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1496 Turku

From Wikipedia, the free encyclopedia
Asteroid

1496 Turku
Shape ofTurku modelled from itslightcurve
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date22 September 1938
Designations
(1496) Turku
Named after
Turku[2](Finnish city)
1938 SA1 · 1928 QN
1928 RE · 1950 EC
1954 MH · 1957 HB
main-belt · (inner)
Flora[3] · background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.02 yr (32,148 days)
Aphelion2.5631AU
Perihelion1.8490 AU
2.2060 AU
Eccentricity0.1619
3.28yr (1,197 days)
90.547°
0° 18m 2.88s / day
Inclination2.5005°
294.38°
0.9272°
Physical characteristics
Dimensions7.47±0.31 km[5]
7.758±0.072 km[6]
7.973±0.018 km[7]
8.19 km(calculated)[3]
6.47±0.01h[8]
6.47375±0.00001 h[9]
0.1930±0.0196[7]
0.203±0.024[6]
0.24(assumed)[3]
0.347±0.043[5]
S(assumed)[3]
12.40[5] · 12.42±0.25[10] · 12.6[1][3] · 12.9[7]

1496 Turku, provisional designation1938 SA1, is a Florianasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 22 September 1938, by astronomerYrjö Väisälä at theIso-Heikkilä Observatory in Turku, Finland.[11] The asteroid was named for the Finnish city ofTurku.[2]

Orbit and classification

[edit]

Turku is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main belt.[3] It is, however, a non-family asteroid from the main belt'sbackground population when applying the Hierarchical Clustering Method to its proper orbital elements.[4]

It orbits the Sun in theinner main-belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,197 days). Its orbit has aneccentricity of 0.16 and aninclination of 3° with respect to theecliptic.[1] The body'sobservation arc begins with its first identification as1928 QN atJohannesburg Observatory in August 1928, more than 10 years prior to its official discovery observation at Turku.[11]

Physical characteristics

[edit]

Turku is an assumedS-type asteroid, which is also the Flora family's overallspectral type.[3]

Rotation period and poles

[edit]

In April 2006, a rotationallightcurve ofTurku was obtained from photometric observations by French amateur astronomerLaurent Bernasconi. Lightcurve analysis gave arotation period of 6.47 hours with a brightness amplitude of 0.51magnitude, indicative of a non-spherical shape (U=3-).[8]

A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database, gave a concurring period of 6.47375 hours, as well as a spin axis of (75.0°, −75.0°) inecliptic coordinates (λ, β).[9]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Turku measures between 7.47 and 7.973 kilometers in diameter and its surface has analbedo between 0.1930 and 0.347.[5][6][7]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of the Flora family – and calculates a diameter of 8.19 kilometers based on anabsolute magnitude of 12.6.[3]

Naming

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Thisminor planet was named after Finnish city ofTurku, location of the discovering observatory and home of the discovererYrjö Väisälä. In ancient times, Turku was the capital of Finland.[2] The officialnaming citation was published by theMinor Planet Center in January 1956 (M.P.C. 1350).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1496 Turku (1938 SA1)" (2016-08-23 last obs.).Jet Propulsion Laboratory. Retrieved27 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1496) Turku".Dictionary of Minor Planet Names – (1496) Turku.Springer Berlin Heidelberg. p. 119.doi:10.1007/978-3-540-29925-7_1497.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1496) Turku". Asteroid Lightcurve Database (LCDB). Retrieved27 September 2017.
  4. ^ab"Asteroid 1496 Turku – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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. Retrieved27 September 2017.
  6. ^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. Retrieved27 September 2017.
  7. ^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.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1496) Turku".Geneva Observatory. Retrieved27 September 2017.
  9. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573.
  10. ^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. Retrieved27 September 2017.
  11. ^ab"1496 Turku (1938 SA1)".Minor Planet Center. Retrieved27 September 2017.
  12. ^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

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