|Discovered by||Johann Palisa|
|Discovery time||October 25, 1888|
|Reference date 30 January, 2005 (JD 2453400.5)|
|Longest distance from the Sun||647.712 Gm (4.33 AU)|
|Shortest distance from the Sun||631.907 Gm (4.224 AU)|
|Longest distance from the center of its orbital path
|639.809 Gm (4.277 AU)|
|How egg-shaped its orbit is
|How long it takes to complete an orbit||3230.561 d (8.84 a)|
|Angle above the reference plane
|Longitude of where it comes up through the reference plane||73.642°|
|Angle between its shortest distance from what it orbits around and where it comes up through the reference plane
("argument of periapsis")
|Size and Other Qualities|
|Slowest speed able to escape into space
|How long it takes to turn around one time||unknown|
|How much light it reflects||unknown|
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.
Other websites[change | edit source]
- 279 Thule on NASA/JPL Small-Body Database