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1550 Tito

From Wikipedia, the free encyclopedia
Asteroid

1550 Tito
Discovery[1]
Discovered byM. B. Protitch
Discovery siteBelgrade Obs.
Discovery date29 November 1937
Designations
(1550) Tito
Named after
Josip Broz Tito(statesman)[2]
1937 WD · 1941 XA
1941 YE · 1945 WB
1949 UR · 1983 CG3
main-belt · (middle)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.34 yr (28,979 days)
Aphelion3.3418AU
Perihelion1.7471 AU
2.5444 AU
Eccentricity0.3134
4.06yr (1,482 days)
256.39°
0° 14m 34.08s / day
Inclination8.8802°
64.500°
311.14°
Physical characteristics
Dimensions9.47±2.13 km[3]
11.391±0.108 km[4]
11.45±0.28 km[5]
11.98±0.15 km[6]
12.39 km(calculated)[7]
12.431±0.062 km[8]
12.88±2.28 km[9]
13.652±2.335 km[10]
30±1h[11]
54.2±0.3 h[12]
54.53±0.01 h[13]
0.181±0.055[10]
0.20(assumed)[7]
0.2021±0.0196[8]
0.22±0.09[9]
0.239±0.007[6]
0.25±0.10[3]
0.257±0.045[5]
SMASS =S[1] · S[7]
11.8[5][6][8][9][10] · 11.9[1][7] · 11.96±0.39[14] · 12.12[3]

1550 Tito (provisional designation1937 WD) is a stonyasteroid from the middle region of theasteroid belt, approximately 12 kilometers in diameter. It was discovered on 29 November 1937, by Serbian astronomerMilorad B. Protić at theBelgrade Astronomical Observatory in Serbia.[15] It was named for Yugoslavian statesmanJosip Broz Tito.[2]

Classification and orbit

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Tito orbits the Sun at a distance of 1.7–3.3 AU once every 4 years and 1 month (1,482 days). Its orbit has aneccentricity of 0.31 and aninclination of 9° with respect to theecliptic.[1] Tito'sobservation arc begins 4 years after its official discovery observation, with its first used observation taken at Belgrade in 1941. Noprecoveries were taken and no prior identifications were made.[15]

Physical characteristics

[edit]

In theSMASS classification, Tito is characterized as a commonS-type asteroid.[1]

Rotation period

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Tito has arotation period of approximately 54 hours. While this does not make it aslow rotator, it has a significantly longer period than the vast majority of minor planets, which typically spin every 2 to 20 hours around their axis. Rotationallightcurves ofTito were obtained from photometric observations byWalter R. Cooney Jr. in January 2003, who derived a period of 54.2 hours (Δmag 0.23,U=2),[12] by Raymond Poncy in December 2006, who obtained a shorter, provisional period of 30 hours (Δmag 0.16,U=2),[11] and byDavid Higgins in December 2010, who derived a period of 54.53 hours (Δmag 0.40,U=2).[13]

Diameter and albedo

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According to the surveys carried out by theSpitzer Space Telescope, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Tito measures between 9.47 and 13.652 kilometers in diameter, and its surface has analbedo between 0.181 and 0.257.[3][4][5][6][8][9][10] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 12.39 kilometers with anabsolute magnitude of 11.9.[7]

Naming

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Tito was named in honour ofJosip Broz Tito (1892–1980), leader of theYugoslavian resistance during theWorld War II, early enthusiast of theUnited Nations, and president of formerYugoslavia.[2] The officialnaming citation was published by theMinor Planet Center on 30 January 1964 (M.P.C. 2277).[16]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1550 Tito (1937 WD)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved5 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1550) Tito".Dictionary of Minor Planet Names – (1550) Tito.Springer Berlin Heidelberg. p. 123.doi:10.1007/978-3-540-29925-7_1551.ISBN 978-3-540-00238-3.
  3. ^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.
  4. ^abMasiero, 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. Retrieved30 December 2016.
  5. ^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.S2CID 46350317. Retrieved30 December 2016.
  6. ^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)
  7. ^abcde"LCDB Data for (1550) Tito". Asteroid Lightcurve Database (LCDB). Retrieved30 December 2016.
  8. ^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.
  9. ^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.S2CID 9341381. Retrieved30 December 2016.
  10. ^abcdRyan, E. L.; Mizuno, D. R.; Shenoy, S. S.; Woodward, C. E.; Carey, S. J.; Noriega-Crespo, A.; et al. (June 2015)."The kilometer-sized Main Belt asteroid population revealed by Spitzer".Astronomy and Astrophysics.578: 12.arXiv:1204.1116.Bibcode:2015A&A...578A..42R.doi:10.1051/0004-6361/201321375.S2CID 21069867. Retrieved30 December 2016.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1550) Tito".Geneva Observatory. Retrieved30 December 2016.
  12. ^abCooney, Walter R. Jr.; Pozzoli, Valentino; Gross, John (March 2004)."Rotation period and lightcurve of minor planet 1550 Tito".The Minor Planet Bulletin.31 (1):23–24.Bibcode:2004MPBu...31...23C.ISSN 1052-8091. Retrieved30 December 2016.
  13. ^abHiggins, David; Benishek, Validimir (April 2011)."Period Determination of Asteroid 1550 Tito".The Minor Planet Bulletin.38 (2):79–80.Bibcode:2011MPBu...38...79H.ISSN 1052-8091. Retrieved30 December 2016.
  14. ^Veres, 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. Retrieved30 December 2016.
  15. ^ab"1550 Tito (1937 WD)".Minor Planet Center. Retrieved30 December 2016.
  16. ^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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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