It was discovered on 7 January 1976, at thePalomar Observatory by American astronomerEleanor Helin,[2] who was the principal scientist for theNEAT project until her retirement in 2002. TheS-type asteroid measures approximately 900 meters in diameter, has a longer-than averagerotation period of 44.77 hours, and approaches the orbit Earth to 44.1lunar distances.
Aten orbits the Sun at a distance of 0.8–1.1 AU once every 11 months (347 days). Its orbit has aneccentricity of 0.18 and aninclination of 19° with respect to theecliptic.[1] A firstprecovery was taken at the discovering observatory in December 1955, extending the body'sobservation arc by more than 20 years prior to its official discovery observation.[2]
Aten was the first asteroid found to have asemi-major orbital axis of less than oneastronomical unit and a period of less than one year.[3] A new category of asteroids was thus created, theAtens. As of 2017, the group consists of more than 1,200 numbered members. Other groups of near-Earth objects (NEOs) are theApollo andAmor asteroids, which are both significantly larger than the Atens, while theAtira asteroids form the smallest NEO-group by far.[13]
In the 1990s, Italian astronomerStefano Mottola obtained a rotationallightcurve ofAten during the EUNEASO survey atLa Silla, which was a European near-Earth object search and follow-up observation program to determine additional physical parameters. Lightcurve analysis gave a longer-than averagerotation period of 40.77 hours with a brightness variation of 0.26magnitude (U=2).[9] No additional lightcurves have been obtained since.[12]
According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Aten measures between 700 and 830 meters in diameter and its surface has a highalbedo between 0.39 and 0.52.[4][5]
in 1994,Tom Gehrels published a diameter of 1.1 kilometers and an albedo of 0.26 in his bookHazards Due to Comets and Asteroids.[1][7] The Warm Spitzer NEO survey ("ExploreNEOs") gives a diameter of 1.3 kilometers with an albedo of 0.20.[8]
TheCollaborative Asteroid Lightcurve Link agrees with a revised thermal model for asteroid diameters and albedos, and adopts an albedo of 0.28 with a diameter of 0.91 kilometers based on anabsolute magnitude of 17.2.[6][12] However, theMinor Planet Center (MPC) classifiesAten as a larger (greater than 1 km) object.[2]
^abcMottola, S.; de Angelis, G.; di Martino, M.; Erikson, A.; Harris, A. W.; Hahn, G.; et al. (March 1995). "The EUNEASO Photometric Follow-up Program".Abstracts of the Lunar and Planetary Science Conference.26: 1003.Bibcode:1995LPI....26.1003M.