The advent of radial velocity (RV) and transit photometry method has resulted in the
detection of more than 5000 exoplanets since 1995. Of these detected planets, a significant …

OVERVIEW Nearly 30 years after the discovery of the first exoplanet around a main
sequence star, thousands of planets have now been confirmed. These discoveries have …

Rocky planet compositions regulate planetary evolution by affecting core sizes, mantle
properties, and melting behaviors. Yet, quantitative treatments of this aspect of exoplanet …

The understanding of planet formation has changed recently, embracing the new idea of
pebble accretion. This means that the influx of pebbles from the outer regions of planet …

Planet formation is expected to be severely limited in disks of low metallicity, owing to both
the small solid mass reservoir and the low-opacity accelerating the disk gas dissipation …

Rocky exoplanets with bulk iron mass fraction of more than 60%, known as super-Mercuries,
appear to be preferentially hosted by stars with higher iron mass fraction than that of the …

Context. Exoplanetary properties strongly depend on stellar properties: to know the planet
with accuracy and precision it is necessary to know the star as accurately and precisely as …

As stellar compositions evolve over time in the Milky Way, so will the resulting planet
populations. In order to place planet formation in the context of Galactic chemical evolution …

Theoretical physical-chemical models for the formation of planetary systems depend on data
quality for the Sun's composition, that of stars in the solar neighbourhood, and of the …

Context. The study of exoplanets at different evolutionary stages can shed light on their
formation, migration, and evolution. The determination of exoplanet properties depends on …