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Scientists observe distant jellyfish galaxy for first time

Astronomers from the University of Waterloo have observed a distant jellyfish galaxy, providing rare insight into how galaxies were transformed in the early universe. The discovery challenges previous beliefs about galaxy clusters and their impact on galaxy properties.

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The simulated Milky Way: 100 billion stars using 7 million CPU cores

Researchers at RIKEN successfully simulated the Milky Way Galaxy with over 100 billion individual stars, far surpassing previous state-of-the-art models. This achievement demonstrates the power of AI-accelerated simulations in tackling complex multi-scale problems in astrophysics and beyond.

‘Messy’ galaxies in the early universe struggled to settle

Researchers used the James Webb Space Telescope to study young galaxies in the early universe, finding most were turbulent and 'clumpy'. Despite this chaos, galaxy dynamics show a gradual transition towards ordered structures, suggesting that galaxies like our Milky Way formed through frequent mergers and bursts of star formation.

Hungry star is eating its cosmic twin at rate never seen before

Astronomers discovered a greedy white dwarf star consuming its closest celestial companion at an unprecedented rate. The study found that the super-dense white dwarf is burning brightly due to the mass transfer between the two stars, potentially leading to a massive explosion visible from Earth.

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Dancing dwarf galaxies predict our Milky Way's future

Researchers studied similar spiral galaxies and found they 'dance' with closely located dwarf satellites, potentially revealing the formation and evolution of our galaxy's satellite system. The study aims to refine models of galaxy evolution and cosmic structure, offering new insights into our understanding of the universe.

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Large and small galaxies may grow in ways more similar than expected

A team of astronomers has obtained detailed images of a small galaxy and its surroundings, revealing features typically associated with larger galaxies. The study found that the mechanisms fueling galaxy growth may be more universal than previously thought, suggesting that even dwarf galaxies can build stellar halos through accretion.

Five galaxy portraits by the Italian VST telescope

The VST-SMASH survey captures new images of five galaxies showcasing their unique structures and assembly histories. The Italian National Institute for Astrophysics (INAF) at ESO Paranal observatory used the VST telescope to produce these glorious galaxy portraits.

Introducing ‘UFO’ galaxies—the Milky Way’s dustier cousins

Researchers discovered a class of unusually large and red galaxies, called Ultra-red Flattened Objects (UFOs), near the limit of Hubble's observable range. The James Webb Space Telescope's infrared capabilities allowed them to spot these 'dustier cousins' of the Milky Way.

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Researchers identify two of the Milky Way's earliest building blocks

Astronomers Khyati Malhan and Hans-Walter Rix identified two proto-galactic fragments, Shakti and Shiva, that merged with an early Milky Way between 12-13 billion years ago. These remnants share low metal content and unusual energy and angular momentum values, making them potential ancestors of the galaxy.

Celestron NexStar 8SE Computerized Telescope

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NASA scientists discover a novel galactic ‘fossil’

Researchers have discovered a novel galactic 'fossil' in the spiral galaxy NGC 4945, which sheds light on the evolution of galaxies. The X-rays outline giant clouds of cold gas that were blasted through the galaxy after its central supermassive black hole erupted 5 million years ago.

New dark matter theory explains two puzzles in astrophysics

A new theory, self-interacting dark matter (SIDM), proposes that dark matter particles interact through a dark force, explaining high-density halos and low-density halos of ultra-diffuse galaxies. SIDM simulates cosmic structure formation with strong dark matter self-interactions, diversifying halo density in central regions.

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How cosmic winds transform galactic environments

Researchers modeled how elements move across star-forming regions, finding that galactic winds influence temperature and metal distribution. The study's findings suggest a non-spherical wind pattern, contrary to previous spherical models.

Galactic explosion offers astrophysicists new insight into the cosmos

Researchers studied a Type 1a supernova in a faraway spiral galaxy, NGC 1566, to understand how certain chemical elements are emitted into the surrounding cosmos. The study confirms that ejecta doesn't escape the confines of the explosion, validating many assumptions about how complex entities work.

Old and new stars paint very different pictures of the Triangulum Galaxy

Researchers used the Panchromatic Hubble Andromeda Treasury Triangulum Extended Region — or PHATTER — survey to study the Triangulum galaxy. The team discovered two drastically different structures depending on the age of the stars, with younger and older stars having distinct distributions.

Astronomers may have uncovered how galaxies change their shape

Researchers used AI to classify galaxies by their shape, leveraging the EAGLE simulation. The study suggests spiral galaxies lose gas as they merge with other galaxies, transforming into elliptical shapes. The findings bring together various pieces of research, providing a new understanding of galaxy evolution and morphology.

