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were measured on 8 12-in. mass spectrometer with on-<br />
Une dtgital proc~lfg. three size fractions have<br />
nearly idbntieal Pbj2&b ages, ranging from 368<br />
to 372 m.y. (table 15); the U-Pb ages range from about<br />
320 to 350 m.y. (table 15). This age variation does not<br />
follow the ordinary dependency on uranium concentration,<br />
which, in this sample, is extremely low, ranging<br />
from about 120 to 154 ppm and increasing with decreasing<br />
grain size. A best-fit line (Ludwig, 1980)<br />
through the data points yields concordia intercepts <strong>of</strong><br />
373~7 m.y. and 256% m.y. (fig. 46). We interpret these<br />
data to indicate that the protolith for the metftrhyod~cite<br />
was erupted during the Late Devonim. The<br />
lowerintercept age reflects either modern lead loss<br />
due to dil~tancy (Goldich and Mudrey, 1972) or, possibly,<br />
late Mcsozoic and Tertiary movement, metamorphism,<br />
and deformation <strong>of</strong> rocks along the Hines Creek<br />
fault.<br />
Most <strong>of</strong> the rocks <strong>of</strong> the Pingston terrane to the<br />
west in the Healy quadrangle or near Mount McKinley<br />
have been assigned u late Paleozoic and Triassic age,<br />
mainly on the besis <strong>of</strong> conodonts (Sherwood and<br />
Craddock, 1979; Reed and Nelson, 1980; Jones and<br />
others, 1981). The age <strong>of</strong> the relatively younger diabase<br />
and gabbro is assumed to be middle or Late Mesozoic.<br />
Before our study, no metavolcanic rock f1.orn the<br />
Pingston terrane had been dated. Our data show that<br />
an important component <strong>of</strong> the Pingston terrane consists<br />
<strong>of</strong> former siliceous volcanic rock <strong>of</strong> Late Devonian<br />
age. On the basis <strong>of</strong> lithology, metamorphic grade,<br />
and structure, we interpret the metarhyodaclte to be<br />
an important constituent <strong>of</strong> the terrae in the western<br />
part <strong>of</strong> the Mount Hayes quadrangle (Nokleberg and<br />
others, 1983). This report sug-gests that the age <strong>of</strong> at<br />
least a part <strong>of</strong> the Pingston terrene is Late Devonian<br />
and thereby extends the tige range <strong>of</strong> the terrane and<br />
revises the stratigraphy <strong>of</strong> the terrane to Include<br />
former siliceous volcanic rock.<br />
REFERENCES CITED<br />
Gilbert, W. G., 1917, General geology md geochemistry<br />
<strong>of</strong> the nealy D-1 and southern Fairbanks A-l<br />
quadrangles and vicinity, <strong>Alas</strong>ka: <strong>Alas</strong>ka <strong>Division</strong><br />
<strong>of</strong> <strong>Geological</strong> and <strong>Geophysical</strong> <strong>Surveys</strong><br />
Open-File Report 195, 13 p.<br />
Gilbcrt, W. G., and Redman, EarI, 1977, Metamorphic<br />
rocks <strong>of</strong> the Toklat-Teklanika Rivers area,<br />
Almka: <strong>Alas</strong>ka <strong>Division</strong> <strong>of</strong> Geology and<br />
Gcophysical <strong>Surveys</strong> Geologic lieport 50, 13 g.<br />
Goldick, S. S., und Mudrey, !\-I. G., Jr., 1972, Dilatancy<br />
model for discordnnt U-Pb zircon ages, &<br />
l'ugarinov, A. I., ed., Recent contributions to<br />
geochemistry and t~nnlytical chemistry: New<br />
York, John Wiley & Sans, p. 466-470.<br />
Jones, D. L., Silberling, N. J., Berg, H. C., and Plafker,<br />
George, 1981, Map showing tectonostra tigraphic<br />
terranes <strong>of</strong> <strong>Alas</strong>ka, columnar sections, and<br />
summary description <strong>of</strong> terranes: U.S. Geologlcal<br />
Survey Open-Pile lleport 81-792, 20 p., scale<br />
1:2,500,000, 2 sheets.<br />
Krogh, T. E., 1973, A low-contamination method for<br />
hydrothermal decomposition <strong>of</strong> zircon and extr~ction<br />
<strong>of</strong> U and Pb for isotopjc age determinations:<br />
