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21873 Jindřichůvhradec

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Main-belt asteroid

21873 Jindřichůvhradec
Discovery[1]
Discovered byJ. Tichá
M. Tichý
Discovery siteKleť Obs.
Discovery date29 October 1999
Designations
(21873) Jindřichůvhradec
Named after
Jindřichův Hradec[2]
(Czech town)
1999 UU3 · 1982 SN8
1988 XA5
main-belt · (outer)[3]
Hygiea[4]
Orbital characteristics[5]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc34.52 yr (12,608 days)
Aphelion3.8041AU
Perihelion2.4999 AU
3.1520 AU
Eccentricity0.2069
5.60yr (2,044 days)
89.398°
0° 10m 33.96s / day
Inclination4.4633°
238.03°
130.91°
Physical characteristics
Dimensions7.183±0.136 km[6][7]
10.44 km(calculated)[3]
50.5874±0.0664 h[8]
0.057(assumed)[3]
0.237±0.088[6][7]
C(assumed)[3] · X[9]
12.9[6] · 12.90±0.17[9] · 13.1[5] · 13.184±0.005(R)[8] · 13.63[3]

21873 Jindřichůvhradec (provisional designation1999 UU3) is a dark Hygieanasteroid and relativelyslower-than average rotator from the outer region of theasteroid belt, approximately 8 kilometers (5.0 miles) in diameter.

It was discovered by Czech astronomersJana Tichá andMiloš Tichý at the South BohemianKleť Observatory on 29 October 1999, and named for the Czech town ofJindřichův Hradec.[1]

Orbit

[edit]

The asteroid is a member of theHygiea family (601),[4] a very largefamily of carbonaceous outer-belt asteroids, named after thefourth-largest asteroid,10 Hygiea.[10] It orbits the Sun in theouter main-belt at a distance of 2.5–3.8 AU once every 5 years and 7 months (2,044 days). Its orbit has aneccentricity of 0.21 and aninclination of 4° with respect to theecliptic.[5] The firstprecovery was obtained atCrimea–Nauchnij in 1982, extending the asteroid'sobservation arc by 17 years prior to its discovery.[1]

Physical characteristics

[edit]

According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer, the asteroid measures 7.2 kilometers in diameter and its surface has analbedo of 0.23.[6] Based on anabsolute magnitude of 13.63, theCollaborative Asteroid Lightcurve Link calculates a diameter of 10.4 kilometers, assuming a standard albedo for carbonaceousC-type asteroids of 0.057,[3] which is in-line with the Hygiea family's overallspectral type.[10]: 23  A large-scale survey byPan-STARRS, however, classifies the body as anX-type asteroid, which metallic core group has an intermediate albedo betweenstony and carbonaceous bodies.[9]

In September 2010, a photometriclightcurve analysis at the U.S.Palomar Transient Factory, California, gave a longrotation period of50.5874±0.0664 hours with a brightness variation of 0.61 inmagnitude (U=2).[8] This makes it a relativelyslow rotator for an asteroid of its size, which normally have periods of just a few hours rather than several days.

Naming

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Thisminor planet was named afterJindřichův Hradec, a south Bohemian town in the Czech Republic. Founded in the 13th century, it is known for its Renaissance château and Gothic church, which is exactly built on the 15th meridian east ofGreenwich. A line marks the course of the meridian in its paving stones.[2] The approved naming citation was published by theMinor Planet Center on 28 January 2002 (M.P.C. 44595).[11]

References

[edit]
  1. ^abc"21873 Jindrichuvhradec (1999 UU3)".Minor Planet Center. Retrieved3 April 2016.
  2. ^abSchmadel, Lutz D. (2007). "(21873) Jindřichůvhradec".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 868.doi:10.1007/978-3-540-29925-7_9693.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (21873) Jindrichuvhradec". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^ab"Asteroid 21873 Jindrichuvhradec – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^abc"JPL Small-Body Database Browser: 21873 Jindrichuvhradec (1999 UU3)" (2017-03-27 last obs.).Jet Propulsion Laboratory. Retrieved5 July 2017.
  6. ^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. Retrieved17 May 2016.
  7. ^abMasiero, 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. Retrieved3 December 2016.
  8. ^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. Retrieved17 May 2016.
  9. ^abcVeres, 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. Retrieved17 May 2016.
  10. ^abNesvorný, 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 978-0-8165-3213-1.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

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