279 Thule

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279 Thule
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Lightcurve-base 3D-model of 279 Thule.
Discovery
Discovered byJohann Palisa
Discovery date25 October 1888
Designations
Pronunciation/ˈθjl/[1]
A888 UA, 1920 GA
1923 RA, 1927 EC
1954 FF[2]
Asteroid belt (Thule)
AdjectivesThulean /ˈθjliən/[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°
Template:Deg2DMS / 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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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.

This asteroid orbits the Sun at a distance of 4.35 au (651 Gm), 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

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Thule was the first discovered member of the Thule dynamical group, which as of 2008 was known to consist of three objects: 279 Thule, Template:Mpl, and Template:Mpl.[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.

Known members as of May 2021[7][better source needed]
Name semimajor axis (au) period (years) eccentricity inclination (°) absolute magnitude Size (km)
279 Thule 4.269 8.82 0.0432 2.334 8.53 126.59±3.7
Template:Mpl 4.290 8.89 0.1335 7.132 13.84 Script error: No such module "sort".
Template:Mpl 4.278 8.85 0.2513 3.238 14.53 Script error: No such module "sort".
Template:Mpl 4.286 8.87 0.0465 5.501 15.1 Script error: No such module "sort".
Template:Mpl 4.288 8.88 0.1161 3.497 15.49 Script error: No such module "sort".
Template:Mpl 4.297 8.91 0.2312 3.193 15.5 Script error: No such module "sort".
Template:Mp 4.283 8.86 0.3722 5.935 16.5 Script error: No such module "sort".

See also

References

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  1. ^ Script error: No such module "template wrapper". (Subscription or participating institution membership required.)
  2. ^ a b c d e f g h i j Page Module:Citation/CS1/styles.css has no content."279 Thule". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
  3. ^ Script error: No such module "template wrapper". (Subscription or participating institution membership required.)
  4. ^ a b c Page Module:Citation/CS1/styles.css has no content.Choukroun, A.; Marciniak, A.; Ďurech, J.; Perła, J.; Ogłoza, W.; Szakats, R.; Molnar, L.; Pal, A.; Monteiro, F. (2025). "Asteroid sizes determined with thermophysical model and stellar occultations". Astronomy & Astrophysics. 698: A298. arXiv:2505.09437. Bibcode:2025A&A...698A.298C. doi:10.1051/0004-6361/202554476.
  5. ^ Page Module:Citation/CS1/styles.css has no content.Pilcher, Frederick (July 2015). "New Photometric Observations of 128 Nemisis, 249 Ilse, and 279 Thule". Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers. 42 (3): 190–192. Bibcode:2015MPBu...42..190P.
  6. ^ Page Module:Citation/CS1/styles.css has no content.Brož, M.; Vokrouhlický, D. (2008). "Asteroid families in the first-order resonances with Jupiter". Monthly Notices of the Royal Astronomical Society. 390 (2): 715–732. arXiv:1104.4004. Bibcode:2008MNRAS.390..715B. doi:10.1111/j.1365-2966.2008.13764.x. S2CID 53965791.
  7. ^ Page Module:Citation/CS1/styles.css has no content.Walker, Andrew J. (11 January 2020). "Thule MP group, 2 more candidates?". Minor Planet Mailing List. Retrieved 1 March 2025.

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