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Canadian telescope directly maps earliest glow of hydrogen, opening a new window on the universe

Researchers at the Canadian Hydrogen Intensity Mapping Experiment (CHIME) have successfully mapped the earliest glow of hydrogen gas from deep in the universe's past using only its own data. This breakthrough enables a faster, less expensive method for studying dark energy, a mysterious force driving the universe's expansion.

SourceUniversity of British Columbia·JournalThe Astrophysical Journal·DateSep 28, 2026

Time’s running out to catch giant planet’s strange orbit

Researchers at the University of Tokyo have discovered a rare, hot Jupiter with an eccentric orbit that provides a unique opportunity to study this class of planet. The planet, TOI-1355 b, orbits its star in just two Earth days and will soon disappear from view due to its rapidly changing orbit.

SourceUniversity of Tokyo·JournalPublications of the Astronomical Society of Japan·TypeObservational study·DateSep 18, 2026

'Born-again' star offers rare chance to watch stellar evolution in real time

Astronomers have confirmed that Sakurai's Object, a 'born-again' star, has entered a new phase of its evolution, developing a powerful stellar wind characteristic of Wolf-Rayet stars. The research provides new insight into the final stages of stellar evolution, allowing scientists to test theories that would otherwise take thousands of...

SourceUniversity of Manchester·JournalMonthly Notices of the Royal Astronomical Society·DateSep 16, 2026

Researchers have uncovered a growing black hole heading toward a merger in the early universe

A team of researchers has discovered four sets of dual 'Little Red Dots' (LRDs) in the early universe, indicating a possible link between galaxy mergers and rapidly growing black holes. The findings suggest that black hole mergers could be responsible for the rapid growth of black holes in the early universe.

SourceKavli Institute for the Physics and Mathematics of the Universe·JournalPublications of the Astronomical Society of Japan·DateAug 31, 2026

New chemical clues shine a light on galactic evolution

Researchers used computational modeling to simulate how electrons interact with manganese ions, predicting emission lines that could be useful for analyzing rapidly expanding objects like supernova remnants. The findings suggest that these emission lines could provide insight into the chemical evolution of galaxies, stars, and the univ...

SourceOhio State University·JournalMonthly Notices of the Royal Astronomical Society·DateAug 31, 2026

Venus’s mysterious clouds may hide an exceptionally strong light absorber

Researchers have estimated that the unknown absorber in Venus's clouds must absorb light very efficiently, occur at a high concentration, or both, with a required decadic absorption coefficient reaching approximately 1,278 cm-1 at 375 nm. This suggests that highly absorbing conjugated organic molecules could be the culprit, but the stu...

SourceInstitute for Basic Science·JournalAstrobiology·TypeObservational study·DateAug 27, 2026

A stellar envelope near the black hole Sgr A* contains water

Astronomers have discovered water molecules in the envelope of star IRS 3, located near the supermassive black hole Sgr A*. The star's enormous envelope, fueled by rapid mass loss, has allowed water to thrive in its vicinity. This finding suggests that Sgr A* is being enriched with fundamental building blocks of life.

SourceUniversity of Cologne·JournalAstronomy and Astrophysics·TypeObservational study·DateAug 11, 2026

The Sun contains more silver than previously estimated

Researchers at Uppsala University recalculated the Sun's silver content using a new model that predicts 55% more silver than previous estimates. This resolves a long-standing problem of missing silver in the solar system and improves our understanding of how elements are produced in stars and incorporated into planets.

SourceUppsala University·JournalAstronomy and Astrophysics·TypeComputational simulation/modeling·DateJul 17, 2026

Capturing the cosmic ‘drift’ before a star is born

A team of researchers from Kyushu University and Max Planck Institute for Extraterrestrial Physics have detected ambipolar diffusion in a prestellar core, weakening magnetic support and leading to gravitational collapse. This finding provides insight into early star formation and the creation of stellar systems like our own.

SourceKyushu University·JournalAstronomy and Astrophysics·TypeObservational study·DateJul 10, 2026

Can organic molecules survive a supernova explosion?

Researchers have discovered stellar cocoons rich in complex organic molecules within a supernova remnant, indicating that newborn stars can remain protected and preserve their molecular composition. The study suggests that the environment of our Solar System's formation may be more diverse than previously recognized.

