Instability of Motion at the Lagrangian Triangular Point in the Earth-Moon System

Details Instability of Motion at the Lagrangian Triangular Point in the Earth-Moon System Instability of Motion at the Lagrangian Triangular Point in the Earth-Moon System

Mar 1962

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1962natur.193.1063b&link_type=abstract

Nature, Volume 193, Issue 4820, pp. 1063 (1962).

Other

Scientific paper

THE kinematic stability of a planetoid orbiting in permanent sextile configuration with two other attracting centres, for which the ratio of the larger to the smaller mass exceeds 25, is well established. Indeed, the Trojan asteroids, the elongation from their theoretical libration points of which is sometimes considerable, do certainly not appear to exhibit the catastrophic instability predicted by Colombo's non-linear model.

Affiliated with

Also associated with

No associations

Rating

Instability of Motion at the Lagrangian Triangular Point in the Earth-Moon System 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 Instability of Motion at the Lagrangian Triangular Point in the Earth-Moon System, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Instability of Motion at the Lagrangian Triangular Point in the Earth-Moon System will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1054080