An article published in the “Planetary Science Journal” reports the results of simulations that reproduce the possible history of the dwarf planet Haumea that led to its peculiar oval shape. A team of researchers used the geophysical and geochemical data available on Haumea and the asteroids that form a family with this dwarf planet to understand what processes led to their formation and evolution. The simulations lead to a reconstruction of the process that resulted in Haumea’s remarkable fast spin, which in turn led to its present shape.