Chapter 8. Glacioaeolian Processes, Sediments, and Landforms
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University of Alberta Caribou Hunting at Ice Patches: Seasonal Mobility and Long-term Land-Use in the Southwest Yukon By Vandy E. Bowyer A thesis submitted to the Faculty of Graduate Studies and Research in partial fulfillment of the requirements for the degree of Doctor of Philosophy Department of Anthropology © Vandy E. Bowyer Spring 2011 Edmonton, Alberta Permission is hereby granted to the University of Alberta Libraries to reproduce single copies of this thesis and to lend or sell such copies for private, scholarly or scientific research purposes only. Where the thesis is converted to, or otherwise made available in digital form, the University of Alberta will advise potential users of the thesis of these terms. The author reserves all other publication and other rights in association with the copyright in the thesis and, except as herein before provided, neither the thesis nor any substantial portion thereof may be printed or otherwise reproduced in any material form whatsoever without the author's prior written permission. In memory of Tagish ABSTRACT Recently documented ice patch sites in the southwest Yukon are ideal for evaluating precontact hunter-gatherer land-use patterns in the western subarctic. Located in the alpine of the mountainous regions of the boreal forest, ice patches are associated with well preserved hunting equipment, caribou (Rangifer tarandus) dung and an abundance of faunal remains dating to over 8000 years ago. However, current models are inadequate for explaining caribou hunting at ice patches as they tend to emphasize large-scale communal hunts associated with latitudinal movements of caribou. Much less is known about the alititudinal movment of caribou and the associated hunting forays to ice patches in the alpine. -
Name These Glacial Features 1.) 1
Name these Glacial Features 1.) 1.)____________________________________ 2.) 2.) ___________________________________ 3.) 3.)_____________________________________ 4.) 4.) ____________________________________ Name these types of Glaciers 5.) 5.)___________________________________________ 6.) 6.) __________________________________________ 7.) 7.) __________________________________________ 8.) 8.) __________________________________________ True or False 9.) __________ The terminus marks the farthest extent of a glacier. 10.) _________ An arête is a bow or amphitheater shape in a glacier. 11.) _________CO2 levels are higher during glacial episodes. 12.) _________ Methane Hydrate breaks down into H20. 13.) _________ Glaciers exist on every continent. 14.) _________ The Great Lakes were created by glaciation. 15.) _________ Calving is a process that creates icebergs. 16.) ________ Glacier National Park is in Alaska 17.) ________ Alaska has 100 glaciers. 18.) ________ 75% of the world’s glaciers are retreating. 19.) ________ A glacier can move forward and retreat at the same time. 20.) ________ Ogives are alternating wave crests and valleys that appear as dark and light bands of ice on glacier surfaces. 21.) ________ A drumlin field east of Rochester, New York is estimated to contain about 100 drumlins. Short Answer 22.) Give a general definition of the milankovitch cycles. _________________________________________________________________________________ _________________________________________________________________________________ _________________________________________________________________________________ -
Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa Region, Mars, with Insights from Modern and Ancient Terrestrial Analogs
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 12-2016 Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa region, Mars, with Insights from Modern and Ancient Terrestrial Analogs Robert Eric Jacobsen II University of Tennessee, Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Geology Commons Recommended Citation Jacobsen, Robert Eric II, "Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa region, Mars, with Insights from Modern and Ancient Terrestrial Analogs. " PhD diss., University of Tennessee, 2016. https://trace.tennessee.edu/utk_graddiss/4098 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Robert Eric Jacobsen II entitled "Geomorphology, Stratigraphy, and Paleohydrology of the Aeolis Dorsa region, Mars, with Insights from Modern and Ancient Terrestrial Analogs." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Devon M. Burr, -
Antarctic Fossil Conchostracans and the Continental Drift Theory
