The detection of life on rocky exoplanets in the habitable zones of nearby stars would be a paradigm-shifting advance, and it is one of the greatest scientific challenges of our […]
![Earth’s spectrum over time (right panel), reproduced from [11]. The biosignature gases present change dramatically from epoch to epoch (left panel), producing significantly different spectra. The simultaneous detection of O2 at 0.8 µm demonstrates the presence of life in the modern Earth spectrum shown in the bottom right panel, but for habitable planets without much evidence of oxygenic biosignatures (e.g. Proterozoic and Archean Earth), coverage beyond 0.8 µm will be key to capture H2O, and CH4 features. -- astro-ph.IM](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/03/The-Key-to-Unlocking-Exoplanet.png?resize=1200%2C719&ssl=1)
The detection of life on rocky exoplanets in the habitable zones of nearby stars would be a paradigm-shifting advance, and it is one of the greatest scientific challenges of our […]