Article Dans Une Revue Astronomy & Astrophysics - A&A Année : 2018

Tensile strength of 67P/Churyumov–Gerasimenko nucleus material from overhangs

1 LAM - Laboratoire d'Astrophysique de Marseille
2 Physikalisches Institut [Bern]
3 DLR Institut für Planetenforschung
4 MPS - Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research
5 Dipartimento di Fisica e Astronomia "Galileo Galilei"
6 PLANETO - LATMOS
7 CAB - Centro de Astrobiologia [Madrid]
8 ISSI - International Space Science Institute [Bern]
9 ESA - Agence Spatiale Européenne = European Space Agency
10 ESA Scientific Support Office
11 Department of Physics and Astronomy [Uppsala]
12 CBK - Space Research Centre of Polish Academy of Sciences
13 IGEP - Institut für Geophysik und Extraterrestrische Physik [Braunschweig]
14 Department of Astronomy [College Park]
15 LESIA (UMR_8109) - Laboratoire d'études spatiales et d'instrumentation en astrophysique
16 OAT - INAF - Osservatorio Astronomico di Trieste
17 LUXOR - Laboratory for Ultraviolet and X-ray Optical Research [Padova]
18 Department of Industrial Engineering [University of Padua]
19 UNITN - Università degli Studi di Trento = University of Trento
20 IAA-CSIC - Instituto de Astrofísica de Andalucía = Institute of Astrophysics of Andalusia
21 Institute of Space Science [Taiwan]
22 Operations Department (ESAC)
23 CAPS - Centre for Astrophysics and Planetary Science [Canterbury]
24 SSERVI - Solar System Exploration Research Virtual Institute
25 CISAS - Centro di Ateneo di Studi e Attività Spaziali “Giuseppe Colombo”
26 ARC - NASA Ames Research Center
27 Konkoly Observatory
David Nébouy
  • Fonction : Auteur
  • PersonId : 771139
  • IdRef : 219555427
Jean-Loup Bertaux
  • Fonction : Auteur
  • PersonId : 914210
Maurizio Pajola
I. Toth
  • Fonction : Auteur

Résumé

We directly measured twenty overhanging cliffs on the surface of comet 67P/Churyumov-Gerasimenko extracted from the latest shape model and estimated the minimum tensile strengths needed to support them against collapse under the comet's gravity. We find extremely low strengths of around 1 Pa or less (1 to 5 Pa, when scaled to a metre length). The presence of eroded material at the base of most overhangs, as well as the observed collapse of two features and the implied previous collapse of another, suggests that they are prone to failure and that the true material strengths are close to these lower limits (although we only consider static stresses and not dynamic stress from, for example, cometary activity). Thus, a tensile strength of a few pascals is a good approximation for the tensile strength of the 67P nucleus material, which is in agreement with previous work. We find no particular trends in overhang properties either with size over the ∼10-100 m range studied here or location on the nucleus. There are no obvious differences, in terms of strength, height or evidence of collapse, between the populations of overhangs on the two cometary lobes, suggesting that 67P is relatively homogenous in terms of tensile strength. Low material strengths are supportive of cometary formation as a primordial rubble pile or by collisional fragmentation of a small body (tens of km).

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Commentaire erratum https://doi.org/10.1051/0004-6361/201732155e published 06 June 2018
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hal-02108713 , version 1 (24-04-2019)

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Nicholas Attree, Olivier Groussin, Laurent Jorda, David Nébouy, Nicholas Thomas, et al.. Tensile strength of 67P/Churyumov–Gerasimenko nucleus material from overhangs. Astronomy & Astrophysics - A&A, 2018, 611, A33 (12p.). ⟨10.1051/0004-6361/201732155⟩. ⟨hal-02108713⟩
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