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ROSS T. SHINYAMA #8830-0 SUMMER II. Kaiawtr I+9599-O First L-Lawaiian Center 999 Bishop Street, 23Rd Floor
WATANABI] ING I-LP A Limited Liability [,aw Parrnership ":r : , 1 I ' I J. DOUGLAS ING #1538-0 i.,,i l i t I i '.tì ROSS T. SHINYAMA #8830-0 SUMMER II. KAIAWtr I+9599-O First l-lawaiian Center 999 Bishop Street, 23rd Floor Honolulu, Ilawaii 968 1 3 Telephone No.: (808) 544-8300 Facsimile No.: (808) 544-8399 E-mails : [email protected] Attorneys for TMT INTBRNATIONAL OBSBRVATORY, I,LC BOARD OF LAND AND NATURAL RESOURCES FOR THE STATE OF I]AWAI'I IN THE MATTER OF Case No. BLNR-CC -16-002 TMT INTERNATIONAL A Contested Case l{earing Re Conservation OBSBRVATORY, LLC'S PRE-HEARING District Use Permit (CDUP) I{A-3568 for the STATEMENT; EXHIBIT ..1,'; Thirty Meter Telescope at the Mauna Kea CERTIFICATE OF SERVICE Science Reserve, I(a'ohe Mauka, Hãmakua District, Island of Hawai'i, TMK (3) 4-4- 0l 5:009 TABLtr OF CONTBNTS IN'IRODUC]'ION II DI]SCRIPI'ION OF THE PROJECT AND ITS PROCI]DURAL HISTORY A. Description ofthe Project.................. 3 B. Procedulal Llistory 3 l. General Lease and the MI(SR 3 2. T'he Project 5 III. BURDEN OF PROOF I IV. ISSUES TO BE DECIDED AND TIO'S STATEMENT OF POSI'|iON.. A. The Project, Including the Plans Incorporatcd in the Application, is Consistent with Chapter 183C of the Hawai'i Revised Statutes, the Criteria in HAR $ 13-5- 30(c), and Other Applicable Conservation District Rules......... ..........9 i. The Project is consistent with the purpose of the Conservation District.. 10 2. The Project is consistent with the objectives of the sub2one................... -
“Mining” Water Ice on Mars an Assessment of ISRU Options in Support of Future Human Missions
National Aeronautics and Space Administration “Mining” Water Ice on Mars An Assessment of ISRU Options in Support of Future Human Missions Stephen Hoffman, Alida Andrews, Kevin Watts July 2016 Agenda • Introduction • What kind of water ice are we talking about • Options for accessing the water ice • Drilling Options • “Mining” Options • EMC scenario and requirements • Recommendations and future work Acknowledgement • The authors of this report learned much during the process of researching the technologies and operations associated with drilling into icy deposits and extract water from those deposits. We would like to acknowledge the support and advice provided by the following individuals and their organizations: – Brian Glass, PhD, NASA Ames Research Center – Robert Haehnel, PhD, U.S. Army Corps of Engineers/Cold Regions Research and Engineering Laboratory – Patrick Haggerty, National Science Foundation/Geosciences/Polar Programs – Jennifer Mercer, PhD, National Science Foundation/Geosciences/Polar Programs – Frank Rack, PhD, University of Nebraska-Lincoln – Jason Weale, U.S. Army Corps of Engineers/Cold Regions Research and Engineering Laboratory Mining Water Ice on Mars INTRODUCTION Background • Addendum to M-WIP study, addressing one of the areas not fully covered in this report: accessing and mining water ice if it is present in certain glacier-like forms – The M-WIP report is available at http://mepag.nasa.gov/reports.cfm • The First Landing Site/Exploration Zone Workshop for Human Missions to Mars (October 2015) set the target -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Permafrost and Active Layer Research on James Ross Island: an Overview
CZECH POLAR REPORTS 9 (1): 20-36, 2019 Permafrost and active layer research on James Ross Island: An overview Filip Hrbáček1*, Daniel Nývlt1, Kamil Láska1, Michaela Kňažková1, Barbora Kampová1, Zbyněk Engel2, Marc Oliva3, Carsten W. Mueller4 1Masaryk University, Faculty of Science, Department of Geography, Brno, Czech Republic 2Charles University, Faculty of Science, Department of Physical Geography and Geoecology, Praha, Czech Republic 3Department of Geography, Universitat de Barcelona, Barcelona, Spain 4Lehrstuhl für Bodenkunde, TU München, Freising-Weihenstephan 85356, Germany Abstract This study summarizes the current state of the active layer and permafrost research on James Ross Island. The analysis of climate parameters covers the reference period 2011– 2017. The mean annual air temperature at the AWS-JGM site was -6.9°C (ranged from -3.9°C to -8.2°C). The mean annual ground temperature at the depth of 5 cm was -5.5°C (ranged from -3.3°C to -6.7°C) and it also reached -5.6°C (ranged from -4.0 to -6.8°C) at the depth of 50 cm. The mean daily ground temperature at the depth of 5 cm correlated moderately up to strongly with the air temperature depending on the season of the year. Analysis of the snow effect on the ground thermal regime confirmed a low insulating effect of snow cover when snow thickness reached up to 50 cm. A thicker snow accumu- lation, reaching at least 70 cm, can develop around the hyaloclastite breccia boulders where a well pronounced insulation effect on the near-surface ground thermal regime was observed. -
