A firstprecovery was taken at Yerkes Observatory, extending the Algeria'sobservation arc by just 16 days prior to its official discovery observation.[13]
The dark asteroid orbits the Sun in theouter main-belt at a distance of 2.7–3.5 AU once every 5 years and 7 months (2,035 days). Its orbit has aneccentricity of 0.13 and aninclination of 13° with respect to theecliptic.[1]
A rotationallightcurve of Algeria was obtained from photometric observations made by French amateur astronomerClaudine Rinner in August 2002. Lightcurve analysis gave arotation period of 16 hours with a brightness variation of 0.19magnitude (U=2).[11]
According to the space-based surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Algeria measures between 29.2 and 34.5 kilometers in diameter and its surface has analbedo in the range of 0.057 to 0.093.[4][5][7][9][8][10]
TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.059 and a diameter of 33.1 kilometers with anabsolute magnitude of 11.1, and characterizes it as aC-type asteroid.[3]
^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)