A comparison of the observation and ephemeris of Phoebe

Details A comparison of the observation and ephemeris of Phoebe A comparison of the observation and ephemeris of Phoebe

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...50..423b&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 50, Dec. 1982, p. 423-449. In French.

Astronomy and Astrophysics

Astrophysics

10

Phoebe, Planet Ephemerides, Astrometry, Geocentric Coordinates, Numerical Integration, Orbit Perturbation, Titan

Scientific paper

A total of 182 observations of Phoebe taken between the years 1904-81 were compared with its position as calculated by numerical integration. Account was made of perturbations caused by Saturn and by the presence of Titan, and an ephemeris was extrapolated out to 1990. An example is provided for use of the new ephemeris in order to obtain the astrometric geocentric equatorial coordinates at any point in time, as well as the distance from the earth.

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