Lethal surface ozone concentrations are possible on habitable zone exoplanets

TL;DR

This study uses climate modeling to show that surface ozone levels on habitable zone exoplanets could reach toxic concentrations, impacting potential habitability assessments.

Contribution

It presents the first detailed modeling of surface ozone concentrations on exoplanets, highlighting conditions that could produce lethal ozone levels.

Findings

Surface ozone can reach toxic levels exceeding 40 ppbv.

Certain atmospheric scenarios produce ozone concentrations up to 2200 ppbv.

Ozone levels vary significantly across different planetary conditions.

Abstract

Ozone ($\textrm{O}_3$) is important for the survival of life on Earth because it shields the surface from ionising ultraviolet (UV) radiation. However, the existence of $\textrm{O}_3$ in Earth's atmosphere is not always beneficial. Resulting from anthropogenic activity, $\textrm{O}_3$ exists as a biologically harmful pollutant at the surface when it forms in the presence of sunlight and other pollutants. As a strong oxidiser, $\textrm{O}_3$ can be lethal to several different organisms; thus, when assessing the potential habitability of an exoplanet, a key part is determining whether toxic gases could be present at its surface. Using the Whole Atmosphere Community Climate Model version 6 (WACCM6; a three-dimensional chemistry-climate model), twelve atmospheric simulations of the terrestrial exoplanet TRAPPIST-1 e are performed with a variety of $\textrm{O}_2$ concentrations and assuming two different stellar spectra proposed in the literature. Four atmospheric simulations of the exoplanet Proxima Centauri b are also included. Some scenarios for both exoplanets exhibit time-averaged surface $\textrm{O}_3$ mixing ratios exceeding harmful levels of 40 ppbv, with 2200 ppbv the maximum concentration found in the cases simulated. These concentrations are toxic and can be fatal to most life on Earth. In other scenarios $\textrm{O}_3$ remains under harmful limits over a significant fraction of the surface, despite there being present regions which may prove inhospitable. In the case that $\textrm{O}_3$ is detected in a terrestrial exoplanet's atmosphere, determining the surface concentration is an important step when evaluating a planet's habitability.