Fig. 5

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C/O ratio and the log scale of metallicity of 100 thousand planets with one Jupiter mass at a distance of 0.02 AU with different compositions. The different compositions are caused by the different formation initial conditions (see Sect. 3). The four different colors show planets that initiated their formation in four different regions of the disk. Cyan indicates planets that initiated their migration within the water ice line, region A. Black indicates planets that initiated their migration farther than the water ice line and within the CO2 ice line, region B. Red indicates planets that initiated their migration beyond the CO2 ice line and within the CO ice line, region C. Blue indicates planets that initiated their migration farther than the CO ice line, region D.
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