Open Access

Table 6

Percentage of systems/stars with specific planetary types (fs) and their mean multiplicity (μp) for the different populations.

Initial number of embryos
1 10 20 50 100
Type fs fs μp fs μp fs μp fs μp
Mass >1 M 49.3% 91.8% 3.3 93.2% 4.3 94.6% 7.0 96.0% 8.4

Earth-like 15.5% 63.7% 2.1 69.0% 3.3 83.7% 4.9 90.1% 5.2
Super Earth 19.1% 73.6% 2.1 75.5% 2.8 79.3% 4.8 82.1% 5.6
Neptunian 13.3% 34.4% 1.2 33.0% 1.3 27.2% 1.3 30.3% 1.4
Sub-giant 5.4% 10.0% 1.1 10.1% 1.2 8.9% 1.2 8.5% 1.2
Giant 3.6% 19.8% 1.5 19.1% 1.5 17.4% 1.5 18.1% 1.6
D-burning 0.1% 3.0% 1.0 3.5% 1.0 4.5% 1.0 4.5% 1.0

Earth-like < 1 au 12.9% 52.8% 1.8 53.3% 2.9 58.7% 3.7 57.2% 2.8
Super Earth < 1 au 17.8% 66.9% 1.9 63.1% 2.5 62.0% 3.7 66.1% 3.7
Neptunian < 1 au 13.1% 32.8% 1.2 30.9% 1.2 24.8% 1.2 26.2% 1.4
Sub-giant < 1 au 5.1% 7.7% 1.0 6.9% 1.1 6.7% 1.1 6.5% 1.1
Giant < 1 au 2.8% 14.0% 1.2 12.6% 1.2 9.3% 1.1 9.2% 1.1

Habitable zone 1.0% 14.4% 1.2 29.9% 1.3 49.4% 1.5 43.7% 1.3
Kepler (Petigura et al. 2018) 40.8% 78.2% 3.0 76.8% 3.5 72.2% 4.6 76.7% 4.4
Kepler (Zhu et al. 2018) 37.2% 78.1% 2.8 77.1% 3.3 71.6% 4.3 65.7% 4.5

Hot Jupiter 0.8% 2.8% 1.0 2.2% 1.1 0.9% 1.1 0.3% 1.0
Jupiter analogue 0.0% 0.5% 1.0 0.4% 1.0 0.2% 1.0 0.8% 1.0
Giant > 5 au 0.0% 0.7% 1.0 1.2% 1.0 2.6% 1.0 3.5% 1.0
Giant > 10 au 0.0% 0.3% 1.0 0.3% 1.0 1.4% 1.0 1.6% 1.0
Giant > 20 au 0.0% 0.1% 1.0 0.1% 1.0 0.9% 1.0 0.8% 1.0

Notes. The multiplicity is the mean number of planets of a given type per star for those stars which have at least one planet of this type. The multiplicity of the single-embryo population is not given because it is 1 per definition.

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