Some aspects of multiple-star ephemeris computation

Details Some aspects of multiple-star ephemeris computation Some aspects of multiple-star ephemeris computation

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101.1063h&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, March 1991, p. 1063, 1064.

Statistics

Computation

1

Ephemerides, Many Body Problem, Triple Stars, Binary Stars, Centaurus Constellation, Computational Astrophysics, Stellar Orbits, Three Body Problem

Scientific paper

For ultraprecise multiple-star ephemeris computation, these systems cannot be considered as stationary multi-two-body systems. For nearby, high-motion systems, the change in perspective must be considered. For close triples, the three-body perturbations must be considered. In any case, it is desirable now for orbit computers and catalogers to start including a weighted mean epoch as part of the reported orbital parameters.

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