The third day of #Biochemistry2026 is off to a great start with an inspiring lecture by Schraga Schwartz. He talked about "RNA at the Edge: Extreme Biology as a Lens on RNA Modification Principles".

https://www.sciencedirect.com/science/article/abs/pii/S0092867425010827
#Biochemistry #Chemistry #ChemBio #RNA #extremophiles #Archaea
CC: @gdch

💎🌡️ The Cueva de los Cristales is home to giant beams of selenite that grew over hundreds of thousands of years in extreme heat. Scientists recently found dormant #microbes trapped inside the #crystals that may provide clues about how life survives in the harshest environments on #Earth.

👉 https://www.discoverwildlife.com/animal-facts/crystal-cave

#cave #mexico #geology #microbiology #extremophiles #science #nature #exploration #minerals #discovery #earthscience #biology

It's a staggering 300 metres underground, features amazing 11-metre-tall crystals – and has a deadly 90% humidity level | Discover Wildlife

Discover Wildlife

🦠🪐 New #research from Johns Hopkins University suggests that the boundary between #planets might be a lot leakier than we thought.

By sandwiching the hardy bacterium Deinococcus radiodurans between steel plates and shooting them at nearly 500 km/h (~300 mph), scientists demonstrated they can survive 30,000 times atmospheric pressure.

👉 https://www.sciencealert.com/extreme-microbes-can-survive-the-journey-between-planets-experiments-show

#science #space #biology #astronomy #mars #panspermia #extremophiles

Extreme Microbes Can Survive The Journey Between Planets, Experiments Show

The idea that life can spread from world to world dates as far back as ancient Greece and the philosopher Anaxagoras.

ScienceAlert

#Extremophiles that can digest #radiation ☢️ and toxicities are already used to clean up everything from oil spills to the fallout of radioactive sites.

This means we could #engineer microbes that are resistant to freezing ❄️ temperatures and high levels of radiation.

Given that #microbes 🦠 helped make Earth habitable, we could use synthetic #biology to engineer microbes to speed up a similar process for #Mars 🔴 https://theconversation.com/how-to-engineer-microbes-to-enable-us-to-live-on-mars-253456

#CrisprCas9 #SyntheticBiology #Terraforming #Mars

How to engineer microbes to enable us to live on Mars

Microbes could pump out oxygen on Mars.

The Conversation

🦠 Life can flourish in Earth’s most hostile corners. What does that resilience suggest about where life could persist beyond Earth?

✍️ Read the full exploration: https://TPC8.short.gy/mgHJjLGk

Perhaps the cosmos holds more tenacious possibilities than we expect.

#Astrobiology #Extremophiles #Tardigrades #Habitability #Biodiversity #Cosmos #Microbes #Science #LifeBeyondEarth #Biology #TPC8

The Unlikely Astronauts: What Earth’s Toughest Survivors Teach Us About the Possibility of Life Elsewhere 🦠

How Earth's extremophiles like tardigrades reshape our search for alien life on Mars, Europa & beyond. Discover astrobiology's new frontier.

The Science of Life Beyond Earth: A Guide to Astrobiology

Astrobiology: Redefining Life’s Boundaries: The Interdisciplinary Quest

Does life exist beyond the pale blue dot we call home? This profound question, once the domain of philosophers and science fiction writers, is now the driving force behind a rigorous, interdisciplinary scientific field: astrobiologyAstrobiology seeks to understand the origin, evolution, distribution, and future of life in the universe. It is not a single discipline but a convergent science, weaving together astronomy, biology, chemistry, geology, and planetary science to tackle one of humanity’s greatest mysteries. The core premise of the astrobiology search for life is that the principles of chemistry and physics are universal, and the conditions that led to life on Earth could—and likely do—arise elsewhere. This search operates on two complementary fronts: studying the limits of life on our own planet to understand where and how it can thrive in extreme environments, and identifying promising locations elsewhere in our Solar System and around other stars where similar conditions might exist. The modern astrobiology search for life is grounded in empirical evidence and follows the scientific method, moving from speculation to hypothesis-driven exploration. It compels us to ask fundamental questions: What is life? How did it begin on Earth? What are the absolute requirements for habitability? And what detectable signs, or biosignatures, would life leave behind? The field has matured alongside our exploration of the Solar System and the discovery of exoplanets, transforming a cosmic wonder into a tangible research program with specific targets, missions, and a framework for evaluating potential evidence. The journey of astrobiology is a testament to human curiosity, pushing us to explore the harshest environments on Earth and the most distant points in our galactic neighborhood in pursuit of an answer that would forever change our understanding of our place in the cosmos.

