n Alas - Alaska Division of Geological & Geophysical Surveys - State ...
n Alas - Alaska Division of Geological & Geophysical Surveys - State ... n Alas - Alaska Division of Geological & Geophysical Surveys - State ...
hleam&gnetie latitude of Paleocene volcanic K&S of the Cantwell Pwmatim, central Alaska The Cantwell basin in the central Alaska Range consists of the Cantwell Formation, which include, in its upper part, calc-alkaline volcanic rocks and intru- slve rocks (the Teklanika Formation of Gilbert and others, 1976). Figure 50 shows the present distribu- tions of the voIcanic and sedimentary rocks of the Cantwell Formetion. Potassium-argon ages deter mined from the extrusive and intrusive rocks, which range from 41.8 to 60.6 rn.y., are considered to be minimum ages at least in part (Hickman, 1974; Gilbert and others, 1976). These ages accord with the Paleo- cene age of plant fossils in the Cantwell Formation (Wolfe and Wahrhaftig, 1070; Wolfe, 1972). The entire n Cantwell Formation has been extensively folded and faulted, and local angular unconformities occur be- tween the volcsllic and sedimentary rocks. We collected paleomagnetic samples at 19 sites (area 10, fig. 44; fig. 50); each site is a separate lava flow or welded tuff and is represented by eight Sam- pla. Except for site 17, which was completely remag- netized by Lightning, the pdeornagnetic data are of high quality. The structural dips at the various locali- ties, which range from 21' to 54O, provide an excellent test of whether the rnegnetfzation in the rocks was acquired before thelr deformation. The angular stan- dard deviation of the 18 mean onsite directions is; 29.4'; after restoration of the bedded rocks to the original horizontal by rotation around the strike, this angular standard deviation is reduced to 12.4'~ which is a typical value representing geomagnetic secular variation. We conclude that the natural magnetization / 0 25 KILOMETERS 4' I I I 1 I I . / I Volcanic rocks Contact-Approximately located Cantwell Fornation -... fault-Dotted where concealed Sedimentary rocks .15-19 Sample site and sample numbers Plgure SO.--Cantwell besin area, showing locations of pleomagnetic sampling sites (dots) in volcanic rocks of the Cantwell Formation. Pre-Tertiary and pat-Paleouene rocks we not differentiated. Geology from Jones and others (1983).
in the 18 lava flows b thermoremanent magnetization acquired during initial cooling. A11 the lavas exhibited reversed polarity, as is appropriate for their age be- cause Peleocene time was dominated by periods of reversed geomagnetic pohrity (Ness and others, 1980). The paleornagnetic inglinations in these rocks range from -65.8' to -87.6 , and the paleomapetic pole calculated from the 18 sites (pole I ,gig. 51) is close to northwestern Alaska at lat 70.0 N., long 165.4' W., with e 95-percent-confidence radius of 10.0'. Figure 51 compares this pole with Cretrceous and Paleocene poles from aratonic North America. Somewhat surprisingly, the Cantwell pole is much closer to the Cretaceous reference pole (135-78 m.y. B.P.) than to the Paleocene reference pole (67-61 m.y. B.P.). This difference could be accounted for if the CantweU volcanic rocks were, in fact, slightly older than the age range of the Paleocene reference because the interval from latest Cretaceous to early Paleocene was a time of rapid apparent polar wander for the North American craton. The paleomagnetic latitude of the CantweU, calculated according to the improved rnethcd of Kono (198O), is 63.0°, with a 95percent- confidence deviation of t9.7 . The locus of this paleo- latitude is shown as a dashed circle in figme 51 around the location of the basin in which the Cantwell Porrna- tion was deposited. The result is the same as when poles are compared: The paleolatitude is what would be expected for Cretaceous time and somewhat, but not significantly, high for Paleocene time. Pigum 51.