Volume 365, Number 2, January 2001
|Page(s)||214 - 221|
|Section||Celestial mechanics and astrometry|
|Published online||15 January 2001|
Detection of arcs in Saturn's F ring during the 1995 Sun ring-plane crossing
Équipe Gamma-Gravitation, Service d'Astrophysique, CEA/Saclay, Orme des Merisiers, 91191 Gif-sur-Yvette Cedex, France
2 Institute for Astronomy, University of Hawai, 2680 Woodlawn Drive, Honolulu, Hawai 96822, Hawai
3 DESPA, Observatoire de Paris, 92195 Meudon Cedex Principal, France
Corresponding author: S. Charnoz, firstname.lastname@example.org
Accepted: 19 October 2000
Observations of the November 1995 Sun crossing of the Saturn's ring-plane made with the 3.6 m CFH telescope, using the UHAO adaptive optics system, are presented here. We report the detection of four arcs located in the vicinity of the F ring. They can be seen one day later in HST images. The combination of both data sets gives accurate determinations of their orbits. Semi-major axes range from 140 020 km to 140 080 km, with a mean of km. This is about 150 km smaller than previous estimates of the F ring radius from Voyager 1 and 2 data, but close to the orbit of another arc observed at the same epoch in HST images.
Key words: planets: individual: Saturn
© ESO, 2001
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