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1378 Leonce
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Main-belt asteroid
October 2019
yes
1378 Leonce
#D6D6D6
File:1378Leonce (Lightcurve Inversion).png
Lightcurve-based 3D-model of Leonce
F. Rigaux
Uccle Obs.
21 February 1936
(1378) Leonce
1936 DB1958 FG1958 GY1962 KBA915 RCA915 WA
Leonce Rigaux(discoverer's father)
main-belt(inner)Nysa–Polana complex
4 September 2017 (JD 2458000.5)
0
101.54 yr (37,088 days)
2.7300 AU
2.0187 AU
2.3743 AU
0.1498
3.66 yr (1,336 days)
38.698°
0.2694 ms / day
3.5913°
43.568°
202.15°
14.94 3.81 km18.16 km (derived)18.18 1.4 km20.54 0.13 km21.228 0.070 km22.20 0.33 km22.456 0.170 km
4.3250 0.0002 h4.325 0.001 h4.32527 0.00005 h4.3586 0.0002 h
0.0348 0.00460.053 0.0020.061 0.0020.0706 (derived)0.0773 0.0130.10 0.05
C (assumed)
11.94 0.2212.1012.20
1378 Leonce, provisional designation 1936 DB, is a dark asteroid from the inner regions of the asteroid belt, approximately 19 kilometers in diameter. It was discovered on 21 February 1936, by Belgian astronomer Fernand Rigaux at the Royal Observatory of Belgium in Uccle, who named it after his father, Leonce Rigaux.
Orbit and classification
Leonce orbits the Sun in the inner main asteroid belt at a distance of 2.0–2.7 AU, once every 3 years and 8 months (1,336 days). Its orbit has an eccentricity of 0.15 and an inclination of 4° with respect to the ecliptic. It is a member of the Nysa–Polana complex, a collection of overlapping asteroid families in the inner main belt.23
The asteroid was first identified as 1915 RC at Heidelberg Observatory in September 1915. One week later, the body's observation arc begins at Bergedorf Observatory, more than 20 years prior to its official discovery observation at Uccle.
Physical characteristics
Leonce is an assumed carbonaceous C-type asteroid.
Rotation period and poles
In 2002, 2007 and 2017, three rotational light curves of Leonce were obtained from photometric observations by amateur astronomers René Roy, Laurent Bernasconi and Daniel Klinglesmith and colleagues at Etscorn Observatory (719), respectively. Analysis gave a well-defined light curve with a consolidated rotation period of 4.3250 hours and a brightness amplitude between 0.49 and 0.63 magnitude (U=3/3/3).
In addition a modeled light curve, using photometric data from various sources, gave a period of 4.32527 hours, as well as two spin axes of (210.0°, −67.0°) and (46.0°, −77.0°) in ecliptic coordinates.
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Leonce measures between 14.94 and 22.456 kilometers in diameter and its surface has an albedo between 0.0348 and 0.10.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0706 and a diameter of 18.16 kilometers based on an absolute magnitude of 12.2.
Naming
This minor planet was named after Leonce Rigaux, father of the discoverer astronomer Fernand Rigaux. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 125).
References
30em 2017-03-28 last obs.
JPL Small-Body Database Browser: 1378 Leonce (1936 DB)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001378
https://web.archive.org/web/20200918045604/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001378
18 September 2020
Jet Propulsion Laboratory
31 October 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
112
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1379 (1378) Leonce
1378 Leonce (1936 DB)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1378
31 October 2017
Asteroids and comets rotation curves – (1378) Leonce
Behrend
Raoul
Geneva Observatory
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31 October 2017
3 August 2003
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The Astrophysical Journal
791
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11
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1406.6645
31 October 2017
Asteroid 1378 Leonce – Nesvorny HCM Asteroid Families V3.0
Small Bodies Data Ferret
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26 October 2019
https://web.archive.org/web/20201107132422/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1378+Leonce#Asteroid%201378%20LeonceEAR-A-VARGBDET-5-NESVORNYFAM-V3.0
7 November 2020
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V. Carruba
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Asteroids IV
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10.2458/azu_uapress_9780816532131-ch016
1502.01628
978-0-8165-3213-1
1378
31 October 2017
6
Joseph R. Masiero
A. K. Mainzer
T. Grav
J. M. Bauer
R. M. Cutri
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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
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1209.5794
31 October 2017
6
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The Astrophysical Journal
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6
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Masateru Ishiguro
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https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab
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6
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The Astrophysical Journal
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2
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Q. Ulisse
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Astronomy and Astrophysics
559
19
2013A&A...559A.134H
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31 October 2017
Daniel A. III Klinglesmith
Jesse Hanowell
Ethan Risley
Janek Turk
Angelica Vargas
Curtis Alan Warren
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Inversion Model Candidates
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013MPBu...40..190K
The Minor Planet Bulletin
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4
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31 October 2017
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
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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
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 (1)-(5000) – Minor Planet Center
1378
1377 Roberbauxa 1378 1379 Lomonosowa
001378
Category:Discoveries by Fernand Rigaux
Category:Named minor planets
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