A&A 414, 749-755 (2004)
DOI: 10.1051/0004-6361:20031610
Optical observations of Comet 67P/Churyumov-Gerasimenko
M. Weiler1, H. Rauer1 and J. Helbert21 Institute of Planetary Research, DLR, Rutherfordstrasse 2, 12489 Berlin, Germany
2 Optical Information Systems and Space Sensor Technologies, DLR, Rutherfordstrasse 2, 12489 Berlin, Germany
(Received 5 August 2003 / Accepted 13 October 2003)
Abstract
From longslit spectra obtained during the 1996 perihelion
passage of Comet 67P/Churyumov-Gerasimenko, a CN production rate of
molecules
was
determined and an upper limit for the
production rate of
molecules
was derived. The dust color
and dust activity were determined from the continuum light in the
spectra. A neutral dust color was determined between 4070 Å and 4600 Å. The CN production rate and the Af
parameter,
determined to
cm, were similar to the values of
the 1982 perihelion passage, indicating that the comet's activity did
not change significantly in recent orbital passages. A first crude
estimate of the dust production rate indicates a high dust to gas mass
ratio.
Key words: comets: general -- comets: individual: 67P/Churyumov-Gerasimenko
Offprint request: M. Weiler, michael.weiler@dlr.de
© ESO 2004
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