Evolution of the density (panel a), temperature (panel b), radiative energy (panel c), radial velocity (panel d), specific entropy (panel e), and Rosseland mean opacity (panel f) profiles, averaged in radial bins and displayed as a function of radius for different times, where t = 0 marks the birth of the protostar. The last curves (dark red) on each panel correspond to t ≈ 241 days. The dashed and dotted gray lines in panels a–c are power law curves representing the expected density, temperature, and radiative energy profiles both prior to and after the accretion of the first Larson core.