Fig. 1
Time evolution of the core mass, envelope mass, and total mass of a planet located just beyond the snow line (~3 au). Chosen a disk ~1.35 times more massive than the MMSN, and a characteristic timescale of τ = 2.5 Myr for the dissipation of the gas disk, a Jupiter-like planet is formed by the accretion of planetesimals with 100 m radius in 2.35 Myr.
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