Astrobiology71- Page

Overview of the atmosphere-interior exchange model we use for this study including the various geological processes that we simulate and the various parameters we consider in this model. The carbon

Increase in atmospheric temperature caused by AGN wind as a function of the mass of the central galactic SMBH in Solar masses. The left panel shows the energy-driven case, while

A drill-core section of the CCBH2 borehole showing a yellowish-red color resulting from the hydrothermal alteration process, with small carbonate mineralizations. In the bottom left, a fragment of the CCBH2

Design and evaluation of random peptide libraries using distinct amino acid alphabets. (a) Chemical structures of 16 α-amino acids assembled through solid phase peptide synthesis to generate random 25-mer peptides

Workflow of space missions. A. BOSS: Cyanobacterial biofilms were air-dried on the ground and integrated in the EXPOSE-R2 facility. Dried samples were exposed in LEO for 1.5 years. After retrieval

Derived CS rotational temperatures (top) and column densities (bottom) for our disk sample, sorted from left to right by column density. The median values are shown by the dashed orange

Survival probability of a single planet in a binary system that initially hosted three planets, across various orbital configurations. Each panel corresponds to a specific value of the binary’s semi-major

Exoplanets, -moons, -comets Status Report astro-ph.IM November 16, 2025 The extracted time-series stellar spectra for the +1 (left) and −1 (right) spectral orders for the transit of HAT-P-41b. The color

Key requirements for a Total Habitability Instrument (THI). — Biomimetic One key objective of astrobiology is to investigate and discover if other planetary bodies are habitable. The determination of whether