Meteorites And The Early Solar System Ii

Author: Dante S. Lauretta
Publisher: University of Arizona Press
ISBN: 9780816525621
Size: 58.32 MB
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Meteorites And The Early Solar System Ii from the Author: Dante S. Lauretta. They range in size from microscopic particles to masses of many tons. The geologic diversity of asteroids and other rocky bodies of the solar system are displayed in the enormous variety of textures and mineralogies observed in meteorites. The composition, chemistry, and mineralogy of primitive meteorites collectively provide evidence for a wide variety of chemical and physical processes. This book synthesizes our current understanding of the early solar system, summarizing information about processes that occurred before its formation. It will be valuable as a textbook for graduate education in planetary science and as a reference for meteoriticists and researchers in allied fields worldwide.


Author: Robert Hutchison
Publisher: Cambridge University Press
ISBN: 9780521470100
Size: 24.85 MB
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Meteorites from the Author: Robert Hutchison. Meteorite research is fundamental to our understanding of the origin and early history of the Solar System. Some meteorites were produced by melting on asteroids, a few are from the Moon and others are martian. Their study yields a chronology of the first 100 million years of Solar System history and provides evidence that our Sun went through a highly radiative, T Tauri stage. This book considers the mechanism and timing of core formation and basaltic volcanism on asteroids and the effects of heating water-rich bodies. Results from meteorite research are placed in a galactic setting, and a theory is proposed for the origin of the planets of our Solar System. This advanced yet succinct introduction provides a classification of meteorites and discusses their ages and origin. It will be valuable to graduate students and scientists in astrophysics, space research, cosmochemistry, geochemistry, isotope geology and earth and planetary sciences.

35 Seasons Of U S Antarctic Meteorites 1976 2010

Author: Kevin Righter
Publisher: John Wiley & Sons
ISBN: 1118798325
Size: 19.37 MB
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35 Seasons Of U S Antarctic Meteorites 1976 2010 from the Author: Kevin Righter. "A copublication between the American Geophysical Union and John Wiley & Sons, Inc."


Author: Brian Harold Mason
Size: 68.63 MB
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Cosmochemistry from the Author: Brian Harold Mason.

Principles Of Meteoritics

Author: E.L. Krinov
Publisher: Elsevier
ISBN: 1483184463
Size: 75.37 MB
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Principles Of Meteoritics from the Author: E.L. Krinov. Principles of Meteoritics examines the significance of meteorites in relation to cosmogony and to the origin of the planetary system. The book discusses the science of meteoritics and the sources of meteorites. Scientists study the morphology of meteorites to determine their motion in the atmosphere. The scope of such study includes all forms of meteorites, the circumstances of their fall to earth, their motion in the atmosphere, and their orbits in space. Meteoric bodies vary in sizes; in calculating their motion in interplanetary space, astronomers apply the laws of Kepler. In the region of retardation, the direction of motion of the meteoric body changes, and a break in the visible and real trajectories follows. The angle of fall of meteorites at a vertical line on the surface of the Earth measures between 20 degrees to 30 degrees. The text also discusses the Tunguska and Sikhote-alin meteorites, two gigantic meteorites that fell in the U.S.S.R. The text also discusses the chemistry, the mineralogy, the petrography, and the physical properties of meteorites. The book is suitable for astronomers, geologists, and general readers who have an interest in sky watching.

Suizhou Meteorite Mineralogy And Shock Metamorphism

Author: Xiande Xie
Publisher: Springer
ISBN: 366248479X
Size: 29.54 MB
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Suizhou Meteorite Mineralogy And Shock Metamorphism from the Author: Xiande Xie. This book introduces the unusual shock-related mineralogical features of the shocked Suizhou L6 (S5) meteorite. The olivine and pyroxene in Suizhou display a mosaic shock feature, while most of plagioclase grains have transformed to glassy maskelynite. A few of the shock-induced melt veins in the meteorite are the simplest, straightest and thinnest ones among all shock-vein-bearing meteorites, and contain the most abundant high-pressure mineral species. Among the 11 identified species, tuite, xieite, and the post-spinel CF-phase of chromite are new minerals. The meteorite experienced a peak shock pressure up to 24 GPa and temperatures of up to 1000° C. Locally developed shock veins were formed at the same pressure, but at an elevated temperature of about 2000° C that was produced by localized shear-friction stress. The rapid cooling of the extremely thin shock veins is the main reason why 11 shock-induced high-pressure mineral phases could be preserved in them so well. This book offers a helpful guide for meteoritics researchers and mineralogists and invaluable resource for specialists working in high-pressure and high-temperature mineralophysics.