The Influence of Lithospheric Flexure Induced by Volcano Loading on Neogene Basin Evolution in Mcmurdo Sound, West Antarctica
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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 ............................................................................. -
Geochemistry This
TORONTOTORONTO Vol. 8, No. 4 April 1998 Call for Papers GSA TODAY — page C1 A Publication of the Geological Society of America Electronic Abstracts Submission — page C3 Antarctic Neogene Landscapes—In the 1998 Registration Refrigerator or in the Deep Freeze? Annual Issue Meeting — June GSA Today Introduction The present Molly F. Miller, Department of Geology, Box 117-B, Vanderbilt Antarctic landscape undergoes very University, Nashville, TN 37235, [email protected] slow environmental change because it is almost entirely covered by a thick, slow-moving ice sheet and thus effectively locked in a Mark C. G. Mabin, Department of Tropical Environmental Studies deep freeze. The ice sheet–landscape system is essentially stable, and Geography, James Cook University, Townsville, Queensland 4811, Australia, [email protected] Antarctic—Introduction continued on p. 2 Atmospheric Transport of Diatoms in the Antarctic Sirius Group: Pliocene Deep Freeze Arjen P. Stroeven, Department of Quaternary Research, Stockholm University, S-106 91 Stockholm, Sweden Lloyd H. Burckle, Lamont-Doherty Earth Observatory of Columbia University, Palisades, NY 10964 Johan Kleman, Department of Physical Geography, Stockholm University, S-106, 91 Stockholm, Sweden Michael L. Prentice, Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH 03824 INTRODUCTION How did young diatoms (including some with ranges from the Pliocene to the Pleistocene) get into the Sirius Group on the slopes of the Transantarctic Mountains? Dynamicists argue for emplacement by a wet-based ice sheet that advanced across East Antarctica and the Transantarctic Mountains after flooding of interior basins by relatively warm marine waters [2 to 5 °C according to Webb and Harwood (1991)]. -
Curiosity's Candidate Field Site in Gale Crater, Mars
Curiosity’s Candidate Field Site in Gale Crater, Mars K. S. Edgett – 27 September 2010 Simulated view from Curiosity rover in landing ellipse looking toward the field area in Gale; made using MRO CTX stereopair images; no vertical exaggeration. The mound is ~15 km away 4th MSL Landing Site Workshop, 27–29 September 2010 in this view. Note that one would see Gale’s SW wall in the distant background if this were Edgett, 1 actually taken by the Mastcams on Mars. Gale Presents Perhaps the Thickest and Most Diverse Exposed Stratigraphic Section on Mars • Gale’s Mound appears to present the thickest and most diverse exposed stratigraphic section on Mars that we can hope access in this decade. • Mound has ~5 km of stratified rock. (That’s 3 miles!) • There is no evidence that volcanism ever occurred in Gale. • Mound materials were deposited as sediment. • Diverse materials are present. • Diverse events are recorded. – Episodes of sedimentation and lithification and diagenesis. – Episodes of erosion, transport, and re-deposition of mound materials. 4th MSL Landing Site Workshop, 27–29 September 2010 Edgett, 2 Gale is at ~5°S on the “north-south dichotomy boundary” in the Aeolis and Nepenthes Mensae Region base map made by MSSS for National Geographic (February 2001); from MOC wide angle images and MOLA topography 4th MSL Landing Site Workshop, 27–29 September 2010 Edgett, 3 Proposed MSL Field Site In Gale Crater Landing ellipse - very low elevation (–4.5 km) - shown here as 25 x 20 km - alluvium from crater walls - drive to mound Anderson & Bell -
Turbulence and Aeolian Morphodynamics in Craters on Mars: Application to Gale Crater, Landing Site of the Curiosity Rover
