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Книги з теми "Meteorites Analysis"

Щоб переглянути інші типи публікацій з цієї теми, перейдіть за посиланням: Meteorites Analysis.

Автор: Grafiati

Опубліковано: 4 червня 2021

Оновлено: 28 січня 2023

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1

I͡Udin, I. A. Mineralogii͡a meteoritov. Sverdlovsk: Akademii͡a nauk SSSR, Uralʹskiĭ nauch. t͡sentr, 1987.

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2

Wilson, Graham C. Petrographic notes on miscellaneous samples: Ten slags and glassy materials, seven alkaline rocks and five mafic-ultramafic rocks : miscellaneous observations on behalf of slag, meteorite and ore deposits research. Toronto: Turnstone Geological Services, 2000.

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3

Mog, R. A. Global nonlinear optimization of spacecraft protective structures design. [Marshall Space Flight Center, Ala.]: National Aeronautics and Space Administration, George C. Marshall Space Flight Center, 1990.

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4

United States. National Aeronautics and Space Administration, ed. Lunar sample analysis: Final report for the period February 3, 1971 through October l, 1986. [Thousand Oaks, CA]: Rockwell International Science Center, 1986.

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5

Eugene, Jarosewich, Clarke Roy S, and Barrows Julie N, eds. The Allende meteorite reference sample. Washington, D.C: Smithsonian Institution Press, 1986.

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6

United States. National Aeronautics and Space Administration., ed. Lunar sample analysis: Annual report 13 for the period January 1, 1984 through December 3l, 1984. [Thousand Oaks, CA]: Rockwell International Science Center, 1985.

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7

Farrington, Oliver C. Analysis Of Iron And Stone Meteorites - Field Columbian Museum. Merchant Books, 2006.

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8

K, Nishiizumi, and United States. National Aeronautics and Space Administration., eds. Exposure history of lunar meteorites Queen Alexandra Range 93069 and 94269. [Washington, DC: National Aeronautics and Space Administration, 1996.

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9

G, Sears D. W., and United States. National Aeronautics and Space Administration., eds. Meteorite infall and transport in Antarctica: An analysis of icefields as accumulation surfaces. [Washington, DC: National Aeronautics and Space Administration, 1997.

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10

G, Sears D. W., and United States. National Aeronautics and Space Administration., eds. Meteorite infall and transport in Antarctica: An analysis of icefields as accumulation surfaces. [Washington, DC: National Aeronautics and Space Administration, 1997.

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11

Meteorite infall and transport in Antarctica: An analysis of icefields as accumulation surfaces. [Washington, DC: National Aeronautics and Space Administration, 1997.

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12

Ding, Gangjian. In situ analysis of 187 Re - 187 Os systematics and silver isotopic compositions in iron meteorites using accelerator mass spectrometry. 1996.

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13

Observatory, Smithsonian Astrophysical, ed. Mineralogic and petrologic studies of meteorites and lunar samples: Grant NAGW 3451, final progress report, for the period 01 February 1993 through 30 September 1997. Cambridge, Mass: Smithsonian Institution, Astrophysical Observatory, 1998.

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14

United States. National Aeronautics and Space Administration., ed. Light stable isotope analysis of meteorites by ion microprobe: Final report, performance period, 1 February 1992 - 31 January 1994, with no-cost extension to 31 July 1994. [Washington, DC: National Aeronautics and Space Administration, 1994.

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15

Bridges, John C. Evolution of the Martian Crust. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.18.

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Анотація:

This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Mars, which has a tenth of the mass of Earth, has cooled as a single lithospheric plate. Current topography gravity maps and magnetic maps do not show signs of the plate tectonics processes that have shaped the Earth’s surface. Instead, Mars has been shaped by the effects of meteorite bombardment, igneous activity, and sedimentary—including aqueous—processes. Mars also contains enormous igneous centers—Tharsis and Elysium, with other shield volcanoes in the ancient highlands. In fact, the planet has been volcanically active for nearly all of its 4.5 Gyr history, and crater counts in the Northern Lowlands suggest that may have extended to within the last tens of millions of years. Our knowledge of the composition of the igneous rocks on Mars is informed by over 100 Martian meteorites and the results from landers and orbiters. These show dominantly tholeiitic basaltic compositions derived by melting of a relatively K, Fe-rich mantle compared to that of the Earth. However, recent meteorite and lander results reveal considerable diversity, including more silica-rich and alkaline igneous activity. These show the importance of a range of processes including crystal fractionation, partial melting, and possibly mantle metasomatism and crustal contamination of magmas. The figures and plots of compositional data from meteorites and landers show the range of compositions with comparisons to other planetary basalts (Earth, Moon, Venus). A notable feature of Martian igneous rocks is the apparent absence of amphibole. This is one of the clues that the Martian mantle had a very low water content when compared to that of Earth.The Martian crust, however, has undergone hydrothermal alteration, with impact as an important heat source. This is shown by SNC analyses of secondary minerals and Near Infra-Red analyses from orbit. The associated water may be endogenous.Our view of the Martian crust has changed since Viking landers touched down on the planet in 1976: from one almost entirely dominated by basaltic flows to one where much of the ancient highlands, particularly in ancient craters, is covered by km deep sedimentary deposits that record changing environmental conditions from ancient to recent Mars. The composition of these sediments—including, notably, the MSL Curiosity Rover results—reveal an ancient Mars where physical weathering of basaltic and fractionated igneous source material has dominated over extensive chemical weathering.

16

Farrington, Oliver C. Analyses of Iron and Stone Meteorites, with the Field Columbian Museum of Meteorites. Wexford College Press, 2003.

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17

Schilk, Alan J. Chemical and statistical analyses of chondrules from the Mokoia (CV3) meteorite. 1991.

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18

Thin-sectioning and analysis of fine-grained meteoritic materials. Westmont, Ill: McCrone Associates, Inc., 1992.

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19

United States. National Aeronautics and Space Administration., ed. Thin-sectioning and analysis of fine-grained meteoritic materials. Westmont, Ill: McCrone Associates, Inc., 1992.

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20

United States. National Aeronautics and Space Administration., ed. Thin-sectioning and analysis of fine-grained meteoritic materials. Westmont, Ill: McCrone Associates, Inc., 1992.

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21

Gregory, Tim. Meteorite: The Stones from Outer Space That Made Our World. Hodder & Stoughton, 2021.

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22

Milstein, Randall L. The Calvin impact crater, Cass County, Michigan: Identification and analysis of a subsurface ordovician astrobleme. 1994.

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23

L, Kirk Randy, Strom Robert G, United States. National Aeronautics and Space Administration, and Geological Survey (U.S.), eds. Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data. [Reston, Va.?]: U.S. Dept. of the Interior, U.S. Geological Survey, 1995.

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24

L, Kirk Randy, Strom Robert G, United States. National Aeronautics and Space Administration., and Geological Survey (U.S.), eds. Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data. [Reston, Va.?]: U.S. Dept. of the Interior, U.S. Geological Survey, 1996.

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25

Data base of impact craters on Venus based on analysis of Magellan radar images and altimetry data. [Menlo Park, CA]: U.S. Geological Survey, 1998.

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