-Locations of paleomegnetic pales Ln North America, with 95percent+xnM&nce circles: I, volcanic rocks of the Paleocene CnntweU Formation; 2, Paleocene intrusive rocks in Montana (Jacobson end others, 1980); 3, Creteceous pole for North American craton (Mankinen, 1978). Star denotes study area. Dashed circle Is locus of poles corresponding to mean geomagnetic latitude of the Cantwell Formation according to Kono's (1 980) statistical method. The timing of accretion of tectonos tro tigraphic terranes in Alaska Is constrained by this new paleolati- tude determination. From paleornagnetic and geologic evidence, the general pat tern of accretion of terranes south of the DenalI fault has been one of northward movement: for example, WrangeUia (Hillhause, 1877; Csejtey and others, 1982), the Peninsular terrane (Stone and Packer, L879), and the Chugach terrane (Grommband Hillhouse, 1981). The volcanic rocks of the Cantwell are just north of the McKinley strand of the DenaLi fault (flg. 50) and overlie the Plngston and McKinley terranes, which ere also bounded on the south by the McKinley strand of the Den& fault (Jones and others, 1882). These terranes and, by implication, other terranes to the north, such as the Nixon Pork and Yukon-Tanana terranes, have under- gone no northward displacements greater than about 500 km since Paleocene time. Moreover, recently dis- covered evidence that strike-slip movement on the McKinley strand has been minimal (Csejtey and others, 1982, 1983) likewise Implies that the northward rnove- rnent and accretlon of Wrmgellia and the Peninsular terrane were complete by Paleocene time. REFERENCES CITED Csejtey, ma, dr., Cox, D. P., Evarts, R. C., Stricker, G. D., and Foster, H. L., 1982, The Cenozoic Denali fault system and the Cretaceous accretionary development of southern Alaska: Journal of Geophysical Research, v. 87, no. 5, p. 3741- 3754. Csejtey, ma, Jr., Yeend, W. E., and Goerz, D. J., IU, 1983, Occurrenae of probable CantweU Formation rocks south of the Denali fault system in the Healy quadrangle, south-central Alaska, in Coomad, W. L., and Elliott, R. L., eds., Thi United States Geological Survey in Alaska: Accomplishments during 1981: U.S. Qeological Survey Circular 868, p. 77-79. Gilbert, W. G., Ferrell, V. M., and Turner, D. L., 1976, The Teklanika Formation--a new Paleocene volcanic formation in the central Alaska Range: Alaska Divislon of Geological and Geophysical Surveys, Geologic Report 47, 16 p. ~rornmd,~. S, and Hillhouse, J. W., 1981, PBleomagnetic evidence for northward movement of the Chugach terrane, southern and southeastern Alaska, Albert, N. R. D., and Hudson, Travis, eds., The United States Geologlcal Survey in Alaska: Accomplishments during 1079: U.S. Geologjcd Survey Circular 823-B, p. B70-B72. HLckman, R. G., 1974, Structural geology and stratigraphy along a segment of the DenaU Pault system, central Alaska Range: Madison, Unlverstty of Wisconsin, Ph. D. thesis, 276 p. Hillhouse, J. W., 1077, Paleornagnetism of the Triassic Nikolai Greenstone, McCarthy quadrangle, Alaska: Canadian Journal of Earth Sctences, v. 14, no. 11, p. 2578-2592. Jacobson, D., Beck, M. E., Jr., Diekl, J. F., and H m , 0. C., Jr., 1980, A Paleocene paleomagnetlc pole for North America from alkalic intrusions, central Montana: Geophysical Research Let ters, v. 7, no. 7, p. 549-552.
- Page 39 and 40: I US I Surlicial dcnrrua,ts [~dater
- Page 41 and 42: I Plafker, George, Hudson, Travis,
- Page 43 and 44: !omlensed iring vapors generated by
- Page 45 and 46: and the thinning. -upward cycles .,
- Page 47 and 48: Kellum, L. B., Devless, S. N., and
- Page 49 and 50: 1912 sample (a mediumwey pumice blo
- Page 51 and 52: various Utholagic units present Thu
- Page 53 and 54: fault, and Its depositional basemen
- Page 55 and 56: suggested by coplanar foUaticm and
- Page 57 and 58: 1 slgnlficarrtly more umnlum (73&1,
- Page 59 and 60: ecrSigtallized catadastic matrix of
- Page 61 and 62: analyzed to determine whether Immob
- Page 63 and 64: are tgplcd of both ocean-floor basa
- Page 65 and 66: & Fclsic in~rutirt rucks 0 Eio~ite
- Page 67 and 68: are Lrdlcated by coexisting @&ite+q
- Page 69 and 70: (Mg3.09 pe2+ 0.69 pe 0.~1~0.01~~0.9
- Page 71 and 72: westward into a narrow band that ex
- Page 73 and 74: EXF'lANATIOW 66600' Contan-Apprnimn
- Page 75 and 76: ! few fold closures are preserved.
