Telescopes

NASA’s Hubble Space Telescope just revealed a mystery in our cosmic neighborhood. In a paper published in The

Some stars, called Luminous Blue Variables, can be confused with supernovae explosions. They exhibit similar outbursts, but unlike supernovae, which explode once and then are gone forever, these stars have periodic outbursts. New research found that one of these 'supernova impostors' is in a binary relationship with a black hole or a neutron star, and that explains its periodic outbursts.

NASA's Nancy Grace Roman Space Telescope could capture images 30% sharper than — and remain operational for twice as long as — initially expected. Researchers say these "remarkable" developments could greatly enhance the volume and quality of the data they will analyze.

Mid-infrared observations with the Subaru Telescope have revealed the shape and surface temperature of the nucleus of Comet 2P/Encke. By analyzing how the nucleus's thermal emission changed as it rotated, the researchers found that the nucleus is elongated, with a long axis of about 7 kilometers and a short axis of about 3 kilometers. They also determined that the surface temperature at the time of observation was 328 ± 7 Kelvin (about 55°C).

Using the James Webb Space Telescope (JWST), a team of astronomers identified 104 magnified stellar events in a galaxy known as the Dragon, located around 6.5 billion light-years away. This discovery more than doubles the previous record of 44 such detections in the same galaxy. Because these kinds of events reveal some of the most luminous stars and likely the presence of dark matter, this study offers a rare look at the galaxy's stellar population along with a possible hint at the nature of dark matter.

Using machine learning, astronomers developed a new way of looking at James Webb telescope data that allows far-off planets to emerge from their star's glare.

After nearly 22 years of exploring the universe’s most violent explosions, NASA’s Swift Observatory has re-entered Earth’s atmosphere over Indonesia. Originally designed to last just two years, the pioneering space telescope transformed our understanding of black holes, exploding stars, and mysterious cosmic outbursts.

A Rescue Window for Hubble The Hubble Space Telescope has no engine to hold its orbit. Atmospheric drag

This NASA/ESA Hubble Space Telescope image provides a lesson in galactic history. The sparkling collection of stars is named Messier 30 (M30) after the French astronomer Charles Messier, who cataloged M30 and other diffuse objects that might be mistaken for comets in the early telescopes of Messier's time. M30 lies about 27,500 light-years away in the constellation Capricornus.

NASA's Neil Gehrels Swift Observatory took its last look at the sky on Oct. 20, 2026, while orbiting about 171 miles (275 kilometers) above Earth. NASA ended the telescope's mission three days later, because Swift had sunk so low that drag from the thin air there meant its telescopes couldn't hold steady.

Johns Hopkins researchers searching the expanse of the universe for the existence of the first black holes are zeroing in on little red dots that may hold the key to the theoretical phenomenon.

Finding dim exoplanets hidden in the glare of their stars is an ongoing challenge in astronomy. Telescopes use coronagraphs to block out starlight, but even they have their limitations. Researchers have developed a new technique with the JWST that can find dim exoplanets more easily than ever.

A half-built neutrino telescope on the floor of the Mediterranean Sea searched for cracks in one of physics' most basic invariances. It came up empty, but its limits rival those of detectors many times its size.

Tiny Worlds Beyond Neptune Planet formation models predict a crowd of small icy bodies in the far reaches

The reentry of NASA's dead Swift space telescope is the end of an era for rapid-response space science.

One of NASA's premier space telescopes plunged to Earth on Wednesday, ending its 22-year investigation of the universe's biggest explosions.

By modeling the James Webb Space Telescope’s tiny movements, a new technique can reveal up to 15 times fainter alien worlds

The observatory had spent decades studying powerful cosmic explosions and was the target of an unsuccessful rescue mission earlier this year

Even the world's most powerful telescopes have their blind spots. Although NASA's James Webb Space Telescope (JWST) can peer billions of years into the past, it still struggles to photograph planets orbiting nearby stars. Stars shine with such extraordinary brightness that their glare overwhelms nearby planets' faint glow.

NASA is exploring a daring plan to save the legendary Hubble Space Telescope from its eventual fiery plunge into Earth's atmosphere. After more than 35 years of groundbreaking discoveries, Hubble is slowly losing altitude, and without intervention, it could fall back to Earth as early as 2033 or 2034. To keep the iconic observatory operating, NASA is asking private space companies to propose innovative ways to boost Hubble into a higher orbit, upgrade its capabilities, or safely dispose of it when its mission finally ends.

