![Deep-sea microbial sample processing. Detailed sample processing steps for HPG assimilating cells and total cell counts are denoted in grey and black arrows/squares, respectively. Processing steps and samples used for metagenomic sequencing are denoted in light-blue arrows and squares. “Whole sample” correspond to triplicate 50 ml aliquots, each filtered onto a 0.22 μm filter directly from the cryopreserved material, and then released with 200 μl of 0.025% (v/v) Tween 20 in PBS to be processed through MDA and DNA sequencing; “all cells” correspond to samples of cryopreserved material that were stained with a DNA dye, collected on a 0.22 μm filter, processed through the BONCAT labelling assay, and then sorted by flow cytometry, aiming to select events that presented the DNA dye; “BONCAT+” cell samples originated from the same material as ‘all cells’, but their sorting aimed for events that presented both the DNA dye and the fluorescent dye Alexa-Fluor 488 (attached to the HPG incorporated by the active cells). The selection of BONCAT+ cells was established for each sample based on the level of BONCAT background labelling to the microbial community when not exposed to HPG, or when fixed before being exposed to HPG (i.e. reflecting the adhesion of the fluorescent label to cells that did not incorporate HPG). -- [ISME Journal via PubMed]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Sample-Return.png?resize=1200%2C719&ssl=1)
[ISME Journal via PubMed] The deep ocean hosts autochthonous pressure-adapted microorganisms that are unique to this environment, as well as allochthonous pressure-sensitive members transported from shallow depths by vertical advection […]
Biochemistry & Organic Chemistry
![A schematic showing the key abitoic (black dashed boxes) and biotic (white dashed box) processes occurring in the model (reproduced from Nicholson et al. 2022). -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/A-generalised-microbial.png?resize=1200%2C719&ssl=1)
Posted inBiosignatures & Paleobiology
A Generalised Microbial Cell Model For Methane Biosignature Predictions
[astro-ph.EP] The majority of potentially habitable planets detected to date are likely quite different to Earth, for example, being larger in radius and mass, differing rotation rates and with host […]
![Microscopic Image of Organic Ice Mixture captured from the O-PTIR high resolution microscope. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Detection-of-Organics.png?resize=1200%2C720&ssl=1)
Posted inAstrochemistry
Detection of Organics in Water Ice by Optical-PhotoThermal Infrared Spectroscopy
[astro-ph.IM] The detection and characterization of organic molecules within water ice is vital for interpreting observations of icy moons and comets. However, organic-ice interactions often distort intrinsic water-ice absorption features, […]
![Potential environments for the origin of life and the corresponding roles of minerals. (a) In the deep-sea hydrothermal vent hypothesis, metal sulfides play a critical role in the formation of chemical precursors and building blocks. (b) In terrestrial hot spring, minerals may concentrate and stabilize molecular building blocks, catalyze polymerization under wet–dry cycling conditions, and provide protection against environmental stresses. (c) Extraterrestrial input of organic matter through meteorites, comets and IDPs. Minerals are the carrier and preserver of organic compounds and may possibly take part in the prebiotic synthesis of organic compounds in extraterrestrial environments. (Background images are modified based on AI-generated illustrations.) -- [Fundamental Research]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/The-role-of-minerals.png?resize=1200%2C717&ssl=1)
Posted inOrigin & Evolution of Life
The Role Of Minerals In Prebiotic Evolution: Implications For Identifying Worlds With The Potential For Life’s Origin
[Fundamental Research] Understanding the origin of life requires explaining how abiotic molecules transitioned into the first living systems within plausible geological settings. Increasing evidence suggests minerals as active participants in […]
Posted inAstrochemistry
The Galactic Centre G+0.633-0.0604 Molecular Cloud: A New Astrochemical Gold Mine. I. Gas Physical Properties
[astro-ph.GA] In the Central Molecular Zone (CMZ), shocks play a key role in triggering star formation and driving chemical enrichment. The Sgr B2 complex is a prime template, hosting massive […]
Posted inAstrochemistry
Benzene Formation On Interstellar Dust Grain Analogues Via Single-Atom Fe Catalysis
[MRAS] Benzene has been detected across a range of astrophysical environments, though the primary mechanism underpinning its formation has not yet been constrained and the extreme conditions of the interstellar […]
![An artist's impression of the warm molecular gas cradle (hot core) surrounding a baby star discovered in a supernova remnant. Blue represents high-energy particles and photons produced by the supernova explosion, while brown represents interstellar matter. Credit: Takashi Shimonishi (Niigata University) [Based on observational results from this study, using drawing assistance from Google Gemini and ChatGPT]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Diverse-Organic.jpg?resize=1200%2C768&ssl=1)
Posted inAstrochemistry
Diverse Organic Molecules Discovered Surrounding A Newly Formed Star
[Niigata University] For the first time, astronomers have discovered stellar cocoons rich in complex organic molecules within a supernova remnant. A research team from Niigata University, Gifu University, RIKEN, and […]
Posted inAstrochemistry
Searching For The Elusive CH2+ With The James Webb Space Telescope. Another Carbocation To Constrain Astrochemical Networks
[astro-ph.GA] Carbocations are key species in interstellar chemistry, providing entry points for building larger hydrocarbons. CH+, and more recently, CH3+, have been detected. Other carbocations await detection to provide a […]
Posted inAstrochemistry
MINDS: Complementary Inclinations In The Binary Ssystem HK Tau Reveal Gas- And Ice-phase Chemistry
[astro-ph.EP] HK Tau is a roughly equal mass pre-main sequence binary system consisting of a low-inclination primary (57 deg) and an edge-on (83 deg) secondary. We present JWST/MIRI observations targeting […]
Posted inAstrochemistry
Dual Use Technology – An Astrochemistry Spin Off
Editor’s note: many of the tools that are used in astronomy to conduct analyses of chemistry in space – astrochemistry – utilize technology that has had long-standing applications in a […]