One of NASA's primary goals is to observationally characterize exoplanet atmospheres, understand the chemical and physical processes of exoplanets and improve the understanding...
The first JWST transmission spectra have revealed the properties of exoplanet atmospheres in exquisite detail but also a characterization bottleneck due to spectral contamination from...
Delivery and loss of volatile elements and compounds (such as water, carbon, nitrogen and the noble gases) during Earth’s accretion set the stage for the rest of our planet's...
Giant planets and brown dwarfs are astrophysical objects with different formation locations – planets in disks and brown dwarfs (we think) in giant molecular clouds. These different...
The JWST User Community is invited to call into Webb Office Hours to ask questions and directly interact with a team of STScI JWST experts via WebEx. We welcome questions about the...