Research-driven reporting on space technology and exploration developments
A team from the Center for Astrobiology (CAB) and CSIC‑INTA used JWST’s infrared spectrographs to examine the heavily dust‑obscured nucleus of a nearby ultra‑luminous infrared galaxy. The observations revealed an unprecedented variety of small organic molecules, including alcohols, nitriles and carbon chains, in quantities comparable to those in local star‑forming clouds. Modeling work from the University of Oxford translated the spectral signatures into precise abundances, confirming that complex chemistry thrives in extreme galactic environments. These results showcase JWST’s power to uncover hidden molecular richness beyond the Milky Way.
The Amaterasu particle, detected in 2021 by the Telescope Array, is the second‑highest‑energy cosmic ray ever recorded, packing roughly 40 million times the energy of LHC particles. A new study in The Astrophysical Journal argues that its origin is more likely...
A new Crew‑12 team—Jessica Meir, Jack Hathaway, Sophie Adenot and Andrey Fedyaev—will launch to the International Space Station on Feb 11 after the unprecedented medical evacuation of Crew‑11. The launch faces added uncertainty as SpaceX temporarily grounds Falcon 9 flights to investigate...
The International Space Station will be de‑orbited in 2030 using a SpaceX‑built vehicle, ending a three‑decade era of continuous human presence in low‑Earth orbit. Launched after the Cold War, the ISS became a flagship of U.S.–Russia cooperation despite recent geopolitical...
A supermassive black hole identified as AT2018hyz, nicknamed “Jetty McJetface,” has been emitting a radio jet that is 50 times brighter than when first detected in 2019. Over the past four years the jet’s radio flux has risen exponentially and is...
A joint analysis of NASA's TESS optical data and Swift BAT hard‑X‑ray monitoring identified quasi‑periodic oscillations (QPOs) in several blazars. Out of 38 variable objects, four showed highly significant periodicity with cycles of five to ten days, and one signal...
An international team using JWST discovered a massive, quiescent red galaxy at redshift 3.25, dubbed the “Red Potato.” The galaxy, MQN01 J004131.9‑493704, has a stellar mass of 110 billion M☉, a half‑light radius of 3,260 light‑years, and a low molecular‑gas fraction (<0.06)....
A new study in Reproductive Biomedicine Online warns that space’s radiation, microgravity and circadian disruption create a hostile environment for human reproduction. It highlights the absence of industry‑wide standards for managing fertility risks, early pregnancy, and ethical dilemmas as commercial...
University of Colorado Boulder has launched an inductively coupled plasma tunnel that reproduces the extreme heat and velocity of spacecraft re‑entry. The facility can generate plasma flows up to 9,000 °F and accelerate gases at thousands of miles per hour, matching...
An international team used the James Webb Space Telescope to directly detect three faint infrared H₂ emission lines in the dark molecular cloud Barnard 68, marking the first observational confirmation of cosmic‑ray‑excited gas. The measurements provide a direct estimate of the...
Physicists at UMass Amherst propose that a quasi‑extremal primordial black hole (PBH) can undergo a runaway Hawking‑radiation explosion, releasing ultra‑high‑energy particles. Their model explains the PeV‑scale neutrino detected by the KM3NeT collaboration in 2023, an event far beyond any known...
Astronomers using JWST’s NIRSpec have identified a new dwarf galaxy, CAPERS‑39810, at redshift 3.654. Spectroscopic analysis shows it has an extremely low metallicity of –1.96 dex, placing it among the rare class of extremely metal‑poor galaxies (EMPGs). The galaxy’s stellar mass is...
A new study combining lunar‑cratering ejecta models with long‑term orbital simulations estimates that roughly 500,000 lunar‑origin asteroids larger than about 5 m exist today, representing less than 1 % of comparable near‑Earth objects. The Vera C. Rubin Observatory’s Legacy Survey of Space...
Astronomers using NASA's TESS have confirmed a new exoplanet, TOI-6692 b, that rivals Jupiter in size but orbits its Sun‑like star every 130 days on a highly eccentric path. The planet was first flagged by citizen scientists as a single‑transit event and...
Physicists led by Mengnan Wang at the University of Edinburgh used high‑pressure experiments combined with optical spectroscopy to map solid methane’s phase behavior up to 45 GPa and 1,100 K. Their work produced two distinct phase diagrams—one reflecting kinetic transformations and another...
A recent paper in Physics Letters B proposes that Newton’s constant may run in the infrared, altering gravity’s strength over galactic distances. The author derives a logarithmic correction to the gravitational potential, producing an effective 1/r force that naturally yields flat...
Scientists have produced the first three‑dimensional map of the Sun’s interior magnetic field using data from multiple space‑based observatories. Published in The Astrophysical Journal Letters, the model reveals the hidden magnetic architecture that drives solar activity. The breakthrough promises more...
Physicists at UC Berkeley and the American University of Beirut have shown that general‑relativistic precession in tight binary stars can resonantly amplify a circumbinary planet’s eccentricity, leading to tidal disruption or ejection. Kepler and TESS have identified only 14 confirmed...
Leonardos Gkouvelis of LMU has delivered the first closed‑form analytical theory for transmission spectroscopy that incorporates pressure‑dependent opacity, a problem that has stymied exoplanet atmosphere modeling for decades. The new formula replaces costly numerical simulations with a transparent, fast solution,...
Astronomers using the James Webb Space Telescope have identified a compact five‑galaxy merger, dubbed JWST’s Quintet, at redshift 6.71—only about 800 million years after the Big Bang. The system spans tens of thousands of light‑years yet forms stars at roughly 250 solar masses...
