Fig. 1

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Dynamical history of comet C/1908 R1 Morehouse (black) as estimated with 1000 clones from Model 1 using the MERCURY integrator (above, as presented in Anderson et al. 2023) and Model 2 using the REBOUND integrator (below). Clones with e < 1 at the end of the 1 Myr are shown in orange, and those with e > 1 are shown in blue. All clones reached the end of the 1 Myr integration.
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