Water is an important component of exoplanets, with its distribution, i.e., whether at the surface or deep inside, fundamentally influencing the planetary properties.
atmosphere
ESA Approves EnVision Mission To Venus – The Closest Planet To Earth
ESA’s next mission to Venus was officially ‘adopted’ today by the Agency’s Science Programme Committee. EnVision will study Venus from its inner core to its outer atmosphere, giving important new […]
Heating of the Atmospheres of Short-orbit Exoplanets by Their Rapid Orbital Motion Through an Extreme Space Environment
Exoplanets with short orbit period reside very close to their host stars. They transition very rapidly between different sectors of the circumstellar space environment along their orbit, leading to large […]
Unraveling The Mysteries Of Planet Formation And Evolution In A Distant Solar System
A recently discovered solar system with six confirmed exoplanets and a possible seventh is boosting astronomers’ knowledge of planet formation and evolution. Relying on a globe-spanning arsenal of observatories and […]
Hubble Finds Water Vapour In The Atmosphere Of Small Exoplanet GJ 9827d
Astronomers are intrigued when finding evidence of water vapour on exoplanets. Based on observations with the Hubble Space Telescope, a recent example is the planet GJ 9827d, which may have […]
Observations Of Scattered Light From Exoplanet Atmospheres
Optical phase curves of hot Jupiters can reveal global scattering properties. We implement a Bayesian inference framework for optical phase curves with flux contributions from: reflected light from a potentially […]
Atmospheric Pressure Changes Could Be Driving Mars’ Elusive Methane Pulses
New research shows that atmospheric pressure fluctuations that pull gases up from underground could be responsible for releasing subsurface methane into Mars’ atmosphere; knowing when and where to look for […]
Dynamical Phenomena In The Martian Atmosphere Through Mars Express Imaging
This review describes the dynamic phenomena in the atmosphere of Mars that are visible in images taken in the visual range through cloud formation and dust lifting.
JWST Observations Of K2-18b Can Be Explained By A Gas-rich Mini-Neptune With No Habitable Surface
JWST recently measured the transmission spectrum of K2-18b, a habitable-zone sub-Neptune exoplanet, detecting CH4 and CO2 in its atmosphere.
Inner Edge Habitable Zone Limits Around Main Sequence Stars: Cloudy Estimates
Understanding the limits of rocky planet habitability is one of the key goals of current and future exoplanet characterization efforts. An intrinsic concept of rocky planet habitability is the Habitable […]
