Mt. Erebus Surprises Ross Island Inhabitants in This Issue Mt
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THE MOUNT EREBUS TRAGEDY Air New Zealand DC10-30 ZK-NZP, Flight NZ901 Th 28 November 1979
THE MOUNT EREBUS TRAGEDY Air New Zealand DC10-30 ZK-NZP, Flight NZ901 th 28 November 1979 A REVIEW WAVERLEY PARSONS Graduate Certificate in Antarctic Studies 2003 1 TABLE OF CONTENTS ABSTRACT ................................................................................................................... 2 Introduction ................................................................................................. 3 Prelude: Before the Flight of NZ901 .......................................................... 4 Flight Preparation .......................................................................................................... 4 The Flight Path ............................................................................................................... 5 The Accident ............................................................................................... 7 Sector Whiteout ............................................................................................................. 8 Discovery of Wreckage ............................................................................................... 10 ‘Operation Overdue’ .................................................................................................... 12 The Aftermath ...........................................................................................14 The Offical Aircraft Accident Report – ‘Chippindale’s Report’ ................................. 14 The Royal Commission of Inquiry ............................................................................. -
MID-LATITUDE MARTIAN ICE AS a TARGET for HUMAN EXPLORATION, ASTROBIOLOGY, and IN-SITU RESOURCE UTILIZATION. D. Viola1 ([email protected]), A
First Landing Site/Exploration Zone Workshop for Human Missions to the Surface of Mars (2015) 1011.pdf MID-LATITUDE MARTIAN ICE AS A TARGET FOR HUMAN EXPLORATION, ASTROBIOLOGY, AND IN-SITU RESOURCE UTILIZATION. D. Viola1 ([email protected]), A. S. McEwen1, and C. M. Dundas2. 1University of Arizona, Department of Planetary Sciences, 2USGS, Astrogeology Science Center. Introduction: Future human missions to Mars will region of late Noachian highlands terrain, and is com- need to rely on resources available near the Martian prised of a series of grabens and ridges surrounded by surface. Water is of primary importance, and is known later Hesperian/Amazonian lava flows from the Thar- to be abundant on Mars in multiple forms, including sis region [7]. The proposed landing site is within these hydrated minerals [1] and pore-filling and excess ice lava flows (HAv), and provides access to a region of deposits [2]. Of these sources, excess ice (or ice which late Hesperian lowlands in the western region of the exceeds the available regolith pore space) may be the EZ. There is evidence for Amazonian glacial and peri- most promising for in-situ resource utilization (ISRU). glacial activity [e.g., HiRISE images Since Martian excess ice is thought to contain a low PSP_008671_2210 and ESP_017374_2210], and the fraction of dust and other contaminants (~<10% by Gamma Ray Spectrometer water map suggests that volume, [3]) only a modest deposit of excess ice will there is abundant subsurface ice in the uppermost me- be sufficient to support a human presence. ter within this region [10]. Meandering channel-like Subsurface water ice may also be of astrobiological features have been identified in HiRISE images (e.g., interest as a potential current habitat or as a preserva- PSP_003529_2195 in close proximity to apparent ice tion medium for biosignatures. -
DRAFT COMPREHENSIVE ENVIRONMENTAL EVALUATION (CEE) for ANDRILL Mcmurdo Sound Portfolio Madrid, 9/20 De Junio 2003
