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Volumn 52, Issue 8, 2004, Pages 685-692

Numerical determination of stability regions for orbital motion in uniformly rotating second degree and order gravity fields

Author keywords

Asteroids; Orbital dynamics; Stability

Indexed keywords

EQUATIONS OF MOTION; GRAVITATIONAL EFFECTS; MOTION ESTIMATION; NORMAL DISTRIBUTION; NUMERICAL ANALYSIS; RESONANCE; ROTATION; STABILITY;

EID: 2342507675     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pss.2004.01.003     Document Type: Article
Times cited : (118)

References (12)
  • 1
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    • Long-term evolution of artificial satellite orbits due to resonant tesseral harmonics
    • Ely T.A., Howell K.C. Long-term evolution of artificial satellite orbits due to resonant tesseral harmonics. J. Astron. Sci. 44(2):1996;167-190.
    • (1996) J. Astron. Sci. , vol.44 , Issue.2 , pp. 167-190
    • Ely, T.A.1    Howell, K.C.2
  • 4
    • 0036641287 scopus 로고    scopus 로고
    • Spacecraft motion about slowly rotating asteroids
    • Hu W., Scheeres D.J. Spacecraft motion about slowly rotating asteroids. J. Guidance Control Dyn. 25(4):2002;765-775.
    • (2002) J. Guidance Control Dyn. , vol.25 , Issue.4 , pp. 765-775
    • Hu, W.1    Scheeres, D.J.2
  • 5
    • 0242720804 scopus 로고    scopus 로고
    • Stability bounds for three-dimensional motion close to asteroids
    • Lara M., Scheeres D.J. Stability bounds for three-dimensional motion close to asteroids. J. Astronaut. Sci. 50(4):2002;389-409.
    • (2002) J. Astronaut. Sci. , vol.50 , Issue.4 , pp. 389-409
    • Lara, M.1    Scheeres, D.J.2
  • 9
    • 0000385904 scopus 로고
    • Dynamics about uniformly rotating tri-axial ellipsoids. Applications to asteroids
    • Scheeres D.J. Dynamics about uniformly rotating tri-axial ellipsoids. Applications to asteroids. Icarus. 110:1994;225-238.
    • (1994) Icarus , vol.110 , pp. 225-238
    • Scheeres, D.J.1
  • 11
    • 0000809087 scopus 로고    scopus 로고
    • Secular motion in a 2nd degree and order gravity field with no rotation
    • Scheeres D.J., Hu W. Secular motion in a 2nd degree and order gravity field with no rotation. Celestial Mech. Dyn. Astron. 79:2001;183-200.
    • (2001) Celestial Mech. Dyn. Astron. , vol.79 , pp. 183-200
    • Scheeres, D.J.1    Hu, W.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.