308 Polyxo
 Orbital diagram | |
| Discovery | |
|---|---|
| Discovered by | A. Borrelly |
| Discovery date | 31 March 1891 |
| Designations | |
| (308) Polyxo | |
| Pronunciation | /pəˈlɪksoʊ/[1] |
Named after | Πολυξώ Polyxō |
| Main belt | |
| Adjectives | Polyxoian /pɒlɪkˈsoʊiən/ |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 124.63 yr (45,521 d) |
| Aphelion | 2.860 AU (427.8 Gm) |
| Perihelion | 2.640 AU (394.9 Gm) |
| 2.750 AU (411.4 Gm) | |
| Eccentricity | 0.040003 |
| 4.56 yr (1,665.5 d) | |
| 70.4189° | |
| 0° 12m 58.158s / day | |
| Inclination | 4.36141° |
| 181.727° | |
| 115.501° | |
| Physical characteristics | |
| Dimensions | 140.69±3.8 km[2] 130 km[3] |
| 12.031 ± 0.009 h (0.50129 ± 0.00038 d)[4] | |
| 0.043±0.002[5] | |
| T[4] (Tholen) | |
| 8.17 | |
308 Polyxo is a main-belt asteroid that was discovered by A. Borrelly on 31 March 1891, in Marseilles. It is orbiting the Sun at a distance of 2.75 AU with a low orbital eccentricity (ovalness) of 0.04 and a period of 4.56 yr. The orbital plane is tilted at an angle of 4.36° to the plane of the ecliptic.[2]
308 Polyxo is classified as a rare T-type asteroid, with a spectrum that bears some similarity to the Tagish Lake meteorite.[6] A spectral feature at a wavelength of 3.0 μm suggests aqueous alteration of some surface materials.[4] Photometric measurements reported in 1983 give a rotation period of 12.03 hours and a brightness variation of 0.20 in magnitude. The adaptive optics instrument at the W. M. Keck Observatory shows an oblate object with a diameter of 130 km. The size ratio between the major and minor axes is 1.26 ± 0.11.[3] Light curves for this object suggests it has a very irregular shape.[4]
Stellar occultation events were observed for this asteroid during 2000 and 2004. The resulting chords provided cross-section diameter estimates of 144.4 and 117.1 km, respectively.[7]
References
[edit]- ^ Webster, Noah (1884), A Practical Dictionary of the English Language
- ^ a b c "308 Polyxo". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
- ^ a b Marchis, F.; et al. (November 2006), "Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey", Icarus, vol. 185, no. 1, pp. 39–63, Bibcode:2006Icar..185...39M, doi:10.1016/j.icarus.2006.06.001, PMC 2600456, PMID 19081813.
- ^ a b c d Dotto, E.; et al. (December 2004), "308 Polyxo: ISO-SWS spectrum up to 26 micron", Astronomy and Astrophysics, 427: 1081–1084, Bibcode:2004A&A...427.1081D, doi:10.1051/0004-6361:20041638.
- ^ Dotto, E.; et al. (October 2002), "ISO observations of low and moderate albedo asteroids. PHT-P and PHT-S results", Astronomy and Astrophysics, 393: 1065–1072, Bibcode:2002A&A...393.1065D, doi:10.1051/0004-6361:20021190.
- ^ Hiroi, Takahiro; Hasegawa, Sunao (March 2003), "Revisiting the search for the parent body of the Tagish Lake meteorite - Case of a T/D asteroid 308 Polyxo", Antarctic Meteorite Research, 16: 176–184, Bibcode:2003AMR....16..176H.
- ^ Shevchenko, Vasilij G.; Tedesco, Edward F. (September 2006), "Asteroid albedos deduced from stellar occultations", Icarus, 184 (1): 211–220, Bibcode:2006Icar..184..211S, doi:10.1016/j.icarus.2006.04.006.
External links
[edit]- 308 Polyxo at AstDyS-2, Asteroids—Dynamic Site
- 308 Polyxo at the JPL Small-Body Database
