Relevant bibliographies by topics / Meteorites – Antarctica

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Meteorites – Antarctica'

Author: Grafiati
Published: 4 June 2021
Last updated: 8 February 2022

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Journal articles on the topic "Meteorites – Antarctica"

1

Wadhwa, Meenakshi, Timothy J. McCoy, and Devin L. Schrader. "Advances in Cosmochemistry Enabled by Antarctic Meteorites." Annual Review of Earth and Planetary Sciences 48, no. 1 (May 30, 2020): 233–58. http://dx.doi.org/10.1146/annurev-earth-082719-055815.

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At present, meteorites collected in Antarctica dominate the total number of the world's known meteorites. We focus here on the scientific advances in cosmochemistry and planetary science that have been enabled by access to, and investigations of, these Antarctic meteorites. A meteorite recovered during one of the earliest field seasons of systematic searches, Elephant Moraine (EET) A79001, was identified as having originated on Mars based on the composition of gases released from shock melt pockets in this rock. Subsequently, the first lunar meteorite, Allan Hills (ALH) 81005, was also recovered from the Antarctic. Since then, many more meteorites belonging to these two classes of planetary meteorites, as well as other previously rare or unknown classes of meteorites (particularly primitive chondrites and achondrites), have been recovered from Antarctica. Studies of these samples are providing unique insights into the origin and evolution of the Solar System and planetary bodies. ▪ Antarctic meteorites dominate the inventory of the world's known meteorites and provide access to new types of planetary and asteroidal materials. ▪ The first meteorites recognized to be of lunar and martian origin were collected from Antarctica and provided unique constraints on the evolution of the Moon and Mars. ▪ Previously rare or unknown classes of meteorites have been recovered from Antarctica and provide new insights into the origin and evolution of the Solar System.
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Graham, A. L., and John O. Annexstad. "Antarctic meteorites." Antarctic Science 1, no. 1 (March 1989): 3–14. http://dx.doi.org/10.1017/s0954102089000039.

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Antarctica is currently the most productive region of the Earth for the recovery of meteorites and over 9800 specimens have been found there, most of these since 1969. This material consists of meteoritic fragments representing a much smaller, but unknown, number of distinct meteorites. The particular climatic and environmental conditions of Antarctica result in the recovery of a much larger fraction of the extraterrestrial material that falls to Earth than would be the case in other regions. Remarkable concentrations of meteorites are found in some ‘blue ice’ areas resulting from the movement and ablation of the ice. Most meteorites are believed to have been derived from asteroids less then 200 km in diameter. The discovery in Antarctica of meteorites of lunar material proved that other sources are possible. Indeed two meteorites from Antarctica may have come from the planet Mars. Antarctic meteorites have much older terrestrial ages than non-Antarctic specimens and may be used to obtain information on the movement of the ice sheets in the past.
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Wilson, John W., Liam A. Marsh, Wouter Van Verre, Michael C. Rose, Geoffrey Evatt, Andrew R. D. Smedley, and Anthony J. Peyton. "Design and construction of a bespoke system for the detection of buried, iron-rich meteorites in Antarctica." Antarctic Science 32, no. 1 (January 22, 2020): 58–69. http://dx.doi.org/10.1017/s0954102019000531.

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AbstractIron-rich meteorites are significantly underrepresented in collection statistics from Antarctica. This has led to a hypothesis that there is a sparse layer of iron-rich meteorites hidden below the surface of the ice, thereby explaining the apparent shortfall. As standard Antarctic meteorite collecting techniques rely upon a visual surface search approach, the need has thus arisen to develop a system that can detect iron objects under a few tens of centimetres of ice, where the expected number density is of the order one per square kilometre. To help answer this hypothesis, a large-scale pulse induction metal detector array has been constructed for deployment in Antarctica. The metal detector array is 6 m wide, able to travel at 15 km h-1 and can scan 1 km2 in ~11 hours. This paper details the construction of the metal detector system with respect to design criteria, notably the ruggedization of the system for Antarctic deployment. Some preliminary results from UK and Antarctic testing are presented. We show that the system performs as specified and should reach the pre-agreed target of the detection of a 100 g iron meteorite at 300 mm when deployed in Antarctica.
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Leary, David. "Blue Ice, Meteorites, Fossil Penguins and Rare Minerals: The Case for Enhanced Protection of Antarctica’s Unique Geoheritage – An International Legal Analysis." Yearbook of Polar Law Online 12, no. 1 (December 13, 2021): 17–40. http://dx.doi.org/10.1163/22116427_012010004.

