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10121 Arzamas

From Wikipedia, the free encyclopedia
Main-belt asteroid

10121 Arzamas
Discovery[1]
Discovered byE. W. Elst
Discovery siteCERGA(Caussols Obs.)
Discovery date27 January 1993
Designations
(10121) Arzamas
Named after
Arzamas(Russian city)[2]
1993 BS4 · 1994 GA11
2118 T-1
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc46.12 yr (16,844 days)
Aphelion3.6918AU
Perihelion2.7164 AU
3.2041 AU
Eccentricity0.1522
5.74yr (2,095 days)
319.65°
0° 10m 18.48s / day
Inclination0.8917°
30.729°
263.08°
Physical characteristics
Dimensions10.28 km(calculated)[3]
10.757±0.391 km[4][5]
12.1±0.3h[6]
12.1991±0.0060 h[7]
0.080±0.024[5]
0.08(assumed)[3]
0.0801±0.0237[4]
C[3]
13.2[4] · 13.375±0.003[7] · 13.4[1][3]

10121 Arzamas, provisional designation1993 BS4, is a dark Themistianasteroid from the outer region of theasteroid belt, approximately 10 kilometers in diameter. The asteroid was discovered on 27 January 1993, by Belgian astronomerEric Elst atCaussols(010) in southeastern France.[8] It was later named after the Russian city ofArzamas.[2]

Orbit and classification

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Arzamas is a member of theThemis family, a dynamical family of outer main-belt asteroids with nearly co-planarecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.7–3.7 AU once every 5 years and 9 months (2,095 days). Its orbit has aneccentricity of 0.15 and aninclination of 1° with respect to theecliptic.[1]

The body'sobservation arc begins 22 years prior to its official discovery observation, when it was identified as2118 T-1 atPalomar Observatory during the firstPalomar–Leiden Trojan survey in 1971.[8]

Physical characteristics

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Lightcurves

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In February 2010, two rotationallightcurves ofArzamas were obtained from photometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of12.1 and12.1991 hours with a brightness variation of 0.7 and 0.6magnitude, respectively (U=2/2).[6][7]

Diameter and albedo

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According to theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Arzamas measures 10.8 kilometer in diameter, and its surface has analbedo of 0.08.[4][5] TheCollaborative Asteroid Lightcurve Link also assumes an albedo of 0.08, characterizes it as aC-type asteroid, and calculates a diameter of 10.3 kilometers with anabsolute magnitude of 13.4.[3]

Naming

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Thisminor planet was named after the Russian city ofArzamas, a major transit center on the road from Moscow to the eastern parts of the country. It was founded in 1578 byIvan the Terrible and is located on the Tyosha River, known for making leather and dyeing fabrics ever since.[2][8] The official naming citation was published by theMinor Planet Center on 24 November 2007 (M.P.C. 61266).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 10121 Arzamas (1993 BS4)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved23 June 2017.
  2. ^abcSchmadel, Lutz D. (2009).Dictionary of Minor Planet Names – (10121) Arzamas, Addendum to Fifth Edition: 2006–2008.Springer Berlin Heidelberg. p. 47.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (10121) Arzamas". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  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.S2CID 118700974. Retrieved17 May 2016.
  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.S2CID 118745497. Retrieved4 December 2016.
  6. ^abPolishook, D.; Ofek, E. O.; Waszczak, A.; Kulkarni, S. R.; Gal-Yam, A.; Aharonson, O.; et al. (April 2012)."Asteroid rotation periods from the Palomar Transient Factory survey".Monthly Notices of the Royal Astronomical Society.421 (3):2094–2108.arXiv:1201.1930.Bibcode:2012MNRAS.421.2094P.doi:10.1111/j.1365-2966.2012.20462.x.S2CID 40538809.
  7. ^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.S2CID 8342929. Retrieved17 May 2016.
  8. ^abc"10121 Arzamas (1993 BS4)".Minor Planet Center. Retrieved1 March 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
Minor planets
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Distant minor planet
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Authority control databasesEdit this at Wikidata
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