The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …

This review presents an insight into our current knowledge of the atmospheres of the planets
Venus, Mars, Jupiter, Saturn, Uranus and Neptune, the satellite Titan, and those of …

Planets orbiting M-dwarf stars are prime targets in the search for rocky exoplanet
atmospheres. The small size of M dwarfs renders their planets exceptional targets for …

The high-energy radiative output, from the X-ray to the ultraviolet, of exoplanet host stars
drives photochemical reactions and mass loss in the upper regions of planetary …

Studying the atmospheres of exoplanets is one of the most promising ways to learn about
distant worlds beyond our solar system. The composition of an exoplanet's atmosphere can …

Observations of cooler atmospheres of super-Earths and Neptune sized objects often show
flat transmission spectra. The most likely cause of this trend is the presence of aerosols (ie …

Transmission spectroscopy presents one of the most successful approaches for
investigating the atmospheres of exoplanets. We analyzed the near-infrared high-resolution …

The study of temperate sub-Neptunes is the new frontier in exoplanetary science. A major
development in the past year has been the first detection of carbon-bearing molecules in the …

Abstract The James Webb Space Telescope (JWST) has provided the first opportunity of
studying the atmospheres of terrestrial exoplanets and estimating their surface conditions …

Many super‐Earths are on very short orbits around their host star and, therefore, more likely
to be tidally locked. Because this locking can lead to a strong contrast between the dayside …