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9000 Hal

From Wikipedia, the free encyclopedia
Main-belt asteroid
This article is about the real-life asteroid. For the fictional computer in2001: A Space Odyssey, seeHAL 9000.

9000 Hal
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date3 May 1981
Designations
(9000) Hal
Pronunciation/ˈhæl/
Named after
HAL 9000[1]
(Fictionalsupercomputer)
1981 JO · 1975 VH3
1981 JJ3 · 1995 US3
main-belt[1][2] · (inner)
background[3] · Flora[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc41.49yr (15,156 d)
Aphelion2.6955AU
Perihelion1.7648 AU
2.2301 AU
Eccentricity0.2087
3.33 yr (1,216 d)
328.38°
0° 17m 45.24s / day
Inclination6.2618°
226.61°
79.871°
Physical characteristics
3.61±0.78 km[5]
4.11 km(calculated)[4]
4.134±0.935 km[6][7]
22.68±0.02 h(poor)[8]
908 h[9]
0.24(assumed)[4]
0.26±0.13[5]
0.375±0.184[6][7]
S(assumed)[4]
13.6[7]
14.0[2]
14.1[4]
14.35±0.66[10]
14.42[5]

9000 Hal, provisional designation1981 JO, is a stony backgroundasteroid andslow rotator from the inner regions of theasteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 3 May 1981, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station near Flagstaff, Arizona, in the United States.[1] The likely elongatedS-type asteroid has an exceptionally longrotation period of 908 hours.[4] It was named after the fictional supercomputerHAL 9000, featured in the 1968 film2001: A Space Odyssey.[1]

Orbit and classification

[edit]

Hal is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[3] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[4]

Hal orbits the Sun in theinner asteroid belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,216 days;semi-major axis of 2.23 AU). Its orbit has aneccentricity of 0.21 and aninclination of 6° with respect to theecliptic.[2] The asteroid was first observed as1975 VH3 atCrimea–Nauchnij in November 1975. The body'sobservation arc begins with its official discovery observation at Anderson Mesa in May 1981.[1]

Physical characteristics

[edit]

Hal is an assumed stonyS-type asteroid, based on theCollaborative Asteroid Lightcurve Link's (CALL) classification into the Flora family.[4]

Rotation period

[edit]

In August 2008, a rotationallightcurve of Hal was obtained fromphotometric observations by Slovak astronomersAdrián Galád,Jozef Világi,Leonard Kornoš andŠtefan Gajdoš atModra Observatory.[9] Lightcurve analysis gave an exceptionally longrotation period of 908 hours with a high brightness variation of 0.9magnitude (U=2+). This makes Halone of the slowest rotators known to exist. In addition, the body's high brightness amplitude is indicative of a non-spherical shape.

An alternative measurement by French amateur astronomersPierre Antonini andRené Roy gave a much shorter period of 22.68 hours.[8] The result, however, is considered of poor quality by CALL (U=1).[4]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Hal measures between 3.61 and 4.134 kilometers in diameter and its surface has analbedo between 0.26 and 0.375.[5][6][7] CALL assumes an albedo of 0.24 – derived from8 Flora, the Flora family'sparent body – and calculates a diameter of 4.11 kilometers based on anabsolute magnitude of 14.1.[4]

Naming

[edit]

Thisminor planet was named after the fictional and homicidal supercomputerHAL 9000, featured in bothArthur C. Clarke's novel andStanley Kubrick's film2001: A Space Odyssey (1968).[1] HAL stands forHeuristically programmed Algorithmic computer. It is one of the best-knownartificial intelligence characters in modern movies. The official naming citation was published by theMinor Planet Center on 4 May 1999 (M.P.C. 34628).[11] The asteroid4923 Clarke and10221 Kubrick were named after the writer and film director, respectively.

References

[edit]
  1. ^abcdefg"9000 Hal (1981 JO)".Minor Planet Center. Retrieved16 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 9000 Hal (1981 JO)" (2017-05-01 last obs.).Jet Propulsion Laboratory. Retrieved16 May 2018.
  3. ^ab"Asteroid 9000 Hal".Small Bodies Data Ferret. Retrieved15 May 2018.
  4. ^abcdefghij"LCDB Data for (9000) Hal". Asteroid Lightcurve Database (LCDB). Retrieved16 May 2018.
  5. ^abcdNugent, 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.
  6. ^abcMasiero, 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.S2CID 118745497.
  7. ^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.S2CID 35447010. (catalog)
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (9000) Hal". Geneva Observatory. Retrieved16 May 2018.
  9. ^abGalad, Adrian; Vilagi, Jozef; Kornos, Leonard; Gajdos, Stefan (July 2009). "Relative Photometry of Nine Asteroids from Modra".The Minor Planet Bulletin.36 (3):116–118.Bibcode:2009MPBu...36..116G.ISSN 1052-8091.
  10. ^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.S2CID 53493339.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved16 May 2018.

External links

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