166P/NEAT

166P/NEAT
Simulation of the orbit of 166P/NEAT between Saturn and Uranus
Discovery
Discovery siteNear Earth Asteroid Tracking (NEAT)
Discovery date15 October 2001
Designations
P/2001 T4
Orbital characteristics[1][2]
Epoch21 November 2025 (JD 2461000.5)
Observation arc7.51 years
Earliest precovery date27 August 2001
Number of
observations
177
Aphelion19.142 AU
Perihelion8.555 AU
Semi-major axis13.849 AU
Eccentricity0.38222
Orbital period51.537 years
Inclination15.386°
64.335°
Argument of
periapsis
321.99°
Mean anomaly163.94°
Last perihelion20 May 2002
Next perihelion26 November 2053[3][4]
TJupiter3.284
Earth MOID7.582 AU
Jupiter MOID3.693 AU
Physical characteristics
Mean radius
14.32 km (8.90 mi)[5]
  • (B–V) = 0.89±0.11[6]
  • (V–R) = 0.56±0.03[6]
  • (B–R) = 1.59±0.05[5]
Comet total
magnitude
(M1)
7.0
Comet nuclear
magnitude (M2)
10.6

166P/NEAT is a Chiron-type comet and centaur in the outer Solar System. It was discovered by the Near Earth Asteroid Tracking (NEAT) project in 2001 and initially classified a comet with provisional designation P/2001 T4 (NEAT), as it was apparent from the discovery observations that the body exhibited a cometary coma. It is one of few known bodies with centaur-like orbits that display a coma, along with 60558 Echeclus, 2060 Chiron, 165P/LINEAR and 167P/CINEOS. It is also one of the reddest centaurs ever known.[7]

166P/NEAT has a perihelion distance of 8.56 AU (1.281 billion km).[1]

References

  1. 1 2 "166P/NEAT – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 14 September 2008.
  2. ↑ "166P/NEAT Orbit". Minor Planet Center. Retrieved 18 June 2014.
  3. ↑ Syuichi Nakano (30 June 2005). "166P/NEAT (2001 T4) (NK 1187)". OAA Computing and Minor Planet Sections. Retrieved 20 February 2012.
  4. ↑ "Horizons Batch for 166P/NEAT on 2053-Nov-26" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 6 July 2023. (JPL#51 Soln.date: 2021-Apr-15)
  5. 1 2 J. C. Shi; Y. H. Ma (2015). "CCD photometry of active Centaur 166P/2001 T4 (NEAT)" (PDF). Monthly Notices of the Royal Astronomical Society. 454 (4): 3635–3640. Bibcode:2015MNRAS.454.3635S. doi:10.1093/mnras/stv2274.
  6. 1 2 D. C. Jewitt (2015). "Color Systematics of Comets and Related Bodies". The Astronomical Journal. 150 (6): 201–219. arXiv:1510.07069. Bibcode:2015AJ....150..201J. doi:10.1088/0004-6256/150/6/201.
  7. ↑ J. M. Bauer; Y. R. Fernández; K. J. Meech (2003). "An Optical Survey of the Active Centaur C/NEAT (2001 T4)". Publications of the Astronomical Society of the Pacific. 115 (81): 981–989. Bibcode:2003PASP..115..981B. doi:10.1086/377012.