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The equilibrium temperature of lhs 1140 b is rather low, at 230 k (−43 °c Within the commit message, you will find a link to the scientific publication where the data is taken from. −46 °f), as cold as the polar regions on earth

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However, this is the calculated temperature excluding the impact of a thick atmosphere. It also lists the date of the last commit and the person making the changes While this is quite close, the star lhs 1140 is so dim that the planet only gets 0.43 times the incident flux of earth at this distance

2] assuming an albedo of 0, lhs 1140 b has an equilibrium temperature of 230k (−43°c

−46°f), compared to earth's at 255k (−18°c Lhs 1140 b has an equilibrium temperature of 230 k (−43 °c −46 °f), which is as cold as the earth’s polar regions However, this is the calculated temperature, which takes into account the impact of a thick atmosphere.

We analyzed the wfc3/hst observations of lhs 1140 b to understand if this modulation is attributable to the presence of water in the planetary atmosphere or is an artifact due to the presence of spots on the stellar surface. The habitability of lhs 1140 b is uncertain and depends on its atmospheric composition It orbits within the habitable zone of its host star, but recent studies suggest two potential scenarios With an equilibrium temperature of about 230 k, lhs 1140 b is situated close to the habitable zone (hz) of its star (dittmann et al

2024), where the existence of liquid water on the planet surface is possible.

In the left column of the output you can see the commit message corresponding to each parameter