section to the northwest of that locality. At both southern continents to one another during the Per- localities, well-preserved conchostracans (Lioes- mian appears to be the only satisfactory way to ex- theria) and ostracods were found. At two localities plain the distribution of these fossils. Accordingly, a in the Marshall Mountains, the underlying sediments program was devised to collect conchostracans and are cut by features that are probably volcanic vents. to gather other paleolimnological data from the Dolerite sheets are conspicuous throughout the Ohio Range and to search for conchostracans in the Queen Alexandra Range. Concordant or only slightly Polarstar Formation of the Sentinel Range. transgressive sills as much as 150 m thick occur Some of the considerations upon which the study in the northern part of the range and at Painted was based and the preliminary results of the field Cliffs, but from the Prebble Glacier southward to work are given in the following paragraphs. Inas- Mount Wild, relationships are more complex. In the much as the discussion has been drawn primarily latter area, there are a few dolerite dikes up to 18 in from field notes, some modification of it may be re- wide. Most of the sheets there are steeply inclined quired when laboratory analysis has been completed. and transgressive, but a few are concordant over considerable distances. Field observations revealed Ohio Range only inconspicuous differentiation within the sheets. Do leaiid beds recur above and/or below the The Permian part of the stratigraphic sequence "Leaia Ledge" of the Mt. Glossopteris Formation? from the base of the Pagoda Formation to the top of The answer to this question is important to the es- the Buckley Coal Measures was found to be similar tablishment of intercontinental correlations and the to lower Beacon strata in the Queen Maud and Hor- continental drift theory. -
The Sherpa and the Snowman
THE SHERPA AND THE SNOWMAN Charles Stonor the "Snowman" exist an ape DOESlike creature dwelling in the unexplored fastnesses of the Himalayas or is he only a myth ? Here the author describes a quest which began in the foothills of Nepal and led to the lower slopes of Everest. After five months of wandering in the vast alpine stretches on the roof of the world he and his companions had to return without any demon strative proof, but with enough indirect evidence to convince them that the jeti is no myth and that one day he will be found to be of a a very remarkable man-like ape type thought to have died out thousands of years before the dawn of history. " Apart from the search for the snowman," the narrative investigates every aspect of life in this the highest habitable region of the earth's surface, the flora and fauna of the little-known alpine zone below the snow line, the unexpected birds and beasts to be met with in the Great Himalayan Range, the little Buddhist communities perched high up among the crags, and above all the Sherpas themselves that stalwart people chiefly known to us so far for their gallant assistance in climbing expeditions their yak-herding, their happy family life, and the wav they cope with the bleak austerity of their lot. The book is lavishly illustrated with the author's own photographs. THE SHERPA AND THE SNOWMAN "When the first signs of spring appear the Sherpas move out to their grazing grounds, camping for the night among the rocks THE SHERPA AND THE SNOWMAN By CHARLES STONOR With a Foreword by BRIGADIER SIR JOHN HUNT, C.B.E., D.S.O. -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
Aeolian Processes and Landforms
Aeolian Processes and Landforms Ms. Deithra L. Archie, New Mexico State University Abstract I will present an overview of Aeolian processes and landforms on Mars. The overview will consist of two components. Component one is an overview of Aeolian processes and landforms on Earth and Mars, where the two planetary bodies are shown in Figures 1a and 1b respectively The second part of this paper will consist of image comparisons using satellite and MOC (Mars Orbiter Camera) images. Figure 1a Figure 1b Introduction Understanding the aeolian activity on the planet Mars and other planets begins with the study and knowledge of similar processes on Earth. Therefore, I will discuss the following: wind, particle entrainment and landforms found in the aeolian environment. This discussion will lead into my later discussion of the Martian sand seas and sand dunes. See Table 1 for a glossary of the terms used throughout this paper. In aeolian processes, wind transports and deposits particles of sediment. Aeolian features form in areas where wind is the primary source of erosion. The particles deposited are of sand, silt and clay size (see Table 2). The particles are entrained in by one of four processes. Creep is when a particle rolls or slides across the surface. Lift is when a particle rises off the surface due to the Bernoulli effect, the same mechanism which causes aircraft to rise. If the airflow is turbulent, larger particles are trajected by a process known as saltation. Finally, impact transport occurs which one particle strikes another causing the second particle to move. Erosional Landforms Wind eroded landforms are rarely preserved on the surface of the Earth except in arid regions. -