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Its isolation and extreme climate means Antarctica is one of the world’s richest regions for untouched geoheritage. The potential of mining in Antarctica is often talked of in public discourse as a future threat to Antarctica even though the prohibition on mining is absolute and is likely to stay so indefinitely. As such mining does not pose a realistic threat to Antarctica’s geoheritage. The impacts of scientific research and tourism pose more pressing challenges to Antarctica’s geoheritage. This paper considers emerging debates in the Antarctic Treaty System on the need for further protection of Antarctica’s geoheritage. After considering the concept of geoheritage the paper considers key threats to Antarctic geoheritage. The role of Antarctic Specially Protected Area system in the protection of Antarctica’s geoheritage is then considered as is the draft code of conduct on geosciences field research currently being developed within the Antarctic Treaty System. The final part of the paper then goes on to examine how the Antarctic Treaty system could in part draw on the experience of other international initiatives, including the frameworks associated with the UNESCO Global Geoparks movement in developing an Antarctic System for protection of geoheritage.
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Bland, Philip A., Alex W. R. Bevan, and A. J. Tim Jull. "Ancient Meteorite Finds and the Earth's Surface Environment." Quaternary Research 53, no. 2 (March 2000): 131–42. http://dx.doi.org/10.1006/qres.1999.2106.

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AbstractThe flux of meteorites to the Earth over the last 50,000 yr has remained approximately constant. Most meteorites that fall in temperate or tropical areas are destroyed on a time scale which is short compared to the rate of infall; however, in arid regions (both “hot” deserts and the “cold” desert of Antarctica) weathering is slower and accumulations of meteorites may occur. The initial composition for many meteorite groups is well known from modern falls, and terrestrial ages may be established from analyses of the abundance of cosmogenic radionuclides, providing an absolute chronology for recording terrestrial processes. As samples are falling constantly, and are distributed approximately evenly over the Earth, meteorites may thus be thought of as an appropriate “standard sample” for studying aspects of the terrestrial surface environment. Studies involving 14C and 36Cl terrestrial ages of meteorites, 57Fe Mössbauer spectroscopy (to quantify the degree of oxidation in samples), stable isotopes, and determination of halogen abundances are yielding information on the terrestrial history of meteorites: (i) terrestrial age and oxidation-frequency distributions for populations of samples allow the ages of surfaces to be estimated; (ii) differences in the weathering rate of samples between sites allows constraints to be imposed on the effect of climate on rock weathering rates; (iii) carbon isotopic compositions of generations of carbonate growth within meteorites allows, in some cases, temperatures of formation of carbonates to be estimated; (iv) structure in the oxidation–terrestrial age distribution for meteorites from some arid accumulation sites (specifically, the Nullarbor of Australia) appears to be linked to previous humid/arid cycles; (v) meteorite accumulations in Antarctica have been used to constrain aspects of the Quaternary evolution of the ice sheet, and terrestrial age and oxidation data have been used to constrain ice flow.
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Korotev, Randy L. "Meteorites, ice, and antarctica." Geochimica et Cosmochimica Acta 68, no. 10 (May 2004): 2399. http://dx.doi.org/10.1016/j.gca.2003.12.011.

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Carmichael, Stephen W. "Out of this World!" Microscopy Today 4, no. 8 (October 1996): 3–5. http://dx.doi.org/10.1017/s1551929500063616.

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If you have been hibernating for several weeks you may have missed the headlines and magazine covers exclaiming about “Life on Mars!” The basis for all of this excitement is an article in Science by Dr. David S. McKay of the Lyndon B. Johnson Space Center in Houston and eight of his colleagues from several academic institutions. The reader of this column will not be surprised by the fact that microscopes were used to detect evidence of life on a meteorite from Mars.The first consideration was whether or not the meteorite was in fact a fragment of the martian surface. The specimen, known as ALH84001, is from a class of meteorites that appear to have resulted from impacts on Mars, some of the specimens landing in Antarctica where this one was recovered. Trapped gases (in glass droplets and stringers) in several of the family of meteorites closely match the martian atmosphere for several gases over 8 orders of magnitude range in abundance. Whereas ALHB4001 did not contain such trapped atmospheric gases, its elemental and isotopic composition closely resemble the meteorites that do.
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Zolensky, Michael. "The flux of meteorites to Antarctica." Geological Society, London, Special Publications 140, no. 1 (1998): 93–104. http://dx.doi.org/10.1144/gsl.sp.1998.140.01.09.