The space agency estimates that there is a one-in-2,100 chance that debris from the Neil Gehrels Swift Observatory could injure someone on the ground.

Astrophysicists think that the supermassive black holes (SMBH) we see in the modern universe are the result of a long, drawn-out process. That process is referred to as the hierarchical black hole mergers framework. It explains how some SMBHs can reach such staggering masses. Some of the most massive appear to have billions of solar masses.

Astrophysicists think that black holes grow through a hierarchical merger framework. But the elusive Intermediate Mass Black Holes are the missing link between stellar mass black holes, and the gargantuan supermassive black holes like the one at the center of the Milky Way. The JWST may have found the ancient sources of IMBH heavy seeds: young massive clusters in the high-redshift Universe.

NASA’s Hubble and James Webb Space Telescopes have uncovered surprising clues about the solar system’s origins by studying 27 tiny, distant objects beyond Neptune. Scientists discovered that these ancient building blocks of planets have remained remarkably unchanged for billions of years, while their unexpected sizes and numbers challenge existing theories of planet formation.

The Cat's Head Nebula shows its ghostly insides and sinister red eye in rival views from the Hubble and James Webb space telescopes.

A surprising discovery by astronomers using the Hubble Space Telescope is challenging a leading explanation for how the early universe emerged from a dense fog of hydrogen roughly 13 billion years ago. Scientists once believed powerful winds from exploding stars helped radiation escape galaxies and clear that cosmic fog, but new observations reveal that these winds actually block radiation instead.

Astronomers using the James Webb Space Telescope (JWST) have found evidence that a distant, exceptionally blue galaxy may allow most of its ionizing radiation to escape into space. Known as EBG-1, the gravitationally lensed galaxy is seen at a redshift of 9.244, about 530 million years after the Big Bang. The paper was posted to the arXiv preprint server on Oct. 16.

Most of us could spend our entire lives looking at the night sky and see very few changes. The moon becomes more or less illuminated, the planets drift placidly through the sky, satellites and the ISS intrude for a few moments at a time, and the bright, momentary streak of a meteor punctuates the occasional evening of stargazing.

Star formation is a complicated process. It involves metallicity, gas temperature and density, dust grains, and stellar feedback from existing stars. Sometimes, studying all these factors and how they work means studying some of Nature's most beautiful structures, like the Cat's Head nebula in the Carina Nebula.

NASA's Hubble and James Webb Space Telescopes have captured a hauntingly dynamic star-forming scene, like a spectral form rising out of a cold mist. It lies within the vast Carina Nebula, a diffuse star-forming region located about 7,500 light-years away from Earth. The small, select area both telescopes observed is nicknamed the Cat's Head Nebula because of its resemblance to a cat sitting with its back toward the viewer. The "head" of the cat is turned to the right, revealing a glowing eye.

James Webb observations suggest interstellar comet 3I/ATLAS contains dust-rich water-ice grains, offering clues about how icy bodies may form around other stars

NASA has committed to launching a new, more powerful UV space telescope. Named UVEX, the UltraViolet EXplorer, it will launch in 2031. It's about 100 times more powerful than its predecessor, GALEX, whose mission ended in 2013. UVEX will perform a survey in UV that will complement infrared surveys by other telescopes.

Astronomers have identified 2026 ED138, a distant object that may qualify as the Solar System's sixth dwarf planet, although its size and shape remain uncertain.

Astronomers using the James Webb Space Telescope have observed a galaxy with a ring of newborn stars as it appeared 2.1 billion years after the Big Bang — hinting that the early universe may have been more chaotic than once thought.

The Nancy Grace Roman Space Telescope will use gravitational microlensing to study dark matter. But it's a wide-field survey telescope, and the venerable Hubble Space Telescope can do things it can't do. That's why the Hubble is lending a hand.

The Lazuli Space Telescope will be the first private space telescope. It's the brainchild of Eric Schmidt, Google's former CEO. It will have a 3-meter mirror (9.8 feet), larger than Hubble's 2.4-meter mirror (7.9 feet), and will be launched by 2029.

A new study reveals a dust-reddened quasar from a time when the universe was less than a billion years old. Located at a redshift of 6.5488, the object J1440+0019 contains a rapidly accreting supermassive black hole with a mass of about 1.1 billion suns. The paper was posted to the arXiv preprint server on Oct. 9.

Get ready for the age of private space telescopes. The Lazuli Space Telescope will launch in a few years and part of its mission is to observe exoplanets. New research presents a list of 27 exoplanet targets, some of which are very well-known and will certainly benefit from deeper observations.

