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14832 Alechinsky
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Asteroid
July 2018
yes
14832 Alechinsky
#D6D6D6
27 August 1987
E. W. Elst
La Silla Obs.
(14832) Alechinsky
1987 QC 31994 PY 32
Pierre Alechinsky(Belgian painter)
main-belt(inner)Vesta
23 March 2018 (JD 2458200.5)
0
30.76 yr (11,234 d)
2.5765 AU
2.0088 AU
2.2926 AU
0.1238
3.47 yr (1,268 d)
247.16°
0.2839 ms / day
5.7284°
307.39°
78.201°
3.92 km (calculated)4.359 0.176 km
8.07 0.02 h
0.194 0.0160.24 (assumed)
S (assumed)
14.214.462 0.010 (R)
14832 Alechinsky (provisional designation 1987 QC 3) is a Vestian asteroid from the inner regions of the asteroid belt, approximately 4 km mi off us in diameter. It was discovered on 27 August 1987, by Belgian astronomer Eric Elst at ESO's La Silla Observatory site in northern Chile. The highly elongated asteroid has a rotation period of 8.1 hours. It was named after Belgian painter Pierre Alechinsky.
Orbit and classification
Alechinsky is a member of the Vesta family. Vestian asteroids have a composition akin to cumulate eucrites (HED meteorites) and are thought to have originated deep within 4 Vesta's crust, possibly from the Rheasilvia crater, a large impact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision. It orbits the Sun in the inner main-belt at a distance of 2.0–2.6 AU once every 3 years and 6 months (1,268 days; semi-major axis of 2.29 AU). Its orbit has an eccentricity of 0.12 and an inclination of 6° with respect to the ecliptic. The asteroid's observation arc begins in 1987, as no precoveries had been taken prior to its discovery.
Naming
This minor planet was named in honor of Belgian painter and internationally prominent 20th century artist, Pierre Alechinsky (born 1927), known for his treatment of colors, versatility and graphic humor. He was a member of the expressionist art group and avant-garde movement CoBrA, a name which was coined from the initials of the members' home cities: Copenhagen, Brussels, and Amsterdam. The approved naming citation was published by the Minor Planet Center on 13 October 2000 (M.P.C. 41387).
Physical characteristics
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Alechinsky measures 4.4 kilometers in diameter and its surface has an albedo of 0.194, while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – which derives from 8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 3.9 kilometers with an absolute magnitude of 14.2.
Rotation period
In February 2013, two rotational lightcurves of Alechinsky were obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory, California. Lightcurve analysis gave a rotation period of 8.07 0.02 and 9.5831 0.1453 hours, with a brightness variation of 0.98 and 1.30 in magnitude, respectively (U=2+/2). Such an exceptionally high amplitude in magnitude indicates that the body has a very elongated shape.
References
30em 2018-05-25 last obs.
JPL Small-Body Database Browser: 14832 Alechinsky (1987 QC3)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2014832
Jet Propulsion Laboratory
27 July 2018
Dictionary of Minor Planet Names – (14832) Alechinsky
Schmadel Lutz D.
Springer Berlin Heidelberg
817
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_9052 (14832) Alechinsky
14832 Alechinsky (1987 QC3)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=14832
27 July 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
27 July 2018
Asteroid 14832 Alechinsky
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=14832+Alechinsky
27 July 2018 October 2026 InternetArchiveBot
14832
6 April 2016
6
A. Mainzer
T. Grav
J. Masiero
E. Hand
J. Bauer
D. Tholen
R. S. McMillan
T. Spahr
R. M. Cutri
E. Wright
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W. Mo
C. Maleszewski
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NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
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The Astrophysical Journal
741
2
25
2011ApJ...741...90M
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1109.6407
8 May 2016
6
Chan-Kao Chang
Wing-Huen Ip Ip Wing-huen
Hsing-Wen Lin
Yu-Chi Cheng
Chow-Choong Ngeow
Ting-Chang Yang
Adam Waszczak
Shrinivas R. Kulkarni
David Levitan
Branimir Sesar
Russ Laher
Jason Surace
Thomas. A. Prince
June 2014
313 New Asteroid Rotation Periods from Palomar Transient Factory Observations
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...788...17C
The Astrophysical Journal
788
1
21
2014ApJ...788...17C
10.1088/0004-637X/788/1/17
1405.1144
6 April 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
6 April 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
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
Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
14832
14831 Gentileschi 14832 14833 Vilenius
014832
Category:Discoveries by Eric Walter Elst
Category:Named minor planets
19870827