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4090 Říšehvězd

From Wikipedia, the free encyclopedia
Asteroid
4090 Říšehvězd
Discovery[1]
Discovered byA. Mrkos
Discovery siteKleť Obs.
Discovery date2 September 1986
Designations
(4090) Říšehvězd
Named after
Říše hvězd
(astronomy journal)[2]
1986 RH1 · 1931 FF
1971 KB · 1982 KX
1988 AR3 · 1989 GU
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.03 yr (31,421 days)
Aphelion2.8513AU
Perihelion1.8632 AU
2.3573 AU
Eccentricity0.2096
3.62yr (1,322 days)
252.91°
0° 16m 20.28s / day
Inclination1.3288°
266.55°
4.4078°
Physical characteristics
Dimensions6.27 km(calculated)[3]
7.195±0.299 km[4][5]
4.5312±0.0090h(R)[6]
4.550±0.020 h(R)[7]
4.5553±0.0090 h(R)[6]
0.149±0.032[4][5]
0.20(assumed)[3]
S[3]
12.91±0.24[8] · 13.080±0.160(R)[7] · 13.114±0.002(R)[6] · 13.2[1] · 13.38[3] · 13.4[4]

4090 Říšehvězd, provisional designation1986 RH1, is a stonyasteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter.

It was discovered by Czech astronomerAntonín Mrkos atKleť Observatory on 2 September 1986. Named for the astronomy journalŘíše hvězd, it is known as having had the mostdiacritics in its name among allnamed minor planets before the naming of229762 Gǃkúnǁʼhòmdímà.[2][9]

Classification and orbit

[edit]

TheS-type asteroid orbits the Sun at a distance of 1.9–2.9 AU once every 3 years and 7 months (1,322 days). Its orbit has aneccentricity of 0.21 and aninclination of 1° with respect to theecliptic.[1] The first observation was made at the U.S.Yerkes Observatory in 1931, extending the asteroid'sobservation arc by 55 years prior to its official discovery.[9]

Physical characteristics

[edit]

In 2009 and 2014, several rotationallightcurves were obtained for this asteroid at thePalomar Transient Factory. They gave a concurringrotation period between 4.53 and 4.56 hours with a brightness variation between 0.32 and 0.41magnitude (U=2/2/2).[6][7]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures 7.2 kilometers in diameter and its surface has analbedo of 0.149,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 6.3 kilometers, based on an absolute magnitude of 13.38.[3]

Naming

[edit]

Thisminor planet was named after the periodically released Czech popularastronomy journal Říše hvězd ("the realm of stars"), which was initially published by the Czech Astronomical Society.[2]

Říše hvězd reported discoveries in the fields of astronomy, astrophysics and space exploration and supplied information about the Czech–Slovak astronomical community. The body's name was proposed byJana Tichá,Miloš Tichý andZdeněk Moravec.[2] Naming citation was published on 28 August 1996 (M.P.C. 27734).[10]

See also

[edit]
  • Jiří Grygar, chairman of theCzech Astronomical Society and editor atŘíše hvězd

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 4090 Risehvezd (1986 RH1)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved19 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(4090) Říšehvězd".Dictionary of Minor Planet Names – (4090) Říšehvězd.Springer Berlin Heidelberg. p. 349.doi:10.1007/978-3-540-29925-7_4067.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4090) Říšehvězd". Asteroid Lightcurve Database (LCDB). Retrieved25 October 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.
  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. Retrieved5 December 2016.
  6. ^abcdWaszczak, 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. Retrieved25 October 2016.
  7. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved25 October 2016.
  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. Retrieved25 October 2016.
  9. ^ab"4090 Risehvezd (1986 RH1)".Minor Planet Center. Retrieved25 October 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved25 October 2016.

External links

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