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Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars
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Modelling the Upper Atmosphere of Gas-Giant Exoplanets Irradiated by Low-Mass Stars

Softcover reprint of the original 1st ed. 2017

Book Details

Format Paperback / Softback
Book Series Springer Theses
ISBN-10 3319875302
ISBN-13 9783319875309
Edition Softcover reprint of the original 1st ed. 2017
Publisher Springer International Publishing AG
Imprint Springer International Publishing AG
Country of Manufacture GB
Country of Publication GB
Publication Date Aug 11th, 2018
Print length 169 Pages
Ksh 8,100.00
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This PhD thesis details the development of a new 1D ionospheric model to describe the upper atmospheres of extrasolar giant plants. The composition and structure of these planets’ upper atmospheres are affected by high-energy emissions from the host star.
This PhD thesis details the development of a new 1D ionospheric model to describe the upper atmospheres of extrasolar giant plants. The upper atmospheres of Hot Jupiters are subject to extreme radiation conditions that can result in rapid atmospheric escape. The composition and structure of these planets’ upper atmospheres are affected by high-energy emissions from the host star. The nature of these emissions depends on the stellar type and age, making them important factors in understanding the behaviour of exoplanetary atmospheres. 

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