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Astrometric Reduction of Cassini ISS Images of Enceladus in 2015 Based on Gaia DR1

Published online by Cambridge University Press:  07 March 2018

Q. F. Zhang*
Affiliation:
Department of Computer Science, Jinan University, Guangzhou 510632, P.R. China
V. Lainey
Affiliation:
IMCCE, Observatoire de Paris, UMR 8028 du CNRS, UPMC, Université de Lille 1, 77 av. Denfert-Rochereau, 75014 Paris, France
A. Vienne
Affiliation:
IMCCE, Observatoire de Paris, UMR 8028 du CNRS, UPMC, Université de Lille 1, 77 av. Denfert-Rochereau, 75014 Paris, France
N. J. Cooper
Affiliation:
Astronomy Unit, School of Mathematical Sciences, Queen Mary University of London, Mile End Road, London E1 4NS, UK
Q. Y. Peng
Affiliation:
Department of Computer Science, Jinan University, Guangzhou 510632, P.R. China
N. Wang
Affiliation:
Department of Computer Science, Jinan University, Guangzhou 510632, P.R. China
*
*email: tqfz@jnu.edu.cn
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Abstract

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The Gaia DR1 catalogue stars are taken as reference ones to reduce the Cassini ISS images of Enceladus in 2015, and a total of 494 Cassini-centered astrometric observation are obtained in right ascension(α) and declination (δ) in the international Celestial Reference Frame(ICRF). Compared with JPL ephemerides SAT367, we derive that their mean residuals are a few tens meters in α*cos(δ) and a few kilometers in δ, and their standard deviation is not over 2 kilometers. Compared with the results from UCAC4 catalogue stars, The Gaia DR1 has the equivalent precision of reduction.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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