Distant activity of 67P/Churyumov-Gerasimenko in 2014: Ground-based results during the Rosetta pre-landing phase

Colin Snodgrass, Emmanuel Jehin, Jean Manfroid, Cyrielle Opitom, Alan Fitzsimmons, Gian Paolo Tozzi, Sara Faggi, Bin Yang, Matthew M. Knight, Blair C. Conn, Tim Lister, Olivier Hainaut, D. M. Bramich, Stephen C. Lowry, Agata Rozek, Cecilia Tubiana, Aurélie Guilbert-Lepoutre

Research output: Contribution to journalArticle

19 Citations (Scopus)

Abstract

Context. As the ESA Rosetta mission approached, orbited, and sent a lander to comet 67P/Churyumov-Gerasimenko in 2014, a large campaign of ground-based observations also followed the comet. Aims. We constrain the total activity level of the comet by photometry and spectroscopy to place Rosetta results in context and to understand the large-scale structure of the comet's coma pre-perihelion. Methods. We performed observations using a number of telescopes, but concentrate on results from the 8 m VLT and Gemini South telescopes in Chile. We use R-band imaging to measure the dust coma contribution to the comet's brightness and UV-visible spectroscopy to search for gas emissions, primarily using VLT/FORS. In addition we imaged the comet in near-infrared wavelengths (JHK) in late 2014 with Gemini-S/Flamingos-2. Results. We find that the comet was already active in early 2014 at heliocentric distances beyond 4 au. The evolution of the total activity (measured by dust) followed previous predictions. No gas emissions were detected despite sensitive searches. Conclusions. The comet maintains a similar level of activity from orbit to orbit, and is in that sense predictable, meaning that Rosetta results correspond to typical behaviour for this comet. The gas production (for CN at least) is highly asymmetric with respect to perihelion, as our upper limits are below the measured production rates for similar distances post-perihelion in previous orbits.

Original languageEnglish
Article numberA80
JournalAstronomy and Astrophysics
Volume588
DOIs
Publication statusPublished - 1 Apr 2016
Externally publishedYes

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landing
comets
comet
coma
orbits
dust
spectroscopy
Rosetta mission
gases
telescopes
Chile
European Space Agency
gas
gas production
photometry
near infrared
brightness
wavelength
prediction
predictions

Keywords

  • Comets: individual: 67P/Churyumov-Gerasimenko

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Snodgrass, C., Jehin, E., Manfroid, J., Opitom, C., Fitzsimmons, A., Tozzi, G. P., ... Guilbert-Lepoutre, A. (2016). Distant activity of 67P/Churyumov-Gerasimenko in 2014: Ground-based results during the Rosetta pre-landing phase. Astronomy and Astrophysics, 588, [A80]. https://doi.org/10.1051/0004-6361/201527834

Distant activity of 67P/Churyumov-Gerasimenko in 2014 : Ground-based results during the Rosetta pre-landing phase. / Snodgrass, Colin; Jehin, Emmanuel; Manfroid, Jean; Opitom, Cyrielle; Fitzsimmons, Alan; Tozzi, Gian Paolo; Faggi, Sara; Yang, Bin; Knight, Matthew M.; Conn, Blair C.; Lister, Tim; Hainaut, Olivier; Bramich, D. M.; Lowry, Stephen C.; Rozek, Agata; Tubiana, Cecilia; Guilbert-Lepoutre, Aurélie.

In: Astronomy and Astrophysics, Vol. 588, A80, 01.04.2016.

Research output: Contribution to journalArticle

Snodgrass, C, Jehin, E, Manfroid, J, Opitom, C, Fitzsimmons, A, Tozzi, GP, Faggi, S, Yang, B, Knight, MM, Conn, BC, Lister, T, Hainaut, O, Bramich, DM, Lowry, SC, Rozek, A, Tubiana, C & Guilbert-Lepoutre, A 2016, 'Distant activity of 67P/Churyumov-Gerasimenko in 2014: Ground-based results during the Rosetta pre-landing phase', Astronomy and Astrophysics, vol. 588, A80. https://doi.org/10.1051/0004-6361/201527834
Snodgrass, Colin ; Jehin, Emmanuel ; Manfroid, Jean ; Opitom, Cyrielle ; Fitzsimmons, Alan ; Tozzi, Gian Paolo ; Faggi, Sara ; Yang, Bin ; Knight, Matthew M. ; Conn, Blair C. ; Lister, Tim ; Hainaut, Olivier ; Bramich, D. M. ; Lowry, Stephen C. ; Rozek, Agata ; Tubiana, Cecilia ; Guilbert-Lepoutre, Aurélie. / Distant activity of 67P/Churyumov-Gerasimenko in 2014 : Ground-based results during the Rosetta pre-landing phase. In: Astronomy and Astrophysics. 2016 ; Vol. 588.
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