ABSTRACT The rich Quaternary history of the Pacific Northwest showcases the important linkages between multiple geologic processes that have shaped its sedimentology and geomorphology. This field trip in eastern Washington explores the evolution of landforms that developed within the Palouse and the Channeled Scabland—geomorphically distinctive areas that were indirectly and directly influenced by multiple Quaternary glacial outburst megafloods. These floods produced expansive fine-grained sediments that were subsequently remobilized by the wind to generate sand dunes, sand sheets, and the thick loess of the Palouse. Landforms and deposits that date from the Last Glacial Maximum (LGM) include dramatically eroded scab-land features, coarse-to fine-grained flood slackwater deposits, sand dunes, loess, and paleosols. Sedimentary, paleopedologic, and geomorphic evidence for similar magnitude glacial outburst megafloods and loess accumulation that are related to the penultimate glaciation, during oxygen isotope stage 4, is recorded in several loess outcrops. This field trip traces the windblown sediments from source to sink and particularly focuses on Eureka Flat—the engine of the Palouse loess—and well-studied sections of thick loess farther downwind. A rich paleoclimate record is emerging from the loess stratigraphy and paleosols based on luminescence ages, tephrochronology, and paleoecologic analyses.

Abstract The Channeled Scabland of east-central Washington comprises a complex of anastomosing fluvial channels that were eroded by Pleistocene megaflooding into the basalt bedrock and overlying sediments of the Columbia Plateau and Columbia Basin regions of eastern Washington State, U.S.A. The cataclysmic flooding produced huge coulees (dry river courses), cataracts, streamlined loess hills, rock basins, butte-and-basin scabland, potholes, inner channels, broad gravel deposits, and immense gravel bars. Giant current ripples (fluvial dunes) developed in the coarse gravel bedload. In the 1920s, J Harlen Bretz established the cataclysmic flooding origin for the Channeled Scabland, and Joseph Thomas Pardee subsequently demonstrated that the megaflooding derived from the margins of the Cordilleran Ice Sheet, notably from ice-dammed glacial Lake Missoula, which had formed in western Montana and northern Idaho. More recent research, to be discussed on this field trip, has revealed the complexity of megaflooding and the details of its history. To understand the scabland one has to throw away textbook treatments of river work. —J. Hoover Mackin, as quoted in Bretz et al. (1956, p. 960)

ABSTRACT The Columbia River Basin (CRB) is home to the best studied examples of two of the most spectacular geologic processes on Earth and Mars: flood volcanism and catastrophic water floods. Additionally, features formed by a variety of eolian, glacial, tectonic, and mass-wasting processes can also be seen in the CRB. These terrains provide exceptional terrestrial analogs for the study of similar processes on Mars. This field guide describes four one-day trips out of Moses Lake, Washington, to observe a wide variety of Mars analogs.

Sedimentary interbeds preserved between flows of the Columbia River Basalt Group provide a record of the depositional and erosional conditions that characterized the Columbia Plateau between eruptions of basalt. Examination of the sedimentary, stratigraphic, and petrologic character of the Sweetwater Creek interbed from within the Lewiston basin of southeastern Washington and north-central Idaho allows insight into the paleogeographic conditions that existed following eruption of the Priest Rapids Member of the Wanapum Basalt, ca. 14.5 Ma. The Sweetwater Creek interbed is composed of generally unconsolidated and inter-stratified beds of clay, silt, sand (with local thin gravel stringers), and volcanic ash-rich sediment. Three broadly defined sedimentary facies are identified on the basis of lithology and texture. The spatial distribution of these facies, abundance of clay- and silt-rich sediment, and internal sedimentary structures suggest that deposition of the interbed resulted primarily from fluvial and mixed fluvial-lacustrine sedimentation. Fluvial drainages that headed in the ancestral Clearwater Mountains entered the Lewiston basin on the east and exited to the northwest. Basin streams appear to have been primarily of the meandering, mixed-load type. Channel sands deposited by these streams were concentrated east and north of the basin center, and transported extrabasinal sediments are characterized by plutonic and metamorphic sand- and gravel-sized clasts. Fine-grained silt- and clay-rich flood-plain and associated lacustrine deposits extend across the basin, but are thickest near the basin center. The Umatilla basalt flow entered the Lewiston basin during deposition of the Sweetwater Creek interbed and locally invaded fine-grained lacustrine sediments. A later flow, the Wilbur Creek basalt, partially buried the interbed. Complete burial of the Sweetwater Creek interbed sediments followed eruption of the Asotin flow.

