The Restricted Hill Four-Body Problem with Applications to the Earth-Moon-Sun System

Celestial Mechanics and Dynamical Astronomy

Volumn 70, Issue 2, 1998, Pages 75-98

  Scheeres, D J ^a  

^a Iowa State University of Science and Technology   (United States)

Author keywords

Earth Moon Sun system; Hill four body problem

Indexed keywords

EID: 0043230850     PISSN: 09232958     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1026498608950     Document Type: Article

References (7)

1. Hénon, M.: 1969, 'Numerical Exploration of the Restricted Problem. V.', Astron. Astrophys. 1, 223-238.
2. Hénon M. and Petit, J.-M.: 1986, 'Series Expansions for Hill's Problem', Celest. Mech. 38, 67-100.
3. Kamel, A. A. and Breakwell, J. V.: 1970, 'Stability of Motion Near Sun-Perturbed Earth-Moon Triangular Libration Points', Periodic Orbits, Stability and Resonances, 82-90.
4. Kolenkiewicz, R. and Carpenter, L.: 1968, 'Stable Periodic Orbits about the Sun-Perturbed Earth-Moon Triangular Points', AIAA J. 6(7), 1301-1304.
5. Marchal, C.: 1990, The Three-Body Problem, Elsevier, pp. 162-163.
6. Schechter, H. B.: 1968, 'Three-Dimensional Nonlinear Stability Analysis of the Sun-Perturbed Earth-Moon Equilateral Points', AIAA J. 6(7), 1223-1228.
7. Wintner, A.: 1947, The Analytical Foundations of Celestial Mechanics, Princeton University Press, pp. 379-410.