INFORMATION

A supernova observed by Chinese and Japanese astronomers in 1181 CE didn’t fully explode, instead it sputtered and left behind a rare “zombie star” surrounded by long filaments resembling fireworks. New research by Syracuse University physicist Eric Coughlin explains how these unusual structures formed. After the failed detonation, the surviving white dwarf launched a fast, dense wind that slammed into surrounding gas. The collision created finger-like plumes through a fluid instability, but a second instability that normally tears such structures apart never activated. In some sense, the stars didn’t quite die! from Universe Today https://ift.tt/EJ57pzc via IFTTT

A female mouse that spent two weeks aboard China’s space station has successfully given birth to healthy pups after returning to Earth. This marks the first time offspring have been born from mammals that have traveled in space. The birth demonstrates that short term spaceflight doesn’t impair reproductive capability and provides crucial data for understanding how space environments affect mammalian development, a critical question for future long-l duration human missions beyond Earth. from Universe Today https://ift.tt/OnAgdWl via IFTTT

How did hot Jupiters end up orbiting so close to their stars, thus earning their moniker? This is what a recent study published in The Astronomical Journal hopes to address as a team of researchers from The University of Tokyo investigated the orbital evolution of hot Jupiters ended, specifically regarding where their orbits started before orbiting so close to their stars. This study has the potential to help scientists better understand the formation and evolution of exoplanets and what this could mean for finding life beyond Earth. from Universe Today https://ift.tt/TINcrht via IFTTT

Scientists have discovered that moons could theoretically orbit all seven planets in the TRAPPIST-1 system despite the complex gravitational environment. Using computer simulations, a team of researchers have mapped stable zones where satellites could survive around each planet. They found that moons can remain stable up to about 40-45% of each planet’s sphere of gravitational influence. The neighbouring planets squeeze these stable zones slightly inward compared to isolated planets, but the effect is modest. Long term calculations suggest only tiny moons, roughly one ten millionth the mass of Earth, could survive the immense tidal forces. from Universe Today https://ift.tt/Jaz58yd via IFTTT

Researchers have been trying to look at interstellar object 3I/ATLAS from every conceivable angle. That includes very unconventional ones. Recently, while 3I/ATLAS passed out of view of the Earth, it moved into a great vantage point for one of our interplanetary probes. Europa Clipper, whose main mission is to explore Jupiter’s active moon, turned its gaze during its six year journey back towards the center of the solar system and observed 3I/ATLAS as it was reaching its perihelion, and out of sight from the Earth. from Universe Today https://ift.tt/Rr6yNFs via IFTTT

A team led by the Institute of Space Sciences (ICE-CSIC) analyzed samples of C-type asteroids in a recent study. Their findings support the idea that these asteroids can serve as a crucial source of materials if and when asteroid mining is realized. from Universe Today https://ift.tt/6giTXfx via IFTTT

Supermassive black holes have a reputation for devouring everything in sight, but new observations from the Atacama Large Millimetre/submillimetre Array reveal they can be surprisingly picky eaters. Even when galaxy mergers deliver enormous amounts of cold molecular gas directly to a black hole’s doorstep, many choose to nibble rather than gorge raising questions about what triggers feeding episodes. The discovery suggests black hole growth during galaxy collisions may be far more inefficient and episodic than we previously thought. from Universe Today https://ift.tt/Dp6iRtw via IFTTT

Astronomers using the Hubble Space Telescope have discovered the largest planet forming disk ever observed around a young star, stretching nearly 40 times the diameter of our Solar System. Nicknamed “Dracula’s Chivito” for its hamburger like appearance when viewed edge on, this massive disk reveals an unexpectedly chaotic and asymmetric structure with wisps of material extending far above and below its central plane. The discovery offers an unprecedented window into how planets might form in extreme environments, challenging previous assumptions about the orderly nature of planetary nurseries. from Universe Today https://ift.tt/YABxMn5 via IFTTT

At the end of their lives, most satellites fall to their death. Many of the smaller ones, including most of those going up as part of the “mega-constellations” currently under construction, are intended to burn up in the atmosphere. This Design for Demise (D4D) principle has unintended consequences, according to a paper by Antoinette Ott and Christophe Bonnal, both of whom work for MaiaSpace, a company designing reusable launch vehicles for the small satellite market. from Universe Today https://ift.tt/QBfzHRs via IFTTT

