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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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The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta

Fabrizio Capaccioni, +79 more
- 23 Jan 2015 - 
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

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.
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The planetary fourier spectrometer (PFS) onboard the European Venus Express mission

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.
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The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter

Oleg Korablev, +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.
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The Surface Composition and Temperature of Asteroid 21 Lutetia As Observed by Rosetta/VIRTIS

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.