Photometric observations of the minor planet in 2011 gave arotation period of10.945±0.001 h with anamplitude of0.09±0.01 in magnitude. This result is consistent with previous determinations.[5] Two stellar occultation events involving this asteroid were observed from multiple sites in 2009. The resulting chords matched a smooth elliptical cross-section with dimensions of134.0±4.0 km ×108.9±0.7 km.[6]
^Tempel, M. (November 1864), "Minor Planet 81 Terpsichore discovered",Monthly Notices of the Royal Astronomical Society,25: 31,Bibcode:1864MNRAS..25...31T.
^Pilcher, Frederick (July 2011), "Rotation Period Determinations for 28 Bellona, 81 Terpsichore, 126 Velleda 150 Nuwa, 161 Athor, 419 Aurelia, and 632 Pyrrha",The Minor Planet Bulletin,38 (3): 156−158,Bibcode:2011MPBu...38..156P.
^Timerson, Brad; Durech, J.; Pilcher, F.; et al. (October 2010), "Occultations by 81 Terpsichore and 694 Ekard in 2009 at Different Rotational Phase Angles",The Minor Planet Bulletin,37 (4): 140−142,Bibcode:2010MPBu...37..140T.