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1509 Esclangona
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Hungaria asteroid and binary system from the inner regions of the asteroid belt
October 2019
yes
1509 Esclangona
#D6D6D6
21 December 1938
A. Patry
Nice Obs.
(1509) Esclangona
1938 YG
Ernest Esclangon(French astronomer)
main-belt(inner)Hungaria
4 September 2017 (JD 2458000.5)
0
77.68 yr (28,374 days)
1.9263 AU
1.8064 AU
1.8663 AU
0.0321
2.55 yr (931 days)
225.08°
0.3866 ms / day
22.320°
283.52°
267.82°
1
6.83 1.32 km7.52 1.78 km8.17 0.6 km (IRAS:2)8.18 km (derived)9.0 1.0 km9.87 0.37 km
2.64 0.02 h3.247 h3.247 0.002 h3.252 0.005 hLighcurve-plot3.2524 0.0003 h3.25250 0.00005 h3.25281 0.00002 hLCDB-Pravec-20093.25283 0.00002 h5.89 hLCDB-CALL-2011
0.107 0.0210.160 0.0130.185 0.0550.2041 (derived)0.2327 0.038 (IRAS:2)0.30 0.140.41 0.18
Tholen = SKSB–V = 0.894U–B = 0.472
12.33 0.14 (R)LCDB-Pravec-200912.6412.7912.858 0.14913.28 0.0
1509 Esclangona (provisional designation 1938 YG) is a rare-type Hungaria asteroid and binary system from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It is named after French astronomer Ernest Esclangon.
Discoveries
Esclangona was discovered on 21 December 1938, by French astronomer André Patry at Nice Observatory. The body's observation arc begins with its official discovery observation as no precoveries were taken, and no prior identifications were made. On 13 February 2003, a satellite was discovered by astronomers at ESO's Very Large Telescope (UT4) on Cerro Paranal in Chile.
Orbit and classification
Esclangona is a member of the Hungaria family, which form the innermost concentration of asteroids in the Solar System. It orbits the Sun in the inner main-belt at a distance of 1.8–1.9 AU once every 2 years and 7 months (931 days). Its orbit has an eccentricity of 0.03 and an inclination of 22° with respect to the ecliptic.
Binary system
Esclangona has a small moon, provisionally designated S/2003 (1509) 1, which measures 4 kilometers in diameter, and orbits 140 kilometers from its parent. This wide separation relative to the pair's size is rather unusual and it is believed that both Esclangona and its moon are ejecta from an asteroidal collision in the past that left the scene as a co-orbiting pair; a similar pairing is 3749 Balam and its outer moon.
Physical characteristics
In the Tholen taxonomy, Esclangona is a common stony S-type asteroid. It has since been characterized as a rare K-type asteroid by polarimetric observations.
Rotation period
In December 2004, photometric measurements of Esclangona made by American astronomer Brian Warner at his Palmer Divide Observatory, California, showed a lightcurve with a rotation period of 3.247 0.002 hours and a brightness variation of 0.17 0.02 in magnitude.Lighcurve-plot
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, Esclangona measures between 6.83 and 9.87 kilometers in diameter and its surface has an albedo between 0.107 and 0.41. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.2041 and a diameter of 8.18 kilometers with an absolute magnitude of 12.858.
Naming
This minor planet was named after French astronomer Ernest Esclangon (1876–1954), was a director of the Paris Observatory and president of the International Astronomical Union. Naming citation was first mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 134).
Notes
Lighcurve-plot http://www.minorplanetobserver.com/pdolc/A1509_2013.HTM Lightcurve plot of 1509 Esclangona Palmer Divide Observatory, B. D. Warner (2013)
LCDB-Pravec-2009 Pravec (2009) web: Date: 2009-10-06. Rotation period 3.25281 0.00002 hours with a brightness amplitude of 0.13 mag. Flagged as binary. Quality code: n.a. Summary figures at http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1509%7CEsclangona Collaborative Asteroid Lightcurve Link (CALL) for (1509) Esclangona
LCDB-CALL-2011 CALL (2011) web: rotation period 5.89 hours with a brightness amplitude of 0.35 mag. Quality code: n.a. Summary figures at http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1509%7CEsclangona Collaborative Asteroid Lightcurve Link (CALL) for (1509) Esclangona
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External links
Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
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
1509
1508 Kemi 1509 1510 Charlois
001509
Category:Discoveries by André Patry
Category:Named minor planets
001509
001509
19381221