Modeling the Early Earth: Core Formation in the Nebular Era Does Not Guarantee a High 3He/4He Ratio

We include the two files used to generate all figures in the manuscript.

"input.csv" - includes the randomly generated parameters used to build the model protoplanet for each iteration of the model (set, phi, radius, t_accr, d_He, thermal gradient, radius fraction of equilibration, kappa)

"results.csv" - includes the parameters calculated within the model for each iteration (surface temperature, M.O. reaction temperature, surface pressure, M.O. reaction pressure, dIW, mole fraction of O in metal, d_U+Th, 3He/4He ratio, 3He/4He ratio after 4.5 Gyrs)