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1536 Pielinen

From Wikipedia, the free encyclopedia
Stony Florian asteroid

1536 Pielinen
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Observatory
Discovery date18 September 1939
Designations
(1536) Pielinen
Named after
Pielinen(lake)[2]
1939 SE · 1929 RZ
1931 ED · 1934 CW
1939 TP · 1939 UK
1952 RW · A903 SF
A916 RA
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc113.68 yr (41,521 days)
Aphelion2.6342AU
Perihelion1.7736 AU
2.2039 AU
Eccentricity0.1953
3.27yr (1,195 days)
295.85°
0° 18m 4.32s / day
Inclination1.5344°
195.69°
170.76°
Physical characteristics
Dimensions7.38±1.62 km[4]
7.82 km(calculated)[3]
7.934±0.037 km[5]
7.975±0.109 km[6]
66.1±0.1 h[7]
66.22 h[a]
66.34±0.02h[b]
67.43±0.06 h[8]
0.24(assumed)[3]
0.253±0.017[6]
0.2557±0.0662[5]
0.30±0.21[4]
S[3][9]
12.57±0.52[9] · 12.6[5] · 12.7[1][3][4]

1536 Pielinen (provisional designation1939 SE) is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 7.8 kilometers in diameter. It was discovered on 18 September 1939, by Finnish astronomerYrjö Väisälä atTurku Observatory, Southwest Finland.[10] It was later named for Finnish lakePielinen.[2]

Classification and orbit

[edit]

Pielinen is a member of theFlora family, a large group of stonyS-type asteroids. It orbits the Sun in theinner main-belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,195 days). Its orbit has aneccentricity of 0.20 and aninclination of 2° with respect to theecliptic.[1]Pielinen was first identified asA903 SF atHeidelberg in 1903, extending the body'sobservation arc by 36 years prior to its official discovery observation.[10]

Lightcurves

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From September to November 2011, four rotationallightcurves of Pielinen were obtained from photometric observations. One lightcurve analysis gave a rotation period of 66.2 hours,[c] which is significantly longer than for most minor planets, that spin every 2 to 20 hours around their axis. However,slow rotators have periods typically above 100 hours. Photometric observations were taken byPetr Pravec (66.22 hours, Δ0.85 mag,U=3),[a]Robert D. Stephens (66.34 hours, Δ0.80mag,U=3-),[b] Giovanni Casalnuovo (66.1 hours, Δ0.75 mag,U=2+),[7] andSilvano Casulli (67.43 hours, Δ0.81 mag,U=2).[8]

Diameter and albedo

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According to the space-based survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Pielinen measures between 7.38 and 7.975 kilometers in diameter and its surface has analbedo between 0.253 and 0.30.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of this family – and calculates a diameter of 7.82 kilometers, with anabsolute magnitude of 12.7.[3]

Naming

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Thisminor planet is named afterPielinen, Finland's fourth largest lake inFinnish Karelia. TheKoli National Park is located on its western shores.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3930).[11]

Notes

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  1. ^abPravec (2011) web: rotation period66.22 hours with a brightness amplitude of0.85 mag. Quality Code: 3. Summary figures for (1536) Pielinen atCollaborative Asteroid Lightcurve Link (CALL)
  2. ^abStephens (2011) web. Observations in September 2011, gave a rotation period of66.34±0.02 hours with a brightness amplitude of0.80 mag. Quality Code of 3-. Summary figures for (1536) Pielinen atCollaborative Asteroid Lightcurve Link (CALL)
  3. ^Lightcurve plot for (1536) Pielinen by Petr Pravec of the Ondrejov Asteroid Photometry Projectsource data)

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1536 Pielinen (1939 SE)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1536) Pielinen".Dictionary of Minor Planet Names – (1536) Pielinen.Springer Berlin Heidelberg. p. 122.doi:10.1007/978-3-540-29925-7_1537.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1536) Pielinen". Asteroid Lightcurve Database (LCDB). Retrieved30 December 2016.
  4. ^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. Retrieved30 December 2016.
  5. ^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.
  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. Retrieved30 December 2016.
  7. ^abCasalnuovo, Giovanni Battista (April 2016)."Lightcurve Analysis for Nine Main Belt Asteroids".The Minor Planet Bulletin.43 (2):112–115.Bibcode:2016MPBu...43..112C.ISSN 1052-8091. Retrieved30 December 2016.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1536) Pielinen".Geneva Observatory. Retrieved30 December 2016.
  9. ^abVeres, 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. Retrieved30 December 2016.
  10. ^ab"1536 Pielinen (1939 SE)".Minor Planet Center. Retrieved30 December 2016.
  11. ^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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