Summary of our method and comparison to the traditional grid modeling approach. — astro-ph.EP JWST is revolutionizing the field of exoplanet atmospheres by delivering unprecedented spectroscopic constraints on their chemical
Summary of our method and comparison to the traditional grid modeling approach. — astro-ph.EP JWST is revolutionizing the field of exoplanet atmospheres by delivering unprecedented spectroscopic constraints on their chemical
Carbon-silicate cycle includes a carbon dioxide (CO2) dissolution in rainwater to form carbonic acid (H2CO3) that falls on land and oceans; b reaction of H2CO3 and silicate (SiO32-) to form
Visualization of the HAT-P-12b transmission spectrum and the underlying opacity contributions. Top: Combined spectra from the three JWST instruments and HST STIS (Alexoudi et al. 2020) with 1σ uncertainties, together
Two images of protoplanetary discs Tau 042021 (left) and Oph 163131 (right). — ESA Larger imagery This month’s ESA/Webb Picture of the Month offers us a two-for-one on brand new
Schematic diagram showing the relative depths of the CROMO well array, Quarry Valley and Core Shed Wells, with reference to the lithostratigraphic levels from CSW1-1 cores. Depth of the well,
Artist’s impression showing possible choices for the scale of human involvement in the future of Mars. Early on, warming occurs only close to human bases. Solid-state greenhouse membranes harvest liquid
WISE, near-infrared, and optical images of all ultracool wide binary candidates. Optical images either come from Pan-STARRS (PS1; Chambers et al. 2016) or DECam images obtained through the Astro Data
Four diagnostics of electron bombardment on Europa’s leading hemisphere: (a) total deposited-energy flux, (b) deposited-energy fraction, (c) mean secondary-electron energy, and (d) e-folding (≈ 63%) deposition depth. Cells with no
MIRI F1500W light curves of GJ 3473 b at secondary eclipse. The raw and binned data are shown in light grey and purple, respectively. The pink curves correspond to the
Simultaneously collected raw spectral images in array coordinates from band 2 (left) and band 5 (right) collected during the first practice survey and the first crossing of the Galactic plane.






