Mercury's interior, surface, and surrounding environment latest discoveries / [electronic resource] :
- 作者： Clark, Pamela Elizabeth.
- 其他作者：
- 其他題名：
- SpringerBriefs in astronomy,
- 出版： New York, NY : Springer New York :Imprint: Springer
- 叢書名： SpringerBriefs in astronomy,
- 主題： Physics , Extraterrestrial Physics, Space Sciences. , Planetology. , Remote Sensing/Photogrammetry. , Mercury (Planet)--Geology. , Mercury (Planet)--Surface.
- ISBN： 9781493922444 (electronic bk.) 、 9781493922437 (paper)
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FIND@SFXID:
CGU
- 資料類型: 電子書
- 內容註: Messenger Mission -- Planetary Formation -- Terrestrial Planet Surface Processes -- Exosphere Dynamic -- Magnetosphere Dynamics -- Data Release Schedule Index.
- 摘要註: This SpringerBrief details the MESSENGER Mission, the findings of which present challenges to widely held conventional views and remaining mysteries surrounding the planet. The work answers the question of why Mercury is so dense, and the implications from geochemical data on its planetary formation. It summarizes imaging and compositional data from the terrestrial planet surface processes and explains the geologic history of Mercury. It also discusses the lack of southern hemisphere coverage. Our understanding of the planet Mercury has been in a transitional phase over the decades since Mariner 10. The influx of new data from the NASA MESSENGER Mission since it was inserted into the orbit of Mercury in March of 2011 has greatly accelerated that shift. The combined compositional data of relatively high volatiles (S, K), relatively low refractories (Al, Ca), and low crustal iron, combined with an active, partially molten iron rich core, has major implications for Mercury and Solar System formation. From a scientist at NASA Goddard Space Flight Center, this presents a comprehensive overview of the discoveries from the ten-year MESSENGER mission.
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讀者標籤：
- 系統號： 005132986 | 機讀編目格式
館藏資訊
This SpringerBrief details the MESSENGER Mission, the findings of which present challenges to widely held conventional views and remaining mysteries surrounding the planet. The work answers the question of why Mercury is so dense, and the implications from geochemical data on its planetary formation. It summarizes imaging and compositional data from the terrestrial planet surface processes and explains the geologic history of Mercury. It also discusses the lack of southern hemisphere coverage. Our understanding of the planet Mercury has been in a transitional phase over the decades since Mariner 10. The influx of new data from the NASA MESSENGER Mission since it was inserted into the orbit of Mercury in March of 2011 has greatly accelerated that shift. The combined compositional data of relatively high volatiles (S, K), relatively low refractories (Al, Ca), and low crustal iron, combined with an active, partially molten iron rich core, has major implications for Mercury and Solar System formation. From a scientist at NASA Goddard Space Flight Center, this presents a comprehensive overview of the discoveries from the ten-year MESSENGER mission.