Frozen orbits for the zonal moon potential

  1. Elipe, A. 1
  2. Lanchares, V. 2
  3. Lara, M. 3
  1. 1 Universidad de Zaragoza
    info

    Universidad de Zaragoza

    Zaragoza, España

    ROR https://ror.org/012a91z28

  2. 2 Universidad de La Rioja
    info

    Universidad de La Rioja

    Logroño, España

    ROR https://ror.org/0553yr311

  3. 3 Real Inst. y Observ. de la Armada, E-11110 San Fernando, Spain
Erakutsi afiliazioak +
Aldizkaria:
Advances in the Astronautical Sciences

ISSN: 0065-3438

Argitalpen urtea: 1996

Alea: 93 PART 1

Orrialdeak: 621-632

Mota: Artikulua

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SCOPUS: 2-s2.0-17144467323 GOOGLE SCHOLAR

Beste argitalpen batzuk: Advances in the Astronautical Sciences

Laburpena

For the zonal problem of the Moon considering up to the J7 harmonic, we found several families of periodic orbits. The strong differences between the Moon and other cases (Earth-like planets) is mainly due to the magnitude of the zonal harmonic J7, that in this case is of the same magnitude that J2.