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308 Polyxo

From Wikipedia, the free encyclopedia
Main-belt asteroid

308 Polyxo
Orbital diagram
Discovery
Discovered byAlphonse Borrelly
Discovery date31 March 1891
Designations
(308) Polyxo
Pronunciation/pəˈlɪks/[1]
Named after
ΠολυξώPolyxō
Main belt
AdjectivesPolyxoian/pɒlɪkˈsiən/
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc124.63 yr (45,521 d)
Aphelion2.860 AU (427.8 Gm)
Perihelion2.640 AU (394.9 Gm)
2.750 AU (411.4 Gm)
Eccentricity0.040003
4.56 yr (1,665.5 d)
70.4189°
0° 12m 58.158s / day
Inclination4.36141°
181.727°
115.501°
Physical characteristics
Dimensions140.69±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 amain-beltasteroid that was discovered byAlphonse Borrelly on 31 March 1891, inMarseille. It is orbiting theSun at a distance of2.75 AU with a loworbital eccentricity (ovalness) of 0.04 and aperiod of 4.56 yr. Theorbital plane is tilted at an angle of 4.36° to theplane of the ecliptic.[2]

308 Polyxo is classified as a rareT-type asteroid, with a spectrum that bears some similarity to theTagish Lake meteorite.[6] A spectral feature at a wavelength of3.0 μm suggests aqueous alteration of some surface materials.[4]Photometric measurements reported in 1983 give arotation period of 12.03 hours and a brightness variation of 0.20 inmagnitude. Theadaptive optics instrument at theW. 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 resultingchords provided cross-section diameter estimates of 144.4 and 117.1 km, respectively.[7]

References

[edit]
  1. ^Webster, Noah (1884),A Practical Dictionary of the English Language
  2. ^abc"308 Polyxo".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved11 May 2016.
  3. ^abMarchis, 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.
  4. ^abcdDotto, 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.
  5. ^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.
  6. ^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.
  7. ^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

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