Abstract
The study of the Trojan problem (i.e. the motion in the vicinity of the equilateral Lagrangian points L 4 or L 5) has a long history in the literature. Starting from a representation of the Elliptic Restricted 3-Body Problem in terms of modified Delaunay variables, we propose a sequence of canonical transformations leading to a Hamiltonian decomposition in the three degrees of freedom (fast, synodic and secular). From such a decomposition, we introduce a model called the ‘basic Hamiltonian’ H b , corresponding to the part of the Hamiltonian independent of the secular angle. Averaging over the fast angle, the 〈H b 〉 turns to be an integrable Hamiltonian, yet depending on the value of the primary’s eccentricity e′. This allows to formally define action-angle variables for the synodic degree of freedom, even when e′ ≠ 0. In addition, we introduce a method for locating the position of secondary resonances between the synodic libration frequency and the fast frequency, based on the use of the normalized 〈H b 〉. We show that the combination of a suitable normalization scheme and the representation by the H b is efficient enough so as to allow to accurately locate secondary resonances as well as higher order resonances involving also the very slow secular frequencies.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Notes
- 1.
We symbolize with arctan (a, b) the function \(\mathrm{tan}^{-1}(a/b): \mathbb{R}^{2} \rightarrow \mathbb{T}^{1}\), of two variables, that maps the value of the arctangent to the corresponding quadrant in the coordinate system with b as the abscissa and a as the ordinate.
References
Brown, E.W., Shook, C.A.: Planetary Theory. Cambridge University Press, New York (1933)
Deprit, A., Delie, A.: Trojan orbits I. d’Alembert series at L 4. Icarus 4, 242–266 (1965)
Érdi, B.: An asymptotic solution for the Trojan case of the plane elliptic restricted problem of three bodies. Celest. Mech. Dyn. Astron. 15, 367–383 (1977)
Érdi, B.: The three-dimensional motion of Trojan asteroids. Celest. Mech. Dyn. Astron. 18, 141–161 (1978)
Érdi, B.: The Trojan problem. Celest. Mech. Dyn. Astron. 65, 149–164 (1996)
Froeschlé, C., Guzzo, M., Lega, E.: Graphical evolution of the Arnold web: from order to chaos. Science 289 (5487), 2108–2110 (2000)
Garfinkel, B.: Theory of the Trojan asteroids, Part I. Astron. J. 82 (5), 368–379 (1977)
Gascheau, G.: Examen d’une classe d’équations difféntielles et applicaction à un cas particulier du problème des trois corps. Compt. Rendus 16 (7), 393–394 (1843)
Gopalswamya, N. et al.: Earth-affecting solar causes observatory (EASCO): A potential international living with a star mission from Sun-Earth L5. J. Atmos. Sol. Terr. Phys. 73 (5–6), 658–663 (2011)
Laskar, J.: Frequency map analysis and quasiperiodic decompositions. In: Benest, D., Froeschlé, C., Lega, E. (eds.) Hamiltonian Systems and Fourier Analysis, pp. 99–134. Cambridge Scientific, Cambridge (2004)
Morais, M.H.M.: Hamiltonian formulation on the secular theory for a Trojan-type motion. Astron. Astrophys. 369, 677–689 (2001)
Murray, C.D., Dermott, S.F.: Solar Systems Dynamics. Cambridge Universiy Press, Cambridge (1999)
Namouni, F.: Secular interactions of coorbiting objects. Icarus 137 (2), 293–314 (1999)
Namouni, F., Murray, C.D.: The effect of eccentricity and inclination on the motion near the Lagrangian points L 4 and L 5. Celest. Mech. Dyn. Astron. 76 (2), 131–138 (2000)
Páez, R.I., Efthymiopoulos, C.: Trojan resonant dynamics, stability and chaotic diffusion, for parameters relevant to exoplanetary systems. Celest. Mech. Dyn. Astron. 121 (2), 139–170 (2015)
Páez, R.I., Locatelli, U.: Trojan dynamics well approximated by a new Hamiltonian normal form. Mon. Not. R. Astron. Soc. 453 (2), 2177–2188 (2015)
Acknowledgements
During this work, RIP was fully supported by the Astronet-II Marie Curie Initial Training Network (PITN-GA-2011-289240).
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2016 Springer International Publishing Switzerland
About this paper
Cite this paper
Páez, R.I., Locatelli, U., Efthymiopoulos, C. (2016). The Trojan Problem from a Hamiltonian Perturbative Perspective. In: Gómez, G., Masdemont, J. (eds) Astrodynamics Network AstroNet-II. Astrophysics and Space Science Proceedings, vol 44. Springer, Cham. https://doi.org/10.1007/978-3-319-23986-6_14
Download citation
DOI: https://doi.org/10.1007/978-3-319-23986-6_14
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-23984-2
Online ISBN: 978-3-319-23986-6
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)