The
meteoritic mineral schreibersite, e.g., Fe3P, is
a proposed abiotic source of phosphorus for phosphate ion (PO4
–) production, needed for nucleobases, phospholipids,
and other life building materials. Schreibersite could have acted
as both a source of elemental phosphorus and as a catalyst, and the
hostile conditions on early Earth could have accelerated its degradation
in different environments. Here, we present results from quantum calculations
of bulk schreibersite and of its low Miller index surfaces. We also
investigate water surface adsorption and identify possible dissociation
pathways on the most stable facet. Our calculations provide useful
chemical insights into schreibersite interactions in aqueous environments,
paving the way for further detailed investigation on more reactive
surfaces. Our results help provide a “bottom-up” understanding
for phosphorylated organic synthesis on the primitive planet and its
role in producing life building molecules.