Ephemeris computation of the relative radial velocity (vr) of the components of a double star, avoiding the kepler's equation resolution. (French Title: Calcul d'une éphéméride de vitesse radiale relative (vr) des composantes d'une étoile double visuelle e

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When conducting our researches on the orientation of the orbital planes of the visual double stars (J. Dommanget, 2004; 2005a), we established two catalogues of ephemerides of relative radial velocitites (J. Dommanget et O.NYS, 1968, 1988). We then encountered some difficulties with the drawing equipment of the analog computer by using the usual way consisting in starting formthe variable 't'. The problems were automatically solved when starting from the true anomaly 'v'. It may be interesting for amateurs astronomers, to know some details about this original computational way. We also show that starting from this parameter 'v' may be interesting to consider for computing a classical ephemerides.

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Ephemeris computation of the relative radial velocity (vr) of the components of a double star, avoiding the kepler's equation resolution. (French Title: Calcul d'une éphéméride de vitesse radiale relative (vr) des composantes d'une étoile double visuelle e does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

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