|Discovered by||Johann Palisa|
|Discovery date||25 October 1888|
|MPC designation||(279) Thule|
|1927 EC, 1954 FF, A920 GA, A923 RA|
|Asteroid belt (Thule)|
|Epoch 31 July 2016 (JD 2457600.5)|
|Uncertainty parameter 0|
|Observation arc||125.34 yr (45780 d)|
|Aphelion||4.4617880 AU (667.47398 Gm)|
|Perihelion||4.2367660 AU (633.81117 Gm)|
|4.3492770 AU (650.64258 Gm)|
|9.07 yr (3313.0 d)|
|0° 6m 31.184s / day|
|Dimensions||126.59±3.7 km (IRAS)|
|23.896 h (0.9957 d)|
The orbit of Thule is unusual. It appears to orbit in the farthest edge of the Main belt in a 3:4 orbital resonance with planet Jupiter. Unlike the Hilda asteroids whose eccentricity is fairly common of main belt asteroids, Thule has a very low eccentricity - actually much lower than that of Jupiter itself and only a bit higher than that of Earth. Why it has this orbit is not clear, as is the reason for the absence of smaller bodies in similar 4:3 resonances with Jupiter.
Some astronomers have argued that Thule's present orbit is the natural result of the force of Jupiter on a body orbiting at exactly the distance from the Sun Thule does, in the same way (though with the reverse effect) as the Kirkwood gaps in the more closer parts of the asteroid belt. It could thus be that the resonance which holds Thule in a very low-eccentricity orbit serves to eject other smaller bodies whose distance from the Sun is only a bit different from that of Thule itself.
It is the main member of the Thule dynamical group.
References[change | change source]
Other websites[change | change source]
- 279 Thule on NASA/JPL Small-Body Database