activity
20092024
most citedAmmonium salts are a reservoir of nitrogen on a cometary nucleus and possibly on some asteroids

180 citations · 784 across the 26 of their papers we have counts for

collaborators

27 papers

astro-ph.EP2024★ 4 cited

No evidence of magma ocean on Io based on Juno/JIRAM data

Federico Tosi, Alessandro Mura, Francesca Zambon

A recent paper (ref. 1) used infrared images of Io acquired by the Juno/JIRAM instrument to derive a latitudinal dependence of the spectral radiance and conclude that such latitudi…

astro-ph.EP2024

Widespread occurrence of lava lakes on Io observed from Juno

Alessandro Mura, Federico Tosi, Francesca Zambon +13

We report recent observations of lava lakes within patera on Io made by the JIRAM imager/spectrometer on board the Juno spacecraft, taken during close observation occurred in the e…

astro-ph.EP2024

Observations of Loki Patera by Juno during close flybys

Alessandro Mura, JIRAM-Io team

We used data from the Juno spacecraft to investigate both the spatial and temporal properties of Loki Patera on Io, acquired in two infrared bands between December 2022 and April 2…

astro-ph.EP2024★ 11 cited

A patchy CO exosphere on Ganymede revealed by the James Webb Space Telescope

Dominique Bockelée-Morvan, Olivier Poch, Françcois Leblanc +25

Jupiter's icy moon Ganymede has a tenuous exosphere produced by sputtering and possibly sublimation of water ice. To date, only atomic hydrogen and oxygen have been directly detect…

astro-ph.IM2024★ 14 cited

Calibration of MAJIS (Moons And Jupiter Imaging Spectrometer): III. Spectral Calibration

Paolo Haffoud, François Poulet, Mathieu Vincendon +13

The Moons And Jupiter Imaging Spectrometer (MAJIS) is the visible and near-infrared imaging spectrometer onboard ESA s Jupiter Icy Moons Explorer (JUICE) mission. Before its integr…

astro-ph.EP2023★ 1 cited

Identification of Ammonium Salts on Comet 67P/C-G Surface from Infrared VIRTIS/Rosetta Data Based on Laboratory Experiments. Implications and Perspectives

Olivier Poch, Istiqomah Istiqomah, Eric Quirico +29

The nucleus of comet 67P/Churyumov-Gerasimenko exhibits a broad spectral reflectance feature around 3.2 m, which is omnipresent in all spectra of the surface, and whose attribut…

astro-ph.EP2021★ 3 cited

The surface of (4) Vesta in visible light as seen by Dawn/VIR

B. Rousseau, M. C. De Sanctis, A. Raponi +9

We analyzed the surface of Vesta at visible wavelengths, using the data of the Visible and InfraRed mapping spectrometer (VIR) on board the Dawn spacecraft. We mapped the variation…

astro-ph.EP2021

The science case for spacecraft exploration of the Uranian satellites: Candidate ocean worlds in an ice giant system

Richard J. Cartwright, Chloe B. Beddingfield, Tom A. Nordheim +15

The 27 satellites of Uranus are enigmatic, with dark surfaces coated by material that could be rich in organics. Voyager 2 imaged the southern hemispheres of Uranus' five largest '…

astro-ph.EP2020★ 4 cited

Correction of the VIR-visible data set from the Dawn mission at Vesta

B. Rousseau, M. C De Sanctis, A. Raponi +7

This work describes the correction method applied to the dataset acquired at the asteroid (4) Vesta by the visible channel of the visible and infrared mapping spectrometer. The ris…

astro-ph.EP2020★ 12 cited

The surface of (1) Ceres in visible light as seen by Dawn/VIR

B. Rousseau, M. C. De Sanctis, A. Raponi +9

We study the surface of Ceres at visible wavelengths, as observed by the Visible and InfraRed mapping spectrometer (VIR) onboard the Dawn spacecraft, and analyze the variations of…

astro-ph.EP2020★ 64 cited

Infrared detection of aliphatic organics on a cometary nucleus

A. Raponi, M. Ciarniello, F. Capaccioni +28

The ESA Rosetta mission has acquired unprecedented measurements of comet 67/P-Churyumov-Gerasimenko (hereafter 67P) nucleus surface, whose composition, as determined by in situ and…

astro-ph.IM2020

The Science Case for Spacecraft Exploration of the Uranian Satellites

Richard J. Cartwright, Chloe B. Beddingfield, Tom Nordheim +14

The five classical Uranian moons are possible ocean worlds that exhibit bizarre geologic landforms, hinting at recent surface-interior communication. However, Uranus' classical moo…

astro-ph.EP2020★ 180 cited

Ammonium salts are a reservoir of nitrogen on a cometary nucleus and possibly on some asteroids

