7th Chianti Topics – Program

23th October

10:00| Registration
10:30| Welcome
11:00| G. Piccioni (invited)INAF, ItalyFrom hot to cold. The environment as “seen” by an imaging spectrometer: the example of Venus Express and the expectation for the JUICE mission to the icy worlds of Jupiter
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11:45| F. VitaliINAF, ItalyExperimental results on the H2- H2 and H2-He CIA in the [3600, 5500] cm-1 spectral range from 120 to 500 K and at typical Jupiter’s upper tropospheric conditions.
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12:05| G. TurchettiUniversità
Roma Tre, Italy
Assessing the performance of radar sounders
in the case of the Jovian moons

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12:25|F. FurnariINAF, Italy
Hexahydrite IR Reflectance Spectroscopy at typical Juipiter icy moons environmental conditions
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12:45| A. Brin
Università
Roma Tre, Italy
Laboratory investigation into dielectric properties of ice analogues for Europa ice shell

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13:05| Lunch Break

14:30|

N. Mangold (invited)

Nantes Université, France
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The growing diversity of past Mars aqueous environments


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15:15 |N. CostaUniversità
di Padova, Italy
Hyperspectral characterization of Martian simulant and water ice mixtures


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15:35| A. PiscopoUniversità
di Chieti, Italy
Analysis of layered deposits of arabia terra,
Mars: Example from a crater and surrounding plateau nearby Schiaparelli crater
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15:55| Coffee break

16:30|

F. Salese (invited)

Università
di Chieti, Italy
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The role of Space Architecture in Shaping Future Human Space Missions


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17:15| Open Debate
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20:00|Social DinnerRistorante il Bargello, Piazza Signoria 4/Red – Florence
GMaps Link

24th October

10:00 Visit of Museo Galileo (with audioguide)
13:00| Lunch Break

14:30| G.Caparelli (invited)
University of Southern Queensland, Australia MARSIS
results at the South Pole


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15:15| P. CianfarraUniversità
di Genova, Italy
Unravelling the tectonic setting of the linking zone between Claritas Fossae and Noctis
Labyrinthus (Mars) through the application of hierarchical-agglomerative clustering analysis
to lineament domains
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15:35 |G. W. SchmidtINAF, ItalyCategorizing the bulged topography of infilled craters on Mercury: Relationship of infill load response, global contraction and lava entry
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15:55|Coffee break

16:20|

D.Antonangeli (invited)

Sorbonne Université, France
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Phase diagrams and thermoelastic properties of planet-forming materials: a key to understanding planetary diversity
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17:00| V. FardellaINAF, Italy Understanding the planets composition from the Radial Velocity and
Transit Photometry measures
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17:20| Round Table
18:15|
End
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