- Page 77 and 78: even thickness and conform to irreg
- Page 79 and 80: (Alnus ap.), heaths (Ericaceae, + E
- Page 81 and 82: terrane extends at least 300 krn to
- Page 83 and 84: Table 19.--6tneral petrography of M
- Page 85 and 86: were measured on 8 12-in. mass spec
- Page 87 and 88: Thin lenses of cabonate packtone to
- Page 89: The cantwell(?) Pormation south of
- Page 93 and 94: Upper Cretaceous shale in contact w
- Page 95 and 96: Gran tz, Arthur, 1960, Generalized
- Page 97 and 98: at 15 to 20 percent. Primary Inolus
- Page 99 and 100: addition, this factor generally def
- Page 101 and 102: Joreskog, K. G., Klovan, J. E., and
- Page 103 and 104: Mineral qItWation end r ~ k t k W e
- Page 105 and 106: 1 "~_liO-/ 200 1000 B roo C E % A B
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- Page 109 and 110: Figme 62.-Plant fassils from the co
- Page 111 and 112: Hallam, Anthony, 1975, Alfred Wegen
- Page 113 and 114: u ALASKA Figure 65.--Sketch map of
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- Page 119 and 120: curve is based indicates that 6.1 c
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- Page 123 and 124: marble is alsa locally present In t
- Page 125 and 126: Bedding in the conglomerate ranges
- Page 127 and 128: 1 purpose of this study wes to dete
- Page 129 and 130: The secona k~~-~ri?tation mmes that
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- Page 133 and 134: 40 40 Forbes, R. B., and Engels, J.
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- Page 137 and 138: I I thy euheclra. Sphene anhedra an
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in the 18 lava flows b thermoremanent magnetization<br />
acquired during initial cooling. A11 the lavas exhibited<br />
reversed polarity, as is appropriate for their age be-<br />
cause Peleocene time was dominated by periods <strong>of</strong><br />
reversed geomagnetic pohrity (Ness and others, 1980).<br />
The paleornagnetic inglinations in these rocks<br />
range from -65.8' to -87.6 , and the paleomapetic<br />
pole calculated from the 18 sites (pole I ,gig. 51) is<br />
close to northwestern <strong>Alas</strong>ka at lat 70.0 N., long<br />
165.4' W., with e 95-percent-confidence radius <strong>of</strong><br />
10.0'. Figure 51 compares this pole with Cretrceous<br />
and Paleocene poles from aratonic North America.<br />
Somewhat surprisingly, the Cantwell pole is much<br />
closer to the Cretaceous reference pole (135-78 m.y.<br />
B.P.) than to the Paleocene reference pole (67-61 m.y.<br />
B.P.). This difference could be accounted for if the<br />
CantweU volcanic rocks were, in fact, slightly older<br />
than the age range <strong>of</strong> the Paleocene reference because<br />
the interval from latest Cretaceous to early Paleocene<br />
was a time <strong>of</strong> rapid apparent polar wander for the<br />
North American craton. The paleomagnetic latitude<br />
<strong>of</strong> the CantweU, calculated according to the improved<br />
rnethcd <strong>of</strong> Kono (198O), is 63.0°, with a 95percent-<br />
confidence deviation <strong>of</strong> t9.7 . The locus <strong>of</strong> this paleo-<br />
latitude is shown as a dashed circle in figme 51 around<br />
the location <strong>of</strong> the basin in which the Cantwell Porrna-<br />
tion was deposited. The result is the same as when<br />
poles are compared: The paleolatitude is what would<br />
be expected for Cretaceous time and somewhat, but<br />
not significantly, high for Paleocene time.<br />
Pigum 51.-Locations <strong>of</strong> paleomegnetic pales Ln North<br />
America, with 95percent+xnM&nce circles: I,<br />
volcanic rocks <strong>of</strong> the Paleocene CnntweU Formation;<br />
2, Paleocene intrusive rocks in Montana (Jacobson end<br />
others, 1980); 3, Creteceous pole for North American<br />
craton (Mankinen, 1978). Star denotes study area.<br />
Dashed circle Is locus <strong>of</strong> poles corresponding to mean<br />
geomagnetic latitude <strong>of</strong> the Cantwell Formation<br />