Geochlrnica et Cosrnochimica Acta, v. 37,<br />
no. 3, p. 495-994.<br />
Ludwig, K. R., 1980, Calculation <strong>of</strong> uncertainties <strong>of</strong> U-<br />
Pb isotope data: Earth and Planetary Science<br />
Letters, v. 46, no. 2, p. 212-220.<br />
Nokleberg, W. J., BWmaster, C. L., and Schwab, C.<br />
E., 1983, Stratigraphy, petrology, and structure<br />
<strong>of</strong> the Pingston terrane, Mount Hayes C-5 and C-<br />
6 quadrangles, eastern <strong>Alas</strong>ka Range, & Coonrad,<br />
W. L., and Elliott, R. L., eds., The United <strong>State</strong>s<br />
<strong>Geological</strong> Survey in <strong>Alas</strong>ka: Accomplishn~ents<br />
during 1981: U.S. <strong>Geological</strong> Survey Circular<br />
868, p. 70-73.<br />
Reed, B. L., and Nelson, S. W., 1980, Geologic map <strong>of</strong><br />
the Talkeetna quadrangle, <strong>Alas</strong>ka: U.S. Geologi-<br />
cal Survey MisceUaneous Investigations Series<br />
Map 1-1174, 15 p., scale 1:250,000.<br />
Sherwood, K. W., and Craddock, Campbell, 1979,<br />
General geology <strong>of</strong> the central <strong>Alas</strong>ka Range<br />
between the Nenana River and Mount Deborah:<br />
<strong>Alas</strong>ka <strong>Division</strong> <strong>of</strong> <strong>Geological</strong> and Ccophysical<br />
<strong>Surveys</strong> Open-P Ue Report AOF-116, 22 p.<br />
Wahrhaftig, Clyde, Turner, D. L., Weber, P. R., and<br />
Smith, T. E., 1975, Nature and timing <strong>of</strong> move-<br />
ment on the Wines Creek strand <strong>of</strong> the Denali<br />
fault system, <strong>Alas</strong>ka: Geology, v. 3, no. 8, p.<br />
463-466.<br />
The Jeanie Point complex revisited<br />
By Julie & ~Umolilin and Martha L. lldiller<br />
The so-called Jeanie Point complex is a dlstinctive<br />
paclrage <strong>of</strong> rocks within the Orca Group, a Ter<br />
tiary turbidite sequence. The rocks cmp out on the<br />
southeast coast <strong>of</strong> Montague Island, Prince William<br />
Sound, approximately 3 kni northeast <strong>of</strong> Jeanie Point<br />
(loc. 7, fig. 44). These rocks consist dominantly <strong>of</strong><br />
fine-grained limestone and lesser amounts <strong>of</strong> siliceous<br />
limestone, chert, tuff, mudstone, argzllite, and smdstone<br />
(fig. 47). The Jeanie Point rock elsO differ from<br />
those typical. <strong>of</strong> the Orca Group in their fold style.<br />
Thus, the Or- Group <strong>of</strong> the area is isoclinally folded<br />
on a large scale (tens to hundreds <strong>of</strong> meters), whereas<br />
the Jeanie Point rocks are tightly folded on a 1- to 3-<br />
m-wavelength scale (differencm in rock competency<br />
may be responsible for this variation in fold style).<br />
Helwig and Bmmet (1981) first described these<br />
rocks and interpreted them as an accreted terrane <strong>of</strong><br />
pelagic origin. They suggested "* * * the complex<br />
could represent a separate terrane andlor a separate<br />
basement to the Orca Group" (Helwig and Emmet,<br />
1981, p. 28). Our studies suggest that the Jeanie Point<br />
rocks are interbedded with the Orca Group and may<br />
have formed in a smr!U ~narginal basin.<br />
The Jeanie Point rocks crop out along the shoreline<br />
on two prominent points and Include about 0.8 km<br />
<strong>of</strong> tidal-flat and cliff exposures (fig. 48). The rocks<br />
are structurally complex; a best estimate <strong>of</strong> their stratigraphic<br />
thickness is 100 to 300 rn. Beds are cornrnonly<br />
2 to 10 cm thick and, though folded, ore laterally<br />
continuous, The dominant rock type Is micritic to<br />
sllghtky coarser grained limestone containing few to<br />
abundant planktic and scarce benthic fovaminifers.<br />
Recrystallized and (or) replaced radiobrian tests are<br />
present but not abundant in the micrite. A subordlnate<br />
rock type consists <strong>of</strong> chert containing few to abundant