Supermassive Black Hole Winds Span 300,000 Light-Years

Schematic illustration of the hierarchical structure of the universe, from a galaxy group (a collection of galaxies) to an individual galaxy and the supermassive black hole at its center. Although a black hole is more than 100 million times smaller than the radius of its host galaxy, it plays a crucial role in the galaxy's central region.
Image Credit: © Tohoku University

Scientific Frontline: Extended "At a Glance" Summary: Quasar-Mode Feedback and Supermassive Black Hole Winds

The Core Concept: Supermassive black holes actively eject gas in the form of immensely powerful winds that drive massive turbulence, carrying explosive energy across distances of up to 300,000 light-years.

Key Distinction/Mechanism: While black holes are primarily known for consuming matter, they also function as violent ejectors of energy. By tracking the emission lines of iron ions in X-ray frequencies, researchers established that the turbulent dispersal of high-temperature gas driven by these winds is approximately 100 times more powerful than previously estimated.

Major Frameworks/Components:

• Supermassive Black Holes: The central, massive engines powering luminous quasars that consume gas while simultaneously ejecting highly energetic winds into the surrounding cluster.
• Quasar-Mode Feedback: The mechanical process by which an active galactic nucleus drives violent turbulence in surrounding high-temperature gas, preventing cooling and regulating both galactic and intergalactic environments.
• Iron Ion Emission Diagnostics: The use of specific X-ray emission lines from iron ions to precisely trace the velocity, spatial distribution, and dynamic motion of hot cosmic gas.
• High-Resolution X-ray Spectroscopy: The observational framework, facilitated by the XRISM satellite, required to capture the unprecedented scale and turbulent energy of extragalactic shock waves.

AI Discovers Rare Quasar Gravitational Lenses

Quasars have been found with luminosities between 10 to 100,000 times that of the Milky Way.
Image Credit: Scientific Frontline / stock image

Scientific Frontline: Extended "At a Glance" Summary: Quasar Gravitational Lenses

The Core Concept: Quasar gravitational lenses are rare, highly luminous active galactic nuclei powered by supermassive black holes that possess enough gravitational force to bend the light of other celestial objects located behind them.

Key Distinction/Mechanism: Finding quasars capable of acting as gravitational lenses is exceptionally difficult, as their extreme brightness typically obscures the host galaxy. To identify them, astronomers utilized a specialized neural network trained on simulated spectra—combining real quasar and background galaxy emission lines—to parse 800,000 potential quasar targets and isolate the subtle spectral signatures of lensing.

Major Frameworks/Components:

• Quasars: Distant, ultra-luminous galaxy cores driven by feeding supermassive black holes, often serving as developmental links in the early universe.
• Gravitational Lensing: A phenomenon where a massive object acts as a cosmic magnifying glass, bending the light of objects situated behind it due to strong gravity.
• Dark Energy Spectroscopic Instrument (DESI): A large-scale astronomical survey providing the massive dataset of 800,000 potential quasar spectra used for this analysis.
• Artificial Neural Networks: Machine learning architecture trained on mock lens systems to identify anomalous emission lines indicating a gravitational lensing event.

Missing Baryonic Matter Found Around Galaxies

Simulated gas distribution (blue, green, and yellow colors) around galaxies (white dots on the image). The study finds that gas in our Universe extends farther from galaxies than most simulations predict, indicating strong activity from galaxies that have expelled gas away from galaxy groups.
Image Credit: IllustrisTNG
(CC BY-NC-ND 3.0)

Scientific Frontline: Extended "At a Glance" Summary: Missing Baryonic Matter

The Core Concept: The universe's missing ordinary matter—unaccounted for in the mass of current stars and galaxies—exists in highly diffuse clouds or "puffs" of gas that extend up to four million light-years around galaxy groups.

Key Distinction/Mechanism: To detect matter with a density as low as one proton per cubic meter, researchers measure the dispersion, or "smearing," of fast radio bursts (FRBs). As these ultrabright radio waves travel through space, the missing matter delays lower-energy wavelengths, allowing astronomers to calculate the precise amount of gas the signal intersected.

