In the late 1990s, a network of astronomers worldwide gatheredlight curve data that was ultimately used to derive the spin states and shape models of 10 new asteroids, including (165) Loreley. The light curve of this asteroid varies by no more than 0.2 inmagnitude, while the derived shape model shows multiple flat spots on the surface.[4][6] The asteroid has an oblate shape with a size ratio of 1.26 ± 0.08 between the major and minor axes, as determined from theW. M. Keck Observatory.[7]
Between 2003 and 2021, 165 Loreley has been observed tooccult thirteen stars.
^Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project",The Minor Planet Bulletin, vol. 34, pp. 113–119,Bibcode:2007MPBu...34..113W.
^Durech, J.; et al. (November 2006), "Asteroid brightness and geometry",VizieR On-line Data Catalog: J/A+A/465/331,Bibcode:2006yCat..34650331D.