Astronoomid on kümne tuhande valgusaasta kauguselt leidnud esimese mitmikplaneedisüsteemi, mille kolm planeeti tiirlevad oma kodutähe ümber sama korrapärastel orbiitidel kui Päikesesüsteemi planeedid.
The fraction of regular orbits obtained by the NAFF method strongly depends on the critical frequency drift parameter, while in the CA method the number of fundamental frequencies strongly depends on the frequency difference parameter Lr and the maximum integer used for searching the linear independence of the fundamental frequencies.
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