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2420 Čiurlionis

From Wikipedia, the free encyclopedia
Main-belt asteroid
2420 Čiurlionis
Discovery[1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date3 October 1975
Designations
(2420) Čiurlionis
Named after
Mikalojus Čiurlionis
(painter and composer)[2]
1975 TN · 1979 QF
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc41.42 yr (15,129 days)
Aphelion2.9008AU
Perihelion2.2190 AU
2.5599 AU
Eccentricity0.1332
4.10yr (1,496 days)
56.325°
0° 14m 26.16s / day
Inclination14.611°
205.64°
197.83°
Physical characteristics
Dimensions8.444±0.198 km[4][5]
10.06 km(calculated)[3]
12.84h[6]
15.760±0.002 h[7]
0.21(assumed)[3]
0.327±0.086[4][5]
S[3]
12.2[4] · 12.28±0.28[8] · 12.3[1][3]

2420 Čiurlionis, provisionally designated1975 TN, is a stony Eunomianasteroid from the central regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 3 October 1975, by Soviet astronomerNikolai Chernykh at theCrimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula, and later named after Lithuanian painter and composerMikalojus Čiurlionis.[2][9]

Orbit and classification

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Čiurlionis is a member of theEunomia family, a large group ofS-type asteroids and the most prominent family in theintermediate main-belt. It orbits the Sun at a distance of 2.2–2.9 AU once every 4 years and 1 month (1,496 days). Its orbit has aneccentricity of 0.13 and aninclination of 15° with respect to theecliptic.[1]

Physical characteristics

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Lightcurves

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Two rotationallightcurves ofČiurlionis were obtained from photometric observations. Lightcurve analysis gave arotation period of 12.84 and 15.760 hours with a brightness amplitude of 0.48 and 0.51magnitude, respectively (U=2/3-).[6][7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Čiurlionis measures 8.444 kilometers in diameter and its surface has analbedo of 0.327.[4][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from15 Eunomia, the family's largest member and namesake – and calculates a diameter of 10.06 kilometers based on anabsolute magnitude of 12.3.[3]

Naming

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Thisminor planet was named after LithuanianArt Nouveau painter and composerMikalojus Konstantinas Čiurlionis (1875–1911).[2] The approved naming citation was published by theMinor Planet Center on 17 February 1984 (M.P.C. 8542).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2420 Ciurlionis (1975 TN)" (2017-03-05 last obs.).Jet Propulsion Laboratory. Retrieved29 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2420) Čiurlionis".Dictionary of Minor Planet Names – (2420) Čiurlionis.Springer Berlin Heidelberg. p. 197.doi:10.1007/978-3-540-29925-7_2421.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2420) Čiurlionis". Asteroid Lightcurve Database (LCDB). Retrieved29 June 2017.
  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.
  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. Retrieved29 June 2017.
  6. ^abDurkee, Russell I.; Syring, Connor W. (April 2013)."Lightcurve of 2420 Ciurlionis".The Minor Planet Bulletin.40 (2): 88.Bibcode:2013MPBu...40...88D.ISSN 1052-8091. Retrieved29 June 2017.
  7. ^abFoylan, Mike; Durkee, Russell I. (April 2017)."A Revised Rotation Period for Minor Planet 2420 Ciurlionis".The Minor Planet Bulletin.44 (2):91–92.Bibcode:2017MPBu...44...91F.ISSN 1052-8091. Retrieved29 June 2017.
  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. Retrieved29 June 2017.
  9. ^"2420 Ciurlionis (1975 TN)".Minor Planet Center. Retrieved29 June 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 June 2017.

External links

[edit]
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