The Encyclopedia of Igneous and Metamorphic Petrology

The Encyclopedia of Igneous and Metamorphic Petrology PDF

Author: Donald Bowes

Publisher: Springer Science & Business Media

Published: 1990-02-28

Total Pages: 635

ISBN-13: 0442206232

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Featuring over 250 contributions from more than 100 earth scientists from 18 countries, The Encyclopedia of Igneous and Metamorphic Petrology deals with the nature and genesis of igneous rocks that have crystallized from molten magma, and of metamorphic rocks that are the products of re-crystallization associated with increases in temperature and pressure, mainly at considerable depths in the Earth's crust. Entries range from alkaline rocks to zeolite facies - providing information on the mineralogical, chemical and textural characters of rock types, the development of concepts and the present state of knowledge across the spectrum of igneous and metamorphic petrology, together with extensive lists of both commonly used and little used terms and bibliographies.

Large Meteorite Impacts and Planetary Evolution VI

Large Meteorite Impacts and Planetary Evolution VI PDF

Author: Wolf Uwe Reimold

Publisher: Geological Society of America

Published: 2021-09-23

Total Pages: 644

ISBN-13: 081372550X

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"This volume contains a sizable suite of contributions dealing with regional impact records (Australia, Sweden), impact craters and impactites, early Archean impacts and geophysical characteristics of impact structures, shock metamorphic investigations, post-impact hydrothermalism, and structural geology and morphometry of impact structures - on Earth and Mars"--

Cathodoluminescence and its Application in the Planetary Sciences

Cathodoluminescence and its Application in the Planetary Sciences PDF

Author: Arnold Gucsik

Publisher: Springer Science & Business Media

Published: 2008-11-14

Total Pages: 168

ISBN-13: 3540875298

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Cathodoluminescence microscopy/spectroscopy is a powerful technique providing detailed information on the shock metamorphism of target rocks, biosignatures of meteorites and mineralogy of the pre-solar grains. Moreover, it can be used as an in-situ method to classify the solid-atmospheric-liquid interactions on the surface of Mars.

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