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Tracing the remnants of Andromeda’s violent history

Researchers studied over 500 stars in a region of Andromeda called the Northeast shelf, finding conclusive evidence of an ancient collision. The findings provide insights into how material from collisions shapes a galaxy's appearance and makeup.

Optical vortex crystals for photonic simulations of complex systems

Scientists at IIT realized coupled light vortices forming an ordered structure, a light crystal. They developed metasurfaces to control laser beams and created 100 light vortices with tunable topology, enabling new properties for optical communications and simulations of complex systems.

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Supermassive black hole caught hiding in a ring of cosmic dust

Astronomers have confirmed a 30-year-old theory about active galactic nuclei (AGNs) by discovering a supermassive black hole hiding in a thick ring of cosmic dust. The findings provide new insight into how AGNs work and could help understand the history of the Milky Way.

Distant galaxies and the true nature of dark matter

A new study published in Astronomy and Astrophysics suggests that dark matter particles interact with ordinary matter, leading to a constant density region that expands over time. The research challenges the current prevailing theory of Lambda-Cold Dark Matter, which posits that particles are inert and only interact through gravity.

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Hubble spots a stunning spiral galaxy

The Hubble Space Telescope has captured a breathtaking image of NGC 2903, a nearby spiral galaxy. The study aims to understand the relationship between a galaxy's central black hole and its rugby-ball-shaped bulge.

Monster colliding black holes might lurk on the edge of spiral galaxies

Researchers at RIT suggest that outer gas disks of big spiral galaxies are suitable for hosting orbiting black holes and merging massive black holes. This discovery could help explain how black-hole pairs form and provide a new way to study the universe using gravitational waves and traditional light measurements.

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Dark matter less influential in galaxies in early universe

A team of astronomers found that distant galaxies were dominated by normal matter, with dark matter playing a smaller role. The study used the KMOS and SINFONI instruments to measure galaxy rotation velocities and created an average rotation curve, which also showed a decreasing velocity trend away from the centers of the galaxies.

Hubble's front row seat when galaxies collide

Astronomers observe IRAS 14348-1447, a gas-rich spiral galaxy merger, showcasing intense gravitational interactions. The galaxy's extreme infrared emission is fueled by massive molecular gas reserves.

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Hubble spies a spiral snowflake

The NASA/ESA Hubble Space Telescope has captured a striking image of the spiral galaxy NGC 6814, showcasing its luminous nucleus and sweeping arms. The galaxy's extremely bright center is believed to host a supermassive black hole with a mass about 18 million times that of the sun.

CWRU astronomers find new details in first known spiral galaxy

A team of researchers from Case Western Reserve University has discovered new features of the 'Whirlpool Galaxy', M51a, using a 20-hour exposure photograph. The image reveals faint plumes extending from the galaxy's northeast and south, providing valuable insights into its history and interaction with neighboring galaxies.

Surprising image provides new tool for studying galaxy

Astronomers observed a spiral galaxy with a strongly-emitting background galaxy nearly directly behind it. The alignment provides valuable data about the nearer galaxy, revealing it is not forming stars as rapidly as thought. Additional analysis also revealed detailed features of the galaxy's gas halo.

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Exploding star in NGC 2397

A team of astronomers from Queen's University Belfast have discovered the nature of five supernova precursor stars using Hubble images. The study reveals that stars with masses as low as seven times the mass of the Sun can explode as supernovae, challenging current understanding of massive star collapse.

Mystery spiral (galaxy) arms explained?

Researchers have confirmed that the 'anomalous arms' in galaxy M106 are regions of gas violently heated by shock waves, not jets of particles. The team's analysis shows clear consistency with their scenario, providing insight into the formation and evolution of these mysterious structures.

Scientists probe black hole's inner sanctum

A team of scientists measured gas motions within 10 light-years of a supermassive black hole, confirming main theories at unprecedented scales. The observations revealed dynamic shifts in the gas and showed spiral arms pulling gas from distant regions.

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Feeding the monster

Astronomers have released images of galaxy NGC 1097, revealing the channelling process of matter toward its central supermassive black hole. The new images show over 300 regions of star formation in a prominent ring surrounding the nucleus.

Super-star clusters may be born small and grow by coalescing

A trio of massive young star clusters embedded in a cloud of stars offers clues about the birth of super-star clusters. The discovery suggests that these large groups could be formed by the merger of smaller clusters. By studying this phenomenon, scientists can better understand the formation and evolution of super-star clusters.

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Hubble reveals ultraviolet galactic ring

The Hubble Space Telescope has revealed a spectacular ultraviolet galactic ring surrounding the spiral galaxy NGC 6782. The bright ring is made up of recently formed hot stars and marks a significant region of ongoing star formation. Astronomers believe that the unique shape of this ring may be linked to the presence of bars in galaxies.