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1059 Mussorgskia

From Wikipedia, the free encyclopedia
Background asteroid

1059 Mussorgskia
Discovery[1]
Discovered byV. Albitzkij
Discovery siteSimeiz Obs.
Discovery date19 July 1925
Designations
(1059) Mussorgskia
Pronunciation/mʊˈsɔːrkskiə/
Named after
Modest Mussorgsky[2]
(Russian composer)
1925 OA · A916 KA
A917 UC · A920 HA
main-belt[1][3] · (middle)[4]
background[5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc97.85yr (35,739 d)
Aphelion3.1377AU
Perihelion2.1435 AU
2.6406 AU
Eccentricity0.1882
4.29 yr (1,567 d)
216.68°
0° 13m 46.92s / day
Inclination10.097°
200.37°
88.072°
Physical characteristics
17.54±3.33 km[6]
23.10±0.32 km[7]
25.227±0.139 km[8]
30.323±0.250 km[9]
36.78 km(calculated)[4]
5.519±0.002 h[10]
5.636 h[4]
5.6362±0.0006 h[11]
0.057(assumed)[4]
0.1010±0.0088[9]
0.174±0.026[8]
0.177±0.006[7]
0.23±0.21[6]
X[12] · C(SDSS-MFB)[4][a]
10.70[7][9] · 10.84±0.24[12]
10.9[3][4] · 11.04[6]

1059 Mussorgskia, provisional designation1925 OA, is a backgroundasteroid from the central regions of theasteroid belt, approximately 25 kilometers (16 miles) in diameter. It was discovered on 19 July 1925, by Soviet astronomerVladimir Albitsky at theSimeiz Observatory on the Crimean peninsula.[1] The asteroid was named for Russian composerModest Mussorgsky.[2] TheX- orC-type asteroid has arotation period of 5.636 hours.[4][a]

Orbit and classification

[edit]

Mussorgskia is a non-family asteroid from the main belt'sbackground population.[5] It orbits the Sun in thecentral asteroid belt at a distance of 2.1–3.1 AU once every 4 years and 3 months (1,567 days;semi-major axis of 2.64 AU). Its orbit has aneccentricity of 0.19 and aninclination of 10° with respect to theecliptic.[3]

The asteroid was first observed asA916 KA at Simeiz in May 1916. The body'sobservation arc begins as1920 HA atHeidelberg Observatory in April 1920, or more than 5 years prior to its official discovery observation at Simeiz.[1]

Physical characteristics

[edit]

Mussorgskia has been characterized as a commonX-type asteroid by Pan-STARRS' photometric survey. It is also characterized as a carbonaceousC-type asteroid in theSDSS-MFB (Masi Foglia Binzel) taxonomy.[4][a]

Rotation period

[edit]

In May 2002, two rotationallightcurves ofMussorgskia were obtained fromphotometric observations by Stephen Brincat at theFlarestar Observatory in Malta and by French amateur astronomerRené Roy. Lightcurve analysis gave arotation period of 5.519 and 5.6362 hours with a brightness amplitude of 0.20 and 0.21magnitude, respectively (U=2/3).[10][11] TheCollaborative Asteroid Lightcurve Link adopts a period of 5.636 hours and a brightness variation between 0.2 and 0.21 magnitude (U=3).[4]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Mussorgskia measures between 17.54 and 30.323 kilometers in diameter and its surface has analbedo between 0.1010 and 0.23.[6][7][8][9]

CALL assumes a standard albedo for carbonaceous asteroids of 0.057 and consequently calculates a larger diameter of 36.78 kilometers based on anabsolute magnitude of 10.9.[4]

Naming

[edit]

Thisminor planet was named after Russian composerModest Mussorgsky (1839–1881).[2] The officialnaming citation was published by theMinor Planet Center in November 1952 (M.P.C. 837).[13]

Notes

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  1. ^abcSearch for Unusual Spectroscopic Candidates Among 40313 minor planets from the 3rd Release of the Sloan Digital Sky Survey Moving Object Catalog (publication).SDSS-MFB (Masi Foglia Binzel) taxonomy (catalog).

References

[edit]
  1. ^abcd"1059 Mussorgskia (1925 OA)".Minor Planet Center. Retrieved26 March 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(1059) Mussorgskia".Dictionary of Minor Planet Names – (1059) Mussorgskia. Springer Berlin Heidelberg. p. 91.doi:10.1007/978-3-540-29925-7_1060.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 1059 Mussorgskia (1925 OA)" (2018-02-25 last obs.).Jet Propulsion Laboratory. Retrieved26 March 2018.
  4. ^abcdefghij"LCDB Data for (1059) Mussorgskia". Asteroid Lightcurve Database (LCDB). Retrieved26 March 2018.
  5. ^ab"Asteroid 1059 Mussorgskia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  6. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  7. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  8. ^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.S2CID 119293330.
  9. ^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.S2CID 35447010.
  10. ^abBrincat, S. H. (December 2002)."Lightcurve Photometry of Asteroid 1059 Mussorgskia".The Minor Planet Bulletin.29: 67.Bibcode:2002MPBu...29...67B. Retrieved26 March 2018.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1059) Mussorgskia". Geneva Observatory. Retrieved26 March 2018.
  12. ^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.S2CID 53493339. Retrieved26 March 2018.
  13. ^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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