16TH EUROPEAN TURBULENCE CONFERENCE, 21-24 AUGUST, 2017, STOCKHOLM,SWEDEN TURBULENCE AND AEOLIAN MORPHODYNAMICS IN CRATERS ON MARS: APPLICATION TO GALE CRATER, LANDING SITE OF THE CURIOSITY ROVER William Anderson1, Gary Kocurek2 & Kenzie Day2 1Mechanical Engineering Dept., Univ. Texas at Dallas, Richardson, Texas, USA 2Dept. Geological Sciences, Jackson School of Geosciences, Univ. Texas at Austin, Austin, Texas, USA Mars is a dry planet with a thin atmosphere. Aeolian processes – wind-driven mobilization of sediment and dust – are the dominant mode of landscape variability on the dessicated landscapes of Mars. Craters are common topographic features on the surface of Mars, and many craters on Mars contain a prominent central mound (NASA’s Curiosity rover was landed in Gale crater, shown in Figure 1a [1], while Figures 1b and 1c show Henry and Korolev crater, respectively). These mounds are composed of sedimentary fill and, therefore, they contain rich information on the evolution of climatic conditions on Mars embodied in the stratigraphic “layering” of sediments. Many other craters no longer house a mound, but contain sediment and dust from which dune fields and other features form (see, for example, Victoria Crater, Figure 1d). Using density-normalized large-eddy simulations, we have modeled turbulent flows over crater-like topographies that feature a central mound. Resultant datasets suggest a deflationary mechanism wherein vortices shed from the upwind crater rim are realigned to conform to the crater profile via stretching and tilting. This was accomplished using three- dimensional datasets (momentum and vorticity) retrieved from LES. As a result, helical vortices occupy the inner region of the crater and, therefore, are primarily responsible for aeolian morphodynamics in the crater (radial katabatic flows are also important to aeolian processes within the crater [2]). -
Ice Caves of Terra Nova Bay (Victoria Land, Antarctica)
SPECIALE GLACIER CAVES NIMBUS 23-24 Ice Caves of Terra Nova Bay (Victoria Land, Antarctica) Mirco Meneghel - Dipartimento di Geografia, University of Padova, Italy Giovanni Badino - Dipartimento di Fisica Generale, University of Torino, Italy Associazione La Venta Abstract Baia Terra Nova, sulla costa occi- wider Terra Nova Bay, on the we- In the 2000/2001 expedition of dentale del Mare di Ross. Sono stern coast of the Ross Sea, at 74° the Italian Programme of Resear- state esplorate tre grotte nella 41' 42" S lat. and 164° 07' 23" E ch in Antarctica (PNRA) an inve- fronte dei ghiacciai al contatto col long. The Transantarctic Mts, stigation on the presence of ca- mare e un'altra sulla sommità del whose relief is often higher than ves in ice has been carried out monte Melbourne, un cono vulca- 3000 m, fringe the coast. South near the Italian Station of Terra nico di 2700 metri di altezza. Le of the Base the mountain chaine Nova Bay, on the western coast of grotte sulla costa sono crepacci is crossed by outlet glaciers that the Ross Sea (Northern Victoria ampliati dalla sublimazione del drain the ice of the inlandsis. On Land). Three caves have been ex- ghiaccio a causa della differenza the north huge valley glaciers plored at the snout of glaciers di temperatura fra il ghiaccio e flow from the mountains to the reaching the sea and an other l'acqua marina. La grotta subgla- sea. The Italian Base is placed one on the summit of Mt Mel- ciale sul monte Melbourne è ge- between the region of the Dry bourne, a volcanic cone 2700 m nerata dal calore delle rocce vul- Valleys to the south, where broad 1 - Below - high. -
Management Plan for Antarctic Specially Protected Area No. 116 NEW COLLEGE VALLEY, CAUGHLEY BEACH, CAPE BIRD, ROSS ISLAND
Management Plan For Antarctic Specially Protected Area No. 116 NEW COLLEGE VALLEY, CAUGHLEY BEACH, CAPE BIRD, ROSS ISLAND 1. Description of values to be protected In 1985, two areas at Cape Bird, Ross Island were designated as SSSI No. 10, Caughley Beach (Recommendation XIII-8 (1985)) and SPA No. 20, New College Valley (Recommendation XIII-12 (1985)), following proposals by New Zealand that these areas should be protected because they contained some of the richest stands of moss and associated microflora and fauna in the Ross Sea region of Antarctica. This is the only area on Ross Island where protection is