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Añadir al carritoCondición: Ottime. italiano Condizioni dell'esterno: Ottime Condizioni dell'interno: Ottime.
Librería: Gallix, Gif sur Yvette, Francia
EUR 34,00
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Añadir al carritoCondición: Neuf.
Idioma: Inglés
Publicado por LAP LAMBERT Academic Publishing, 2015
ISBN 10: 3659675970 ISBN 13: 9783659675973
Librería: Mispah books, Redhill, SURRE, Reino Unido
EUR 131,83
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Añadir al carritopaperback. Condición: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.
Idioma: Inglés
Publicado por LAP LAMBERT Academic Publishing, 2015
ISBN 10: 3659675970 ISBN 13: 9783659675973
Librería: moluna, Greven, Alemania
EUR 46,18
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Añadir al carritoCondición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: La Forgia FiorangelaI hold a PhD in Astronomy from the University of Padova in the field of physics of asteroids and comets from space missions.I am currently involved in the European Rosetta mission as an Associate Scientist for the.
Idioma: Inglés
Publicado por LAP LAMBERT Academic Publishing, 2015
ISBN 10: 3659675970 ISBN 13: 9783659675973
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 56,57
Cantidad disponible: 1 disponibles
Añadir al carritoTaschenbuch. Condición: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The European space mission Rosetta, during its 10 years journey to the comet 67P/Churyumov-Gerasimenko, on 10 July 2010 made an intermediate stop flying close to the asteroid 21 Lutetia and observed it from varying viewing angles, otherwise inaccessible from Earth. Less than four months later, on 4 November 2010, the NASA EPOXI mission offered another unexpected opportunity approaching the small hyperactive Jupiter-family comet 103P/Hartley 2, a few days after its perihelion passage. Those encounters provided an exceptional possibility for the advance in understanding our Solar System formation and history. Asteroids and comets are indeed the unique left samples of the primordial planetesimals that accreted in the original solar nebula. They are therefore key bodies for understanding the conditions and the processes occurred during the Solar System initial formation phases. The principal aim of this thesis is therefore to provide an advance in the small body science through the photometric analysis of high-resolution observations of the surface and the gas inner coma of an asteroid and a comet respectively, obtained by the mentioned two space missions.