Abstract—
The restricted problem of three bodies (material points) is considered. The orbits of the main attracting bodies are assumed to be ellipses of small eccentricity, and the passively gravitating body during its motion can leave the plane of the orbits of the main bodies (spatial problem). The stability of body motion corresponding to triangular Lagrangian libration points is investigated. A characteristic feature of the spatial problem under study is the presence of resonance due to the equality of the Keplerian motion period of the main bodies and the linear oscillation period of the passively gravitating body in the direction perpendicular to the plane of their orbits. Using the methods of classical perturbation theory, Kolmogorov—Arnold—Moser (KAM) theory and computer algebra algorithms, the nonlinear problem of stability for most (in the Lebesgue-measure sense) initial conditions and formal stability (stability in any arbitrarily high finite approximation with respect to the coordinates and impulses of perturbed motion) are investigated.
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REFERENCES
G. N. Duboshin, Celestial Mechanics: Analytical and Qualitative Methods (Nauka, Moscow, 1978) [in Russian].
A. P. Markeev, Libration Points in Celestial Mechanics and Cosmodynamics (Nauka, Moscow, 1978) [in Russian].
L. Euler, “De motu rectilineo trium corporum se mutuo attrahentum,” Novi Comm. Acad. Sci. Imp. Petrop. 11, 144–151 (1767).
J. L. Lagrange, Essai sur le Problème des Trois Corps. Oeuvres de Lagrange (Gauthier Villars, Paris, 1873), Vol. 6, pp. 229–324.
A. M. Lyapunov, “On the stability of motion in one particular case of the three-body problem,” in Collection of Works (Academy of Sciences of the USSR, Moscow, 1956), Vol. 1, pp. 327–401.
J. M. A. Danby, “Stability of the triangular points in the elliptic restricted problem of three bodies,” Astron. J. 69 (2), 165–172 (1964).
G. E. O. Giacaglia, “Characteristics exponents at L4 and L5 in the elliptic restricted problem of three bodies,” Celestial Mech. Dyn. Astron. 4 (3/4), 468–489 (1971).
A. H. Nayfeh and A. A. Kamel, “Stability of the triangular points in the elliptic restricted problem of three bodies,” AIAA J. 8 (2), 221–223 (1970).
M. G. Yumagulov and O. N. Belikova, “Bifurcation of 4π-periodic solutions of the planar, restricted, elliptical three-body problem,” Astron. Rep. 86 (2), 148–152 (2009).
T. Kovacs, “Stability chart of the triangular points in the elliptic restricted problem of three bodies,” Mon. Not. R. Astron. Soc. 430 (4), 2755–2760 (2013).
N. R. Isanbaeva, “On the construction of the boundaries of stability regions of triangular libration points of a planar bounded elliptic three-body problem,” Vestn. Bashk. Univ., Mat. Mekh. 22 (1), 5–9 (2017).
C. Simo, “Periodic orbits of the planar N-body problem with equal masses and all bodies on the same path,” in Proc. 54th Scottish Universities Summer School in Physics “The Restless Universe. Applications of Gravitational N-Body Dynamics to Planetary, Stellar and Galactic Systems”, Blair Atholl, July 23–Aug. 5, 2000 (CRC Press, New York, 2001), pp. 265–284.
A. L. Whipple and V. Szebehely, “The restricted problem of n + v bodies,” Celestial Mech. Dyn. Astron. 32 (2), 137–144 (1984).
D. A. Budzko and A. N. Prokopenya, “On the stability of equilibrium positions in the circular restricted four-body problem,” in Computer Algebra in Scientific Computing, Ed. by V. P. Gerdt (Springer-Verlag, Heidelberg, 2011), Vol. 6885, pp. 88–100.
E. A. Grebenikov, Mathematical Problems of Homographic Dynamics (Peoples’ Friendship University of Russia, Moscow, 2011).
A. L. Kunitsyn and A. T. Turesbaev, “Stability of triangular libration points of the photogravitational three-body problem,” Pis’ma Astron. Zh. 11 (2), 145–148 (1985).
L. G. Luk’yanov and A. Yu. Kochetkova, “On the stability of Lagrangian libration points in a restricted elliptic photogravitational three-body problem,” Vestn. Mosk. Univ., Ser. 3: Fiz., Astron., No. 5, 71–76 (1996).
A. S. Zimovshikov and V. N. Tkhai, “Stability diagrams for a heterogeneous ensemble of particles at the collinear libration points of the photogravitational three-body problem,” J. Appl. Math. Mech. 74 (2), 158–163 (2010).
A. Kononenko, “Libration points of the Earth–Moon system,” Aviats. Kosmonavt., No. 5, 71–73 (1968).
N. F. Averkiev, S. A. Vas’kov, and V. V. Salov, “Ballistic construction of communication spacecraft systems and passive radar of the Lunar surface,” Izv. Vyssh. Uchebn. Zaved., Priborostr. 51 (12), 66–72 (2008).
