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Titlebook: Formation and Evolution of Solids in Space; J. Mayo Greenberg,Aigen Li Book 1999 Springer Science+Business Media Dordrecht 1999 LOPES.Supe

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書目名稱Formation and Evolution of Solids in Space
編輯J. Mayo Greenberg,Aigen Li
視頻videohttp://file.papertrans.cn/347/346032/346032.mp4
叢書名稱Nato Science Series C:
圖書封面Titlebook: Formation and Evolution of Solids in Space;  J. Mayo Greenberg,Aigen Li Book 1999 Springer Science+Business Media Dordrecht 1999 LOPES.Supe
描述Interstellar dust, meteorites, interplanetary dust particles(IDP‘s), the zodiacal light, comets, comet dust. Where do they comefrom, what are they made of, how do they evolve, and finally, arethere connections between them? These are the questions discussed inthis volume by some of the world‘s outstanding experts in theirrespective fields. The techniques used for studying the `small‘ solidobjects of space are thoroughly discussed. Some of the methods involvea synthetic approach using the laboratory to create analogenvironments and materials which are believed to resemble those inspace. Others use direct laboratory methods with state-of-the-artanalytical tools to study the material of the objects themselves- meteorites, IDP‘S. And others apply the latest inastronomical facilities to provide quantitative data on the materialproperties of the solids which can only be deduced from remoteobservations, These are compared with the laboratory results. In oneinstance there was a possibility to study a solar system body in situand that was the case of comet Halley and some of the results of thesestudies obtained from space `laboratories‘ launched to meet it arediscussed here. Finally, there
出版日期Book 1999
關(guān)鍵詞LOPES; Supernova; astronomy; carbon; morphology; organic chemistry; planet; solar system; spectroscopy; stell
版次1
doihttps://doi.org/10.1007/978-94-011-4806-1
isbn_softcover978-94-010-6018-9
isbn_ebook978-94-011-4806-1Series ISSN 1389-2185
issn_series 1389-2185
copyrightSpringer Science+Business Media Dordrecht 1999
The information of publication is updating

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