[NASA]. The Habitable Worlds Observatory (HWO) is a large-aperture ultraviolet/visible/near-infrared observatory concept recommended by the National Academies of Science, Engineering, and Medicine decadal survey, “Pathways to Discovery in Astronomy and […]
Biosignatures
Posted inExtremeophiles and Extreme Environments
Microbial Evolution, Biogeochemical Functions, And Environmental Adaptations In A Desert Saline Lake On The Qinghai–Tibet Plateau
[biorxiv.org] The Eboliang Hu saline lakes in the hyper-arid Qaidam Basin is a high-altitude, weakly acidic hypersaline system with strong environmental gradients and limited nitrogen availability.
![Bifurcated best-fit solutions. The noisy generated data is shown with gray error bars. The true spectrum of Earth is in black, while the Earth-like solution and thick- -atmosphere solution are shown in blue and orange, respectively. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Impacts.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
Impacts Of Correlated Noise On Retrievals Of Exo-Earth Atmospheres
[astro-ph.EP] The Habitable Worlds Observatory (HWO) aims to accomplish high-contrast imaging and spectroscopy of true Earth analogs for the first time. However, high-contrast spectroscopy with HWO may be limited by […]
![Best-fit model spectra and residuals for the HWO and LIFE datasets (grey and black data points with error bars). Shaded regions show posterior predictive intervals, and the lower panel shows residuals in units of σ. Bottom: Residual between the data and model as measured by 1-σ uncertainty. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/on-the.png?resize=1200%2C715&ssl=1)
Posted inBiosignatures & Paleobiology
On The Impact Of Correlated Noise and Spectral Resolution On The Retrieval Analysis Of The Habitable World Observatory
[astro-ph.EP] Finding signs of life elsewhere in the universe is the holy grail of the field of exoplanets. Future space missions such as the Habitable World Observatory (HWO) are under […]
Posted inMoon
Potential Survivable Niches For Microbial Life On The Lunar South Pole
[astro-ph.EP]. Most lunar surface conditions are incredibly harsh for microbial survival. High ultraviolet radiation, temperatures, and energetic particle radiation limit survival over most unprotected lunar surfaces, particularly in equatorial regions […]
Posted inBiosignatures & Paleobiology
Proto-Biosignatures and Planetary Geochemical Metabolism: A Thermodynamic Screening Model of Prebiotic Geochemical Organization
[Life (Basel)] Astrobiological observations usually return atmospheric, mineralogical, molecular, isotopic, or textural states rather than organisms.
Posted inAstronomy & Telescopes
Roman Space Telescope Leaves Earth
[NASA]. Now on a three-month, million-mile journey to its final orbit, NASA’s Nancy Grace Roman Space Telescope will soon reveal the universe’s darkest secrets. The mission launched at 7:26 a.m. […]
![[LEFT] The MIRI F2100W observation of the HD 107146 system, shown in logarithmic scaling with the corresponding intensity levels indicated in the colorbar. [RIGHT] Contours from the ALMA observations obtained within the ARKS program (S. Marino et al. 2026), overlaid on the combined F182M and F210M JWST/NIRCam observations for HD 107146. -- [astro-ph.SR]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/The-JWSTNIRCam.png?resize=1200%2C720&ssl=1)
Posted inAstrogeology
The JWST/NIRCam Scattered Light Disks GTO 2780 program: Panchromatic coronagraphic imaging of the HD 10647, HD 32297, HD 61005, HD 107146, and HD 181327 debris disk systems
[astro-ph.SR]. Debris disks, composed of rocks, boulders, planetesimals, and the dust produced in their collisions, present the most readily observable components of mature planetary systems.
![Three-dimensional layout of the four-aperture SELF optical model implemented in Ansys Zemax OpticStudio (Ansys, Inc. 2024), showing the arrangement of the primary and secondary mirrors, together with the optical path used for focalplane image generation. The inset provides a magnified view of the secondary mirrors. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Deep-Learning.png?resize=1200%2C720&ssl=1)
Posted inBiosignatures & Paleobiology
Deep Learning-Based Coarse Alignment and Cophasing of a Distributed-Aperture Telescope. Application to the Small ExoLife Finder (SELF)
[astro-ph.IM] The ExoLife Finder (ELF), a 35–50-meter-class Fizeau interferometric telescope, was designed to detect biosignatures on exoplanets through direct imaging. The Small ExoLife Finder (SELF), a 3.5-meter prototype, serves as […]
![Global maps of predicted pigment concentrations (left column) and pigment-to-chlorophyll-a ratios (right column) for May 2010 generated using the Random Forest model. Panels (a–f) show fucoxanthin, peridinin and zeaxanthin.-- [q-bio.OT]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/beyond.png?resize=1200%2C717&ssl=1)
Posted inBiosignatures & Paleobiology
Beyond Chlorophyll: Machine Learning Estimates Of Diagnostic Phytoplankton Pigments From Multispectral Ocean Colour Data
[q-bio.OT] Phytoplankton play a central role in marine ecosystems and the global carbon cycle, with different groups contributing differently to ocean biogeochemical processes.