Launched in March, NASA’s SPHEREx space telescope has completed its first infrared map of the entire sky in 102 colors. This map will enable 3D distance measurements to other galaxies and allow astronomers to measure the influence of Cosmic Inflation on the large-scale structure of the Universe. from Universe Today https://ift.tt/IiWJgzE via IFTTT

Solar sails have some major advantages over traditional propulsion methods - most notably they don’t use any propellant. But, how exactly do they turn? In traditional sailing, a ship’s captain can simply adjust the angle of the sail itself to catch the wind at a different angle. But they also have the added advantage of a rudder, which doesn’t work when sailing on light. This has been a long-standing challenge, but a new paper available in pre-print from arXiv, by Gulzhan Aldan and Igor Bargatin at the University of Pennsylvania describes a new technique to turn solar sails - kirigami. from Universe Today https://ift.tt/TSCWNJo via IFTTT

Ready for another amazing year of skywatching? 2025 was a wild year, with a steady parade of comets knocking on naked eye visibility, and one extra special interstellar comet, 3I/ATLAS. The sky just keeps on turning into 2026. Watch for mutual eclipse season for the major moons of Jupiter, as the moons pass one if front of the other. The ongoing solar cycle is also still expected to be active into 2026, producing sunspots space weather and more. And (finally!) we’ll see the return of total solar eclipses on August 12th, as umbral shadow of the Moon crosses Greenland, Iceland and northern Spain. from Universe Today https://ift.tt/4odh8jN via IFTTT

The James Webb Space Telescope (JWST) was involved in yet another first discovery recently available in pre-print form on arXiv from Cicero Lu at the Gemini Observatory and his co-authors. This time, humanity’s most advanced space telescope found UV-fluorescent carbon monoxide in a protoplanetary debris disc for the first time ever. It also discovered some features of that disc that have considerable implications for planetary formation theory. from Universe Today https://ift.tt/FqX5Ew4 via IFTTT

Oleg Orlov, Director of the Institute of Biomedical Problems at the Russian Academy of Sciences (RAS), announced that the Russian Orbital Station (ROS) will include the modules that make up the Russian Orbital Segment of ISS. from Universe Today https://ift.tt/3uFAU4J via IFTTT

Saturn’s largest moon, Titan, may not have a subsurface ocean after all. That’s according to a re-examination of data captured by NASA’s Cassini mission, which flew by Titan dozens of times starting in 2004. By 2008, all the evidence suggested a subsurface ocean of liquid water waited beneath Titan’s geologically complex crust. But the latest analysis says the interior is more likely to be made of ice and slush, albeit with pockets of warm water that cycle from core to surface. from Universe Today https://ift.tt/1JyTO0I via IFTTT

One of the primary goals of the James Webb Space Telescope (JWST) is to detect atmospheres around exoplanets, to try to suss out whether or not they could potentially support life. But, in order to do that, scientists have to know where to look, and the exoplanet has to actually have an atmosphere. While scientists know the location of about 6000 exoplanets currently, they also believe that many of them don’t have atmospheres and that, of the ones that do, many aren’t really Earth-sized. And of those, many are around stars that are too bright for our current crop of telescopes to see their atmosphere. All those restrictions mean, ultimately, even with 6000 potential candidates, the number of Earth-sized ones that we could find an atmosphere for is relatively small. So a new paper available on arXiv from Jonathan Barrientos of Cal Tech and his co-authors that describes five new exoplanets around M-dwarf stars - two of which may have an atmosphere - is big news for astrobiologists and e...

During November 2025, ESA’s Jupiter Icy Moons Explorer (JUICE) used five of its science instruments to observe 3I/ATLAS. The instruments collected information about how the comet is behaving and what it is made of. from Universe Today https://ift.tt/oPfV8S5 via IFTTT

Engineers need good data to build lasting things. Even the designers of the Great Pyramids knew the limestone they used to build these massive structures would be steady when stacked on top of one another, even if they didn’t have tables of the compressive strength of those stones. But when attempting to build structures on other worlds, such as the Moon, engineers don’t yet know much about the local materials. Still, due to the costs of getting large amounts of materials off of Earth, they will need to learn to use those materials even for critical applications like a landing pad to support the landing / ascent of massive rockets used in re-supply operations. A new paper published in Acta Astronautica from Shirley Dyke and her team at Purdue University describes how to build a lunar landing pad with just a minimal amount of prior knowledge of the material properties of the regolith used to build it. from Universe Today https://ift.tt/iSvmclQ via IFTTT

