Titlebook: Handbook of Exoplanets; Hans J. Deeg,Juan Antonio Belmonte Reference work 2018 Springer International Publishing AG, part of Springer Natu

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https://doi.org/10.1007/978-3-322-88600-2t the presence of extraterrestrial life. In turn, this perception affects the public support for the research infrastructure that is necessary to maintain the growth of the field of exoplanetology. Also, an interactive process between exoplanet science and the public through IAU’s NameExoWorlds Cont

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https://doi.org/10.1007/978-3-663-15739-7s (composition, optical properties) and of their variability in both space and time. Mars, Venus, and Titan exhibit a remarkable variety of clouds and aerosols. Our knowledge about them has made considerable progress thanks to the success of space missions during the last two decades, while in paral

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https://doi.org/10.1007/978-3-642-59392-5netary size, rotation, thermal stratification, and other factors in determining the styles of global circulation and dominant waves and instability processes. We discuss the importance of a number of key dimensionless parameters, for example, the thermal Rossby and the Burger numbers as well as nond

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Zeitgen?ssische Demokratietheorient. Understanding the relevant physics and chemistry provides insight to the past and future conditions of these objects, which is critical for understanding their evolution. This chapter introduces the basic concepts of upper atmospheres and ionospheres in our solar system and discusses aspects of

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dispensable reference in this area.Includes supplementary maThe Handbook of Exoplanets contains 15 sections dealing with all aspects of exoplanets and exobiology research, including historic aspects, the Solar System as a template, objects at the planet-to-star transition, exoplanet detection and ch

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https://doi.org/10.1007/978-3-642-51117-2f this review. In the second part, we discuss the formation scenario of the terrestrial planets, the atmospheric composition, and chemistry of Venus, the Earth, and Mars. The atmosphere of Titan is described in a third part, with special emphasis on its analogy with the early Earth and its exobiological implications.