XXVI ATCM Working Paper WP-002-NZ Agenda Item: IV CEP 4a NEW ZEALAND Original: English DRAFT COMPREHENSIVE ENVIRONMENTAL EVALUATION (CEE) FOR ANDRILL McMurdo Sound Portfolio Madrid, 9/20 de junio 2003 ANDRILL - The McMurdo Sound Portfolio An international research effort with the participation of Germany, Italy, New Zealand, the United Kingdom and the United States of America. DRAFT COMPREHENSIVE ENVIRONMENTAL EVALUATION (CEE) FOR ANDRILL McMurdo Sound Portfolio Antarctica New Zealand Private Bag 4745, Christchurch Administration Building International Antarctic Centre 38 Orchard Road, Christchurch January 22, 2003 2 CONTENTS 1. NON-TECHNICAL SUMMARY.....................................................................................11 2. INTRODUCTION...........................................................................................................13 2.1 What is ANDRILL?...............................................................................................13 2.2 The CEE process.................................................................................................15 2.2.1 What is a CEE and why is it needed?....................................................15 2.2.2 Process for preparing the Draft CEE .....................................................15 3. DESCRIPTION OF PROPOSED ACTIVITES ..............................................................17 2.1 Purpose and Need...............................................................................................17 3.1.1 Scientific justification..............................................................................17 -
Federal Register/Vol. 84, No. 78/Tuesday, April 23, 2019/Rules
Federal Register / Vol. 84, No. 78 / Tuesday, April 23, 2019 / Rules and Regulations 16791 U.S.C. 3501 et seq., nor does it require Agricultural commodities, Pesticides SUPPLEMENTARY INFORMATION: The any special considerations under and pests, Reporting and recordkeeping Antarctic Conservation Act of 1978, as Executive Order 12898, entitled requirements. amended (‘‘ACA’’) (16 U.S.C. 2401, et ‘‘Federal Actions to Address Dated: April 12, 2019. seq.) implements the Protocol on Environmental Justice in Minority Environmental Protection to the Richard P. Keigwin, Jr., Populations and Low-Income Antarctic Treaty (‘‘the Protocol’’). Populations’’ (59 FR 7629, February 16, Director, Office of Pesticide Programs. Annex V contains provisions for the 1994). Therefore, 40 CFR chapter I is protection of specially designated areas Since tolerances and exemptions that amended as follows: specially managed areas and historic are established on the basis of a petition sites and monuments. Section 2405 of under FFDCA section 408(d), such as PART 180—[AMENDED] title 16 of the ACA directs the Director the tolerance exemption in this action, of the National Science Foundation to ■ do not require the issuance of a 1. The authority citation for part 180 issue such regulations as are necessary proposed rule, the requirements of the continues to read as follows: and appropriate to implement Annex V Regulatory Flexibility Act (5 U.S.C. 601 Authority: 21 U.S.C. 321(q), 346a and 371. to the Protocol. et seq.) do not apply. ■ 2. Add § 180.1365 to subpart D to read The Antarctic Treaty Parties, which This action directly regulates growers, as follows: includes the United States, periodically food processors, food handlers, and food adopt measures to establish, consolidate retailers, not States or tribes. -
Geology of Hut Point Peninsula, Ross Island