The field gained formal recognition and structure with the establishment of NASA’s Astrobiology Institute in 1998 and has since become a global endeavor. A pivotal moment in the astrobiology search for life was the discovery of extremophiles—organisms on Earth that thrive in conditions once thought utterly inhospitable. Scientists have found life flourishing in the boiling waters of deep-sea hydrothermal vents, within rocks in the arid Antarctic Dry Valleys, in highly acidic lakes, and deep underground, independent of sunlight. These discoveries dramatically expanded the “habitable zone” concept beyond the traditional notion of a planet orbiting at the right distance from its star for liquid water. It introduced the idea of “subsurface habitable zones,” where internal heat from a planet or moon (via radioactive decay or tidal friction) could maintain liquid oceans beneath icy shells, as is suspected on Jupiter’s moon Europa and Saturn’s moon Enceladus. This paradigm shift means that habitability is not a binary state of a planet, but a potential that can exist in specific niches. The astrobiology search for life is therefore not just about finding Earth-twins; it is about identifying worlds with energy sources, liquid solvents (like water, but potentially others like methane on Titan), and the necessary chemical building blocks. The guiding strategy is “follow the water, follow the carbon, follow the energy.” This approach has led to a prioritized list of targets within our reach: Mars, with its evidence of a wet past; the icy ocean moons Europa and Enceladus; Titan’s unique methane cycle; and, increasingly, the atmospheres of potentially habitable exoplanets. Each target represents a different chapter in the story of how life might arise and persist, making astrobiology the most ambitious detective story ever undertaken.

The Building Blocks: Habitability and Life’s Raw Materials

A habitable world is one that can support life, not necessarily one that does. Key ingredients include:

  • A Liquid Solvent: Water is the primary candidate due to its excellent properties as a solvent for biochemical reactions. However, astrobiologists theorize about other possibilities, such as liquid methane/ethane on Titan or even ammonia.
  • Essential Elements: Life as we know it requires key elements, primarily carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur (CHNOPS). Carbon’s unique ability to form complex, stable molecules makes it central, though silicon-based life is a speculative alternative.
  • An Energy Source: Life needs energy to drive metabolism. On Earth, the primary source is sunlight (photosynthesis), but chemosynthetic life around hydrothermal vents uses chemical energy from minerals, proving alternative pathways exist.
  • Environmental Stability: Conditions must be stable enough over geological timescales for life to originate and evolve. This includes factors like planetary climate, protection from harmful radiation (via an atmosphere or magnetic field), and geological activity to recycle nutrients.

The Detective’s Clues: Biosignatures and Technosignatures

Since we cannot yet visit most promising worlds, we must look for remote signs. A biosignature is any measurable substance, pattern, or signal that provides scientific evidence of past or present life. These can be:

