Fig. 2
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Distribution of the final heliocentric distance (left) and eccentricities (right) of comet C/1908 R1’s clones from Model 1 at the end of the −1 Myr simulation. The average eccentricity is 1.16 ± 0.27, with a median value of 1.07, meaning this comet likely had a hyperbolic orbit. The average heliocentric distance is (8.6 ±2.8) × 104 au.
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