The diversity in mass and composition of planetary atmospheres stems from the different
building blocks present in protoplanetary discs and from the different physical and chemical …

Over the past several decades, thousands of planets have been discovered outside our
Solar System. These planets exhibit enormous diversity, and their large numbers provide a …

In Lammer et al.(2024), we defined Earth-like habitats (EHs) as rocky exoplanets within the
habitable zone of complex life (HZCL) on which Earth-like N2-O2-dominated atmospheres …

Chemical compositions of exoplanets can provide key insights into their physical processes
and formation and evolutionary histories. Atmospheric spectroscopy provides a direct …

High-energy radiation from a planet host star can have strong influence on the final
habitability of a system through several mechanisms. In this context we have constructed a …

The search for exoplanets has revealed a diversity of planetary system architectures, the
vast majority of which diverge significantly from the template of the solar system. In …

Progressive astronomical characterization of planet-forming disks and rocky exoplanets
highlight the need for increasing interdisciplinary efforts to understand the birth and life cycle …

From the thousands of known exoplanets, those that transit bright host stars provide the
greatest accessibility toward detailed system characterization. The first known such planets …

Context. Observations of exoplanetary systems demonstrate that a wide variety of planetary
architectures are possible. Determining the rate of occurrence of Solar System analogues …

Discoveries of exoplanets using the radial velocity method are progressively reaching out to
increasingly longer orbital periods as the duration of surveys continues to climb. The …