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279 Thule
From Wikipedia, the free encyclopedia
| Discovery A | |
|---|---|
| Discoverer | Johann Palisa |
| Discovery date | October 25, 1888 |
| Alternate designations B |
|
| Category | Main belt (Thule) |
| Orbital elements C | |
|
|
|
| Eccentricity (e) | 0.012 |
| Semi-major axis (a) | 639.809 Gm (4.277 AU) |
| Perihelion (q) | 631.907 Gm (4.224 AU) |
| Aphelion (Q) | 647.712 Gm (4.33 AU) |
| Orbital period (P) | 3230.561 d (8.84 a) |
| Mean orbital speed | 14.4 km/s |
| Inclination (i) | 2.338° |
| Longitude of the ascending node (Ω) |
73.642° |
| Argument of perihelion (ω) |
82.821° |
| Mean anomaly (M) | 274.796° |
| Physical characteristics D | |
| Dimensions | 127.0 km |
| Mass | unknown |
| Density | unknown |
| Surface gravity | unknown |
| Escape velocity | unknown |
| Rotation period | unknown |
| Spectral class | D |
| Absolute magnitude | 8.57 |
| Albedo (geometric) | unknown |
| Mean surface temperature |
unknown |
279 Thule (pronounced[help] /ˈθjuːli/ thew'-lee) is a very large Main belt asteroid. It is classified as a D-type asteroid and is probably composed of organic rich silicates, carbon and anhydrous silicates.
The orbit of Thule is unusual. It appears to orbit in the outermost edge of the Main belt in a 3:4 orbital resonance with planet Jupiter. Unlike the Hilda asteroids whose eccentricity is fairly typical of main belt asteroids, Thule has a very low eccentricity - actually much lower that that of Jupiter itself and only slightly higher than that of Earth. The origin of 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 precisely the distance from the Sun Thule does, in the same way (though with the reverse effect) as the Kirkwood gaps in the more inner parts of the asteroid belt. It could thus be that the resonance which holds Thule in an extremely low-eccentricity orbit serves to eject other smaller bodies whose distance from the Sun is only slightly different from that of Thule itself.
It is the sole member of the Thule dynamical group.
It was discovered by Johann Palisa on October 25, 1888 in Vienna and was named aptly after the ultimate northern land of Thule.
- 279 Thule on NASA/JPL Small-Body Database
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| Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Neptune Trojans · Comets · Trans-Neptunians (Kuiper belt • Scattered disc objects • Oort cloud) |
| For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons, meteoroids and the Solar System. For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. |