The mass estimate is based on the assumed density of 1.2 g/cm³, and a volume of 3.5 ·106 km³ obtained from a detailed shape model in P.J. Stooke. 1994. The surfaces of Larissa and Proteus. Earth, Moon ad Planets. 65: 31. doi:10.1007/BF00572198
The mass estimate is based on the assumed density of 1.2 g/cm³, and a volume of 3.5 ·106 km³ obtained from a detailed shape model in P.J. Stooke. 1994. The surfaces of Larissa and Proteus. Earth, Moon ad Planets. 65: 31. doi:10.1007/BF00572198