I am a student collaborator on the Dawn Mission, which is a spacecraft currently orbiting the dwarf planet Ceres. Ceres represents a transition between the rocky bodies of the inner solar system and icy bodies of the outer solar system. By understanding the processes that shape its surface and subsurface, we can better constrain its development and evolution. The surface of Ceres is dotted with hundreds of anomalously bright, carbonate-bearing areas that are usually associated with impact craters. I work with Bethany Ehlmann to study the formation of these bright spots. I recently published a paper cataloging the bright spots and discussing hypotheses for how they formed and are modified over time (see below). Now I am using data from Dawn's VIR instrument to model the composition of the bright spots to better constrain their formation.