Chronology and evolution of Mars : proceedings of an ISSI Workshop, 10-14 April 2000, Bern, Switzerland

Bibliographic Information

Chronology and evolution of Mars : proceedings of an ISSI Workshop, 10-14 April 2000, Bern, Switzerland

edited by Reinald Kallenbach, Johannes Geiss, William K. Hartmann ; editorial assistant Ursula Pfander

(Space sciences series of ISSI, v. 12)

Kluwer Academic Publishers, c2001

Available at  / 6 libraries

Search this Book/Journal

Note

Includes index

"Reprinted from Space science reviews, vol. 96, Nos. 1-4, 2001"

Description and Table of Contents

Description

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.

Table of Contents

  • Friends of this book. Introduction: A New Chapter in Mars Research
  • R. Kallenbach. I. Chronology of Mars and of the Inner Solar System. Stratigraphy and Isotope Ages of Lunar geologic Units: Chronological Standard for the Inner Solar System
  • D. Stoeffler, G. Ryder. Cratering Records in the Inner Solar System in Relation to the Lunar Reference System
  • G. Neukum, et al. Mars/Moon Cratering Rate Ratio Estimates
  • B.A. Ivanov. Ages and Geologic Histories of Martian Meteorites
  • L.E. Nyquist, et al. Cratering Chronology and the Evolution of Mars
  • W.K. Hartmann, G. Neukum. II: Evolution of the Interior and Surface of Mars. The Accretion, Composition and Early Differentiation of Mars
  • A.N. Halliday, et al. Geophysical Constraints on the Evolution of Mars
  • T. Spohn, et al. Geological Processes and Evolution
  • J.W. Head, et al. The Martian Surface Composition
  • J.P. Bibring, S. Erard. Chemical Composition of Rocks and Soils at the Pathfinder Site
  • H. Wanke, et al. III: History and Fate of the Martian Atmosphere and Hydrosphere. Geomorphologic Evidence for Liquid Water
  • P. Masson, et al. Alteration Assemblages in Martian Meteorites: Implications for Near-Surface Processes
  • J.C. Bridges, et al. Aeolian Processes and Their Effects on Understanding the Chronology of Mars
  • R. Greeley, et al. Martian Seeps and Their Relation to Youthful Geothermal Activity
  • W.K. Hartmann. The Atmosphere of Mars as Constrained by Remote Sensing
  • T. Encrenaz. Martian Volatiles: Isotopic Composition, Origin, and Evolution
  • D.D. Bogard, et al. Epilogue. Summary: New Views and New Directions in Mars Research
  • W.K. Hartmann, et al. Glossary. Subject Index. List of Acronyms and Basic Mars Data. Author Index.List of Participants.

by "Nielsen BookData"

Related Books: 1-1 of 1

Details

  • NCID
    BA53642291
  • ISBN
    • 0792370511
  • Country Code
    ne
  • Title Language Code
    eng
  • Text Language Code
    eng
  • Place of Publication
    Dordrecht
  • Pages/Volumes
    ix, 498 p.
  • Size
    25 cm
  • Classification
  • Parent Bibliography ID
Page Top