Astronomy:8318 Averroes
| Discovery [1] | |
|---|---|
| Discovered by | C. J. van Houten I. van Houten-G. T. Gehrels |
| Discovery site | Palomar Obs. |
| Discovery date | 29 September 1973 |
| Designations | |
| (8318) Averroes | |
| Pronunciation | /əˈvɛroʊiːz/[6] |
| Named after | Averroës [1] (medieval Muslim astronomer) |
| 1306 T-2 · 1990 QC7 | |
| Minor planet category | main-belt [1][2] · (outer) Themis [3][4] · background [5] |
| Orbital characteristics [2] | |
| Epoch 23 March 2018 (JD 2458200.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 64.13 yr (23,425 d) |
| |{{{apsis}}}|helion}} | 3.6928 AU |
| |{{{apsis}}}|helion}} | 2.6721 AU |
| 3.1824 AU | |
| Eccentricity | 0.1604 |
| Orbital period | 5.68 yr (2,074 d) |
| Mean anomaly | 245.92° |
| Mean motion | 0° 10m 24.96s / day |
| Inclination | 0.5168° |
| Longitude of ascending node | 113.64° |
| 297.35° | |
| Physical characteristics | |
| Mean diameter | 10.159±0.244 km[7] |
| Geometric albedo | 0.075±0.008[7] |
| C (est. Themis family) | |
| Absolute magnitude (H) | 13.5[1][2] |
8318 Averroes /əˈvɛroʊiːz/ is a dark Themistian asteroid from the outer regions of the asteroid belt, approximately 10 kilometers (6 miles) in diameter. It was discovered on 29 September 1973, by Dutch astronomers Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels the Palomar Observatory, and assigned the provisional designation 1306 T-2.[1] The likely C-type asteroid was named after medieval Muslim astronomer Averroës.[1]
Orbit and classification
Averroes is a core member of the Themis family (602),[3][4] a prominent family. Alternatively, a different HCM-analysis by Nesvorny found it to be a Background asteroid.[5]
It orbits the Sun in the outer asteroid belt at a distance of 2.7–3.7 AU once every 5 years and 8 months (2,074 days; semi-major axis of 3.18 AU). Its orbit has an eccentricity of 0.16 and an inclination of 1° with respect to the ecliptic.[2] The body's observation arc begins with a precovery taken at Palomar in April 1953, more than 20 years prior to its official discovery observation.[1]
Palomar–Leiden Trojan survey
Physical characteristics
While no spectral type has been determined, Averroes is likely a carbonaceous C-type asteroid, based on its membership to the Themis family and the most common type in the outer main-belt.[3] The asteroid has an absolute magnitude of 13.5.[1][2] As of 2018, no rotational lightcurve of Averroes has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[2]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Averroes measures 10.159 kilometers in diameter and its surface has an albedo of 0.075.[7]
Naming
This minor planet was named after Muhammad ibn Rushd (1126–1198),[1] also known by his Latin name as Averroes, a medieval Muslim polymath from Andalusia,[8] whose many scientific accomplishments include a study of astronomy. The name "ibn Rushd" was Latinized to "Averroes", as his commentaries on Aristotle were being translated into Latin, bringing knowledge of that famous philosopher back to Christendom, where it had been nearly forgotten. These kinds of Latin translations of the 12th century brought classical and Islamic knowledge into Europe, spurring the Renaissance. The official naming citation was published by the Minor Planet Center on 5 October 1998 (M.P.C. 32792).[9]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 "8318 Averroes (1306 T-2)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=8318.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 "JPL Small-Body Database Browser: 8318 Averroes (1306 T-2)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2008318.
- ↑ 3.0 3.1 3.2 "Asteroid 8318 Averroes". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=8318+Averroes.
- ↑ 4.0 4.1 "Asteroid (8318) Averroes". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?n=8318&pc=1.1.6.
- ↑ 5.0 5.1 "Small Bodies Data Ferret". Nesvorny HCM Asteroid Families V3.0. https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action.
- ↑ "Averroës". Averroës. Oxford University Press. http://www.lexico.com/definition/Averro%C3%ABs.[|permanent dead link|dead link}}]
- ↑ 7.0 7.1 7.2 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J. et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal 741 (2): 20. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 28 May 2018.
- ↑ Ana Ruiz, Vibrant Andalusia: The Spice of Life in Southern Spain, p. 42.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.
<ref> tag with name "MPC-Discoverers" defined in <references> is not used in prior text.External links
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
- 8318 Averroes at AstDyS-2, Asteroids—Dynamic Site
- 8318 Averroes at the JPL Small-Body Database
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