D
Davide Grassi
Researcher at INAF
Publications - 163
Citations - 4363
Davide Grassi is an academic researcher from INAF. The author has contributed to research in topics: Jupiter & Jovian. The author has an hindex of 32, co-authored 145 publications receiving 3615 citations. Previous affiliations of Davide Grassi include Paris Diderot University & University of Padua.
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Journal ArticleDOI
The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta
Fabrizio Capaccioni,Angioletta Coradini,Gianrico Filacchione,Stéphane Erard,Gabriele Arnold,Pierre Drossart,M. C. De Sanctis,D. Bockelee-Morvan,Maria Teresa Capria,Federico Tosi,C. Leyrat,Bernard Schmitt,Eric Quirico,Priscilla Cerroni,Vito Mennella,Andrea Raponi,Mauro Ciarniello,T. B. McCord,L. Moroz,Ernesto Palomba,Eleonora Ammannito,M. A. Barucci,Giancarlo Bellucci,Johannes Benkhoff,Jean-Pierre Bibring,Armando Blanco,M. I. Blecka,Robert W. Carlson,Uri Carsenty,Luigi Colangeli,M. Combes,Michael R. Combi,J. Crovisier,T. Encrenaz,Costanzo Federico,Uwe Fink,Sergio Fonti,Wing-Huen Ip,Patrick G. J. Irwin,Ralf Jaumann,Ralf Jaumann,E. Kuehrt,Yves Langevin,Gianfranco Magni,Stefano Mottola,Vincenzo Orofino,Pasquale Palumbo,Giuseppe Piccioni,Ulrich Schade,Fredric W. Taylor,D. Tiphene,G. P. Tozzi,Pierre Beck,N. Biver,Lydie Bonal,J. Ph. Combe,D. Despan,Enrico Flamini,Sonia Fornasier,Alessandro Frigeri,Davide Grassi,M. Gudipati,M. Gudipati,Andrea Longobardo,Kathrin Markus,F. Merlin,Roberto Orosei,Giovanna Rinaldi,Katrin Stephan,M. Cartacci,Andrea Cicchetti,S. Giuppi,Y. Hello,F. Henry,S. Jacquinod,Raffaella Noschese,G. Peter,Romolo Politi,J. M. Reess,A. Semery +79 more
TL;DR: The VIRTIS instrument on board the Rosetta spacecraft has provided evidence of carbon-bearing compounds on the nucleus of the comet 67P/Churyumov-Gerasimenko, and no ice-rich patches are observed, indicating a generally dehydrated nature for the surface currently illuminated by the Sun.
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Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft
Scott Bolton,Alberto Adriani,Virgil Adumitroaie,Matthew A. Allison,J. D. Anderson,Sushil K. Atreya,Jeremy Bloxham,Shannon Brown,John E. P. Connerney,E. DeJong,William M. Folkner,D. Gautier,Davide Grassi,Samuel Gulkis,Tristan Guillot,Candice Hansen,William B. Hubbard,Luciano Iess,Andrew P. Ingersoll,M. A. Janssen,John Leif Jørgensen,Yohai Kaspi,Steven Levin,Cheng Li,Jonathan I. Lunine,Yamila Miguel,Alessandro Mura,Glenn S. Orton,Tobias Owen,M. A. Ravine,Edward J. Smith,Paul G. Steffes,E. C. Stone,D. J. Stevenson,Richard M. Thorne,J. H. Waite,Daniele Durante,Robert Ebert,Thomas K. Greathouse,Vincent Hue,Marzia Parisi,Jamey Szalay,Robert W. Wilson +42 more
TL;DR: Juno’s first close pass over Jupiter provides answers and fresh questions about the giant planet, including images of weather in the polar regions and measurements of the magnetic and gravitational fields and microwaves to peer below the visible surface.