Origin/History: The deficit of baryonic matter has been a recognized cosmic conflict for decades, with estimates showing that all observable stars and galaxies account for only a tenth of the ordinary matter produced shortly after the Big Bang. In July 2026, an MIT-led team within the CHIME/FRB Collaboration published a novel method utilizing FRBs (first discovered in 2007) to successfully map the shape and location of this missing mass.

Major Frameworks/Components:

• Baryonic Matter: Subatomic particles, including protons and neutrons, that make up ordinary, observable matter (distinct from invisible dark matter).
• Fast Radio Bursts (FRBs): Millisecond flashes of radio waves emitted by energetic phenomena in the distant universe, utilized here as cosmic probes.
• Galactic Fountains: The theoretical mechanism by which matter is violently expelled from a galaxy through black hole jets, star-forming activity, and exploding stars.
• Cross-Correlation Mapping: The analytical integration of radio signal detections from the Canadian Hydrogen Intensity Mapping Experiment (CHIME) with 3D galactic maps from the Dark Energy Spectroscopic Instrument (DESI).

Identifying the LHAASO J1912+1014u Proton PeVatron

Observation by NASA’s Fermi Gamma-ray Space Telescope identified GeV gamma-ray excess toward LHAASO J1912-1014u and confirm it to be a proton PeVatron through multiwavelength observations and modeling. The source is marked by a solid circle and is largely extended, with a diameter of more than 1 degree. For comparison, the size of the Moon is indicated by a dashed circle.
Image Credit: Adapted from Tsunefumi Mizuno, et al. Astrophysical Journal. July 16, 2026

Scientific Frontline: Extended "At a Glance" Summary: LHAASO J1912+1014u

The Core Concept: LHAASO J1912+1014u has been identified as a proton "PeVatron," an elusive celestial object capable of accelerating protons to energies reaching or exceeding one quadrillion (10^15) electron volts (PeV).

Key Distinction/Mechanism: Unlike electron accelerators, which are ruled out by the smooth, wide-range gamma-ray emission spectrum, this source demonstrates a hadronic origin supported by the correlation between gamma-ray data and interstellar gas distribution.

Major Frameworks/Components:

• Fermi Large Area Telescope (Fermi-LAT) gamma-ray data (GeV range).
• FUGIN radio telescope survey data tracing interstellar gas distribution.
• Chandra X-ray Observatory data confirming weak diffuse X-ray emissions.
• Large High Altitude Air Shower Observatory (LHAASO) and Tibet AS gamma experiment data (TeV range).

Little Red Dots and Cosmic Neutrinos

At the center of the Little Red Dot, there may be a black hole surrounded by a thick outer gaseous envelope. In this environment, photons produced near the center are absorbed and scattered by the gas, so neutrinos can escape the envelope without interacting with the surrounding gases. If there are many Little Red Dots, they may account for a part of the high-energy neutrinos arriving from the universe.
 Image Credit: KyotoU / Riku Kuze

Scientific Frontline: Extended "At a Glance" Summary: Little Red Dots as Hidden Neutrino Sources

The Core Concept: "Little Red Dots" are abundant, high-redshift, small red galaxies recently observed by the James Webb Space Telescope. Researchers hypothesize that these galaxies harbor growing supermassive black holes enveloped in dense gas, making them a primary candidate for the universe's mysterious all-sky high-energy neutrino background.

Key Distinction/Mechanism: High-energy neutrinos are produced when accelerated particles collide with surrounding matter or photons. Unlike typical high-energy neutrino sources, which also emit detectable gamma rays, the dense gaseous envelopes surrounding the black holes in Little Red Dots suppress gamma-ray emissions while allowing neutrinos to escape, thereby matching observed cosmic background levels.

Major Frameworks/Components:

• Supermassive Black Holes: Central celestial objects generating the extreme energetic forces required for particle collisions.
• Particle Acceleration: The mechanism by which protons and other particles achieve high velocities within buried jets, leading to the production of secondary particles.
• Gaseous Envelopes: Thick, dense layers of gas surrounding the central black hole that absorb scattered photons (gamma rays) while permitting electrically neutral neutrinos to escape.
• Neutrino Spectrum Analysis: Complex numerical modeling utilized to evaluate cooling processes, particle collisions, and the expected neutrino output from these distant galaxies.

