AI Article Synopsis

  • Observations of comet nuclei show they're primarily made of a mixture of ice and durable materials, with high porosity and low bulk strength, though their properties are not fully understood.
  • By examining comet 67P/Churyumov-Gerasimenko's surface and modeling its layered structure, researchers suggest that its formation involved significant motion and deformation without severe damage.
  • The findings indicate that the comet's physical characteristics support the idea of an impact between two comet-like bodies, leading to extensive structural changes driven by both folding and cracking.

Article 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 (10-10 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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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC7229685PMC
http://dx.doi.org/10.1073/pnas.1914552117DOI Listing

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