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Synthesis of late Paleozoic and Mesozoic eolian deposits of the ...

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30<br />

Blakey (1986) documented <strong>the</strong> presence <strong>of</strong> small<br />

<strong>eolian</strong> dunes <strong>and</strong> sabkha <strong>and</strong>/or wet interdune<br />

<strong>deposits</strong> for this facies.<br />

The Coconino S<strong>and</strong>stone formed downwind<br />

from eroding <strong>eolian</strong> <strong>and</strong> marine rocks to <strong>the</strong> north.<br />

Reworked <strong>eolian</strong> s<strong>and</strong> moved southward across<br />

<strong>the</strong> featureless terrain <strong>of</strong> central <strong>and</strong> nor<strong>the</strong>rn<br />

Utah until it encountered an area <strong>of</strong> subsidence<br />

associated with <strong>the</strong> last stages <strong>of</strong> <strong>the</strong> Holbrook<br />

Basin. Some areas in <strong>the</strong> Mogollon Rim were close<br />

enough to marine areas to <strong>the</strong> south to form<br />

interbedded sabkha <strong>and</strong> coastal dune <strong>deposits</strong>.<br />

However, most <strong>of</strong> <strong>the</strong> Coconino <strong>and</strong> at least some<br />

<strong>of</strong> <strong>the</strong> Glorieta were deposited in an inl<strong>and</strong> erg far<br />

removed from direct marine influence as shown by<br />

a dominance <strong>of</strong> <strong>deposits</strong> formed by large dunes<br />

with few wet interdune <strong>deposits</strong>.<br />

Leonardian 111 <strong>eolian</strong> <strong>deposits</strong><br />

The <strong>late</strong>st Leonardian ergs, possibly partially<br />

Guadalupian in age occur in widely separated<br />

areas <strong>of</strong> <strong>the</strong> Colorado P<strong>late</strong>au <strong>and</strong> north-central<br />

Colorado. Correlation <strong>of</strong> <strong>the</strong>se two <strong>eolian</strong> com-<br />

plexes is considered somewhat tentative but is<br />

based on relations with adjacent marine rocks <strong>and</strong><br />

regional correlation as shown by Rascoe <strong>and</strong> Baars<br />

(1972). The White Rim S<strong>and</strong>stone <strong>and</strong> upper<br />

Coconino S<strong>and</strong>stone form <strong>the</strong> western erg <strong>deposits</strong><br />

<strong>and</strong> <strong>the</strong> Lyons S<strong>and</strong>stone forms <strong>the</strong> eastern one<br />

(Fig. 11). Eolian <strong>deposits</strong> have also recently been<br />

identified to <strong>the</strong> east in <strong>the</strong> Leonardian <strong>and</strong><br />

Guadalupian <strong>of</strong> west Texas <strong>and</strong> adjacent New<br />

Mexico (Nance, this volume). At present it is<br />

uncertain as to how <strong>the</strong>se <strong>deposits</strong> re<strong>late</strong>d to <strong>the</strong><br />

major erg systems to <strong>the</strong> west. The Lyons S<strong>and</strong>-<br />

stone was carefully documented to be <strong>of</strong> <strong>eolian</strong><br />

origin by Walker <strong>and</strong> Harms (1972). Stratigraphic<br />

relations were provided by Thompson (1959) <strong>and</strong><br />

Hoyt (1963). The Lyons forms a parabolic-shaped<br />

deposit in which <strong>the</strong> trough <strong>of</strong> <strong>the</strong> parabola trends<br />

east-nor<strong>the</strong>ast (Fig. 11). The center <strong>of</strong> <strong>the</strong> unit is<br />

about 60 m thick. To <strong>the</strong> north <strong>the</strong> Lyons inter-<br />

tongues with marine carbonate <strong>and</strong> sabkha red-<br />

beds <strong>of</strong> <strong>the</strong> Owl Canyon <strong>and</strong> Satanka Formations<br />