Spacetime Crystals & Microscopic Black Holes

Left: visualization of a space-time-crystal. Right: a cubic crystal structure
Image Credit: Technische Universität Wien

Scientific Frontline: Extended "At a Glance" Summary: Spacetime Crystals and Microscopic Black Holes

The Core Concept: Researchers have developed an exact mathematical formula describing how arbitrarily small, microscopic black holes can spontaneously form from highly ordered, unstable states known as spacetime crystals.

Key Distinction/Mechanism: Unlike massive black holes formed by the collapse of dying stars, these microscopic black holes emerge through "critical collapse." Spacetime curvature temporarily organizes into a regular, repeating pattern (a spacetime crystal)—an intermediate state that either dissolves or, with the slightest addition of energy, collapses into a tiny black hole.

Origin/History: The possibility of spontaneous microscopic black hole formation was first observed in computer simulations in 1993. It was only recently confirmed analytically, using paper-and-pencil mathematics, by physicists at TU Wien and Goethe University Frankfurt.

A new way to read the Universe

Image Credit: Courtesy of University of Barcelona / CANVAS

Scientific Frontline: Extended "At a Glance" Summary: The CIGaRS Framework

The Core Concept: CIGaRS is an advanced computational framework that utilizes simulation-based inference to jointly analyze Type Ia supernovae and their host galaxies. It enables scientists to accurately extract cosmological data—such as distances and expansion rates—primarily through photometric imaging rather than requiring costly spectroscopic observations.

Key Distinction/Mechanism: Traditional methods analyze supernovae and environmental factors separately, relying on simple adjustments for host galaxy effects. CIGaRS links all elements—supernova explosions, host galaxies, cosmic dust, and universe expansion—into a single self-consistent physical and statistical model, utilizing neural networks to infer underlying physical parameters directly from vast datasets of real observations.

Major Frameworks/Components:

• Simulation-Based Inference: The generation of comprehensive, ab initio computer simulations of possible universes to train predictive models.
• Bayesian Inference: A statistical method used to vary all possible cosmic parameters simultaneously, allowing researchers to account for previously "unknown unknown" systematics.
• Neural Networks: Artificial intelligence trained on the simulated physics data to rapidly and accurately analyze tens of thousands of real supernova images simultaneously.
• Photometric Redshift Estimation: The ability to accurately estimate galaxy distances and cosmic expansion without the need for traditional spectra.

Dark matter could explain earliest supermassive black holes

Dark matter decays could be the missing ingredient explaining how giant black holes formed before the first stars
Image Credit: Scientific Frontline

Scientific Frontline: Extended "At a Glance" Summary: Decaying Dark Matter and Early Supermassive Black Holes

The Core Concept: The decay of dark matter particles in the early universe may have released sufficient energy to alter the chemistry of primordial gas clouds, causing them to collapse directly into supermassive black holes instead of forming stars.

Key Distinction/Mechanism: Standard astrophysical models suggest black holes form from the collapse of individual stars and grow slowly over time, a timeline that cannot account for the massive scale of the earliest known black holes. This new mechanism posits that decaying dark matter particles (specifically axions) inject trace amounts of energy into pristine hydrogen gas, supercharging the direct collapse rate without requiring the historically assumed, and statistically rare, presence of nearby stellar radiation.

Major Frameworks/Components:

• Direct Collapse Black Holes (DCBH): A theoretical pathway where massive clouds of primordial gas bypass the star-formation phase and collapse directly into a black hole.
• Axion Dark Matter Decay: A specific dark matter model utilizing particles with masses between 24 and 27 electronvolts, which release billion-trillionths of an energy unit upon decay.
• Thermo-Chemical Dynamics: The analysis of how microscopic energy injections from dark matter alter the thermodynamic evolution and cooling processes of pristine hydrogen gas.

New simulations reveal the cold, dusty reality of galaxy formation

Visual impression of the dynamic range in the high-resolution COLIBRE simulation L025m5 at redshift z = 0.1. The top left panel shows a projection of the entire simulation with the colour encoding baryon surface density. The other panels zoom into different regions and show the stellar light in HST colours accounting for attenuation by dust.
Hi-Res Zoomable Version
Image Credit: Schaye et al. (2026)

Scientific Frontline: Extended "At a Glance" Summary: COLIBRE Cosmological Simulations

The Core Concept: COLIBRE is a groundbreaking set of advanced cosmological simulations that models the evolution of galaxies by integrating cold interstellar gas and cosmic dust, offering the most realistic digital representation of galaxy formation from the early universe to the present day.

