Diamond Craters Recreation Area Management Plan
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Hawaii Volcanoes National Park Geologic Resources Inventory Report
National Park Service U.S. Department of the Interior Natural Resource Program Center Hawai‘i Volcanoes National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2009/163 THIS PAGE: Geologists have lloongng been monimonittoorriing the volcanoes of Hawai‘i Volcanoes National Park. Here lalava cascades durduriingng the 1969-1971 Mauna Ulu eruption of Kīlauea VolVolcano. NotNotee the Mauna Ulu fountountaiain in the background. U.S. Geologiogicalcal SurSurvveyey PhotPhotoo by J. B. Judd (12/30/1969). ON THE COVER: ContContiinuouslnuouslyy eruptuptiingng since 1983, Kīllaueaauea Volcano contcontiinues to shapshapee Hawai‘Hawai‘i VoVollccanoes NatiNationalonal ParkPark.. Photo courtesy Lisa Venture/UniversiUniversitty of Cincinnati. Hawai‘i Volcanoes National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2009/163 Geologic Resources Division Natural Resource Program Center P.O. Box 25287 Denver, Colorado 80225 December 2009 U.S. Department of the Interior National Park Service Natural Resource Program Center Denver, Colorado The National Park Service, Natural Resource Program Center publishes a range of reports that address natural resource topics of interest and applicability to a broad audience in the National Park Service and others in natural resource management, including scientists, conservation and environmental constituencies, and the public. The Natural Resource Report Series is used to disseminate high-priority, current natural resource management information with managerial application. The series targets a general, diverse audience, and may contain NPS policy considerations or address sensitive issues of management applicability. All manuscripts in the series receive the appropriate level of peer review to ensure that the information is scientifically credible, technically accurate, appropriately written for the intended audience, and designed and published in a professional manner. -
Guide to the Betty J. Meggers and Clifford Evans Papers
Guide to the Betty J. Meggers and Clifford Evans papers Tyler Stump and Adam Fielding Funding for the processing of this collection was provided by the Smithsonian Institution's Collections Care and Preservation Fund. December 2015 National Anthropological Archives Museum Support Center 4210 Silver Hill Road Suitland, Maryland 20746 [email protected] http://www.anthropology.si.edu/naa/ Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Biographical / Historical.................................................................................................... 2 Scope and Contents........................................................................................................ 5 Arrangement..................................................................................................................... 5 Bibliography...................................................................................................................... 6 Names and Subjects ...................................................................................................... 6 Container Listing ............................................................................................................. 8 Series 1: Personal, 1893-2012................................................................................. 8 Series 2: Writings, 1944-2011............................................................................... -
Discrete Element Modelling of Pit Crater Formation on Mars
