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4606 Saheki

From Wikipedia, the free encyclopedia
Main belt asteroid

4606 Saheki
Lightcurve-based 3D-model ofSaheki
Discovery[1]
Discovered byT. Seki
Discovery siteGeisei Obs.
Discovery date27 October 1987
Designations
(4606) Saheki
Named after
Tsuneo Saheki(astronomer)[2]
1987 UM1 · 1972 GA1
1977 TJ7 · 1977 VF2
1982 FH4
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.81 yr (23,305 days)
Aphelion2.4805AU
Perihelion2.0231 AU
2.2518 AU
Eccentricity0.1016
3.38yr (1,234 days)
202.74°
0° 17m 30.12s / day
Inclination2.6338°
241.26°
251.92°
Physical characteristics
Dimensions6.655±0.069[4]
6.712±0.041 km[5]
7.14 km(calculated)[3]
4.969±0.003h[a]
4.97347±0.00005 h[6]
5.032±0.001 h[7]
0.24(assumed)[3]
0.3266±0.0245[5]
0.332±0.088[4]
S[3]
12.7[5] · 13.0[1][3] · 13.35±0.32[8]

4606 Saheki, provisional designation1987 UM1, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter.

The asteroid was discovered on 27 October 1987, by Japanese astronomerTsutomu Seki atGeisei Observatory, Japan.[9] It was later named after Japanese astronomerTsuneo Saheki.[2]

Classification and orbit

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Saheki is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,234 days). Its orbit has aneccentricity of 0.10 and aninclination of 3° with respect to theecliptic.[1] The firstprecovery was taken atPalomar Observatory in 1953, extending the asteroid'sobservation arc by 34 years prior to its discovery.[9]

Physical characteristics

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Rotation period

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In January 2009, a rotationallightcurve ofSaheki was obtained from photometric observations byDavid Higgins at Hunters Hill Observatory, Australia. Lightcurve analysis rendered a well-definedrotation period of4.969 hours with a brightness variation of 0.56 inmagnitude (U=3).[a]

Two months later, in March 2009, a second lightcurve was obtained at the Via Capote Observatory (G69), California. It gave a period of5.032 and an amplitude of 0.68 in magnitude (U=3-).[7]

Spin axis

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In 2013, an international study modeled a lightcurve with a concurring period of 4.97347 hours and found aspin axis of (44.0°, 59.0°) and (222.0°, 68.0°) inecliptic coordinates (λ, β), respectively (Q=2).[6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Saheki has a highalbedo of 0.33 and a diameter of 6.7 kilometers,[4][5] while theCollaborative Asteroid Lightcurve Link calculates a diameter of 7.1 kilometers, based on an assumed albedo of 0.24, derived from8 Flora, the Flora family's namesake and largest member.[3]

Naming

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Thisminor planet was named after Japanese astronomer and president of theToa Astronomical Society, Tsuneo Saheki (1916–1996). Over half a century, Saheki as gathered large inventory of observational data of the planet Mars.[2] The Martian craterSaheki is also named in his honour. The official naming citation was published by theMinor Planet Center on 28 May 1991 (M.P.C. 18308).[10]

Notes

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  1. ^abHiggins (2011) web: rotation period4.969±0.003 hours with a brightness amplitude of0.56 mag. The Collaborative Asteroid Lightcurve Link assigns a quality code of U=3 to the period solution, which denotes a secure result within the precision given and no ambiguity. Summary figures for (4606) Saheki atCollaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^abcd"JPL Small-Body Database Browser: 4606 Saheki (1987 UM1)" (2017-06-06 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4606) Saheki".Dictionary of Minor Planet Names – (4606) Saheki.Springer Berlin Heidelberg. p. 396.doi:10.1007/978-3-540-29925-7_4531.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4606) Saheki". Asteroid Lightcurve Database (LCDB). Retrieved23 January 2016.
  4. ^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.
  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. Retrieved23 January 2016.
  6. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved23 January 2016.
  7. ^abBrinsfield, James W. (July 2009)."Asteroid Lightcurve Analysis at the Via Capote Observatory: 2009 1st Quarter".The Minor Planet Bulletin.36 (3):127–128.Bibcode:2009MPBu...36..127B.ISSN 1052-8091. Retrieved23 January 2016.
  8. ^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. Retrieved26 April 2016.
  9. ^ab"4606 Saheki (1987 UM1)".Minor Planet Center. Retrieved23 January 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

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