Kerberos (moon)

Physical characteristics

Kerberos is much smaller than Charon and is classed among Pluto's minor satellites. Its size is only loosely constrained: estimates place it on the order of a few to a few tens of kilometres across, depending on uncertain surface reflectivity (albedo). Imaging shows an irregular, non-spherical shape typical of small bodies, and its surface appears relatively dark compared with some of Pluto's other small moons. Kerberos orbits close to the plane of Pluto's satellite system and follows an approximately circular path.

Orbit and dynamical context

The moon occupies an orbit between those of two other small satellites, contributing to a compact family of co-orbital bodies around Pluto. The small moons of Pluto display near-coplanar, low-eccentricity orbits and show signs of dynamical interactions and near-resonant relationships with one another and with the barycentre dominated by Charon. These configurations are useful for tests of orbital stability in multi-body, tidally influenced systems.

Discovery and naming

Kerberos was discovered in images taken with the Hubble Space Telescope and announced in 2011. The provisional label reflected the year and the primary body (Pluto). In 2013 the International Astronomical Union approved the name Kerberos, drawn from Greek mythology, as part of a naming convention linking Pluto's satellites to underworld figures. The chosen spelling avoids duplication with existing asteroid names.

Origin and scientific importance

Most researchers consider Pluto's small moons, including Kerberos, to be remnants of a collisional event early in the system's history, in which material ejected from a giant impact coalesced into multiple satellites. Studying Kerberos helps constrain models for satellite formation around binary or near-binary primaries and provides insight into collisional processes in the outer Solar System.

Exploration, observations, and notable facts

Kerberos was observed at higher resolution during the New Horizons flyby of the Pluto system in 2015, though its small size limited the level of detail that could be obtained compared with Pluto and Charon. Ground- and space-based follow-up observations continue to refine its orbit, size estimates and surface properties. As a member of a compact and dynamically interesting satellite ensemble, Kerberos remains a subject for studies of formation, evolution and small-body properties in trans-Neptunian space.

• small moon of Pluto
• dwarf planet primary