Analysis of the bimodal light curve generated using photometric data show a lengthy rotation period of 433.2 ± 0.5 hours (18.05 ± 0.02 days) with a brightness variation of 0.35±0.05 in magnitude. It also appears to be tumbling.[6] 437 Rhodia is classified as an E-type asteroid with a diameter of approximately 13 km. This object has the highest albedo in the IRAS dataset, with a value of 0.70±0.08.[7]
References
^Noah Webster (1884) A Practical Dictionary of the English Language
^Pilcher, Frederick; Polakis, Tom (July 2018), "A Photometric Study of 437 Rhodia", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 45 (3): 287–289, Bibcode:2018MPBu...45..287P.