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Titlebook: Dynamic Planet; Mercury in the Conte Pamela Elizabeth Clark Book 2007 Springer-Verlag New York 2007 Clark.Dynamic.Environment.Geology.Inter

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書目名稱Dynamic Planet
副標(biāo)題Mercury in the Conte
編輯Pamela Elizabeth Clark
視頻videohttp://file.papertrans.cn/284/283701/283701.mp4
概述Views Mercury as a whole in the context of its environment, illustrating what we know and what we need to know and why understanding Mercury is so crucial to our understanding of solar system origin a
圖書封面Titlebook: Dynamic Planet; Mercury in the Conte Pamela Elizabeth Clark Book 2007 Springer-Verlag New York 2007 Clark.Dynamic.Environment.Geology.Inter
描述UNDERSTANDING THE PLANET MERCURY Thirty years have elapsed since the one and only mission to Mercury, Mariner 10, performed three ?ybys of the planet, capturing moderate-reso- tion (100 m at best) images of one hemisphere (45% of the surface) and d- covering that Mercury could be the only other terrestrial planet to have a global magnetic ?eld and core dynamo analogous to the Earth’s. At the time of this writing, the MESSENGER mission to Mercury has been launched. We are still a couple of years away from the ?rst of the next ?ybys of Mercury, by MESSENGER, on its way to insertion into a nearly polar, but highly ellip- cal, orbit, seven years from launch. In the interim, a plethora of ground-based observations has been providing information on hitherto unseen aspects of Mercury’s surface and exosphere. Furthermore, Mariner 10 data have been analyzed and reanalyzed as the technology for modeling and image processing has improved, leading to important breakthroughs in our understanding of Mercury and its environment. Thus, we are writing this book with the realization that we are in a time of transition in our understanding of the planet Mercury. Of particular interest to us in this b
出版日期Book 2007
關(guān)鍵詞Clark; Dynamic; Environment; Geology; Interior; Mercury; Planet; Solar; Solar System
版次1
doihttps://doi.org/10.1007/978-0-387-48214-9
isbn_softcover978-1-4419-2370-7
isbn_ebook978-0-387-48214-9
copyrightSpringer-Verlag New York 2007
The information of publication is updating

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,Mercury’ Exosphere,(the e-folding height for density). Because collisions are rare in an exosphere, each constituent maintains its own distribution, defined by its unique combination of source energy and distribution, mass, radiation pressure and loss processes (e.g. Jeans escape, photo-dissociation; adsorption; ioniz
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M. Stücker,T. Auer,K. Hoffmann,P. Altmeyer Solar System formation, evolution, and structure. Two of the most fundamental problems in planetary science, the formation of the solar system and the dynamo generation of magnetic fields in planetary interiors, can be addressed by studying Mercury‘s deep interior. Yet, Mercury is the terrestrial p
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Measurement of Microcirculation Mercury’s surface, including its physical and compositional nature, were, until recently, almost exclusively based on analyses of Mariner 10 data (.) (Strom and Sprague, 2003). Included in the Mariner 10 dataset are images covering most of one hemisphere with resolution no better than 100 meters an
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