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Titlebook: Host Stars and their Effects on Exoplanet Atmospheres; An Introductory Over Jeffrey Linsky Book 20191st edition Springer Nature Switzerland

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发表于 2025-3-21 16:44:55 | 显示全部楼层 |阅读模式
书目名称Host Stars and their Effects on Exoplanet Atmospheres
副标题An Introductory Over
编辑Jeffrey Linsky
视频video
概述First topical primer for non-specialists in the field.Written by a leading expert in the field.Includes many figures and tables
丛书名称Lecture Notes in Physics
图书封面Titlebook: Host Stars and their Effects on Exoplanet Atmospheres; An Introductory Over Jeffrey Linsky Book 20191st edition Springer Nature Switzerland
描述.Like planets in our solar system, exoplanets form, evolve, and interact with their host stars in many ways. As exoplanets acquire material and grow to the final size, their atmospheres are subjected to intense UV and X-radiation and high-energy particle bombardment from the young host star. Whether a planet can retain its atmosphere and the conditions for significant mass loss both depend upon the strength of the host star‘s high-energy radiation and wind, the distance of the exoplanet from its host star, the gravitational potential of the exoplanet, and the initial  chemical composition of the exoplanet atmosphere... .This introductory overview describes the physical processes responsible for the emission of radiation and acceleration of winds of host stars that together control the environment of an exoplanet, focusing on topics that are critically important for understanding exoplanetary atmospheres but are usually not posed from the perspective of host stars. Accordingly, both host stars and exoplanets are not studied in isolation but are treated as integrated systems. Stellar magnetic fields, which are the energy source for activity phenomena including high-energy radiation a
出版日期Book 20191st edition
关键词Planetary atmospheres; Exoplanetary aeronomy; Stellar photochemistry; Star-planet interactions; Habitabl
版次1
doihttps://doi.org/10.1007/978-3-030-11452-7
isbn_softcover978-3-030-11451-0
isbn_ebook978-3-030-11452-7Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer Nature Switzerland AG 2019
The information of publication is updating

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Stellar Chromospheres: The Source of UV Emission,vection heat from below and the loss of radiation to space. With increasing height in a stellar atmosphere, magnetic heating processes become important in the energy balance, forcing the temperature to increase with height in a region called the chromosphere. Magnetic heating processes include the d
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Stellar Coronae: The Source of X-ray Emission, space. However, the hottest region of a star can be its outermost layer, the corona with temperatures of 10. K to 10. K or even hotter. The heating mechanism responsible for hot coronae has been debated since the existence of hot coronal gas was first identified in the early 1940s.
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Stellar Winds,r layers of exoplanet atmospheres producing charge-exchange and other reactions that facilitate mass loss. In this chapter, I describe the different types of winds observed in hot and cool stars. For some star types, it is relatively easy to measure diagnostics of mass loss but in solar type stars i
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Host Star Driven Exoplanet Mass Loss and Possible Surface Water,planet atmospheres. The main thermal process is hydrodynamical outflow driven by extreme ultraviolet and x-radiation from the host star that heat and inflate an exoplanet’s exosphere leading to mass loss. Non-thermal mass loss occurs when ions and electrons in the host star’s wind remove neutrals an
发表于 2025-3-23 01:50:32 | 显示全部楼层
Space Weather: The Effects of Host Star Flares on Exoplanets,s usually benign, exoplanets located close to their host stars, especially active M dwarfs, must suffer through powerful flares, stellar winds, CMEs, and very high energy radiation. The environment in which exoplanets must live is now called “stellar space weather” in analogy with the extensively mo
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