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12999 Toruń
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Baptistina asteroid
October 2019
yes
12999 Toruń
#D6D6D6
30 August 1981
E. Bowell
Anderson Mesa Stn.
(12999) Toruń
1981 QJ 21957 TF1998 QL 8
Toruń (Polish city)
main-beltBaptistina
4 September 2017 (JD 2458000.5)
0
59.49 yr (21,730 days)
2.7036 AU
1.8438 AU
2.2737 AU
0.1891
3.43 yr (1,252 days)
168.46°
0.2875 ms / day
5.7705°
152.34°
210.91°
3.523 0.136 km7.96 km (calculated)
3.5521 0.0026 h
0.057 (assumed)0.392 0.028
C
13.773 0.002 (R)13.813.914.22
12999 Toruń, provisional designation 1981 QJ 2, is a carbonaceous Baptistina asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 30 August 1981, by British–American astronomer Edward Bowell at Lowell Observatory's Anderson Mesa Station in Flagstaff, Arizona, and named after the Polish city of Toruń.
Orbit and classification
Toruń is a carbonaceous C-type asteroid and a member of the small Baptistina family. It orbits the Sun in the inner main-belt at a distance of 1.8–2.7 AU once every 3 years and 5 months (1,252 days). Its orbit has an eccentricity of 0.19 and an inclination of 6° with respect to the ecliptic. The first precovery was taken at Goethe Link Observatory in 1957, extending the asteroid's observation arc by 24 years prior to its discovery.
Physical characteristics
thumb|left|upright=0.6|Monument of this asteroid in Toruń, Poland
Rotation period
A rotational lightcurve of Toruń was obtained from photometric observations at the U.S. Palomar Transient Factory in December 2009. The provisional lightcurve gave a rotation period of 3.5521 0.0026 hours with a brightness amplitude of 0.09 in magnitude (U=1).
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Toruń measures 3.5 kilometers in diameter and its surface has a very high albedo of 0.39. The Collaborative Asteroid Lightcurve Link (CALL) disagrees with the findings by the space-based mission and assumes a standard albedo for carbonaceous asteroids of 0.057, with a correspondingly larger diameter of 8.0 kilometers with an absolute magnitude of 14.22. As with 1696 Nurmela, another member of the Baptistina family, CALL assumes this asteroid's composition (also see carbonaceous chondrites) to differ significantly from the much brighter asteroid 298 Baptistina, which is considered to be an interloper in its own family.
Naming
In 2008, this minor planet was named after the city of Toruń, Poland. It is the birthplace of Nicolaus Copernicus, significant to Polish and European history, a UNESCO World Heritage listed Old Town, and the main site of the Nicolaus Copernicus University, where its observatory at Piwnice, the largest in Poland, is located. The naming followed a suggestion by Polish astronomer T. Michałowski. The approved naming citation was published by the Minor Planet Center 21 March 2008 (M.P.C. 62354).
References
30em 2017-03-31 last obs.
JPL Small-Body Database Browser: 12999 Torun (1981 QJ2)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2012999
Jet Propulsion Laboratory
5 July 2017
12999 Torun (1981 QJ2)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=12999
8 April 2016
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
19 May 2016
12999
19 May 2016
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
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
1109.6407
19 May 2016
6
Adam Waszczak
Chan-Kao Chang
Eran O. Ofek
Russ Laher
Frank Masci
David Levitan
Jason Surace
Yu-Chi Cheng
Wing-Huen Ip
Daisuke Kinoshita
George Helou
Thomas A. Prince
Shrinivas Kulkarni
September 2015
Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W
The Astronomical Journal
150
3
35
2015AJ....150...75W
10.1088/0004-6256/150/3/75
1504.04041
19 May 2016
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
J. Dailey
P. R. M. Eisenhardt
R. S. McMillan
T. B. Spahr
M. F. Skrutskie
D. Tholen
R. G. Walker
E. L. Wright
E. DeBaun
D. Elsbury
T. IV Gautier
S. Gomillion
A. Wilkins
November 2011
Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M
The Astrophysical Journal
741
2
20
2011ApJ...741...68M
10.1088/0004-637X/741/2/68
1109.4096
3 December 2016
External links
Baptistina Asteroid Family and K/T Mass Extinction, Vishnu Reddy, 2013
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
12999
12999 (13000) 1981 QK3
012999
Category:Discoveries by Edward L. G. Bowell
Category:Named minor planets
19810830
Category:History of Toruń