266P/Christensen

266P/Christensen
Discovery[1]
Discovered byEric J. Christensen
Discovery siteCatalina Sky Survey
Discovery date27 October 2006
Designations
P/2006 U5, P/2012 P1
Orbital characteristics[2][3]
Epoch26 December 2026 (JD 2461400.5)
Observation arc18.93 years
Number of
observations
908
Aphelion4.733 AU
Perihelion2.324 AU
Semi-major axis3.529 AU
Eccentricity0.34133
Orbital period6.628 years
Inclination3.429°
4.941°
Argument of
periapsis
97.951°
Mean anomaly2.763°
Last perihelion19 April 2020
Next perihelion7 December 2026
TJupiter3.020
Earth MOID1.351 AU
Jupiter MOID0.526 AU
Physical characteristics[2]
Mean radius
1.66 km (1.03 mi)[4]
Comet total
magnitude
(M1)
11.0
Comet nuclear
magnitude (M2)
15.9

266P/Christensen is a Encke-type comet with a 6.63-year orbit around the Sun. It will next come to perihelion in December 2026. It has been suggested as the source of the 1977 "Wow! Signal".[5]

Physical characteristics

Observations conducted by the Sloan Digital Sky Survey (SDSS) in 2012 revealed that the nucleus of 266P has an upper limit no greater than 1.66 km (1.03 mi) in radius.[4]

References

  1. ^ E. J. Christensen; G. Hug; G. Sostero; et al. (29 October 2006). D. W. Green (ed.). "Comet C/2006 U5 (Christensen)". IAU Circular (8768). Bibcode:2006IAUC.8768....1C.
  2. ^ a b "266P/Christensen – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 10 November 2025.
  3. ^ "266P/Christensen Orbit". Minor Planet Center. Retrieved 8 June 2017.
  4. ^ a b M. Solontoi; Ž. Ivezíc; M. Juríc (2012). "Ensemble properties of comets in the Sloan Digital Sky Survey". Icarus. 218 (1): 571–584. arXiv:1202.3999. Bibcode:2012Icar..218..571S. doi:10.1016/j.icarus.2011.10.008.
  5. ^ A. Paris; E. Davies (2015). "Hydrogen Clouds from Comets 266/P Christensen and P/2008 Y2 (Gibbs) are Candidates for the Source of the 1977 "WOW" Signal" (PDF). Washington Academy of Sciences. 101 (4): 25–32. arXiv:1706.04642. Bibcode:2017arXiv170604642P. JSTOR jwashacadscie.101.4.25.