308 Polyxo

{{Short description|Main-belt asteroid}}

{{Use dmy dates|date=October 2024}}

{{Infobox planet

| minorplanet = yes

| background = #D6D6D6

| name = 308 Polyxo

| discoverer = Alphonse Borrelly

| discovered = 31 March 1891

| mpc_name = (308) Polyxo

|image= 308 Polyxo Orbit Diagram.png

|caption=Orbital diagram

| pronounced = {{IPAc-en|p|ə|'|l|ɪ|k|s|oʊ}}

| alt_names =

| named_after = Πολυξώ Polyxō

| adjective = Polyxoian {{IPAc-en|p|ɒ|l|ᵻ|k|'|s|oʊ|i|ə|n}}

| mp_category = Main belt

| epoch = 31 July 2016 (JD 2457600.5)

| semimajor = {{cvt|2.74975|AU|Gm|1|adj=ri3}}

| perihelion = {{cvt|2.63975|AU|Gm|1|adj=ri3}}

| aphelion = {{cvt|2.85974|AU|Gm|1|adj=ri3|lk=on}}

| eccentricity = 0.040003

| period = {{cvt|1665.5|days|years|2|order=flip}}

| inclination = 4.36141°

| asc_node = 181.727°

| arg_peri = 115.501°

| mean_anomaly = 70.4189°

| dimensions = {{val|140.69|3.8|ul=km}}
{{val|130|u=km}}

| mass =

| density =

| rotation = {{Convert|12.031|±|0.009|h|d|abbr=on|lk=on}}

| spectral_type = T (Tholen)

| abs_magnitude = 8.17

| albedo = {{val|0.043|0.002}}

| mean_motion = {{Deg2DMS|0.216155|sup=ms}} / day

| orbit_ref =

| observation_arc = {{cvt|45521|days|years|order=flip}}

| uncertainty = 0

}}

308 Polyxo is a main-belt asteroid that was discovered by Alphonse Borrelly on 31 March 1891, in Marseille. It is orbiting the Sun at a distance of {{val|2.75|ul=AU}} with a low orbital eccentricity (ovalness) of 0.04 and a period of {{cvt|1665.5|days|years|2|disp=out}}. The orbital plane is tilted at an angle of 4.36° to the plane of the ecliptic.

308 Polyxo is classified as a rare T-type asteroid, with a spectrum that bears some similarity to the Tagish Lake meteorite. A spectral feature at a wavelength of {{val|3.0|u=micrometre}} suggests aqueous alteration of some surface materials. 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. Light curves for this object suggests it has a very irregular shape.

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.

References

{{Reflist|refs=

{{citation

| first=Noah | last=Webster | date=1884

| title=A Practical Dictionary of the English Language }}

{{Cite web

| url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=308;cad=1

| title=308 Polyxo

| work=JPL Small-Body Database

| publisher=NASA/Jet Propulsion Laboratory

| access-date=11 May 2016 }}

{{Citation

| title=Revisiting the search for the parent body of the Tagish Lake meteorite - Case of a T/D asteroid 308 Polyxo

| last1=Hiroi | first1=Takahiro | last2=Hasegawa | first2=Sunao

| journal=Antarctic Meteorite Research | postscript=.

| volume=16 | pages=176–184 | date=March 2003

| bibcode=2003AMR....16..176H }}

{{Citation

| title=308 Polyxo: ISO-SWS spectrum up to 26 micron

| display-authors=1 | last1=Dotto | first1=E.

| last2=Barucci | first2=M. A. | last3=Brucato | first3=J. R.

| last4=Müller | first4=T. G. | last5=Carvano | first5=J.

| journal=Astronomy and Astrophysics | postscript=.

| volume=427 | pages=1081–1084 | date=December 2004

| doi=10.1051/0004-6361:20041638 | bibcode=2004A&A...427.1081D | doi-access=free }}

{{citation

| title=ISO observations of low and moderate albedo asteroids. PHT-P and PHT-S results

| display-authors=1 | last1=Dotto | first1=E.

| last2=Barucci | first2=M. A. | last3=Müller | first3=T. G.

| last4=Brucato | first4=J. R. | last5=Fulchignoni | first5=M.

| last6=Mennella | first6=V. | last7=Colangeli | first7=L.

| journal=Astronomy and Astrophysics | postscript=.

| volume=393 | pages=1065–1072 | date=October 2002

| doi=10.1051/0004-6361:20021190 | bibcode=2002A&A...393.1065D | doi-access=free }}

{{Citation

| title=Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey

| first1=F. | last1=Marchis | first2=M. | last2=Kaasalainen

| first3=E. F. Y. | last3=Hom | first4=J. | last4=Berthier

| first5=J. | last5=Enriquez | first6=D. | last6=Hestroffer

| first7=D. | last7=Le Mignant | first8=I. | last8=de Pater

| display-authors=1 | work=Icarus

| volume=185 | issue=1 | pages=39–63 | date=November 2006

| bibcode=2006Icar..185...39M | pmid=19081813

| doi=10.1016/j.icarus.2006.06.001 | pmc=2600456

| postscript=. }}

{{citation

| title=Asteroid albedos deduced from stellar occultations

| last1=Shevchenko | first1=Vasilij G. | last2=Tedesco | first2=Edward F.

| journal=Icarus | postscript=.

| volume=184 | issue=1 | pages=211–220 | date=September 2006

| doi=10.1016/j.icarus.2006.04.006 | bibcode=2006Icar..184..211S }}

}}