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Titlebook: Mars: A Volcanic World; Giovanni Leone Book 2021 Springer Nature Switzerland AG 2021 Mars Exploration Program.Planetary Volcanology.Early

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書目名稱Mars: A Volcanic World
編輯Giovanni Leone
視頻videohttp://file.papertrans.cn/625/624858/624858.mp4
概述Is a first comprehensive summary of the formation of the Martian dichotomy.Provides interdisciplinary information about the volcanism of Mars.Contains information for the future of the exploration of
圖書封面Titlebook: Mars: A Volcanic World; Giovanni Leone Book 2021 Springer Nature Switzerland AG 2021 Mars Exploration Program.Planetary Volcanology.Early
描述.This book is a comprehensive advancement about the understanding of the volcanology of Mars in all its aspects, from its primary formation to its evolution in time, from the smaller structures to the bigger structures. It discusses the implications of volcanism in the general environmental and geological context of Mars. The book is validating the Southern Giant Impact Hypothesis explaining the formation of Mars in an interdisciplinary approach, including mineralogical, geochemical, volcanological as well as geomorphological information. Implications for future explorations in terms of resources are provided. This book serves as a textbook for undergraduate and graduate level to foster new basic research in the field of planetary volcanology and is a new guide for future missions toward a volcanic world, including new detailed information for the general audience who is always keen to know more about the history of Mars and its large volcanoes. The book also presents an updated situation about the water resources of the planet..
出版日期Book 2021
關(guān)鍵詞Mars Exploration Program; Planetary Volcanology; Early Noachian crust; Martian Meteorites; Porous-media
版次1
doihttps://doi.org/10.1007/978-3-030-84103-4
isbn_softcover978-3-030-84105-8
isbn_ebook978-3-030-84103-4
copyrightSpringer Nature Switzerland AG 2021
The information of publication is updating

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Volcanic Eruptions on Mars, Lava Flow Morphology, and Thermodynamics,se eruption processes, from plumbing systems, supply rates, and magma mineralogy can all affect the eruption style. Understanding these different types of eruption styles represents a distinct geophysical process on Mars that in some cases resemble volcanic systems of Earth. The similarities are in
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Volcanic Channels and Volcanic Features on Mars,ntially collapsed lava tubes. Many of these channels are a part of a typical igneous assemblage of landforms. In addition, some channels have an ambiguous origin, where a volcanic interpretation explains many of the observed features in some settings. This chapter describes volcanically formed sinuo
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Buried Volcano-Hydrothermal Systems and Minerals on Mars,tered olivines of any age since the Naochian. Nevertheless, iron sulphates at the surface suggest hydrothermal activity at some point in time and space, arguably at depth, from where minerals were expulsed by volcanic activity and/or “sweating out” during phases of heating upon meteorite impacts. Be
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Infrasound Propagation on Mars Atmosphere,carried out considering the real infrasonic records on Earth for long-range propagation (>100?km) and comparing with those would have been recorded for Martian atmosphere. As well known, infrasound propagates on Earth at ranges of hundreds or thousands kilometres mainly due to the combination of low
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