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Table 3
Osculating orbital elements obtained through the inversion of the harmonic terms fitted to the observational data (Table 2).
Tadpole | Horseshoe | |||
param. | planet 1 | planet 2 | planet 1 | planet 2 |
|
||||
m [M⊕] | 226.4 | 101.6 | 18.19 ** | 2.74 ** |
a [au] | 0.099 | 0.101 | 0.1002 | 0.0987 |
λ [deg] | 1.380 | 303.5 | 5.10 | 320.78 |
e | 0* | 0* | 0* | 0* |
ϖ [deg] | 0* | 0* | 0* | 0* |
I [deg] | 59.85 | 59.85 | 90* | 90* |
|
||||
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0.09948 | 0.09999 | ||
ζ0 [deg] | 38.01 | 18.5* | ||
δ | 0.3440 | 0.1309 |
Notes. The elements marked with
(*)
cannot be determined with the Keplerian circular orbit approximation (Eq. (18)), so they have been fixed at constant values.
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