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Fig. 10

image

Same as in Fig. 9 but now a vs time (top), and mean e vs. time (bottom). The mean semimajor axis of 495 Eulalia is 2.487 au, the mean eccentricity of 495 Eulalia is 0.129, both at the center of the respective zones delimited by black lines (their limits computed from excursions of the mean orbital elements of Eulalia’s clones as described in the text). Recall that the particles used in the simulation had 4 times smaller size than 495 Eulalia (10 km vs. 40 km); this means that the abscissa scale needs to be multiplied by a factor of 4 to interpret these results as potential past evolutionary tracks of 495 Eulalia.

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