dc.creatorAltavista, Carlos Alberto
dc.date1963
dc.date2020-03-26T10:44:06Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/91811
dc.descriptionA method for computing special perturbations has been devised. At the present time we have only considered the case with three co-planar bodies. Only one differential equation is to be solved. The radius vector r is the dependent variable. The time has been taken as independent variable. The true anomaly ν is the remaining quantity to be disturbed. The corresponding set of equations algebraic ones. The whole process is an iterative one. Special attention is to be paid for determining the most favorable cases for the applications.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.format94-94
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectspecial perturbations
dc.titleMethod for special perturbations
dc.typeArticulo
dc.typeComunicacion


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