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Fig. 12


Eccentricity vs. inclination of the terrestrial planets. White circles correspond to planets formed in coplanar giant planetsystems (2D-POP) and black circles to planets formed in 3D systems (3D-POP). The size of each circle is proportionalto the cubic root of their mass. We observe that all the bodies that form after 100 Myr evolve in orbits with e < 0.3 and i < 10°.

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