Based upon photometry observations between 1984 and 2007, it has a sidereal rotation period of 8.283065 h with an amplitude that can range up to 0.34±0.01 in magnitude. The lightcurve shows some shape irregularities. There are two valid solutions for the pole's ecliptic coordinates: (λ1, β1) = (38°, +75°) and (λ2, β2) = (237°, +73°).[3]
References
^'Clytie, Clytia' in Benjamin Smith (1903) The Century Dictionary and Cyclopedia
^ abMarciniak, A.; et al. (February 2008), "Photometry and models of selected main belt asteroids. V. 73 Klytia, 377 Campania, and 378 Holmia", Astronomy and Astrophysics, 478 (2): 559–565, Bibcode:2008A&A...478..559M, doi:10.1051/0004-6361:20078930.
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