The Dawn spacecraft, which orbited Ceres from 2015 to 2018, captured images of several bright craters on the dwarf planet's surface. These craters are thought to be relatively young, and the impact events that created them may have exposed fresh material from Ceres' interior. Some of the bright craters observed by Dawn include:

1. Occator Crater: Occator, located near Ceres' north pole, was one of the first bright spots identified on the dwarf planet. The bright material in Occator is highly reflective and has been linked to salts or icy material.

2. Yarrunabie Crater: Another prominent bright crater on Ceres is Yarrunabie, which measures approximately 84 kilometers in diameter. Yarrunabie exhibits bright deposits that extend beyond the crater rim, resembling rays.

3. Oxox Crater: Oxox Crater, measuring approximately 44 kilometers in diameter, also displays bright ejecta that spread across a large area of the surface.

4. Ahuna Mons: Ahuna Mons, although not a crater, appears as a bright feature due to highly reflective salts on its slopes. Similar to Occator, Ahuna Mons has been a focus of attention in understanding the geology and composition of Ceres.

These bright craters and areas on Ceres provide clues about the composition and evolution of the dwarf planet's surface and may represent important sites for future study and exploration.