Simulation method for study of the effects of systematic errors in orbits

Details Simulation method for study of the effects of systematic errors in orbits Simulation method for study of the effects of systematic errors in orbits

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...204..337d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 204, no. 1-2, Oct. 1988, p. 337-340. In French.

Statistics

Computation

2

Asteroids, Computational Astrophysics, Error Analysis, Orbit Calculation, Orbital Mechanics, Orbital Elements, Periodic Variations, Precision, Variational Principles

Scientific paper

The Gauss-Enke method is presently used to compute elliptical orbits, in order to ascertain the method's sensitivity to systematic observational errors. After refining the method through incorporation of the geocentric-distance variation due to Stracke (1929), five asteroids discovered at ESO-La Silla are studied. For constant theta, the error effect vs rho is found to be linear.

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