Key Distinction/Mechanism: Unlike previous large-scale models that were limited to simulating gas at temperatures of 10,000 Kelvin or higher, COLIBRE directly models the physical and chemical processes of cold gas and microscopic dust grains. Utilizing up to 20 times more resolution elements than earlier frameworks, it accurately reproduces complex real-world observations, including those captured by the James Webb Space Telescope (JWST).

Major Frameworks/Components: 

• Cold Interstellar Gas Modeling: Direct computational simulation of the low-temperature gas where actual stellar formation occurs, overcoming the computational limitations of previous high-temperature models.
• Cosmic Dust Integration: Simulation of dust grains that catalyze the formation of hydrogen molecules, shield gas from harsh ultraviolet radiation, and re-emit absorbed starlight as infrared energy.
• High-Resolution Supercomputing: Execution via the SWIFT simulation code on advanced supercomputer architecture, consuming up to 72 million CPU hours for the largest iterations to generate vast cosmic volumes with high statistical accuracy.
• Standard Cosmological Model Validation: Confirms that the standard theoretical framework of cosmology aligns with observational data once essential localized physical processes (like cold gas and dust) are properly represented.

The Local Universe’s Expansion Rate Is Clearer Than Ever, but Still Doesn’t Add Up

Artist’s interpretation of the cosmic distance ladder — a succession of overlapping methods used to measure distances across the Universe, where each rung of the ladder provides information that can be used to determine the distances at the next higher rung. Methods include observations of pulsating Cepheid variable stars, red giant stars that shine with a known brightness, Type Ia supernovae, and certain types of galaxies.  In this illustration, the distance ladder begins at the Coma Cluster, which is the nearest extremely rich galaxy cluster to us. The distance to the Coma Cluster can be measured directly using observations of Type Ia supernovae within the cluster. Type Ia supernovae have a predictable luminosity that makes them reliable objects for distance calculations. 
Image Credit: CTIO/NOIRLab/DOE/NSF/AURA/J. Pollard

Scientific Frontline: Extended "At a Glance" Summary: The Hubble Tension and the Local Distance Network

The Core Concept: The Hubble tension is a persistent, statistically significant discrepancy between the Universe's expansion rate measured in the local Universe and the rate predicted from the early Universe using the standard model of cosmology.

Key Distinction/Mechanism: Rather than relying on a single measurement method, this breakthrough framework unites decades of independent distance measurements into a unified "distance network." By cross-linking overlapping techniques—such as observing Cepheid variable stars, red giant stars, and Type Ia supernovae—astronomers achieved a local expansion rate of 73.50 ± 0.81 km/s/Mpc with roughly 1% precision. This multi-path approach effectively rules out single-method observational errors as the cause of the discrepancy with the early Universe prediction of 67–68 km/s/Mpc.

Major Frameworks/Components: 

• The Standard Model of Cosmology: The theoretical baseline used to predict the present-day expansion rate based on cosmic microwave background measurements.
• The Cosmic Distance Ladder/Network: An observational methodology utilizing multiple independent, overlapping distance indicators to measure the local Universe.
• H0 Distance Network (H0DN) Collaboration: An international, community-built framework synthesizing independent astrophysical measurements from both ground and space-based observatories, including the NSF NOIRLab programs.

Ghostly particles: Is dark radiation masquerading as neutrinos?

Bhupal Dev / Associate Professor of Physics
Photo Credit: Courtesy of Washington University in St. Louis

Scientific Frontline: Extended "At a Glance" Summary: Dark Radiation and Neutrino Cosmology

The Core Concept: During the earliest moments of the universe, a fraction of neutrinos may have transformed into a previously unknown form of fast-moving light radiation known as "dark radiation." This theoretical conversion offers a novel explanation for cosmological anomalies regarding how the universe evolved and expanded.