Journal ArticleDOI
The planetary fourier spectrometer (PFS) onboard the European Venus Express mission
Vittorio Formisano,Francesco Angrilli,Gabriele Arnold,Sushil K. Atreya,Kevin H. Baines,Giancarlo Bellucci,Bruno Bézard,F. Billebaud,D. Biondi,M. I. Blecka,Luigi Colangeli,Lorenzo Comolli,David Crisp,Mario D'Amore,T. Encrenaz,A. P. Ekonomov,Francesca Esposito,C. Fiorenza,Sergio Fonti,Marco Giuranna,Davide Grassi,B. Grieger,Anatoly I. Grigoriev,Jörn Helbert,H. Hirsch,Nikolay Ignatiev,A. Jurewicz,Igor Khatuntsev,Sébastien Lebonnois,Emmanuel Lellouch,A. Mattana,A. Maturilli,E. Mencarelli,M. Michalska,J. J. Lopez Moreno,B. E. Moshkin,F. Nespoli,Y. U. Nikolsky,F. Nuccilli,Piotr Orleanski,Ernesto Palomba,Giuseppe Piccioni,M. Rataj,Giovanna Rinaldi,M. Rossi,Bortolino Saggin,Daphne Stam,D.V. Titov,G. Visconti,L. V. Zasova +49 more
TL;DR: The planetary fourier spectrometer (PFS) as discussed by the authors was used for atmospheric studies on the mission of the Venus Express, which has a short wavelength (SW) channel that covers the spectral range from 1700 to 11400 cm−1 (0.9−5.5μm) and a long wavelength (LW) channel with a uniform spectral resolution of 1.3−3.3μm.
Journal ArticleDOI
The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter
Oleg Korablev,Franck Montmessin,Alexander Trokhimovskiy,Anna Fedorova,Alexey Shakun,Alexey Grigoriev,B. E. Moshkin,Nikolay Ignatiev,François Forget,Franck Lefèvre,Konstantin Anufreychik,I. Dzuban,Yurii S. Ivanov,Y. Kalinnikov,T. O. Kozlova,A. Kungurov,V. S. Makarov,F. Martynovich,Igor A. Maslov,D. Merzlyakov,P. Moiseev,Y. Nikolskiy,Andrey Patrakeev,D. Patsaev,A. Santos-Skripko,O. Sazonov,N. Semena,A. Semenov,Viktor Shashkin,A. Sidorov,Alexander V. Stepanov,I. Stupin,D. Timonin,A. Titov,Alexey I. Viktorov,A. V. Zharkov,Francesca Altieri,Gabriele Arnold,Denis Belyaev,Jean-Loup Bertaux,Daria Betsis,N. S. Duxbury,Thérèse Encrenaz,Thierry Fouchet,Jean-Claude Gérard,Davide Grassi,Sandrine Guerlet,Paul Hartogh,Yasumasa Kasaba,Igor Khatuntsev,Vladimir A. Krasnopolsky,Vladimir A. Krasnopolsky,Ruslan O. Kuzmin,Emmanuel Lellouch,Miguel Lopez-Valverde,Mikhail Luginin,Anni Määttänen,Emmanuel Marcq,J. Martín Torres,Alexander S. Medvedev,Ehouarn Millour,Kevin Olsen,Manish R. Patel,C. Quantin-Nataf,Alexander Rodin,Alexander Rodin,Valery I. Shematovich,Ian Thomas,N. Thomas,Luis Vázquez,Mathieu Vincendon,Valérie Wilquet,Colin Wilson,L. V. Zasova,Lev Zelenyi,María Paz Zorzano +75 more
TL;DR: The Atmospheric Chemistry Suite (ACS) as discussed by the authors is an element of the Russian contribution to the ESA-Roscosmos ExoMars 2016 Trace Gas Orbiter (TGO) mission.
Journal ArticleDOI
The Surface Composition and Temperature of Asteroid 21 Lutetia As Observed by Rosetta/VIRTIS
Angioletta Coradini,Fabrizio Capaccioni,Stéphane Erard,G. Arnold,M. C. De Sanctis,Gianrico Filacchione,Federico Tosi,M. A. Barucci,Maria Teresa Capria,Eleonora Ammannito,Davide Grassi,Giuseppe Piccioni,S. Giuppi,Giancarlo Bellucci,Johannes Benkhoff,Jean-Pierre Bibring,Armando Blanco,M. I. Blecka,D. Bockelee-Morvan,F. Carraro,R. W. Carlson,Uri Carsenty,Priscilla Cerroni,Luigi Colangeli,M. Combes,Michael R. Combi,J. Crovisier,Pierre Drossart,E. T. Encrenaz,Costanzo Federico,Uwe Fink,Sergio Fonti,Lorenza Giacomini,Wing-Huen Ip,Ralf Jaumann,E. Kuehrt,Yves Langevin,Gianfranco Magni,T. B. McCord,Vito Mennella,Stefano Mottola,G. Neukum,Vincenzo Orofino,Pasquale Palumbo,Ulrich Schade,Bernard Schmitt,Fredric W. Taylor,D. Tiphene,G. P. Tozzi +48 more
TL;DR: Lutetia is likely a remnant of the primordial planetesimal population, unaltered by differentiation processes and composed of chondritic materials of enstatitic or carbonaceous origin, dominated by iron-poor minerals that have not suffered aqueous alteration.