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3724 Annenskij

From Wikipedia, the free encyclopedia
Asteroid

3724 Annenskij
Discovery[1]
Discovered byL. Zhuravleva
Discovery siteCrimean Astrophysical Obs.
Discovery date23 December 1979
Designations
(3724) Annenskij
Named after
Innokenty Annensky[1]
(Russian poet)
1979 YN8 · 1933 XB
1955 QQ · 1965 YM
1969 RF2 · 1974 VM2
1980 AE · 1985 DF1
main-belt[1][2] · (middle)
Gefion[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc84.28yr (30,783 d)
Aphelion3.2198AU
Perihelion2.3123 AU
2.7660 AU
Eccentricity0.1640
4.60 yr (1,680 d)
176.15°
0° 12m 51.48s / day
Inclination7.7351°
269.19°
117.85°
Physical characteristics
12.09±2.86 km[4]
13.55±0.37 km[5]
13.74±0.47 km[6]
14.15±1.3 km[7]
15.229±0.114 km[8]
15.386±0.248 km[9]
3.969±0.001 h[10]
3.974±0.002 h[10]
0.1744±0.0145[8]
0.19±0.09[4]
0.2021(derived)[11]
0.2022±0.043[7]
0.227±0.013[5]
0.235±0.028[6]
S(family-based)[12]
11.47±0.33[13]
11.50[6]
11.60[2][5][7][8][11]
12.00[4]

3724 Annenskij, provisional designation1979 YN8, is a stony Gefionianasteroid from the central regions of theasteroid belt, approximately 14 kilometers (9 miles) in diameter. It was discovered on 23 December 1979, by Soviet astronomerLyudmila Zhuravleva at theCrimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula.[1] TheS-type asteroid has a rotation period of 3.97 hours.[11] It was named for Russian poetInnokenty Annensky.[1]

Orbit and classification

[edit]

Annenskij is a member of theGefion family (516),[3] a largeasteroid family in the intermediate asteroid belt, named after1272 Gefion.[12] It is also known as the Ceres or Minerva family.

It orbits the Sun in thecentral main-belt at a distance of 2.3–3.2 AU once every 4 years and 7 months (1,680 days;semi-major axis of 2.77 AU). Its orbit has aneccentricity of 0.16 and aninclination of 8° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation as1933 XB atHeidelberg Observatory in December 1933, or 46 years prior to its official discovery observation at Nauchnij.[1]

Physical characteristics

[edit]

Based on its classification into the Gefion family,Annenskij is a stonyS-type asteroid.[12]: 23 

Rotation period

[edit]

Two rotationallightcurves ofAnnenskij were obtained fromphotometric observations by Italian and French amateur astronomersSilvano Casulli,Laurent Bernasconi andCyril Cavadore . Lightcurve analysis gave arotation period of 3.969 and 3.974 hours with a brightness amplitude of 0.30 and 0.28magnitude (U=3-/3).[10]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Annenskij measures between 12.09 and 15.386 kilometers in diameter and its surface has analbedo between 0.1744 and 0.235.[4][5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2021 and a diameter of 14.15 kilometers based on anabsolute magnitude of 11.6.[11]

Naming

[edit]

Thisminor planet was named after Russian poet and writerInnokenty Annensky (1855–1909).[1] The official naming citation was published by theMinor Planet Center on 4 June 1993 (M.P.C. 22246) with a correction on Annensky's date of death published on 4 February 1996 (M.P.C. 26439).[14]

References

[edit]
  1. ^abcdefg"3724 Annenskij (1979 YN8)".Minor Planet Center. Retrieved4 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 3724 Annenskij (1979 YN8)" (2018-03-27 last obs.).Jet Propulsion Laboratory. Retrieved4 May 2018.
  3. ^ab"Asteroid 3724 Annenskij – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  4. ^abcdNugent, 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.
  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. ^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.S2CID 46350317.
  7. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  8. ^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. (catalog)
  9. ^abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.S2CID 119293330.
  10. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (3724) Annenskij". Geneva Observatory. Retrieved4 May 2018.
  11. ^abcd"LCDB Data for (3724) Annenskij". Asteroid Lightcurve Database (LCDB). Retrieved4 May 2018.
  12. ^abcNesvorný, 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 9780816532131.S2CID 119280014.
  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. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 May 2018.

External links

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