Table 1: Initial orbital elements and evolution of case-study objects. Notes: Columns are, from left: Object designation; initial orbital elements (epoch is JD 2 452 120.5); number of approaches within the Hill spheres of Mercury and Venus; time until achievement of Venus crossing orbit; time until first Venus close approach; lifetime; note ("CO'' means collision). Data from integration 4.
Object a e i $\omega$ $\Omega$ M $N_{\rm Me}$ $N_{\rm Ve}$ $T_{\rm VCO}$ $T_{\rm VCA}$ $T_{\rm int}$ Note
  (AU)   ( $\hbox{$^\circ$ }$) ( $\hbox{$^\circ$ }$) ( $\hbox{$^\circ$ }$) ( $\hbox{$^\circ$ }$)     (Myr) (Myr) (Myr)  
38 0.3784229 0.1945032 7.20561 26.88380 47.82560 12.86873 1763 1 1.38 1.6 1.6 Venus CO
60 0.3952884 0.2177328 6.96164 31.95132 43.96596 7.37471 1080 587 0.056 4.9 11.0 Int. aborted
91 0.3651101 0.1603426 7.47004 26.93263 49.79761 12.39453 726 4502 0.076 4.9 11.0 Int. aborted. Fig. 1
96 0.3655905 0.1638854 6.80923 30.54178 44.94961 9.15255 2984 0 - - 6.0 Mercury CO
134 0.3775369 0.1924173 6.77262 23.02849 47.98355 11.55416 289 0 - - 0.11 Mercury CO

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