Using the James Webb Space Telescope, a team of international researchers has discovered chemical fingerprints of gigantic primordial stars that were among the first to form after the Big Bang. from Universe Today https://ift.tt/bZJHt2A via IFTTT

During the deployment of new space telescopes that are several critical steps each has to go through. Launch is probably the one most commonly thought of, another is “first light” of all of the instruments on the telescope. Ultimately, they’re responsible for the data the telescope is intended to collect - if they don’t work properly then the mission itself it a failure. Luckily, the Interstellar Mapping and Acceleration Probe (IMAP) recently collected first light on its 10 primary instruments, and everything seems to be in working order, according to a press release from the Southwest Research Institute who was responsible for ensuring the delivery of all 10 instruments went off without a hitch. from Universe Today https://ift.tt/T7lA0ua via IFTTT

For the first time, astronomers using the Hubble Space Telescope have spotted a pair of catastrophic collisions in another solar system. They were observing Fomalhaut, a bright star about 25 light-years away, and detected a pair of planetesimal collisions and their light-reflecting dust clouds. The system is young, and the collisions reflect what our Solar System was like when it was young. from Universe Today https://ift.tt/URnxMcL via IFTTT

Getting close to things is one way for scientists to collect better data about them. But that's been hard to do for the Sun, since getting close to it typically entails getting burnt to a crisp. Just ask Icarus. But if Icarus had survived his close encounter with the Sun, he might have been able to see massive magnetic “tadpoles” tens of thousands of kilometers wide reconnecting back down to the surface of our star. Or maybe not, because he had human eyes, not the exceptionally sensitive Wide-Field imagers the Parker Solar Probe used to look at the Sun while it made its closest ever pass to our closest star. A new paper in The Astrophysical Journal Letters from Angelos Vourlidas of Johns Hopkins University’s Applied Physics Laboratory and his co-authors describes what they say on humanity’s closest brush with the Sun so far. from Universe Today https://ift.tt/wiR1aG9 via IFTTT

In a new paper, a team of researchers explores how non-human species (in this case, fireflies) could inform new approaches in the Search for Extraterrestrial Intelligence (SETI). from Universe Today https://ift.tt/XA90Qen via IFTTT

Astronomers may have just seen the first ever ‘superkilonova,’ a combination of a supernova and a kilonova. These are two very different kinds of stellar explosions, and if this discovery stands, it could change the way scientists understand stellar birth and death. from Universe Today https://ift.tt/8LMoNdU via IFTTT

In 2024, astronomers discovered the brightest Luminous Fast Blue Optical Transient (LFBOT) ever observed. LFBOTs are extremely bright flashes of blue light that shine for brief periods before fading away. New analysis of this record-breaking burst, which includes observations from the International Gemini Observatory, funded in part by the U.S. National Science Foundation, challenges all prior understanding of these rare explosive events. from Universe Today https://ift.tt/bpBfGO7 via IFTTT

In a glimpse of the early universe, astronomers have observed a galaxy as it appeared just 800 million years after the Big Bang – a cosmic Jekyll and Hyde that looks like any other galaxy when viewed in visible and even ultraviolet light but transforms into a cosmic beast when observed at infrared wavelengths. This object, dubbed Virgil, is forcing astronomers to reconsider their understanding of how supermassive black holes grew in the infant universe. from Universe Today https://ift.tt/vt59xaA via IFTTT

With new technologies comes new discoveries. Or so Spider Man’s Uncle Ben might have said if he was an astronomer. Or a scientist more generally - but in astronomy that saying is more true than many other disciplines, as many discoveries are entirely dependent on the technology - the telescope, imager, or processing algorithm, used to collect data on them. A new piece of technology, the Nancy Grace Roman Space Telescope, is exciting scientists enough that they are even starting to predict what kind of discoveries it might make. One such type of discovery, described in a pre-print paper on arXiv by Vito Saggese of the Italian National Institute for Astrophysics and his co-authors on the Roman Galactic Exoplanet Survey Project Infrastructure Team, is the discovery of many more multiplantery exoplanet systems an astronomical phenomena Roman is well placed to detect - microlensing. from Universe Today https://ift.tt/RcfG0Cl via IFTTT

Everyone’s favorite interstellar comet posed for one more portrait recently. The European Space Agency’s XMM-Newton mission nabbed 3I/ATLAS on December 3rd from about 283 million kilometers distant. This comes as the comet is set to make its closest passage versus Earth this coming Friday, on December 19th. from Universe Today https://ift.tt/iTPGroH via IFTTT

