Mature super-Earths and sub-Neptunes are predicted to be≃ Jovian radius when younger
than 10 Myr. Thus, we expect to find 5–15 R⊕ planets around young stars even if their older …

Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits,
and structures are shaped by their environment. Young planets (< 1 Gyr) offer an opportunity …

The detection and characterization of young planetary systems offer a direct path to study
the processes that shape planet evolution. We report on the discovery of a sub-Neptune …

We report the discovery and characterization of a nearby (∼ 85 pc), older (27±3 Myr),
distributed stellar population near Lower Centaurus Crux (LCC), initially identified by …

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 …

Giant planets on short-period orbits are predicted to be inflated and eventually engulfed by
their host stars. However, the detailed timescales and stages of these processes are not well …

Young exoplanets can offer insight into the evolution of planetary atmospheres,
compositions, and architectures. We present the discovery of the young planetary system …

Young terrestrial worlds are critical test beds to constrain prevailing theories of planetary
formation and evolution. We present the discovery of HD 63433 d—a nearby (22 pc), Earth …

We present the discovery of a transiting hot Jupiter orbiting HIP 67522 (T eff∼ 5650 K; M*∼
1.2M⊙) in the 10–20 Myr old Sco-Cen OB association. We identified the transits in the TESS …

We present the discovery of a pair of transiting giant planets using four sectors of TESS
photometry. TOI-216 is a 0.87 M⊙ dwarf orbited by two transiters with radii of 8.2 and 11.3 …