| Many asteroids have been observed around the triangular Lagrangian points (L4 and L5) of Jupiter, but none around Saturn's where they are difficult to observe. Hence, a study of their orbital stability would focus future searches, or place constraints on the last phases of Solar system formation.;I numerically integrated orbits around the L4 and L5 points of Jupiter (Trojans) and Saturn ("Bruins"): 40 Trojans and 350 Bruins, all of inclination less than 12;While Bruins of small libration angle went unstable, no unstable region was found around Jupiter's triangular Lagrangian points, and stable Trojans may have longitudes of perihelion that either circulate or librate with respect to Jupiter's, with proper eccentricities as much as an order of magnitude larger than those for the Bruins.;A major contributor to Bruins going unstable near L4 and L5 is the presence of three separatrices of motion caused, in part, by the Great Inequality (GI) between Jupiter and Saturn. The GI separatrices drive up the eccentricity of Bruins on small tadpole orbits, but have much less effect on large tadpole orbits (like the four long-lived Bruins). |
