Methane hint on TRAPPIST 1e seen as likely stellar noise not proof of an atmosphere

Written by Copernical Team Monday, 08 December 2025 08:14

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Los Angeles CA (SPX) Dec 05, 2025

Two recent papers based on James Webb Space Telescope observations describe initial attempts to probe the atmosphere of TRAPPIST-1e, an Earth-sized planet orbiting in the habitable zone of the nearby red dwarf star TRAPPIST-1. In a follow-up analysis, University of Arizona planetary scientist Sukrit Ranjan argues that the current evidence is not yet sufficient to confirm that TRAPPIST-1e has an

by Clarence Oxford
Los Angeles CA (SPX) Dec 05, 2025

Two recent papers based on James Webb Space Telescope observations describe initial attempts to probe the atmosphere of TRAPPIST-1e, an Earth-sized planet orbiting in the habitable zone of the nearby red dwarf star TRAPPIST-1. In a follow-up analysis, University of Arizona planetary scientist Sukrit Ranjan argues that the current evidence is not yet sufficient to confirm that TRAPPIST-1e has an atmosphere and that tentative methane signatures could instead arise from the host star.

The TRAPPIST-1 system, discovered by the Transiting Planets and Planetesimals Small Telescope project, lies about 39 to 40 light-years from Earth and consists of seven roughly Earth-sized planets packed into orbits that would all fit inside Mercury's path around the Sun. TRAPPIST-1e sits in the star's temperate zone, where conditions could allow liquid water on the surface if the planet retains an atmosphere.

Ranjan, an assistant professor in the Lunar and Planetary Laboratory, notes that recent Webb spectra of TRAPPIST-1e have been interpreted as showing hints of methane, a gas that on Earth is strongly linked to biological and geological activity. He cautions that before discussing habitability, researchers must first answer the basic question of whether any atmosphere exists on the planet at all.

Webb's Near-Infrared Spectrograph observed TRAPPIST-1e during four separate transits, when the planet crossed the face of its star and a fraction of the starlight passed through any surrounding atmosphere. By combining these transit spectra, the team searched for absorption features from gases such as methane that would imprint themselves on the light.

Interpreting those spectra is complicated because TRAPPIST-1 is an ultracool M dwarf, only about one-tenth the Sun's mass and slightly larger than Jupiter, with a low surface temperature that allows molecules to exist in the stellar atmosphere. Ranjan points out that such stars can contribute molecular absorption features of their own, raising the possibility that the methane-like signal could originate from the star rather than the planet.

To investigate this, Ranjan and colleagues modeled a range of possible atmospheres for TRAPPIST-1e and compared their predicted spectra with the Webb data. One scenario treated TRAPPIST-1e as a "warm exo-Titan" with a methane-rich atmosphere analogous to Saturn's moon Titan but orbiting closer to an M dwarf star.

Their analysis, published as "The Photochemical Plausibility of Warm Exo-Titans Orbiting M Dwarf Stars" in The Astrophysical Journal Letters, found that even this relatively favorable methane-rich case is unlikely under current constraints. The work concludes that the apparent methane signature is more plausibly explained by spectral contamination from the host star than by a confirmed planetary atmosphere signal, although the existence of an atmosphere on TRAPPIST-1e cannot yet be ruled out.

Ranjan emphasizes that Webb was conceived before astronomers knew how common Earth-sized planets around M dwarfs would be, and only a small number of such worlds are bright enough for atmospheric spectroscopy. That makes TRAPPIST-1e a priority target but also means the community must be conservative when interpreting the first, relatively noisy datasets.

Future observations and analysis techniques are expected to sharpen the picture. The team is planning larger Webb campaigns and is developing methods to better disentangle stellar and planetary contributions, including "dual transit" observations in which both TRAPPIST-1e and TRAPPIST-1b pass in front of the star at the same time. Because TRAPPIST-1b appears to be airless, comparing its transit signal to that of TRAPPIST-1e may help isolate how much of the spectral structure comes from the star itself.

Additional measurements from dedicated missions such as NASA's upcoming Pandora small satellite, which will track exoplanet host stars and their planets through multiple transits, could further reduce uncertainties tied to stellar variability. Together, these efforts aim to determine whether TRAPPIST-1e truly bears an atmosphere and, if so, what its composition implies for the possibility of liquid water and habitability on this nearby world.?

Research Report:The Photochemical Plausibility of Warm Exo-Titans Orbiting M Dwarf Stars