specifically given to plant assemblages and associated ecosystems. At that time, SPA No. 20 was enclosed within SSSI No. 10, in order to provide more stringent access conditions to that part of the Area. In 2000, SSSI No. 10 was incorporated with SPA No. 20 by Measure 1 (2000), with the former area covered by SPA No. 20 becoming a Restricted Zone within the revised SPA No. 20. The boundaries of the Area were revised from the boundaries in the original recommendations, in view of improved mapping and to follow more closely the ridges enclosing the catchment of New College Valley. Caughley Beach itself was adjacent to, but never a part of, the original Area, and for this reason the entire Area was renamed as New College Valley, which was within both of the original sites. The Area was redesignated by Decision 1 (2002) as Antarctic Specially Protected Area (ASPA) No. 116 and a revised Management Plan was adopted through Measure 1 (2006). -
The Antarctic Treaty
The Antarctic Treaty Measures adopted at the Thirty-ninth Consultative Meeting held at Santiago, Chile 23 May – 1 June 2016 Presented to Parliament by the Secretary of State for Foreign and Commonwealth Affairs by Command of Her Majesty November 2017 Cm 9542 © Crown copyright 2017 This publication is licensed under the terms of the Open Government Licence v3.0 except where otherwise stated. To view this licence, visit nationalarchives.gov.uk/doc/open-government-licence/version/3 Where we have identified any third party copyright information you will need to obtain permission from the copyright holders concerned. This publication is available at www.gov.uk/government/publications Any enquiries regarding this publication should be sent to us at Treaty Section, Foreign and Commonwealth Office, King Charles Street, London, SW1A 2AH ISBN 978-1-5286-0126-9 CCS1117441642 11/17 Printed on paper containing 75% recycled fibre content minimum Printed in the UK by the APS Group on behalf of the Controller of Her Majestyʼs Stationery Office MEASURES ADOPTED AT THE THIRTY-NINTH ANTARCTIC TREATY CONSULTATIVE MEETING Santiago, Chile 23 May – 1 June 2016 The Measures1 adopted at the Thirty-ninth Antarctic Treaty Consultative Meeting are reproduced below from the Final Report of the Meeting. In accordance with Article IX, paragraph 4, of the Antarctic Treaty, the Measures adopted at Consultative Meetings become effective upon approval by all Contracting Parties whose representatives were entitled to participate in the meeting at which they were adopted (i.e. all the Consultative Parties). The full text of the Final Report of the Meeting, including the Decisions and Resolutions adopted at that Meeting and colour copies of the maps found in this command paper, is available on the website of the Antarctic Treaty Secretariat at www.ats.aq/documents. -
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. -
The Antarctic Crustal Profile Seismic Project, Ross Sea, Antarctica ALAN K
200,000 years are obviously affected to a lesser degree than argon (40Ar) to excess argon (40ArE) and are, therefore, taken younger samples containing a lower proportion of radiogenic to be a truer representation of the actual age of that particu- _______________________ lar sample. Still, it must be noted that all the 40Ar/ 39Ar ages pro- 40Ar139Ar ages for Mount Erebus as determined in this study duced from Mount Erebus are maximum ages owing to the uncertainty of complete removal (through sample preparation) of all excess argon. 48±9a Excess argon—Too Old Summit phenocrysts Evaluation of these new data Summit phenocrysts -10 179±16a Excess argon—Too Old Summit phenocrysts #2 49±27a Excess argon—Too Old is still in progress; however, it is Summit phenocrysts #2 30-40 641±27a Excess argon—Too Old apparent that our new age deter- Summit (bomb) glass 100 101±16a Excess argon—Too Old minations are significantly Lower Hut flow <1 24±4b Acceptable younger than those previously Three Sisters cones -4 26±2b Acceptable obtained by the conventional Three Sisters cones 11 1±8b Contamination? K/Ar method. The evolution and 36±4 Hoopers Shoulder <1 b Acceptable growth of Mount Erebus may Hoopers Shoulder cone 32±5b Acceptable have been much faster than pre- a Hoopers Shoulder cone -5 94±15 Excess argon viously thought. 42±4b Contamination? Cape Evans This research was supported Cape Evans -5 32±6b Acceptable Cape Royds -2 735b Acceptable by National Science Foundation Cape Royds -20 153±32a Excess argon grant OPP 91-18056. -
