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Global-scale brittle plastic rheology at the cometesimals merging of comet 67P/Churyumov-Gerasimenko.
Franceschi, Marco; Penasa, Luca; Massironi, Matteo; Naletto, Giampiero; Ferrari, Sabrina; Fondriest, Michele; Bodewits, Dennis; Güttler, Carsten; Lucchetti, Alice; Mottola, Stefano; Pajola, Maurizio; Toth, Imre; Deller, Jacob; Sierks, Holger; Tubiana, Cecilia.
Afiliación
  • Franceschi M; Department of Mathematics and Geosciences, University of Trieste, 34128 Trieste, Italy; mfranceschi@units.it.
  • Penasa L; Department of Geosciences, University of Padova, 35131 Padova, Italy.
  • Massironi M; Center of Studies and Activities for Space "G. Colombo," University of Padova, 35131 Padova, Italy.
  • Naletto G; Department of Geosciences, University of Padova, 35131 Padova, Italy.
  • Ferrari S; Center of Studies and Activities for Space "G. Colombo," University of Padova, 35131 Padova, Italy.
  • Fondriest M; Department of Physics and Astronomy "Galileo Galilei," University of Padova, 35131 Padova, Italy.
  • Bodewits D; Center of Studies and Activities for Space "G. Colombo," University of Padova, 35131 Padova, Italy.
  • Güttler C; Consiglio Nazionale delle Ricerche - Istituto di Fotonica e Nanotecnologie Padova, 35131 Padova, Italy.
  • Lucchetti A; Center of Studies and Activities for Space "G. Colombo," University of Padova, 35131 Padova, Italy.
  • Mottola S; Department of Geosciences, University of Padova, 35131 Padova, Italy.
  • Pajola M; Physics Department, Auburn University, Leach Science Center, Auburn, AL 36849.
  • Toth I; Max Planck Institute for Solar System Research, 37077 Göttingen, Germany.
  • Deller J; Istituto Nazionale di Astrofisica, Astronomical Observatory of Padova, 35122 Padova, Italy.
  • Sierks H; Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt, 12489 Berlin, Germany.
  • Tubiana C; Istituto Nazionale di Astrofisica, Astronomical Observatory of Padova, 35122 Padova, Italy.
Proc Natl Acad Sci U S A ; 117(19): 10181-10187, 2020 05 12.
Article en En | MEDLINE | ID: mdl-32341151
ABSTRACT
Observations of comet nuclei indicate that the main constituent is a mix of ice and refractory materials characterized by high porosity (70-75%) and low bulk strength (10-4-10-6 MPa); however, the nature and physical properties of these materials remain largely unknown. By combining surface inspection of comet 67P/Churyumov-Gerasimenko and three-dimensional (3D) modeling of the independent concentric sets of layers that make up the structure of its two lobes, we provide clues about the large-scale rheological behavior of the nucleus and the kinematics of the impact that originated it. Large folds in the layered structure indicate that the merging of the two cometesimals involved reciprocal motion with dextral strike-slip kinematics that bent the layers in the contact area without obliterating them. Widespread long cracks and the evidence of relevant mass loss in absence of large density variations within the comet's body testify that large-scale deformation occurred in a brittle-plastic regime and was accommodated through folding and fracturing. Comparison of refined 3D geologic models of the lobes with triaxial ellipsoids that suitably represent the overall layers arrangement reveals characteristics that are consistent with an impact between two roughly ellipsoidal cometesimals that produced large-scale axial compression and transversal elongation. The observed features imply global transfer of impact-related shortening into transversal strain. These elements delineate a model for the global rheology of cometesimals that could be possible evoking a prominent bonding action of ice and, to a minor extent, organics.
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Texto completo: 1 Base de datos: MEDLINE Tipo de estudio: Prognostic_studies Idioma: En Revista: Proc Natl Acad Sci U S A Año: 2020 Tipo del documento: Article

Texto completo: 1 Base de datos: MEDLINE Tipo de estudio: Prognostic_studies Idioma: En Revista: Proc Natl Acad Sci U S A Año: 2020 Tipo del documento: Article