Cold-Climate Landform Patterns in the Sudetes. Effects of Lithology, Relief and Glacial History
ACTA UNIVERSITATIS CAROLINAE 2000 GEOGRAPHICA, XXXV, SUPPLEMENTUM, PAG. 185–210 Cold-climate landform patterns in the Sudetes. Effects of lithology, relief and glacial history ANDRZEJ TRACZYK, PIOTR MIGOŃ University of Wrocław, Department of Geography, Wrocław, Poland ABSTRACT The Sudetes have the whole range of landforms and deposits, traditionally described as periglacial. These include blockfields and blockslopes, frost-riven cliffs, tors and cryoplanation terraces, solifluction mantles, rock glaciers, talus slopes and patterned ground and loess covers. This paper examines the influence, which lithology and structure, inherited relief and time may have had on their development. It appears that different rock types support different associations of cold climate landforms. Rock glaciers, blockfields and blockstreams develop on massive, well-jointed rocks. Cryogenic terraces, rock steps, patterned ground and heterogenic solifluction mantles are typical for most metamorphic rocks. No distinctive landforms occur on rocks breaking down through microgelivation. The variety of slope form is largely inherited from pre- Pleistocene times and includes convex-concave, stepped, pediment-like, gravitational rectilinear and concave free face-talus slopes. In spite of ubiquitous solifluction and permafrost creep no uniform characteristic ‘periglacial’ slope profile has been created. Mid-Pleistocene trimline has been identified on nunataks in the formerly glaciated part of the Sudetes and in their foreland. Hence it is proposed that rock-cut periglacial relief of the Sudetes is the cumulative effect of many successive cold periods during the Pleistocene and the last glacial period alone was of relatively minor importance. By contrast, slope cover deposits are usually of the Last Glacial age. Key words: cold-climate landforms, the Sudetes 1. -
Regional Investigations of the Effects of Secondaries Upon the Martian Cratering Record
46th Lunar and Planetary Science Conference (2015) 2630.pdf REGIONAL INVESTIGATIONS OF THE EFFECTS OF SECONDARIES UPON THE MARTIAN CRATERING RECORD. Asmin V. Pathare1 and Jean-Pierre Williams2 1Planetary Science Institute, Tucson, AZ 85719 ([email protected]) 2Earth, Planetary, and Space Sciences, University of California , Los Angeles, CA 90095. Motivation: We consider the following paradox: if Zunil-type impacts can generate tens of millions of secondary craters on Mars approximately once every million years [1], then why do so many martian crater counts show so little isochronal evidence (e.g., [2]) of secondary “contamination”? We suggest three possible explanations for this incongruity: (1) Atmospheric Pressure Variations: lower pres- sures at low obliquities may have facilitated massive secondary generation at the time of the Zunil impact; alternatively, higher pressures at high obliquities may have inhibited secondary cratering from other Zunil- sized impacts. (2) Target Material Strength: Zunil impacting into a notably weak regolith may have augmented second- ary crater production relative to similar-sized craters. (3) Surface Modification: secondary craters from previous Zunil-sized impacts may have once been just as prominent as those emanating from Zunil, but have since been obliterated by rapid resurfacing over the past 100 Myr. Figure 1. Modeled annual SFDs for the locations of As part of a newly-funded MDAP, we will conduct Zunil and Pangboche craters and isochrons derived regional investigations of secondary cratering to help from polynomial fits. The crater counts from the two locations are scaled to the same time/area for compari- distinguish amongst these three potential explanations. son with the annual isochrons. -
Glacial Processes and Landforms
