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Table 2
Largest convergence of orbits of real meteors found from three filaments (fils. F1 to F3) of the C/1917 F1 stream.
| fil. | IC | q | e | ω | Ω | i | D |
| [AU] | [1] | [deg] | [deg] | [deg] | |||
|
|
|||||||
| F1 | 118490 | 0.313 | 0.993 | 34.3 | 215.5 | 56.7 | |
| F2 | 49303 | 0.442 | 0.977 | 32.7 | 214.9 | 58.8 | 0.140 |
|
|
|||||||
| F1 | 118490 | 0.313 | 0.993 | 34.3 | 215.5 | 56.7 | |
| F3 | 112248 | 0.317 | 0.988 | 41.1 | 212.6 | 56.8 | 0.099 |
Notes. IC is the identification code of a meteor in the SonotaCo video database; q, e, ω, Ω, and i are the orbital elements from September 26.5, 28005 B.C., when the similarity occurred.
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