significantly below their Curie temperatures (approxi- Wilson, R. L., and N. D. Watkins. 1967. Correlation of mately 550°C.). petrology and natural magnetic polarity in Columbia Plateau basalts. Geophysical Journal of the Royal Astro- Previous work (Pucher, 1969; Stacey and Banerjee, nomical Society, 12(4): 405-424. 1974) indicates that the CRM intensity acquired in a low field is significantly less than the TRM intensity. It thus would appear that if a CRM induced at temperatures considerably below the Curie tempera- Geology of Hut Point Peninsula, ture, contributes a significant proportion to the ob- Ross Island served NRM intensity, too low an intensity value will be assigned to the ancient field. Although it is too early to report a firm value for PHILIP R. KYLE the intensity of the ancient field during the imprint- Department of Geology ing of unit 13 and related flows, we think that the Victoria University strength of the ambient field was more likely to Wellington, New Zealand have been about 0.5 oe (based on samples at about 141 meters) than about 0.1 oe (based on samples SAMUEL B. TREVES 122.18 and 126.06 meters). The virtual dipole Department of Geology moment (Smith, 1967b) calculated for an estimated University of Nebraska field intensity of 0.5 oe at the site is 7 X 10 25 gauss Lincoln, Nebraska 68508 cubic centimeters. This is larger than the value of 5.5 X 1025 gauss cubic centimeters (Smith, 1967b) Hut Point Peninsula is about 20 kilometers long calculated on the basis of paleointensity experiments and 2 to 4 kilometers wide. -
U.S. Advance Exchange of Operational Information, 2005-2006
Advance Exchange of Operational Information on Antarctic Activities for the 2005–2006 season United States Antarctic Program Office of Polar Programs National Science Foundation Advance Exchange of Operational Information on Antarctic Activities for 2005/2006 Season Country: UNITED STATES Date Submitted: October 2005 SECTION 1 SHIP OPERATIONS Commercial charter KRASIN Nov. 21, 2005 Depart Vladivostok, Russia Dec. 12-14, 2005 Port Call Lyttleton N.Z. Dec. 17 Arrive 60S Break channel and escort TERN and Tanker Feb. 5, 2006 Depart 60S in route to Vladivostok U.S. Coast Guard Breaker POLAR STAR The POLAR STAR will be in back-up support for icebreaking services if needed. M/V AMERICAN TERN Jan. 15-17, 2006 Port Call Lyttleton, NZ Jan. 24, 2006 Arrive Ice edge, McMurdo Sound Jan 25-Feb 1, 2006 At ice pier, McMurdo Sound Feb 2, 2006 Depart McMurdo Feb 13-15, 2006 Port Call Lyttleton, NZ T-5 Tanker, (One of five possible vessels. Specific name of vessel to be determined) Jan. 14, 2006 Arrive Ice Edge, McMurdo Sound Jan. 15-19, 2006 At Ice Pier, McMurdo. Re-fuel Station Jan. 19, 2006 Depart McMurdo R/V LAURENCE M. GOULD For detailed and updated schedule, log on to: http://www.polar.org/science/marine/sched_history/lmg/lmgsched.pdf R/V NATHANIEL B. PALMER For detailed and updated schedule, log on to: http://www.polar.org/science/marine/sched_history/nbp/nbpsched.pdf SECTION 2 AIR OPERATIONS Information on planned air operations (see attached sheets) SECTION 3 STATIONS a) New stations or refuges not previously notified: NONE b) Stations closed or refuges abandoned and not previously notified: NONE SECTION 4 LOGISTICS ACTIVITIES AFFECTING OTHER NATIONS a) McMurdo airstrip will be used by Italian and New Zealand C-130s and Italian Twin Otters b) McMurdo Heliport will be used by New Zealand and Italian helicopters c) Extensive air, sea and land logistic cooperative support with New Zealand d) Twin Otters to pass through Rothera (UK) upon arrival and departure from Antarctica e) Italian Twin Otter will likely pass through South Pole and McMurdo. -
Continental Field Manual 3 Field Planning Checklist: All Field Teams Day 1: Arrive at Mcmurdo Station O Arrival Brief; Receive Room Keys and Station Information
