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The Goldilocks Problem for Detecting Water in Terrestrial Planets: Constraining Water Abundances in the Mid-infrared with LIFE

  • Authors: S. Rugheimer, E. Alei, B.S. Konrad, B. Taysum, J. L. Grenfell, T. Lichtenberg, D. Kitzmann, F. van der Tak, S.P. Quanz

S. Rugheimer et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 4.

Water posteriors for simulations for a range of surface H2O abundances from 1 bar to 10−7 bar at a resolution and S/N of R = 100 and S/N = 10, respectively. The black lines are the H2O profiles in volume mixing ratios in log10 (L) overlaying the H2O posteriors. The left panel assumes an altitude-invariant profile for water, commonly used in retrievals. The center panel fixes the surface abundance and then assumes a scaled Earth-like profile. The right panel fixes the surface H2O abundance and has diffusion and photochemical production at all other altitudes.

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