Surface evolution of the Anhur region on comet 67P/Churyumov-Gerasimenko from high-resolution OSIRIS images - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2019

Surface evolution of the Anhur region on comet 67P/Churyumov-Gerasimenko from high-resolution OSIRIS images

Jean-Baptiste Vincent
  • Function : Author
  • PersonId : 992874
Philippe Lamy
Dennis Bodewits
  • Function : Author
  • PersonId : 991882
Gabriele Cremonese
  • Function : Author
  • PersonId : 1005814
Stefano Debei
  • Function : Author
  • PersonId : 1002201
Pedro J. Gutiérrez
  • Function : Author
  • PersonId : 880386
Laurent Jorda
Alice Lucchetti
  • Function : Author
  • PersonId : 1014663
Maurizio Pajola
  • Function : Author
  • PersonId : 1046343
I. Toth
  • Function : Author

Abstract

The southern hemisphere of comet 67P/Churyumov-Gerasimenko (67P) became observable by the Rosetta mission in March 2015, a few months before cometary southern vernal equinox. The Anhur region in the southern part of the comet’s larger lobe was found to be highly eroded, enriched in volatiles, and highly active. We analyze high-resolution images of the Anhur region pre- and post-perihelion acquired by the OSIRIS imaging system on board the Rosetta mission. The Narrow Angle Camera is particularly useful for studying the evolution in Anhur in terms of morphological changes and color variations. Radiance factor images processed by the OSIRIS pipeline were coregistered, reprojected onto the 3D shape model of the comet, and corrected for the illumination conditions. We find a number of morphological changes in the Anhur region that are related to formation of new scarps; removal of dust coatings; localized resurfacing in some areas, including boulders displacements; and vanishing structures, which implies localized mass loss that we estimate to be higher than 50 million kg. The strongest changes took place in and nearby the Anhur canyon-like structure, where significant dust cover was removed, an entire structure vanished, and many boulders were rearranged. All such changes are potentially associated with one of the most intense outbursts registered by Rosetta during its observations, which occurred one day before perihelion passage. Moreover, in the niche at the foot of a new observed scarp, we also see evidence of water ice exposure that persisted for at least six months. The abundance of water ice, evaluated from a linear mixing model, is relatively high (>20%). Our results confirm that the Anhur region is volatile-rich and probably is the area on 67P with the most pristine exposures near perihelion.
Fichier principal
Vignette du fichier
aa34824-18.pdf (25.86 Mo) Télécharger le fichier
Origin : Publisher files allowed on an open archive
Loading...

Dates and versions

insu-02114680 , version 1 (20-09-2019)

Identifiers

Cite

Sonia Fornasier, Clément Feller, Pedro H. Hasselmann, Maria Antonella Barucci, J. Sunshine, et al.. Surface evolution of the Anhur region on comet 67P/Churyumov-Gerasimenko from high-resolution OSIRIS images. Astronomy and Astrophysics - A&A, 2019, Rosetta mission full comet phase results, 630, pp.A13. ⟨10.1051/0004-6361/201834824⟩. ⟨insu-02114680⟩
235 View
67 Download

Altmetric

Share

Gmail Facebook X LinkedIn More