Lunar Crater Volcanic Field (Reveille and Pancake Ranges, Basin and Range Province, Nevada, USA)
Research Paper GEOSPHERE Lunar Crater volcanic field (Reveille and Pancake Ranges, Basin and Range Province, Nevada, USA) 1 2,3 4 5 4 5 1 GEOSPHERE; v. 13, no. 2 Greg A. Valentine , Joaquín A. Cortés , Elisabeth Widom , Eugene I. Smith , Christine Rasoazanamparany , Racheal Johnsen , Jason P. Briner , Andrew G. Harp1, and Brent Turrin6 doi:10.1130/GES01428.1 1Department of Geology, 126 Cooke Hall, University at Buffalo, Buffalo, New York 14260, USA 2School of Geosciences, The Grant Institute, The Kings Buildings, James Hutton Road, University of Edinburgh, Edinburgh, EH 3FE, UK 3School of Civil Engineering and Geosciences, Newcastle University, Newcastle, NE1 7RU, UK 31 figures; 3 tables; 3 supplemental files 4Department of Geology and Environmental Earth Science, Shideler Hall, Miami University, Oxford, Ohio 45056, USA 5Department of Geoscience, 4505 S. Maryland Parkway, University of Nevada Las Vegas, Las Vegas, Nevada 89154, USA CORRESPONDENCE: gav4@ buffalo .edu 6Department of Earth and Planetary Sciences, 610 Taylor Road, Rutgers University, Piscataway, New Jersey 08854-8066, USA CITATION: Valentine, G.A., Cortés, J.A., Widom, ABSTRACT some of the erupted magmas. The LCVF exhibits clustering in the form of E., Smith, E.I., Rasoazanamparany, C., Johnsen, R., Briner, J.P., Harp, A.G., and Turrin, B., 2017, overlapping and colocated monogenetic volcanoes that were separated by Lunar Crater volcanic field (Reveille and Pancake The Lunar Crater volcanic field (LCVF) in central Nevada (USA) is domi variable amounts of time to as much as several hundred thousand years, but Ranges, Basin and Range Province, Nevada, USA): nated by monogenetic mafic volcanoes spanning the late Miocene to Pleisto without sustained crustal reservoirs between the episodes. -
Biodiversity in Sub-Saharan Africa and Its Islands Conservation, Management and Sustainable Use
Biodiversity in Sub-Saharan Africa and its Islands Conservation, Management and Sustainable Use Occasional Papers of the IUCN Species Survival Commission No. 6 IUCN - The World Conservation Union IUCN Species Survival Commission Role of the SSC The Species Survival Commission (SSC) is IUCN's primary source of the 4. To provide advice, information, and expertise to the Secretariat of the scientific and technical information required for the maintenance of biologi- Convention on International Trade in Endangered Species of Wild Fauna cal diversity through the conservation of endangered and vulnerable species and Flora (CITES) and other international agreements affecting conser- of fauna and flora, whilst recommending and promoting measures for their vation of species or biological diversity. conservation, and for the management of other species of conservation con- cern. Its objective is to mobilize action to prevent the extinction of species, 5. To carry out specific tasks on behalf of the Union, including: sub-species and discrete populations of fauna and flora, thereby not only maintaining biological diversity but improving the status of endangered and • coordination of a programme of activities for the conservation of bio- vulnerable species. logical diversity within the framework of the IUCN Conservation Programme. Objectives of the SSC • promotion of the maintenance of biological diversity by monitoring 1. To participate in the further development, promotion and implementation the status of species and populations of conservation concern. of the World Conservation Strategy; to advise on the development of IUCN's Conservation Programme; to support the implementation of the • development and review of conservation action plans and priorities Programme' and to assist in the development, screening, and monitoring for species and their populations. -
