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3288 Seleucus

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3288 Seleucus
Discovery 
Discovered byH.-E. Schuster
Discovery siteLa Silla Obs.
Discovery date28 February 1982
Designations
MPC designation(3288) Seleucus
Pronunciation/sɪˈluːkəs/
Named afterSeleucus I Nicator
(Seleucid Empire)
Alternative designations1982 DV
Minor planet categoryAmor · NEO
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc35.34 yr (12,907 days)
Aphelion2.9605 AU
Perihelion1.1053 AU
Semi-major axis2.0329 AU
Eccentricity0.4563
Orbital period (sidereal)2.90 yr (1,059 days)
Mean anomaly77.175°
Mean motion0° 20 24 / day
Inclination5.9306°
Longitude of ascending node218.65°
Argument of perihelion349.29°
Earth MOID0.1029 AU · 40.1 LD
Physical characteristics
Dimensions2.2 km
2.49±0.07 km
2.8 km (Gehrels)
2.832±1.100 km
Synodic rotation period16 h (dated)
75±5 h
75 h
Geometric albedo0.139±0.127
0.22 (Gehrels)
0.23
0.24±0.04
Spectral typeS (Tholen)  · K (SMASS)  · S
B–V = 0.910
U–B = 0.500
Absolute magnitude (H)15.2 · 15.3 · 15.5 · 15.50±0.3 · 15.6±0.3

3288 Seleucus, provisional designation 1982 DV, is a rare-type stony asteroid, classified as near-Earth object of the Amor group of asteroids, approximately 2.5 kilometers in diameter. It was discovered on 28 February 1982, by German astronomer Hans-Emil Schuster at ESO's La Silla Observatory site in northern Chile. It was named after the Hellenistic general and Seleucid ruler Seleucus I Nicator.

Orbit

Seleucus orbits the Sun in the inner main-belt at a distance of 1.1–3.0 AU once every 2 years and 11 months (1,059 days). Its orbit has an eccentricity of 0.46 and an inclination of 6° with respect to the ecliptic. Seleucus has an Earth minimum orbital intersection distance of 0.1029 AU (15,400,000 km), which corresponds to 40.1 lunar distances. As no precoveries were taken, and no prior identifications were made, the body's observation arc begins with its official discovery observation at La Silla.

Physical parameters

Spectral type

On the Tholen and SMASS taxonomic scheme, Seleucus is classified as a featureless S-type and rare K-type asteroid, respectively.

Rotation period

It has a relatively long rotation period of 75 hours with a brightness variation of 1.0 magnitude, indicative of a non-spheroidal shape (U=3/3). While most minor planets have spin rate between 2 and 20 hours, Seleucus still rotates faster than a typical slow rotator, which have periods above 100 hours.

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Seleucus measures 2.49 and 2.83 kilometers in diameter, and its surface has an albedo of 0.139 and 0.24, respectively. The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.23 and a diameter of 2.2 kilometers, based on modeled data by Alan Harris.

Naming

This minor planet is named for Seleucus I Nicator, a general in the army of Alexander the Great, and, after the death of Alexander, founder and king of the Seleucid Empire. The approved naming citation was published by the Minor Planet Center on 29 September 1985 (M.P.C. 10046).

See also

References

  1. ^ "JPL Small-Body Database Browser: 3288 Seleucus (1982 DV)" (2017-07-01 last obs.). Jet Propulsion Laboratory. Retrieved 3 July 2017.
  2. ^ Schmadel, Lutz D. (2007). "(3288) Seleucus". Dictionary of Minor Planet Names – (3288) Seleucus. Springer Berlin Heidelberg. p. 274. doi:10.1007/978-3-540-29925-7_3289. ISBN 978-3-540-00238-3.
  3. ^ "3288 Seleucus (1982 DV)". Minor Planet Center. Retrieved 9 January 2017.
  4. ^ Harris, Alan W. (February 1998). "A Thermal Model for Near-Earth Asteroids". Icarus. 131 (2): 291–301. Bibcode:1998Icar..131..291H. doi:10.1006/icar.1997.5865. Retrieved 9 January 2017.
  5. ^ Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID 9341381. Retrieved 9 January 2017.
  6. ^ Mainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; Cutri, R. M.; McMillan, R. S.; et al. (November 2012). "Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey". The Astrophysical Journal Letters. 760 (1): 6. arXiv:1210.0502. Bibcode:2012ApJ...760L..12M. doi:10.1088/2041-8205/760/1/L12. S2CID 41459166. Retrieved 9 January 2017.
  7. Debehogne, H.; de Sanctis, G.; Zappala, V. (August 1983). "Photoelectric photometry of asteroids 45, 120, 776, 804, 814, and 1982DV". Icarus. 55 (2): 236–244. Bibcode:1983Icar...55..236D. doi:10.1016/0019-1035(83)90078-7. ISSN 0019-1035. Retrieved 9 January 2017.
  8. ^ Harris, A. W.; Young, J. W.; Bowell, E.; Tholen, D. J. (November 1999). "Asteroid Lightcurve Observations from 1981 to 1983". Icarus. 142 (1): 173. Bibcode:1999Icar..142..173H. doi:10.1006/icar.1999.6181. Retrieved 9 January 2017.
  9. ^ Pravec, P.; Harris, A. W.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Hergenrother, C. W.; et al. (January 2005). "Tumbling asteroids". Icarus. 173 (1): 108–131. Bibcode:2005Icar..173..108P. doi:10.1016/j.icarus.2004.07.021. Retrieved 9 January 2017.
  10. ^ "LCDB Data for (3288) Seleucus". Asteroid Lightcurve Database (LCDB). Retrieved 9 January 2017.
  11. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 9 January 2017.

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