1619 Ueta
Discovery [1] | |
---|---|
Discovered by | T. Mitani |
Discovery site | Kwasan Observatory |
Discovery date | 11 October 1953 |
Designations | |
MPC designation | 1619 Ueta |
Named after |
Mr Ueta (observatory's director)[2] |
1953 TA · 1926 RR 1931 AO · 1940 YJ 1951 AG1 · 1978 GM | |
main-belt · (inner) [3] | |
Orbital characteristics [1] | |
Epoch 27 June 2015 (JD 2457200.5) | |
Uncertainty parameter 0 | |
Observation arc | 84.42 yr (30,835 days) |
Aphelion | 2.6359 AU |
Perihelion | 1.8469 AU |
2.2414 AU | |
Eccentricity | 0.1760 |
3.36 yr (1,226 days) | |
130.77° | |
Inclination | 6.2127° |
61.512° | |
328.26° | |
Physical characteristics | |
Dimensions |
±0.066 km 9.927[4] ±0.40 km 7.13[5] 11.04 km (calculated)[3] |
2.720 h[6][7] h 2.94[8] ±0.0005 h 2.7180[9] 943±0.000005 h 2.717[10] | |
±0.0317 0.2517[4] ±0.056 0.479[5] 0.20 (assumed)[3] | |
B–V = 0.900 U–B = 0.546 Tholen = S S [3] | |
12.15 | |
|
1619 Ueta, provisional designation 1953 TA, is a stony asteroid from the inner regions of the asteroid belt, about 11 kilometers in diameter. It was discovered by Japanese astronomer Tetsuyasu Mitani at Kyoto University's Kwasan Observatory on 11 October 1953.[11]
The S-type asteroid orbits the Sun at a distance of 1.8–2.6 AU once every 3 years and 4 months (1,226 days). Its orbit shows an eccentricity of 0.18 and is tilted by 6 degrees to the plane of the ecliptic. It has a rotation period of 2.7 hours and an albedo around 0.25,[4] with a divergent result of 0.5.[5]
It was named by the discoverer after the former Director of Kwasan Observatory (also see § External links) who encouraged him to keep on with his observations of asteroids and comets.[2]
References
- 1 2 "JPL Small-Body Database Browser: 1619 Ueta (1953 TA)" (2015-06-14 last obs.). Jet Propulsion Laboratory. Retrieved November 2015.
- 1 2 Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1619) Ueta. Springer Berlin Heidelberg. p. 128. ISBN 978-3-540-29925-7. Retrieved November 2015.
- 1 2 3 4 "LCDB Data for (1619) Ueta". Asteroid Lightcurve Database (LCDB). Retrieved November 2015.
- 1 2 3 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; 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.
- 1 2 3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved November 2015.
- ↑ Stephens, Robert D. (January 2011). "Asteroids Observed from GMARS and Santana Observatories: 2010 July - September". Bulletin of the Minor Planets (Section of the Association of Lunar and Planetary Observers) 38 (1): 23–24. Bibcode:2011MPBu...38...23S. ISSN 1052-8091. Retrieved November 2015.
- ↑ Higgins, David (January 2011). "Period Determination of Asteroid Targets Observed at Hunters Hill Observatory: May 2009 - September 2010". Bulletin of the Minor Planets (Section of the Association of Lunar and Planetary Observers) 38 (1): 41–46. Bibcode:2011MPBu...38...41H. ISSN 1052-8091. Retrieved November 2015.
- ↑ Almeida, R.; Angeli, C. A.; Duffard, R.; Lazzaro, D. (February 2004). "Rotation periods for small main-belt asteroids". Astronomy and Astrophysics. Bibcode:2004A&A...415..403A. doi:10.1051/0004-6361:20034585. Retrieved November 2015.
- ↑ Kryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; et al. (October 2012). "Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region". Astronomy & Astrophysics 546: 51. Bibcode:2012A&A...546A..72K. doi:10.1051/0004-6361/201219199. Retrieved November 2015.
- ↑ Hanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; 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.
- ↑ "1619 Ueta (1953 TA)". Minor Planet Center. Retrieved November 2015.
External links
- Kwasan Observatory – Kyoto University
- Kwasan and Hida observatories
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1619 Ueta at the JPL Small-Body Database
|
|