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4142 Dersu-Uzala

4142 Dersu-Uzala, provisional designation 1981 KE, is a Hungaria asteroid, sizable Mars-crosser and potentially slow rotator from the innermost region of the asteroid belt, approximately 6 kilometers (3.7 miles) in diameter. It was discovered by Czech astronomer Zdeňka Vávrová at Kleť Observatory on 28 May 1981.[1] The rare A-type asteroid has a rotation period of 140 hours.[4] It was named after the Siberian trapper and hunter Dersu Uzala.[1]

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 arc48.38 yr (17,672 d)
Aphelion2.2005 AU
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
Mean diameter
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]

Orbit and characterization Edit

Dersu-Uzala is a member of the dynamical Hungaria group of asteroids, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun in the inner 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 an eccentricity of 0.15 and an inclination of 26° with respect to the ecliptic. As its orbit crosses that of Mars at 1.66 AU, it is also a Mars crossing asteroid.[3] The body's observation arc begins with its first observation as 1970 AB at Crimea-Nauchnij in January 1970, or 11 years prior to its official discovery observation at Kleť Observatory.[1]

Naming Edit

This minor planet was named after Dersu Uzala, a Siberian trapper and hunter and friend of Russian writer Vladimir Arsenyev, who named the main character of his novel Dersu Uzala after him. The approved naming citation was published by the Minor Planet Center on 6 February 1993 (M.P.C. 21609).[11]

Physical characteristics Edit

In the SMASS classification, Dersu-Uzala is an A-type asteroid.[3] It has also been characterized as an Srw-type, a subtype of the stony S-type asteroids.[10]

Rotation period Edit

In December 2006, a rotational lightcurve of Dersu-Uzala was obtained from photometric observations by American photometrist Brian Warner at the Palmer Divide Observatory in Colorado. Lightcurve analysis gave a rotation period of 140±3 hours with a brightness amplitude of 0.60 magnitude (U=2).[4][8][a] Alternative observations gave a period of 71 and 71.2 hours, respectively.[12][13]

Diameter and albedo Edit

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Dersu-Uzala measures 6.01 and 6.34 kilometers in diameter and its surface has an albedo of 0.164 and 0.30, respectively. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.2 and calculates a diameter of 7.13 kilometers based on an absolute magnitude of 13.1.[4]

Notes Edit

  1. ^ a b Lightcurve plot of 4142 Dersu-Uzala, Palmer Divide Observatory, B. D. Warner (2006). Quality code is 3. Summary figures at the LCDB.

References Edit

  1. ^ a b c d e "4142 Dersu-Uzala (1981 KE)". Minor Planet Center. Retrieved 8 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. ^ a b c d e f "JPL Small-Body Database Browser: 4142 Dersu-Uzala (1981 KE)" (2018-05-24 last obs.). Jet Propulsion Laboratory. Retrieved 8 September 2018.
  4. ^ a b c d e f "LCDB Data for (4142) Dersu-Uzala". Asteroid Lightcurve Database (LCDB). Retrieved 15 June 2017.
  5. ^ a b c Nugent, 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. ^ a b c Alí-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.
  7. ^ a b c Usui, 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. ^ a b Warner, 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. Retrieved 8 September 2018.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  9. ^ "Asteroid 4142 Dersu-Uzala". Small Bodies Data Ferret. Retrieved 8 September 2018.
  10. ^ a b Lucas, 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. Retrieved 8 September 2018.
  11. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 15 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. Retrieved 8 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. Retrieved 8 September 2018.

External links Edit

  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • 4142 Dersu-Uzala at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 4142 Dersu-Uzala at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

