7517 Alisondoane, provisional designation 1989 AD, is a carbonaceous asteroid from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 3 January 1989, by Japanese amateur astronomer Takuo Kojima at the YGCO Chiyoda Station in the northern Kantō region of Japan.
Orbit and classification [ ]
Alisondoane orbits the Sun in the inner main-belt at a distance of 1.8–3.1 AU once every 3 years and 10 months (1,397 days). Its orbit has an eccentricity of 0.26 and an inclination of 6 ° with respect to the ecliptic.
Physical characteristics [ ]
Alisondoane has been characterized as a carbonaceous C-type asteroid by PanSTARRS photometric survey.
Lightcurves [ ]
lightcurve analysis by Czech astronomer Petr Pravec in 2007 rendered a rotation period of hours with a high brightness amplitude of 1.13 in 9.701 ±0.001 magnitude ( ). U=3
Diameter and albedo [ ]
According to the surveys carried out by the Japanese
Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Alisondoane measures between 8.52 and 9.99 kilometers in diameter and its surface has an albedo between 0.04 and 0.122.      The  Collaborative Asteroid Lightcurve Link (CALL) calculates a smaller diameter of 5.16 kilometers based on an assumed albedo of 0.18 for a X-type asteroid. 
Naming [ ]
minor planet was named in honor of Alison Doane (1958-2017), Curator of Astronomical Photographs at the Harvard College Observatory. She was also principal oboe with the Boston Philharmonic Orchestra from 1982 to 2001. The official naming citation was published by the  Minor Planet Center on 25 December 2015 ( ). M.P.C. 97567
Notes [ ]
^ a b Pravec (2007): rotation period
hours with a brightness amplitude of 9.701 ±0.001 mag. CALL assigns a "Quality Code" of 3, which denotes a secure result within the precision given and no ambiguity. Summary figures for (7517) Alisondoane at 1.13 Collaborative Asteroid Lightcurve Link (CALL)
^ a b c Summary Notes by the LCDB: "The Masi et al. paper gave this as a C-type on the basis of a neutral spectrum. However, given its location in the inner main belt, we adopted class X and a Pv = 0.18"
References [ ]
^ a b c d
"JPL Small-Body Database Browser: 7517 Alisondoane (1989 AD)" (2017-05-05 last obs.). Jet Propulsion Laboratory . Retrieved . 22 June 2017
Schmadel, Lutz D. (2007). "(9448) Donaldavies". Dictionary of Minor Planet Names – (9448) Donaldavies. Springer Berlin Heidelberg. p. 692. doi: 10.1007/978-3-540-29925-7_7518. ISBN . 978-3-540-00238-3
^ a b c d e f
"LCDB Data for (7517) Alisondoane". Asteroid Lightcurve Database (LCDB) . Retrieved . 7 February 2016
^ a b c d
Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv: . 1509.02522 Bibcode: 2015ApJ...814..117N. doi: 10.1088/0004-637X/814/2/117 . Retrieved . 11 March 2017
^ a b c d
Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: . 1109.6407 Bibcode: 2011ApJ...741...90M. doi: 10.1088/0004-637X/741/2/90.
^ a b c
Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal. 741 (2): 20. arXiv: . 1109.4096 Bibcode: 2011ApJ...741...68M. doi: 10.1088/0004-637X/741/2/68 . Retrieved . 11 March 2017
^ a b c d
Alí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics. 591: 11. Bibcode: 2016A&A...591A..14A. doi: 10.1051/0004-6361/201527660 . Retrieved . 11 March 2017
^ a b c d
Usui, 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 . Retrieved . 17 October 2019 ( online, AcuA catalog p. 153)
^ a b c d
Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv: . 1606.08923 Bibcode: 2016AJ....152...63N. doi: 10.3847/0004-6256/152/3/63 . Retrieved . 11 March 2017
^ a b c
Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv: . 1506.00762 Bibcode: 2015Icar..261...34V. doi: 10.1016/j.icarus.2015.08.007 . Retrieved . 11 March 2017
^ a b
"7517 Alisondoane (1989 AD)". Minor Planet Center . Retrieved . 7 February 2016
"MPC/MPO/MPS Archive". Minor Planet Center . Retrieved . 11 March 2017
External links [ ]