Stars

The Star That Exploded Without Hydrogen

By Mark Thompson - July 31, 2026

Twenty five years ago a star in the constellation Puppis blew itself apart and then vanished behind a curtain of its own soot. Astronomers knew only that the explosion contained no hydrogen at all, which for the most abundant element in the universe is a very strange absence. Now the dust has finally thinned, and the culprits have stepped into view, a white dwarf quietly stripping a rare helium star of its substance. But the emerging picture came with something nobody expected, clumps of gas tearing outwards at twenty million miles an hour, of a kind never seen in any other nova. Nobody yet knows what fired them.

It Took a Century, but Astronomers Imaged Betelgeuse's Companion

By Carolyn Collins Petersen - July 31, 2026

Most of us are familiar with Betelgeuse (also known as alpha Orionis), the bright shoulder star in the constellation Orion. It's a red supergiant star that lies somewhere between 400 and 550 light-years away from us and is quite bright. Betelgeuse contains about 14 times the mass of the Sun and is a fairly young star compared to ours. It appears to be no more than 10 million years old, which means that it evolved rapidly from a protostar to the red giant we see today. That lifecycle means Betelgeuse will explode as a supernova sometime in the relatively near future — say within the next 100,000 years.

White Dwarfs Eat More Planetary Debris Than Thought, But Magnetic Fields Hide It

By Evan Gough - July 29, 2026

Planetary debris disks around white dwarfs appear to be more plentiful than thought. That's because some white dwarfs are magnetic, and those magnetic fields create patches of metallic debris near the stars' poles, where it's more difficult to detect. This leads to an underestimation of debris, something new research is trying to correct.

Meet Our Newest Stellar Neighbours That Hid in the Glare of Other Stars

By Evan Gough - July 20, 2026

Astronomers have found four new white dwarfs within about 65 light years. Even though the sky has been studied thoroughly, these escaped detection. That's because they're tight binaries with red dwarf partners, and the much brighter red dwarfs hide the white dwarfs. The binaries used to share common envelopes.

The Case of the Sun's Missing Silver

By Mark Thompson - July 20, 2026

Astronomers have solved a decades old puzzle about the Sun's missing silver, not by finding something new, but by modelling something old far more accurately. A revised, more realistic model of the Sun's atmosphere reveals it actually contains 55 per cent more silver than previously calculated, finally matching what meteorites have been telling us all along. It's a quiet reminder that some of the biggest revelations in astronomy come not from new data, but from asking familiar questions with sharper tools.

The Dark Energy Camera's New Image is Reminiscent of van Gogh

By Evan Gough - July 17, 2026

The Dark Energy Camera (DECam) has a massive 570 megapixel camera, and its new image is of the Corona Australis Molecular Cloud. Corona Australis is one of the closest star-forming regions to Earth. It's not as well-studied as the Orion Molecular Cloud or Ophiuchus, but as DECam's new iage of Corona Australis shows, it's just as fascinating.

X-Ray Eyes Reveal the Magnetic Secrets of the Lighthouse Pulsar's Cosmic Wake

By Andy Tomaswick - July 17, 2026

Occasionally, when a massive star dies in a supernova, it can leave behind a dense, rapidly spinning core known as a pulsar. These extreme objects are some of the most fascinating in the universe, and are extremely useful for astronomers when measuring distances or navigating the void of space. A new paper from Jack Dinsmore, a graduate student at Stanford, and his co-authors, and published in The Astrophysical Journal, takes a look at some of the features of one of the most famous examples of a pulsar - PSR J1101-6101, commonly known as the Lighthouse pulsar.

Listening for the Universe's Faintest Whispers, a Billion Supernovae at Once

By Mark Thompson - July 13, 2026

Buried a kilometre underground in Japan, one of the world's most sensitive detectors may have caught its first faint trace of a sound scientists have been straining to hear for decades, the combined whisper of every supernova that has ever exploded across the universe. It is not yet a confirmed discovery, but if it holds up, it could rewrite how we trace the life and death of stars.

Only Binary Stars Can Create Interacting Supernovae

By Evan Gough - July 10, 2026

When a massive star reaches the end of its life, it explodes as a supernova that can light up the sky for months. But some supernovae stay luminous for much longer, and astrophysicists have wondered what causes their extended brightness. New research points to binary stars, where one star expels material right before the explosion that creates a cocoon of circumstellar medium.

