Produced by: Tarun Mishra
Insights from a new study suggest that the European Extremely Large Telescope (ELT) could offer the best prospects for detecting biosignatures on nearby rocky exoplanets within the next two decades, said a report published in The Astronomical Journal
The forthcoming European Extremely Large Telescope (ELT) emerges as a promising tool for characterizing exoplanets, including candidates like Proxima Centauri b, with the potential to harbour life.
Exoplanetary research relies heavily on studying atmospheres, with instruments like the James Webb Space Telescope (JWST) utilizing transit spectroscopy to analyse the chemical compositions of distant worlds.
Direct imaging of exoplanets poses challenges, despite recent successes in observing young, large planets. Spectral analysis of these distant worlds requires sophisticated telescopes with high signal-to-noise ratios.
Three giant ground-based telescopes, including the ELT, Thirty Meter Telescope (TMT), and Giant Magellan Telescope (GMT), are poised to revolutionize exoplanet characterization in the coming decade.
Scientists simulate the capabilities of ELT instruments, such as METIS and HARMONI, in detecting biosignatures on ten real-life exoplanets orbiting nearby red dwarf stars.
While the ELT shows promise in detecting biosignatures on certain exoplanets like GJ 887b, challenges persist in imaging and characterizing all seven worlds of the TRAPPIST-1 system.
Despite its limitations, the JWST continues to play a crucial role in exoplanet research, offering insights into the atmospheres of distant worlds like TRAPPIST-1's innermost planets.
Scientists emphasise the importance of leveraging next-generation telescopes, both ground-based and space-based, to advance our understanding of exoplanetary systems and the search for extraterrestrial life.