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1405 Sibelius

From Wikipedia, the free encyclopedia
Stony Florian asteroid

1405 Sibelius
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date12 September 1936
Designations
(1405) Sibelius
Named after
Jean Sibelius
(Finnish composer)[2]
1936 RE · 1951 CO
1953 VK3 · 1963 ST
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.40 yr (24,254 days)
Aphelion2.5817AU
Perihelion1.9215 AU
2.2516 AU
Eccentricity0.1466
3.38yr (1,234 days)
312.34°
0° 17m 30.12s / day
Inclination7.0301°
312.08°
95.795°
Physical characteristics
Dimensions6.21±0.35 km[4]
6.810±0.098 km[5]
7.175±0.089 km[6]
7.20 km(taken)[3]
7.204 km[7]
9.26±1.95 km[8]
12.18±1.1 km[9]
6.051±0.001h[a][b]
0.1432±0.029[9]
0.27±0.15[8]
0.3191[7]
0.3516±0.0646[6]
0.388±0.040[5]
0.458±0.068[4]
S[3][10]
12.03(R)[a] · 12.3[9] · 12.48[6] · 12.5[1][4][8] · 12.57±0.078[3][7] · 12.57±0.33[10]

1405 Sibelius (provisional designation1936 RE) is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 12 September 1936, by Finnish astronomerYrjö Väisälä atTurku Observatory in Southwest Finland.[11] The asteroid was named after composerJean Sibelius.[2]

Orbit and classification

[edit]

Sibelius is a member of theFlora family, one of the largest populations of stony asteroids in the entire main-belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,234 days). Its orbit has aneccentricity of 0.15 and aninclination of 7° with respect to theecliptic.[1] The body'sobservation arc begins with an observation taken at Turku two weeks prior to its official discovery observation.[11]

Physical characteristics

[edit]

Sibelius has been characterized as anS-type asteroid by thePan-STARRS photometric survey.[10]

Rotation period

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In October 2007, a rotationallightcurve of Sibelius was obtained from photometric observations taken byPetr Pravec at theOndřejov Observatory in theCzech Republic. Lightcurve analysis gave arotation period of 6.051 hours with a brightness variation of 0.11magnitude (U=3-).[a][b]

Diameter and albedo

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According to the surveys carried out by theInfrared Astronomical Satellite (IRAS) and NASA'sWide-field Infrared Survey Explorer (WISE) with its subsequentNEOWISE mission, Sibelius measures between 6.21 and 12.18 kilometres (3.86 and 7.57 mi) in diameter and its surface has analbedo between 0.14 and 0.48.[4][5][6][8][9] TheCollaborative Asteroid Lightcurve Link adopts an albedo of 0.3191 and a diameter of 7.20 kilometres (4.47 mi) from Petr Pravec's revised WISE thermal observations.[3][7]

Naming

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Thisminor planet was named forJean Sibelius (1865–1957), Finnish violinist and composer of the late Romantic and early-modern periods.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3928).[12]

Notes

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  1. ^abcPravec (2007) web: rotation period6.051±0.001 hours with a brightness amplitude of0.11 mag. Summary figures for (1405) Sibelius atCollaborative Asteroid Lightcurve Link andPravec, P.; Wolf, M.; Sarounova, L. (2007)
  2. ^abLightcurve plot of (1405) Sibelius from October 2007;unpublished data.

References

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  1. ^abcd"JPL Small-Body Database Browser: 1405 Sibelius (1936 RE)" (2017-07-02 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1405) Sibelius".Dictionary of Minor Planet Names – (1405) Sibelius.Springer Berlin Heidelberg. p. 113.doi:10.1007/978-3-540-29925-7_1406.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1405) Sibelius". Asteroid Lightcurve Database (LCDB). Retrieved10 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. Retrieved10 January 2017.
  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. Retrieved10 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. ^abcdPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved10 January 2017.
  8. ^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. Retrieved10 January 2017.
  9. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  10. ^abcVeres, 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. Retrieved10 January 2017.
  11. ^ab"1405 Sibelius (1936 RE)".Minor Planet Center. Retrieved10 January 2017.
  12. ^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

[edit]
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