2. the 1984-1985 Antarctic Search for Meteorites (ANSMET) Field Program
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Mcmurdo Dry Valleys, Southern Victoria Land
Measure 1 (2004) Annex Management Plan for Antarctic Specially Managed Area No. 2 MCMURDO DRY VALLEYS, SOUTHERN VICTORIA LAND 1. Description of values to be protected and activities to be managed The McMurdo Dry Valleys are characterized as the largest relatively ice-free region in Antarctica with approximately thirty percent of the ground surface largely free of snow and ice. The region encompasses a cold desert ecosystem, whose climate is not only cold and extremely arid (in the Wright Valley the mean annual temperature is –19.8°C and annual precipitation is less than 100 mm water equivalent), but also windy. The landscape of the Area contains glaciers, mountain ranges, ice-covered lakes, meltwater streams, arid patterned soils and permafrost, sand dunes, and interconnected watershed systems. These watersheds have a regional influence on the McMurdo Sound marine ecosystem. The Area’s location, where large-scale seasonal shifts in the water phase occur, is of great importance to the study of climate change. Through shifts in the ice-water balance over time, resulting in contraction and expansion of hydrological features and the accumulations of trace gases in ancient snow, the McMurdo Dry Valley terrain also contains records of past climate change. The extreme climate of the region serves as an important analogue for the conditions of ancient Earth and contemporary Mars, where such climate may have dominated the evolution of landscape and biota. The Area is characterized by unique ecosystems of low biodiversity and reduced food web complexity. However, as the largest ice-free region in Antarctica, the McMurdo Dry Valleys also contain relatively diverse habitats compared with other ice-free areas. -
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. -
PDF of Project Description
EXTENDING THE RECORD OF ANTARCTIC LANDSCAPE EVOLUTION INTO THE PLIOCENE WITH COSMOGENIC NEON-21 MEASUREMENTS I. OVERALL PROJECT GOAL This proposal seeks limited funding to measure the stable cosmogenic nuclide 21Ne in an existing set of bedrock and sediment samples from the Antarctic Dry Valleys (DV). We collected these samples during two previous Antarctic field seasons, in the course of a project whose goal was to make a systematic survey of rates of erosion and landscape evolution in the DV. Part of this project involved measuring concentrations of the cosmogenic radionuclides 26Al and 10Be in surface rock and sediment, in order to i) determine whether the observed antiquity of DV surface sediments and landforms was the result of vanishingly small erosion and degradation rates, or of long periods of cover by cold-based glaciers; and ii) if the former, measure the rates of these processes. Results of these measurements quantify existing stratigraphic observations that many DV landscape surfaces are very old, do not appear to have been covered by cold-based ice for significant amounts of time, and erode very slowly. One consequence of these results is that, unlike in most other environments worldwide where relatively rapid surface erosion limits the time period about which cosmogenic-nuclide measurements can provide information, surfaces in the DV are stable enough that the limiting factor is often the radioactive decay of 26Al and 10Be instead. We propose that by combining the stable cosmogenic nuclide 21Ne – which, like 26Al and 10Be, is both produced in quantity and can be measured in the common mineral quartz – with existing 10Be and 26Al measurements, we can learn about surface processes in the DV over a longer time period than has been previously possible. -
Wilderness and Aesthetic Values of Antarctica
Wilderness and Aesthetic Values of Antarctica Abstract Antarctica is the least inhabited region in the world and has therefore had the least influence from human activities and, unlike the majority of the Earth’s continents and oceans, can still be considered as mostly wilderness. As every visitor to Antarctica knows, its landscapes are exceptionally beautiful. It was the recognition of the importance of these characteristics that resulted in their protection being included in the Madrid Protocol. Both wilderness and aesthetic values can be impaired by human activities in a variety of ways with the severity varying from negligible to severe, according to the type Protocol on Environmental Protec tion to the Antarctic Trea ty - of activity and its duration, spatial extent and intensity. A map of infrastructure and major travel routes the "M adrid Protocol" in Antarctica will be the first step in visually representing where wilderness and aesthetic values Article 3[1] may be impacted. It is hoped that this will stimulate further discussion on how to describe, acknowledge, The protection of the Antarctic environment and dependent an d associated ecosystems and the intrinsic value of Antarctica, understand and further protect the wilderness and aesthetic values of Antarctica. including its wilderness and aesthetic values and its value as an area for the conduct of scientific research, in particular research essential to understanding the global environment, shall be fundamental considerations in the planning and condu ct of all activities -