A sweeping barred spiral galaxy marks the spot in this image, but the real treasure is the gravitational lens in the lower-right corner, where a distant background galaxy is being magnified and distorted by the gravity of a closer galaxy.

Typically, when we think of exoplanets, we think of neat spheres floating directly in front of their star, which acts as a giant spotlight. From our vantage point, they would look more like two perfect two dimensional circles than spheres, though. But nature is almost never so clean-cut. A new paper published in Nature Astronomy from researchers at Cornell and the University of Bristol details the first-ever study of an exoplanet that is noticeably lopsided.

New observations from the James Webb Space Telescope reveal a concentration of heavy metals near the Milky Way's central black hole. The discovery deepens a mystery about why our black hole behaves the way it does.

An international team of researchers, including members from the University of Michigan, has revealed surprising results that could rewrite our understanding of a key transition in the early universe.

Astronomers using the James Webb Space Telescope may have discovered a supernova erupting just 1.1 billion years after the Big Bang.

When picturing a star, typically people think of giant balls of burning gas in the sky that emit enough light they are hard to miss. Planets, on the other hand, come in one of two general categories - rocky worlds like Earth or gas giants similar to Jupiter. But there is a third category of astronomical object that doesn’t really fit either of those descriptions, and also doesn’t exist in our own solar system. Known as a brown dwarf, they are sometimes called a “failed star” as they form the same way stars do, but never reach the critical mass of material to create active fusion in the cores. They are also much too massive to be considered a regular planet. But a new paper from researchers led by Brittany Miles of the University of Arizona describes one similarity between the coldest known brown dwarf and some of the planets in our solar system - it has

The ESA's Euclid space telescope was launched in July, 2026, and its mission is to observe billions of galaxies. The goal is to measure their redshifts over 10 billion years of Universal expansion, to better understand dark matter and dark energy. Surprisingly, the telescope has discovered a brand new comet, now named C/2026 S1 (Euclid).

NASA’s Nancy Grace Roman Space Telescope has exceeded expectations after engineers made incredibly tiny adjustments to sharpen its view of the universe. By moving a mirror just one-sixteenth the width of a human hair, the team helped bring its powerful instruments into near-perfect alignment. Roman’s Wide Field Instrument now produces image quality nearly 30% better than predicted, promising exceptionally sharp cosmic surveys.

This NASA Hubble Space Telescope image features the edge-on, intermediate spiral galaxy NGC 1827, located roughly 37 million light-years away in the constellation Columba, the Dove. Hubble captured the image as part of a survey looking at 260 satellite galaxies around 22 Milky Way–like host galaxies within a radius of about 32 million light-years from Earth. Hubble has already observed 111 of these satellite galaxies. The remaining galaxies will take an additional 149 Hubble orbits, one orbit for each galaxy, to observe.

Webb Maps a Lopsided Exoplanet Atmosphere Models of distant planets usually treat them as perfect circles. A new

NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) space telescope is

Diligent sleuthing by astronomers has broken open a cold case in the data archive of NASA’s Hubble Space Telescope. In a study published Monday in Nature Astronomy, researchers report uncovering a surprising chemical clue that indicates the white dwarf star HS 0209+0832 may host a second-generation planet.

A strange chemical signature in old Hubble observations may point to a planet that formed after its star had already died. Astronomers found unusually high levels of niobium around the white dwarf HS 0209+0832, suggesting some of the star’s expelled material may have assembled into a new gas giant. TESS data also hints at a Jupiter-sized planet orbiting just 3.7 million miles from the star.

There’s lots of things you can do with balloons. Children’s birthday parties come to mind, as do retirement parties. But you can also observe the Sun in unprecedented detail with one - or at least with a suite of equipment attached to a gondola floating beneath one. That’s what the SUNRISE III mission did back in 2024, and scientists have had time to compile a series of three scientific papers on the results from that mission, which have been published in the Astrophysical Journal Letters.

Nobel Physics Prize for IceCube For the first time since 1991, the Nobel Prize in Physics belongs to

NASA has taken the next step in the process of developing a new all-glass telescope for the LISA (Laser Interferometer Space Antenna) mission, a space observatory designed to detect ripples in space-time called gravitational waves.

The James Webb Space Telescope has detected the farthest "fast radio burst" ever seen, providing more clues about these mysterious explosions.

The core of the Milky Way is a dense, active, messy region, dominated by a supermassive black hole called Sagittarius A* (Sgr A*) hiding at the heart of the galaxy. But Sgr A* is only a supporting actor in this stunning new image from the Chandra X-ray Observatory.

