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4142 Dersu-Uzala

From Wikipedia, the free encyclopedia
Mars-crossing asteroid

4142 Dersu-Uzala
Discovery[1]
Discovered byZ. Vávrová
Discovery siteKleť Obs.
Discovery date28 May 1981
Designations
(4142) Dersu-Uzala
Named after
Dersu Uzala[2]
(Siberian trapper and hunter)
1981 KE · 1970 AB
1982 VB
Mars-crosser[3]
Hungaria[1][4]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc48.38yr (17,672 d)
Aphelion2.2005AU
Perihelion1.6230 AU
1.9117 AU
Eccentricity0.1510
2.64 yr (965 d)
71.888°
0° 22m 22.44s / day
Inclination26.494°
60.661°
55.384°
Physical characteristics
6.01±1.81 km[5]
6.02±0.60 km[6]
6.34±0.19 km[7]
140±3 h[8][a]
0.164[7]
0.30[5]
0.307[6]
SMASS =A[3][9]
Srw[4][10]
13.00[6]
13.1[3][4]
13.42[5]
13.60[7]

4142 Dersu-Uzala, provisional designation1981 KE, is aHungaria asteroid, sizableMars-crosser and potentiallyslow rotator from the innermost region of theasteroid belt, approximately 6 kilometers (3.7 miles) in diameter. It was discovered by Czech astronomerZdeňka Vávrová atKleť Observatory on 28 May 1981.[1] The rareA-type asteroid has arotation period of 140 hours.[4] It was named after the Siberian trapper and hunterDersu Uzala.[1]

Orbit and characterization

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Dersu-Uzala is a member of the dynamicalHungaria group of asteroids, which form the innermost dense concentration of asteroids in theSolar System. It orbits the Sun in theinner asteroid belt at a distance of 1.6–2.2 AU once every 2 years and 8 months (965 days;semi-major axis of 1.91 AU). Its orbit has aneccentricity of 0.15 and aninclination of 26° with respect to theecliptic. As its orbit crosses that ofMars at 1.66 AU, it is also aMars crossing asteroid.[3] The body'sobservation arc begins with its first observation as1970 AB atCrimea-Nauchnij in January 1970, or 11 years prior to its official discovery observation atKleť Observatory.[1]

Naming

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Thisminor planet was named afterDersu Uzala, a Siberian trapper and hunter and friend of Russian writerVladimir Arsenyev, who named the main character of his novelDersu Uzala after him. The approved naming citation was published by theMinor Planet Center on 6 February 1993 (M.P.C. 21609).[11]

Physical characteristics

[edit]

In theSMASS classification,Dersu-Uzala is anA-type asteroid.[3] It has also been characterized as an Srw-type, a subtype of the stonyS-type asteroids.[10]

Rotation period

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In December 2006, a rotationallightcurve ofDersu-Uzala was obtained fromphotometric observations by American photometristBrian Warner at thePalmer Divide Observatory in Colorado. Lightcurve analysis gave arotation period of140±3 hours with a brightness amplitude of 0.60magnitude (U=2).[4][8][a] Alternative observations gave a period of 71 and 71.2 hours, respectively.[12][13]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Dersu-Uzala measures 6.01 and 6.34 kilometers in diameter and its surface has analbedo of 0.164 and 0.30, respectively. TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.2 and calculates a diameter of 7.13 kilometers based on anabsolute magnitude of 13.1.[4]

Notes

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  1. ^abLightcurve plot of 4142 Dersu-Uzala, Palmer Divide Observatory,B. D. Warner (2006). Quality code is 3. Summary figures at theLCDB.

References

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  1. ^abcde"4142 Dersu-Uzala (1981 KE)".Minor Planet Center. Retrieved8 September 2018.
  2. ^Schmadel, Lutz D. (2007). "(4142) Dersu-Uzala".Dictionary of Minor Planet Names – (4142) Dersu-Uzala.Springer Berlin Heidelberg. p. 354.doi:10.1007/978-3-540-29925-7_4115.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 4142 Dersu-Uzala (1981 KE)" (2018-05-24 last obs.).Jet Propulsion Laboratory. Retrieved8 September 2018.
  4. ^abcdef"LCDB Data for (4142) Dersu-Uzala". Asteroid Lightcurve Database (LCDB). Retrieved15 June 2017.
  5. ^abcNugent, 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.
  6. ^abcAlí-Lagoa, V.; Delbo', M. (July 2017). "Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data".Astronomy and Astrophysics.603: 8.arXiv:1705.10263.Bibcode:2017A&A...603A..55A.doi:10.1051/0004-6361/201629917.S2CID 119224590.
  7. ^abcUsui, 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)
  8. ^abWarner, Brian D.; Stephens, Robert, D.; Harris, Alan W.; Pravec, Petr (October 2009)."A Re-examination of the Lightcurves for Seven Hungaria Asteroids".The Minor Planet Bulletin.36 (4):176–179.Bibcode:2009MPBu...36..176W.ISSN 1052-8091. Retrieved8 September 2018.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  9. ^"Asteroid 4142 Dersu-Uzala".Small Bodies Data Ferret. Retrieved8 September 2018.
  10. ^abLucas, Michael P.; Emery, Joshua P.; Pinilla-Alonso, Noemi; Lindsay, Sean S.; Lorenzi, Vania (July 2017)."Hungaria asteroid region telescopic spectral survey (HARTSS) I: Stony asteroids abundant in the Hungaria background population".Icarus.291:268–287.Bibcode:2017Icar..291..268L.doi:10.1016/j.icarus.2016.11.002.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 June 2017.
  12. ^Warner, Brian D. (October 2015)."Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2015 March-June".The Minor Planet Bulletin.42 (4):267–276.Bibcode:2015MPBu...42..267W.ISSN 1052-8091.PMC 7244090.PMID 32455362. Retrieved8 September 2018.
  13. ^Warner, Brian D. (June 2007)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory - September-December 2006".The Minor Planet Bulletin.34 (2):32–37.Bibcode:2007MPBu...34...32W.ISSN 1052-8091. Retrieved8 September 2018.

External links

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