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Table 2
Orbital elements (a-e-i) and 10 kyr simulation results for three very bright fireballs reported to be originating from the JFC population observed by the Spanish Meteor Netork (SPMN) and the Spalding Allsky Camera Network (SACN).
| Network | a (au) | e | ι(°) | % of clones q > 2.5 | fq | fa | Ref. |
|---|---|---|---|---|---|---|---|
| SPMN | 4.3 ± 0.7 | 0.79 ± 0.04 | 7.1 ± 0.1 | 17.3 | 0.07 | 0.08 | Madiedo et al. (2014) |
| SPMN | 2.89 ± 0.27 | 0.737 ± 0.024 | 29.9 ± 0.6 | 18.9 | 0.05 | 0.03 | Trigo-Rodríguez et al. (2009) |
| SACN | 3.58 ± 0.02 | 0.725 ± 0.002 | 9.06 ± 0.02 | 39.7 | 0.15 | 0.08 | Hughes et al. (2022) |
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