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The 67P/Churyumov- Gerasimenko observation campaign in support of the Rosetta mission

  • C. Snodgrass
  • , M. F. A'Hearn
  • , F. Aceituno
  • , V. Afanasiev
  • , S. Bagnulo
  • , J. Bauer
  • , G. Bergond
  • , S. Besse
  • , N. Biver
  • , D. Bodewits
  • , H. Boehnhardt
  • , B. P. Bonev
  • , G. Borisov
  • , B. Carry
  • , V. Casanova
  • , A. Cochran
  • , B. C. Conn
  • , B. Davidsson
  • , J. K. Davies
  • , J. De León
  • E. De Mooij, M. De Val-Borro, M. Delacruz, M. A. DiSanti, J. E. Drew, R. Duffard, N. J.T. Edberg, S. Faggi, L. Feaga, A. Fitzsimmons, H. Fujiwara, E. L. Gibb, M. Gillon, S. F. Green, A. Guijarro, A. Guilbert-Lepoutre, P. J. Gutiérrez, E. Hadamcik, O. Hainaut, S. Haque, R. Hedrosa, D. Hines, U. Hopp, F. Hoyo, D. Hutsemékers, M. Hyland, O. Ivanova, E. Jehin, G. H. Jones, J. V. Keane, M. S.P. Kelley, N. Kiselev, J. Kleyna, M. Kluge, M. M. Knight, R. Kokotanekova, D. Koschny, E. A. Kramer, J. J. López-Moreno, P. Lacerda, L. M. Lara, J. Lasue, H. J. Lehto, A. C. Levasseur-Regourd, J. Licandro, Z. Y. Lin, T. Lister, S. C. Lowry, A. Mainzer, J. Manfroid, J. Marchant, A. J. McKay, A. McNeill, K. J. Meech, M. Micheli, I. Mohammed, M. Monguió, F. Moreno, O. Muñoz, M. J. Mumma, P. Nikolov, C. Opitom, J. L. Ortiz, L. Paganini, M. Pajuelo, F. J. Pozuelos, S. Protopapa, T. Pursimo, B. Rajkumar, Y. Ramanjooloo, E. Ramos, C. Ries, A. Riffeser, V. Rosenbush, P. Rousselot, E. L. Ryan, P. Santos-Sanz, D. G. Schleicher, M. Schmidt, R. Schulz, A. K. Sen, A. Somero, A. Sota, A. Stinson, J. M. Sunshine, A. Thompson, G. P. Tozzi, C. Tubiana, G. L. Villanueva, X. Wang, D. H. Wooden, M. Yagi, B. Yang, B. Zaprudin, T. J. Zegmott
  • Open University
  • University of Maryland
  • Instituto de Astrofísica de Andalucía - CSIC
  • Special Astrophysical Observatory, Russian Academy of Sciences
  • Armagh Observatory
  • Jet Propulsion Laboratory
  • CSIC-MPG
  • European Space Astronomy Centre
  • LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
  • Max Planck Institute for Solar System Research
  • American University Washington DC
  • Institute of Astronomy and National Astronomical Observatory
  • Université Côte d'Azur
  • Sorbonne Université
  • University of Texas at Austin
  • Australian National University
  • Gemini ObservatorySouthern Operations Center
  • Royal Observatory
  • Instituto de Astrofísica de Canarias
  • University of La Laguna
  • Queens University Belfast
  • Princeton University
  • NASA Goddard Space Flight Center
  • Catholic University of America
  • Institute for Astronomy
  • University of Hertfordshire
  • Uppsala University
  • Osservatorio Astrofisico Di Arcetri, Florence
  • National Institutes of Natural Sciences - National Astronomical Observatory of Japan
  • University of Missouri-St. Louis
  • Université de Liège
  • CNRS
  • European Southern Observatory
  • The University of the West Indies
  • Space Telescope Science Institute
  • University Observatory
  • Slovak Academy of Sciences
  • University College London
  • University College London
  • Main Astronomical Observatory of National Academy of Sciences
  • European Space Agency
  • Université de Toulouse
  • University of Turku
  • National Central University
  • Las Cumbres Observatory Global Telescope Network, Inc.
  • University of Kent
  • Liverpool John Moores University
  • ESA SSA-NEO Coordination Centre
  • Caribbean Institute of Astronomy
  • Nordic Optical Telescope
  • SETI Institute
  • Lowell Observatory
  • Assam University
  • Yunnan Observatories
  • Chinese Academy of Sciences
  • NASA Ames Research Center

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

25 Citas (Scopus)

Resumen

We present a summary of the campaign of remote observations that supported the European Space Agency's Rosetta mission. Telescopes across the globe (and in space) followed comet 67P/Churyumov-Gerasimenko from before Rosetta's arrival until nearly the end of the mission in September 2016. These provided essential data for mission planning, large-scale context information for the coma and tails beyond the spacecraft and a way to directly compare 67P with other comets. The observations revealed 67P to be a relatively 'well-behaved' comet, typical of Jupiter family comets and with activity patterns that repeat from orbit to orbit. Comparison between this large collection of telescopic observations and the in situ results from Rosetta will allow us to better understand comet coma chemistry and structure. This work is just beginning as the mission ends-in this paper, we present a summary of the ground-based observations and early results, and point to many questions that will be addressed in future studies. This article is part of the themed issue 'Cometary science after Rosetta'.

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