Based uponphotometric observations made between 2010 and 2014, this asteroid has a rotation period of 21.812 ± 0.001 hours and a brightnessvariation of 0.08 ± 0.01 inmagnitude. Atopposition, theabsolute magnitude was measured at 7.45 ± 0.01. It displays a hemispheric albedo dichotomy similar to that on4 Vesta.[4]
As of 17 September 2020, there have been thirteen observedoccultations of stars by Eunike.
^abcPilcher, Frederick; et al. (October 2014), "A Comprehensive Photometric Investigation of 185 Eunike",of the Minor Planets Section of the Association of Lunar and Planetary Observers,41 (4):244–250,Bibcode:2014MPBu...41..244P.