Rocks in SpaceFamilies › Centaurs
CEN · 5.5–30 AU

Centaurs

Objects on unstable orbits among the giant planets: too far out to be asteroids, too close in to be Kuiper Belt objects, and not gravitationally safe anywhere. They are comets in transit — caught in the act of becoming something else.

1,038
known Centaurs
5.5–30 AU
between Jupiter and Neptune
a few Myr
typical orbital lifetime
2060 Chiron
the first one found, in 1977
Every Centaur's closest and furthest distance from the Sun, with the four giant planets marked on both axes. A point that sits left of a gold vertical and above the matching horizontal is an orbit that crosses that planet's: 94.4% of Centaurs cross at least one giant planet's orbit and 51.3% cross two or more. That is the reason none of these orbits lasts — each object repeatedly meets a planet massive enough to throw it somewhere else.

A population defined by impermanence

A Centaur's orbit crosses those of one or more giant planets, so close encounters are inevitable. Typical dynamical lifetimes are a few million years, ending in ejection from the solar system, a collision, or capture into the inner system as a Jupiter-family comet.

Like the near-Earth asteroids, then, this is a transient population that must be resupplied — in this case from the Kuiper Belt. Centaurs are the middle of a conveyor belt running from beyond Neptune to the inner solar system.

Asteroid or comet?

The category dissolves on inspection. 2060 Chiron was discovered in 1977 and catalogued as an asteroid; years later it developed a coma and received a cometary designation as well. It now holds both. Several Centaurs show intermittent activity far from the Sun, where water ice is too cold to sublimate — more volatile ices, or crystallising amorphous ice, are the likely drivers.

Our schema inherits this ambiguity honestly rather than resolving it: an object's dynamical class and its activity are separate facts, and the schema records the classification the source asserts rather than forcing a choice.

Rings where nobody expected them

In 2013, occultation observations of the Centaur 10199 Chariklo revealed two narrow rings — the first found around anything other than a giant planet. Ring systems around small bodies now appear to be a real phenomenon rather than a curiosity.

That result came from stellar occultations: watching a star blink out as the object passes in front. It needs precise timing rather than a large aperture, which makes it one of the genuinely open frontiers for coordinated small-telescope work.

What is still unmeasured

With only about a thousand known and lifetimes of a few million years, the Centaur population's size and resupply rate are still poorly constrained.

Best-known members

Brightest by absolute magnitude, named objects first. Queried live from the catalog.

ObjectHDiameteraeiPeriod
2060 Chiron (1977 UB)5.54166 km13.68 AU0.3806.9°50.6 yr
10199 Chariklo (1997 CU26)6.55302 km15.73 AU0.17123.4°62.4 yr
5145 Pholus (1992 AD)7.07190 km20.29 AU0.57524.8°91.4 yr
463368 Eurytus (2012 VU85)7.3229.47 AU0.31515.1°160.0 yr
54598 Bienor (2000 QC243)7.49188 km16.60 AU0.20620.7°67.7 yr
55576 Amycus (2002 GB10)7.56101 km24.94 AU0.39313.4°125.0 yr
10370 Hylonome (1995 DW2)8.2024.95 AU0.2474.1°125.0 yr
121725 Aphidas (1999 XX143)8.8817.96 AU0.4616.8°76.1 yr
See it in three dimensions

The 3-D viewer plots all 1,557,369 catalogued objects at a fixed instant. Each population can be isolated, so this family can be viewed on its own against the planets.

Research & development — not peer-reviewed. The catalog, analysis, and software behind this site were developed in collaboration with AI and have not been validated by the scientific community. No claims are made as to scientific validity. Source measurements are credited to NASA/JPL and the Minor Planet Center; the interpretation is ours.