Method for special perturbations

A 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 an...

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Autor principal: Altavista, Carlos Alberto
Formato: Articulo Comunicacion
Lenguaje:Inglés
Publicado: 1963
Materias:
Ciencias Astronómicas
special perturbations
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/91811
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-91811
record_format dspace
spelling I19-R120-10915-918112024-07-04T18:52:32Z http://sedici.unlp.edu.ar/handle/10915/91811 Method for special perturbations Altavista, Carlos Alberto 1963 2020-03-26T10:44:06Z en Ciencias Astronómicas special perturbations A 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. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 94-94
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
special perturbations
spellingShingle Ciencias Astronómicas
special perturbations
Altavista, Carlos Alberto
Method for special perturbations
topic_facet Ciencias Astronómicas
special perturbations
description A 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.
format Articulo
Comunicacion
author Altavista, Carlos Alberto
author_facet Altavista, Carlos Alberto
author_sort Altavista, Carlos Alberto
title Method for special perturbations
title_short Method for special perturbations
title_full Method for special perturbations
title_fullStr Method for special perturbations
title_full_unstemmed Method for special perturbations
title_sort method for special perturbations
publishDate 1963
url http://sedici.unlp.edu.ar/handle/10915/91811
work_keys_str_mv AT altavistacarlosalberto methodforspecialperturbations
_version_ 1807220485212078080

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