about
Detection of widespread hydrated materials on vesta by the Vir imaging spectrometer on board the dawn missionSpectroscopic characterization of mineralogy and its diversity across Vesta.Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres.Bright carbonate deposits as evidence of aqueous alteration on (1) Ceres.Distribution of phyllosilicates on the surface of Ceres.Localized aliphatic organic material on the surface of Ceres.Pitted terrains on (1) Ceres and implications for shallow subsurface volatile distribution.Variations in the amount of water ice on Ceres' surface suggest a seasonal water cycle.Nature, formation, and distribution of carbonates on Ceres.The surface composition of Ceres’ Ezinu quadrangle analyzed by the Dawn missionOlivine in an unexpected location on Vesta’s surfaceMineralogic mapping of the Av-9 Numisia quadrangle of VestaDantu's mineralogical properties - A view into the composition of Ceres' crustCeres's global and localized mineralogical composition determined by Dawn's Visible and Infrared Spectrometer (VIR)Mineralogy and temperature of crater Haulani on CeresRing-Mold Craters on Ceres: Evidence for Shallow Subsurface Water Ice SourcesMineralogy of Occator crater on Ceres and insight into its evolution from the properties of carbonates, phyllosilicates, and chloridesPhotometry of Ceres and Occator faculae as inferred from VIR/Dawn dataExposed H 2 O-rich areas detected on Ceres with the dawn visible and infrared mapping spectrometerGeologic constraints on the origin of red organic-rich material on CeresThe mineralogy of Ceres’ Nawish quadrangleThe spectral parameter maps of Ceres from NASA/DAWN VIR dataMineralogical analysis of the Ac-H-6 Haulani quadrangle of the dwarf planet CeresSpectral analysis of Ahuna Mons from Dawn mission's visible-infrared spectrometerAc-H-11 Sintana and Ac-H-12 Toharu quadrangles: Assessing the large and small scale heterogeneities of Ceres’ surfaceAn investigation of the bluish material on CeresCeres’ impact craters – relationships between surface composition and geologyCompositional differences among Bright Spots on the Ceres surfaceMineralogical analysis of quadrangle Ac-H-10 Rongo on the dwarf planet CeresMineralogical mapping of Coniraya quadrangle of the dwarf planet CeresMineralogical mapping of the Kerwan quadrangle on CeresMineralogy of the Occator quadrangleMineralogy of the Urvara–Yalode region on CeresSpectral investigation of quadrangle A C -H 3 of the dwarf planet Ceres – The region of impact crater DantuSpectrophotometric properties of dwarf planet Ceres from the VIR spectrometer on board the Dawn missionTesting linear spectral unmixing on laboratory mixtures: Application to VIR data for asteroid VestaThe unique geomorphology and structural geology of the Haulani crater of dwarf planet Ceres as revealed by geological mapping of equatorial quadrangle Ac-6 HaulaniThermal analysis of unusual local-scale features on the surface of VestaCryogenic flow features on Ceres: Implications for crater-related cryovolcanismDisk-resolved photometry of Vesta and Lutetia and comparison with other asteroids
P50
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P50
description
Italiaans onderzoeker
@nl
forsker
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researcher
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հետազոտող
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name
F. Zambon
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F. Zambon
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F. Zambon
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Francesca Zambon
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Francesca Zambon
@es
Francesca Zambon
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Francesca Zambon
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type
label
F. Zambon
@ast
F. Zambon
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F. Zambon
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Francesca Zambon
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Francesca Zambon
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Francesca Zambon
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Francesca Zambon
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F. Zambon
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prefLabel
F. Zambon
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F. Zambon
@nl
F. Zambon
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Francesca Zambon
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Francesca Zambon
@es
Francesca Zambon
@nb
Francesca Zambon
@sq
P106
P1153
55213469000
P27
P31
P496
0000-0002-4190-6592