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Carina is a nearby young stellar association. So far, only a small number ofstars have been clearly identified as members of this association. In thispaper we reanalyse the membership of the association in light of Gaia DR2 data,in particular finding that HD 95086 is a potential member (probability of 71%).This star is noteworthy as one of the few stars that hosts both a detecteddebris disc and a directly imaged planet. It has previously only beenconsidered as a potential member of the Lower Centaurus Crux (LCC) - part ofthe Scorpius-Centaurus association. We also reanalyse the age of the Carinaassociation. Using a Bayesian inference code applied to infer a solution fromstellar evolution models for the most probable (>99%) members of Carina, weinfer an age for the association of 13.3$^{+1.1}_{-0.6}$ Myr, much younger thanprevious studies. Whilst we have revised HD 95086's association membership fromLCC to Carina, the fact that we also find Carina to have a younger age, similarto that of LCC, means that the estimates of HD 95086b's mass remain unchanged.However, the younger age of Carina does mean that the companion to anotherCarina member, HD 44627 (or AB Pic), has a mass that is more clearly in theplanet rather than brown dwarf range.

The Age of the Carina Young Association and Potential Membership of HD 95086