Ultraviolet (UV) photons are diagnostic of many stellar and planetary processes, including system formation, planet atmospheres, habitability, stellar activity, and star-planet interactions. With very limited access to UV observations of exoplanetary systems, it is time to bring the exoplanet, stellar, and solar-system communities together to discuss the state of knowledge, identify the missing information, and plan the instrumentation needed for future space-based UV observatorie
we suppose that you agree to their usage. You can change the configuration or obtain more information
about our cookies policy by clicking here.