From Surf Wiki (app.surf) — the open knowledge base
167P/CINEOS
Chiron-type comet
Chiron-type comet
| Field | Value | |
|---|---|---|
| name | 167P/CINEOS | |
| discoverer | CINEOS | |
| discovery_date | August 10, 2004 | |
| designations | ||
| orbit_ref | ||
| epoch | 2066-03-11 | |
| observation_arc | 9.35 years | |
| semimajor | 16.28 AU | |
| perihelion | 11.77 AU | |
| (outside Saturn's orbit) | ||
| aphelion | 20.8 AU | |
| eccentricity | 0.27705 | |
| inclination | 19.0529° | |
| max_speed | 9.8 km/s | |
| min_speed | 5.6 km/s (2033-Nov-30) | |
| period | 65.67 yr | |
| tjup | 3.527 | |
| physical_ref | ||
| dimensions | ||
| albedo | ||
| spectral_type | {{unbulleted | |
| (B–V) {{ | }} | |
| (V–R) {{ | }} | |
| (R–I) {{ | }} | |
| (B–R) {{ | }} }} | |
| M2 | 9.7 | |
| last_p | April 24, 2001 | |
| next_p | March 22, 2066 |
(outside Saturn's orbit) (B–V) | (V–R) | (R–I) | (B–R) }}
167P/CINEOS, also known as ****, is a large periodic comet and active, grey centaur, approximately 66 km in diameter, orbiting the Sun outside the orbit of Saturn. It was discovered on August 10, 2004, by astronomers with the CINEOS survey at Gran Sasso in Italy. It is one of only a handful known Chiron-type comets.
The comet nucleus (~66 km) is roughly half the size of (Bernardinelli–Bernstein) and it has a similar perihelion point just outside the orbit of Saturn.
| Comet | Nucleus | ||
|---|---|---|---|
| diameter | Perihelion | ||
| (Sun approach) | Perihelion | ||
| velocity | |||
| [95P/Chiron](95p-chiron) | 215 km | 8.5 AU | 12.0 km/s |
| C/2014 UN271 (Bernardinelli–Bernstein) | 120 km | 10.95 AU | 12.7 km/s |
| **167P/CINEOS** | 66 km | 11.77 AU | 9.8 km/s |
Description
Due to its high Jupiter tisserand of 3.5, and a semi-major axis larger than that of Jupiter, 167P/CINEOS is classified as a Chiron-type comet, named after the groups namesake, 2060 Chiron or 95P/Chiron, designated as both minor planet and comet.
167P/CINEOS was first reported as a minor planet, designated , but was found to have a very faint asymmetric cometary coma. Contrary to Chiron, which is the prototype object for the dynamical group of centaurs, 167P/CINEOS has no "dual status" as comet and minor planet, and demonstrates the inconsistencies in applying the current rules for designating small Solar System bodies. 167P/CINEOS not only has orbital parameters similar to those of Chiron, but also a low B–R magnitude of , which places it into the group grey centaurs.
In June 2039, 167P/CINEOS will pass 1.64 AU from Uranus.
References
| display-authors= etal | doi-access= free }}
| doi-access= free }}
| access-date= 2012-07-12 }}
| access-date= 2014-06-18 }}
| doi-access= free }}
|archive-url=https://web.archive.org/web/20220624114237/https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27167P%27&START_TIME=%272066-Mar-17%27&STOP_TIME=%272066-Mar-21%27&STEP_SIZE=%271%20hours%27&QUANTITIES=%2719%27 |archive-date=2022-06-24 |url-status=live
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about 167P/CINEOS — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report