The Role of Atmospheric Composition in Defining the Habitable Zone Limits and Supporting E. coli Growth
Asena Kuzucan (1, 2), Emeline Bolmont (1, 2), Guillaume Chaverot, (2, 3), Jaqueline Quirino Ferreira (2, 4), Bastiaan Willem Ibelings (2, and 4), Siddharth Bhatnagar (1, 2, 5), Daniel Frank McGinnis (2, 4), ((1) Observatoire de Gen\`eve, Universit\'e de Gen\`eve, Switzerland (2)

TL;DR
This study combines climate modeling and biological experiments to explore how atmospheric composition influences exoplanet habitability and microbial survival, providing new insights into the conditions supporting life beyond Earth.
Contribution
It introduces a novel approach by integrating 3D climate modeling with laboratory experiments on E. coli to assess habitability under different atmospheric compositions.
Findings
Atmospheric composition significantly impacts bacterial growth.
Refined inner boundaries of the habitable zone for H2 and CO2 atmospheres.
Microbial survival varies with different atmospheric gases.
Abstract
Studying exoplanet atmospheres is essential for assessing their potential to host liquid water and their capacity to support life (their habitability). Each atmosphere uniquely influences the likelihood of surface liquid water, defining the habitable zone (HZ), the region around a star where liquid water can exist. However, being within the HZ does not guarantee habitability, as life requires more than just liquid water. In this study, we adopted a two-pronged approach. First, we estimated the surface conditions of planets near the HZ's inner edge under various atmospheric compositions. By utilizing a 3D climate model, we refined the inner boundaries of the HZ for planets with atmospheres dominated by H2 and CO2 for the first time. Second, we investigated microbial survival in these environments, conducting laboratory experiments on the growth and survival of E. coli K-12, focusing on…
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Taxonomy
TopicsClimate Change Communication and Perception · Climate Change Policy and Economics