Key Distinction/Mechanism: While recent cosmological data suggested that neutrinos might interact with one another more strongly than predicted by the standard model, laboratory experiments place strict limits on such interactions. The newly proposed mechanism resolves this mismatch: rather than neutrinos interacting strongly, the presence of dark radiation mimics the cosmological effects of strongly interacting neutrinos without violating the constraints established by terrestrial physics experiments.

Origin/History: This theoretical framework was published on April 2, 2026, in Physical Review Letters by a research team led by Bhupal Dev at Washington University in St. Louis. The study posits that the transformation into dark radiation must have occurred in a specific chronological window: after Big Bang nucleosynthesis but before the formation of the cosmic microwave background.

Major Frameworks/Components: 

• The Standard Model of Particle Physics: The baseline theoretical framework that accurately predicts weak interactions of standard neutrinos.
• Big Bang Nucleosynthesis: The early universe process during which the first nuclei were formed, serving as the lower temporal bound for the dark radiation conversion.
• Cosmic Microwave Background (CMB): The remnant radiation from the early universe, serving as the upper temporal bound for when this conversion could have taken place.
• The Hubble Tension: The persistent discrepancy between different scientific measurements of the universe's expansion rate, which the dark radiation model attempts to reconcile.

'Space Archaeology' Reveals First Dynamic History of a Giant Spiral Galaxy

An artist's impression shows the giant spiral galaxy NGC 1365 as it collides and merges with a smaller companion galaxy, stirring up star formation and redistributing gas and heavy elements. Using a new "space archaeology" technique that reads the chemical fingerprints in the galaxy’s gas, astronomers have reconstructed how NGC 1365 grew over 12 billion years.
Image Credit: Melissa Weiss/CfA

Scientific Frontline: Extended "At a Glance" Summary: Extragalactic Archaeology and the Evolution of NGC 1365

The Core Concept: Extragalactic archaeology is a novel astronomical technique that reconstructs the multi-billion-year evolutionary history of distant galaxies by analyzing the detailed chemical fingerprints embedded in their gas and star-forming clouds.

Key Distinction/Mechanism: Unlike traditional observations that capture a static snapshot of a galaxy, this method maps the distribution of heavy elements (such as oxygen) across a galaxy's structure using high-resolution spectroscopy. These chemical patterns are then compared against state-of-the-art cosmological simulations to infer the galaxy's historical timeline, including past mergers, gas flows, and star formation rates over cosmic time.

Major Frameworks/Components:

• TYPHOON Survey: An observational initiative utilizing the Irénée du Pont telescope to achieve sharp resolutions of individual star-forming clouds, isolating specific diagnostic emission lines (like ionized hydrogen, nitrogen, and oxygen) across the galaxy's disk.
• Chemical Fingerprinting: The process of analyzing the light emitted by excited gases around young, hot stars to measure the concentration and distribution of heavy elements from the galactic center to the outer spiral arms.
• The Illustris Project: Advanced cosmological simulations that model the physical processes of the universe—such as gas motion, black hole activity, and chemical evolution—used to find a precise theoretical match to the observed data.

Cosmology: In-Depth Description

Cosmology is the scientific study of the origin, evolution, large-scale structures, and eventual fate of the universe as a whole. Its primary goal is to understand the universe in its totality—how it began (most notably through the Big Bang), how it has expanded and developed over billions of years, and the fundamental physical laws that govern its macroscopic behavior. Unlike astronomy, which often focuses on individual celestial objects like stars or galaxies, cosmology examines the universe as a singular, cohesive entity.

Supermassive black holes sit in ‘eye of their own storms,’ studies find

An artist’s rendition of the immediate vicinity around the supermassive black hole known as M87*. However, the roiling, superhot gases around these black holes extend much further than seen in this visualization. Two new studies give us new insight into the regions around these black holes and how they influence their surrounding galaxies.
Illustration Credit: S. Dagnello NRAO/AUI/NSF

