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Titlebook: Characterizing Stellar and Exoplanetary Environments; Helmut Lammer,Maxim Khodachenko Book 2015 The Editor(s) (if applicable) and The Auth

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書(shū)目名稱(chēng)Characterizing Stellar and Exoplanetary Environments
編輯Helmut Lammer,Maxim Khodachenko
視頻videohttp://file.papertrans.cn/225/224035/224035.mp4
概述Presents studies of exoplanets under extreme stellar radiation and plasma conditions.Analyzes findings from Hubble Space Telescope observations of transiting exoplanets.Presents applications of advanc
叢書(shū)名稱(chēng)Astrophysics and Space Science Library
圖書(shū)封面Titlebook: Characterizing Stellar and Exoplanetary Environments;  Helmut Lammer,Maxim Khodachenko Book 2015 The Editor(s) (if applicable) and The Auth
描述.In this book an international group of specialists discusses studies of exoplanets subjected to extreme stellar radiation and plasma conditions. It is shown that such studies will help us to understand how terrestrial planets and their atmospheres, including the early Venus, Earth and Mars, evolved during the host star’s active early phase. The book presents an analysis of findings from Hubble Space Telescope observations of transiting exoplanets, as well as applications of advanced numerical models for characterizing the upper atmosphere structure and stellar environments of exoplanets. The authors also address detections of atoms and molecules in the atmosphere of “hot Jupiters” by NASA’s Spitzer telescope. The observational and theoretical investigations and discoveries presented are both timely and important in the context of the next generation of space telescopes..The book is divided into four main parts, grouping chapters on exoplanet host star radiation and plasma environments, exoplanet upper atmosphere and environment observations, exoplanet and stellar magnetospheres, and exoplanet observation and characterization. The book closes with an outlook on the future of this r
出版日期Book 2015
關(guān)鍵詞CoRoT Space Observatory; Exoplanet Atmospheres; Exoplanet Environment; Exoplanet Observations; Exoplanet
版次1
doihttps://doi.org/10.1007/978-3-319-09749-7
isbn_softcover978-3-319-37936-4
isbn_ebook978-3-319-09749-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightThe Editor(s) (if applicable) and The Author(s) 2015
The information of publication is updating

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Exoplanet Host Star Radiation and Plasma Environmenttmosphere depends on the evolution of its host star. We summarize the available techniques for measuring or estimating the X-ray, EUV, and UV radiation of host stars with different spectral types and ages.
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Stellar Driven Evolution of Hydrogen-Dominated Atmospheres from Earth-Like to Super-Earth-Type Exoplicant importance for planets with relatively weak Jeans-type escape or heavier particles (e.g., O, C, N). From the diversity of non-thermal escape mechanisms, in the present chapter we focus on ion pick-up and discuss the importance of other loss mechanisms. The general conclusion of the chapter is,
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0067-0057 vironments, exoplanet upper atmosphere and environment observations, exoplanet and stellar magnetospheres, and exoplanet observation and characterization. The book closes with an outlook on the future of this r978-3-319-37936-4978-3-319-09749-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
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