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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
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R. S. McMillan
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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