Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Orbital stability in the Solar System for arbitrary inclinations and
  eccentricities: planetary perturbations versus resonances   Applying the technique of dynamical maps we study the orbital stability of
test particles in the Solar System in the space (a,e,i) defined by 0.1<a<38 au,
0<e<0.9 and 0<i<180 identifying the unstable and stable regions. We find stable
niches where small bodies can survive even for very high eccentricities. Mean
motion resonances play a fundamental role providing stability against the
planetary perturbations specially for high inclination orbits. A stability
stripe around i=150 is present all along the Solar System. We found that the
population of objects with semimajor axes between 10 and 30 au is evolving
inside a highly unstable region according to our maps. For the inner Solar
System we found that the region between the Hildas and Jupiter is more stable
for high eccentricity orbits than for low eccentricity ones.

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The categories of this paper are: cs
24
The categories of this paper are: dg-ga
17
The categories of this paper are: q-fin
25
The categories of this paper are: patt-sol
37
The categories of this paper are: supr-con
27
The categories of this paper are: comp-gas
3
The categories of this paper are: physics
28
The categories of this paper are: alg-geom
32
The categories of this paper are: atom-ph
34
The categories of this paper are: chem-ph
23
The categories of this paper are: solv-int
22
The categories of this paper are: chao-dyn
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The categories of this paper are: nlin
31
The categories of this paper are: ao-sci
4
The categories of this paper are: cond-mat
29
The categories of this paper are: funct-an