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5025 Mecisteus

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(5025) 1986 TS6
Discovery [1]
Discovered byM. Antal
Discovery siteToruń–Piwnice
Discovery date5 October 1986
Designations
(5025) 1986 TS6
1986 TS6 · 1989 BX
Jupiter trojan[2][3]
(Greek camp)
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc29.65 yr (10,829 days)    
Aphelion5.5867 AU
Perihelion4.8144 AU
5.2005 AU
Eccentricity0.0743
11.86 yr (4,332 days)
171.34°
0° 4m 59.16s / day
Inclination11.021°
347.83°
73.365°
Jupiter MOID0.1061 AU
TJupiter2.9580
Physical characteristics
Dimensions39.84±3.64 km[4]
57.56 km (derived)[3]
57.83±4.9 km (IRAS:2)[1]
250±25 h[5]
0.0635±0.012 (IRAS:2)[1]
0.084±0.009[4]
0.0404 (derived)[3]
C[3]
10.3[1][3][4]
10.62±0.65[6]

(5025) 1986 TS6, is a carbonaceous Jupiter trojan from the Greek camp and potentially slow rotating asteroid, approximately 58 kilometers in diameter. It was discovered on 5 October 1986, by Slovak astronomer Milan Antal at the Toruń Centre for Astronomy in Piwnice, Poland.[2]

The dark Jovian asteroid is orbiting in the leading Greek camp at Jupiter's L4 Lagrangian point, 60° ahead of its orbit (see Trojans in astronomy). It orbits the Sun at a distance of 4.8–5.6 AU once every 11 years and 10 months (4,332 days). Its orbit has an eccentricity of 0.07 and an inclination of 11° with respect to the ecliptic.[1]

Based on a large-scale survey performed by Pan-STARRS, the C-type asteroid has also been rated as a transitional CX-type, an intermediate between the carbonaceous C-type and X-type asteroids.[6] In November 2009, the body was observed in a photometric light-curve survey of 80 Jupiter trojans, which rendered a very long rotation period of 250±25 hours with a brightness variation of 0.2 in magnitude (U=1).[5] However, the Collaborative Asteroid Lightcurve Link (CALL) considers the result as incorrect.[3]

According to the surveys carried out by the Infrared Astronomical Satellite (IRAS), and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 57.8 and 39.8 kilometers in diameter with an albedo of 0.064 and 0.084, respectively.[1][4] CALL agrees with the results obtained by IRAS, assumes an even lower albedo of 0.04, and calculates a similar diameter of 57.6 kilometers.[3]

References

  1. ^ a b c d e f g "JPL Small-Body Database Browser: 5025 (1986 TS6)" (2016-05-29 last obs.). Jet Propulsion Laboratory. Retrieved June 2016. {{cite web}}: Check date values in: |accessdate= (help)
  2. ^ a b "5025 (1986 TS6)". Minor Planet Center. Retrieved June 2016. {{cite web}}: Check date values in: |accessdate= (help)
  3. ^ a b c d e f g "LCDB Data for (5025)". Asteroid Lightcurve Database (LCDB). Retrieved June 2016. {{cite web}}: Check date values in: |accessdate= (help)
  4. ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results" (PDF). The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved June 2016. {{cite journal}}: Check date values in: |access-date= (help)
  5. ^ a b Mottola, 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. Retrieved June 2016. {{cite journal}}: Check date values in: |access-date= (help)
  6. ^ a b 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. Retrieved June 2016. {{cite journal}}: Check date values in: |access-date= (help)

External links