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13390 Bouška

From Wikipedia, the free encyclopedia
Main-belt asteroid

13390 Bouška
Discovery[1]
Discovered byP. Pravec
M. Wolf
Discovery siteOndřejov Obs.
Discovery date18 March 1999
Designations
(13390) Bouška
Named after
Jiří Bouška(astronomer)[2]
1999 FQ3 · 1981 RH
1987 DN2
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc35.75 yr (13,059 days)
Aphelion3.0394AU
Perihelion2.1243 AU
2.5819 AU
Eccentricity0.1772
4.15yr (1,515 days)
212.31°
0° 14m 15.36s / day
Inclination13.246°
148.55°
250.99°
Physical characteristics
Dimensions6.48 km(calculated)[3]
7.04±0.26 km[4]
7.470±0.076[5]
7.524±0.100 km[6]
7.7572±0.0027h[7]
0.21(assumed)[3]
0.2597±0.0445[6]
0.263±0.021[5]
0.270±0.048[4]
S[3]
12.7[6] · 12.80[4] · 12.804±0.002(R)[7] · 12.9[1] · 13.25±0.41[3][8]

13390 Bouška, provisional designation1999 FQ3, is a stony Eunomiaasteroid from the central region of theasteroid belt, approximately 7 kilometers in diameter. It was discovered by Czech astronomersPetr Pravec andMarek Wolf atOndřejov Observatory in the Czech Republic on 18 March 1999.[9] It was named after astronomerJiří Bouška.[2]

Classification and orbit

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Bouška is a member of theEunomia family, a large group ofS-type asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in thecentral main-belt at a distance of 2.1–3.0 AU once every 4 years and 2 months (1,515 days). Its orbit has aneccentricity of 0.18 and aninclination of 13° with respect to theecliptic.[1] The body'sobservation arc begins 18 years prior to its official discovery observation, with its identification as1981 RH at Lowell'sAnderson Mesa Station in 1981.[9]

Physical characteristics

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A rotationallightcurve ofBouška was obtained from photometric observations made at the U.S.Palomar Transient Factory, California, in January 2012. It gave arotation period of7.7572±0.0027 hours with a brightness variation of 0.30 inmagnitude (U=2).[7]

Diameter and albedo

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According to the surveys carried out by NASA's space-basedWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bouška measures 7.5 and 7.0 kilometers in diameter and its surface has analbedo of 0.26 and 0.27, respectively.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from15 Eunomia, the family's largest member and namesake – and calculates a diameter of 6.5 kilometers.[3]

Naming

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Thisminor planet was named in honor of Jiří Bouška (born 1925), Czech astronomer and retired professor atCharles University, whose research concentrated on the material found between the planets of the Solar System.[2]

Bouška has been a teacher of several generations of Czech astronomers, including one of the discoverers. For decades he has also been the editor of theCzech Astronomical Yearbook and the popular astronomy journalRíše hvězd (The Realm of Stars), after which the minor planet4090 Říšehvězd is named.[2] The approved naming citation was published by theMinor Planet Center on 20 March 2000 (M.P.C. 39659).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 13390 Bouska (1999 FQ3)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved5 July 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(13390) Bouška".Dictionary of Minor Planet Names – (13390) Bouška.Springer Berlin Heidelberg. p. 798.doi:10.1007/978-3-540-29925-7_8808.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (13390) Bouska". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^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. Retrieved17 May 2016.
  5. ^abcMasiero, 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. Retrieved3 December 2016.
  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. ^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.
  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. Retrieved17 May 2016.
  9. ^ab"13390 Bouska (1999 FQ3)".Minor Planet Center. Retrieved6 April 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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