(6545)_1986_TR6

6545 Leitus

6545 Leitus, provisional designation: 1986 TR6, is a Jupiter trojan from the Greek camp, approximately 53 kilometers (33 miles) in diameter. It was discovered on 5 October 1986, by Slovak astronomer Milan Antal at the Piwnice Astronomical Observatory in Poland.[1] The dark D-type asteroid has a rotation period of 16.3 hours and belongs to the 90 largest Jupiter trojans.[9] Numbered in 1995, it was named in 2021, after the Argonaut Leitus from Greek mythology, who fought in the Trojan War.[13]

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Orbit and classification

Leitus is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's L4 Lagrangian point, 60° ahead of the Gas Giant's orbit in a 1:1 resonance (see Trojans in astronomy).[4] It is also a non-family asteroid in the Jovian background population.[5] It orbits the Sun at a distance of 4.9–5.4 AU once every 11 years and 8 months (4,265 days; semi-major axis of 5.15 AU). Its orbit has an eccentricity of 0.05 and an inclination of 12° with respect to the ecliptic.[3] The body's observation arc begins with its official discovery observation at Piwnice in October 1986.[1]

Numbering and naming

This minor planet was numbered on 9 September 1995 (M.P.C. 25628).[13] On 29 November 2021, IAU's Working Group for Small Bodies Nomenclature named it after the Argonaut Leitus from Greek mythology. He was one of the seven Achaean Leaders in front of whom Poseidon appeared during the Trojans' attack on the Achaean ships, urging them to fight back instead of acting like cowards. Wounded by Hector, Leitus was one of the few to safely return home after the Trojan War.[1][2]

Physical characteristics

In the SDSS-based taxonomy, Leitus is dark D-type asteroid,[7][11] which agrees with the determined spectral type by Pan-STARRS.[9][10] Its V–I color index of 0.91 is typical for most larger Jupiter trojans (also see table below).[9]

Rotation period

In March 2013, a rotational lightcurve of Leitus was obtained from photometric observations by Robert Stephens at the Center for Solar System Studies in Landers, California. Lightcurve analysis gave a rotation period of 16.26±0.01 hours with a brightness amplitude of 0.31 magnitude (U=2+).[8][9][lower-alpha 1]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Infrared Astronomical Satellite IRAS, Leitus measures 50.95 and 56.96 kilometers in diameter and its surface has an albedo of 0.068 and 0.0545, respectively.[6][7] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 53.16 kilometers based on an absolute magnitude of 10.1.[9]

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Notes

  1. Lightcurve plot of (6545) 1986 TR6 from Mar 2013 by Robert Stephens at the Center for Solar System Studies (U81). Quality code is not available (lightcurve rating at CS3). Summary figures at the LCDB and CS3.

References

  1. "6545 (1986 TR6)". Minor Planet Center. Retrieved 20 June 2018.
  2. "WGSBN Bulletin Archive". Working Group for Small Bodies Nomenclature. 29 November 2021. Retrieved 29 November 2021. (Bulletin #12)
  3. "List of Jupiter Trojans". Minor Planet Center. 1 June 2018. Retrieved 20 June 2018.
  4. "Asteroid (6545) 1986 TR6 – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 20 June 2018.
  5. Grav, 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. (online catalog)
  6. "Asteroid (6545) 1986 TR6". Small Bodies Data Ferret. Retrieved 20 June 2018.
  7. French, Linda M.; Stephens, Robert, D.; Coley, Daniel R.; Wasserman, Lawrence H.; Vilas, Faith; La Rocca, Daniel (October 2013). "A Troop of Trojans: Photometry of 24 Jovian Trojan Asteroids". The Minor Planet Bulletin. 40 (4): 198–203. Bibcode:2013MPBu...40..198F. ISSN 1052-8091.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  8. "LCDB Data for (6545)". Asteroid Lightcurve Database (LCDB). Retrieved 20 June 2018.
  9. Veres, 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.
  10. Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010). "SDSS-based taxonomic classification and orbital distribution of main belt asteroids". Astronomy and Astrophysics. 510: 12. Bibcode:2010A&A...510A..43C. doi:10.1051/0004-6361/200913322. Retrieved 30 October 2019. (PDS data set)
  11. Hainaut, O. R.; Boehnhardt, H.; Protopapa, S. (October 2012). "Colours of minor bodies in the outer solar system. II. A statistical analysis revisited". Astronomy and Astrophysics. 546: 20. arXiv:1209.1896. Bibcode:2012A&A...546A.115H. doi:10.1051/0004-6361/201219566. S2CID 54776793.
  12. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 20 June 2018.

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