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4944 Kozlovskij

From Wikipedia, the free encyclopedia
Asteroid

4944 Kozlovskij
Discovery [1]
Discovered byL. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date2 September 1987
Designations
(4944) Kozlovskij
Named after
Ivan Kozlovsky[2]
(Russian opera singer)
1987 RP3 · 1978 VK13
1985 DP2 · 1991 NX7
main-belt[1][3] · (middle)
Witt[4]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc65.41yr (23,890 d)
Aphelion2.9170AU
Perihelion2.5733 AU
2.7451 AU
Eccentricity0.0626
4.55 yr (1,661 d)
252.23°
0° 13m 0.12s / day
Inclination4.4903°
279.41°
84.781°
Physical characteristics
Dimensions9.25±1.11 km[5]
9.89±2.71 km[6]
9.91 km(calculated)[7]
10.85±2.35 km[8]
11.125±0.083 km[9][10]
3.573±0.0006h[11]
0.057(assumed)[7]
0.061±0.006[9][10]
0.086±0.032[8]
0.09±0.09[6]
0.157±0.038[5]
SMASS =Cb[3] · C[7]
12.80[5] · 13.1[8][9] · 13.20[6] · 13.297±0.003(R)[11] · 13.3[3] · 13.42±0.25[12] · 13.75[7]

4944 Kozlovskij, provisional designation1987 RP3, is a carbonaceous Wittasteroid from the central regions of theasteroid belt, approximately 10 kilometers (6 miles) in diameter. It was discovered on 2 September 1987, by Soviet astronomerLyudmila Chernykh at theCrimean Astrophysical Observatory in Nauchnij, on the Crimean Peninsula.[1] The asteroid was named for Russian opera singerIvan Kozlovsky.[2]

Classification

[edit]

Kozlovskij is a member of theWitt family (535),[4] a largefamily of (predominantly) stony asteroids with more than 1,600 known members.[13] It orbits the Sun in thecentral main-belt at a distance of 2.6–2.9 AU once every 4 years and 7 months (1,661 days;semi-major axis of 2.75 AU). Its orbit has aneccentricity of 0.06 and aninclination of 4° with respect to theecliptic.[3] The asteroid'sobservation arc begins 36 years prior to its official discovery observation, with aprecovery taken atPalomar Observatory in December 1951.[1]

Physical characteristics

[edit]

In theSMASS classification,Kozlovskij is a Cb-type asteroid, an intermediary between the carbonaceousC-type and the somewhat brighterB-type asteroids.[3]

Lightcurves

[edit]

In October 2010, a rotationallightcurve ofKozlovskij was obtained from photometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 3.573 hours with a brightness amplitude of 0.46magnitude (U=2).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Kozlovskij measures 9.25 and 9.89 kilometers in diameter and its surface has analbedo of 0.157 and 0.09, respectively.[5][6] Preliminary WISE results gave a larger diameter of 10.85 and 11.125 kilometers with lower albedo of 0.086 and 0.061, respectively.[8][9][10]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and calculates a diameter of 9.91 kilometers based on anabsolute magnitude of 13.75.[7]

Naming

[edit]

Thisminor planet was named after Russian opera singerIvan Kozlovsky (1900–1993), who was a rarelyric tenor and a popular singer in the formerSoviet Union.[2] The approved naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22504).[14]

References

[edit]
  1. ^abcd"4944 Kozlovskij (1987 RP3)".Minor Planet Center. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4944) Kozlovskij".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. pp. 425–426.doi:10.1007/978-3-540-29925-7_4826.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 4944 Kozlovskij (1987 RP3)" (2017-04-28 last obs.).Jet Propulsion Laboratory. Retrieved18 April 2018.
  4. ^ab"Asteroid 4944 Kozlovskij – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^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)
  6. ^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.
  7. ^abcde"LCDB Data for (4944) Kozlovskij". Asteroid Lightcurve Database (LCDB). Retrieved1 July 2017.
  8. ^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. Retrieved1 July 2017.
  9. ^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.
  10. ^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. Retrieved1 July 2017.
  11. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.
  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.
  13. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 July 2017.

External links

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