Photometric observations taken in 2018 provided a light curve showing a synodic rotation period of 6.916±0.001 h for the asteroid with an amplitude of 0.20±0.02 in magnitude. This result is mostly consistent with previous measurements.[3]
The spectrum of 289 Nenetta reveals the strong presence of the mineral olivine, a relative rarity in the asteroid belt.[4]
^Pilcher, Frederick (October 2018), "New Lightcurves of 33 Polyhymnia, 49 Pales, 289 Nenetta 504 Cora, and 821 Fanny", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 45 (4): 356–359, Bibcode:2018MPBu...45..356P.
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