Nofretete is a non-family asteroid from the main belt's background population.[4] It orbits the Sun in the outer asteroid belt at a distance of 2.6–3.2 AU once every 4 years and 12 months (1,810 days; semi-major axis of 2.91 AU). Its orbit has an eccentricity of 0.10 and an inclination of 5° with respect to the ecliptic.[1] The body's observation arc begins at Uccle in September 1926, three nights after its official discovery observation.[11]
In May 1984, a rotational lightcurve of Nofretete was obtained from photometric observations by Richard Binzel which gave a rotation period of 6.15 hours with a low brightness amplitude of 0.04 magnitude, indicative for a nearly spheroidal shape (U=2).[9]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 22.03 kilometers based on an absolute magnitude of 10.65.[3]
^ abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
^ abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)