| Minorplanet | yes |
|---|---|
| Background |
|
| Discoverer | A. Maury |
| Discovery site | Palomar Obs. |
| Discovered | 2 September 1986 |
| Mpc name | (5370) Taranis |
| Alt names | 1986 RA |
| Named after | Taranis[1] (Celtic mythology) |
| Mp category | NEO · Amor[2][1] |
| Epoch | 4 September 2017 (JD 2458000.5) |
| Uncertainty | 0 |
| Observation arc | 29.93 yr (10,932 d) |
| Aphelion | 5.4438 AU |
| Perihelion | 1.2118 AU |
| Semimajor | 3.3278 AU |
| Eccentricity | 0.6359 |
| Period | 6.07 yr (2,217 days) |
| Mean anomaly | 27.914° |
| Mean motion | / day |
| Inclination | 19.131° |
| Asc node | 177.85° |
| Arg peri | 161.27° |
| Moid | 0.2196 AU · 85.6 LD |
| Jupiter moid | 0.3673 AU |
| Dimensions | 2.30 km (derived)[3] 3.6 km (Gehrels)[2] 5.308 ± 0.082 km[4][5] 6.3 ± 0.05 km[5][6] |
| Albedo | 0.037 ± 0.009[5][6] 0.051 ± 0.009[4][5] 0.20 (assumed)[3] |
| Abs magnitude | 15.2[2][4] · 15.56[3][7] |
5370 Taranis, provisional designation , is an asteroid and suspected dormant comet on an eccentric orbit, classified as near-Earth object of the Amor group, approximately 5 kilometers in diameter.
Description
Taranis was discovered on 2 September 1986, by French astronomer Alain Maury at the Palomar Observatory in California, United States.[1] It is one of very few asteroids located in the 2:1 mean-motion resonance with Jupiter.[8] When at aphelion of 5.4 AU,[2] the object is roughly the same distance from the Sun as Jupiter is when Jupiter is at aphelion. The unstable resonance with Jupiter is expected to last roughly 7.3 million years.[8]
Taranis also is expected of being a dormant comet.[5] On 10 September 2099 it will pass 0.1325 AU (19,820,000 km; 12,320,000 mi) from Earth.[2]
This minor planet was named after the Gaulish god of thunder Taranis from Celtic mythology. The official naming citation was published by the Minor Planet Center on 1 September 1993 (M.P.C. 22509).[9]
References
- ^ "5370 Taranis (1986 RA)". Minor Planet Center. Retrieved 2 February 2018.
- ^ "JPL Small-Body Database Browser: 5370 Taranis (1986 RA)" (2016-07-16 last obs.). Jet Propulsion Laboratory. Retrieved 2 February 2018.
- ^ No. 5370. Retrieved 2 February 2018.
- ^ Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D. et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 35447010
- ^ Mommert, M.; Harris, A. W.; Mueller, M.; Hora, J. L.; Trilling, D. E.; Bottke, W. F. et al. (October 2015). "ExploreNEOs. VIII. Dormant Short-period Comets in the Near-Earth Asteroid Population". The Astronomical Journal. 150 (4): 9. arXiv:1508.04116. Bibcode:2015AJ....150..106M. doi:10.1088/0004-6256/150/4/106. S2CID 34373031
- ^ Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M. et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results". The Astrophysical Journal. 743 (2): 17. arXiv:1109.6400. Bibcode:2011ApJ...743..156M. doi:10.1088/0004-637X/743/2/156. S2CID 239991
- ^ Wisniewski, W. Z. (June 1987). "Photometry of six radar target asteroids". Icarus. 70 (3): 566–572. Bibcode:1987Icar...70..566W. doi:10.1016/0019-1035(87)90096-0. ISSN 0019-1035
- ^ Roig, F.; Nesvorný, D.; Ferraz-Mello, S. (September 2002). "Asteroids in the 2 : 1 resonance with Jupiter: dynamics and size distribution [ Erratum: 2002MNRAS.336.1391R ]". Monthly Notices of the Royal Astronomical Society. 335 (2): 417–431. Bibcode:2002MNRAS.335..417R. doi:10.1046/j.1365-8711.2002.05635.x
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 2 February 2018.
External links
- (5370) Taranis at AstDyS-2
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books