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6267 Rozhen

From Wikipedia, the free encyclopedia
Main-belt asteroid

6267 Rozhen
Discovery[1]
Discovered byE. W. Elst
Discovery siteRozhen Obs.
Discovery date20 September 1987
Designations
(6267) Rozhen
Named after
Rozhen Observatory
(discovering observatory)[2]
1987 SO9 · 1971 SP
1979 BR2
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc67.30 yr (24,583 days)
Aphelion2.3582AU
Perihelion1.9663 AU
2.1623 AU
Eccentricity0.0906
3.18yr (1,161 days)
72.417°
0° 18m 36s / day
Inclination2.1034°
136.75°
315.64°
Physical characteristics
Dimensions3.02 km(calculated)[3]
3.980±0.020h[4]
3.9847±0.0007 h[5]
0.24(assumed)[3]
S[3]
14.270±0.120(R)[4] · 14.3[1] · 14.316±0.001(R)[5] · 14.77[3] · 14.79±0.28[6]

6267 Rozhen, provisional designation1987 SO9, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 3 kilometers in diameter. In 1987, the asteroid was discovered byEric Elst atRozhen Observatory, Bulgaria, and was later named after the discovering observatory.

Discovery

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Rozhen was discovered on 20 September 1987, by Belgian astronomerEric Elst atRozhen Observatory near Smoljan, Bulgaria.[7] For four days, between 27 and 31 January 2005, the body was briefly and erroneously renamed6267 Smolyan.[8] In November 1949, aprecovery was taken atPalomar Observatory, extending the body'sobservation arc by 38 years prior to its official discovery observation at Rozhen.[7]

Orbit and classification

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TheS-type asteroid is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.0–2.4 AU once every 3 years and 2 months (1,161 days). Its orbit has aneccentricity of 0.09 and aninclination of 2° with respect to theecliptic.[1]

Physical characteristics

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Lightcurves

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In January 2014, two rotationallightcurves ofRozhen were obtained from photometric observations at thePalomar Transient Factory in California, United States. They gave arotation period of3.9847 and3.980 hours with a brightness variation of 0.14 and 0.12magnitude, respectively (U=2/2).[4][5]

Diameter and albedo

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TheCollaborative Asteroid Lightcurve Link assumes analbedo of 0.24, derived from8 Flora, the asteroid family's largest member and namesake, and calculates a diameter of 3.0 kilometers with anabsolute magnitude of 14.77.[3]

Naming

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Thisminor planet was named for the discoveringRozhen Observatory, also known as the "Bulgarian National Astronomical Observatory", that has been established at Rozhen in 1981.[2]

Rozhen is located near the city ofSmoljan and in proximity to the border with Greece. At 1700 meters above sea leavel, the observatory benefits from favorable instrumental and observational conditions. An exhaustive survey for the discovery of minor planets was launched at Rozhen in 1986.[2] The approved naming citation was published by theMinor Planet Center on 20 November 2002 (M.P.C. 47163).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 6267 Rozhen (1987 SO9)" (2017-03-14 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved21 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(6267) Rozhen".Dictionary of Minor Planet Names – (6267) Rozhen.Springer Berlin Heidelberg. p. 522.doi:10.1007/978-3-540-29925-7_5763.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (6267) Rozhen". Asteroid Lightcurve Database (LCDB). Retrieved4 July 2016.
  4. ^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. Retrieved4 July 2016.
  5. ^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. Retrieved4 July 2016.
  6. ^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. Retrieved4 July 2016.
  7. ^ab"6267 Rozhen (1987 SO9)".Minor Planet Center. Retrieved4 July 2016.
  8. ^"Major News about Minor Planets".hohmanntransfer.com. 28 February 2005. Archived fromthe original on 4 February 2012. Retrieved1 January 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 July 2016.

External links

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