Chapter 11

Application of Implicit 3D Modelling to Reconstruct the Layered Structure of the Comet 67P

Luca Penasa

Luca Penasa

University of Padova, Center of Studies and Activities for Space (CISAS) “G. Colombo,” Via Venezia 15, 35131, Padova, Italy

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Matteo Massironi

Matteo Massironi

University of Padova, Department of Geosciences, Via G. Gradenigo 6, 35131, Padova, Italy

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Emanuele Simioni

Emanuele Simioni

INAF, Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy

CNR-IFN UOS Padova LUXOR, Via Trasea 7, 35131, Padova, Italy

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Marco Franceschi

Marco Franceschi

University of Padova, Department of Geosciences, Via G. Gradenigo 6, 35131, Padova, Italy

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Giampiero Naletto

Giampiero Naletto

University of Padova, Center of Studies and Activities for Space (CISAS) “G. Colombo,” Via Venezia 15, 35131, Padova, Italy

CNR-IFN UOS Padova LUXOR, Via Trasea 7, 35131, Padova, Italy

University of Padova, Department of Physics and Astronomy “Galileo Galilei,” Via Marzolo 8, 35131, Padova, Italy

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Sabrina Ferrari

Sabrina Ferrari

University of Padova, Center of Studies and Activities for Space (CISAS) “G. Colombo,” Via Venezia 15, 35131, Padova, Italy

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Ivano Bertini

Ivano Bertini

University of Padova, Department of Physics and Astronomy “Galileo Galilei,” Via Marzolo 8, 35131, Padova, Italy

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Pamela Cambianica

Pamela Cambianica

INAF, Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy

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Elisa Frattin

Elisa Frattin

INAF, Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy

University of Padova, Department of Physics and Astronomy “Galileo Galilei,” Via Marzolo 8, 35131, Padova, Italy

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Fiorangela La Forgia

Fiorangela La Forgia

University of Padova, Department of Physics and Astronomy “Galileo Galilei,” Via Marzolo 8, 35131, Padova, Italy

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Alice Lucchetti

Alice Lucchetti

INAF, Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy

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Maurizio Pajola

Maurizio Pajola

INAF, Astronomical Observatory of Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy

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Frank Preusker

Frank Preusker

Deutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für Planetenforschung, Rutherfordstraße 23, 12489, Berlin, Germany

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Frank Scholten

Frank Scholten

Deutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für Planetenforschung, Rutherfordstraße 23, 12489, Berlin, Germany

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Laurent Jorda

Laurent Jorda

Laboratoire d'Astrophysique de Marseille, UMR 7326, CNRS & Aix Marseille Université, 13388, Marseille Cedex 13, France

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Robert Gaskell

Robert Gaskell

Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719, USA

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Holger Sierks

Holger Sierks

Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Göttingen, Germany

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First published: 01 April 2022

Summary

We provide details about the procedure employed for the three-dimensional geological modelling of the lobes of comet Churyumov-Gerasimenko (67P). The two lobes of 67P are characterized by well visible terraces and elongated cliffs that revealed a pervasive layering arranged in an onion-like fashion. None of the layers can be traced for a continuity large enough to provide a means of stratigraphic correlation. Therefore, an explicit modelling approach of the layered structure is not easily applicable. We show how a very simple modelling strategy based on implicitly-defined analytical surfaces (spheres or ellipsoids), and requiring very limited operator decision-making, can be successfully applied to produce a geological model that easily fits the available scattered attitude observations. Our formulation has the advantage of providing a small set of parameters with a precise geometrical meaning that can be compared with other parameters of the lobes (i.e. center of ellipsoids and center of mass). The presented method originates outside commercial geological modelling software packages and required devising some ad-hoc solutions for the visualization of the resulting models in comparison with observations made on OSIRIS images. Some extracts of the visualization code, helpful for applying this procedure in similar operational contexts, are also presented.

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