Saturn's position derived from meridian circle observations of Titan and Iapetus

Details Saturn's position derived from meridian circle observations of Titan and Iapetus Saturn's position derived from meridian circle observations of Titan and Iapetus

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...249..569t&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 249, no. 2, Sept. 1991, p. 569-573.

Astronomy and Astrophysics

Astrophysics

6

Celestial Mechanics, Iapetus, Planetary Orbits, Saturn (Planet), Titan, Astronomical Catalogs, Cassini Mission, Ephemeris Time, Orbital Elements, Saturn Satellites, Celestial Mechanics, Saturn Satellites, Meridian Observations, Orbit Improvement, Ephemeris Of Saturn

Scientific paper

Carlsberg and Bordeaux meridian circle observations of Titan and Iapetus made in the years 1987 to 1989 are analysed for corrections to their orbital elements and to the JPL Development Ephemeris, DE200, position of Saturn. The only significant correction to the elements is to the mean longitude of Iapetus. The corrections to the position of Saturn agree well with the latest ephemeris, DE202.

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