Scientific Frontline: "At a Glance" Summary

• Main Discovery: A powerful, rotating magnetic wind has been identified encircling a supermassive black hole, acting as a feeding mechanism that enables the black hole’s growth rather than pushing material away.
• Methodology: Researchers utilized the Atacama Large Millimeter/submillimeter Array (ALMA) to detect and analyze specific light wavelengths from hydrogen cyanide (HCN) molecules, using the Doppler effect to trace the motion and structure of gas hidden behind thick dust layers.
• Key Data: The study focused on the galaxy ESO320-G030, located approximately 120 million light-years from Earth, revealing a wind structure that contradicts previous models of purely repulsive outflows.
• Significance: This discovery solves a persistent mystery in astrophysics regarding how supermassive black holes accrete mass efficiently, demonstrating that magnetic fields can create a "storm" that funnels matter inward rather than expelling it.
• Future Application: Astronomers intend to survey other active galaxies to determine if this magnetic wind phase is a universal stage in the lifecycle of all supermassive black holes.
• Branch of Science: Astrophysics and Cosmology
• Additional Detail: The observed process parallels the mechanics of star formation ("baby stars"), suggesting that similar physical laws govern growth across vastly different cosmic scales, from small suns to galactic monsters.

The infant universe’s “primordial soup” was actually soup

A quark zooms through quark-gluon plasma, creating a wake in the plasma. “Studying how quark wakes bounce back and forth will give us new insights on the quark-gluon plasma’s properties,” Yen-Jie Lee says.
Image Credit: Jose-Luis Olivares, MIT
(CC BY-NC-ND 4.0)

Scientific Frontline: "At a Glance" Summary

• Main Discovery: Researchers have observed the first direct evidence that the "primordial soup" of the early universe—quark-gluon plasma—behaves as a dense, frictionless liquid rather than a gas, indicated by the formation of wakes behind speeding quarks.
• Methodology: The team utilized data from the Compact Muon Solenoid (CMS) experiment at CERN's Large Hadron Collider, where heavy lead ions were smashed together at near-light speeds to briefly recreate the primordial plasma; they then analyzed the trajectories of quark-antiquark pairs to detect specific "sloshing" or wake patterns generated as particles moved through the medium.
• Key Data: The laboratory-created plasma droplets existed for less than a quadrillionth of a second and reached temperatures of several trillion degrees Celsius, mirroring conditions just a few millionths of a second after the Big Bang.
• Significance: This confirmation resolves a longstanding debate in physics, proving that the infant universe's matter functioned as a cohesive fluid that creates ripples and swirls (similar to a boat in water) rather than a system of randomly scattering individual particles.
• Future Application: The novel technique of using quark wakes as probes will allow physicists to measure the viscosity and internal properties of quark-gluon plasma with greater precision, effectively providing a detailed "snapshot" of the universe's earliest moments.
• Branch of Science: High-Energy Particle Physics / Cosmology
• Additional Detail: The study validates the theoretical "hybrid model" which predicted that high-energy jets (quarks) would induce a hydrodynamic response in the plasma, slowing down the particles and generating a detectable wake.

NASA Reveals New Details About Dark Matter’s Influence on the Universe

Created using data from NASAs Webb telescope in 2026 (right) and from the Hubble Space Telescope in 2007 (left), these images show the presence of dark matter in the same region of sky. Webb's higher resolution is providing new insights into how this invisible component influences the distribution of ordinary matter in the universe.
Image Credit:NASA/STScl/A Pagan

Scientific Frontline: Extended "At a Glance" Summary

The Core Concept: A highly detailed map of dark matter distribution created using data from the James Webb Space Telescope (JWST), revealing the invisible "scaffolding" that structures the universe.

Key Distinction/Mechanism: Unlike previous, blurrier maps, this new visualization is twice as sharp and provides empirical confirmation that dark matter and ordinary matter are tightly interlocked. It utilizes gravitational lensing—observing how dark matter's mass warps space and bends light from distant galaxies—to trace invisible structures with unprecedented precision.

Major Frameworks/Components:

• Gravitational Lensing: The primary method used to detect non-luminous dark matter by measuring how it distorts background light.
• Cosmic Evolution Survey (COSMOS): The specific region of the sky (in the constellation Sextans) observed for this study.
• Mid-Infrared Instrument (MIRI): A key JWST instrument used to measure galactic distances and penetrate cosmic dust.
• Matter Correlation: The study confirms a direct spatial overlap between "clumps" of dark matter and clusters of ordinary (baryonic) matter.

