Is this a quasi-Hilda object?
Clone Generation
100 clones were generated in order to have the same orbital paameters and uncertainty as the nominal asteroid
| Clones | Target | ||||
|---|---|---|---|---|---|
| mean | sd | mean | sd | ||
| q | 3.61245270083945 | 3.39064109921033e-07 | 3.61245264912673 | 3.4136e-07 | |
| e | 0.129667339794439 | 8.11352970562344e-08 | 0.12966735411561 | 8.0309e-08 | |
| i | 8.9645643748396 | 9.73657795759391e-06 | 8.96456457281582 | 9.6087e-06 | |
| peri | 344.487704195712 | 4.69757841212335e-05 | 344.487707120445 | 4.6654e-05 | |
| node | 359.469501444993 | 3.82226393976073e-05 | 359.469498781976 | 3.8729e-05 | |
| tp | 2461090.03289397 | 0.000262107424207425 | 2461090.03290289 | 0.00026503 | |
Backward Simulation
This was performed using Mercury Integrator Package Version 6 - Bulirsch-Stoer N-body algorithm - 10^8 days in the past - output every 100 days
66% of the clones entered the solar system from a distance greater than 100 AU (i.e. from the point of view of the backward simulation they were "ejected")