NASA’s Roman Space Telescope has demonstrated remarkable pointing stability and given its powerful planet-imaging coronagraph its first look at the cosmos. The telescope can already stay locked on a target with precision comparable to aiming a laser at a dime from about 150 miles away. Its coronagraph also captured stars in the Large Magellanic Cloud, confirming that the instrument can produce focused images.

NASA announced Wednesday a mission to explore the history and evolution of the universe, PRIMA (PRobe far-Infrared Mission for Astrophysics), is advancing to the next phase of development. This space telescope is the first in a new class of NASA astrophysics missions, called Probe Explorers, within the agency’s longstanding Explorers Program.

NASA’s Hubble Space Telescope completed its 200,000th orbit around Earth on Sept. 19th and marked this milestone with observations that could help refine astronomers' measurements of cosmic expansion (aka. the Hubble Constant).

After seven years of work, Canada's CHIME telescope has a measurement of dark energy from 2019. More detailed studies are planned to expand the research.

Look up at the night sky with the naked eye and it may seem like it rarely changes. Yet the universe is in constant flux. Stars drift through space, orbiting the center of the Milky Way as planets orbit them. They rotate, showing spots on their surfaces and sometimes producing violent outbursts that affect planetary atmospheres much like solar storms produce auroras on Earth.

Astronomers have cataloged billions of stars and hundreds of billions of galaxies. We have found thousands of planets orbiting stars. We can also map where galaxies sit and trace how the universe changes over time.

NASA's Nancy Grace Roman Space Telescope is about to begin scanning our universe as it journeys through space. Live Science readers shared their thoughts about what they're most excited to see from the new space telescope.

Scientists love taking inspiration from nature. The evolutionary processes that have created such a diverse panoply of life on Earth can be a great source of ideas in solving technical problems. One such example is the pattern of sunflower seeds - they are arranged in a mathematically optimized pattern known as a Vogel spiral, and the international team building the Square Kilometer Array (SKA) in Australia decided to lay out their antennas in a similar pattern. But, as they report in a paper recently published in the Journal of Astronomical Telescopes, Instruments, and Systems, when they did so they found a huge blind spot in the data which hints that maybe this particular natural pattern might need to be modified to work well for this particular application.

One of the largest images from the James Webb Space Telescope so far reveals an intricate landscape of dwarf stars and spectacular clouds.

When we think of asteroids, we often think of the main asteroid belt between Mars and Jupiter that contains the majority of the known asteroids in our solar system. However, our solar system hosts several other populations of asteroids and icy rocks, including the Jupiter Trojan asteroids that orbit in Jupiter’s orbit, and the icy bodies and comets of the Kuiper Belt. But there’s one population of asteroids that often gets overlooked called Centaurs, primarily because their orbits are not in a fixed location and instead whose orbits cross the orbits of the outer planets.

NASA has announced that a new telescope concept called PRIMA is moving forward in consideration for a 2033 launch to look at the origins of planets and galaxies.

SKA-Low is a radio telescope under construction in Western Australia. It will operate across a wide frequency range, from 50 to 350 MHz, and will be the most sensitive telescope of its kind ever built. The completed instrument will link 512 stations spread across an area roughly 75 km (47 miles) wide. Each station's antennas work together like a single large dish, so their arrangement directly shapes what the telescope can detect.

The robotic spacecraft that failed to rescue an aging NASA telescope plunged back to Earth on Friday less than three months after launching on the bold mission.

When the universe was still in its infancy—only 500 million years after the Big Bang, or about 3% of its current age—some of the universe's earliest stars and galaxies had already formed. Astronomers have long predicted that much of the gas surrounding these young galaxies must have remained relatively pristine, composed mostly of hydrogen and helium, the primordial ingredients available in the newborn cosmos.

NASA's Hubble Space Telescope completed its 200,000th orbit around Earth on Sept. 19, marking another milestone for an observatory that continues to transform our understanding of the universe.

For more than a decade, PI (Physik Instrumente) has supplied precision motion and piezoelectric technologies for the development, alignment, testing, and flight hardware of NASA’s Nancy Grace Roman Space Telescope.

NASA's Nancy Grace Roman Space Telescope has taken its first pictures of space as it heads toward its orbital location. From there, it will begin scanning deep space to uncover more about our universe.