(Figs. 2 <strong>and</strong> 7B). Eastward <strong>and</strong> sou<strong>the</strong>astward it<br />

grades into marine carbonates <strong>and</strong> redbeds <strong>and</strong><br />

southwestward it intertongues with <strong>the</strong> upper<br />

Fountain Formation. The west edge <strong>of</strong> <strong>the</strong><br />

parabola is truncated by <strong>the</strong> present-day Front<br />

Range, though it seems probable that <strong>the</strong> Lyons<br />

once extended several tends <strong>of</strong> kilometers west<br />

across <strong>the</strong> edge <strong>of</strong> <strong>the</strong> Ancestral Front Range.<br />

The White Rim <strong>and</strong> upper Coconino S<strong>and</strong>stone<br />

complex is confined to <strong>the</strong> west <strong>of</strong> <strong>the</strong> Sedona <strong>and</strong><br />

Monument Arches <strong>and</strong> extends from central Utah<br />

to <strong>the</strong> Mogollon Rim in Arizona. Sedimentologic<br />

data are provided by Baars <strong>and</strong> Seager (1970),<br />

Rawson <strong>and</strong> Turner-Peterson (1980), <strong>and</strong> Kamola<br />

<strong>and</strong> Chan (this volume). Stratigraphic data are<br />

provided by Irwin (1976) as well as <strong>the</strong> above<br />

authors. The eastern fea<strong>the</strong>r edge <strong>of</strong> <strong>the</strong> White<br />

Rim follows <strong>the</strong> present course <strong>of</strong> <strong>the</strong> Colorado<br />

River southward into Arizona; however, in Arizona<br />

<strong>the</strong> upper Coconino extends eastward to an area<br />

across <strong>the</strong> Sedona Arch where it can no longer be<br />

separated from <strong>the</strong> lower Coconino <strong>and</strong> is <strong>the</strong>re-<br />

fore included with it on Fig. 10. The White Rim<br />

S<strong>and</strong>stone averages about 60 m in thickness across<br />

much <strong>of</strong> its extent but thickens to over 250 m in<br />

<strong>the</strong> Circle Cliffs trough (Figs. 7D <strong>and</strong> 10). Baars<br />

<strong>and</strong> Seager (1970) pointed out that <strong>the</strong> eastern<br />

margin is not a true fea<strong>the</strong>r edge but ra<strong>the</strong>r <strong>the</strong><br />

unit thins to less than 10 m <strong>and</strong> grades eastward<br />

into redbeds <strong>of</strong> <strong>the</strong> Organ Rock Formation. In<br />

some areas this edge has been modified by pre-<br />

Triassic erosion. The White Rim <strong>and</strong> upper<br />

Coconino everywhere grade westward through a<br />

zone <strong>of</strong> complex facies change into marine<br />

carbonate <strong>and</strong> sabkha evaporite <strong>and</strong> s<strong>and</strong>stone <strong>of</strong><br />

<strong>the</strong> Toroweap Formation (Fig. 7D <strong>and</strong> E). This<br />

change is well documented by Irwin (1976) <strong>and</strong><br />

Rawson <strong>and</strong> Turner-Peterson (1980). The facies<br />

change follows <strong>the</strong> west edge <strong>of</strong> <strong>the</strong> Sedona Arch<br />

from <strong>the</strong> Mogollon Rim northward to near Page,<br />

Arizona <strong>and</strong> <strong>the</strong>n swings northwestward along <strong>the</strong><br />

Kaibab Arch; <strong>the</strong>n it swings back to <strong>the</strong> nor<strong>the</strong>ast<br />

near <strong>and</strong> parallel to <strong>the</strong> west edge <strong>of</strong> <strong>the</strong> Colorado<br />

P<strong>late</strong>au (Fig. 11). The White Rim S<strong>and</strong>stone is<br />

truncated by erosion along <strong>the</strong> northwest-trending<br />

Emery Arch in central Utah (Rascoe <strong>and</strong> Baars,<br />

1972; Irwin, 1976).<br />

We have field-checked some <strong>of</strong> <strong>the</strong> reports <strong>of</strong><br />

intertonguing <strong>of</strong> <strong>the</strong> White Rim <strong>and</strong> upper<br />

Coconino with <strong>the</strong> overlying Kaibab Formation.<br />

In areas that we have field checked, we have not

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