Volume 408, Number 2, September III 2003
|Page(s)||767 - 774|
|Section||Planets and planetary systems|
|Published online||17 November 2003|
Dust production and coma morphology of 67P/Churyumov-Gerasimenko during the 2002–2003 apparition
Instituto de Astrofísica de Canarias (IAC), C/Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain
Corresponding author: firstname.lastname@example.org
Accepted: 17 June 2003
Light curves and images of 67P/Churyumov-Gerasimenko are presented for the 2002–2003 apparition based on amateur CCD monitoring using a standardised method to produce consistent photometry in Johnson-Kron-Cousins system. Multiaperture data shows a large outburst at perihelion during which dust production increased by a factor of 2 to give a peak value of cm. A similar outburst was seen at the same epoch of the previous apparition in 1995–96 and probably in 1982–83, suggesting that the light curve is similar at succesive returns. A considerable change is seen in the slope of the light curve at AU ( days) corresponding to a second significant increase in dust production. Overall though the dust production shows a very steep dependence with heliocentric distance, falling as r-5.8.
Key words: comets: individual: 67P/Churyumov-Gerasimenko / techniques: photometric
© ESO, 2003
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