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5023 Agapenor

From Wikipedia, the free encyclopedia
Trojan asteroid

5023 Agapenor
Discovery[1]
Discovered byC. Shoemaker
E. Shoemaker
Discovery sitePalomar Obs.
Discovery date11 October 1985
Designations
(5023) Agapenor
Pronunciation/æɡəˈpnɔːr/[2]
Named after
Agapenor
(Greek mythology)[3]
1985 TG3
Jupiter trojan[4][5]
(Greek camp)[6]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc31.72 yr (11,585 days)
Aphelion5.4430AU
Perihelion4.9085 AU
5.1758 AU
Eccentricity0.0516
11.78yr (4,301 days)
227.44°
0° 5m 1.32s / day
Inclination11.777°
308.36°
84.242°
Jupiter MOID0.0440 AU
TJupiter2.9550
Physical characteristics
Dimensions27.850±3.511 km[7][8]
46.30 km(calculated)[5]
5.4020±0.0017h[9]
0.057(assumed)[5]
0.173±0.093[7][8]
X[10] · C[5]
10.3[7] · 10.4[1][5] · 10.88±0.13[10]

5023 Agapenor/æɡəˈpnɔːr/ is aJupiter trojan from theGreek camp, approximately 30 kilometers in diameter. It was discovered on 11 October 1985, by American astronomer coupleCarolyn andEugene Shoemaker at thePalomar Observatory in California, United States.[4] The Jovianasteroid was named forAgapenor from Greek mythology.

Orbit and classification

[edit]

Agapenor orbits in the leading Greek camp at Jupiter'sL4Lagrangian point, 60° ahead of its orbit(seeTrojans in astronomy). It orbits the Sun in theouter main-belt at a distance of 4.9–5.4 AU once every 11 years and 9 months (4,301 days). Its orbit has aneccentricity of 0.05 and aninclination of 12° with respect to theecliptic.[1]

Aprecovery was taken at the discovering observatory in September 1985, extending the body'sobservation arc by 25 days prior to its official discovery observation.[4]

Physical characteristics

[edit]

Agapenor has been characterized as anX-type asteroid byPanSTARRS photometric survey.[10]

Rotation period

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In September 2009,Agapenor was observed by Italian astronomerStefano Mottola in a photometric survey of 80 Jupiter trojans, using the 1.2-meter reflector atCalar Alto Observatory in southeastern Spain. The obtainedlightcurve gave arotation period of5.4020 hours with a brightness variation of0.12 inmagnitude (U=2+).[9]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Agapenor measures 27.9 kilometers in diameter and its surface has analbedo of 0.17.[7][8]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous of 0.057 and calculates a significantly larger diameter of 46.3 kilometers.[5]

Naming

[edit]

Thisminor planet was named from Greek mythology afterAgapenor. He was the leader of the Greek contingent of Arcadians in theTrojan War. The minor planet1020 Arcadia is named after this able group of warriors. Agapenor was the commander of 60 ships lend to him byAgamemnon, the king of Mycenae and leader of the Greeks in the Trojan War.911 Agamemnon, one of the largest Jupiter trojans known to exist, is named after the commander of the Greek forces.[3] The official naming citation was published by theMinor Planet Center on 12 July 1995 (M.P.C. 25443).[11]

References

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  1. ^abcd"JPL Small-Body Database Browser: 5023 Agapenor (1985 TG3)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 17 September 2020. Retrieved20 June 2017.
  2. ^Noah Webster (1884)A Practical Dictionary of the English Language
  3. ^abSchmadel, Lutz D. (2007). "(5023) Agapenor".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 432.doi:10.1007/978-3-540-29925-7_4891.ISBN 978-3-540-00238-3.
  4. ^abc"5023 Agapenor (1985 TG3)".Minor Planet Center. Retrieved16 April 2016.
  5. ^abcdef"LCDB Data for (5023) Agapenor". Asteroid Lightcurve Database (LCDB). Retrieved16 April 2016.
  6. ^"List of Jupiter Trojans".Minor Planet Center. 20 June 2016. Retrieved4 December 2016.
  7. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011)."NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 118700974. Retrieved18 May 2016.
  8. ^abcGrav, T.; Mainzer, A. K.; Bauer, J. M.; Masiero, J. R.; Nugent, C. R. (November 2012)."WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy".The Astrophysical Journal.759 (1): 10.arXiv:1209.1549.Bibcode:2012ApJ...759...49G.doi:10.1088/0004-637X/759/1/49.S2CID 119101711. Retrieved5 December 2016.
  9. ^abMottola, Stefano; Di Martino, Mario; Erikson, Anders; Gonano-Beurer, Maria; Carbognani, Albino; Carsenty, Uri; et al. (May 2011)."Rotational Properties of Jupiter Trojans. I. Light Curves of 80 Objects".The Astronomical Journal.141 (5): 32.Bibcode:2011AJ....141..170M.doi:10.1088/0004-6256/141/5/170.
  10. ^abcVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved18 May 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 May 2016.

External links

[edit]
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