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Titlebook: Habitability of Other Planets and Satellites; Jean-Pierre de Vera,Joseph Seckbach Book 2013 Springer Science+Business Media Dordrecht 2013

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發(fā)表于 2025-3-21 19:24:37 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Habitability of Other Planets and Satellites
編輯Jean-Pierre de Vera,Joseph Seckbach
視頻videohttp://file.papertrans.cn/421/420381/420381.mp4
概述Dedicated chapter illustrating alternative life compared to our Earth-centric considerations.New mission concepts for remote studying of habitability of exo-planets.In situ investigations of the Polar
叢書(shū)名稱(chēng)Cellular Origin, Life in Extreme Habitats and Astrobiology
圖書(shū)封面Titlebook: Habitability of Other Planets and Satellites;  Jean-Pierre de Vera,Joseph Seckbach Book 2013 Springer Science+Business Media Dordrecht 2013
描述Is the Earth the right model and the only universal key to understand habitability, the origin and maintenance of life? Are we able to detect life elsewhere in the universe by the existing techniques and by the upcoming space missions? This book tries to give answers by focusing on environmental properties, which are playing a major role in influencing planetary surfaces or the interior of planets and satellites. The book gives insights into the nature of planets or satellites and their potential to harbor life. Different scientific disciplines are searching for the clues to classify planetary bodies as a habitable object and what kind of instruments and what kind of space exploration missions are necessary to detect life. Results from model calculations, field studies and from laboratory studies in planetary simulation facilities will help to elucidate if some of the planets and satellites in our solar system as well as in extra-solar systems are potentially habitable for life.
出版日期Book 2013
關(guān)鍵詞Astrobiology; Biosignatures; Exo-planets; Habitability; Solar System
版次1
doihttps://doi.org/10.1007/978-94-007-6546-7
isbn_softcover978-94-007-9216-6
isbn_ebook978-94-007-6546-7Series ISSN 1566-0400 Series E-ISSN 2215-0048
issn_series 1566-0400
copyrightSpringer Science+Business Media Dordrecht 2013
The information of publication is updating

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Your Majesty is Welcome to a Fair,ial velocity and transit surveys to planets at longer periods is fundamentally limited by the survey duration. Many of the radial velocity surveys are now pushing this detection threshold beyond orbital periods of 10 years and with upgraded instruments are sensitive to masses only a few times that of the Earth.
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發(fā)表于 2025-3-22 04:11:53 | 只看該作者
Exoplanets and Habitabilityial velocity and transit surveys to planets at longer periods is fundamentally limited by the survey duration. Many of the radial velocity surveys are now pushing this detection threshold beyond orbital periods of 10 years and with upgraded instruments are sensitive to masses only a few times that of the Earth.
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1566-0400 itability of exo-planets.In situ investigations of the PolarIs the Earth the right model and the only universal key to understand habitability, the origin and maintenance of life? Are we able to detect life elsewhere in the universe by the existing techniques and by the upcoming space missions? This
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The Habitable Zone and the Generalized Greenhouse Effect
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The Influence of UV Radiation on Exoplanets’ Habitability
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Organic Molecules in Lunar Ice: A Window to the Early Evolution of Life on Earth
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