Families of Halo-like invariant tori around L2 in the Earth-Moon Bicircular Problem

dc.contributor.author	Rosales, José J.
dc.contributor.author	Jorba, Ángel
dc.contributor.author	Jorba-Cuscó, Marc
dc.date	2021
dc.date.accessioned	2021-07-22T12:04:05Z
dc.date.available	2021-07-22T12:04:05Z
dc.identifier.issn	0923-2958
dc.identifier.uri	https://reunir.unir.net/handle/123456789/11648
dc.description.abstract	The Bicircular Problem (BCP) is a periodic time dependent perturbation of the Earth-Moon Restricted Three-Body Problem that includes the direct gravitational effect of the Sun. In this paper we use the BCP to study the existence of Halo-like orbits around L2 in the Earth-Moon system taking into account the perturbation of the Sun. By means of computing families of 2D invariant tori, we show that there are at least two different families of Halo-like quasi-periodic orbits around L2.	es_ES
dc.language.iso	eng	es_ES
dc.publisher	Celestial mechanics and dynamical astronomy	es_ES
dc.relation.ispartofseries	;vol. 133, nº 4
dc.relation.uri	https://link.springer.com/article/10.1007%2Fs10569-021-10012-0	es_ES
dc.rights	restrictedAccess	es_ES
dc.subject	quasi-periodic halo orbits	es_ES
dc.subject	stability of invariant curves	es_ES
dc.subject	translunar point	es_ES
dc.subject	Scopus	es_ES
dc.subject	WOS(2)	es_ES
dc.title	Families of Halo-like invariant tori around L2 in the Earth-Moon Bicircular Problem	es_ES
dc.type	Articulo Revista Indexada	es_ES
reunir.tag	~ARI	es_ES
dc.identifier.doi	https://doi.org/10.1007/s10569-021-10012-0

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