  • Atmospheric Biosignatures: Chemical disequilibrium in an atmosphere. For example, the simultaneous presence of abundant oxygen (O₂) and methane (CH₄) in Earth’s atmosphere is a strong biosignature, as these gases rapidly react with each other and require continuous biological production to maintain their levels. James Webb Space Telescope observations of exoplanet atmospheres aim to detect such imbalances.
  • Surface Biosignatures: Spectral signatures of pigments like chlorophyll (which causes the “vegetation red edge” on Earth) or other biological materials detectable on a planet’s surface.
  • Context is Critical: A major focus in astrobiology is avoiding “false positives.” For instance, oxygen can be produced abiotically by photolysis of water vapor. Therefore, a convincing case for life requires not just a potential biosignature gas, but a holistic understanding of the planetary context—its star, geology, and climate.
  • Technosignatures: These are signs of advanced technological civilizations, such as narrow-band radio signals, laser pulses, atmospheric pollution (like CFCs), or structures like Dyson spheres. The search for technosignatures, often associated with SETI (Search for Extraterrestrial Intelligence), is a complementary strand of the astrobiology search for life.

Prime Targets in Our Cosmic Backyard and Beyond

The astrobiology search for life is actively pursued on multiple fronts:

  • Mars: The search focuses on evidence of past habitability (ancient riverbeds, lake sediments) and potential present-day subsurface liquid water or brines. Rovers like Perseverance are caching samples for return to Earth, where they can be analyzed for potential microscopic fossils or chemical traces of ancient life.
  • Icy Ocean Worlds (Europa & Enceladus): These moons are believed to harbor global subsurface oceans in contact with rocky, chemically active seafloors—environments analogous to Earth’s life-supporting hydrothermal vents. Future missions (Europa Clipper, concepts for an Enceladus orbiter) will study their plumes and ice shells in detail.
  • Titan: Saturn’s largest moon has a thick atmosphere and a complex hydrocarbon cycle with liquid methane lakes. While too cold for liquid water, it is a prebiotic laboratory where chemistries that might lead to alternative forms of life could be occurring.
  • Exoplanets: The statistical abundance of planets suggests habitable environments must be common. Characterizing the atmospheres of terrestrial planets in habitable zones is the long-term goal, with JWST beginning this work on larger, hotter targets and future observatories like the Habitable Worlds Observatory designed for Earth-analogs.

Philosophical Implications and the Future

The discovery of even simple microbial life beyond Earth would be a monumental event, demonstrating that life is a cosmic phenomenon and that the universe is biologically active. It would revolutionize biology by providing a “second genesis” for comparative study. Finding no life after exhaustive searching in seemingly habitable places would also be profound, suggesting Earth’s biosphere might be rarer than we think. The astrobiology search for life is ultimately a search for context—for understanding whether life on Earth is a singular miracle or a common piece of the universe’s fabric. As our tools become more sophisticated, this centuries-old question inches closer to an empirical answer, making astrobiology one of the most compelling and consequential scientific endeavors of our time.

👉 Share your thoughts in the comments, and explore more insights on our Journal and Magazine. Please consider becoming a subscriber, thank you: https://borealtimes.org/subscriptions – Follow The Dunasteia News on social media. Join the Oslo Meet by connecting experiences and uniting solutions: https://oslomeet.org

References

  • NASA Astrobiology Institute. (n.d.). What is Astrobiology? https://astrobiology.nasa.gov/about/
  • Des Marais, D.J., et al. (2008). The NASA Astrobiology Roadmap. Astrobiology, 8(4). https://www.liebertpub.com/doi/10.1089/ast.2008.0819
  • National Academies of Sciences, Engineering, and Medicine. (2019). An Astrobiology Strategy for the Search for Life in the Universehttps://nap.nationalacademies.org/catalog/25252/an-astrobiology-strategy-for-the-search-for-life-in-the-universe
  • Hoehler, T.M., & Westall, F. (2010). Mars: A new frontier for astrobiology. Space Science Reviews, 129. https://link.springer.com/article/10.1007/s11214-010-9735-y
  • Catling, D.C., et al. (2018). Exoplanet Biosignatures: A Framework for Their Assessment. Astrobiology, 18(6). https://www.liebertpub.com/doi/10.1089/ast.2017.1737
  • #Astrobiology #biosignatures #extremophiles #habitableWorlds #searchForLife

