Skip to main navigation Skip to search Skip to main content

Long-term monitoring of comet 67P/Churyumov-Gerasimenko's jets with OSIRIS onboard Rosetta

  • M. I. Schmitt
  • , C. Tubiana
  • , C. Güttler
  • , H. Sierks
  • , J. B. Vincent
  • , M. R. El-Maarry
  • , D. Bodewits
  • , S. Mottola
  • , S. Fornasier
  • , M. Hofmann
  • , C. Barbieri
  • , P. L. Lamy
  • , R. Rodrigo
  • , D. Koschny
  • , H. Rickman
  • , M. F. A'Hearn
  • , J. Agarwal
  • , M. A. Barucci
  • , J. L. Bertaux
  • , I. Bertini
  • G. Cremonese, V. Da Deppo, B. Davidsson, S. Debei, M. De Cecco, J. Deller, M. Fulle, A. Gicquel, O. Groussin, P. J. Gutiérrez, S. F. Hviid, W. H. Ip, L. Jorda, H. U. Keller, J. Knollenberg, J. R. Kramm, E. Kührt, M. Küppers, L. M. Lara, M. Lazzarin, J. J. López-Moreno, F. Marzari, G. Naletto, N. Oklay, M. Pajola, D. Prasanna, X. Shi, F. Scholten, I. Toth, N. Thomas
  • Max-Planck Institut für Sonnensystemforschung
  • Georg-August University
  • Deutsches Zentrum für Luft- und Raumfahrt (DLR)
  • University of Maryland, College Park
  • LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
  • University of Padova
  • Université de la Méditerranée
  • Centro de Astrobiologia (INTA-CSIC)
  • International Space Science Institute
  • European Space Agency
  • Uppsala University
  • PAS Space Research Center
  • CNRS Centre National de la Recherche Scientifique
  • INAF Osservatorio Astronomico di Padova
  • CNR-IFN UOS Padova LUXOR
  • JPL
  • University of Trento
  • INAF - Osservatorio Astronomico di Trieste
  • Instituto de Astrofísica de Andalucía (CSIC)
  • National Central University
  • Macau University of Science and Technology
  • Technische Universität Braunschweig
  • European Space Astronomy Centre
  • NASA Ames Research Center
  • MTA CSFK Konkoly Observatory
  • University of Bern

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

We used the OSIRIS camera system onboard the Rosetta spacecraft to monitor jet activity of comet 67P/Churyumov-Gerasimenko. With a monthly cadence, we covered an epoch from 2014 December to 2015 October, thereby including the first equinox and the perihelion passage. Jet features were measured in individual images, which were used to perform a statistical inversion. The study provides maps for the locations of likeliest sources of jet activity on the comet's surface as a function of time. The sources follow the subsolar latitude, show clustering and a broadening of the activity band with time in the Northern hemisphere. In the Southern hemisphere, they are not clustered but show a broader spread over all longitudes which is either related to the north-south dichotomy of the comet's topography or due to a higher insolation during southern summer.

Original languageBritish English
Pages (from-to)S380-S385
JournalMonthly Notices of the Royal Astronomical Society
Volume469
DOIs
StatePublished - 2017

Keywords

  • Comets: individual: 67P/Churyumov
  • Gerasimenko

Fingerprint

Dive into the research topics of 'Long-term monitoring of comet 67P/Churyumov-Gerasimenko's jets with OSIRIS onboard Rosetta'. Together they form a unique fingerprint.

Cite this