The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …

WASP-107b is a warm (approximately 740 K) transiting planet with a Neptune-like mass of
roughly 30.5 M⊕ and Jupiter-like radius of about 0.94 RJ (refs.,), whose extended …

Interactions between exoplanetary atmospheres and internal properties have long been
proposed to be drivers of the inflation mechanisms of gaseous planets and apparent …

Observations of transiting gas giant exoplanets have revealed a pervasive depletion of
methane,,–, which has only recently been identified atmospherically,. The depletion is …

The population of planets smaller than approximately 1.7 Earth radii (R⊕) is widely
interpreted as consisting of rocky worlds, generally referred to as super-Earths. This picture …

We present a systematic search for transiting giant planets () orbiting nearby low-mass stars
(). The formation of giant planets around low-mass stars is predicted to be rare by the core …

The distribution of close-in exoplanets is shaped by a complex interplay between
atmospheric and dynamical processes. The Desert-Rim Exoplanets Atmosphere and …

With sizable volatile envelopes but smaller radii than the solar system ice giants, sub-
Neptunes have been revealed as one of the most common types of planet in the galaxy …

Planets between the sizes of Earth and Neptune are the most common in the Galaxy,
bridging the gap between the terrestrial and giant planets in our solar system. Now that we …

We present two transit observations of the∼ 870 K, 1.7 R⊕ super-Earth TOI-836b with
JWST NIRSpec/G395H, resulting in a 2.8–5.2 μm transmission spectrum. Using two different …