Four classical methods for determining planetary elliptic elements: a comparison

DOI10.1007/S10569-005-8663-8zbMath1129.70013OpenAlexW2001736037MaRDI QIDQ816920

Alessandra Celletti, Gabriella Pinzari

Publication date: 2 March 2006

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-005-8663-8

zbMATH Keywords

orbit determinationLaplace's methodGauss' methodMossotti's method

Mathematics Subject Classification ID

Celestial mechanics (70F15) History of mechanics of particles and systems (70-03)

Related Items (5)

Dependence on the observational time intervals and domain of convergence of orbital determination methods ⋮ Multiple solutions in preliminary orbit determination from three observations ⋮ Single lunation \(N\)-observation orbits ⋮ Perihelia Reduction and Global Kolmogorov Tori in the Planetary Problem ⋮ Generalization of a method by Mossotti for initial orbit determination

Cites Work

• Unnamed Item
• Unnamed Item

This page was built for publication: Four classical methods for determining planetary elliptic elements: a comparison