To Ancient Astronomers, Theta Eridani Was Brighter For A Thousand Years. Now We Know Why

By Evan Gough - July 09, 2026

Ptolemy and al-Sufi were keen ancient astronomers, one in Greece and one in Persia, whose observations were separated by almost a thousand years. They both noted that the star Theta Eridani was far brighter than it is today. Now we know why.

A Star’s Death Throes Involves a Lot of Kicking

By Mark Thompson - July 01, 2026

When stars like the Sun reach the end of their lives, the textbook story has them puffing up and quietly shedding their outer layers to leave a white dwarf behind. A new model suggests it is far less serene than that. As dying stars eject mass asymmetrically, each burst delivers a tiny recoil, and over hundreds of thousands of years roughly ten thousand of these kicks add up to send the star drifting through space at a respectable speed. The idea neatly explains why wide binary star systems tend to fall apart once one star becomes a white dwarf, and it hints at something more dramatic still waiting to be confirmed

An Island of Calm at the Violent Heart of the Galaxy

By Mark Thompson - June 29, 2026

The centre of the Milky Way is one of the most violent places in the Galaxy, a churning storm of gas moving faster than sound, and about the last spot you would expect a star to be born. Yet astronomers mapping that chaos with the ALMA telescope have stumbled on a hidden pocket of calm, where the gas slows, settles and quietly begins gathering itself into the seeds of new stars. The find suggests stars may take their first steps the same way everywhere, even here, and that our own Sun was likely born from just such an island of stillness, billions of years ago.

Feedback from Young Stars Influences Galaxy Evolution

By Carolyn Collins Petersen - June 29, 2026

Star formation is a major driver in galaxy evolution, right up there with the collisions and mergers that shape all galaxies. Researchers led by Ohio State University graduate student Debosmita Pathak, studied 18,000 star-forming regions in nearby spiral galaxies to get a better handle on the influence of starbirth.

Magnetic Fields Channel Gas Through Filaments into Star Formation Sites

By Evan Gough - June 25, 2026

Stars form inside molecular clouds where cold gas collapses gravitationally on itself. But there's more to this process than gravity. New research shows how magnetic field lines funnel gas through sub-filaments into star formation sites.

The Universe's First Stars Were Shaped By Turbulence and Were Not As Massive as Thought

By Evan Gough - June 25, 2026

For a long time, astrophysicists thought that the Universe's first stars, called Population III stars, were uniformly massive. It seemed like the conditions they formed in were calm and serene, which favoured massive stars. But new research based on high-resolution simulations show that conditions were more chaotic than thought, and gas cloud turbulence means that Population III stars were not all massive. This affected the metallicity of the next stars to form.

A Star Dying by the Wrong Rules

By Mark Thompson - June 25, 2026

Half the stars in the universe live in pairs and when one of them dies it can feed hungrily off the other in a slow, violent dance. Now a Korean team has caught a couple of stars breaking the rules, locked in an orbit so impossibly fast that our best theories of how stars grow old cannot account for it. So what is this dying star trying to tell us?

Astronomers Find Stellar Evidence of an Engulfed Planet

By Carolyn Collins Petersen - June 25, 2026

A team of 14 researchers from the United States and Chile have found evidence of a subgiant star eating one of its planets. The star, called TOI-5882, was already known to astronomers because of its massive companion, a brown dwarf called TOI-5882 b. The companion may well have helped kick a planet onto a spiraling journey into the star.

This is the First Pair of Sibling Supernova Remnants

By Evan Gough - June 23, 2026

Astrophysicists have found what is likely the very first pair of sibling supernova remnants. One is the well-known Jellyfish Nebula, and the other was long thought to be hidden in the bright glare from the Jellyfish. The pair are connected by a bright filament of gas.

FAST Finds a Pulsar in an Almost Flawless Circular Orbit

By Mark Thompson - June 15, 2026

Somewhere in the plane of the Milky Way, a dead star is spinning 220 times a second, and it's circling its companion in almost the most perfect orbit astronomers have ever measured. China's giant FAST radio telescope has just found it, and the shape of that orbit is a near flawless record of a billion year relationship between two stars.

Where Not to Look in the Search for ET

By Mark Thompson - June 10, 2026

When we scan the skies for signs of alien civilisations, where exactly should we be looking and perhaps more importantly, where should we not? A high school student from Ankara has just published a remarkably sophisticated answer to that question, building a filtering system that sifts nearly 1.75 million stars and identifies which ones are genuinely worth our attention. The result is a publicly available catalogue that could transform how the search for extraterrestrial intelligence allocates its most precious resource - time.

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