Branch of Science: Astrophysics, Cosmology.

Future Application: These detailed maps will help refine models of cosmic evolution, specifically clarifying how early dark matter structures accelerated the formation of the first stars and galaxies, thereby enabling the creation of planetary systems.

Why It Matters: It validates the theory that dark matter acts as the gravitational anchor for the visible universe. By proving that dark matter grew alongside ordinary matter, scientists can better understand the timeline of the universe's development, including the conditions that allowed for the emergence of planets like Earth.

Space Science: In-Depth Description

Image Credit: Scientific Frontline / AI generated (Gemini)

Space Science is the multifaceted scientific discipline dedicated to the exploration and study of natural phenomena and physical bodies occurring beyond Earth's atmosphere. Its primary goals are to understand the origins, evolution, and future of the Universe, to discover the fundamental physical laws governing the cosmos, and to explore the potential for life beyond our planet.

A speed camera for the universe

The stars (or rather galaxies) of the show.
A montage of eight time-delay gravitational lens systems. There’s an entire galaxy at the center of each image, and the bright points in rings around them are gravitationally lensed images of quasars behind the galaxy. These images are false-color and are composites of data from different telescopes and instruments.
Image Credit: ©2025 TDCOSMO Collaboration et al.
(CC BY-ND 4.0)

There is an important and unresolved tension in cosmology regarding the rate at which the universe is expanding, and resolving this could reveal new physics. Astronomers constantly seek new ways to measure this expansion in case there may be unknown errors in data from conventional markers such as supernovae. Recently, researchers including those from the University of Tokyo measured the expansion of the universe using novel techniques and new data from the latest telescopes. Their method exploits the way light from extremely distant objects takes multiple pathways to get to us. Differences in these pathways help improve models on what happens at the largest cosmological scales, including expansion.

After nearly 100 years, scientists may have detected dark matter

Gamma-ray image of the Milky Way halo (with details).
Gamma-ray intensity map excluding components other than the halo, spanning approximately 100 degrees in the direction of the Galactic center. The horizontal gray bar in the central region corresponds to the Galactic plane area, which was excluded from the analysis to avoid strong astrophysical radiation.
 Image Credit: ©2025 Tomonori Totani, The University of Tokyo

In the early 1930s, Swiss astronomer Fritz Zwicky observed galaxies in space moving faster than their mass should allow, prompting him to infer the presence of some invisible scaffolding — dark matter — holding the galaxies together. Nearly 100 years later, NASA’s Fermi Gamma-ray Space Telescope may have provided direct evidence of dark matter, allowing the invisible matter to be “seen” for the very first time.

Dark matter has remained largely a mystery since it was proposed so many years ago. Up to this point, scientists have only been able to indirectly observe dark matter through its effects on observable matter, such as its ability to generate enough gravitational force to hold galaxies together. The reason dark matter can’t be observed directly is because the particles that make up dark matter don’t interact with electromagnetic force — meaning dark matter doesn’t absorb, reflect or emit light.

X-Ray Study Reveals New Details About Betelgeuse’s Elusive Companion Star

Betelbuddy, the companion star to Betelgeuse. This image is a color composite made from exposures from the Digitized Sky Survey 2.
Image Credit: ESO/Digitized Sky Survey 2. Acknowledgment: Davide De Martin

Astronomers have long suspected that Betelgeuse — the bright red star blazing in Orion's shoulder — wasn't alone. Now, thanks to a fleeting cosmic window and swift action by Carnegie Mellon University researchers, the true nature of its elusive companion has been illuminated.

In a race against time, the CMU researchers secured director’s discretionary time on both NASA’s Chandra X-ray Observatory and the Hubble Space Telescope to investigate the long-predicted — but never detected — companion star to Betelgeuse. The timing was critical: Around Dec. 6, the companion, nicknamed “Betelbuddy,” reached its maximum separation from the massive red supergiant just before it would disappear behind it for two more years.

“It turns out that there had never been a good observation where Betelbuddy wasn't behind Betelgeuse,” said Anna O’Grady, a McWilliams Postdoctoral Fellow at Carnegie Mellon’s McWilliams Center for Cosmology and Astrophysics. “This represents the deepest X-ray observations of Betelgeuse to date.”