[Frontiers in Microbiology] On the north shore of Great Salt Lake, Utah, USA, naturally occurring tar seeps at Rozel Point provide an opportunity to study a petroleum-rich environment adjacent to […]
Desert Worlds
Posted inCryobiology
Ancient Marine Life May Be Hiding In Antarctica’s Blood Falls
[Scripps/JCVI] Blood Falls has long been one of Antarctica’s strangest landmarks: a red-stained outflow that spills from the face of Taylor Glacier into the cold, dry landscape of the McMurdo […]
![Physical and chemical gradients predicted to dictate habitability across depth in the martian subsurface. These include (1) constraints on water; although water activity (aw) gradients are not yet known for Mars, predicted liquid brine stability depends on primary ionic composition with perchlorate-rich brines transitioning into chloride- and sulfate-enriched brines with depth and temperature (Chevrier and Slank, 2024; Stevens and Cockell, 2023). It is important to note that porosity is expected to decrease with depth, which may also influence water availability, with any potential brines increasingly localized to pore spaces and fractures (Michalski et al., 2018). (2) Surface radiation exposure is expected to subside to lower background radionuclide decay around 3–5 m depth. (3) If liquid water is present at depth, chemotrophic microbial communities could utilize the products of water–rock interaction including inorganic electron donors/acceptors and simple abiotic organics. Image created using biorender.com.-- [Astrobiology (Journal)]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Life-Detection.png?resize=1200%2C719&ssl=1)
Posted inMars
Life Detection In The Martian Subsurface: Advancements In Microbial Metabolic Research Under Mars Laboratory And Field-Analog Conditions Since Viking
[Astrobiology (Journal)] Following the Viking experiments in 1976, many of the original inferences of biological metabolism have been replicated via abiotic mechanisms we now know are plausible on Mars’ surface.
Posted inAstropharmacy / Biotechnology
Pigmented Fungi Derived From Hot And Cold deserts Ecosystems: Taxonomy, Genomic And Biotechnological Approach
[World Journal of Microbiology and Biotechnology] Safer and more efficient products and processes are current global demands that drive the field of bioprospective research. Microbial sources are the main natural […]
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 […]
![A close-up of the polygon fractures discovered by NASA’s Curiosity Mars rover highlights their honeycomb-like textures. Credit: NASA/JPL-Caltech/MSSS [Larger Image]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Curiosity-Mars.png?resize=1200%2C719&ssl=1)
Posted inMars
Curiosity Mars Rover Discovers A Field Of Honeycomb Textures
[NASA] Mission scientists have never seen so many of the many-sided geologic features in one place on the Red Planet.
Posted inMars
Viking Science
[Astrobiology (Journal)] The Viking missions hosted identical payloads on each of two orbiters and landers. All four missions far exceeded their pre-planned operating times and science objectives, with all but […]
Posted inMars
Current Water Trapping Micro-habitats On The Surface Of Mars
[Science Direct] This paper presents a conceptual model exploring a possible mechanism by which liquid water could potentially be maintained in direct contact with hypothetical microorganisms during warm daytime periods […]
![(A) Summary interpolation of the extent of bedrock geologic units based on in situ mapping. The width of the mapping corridor is ∼120 m. White dots are positions occupied during the traverse for which images are available for mapping. (B) Summary of interpreted stratigraphic relationships between identified lithologic units along the Jezero crater floor traverse (A and B adapted from Crumpler et al., 2023; Fig. 19). (C) Orbital image of Jezero crater floor with the path of the Perseverance overlaid in white. (D) Inset of the crater floor campaign, with all Máaz abrasion patches shown (Guillaumes, Montpezat, Bellegarde, and Alfalfa), and the OEB (Octavia E. Butler) landing site indicated. The Guillaumes and Alfalfa abrasions are highlighted, as they are the focus of this article (altered from NASA). -- [Astrobiology (journal)]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/The-Possible-Aqueous.png?resize=1200%2C718&ssl=1)
Posted inMars
The Possible Aqueous Origins of Manganese Alteration Minerals in the Máaz Formation of Jezero Crater
[Astrobiology (journal)] Home to a lake around 4 billion years ago, Jezero Crater is a unique location to study the interplay between igneous processes and aqueous alteration on ancient Mars.
Posted inFossils & Paleontology
Where Was This Fossil 200 Million Years Ago?
[University of Barcelona] Calculating a fossil’s position throughout geological history is a complex process. In palaeontology and other disciplines, determining a location in the past is quite a challenge that […]