| Discovery [1] | |
|---|---|
| Discovered by | Eric J. Christensen |
| Discovery site | Catalina Sky Survey |
| Discovery date | 27 October 2006 |
| Designations | |
| P/2006 U5, P/2012 P1 | |
| Orbital characteristics [2] [3] | |
| Epoch | 26 December 2026 (JD 2461400.5) |
| Observation arc | 18.93 years |
| Number of observations | 908 |
| Aphelion | 4.733 AU |
| Perihelion | 2.324 AU |
| Semi-major axis | 3.529 AU |
| Eccentricity | 0.34133 |
| Orbital period | 6.628 years |
| Inclination | 3.429° |
| 4.941° | |
| Argument of periapsis | 97.951° |
| Mean anomaly | 2.763° |
| Last perihelion | 19 April 2020 |
| Next perihelion | 7 December 2026 |
| TJupiter | 3.020 |
| Earth MOID | 1.351 AU |
| Jupiter MOID | 0.526 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]
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]