Improved Method for Orbital Elements Differential Correction.
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Scholar |
Otros documentos de la autoría: López García, A.; López Ortí, José Antonio; López Machí, R.
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Título
Improved Method for Orbital Elements Differential Correction.Fecha de publicación
1990Editor
© Springer Netherlands; INTERNATIONAL ASTRONOMIC UNION (IAU)ISBN
978-0-7923-0787-7Cita bibliográfica
GARCIA, A. Lopez; ORTI, JA Lopez; MACHI, R. Lopez. Improved Method for Orbital Elements Differential Correction. In: Inertial Coordinate System on the Sky. Springer Netherlands, 1990. p. 199-200.Tipo de documento
info:eu-repo/semantics/bookPartVersión de la editorial
http://rd.springer.com/chapter/10.1007/978-94-009-0613-6_75Versión
info:eu-repo/semantics/publishedVersionPalabras clave / Materias
Resumen
As was pointed out by IAU in 1976, an important problem in fundamental astronomy is the improvement of the vernal equinox and equator positions. To this aim, it is necessary to know the accurate values of minor planets ... [+]
As was pointed out by IAU in 1976, an important problem in fundamental astronomy is the improvement of the vernal equinox and equator positions. To this aim, it is necessary to know the accurate values of minor planets orbital elements. The classical methods of orbital elements differential corrections are based on linking the observations at different epochs considering equal derivatives respect to the initial and osculating elements.
In this paper we present an improved method in which the least squares matrix coefficients is calculated from the integration of the Lagrange planetary equations and its derivatives. [-]
Publicado en
Inertial Coordinate System on the Sky Volume 141 of the series International Astronomical Union / Union Astronomique Internationale pp 199-200Derechos de acceso
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