MARC全文
02h0113551 20160517165903.0 160330s2015 njua frb |001|||eng d 9781118860571(hardback) : CNY1629.00 BTCTA eng rda BTCTA BDX ; YDXCP ; GZN ; OCLCO ; COD ; OCLCF ; NAM ; CNNGL QE509 .E22 2015 525 23 a200 aP311 The early earth : accretion and differentiation / James Badro, Michael Walter, editors. Hoboken, NJ : Wiley, c2015. aHoboken, New Jersey : ; aWashington, D.C. : bJohn Wiley & Sons, Inc. ; ; bAmerican Geophysical Union, c[2015] ; c@2015 xi, 181 pages : illustrations (some color) ; 29 cm. atext btxt 2rdacontent aunmediated bn 2rdamedia avolume bnc 2rdacarrier Geophysical monograph ; 212 "This work is a co-publication between the American Geophysical Union and John Wiley & Sons, Inc." Includes bibliographical references and index. Timing of nebula processes which shaped the precursors of the terrestrial planets / ; The Earth's building blocks / ; Earth and Terrestrial Planet Formation / ; Late accretion and the late veneer / ; Early differentiation and core formation: processes and timescales / ; An experimental geochemistry perspective on Earth's core formation / ; Fractional melting and freezing in the deep mantle and implications for the formation of a basal magma ocean / ; Early Differentiation and its Long Term Consequences for Earth Evolution / Marc Chaussidon, Ming-Chang Liu -- ; Fre虂de虂ric Moynier, Bruce Fegley, Jr. -- ; Seth Jacobson, Kevin J. Walsh -- ; Alessandro Morbidelli, Bernard J. Wood -- ; Francis Nimmo, Thorsten Kleine -- ; Julien Siebert, Anat Shahar -- ; Ste虂phane Labrosse, John W. Hernlund, Kei Hirose -- ; Richard W. Carlson, Maud Boyet, Jonathan O'Neil, Hanika Rizo, Richard J. Walker. Provides a multidisciplinary overview of the state-of-the-art in understanding the formation and primoridal evolution of the Earth. The fundamental structure of the Earth as we know it today was inherited from the initial conditions 4.56 billion years ago as a consequence of planetesimal accretion, large impacts among planetary objects, and planetary-scale differentiation. The evolution of the Earth from a molten ball of metal and magma to the tectonically active, dynamic habitable planet that we know today is unique among the terrestrial planets, and understanding the earliest processes that led to Earth's current state is the essence of this volume. Important results have emerged from a wide range of disciplines including cosmochemistry, geochemistry, experimental petrology, experimental and theoretical mineral physics and geodynamics. Geodynamics. ; Nebular hypothesis. Earth (Planet) ; Earth (Planet) Internal structure. ; Geology. aBadro, James, ; eeditor. ; aWalter, Michael ; q(Michael J.), ; eeditor. Geophysical monograph ; 212. aCN b010001 010001 P 260.64 G29m v212 ; h1 ; rCNY1629.00 gljx1604