geosciences Article Discrete Element Modelling of Pit Crater Formation on Mars Stuart Hardy 1,2 1 ICREA (Institució Catalana de Recerca i Estudis Avançats), Passeig Lluís Companys 23, 08010 Barcelona, Spain; [email protected]; Tel.: +34-934-02-13-76 2 Departament de Dinàmica de la Terra i de l’Oceà, Facultat de Ciències de la Terra, Universitat de Barcelona, C/Martí i Franqués s/n, 08028 Barcelona, Spain Abstract: Pit craters are now recognised as being an important part of the surface morphology and structure of many planetary bodies, and are particularly remarkable on Mars. They are thought to arise from the drainage or collapse of a relatively weak surficial material into an open (or widening) void in a much stronger material below. These craters have a very distinctive expression, often presenting funnel-, cone-, or bowl-shaped geometries. Analogue models of pit crater formation produce pits that typically have steep, nearly conical cross sections, but only show the surface expression of their initiation and evolution. Numerical modelling studies of pit crater formation are limited and have produced some interesting, but nonetheless puzzling, results. Presented here is a high-resolution, 2D discrete element model of weak cover (regolith) collapse into either a static or a widening underlying void. Frictional and frictional-cohesive discrete elements are used to represent a range of probable cover rheologies. Under Martian gravitational conditions, frictional-cohesive and frictional materials both produce cone- and bowl-shaped pit craters. For a given cover thickness, the specific crater shape depends on the amount of underlying void space created for drainage. -
Mars Reconnaissance Orbiter and Opportunity Observations Of
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Mars Reconnaissance Orbiter and Opportunity 10.1002/2014JE004686 observations of the Burns formation: Crater Key Point: hopping at Meridiani Planum • Hydrated Mg and Ca sulfate Burns formation minerals mapped with MRO R. E. Arvidson1, J. F. Bell III2, J. G. Catalano1, B. C. Clark3, V. K. Fox1, R. Gellert4, J. P. Grotzinger5, and MER data E. A. Guinness1, K. E. Herkenhoff6, A. H. Knoll7, M. G. A. Lapotre5, S. M. McLennan8, D. W. Ming9, R. V. Morris9, S. L. Murchie10, K. E. Powell1, M. D. Smith11, S. W. Squyres12, M. J. Wolff3, and J. J. Wray13 1 2 Correspondence to: Department of Earth and Planetary Sciences, Washington University in Saint Louis, Missouri, USA, School of Earth and Space R. E. Arvidson, Exploration, Arizona State University, Tempe, Arizona, USA, 3Space Science Institute, Boulder, Colorado, USA, 4Department of [email protected] Physics, University of Guelph, Guelph, Ontario, Canada, 5Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 6U.S. Geological Survey, Astrogeology Science Center, Flagstaff, Arizona, USA, 7 8 Citation: Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, Massachusetts, USA, Department Arvidson, R. E., et al. (2015), Mars of Geosciences, Stony Brook University, Stony Brook, New York, USA, 9NASA Johnson Space Center, Houston, Texas, USA, Reconnaissance Orbiter and Opportunity 10Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA, 11NASA Goddard Space Flight Center, observations of the Burns formation: Greenbelt, Maryland, USA, 12Department of Astronomy, Cornell University, Ithaca, New York, USA, 13School of Earth and Crater hopping at Meridiani Planum, J. -
Diamond Craters Oregon's Geologic
Text by Ellen M. Benedict, 1985 Features at stops correspond to points on a clock ago, a huge mass of hot gases, volcanic ashes, bits face. Imagine that you are standing in the middle of a of pumice and other pyroclastics (fire-broken rock) Travel And Hiking Hints clock face. Twelve o’clock is the road in front of you violently erupted. The blast – greater than the May and 6 o’clock the road behind. If you always align the 18, 1980, eruption of Mt. St. Helens – deposited a Diamond Craters is located in the high desert country clock face with the road, you should be able to locate layer of pyroclastics 30 to 130 feet thick over an area about 55 miles southeast of Burns, Oregon. It’s an the features. almost 7,000 square miles! isolated place and some precautions should be taken . when traveling in the area. Start Tour. Mileage begins halfway Pyroclastics are between milepost 40 and 41 on State normal behavior Diamond Craters has no tourist facilities. The nearest Highway 205 at the junction to Diamond. for magmas place where gasoline is sold is at Frenchglen. Turn left. (subsurface That’s the opinion held by scores of molten rocks) Keep your scientists and educators who have visited Diamond, Oregon, a small ranching community, was of rhyolitic (a vehicle on named in 1874 for Mace McCoy’s Diamond brand. volcanic material and studied the area. It has the “best and hard-packed The nearby craters soon became known as Diamond related to granite) most diverse basaltic volcanic features in the road surfaces Craters. -
