This paper presents orbital elements for the asteroid 1979 HB discovered during the period from april 20 through april 29 , 1979 at the GPO telescope (f= 4m, d2 40 cm) of the European Southern Observatory - ESO, La Silla, Chile. The orbit has been computed by Gauss-Encke Method (with successive improvements of the geocentric distances based on 21 positions). All plates were measured at the Ascorecord Zeiss/Jena measuring machine of the Valongo Observatory . The positions were computed by means of dependences and of the least squares, with the computer Burrough's B6700 of the Núcleo de Computação Eletrônica - NCE, of the Universidade Federal do Rio de Janeiro . The observations are reduced to the equinox 1950, and the coordinates of the refe...
In february 1983. we have observed the Satellites of Saturn and Minor Planets at the ESO, La Silla, ...
We have studied the possibilities of improving the orbits of asteroids by using observations made in...
International audienceBased on all published astrometric observations, we have determined the moon o...
This paper presents orbital elements for the asteroid 1979 HB discovered during the period from apri...
268 astrometric positions and dependences of asteroids as obtained from photographic observations ma...
Dependencies and 165 astrometric positions of asteroids are given; 58 of these refer to asteroids of...
peer reviewedThe results are presented of photographic observations of asteroid positions made in Au...
We present the orbital elements of asteroid QE1 (pro visional designation) identified in august 26, ...
The discovery of the asteroid Ceres by Piazzi in 1801 motivated the development of a mathematical te...
More than 7000 positions of moving objects have been detected on 33 films obtained with the Schmidt ...
Based on four observations, the equations to determine the orbit (position and velocity) of an objec...
More than 7000 positions of moving objects were detected on 33 films obtained with the Schmidt teles...
In this thesis I will present Gaia, an ESA mission which is observing stars and Solar System objects...
International audienceA new astrometric reduction of old photographic plates, benefiting from modern...
International audienceA new astrometric reduction of old photographic plates, benefiting from modern...
In february 1983. we have observed the Satellites of Saturn and Minor Planets at the ESO, La Silla, ...
We have studied the possibilities of improving the orbits of asteroids by using observations made in...
International audienceBased on all published astrometric observations, we have determined the moon o...
This paper presents orbital elements for the asteroid 1979 HB discovered during the period from apri...
268 astrometric positions and dependences of asteroids as obtained from photographic observations ma...
Dependencies and 165 astrometric positions of asteroids are given; 58 of these refer to asteroids of...
peer reviewedThe results are presented of photographic observations of asteroid positions made in Au...
We present the orbital elements of asteroid QE1 (pro visional designation) identified in august 26, ...
The discovery of the asteroid Ceres by Piazzi in 1801 motivated the development of a mathematical te...
More than 7000 positions of moving objects have been detected on 33 films obtained with the Schmidt ...
Based on four observations, the equations to determine the orbit (position and velocity) of an objec...
More than 7000 positions of moving objects were detected on 33 films obtained with the Schmidt teles...
In this thesis I will present Gaia, an ESA mission which is observing stars and Solar System objects...
International audienceA new astrometric reduction of old photographic plates, benefiting from modern...
International audienceA new astrometric reduction of old photographic plates, benefiting from modern...
In february 1983. we have observed the Satellites of Saturn and Minor Planets at the ESO, La Silla, ...
We have studied the possibilities of improving the orbits of asteroids by using observations made in...
International audienceBased on all published astrometric observations, we have determined the moon o...