Three-Dimensional Periodic Halo Orbits

Details Three-Dimensional Periodic Halo Orbits Three-Dimensional Periodic Halo Orbits

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cemec..32...53h&link_type=abstract

Celestial Mechanics, Vol.32:1, P. 53, 1984

Other

18

Scientific paper

A largely numerical study was made of families of three-dimensional, periodic, 'halo' orbits near the collinear libration points in the restricted three-body problem. Families extend from each of the libration points to the nearest primary. They appear to exist for all values of the mass ratio μ, from 0 to 1. Most of the families contain a range of stable orbits. Only near L1, there are no stable orbits for certain values of μ. In that case the stable range decreases with increasing μ, until it disappears at μ = 0.0573. Near the other libration points, stable orbits exist for all mass ratios investigated between 0 and 1. In addition, the orbits increase in size with increasing μ.

Affiliated with

Also associated with

No associations

Rating

Three-Dimensional Periodic Halo Orbits 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 Three-Dimensional Periodic Halo Orbits, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Three-Dimensional Periodic Halo Orbits will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-936660