Table 1: Computed late time (A, B) and adopted (C) gas-phase abundances with respect to H₂ for the main S-bearing molecules prior to mantle evaporation.
Species A B C

SO $9\times 10^{-9}$ $3\times 10^{-9}$ $3.1\times 10^{-9}$

SO₂ $4\times 10^{-10}$ $1.5\times 10^{-10}$ $1\times 10^{-9}$ ^a

H₂S $1\times 10^{-10}$ $1\times 10^{-11}$ $8\times 10^{-10}$

CS $4\times 10^{-10}$ $2\times 10^{-8}$ $1.7\times 10^{-9}$

**Table 1:** Computed late time (A, B) and adopted (C) gas-phase abundances with respect to H₂ for the main S-bearing molecules prior to mantle evaporation.
Species	A	B	C
SO	$9\times 10^{-9}$	$3\times 10^{-9}$	$3.1\times 10^{-9}$
SO₂	$4\times 10^{-10}$	$1.5\times 10^{-10}$	$1\times 10^{-9}$ ^a
H₂S	$1\times 10^{-10}$	$1\times 10^{-11}$	$8\times 10^{-10}$
CS	$4\times 10^{-10}$	$2\times 10^{-8}$	$1.7\times 10^{-9}$

^a Here we took the value of the upper limit.

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