F. Salazar, O. Winter, E. Macau, J. Masdemont, and G. Gomez, “Natural configuration for formation flying around triangular libration points for the elliptic and the bicircular problem in the Earth–Moon system,” in Proc. 65th Int. Astronautical Congress (Toronto, 2014).
I. G. Malkin, Theory of Stability of Motion (Office Techn. Inform, Washington, 1952).
A. P. Markeev, “On normal voordinates in the vicinity of the Lagrangian libration points of the restricted elliptic three-body problem,” Vestn. Udmurt. Univ. Mat. Mekh. Komp’yut. Nauki 30 (4), 657–671 (2020).
G. E. O. Giacaglia, Perturbation Methods in Non-Linear Systems (Springer, New York, 1972).
A. X. Nayfeh, Perturbation Methods (Wiley, New York, 1973).
A. N. Kolmogorov, “Preservation of conditionally periodic movements with small change in the Hamilton function,” in Stochastic Behaviour in Classical and Quantum Hamiltonian Systems, Ed. by G. Casati and J. Ford (Springer-Verlag, Berlin, 1979), Vol. 93, pp. 51–56.
V. I. Arnol’d, “Proof of a theorem of A. N. Kolmogorov on the invariance of quasi-periodic motions under small perturbations of the Hamiltonian,” Russ. Math. Surv. 18 (5), 9–36 (1963).
V. I. Arnol’d, “Small denominators and problems of stability of motion in classical and celestial mechanics,” Russ. Math. Surv. 18 (6), 85–191 (1963).
V. I. Arnol’d, Mathematical Methods of Classical Mechanics (Springer-Verlag, New York, 1989).
V. I. Arnol’d, V. V. Kozlov, and A. I. Neishtadt, Mathematical Aspects of Classical and Celestial Mechanics Encyclopaedia Math. Sci. Ser., vol. 3 (Springer-Verlag, Berlin, 2006).
Ch. Lhotka, C. Efthymiopoulos, and R. Dvorak, “Nekhoroshev stability at L4 or L5 in the elliptic-restricted three-body problem-application to Trojan asteroids,” Mon. Not. R. Astron. Soc. 384, 1165–1177 (2008).
A. Deprit and A. Deprit-Bartholomé, “Stability of the triangular Lagrangian points,” Astron. J. 72 (2), 173–179 (1967).
A. P. Markeev, “On the stability of triangular Lagrangian solutions in the spatial circular restricted three-body problem,” Astron. Zh 48 (4), 862–868 (1971).
N. N. Nekhoroshev, “Behavior of Hamiltonian systems close to integrable,” Funct. Anal. Appl. 5 (4), 338–339 (1971).
N. N. Nekhoroshev, “An exponential estimate of the stability time of near-integrable Hamiltonian systems,” Russ. Math. Surv. 32 (6), 1–65 (1977).
N. N. Nekhoroshev, “An exponential estimate of the time of stability of nearly integrable Hamiltonian systems. II,” in Topics in Modern Mathematics. Petrovskii Seminar, Ed. by O. A. Oleinik (Consultant Bureau, New York, 1985), No. 5, pp. 1–58.
J. Moser, “New aspects in the theory of stability of Hamiltonian systems,” Commun. Pure Appl. Math. 11 (1), 81–114 (1958).
J. Moser, “Stabilitatsverhalten Kanonischer Differentialgleichungs Systeme,” Nachr. Akad. Wiss. Göttingen Math.-Phys. Kl. IIa 1955, 87–120 (1955).
J. Moser, “On the elimination of the irrationality condition and Birkhoff'’s concept of complete stability,” Bol. Soc. Mat. Mexicana 5, 167–175 (1960).
J. Moser, “Stability of the asteroids,” Astron. J. 63 (10), 439–443 (1958).
C. L. Siegel, Vorlesungen über Himmelsmechanik, Grundlehren Math. Wiss., vol. 85 (Springer-Verlag, Berlin, 1956)).
J. Glimm, “Formal stability of Hamiltonian systems,” Commun. Pure Appl. Math. 17 (4), 509–526 (1964).
A. D. Bruno, “Formal stability of Hamiltonian systems,” Math. Zametki 1 (3), 216–219 (1967).
A. D. Bruno, The Restricted 3-Body Problem: Plane Periodic Orbits (Walter de Gruyter, Berlin, 1994), Vol. 17.
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This work was supported by a grant from the Russian Science Foundation (project no. 19-11-00116) at Moscow Aviation Institute (National Research University) and at Ishlinsky Institute for Problems in Mechanics, Russian Academy of Sciences.
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Translated by T. N. Sokolova
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Markeev, A.P. On the Stability of Lagrange Solutions in the Spatial Near-Circular Restricted Three-Body Problem. Mech. Solids 56, 1541–1549 (2021). https://doi.org/10.3103/S0025654421080124
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DOI: https://doi.org/10.3103/S0025654421080124