Fig. 4From: Terrestrial planet compositions controlled by accretion disk magnetic fieldDensity of the rocky solar system bodies. Uncompressed and solid densities are shown for terrestrial planets and chondrites (gray), respectively. Bulk planetary densities are shown for asteroids (blue). For 1 Ceres, its bulk density is a lower limit of its solid density, given its high ice abundance and porosity. The red line shows a fit curve for the planets (ρ=4100r−0.21). Data sources: density of planetary bodies are from Russell et al. (2012); Park et al. (2019); Sierks et al. (2011); Consolmagno et al. (2006); Macke et al. (2010); Macke et al. (2011); Britt and Consolmagno (2003); Lewis (1972); Stacey (2005); heliocentric distances of chondrite parent bodies are from Desch et al. (2018)Back to article page