Silicic Volcanism on Mars Evidenced by Tridymite in High-Sio2 Sedimentary Rock at Gale Crater Richard V
Silicic volcanism on Mars evidenced by tridymite in high-SiO2 sedimentary rock at Gale crater Richard V. Morrisa,1, David T. Vanimanb, David F. Blakec, Ralf Gellertd, Steve J. Chiperae, Elizabeth B. Rampef, Douglas W. Minga, Shaunna M. Morrisong, Robert T. Downsg, Allan H. Treimanh, Albert S. Yeni, John P. Grotzingerj,1, Cherie N. Achillesg, Thomas F. Bristowc, Joy A. Crispi, David J. Des Maraisc, Jack D. Farmerk, Kim V. Fendrichg, Jens Frydenvangl,m, Trevor G. Graffn, John-Michael Morookiani, Edward M. Stolperj, and Susanne P. Schwenzerh,o aNASA Johnson Space Center, Houston, TX 77058; bPlanetary Science Institute, Tucson, AZ 85719; cNASA Ames Research Center, Moffitt Field, CA 94035; dDepartment of Physics, University of Guelph, Guelph, ON, Canada N1G 2W1; eChesapeake Energy, Oklahoma City, OK 73118; fAerodyne Industries, Houston, TX 77058; gDepartment of Geosciences, University of Arizona, Tucson, AZ 85721; hLunar and Planetary Institute, Houston, TX 77058; iJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109; jDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125; kSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287; lLos Alamos National Laboratory, Los Alamos, NM 87545; mNiels Bohr Institute, University of Copenhagen, 2100 Copenhagen, Denmark; nJacobs, Houston, TX 77058; and oDepartment of Environment, Earth and Ecosystems, The Open University, Milton Keynes MK7 6AA, United Kingdom Contributed by John P. Grotzinger, May 5, 2016 (sent for review March 18, 2016); reviewed by Jon Blundy, Robert M. Hazen, and Harry Y. McSween) Tridymite, a low-pressure, high-temperature (>870 °C) SiO2 poly- (1), where three drill samples were analyzed by CheMin [Confi- morph, was detected in a drill sample of laminated mudstone (Buck- dence Hills, Mojave2, and Telegraph Peak (2)]. -
Lectures on Geothermal in Kenya and Africa
GEOTHERMAL TRAINING PROGRAMME Reports 2005 Orkustofnun, Grensásvegur 9, Number 4 IS-108 Reykjavík, Iceland LECTURES ON GEOTHERMAL IN KENYA AND AFRICA Martin N. Mwangi (lecturer and co-ordinator) Kenya Electricity Generating Co., Ltd. - KenGen Olkaria Geothermal Project P.O. Box 785 Naivasha KENYA Lectures on geothermal energy given in September 2005 United Nations University, Geothermal Training Programme Reykjavík, Iceland Published in April 2006 ISBN - 9979-68-187-X Mwangi ii Lectures PREFACE Kenya is the leading African country in geothermal exploration and development. Electricity generation from geothermal started in 1981 at the Olkaria I power station. In 2005 the installed generation capacity is 129 MWe, and the electricity production constitutes 11% of the total electricity production in the country. There is a plan to increase the generation capacity by 576 MWe by 2026. Behind all this is the Kenya Electricity Generating Company Ltd. (KenGen) and their very able staff. The UNU Visiting Lecturer 2005 was Mr. Martin N. Mwangi, Chief Manager of KenGen´s Olkaria Geothermal Project, who is one of the leading geothermal experts of Africa. He received training in geophysical exploration as UNU Fellow at the UNU-GTP in 1982. With him came a geochemist (Mr. Zaccheus Muna) and a drilling engineer (Mr. Joseph Ng´ang´a). Including the trio from that vintage year in geothermal studies, a total of 37 Kenyans have completed the six months specialized training at the UNU-GTP. Of these, 33 have come from KenGen. Martin gave an excellent summary of geothermal work in Kenya. In the first lecture (co-authored by Mrs. -
Mars Pathfinder Landing Site Workshop Ii: Characteristics of the Ares Vallis Region and Field Trips in the Channeled Scabland, Washington
