Table 3
Results of a 5 Myr integration on transport to Phaethon, UD, and YC.
| (3200) Phaethon | (155140) 2005 UD | (225416) 1999 YC | ||
|---|---|---|---|---|
| % of arrived objects | ||||
| Orbit9 | (329) Svea | 56.6% | 42.1% | 17.5% |
| (142) Polana | 30.1% | 9.7% | 6.6% | |
| Rebound | (329) Svea | 19.20% | 17.20% | 14.60% |
| (142) Polana | 9.80% | 6.50% | 3.80% | |
| tfirst arrival (Kyr) | ||||
| Orbit9 | (329) Svea | 141.2 | 138.6 | 120.0 |
| (142) Polana | 90.5 | 322.0 | 282.3 | |
| Rebound | (329) Svea | 176.62 | 178.83 | 161.58 |
| (142) Polana | 115.11 | 123.11 | 124.59 | |
| tmedian (Myr) | ||||
| Orbit9 | (329) Svea | 1.253 | 1.323 | 1.319 |
| (142) Polana | 1.061 | 1.343 | 1.320 | |
| Rebound | (329) Svea | 1.296 | 1.435 | 1.490 |
| (142) Polana | 0.534 | 0.475 | 0.445 | |
Notes. The initial conditions are taken from the chaotic edges of the 3:1J resonance from Fig. 4. The table shows the percentage of arrived objects and their first and median arrival times to the three asteroids from the (329) Svea and (142) Polana families. The results are obtained with Orbit9 and Rebound/Mercurius. On average, the delivery of asteroids from the Polana orbital plane is somewhat faster but less effective regarding the number of transported bodies.
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