Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991cemda..51...75p&link_type=abstract
Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 51, no. 1, 1991, p. 75-81.
Astronomy and Astrophysics
Astronomy
6
Celestial Mechanics, Lagrangian Equilibrium Points, Orbital Mechanics, Periodic Functions, Three Body Problem, Jupiter (Planet), Motion Stability, Orbit Calculation, Solar System
Scientific paper
The vertical stability character of the families of short and long period solutions around the triangular equilibrium points of the restricted three-body problem is examined. For three values of the mass parameter less than equal to the critical value of Routh mu(R), i.e., for mu = 0.000953875 (sun-Jupiter), mu = 0.01215 (earth-moon) and mu = mu(R) = 0.038521, it is found that all such solutions are vertically stable. For mu above mu(R), vertical stability is studied for a number of 'limiting' orbits extended to mu = 0.45. The last limiting orbit computed by Deprit for mu = 0.044 is continued to a family of periodic orbits into which the well known families of long and short period solutions merge. The stability characteristics of this family are also studied.
Perdios E.
Zagouras C. G.
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