Quantifying the martian geochemical reservoirs
著者
書誌事項
Quantifying the martian geochemical reservoirs
(Space sciences series of ISSI, v.44)
Springer, c2013
大学図書館所蔵 全2件
  青森
  岩手
  宮城
  秋田
  山形
  福島
  茨城
  栃木
  群馬
  埼玉
  千葉
  東京
  神奈川
  新潟
  富山
  石川
  福井
  山梨
  長野
  岐阜
  静岡
  愛知
  三重
  滋賀
  京都
  大阪
  兵庫
  奈良
  和歌山
  鳥取
  島根
  岡山
  広島
  山口
  徳島
  香川
  愛媛
  高知
  福岡
  佐賀
  長崎
  熊本
  大分
  宮崎
  鹿児島
  沖縄
  韓国
  中国
  タイ
  イギリス
  ドイツ
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  フランス
  ベルギー
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  スウェーデン
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注記
"Previously published in Space Science Reviews, volume 174, Issues 1-4, 2013."--T.p
Includes bibliographical references
内容説明・目次
内容説明
Over the last fifteen years, space-based exploration of the solar system has increased dramatically, with more and more sophisticated orbiters and landers being sent to Mars. This intense period, rich in unprecedented scientific results, has led to immense progress in our perception of Mars and of its evolution over geological time. In parallel, advances in numerical simulations and laboratory experiments also shed new light on the geochemical evolution of the planet Mars.
The ISSI-Europlanet Workshop entitled "Quantifying the Martian Geochemical Reservoirs" was held in Bern in April 2011 with the objective to create a diverse interdisciplinary forum composed of scientists directly involved in space-based exploration of the Martian surface, meteoriticists studying SNC meteorites, and planetary and/or Earth scientists simulating, numerically or experimentally, the physical and chemical processes occurring on or within Mars. The chapters of this book provide an overview of current knowledge of the past and present Martian geochemical reservoirs, from the accretionary history to the secondary alteration processes at the surface. In addition to the detailed description of data from Mars and the methods used to obtain them, the contributions also emphasize comparison with features on Earth, providing a perspective on the extent to which our knowledge of terrestrial systems influences interpretation of data from Mars. Areas that would benefit from future work and measurements are also identified, providing a view of the short-term and long-term future of the study of Mars.
This collection of chapters constitutes a timely perspective on current knowledge and thinking concerning the geochemical evolution of Mars, providing context and a valuable reference point for even more exciting future discoveries. It is aimed at graduate students and researchers active in geochemistry and space science. Previously published in Space Science Reviews, Vol. 174/1-4, 2013.
目次
The Formation of Mars: Building Blocks and Accretion Time Scale.- Core Formation and Mantle Differentiation on Mars.- Long-Term Evolution of the Martian Crust-Mantle System.- Outgassing History and Escape of the Martian Atmosphere and Water Inventory.- Quantifying the Martian Hydrosphere: Current Evidence, Time Evolution and Implications for the Habitability of the Planet.- Volatile Trapping in Martian Clathrates.- Geochemical Reservoirs and Timing of Sulphur Cycling on Mars.- Geochemistry of Carbonates on Mars.- Implications for Climate History and Nature of Aqueous Environments.- Geochemical Consequences of Widespread Clay Mineral Formation in Mars' Ancient Crust.
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