Relative equilibria for general gravity fields in the sphere-restricted full 2-body problem

Celestial Mechanics and Dynamical Astronomy

Volumn 94, Issue 3, 2006, Pages 317-349

  Scheeres, D J ^a  

^a UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33745026031     PISSN: 09232958     EISSN: 15729478     Source Type: Journal    
DOI: 10.1007/s10569-005-6182-2     Document Type: Article

References (12)

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2. Kinoshita, H.: 1972, 'First-order perturbations of the two finite body problem', Publ. Astron. Soc. Japan 24, 423-457.
3. Koon, W.-S., Marsden, J. E., Ross, S., Lo, M. W. and Scheeres, D. J.: 2004, 'Geometric mechanics and the dynamics of asteroid pairs', In: E. Belbruno, D. Folta and P. Gurfil (eds.), Astrodynamics, Space Missions, and Chaos, Annals of the New York Academy of Science, Vol. 1017, pp. 11-38.
4. Maciejewski, A. J.: 1995, 'Reduction, relative equilibria and potential in the two rigid bodies problem', Celest. Mech. Dyn. Astron. 63, 1-28.
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7. Scheeres D. J.: 2002a, 'Stability of binary asteroids', Icarus 159(2), 271-283.
8. Scheeres, D. J.: 2002b, 'Stability in the full two-body problem', Celest. Mech. Dyn. Astron. 83, 155-169.
9. Scheeres, D. J.: 2004, 'Stability of relative equilibria in the full two-body problem', In: E. Belbruno, D. Folta and P. Gurfil (eds.), Astrodynamics, Space Missions, and Chaos, Annals of the New York Academy of Science, Vol. 1017, pp. 81-94.
10. Simo, J. C., Lewis, D. and Marsden, J. E.: 1991, 'Stability of relative equilibria. I. The reduced energy-momentum method', Arch. Rational Mech. Anal. 115(1), 15-59.
11. Wang, L.-I., Krishnaprasad, P. S. and Maddocks, J. H.: 1991, 'Hamiltonian Dynamics of a rigid body in a central gravitational field', Celest. Mech. Dyn. Astron. 50, 349-386.
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