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Raw images from Angle 5.  CTH simulation of a M_t=6.38M_E planet colliding with a M_i=0.82M_E impactor at v_{imp}/v_{esc}= 0.7, at 70 degrees.  Both objects are composed of 70 % dunite and 30 % iron by mass.  The domain extends from -800 Mm to 800 Mm in the x, y, and z directions, 20 times wider than shown here.  Colors indicate densities on a logarithmic scale, with orange/red indicating $\rho > 1 $ g/cm$^3$ (solid material), blue/green indicating rho ~ 10^{-3} g/cm^3 (vapor), and dark blue indicating rho \sim 10^{-6} g/cm^3 (diffuse vapor).  The collision yields an orbiting disk of mass M_o ~ 0.15 M_E.  If all of the disk material accumulates into a single moon, and R_L ~ 3570 km (0.58 R_E).  The planet's final mass is 7 M_E. An animation of this figure may be viewed online: https://youtu.be/gKjtae_aECA

Author: amybarr