279 Thule

Outer main-belt asteroid From Wikipedia, the free encyclopedia

279 Thule is a large asteroid from the outer asteroid belt. It was discovered by Austrian astronomer Johann Palisa on 25 October 1888 in Vienna. This body was named after the ultimate northern land of Thule, according to ancient Greek and Roman lore.

Discoverydate25 October 1888
(279) Thule
Quick facts Discovery, Discovered by ...
279 Thule
Lightcurve-base 3D-model of 279 Thule.
Discovery
Discovered byJohann Palisa
Discovery date25 October 1888
Designations
(279) Thule
Pronunciation/ˈθjuːliː/[1]
A888 UA, 1920 GA
1923 RA, 1927 EC
1954 FF[2]
Asteroid belt (Thule)
AdjectivesThulean /ˈθjuːliən/[3]
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc125.34 yr (45780 d)
Aphelion4.4617880 AU (667.47398 Gm)
Perihelion4.2367660 AU (633.81117 Gm)
4.3492770 AU (650.64258 Gm)
Eccentricity0.025869
9.07 yr (3313.0 d)
62.75874°
0° 6m 31.184s / day
Inclination2.323774°
72.46791°
42.36797°
Physical characteristics
Dimensions115±12 km[4]
119±13 km[4]
23.896 h (0.9957 d)[2]
0.0412±0.003[2]
Temperature133 K
B−V=0.75[2]
U−B=0.32[2]
D (Tholen)[2]
X (SMASSII)[2]
8.57[2]
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This asteroid is orbiting the Sun at a distance of 4.35 km with an eccentricity of 0.026 and an orbital period of 9.07 years. The orbital plane is inclined at an angle of 2.32° to the plane of the ecliptic.[2] Thule was the first asteroid discovered with a semi-major axis greater than 4 AU.[citation needed] It is the only large asteroid with a 4:3 resonance orbital with Jupiter that also has a small eccentricity and orbital inclination.[5]

279 Thule is classified as a D-type asteroid and is probably composed of organic-rich silicates, carbon and anhydrous silicates. Based on infrared measurements, it spans a diameter of approximately 115 km.[4]

Thule asteroids

Thule was the first discovered member of the Thule dynamical group, which as of 2008 was known to consist of three objects: 279 Thule, (186024) 2001 QG207, and (185290) 2006 UB219.[6] The orbits of these bodies are unusual. They orbit in the outermost edge of the asteroid belt in a 4:3 orbital resonance with Jupiter, the result of the periodic force Jupiter exerts on a body with Thule's orbital period, in the same way (though with the reverse effect) as the Kirkwood gaps in the more inner parts of the asteroid belt.

More information Name, semimajor axis (au) ...
Known members as of May 2021[7][better source needed]
Name semimajor axis (au) period (years) eccentricity inclination (°) absolute magnitude Size (km)
279 Thule4.2698.820.04322.3348.53126.59±3.7
(185290) 2006 UB2194.2908.890.13357.13213.844.1–10.1
(186024) 2001 QG2074.2788.850.25133.23814.533.0–7.4
(570461) 2006 SJ424.2868.870.04655.50115.12.3–5.7
(684250) 2008 RE934.2888.880.11613.49715.491.9–4.7
(654117) 2014 WN5044.2978.910.23123.19315.51.9–4.7
2014 QX2314.2838.860.37225.93516.51.2–3.0
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See also

References

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