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2013 Tucapel

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Main-belt asteroid October 2019 yes 2013 Tucapel #D6D6D6 22 October 1971 University of Chile(National Astronomical Observatory of Chile) Cerro El Roble Stn. (2013) Tucapel 1971 UH 41936 PL1940 XC1942 EP 11950 TP 21969 AT1974 MM1974 NA1974 OJ Battle of Tucapel main-beltFlora 4 September 2017 (JD 2458000.5) 0 76.32 yr (27,876 days) 2.8074 AU 1.7714 AU 2.2894 AU 0.2263 3.46 yr (1,265 days) 130.64° 0.2845 ms / day 7.5036° 96.545° 238.12° 10.61 0.72 km11.187 0.380 km11.84 km (calculated)12.16 0.75 km12.685 0.065 km 9.028 0.008 h 0.1003 0.01790.110 0.0140.24 (assumed)0.328 0.044 S 11.7011.812.27 0.6112.6 2013 Tucapel, provisional designation 1971 UH 4, is an eccentric Florian asteroid from the inner regions of the asteroid belt, approximately 11 kilometers in diameter. It was discovered on 22 October 1971, by the University of Chile's National Astronomical Observatory at Cerro El Roble Astronomical Station. It was named for one of the indigenous Mapuche chiefs. Orbit and classification Tucapel is a member of the Flora family, one of the largest groups of stony asteroids. It orbits the Sun in the inner main-belt at a distance of 1.8–2.8 AU once every 3 years and 6 months (1,265 days). Its orbit has an eccentricity of 0.23 and an inclination of 8° with respect to the ecliptic. It was first observed as 1936 PL at Johannesburg Observatory in 1936. Its first used observation was taken at Turku Observatory in 1942, when it was identified as 1942 EP 1, thereby extending the body's observation arc by 29 years prior to its official discovery observation at Cerro El Roble. Physical characteristics Tucapel has been characterized as a common S-type asteroid. Rotation period In October 2009, a rotational lightcurve of Tucapel was obtained from photometric observations at the Oakley Southern Sky Observatory (E09) in Australia. Lightcurve analysis gave a well-defined rotation period of 9.028 hours with a brightness variation of 0.34 magnitude (U=3). Diameter and albedo According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Tucapel measures between 10.61 and 12.685 kilometers in diameter and its surface has an albedo between 0.1003 and 0.328. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 — derived from 8 Flora, the family's largest member and namesake – and calculates a diameter of 11.84 kilometers with an absolute magnitude of 11.8. Naming This minor planet was named for one of the brave chiefs of the Mapuche, indigenous inhabitants of south-central Chile and southwestern Argentina, who, with his wife Gualeva, victoriously entered the city of Imperial. He died in 1560, fighting against the colonial Spaniards (also see Arauco War, Battle of Tucapel and Lautaro). The official naming citation was published by the Minor Planet Center on 1 June 1980 (M.P.C. 5359). References 30em 2017-03-29 last obs. JPL Small-Body Database Browser: 2013 Tucapel (1971 UH4) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002013 Jet Propulsion Laboratory 10 June 2017 Dictionary of Minor Planet Names – (2013) Tucapel Schmadel Lutz D. Springer Berlin Heidelberg 163 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_2014 (2013) Tucapel 2013 Tucapel (1971 UH4) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=2013 8 December 2016 MPC/MPO/MPS Archive Minor Planet Center https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html 8 December 2016 2013 8 December 2016 6 Fumihiko Usui Daisuke Kuroda Thomas G. Müller Sunao Hasegawa Masateru Ishiguro Takafumi Ootsubo Daisuke Ishihara Hirokazu Kataza Satoshi Takita Shinki Oyabu Munetaka Ueno Hideo Matsuhara Takashi Onaka October 2011 Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey Publications of the Astronomical Society of Japan 63 5 1117–1138 2011PASJ...63.1117U 10.1093/pasj/63.5.1117 free (online, AcuA catalog p. 153) 6 A. Mainzer T. Grav J. Masiero E. Hand J. Bauer D. Tholen R. S. McMillan T. Spahr R. M. Cutri E. Wright J. Watkins W. Mo C. Maleszewski November 2011 NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results The Astrophysical Journal 741 2 25 2011ApJ...741...90M 10.1088/0004-637X/741/2/90 1109.6407 6 Joseph R. Masiero A. K. Mainzer T. Grav J. M. Bauer R. M. Cutri C. Nugent M. S. Cabrera November 2012 Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M The Astrophysical Journal Letters 759 1 5 2012ApJ...759L...8M 10.1088/2041-8205/759/1/L8 1209.5794 8 December 2016 6 Jonathan Krotz Kendra Albers Landry Carbo Katherine Kragh Andrew Meiers Arnold Yim Richard Ditteon July 2010 Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37...99K The Minor Planet Bulletin 37 3 99–101 1052-8091 2010MPBu...37...99K 8 December 2016 6 Peter Veres Robert Jedicke Alan Fitzsimmons Larry Denneau Mikael Granvik Bryce Bolin Serge Chastel Richard J. Wainscoat William S. Burgett Kenneth C. Chambers Heather Flewelling Nick Kaiser Eugen A. Magnier Jeff S. Morgan Paul A. Price John L. Tonry Christopher Waters November 2015 Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V Icarus 261 34–47 2015Icar..261...34V 10.1016/j.icarus.2015.08.007 1506.00762 8 December 2016 6 Joseph R. Masiero T. Grav A. K. Mainzer C. R. Nugent J. M. Bauer R. Stevenson S. Sonnett August 2014 Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M The Astrophysical Journal 791 2 11 2014ApJ...791..121M 10.1088/0004-637X/791/2/121 1406.6645 8 December 2016 2012 Guo Shou-Jing 2013 2014 Vasilevskis 002013 002013 Category:Named minor planets 19711022