Mm^Umamm a N E W S B U L L E T I N
mm^umamm A N E W S B U L L E T I N p u b l i s h e d q u a r t e r l y b y t h e NEW ZEALAND ANTARCTIC SOCIETY ■ H.M.N.Z.S. ENDEAVOUR about to tie up in Winter Quarters Bay. On right, Vince's Cross and Scott's hut. J. Calvert photo. MARCH, 1965 AUSTRALIA Winter and Summer bases Scott- S u m m e r b a s e o n l y t H a l l e f t "cton NEW ZEALAND Transferred base Wilkes UStcAust Temporarily non -operational. .KSyowa TASMANIA , Campbell I. (N-l) , ^ V - r . ^ ^ N . AT // \$ 5«|* Pasar'C ^rd(i/.sA . *"Vp»tuk , N |(I/.«.AJ i - S c o t t ( U . 5 J i t - A N T A R. M^ciJ ^>cwj a fi/V wX " < S M a u d **$P -Marion I. ttM DRAWN BY DEPARTMENT OF LANDS 1 SURVEY WELLINGTON, NEW ZEALAND, MAR.I9l»4- 1 " . " E D I T I O N m ilHl^IBS^IKB^k (Successor to "Antarctic News Bulletin") MARCH, 1965 Editor: L. B. Quartermain, M.A., 1 Ariki Road, Wellington, E.2, New Zealand. Business Communications, Subscriptions, etc., to: Secretary, New Zealand Antarctic Society, P.O. Box 2110, Wellington, N.Z. CONTENTS EXPEDITIONS New Zealand The Central Nimrod Glacier Geological Expedition: M. G. Laird Victoria University Research in Ice-free Areas: W. M. Prebble The D-region Project: J. B. Gregory France United States First Leg of Traverse Australia Belgium-Holland U.S.S.R South Africa Argentina United Kingdom Chile Japan Sub-Antarctic Islands British South Georgia Expedition Big Ben Conquered Special Articles: Hallett Closed Antarctic Stations—I. -
Geological Evolution of the Coombs-Allan Hills Area, Ferrar Large Igneous Province, Antarctica
The following document is a pre-print version of: Ross, P.-S., White, J.D.L. et McClintock, M. (2008) Geological evolution of the Coombs-Allan Hills area, Ferrar large igneous province, Antarctica: debris avalanches, mafic pyroclastic density currents, phreatocauldrons. Journal of Volcanology and Geothermal Research 172: 38-60 Geological evolution of the Coombs-Allan Hills area, Ferrar large igneous province, Antarctica: debris avalanches, mafic pyroclastic density currents, phreatocauldrons… Pierre-Simon Ross 1, James D.L. White, and Murray McClintock Department of Geology, University of Otago, PO Box 56, Dunedin, New Zealand 1. Corresponding author Abstract The Jurassic Ferrar large igneous province of Antarctica comprises igneous intrusions, flood lavas, and mafic volcaniclastic deposits (now lithified). The latter rocks are particularly diverse and well-exposed in the Coombs-Allan Hills area of South Victoria Land, where they are assigned to the Mawson Formation. In this paper we use these rocks in conjunction with the pre-Ferrar sedimentary rocks (Beacon Supergroup) and the lavas themselves (Kirkpatrick Basalt) to reconstruct the geomorphological and geological evolution of the landscape. In the Early Jurassic, the surface of the region was an alluvial plain, with perhaps 1 km of mostly continental siliciclastic sediments underlying it. After the fall of silicic ash from an unknown but probably distal source, mafic magmatism of the Ferrar province began. The oldest record of this event at Allan Hills is a ≤180 m-thick debris avalanche deposit (member m 1 of the Mawson Formation) which contains globular domains of mafic igneous rock. These domains are inferred to represent dismembered Ferrar intrusions emplaced in the source area of the debris avalanche; shallow emplacement of Ferrar magmas caused a slope failure that mobilized the uppermost Beacon Supergroup, and the silicic ash deposits, into a pre-existing valley or basin. -
ARCHIVED-CARN Vol 16, May 2003 [PDF-4.42
