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(9928) 1981 WE9

From Wikipedia, the free encyclopedia
Asteroid
(9928)1981 WE9
Discovery[1]
Discovered byPerth Obs.
Discovery sitePerth Obs.
Discovery date16 November 1981
Designations
(9928)1981 WE9
1981 WE9 · 1971 TJ1
1993 FC43
main-belt[1][2] · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc65.74 yr (24,012 days)
Aphelion2.6101AU
Perihelion1.8246 AU
2.2174 AU
Eccentricity0.1771
3.30yr (1,206 days)
340.29°
0° 17m 54.6s / day
Inclination2.8472°
179.45°
176.04°
Physical characteristics
Dimensions2.441±0.327 km[4]
2.938±0.660 km[5]
3.00±0.42 km[6]
3.11 km(calculated)[3]
5.547±0.005h[7]
18.310±0.0034 h[8]
18.3980±0.0034 h[3][8]
0.24(assumed)[3]
0.283±0.152[6]
0.3557±0.2289[5]
0.428±0.109[4]
S[3]
14.4[5] · 14.60[4][6] · 14.7[1][3]

(9928) 1981 WE9, provisional designation1981 WE9, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 3 kilometers in diameter. It was discovered on 16 November 1981, by astronomers atPerth Observatory in Bickley, Australia.[2]

Orbit and classification

[edit]
Orbit of1981 WE9 (blue), with theinner planets andJupiter

The stonyS-type asteroid is a member of theFlora family, one of the largest groups of asteroids in the main-belt. It orbits the Sun at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,206 days).

Its orbit has aneccentricity of 0.18 and aninclination of 3° with respect to theecliptic.[1] A firstprecovery was taken atPalomar in 1951, extending the body'sobservation arc by 30 years prior to its official discovery observation at Bickley.[2]

Physical characteristics

[edit]

In December 2014, astronomer Maurice Clark obtained a rotationallightcurve from photometric observations at Preston Gott Observatory. Lightcurve analysis gave an ambiguousrotation period of 18.3980 hours with a brightness variation of 0.41magnitude, suggesting a non-spheroidal shape (U=2+). The alternative period solution is 9.14 hours with an amplitude of 0.32 magnitude.[8] The results supersede a previously obtained period of 5.547 hours (U=2).[7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures between 2.44 and 3.00 kilometers in diameter, and its surface has analbedo between 0.283 and 0.428.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – derived from8 Flora, the largest member and namesake of this asteroid family – and calculates a diameter of 3.11 kilometers with anabsolute magnitude of 14.7.[3]

Numbering and naming

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Thisminor planet wasnumbered by theMinor Planet Center on 2 February 1999.[9] As of 2018, it has not beennamed.[2]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 9928 (1981 WE9)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved26 May 2017.
  2. ^abcd"9928 (1981 WE9)".Minor Planet Center. Retrieved17 March 2017.
  3. ^abcdefg"LCDB Data for (9928)". Asteroid Lightcurve Database (LCDB). Retrieved17 March 2017.
  4. ^abcdNugent, 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.
  5. ^abcdMainzer, 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.
  6. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8.
  7. ^abClark, Maurice (June 2008). "Asteroid Lightcurves from the Chiro Observatory".The Minor Planet Bulletin.35 (2):42–43.Bibcode:2008MPBu...35...42C.ISSN 1052-8091.
  8. ^abcClark, Maurice (July 2015). "Asteroid Photometry from the Preston Gott Observatory".The Minor Planet Bulletin.42 (3):163–166.Bibcode:2015MPBu...42..163C.ISSN 1052-8091.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved24 February 2018.

External links

[edit]
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