The JWST has ushered in a new era in atmospheric characterisations of temperate low-mass exoplanets with recent detections of carbon-bearing molecules in the candidate Hycean world K2-18 b.
JWST
JWST Captures The End Of Planet Formation
The James Webb Space Telescope (JWST) is helping scientists uncover how planets form by advancing understanding of their birthplaces and the circumstellar disks surrounding young stars, in a paper published […]
Transiting Exoplanets With The Mid-InfraRed JWST Instrument: From Simulations To Observations
The James Webb Space Telescope (JWST) has now started its exploration of exoplanetary worlds. In particular, the Mid-InfraRed Instrument (MIRI) with its Low-Resolution Spectrometer (LRS) carries out transit, eclipse, and […]
Radiation From Massive Stars Shapes Planetary Systems
How do planetary systems such as the Solar System form? To find out, CNRS scientists taking part in an international research team studied a stellar nursery, the Orion Nebula, using […]
Measuring Tracers of Planet Formation in the Atmosphere of WASP-77A b: Sub-stellar O/H and C/H ratios, with a stellar C/O ratio and a potentially Super-stellar Ti/H ratio
We present a comprehensive atmospheric retrieval study of the hot Jupiter WASP-77A b using eclipse observations from the Hubble Space Telescope (HST) and JWST.
Destruction Of An Oceans’ Worth Of Water Per Month In The Orion Nebula
An international team, including Western astrophysicists Els Peeters and Jan Cami, has found the destruction and re-formation of a large quantity of water in a planet-forming disk located at the […]
Water-Ice Dominated Spectra of Saturn’s Rings and Small Moons from JWST
JWST measured the infrared spectra of Saturn’s rings and several of its small moons (Epimetheus, Pandora, Telesto and Pallene) as part of Guaranteed Time Observation program 1247.
Automated Chemical Reaction Network Generation And Its Application To Exoplanet Atmospheres
With the advent of JWST and spectroscopic characterization of exoplanet atmospheres with unprecedented detail, there is a demand for a more complete picture of chemical and photochemical reactions and their […]
The Imprint of Escaping Hydrogen Atmospheres on Super-Earth Interiors
Small, close-in exoplanets are divided into two sub-populations: super-Earths and sub-Neptunes. Most super-Earths are thought to have lost their primordially accreted hydrogen-dominated atmospheres via thermally driven winds.
On The Ocean Conditions Of Hycean Worlds
Recent studies have suggested the possibility of Hycean worlds, characterised by deep liquid water oceans beneath H2-rich atmospheres.
