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2046 Leningrad

From Wikipedia, the free encyclopedia
Main-belt asteroid

2046 Leningrad
Discovery[1]
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date22 October 1968
Designations
(2046) Leningrad
Named after
Saint Petersburg
(Russian city)[2]
1968 UD1 · 1929 VK
1934 RK · 1940 UF
1955 HN · 1957 YV
1973 QS · 1973 SH3
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.51 yr (31,964 days)
Aphelion3.7227AU
Perihelion2.5902 AU
3.1565 AU
Eccentricity0.1794
5.61yr (2,048 days)
288.85°
0° 10m 32.88s / day
Inclination2.7356°
73.570°
284.26°
Physical characteristics
Dimensions23.55 km(calculated)[3]
23.968±0.292 km[4][5]
27.67±0.67 km[6]
5.296±0.003h[7]
0.060±0.003[6]
0.08(assumed)[3]
0.085±0.017[4][5]
C[3]
11.15±0.23[8] · 11.4[4] · 11.5[1][3][6]

2046 Leningrad, provisional designation1968 UD1, is a carbonaceous Themistianasteroid from the outer regions of theasteroid belt, approximately 24 kilometers in diameter. It was discovered on 22 October 1968, by Soviet astronomerTamara Smirnova at theCrimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula.[9] The asteroid was named after the Soviet city ofLeningrad (now St. Petersburg).[2]

Orbit and classification

[edit]

Leningrad is a member of theThemis family, a dynamical family ofcarbonaceous asteroids with nearly coplanarecliptical orbits, located in theouter-belt main. It orbits the Sun at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,048 days). Its orbit has aneccentricity of 0.18 and aninclination of 3° with respect to theecliptic.[1]

The body'sobservation arc begins 39 years prior to its official discovery observation, with aprecovery taken atLowell Observatory in October 1929. One week later, the asteroid was identified as1929 VK at Lowell Observatory.[9]

Lightcurves

[edit]

In August 2012, a rotationallightcurve ofLeningrad was obtained from photometric observations by astronomers at the Oakley Southern Sky Observatory (E09). Lightcurve analysis gave arotation period of 5.296 hours with a brightness variation of 0.11magnitude (U=2+).[7]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Leningrad measures 23.968 and 27.67 kilometers in diameter and its surface has analbedo of 0.060 and 0.085, respectively.[4][5][6]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for Themistian asteroids of 0.08 and calculates a diameter of 23.55 kilometers based on anabsolute magnitude of 11.5.[3]

Naming

[edit]

Thisminor planet was named forSaint Petersburg, the second largest city of Russia after Moscow. During theSoviet Union, the city was named "Leningrad" between 1924 and 1991. It was also called Petrograd during 1914–1924.[2] The approved naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5282).[10]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2046 Leningrad (1968 UD1)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved29 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2046) Leningrad".Dictionary of Minor Planet Names – (2046) Leningrad.Springer Berlin Heidelberg. p. 166.doi:10.1007/978-3-540-29925-7_2047.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2046) Leningrad". Asteroid Lightcurve Database (LCDB). Retrieved29 June 2017.
  4. ^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.
  5. ^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. Retrieved29 June 2017.
  6. ^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)
  7. ^abSimpson, Gary; Chong, Elena; Gerhardt, Michael; Gorsky, Sean; Klaasse, Matthew; Kodalen, Brian; et al. (July 2013)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 August - October".The Minor Planet Bulletin.40 (3):146–151.Bibcode:2013MPBu...40..146S.ISSN 1052-8091. Retrieved29 June 2017.
  8. ^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. Retrieved29 June 2017.
  9. ^ab"2046 Leningrad (1968 UD1)".Minor Planet Center. Retrieved29 June 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 June 2017.


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