The Rosetta/OSIRIS cameras unveiled the layered nature of comet 67P/Churyumov-Gerasimenko, suggesting that the comet bilobate shape results from the low-velocity merging of two independent onion-like objects. Several physiographical regions of the southern-hemisphere big lobe show stacks of layers forming high scarps, terraces and mesas. A spectrophotometric analysis of OSIRIS images based on multispectral data classifications was conducted in order to identify possible morphological, textural and/or compositional characters that allow to distinguish regional stacks of layers.

Comparison between layers stacks of 67P/CG comet and spectrophotometric variability obtained from OSIRIS data

Ferrari, S.;Penasa, L.;La Forgia, F.;Massironi, M.;Naletto, G.;Lazzarin, M.;Frattin, E.;Bertini, I.;Ferri, F.;
2017

Abstract

The Rosetta/OSIRIS cameras unveiled the layered nature of comet 67P/Churyumov-Gerasimenko, suggesting that the comet bilobate shape results from the low-velocity merging of two independent onion-like objects. Several physiographical regions of the southern-hemisphere big lobe show stacks of layers forming high scarps, terraces and mesas. A spectrophotometric analysis of OSIRIS images based on multispectral data classifications was conducted in order to identify possible morphological, textural and/or compositional characters that allow to distinguish regional stacks of layers.
2017
European Planetary Science Congress 2017
European Planetary Science Congress 2017
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/3247295
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