A new piece of evidence supporting the photoevaporation-driven evolution model for low-
mass, close-in exoplanets was recently presented by the California–Kepler Survey. The …

Thousands of exoplanets have now been discovered with a huge range of masses, sizes
and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host …

M dwarf stars, which have masses less than 60 per cent that of the Sun, make up 75 per cent
of the population of the stars in the Galaxy. The atmospheres of orbiting Earth-sized planets …

We determine the orbital eccentricities of individual small Kepler planets, through a
combination of asteroseismology and transit light-curve analysis. We are able to constrain …

Mass, radius, and age measurements of young (≲ 100 Myr) planets have the power to
shape our understanding of planet formation. However, young stars tend to be extremely …

Detecting and confirming terrestrial planets is incredibly difficult due to their tiny size and
mass relative to Sun-like host stars. However, recent instrumental advancements are making …

The exoplanet population characterized by relatively short orbital periods (P< 100 d) around
solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets …

Young exoplanets are snapshots of the planetary evolution process. Planets that orbit stars
in young associations are particularly important because the age of the planetary system is …

Abstract Since 2014, NASA's K2 mission has observed large portions of the ecliptic plane in
search of transiting planets and has detected hundreds of planet candidates. With …

Diving Beneath the Sea of Stellar Activity: Chromatic Radial Velocities of the Young AU Mic
Planetary System - IOPscience This site uses cookies. By continuing to use this site you agree …