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Table 1

Parameters for the simulations in the parameter study.

Solar System

Run Jupiter Saturn α 0
Mp Comp. Mp Comp. (M yr−1)
#1 Nominal 90 M H2O, CO2 30 M H2O, CO2 10−2 10−7
#2 Nominal (–CO2) 90 H2O 30 H2O 10−2 10−7
#3 Mp 30 H2O, CO2 10 H2O, CO2 10−2 10−7
#4 Mp 150 H2O, CO2 50 H2O, CO2 10−2 10−7
#5 α ↓ 90 H2O, CO2 30 H2O, CO2 10−3 10−7
#6 0 90 H2O 30 H2, CO2 10−2 10−8

HL Tau

Run Planet 1 Planet 2 Planet 3 α 0
Mp Comp. Mp Comp. Mp Comp. (M yr−1)

#7 Nominal 59.6 M H2O, CO2 141.2 M H2O, CO2 313.7 M H2O, CO2 10−2 10−7
#8 α ↓ -//- H2O, CO2 -//- H2O, CO2 -//- H2O, CO2, CO 10−3 10−7
#9 α ↓ (–CO) -//- H2O, CO2 -//- H2O, CO2 -//- H2O, CO2 10−3 10−7
#10 α ↓ (–CO, –CO2) -//- H2O -//- H2O -//- H2O 10−3 10−7
#11 0 -//- H2O, CO2 -//- H2O, CO2 -//- H2O, CO2 10−2 10−8

Notes. Here, Mp denotes planetary mass and “comp.” refers to the volatile composition of the planetesimals initiated at the gap edge of the specified planet.

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