http://arxiv.org/abs/1807.07956
In the framework of the circular restricted three body problem we show that the numerically computed strength SR(e,i,w) is a good indicator of the strength and width of the mean-motion resonances in the full space (e,i,w). We present a survey of strengths in the space (e,i) for typical interior and exterior resonances. The resonance strength is highly dependent on (e,i,w) except for exterior resonances of the type 1:k for which the dependence with (i,w) is softer. Such resonances are thus strong even for retrograde orbits. All other resonances are weaker at very-high eccentricities for w ~ 90 or 270 and 60 < i < 120. We explore the resonance structure in the space (a,i) by means of dynamical maps and we find structures similar to those of space (a,e).
T. Gallardo
Mon, 23 Jul 18
48/48
Comments: N/A
You must be logged in to post a comment.