Table 2
Parameters of the Earth around the Sun and Earth-like planets around M-dwarf host stars.
Host star | S∕S⊙ | a(AU) | P(d) | tD (h) | δ (ppm) | αp | Teq (K) |
---|---|---|---|---|---|---|---|
Sun | 1.000 | 1.000 | 365.3 | 13.10 | 84.1 | 0.201 | 263.4 |
GJ 832 | 0.886 | 0.205 | 50.4 | 4.28 | 364.8 | 0.117 | 262.0 |
GJ 176 | 0.915 | 0.192 | 45.9 | 3.92 | 409.6 | 0.095 | 265.8 |
GJ 581 | 0.920 | 0.114 | 25.8 | 2.47 | 940.1 | 0.086 | 266.8 |
GJ 436 | 0.918 | 0.166 | 34.8 | 3.45 | 406.0 | 0.086 | 266.6 |
GJ 644 | 0.888 | 0.242 | 67.6 | 6.81 | 182.8 | 0.096 | 263.7 |
AD Leo | 0.878 | 0.143 | 30.4 | 3.02 | 552.6 | 0.094 | 263.1 |
GJ 667C | 0.913 | 0.162 | 41.5 | 4.27 | 397.2 | 0.096 | 265.5 |
GJ 876 | 0.951 | 0.113 | 22.9 | 2.77 | 594.5 | 0.071 | 270.1 |
GJ 1214 | 0.958 | 0.068 | 15.6 | 1.78 | 1887.9 | 0.068 | 270.8 |
Proxima Cen. | 0.986 | 0.040 | 8.4 | 1.13 | 4227.7 | 0.059 | 273.4 |
TRAPPIST-1 | 1.045 | 0.022 | 4.4 | 0.87 | 6036.4 | 0.053 | 277.9 |
Notes. The value S∕S⊙
is the ratio of the total stellar irradiance to the TSI to reach a surface temperature of 288.15 K. The transit duration was calculated via Eq. (7). We assume circular orbits for all planets. The transit depth,
, is calculated using the stellar radii from Table 1 and the radius of the Earth. The equilibrium temperature (Teq) was calculated using the corresponding planetary albedo (αp).
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