Glacial Processes and Landforms I. INTRODUCTION A. Definitions 1. Glacier- a thick mass of flowing/moving ice a. glaciers originate on land from the compaction and recrystallization of snow, thus are generated in areas favored by a climate in which seasonal snow accumulation is greater than seasonal melting (1) polar regions (2) high altitude/mountainous regions 2. Snowfield- a region that displays a net annual accumulation of snow a. snowline- imaginary line defining the limits of snow accumulation in a snowfield. (1) above which continuous, positive snow cover 3. Water balance- in general the hydrologic cycle involves water evaporated from sea, carried to land, precipitation, water carried back to sea via rivers and underground a. water becomes locked up or frozen in glaciers, thus temporarily removed from the hydrologic cycle (1) thus in times of great accumulation of glacial ice, sea level would tend to be lower than in times of no glacial ice. II. FORMATION OF GLACIAL ICE A. Process: Formation of glacial ice: snow crystallizes from atmospheric moisture, accumulates on surface of earth. As snow is accumulated, snow crystals become compacted > in density, with air forced out of pack. 1. Snow accumulates seasonally: delicate frozen crystal structure a. Low density: ~0.1 gm/cu. cm b. Transformation: snow compaction, pressure solution of flakes, percolation of meltwater c. Freezing and recrystallization > density 2. Firn- compacted snow with D = 0.5D water a. With further compaction, D >, firn ---------ice. b. Crystal fabrics oriented and aligned under weight of compaction 3. Ice: compacted firn with density approaching 1 gm/cu. cm a. -
Geotechnical and Geologic Constraints on Tsunamigenic Submarine Landslides
GEOTECHNICAL AND GEOLOGIC CONSTRAINTS ON TSUNAMIGENIC SUBMARINE LANDSLIDES H.J. LEE U.S. Geological Survey, 345 Middlefield Road, Menlo Park, CA 94025 USA Abstract Modeling submarine-landslide-induced tsunamis requires many simplifications of the landslide process, although the real world is much more complicated. Clearly tsunami modelers cannot consider all facets, but there is value in being aware of the complications. This paper describes the many environments in which submarine landslides can occur and the triggers that typically initiate them. Earthquakes acting on continental or canyon slopes comprise probably the most common scenario but many other combinations of environments and triggers are possible. Surprisingly, many sediment-covered slopes in highly seismically active areas have not failed. A possible explanation for this phenomenon is a process called “seismic strengthening.” The existence of such a process reduces somewhat the risk of landslide tsunamis along active margins while maintaining the risk along passive margins. Once a trigger has initiated a landslide in one of the vulnerable environments, failed masses begin to move downslope. Depending upon initial density state, the masses may convert into fluid-like sediment flows or even more dilute turbidity currents. A model for quantifying the tendency to flow is provided. Finally, a case study of the landslides and landslide tsunamis that occurred in Port Valdez, Alaska, during the 1964 Great Alaska Earthquake is provided. The excellent data base, including before and after bathymetry, shows that both large rigid block motion and mobilized sediment flows can occur near each other during the same event. The intact blocks are more efficient in producing tsunamis but the sediment flow can move farther and can erode and entrain considerable bottom sediment as they progress across the seafloor. -
Challenges Using Small Craters for Dating Planetary Surfaces
Workshop on Issues in Crater Studies and the Dating of Planetary Surfaces (2015) 9051.pdf CHALLENGES USING SMALL CRATERS FOR DATING PLANETARY SURFACES. J.-P. Williams1 and A. V. Pathare2, 1Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095 ([email protected]), 2Planetary Science Institute, Tuscon, AZ 85719 ([email protected]). Introduction: Impact craters can be used to esti- mate the age of a planetary surface, given knowledge of the rate of crater accumulation, and are the primary method for age dating planetary surfaces (excluding Earth) (e.g. [1][2]). The factors shaping crater produc- tion at diameters < 100 m are not well understood and under debate. However, because of the frequency at which these craters form, they are utilized to discrimi- nate surface ages of geologically young regions and features at a higher spatial resolution. This level of resolution is required to establish the temporal relation of recent geologic activity on the Moon such as Co- pernican impacs, including North Ray, South Ray, and Cone craters, sites used to anchor the crater chronolo- Fig 1. Impact melt deposit on the ejecta of Giordano gy, and Mars such as gully, landslide, and outflow Bruno crater and crater SFD on and off of the melt channel formation, volcanic resurfacing, sedimenta- deposit with nominal lunar regolith and hard rock tion, exhumation, dune activity, glaciation and other isochrons [7]. periglacial landforms, and the possible relation of such 7 features to obliquity variations of ~10 y timescale. Self-Secondary Craters: The melt deposit also il- Radiometric and cosmic ray exposure ages of lustrates another issue that may confound crater count- Apollo and Luna samples, correlated with crater popu- ing on the ejecta of craters.