Abstract The solar radiation pressure can affect significantly orbits around binary asteroid system (i.e., BAS). One novel three-dimensional resonance orbit family for BASs is constructed due to primary resonance and 1:1 internal resonance between the in-plane motion and the out-of-plane motion, by treating the solar radiation pressure as excitation. Since the periodic orbits are disturbed by the solar radiation, the multiple scales method can be used to derive the first-order approximated solution. Then, the stabilities of such orbit solutions are investigated. The energy transferring mechanism that “pumps” SRP energy from in-plane motion to out-of-plane motion is also illustrated. The accuracy of such approximated solutions is further verified by numerical iterations. The 7088 Ishtar BAS and1996 FG3 BAS are taken as examples to verify the proposed method.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Three-dimensional resonance orbit design for binary asteroid system


    Beteiligte:
    Li, Jianqing (Autor:in) / Qian, Ying-Jing (Autor:in) / Zong, Kai (Autor:in) / Yang, Xiao-Dong (Autor:in) / Li, Chaoyong (Autor:in)

    Erschienen in:

    Advances in Space Research ; 72 , 6 ; 2078-2090


    Erscheinungsdatum :

    2023-06-05


    Format / Umfang :

    13 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




    Estimation of Binary Asteroid Gravity Using Mutual Orbit Observations

    Meyer, Alex J. / Scheeres, Daniel J. | AIAA | 2022


    GNC Design for Asteroid Orbit Modification Missions

    Hagenfeldt, Miguel / Cano, Juan Luis / Penin, Luis F. et al. | AIAA | 2013


    Near Earth Asteroid Rendezvous Orbit Phase Trajectory Design

    Miller, J. / Carranza, E. / Helfrich, C. et al. | British Library Conference Proceedings | 1998


    Near Earth Asteroid Rendezvous orbit phase trajectory design

    Miller, J. / Carranza, E. / Helfrich, C. et al. | AIAA | 1998