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1554 Yugoslavia

From Wikipedia, the free encyclopedia
Stony Eunomian asteroid from the middle region of the asteroid belt

1554 Yugoslavia
Shape model of Yugoslavia from itslightcurve
Discovery[1]
Discovered byM. B. Protitch
Discovery siteBelgrade Observatory
Discovery date6 September 1940
Designations
(1554) Yugoslavia
Named after
Yugoslavia
(country, 20th century)[2]
1940 RE · 1932 YA
1935 JN · 1936 UH
1948 MH
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc83.98 yr (30,672 days)
Aphelion3.1486AU
Perihelion2.0889 AU
2.6188 AU
Eccentricity0.2023
4.24yr (1,548 days)
62.174°
0° 13m 57.36s / day
Inclination12.151°
217.12°
131.60°
Physical characteristics
Dimensions14.73±1.13 km[4]
15.94 km(calculated)[3]
16.185±0.107 km[5]
17.198±0.160 km[6]
21.39±1.31 km[7]
3.8876±0.0001h[8]
3.8879±0.0003 h[9]
3.89±0.01 h[10]
0.070±0.009[7]
0.1043±0.0145[6]
0.117±0.026[5]
0.21(assumed)[3]
0.269±0.048[4]
S[3]
11.20[4] · 11.3[1][3] · 11.9[7][6]

1554 Yugoslavia (provisional designation1940 RE) is a stony Eunomianasteroid from the middle region of theasteroid belt, approximately 16 kilometres (9.9 mi) in diameter. It was discovered by Serbian astronomerMilorad Protić atBelgrade Astronomical Observatory, Serbia, on 6 September 1940.[11] It was named for the former country ofYugoslavia.[2]

Orbit and classification

[edit]

The asteroid is a member of theEunomia family, a large group of mostly stonyS-type asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in thecentral main-belt at a distance of 2.1–3.1 AU once every 4 years and 3 months (1,548 days). Its orbit has aneccentricity of 0.20 and aninclination of 12° with respect to theecliptic.[1] Yugoslavia was first identified as1932 YA atUccle Observatory in 1932. Itsobservation arc begins 4 year prior to its official discovery observation, with aprecovery taken atNice Observatory in 1936.[11]

Physical characteristics

[edit]

From 2007 to 2012, several photometriclightcurve observations of Yugoslavia established a well-definedrotation period of 3.89 hours with a brightness variation between 0.64 and 0.74magnitude (U=3/3/3).[8][9][10]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Yugoslavia measures between 14.73 and 21.39 kilometers in diameter, and its surface has analbedo between 0.070 and 0.269.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from15 Eunomia, the family's largest member and namesake – and calculates a diameter of 15.94 kilometers with anabsolute magnitude of 11.3.[3]

Naming

[edit]

Thisminor planet was named after the former country ofYugoslavia.[2] The officialnaming citation was published by theMinor Planet Center on 30 January 1964 (M.P.C. 2277).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1554 Yugoslavia (1940 RE)" (2016-12-14 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1554) Yugoslavia".Dictionary of Minor Planet Names – (1554) Yugoslavia.Springer Berlin Heidelberg. p. 123.doi:10.1007/978-3-540-29925-7_1555.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1554) Yugoslavia". Asteroid Lightcurve Database (LCDB). Retrieved30 December 2016.
  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. Retrieved30 December 2016.
  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. Retrieved30 December 2016.
  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. ^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. ^abBenishek, Vladimir (April 2013)."Lightcurves for 366 Vincentina, 592 Bathseba, and 1544 Yugoslavia from Belgrade Astronomical Observatory".The Minor Planet Bulletin.40 (2):100–101.Bibcode:2013MPBu...40..100B.ISSN 1052-8091. Retrieved30 December 2016.
  9. ^abHiggins, David (March 2008)."Asteroid Lightcurve Analysis at Hunters Hill Observatory and Collaborating Stations: April 2007 - June 2007".The Minor Planet Bulletin.35 (1):30–32.Bibcode:2008MPBu...35...30H.ISSN 1052-8091. Retrieved30 December 2016.
  10. ^abRuthroff, John C. (April 2013)."Lightcurve Analysis of Main Belt Asteroids 1115 Sabauda 1554 Yugoslavia, 1616 Filipoff, 2890 Vilyujsk, (5153) 1940 GO, and (31179) 1997 YR2".The Minor Planet Bulletin.40 (2):90–91.Bibcode:2013MPBu...40...90R.ISSN 1052-8091. Retrieved30 December 2016.
  11. ^ab"1554 Yugoslavia (1940 RE)".Minor Planet Center. Retrieved30 December 2016.
  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]
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Authority control databasesEdit this at Wikidata
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