South End Complex Basque Wells & Craters Fires C
SSSOOOUUUTTTHHH EEENNNDDD CCCOOOMMMPPPLLLEEEXXX & BASQUE WELLS & CRATERS FIRES BURNED AREA EMERGENCY STABILIZATION PLAN Bureau of Land Management Burns District Office U.S. Fish and Wildlife Service Malheur National Wildlife Refuge August – September 2006 Prepared1 by U.S. Department of the Interior Burned Area Emergency Response Team BURNED AREA EMERGENCY RESPONSE PLAN South End Complex & Basque Wells & Craters Fires EXECUTIVE SUMMARY This plan addresses emergency stabilization of fire effects resulting from the South End Complex and Basque Wells and Craters Fires that occurred on the Bureau of Land Management, Burns District and Malheur National Wildlife Refuge. The South End Complex includes the Krumbo Butte, Grandad, Pueblo, Trout Creek, and Black Point Fires. The plan has been prepared in accordance with the U.S. Department of the Interior, Department Manual, Part 620: Wildland Fire Management, Chapter 3: Burned Area Emergency Stabilization and Rehabilitation (September, 2003) the Bureau of Land Management (BLM), Emergency Stabilization and Rehabilitation, H-1742-1, and U.S. Fish and Wildlife Service Fire Management Handbook, Chapter 11. The plan also includes recommendations for inter mixed private lands within the burned area. The primary objectives of this Burned Area Emergency Response Plan are: Human Life and Safety • To prescribe post-fire mitigation measures necessary to protect human life and property Soil/Water Stabilization • To promptly stabilize and prevent further degradation to affected watersheds and soils Threatened -
Library QPY OL;I22 *X
_ f NASA-TM-82180 19800025792 NASA Technical Memorandum 821 _,,. _.:.._._ _r _,.x_TM,. A Bibliography of Planetary Geology Principal Investigators and Their Associates, 1979-1980 LIBRarY_QPY OL;I22 _*x_ L,#_C_-EYRESEARCH C,ENTFr...I_ L_BRARY,NASA SEPTEMBER 1980 _tAMPTON,VIRGtNt_ N/L A NASA Technical Memorandum 82180 A Bibliography of Planetary Geology Principal Investigators and Their Associates, 1979-1980 ComI_iled by Ellen Lettvin and Joseph M. Boyce NASA O_ce of Space Science IVashington, D.C. National Aeronautics and Space Administration ScientificandTechnical Information Branch 1980 CONTENTS PAGE General Interest Topics ............................... 3 Solar System, Asteroids, Comets and Satellites ........ 7 Structure, Tectonics, Stratigraphy .................... ii Regolith and Volatiles ................................ 27 Volcanism Studies ..................................... 35 Impact Crater Studies ................................. 43 Eolian Studies ........................................ 51 Fluvial, Glacial, Periglacial and Mass Wasting ........ 61 Remote Sensing, Radar, Photometry ..................... 67 Planetary Mapping, Geological and Cartographic ........ 73 Author/Editor Index ................................... 81 A BIBLIOGRAPHY OF PLANETARY GEOLOGY PRINCIPAL INVESTIGATORS AND THEIR ASSOCIATES, 1979-1980 A compilation of selected bibliographic data specifically relating to recent publications (May 1979 through May 1980) submitted by principal investigators and their associates, supported through NASA's Office of -
Stratigraphy and Sedimentology of a Dry to Wet Eolian Depositional System, Burns Formation, Meridiani Planum, Mars