Researchers at the Indian Institute of Science examined how perchlorate, a toxic chemical in Martian regolith, influences biocementation by a robust native strain of Sporosarcina pasteurii. While perchlorate slows bacterial growth, it triggers extracellular matrix formation that creates microbridges, resulting...
NASA and ISRO’s NISAR satellite used its L‑band synthetic aperture radar to capture a cloud‑free image of the Mississippi River Delta on Nov. 29, 2025. The radar’s 24‑centimeter wavelength penetrates clouds, revealing land‑cover details from urban structures to wetlands and crops. The...
NASA’s Goddard team leveraged the Pleiades supercomputer to run over 100 high‑resolution simulations of two 1.4‑solar‑mass neutron stars merging. The models reveal how tangled magnetospheres reconnect and generate rapidly varying electromagnetic emission in the final 7.7 ms before coalescence. Emission intensity...
A UBC Okanagan‑led team released the first broadband Faraday‑rotation map of the northern sky, called DRAGONS, using the DRAO 15‑meter telescope. The survey reveals that more than half of the sky exhibits intricate magnetic structures, overturning the notion of a largely...
A new study in New Phytologist reveals that tree species record radiocarbon spikes from extreme solar storms—known as Miyake events—differently due to variations in carbon uptake, storage, and allocation. These biological nuances can shift the timing and intensity of the...
Northwestern University researchers have demonstrated a novel laboratory search for ultralight dark‑matter particles using two Fabry‑Perot optical cavities of different lengths. By exploiting the pendulum‑like response of rigid cavities in the 34‑64 kHz band, the experiment can detect minute length oscillations...
Astronomers used ESA’s Gaia Data Release 3 to conduct a detailed analysis of three Milky Way open clusters—Berkeley 17, 18 and 39—identifying 600, 1,042 and 907 probable members respectively. The study reports ages ranging from 3.4 billion to 9.1 billion years, stellar masses from 536 M☉ to...
Researchers from ICCUB, IEEC and IAC published the most extensive observational study of massive runaway O‑type stars in the Milky Way. Using Gaia astrometry and IACOB spectroscopy, they examined 214 O‑type runaways, measuring rotation speeds and binarity. The analysis shows...
An international team led by Cyril Tasse and Cornell’s Jake Turner introduced Multiplexed Interferometric Radio Spectroscopy (RIMS), a method that mines existing low‑frequency radio archives to reveal minute‑by‑minute variability of hundreds of stars simultaneously. Applying RIMS to over 1.4 years of LOFAR LoTSS...
A joint University of Hong Kong‑UCLA study published in Nature Communications identifies Alfvén waves as the primary energy source that drives Earth’s auroral displays. By analyzing particle trajectories and electric fields, the researchers showed that these plasma waves continuously feed...
Researchers conducted a multi‑wavelength campaign on the accreting millisecond X‑ray pulsar MAXI J1957+032, covering its 2022 and 2025 outbursts and quiescent intervals. Timing analysis revealed a 3.19 ms spin period, ~1.01 h orbital period, a spin‑down rate of –0.0573 pHz s⁻¹ and a dipolar magnetic...
NASA’s Artemis II mission, slated for a February 2026 launch, will send a four‑person crew on a lunar flyby without landing. The flight tests life‑support, navigation and deep‑space operations that are essential for the planned Artemis III landing in 2028. Unlike the Cold‑War...
Researchers from the University of Groningen and European partners have used constrained cosmological simulations to reveal that the Milky Way and Andromeda reside within a large‑scale, flat sheet of dark matter extending tens of millions of light‑years. This planar mass...
WOH G64, one of the Large Magellanic Cloud's most luminous red supergiants, has been confirmed to remain in the red‑supergiant phase despite recent dimming and spectral changes. High‑resolution SALT spectra revealed titanium‑oxide absorption bands, a definitive sign of a cool photosphere,...
Using ALMA’s full‑polarization capabilities, astronomers mapped the magnetic fields of the merging ultraluminous infrared galaxy Arp 220 and uncovered a magnetized, high‑speed molecular outflow that functions as a “magnetic superhighway.” The study reports the first polarized CO(3‑2) detection, revealing field strengths...
A team led by Dr. Valentin Bickel used deep‑learning to catalog roughly 400 bright slope streaks—known as lineae—across Mercury’s surface, creating the first systematic inventory of these features. Geostatistical analysis shows the streaks concentrate on sun‑facing crater walls and are...
Astronomers have recorded the first radio emission from a Type Ibn supernova (SN 2023fyq) using the VLA, revealing the star's mass‑loss history in the decade before its explosion. The radio waves, observed over 18 months, show interaction with helium‑rich gas shed shortly before...
NASA and GE Aerospace successfully completed the first integrated hybrid‑electric jet engine test in December at GE’s Peebles Test Operation in Ohio. The demonstration used a modified GE Passport engine that extracts energy and feeds it back through electric motors,...
NASA's Perseverance rover has identified wave‑formed beach deposits and carbonate‑altered rocks in the Margin unit of Jezero crater, confirming an ancient shoreline dating back roughly 3.5 billion years. The study shows that igneous rocks were later transformed by subsurface, CO₂‑rich water,...
New theoretical work by Colin McInnes at the University of Glasgow shows that both stellar engines and Dyson bubbles—hypothetical alien megastructures designed to harvest a star’s energy—can achieve passive gravitational stability under specific conditions. The study, published in Monthly Notices of...