PROGRAM INFO USAP Operational Risk Management Consequences Probability none (0) Trivial (1) Minor (2) Major (4) Death (8) Certain (16) 0 16 32 64 128 Probable (8) 0 8 16 32 64 Even Chance (4) 0 4 8 16 32 Possible (2) 0 2 4 8 16 Unlikely (1) 0 1 2 4 8 No Chance 0% 0 0 0 0 0 None No degree of possible harm Incident may take place but injury or illness is not likely or it Trivial will be extremely minor Mild cuts and scrapes, mild contusion, minor burns, minor Minor sprain/strain, etc. Amputation, shock, broken bones, torn ligaments/tendons, Major severe burns, head trauma, etc. Injuries result in death or could result in death if not treated Death in a reasonable time. USAP 6-Step Risk Assessment USAP 6-Step Risk Assessment 1) Goals Define work activities and outcomes. 2) Hazards Identify subjective and objective hazards. Mitigate RISK exposure. Can the probability and 3) Safety Measures consequences be decreased enough to proceed? Develop a plan, establish roles, and use clear 4) Plan communication, be prepared with a backup plan. 5) Execute Reassess throughout activity. 6) Debrief What could be improved for the next time? USAP Continental Field Manual 3 Field Planning Checklist: All Field Teams Day 1: Arrive at McMurdo Station o Arrival brief; receive room keys and station information. PROGRAM INFO o Meet point of contact (POC). o Find dorm room and settle in. o Retrieve bags from Building 140. o Check in with Crary Lab staff between 10 am and 5 pm for building keys and lab or office space (if not provided by POC). -
Mt. Erebus: Mt
8 7 Mt. Erebus Image Gallery. Image Erebus Mt. Pennycook, Jean of courtesy Photo hut. point up into the sky! the into up point and melt ice the makes steam The rock. the in Opening to an ice tower near the lower Erebus Erebus lower the near tower ice an to Opening They look like icicles that that icicles like look They cracks through sides the out comes volcano the it freezes into pillars. pillars. into freezes it of inside the from Steam hot. very is volcano moves into the cold air, air, cold the into moves the of inside the But long. year all ice and ice. When the hot steam steam hot the When ice. snow by covered is Erebus Mt. that means This forms caves made out of of out made caves forms Antarctica. near is It place. cold a is Island Ross MT. EREBUS: A SURPRISING VOLCANO SURPRISING A EREBUS: MT. VOLCANO SURPRISING A EREBUS: MT. http://beyondpenguins.nsdl.org ABOUT THE AUTHOR Jessica Fries-Gaither Issue 9: Earth’s Changing Surface Elementary Resource Specialist, (December 2008) The Ohio State University Copyright December 2008 – The Ohio State University Jessica taught at the elementary level (grades 4-6) Supported by the National and middle school (grades 5-8 math and science) Science Foundation in Memphis, TN and Anchorage, AK. Her work with MT. EREBUS: Beyond Penguins and Polar Bears involves creating Licensed Under a Creative Commons license. A SURPRISING VOLCANO and managing content for the magazine and blog. http://creativecommons.org/licenses/by-sa/3.0/ BY JESSICA FRIES-GAITHER Find this story and others at: DECEMBER 2008 http://beyondpenguins.nsdl.org/information.php?topic=stories Flesch - Kincaid RL = 3.7 13 2 60 °S ANTARCTICA like to study volcanoes, too? volcanoes, study to like about what happens deep inside it. -
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The Red Planet's Watery Past
New observations by rovers and orbiters indicate that liquid water not only existed on Mars, it once covered large parts of the planet’s surface, perhaps for more than a billion years WATER FLOWS ACROSS the Martian surface in an artist’s rendering of how the Red Planet may have looked 2.5 billion to four billion years ago. Salt deposits along the water’s edge C REDI T appear purple in this twilight view. 62 SCIENTIFIC AMERICAN DECEMBER 2006 COPYRIGHT 2006 SCIENTIFIC AMERICAN, INC. RedThe Planet’s atery W Pastast BY JIM BELL y February 2005 the Mars Exploration Rover named Spirit had already spent more than a year in Gusev Crater, a two-kilometer-deep, Connecticut-size hole in the Red Planet’s surface. Because Gusev lies at the end of an ancient, dry river valley longer than the Grand Canyon, many of us on the rover’s mission team Bhad expected Spirit to fi nd