4142, dersu, uzala, provisional, designation, 1981, hungaria, asteroid, sizable, mars, crosser, potentially, slow, rotator, from, innermost, region, asteroid, belt, approximately, kilometers, miles, diameter, discovered, czech, astronomer, zdeňka, vávrová, kle. 4142 Dersu Uzala provisional designation 1981 KE is a Hungaria asteroid sizable Mars crosser and potentially slow rotator from the innermost region of the asteroid belt approximately 6 kilometers 3 7 miles in diameter It was discovered by Czech astronomer Zdenka Vavrova at Klet Observatory on 28 May 1981 1 The rare A type asteroid has a rotation period of 140 hours 4 It was named after the Siberian trapper and hunter Dersu Uzala 1 4142 Dersu UzalaDiscovery 1 Discovered byZ VavrovaDiscovery siteKlet Obs Discovery date28 May 1981DesignationsMPC designation 4142 Dersu UzalaNamed afterDersu Uzala 2 Siberian trapper and hunter Alternative designations1981 KE 1970 AB1982 VBMinor planet categoryMars crosser 3 Hungaria 1 4 Orbital characteristics 3 Epoch 23 March 2018 JD 2458200 5 Uncertainty parameter 0Observation arc48 38 yr 17 672 d Aphelion2 2005 AUPerihelion1 6230 AUSemi major axis1 9117 AUEccentricity0 1510Orbital period sidereal 2 64 yr 965 d Mean anomaly71 888 Mean motion0 22m 22 44s dayInclination26 494 Longitude of ascending node60 661 Argument of perihelion55 384 Physical characteristicsMean diameter6 01 1 81 km 5 6 02 0 60 km 6 6 34 0 19 km 7 Synodic rotation period140 3 h 8 a Geometric albedo0 164 7 0 30 5 0 307 6 Spectral typeSMASS A 3 9 Srw 4 10 Absolute magnitude H 13 00 6 13 1 3 4 13 42 5 13 60 7 Contents 1 Orbit and characterization 2 Naming 3 Physical characteristics 3 1 Rotation period 3 2 Diameter and albedo 4 Notes 5 References 6 External linksOrbit and characterization EditDersu Uzala is a member of the dynamical Hungaria group of asteroids which form the innermost dense concentration of asteroids in the Solar System It orbits the Sun in the inner 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 an eccentricity of 0 15 and an inclination of 26 with respect to the ecliptic As its orbit crosses that of Mars at 1 66 AU it is also a Mars crossing asteroid 3 The body s observation arc begins with its first observation as 1970 AB at Crimea Nauchnij in January 1970 or 11 years prior to its official discovery observation at Klet Observatory 1 Naming EditThis minor planet was named after Dersu Uzala a Siberian trapper and hunter and friend of Russian writer Vladimir Arsenyev who named the main character of his novel Dersu Uzala after him The approved naming citation was published by the Minor Planet Center on 6 February 1993 M P C 21609 11 Physical characteristics EditIn the SMASS classification Dersu Uzala is an A type asteroid 3 It has also been characterized as an Srw type a subtype of the stony S type asteroids 10 Rotation period Edit In December 2006 a rotational lightcurve of Dersu Uzala was obtained from photometric observations by American photometrist Brian Warner at the Palmer Divide Observatory in Colorado Lightcurve analysis gave a rotation period of 140 3 hours with a brightness amplitude of 0 60 magnitude U 2 4 8 a Alternative observations gave a period of 71 and 71 2 hours respectively 12 13 Diameter and albedo Edit According to the surveys carried out by the Japanese Akari satellite and NASA s Wide field Infrared Survey Explorer with its subsequent NEOWISE mission Dersu Uzala measures 6 01 and 6 34 kilometers in diameter and its surface has an albedo of 0 164 and 0 30 respectively The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0 2 and calculates a diameter of 7 13 kilometers based on an absolute magnitude of 13 1 4 Notes Edit a b Lightcurve plot of 4142 Dersu Uzala Palmer Divide Observatory B D Warner 2006 Quality code is 3 Summary figures at the LCDB References Edit a b c d e 4142 Dersu Uzala 1981 KE Minor Planet Center Retrieved 8 September 2018 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 a b c d e f JPL Small Body Database Browser 4142 Dersu Uzala 1981 KE 2018 05 24 last obs Jet Propulsion Laboratory Retrieved 8 September 2018 a b c d e f LCDB Data for 4142 Dersu Uzala Asteroid Lightcurve Database LCDB Retrieved 15 June 2017 a b c Nugent 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 a b c Ali 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 amp A 603A 55A doi 10 1051 0004 6361 201629917 a b c Usui Fumihiko Kuroda Daisuke Muller 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 a b Warner 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 Retrieved 8 September 2018 a href Template Cite journal html title Template Cite journal cite journal a CS1 maint multiple names authors list link Asteroid 4142 Dersu Uzala Small Bodies Data Ferret Retrieved 8 September 2018 a b Lucas 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 Retrieved 8 September 2018 MPC MPO MPS Archive Minor Planet Center Retrieved 15 June 2017 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 Retrieved 8 September 2018 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 Retrieved 8 September 2018 External links EditAsteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 4142 Dersu Uzala at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 4142 Dersu Uzala at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 4142 Dersu Uzala amp oldid 1123255106, wikipedia, wiki, book, books, library,

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