This artist’s impression displays TRAPPIST-1 and its planets reflected in a surface. The potential for water on each of the worlds is also represented by the frost, water pools, and

Single-molecule Peptide Sequencing Through Reverse Translation Of Peptides Into DNA – PNAS Editor’s note: with recent speculation about the potential habitability of other worlds and understanding the processes whereby other

Exoplanet 29 Cygni b, seen in this artist’s concept, is a gas giant weighing about 15 times the mass of Jupiter. It orbits a type A star (shown at upper

NCCR PlanetS This chapter reviews the current state of observational and theoretical efforts in the characterization of exoplanet atmospheres, with a focus on developments enabled through the Swiss National Centre

Picture of the construction of ELT@ESO (Credit: ESO) High-precision high-fidelity spectrographs are the most powerful instruments for exoplanets detection and characterization. The sub-m/s radial-velocity precision, required to detect Earth-mass exoplanets,