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Chronology and Evolution of Mars: Proceedings from an Issi Workshop, 10-14 April 2000, Bern, Switzerland - Couverture rigide
Synopsis
Mars is about one-eighth the mass of the Earth and it may provide an analogue of what the Earth was like when it was at such an early stage of accretion. The fur- ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth's moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which lasted more than 50 Myr in the case of the Earth (Halliday, 2000a, b), appears to have been shorter and less catastrophic in the case of Mars (Harper et ai., 1995; Lee and Halliday, 1997). In this article we review the basic differences between the bulk composition of Mars and the Earth and the manner in which this plays into our understanding of the timing and mechanisms of accretion and core formation. We highlight some of the evidence for early cessation of major collisional growth on Mars. Finally, we reevaluate the isotopic evidence that Mars differentiated quickly. Fundamental differences between the composition of Mars and that of other terrestrial planets are apparent from the planet's slightly lower density and from the compositions of Martian meteorites. The low density is partially explicable if there is a greater proportion of more volatile elements.
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Chronology and Evolution of Mars: Proceedings of an ISSI Workshop, 10?14 April 2000, Bern, Switzerland (Space Sciences Series of ISSI (12))
Edité par
Springer, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
Ancien ou d'occasion
Couverture rigide
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Hardcover. Etat : Gut bis sehr gut. 1. Auflage. vignette auf vorblatt, gut, eher sehr gut, nur geringe lagerspuren, 498 seiten. N° de réf. du vendeur A-648-Vtg
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Chronology and evolution of Mars. Proceedings of an ISSI workshop, 10-14 April 2000, Bern, Switzerland.
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Dordrecht, Kluwer Academic Publishers, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
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Hardcover. ix, 491 S. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. Ex-library with stamp and library-signature. GOOD condition, some traces of use. w04759 9780792370512 Sprache: Englisch Gewicht in Gramm: 1100. N° de réf. du vendeur 2429583
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CHRONOLOGY AND EVOLUTION OF MARS
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Kluwer Academic Publishers, Dordrecht, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
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Hardcover. Octavo, 498 pages. In Good condition. Bound in light blue paper with dark blue lettering. Boards have scuffing and bumping to corners, minor scratching, and minor staining. Text block has foxing in the back and head edge, and some writing in the front pages. NOTE: Shelved in ND-E. 1377284. FP New Rockville Stock. N° de réf. du vendeur 1377284
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Chronology and Evolution of Mars - Space Science Series of ISSI Volume 12 - Proceedings of an ISSI Workshop, 10-14 April, 2000, Bern, Switzerland - Reprinted from Space Science Reviews, Vol. 96, Nos. 1-4, 2001
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Kluwer Academic Publishers (KAP), Boston, Dordrecht, London, 2001
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ISBN 13 : 9780792370512
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Hardcover. Etat : Very Good. No Jacket. Hardback copy, no dustjacket as issued. 498pp. Colour and b/w charts and graphs throughout. Not library copy, no inscriptions. (45/4). N° de réf. du vendeur ABE-1588415364122
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Chronology and Evolution of Mars
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Springer Netherlands, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
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Chronology and Evolution of Mars
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Springer Netherlands Sep 2001, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
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Buch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Mars is about one-eighth the mass of the Earth and it may provide an analogue of what the Earth was like when it was at such an early stage of accretion. The fur ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth's moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which lasted more than 50 Myr in the case of the Earth (Halliday, 2000a, b), appears to have been shorter and less catastrophic in the case of Mars (Harper et ai. , 1995; Lee and Halliday, 1997). In this article we review the basic differences between the bulk composition of Mars and the Earth and the manner in which this plays into our understanding of the timing and mechanisms of accretion and core formation. We highlight some of the evidence for early cessation of major collisional growth on Mars. Finally, we reevaluate the isotopic evidence that Mars differentiated quickly. Fundamental differences between the composition of Mars and that of other terrestrial planets are apparent from the planet's slightly lower density and from the compositions of Martian meteorites. The low density is partially explicable if there is a greater proportion of more volatile elements. 512 pp. Englisch. N° de réf. du vendeur 9780792370512
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Chronology and Evolution of Mars
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Springer Netherlands, Springer Netherlands Sep 2001, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
Neuf
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Vendeur : buchversandmimpf2000, Emtmannsberg, BAYE, Allemagne
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Buch. Etat : Neu. Neuware -Mars is about one-eighth the mass of the Earth and it may provide an analogue of what the Earth was like when it was at such an early stage of accretion. The fur ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth's moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which lasted more than 50 Myr in the case of the Earth (Halliday, 2000a, b), appears to have been shorter and less catastrophic in the case of Mars (Harper et ai. , 1995; Lee and Halliday, 1997). In this article we review the basic differences between the bulk composition of Mars and the Earth and the manner in which this plays into our understanding of the timing and mechanisms of accretion and core formation. We highlight some of the evidence for early cessation of major collisional growth on Mars. Finally, we reevaluate the isotopic evidence that Mars differentiated quickly. Fundamental differences between the composition of Mars and that of other terrestrial planets are apparent from the planet's slightly lower density and from the compositions of Martian meteorites. The low density is partially explicable if there is a greater proportion of more volatile elements.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 512 pp. Englisch. N° de réf. du vendeur 9780792370512
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Chronology and Evolution of Mars : Proceedings of an ISSI Workshop, 10-14 April 2000, Bern, Switzerland
Edité par
Springer Netherlands, Springer Netherlands, 2001
ISBN 10 : 0792370511
ISBN 13 : 9780792370512
Neuf
Couverture rigide
Vendeur : AHA-BUCH GmbH, Einbeck, Allemagne
Évaluation du vendeur 5 sur 5 étoiles
Buch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Mars is about one-eighth the mass of the Earth and it may provide an analogue of what the Earth was like when it was at such an early stage of accretion. The fur ther growth of the Earth was sustained by major collisions with planetesimals and planets such as that which resulted in the formation ofthe Earth's moon (Hartmann and Davis, 1975; Cameron and Ward, 1976; Wetherill, 1986; Cameron and Benz, 1991). This late accretionary history, which lasted more than 50 Myr in the case of the Earth (Halliday, 2000a, b), appears to have been shorter and less catastrophic in the case of Mars (Harper et ai. , 1995; Lee and Halliday, 1997). In this article we review the basic differences between the bulk composition of Mars and the Earth and the manner in which this plays into our understanding of the timing and mechanisms of accretion and core formation. We highlight some of the evidence for early cessation of major collisional growth on Mars. Finally, we reevaluate the isotopic evidence that Mars differentiated quickly. Fundamental differences between the composition of Mars and that of other terrestrial planets are apparent from the planet's slightly lower density and from the compositions of Martian meteorites. The low density is partially explicable if there is a greater proportion of more volatile elements. N° de réf. du vendeur 9780792370512
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