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21088 Chelyabinsk

From Wikipedia, the free encyclopedia
Stony asteroid and near-Earth object of the Amor group

21088 Chelyabinsk
Discovery[1]
Discovered byE. W. Elst
Discovery siteLa Silla Obs.
Discovery date30 January 1992
Designations
(21088) Chelyabinsk
Named after
Chelyabinsk[2](city andmeteor)
1992 BL2
NEO · Amor[1][2]
Mars-crosser
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.41 yr (10,012 days)
Aphelion2.1135AU
Perihelion1.2996 AU
1.7065 AU
Eccentricity0.2384
2.23yr (814 days)
318.92°
0° 26m 31.56s / day
Inclination38.455°
297.85°
27.133°
Earth MOID0.3083 AU · 120.1LD
Physical characteristics
Dimensions2.79±0.10 km[3]
3.46±0.25 km[4]
4.23 km(taken)[5]
4.231±0.113 km[6][7]
4.232 km[8]
22.426±0.02h[a][b]
22.49 h[a]
0.1794[8]
0.206[6]
0.257±0.038[4]
0.26±0.32[9]
0.37±0.06[3]
Q[10] · L[11] · S[5]
B–V =0.855±0.073[12]
V–R =0.464±0.015[12] 
V–I =0.910±0.032[12]
13.86±0.14(R)[a] · 14.00[11] · 14.2[6] · 14.29±0.24[13] · 14.3[1] · 14.35±0.149[5][8] · 14.40[4]

21088 Chelyabinsk (provisional designation1992 BL2) is a stonyasteroid andnear-Earth object of theAmor group, approximately 4 kilometers in diameter. It was discovered on 30 January 1992, by Belgian astronomerEric Elst atESO'sLa Silla Observatory in northern Chile. The asteroid was named after the Russian city ofChelyabinsk and for its spectacularChelyabinsk meteor event in 2013.[2] It is not related to the Chelyabinsk impactor.

Classification and orbit

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Chelyabinsk orbits the Sun at a distance of 1.3–2.1 AU once every 2 years and 3 months (814 days). Its orbit has aneccentricity of 0.24 and aninclination of 38° with respect to theecliptic. A firstprecovery was taken during theDigitized Sky Survey at the AustraliaSiding Spring Observatory in January 1990, extending the asteroid'sobservation arc by 2 years prior to its official discovery at La Silla.[2]

Close approaches

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As anear-Earth object, Chelyabinsk has a low Earthminimum orbit intersection distance of 0.3083 AU (46,100,000 km), which translates into 120.1lunar distances (LD). This is, however, far too large to make it apotentially hazardous asteroid, which have intersection distances of less than 20 LD.[1] It also crosses the orbit of Mars at 1.666 AU which makes it aMars-crossing asteroid. In August 2142, it will approach Mars at 0.0986 AU (14,800,000 km).[1]

Physical characteristics

[edit]

Chelyabinsk has been characterized as both aQ-type andL-type asteroid.[10][11] It is also a generically assumedS-type asteroid.[5]

Lightcurves

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Two rotationallight-curves of Chelyabinsk were obtained by Czech astronomerPetr Pravec atOndřejov Observatory in December 2002 and September 2004, respectively. They gave arotation period of 22.490 and22.426 hours, each with a brightness variation of 0.13magnitude (U=n.a./3-).[a][b]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE), Chelyabinsk measures between 2.79 and 4.2 kilometers in diameter and its surface has analbedo between 0.21 and 0.37,[6][7][8] while observations by the JapaneseAkari satellite gave an albedo of 0.26 and a diameter of 3.5 kilometers.[4] TheCollaborative Asteroid Lightcurve Link adopts Petr Pravec's revised WISE results, that is, a diameter of 4.23 kilometers and an albedo of 0.179 based on anabsolute magnitude of 14.35.[5][8]

Naming

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Thisminor planet is named after the Russian cityChelyabinsk, located in theUral region. The city is well known for theChelyabinsk meteor, a 20-meter sized, extremely brightfireball that exploded to the south of the city at an altitude of 30 kilometers on 15 February 2013. The indirect effects of the explosion injured more than 1,500 people.[2] The official naming citation was published by theMinor Planet Center (MPC) on 21 August 2013 (M.P.C. 84674).[14]

Erratum

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Originally, the name "Chelyabinsk" was erroneously given by the MPC to the numerically similar asteroid(20188) 1997 AC18 on 22 July (M.P.C. 84379). The wrong designation20188 Chelyabinsk was deleted in the subsequent publication of theMinor Planet Circulars on 21 August 2013 (M.P.C. 84385)[14]

Notes

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  1. ^abcdPravec (2002 and 2004) web: rotation period of 22.49 and22.426±0.02 hours, both with a brightness amplitude of0.13 mag. Summary figures of (21088) Chelyabinsk at theLCDB andPravec, P.; Wolf, M.; Sarounova, L. (2002/2004)
  2. ^abLightcurve plot by Pravec from 7 June 2005 with period of 22.431 hours.Data sheet from unpublished observations atOndrejov Asteroid Photometry Project

References

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  1. ^abcdef"JPL Small-Body Database Browser: 21088 Chelyabinsk (1992 BL2)" (2016-02-19 last obs.).Jet Propulsion Laboratory.Archived from the original on 20 September 2020. Retrieved12 October 2016.
  2. ^abcde"21088 Chelyabinsk (1992 BL2)".Minor Planet Center.Archived from the original on 4 March 2016. Retrieved12 October 2016.
  3. ^abNugent, 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.
  4. ^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. (onlineArchived 3 September 2024 at theWayback Machine,AcuA catalog p. 153Archived 25 March 2019 at theWayback Machine)
  5. ^abcde"LCDB Data for (21088) Chelyabinsk". Asteroid Lightcurve Database (LCDB).Archived from the original on 13 September 2020. Retrieved12 October 2016.
  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.
  7. ^abMainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results".The Astrophysical Journal.743 (2): 17.arXiv:1109.6400.Bibcode:2011ApJ...743..156M.doi:10.1088/0004-637X/743/2/156.S2CID 239991.
  8. ^abcdePravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026.
  9. ^Thomas, C. A.; Trilling, D. E.; Emery, J. P.; Mueller, M.; Hora, J. L.; Benner, L. A. M.; et al. (September 2011)."ExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid Population".The Astronomical Journal.142 (3): 12.Bibcode:2011AJ....142...85T.doi:10.1088/0004-6256/142/3/85.
  10. ^abThomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014). "Physical characterization of Warm Spitzer-observed near-Earth objects".Icarus.228:217–246.arXiv:1310.2000.Bibcode:2014Icar..228..217T.doi:10.1016/j.icarus.2013.10.004.S2CID 119278697.
  11. ^abcCarry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry".Icarus.268:340–354.arXiv:1601.02087.Bibcode:2016Icar..268..340C.doi:10.1016/j.icarus.2015.12.047.S2CID 119258489.
  12. ^abcYe, Q.-z. (February 2011). "BVRI Photometry of 53 Unusual Asteroids".The Astronomical Journal.141 (2): 8.arXiv:1011.0133.Bibcode:2011AJ....141...32Y.doi:10.1088/0004-6256/141/2/32.S2CID 119307210.
  13. ^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.
  14. ^ab"MPC/MPO/MPS Archive".Minor Planet Center.Archived from the original on 7 October 2010. Retrieved12 October 2016.

External links

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