O. Poch, I. Istiqomah, E. Quirico +29

The measured nitrogen-to-carbon ratio in comets is lower than for the Sun, a discrepancy which could be alleviated if there is an unknown reservoir of nitrogen in comets. The nucle…

astro-ph.IM2019★ 12 cited

Correction of the VIR-Visible data set from the Dawn mission

B. Rousseau, A. Raponi, M. Ciarniello +6

Data acquired at Ceres by the visible channel of the Visible and InfraRed mapping spectrometer (VIR) on board the NASA Dawn spacecraft are affected by the temperatures of both the…

astro-ph.IM2019★ 6 cited

GAUSS -- A Sample Return Mission to Ceres

Xian Shi, Julie Castillo-Rogez, Henry Hsieh +26

The goal of Project GAUSS is to return samples from the dwarf planet Ceres. Ceres is the most accessible ocean world candidate and the largest reservoir of water in the inner solar…

astro-ph.EP2019★ 3 cited

Ice Giant Systems: The Scientific Potential of Orbital Missions to Uranus and Neptune

Leigh N. Fletcher, Ravit Helled, Elias Roussos +27

Uranus and Neptune, and their diverse satellite and ring systems, represent the least explored environments of our Solar System, and yet may provide the archetype for the most comm…

astro-ph.EP2018

Solar System Ice Giants: Exoplanets in our Backyard

Abigail Rymer, Kathleen Mandt, Dana Hurley +110

Future remote sensing of exoplanets will be enhanced by a thorough investigation of our solar system Ice Giants (Neptune-size planets). What can the configuration of the magnetic f…

astro-ph.EP2017★ 35 cited

Laboratory simulations of the Vis-NIR spectra of comet 67P using sub-μm sized cosmochemical analogues

Batiste Rousseau, Stéphane Érard, Pierre Beck +15

Laboratory spectral measurements of relevant analogue materials were performed in the framework of the Rosetta mission in order to explain the surface spectral properties of comet…

astro-ph.EP2016★ 39 cited

The temporal evolution of exposed water ice-rich areas on the surface of 67P/Churyumov-Gerasimenko: spectral analysis

A. Raponi, M. Ciarniello, F. Capaccioni +16

Water ice-rich patches have been detected on the surface of comet 67P/Churyumov-Gerasimenko by the VIRTIS hyperspectral imager on-board the Rosetta spacecraft, since the orbital in…

astro-ph.EP2016★ 45 cited

Detection of exposed HO ice on the nucleus of comet 67P/Churyumov-Gerasimenko

M. A. Barucci, G. Filacchione, S. Fornasier +42

Since the orbital insertion of the Rosetta spacecraft, comet 67P/Churyumov-Gerasimenko (67P/C-G) has been mapped by OSIRIS camera and VIRTIS spectro-imager, producing a huge quanti…

astro-ph.EP2016★ 76 cited

Spectrophotometric properties of dwarf planet Ceres from the VIR spectrometer on board the Dawn mission

M. Ciarniello, M. C. De Sanctis, E. Ammannito +14

We study the spectrophotometric properties of dwarf planet Ceres in the VIS-IR spectral range by means of hyper-spectral images acquired by the VIR imaging spectrometer on board th…

astro-ph.EP2016★ 71 cited

The global surface composition of 67P/CG nucleus by Rosetta/VIRTIS. I) Prelanding mission phase

Gianrico Filacchione, Fabrizio Capaccioni, Mauro Ciarniello +27

From August to November 2014 the Rosetta orbiter has performed an extensive observation campaign aimed at the characterization of 67P/CG nucleus properties and to the selection of…

astro-ph.EP2015★ 17 cited

Dielectric Properties of Vesta's Surface as Constrained by Dawn VIR Observations

Elizabeth M. Palmer, Essam Heggy, Maria Teresa Capria +1

Earth and orbital-based radar observations of asteroids provide a unique opportunity to characterize surface roughness and the dielectric properties of their surfaces, as well as p…

astro-ph.EP2013★ 33 cited

The radial distribution of water ice and chromophores across Saturn's system

G. Filacchione, F. Capaccioni, R. N. Clark +11

Over the last eight years, the Visual and Infrared Mapping Spectrometer (VIMS) aboard the Cassini orbiter has returned hyperspectral images in the 0.35-5.1 micron range of the icy…