Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength : Proceedings of the ESO/VUB Conference held in Brussels, Belgium, 7-10 August 2006. 1st ed. 2009

種類:

電子ブック

責任表示:

edited by Hans Ulrich Käufl, Christiaan Sterken

出版情報:

Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2009

著者名:

• Käufl, Hans Ulrich.
• Sterken, Christiaan.
• SpringerLink (Online service)

シリーズ名:

ESO Astrophysics Symposia, European Southern Observatory ;

ISBN:

9783540769590 [3540769595]    

注記:

The Deep Impact Event -- Previously Unobserved Water Lines Detected in the Post-Impact Spectrum -- Keck 1 HIRES Observations of Tempel 1 at the Time of Impact -- Deep Impact Groundsupport Observations of Comet 9P/Tempel 1: a Student Contribution -- Observations of Comet 9P/Tempel 1 and Deep Impact by the OSIRIS Cameras onboard Rosetta -- Comets, Charisma, and Celebrity: Reflections on Their Deep Impact -- The Grain Evolution Model for Icy Grains Ejected from 9P/Tempel 1 by Deep Impact -- JCMT Observations of the Deep Impact Event -- The Visual Brightness Behavior of Comet 9P/Tempel 1 During 1972–2005 -- Imaging Polarimetry of the Dust Coma of the Deep Impact Target Comet Tempel 1 -- Radio Observations from Australia of Comet 9P/Tempel 1 for Deep Impact -- The Deep Impact Event as Seen from the University of Nariñno Observatory – Colombia -- The Earth-Based Deep Impact Observing Program -- The Cometary Dust -- Gemini-N Observations of the Dust Excavated from Comet 9P/Tempel 1 During Deep Impact -- Release of C
In the context of the NASA Deep Impact space mission, comet 9P/Tempel1 has been at the focus of an unprecedented worldwide long-term multi-wavelength observation campaign. The comet was also studied throughout its perihelion passage by various sources including the Deep Impact mission itself, the Hubble Space Telescope, Spitzer, Rosetta, XMM and all major ground-based observatories in a wavelength band from cm-wave radio astronomy to x-rays. This book includes the proceedings of a meeting that brought together an audience of theoreticians and observers - across the electromagnetic spectrum and from different sites and projects - to make full use of the massive ground-based observing data set. The coherent presentation of all data sets illustrates and examines the various observational constraints on modelling the cometary nucleus, cometary gas, cometary plasma, cometary dust, and the comet's surface and its activity.

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