J2-perturbed Rendezvous

J2-Perturbed Rendezvous is a spacecraft rendezvous model that accounts for the secular and periodic orbital perturbations caused by Earth's oblateness (J₂ term) in the gravitational potential, distinguishing it from simplified two-body rendezvous formulations by incorporating the dominant non-spherical gravitational effects on relative orbital motion.

11

Publications

455

Citations

31

Authors

15

Institutions

Publications per year

2017–2026

3

Authors

31

  1. HL
    Haiyang Li

    Tsinghua University, China

    1 publications · 60 citations

    1

    h-index

  2. HB
    Hexi Baoyin

    Tsinghua University, China

    1 publications · 60 citations

    1

    h-index

  3. XS
    Xiaowei Shao

    The University of Tokyo, Japan

    1 publications · 17 citations

    1

    h-index

  4. JZ
    Jiamin Zhu

    Wadsworth Center, United States

    1 publications · 20 citations

    1

    h-index

  5. CL
    Charlotte Lücking

    University of Strathclyde, United Kingdom

    1 publications · 65 citations

    1

    h-index

1–5 of 31

Venues

  1. Acta Astronautica

    3 publications · 113 citations

    3

    h-index

  2. Journal of Guidance Control and Dynamics

    3 publications · 243 citations

    3

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    2 publications · 38 citations

    2

    h-index

  4. Aircraft Engineering and Aerospace Technology

    1 publications · 17 citations

    1

    h-index

  5. 1

    h-index

1–5