1982-1984 observations of Neried - New orbital determination

Details 1982-1984 observations of Neried - New orbital determination 1982-1984 observations of Neried - New orbital determination

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...189..303v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 189, no. 1-2, Jan. 1988, p. 303-305.

Astronomy and Astrophysics

Astrophysics

7

Natural Satellites, Neptune (Planet), Orbit Calculation, Orbital Elements, Eccentric Orbits, Kepler Laws, Least Squares Method, Orbit Perturbation

Scientific paper

11 new positions of Nereid are given from observations made in May 1982 and April 1984 on the Danish-ESO 1.5-m reflector, and in March 1982 on the CFH 3.6-m reflector. These accurate measurements permit an improved determination of the orbital elements. The Keplerian motion is no longer valid, and the available theory of a disturbed motion is a much better model of the observed motion. However, the residuals suggest that this theory is not sufficient with respect to the quality of the modern data.

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