Table 3.
Relative angle between the total angular momentum vectors of the Sun-planets system and the minor planets.
| Population | α1(°) | α2(°) |  |
 |
|---|---|---|---|---|
| NEOs+MBAs+JTs+TSCs | 14.7449 | 1.7635 | 1.8020 | – |
| TSCs | 14.9210 | 1.8218 | 1.8612 | – |
| TNOs | 9.7645 | 1.9105 | 1.9651 | – |
| SDOs | 29.1900 | 4.6759 | 4.6861 | – |
| MBAs | 3.0922 | 3.0922 | 3.1165 | 3.0947 |
| JTs | 3.1107 | 3.1107 | 3.4876 | 3.1541 |
Notes. α1 and α2 are for the cases with and without the three dwarf planets Eris, Pluto, and Haumea, respectively. The last two columns refer to the changed values of α2 by taking into account some uncertainties, as we will illustrate in Sect. 3.2.
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