Earth and Planetary Science Letters 240 (2005) 11–72 www.elsevier.com/locate/epsl Stratigraphy and sedimentology of a dry to wet eolian depositional system, Burns formation, Meridiani Planum, Mars J.P. Grotzinger a,*, R.E. Arvidson b, J.F. Bell III c, W. Calvin d, B.C. Clark e, D.A. Fike a, M. Golombek f, R. Greeley g, A. Haldemann f, K.E. Herkenhoff h, B.L. Jolliff b, A.H. Knoll i, M. Malin j, S.M. McLennan k, T. Parker e, L. Soderblom g, J.N. Sohl-Dickstein b, S.W. Squyres b, N.J. Tosca k, W.A. Watters a a Massachusetts Inst. of Technology, Earth, Atmos. and Planetary Sci., Cambridge, MA 02139, USA b Department Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA c Department of Astronomy, Space Sciences Bldg. Cornell University, Ithaca, NY 14853, USA d University of Nevada, Reno, NV 89501, USA e Lockheed Martin Corporation, Littleton, CO 80127, USA f Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA g Department Geological Sciences, Arizona State University, Box 871404, Tempe, AZ 85287-1404, USA h U.S. Geological Survey, Flagstaff, AZ 86001, USA i Botanical Museum, Harvard University, Cambridge MA 02138, USA j Malin Space Science Systems, Inc., San Diego, CA 92191, USA k Department of Geosciences, State University of New York, Stony Brook, NY 11794-2100, USA Accepted 22 September 2005 Editor: A.N. Halliday Abstract Outcrop exposures of sedimentary rocks at the Opportunity landing site (Meridiani Planum) form a set of genetically related strata defined here informally as the Burns formation. -
Get Smart with Art Is Made Possible with Support from the William K
From the Headlines About the Artist From the Artist Based on the critics’ comments, what aspects of Albert Bierstadt (1830–1902) is Germany in 1830, Albert Bierstadt Bierstadt’s paintings defined his popularity? best known for capturing majestic moved to Massachusetts when he western landscapes with his was a year old. He demonstrated an paintings of awe-inspiring mountain early interest in art and at the age The striking merit of Bierstadt in his treatment of ranges, vast canyons, and tumbling of twenty-one had his first exhibit Yosemite, as of other western landscapes, lies in his waterfalls. The sheer physical at the New England Art Union in power of grasping distances, handling wide spaces, beauty of the newly explored West Boston. After spending several years truthfully massing huge objects, and realizing splendid is evident in his paintings. Born in studying in Germany at the German atmospheric effects. The success with which he does Art Academy in Düsseldorf, Bierstadt this, and so reproduces the noblest aspects of grand returned to the United States. ALBERT BIERSTADT scenery, filling the mind of the spectator with the very (1830–1902) sentiment of the original, is the proof of his genius. A great adventurer with a pioneering California Spring, 1875 Oil on canvas, 54¼ x 84¼ in. There are others who are more literal, who realize details spirit, Bierstadt joined Frederick W. Lander’s Military Expeditionary Presented to the City and County of more carefully, who paint figures and animals better, San Francisco by Gordon Blanding force, traveling west on the overland who finish more smoothly; but none except Church, and 1941.6 he in a different manner, is so happy as Bierstadt in the wagon route from Saint Joseph, Watkins Yosemite Art Gallery, San Francisco. -
USGS Professional Paper 1350, Vol. 2 of 2
VOLCANISM IN HAWAII Chapter 59 THE ROLE OF LAVA TUBES IN HAWAIIAN VOLCANOES By Ronald Greeley I ABSTRACT set on the initiation and evolution of lava tubes and their associated Lava tubes develop from eruptions that typically involve: flows. (1) moderate rates of effusion, (2) durations greater than one or Numerous studies of lava tubes have been made in areas two days, and (3) effusion of fluid lava (for example, pahoehoe) outside Hawaii, including Mount Elna (Guest and others, 1980), that has not been greatly degassed. Although some fountain-fed Mount St. Helens (Greeley and Hyde, 1972), and New Mexico lava and aa flows can fonn lava tubes, such occurrences are rare (Hatheway and Herring, 1970). From these studies and those in in Hawaii. Lava tubes feed flows: (1) directly from the vent (acting as extensions of the conduit), (2) from various holding Hawaii, lava tubes clearly reflect a particular style of volcanism and reservoirs (for example, lava ponds, lava lakes, filled pit cra are the primary means for the spread of some types of lava flows. ters), and (3) from flows on the flanks of volcanoes. Historical flows of greatest length in Hawaii were emplaced primarily via lava tubes, and many subaqueous flows involve lava tubes. 166'00' 166'00' Sustained flow of lava in tubes appears capable of erosion into preflow terrain. Photogeological analyses suggest that at least 30 percent of the flows (by area) on Mauna Loa, 58 percent of the flows on Kilauea, and 18 percentof the flows on Mount Etna were at least partly emplaced via tubes. -
