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1276 Ucclia
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Main-belt asteroid
October 2019
yes
1276 Ucclia
#D6D6D6
001276-asteroid shape model (1276) Ucclia.png
Modelled shape of Ucclia from its lightcurve
24 January 1933
E. Delporte
Uccle Obs.
(1276) Ucclia
1933 BA1963 KF
Uccle (city and observatory)
main-belt(outer)Alauda
16 February 2017 (JD 2457800.5)
0
83.79 yr (30,604 days)
3.4772 AU
2.8781 AU
3.1776 AU
0.0943
5.66 yr (2,069 days)
351.04°
0.1740 ms / day
23.274°
114.46°
333.68°
30.09 0.51 km30.34 km (derived)30.63 2.1 km (IRAS:8)33.50 0.79 km36.499 0.24040.010 0.505 km
4.9 h4.9073 0.0004 h4.90748 0.00005 h4.90768 0.00002 h
0.0528 0.00760.075 0.0090.0837 (derived)0.1303 0.019 (IRAS:8)0.141 0.006
C
10.4010.810.910.92 0.30
1276 Ucclia (prov. designation: 1933 BA) is a carbonaceous Alauda asteroid from the outer region of the asteroid belt, approximately 31 km mi off 2 us in diameter. It was discovered on 24 January 1933 by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle. Two nights later, the body was independently discovered by Richard Schorr at Bergedorf Observatory in Hamburg, Germany. It was named for the Belgium city of Uccle and its discovering observatory.
Orbit and classification
Ucclia is a member of the Alauda family (902), a large family of typically bright carbonaceous asteroids named after its parent body, 702 Alauda.23 It orbits the Sun in the outer main-belt at a distance of 2.9–3.5 AU once every 5 years and 8 months (2,069 days). Its orbit has an eccentricity of 0.09 and an inclination of 23° with respect to the ecliptic. No precoveries were taken prior to its discovery.
Naming
This minor planet was named after Uccle, in honor of both, the city and the discovering observatory (H 117).
Physical characteristics
Rotation period
A rotational lightcurve of Ucclia was obtained from photometric observations by Italian and French astronomers Silvano Casulli, Federico Manzini and Pierre Antonini in March 2007. It showed a well-defined rotation period of 4.90768 hours with a brightness variation of 0.40 in magnitude (U=3). In June 2008, a second light-curve by Slovak astronomer Adrián Galád at Modra Observatory, gave a concurring period of 4.9073 hours with an amplitude of 0.29 in magnitude (U=3-).
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Ucclia measures between 30.1 and 40.0 kilometers in diameter and its surface has an albedo between 0.05 and 0.14. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.08 and a diameter of 30.3 kilometers.
References
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1276 Ucclia (1933 BA)
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3 August 2003
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dead
Asteroid 1276 Ucclia – Nesvorny HCM Asteroid Families V3.0
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https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1276+Ucclia#Asteroid%201276%20UccliaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
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NASA Planetary Data System
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Fumihiko Usui
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External links
Lightcurve Database Query (LCDB), at www.minorplanet.info
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 – Geneva Observatory, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1276
1275 Cimbria 1276 1277 Dolores
001276
Category:Discoveries by Eugène Joseph Delporte
Category:Named minor planets
19330124