Volume 420, Number 1, June II 2004
|Page(s)||389 - 395|
|Section||Planets and planetary systems|
|Published online||14 May 2004|
Dust production and coma morphology of 67P/Churyumov-Gerasimenko during the 2002/2003 apparition
II. A comparative study of dust production in 46P/Wirtanen and 67P/Churyumov-Gerasimenko during their 2002/2003 apparition
Instituto de Astrofísica de Canarias (IAC), C/vía Láctea, s/n, 38205 La Laguna, Tenerife, Spain
Corresponding author: email@example.com
Accepted: 12 March 2004
A comparison is made of the light curves and and dust production of the initial target for the ROSETTA mission, 46P/Wirtanen and the new target 67P/Churyumov-Gerasimenko during their recent 2002/2003 apparition. The study is based on amateur CCD monitoring using a standardised method to produce consistent photometry in Johnson-Kron-Cousins system. Although the dust production of the two comets is similar at perihelion (-cm), dust production in 46P/Wirtanen peaked before perihelion, while in 67P/Churyumov-Gerasimenko it peaks after perihelion. Dust activity shows the same post-perihelion dependence with heliocentric distance in both comets. Overall 67P/Churyumov-Gerasimenko has a dust production rate an order of magnitude greater at the same heliocentric distance post-perihelion as 46P/Wirtanen, but 46P/Wirtanen has greater maximum dust production immediately prior to perihelion.
Key words: comets: individual: 46P/Wirtanen, 67P/Churyumov-Gerasimenko / techniques: photometric / instrumentation: miscellaneous
© ESO, 2004
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