evidence that the crater had been fi lled with water billions of years ago. On the fl at plains where the craft had landed, however, the rover found neither lake deposits nor other preserved signs that water had once fl owed inside Gusev. The rover’s photographs showed only dust and sand and bone-dry volcanic lava rocks. But everything changed once Spirit reached the slopes of the Columbia Hills, about 2.6 kilometers from the landing site. (Each of the hills is named after one of the seven astronauts who died in the space shuttle Columbia disaster in 2003.) As Spirit struggled to climb the western slope of Husband Hill, its wheels dislodged rocks and dug deep C REDI T tracks in the Martian soil. -
Flnitflrclid
flNiTflRClID A NEWS BULLETIN published quarterly by the NEW ZEALAND ANTARCTIC SOCIETY (INC) A New Zealand geochemist, Dr W. F. Giggenbach, descends into the inner crater of Mt Erebus on December 23 last year in an unsuccessful attempt to take gas samples. Behind him in the lava lake of the volcano where the temperature is 1000deg Celsius. On his rucksack he carries titanium gas sampling rods. Photo by Colin Monteath VOl. 8, NO. 1 1 . Wellington, New Zealand, as a magazine. o6pt61*11061% I 979I ' . SOUTH SANDWICH Is SOUTH GEORGIA f S O U T H O R K N E Y I s x \ *#****t ■ /o Orcadas arg \ - aanae s» Novolazarevskaya ussr XJ FALKLAND Is /*Signyl.uK ,,'\ V\60-W / -'' \ Syowa japan SOUTH AMERICA /'' /^ y Borga 7 s a "Molodezhnaya A SOUTH , .a /WEDDELL T\USSR SHETLAND DRONNING MAUD LAND ENOERBY \] / Halley Bay^ ununn n mMUU / I s 'SEA uk'v? COATS Ld LAND JJ Druzhnaya ^General Belgrano arg ANTARCTIC %V USSR *» -» /\ ^ Mawson MAC ROBERTSON LANO\ '■ aust /PENINSULA,' "*■ (see map below) /Sohral arg _ ■ = Davis aust /_Siple — USA Amundsen-Scott / queen MARY LAND gMirny [ELLSWORTH u s a / ; t h u s s i " LANO K / ° V o s t o k u s s r / k . MARIE BYRD > LAND WILKES LAND Scott kOSS|nzk SEA I ,*$V /VICTORIA TERRE ' •|Py»/ LAND AOEilE ,y Leningradskaya X' USSR,''' \ 1 3 -------"';BALLENYIs ANTARCTIC PENINSULA ^ v . : 1 Teniente Matienzo arg 2 Esperanza arc 3 Almirante Brown arg 4 Petrel arg 5 Decepcion arg 6 Vicecomodoro Marambio arg ' ANTARCTICA 7 Arturo Prat chile 8 Bernardo O'Higgins chile 1000 Miles 9 Presidents Frei chile * ? 500 1000 Kilometres 10 Stonington I. -
14Yearsofdiscovery
14 YEARS OF DISCOVERIES 14 years of discoveries 14 YEARS OF DISCOVERIES DesignedMARS to last 90 days, Opportunity survived for over a 1 Martian solar decade on Mars. Here day (Sol) we look back on how = the record-breaking 1.027 rover changed the way Earth days we see the Red Planet 2 14 years of discoveries 39 Sols 91 Sols Opportunity’s Opportunity from orbit Opportunity’s journey across Mars has objectives been closely watched and calibrated by the satellites in orbit around the Red Search for signs of past Planet. This image from NASA’s Mars ✔ Global Surveyor shows some of the liquid water tracks of the rover, the craters it was visiting, its back shell and parachute, Determine distribution along with the location of its discarded and composition of heat shield. It was taken on 26 April Martian rocks ✔ 2004 on Sol 91 from a distance of around 400 kilometres (249 miles). Discover the geological processes which formed the Martian terrain ✔ Validate measurements made by probes orbiting Mars ✔ Search for iron containing minerals that may have been formed in water ✔ Signs of past water This is a microscopic image of part of a rock called 'Last Determine the texture of Chance'. The view here is around five centimetres (two rocks and soils and what inches) across and was taken on Opportunity’s 39th created them ✔ Martian day. The texture of the rock has led scientists to believe that water was once present in the area in which Assess whether Mars’ climate it was found – the Meridiani Planum area of Mars, which was ever fit for life ✔ is close to its equator.