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1446 Sillanpää

From Wikipedia, the free encyclopedia
Stony Florian asteroid

1446 Sillanpää
Shape ofSillanpää modelled from itslightcurve
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date26 January 1938
Designations
(1446) Sillanpaa
Named after
Frans Sillanpää(writer)[2]
1938 BA · 1935 GB
1952 HQ3 · 1955 DQ
1965 EA
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc78.53 yr (28,683 days)
Aphelion2.4732AU
Perihelion2.0179 AU
2.2455 AU
Eccentricity0.1014
3.37yr (1,229 days)
98.112°
0° 17m 34.44s / day
Inclination5.2572°
17.549°
196.25°
Physical characteristics
Dimensions7.35±0.29 km[4]
8.167±0.154 km[5]
8.19 km(calculated)[3]
8.763±0.063 km[6]
9.65855±0.00005h[7]
9.659±0.001 h[8]
9.6597±0.0172 h[9]
9.6602±0.0008 h[a]
0.2109±0.0108[6]
0.24(assumed)[3]
0.241±0.046[5]
0.327±0.080[4]
S[3]
12.394±0.002(R)[9] · 12.50[4] · 12.6[1][3][6]

1446 Sillanpää, provisional designation1938 BA, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 8.2 kilometers in diameter. It was discovered on 26 January 1938, by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland.[10] It was later named after writerFrans Eemil Sillanpää.[2]

Orbit and classification

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TheS-type asteroid is a member of theFlora family, one of the largest populations of stony asteroids in the main-belt. It orbits the Sun at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,229 days). Its orbit has aneccentricity of 0.10 and aninclination of 5° with respect to theecliptic.[1]Sillanpää was first identified as1935 GB atSimeiz Observatory in 1935, while itsobservation arc begins with its official discovery observation at Turku in 1938.[10]

Lightcurves

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In March 2009, Czech astronomerPetr Pravec obtained a rotationallight-curve from photometric observations atOndřejov Observatory.[b] It gave a well-definedrotation period of 9.6602 hours with a brightness variation of 0.55magnitude (U=3).[a] One month later, a concurring period of 9.659 hours with an amplitude of 0.71 magnitude was obtained byAdrián Galád atModra Observatory (U=3).[8] Photometric observations at thePalomar Transient Factory in December 2011. gave a 9.6597 hours and Δ0.59 in magnitude (U=2).[9] A modeled light-curve using data from theUppsala Asteroid Photometric Catalogue and other data sources, gave a period of 9.65855 hours, as well as a spin axis of (129.0°, 76.0°) inecliptic coordinates (U=n.a.).[7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Sillanpää measures between 7.35 and 8.76 kilometers in diameter, and its surface has analbedo between 0.21 and 0.327.[5][6][4] TheCollaborative Asteroid Lightcurve Link assumes an intermediate albedo of 0.24 – derived from8 Flora, the largest member and namesake of this asteroid family – and calculates a larger diameter of 8.19 kilometers using anabsolute magnitude of 12.6.[3]

Naming

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Thisminor planet was named after one of the most famous Finnish writers,Frans Eemil Sillanpää (1888–1964), first Finnish writer to receive theNobel Prize in Literature in 1939(also seeList of Laureates since 1901).[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3928).[11]

References

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  1. ^abPravec (2009) web: rotation period9.6602±0.0008 hours with a brightness amplitude of0.55 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1446) Sillanpaa andPravec, P.; Wolf, M.; Sarounova, L. (2009)
  2. ^Light-curve analysis:screenshot
  1. ^abcd"JPL Small-Body Database Browser: 1446 Sillanpaa (1938 BA)" (2016-08-07 last obs.).Jet Propulsion Laboratory. Retrieved4 January 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1446) Sillanpää".Dictionary of Minor Planet Names – (1446) Sillanpää.Springer Berlin Heidelberg. p. 116.doi:10.1007/978-3-540-29925-7_1447.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1446) Sillanpää". Asteroid Lightcurve Database (LCDB). Retrieved4 January 2017.
  4. ^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.
  5. ^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. 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. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved4 January 2017.
  8. ^abGalad, Adrian (October 2009)."Byproduct Targets During Photometric Observations from Modra".The Minor Planet Bulletin.36 (4):183–186.Bibcode:2009MPBu...36..183G.ISSN 1052-8091. Retrieved4 January 2017.
  9. ^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. Retrieved4 January 2017.
  10. ^ab"1446 Sillanpaa (1938 BA)".Minor Planet Center. Retrieved4 January 2017.
  11. ^Schmadel, Lutz D. (2009). "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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