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Titlebook: Geology and Habitability of Terrestrial Planets; Kathryn E. Fishbaugh,Philippe Lognonné,Oleg Korabl Book 2007 Springer-Verlag New York 200

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发表于 2025-3-21 19:29:23 | 显示全部楼层 |阅读模式
书目名称Geology and Habitability of Terrestrial Planets
编辑Kathryn E. Fishbaugh,Philippe Lognonné,Oleg Korabl
视频video
概述Presents the combined scientific expertise of researchers studying the conditions of life on other planets
丛书名称Space Sciences Series of ISSI
图书封面Titlebook: Geology and Habitability of Terrestrial Planets;  Kathryn E. Fishbaugh,Philippe Lognonné,Oleg Korabl Book 2007 Springer-Verlag New York 200
描述.Given the fundamental importance of and universal interest in whether extraterrestrial life has developed or could eventually develop in our solar system and beyond, it is vital that an examination of planetary habitability go beyond simple assumptions such as, "Where there is water, there is life". This book has resulted from a workshop at the International Space Science Institute (ISSI) in Bern, Switzerland which brought together planetary geologists, geophysicists, atmospheric scientists and biologists to discuss the multi-faceted problem of how the habitability of a planet co-evolves with the geology of the surface and interior, the atmosphere, and the magnetosphere...Each of the six chapters have been written by authors with a range of expertise so that each chapter is itself multi-disciplinary, comprehensive, and accessible to scientists in all disciplines. These chapters delve into what life needs to exist and ultimately to thrive, the early environments of the young terrestrial planets, the role of volatiles in habitability, currently habitable (but possibly not inhabited) geologic environments, the connection between a planet’s inner workings and the habitability of its s
出版日期Book 2007
关键词Extraterrestrial life; Planet; Solar System; biomarkers; conditions for life; earth; evolution; habitable z
版次1
doihttps://doi.org/10.1007/978-0-387-74288-5
isbn_softcover978-1-4419-2553-4
isbn_ebook978-0-387-74288-5Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer-Verlag New York 2007
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发表于 2025-3-21 20:43:26 | 显示全部楼层
https://doi.org/10.1007/978-3-031-12000-8eductants (e.g. dead organic matter) and oxidants (including waste products). Potential Martian habitats are discussed: by comparison with Earth there are many potential environmental settings on Mars in which life may once have occurred, or may even continue to exist. The long-term evolution of habitability in the Solar System is considered.
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Creating Habitable Zones, at all Scales, from Planets to Mud Micro-Habitats, on Earth and on Mars,eductants (e.g. dead organic matter) and oxidants (including waste products). Potential Martian habitats are discussed: by comparison with Earth there are many potential environmental settings on Mars in which life may once have occurred, or may even continue to exist. The long-term evolution of habitability in the Solar System is considered.
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Three-Level Schemes with Operator Factors,, as well as the presence of a magnetic field, are important factors contributing to the habitability of a planet. This chapter reviews these processes, their mutual interactions, and the role life plays in regulating or modulating them.
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Planetary Magnetic Dynamo Effect on Atmospheric Protection of Early Earth and Mars,out 4 Gyr ago), atmospheric escape induced by solar wind began. We consider scenarios which could ultimately lead to a decrease of atmospheric pressure to the presently observed value of 7 mbar: a much weaker early martian magnetic field, a late onset of the dynamo, and high erosion rates of a denser early atmosphere.
发表于 2025-3-22 21:44:41 | 显示全部楼层
Water, Life, and Planetary Geodynamical Evolution,, as well as the presence of a magnetic field, are important factors contributing to the habitability of a planet. This chapter reviews these processes, their mutual interactions, and the role life plays in regulating or modulating them.
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978-1-4419-2553-4Springer-Verlag New York 2007
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