Astronomy:2934 Aristophanes
Discovery [1] | |
---|---|
Discovered by | C. J. van Houten I. van Houten-G. T. Gehrels |
Discovery site | Palomar Obs. |
Discovery date | 25 September 1960 |
Designations | |
(2934) Aristophanes | |
Pronunciation | /ˌærɪˈstɒfəniːz/[4] |
Named after | Ἀριστοφάνης Aristophanēs[2] (ancient Greek dramatist) |
4006 P-L · 1971 OQ1 1977 RM5 · 1980 FC9 | |
Minor planet category | main-belt · (outer) Veritas [3] |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 56.24 yr (20,543 days) |
|{{{apsis}}}|helion}} | 3.3326 AU |
|{{{apsis}}}|helion}} | 3.0085 AU |
3.1705 AU | |
Eccentricity | 0.0511 |
Orbital period | 5.65 yr (2,062 days) |
Mean anomaly | 99.361° |
Mean motion | 0° 10m 28.56s / day |
Inclination | 8.7965° |
Longitude of ascending node | 202.23° |
89.870° | |
Physical characteristics | |
Dimensions | 21.941±0.390 km[5] |
Geometric albedo | 0.110±0.006[5] |
SMASS = Ch [1] | |
Absolute magnitude (H) | 11.7[1] |
2934 Aristophanes /ˌærɪˈstɒfəniːz/, provisional designation 4006 P-L, is a carbonaceous Veritasian asteroid from the outer regions of the asteroid belt, approximately 22 kilometers in diameter. It was discovered during the Palomar–Leiden survey in 1960, and later named after ancient Greek dramatist Aristophanes.
Discovery
Aristophanes was discovered on 25 September 1960, by Dutch astronomers Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at the Palomar Observatory, California, United States.[6]
Palomar–Leiden survey
Orbit and classification
Aristophanes is a member of the Veritas family (609),[3] a young family of carbonaceous asteroids, that formed approximately 8.5±0.5 million years ago. The family is named after 490 Veritas and consists of nearly 1,300 members.[7]:8,23
It orbits the Sun in the outer main-belt at a distance of 3.0–3.3 AU once every 5 years and 8 months (2,062 days). Its orbit has an eccentricity of 0.05 and an inclination of 9° with respect to the ecliptic.[1] The body's observation arc begins at Palomar, the night prior to its official discovery observation.[6]
Physical characteristics
In the SMASS classification, Aristophanes is a Ch-type,[1] a hydrated subtype of the carbonaceous C-type asteroid with absorption features at 0.7 μm.[8]
Rotation period
As of 2017, no rotational lightcurve of Aristophanes has been obtained from photometric observations. The asteroid's rotation period, shape and poles remain unknown.[1][9]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Aristophanes measures 21.941 kilometers in diameter and its surface has an albedo of 0.110.[5]
Naming
This minor planet was named after Aristophanes (445–385 B.C.), a Greek comic playwright of ancient Athens.[2] The official naming citation was published by the Minor Planet Center on 29 September 1985 (M.P.C. 10044).[10]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "JPL Small-Body Database Browser: 2934 Aristophanes (4006 P-L)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002934.
- ↑ 2.0 2.1 Schmadel, Lutz D. (2007). "(2934) Aristophanes". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 241. doi:10.1007/978-3-540-29925-7_2935. ISBN 978-3-540-00238-3.
- ↑ 3.0 3.1 "Asteroid 2934 Aristophanes – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=2934+Aristophanes#Asteroid%202934%20AristophanesEAR-A-VARGBDET-5-NESVORNYFAM-V3.0.
- ↑ "Aristophanes". Aristophanes. Oxford University Press. http://www.lexico.com/definition/Aristophanes.
- ↑ 5.0 5.1 5.2 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 8 October 2017.
- ↑ 6.0 6.1 "2934 Aristophanes (4006 P-L)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=2934.
- ↑ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 978-0-8165-3213-1. Bibcode: 2015aste.book..297N.
- ↑ Bus, Schelte J.; Binzel, Richard P. (July 2002). "Phase II of the Small Main-Belt Asteroid Spectroscopic Survey. A Feature-Based Taxonomy". Icarus 158 (1): 146–177. doi:10.1006/icar.2002.6856. Bibcode: 2002Icar..158..146B. http://vigarano.ep.sci.hokudai.ac.jp/shogo/adv_geochemistry2015/Week%204/Background%20reading/Bus%20and%20Binzel%202002.pdf. Retrieved 8 October 2017.
- ↑ "LCDB Data for (2934) Aristophanes". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2934%7CAristophanes.
- ↑ "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
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 2934 Aristophanes at AstDyS-2, Asteroids—Dynamic Site
- 2934 Aristophanes at the JPL Small-Body Database
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