000124452 001__ 124452
000124452 005__ 20241125101150.0
000124452 0247_ $$2doi$$a10.1007/s10569-022-10118-z
000124452 0248_ $$2sideral$$a132851
000124452 037__ $$aART-2023-132851
000124452 041__ $$aeng
000124452 100__ $$0(orcid)0000-0002-5692-5876$$aAbad, A.$$uUniversidad de Zaragoza
000124452 245__ $$aEvolution of the characteristic curves in the restricted three-body problem in terms of the mass parameter
000124452 260__ $$c2023
000124452 5060_ $$aAccess copy available to the general public$$fUnrestricted
000124452 5203_ $$aIn this work, we study the evolution of the families of simple symmetric periodic orbits in the restricted three-body problem whatever the value of the mass parameter μ. To classify these characteristic curves, we introduce a topological characterization of both orbits and families. Starting from the work of Strömgren for the Copenhagen case, we analyze the evolution of these families, when the mass parameter μ varies in (0, 1/2], focusing on their topological characterization, the existence of asymptotic points and the appearance of certain types of orbits such as horseshoe orbits. Lastly, we consider two samples, the Earth–Moon and Sun–Jupiter systems and classify the different types of orbits for these systems.
000124452 536__ $$9info:eu-repo/grantAgreement/ES/DGA-FSE/E24-20R$$9info:eu-repo/grantAgreement/ES/MICINN/PID2020-117066GB-I00
000124452 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000124452 590__ $$a1.6$$b2023
000124452 592__ $$a0.521$$b2023
000124452 591__ $$aMATHEMATICS, INTERDISCIPLINARY APPLICATIONS$$b70 / 135 = 0.519$$c2023$$dQ3$$eT2
000124452 593__ $$aApplied Mathematics$$c2023$$dQ2
000124452 591__ $$aASTRONOMY & ASTROPHYSICS$$b51 / 84 = 0.607$$c2023$$dQ3$$eT2
000124452 593__ $$aAstronomy and Astrophysics$$c2023$$dQ2
000124452 593__ $$aComputational Mathematics$$c2023$$dQ2
000124452 593__ $$aMathematical Physics$$c2023$$dQ2
000124452 593__ $$aModeling and Simulation$$c2023$$dQ2
000124452 593__ $$aSpace and Planetary Science$$c2023$$dQ3
000124452 594__ $$a3.0$$b2023
000124452 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000124452 700__ $$0(orcid)0000-0002-4426-6885$$aArribas, M.$$uUniversidad de Zaragoza
000124452 700__ $$0(orcid)0000-0002-1374-4645$$aPalacios, M.
000124452 700__ $$0(orcid)0000-0001-5208-4494$$aElipe, A.$$uUniversidad de Zaragoza
000124452 7102_ $$12005$$2595$$aUniversidad de Zaragoza$$bDpto. Matemática Aplicada$$cÁrea Matemática Aplicada
000124452 7102_ $$12004$$2398$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Física de la Tierra
000124452 773__ $$g135, 2 (2023), [23 pp.]$$pCelest. mech. dyn. astron.$$tCelestial Mechanics and Dynamical Astronomy$$x0923-2958
000124452 8564_ $$s1597188$$uhttps://zaguan.unizar.es/record/124452/files/texto_completo.pdf$$yVersión publicada
000124452 8564_ $$s1223528$$uhttps://zaguan.unizar.es/record/124452/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000124452 909CO $$ooai:zaguan.unizar.es:124452$$particulos$$pdriver
000124452 951__ $$a2024-11-22-12:06:43
000124452 980__ $$aARTICLE