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This is the first book to explain how and why solid planets and satellites develop crusts. Extensively referenced and annotated, it presents a geochemical and geological survey of the crusts of the Moon, Mercury, Venus, Earth and Mars, the asteroid Vesta, and several satellites like Europa, Ganymede, and Callisto. After describing the nature and formation of solar system bodies, the book presents a comparative investigation of different planetary crusts and discusses many current crustal controversies. The authors propose the theory of stochastic processes dominating crustal development, and debate the possibility of Earth-like planets existing elsewhere in the cosmos. Written by two leading authorities on the subject, this book presents an up-to-date survey of the scientific problems of crustal development.
Preface; 1. The planets: their formation and differentiation; 2. A primary crust: the highland crust of the Moon; 3. A secondary crust: the Lunar Maria; 4. Mercury; 5. Mars: early differentiation and planetary composition; 6. Mars: crustal composition and evolution; 7. Venus: a twin planet to Earth?; 8. The oceanic crust of the Earth; 9. The Hadean crust of the Earth; 10. The Archean crust of the Earth; 11. The post-Archean continental crust; 12. Composition and evolution of the continental crust; 13. Crusts on minor bodies; 14. Reflections: the elusive patterns of planetary crusts; Index.
Ross Taylor was born in New Zealand and is now an Emeritus Professor at the Australian National University. He is a trace element geochemist and carried out the initial analysis of the first lunar sample returned to Earth at NASA, Houston in 1969. He has a D.Sc. from the University of Oxford, is a Foreign Member of the US National Academy of Sciences. and has received the Goldschmidt Medal of the Geochemical Society, the Leonard Medal of the Meteoritical Society and the Bucher Medal of the American Geophysical Union. He is the author of six other books including Solar System Evolution, Second edition (Cambridge University Press, 2001). Asteroid 5670 is named Rosstaylor in his honour. Scott M. McLennan is Professor of Geochemistry at the State University of New York at Stony Brook. He conducts research into the geochemistry of sedimentary rocks, and has published 140 papers in the fields of geochemistry, planetary science and sedimentology. Since 1998, he has applied laboratory experiments and data returned from missions to Mars to understand the sedimentary processes of that planet, and is on the science teams of the 2003 Mars Exploration Rover and 2001 Mars Odyssey missions. He received a Presidential Young Investigator Award from the National Science Foundation in 1989 and a NASA Group Achievement Award as part of the Mars Exploration Rover Science Operations Team in 2004.
Review of the hardback: 'Rarely does one find a book which truly examines in detail the subject of comparative planetology. This is just such a book. ... an excellent starting point to delve deeper into the specific subject. ... In summary this is a unique book, addressing for the first time the subject of planetary crusts from a comparative point of view in a clear and thorough manner; I recommend it to students and specialists alike.' Planetary and Space Science Review of the hardback: 'In conclusion, Planetary Crusts: Their Composition, Origin and Evolution is a well-written and researched book that would complement the library of any crustal scientist, graduate-level student studying planets, or a person curious as to how planets and their crusts came about.' The Meteoritical Society Review of the hardback: '... a comprehensive description and insightful discussion of virtually all salient aspects of the formation and the evolution of planets and their interiors.' Nature Geoscience
