Issue |
A&A
Volume 635, March 2020
|
|
---|---|---|
Article Number | A91 | |
Number of page(s) | 10 | |
Section | Celestial mechanics and astrometry | |
DOI | https://doi.org/10.1051/0004-6361/201937148 | |
Published online | 12 March 2020 |
Analytical representation for ephemeride with short time spans
Application to the longitude of Titan
1
National Time Service Centre (NTSC), Chinese Academy of Sciences, PO Box 18, Lintong, Shaanxi 710600, PR China
2
IMCCE, Observatoire de Paris, PSL Research University, CNRS, UPMC Univ. Paris 06, Paris, France
e-mail: Xiaojin.Xi@obspm.fr
3
Université de Lille, Observatoire de Lille, 59000 Lille, France
e-mail: alain.vienne@univ-lille.fr
Received:
20
November
2019
Accepted:
15
January
2020
Context. The ephemerides of natural satellites resulting from numerical integration have a very good precision on the fitting to recent observations, in a limited interval. Meanwhile, synthetic ephemerides like the Théorie Analytique des Satellites de Saturne (TASS) by Vienne and Duriez describe in detail the dynamical system by a representation based on the combinations of the proper frequencies. Some theoretical studies need to have both advantages. For example, to study the rotation of Titan, one needs to know the representation of its longitude.
Aims. We aim to use these two types of ephemerides in order to rebuild a long-lasting and high-precision ephemeris with proper frequencies based on the numerical integration ephemeris. The aim is to describe the numerical ephemerides with formulas similar to analytical ones.
Methods. We used the representation of the orbital elements from the TASS ephemeris analysed over 10 000 years as a reference template. We obtained the proper frequencies with both numerical and the TASS ephemeris over 1000 years only. A least-square procedure allowed us to get the analytical representation of an orbital element in this limited interval.
Results. We acquire the representation of the mean longitude of Titan from JPL ephemeris over 1000 years. For almost all components, the corresponding amplitudes and phases are similar to the relative terms from TASS. The biggest difference between our representation and the mean longitude of Titan of JPL is less than 100 km over 1000 years, and the standard deviation is about 26 km.
Key words: ephemerides / celestial mechanics / planets and satellites: individual: Titan / methods: numerical
© X. J. Xi and A. Vienne 2020
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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