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)本文收录了用于生成手稿中所有图表的两份数据文件。 "input.csv"：包含模型每一次迭代中用于构建模型原行星的随机生成参数（set、phi、radius、t_accr、d_He、热梯度（thermal gradient）、平衡半径占比（radius fraction of equilibration）、kappa） "results.csv"：包含模型每一次迭代中计算得到的模型参数（表面温度、M.O.反应温度、表面压强、M.O.反应压强、dIW、金属相中氧的摩尔分数、d_U+Th、³He/⁴He比值、45亿年后的³He/⁴He比值）