Evolution of the reservoirs of volatiles in the protosolar nebula

Open Access

Fig. 4

Time evolution of the mass abundance of water, defined as the radial profile of , for both scenarios at t = 10⁴, 10⁵, and 10⁶ yr. Solid lines represent H₂O in the gaseous phase (orange line), crystalline phase (blue line), and in amorphous phase (red line).

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