Scanning vast swaths of sky, NASA’s next flagship observatory, the Nancy Grace Roman Space Telescope, promises to revolutionize our

This week, NASA turned on the Nancy Grace Roman Space Telescope's powerful 300-megapixel camera for the first time. The debut test image promises "groundbreaking science" to come with NASA already talking about doubling the mission's lifespan.

Though the spiral galaxy in this new image from the NASA/ESA Hubble Space Telescope seems serene, it hides a chaotic secret. This galaxy is NGC 4698, and it lies about 55 million light-years away in the constellation Virgo. It's one of more than a thousand galaxies in the Virgo Cluster, the nearest large cluster of galaxies bound together by gravity.

The space telescope is set to reveal thousands of new exoplanets and scour the universe for signs of dark matter and energy

NASA’s Roman Space Telescope may now have enough fuel for at least 22 years of science, more than double its original 10 year design life. An extremely precise course correction, extra fuel at launch, and additional expected savings could keep the powerful observatory studying the universe for decades.

The discovery of “hypersoft” X-ray beacons could help solve some mysteries about the universe.

New supercomputer simulations suggest JWST’s puzzling Little Red Dots are rapidly growing black holes from the early Universe. Extreme radiation may have helped create unusually massive black hole seeds, while dense surrounding gas allowed them to grow dozens of times faster than black holes can today. The simulated objects closely resemble the Little Red Dots seen by Webb. If correct, they could solve the mystery of how enormous black holes formed so soon after the Big Bang.

Research initiated as part of a bachelor's thesis in physics at the Universitat Autònoma de Barcelona (UAB) has culminated in a new analytical description of the muon-based calibration of dual-mirror Cherenkov telescopes. The work solves a problem that had remained open for more than 30 years because of the geometric complexity of these optical systems: determining precisely how much Cherenkov light produced by a muon reaches the camera, taking into account the shadows cast by the secondary mirror and the camera itself.

The Nancy Grace Roman Space Telescope hasn't yet reached its Sun–Earth L2 orbit, and it already has some good news. NASA has announced that the mission has enough fuel to potentially double its mission length. Though initially scheduled for five years of observations, followed by a five-year extended mission, the entire mission could now reach 22 years.

Roman Telescope’s 22-Year Fuel Supply NASA fitted the Nancy Grace Roman Space Telescope with a grapple fixture and

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James Webb Space Telescope observations of Chariklo, one of the smallest ringed worlds in the solar system, reveal some inexplicable changes.

More good news for NASA's Nancy Grace Roman Space Telescope. The telescope's first mid-course correction was extremely efficient, using only 10% of the fuel allotted for it. This efficiency, coupled with other factors, means the powerful space telescope will likely have an additional ~12 years of observing time.

The James Webb Space Telescope spots mysterious “little red dots” everywhere. A bold new theory suggests they’re suns dozens of times larger than our entire solar system. The post Black Holes or Black Hole Stars? Astronomers Spar Over Webb Telescope’s ‘Little Red Dots.’ first appeared on Quanta Magazine

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The James Webb Space Telescope (JWST) has opened many wonders of the cosmos to scientists since it began science operations a few years ago. But one thing it hasn't done is find an "exomoon." These still-theoretical moons orbit exoplanets in other star systems, and JWST was supposed to find a plethora of them.

A spectacular new Hubble Space Telescope image reveals almost 30,000 newborn stars around an enormous cavity carved into a stellar nursery in a neighboring galaxy.

NASA’s formidable gamma-ray burst hunter is doomed to soon reenter Earth’s atmosphere, leaving a glaring gap in our view of the high-energy sky

The James Webb Space Telescope (JWST) has opened up many wonders of the cosmos to scientists since it began its science operations a few years ago. But one thing that it hasn’t done is find an “exomoon”. These, as yet still theoretical, moons orbit exoplanets in other star systems, and JWST was supposed to find a plethora of them. However, so far it has found precisely none. It seems the cause is noise in the telescope’s instrumentation or noise from the star itself. But a new paper, available in pre-print form on arXiv from David Kipping, an astronomer at Columbia and also the host of the Cool Worlds YouTube Channel, shows how JWST can, in fact, find an exomoon. It likely just has to look for one in the same place repeatedly.

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Until just over a decade ago, ring systems were thought to be exclusive to the giant planets of the solar system, such as Jupiter, Saturn, Uranus and Neptune. However, in 2013, a small body barely 250 kilometers (155 miles) in diameter, located at nearly 17 times the Earth–sun distance, joined this small group. The object is Chariklo, a small body orbiting between Saturn and Uranus, around which astronomers discovered two dense rings.

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