Astron. Astrophys. Suppl. Ser. 136, 445-451
C.H. Veiga1, R. Vieira Martins1, and Cl. Le Guyader2
1 - Observatório Nacional, Rua Gal. José Cristino 77,
20921-400 Rio de Janeiro, Brazil
e-mail: cave@on.br or rvm@on.br
2 -
Institut de Mécanique Céleste et de Calcul des Éphémérides, 77 avenue
Denfert-Rochereau F-75014 Paris, France
e-mail: Claude.Leguyader@bdl.fr
Received September 14, 1998; accepted January 8, 1999
229 CCD positions of Nereid taken between 1993 and 1998 are
presented. Many of the observations were taken near the periapsis.
Considering also the other published positions we have a good distribution
of the observations on the eccentric orbit of the satellite. Using a numeric
integration method we fitted all these observations in order to determine one
state vector for the orbit. The observed minus calculated standard deviation
for all observations is 023, and for our observations it is 0
16.
Key words: astrometry -- planets and satellites: Nereid
Copyright The European Southern Observatory (ESO)