Fig. 8
Cumulative distribution of the cosine of obliquity cosγ from the converging clones of six small Adelaide members in our experiment. The asteroids in box B (2015 TD44, 2016 CX104 and 2016 GO11) are in the left panel; the asteroids in box A ((452 322) 2000 GG121, 2014 JY105 and 2015 RM186) are in the right panel. The dominantly negative values of cos γ (e.g. 2015 TD44 or 2016 CX104) imply a retrograde rotation and migration towards the Sun, while the opposite tendency (e.g. 2014 JY105) implies a prograde rotation and migration away from the Sun.
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