northwestward view of<br />

Bramblett Ridge, composed of near-vertical beds of Bluff Limestone;<br />

<strong>Eagle</strong> Bluffs, Upper Rhyolite, <strong>in</strong> background.<br />

Figure 3. Sou<strong>the</strong>rn Indio Mounta<strong>in</strong>s; northwestward view along<br />

western boundary fault; Red Light bolson fill, left; Yucca Formation,<br />

right; Red Mounta<strong>in</strong>, right skyl<strong>in</strong>e; <strong>Eagle</strong> Mounta<strong>in</strong>s, left <strong>and</strong><br />

distant skyl<strong>in</strong>e.<br />

open <strong>and</strong> symmetrical but are offset along transverse strike-slip<br />

faults or along normal faults parallel to <strong>the</strong> fold axes.<br />

In Devil Ridge <strong>the</strong> pr<strong>in</strong>cipal deformation was <strong>the</strong> nor<strong>the</strong>astward<br />

movement of two imbricate thrust blocks, <strong>the</strong> Red Hills <strong>and</strong> <strong>the</strong><br />

Devil Ridge blocks. With <strong>the</strong> exception of <strong>the</strong> anticl<strong>in</strong>e overturned<br />

to <strong>the</strong> nor<strong>the</strong>ast that forms much of Back Ridge, folds <strong>the</strong>re mostly<br />

are open <strong>and</strong> symmetrical.<br />

Love Hogback (fig. 5) is part of <strong>the</strong> Devil Ridge thrust block; <strong>the</strong>re<br />

<strong>the</strong> oldest exposed Cretaceous rock <strong>in</strong> <strong>the</strong> immediate area, <strong>the</strong><br />

Yucca Formation, rests on <strong>the</strong> youngest exposed Cretaceous rock,<br />

<strong>the</strong> Chispa Summit. Stratigraphic separation is about 2,400 m; estimated<br />

horizontal movement along both <strong>the</strong> Red Hills <strong>and</strong> Devil<br />

Ridge thrust faults totals 5,800 m (Underwood, 1963).<br />

In <strong>the</strong> Devil Ridge area, <strong>the</strong> orientation of <strong>the</strong> greatest pr<strong>in</strong>cipal<br />

stress dur<strong>in</strong>g <strong>the</strong> Laramide orogeny was nor<strong>the</strong>ast-southwest. The<br />

more easterly orientation of <strong>the</strong> greatest pr<strong>in</strong>cipal stress <strong>in</strong> <strong>the</strong> Indio<br />

Mounta<strong>in</strong>s was <strong>the</strong> result of local irregularities <strong>in</strong> <strong>the</strong> stress<br />

field. These, <strong>in</strong> turn, reflected <strong>the</strong> <strong>in</strong>fluence of such diverse factors<br />

as <strong>the</strong> configuration of <strong>the</strong> basement, size <strong>and</strong> shape of <strong>the</strong> body<br />

•<br />

Figure 4. Aerial view northward of Black Butte, right center,<br />

capped by dark-colored Trachyte Porphyry. In near foreground,<br />

F<strong>in</strong>lay Limestone <strong>and</strong> Cox S<strong>and</strong>stone <strong>in</strong> sou<strong>the</strong>astern part of Speck<br />

Ridge. Left background, sou<strong>the</strong>ast-plung<strong>in</strong>g anticl<strong>in</strong>e of F<strong>in</strong>lay<br />

Limestone; right background, Roof Garden.<br />

Ew

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