according to Kono's (1 980) statistical method.<br />
The timing <strong>of</strong> accretion <strong>of</strong> tectonos tro tigraphic<br />
terranes in <strong>Alas</strong>ka Is constrained by this new paleolati-<br />
tude determination. From paleornagnetic and geologic<br />
evidence, the general pat tern <strong>of</strong> accretion <strong>of</strong> terranes<br />
south <strong>of</strong> the DenalI fault has been one <strong>of</strong> northward<br />
movement: for example, WrangeUia (Hillhause, 1877;<br />
Csejtey and others, 1982), the Peninsular terrane<br />
(Stone and Packer, L879), and the Chugach terrane<br />
(Grommband Hillhouse, 1981). The volcanic rocks <strong>of</strong><br />
the Cantwell are just north <strong>of</strong> the McKinley strand <strong>of</strong><br />
the DenaLi fault (flg. 50) and overlie the Plngston and<br />
McKinley terranes, which ere also bounded on the<br />
south by the McKinley strand <strong>of</strong> the Den& fault<br />
(Jones and others, 1882). These terranes and, by<br />
implication, other terranes to the north, such as the<br />
Nixon Pork and Yukon-Tanana terranes, have under-<br />
gone no northward displacements greater than about<br />
500 km since Paleocene time. Moreover, recently dis-<br />
covered evidence that strike-slip movement on the<br />
McKinley strand has been minimal (Csejtey and others,<br />
1982, 1983) likewise Implies that the northward rnove-<br />
rnent and accretlon <strong>of</strong> Wrmgellia and the Peninsular<br />
terrane were complete by Paleocene time.<br />
REFERENCES CITED<br />
Csejtey, ma, dr., Cox, D. P., Evarts, R. C., Stricker,<br />
G. D., and Foster, H. L., 1982, The Cenozoic<br />
Denali fault system and the Cretaceous accretionary<br />
development <strong>of</strong> southern <strong>Alas</strong>ka: Journal<br />
<strong>of</strong> <strong>Geophysical</strong> Research, v. 87, no. 5, p. 3741-<br />
3754.<br />
Csejtey, ma, Jr., Yeend, W. E., and Goerz, D. J., IU,<br />
1983, Occurrenae <strong>of</strong> probable CantweU Formation<br />
rocks south <strong>of</strong> the Denali fault system in the<br />
Healy quadrangle, south-central <strong>Alas</strong>ka, in<br />
Coomad, W. L., and Elliott, R. L., eds., Thi<br />
United <strong>State</strong>s <strong>Geological</strong> Survey in <strong>Alas</strong>ka:<br />
Accomplishments during 1981: U.S. Qeological<br />
Survey Circular 868, p. 77-79.<br />
Gilbert, W. G., Ferrell, V. M., and Turner, D. L., 1976,<br />
The Teklanika Formation--a new Paleocene volcanic<br />
formation in the central <strong>Alas</strong>ka Range:<br />
<strong>Alas</strong>ka Divislon <strong>of</strong> <strong>Geological</strong> and <strong>Geophysical</strong><br />
<strong>Surveys</strong>, Geologic Report 47, 16 p.<br />
~rornmd,~. S, and Hillhouse, J. W., 1981, PBleomagnetic<br />
evidence for northward movement <strong>of</strong> the<br />
Chugach terrane, southern and southeastern<br />
<strong>Alas</strong>ka, Albert, N. R. D., and Hudson, Travis,<br />
eds., The United <strong>State</strong>s Geologlcal Survey in<br />
<strong>Alas</strong>ka: Accomplishments during 1079: U.S.<br />
Geologjcd Survey Circular 823-B, p. B70-B72.<br />
HLckman, R. G., 1974, Structural geology and stratigraphy<br />
along a segment <strong>of</strong> the DenaU Pault<br />
system, central <strong>Alas</strong>ka Range: Madison, Unlverstty<br />
<strong>of</strong> Wisconsin, Ph. D. thesis, 276 p.<br />
Hillhouse, J. W., 1077, Paleornagnetism <strong>of</strong> the Triassic<br />
Nikolai Greenstone, McCarthy quadrangle,<br />
<strong>Alas</strong>ka: Canadian Journal <strong>of</strong> Earth Sctences, v.<br />
14, no. 11, p. 2578-2592.<br />
Jacobson, D., Beck, M. E., Jr., Diekl, J. F., and H m ,<br />
0. C., Jr., 1980, A Paleocene paleomagnetlc pole<br />
for North America from alkalic intrusions, central<br />
Montana: <strong>Geophysical</strong> Research Let ters, v.<br />
7, no. 7, p. 549-552.