
Dwarf Planets
Ceres’ Bright Cerealia Facula May Be Geologically Young
A new EGU General Assembly 2026 study revisits the crater-based age of Cerealia Facula, the bright deposit inside Occator Crater on dwarf planet Ceres. Using high-resolution Dawn XMO7 imagery and improved crater counts, researchers estimate that the deposit is younger than the Occator impact and most likely formed within the single-digit million-year range, though model ages vary widely depending on chronology assumptions.















