As starlight passes through the atmosphere of the transiting exoplanet, it changes.
The signal is faint, but with a powerful enough telescope, and a stack of transits, the changing absorption and emission features on the spectrum can be decoded to determine the contents of an exoplanet's atmosphere.With the first detailed exoplanet atmosphere analysis, it seems that the space telescope is going to live up to its promise.
We may not detect the signatures of life in an exoplanet atmosphere with JWST – perhaps an even more powerful telescope will be required to deliver that level of fine detail – but with the analysis of WASP-39b, that discovery is feeling ever more tantalizingly within grasp.