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Dust clouds glow around the aging star R Doradus as it sheds its outer layers. Astronomers once thought starlight reflecting off this dust could drive the star’s powerful wind, but the colors reveal the grains are too small to do the job. This polarized-light image was captured by VLT/SPHERE, with ALMA’s view of the star’s surface shown at the center in yellow and orange.

Dying Stars Lose Mass Through a Mechanism Scientists Can’t Explain

supermassive black hole at the center of the galaxy Messier 87

Scientists Will Track Black Holes in Motion for the First Time

Quantum detective Christina Giarmatzi

Quantum Computers Can’t Forget Their Errors, And That’s Derailing Progress

chaotic mess of wires

AI Cracks the Hidden Order Inside Chaotic Systems

Illustration of circadian clocks in a cell

Cell Membranes Generate Their Own Electricity From Molecular Restlessness

An illustration of a Jupiter mass planet migrating through a protoplanetary disk

30 Hot Jupiters Reveal They Skipped the Violent Route Inward

A new approach developed by MIT CSAIL researchers uses an LLM to plan how to answer complex reasoning tasks, then divides the legwork of that strategy among smaller language models. Their method helps LMs provide more accurate responses than leading LLMs and approach the precision of top reasoning systems, while being more efficient than both.

Small Models, Big Rules: A New Way To Make AI Behave

digital illustration of ones and zeroes

Engineers Remove Analog Bottleneck From Next-Gen Probabilistic Computing

supernova illustration

Webb Captures Universe’s Earliest Star Death And It Looks Familiar

An artist’s concept of a supermassive black hole surrounded by an accretion disk.

Black Holes Get X-Rayed: New ‘Arithmetic’ Decodes How Explosions Rule Galaxy Groups

Figure 3. Participant vocal fold lesions following scream (courtesy of authors).

The Biomechanics of a Scream: Why an Angry Yell Can Hurt Your Voice

Artist's rendition of GRB 250702B's ultra-relativistic jet (moving at nearly the speed of light) escaping from its dusty, massive host galaxy.

An Unruly Cosmic Blast Defies All Models

An illustration depicting the newly discovered cosmic structure: a long, thin cosmic filament composed of galaxies (center, a "thread of pearls") embedded within a colossal field of dark matter that exhibits coherent bulk rotation (the colorful outer rings). The image highlights the dual motion—galaxies spinning within a spinning filament—which challenges current models of how angular momentum flows through the cosmic web.

Astronomers Spot Gigantic Rotating Galaxy Filament

Images of Nova Herculis 2021 (V1674 Her) taken with the CHARA Array, two and three days after the eruption began. The images show two outflows expanding in nearly perpendicular directions, forming an hourglass-like structure consistent with theoretical predictions (illustrated in the rightmost artistic impression).

Real-Time Images Of Exploding Stars Defy Simple Theories

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