In astronomy, there is a concept called “degeneracy”. It has nothing to do with delinquent people, but instead is used to describe data that could be interpreted multiple ways. In some cases, that interpretation is translated into exciting new possibilities. But many times, when that happens, other, more mundane explanations are ignored for the publicity that the more interesting possibilities provide. That seems to have been the case for many “sub-Neptune” exoplanets discovered recently. Some theories have described them as Hycean worlds - worlds that are filled with water oceans or ice. But a new paper from Robb Calder of the University of Cambridge and his co-authors shows that, most likely, these planets are almost all made of molten lava instead. from Universe Today https://ift.tt/CRXeyI8 via IFTTT

When we gaze up at the night sky, we assume that what we're seeing is a representative population of similar stars at similar distances. But it's not. The stars we see are a mixture of massive and small, distant and near. In fact, we can't even see our closest neighbour, Proxima Centauri. We see these stars because they have large observational signals, and that illustrates one of the problems in astronomy. from Universe Today https://ift.tt/G7k1ejW via IFTTT

If you read enough articles about planets in binary star systems, you’ll realize almost all of them make some sort of reference to Tatooine, the fictional home of Luke Skywalker (and Darth Vader) in the Star War saga. Since that obligatory reference is now out of the way, we can talk about the new “super-Jupiter” that researchers from two separate research teams, including one at Northwestern University and one at the University of Exeter, simultaneously found in old data from the Gemini Planet Imager (GPI). from Universe Today https://ift.tt/vxo6Xk7 via IFTTT

The Shenzhou-21 crew on board China's orbiting space station completed its first extravehicular activities on Tuesday, Dec. 9th, during which they validated the new EVA spacesuits. from Universe Today https://ift.tt/r3StuIB via IFTTT

A team of researchers from the University of Zurich and the NCCR PlanetS is challenging our understanding of the interior of the Solar System's planets. The composition of Uranus and Neptune, the two outermost planets, might be more rocky and less icy than previously thought. from Universe Today https://ift.tt/Y1CN9fF via IFTTT

For roughly two billion years of Earth’s early history, the atmosphere contained no oxygen, the essential ingredient required for complex life. Oxygen began building up in the atmosphere during the period known as the Great Oxidation Event (GOE), but it had to enter the oceans first. When and how it first entered the oceans has remained uncertain. from Universe Today https://ift.tt/RbSm7fp via IFTTT

Astronomers at the University of Tokyo have used gravitational lensing to measure how fast the universe is expanding, adding weight to one of cosmology's most intriguing mysteries. Their technique exploits the way massive galaxies bend light from distant quasars, creating multiple distorted images that arrive at different times. The measurement supports recent observations showing the universe expands faster than predictions based on the early universe suggest, strengthening evidence that the "Hubble tension" represents genuine new physics rather than experimental error. from Universe Today https://ift.tt/FluqJjX via IFTTT

Researchers using NASA’s James Webb Space Telescope have detected the strongest evidence yet for an atmosphere on a rocky planet outside our solar system. Observations of the ultra-hot super-Earth TOI-561 b suggest that the exoplanet is surrounded by a thick blanket of gases above a global magma ocean. from Universe Today https://ift.tt/tliWLHg via IFTTT

The early universe was a very different place than today. And by “early” I don’t mean a billion or even ten billion years ago. The universe is about 13.77 billion years old, and when it was only a handful of seconds old, it was completely unrecognizable. from Universe Today https://ift.tt/liV3wgf via IFTTT

In the early 20th century, after years of effort, Albert Einstein developed his general theory of relativity. This was a massive improvement in our understanding of gravity, giving us a sophisticated view into the inner workings of that fundamental force. from Universe Today https://ift.tt/9QwEeFf via IFTTT

Tracking down resources on the Moon is a critical process if humanity decides to settle there permanently. However, some of our best resources to do that currently are orbiting satellites who use various wavelengths to scan the Moon and determine what the local environment is made out of. One potential confounding factor in those scans is “space weathering” - i.e. how the lunar surface might change based on bombardment from both the solar wind and micrometeroid impacts. A new paper from a researchers at the Southwest Research Institute adds further context to how to interpret ultra-violet data from one of the most prolific of the resource assessment satellites - the Lunar Reconnaissance Orbiter (LRO) - and unfortunately, the conclusion they draw is that, for some resources such as titanium, their presence might be entirely obscured by the presence of “old” regolith. from Universe Today https://ift.tt/0jRLEtD via IFTTT

