EDP Sciences
Free Access
Volume 422, Number 1, July IV 2004
Page(s) 357 - 368
Section Planets and planetary systems
DOI https://doi.org/10.1051/0004-6361:20035806
Published online 06 July 2004

A&A 422, 357-368 (2004)
DOI: 10.1051/0004-6361:20035806

The dust environment of comet 67P/Churyumov-Gerasimenko

M. Fulle1, C. Barbieri2, G. Cremonese3, H. Rauer4, M. Weiler4, G. Milani5 and R. Ligustri6

1  INAF - Osservatorio Astronomico di Trieste, Via Tiepolo 11, 34131 Trieste, Italy
2  Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
3  INAF - Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
4  Institute of Planetary Research, DLR Rutherfordstrasse 2, 12849 Berlin, Germany
5  Unione Astrofili Italiani, UAI
6  Osservatorio di Talmassons, CAST, Talmassons (Ud), Italy

(Received 4 December 2003 / Accepted 6 April 2004)

The new target of the ESA Rosetta Mission is comet 67P/Churyumov-Gerasimenko, which passed its last perihelion on 18 August 2002 and was well observed from fall 2002 to spring 2003. Its most prominent feature was a thin dust tail, which is best fitted by the Neck-Line model. Fits of the whole tail provide the dust environment of 67P during a year around perihelion; it shows a strong asymmetry between pre and post perihelion times. The dust mass loss rate appears constant since 2 AU before perihelion at about 200 kg s -1, a factor 100 higher than 46P/Wirtanen, the previous Rosetta target. Neck-Line photometry during 2002 and 2003 suggests that such a dust environment has remained similar since 3.6 AU before perihelion, i.e. the distance at which Rosetta science operations will start and the lander will be delivered to the surface.

Key words: space vehicles -- comets: general -- comets: individual: 67P/Churyumov-Gerasimenko

Offprint request: M. Fulle, fulle@ts.astro.it

© ESO 2004

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