![Pollux optical layout. The exact sequence in the optical path of the retractable polarimeters and fiber link connections of the OPT and NIR is still to be discussed and what shown here is not representative of the final configuration. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Pollux.png?resize=1200%2C715&ssl=1)
[astro-ph.IM] Pollux is a high-resolution spectrograph and spectropolarimeter (R from 65000 to 100000) covering a spectral range from 100 nm to 1750 nm, proposed by a European consortium to equip […]
Habitable Zones
![Retrieved emission spectra (blue regions) plotted with the true planet’s flux from our forward model (red) for each redox state considered (IW-6 to IW+6). The retrieved spectra denser region represents the 1𝜎 confidence level, intermediate region 2𝜎, thin region the 3𝜎 level. The observational noise from LIFEsim is shown as a gray envelope. The retrieved spectra capture most spectral features in observed planets, especially in the more pronounced oxidised cases (bottom row). -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Characterizing-the.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
Characterizing The Oxidation State Of Rocky Exoplanets With The Large Interferometer For Exoplanets (LIFE)
[astro-ph.EP] The oxidation state of rocky exoplanets is expected to play a fundamental role in shaping the chemical composition of their secondary atmospheres by influencing the chemical composition of volcanically […]
![Stellar influence on planetary habitability. Figure credit: solar images from NASA/ESA and KPNO/NSO/AURA/NSF, background pictures generated through OpenAI’s image-generation system (i.e., Adobe Firefly and ChatGPT Images 2.0). Illustration: K. Herbst - [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/StellarActivity.jpg?resize=1200%2C720&ssl=1)
Posted inHabitable Zones
Stellar Activity, Exoplanet, Habitability, Planetary Atmospheres
[astro-ph.EP] This chapter will review the deep connection of planetary habitability and stellar irradiation. We present the long-term stellar evolution as one of the drivers of atmospheric escape and climate […]
![This global map of Mars (greys) is overlaid with a map of ice “consistency,” C. Values of C near one (dark blue) indicate a high likelihood of ice in three independent mappings. Lower values of C (lighter blues) indicate lower confidence in ice being present, and indicate detection in at least one dataset. The extreme north and south are both rich in ice (dark blues), ice is absent near the equator, and the presence of ice is uncertain (light blues) in the mid-latitude regions best for astronauts. Credit: Morgan & Putzig et al., 2025; Sizemore et al., 2026 -- [PSI]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Laying-Odds.png?resize=1200%2C719&ssl=1)
Posted inMars
Laying Odds On The Potential For Martian Water
[PSI] We know Mars has water ice in its polar regions, but astronauts (and their solar powered equipment!) would much rather experience life closer to Mars’ equator. As NASA looks […]
Posted inSpace Life Science
Assessing The Susceptibility Of Microalgae To Space Conditions Using Stratospheric Balloons
[Scientific Reports via Xmol] Biological exposure experiments under near-space conditions remain limited by the high cost and low accessibility of spaceflight platforms, motivating low-cost analog approaches for initial screening.
Posted inAway Teams & Field Reports
Microorganisms Actively Shape Earth’s Ocean Floor
[MARUM]. In August 2023, the German research vessel METEOR set sail on Expedition M192 to the Greek island of Milos with Dr. Solveig Bühring as the chief scientist. The mission […]
Posted inExtremeophiles and Extreme Environments
Rock-eating Fungi Flourish Deep Within Earth
[University of Michigan] Hundreds of feet below Earth’s surface, rocks and water teem with fungi and support complex ecosystems of tiny organisms, according to a University of Michigan study, which […]
Posted inMicrobiology & Virology
Methane Production On Mars-Relevant Clay Minerals And Simulant Regolith
[Microorganisms]. Over the course of Martian history, the presence of atmospheric carbon dioxide and potential subsurface molecular hydrogen (H2), in addition to potential surface and subsurface liquid water, suggests that […]
Posted inExoplanets, -moons, -comets
SCoRE: The Surface Composition Of Rocky Exoplanets
[astro-ph.EP] Context. The crust composition of rocky exoplanets with a substantial atmosphere can not be observed directly. However, recent developments are starting to allow for the observation and characterisation of […]
Posted inExoplanets, -moons, -comets
Atmospheric Escape Rates of Planets in Stellar Tidal Fields from 3-D Hydrodynamic Simulations
[astro-ph.EP] Thermally driven atmospheric escape, including photo-evaporation and core-powered mass-loss, plays a key role in shaping the evolution of close-in exoplanets, yet most current models rely on simplified one-dimensional descriptions […]