Table 1
Mean values of planet samples divided by stellar type.
| Stellar type | Stellar T (K) | No. | μ(R) | σ(R) | μ(M) | σ(M) | μ (Teq) | σ(Teq) |
|---|---|---|---|---|---|---|---|---|
| F | 5200–6000 | 8 | 3.32 | 1.84 | 8.03 | 4.17 | 1085.80 | 489.67 |
| G | 5200–6000 | 51 | 2.84 | 1.19 | 9.41 | 4.42 | 943.09 | 339.35 |
| K | 3700–5200 | 32 | 2.09 | 0.61 | 7.33 | 4.10 | 822.02 | 315.55 |
| M | 2400–3700 | 16 | 1.72 | 0.92 | 4.13 | 3.17 | 529.49 | 241.09 |
Notes. Mean values of planet samples (as described in Sect. 2.1) divided by stellar type. Teq is the equilibrium planet temperature that assumes zero albedo (see Sect. 2.1.1). No. stands for the number of planets in the sample, μ stands for the mean value, and σ is the standard deviation, assuming a normal distribution. Planetary mass, radius, and temperatures are given in M⊕, R⊕, and K, respectively.
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