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Wang, Bao Hua, Shi Jie Li, and Bing Kui Miao. "The Mineral Chemistry and Classification of New Ordinary Chondrites Collected in Antarctica." Advanced Materials Research 621 (December 2012): 125–29. http://dx.doi.org/10.4028/www.scientific.net/amr.621.125.

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Petrography and mineral chemistry of ninety-eight ordinary chondrites from Grove Mountains, Antarctica, have been studied, in order to assign their chemical-petrographic types. The chemical-petrographic types of these meteorites are presented below: 36 H-groups (21 H4, 9 H5, 6 H6) and 62 L-groups (25 L5, 37 L6). The compositions of olivines and low-Ca pyroxenes in the all these ordinary chondrites have similar composition, respectively, reflecting some degree thermodynamics equilibration in them. The weathering degrees of all the ordinary chondrites, consisting of predominant weathering degrees of W1, suggest lightly weathered among them. More than 30% meteorites experienced severe shock metamorphism, as indicated by the presences of shock-induced melt veins and pockets. These heavily shocked meteorites provide us with natural samples for study of high-pressure polymorphs of minerals.
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Genge, Matthew. "Meteorites, ice, and Antarctica, by William A. Cassidy." Meteoritics & Planetary Science 39, no. 1 (January 2004): 157–58. http://dx.doi.org/10.1111/j.1945-5100.2004.tb00055.x.

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Dissertations / Theses on the topic "Meteorites – Antarctica"

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Steer, Elisabeth. "Antarctic alteration of meteorites." Thesis, Open University, 2016. http://oro.open.ac.uk/48208/.

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The discovery of large accumulations of meteorites in Antarctica is comparably recent, with annual collection expeditions beginning in 1974. Since then, over 50,000 meteorites have been recovered from the icefields of Antarctica. Many of those meteorites have had long residence times of up to 2 Ma mostly encased in ice; during which many of the meteorites have undergone considerable alteration. Understanding the paths of alteration allows reconstruction of original features, but additionally it gives a unique opportunity to examine a natural laboratory of cold, water-restricted alteration environments similar to those on Mars today and in its history. To fully understand the weathering of meteorites in these environments, six L6 chondrites in a variety of weathering states have been examined and characterised petrologically, chemically, and magnetically. Chemical analyses undertaken are major and trace elements measured in bulk and in spatially resolved analysis and bulk oxygen isotopes. Petrology has proven to control the weathering patterns and alteration state of the meteorite. A chemical weathering index has been developed to characterise the state of weathering using bulk chemical data, which also links with the petrological findings. This is especially evident in micro features created by shock, which promote rapid mineral breakdown and acidification of alteration fluids, which, fundamentally changes the nature and speed of the alteration. Shock generated features have created increased vulnerability to weathering and so areas that have undergone significant shock on Mars are more vulnerable to weathering and breakdown. However, the heterogeneity that is inherent to alteration environments of low water to rock ratios results in short transport distances for elements, resulting in little bulk chemical change with significant mineralogical alteration.
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Solberg, Teresa Christine. "Fe oxidation and weathering studies of Antarctic and SNC meteorites." Thesis, Massachusetts Institute of Technology, 1987. http://hdl.handle.net/1721.1/57631.

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Tyra, Mark Anthony. "Terrestrial alteration of CM2 chondritic carbonates in a suite of paired Antarctic meteorites." College Park, Md. : University of Maryland, 2005. http://hdl.handle.net/1903/2672.

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Thesis (M.S.) -- University of Maryland, College Park, 2005.
Thesis research directed by: Geology. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.
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Hagen, Erik H. "A geochemical and petrological investigation of meteorite ablation products in till and ice of Antarctica /." The Ohio State University, 1995. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487867541732056.

