Meter-scale thermal contraction crack polygons on the nucleus of comet 67P/Churyumov-Gerasimenko

Anne-Thérèse Auger 1, 2 Olivier Groussin 1 Laurent Jorda 3 Mohamed Ramy El-Maarry 4 Sylvain Bouley 2, 5 Antoine Séjourné 2 Robert Gaskell 6 Claire Capanna 1 Björn Davidsson 7 Simone Marchi 8 Sebastian Höfner 9 Philippe Lamy 1 Holger Sierks 9 Cesare Barbieri 10 Rafael Rodrigo 11, 12 Detlef Koschny 13 Hans Rickman 14, 7 Horst Uwe Keller 15 Jessica Agarwal 9 Michael F. A'Hearn 16 Maria Antonella Barucci 17 Jean-Loup Bertaux 18 Ivano Bertini 19 Gabriele Cremonese 20 Vania Da Deppo 21 Stefano Debei 20 Mariolino De Cecco 22 Sonia Fornasier 17 Marco Fulle 23 Pedro J. Gutierrez 24 Carsten Güttler 9 Stubbe Hviid 25 Wing-Huen Ip 26 Jörg Knollenberg 25 Jörg-Rainer Kramm 9 Ekkerhard Kührt 25 Michael Küppers 27 Luisa-Maria Lara 24 Monica Lazzarin 10 Josè J. Lopez-Moreno 24 Francesco Marzari 10 Matteo Massironi 19, 28 Harald Michalik 29 Giampiero Naletto 19, 21, 30 Nilda Oklay 25 Antoine Pommerol 4 Lola Sabau 31 Nicolas Thomas 4 Cécilia Tubiana 9 Jean-Baptiste Vincent 9 Klaus-Peter Wenzel 32
1 LAM - Laboratoire d'Astrophysique de Marseille
2 GEOPS - Géosciences Paris Sud
3 AMU - Aix Marseille Université
4 Physikalisches Institut [Bern]
5 IMCCE - Institut de Mécanique Céleste et de Calcul des Ephémérides
6 PSI - Planetary Science Institute [Tucson]
7 JPL - Jet Propulsion Laboratory
8 SSERVI - Solar System Exploration Research Virtual Institute
9 MPS - Max-Planck-Institut für Sonnensystemforschung
10 Dipartimento di Fisica e Astronomia "Galileo Galilei"
11 CAB - Centro de Astrobiologia [Madrid]
12 ISSI - International Space Science Institute
13 ESTEC - European Space Research and Technology Centre
14 CBK - Space Research Centre [Warsaw]
15 IGEP - Institut für Geophysik und Extraterrestrische Physik [Braunschweig]
16 Department of Astronomy [College Park]
17 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
18 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
19 CISAS - Centro di Ateneo di Studi e Attività Spaziali “Giuseppe Colombo”
20 Department of Industrial Engineering [Padova]
21 LUXOR - Laboratory for Ultraviolet and X-ray Optical Research [Padova]
22 University of Trento [Trento]
23 OAT - INAF - Osservatorio Astronomico di Trieste
24 IAA - Instituto de Astrofísica de Andalucía
25 DLR Institut für Planetenforschung
26 Institute of Space Science [Taiwan]
27 ESAC - European Space Astronomy Centre
28 OAPD - INAF - Osservatorio Astronomico di Padova
29 Institut für Datentechnik und Kommunikationsnetze
30 DEI - Department of Information Engineering [Padova]
31 INTA - Instituto Nacional de Técnica Aeroespacial
32 RSSD - Research and Scientific Support Department, ESTEC
Abstract : We report on the detection and characterization of more than 6300 polygons on the surface of the nucleus of comet 67P/Churyumov-Gerasimenko, using images acquired by the OSIRIS camera onboard Rosetta between August 2014 and March 2015. They are found in consolidated terrains and grouped in localized networks. They are present at all latitudes (from North to South) and longitudes (head, neck, and body), sometimes on pit walls or following lineaments. About 1.5% of the observed surface is covered by polygons. Polygons have an homogeneous size across the nucleus, with 90% of them in the size range 1 – 5 m and a mean size of 3.0 ± 1.4 m. They show different morphologies, depending on the width and depth of their trough. They are found in networks with 3- or 4-crack intersection nodes. The polygons observed on 67P are consistent with thermal contraction crack polygons formed by the diurnal or seasonal temperature variations in a hard (MPa) and consolidated sintered layer of water ice, located a few centimeters below the surface. Our thermal analysis shows an evolution of thermal contraction crack polygons according to the local thermal environment, with more evolved polygons (i.e. deeper and larger troughs) where the temperature and the diurnal and seasonal temperature range are the highest. Thermal contraction crack polygons are young surface morphologies that probably formed after the injection of 67P in the inner solar system, typically 100 000 years ago, and could be as young as a few orbital periods, following the decreasing of its perihelion distance in 1959 from 2.7 to 1.3 a.u. Meter scale thermal contraction crack polygons should be common features on the nucleus of Jupiter family comets.
Keywords : Geological processes Nucleus Comets
Type de document :
Article dans une revue
Icarus, Elsevier, 2018, 301, pp.173-188. 〈10.1016/j.icarus.2017.09.037〉
Liste complète des métadonnées
https://hal-insu.archives-ouvertes.fr/insu-01610197
Contributeur : Catherine Cardon <>
Soumis le : mercredi 4 octobre 2017 - 15:22:07
Dernière modification le : vendredi 16 novembre 2018 - 02:20:28

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INSU | OBSPM | LATMOS | OSU-INSTITUT-PYTHEAS | LAM | IMCCE | UNIV-AMU | GEOPS | PSL | LESIA | UPMC | UVSQ | USPC | UNIV-PARIS-SACLAY | SORBONNE-UNIVERSITE

Citation

Anne-Thérèse Auger, Olivier Groussin, Laurent Jorda, Mohamed Ramy El-Maarry, Sylvain Bouley, et al.. Meter-scale thermal contraction crack polygons on the nucleus of comet 67P/Churyumov-Gerasimenko. Icarus, Elsevier, 2018, 301, pp.173-188. 〈10.1016/j.icarus.2017.09.037〉. 〈insu-01610197〉

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