Radio astronomers hunting for the faint whispers of the early universe face an unexpected threat from above: satellites designed to be silent are leaking radio noise into space. New research using the Murchison Widefield Array has set the first limits on unintended radio emissions from distant geostationary satellites, revealing that most remain mercifully quiet in the frequency range crucial for next-generation telescopes. The findings offer cautious hope that the Square Kilometre Array, set to become the world's most sensitive radio telescope, might avoid the radio pollution crisis now plaguing observations of low Earth orbit satellites. from Universe Today https://ift.tt/XMwNdW5 via IFTTT

The NASA/ESA Hubble Space Telescope reobserved interstellar comet 3I/ATLAS on 30 November with its Wide Field Camera 3 instrument. At the time, the comet was about 286 million km from Earth. Hubble tracked the comet as it moved across the sky. from Universe Today https://ift.tt/etfZP7E via IFTTT

Astronomers have been observing the Cosmic Owl for years, wondering if what they were seeing was a long-predicted runaway black hole. Now, 50 years after scientists first predicted the phenomenon, the JWST has provided the clinching evidence. from Universe Today https://ift.tt/5HpuPtz via IFTTT

The Hubble Tension is one of the great mysteries of cosmology. Solving it might require a fundamental change in how we understand the universe - but scientists have to prove it actually exists first. A new paper from a collective of cosmologist researchers known as the TDCOSMO Collaboration adds further fuel to that first with updated measurements of the “Late Universe” measurement of the Hubble Constant using gravitational lenses of quasars, which shows that the Tension might exist after all. from Universe Today https://ift.tt/cRKT6Ho via IFTTT

What geological features on Earth can be used to better understand unique geological features on Jupiter’s icy moon, Europa? This is what a recent study published in The Planetary Science Journal hopes to address as a team of researchers investigated potential Earth analogs for studying a unique geological feature on Europa scientists identified almost 30 years ago. This study has the potential help scientists gain insights into Europa’s unique geological features, some of which scientists hypothesize are caused by the moon’s internal liquid water ocean. from Universe Today https://ift.tt/fa3p7Pt via IFTTT

Surface-bound gels may have provided the structure and chemistry necessary for life to take root on Earth. These findings could also have implications in the search for life beyond Earth. from Universe Today https://ift.tt/Bxl5inq via IFTTT

The Leibniz Institute for Astrophysics Potsdam (AIP) is forming a new research group that will focus solely on the Large and Small Magellanic Clouds. The pair of irregular dwarf galaxies are satellites of the Milky Way, and are natural, nearby laboratories for studying how galaxies form and evolve. The research group will make heavy use of the spectroscopic 4MOST survey from the VISTA telescope. from Universe Today https://ift.tt/MVa7zgG via IFTTT

The challenge is that nothing in this universe is simple. And if there’s one thing you take away from today’s episode, then let it be that. Don’t ever let yourself fall into the trap of simple answers for difficult questions. We’re cosmologists, we study the universe as it is, not as we wish it would be. from Universe Today https://ift.tt/nXz2s95 via IFTTT

arXiv:2512.07695v1 Announce Type: new Abstract: One of the forefront goals in the field of exoplanets is the detection of an atmosphere on a temperate terrestrial exoplanet, and among the best suited systems to do so is TRAPPIST-1. However, JWST transit observations of the TRAPPIST-1 planets show significant contamination from stellar surface features that we are unable to confidently model. Here, we present the motivation and first observations of our JWST multi-cycle program of TRAPPIST-1 e... from Universe Today https://ift.tt/Bx6N85f via IFTTT

An international team of astronomers observed a sudden outburst of matter near the supermassive black hole NGC 3783 at speeds reaching up to 20% of the speed of light. During a ten-day observation, mainly with the XRISM space telescope, the researchers witnessed its formation and acceleration. Scientists often find that these outbursts are powered by strong radiation, but this time the most likely cause is a sudden change in the magnetic field, similar to bursts on the Sun that cause solar flares. from Universe Today https://ift.tt/BnAPWvo via IFTTT

An international team of astronomers has published a series of papers detailing their observations of the rocky exoplanet TRAPPIST-1e using the James Webb Space Telescope (JWST). Their results, though ambiguous, are a big step towards exoplanet characterization. from Universe Today https://ift.tt/2WbUpRM via IFTTT