Abstract This geological field site, notorious for strong, persistent, unidirectional winds that have created classic eolian landforms, is located in the SW¼ Sec.30, T.25N., R.84W., Carbon County, Wyoming (Figs.1), 1,). The area is readily accessible via paved road by traveling north from the town of Sinclair, Wyoming, a distanceof 30 mi (48 km) on the Seminoe Road. This highway is the main access route to Seminoe State Park. The locale is on public land, administered by the Bureau of Land Management, but it borders on private ranch land to the north and state-owned land to the west. The area is within the broad, windswept zone of central Wyoming (Fig. 1) known as the Wyoming Wind Corridor(Marrs and Kolm, Kolm 1982). The large active dunes at this site and older stabilized dunes in the area are part of the Seminoe Dune Field (Fig. 1) 2). Most dunes in the area are marginally stabilized parabolic dunes. The few active dunes are relatively large and slow moving with active fronts and partially stabilized tails.

Eolian features provide a record of the interaction between winds and the Earth’s surface. Most eolian features are identifiable on aerial photographs; some are large enough to be mapped from LANDSAT imagery. Therefore, eolian features can be remotely identified and interpreted in terms of the strength and flow pattern of the winds that produced them. The techniques that are useful in interpreting wind patterns from eolian features include: (1) Interpretation of wind direction, wind energy, and wind velocity from sand dunes and dune fields; (2) interpretation of wind direction and wind velocity from playas; and (3) interpretation of wind direction and relative wind velocity from scour features, dust and smoke plumes, vegetation patterns, and snow drifts. Wind patterns can be interpreted from eolian features even if the researcher does not have a direct knowledge of the field area nor ancillary data from wind-measuring stations in the region. However, the reliability of the interpretation and the amount of information that can be derived from eolian features are greatly increased if the observer has meteorological and sedimentological information about the area.

The Ferris Dune Field of south-central Wyoming lies in a topographically-regulated “corridor” of high wind that extends over much of southern Wyoming. Examination of geomorphology, sedimentology, and stratigraphy reveals that winds did not vary significantly in either average direction or speed during the Holocene period, but variations in precipitation, and hence plant growth, produced varying degrees of eolian activity. Deposition of dune sand resulted mainly from a decrease in the carrying capacity of the wind as it encountered the Ferris-Seminoe Mountain barrier. The Ferris dunes geomorphically resemble other dune fields in the western United States. Phytogenic dunes, varying in size and shape from small blowout dunes to large, well-developed parabolic dunes, dominate the landscape. A few actively migrating dunes occur both where the stabilized ground surface has been disturbed and where the highest wind speeds occur. Mineral analyses indicate that the Ferris dune sands were derived primarily from the Tertiary Battle Spring Formation. The Killpecker Dune Field “tail” sands and certain Cretaceous through Paleocene sandstones exposed along the Lost Soldier Divide were lesser contributors. The valley of Clear Creek reveals a relatively continuous Holocene section of interbedded dune and interdunal pond deposits. Bioturbated, low-angle (less than 15°) bedding, which characterized large portions of the eolian sands exposed there, attests to the long-term influence of vegetation and moisture on dune activity. Artifacts recovered in the vicinity of Clear Creek demonstrate Late Plains Archaic to Late Prehistoric occupations in this area. Radiocarbon dates from Clear Creek, comparison of Clear Creek chronology to other radiometrically-dated geologic-climatic events from the western United States, and theoretical dune migration rates reveal a general sequence of geologic-climatic events for the Ferris Dune Field: Eolian activity had begun in the Ferris-Lost Soldier area by at least ca. 9,950 to 10,330 years b.p. Major depositional intervals (indicating widespread Ferris dune activity) correlate with two radiocarbon-dated periods of drought. The first occurred between ca. 7,660 and 6,460 years b.p.; the second occurred following ca. 6,460 years b.p. (and lasted until ca. 5,500 years b.p.). Since the last major depositional (drought) interval, the climate in the Ferris-Lost Soldier area has moderated. Drought intervals have been short and vegetation has largely stabilized the dunes.