Issue |
A&A
Volume 437, Number 3, July III 2005
|
|
---|---|---|
Page(s) | 1109 - 1113 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361:20052728 | |
Published online | 30 June 2005 |
Re-determination of Phoebe's orbit
1
National Time Service Center, The Chinese Academy of Science, PO Box 18, Lintong, Shaanxi 710600, PR China e-mail: shenkx@ntsc.ac.cn
2
United Laboratory for Optical Astrometry, The Chinese Academy of Science, PR China
3
Wellcome Trust Sanger Institute, Wellcome Trust Genome Campus, Hinxton, Cambridge CB10 1SA, UK
4
Observatoire Aquitain des Sciences de l'Univers, UMR 5804 Laboratoire d'Astrodynamique, d'Astrophysique et d'Aéronomie de Bordeaux (L3AB), 2 rue de l'Observatoire, 33270 Floirac, France
Received:
20
January
2005
Accepted:
10
March
2005
In order to improve the orbit of Phoebe, the ninth
satellite of the Saturnian system, 101 new observations were made
by our research team in 2003, using a CCD detector of large size
( pixels) mounted on the 1.56 m astrometric
reflector at the Sheshan Station of Shanghai Astronomical
Observatory. We fitted a numerical integration of its
orbit to all of the collected Earth-based astrometric
observations from 1904 to 2003, including the newest
precise data sets from Qiao & Tang and from
Peng et al. A new set of initial conditions of Phoebe has been
obtained, leading to an improved orbit of this
satellite.
Key words: gravitation / ephemerides / methods: numerical / reference systems / astrometry / time
© ESO, 2005
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.