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4151 Alanhale

From Wikipedia, the free encyclopedia
Carbonaceous main-belt asteroid

4151 Alanhale
Discovery[1]
Discovered byC. S. Shoemaker
E. M. Shoemaker
Discovery sitePalomar Obs.
Discovery date24 April 1985
Designations
(4151) Alanhale
Named after
Alan Hale(astronomer)[2]
1985 HV1 · 1968 HD
1976 SO1 · 1979 FX1
1982 SZ4 · 1985 JX
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc48.95 yr (17,878 days)
Aphelion3.5904AU
Perihelion2.7017 AU
3.1461 AU
Eccentricity0.1412
5.58yr (2,038 days)
346.46°
0° 10m 35.76s / day
Inclination1.0079°
67.051°
75.088°
Physical characteristics
Dimensions15.37 km(calculated)[3]
19.526±0.269 km[4][5]
22.66±0.59 km[6]
11.9177±0.0047h[7]
0.045±0.006[5][6]
0.0734±0.0099[4]
0.08(assumed)[3]
C[3][8]
11.976±0.003(R)[7] · 12.0[4] · 12.20[6] · 12.3[1] · 12.43[3] · 12.78±0.21[8]

4151 Alanhale, provisional designation1985 HV1, is a carbonaceous Themistianasteroid from the outer region of theasteroid belt, approximately 19 kilometers in diameter. It was discovered by the American astronomer coupleCarolyn andEugene Shoemaker at the U.S.Palomar Observatory, California, on 24 April 1985.[9] It was named for American astronomerAlan Hale.[2]

Orbit and classification

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Alanhale is a member of theThemis family, a dynamical family of outer-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,038 days). Its orbit has aneccentricity of 0.14 and aninclination of 1° with respect to the ecliptic.[1] It was first identified as1968 HD atZimmerwald Observatory in 1968, extending the body'sobservation arc by 17 years prior to its official discovery observation at Palomar.[9]

Physical characteristics

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Alanhale has been characterized as a darkC-type asteroid byPanSTARRS' photometric survey.[3][8]

Rotation period

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A rotationallightcurve ofAlanhale was obtained from photometric observations made at the U.S.Palomar Transient Factory in October 2010. The fragmentary lightcurve gave arotation period of11.9177±0.0047 hours with a low brightness variation of 0.07 inmagnitude (U=1).[7]

Diameter and albedo

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According to the surveys carried out by NASA's spaced-basedWide-field Infrared Survey Explorer and its subsequentNEOWISE mission,Alanhale measures 19.5 and 22.7 kilometers in diameter, respectively, with a correspondingalbedo of 0.07 and 0.05.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a smaller diameter of 15.4 kilometers with anabsolute magnitude of 12.43.[3]

Naming

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Thisminor planet was named in honor of American astronomerAlan Hale (born 1958), co-discoverer ofcomet Hale–Bopp.[2]

His precise visual observations include more than 130 comets, several at more than one apparition, and both, magnitude estimates and confirmations of discoveries. He has also skillfully estimated the magnitudes of the near-Earth objects,4179 Toutatis and(99907) 1989 VA, and has performedasteroid occultation. Hale has promoted the study of small Solar System bodies in articles and in his astronomy lectures.[2] The official naming citation was published by theMinor Planet Center on 28 April 1991 (M.P.C. 18139).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 4151 Alanhale (1985 HV1)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(4151) Alanhale".Dictionary of Minor Planet Names – (4151) Alanhale.Springer Berlin Heidelberg. p. 355.doi:10.1007/978-3-540-29925-7_4123.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (4151) Alanhale". Asteroid Lightcurve Database (LCDB). Retrieved4 May 2016.
  4. ^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. Retrieved4 May 2016.
  5. ^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. Retrieved5 December 2016.
  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. Retrieved4 May 2016.
  7. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved4 May 2016.
  8. ^abcVeres, 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. Retrieved4 May 2016.
  9. ^ab"4151 Alanhale (1985 HV1)".Minor Planet Center. Retrieved4 May 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 May 2016.

External links

[edit]
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