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Temporal morphological changes in the Imhotep region of comet 67P/Churyumov-Gerasimenko

  • O. Groussin
  • , H. Sierks
  • , C. Barbieri
  • , P. Lamy
  • , R. Rodrigo
  • , D. Koschny
  • , H. Rickman
  • , H. U. Keller
  • , M. F. A'Hearn
  • , A. T. Auger
  • , M. A. Barucci
  • , J. L. Bertaux
  • , I. Bertini
  • , S. Besse
  • , G. Cremonese
  • , V. Da Deppo
  • , B. Davidsson
  • , S. Debei
  • , M. De Cecco
  • , M. R. El-Maarry
  • S. Fornasier, M. Fulle, P. J. Gutiérrez, C. Güttler, S. Hviid, W. H. Ip, L. Jorda, J. Knollenberg, G. Kovacs, J. R. Kramm, E. Kührt, M. Küppers, L. M. Lara, M. Lazzarin, J. J. Lopez Moreno, S. Lowry, S. Marchi, F. Marzari, M. Massironi, S. Mottola, G. Naletto, N. Oklay, M. Pajola, A. Pommerol, N. Thomas, I. Toth, C. Tubiana, J. B. Vincent
  • Aix-Marseille Université
  • Max-Planck Institut für Sonnensystemforschung
  • University of Padova
  • Centro de Astrobiologia (INTA-CSIC)
  • International Space Science Institute
  • European Space Agency
  • Uppsala University
  • PAS Space Research Center
  • Deutsches Zentrum für Luft- und Raumfahrt (DLR)
  • Technische Universität Braunschweig
  • University of Maryland, College Park
  • Universite Paris Sud
  • LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
  • CNRS Centre National de la Recherche Scientifique
  • CNR-IFN UOS Padova LUXOR
  • University of Trento
  • INAF - Osservatorio Astronomico di Trieste
  • Instituto de Astrofísica de Andalucía (CSIC)
  • National Central University
  • European Space Astronomy Centre
  • University of Kent
  • Southwest Research Institute
  • INAF Osservatorio Astronomico di Padova
  • University of Bern
  • MTA CSFK Konkoly Observatory

Research output: Contribution to journalArticlepeer-review

70 Scopus citations

Abstract

Aims. We report on the first major temporal morphological changes observed on the surface of the nucleus of comet 67P/Churyumov-Gerasimenko in the smooth terrains of the Imhotep region. Methods. We used images of the OSIRIS cameras onboard Rosetta to follow the temporal changes from 24 May 2015 to 11 July 2015. Results. The morphological changes observed on the surface are visible in the form of roundish features that are growing in size from a given location in a preferential direction at a rate of 5.6-8.1 × 10-5 m s-1 during the observational period. The location where the changes started and the contours of the expanding features are bluer than the surroundings, which suggests that ices (H2O and/or CO2) are exposed on the surface. However, sublimation of ices alone is not sufficient to explain the observed expanding features. No significant variations in the dust activity pattern are observed during the period of changes.

Original languageBritish English
Article numberA36
JournalAstronomy and Astrophysics
Volume583
DOIs
StatePublished - 1 Nov 2015

Keywords

  • Comets: general
  • Comets: individual: 67P/Churyumov-Gerasimenko
  • Methods: data analysis

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