/, NASA-CR-200508 L / MARS PATHFINDER LANDING SITE WORKSHOP II: CHARACTERISTICS OF THE ARES VALLIS REGION AND FIELD TRIPS IN THE CHANNELED SCABLAND, WASHINGTON LPI Technical Report Number 95-01, Part 1 Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI/TR--95-01, Part 1 "lp MARS PATHFINDER LANDING SITE WORKSHOP II: CHARACTERISTICS OF THE ARES VALLIS REGION AND FIELD TRIPS IN THE CHANNELED SCABLAND, WASHINGTON Edited by M. P. Golombek, K. S. Edgett, and J. W. Rice Jr. Held at Spokane, Washington September 24-30, 1995 Sponsored by Arizona State University Jet Propulsion Laboratory Lunar and Planetary Institute National Aeronautics and Space Administration Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 95-01, Part 1 LPI/TR--95-01, Part 1 Compiled in 1995 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the University Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may he copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may he cited as Golomhek M. P., Edger K. S., and Rice J. W. Jr., eds. ( 1992)Mars Pathfinder Landing Site Workshop 11: Characteristics of the Ares Vallis Region and Field Trips to the Channeled Scabland, Washington. LPI Tech. Rpt. 95-01, Part 1, Lunar and Planetary Institute, Houston. 63 pp. -
NASA Astronauts
PUBLISHED BY Public Affairs Divisio~l Washington. D.C. 20546 1983 IColor4-by-5 inch transpar- available free to information lead and sent to: Non-informstionmedia may obtain identical material for a fee through a photographic contractor by using the order forms in the rear of this book. These photqraphs are government publications-not subject to copyright They may not be used to state oiimply the endorsement by NASA or by any NASA employee of a commercial product piocess or service, or used in any other manner that might mislead. Accordingly, it is requested that if any photograph is used in advertising and other commercial promotion. layout and copy be submitted to NASA prior to release. Front cover: "Lift-off of the Columbia-STS-2 by artist Paul Salmon 82-HC-292 82-ti-304 r 8arnr;w u vowzn u)rorr ~ nsrvnv~~nrnno................................................ .-- Seasat .......................................................................... 197 Skylab 1 Selected Pictures .......................................................150 Skylab 2 Selected Pictures ........................................................ 151 Skylab 3 Selected Pictures ........................................................152 Skylab 4 Selected Pictures ........................................................ 153 SpacoColony ...................................................................183 Space Shuttle ...................................................................171 Space Stations ..................................................................198 \libinn 1 1f.d Apoiio 17/Earth 72-HC-928 72-H-1578 Apolb B/Earth Rise 68-HC-870 68-H-1401 Voyager ;//Saturn 81-HC-520 81-H-582 Voyager I/Ssturian System 80-HC-647 80-H-866 Voyager IN~lpiterSystem 79-HC-256 79-H-356 Viking 2 on Mars 76-HC-855 76-H-870 Apollo 11 /Aldrin 69-HC-1253 69-H-682 Apollo !I /Aldrin 69-HC-684 69-H-1255 STS-I /Young and Crippen 79-HC-206 79-H-275 STS-1- ! QTPLaunch of the Columbia" 82-HC-23 82-H-22 Major Launches NAME UUNCH VEHICLE MISSIONIREMARKS 1956 VANGUARD Dec. -
1912 the Mountaineers
The Mountaineer. Volume Five Nineteen Hundred Twelve h611, •• , ,, The Mountaineen Sea11le. Wa1hla1100 :J1'.)1'1zec1 bv G oog I e 2,-�a""" ...._� _..,..i..c.. tyJ Vi) Copyright 1912 The Mountaineers Din,tiZ<'d by Google CONTENTS Page Greeting ................... ................................John Muir .......................................... Greeting ..................................................... Enos Mills ........................................ The Higher Functions of a Mountain Club................................................... \ Wm. Frederic Bade.......................... 9 Little Tahoma ............ ............................. .Edmond S. Meany............................ 13 Mountaineer Outing of 1912 on north side of Mt. Rainier....................... Mary Paschall ................................... 14 Itinerary of Outing of 1912................... .Charles S. Gleason........................... 26 The Ascent of Mt. Rainier.................... £. M.Hack ........................................ 28 Grand Park .............................................. 1=dmond S. Meany............................ 36 A New Route up Mt. Rainier.............. 'Jara Keen ........................................ 37 Naches Pass .............................................. Edmond S. Meany....... ,.................... 40 Undescribed Glaciers of Mt. Rainier .. Fran,ois Matthes ............................. 42 Thermal Caves ....................................... J. B. Flett .......................................... 58 Change in Willis