Vol 16, May 2003 NEWSLETTER FOR THE Canadian Antarctic Research Network Inside Canada to Ratify Protocol on Environmental Protection Canada to Ratify Protocol on Environmental Protection 1 Environment Canada issued the following press release as legislation was introduced Canada and CCAMLR 3 in Parliament to ratify the Protocol on Environmental Protection. Discontinuous Volcanic Eruptions in a Phreatomagmatic Vent Complex: Ottawa, June 6, 2003 – The Honourable David Anderson, Minister of the Envi- Coombs Hills, ronment and the Honourable Bill Graham, Minister of Foreign Affairs, today South Victoria Land 4 introduced legislation that would allow Canada to ratify the Protocol on Envi- Biogeochemical Transformations ronmental Protection to the Antarctic Treaty (the Madrid Protocol) to protect of Organic Carbon in Cold-based the Antarctic environment. Glacier Systems 7 “I am pleased to introduce Bill C-42 today which will allow Canada to rati- Contaminants fy the Madrid Protocol and officially join its global partners to further prevent in Polar Ecosystems 9 pollution and environmental degradation in the Antarctic,” said Minister Ander- son. “And I am proud that since signing the Protocol in 1991, Canada and Cana- News in Brief 10 dians have been meeting or exceeding the obligations of the Protocol.” Workshop to plan a Canadian “By ratifying the Madrid Protocol, Canada will contribute to the protection Antarctic Research Program 11 of one of the most fragile ecosystems in the world,” said Minister Graham. “Canada is pleased to join other countries around the world in ensuring that the Antarctic environment is preserved for future generations.” The Madrid Protocol is part of the Antarctic Treaty System, which in- cludes the Antarctic Treaty (1961) to which Canada is a Party. -
Management Plan for Antarctic Specially Managed Area No. 2
Management Plan for Antarctic Specially Managed Area No. 2 MCMURDO DRY VALLEYS, SOUTHERN VICTORIA LAND 1. Description of values to be protected and activities to be managed The McMurdo Dry Valleys are characterized as the largest relatively ice-free region in Antarctica with approximately thirty percent of the ground surface largely free of snow and ice. The region encompasses a cold desert ecosystem, whose climate is not only cold and extremely arid (in the Wright Valley the mean annual temperature is –19.8°C and annual precipitation is less than 100 mm water equivalent), but also windy. The landscape of the Area contains glaciers, mountain ranges, ice-covered lakes, meltwater streams, arid patterned soils and permafrost, sand dunes, and interconnected watershed systems. These watersheds have a regional influence on the McMurdo Sound marine ecosystem. The Area’s location, where large-scale seasonal shifts in the water phase occur, is of great importance to the study of climate change. Through shifts in the ice-water balance over time, resulting in contraction and expansion of hydrological features and the accumulations of trace gases in ancient snow, the McMurdo Dry Valley terrain also contains records of past climate change. The extreme climate of the region serves as an important analogue for the conditions of ancient Earth and contemporary Mars, where such climate may have dominated the evolution of landscape and biota. The Area is characterized by unique ecosystems of low biodiversity and reduced food web complexity. However, as the largest ice-free region in Antarctica, the McMurdo Dry Valleys also contain relatively diverse habitats compared with other ice-free areas. -
Ejection of Martian Meteorites
Meteoritics & Planetary Science 40, Nr 9/10, 1393–1411 (2005) Abstract available online at http://meteoritics.org Ejection of Martian meteorites Jˆrg FRITZ1*, Natalia ARTEMIEVA2, and Ansgar GRESHAKE1 1Institut f¸r Mineralogie, Museum f¸r Naturkunde, Humboldt-Universit‰t zu Berlin, Invalidenstrasse 43, 10115 Berlin, Germany 2Institute for Dynamics of Geospheres, Russian Academy of Science, Leninsky Prospect 38, Building 1, Moscow 119334, Russia *Corresponding author. E-mail: [email protected] (Received 29 March 2005; revision accepted 11 April 2005) Abstract–We investigated the transfer of meteorites from Mars to Earth with a combined mineralogical and numerical approach. We used quantitative shock pressure barometry and thermodynamic calculations of post-shock temperatures to constrain the pressure/temperature conditions for the ejection of Martian meteorites. The results show that shock pressures allowing the ejection of Martian meteorites range from 5 to 55 GPa, with corresponding post-shock temperature elevations of 10 to about 1000 °C. With respect to shock pressures and post-shock temperatures, an ejection of potentially viable organisms in Martian surface rocks seems possible. A calculation of the cooling time in space for the most highly shocked Martian meteorite Allan Hills (ALH) 77005 was performed and yielded a best-fit for a post-shock temperature of 1000 °C and a meteoroid size of 0.4 to 0.6 m. The final burial depths of the sub-volcanic to volcanic Martian rocks as indicated by textures and mineral compositions of meteorites are in good agreement with the postulated size of the potential source region for Martian meteorites during the impact of a small projectile (200 m), as defined by numerical modeling (Artemieva and Ivanov 2004). -
II. Expedition Dates