SourceNiigata University·JournalThe Astrophysical Journal·DateJul 9, 2026

HKU-HKIAA astronomer joins international study to weigh inactive black hole seen 10 billion years ago

An international team of astronomers has directly measured the mass of an inactive supermassive black hole in the early Universe for the first time. The study found that the black hole is about 12 times more massive than expected from its host galaxy, suggesting that the central engine was already fully grown while the galaxy around it...

SourceThe University of Hong Kong·JournalScience·TypeObservational study·DateJul 7, 2026

XMM-Newton helps revise distance to outer spiral arms

The XMM-Newton and Chandra space telescopes have spotted the aftermath of three bright explosions echoing through the Milky Way's outer spiral arms. The team measured the distance to these echoes directly, finding two arms - Outer Scutum-Centaurus Arm and Outer Arm - lie up to 10% further away than previously thought.

SourceEuropean Space Agency·JournalAstronomy and Astrophysics·TypeObservational study·DateJul 1, 2026

Star light, star bright, baby stars blow rings alight

Researchers from Kyushu University used ALMA to observe a baby star producing a giant ring of gas about 1,000 au in size, which helps the star release excess energy. The team found that this ring is slightly warmer than its surroundings and hypothesize it's produced through magnetic field threading.

SourceKyushu University·JournalThe Astrophysical Journal Letters·TypeExperimental study·DateApr 2, 2026

The origin of the mysterious X-rays from Gamma Cas identified

Astronomers from the University of Liège have solved a 50-year-old stellar mystery by attributing the X-rays emitted by Gamma Cas to a magnetic white dwarf orbiting the star. The study used high-energy astrophysics instrumentation and revealed that the X-rays are associated with the compact companion, not the massive Be star itself.

SourceUniversity of Liège·JournalAstronomy and Astrophysics·DateMar 24, 2026

Study: New explanation for unique ‘negative superhump’ features of deep-space binary star systems

A team of astrophysicists offers a new explanation for negative superhumps in cataclysmic variable star systems, proposing an eccentric accretion disk model. This theory explains the prevalence of negative superhumps across a wide range of binary star masses and may also explain positive superhumps in high mass ratio systems.

SourceUniversity of Nevada, Las Vegas·JournalThe Astrophysical Journal Letters·TypeObservational study·DateMar 23, 2026

New map of the Milky Way’s magnetism offers insights into cosmic evolution

Researchers have created the first broadband map of Faraday rotation, revealing a complex magnetic field in the Milky Way. The dataset, DRAGONS, captures polarized radio emissions across a wide range of frequencies, allowing astronomers to see magnetic structures invisible before.

SourceUniversity of British Columbia Okanagan campus·JournalThe Astrophysical Journal Supplement Series·TypeObservational study·DateJan 29, 2026

Stardust study resets how life’s atoms spread through space

A team of astronomers has discovered that the winds of giant stars like R Doradus are driven by complex processes, rather than being powered solely by starlight and stardust. The study used advanced computer simulations to model how starlight interacts with dust grains, finding that they are too small to be pushed outward by starlight ...

SourceChalmers University of Technology·JournalAstronomy and Astrophysics·TypeObservational study·DateDec 22, 2025

Rare image of Tatooine-like planet is closest to its twin stars yet

Astronomers at Northwestern University have directly imaged a Tatooine-like exoplanet orbiting two suns, revealing unique insights into how planets form around multiple stars. The discovery provides an unprecedented look at the complex dynamics of binary systems and offers new opportunities to test theories of planet formation.

SourceNorthwestern University·JournalThe Astrophysical Journal Letters·TypeObservational study·DateDec 11, 2025

Einstein’s theory comes wrapped up with a bow: astronomers spot star “wobbling” around black hole

Scientists have observed a swirling vortex in spacetime caused by a rapidly rotating black hole, confirming predictions made by Einstein more than a century ago. The team detected rhythmic changes in X-ray and radio signals from the event, showing that the disk and jet were wobbling in unison every 20 days.

SourceCardiff University·JournalScience Advances·TypeObservational study·DateDec 10, 2025

Flaring black hole whips up ultra-fast winds

Astronomers discovered a never-seen-before blast from a supermassive black hole, whipping up powerful winds at 60,000 km per second. The event was triggered by an X-ray flare and formed in just one day, providing new insights into the magnetism of active galactic nuclei (AGNs).

SourceEuropean Space Agency·JournalAstronomy and Astrophysics·TypeObservational study·DateDec 9, 2025