Detectability of Biosignatures in Anoxic Atmospheres with the James Webb Space Telescope: A TRAPPIST-1e Case Study
Year: 2018
Type: article
Abstract: The James Webb Space Telescope (JWST) may be capable of finding biogenic gases in the atmospheres of habitable exoplanets around low-mass stars. Considerable attention has been given to the detectability of biogenic oxygen, which could be found using an ozone proxy, but ozone detection with JWST will be extremely challenging, even for the most favorable targets. Here, we investigate the detectability of biosignatures in anoxic atmospheres analogous to those that likely existed on the early Earth. Arguably, such anoxic biosignatures could be more prevalent than oxygen biosignatures if life exists elsewhere. Specifically, we simulate JWST retrievals of TRAPPIST-1e to determine whether the methane plus carbon dioxide disequilibrium biosignature pair is detectable in transit transmission. We find that ∼10 transits using the Near InfraRed Spectrograph prism instrument may be sufficient to detect carbon dioxide and constrain methane abundances sufficiently well to rule out known, nonbiological CH4 production scenarios to ∼90% confidence. Furthermore, it might be possible to put an upper limit on carbon monoxide abundances that would help rule out nonbiological methane-production scenarios, assuming the surface biosphere would efficiently draw down atmospheric CO. Our results are relatively insensitive to high-altitude clouds and instrument noise floor assumptions, although stellar heterogeneity and variability may present challenges.
Source: The Astronomical Journal
Institutions: University of Washington, University of Oxford
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
SDG: Climate action
Open Access status: bronze
Awards: NASA HAS A LONGSTANDING INTEREST IN LOOKING FOR LIFE ELSEWHERE IN THE UNIVERSE. TELESCOPES ARE CURRENTLY BEING DESIGNED AND BUILT THAT WILL BE CAPABL, Solar System Planetary Science at Oxford 2016-2019, FPDS BASE DESCRIPTION, MULTIPLE YEAR AWARD&INCREMENTAL FUNDING FOR YEARS 1 OF 5. THIS PROPOSAL IS ENTITLED, "THE VIRTUAL PLANETARY LABORATORY." THI, G465804250, Astrophysics and Planetary Science at Oxford 2013-16, Astrophysics at Oxford 2016-2019
OpenAlex ID: W2888433204
