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.
atmosphere
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 […]
Behind The Mask: Can HARMONI@ELT Detect Biosignatures In The Reflected Light Of Proxima b?
Proxima b is a rocky exoplanet in the habitable zone of the nearest star system and a key test case in the search for extraterrestrial life.
A 3D Picture Of Moist-convection Inhibition In Hydrogen-rich Atmospheres: Implications For K2-18 b
While small, Neptune-like planets are among the most abundant exoplanets, our understanding of their atmospheric structure and dynamics remains sparse.
Distinguishing Oceans Of Water From Magma On Mini-Neptune K2-18b
Mildly rradiated mini-Neptunes have densities potentially consistent with them hosting substantial liquid water oceans (`Hycean’ planets).
A Radius Valley Between Migrated Steam Worlds And Evaporated Rocky Cores
The radius valley (or gap) in the observed distribution of exoplanet radii, which separates smaller super-Earths from larger sub-Neptunes, is a key feature that theoretical models must explain. Conventionally, it […]
Hot Saturn Exoplanet HAT-P-18 b And Its Parent Star
Led by researchers from Université de Montréal’s Trottier Institute for Research on Exoplanets (iREx), a team of astronomers has harnessed the power of the revolutionary James Webb Space Webb Telescope […]
FlopPITy: Enabling Self-consistent Exoplanet Atmospheric Retrievals With Machine Learning
Interpreting the observations of exoplanet atmospheres to constrain physical and chemical properties is typically done using Bayesian retrieval techniques.
Astrobiological Potential of Venus Atmosphere Chemical Anomalies and Other Unexplained Cloud Properties
Long-standing unexplained Venus atmosphere observations and chemical anomalies point to unknown chemistry but also leave room for the possibility of life.
