1339 Désagneauxa
| Discovery [1] | |
|---|---|
| Discovered by | L. Boyer |
| Discovery site | Algiers Observatory |
| Discovery date | 4 December 1934 |
| Designations | |
| 1339 Desagneauxa | |
Named after | brother-in-law of Louis Boyer[2] |
| 1934 XB · 1951 AF | |
| main-belt · Eos [3] | |
| Orbital characteristics [1] | |
| Epoch 27 June 2015 (JD 2457200.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 80.55 yr (29,420 days) |
| Aphelion | 3.1936 AU |
| Perihelion | 2.8440 AU |
| 3.0188 AU | |
| Eccentricity | 0.0578 |
| 5.25 yr (1,916 days) | |
| 109.81° | |
| Inclination | 8.6923° |
| 291.00° | |
| 162.55° | |
| Physical characteristics | |
| Dimensions | 22.96 km[4] 24.20±0.65 km[5] 25.733±0.200 km[6] 23.04 km (derived)[3] |
| 9.380 h[7] 9.3209±0.0006 h[8] 9.37510±0.00005 h[9] | |
| 0.1589[4] 0.151±0.009[5] 0.1274±0.0165[6] 0.1747 (derived)[3] | |
| B–V = 0.790 U–B = 0.425 Tholen = S S [3] | |
| 10.7 | |
1339 Désagneauxa, provisional designation 1934 XB, is an asteroid from the outer region of the asteroid belt, about 23 kilometers in diameter. It was discovered on 4 December 1934 by French astronomer Louis Boyer at the Algiers Observatory in Algeria, North Africa.[10] The body was independently discovered, just a few nights later, by the Russian and Belgian astronomers, Grigory Neujmin and Eugène Delporte, at the Crimean Simeiz and Belgian Uccle Observatory, respectively.[2]
The S-type asteroid is a member of the Eos family, thought to have formed from a catastrophic collision of its parent body resulting in more than 4,000 known members of the family. It orbits the Sun at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,916 days). Its orbit shows an eccentricity of 0.06 and is tilted by 9 degrees to the plane of the ecliptic. It has a rotation period of about 9.4 hours.[7][8][9] Based on observations carried out by the Infrared Astronomical Satellite, IRAS, the Japanese Akari satellite, and the Wide-field Infrared Survey Explorer, the body's geometric albedo is in the range of 0.13– 0.16, while the Collaborative Asteroid Lightcurve Link derives a value for its albedo of 0.17.[3][4][5][6]
The discoverer, Louis Boyer, named the asteroid in honour of his brother-in-law.[2]
References
- ^ a b "JPL Small-Body Database Browser: 1339 Desagneauxa (1934 XB)" (2015-06-22 last obs.). Jet Propulsion Laboratory. Retrieved November 2015.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b c Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1339) Désagneauxa. Springer Berlin Heidelberg. p. 109. ISBN 978-3-540-29925-7. Retrieved November 2015.
{{cite book}}: Check date values in:|accessdate=(help) - ^ a b c d e "LCDB Data for (1339) Desagneauxa". Asteroid Lightcurve Database (LCDB). Retrieved November 2015.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b c Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. Bibcode:2004PDSS...12.....T. Retrieved November 2015.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b c Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved November 2015.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b c Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved November 2015.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Bennefeld, Craig; Cantu, Jenel; Holly, Vashti; Jordon, Latoya; Martin, Tierra; Soar, Elysabeth; et al. (April 2009). "Asteroid Lightcurve Analysis at Ricky Observatory". Bulletin of the Minor Planets. 36 (2). Section of the Association of Lunar and Planetary Observers: 45–48. Bibcode:2009MPBu...36...45B. ISSN 1052-8091. Retrieved November 2015.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1339) Desagneauxa". Geneva Observatory. Retrieved November 2015.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b Hanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013). "An anisotropic distribution of spin vectors in asteroid families". Astronomy & Astrophysics. 559: 19. arXiv:1309.4296. Bibcode:2013A&A...559A.134H. doi:10.1051/0004-6361/201321993. Retrieved November 2015.
{{cite journal}}: Check date values in:|access-date=(help) - ^ "1339 Desagneauxa (1934 XB)". Minor Planet Center. Retrieved November 2015.
{{cite web}}: Check date values in:|accessdate=(help)
External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1339 Désagneauxa at the JPL Small-Body Database
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