Periodic motions of a three-axis gyrostatic satellite at a triangular libration point

Details Periodic motions of a three-axis gyrostatic satellite at a triangular libration point Periodic motions of a three-axis gyrostatic satellite at a triangular libration point

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..144e&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Jan.-Feb. 1989, p. 144-146. In Russian.

Mathematics

Celestial Mechanics, Center Of Mass, Gyroscopes, Satellite Rotation, Spacecraft Motion, Equations Of Motion, Gravitational Effects, Libration, Transformations (Mathematics)

Scientific paper

Consideration is given to a problem in which the center of mass of a gyrostatic satellite M is located at the L4 triangular libration point of the gravitating bodies M sub 0 and M sub 1, which move with respect to a common center of mass in circular Keplerian orbits. The mass of M is considered to be negligibly small compared with the masses of M sub 0 and M sub 1, and the dimensions of M are considered to be negligibly small compared with the distance between M sub 0 and M sub 1. The periodic motions of the gryostat under the effect of the gravitational moments produced by M sub 0 and M sub 1 are analyzed on the basis of equations of rotational motion in dimensionless Andoyer variables.

Affiliated with

Also associated with

No associations

Rating

Periodic motions of a three-axis gyrostatic satellite at a triangular libration point does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Periodic motions of a three-axis gyrostatic satellite at a triangular libration point, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Periodic motions of a three-axis gyrostatic satellite at a triangular libration point will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828007