We use the C/N ratio as a monitor of the delivery of key ingredients of life
to nascent terrestrial worlds. Total elemental C and N contents, and their
ratio, are examined for the interstellar medium, comets, chondritic meteorites
and terrestrial planets; we include an updated estimate for the Bulk Silicate
Earth (C/N = 49.0 +/- 9.3). Using a kinetic model of disk chemistry, and the
sublimation/condensation temperatures of primitive molecules, we suggest that
organic ices and macro-molecular (refractory or carbonaceous dust) organic
material are the likely initial C and N carriers. Chemical reactions in the
disk can produce nebular C/N ratios of ~1-12, comparable to those of comets and
the low end estimated for planetesimals. An increase of the C/N ratio is traced
between volatile-rich pristine bodies and larger volatile-depleted objects
subjected to thermal/accretional metamorphism. The C/N ratios of the dominant
materials accreted to terrestrial planets should therefore be higher than those
seen in carbonaceous chondrites or comets. During planetary formation, we
explore scenarios leading to further volatile loss and associated C/N
variations owing to core formation and atmospheric escape. Key processes
include relative enrichment of nitrogen in the atmosphere and preferential
sequestration of carbon by the core. The high C/N BSE ratio therefore is best
satisfied by accretion of thermally processed objects followed by large-scale
atmospheric loss. These two effects must be more profound if volatile
sequestration in the core is effective. The stochastic nature of these
processes hints that the surface/atmospheric abundances of biosphere-essential
materials will likely be variable.Comment: Accepted by PNAS per
http://www.pnas.org/content/early/2015/07/01/1500954112.abstract?sid=9fd8abea-9d33-46d8-b755-217d10b1c24