Stability of permanent rotations of a heavy asymmetric gyrostat

  1. Iñarrea, M. 1
  2. Lanchares, V. 1
  3. Pascual, A.I. 1
  4. Elipe, A. 2
  1. 1 Universidad de La Rioja
    info

    Universidad de La Rioja

    Logroño, España

    ROR https://ror.org/0553yr311

  2. 2 Universidad de Zaragoza
    info

    Universidad de Zaragoza

    Zaragoza, España

    ROR https://ror.org/012a91z28

Aldizkaria:
Advances in the Astronautical Sciences

ISSN: 0065-3438

Argitalpen urtea: 2017

Alea: 160

Orrialdeak: 2663-2682

Mota: Artikulua

beta Ver similares en nube de resultados

Beste argitalpen batzuk: Advances in the Astronautical Sciences

Laburpena

For this problem, we obtain the possible permanent rotations, that is, the equilibria of the system. The stability of those permanent rotations is analyzed by means of the Energy-Casimir method. We are able to give necessary and sufficient conditions for some of the permanent rotations. The geometry of the gyrostat and the value of the gyrostatic moment are relevant in order to get stable permanent rotations. Moreover, it seems that the necessary conditions are also sufficient, but, however, this fact can only be proved partially.

Finantzaketari buruzko informazioa

This work has been partially supported by the Spanish Ministry of Economy, projects MTM2014-59433-C2-2-P and ESP2013-44217-R. A.E. also acknowledges support from the group E-48 of the Aragon Government and FEDER funds.

Finantzatzaile

  • Spanish Ministry of Economy
    • MTM2014-59433-C2-2-P
    • ESP2013-44217-R
  • group E-48 of the Aragon Government
  • FEDER funds