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Minami, Masayo, Atsushi Terui, Nobuo Takaoka, and Toshio Nakamura. "An improved extraction system to measure carbon-14 terrestrial ages of meteorites and pairing of the Antarctic Yamato-75097 group chondrites(Proceedings of the 19^ Symposium on Chronological Studies at the Nagoya University Center for Chronological Research in 2006,Part1)." 名古屋大学年代測定資料研究センター, 2007. http://hdl.handle.net/2237/13686.

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第19回名古屋大学年代測定総合研究センターシンポジウム平成18(2006)年度報告<第1部> Proceedings of the 19th symposiumon on Chronological Studies at the Nagoya University Center for Chronological Research in 2006 日時:平成19 (2007)年1月15日(月)～17日(水) 会場:名古屋大学シンポジオン Date:January15th-17th, 2007 Venue:Nagoya Uhiversity Symposion Hall
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Stopar, Julie D. "Aqueous alteration of olivine in nakhlite Miller Range (MIL) 03346." Thesis, 2007. http://hdl.handle.net/10125/20625.

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Books on the topic "Meteorites – Antarctica"

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Cassidy, W. A. Meteorites, ice, and Antarctica. Cambridge: Cambridge University Press, 2003.

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1962-, Mardon Catherine A., ed. The use of geographic remote sensing, mapping and aerial photography to aid in the recovery of blue ice surficial meteorites in Antarctica. Edmonton: Golden Meteorite Press, 2009.

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Symposium, on Antarctic Meteorites (22th 1997 Tokyo Japan). Antarctic Meteorites XXII: Papers presented to the Twentysecond Symposium on Antarctic Meteorites : June 10-12, 1997. Tokyo: National Institute of Polar Research, 1997.

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Symposium, on Antarctic Meteorites (23rd 1998 Tokyo Japan). Antarctic Meteorites XXIII: Papers presented to the Twentythird Symposium on Antarctic Meteorites : June 10-12, 1998. Tokyo: National Institute of Polar Research, 1998.

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Symposium on Antarctic Meteorites (20th 1995 National Institute of Polar Research). Antarctic Meteorites XX: Papers presented to the Twentieth Symposium on Antarctic Meteorites, June 6-8, 1995. Tokyo: National Institute of Polar Research, 1995.

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Symposium on Antarctic Meteorites (18th 1993 Tokyo, Japan). Proceedings of the NIPR Symposium on Antarctic Meteorites. Tokyo: National Institute of Polar Research, 1994.

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Symposium on Antarctic Meteorites (20th 1995 Tokyo, Japan). Proceedings of the NIPR Symposium on Antarctic Meteorites. Tokyo: National Institute of Polar Research, 1996.

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Righter, Kevin, Catherine M. Corrigan, Timothy J. McCoy, and Ralph P. Harvey, eds. 35 Seasons of U.S. Antarctic Meteorites (1976-2010). Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.

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Symposium on Antarctic Meteorites (16th 1991 Tokyo, Japan). Proceedings of the NIPR Symposium on Antarctic Meteorites. Tokyo: National Institute of Polar Research, 1992.

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Symposium on Antarctic Meteorites (21th 1996 Tokyo, Japan). measurements of evaporation rates Antarctic Meteorites XXI: Papers presented to the Twentyfirst Symposium on Antarctic Meteorites : June 5-7, 1996. Tokyo: National Institute of Polar Research, 1996.

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Book chapters on the topic "Meteorites – Antarctica"

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McSween, Harry Y., Ralph P. Harvey, and Catherine M. Corrigan. "Meteorites from Mars, via Antarctica." In Special Publications, 131–43. Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.ch7.

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Herzog, Gregory F., Marc W. Caffee, and A. J. Timothy Jull. "Cosmogenic Nuclides in Antarctic Meteorites." In Special Publications, 153–72. Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.ch9.

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García, Víctor Manuel. "Meteorites Found in the Argentine Antarctic Sector." In Springer Geology, 357–58. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-60683-1_19.

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Harvey, Ralph P., John Schutt, and Jim Karner. "Fieldwork Methods of the U.S. Antarctic Search for Meteorites Program." In Special Publications, 23–41. Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.ch2.

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Corrigan, Catherine M., Linda C. Welzenbach, Kevin Righter, Kathleen M. McBride, Timothy J. McCoy, Ralph P. Harvey, and Cecilia E. Satterwhite. "A Statistical Look at the U.S. Antarctic Meteorite Collection." In Special Publications, 173–87. Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.ch10.

