With an absolute magnitude of 11.7,[2] the asteroid is about 12–27 km in diameter.[3] It is classified as a stony Sk[5] or Sq-type[2] asteroid in the SMASS taxonomy. Photometry data used to produce light curves provide a rotation period of 3.39624±0.00006 h. The lightcurve inversion method was used to build a shape model with a rounded form and an equatorial bulge.[6]
References
^Noah Webster (1884) A Practical Dictionary of the English Language
^Angeli, C. A.; Lazzaro, D. (August 2002), "Spectral properties of Mars-crossers and near-Earth objects. Results of the S3OS2 survey", Astronomy and Astrophysics, 391: 757–765, Bibcode:2002A&A...391..757A, doi:10.1051/0004-6361:20020834.
^Alonso, E. Díez; et al. (April 2021), "Asteroids 4092 Tyr (Follow Up, Analysis, Preliminary Results) and 699 Hela (Spin-Shape Model)", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 48 (2): 136–139, Bibcode:2021MPBu...48..136A.