Information Exchange Under United States Antarctic Activities Articles III and VII(5) of the Activities Planned for 2003- 2004 ANTARCTIC TREATY II. Expedition Dates II. Expedition Dates Section II of the 2003-2004 season plan includes information concerning vessel and aircraft operations along with estimated dates of expeditions and other significant events. Winfly Activities Annual augmentation of the U.S. Antarctic Program (USAP) begins with austral winter flights (WINFLY), departing Christchurch, New Zealand, and arriving McMurdo Station, Antarctica, about 20 August 2003. The aircraft will carry scientists and support personnel to start early pre-summer projects, to augment maintenance personnel, and to prepare skiways and ice runways at McMurdo Station. This will involve 3 U.S. Air Force C-17 flights and will increase station population from the winter-over level of about 154 to a transition level of about 580 (285 personnel expected to deploy at WINFLY). Mainbody Activities Austral summer activities will be initiated on 30 September 2003 with wheeled aircraft operations between Christchurch, New Zealand and the sea-ice runways at McMurdo Station, Antarctica. This will involve approximately 21 C-141 flights, 11 C-17 flights and 4 C-5 flights of transport aircraft of the U.S. Air Force Air Mobility Command (AMC), and 15 flights by C-130 transport aircraft of the Royal New Zealand Air Force. The sea- ice runway operations will cease about mid December 2003. Williams Field will open for the ski-equipped LC-130 aircrafts and at the same time approximately 2 days pass the Ice Runway closure, Pegasus Blue Ice Runway will be open for wheeled aircraft from Christchurch to McMurdo. -
United States Antarctic Activities 2003-2004
United States Antarctic Activities 2003-2004 This site fulfills the annual obligation of the United States of America as an Antarctic Treaty signatory to report its activities taking place in Antarctica. This portion details planned activities for July 2003 through June 2004. Modifications to these plans will be published elsewhere on this site upon conclusion of the 2003-2004 season. National Science Foundation Arlington, Virginia 22230 November 30, 2003 Information Exchange Under United States Antarctic Activities Articles III and VII(5) of the ANTARCTIC TREATY Introduction Organization and content of this site respond to articles III(1) and VII(5) of the Antarctic Treaty. Format is as prescribed in the Annex to Antarctic Treaty Recommendation VIII-6, as amended by Recommendation XIII-3. The National Science Foundation, an agency of the U.S. Government, manages and funds the United States Antarctic Program. This program comprises almost the totality of publicly supported U.S. antarctic activities—performed mainly by scientists (often in collaboration with scientists from other Antarctic Treaty nations) based at U.S. universities and other Federal agencies; operations performed by firms under contract to the Foundation; and military logistics by units of the Department of Defense. Activities such as tourism sponsored by private U.S. groups or individuals are included. In the past, some private U.S. groups have arranged their activities with groups in another Treaty nation; to the extent that these activities are known to NSF, they are included. Visits to U.S. Antarctic stations by non-governmental groups are described in Section XVI. This document is intended primarily for use as a Web-based file, but can be printed using the PDF option. -
The Antarctic Treaty
The Antarctic Treaty Measures adopted at the Thirty-fourth Consultative Meeting held at Buenos Aires, 20 June – 1 July 2011 Presented to Parliament by the Secretary of State for Foreign and Commonwealth Affairs by Command of Her Majesty January 2014 Cm 8809 £31.50 © Crown copyright 2014 You may re-use this information (excluding logos) free of charge in any format or medium, under the terms of the Open Government Licence. To view this licence, visit http://www.nationalarchives.gov.uk/doc/open-government-licence or email. [email protected] Where we have identified any third party copyright information you will need to obtain permission from the copyright holders concerned. Any enquiries regarding this publication should be sent to us at Treaty Section, Foreign and Commonwealth Office, King Charles Street, London, SW1A 2AH. ISBN: 9780101880923 Printed in the UK by The Stationery Office Limited on behalf of the Controller of Her Majesty’s Stationery Office ID P002619602 01/14 36734 19585 Printed on paper containing 30% recycled fibre content minimum. MEASURES ADOPTED AT THE THIRTY-FOURTH ANTARCTIC TREATY CONSULTATIVE MEETING Buenos Aires, Argentina 20 June – 1 July 2011 The Measures1 adopted at the Thirty-fourth 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.