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1283 Komsomolia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1283 Komsomolia
Modelled shape ofKomsomolia
Discovery[1]
Discovered byV. Albitzkij
Discovery siteSimeiz Obs.
Discovery date25 September 1925
Designations
(1283) Komsomolia
Named after
Komsomol[2]
(USSR youth organization)
1925 SC · 1931 VE1
1951 EO2 · 1960 VC
1962 EB · A902 TE
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc115.00 yr (42,002 days)
Aphelion3.8872AU
Perihelion2.4794 AU
3.1833 AU
Eccentricity0.2211
5.68yr (2,075 days)
344.98°
0° 10m 24.6s / day
Inclination8.9078°
157.74°
235.05°
Physical characteristics
26.78 km(derived)[5]
26.87±1.1 km[6]
29.205±0.338 km[7]
29.569±0.373 km[8]
33.12±0.57 km[9]
36.09±7.15 km[10]
96h[11]
0.071±0.334[10]
0.123±0.005[9]
0.153±0.037[8]
0.1577±0.0113[7]
0.1703(derived)[5]
0.1856±0.017[6]
M[7]
10.30[6][7][9] · 10.4[1][5] · 10.61±0.27[12] · 10.70[10]

1283 Komsomolia (prov. designation:1925 SC) is a metallicbackground asteroid and potentiallyslow rotator from the outer regions of theasteroid belt. Discovered byVladimir Albitsky in 1925, it was later named afterKomsomol, a political youth organization of the former Soviet Union. TheM-type asteroid has roughly arotation period 96 hours of and measures approximately 30 kilometers (19 miles) in diameter.

Discovery

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Komsomolia was discovered on 25 September 1925, by Soviet astronomerVladimir Albitsky at theSimeiz Observatory on the Crimean peninsula.[3] It was independently discovered by German astronomerKarl Reinmuth atHeidelberg Observatory on 10 October 1925.[2] Only the first discoverer is officially recognized.[2] The asteroid was first observed asA902 TE at Heidelberg in October 1902.[3]

Orbit and classification

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Komsomolia is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[4] It orbits the Sun in theouter main-belt at a distance of 2.5–3.9 AU once every 5 years and 8 months (2,075 days). Its orbit has aneccentricity of 0.22 and aninclination of 9° with respect to theecliptic.[1] The body'sobservation arc begins at Heidelberg in October 1902, almost 23 years prior to its official discovery observation.[3]

Naming

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Thisminor planet was named afterKomsomol ("All-Union Leninist Young Communist League"), the youth wing of theCommunist Party of the Soviet Union (CPSU).[2] The officialnaming citation was published by theMinor Planet Center in November 1952 (M.P.C. 838).[13]

Physical characteristics

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Komsomolia has been characterized as a metallicM-type asteroid by theWide-field Infrared Survey Explorer (WISE).[7] The Asteroid Lightcurve Database assumes it to be a carbonaceousC-type asteroid.[5]

Rotation period

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In December 2006, a fragmentary rotationallightcurve ofKomsomolia was obtained from photometric observations by French amateur astronomerPierre Antonini. Lightcurve analysis gave arotation period of 96 hours with a brightness amplitude of 1.03magnitude (U=1+).[11]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Komsomolia measures between 26.87 and 36.09 kilometers in diameter and its surface has analbedo between 0.071 and 0.1856.[6][7][8][9][10] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1703 and a diameter of 26.78 kilometers based on anabsolute magnitude of 10.4.[5]

References

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  1. ^abcde"JPL Small-Body Database Browser: 1283 Komsomolia (1925 SC)" (2017-09-29 last obs.).Jet Propulsion Laboratory. Retrieved13 October 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1283) Komsomolia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 106.doi:10.1007/978-3-540-29925-7_1284.ISBN 978-3-540-00238-3.
  3. ^abcd"1283 Komsomolia (1925 SC)".Minor Planet Center. Retrieved13 October 2017.
  4. ^ab"Asteroid 1283 Komsomolia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^abcde"LCDB Data for (1283) Komsomolia". Asteroid Lightcurve Database (LCDB). Retrieved13 October 2017.
  6. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  7. ^abcdefMainzer, 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.
  8. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved13 October 2017.
  9. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  10. ^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. Retrieved13 October 2017.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1283) Komsomolia".Geneva Observatory. Retrieved13 October 2017.
  12. ^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. Retrieved13 October 2017.
  13. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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