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7545 Smaklösa

From Wikipedia, the free encyclopedia
Main-belt asteroid

7545 Smaklösa
Discovery[1]
Discovered byC.-I. Lagerkvist
Discovery siteMount Stromlo Obs.
Discovery date28 July 1978
Designations
(7545) Smaklösa
Named after
Smaklösa
(Swedish band)[2]
1978 OB · 1995 OP
main-belt · (inner)[3]
background
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.61 yr (14,104 days)
Aphelion2.7888AU
Perihelion1.7342 AU
2.2615 AU
Eccentricity0.2332
3.40yr (1,242 days)
174.45°
0° 17m 23.28s / day
Inclination6.5200°
114.89°
200.04°
Physical characteristics
Dimensions4.131±0.112 km[4][5]
4.30 km(calculated)[3]
14.3002±0.0218h[6]
14.322±0.004[7]
14.330±0.220 h[8]
0.20(assumed)[3]
0.237±0.025[4][5]
S[3]
14.1[4] · 14.2[1][3] · 14.650±0.300(R)[8] · 14.666±0.005(R)[6]

7545 Smaklösa, provisional designation1978 OB, is a stony backgroundasteroid from the inner regions of theasteroid belt, approximately 4 kilometers in diameter. It was discovered on 28 July 1978, by Swedish astronomerClaes-Ingvar Lagerkvist atMount Stromlo Observatory in Canberra, Australia.[9] The asteroid was named for the Swedish bandSmaklösa.[2]

Orbit and classification

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Smaklösa orbits the Sun in theinner main-belt at a distance of 1.7–2.8 AU once every 3 years and 5 months (1,242 days). Its orbit has aneccentricity of 0.23 and aninclination of 7° with respect to theecliptic.[1] As noprecoveries were taken, the asteroid'sobservation arc begins with its discovery in 1978.[9]

Physical characteristics

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Lightcurves

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In August 2012, a rotationallightcurve ofSmaklösa was obtained at the Oakley Southern Sky Observatory in Coonabarabran, Australia. Thephotometric observation showed a well-definedrotation period of14.322±0.004 hours with a brightness variation of 0.75 inmagnitude (U=3).[7] Similar periods of14.330±0.220 and14.3002±0.0218 hours were derived at the U.SPalomar Transient Factory in 2014 (U=2/2).[6][8]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Smaklösa measures 4.1 kilometers in diameter and its surface has analbedo of 0.24,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo forstony asteroids of 0.20 and calculates a diameter of 4.3 kilometers.[3]

Naming

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Thisminor planet was named after theGotlandic music groupSmaklösa. (Literally "Flavourless", but also "Tasteless" or "Tacky". The latter meaning is intended here as indicated by the name of their own record label "Tasteless Records").[10]

The Swedish band gave a number of concerts on the island of Gotland. They are known for their cleverly phrased lyrics mixed with the local humor of the island. The discoverer of this minor planet has named it after the band, grateful for having attended their concerts in 1998, which are unforgettable to him.[2] The official naming citation was published by theMinor Planet Center on 8 December 1998 (M.P.C. 33387).[11]

See also

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References

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  1. ^abcd"JPL Small-Body Database Browser: 7545 Smaklosa (1978 OB)" (2017-03-09 last obs.).Jet Propulsion Laboratory. Retrieved22 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(7545) Smaklösa".Dictionary of Minor Planet Names – (7545) Smaklösa.Springer Berlin Heidelberg. p. 602.doi:10.1007/978-3-540-29925-7_6546.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (7545) Smaklosa". Asteroid Lightcurve Database (LCDB). Retrieved17 May 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. Retrieved17 May 2016.
  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. Retrieved4 December 2016.
  6. ^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.
  7. ^abSimpson, Gary; Chong, Elena; Gerhardt, Michael; Gorsky, Sean; Klaasse, Matthew; Kodalen, Brian; et al. (July 2013)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 August - October".The Minor Planet Bulletin.40 (3):146–151.Bibcode:2013MPBu...40..146S.ISSN 1052-8091. Retrieved14 April 2016.
  8. ^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. Retrieved17 May 2016.
  9. ^ab"7545 Smaklosa (1978 OB)".Minor Planet Center. Retrieved14 April 2016.
  10. ^Larson, Johanna (16 December 2014)."Kulturpriset till Smaklösa" [Culture Prize awarded to "Smaklösa"].www.gotland.se (in Swedish).Gotland Municipality. Retrieved23 June 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

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