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Fig. 21

image

Perihelion distance as a function of time under action of EFE for the known population of trans-Neptunian bodies, with a> 150 au and q> 30 au. , and a0 = 8.1 × 10-11 m s-2 were used instead of and a0 = 1.2 × 10-10 m s-2, as in Fig. 16. Thick solid lines are 2012 VP113 and Sedna.

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