Arago orbits the Sun in theouter main-belt at a distance of 2.8–3.5 AU once every 5 years and 8 months (2,058 days). Its orbit has aneccentricity of 0.12 and aninclination of 19° with respect to theecliptic.[1] The asteroid'sobservation arc begins atUccle Observatory in 1935, twelve years after its official discovery observation at Simeiz.[12]
According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer (WISE) with its subsequentNEOWISE mission,Arago measures between 48.57 and 68.404 kilometers (30.180 and 42.504 mi) in diameter and its surface has analbedo between 0.0498 and 0.08.[4][5][6][7][8][10] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0582 and a diameter of 57.69 kilometers (35.85 mi) based on anabsolute magnitude of 9.9.[3]
In October 2010, a rotationallightcurve ofArago was obtained from photometric observations that was later submitted to the CALL website. Lightcurve analysis gave arotation period of 8.7819 hours with a brightness amplitude of 0.22magnitude (U=n.a.).[a] In April 2016, another lightcurve was obtained by the group of Spanish amateur astronomers OBAS. It gave a concurring period of 8.784 hours with an amplitude of 0.22 magnitude (U=3).[11]
^abCALL (2002): Submitted observations to the CALL website with a rotation period8.7819±0.0001 hours with a brightness amplitude of0.22 mag. Summary figures for (1005) Arago atCollaborative Asteroid Lightcurve Link (CALL)