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Righter, Kevin, Cecilia E. Satterwhite, Kathleen M. McBride, Catherine M. Corrigan, and Linda C. Welzenbach. "Curation and Allocation of Samples in the U.S. Antarctic Meteorite Collection." In Special Publications, 43–63. Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.ch3.

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Okano, J., and H. Nishimura. "Ion Microprobe Studies of the Magnesium Isotopic Abundance in Allende and Antarctic Meteorites." In Springer Series in Chemical Physics, 447–50. Berlin, Heidelberg: Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-82724-2_120.

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Marvin, Ursula B. "The Origin and Early History of the U.S. Antarctic Search for Meteorites Program (ANSMET)." In Special Publications, 1–22. Hoboken, NJ: John Wiley & Sons, Inc, 2014. http://dx.doi.org/10.1002/9781118798478.ch1.

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Weintraub, David A. "Hot Potato." In Life on Mars, 161–85. Princeton University Press, 2020. http://dx.doi.org/10.23943/princeton/9780691209258.003.0011.

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This chapter refers to Roberta Score, the curator of the Antarctic Meteorite Laboratory at the Johnson Space Center in Texas, who was hunting for meteorites in Antarctica during the last days of 1984. It discusses the National Science Foundation's Antarctic Search for Meteorites (ANSMET) program, which excavated pristine meteorites collected on the blue ice of Antarctica that had fallen thousands or millions of years ago. It also describes the meteorites as a scientific windfall for the scientific community and worth the difficult work involved in obtaining them. The chapter focuses on the meteorite that was discovered by Score and was named ALH 84001. It points out that the greenish color of ALH 84001 was so unusual that it became a high-priority meteorite when it arrived in Houston.
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"Meteorites from the moon." In Meteorites, Ice, and Antarctica, 144–85. Cambridge University Press, 2003. http://dx.doi.org/10.1017/cbo9780511536083.011.

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Conference papers on the topic "Meteorites – Antarctica"

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Sipiera, Paul P., Richard B. Hoover, and Gregory A. Jerman. "Meteorites and microbes: meteorite collection and ice sampling at Patriot Hills, Thiel Mountains, and South Pole, Antarctica." In International Symposium on Optical Science and Technology, edited by Richard B. Hoover. SPIE, 2000. http://dx.doi.org/10.1117/12.411617.

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Sipiera, Paul P., Richard B. Hoover, and Gregory A. Jerman. "Mineralogical and petrological analyses of two possible achondrite meteorites recovered from the Thiel Mountains, Antarctica." In International Symposium on Optical Science and Technology, edited by Richard B. Hoover, Gilbert V. Levin, Roland R. Paepe, and Alexei Y. Rozanov. SPIE, 2002. http://dx.doi.org/10.1117/12.454767.

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Sipiera, Paul P., and Birgit I. Sattler. "Meteorite collection and ice samples from the Pecora Escarpment, Antarctica." In Optical Science and Technology, the SPIE 49th Annual Meeting, edited by Richard B. Hoover, Gilbert V. Levin, and Alexei Y. Rozanov. SPIE, 2004. http://dx.doi.org/10.1117/12.564553.

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Wang, Fang, Xiao Cheng, Yan Liu, Fengming Hui, Tingbiao Chen, Yufang Ye, Zhixin Wang, and Chen Zhao. "Prediction of meteorite concentration areas in Prince Charles Mountains, East Antarctica." In 2011 19th International Conference on Geoinformatics. IEEE, 2011. http://dx.doi.org/10.1109/geoinformatics.2011.5980765.

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Becker, Luann, Daniel P. Glavin, and Jeffrey L. Bada. "Polycyclic aromatic hydrocarbons (PAHs) in Antarctic Martian meteorites, carbonaceous chondrites, and polar ice." In Optical Science, Engineering and Instrumentation '97, edited by Richard B. Hoover. SPIE, 1997. http://dx.doi.org/10.1117/12.278782.

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Marsh, Liam A., Wouter van Verre, John Wilson, Geoffrey W. Evatt, and Anthony J. Peyton. "Evaluation of a Bespoke Antarctic Meteorite Detection System in Polar Operating Conditions." In 2020 IEEE Sensors Applications Symposium (SAS). IEEE, 2020. http://dx.doi.org/10.1109/sas48726.2020.9220085.

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