881 Athene (prov. designation:A917 ODor1917 CL) is a stonybackground asteroid from the central region of theasteroid belt. It was discovered on 22 July 1917, by astronomerMax Wolf at theHeidelberg-Königstuhl State Observatory in southwest Germany.[1] The likely elongatedS/L-type asteroid has arotation period of 13.9 hours and measures approximately 12 kilometers (7.5 miles) in diameter. It was named afterAthena, the goddess of wisdom inGreek mythology.[3]According to Astrophysicist Rayme Traub at JHU APL NASA, Europa Clipper will make a pass by Athene in 2027 after passing Earth on its way to Jupiter. Europa Clipper will test its sensors on Athene in preparation for Europa in 2030.
In August 2006, a rotationallightcurve ofAthene was obtained fromphotometric observations by Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station (A12), Italy, and by Jean-Gabriel Bosch at the Collonges Observatory (178), France. Lightcurve analysis gave arotation period of13.895±0.003 hours with a high brightness variation of0.53±0.01magnitude, indicative of a non-spherical, elongated shape (U=3−). In September 2010, French amateur astronomerRené Roy measured a similar period of13.881±0.001 hours and an amplitude of0.39±0.02 (U=2+).[12][11]
Two lightcurves, published in 2016, using modeled photometric data from the Lowell Photometric Database (LPD) and other sources, gave a concurring sidereal period of13.89449±0.00001 and13.8943±0.0005 hours, respectively. Each modeled lightcurve also determined twospin axes of (123.0°, −58.0°) and (337.0°, −47.0°), as well as (115.0°, −77.0°) and (338.0°, −43.0°) inecliptic coordinates (λ, β).[6][13][14]
According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Athene measures (12.04±0.28) and (12.153±0.101) kilometers in diameter and its surface has analbedo of (0.237±0.012) and (0.237±0.039), respectively.[7][8] TheCollaborative Asteroid Lightcurve Link assumes a standard Eunomian albedo of 0.21 and calculates a diameter of 12.66 kilometers based on anabsolute magnitude of 11.8.[11] Alternativemean diameter measurements published by the WISE team include (12.152±2.176 km), (12.369±0.285 km) and (12.671±0.077 km) with corresponding albedos of (0.278±0.128), (0.241±0.044) and (0.2111±0.0234).[6][11]
^abcUsui, 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)
^abcMasiero, 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.