Candidate Cave Entrances on Mars
G.E. Cushing – Candidate cave entrances on Mars. Journal of Cave and Karst Studies, v. 74, no. 1, p. 33–47. DOI: 10.4311/ 2010EX0167R CANDIDATE CAVE ENTRANCES ON MARS GLEN E. CUSHING U.S. Geological Survey, Astrogeology Science Center, 2255 N. Gemini Dr., Flagstaff, AZ 86001, USA, [email protected] Abstract: This paper presents newly discovered candidate cave entrances into Martian near-surface lava tubes, volcano-tectonic fracture systems, and pit craters and describes their characteristics and exploration possibilities. These candidates are all collapse features that occur either intermittently along laterally continuous trench-like depressions or in the floors of sheer-walled atypical pit craters. As viewed from orbit, locations of most candidates are visibly consistent with known terrestrial features such as tube-fed lava flows, volcano-tectonic fractures, and pit craters, each of which forms by mechanisms that can produce caves. Although we cannot determine subsurface extents of the Martian features discussed here, some may continue unimpeded for many kilometers if terrestrial examples are indeed analogous. The features presented here were identified in images acquired by the Mars Odyssey’s Thermal Emission Imaging System visible- wavelength camera, and by the Mars Reconnaissance Orbiter’s Context Camera. Select candidates have since been targeted by the High-Resolution Imaging Science Experi- ment. Martian caves are promising potential sites for future human habitation and astrobiology investigations; understanding their characteristics is critical for long-term mission planning and for developing the necessary exploration technologies. INTRODUCTION cosmic rays (e.g., Mazur et al., 1978; De Angeles et al., 2002; Boston et al., 2004; Cushing et al., 2007). -
Tuesday, May 4, 2021 1. Call to Order 2:30 Pm Leiopapa a Kamehameha Building Office
HA WAI'I BOARDON GEOGRAPHIC NAMES (HBGN) Tuesday, May 4, 2021 2:30 p.m. Leiopapa A Kamehameha Building Officeof Planning, 6th Floor Conference Room 235 S. Beretania Street Honolulu, Hawai'i 96813 Zoom Meeting information: https://bit.ly/hbgn-20210504 Meeting ID: 932 3302 1740 Passcode: 581819 1. Call to Order 2. Review ofMeeting Minutes forApril 6, 2021 3. Public Comments 4. Announcements 5. Status ofbills and resolutions in the Legislature 6. Discussion and Action on Permitted Interaction Group for Lo'ihi / Kama'ehu 7. Review selected place names on the island ofHawai'i (Camara) 8. Adjournment This meeting of the Hawai'i Board on Geographic Names (HBGN) will be available forlive viewing via Zoom. Zoom Meeting information: https://bit.ly/hbgn-20210504 or https://zoom.us/j/93233021740?pwd=Ui9LbmxwMERYRkhDWDR WUHZaeHFRdz09 Meeting ID: 932 3302 1740 Passcode: 581819 MINUTES DRAFT FOR THE MEETING OF THE HAWAI‘I BOARD ON GEOGRAPHIC NAMES DATE: April 6, 2021 TIME: 2:30 p.m. PLACE: Leiopapa A Kamehameha Building Office of Planning, 6th Floor Library 235 S. Beretania Street Honolulu, Hawai‘i 96813 AGENDA ITEM 1: Call to Order Mr. Marzan called the meeting to order at 2:36 p.m. The following were in attendance: MEMBERS: Marques Marzan (Bishop Museum) Arthur Buto for Mary Alice Evans (Office of Planning) Meyer Cummins (Land Survey Division) Holly McEldowney (Department of Land and Natural Resources) left early at 3:20pm Niniau Kawaihae (Department of Hawaiian Home Lands) Kapā Oliveira (University of Hawaiʻi at Mānoa) Brad Kaʻaleleo Wong (Office of Hawaiian Affairs) ABSENT: None GUESTS: Jennifer Runyon (USGS) Lāmaku Mikahala Roy Melia Lane-Kamahele Regina Hilo Bobby Camara Renee Pualani Louis Catherine Sullivan AGENDA ITEM 2: Review of Meeting Minutes for March 2, 2021 Lamakū Roy asked for her attendance to be recognized and that she is here to comment on the minutes from the March meeting.