Geological Investigations of Volcanic Rocks at Mount Discovery, Mount Morning, and Mason Spur, Mcmurdo Sound Unusual Magnesium
Geological investigations mountain. A sample from one of these parasitic domes has been dated at 1.15 million years (Armstrong 1978). Younger basanite of volcanic rocks cinder cones and lava flows form two north-northeast trending at Mount Discovery, Mount Morning, ridges on the northeast side of Mount Morning, which are interpreted as being aligned along fracture zones parallel to the and Mason Spur, McMurdo Sound range front on the Royal Society Range located 30 kilometers to the northwest. Older trachytic rocks crop out at the lower end of both ridges. Detailed mapping of the trachyte outcrops on the A.C. WRIGHT, P.R. KYLE, J.A. MORE, and K. MEEKER western ridge confirms the similarity of this area to the trachyte outcrops on the eastern ridge, which has been mapped pre- Department of Geoscience, viously by Muncy (1979). Rocks intermediate in age between New Mexico Institute of Mining and Technology the older trachytes and the young basanites, comprise tra- Socorro, New Mexico 87801 chybasalt to trachyandesite flows and domes on the lower end of the western ridge. Description of five geologic sections at Mason Spur has provided a more detailed understanding of the older trachytic Between November 1985 and January 1986, we examined volcanic complex, which is now dated at 11.5 to 12.8 million rocks of the McMurdo Volcanic Group in the southern McMur- years (unpublished argon-40/argon-39 age determinations by do Sound area and at Mount Discovery, Mount Morning, and D. Lux, University of Maine) and is divided into seven mapped Mason Spur. This work is a continuation of field work carried units. -
The Antarctic Treaty
! ! ! ! ! ! The Antarctic Treaty ! ! ! ! Measures adopted at the Thirty-ninth Consultative Meeting held at Santiago, Chile 23 May – 1 June 2016 ! ! ! ! ! ! ! ! ! ! Presented to Parliament by the Secretary of State for Foreign and Commonwealth Affairs by Command of Her Majesty November 2017! Cm 9542 © Crown copyright 2017 This publication is licensed under the terms of the Open Government Licence v3.0 except where otherwise stated. To view this licence, visit nationalarchives.gov.uk/doc/open-government-licence/version/3 Where we have identified any third party copyright information you will need to obtain permission from the copyright holders concerned. This publication is available at www.gov.uk/government/publications Any enquiries regarding this publication should be sent to us at Treaty Section, Foreign and Commonwealth Office, King Charles Street, London, SW1A 2AH ISBN 978-1-5286-0126-9 CCS1117441642 11/17 Printed on paper containing 75% recycled fibre content minimum Printed in the UK by the APS Group on behalf of the Controller of Her Majesty!s Stationery Office MEASURES ADOPTED AT THE THIRTY-NINTH ANTARCTIC TREATY CONSULTATIVE MEETING Santiago, Chile 23 May – 1 June 2016 The Measures1 adopted at the Thirty-ninth Antarctic Treaty Consultative Meeting are reproduced below from the Final Report of the Meeting. In accordance with Article IX, paragraph 4, of the Antarctic Treaty, the Measures adopted at Consultative Meetings become effective upon approval by all Contracting Parties whose representatives were entitled to participate in the meeting at which they were adopted (i.e. all the Consultative Parties). The full text of the Final Report of the Meeting, including the Decisions and Resolutions adopted at that Meeting and colour copies of the maps found in this command paper, is available on the website of the Antarctic Treaty Secretariat at www.ats.aq/documents.