Table 1
Close encounters for S5a (top) and S5b (bottom).
| Te (Myr) | δH × 1013 | A1 | A2 | Δ (AU) |
|
|
||||
| −2.3065 | 4.1 | 1 | 7 | 2.22E − 04 |
| −61.9215 | 10.4 | 1 | 4 | 2.34E − 04 |
| −93.9535 | −3.8 | 2 | 4 | 8.94E − 04 |
|
|
||||
| −6.4985 | 18.8 | 1 | 4 | 3.99E − 04 |
| −20.9295 | −3.8 | 2 | 4 | 7.42E − 04 |
| −40.7115 | 4.0 | 2 | 4 | 9.72E − 04 |
| −55.6035 | −2.5 | 2 | 4 | 1.14E − 03 |
| −59.0680 | −7.2 | 1 | 2 | 7.08E − 04 |
| −71.8610 | −3.4 | 1 | 2 | 6.02E − 04 |
| −90.4210 | −2.5 | 1 | 2 | 1.12E − 03 |
| −93.1865 | 12.0 | 1 | 4 | 4.34E − 04 |
| −97.8895 | 4.1 | 1 | 2 | 9.68E − 04 |
Notes. Te: date of the encounter; δH: planetary relative variation in energy; A1,A2: involved asteroids; Δ: distance of closest approach. Compare to the Hill radii RH (Table 3).
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