    "Life can exist on orders of magnitude lower power and sustain their living cells for orders of magnitude more years than previously thought possible. This means that many of these living beings bump up against the energetic limits of life, and in the process seem to have cracked the code for near-immortality. These types of intraterrestrials have such extremely long lifespans that we need a new term to describe the type of extremophiles that they are. The word aeonophiles fits, since they like (-phile) long periods of time (aeon-)."

    https://aeon.co/essays/the-discovery-of-aeonophiles-expands-our-definition-of-life

    #AeonMagazine #Aeons #Biology #Extremophiles #DeepLife

    The discovery of aeonophiles expands our definition of life | Aeon Essays

    The discovery of organisms that have been alive for many thousands of years requires a revolution in how we understand life

    🌋🦠 Extreme life redefined! This “fire amoeba” survives scorching 80°C temps—hotter than any complex life before—proving eukaryotes can thrive in hellish spots. Clues for alien worlds? Rethinking biology’s limits! Read more: https://thedebrief.org/we-need-to-rethink-whats-possible-this-fire-amoeba-proves-complex-life-can-survive-new-extremes/

    @goodnews

    #GoodNews #FireAmoeba #Extremophiles #LifeDiscovery #ScienceWin

    “We Need to Rethink What’s Possible:” This "Fire Amoeba" Proves Complex Life Can Survive New Extremes

    Science, Tech and Defense for the Rebelliously Curious.

    The Debrief

    Polar Microbes and Climate Change by Alysson Wagner, 2025

    A Molecular Understanding for Sustainable Future

    Recent studies on #extremophiles have focused on #thermophiles, microbes that thrive in high temperatures, while #psychrophiles, which prefer cold environments, have received less attention. However, interest in cold-adapted microbes, especially those in polar regions, has increased significantly in recent decades.

    #books
    #nonfiction
    #microbes
    #PolarRegions
    #ClimateChange
    #Springer

    The genome of an animal, a deep-sea annelid, that grazes on bacterial growing off hot thermal vents in largely anoxic environments at the bottom of the ocean. Great potential for being a treasure trove of new proteins for use in molecular biology.

    "Chromosome-scale genome assembly and gene annotation of the hydrothermal vent annelid Alvinella pompejana yield insight into animal evolution in extreme environments", El Hilali et al. 2025
    https://link.springer.com/article/10.1186/s12915-025-02369-7

    #annelids #extremophiles #science #genomics

    Chromosome-scale genome assembly and gene annotation of the hydrothermal vent annelid Alvinella pompejana yield insight into animal evolution in extreme environments - BMC Biology

    Background The Pompeii worm Alvinella pompejana, a terebellid annelid, has long been an exemplar of a metazoan that lives in an extreme environment, on the chimney wall of deep-sea hydrothermal vents, but this very environment has made it difficult to study. Comprehensive assessment of Alvinella pompejana genome content, and the factors that could explain its ability to thrive in seemingly hostile conditions has been lacking. Results We report the chromosome-level genome sequence of Alvinella pompejana and population-level sequence variants. We produced a set of gene models and analysed the predicted protein set in the light of past hypotheses about the thermotolerance of Alvinella, comparing it to other recently sequenced vent annelids. Despite its extreme environment, we find evidence for relatively conservative evolution of protein amino acid composition and genome evolution as measured by synteny. We suggest that prior hypotheses of loss of amino acid biosynthesis genes associated with obligate symbioses reported in siboglinid annelids are mistaken, and that Alvinella and siboglinids are typical metazoans in this regard. Alvinella encodes a number of respiratory enzymes unusual for bilaterian animals, suggesting an ability to better tolerate hypoxic environments. We find evidence of a parallel increase in the number of globin encoding genes and loss of light sensitive opsins and cryptochromes in deep-sea annelids. Conclusions Our results provide a comprehensive Alvinella protein and genome resource and shed light on the adaptation of Alvinella to temperature, hypoxia and darkness, as well as cryptic speciation, giving a firm base from which future studies can be taken forward.

    SpringerLink