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2571 Geisei

From Wikipedia, the free encyclopedia
Stony Florian asteroid from the inner regions of the asteroid belt

2571 Geisei
Discovery[1]
Discovered byT. Seki
Discovery siteGeisei Obs.
Discovery date23 October 1981
Designations
(2571) Geisei
Named after
Geisei(Japanese village)[2]
1981 UC · 1931 TA4
1934 NV · 1944 OD
1961 XG · 1981 WR6
A911 UC
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc85.64 yr (31,280 days)
Aphelion2.6607AU
Perihelion1.7953 AU
2.2280 AU
Eccentricity0.1942
3.33yr (1,215 days)
317.69°
0° 17m 47.04s / day
Inclination2.8722°
66.915°
284.78°
Physical characteristics
Dimensions5.21±0.95 km[4]
5.23±1.07 km[5]
6.582±0.035 km[6][7]
6.81 km(calculated)[3]
7.823±0.005h[8]
0.24(assumed)[3]
0.2573±0.0688[6]
0.275±0.059[7]
0.34±0.14[4]
0.38±0.24[5]
S[3]
12.9[5] · 13.0[1][3][6] · 13.32±0.26[9] · 13.38[4]

2571 Geisei, provisional designation1981 UC, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 6 kilometers in diameter. It was discovered by Japanese astronomerTsutomu Seki atGeisei Observatory on 23 October 1981, and named for the Japanese village ofGeisei.[2][10]

Classification and Orbit

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Geisei 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 1.8–2.7 AU once every 3 years and 4 months (1,215 days). Its orbit has aneccentricity of 0.19 and aninclination of 3° with respect to theecliptic.[1]

In October 1911,Geisei was first identified asA911 UC atHeidelberg Observatory. The asteroid'sobservation arc begins 50 years prior to its discovery, with aprecovery taken atLowell Observatory in 1931.[10]

Physical characteristics

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Lightcurves

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A rotationallightcurve for this asteroid was obtained from photometric observations made at the Australian Oakley Southern Sky Observatory (E09) in September 2014. The lightcurve gave arotation period of7.823±0.005 hours with a brightness variation of 0.50 inmagnitude (U=3-).[8]

Diameter and albedo

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According to the 2015/16NEOWISE mission results of NASA's space-basedWide-field Infrared Survey Explorer,Geisei measures 5.21 and 5.23 kilometers in diameter and its surface has analbedo of 0.34 and 0.38, respectively.[4][5] Preliminary WISE results gave a diameter of 6.582 kilometers and an albedo of 0.275.[6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 6.81 kilometers using anabsolute magnitude of 13.0.[3]

Naming

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Thisminor planet is named after the small Japanese village ofGeisei, where the discovering observatory is located. Geisei is situated near the city ofKōchi, after which Tsutomu Seki's first discovery, the asteroid2396 Kochi, is named.[2] The approved naming citation was published by theMinor Planet Center on 6 June 1982 (M.P.C. 6956).[11]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2571 Geisei (1981 UC)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2571) Geisei".Dictionary of Minor Planet Names – (2571) Geisei.Springer Berlin Heidelberg. p. 210.doi:10.1007/978-3-540-29925-7_2572.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2571) Geisei". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^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.
  5. ^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.S2CID 9341381. Retrieved3 July 2017.
  6. ^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. Retrieved17 May 2016.
  7. ^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. Retrieved6 December 2016.
  8. ^abBohn, Lucas; Hibbler, Brianna; Stein, Gregory; Ditteon, Richard (April 2015)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2014 September".The Minor Planet Bulletin.42 (2):89–90.Bibcode:2015MPBu...42...89B.ISSN 1052-8091. Retrieved17 May 2016.
  9. ^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. Retrieved17 May 2016.
  10. ^ab"2571 Geisei (1981 UC)".Minor Planet Center. Retrieved17 May 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

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