Photometric measurements during 2020–2021 was used to produce a light curve, which shows a rotation period of 49.353±0.004 h with a brightness variation of 0.26 in magnitude. This differs substantially from previous studies.[3]
^Bonamico, Roberto; van Belle, Gerard (July 2021), "Determining the Rotational Period of Main-Belt Asteroid 282 Clorinde", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, vol. 48, no. 3, p. 210, Bibcode:2021MPBu...48..210B.