279 Thule
279 Thule is a very big Main belt asteroid. It is classified as a D-type asteroid and is probably made of organic rich silicates, carbon and anhydrous silicates
| Discovery | |
|---|---|
| Discovered by | Johann Palisa |
| Discovery date | 25 October 1888 |
| Designations | |
| MPC designation | (279) Thule |
| Pronunciation | /ˈθjuːli/ THEW-lee[2] |
| 1927 EC, 1954 FF, A920 GA, A923 RA[1] | |
| Asteroid belt (Thule) | |
| Orbital characteristics[1] | |
| 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) | |
| Eccentricity | 0.025869 |
| 9.07 yr (3313.0 d) | |
| 62.75874° | |
| 0° 6m 31.184s / day | |
| Inclination | 2.323774° |
| 72.46791° | |
| 42.36797° | |
| Physical characteristics | |
| Dimensions | 126.59±3.7 km (IRAS)[1] |
| 23.896 h (0.9957 d)[1] | |
| 0.0412±0.003[1] | |
| Temperature | 133 K |
| B−V=0.75[1] U−B=0.32[1] D (Tholen)[1] X (SMASSII)[1] | |
| 8.57[1] | |
279 Thule is a very big Main belt asteroid. It is classified as a D-type asteroid and is probably made of organic rich silicates, carbon and anhydrous silicates.
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 closer parts of the asteroid belt. It could 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.
It was found by Johann Palisa on October 25, 1888 in Vienna and was named after the ultimate northern land of Thule.
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 "279 Thule". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
- ↑ "Thule". Oxford English Dictionary second edition. Oxford University Press. 1989. Retrieved 7 December 2018.
Other websites
- 279 Thule on NASA/JPL Small-Body Database
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.