1619 Ueta

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 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 85.18 yr (31113 days)
Aphelion 2.6360 AU (394.34 Gm)
Perihelion 1.8455 AU (276.08 Gm)
2.2408 AU (335.22 Gm)
Eccentricity 0.17637
3.35 yr (1225.2 d)
189.56°
0° 17m 37.824s / day
Inclination 6.2141°
61.498°
328.25°
Earth MOID 0.853189 AU (127.6353 Gm)
Jupiter MOID 2.80236 AU (419.227 Gm)
Jupiter Tisserand parameter 3.606
Physical characteristics
Dimensions 9.927±0.066 km[4]
7.13±0.40 km[5]
11.04 km (calculated)[3]
2.720 h (0.1133 d)[1][6][7]
2.94 h[8]
2.7180±0.0005 h[9]
2.717943±0.000005 h[10]
0.2517±0.0317[4]
0.479±0.056[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. 1 2 3 "JPL Small-Body Database Browser: 1619 Ueta (1953 TA)" (2015-06-14 last obs.). Jet Propulsion Laboratory. Retrieved 22 April 2016.
    2. 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 15 November 2015.
    3. 1 2 3 4 "LCDB Data for (1619) Ueta". Asteroid Lightcurve Database (LCDB). Retrieved 15 November 2015.
    4. 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:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 15 November 2015.
    5. 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:1209.5794Freely accessible. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved 15 November 2015.
    6. ↑ Stephens, Robert D. (January 2011). "Asteroids Observed from GMARS and Santana Observatories: 2010 July - September". The Minor Planet Bulletin. 38 (1): 23–24. Bibcode:2011MPBu...38...23S. ISSN 1052-8091. Retrieved 15 November 2015.
    7. ↑ Higgins, David (January 2011). "Period Determination of Asteroid Targets Observed at Hunters Hill Observatory: May 2009 - September 2010". The Minor Planet Bulletin. 38 (1): 41–46. Bibcode:2011MPBu...38...41H. ISSN 1052-8091. Retrieved 15 November 2015.
    8. ↑ 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 15 November 2015.
    9. ↑ 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 15 November 2015.
    10. ↑ 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:1309.4296Freely accessible. Bibcode:2013A&A...559A.134H. doi:10.1051/0004-6361/201321993. Retrieved 15 November 2015.
    11. ↑ "1619 Ueta (1953 TA)". Minor Planet Center. Retrieved 15 November 2015.

    External links


    This article is issued from Wikipedia - version of the 9/23/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.