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1447 Utra

From Wikipedia, the free encyclopedia
Stony asteroid, slow rotator and suspected tumbler

1447 Utra
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date26 January 1938
Designations
(1447) Utra
Named after
Utra(Finnish town)[2]
1938 BB · 1936 SB
1951 KO · A918 FA
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc98.67 yr (36,038 days)
Aphelion2.6404AU
Perihelion2.4299 AU
2.5352 AU
Eccentricity0.0415
4.04yr (1,474 days)
285.64°
0° 14m 39.12s / day
Inclination4.7865°
35.528°
64.085°
Physical characteristics
Dimensions11.83±0.86 km[4]
11.834±0.122 km[5]
12.634±0.103 km[6]
13.26±0.53 km[7]
13.58 km(calculated)[3]
257±30h[a]
0.20(assumed)[3]
0.303±0.038[7]
0.3381±0.0591[6]
0.381±0.058[4]
S[3]
11.30[4][6][7] · 11.60±0.44[8] · 11.7[1][3]

1447 Utra, provisional designation1938 BB, is a stonyasteroid,slow rotator and suspected tumbler from the central region of theasteroid belt, approximately 12 kilometers in diameter. It was discovered on 26 January 1938, by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland.[9] The asteroid was named for the Finnish town ofUtra (now a part ofJoensuu).[2]

Orbit and classification

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Utra is aS-type asteroid. It orbits the Sun in thecentral main-belt at a distance of 2.4–2.6 AU once every 4.04 years (1,474 days). Its orbit has aneccentricity of 0.04 and aninclination of 5° with respect to theecliptic.[1]Utra was first identified asA918 FA atHeidelberg Observatory in 1918. The body'sobservation arc begins with its official discovery observation at Turku in 1938.[9]

Physical characteristics

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Slow rotator

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In March 2011, a rotationallightcurve ofUtra was obtained from photometric observations by astronomer Luis E. Martinez. Lightcurve analysis gave a longrotation period of 257 hours with a brightness variation of 0.63magnitude (U=2). Thisslow rotator is also a suspected tumbler (T0).[a]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Utra measures between 11.83 and 13.26 kilometers in diameter, and its surface has analbedo between 0.303 and 0.381.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 13.58 kilometers with anabsolute magnitude of 11.7.[3]

Naming

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Thisminor planet was named for Utra, a northeastern Finnish town and birthplace of the discoverer.[2] The officialnaming citation was published by theMinor Planet Center on 30 January 1964 (M.P.C. 2277).[10]

Notes

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  1. ^abMartinez (2011) web: rotation period257±30 hours with a brightness amplitude of0.63 mag. Summary figures for (1447) Utra atCollaborative Asteroid Lightcurve Link (CALL). Thereferenced website was a non-recoverable dead link.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1447 Utra (1938 BB)" (2016-11-14 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1447) Utra".Dictionary of Minor Planet Names – (1447) Utra.Springer Berlin Heidelberg. p. 116.doi:10.1007/978-3-540-29925-7_1448.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1447) Utra". Asteroid Lightcurve Database (LCDB). Retrieved4 January 2017.
  4. ^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)
  5. ^abMasiero, 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. Retrieved4 January 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.
  7. ^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. Retrieved4 January 2017.
  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. Retrieved4 January 2017.
  9. ^ab"1447 Utra (1938 BB)".Minor Planet Center. Retrieved4 January 2017.
  10. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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