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2747 Český Krumlov

From Wikipedia, the free encyclopedia
Carbonaceous main-belt asteroid

2747 Cesky Krumlov
Orbital diagram of Český Krumlov
Discovery[1]
Discovered byA. Mrkos
Discovery siteKleť Obs.
Discovery date19 February 1980
Designations
(2747) Cesky Krumlov
PronunciationCzech:[ˈtʃɛskiːˈkrʊmlof]
Named after
Český Krumlov
(Czech town)[2]
1980 DW · 1953 FO1
1975 EK5 · 1977 SV2
1977 TM3 · 1977 TS7
1982 OM
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.93 yr (23,351 days)
Aphelion3.4959AU
Perihelion2.6996 AU
3.0978 AU
Eccentricity0.1285
5.45yr (1,991 days)
183.40°
0° 10m 50.88s / day
Inclination5.8182°
344.88°
302.03°
Physical characteristics
Dimensions20.62 km(calculated)[3]
22.51±6.03 km[4]
22.57±7.52 km[5]
28.39±0.98 km[6]
29.804±0.174 km[7]
32.103±0.239 km[8]
32.63 km[9]
36.33±0.66 km[10]
438.7098±9.1557h[11]
0.028±0.004[7][10]
0.0380±0.004[9]
0.0393±0.0040[8]
0.05±0.08[4]
0.051±0.004[6]
0.057(assumed)[3]
0.06±0.07[5]
X[12] · C[3]
11.6[6][8] · 11.70[5][10] · 11.706±0.003(R)[11] · 11.8[1] · 11.97±0.27[12] · 12.16[3]

2747 Český Krumlov (Czech:[ˈtʃɛskiːˈkrumlof]), provisional designation1980 DW, is a carbonaceousasteroid andslow rotator from the outer regions of theasteroid belt, approximately 22 kilometers in diameter. It was discovered by Czech astronomerAntonín Mrkos atKleť Observatory on 19 February 1980, and named for the Czech town ofČeský Krumlov.[2][13]

Orbit and classification

[edit]

Český Krumlov belongs to theHygiea family.[citation needed] It orbits the Sun in theouter main-belt at a distance of 2.7–3.5 AU once every 5 years and 5 months (1,991 days). Its orbit has aneccentricity of 0.13 and aninclination of 6° with respect to theecliptic.[1]

It was first identified as1953 FO1 atAlmaty Observatory (210) in 1953. The body'sobservation arc begins four weeks later with aprecovery taken atPalomar Observatory, 27 years prior to its official discovery observation at Klet Observatory.[13]

Physical characteristics

[edit]

Český Krumlov has been characterized as anX-type and carbonaceousC-type asteroid.[3][12]

Slow rotator

[edit]

In October 2010, a rotationallightcurve of Český Krumlov was obtained from photometric observations by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 438.7098 hours with a brightness variation of 0.63magnitude (U=2).[11] This makes it a veryslow rotator.

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Český Krumlov measures between 22.51 and 36.33 kilometers in diameter and its surface has analbedo between 0.028 and 0.06.[4][5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 20.62 kilometers with anabsolute magnitude of 12.16.[3]

Naming

[edit]

Thisminor planet was named after the historic Czech town ofČeský Krumlov, near to the location of the discovering Kleť Observatory.[2] The approved naming citation was published by theMinor Planet Center on 29 November 1993 (M.P.C. 22828).[14]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2747 Cesky Krumlov (1980 DW)" (2017-03-21 last obs.).Jet Propulsion Laboratory. Retrieved18 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2747) Český Krumlov".Dictionary of Minor Planet Names – (2747) Český Krumlov.Springer Berlin Heidelberg. p. 225.doi:10.1007/978-3-540-29925-7_2748.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2747) Český Krumlov". Asteroid Lightcurve Database (LCDB). Retrieved18 June 2017.
  4. ^abcNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  5. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved18 June 2017.
  6. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  7. ^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.S2CID 119293330. Retrieved18 June 2017.
  8. ^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 35447010.
  9. ^abcTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  10. ^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.S2CID 46350317. Retrieved18 June 2017.
  11. ^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. Retrieved18 June 2017.
  12. ^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.S2CID 53493339. Retrieved18 June 2017.
  13. ^ab"2747 Cesky Krumlov (1980 DW)".Minor Planet Center. Retrieved18 June 2017.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 June 2017.

External links

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