Abstract
The dynamics of a very young compact asteroid cluster associated with asteroid 39991 Iochroma is studied. It is shown that Iochroma family lies between the two three body resonances 3J-1M-3 and 5J 3S-2. In this paper we have determined the position of these resonances and the boundary between them. We have included the orbital elements approximations which may be useful in the future study of the dynamics of the family. Additionally, we report on a new candidate member, namely asteroid 2016 UT3.
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