Astrobiology28- Page

Disk physical structure from our three parametric models (Models 1 to 3 from top to bottom, see Tables 1 and 2). The 2D gas temperature (left) and total H density

Variation of the planetary radius, expressed as transit depth, as a function of wavelength. Sky-blue points correspond to DanishDFOSC (this work), lime to TESS (this work), orange to GROND (Mancini

(A) The model of EnINpro is colored by different domains with arrows representing β strands. The model highlights a β-solenoid fold (gray, purple) adjacent to the disulfide capping motif (orange).

Mg/Si ratios of JWST-observed hot Jupiter host stars versus separation (semi-major axis). Mg/Si ratios compiled from Brewer et al. (2016) with an error of 3.3% as quoted in Brewer &

Keith Cowing Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻 Follow on

Dale Andersen in an ice hole preparing to dive in Lake Untersee, Antarctica in February 2026 — Alessandro Cuzzeri Hi Keith, The team and I have been home for about

Qualitative projections of the best-fit three-dimensional spherical-harmonic model to the jointly decomposed first spatial mode, u(1), derived from three viewing geometries of Europa’s leading hemisphere. (e) Water-ice 3.1 µm Fresnel

A Representation of two possible evolution models of the RNA replication system containing two replicases and two parasites. B Illustration of the deterministic assumptions. C Transient compartmentalization with pooling (homogeneous