  Low-albedo asteroids preserve a record of the primordial solar system
planetesimals and the conditions in which the solar nebula was active. However,
the origin and evolution of these asteroids are not well-constrained. Here we
measured visible and near-infrared (0.5 - 4.0 microns) spectra of low-albedo
asteroids in the mid-outer main belt. We show that numerous large (d > 100 km)
and dark (geometric albedo < 0.09) asteroids exterior to the dwarf planet
Ceres' orbit share the same spectral features, and presumably compositions, as
Ceres. We also developed a thermal evolution model that demonstrates that these
Ceres-like asteroids have highly-porous interiors, accreted relatively late at
1.5 - 3.5 Myr after the formation of calcium-aluminum-rich inclusions, and
experienced maximum interior temperatures of < 900 K. Ceres-like asteroids are
localized in a confined heliocentric region between 3.0 - 3.4 au but were
likely implanted from more distant regions of the solar system during the giant
planet's dynamical instability.
