Revisiting the Greenhouse Effect of Non-greenhouse Gases in the Atmospheres of Earth-like Planets

editorAstrobiology6 hours ago7 Views

Revisiting the Greenhouse Effect of Non-greenhouse Gases in the Atmospheres of Earth-like Planets

Schematic summary of the surface temperature response to increasing pN2 on the pCO2 –pN2 plane, comparing Goldblatt et al. (2009, G+09), Wordsworth & Pierrehumbert (2013, WP13), and this work. For Goldblatt et al. (2009), the pink shaded region denotes the parameter range they explored, within which all cases show warming as pN2 increases. For Wordsworth & Pierrehumbert (2013), circles mark the parameter sets shown in their Figure 14a, and the annotation at the top summarizes their reported response. Circle size and color qualitatively indicate the surface temperature, with larger circles and warmer colors corresponding to higher temperatures. In Wordsworth & Pierrehumbert (2013), the sign of the response is inferred from the two data points connected by arrows, which indicate the direction of increasing pN2 . Background shading shows the approximate regimes obtained in this work, namely cooling, warming, and neutral surface-temperature response to increasing pN2. — astro-ph.EP

Although non-greenhouse gases can vary substantially in abundance in Earth-like atmospheres, their climatic influences remain insufficiently understood.

To investigate how such gases regulate climate, we vary the abundance of N2 as a representative non-greenhouse component in one-dimensional N2–CO2–H2O model atmospheres. Beyond pressure broadening of absorption lines and Rayleigh scattering emphasized in previous studies, our results show that changes in background N2 pressure influence climate by modifying the amount of atmospheric H2O, producing two effects: altering the thermodynamic lapse rate (H2O-dilute warming) and changing the radiative contribution of H2O to the greenhouse effect (H2O-load warming).

The resulting climate response to increasing N2 depends on the CO2 abundance. Under low CO2 conditions, dilution of atmospheric H2O leads to warming, whereas under high CO2 conditions, increased H2O loading also produces warming.

At sufficiently high N2 abundances, Rayleigh scattering induces cooling, an effect further amplified by the accompanying decrease in atmospheric H2O. Under high CO2 conditions, however, enhanced H2O loading increases the absorption of stellar radiation and overwhelms the contribution of Rayleigh scattering, causing the cooling response to disappear.

These results reveal multiple physical pathways through which non-greenhouse gases influence climate and provide a framework for understanding climate responses and habitability in diverse Earth-like atmospheres.

Tetsuo Taki, Hiroyuki Kurokawa, Yuka Fujii, Kosuke Aoki

Comments: 15 pages, 5 figures, accepted for publication in the Astrophysical Journal
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2605.10757 [astro-ph.EP] (or arXiv:2605.10757v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2605.10757
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Submission history
From: Tetsuo Taki
[v1] Mon, 11 May 2026 15:55:19 UTC (769 KB)
https://arxiv.org/abs/2605.10757

Astrobiology, Atmosphere,

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