3288 Seleucus

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Discoverydate28 February 1982
(3288) Seleucus
3288 Seleucus
Discovery[1]
Discovered byH.-E. Schuster
Discovery siteLa Silla Obs.
Discovery date28 February 1982
Designations
(3288) Seleucus
Pronunciation/sɪˈlkəs/
Named after
Seleucus I Nicator
(Seleucid Empire)[2]
1982 DV
Amor · NEO[1][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc35.34 yr (12,907 days)
Aphelion2.9605 AU
Perihelion1.1053 AU
2.0329 AU
Eccentricity0.4563
2.90 yr (1,059 days)
77.175°
0° 20m 24s / day
Inclination5.9306°
218.65°
349.29°
Earth MOID0.1029 AU · 40.1 LD
Physical characteristics
Dimensions2.2 km[4]
2.49±0.07 km[5]
2.8 km (Gehrels)[1]
2.832±1.100 km[6]
16 h (dated)[7]
75±5 h[8]
75 h[9]
0.139±0.127[6]
0.22 (Gehrels)[1]
0.23[4]
0.24±0.04[5]
S (Tholen)[1] · K (SMASS)[1] · S[10]
B–V = 0.910[1]
U–B = 0.500[1]
15.2[5] · 15.3[1] · 15.5[4][10] · 15.50±0.3[6] · 15.6±0.3[8]

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.[3] It was named after the Hellenistic general and Seleucid ruler Seleucus I Nicator.[2]

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.[1] Seleucus has an Earth minimum orbital intersection distance of 0.1029 AU (15,400,000 km), which corresponds to 40.1 lunar distances.[1] 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.[3]

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.[1]

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).[8][9] 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.[5][6] 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.[4][10]

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.[2] The approved naming citation was published by the Minor Planet Center on 29 September 1985 (M.P.C. 10046).[11]

See also

References

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