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astro-ph2005
High-resolution simulations of the final assembly of Earth-like planets 2: water delivery and planetary habitability
Sean N. Raymond, Thomas Quinn, Jonathan I. Lunine
The water content and habitability of terrestrial planets are determined during their final assembly, from perhaps a hundred 1000-km "planetary embryos" and a swarm of billions of…
astro-ph2005
Terrestrial Planet Formation in Disks with Varying Surface Density Profiles
Sean N. Raymond, Thomas Quinn, Jonathan I. Lunine
The ``minimum-mass solar nebula'' (MMSN) model estimates the surface density distribution of the protoplanetary disk by assuming the planets to have formed in situ. However, signif…