Contributions to Geology 30.2
Therian
mammals of the Terlingua local fauna (Judithian), Aguja Formation, Big Bend of
the Rio Grande, Texas
RICHARD
L. CIFELLI Oklahoma Museum of Natural History and Department of Zoology,
University of Oklahoma, Norman, OK 73019
Pages
117-136
Keywords
Therian
mammals, Terlingua, Aguja Formation, Texas
Abstract
The
Aguja Formation (Campanian) of southern Texas has yielded a diverse vertebrate
assemblage which is of interest in that it represents a significant, southern
range extension for local faunas of Judithian age. One tribosphenic therian,
Paleomolops langstoni, new genus and species, cannot be confidently allied with
either marsupials or eutherians. It is morphologically most similar to
Iugomortiferum, from the early Campanian of Utah, but a special relationship is
not supported by unambiguous synapomorphy. A possible second "tribothere" is
represented by teeth not surely of the adult dentition. Five or more marsupials
are present in the fauna. Of the four generically-identified taxa, one is
described as a new species of Alphadon, A. perexiguus; two others are
tentatively referred to the Judithian species A. halleyi and A. sahnii,
respectively, and the last is most similar to Judithian Turgidodon lillegraveni.
A eutherian is described as new and referred to the enigmatic genus Gallolestes,
as G. agujaensis. Gallolestes is otherwise known only from the Campanian of
Baja, California. Upper molars referred to G. agujaensis are of eutherian design
and, assuming generic referral is correct, support placement of Gallolestes
within the Eutheria. Although some of the therian taxa of the Terlingua local
fauna are tentatively referred to Judithian species known from the central and
northern Western Interior, at least half of the species represented are endemic.
In addition, some taxa typical of Judithian and later faunas from the north are
lacking; both the high degree of endemism and these apparent absences are
presumably owing to biogeographic differentiation of the terrestrial biota
during the Late Cretaceous of North America.
Geomorphic and structural features of the Alliance 1¡ x 2¡ Quadrangle, western
Nebraska, discernible from synthetic-aperture radar imagery and digital
shaded-relief maps
R. F.
DIFFENDAL, JR. Conservation and Survey Division, IANR, University of
Nebraska-Lincoln, Lincoln, Nebraska 68588-0517
Pages
137-148
Keywords
Alliance, Nebraska, geomorphology, structural features, synthetic-aperture,
shaded-relief
Abstract
The
digital shaded-relief map of the United States and the synthetic-aperture radar
map of the Alliance Nebraska 1¡ x 2¡ area prepared by the U.S. Geological Survey
(USGS) in the former case and for the USGS in the latter show oriented landforms
and lineaments in northwest Nebraska. Parallel and subparallel hills and valleys
developed on different geologic materials ranging from shales through sandstones
to loess and eolian sand appear to be wind erosional features subsequently
modified by running water. The long axes of these hills and valleys generally
trend between N40¡W and N50¡W. Similar features also occur across major areas of
the Great Plains from Montana southeast at least to Kansas. Most of the
lineaments are in two sets, one trending northeast, the other northwest. There
are some east-west and north-south trending lineaments in the western part of
the quadrangle, some circular features in the northwest, and some chevronlike
lineaments in the north-central part. Some lineaments appear to coincide wholly
or in part with known faults in western Nebraska or with extensions of faults in
east-central Wyoming into northwest Nebraska. All other lineaments are probably
reflections of either jointing or, more likely, of faulting. Additional field
work will be needed to verify which of these two, if either, is responsible for
any particular lineament.
Time
resolution at Carnegie Quarry (Morrison Formation: Dinosaur National Monument,
Utah): implications for dinosaur paleoecology
ANTHONY
R. FIORILLO Museum of Paleontology, University of California, Berkeley,
California 94720
Pages
149-156
Keywords
Carnegie Quarry, Morrison Formation, paleoecology, Dinosaur National Monument
Abstract
Theoretical minimum and maximum time estimates for the formation of the Carnegie
Quarry (Morrison Formation) in Dinosaur National Monument can be derived from
the recognition of preburial bone weathering rates combined with a basic
understanding of the stream-flow characteristics of a fluvial system. These time
estimates suggest that the time of formation of the quarry assemblage was on the
order of a few months to only a few years, thereby recording ecological time
rather than evolutionary time.
Recognizing that ecological time is represented at Dinosaur Monument, the issue
of coexistence of the dinosaur taxa within this ecosystem is confirmed from the
preservational state of the various specimens. How did the different sauropod
taxa coexist with respect to food resources? Preliminary work on the dental
microwear patterns on the teeth of two of the most common sauropods,
Camarasaurus and Diplodocus, suggests that some degree of partitioning of food
resources took place by these animals within the Late Jurassic ecosystem,
recorded by the Morrison Formation.
A
sedimentary origin for the "microbreccia" associated with the Heart Mountain
detachment fault
ANTONI
K. TOKARSKI Polish Academy of Sciences, 31-002, Krakow, Poland
WILLIAM G. PIERCE U.S. Geological Survey, Menlo Park, California 94025
EWA PIEKARSKA Polish Academy of Sciences, 31-002, Krakow, Poland
WILLIS H. NELSON U.S. Geological Survey, Menlo
Pages
157-162
Keywords
microbreccia, Heart Mountain, volcanic, Wapiti Formation
Abstract
The
volcanic rock in contact with the Heart Mountain fault has been interpreted by
Hauge (1985; 1990) to be a microbreccia or cataclasite, an interpretation that
is a basic tenet of the continuous allochthon model. However, thin sections of
this rock show none of the distinctive features associated with cataclasites,
such as grain fracture, grain angularity increase, grain size reduction,
cataclasite foliation, feather fractures, Riedel shears, or angularity decrease
in relation to the Wapiti Formation of which it is the basal unit. We interpret
the widespread, very thin to absent, volcanic rock lying on the Bighorn Dolomite
to be an airfall tuff, not microbreccia or cataclasite.