Three views of the Cat's Head Nebula. A visible light image captured by NASA's Hubble Space Telescope (left); a mid-infrared image taken by James Webb Space Telescope (center); and the James Webb Space Telescope's near-infrared view (right). (Image credit: NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI))
This "cat's head" would work perfectly in a witch's cauldron, glowing red "eyes" and all.
Just in time for Halloween, we have new, ghostly views of the Cat's Eye Nebula haunting the outer reaches of the cosmos.
What is it?
This nebula earned its name from its distinctive "cat's head" shape, which you can see on the left-hand side of these two images snapped by both the Hubble and James Webb Space Telescopes. In these new images, you can even see the cat's glowing red "eye," which experts suggest could be a young star trapped in the nebula's dusty clutches.
A visible light image of the Cat's Head Nebula captured by NASA's Hubble Space Telescope. The nebula's distinctive "cat's head" shape was formed over eons by intense ultraviolet radiation and winds of gases streaming from massive stars in the Carina Nebula. (Image credit: NASA, ESA, CSA, STScI; Image Processing: Joseph DePasquale (STScI))
Found about 7,500 light-years away from Earth, this star-forming region can be found within the larger Carina Nebula.
As the stars in the Carina Nebula continue to form, grow and evolve over time, the Nebula itself will change and eventually, this "cat's head" won't look much like a cat anymore. But for now, we can enjoy this vision of a domestic cat somehow depicted in this colossal tour of gas and dust.
Why is it incredible?
As a special Halloween treat, we have not one, but three new images of the cosmic cat's head.
In the snapshot captured by Hubble, we can see the nebula in visible light. This view shows the nebula as a brown pillar of dust embedded in a hazy, almost rainbow field of dust and gas. These colors are captured through Hubble's filters that can see the light coming from oxygen, hydrogen and sulfur and the light scattered by nebula dust.
JWST also took a look at this cat's head, observing the nebula in near- and mid-infrared wavelengths.
By looking at the same objects in space through different wavelengths and with different instruments and telescopes, we can uncover completely new and different details about these far-off celestial objects.
Earth would be terrifying if we celebrated Halloween every 11 hours, a possibility on a super-Earth investigated by the James Webb Space Telescope (JWST). That is, if this extrasolar planet, or exoplanet, wasn't so hellishly hot that no life could survive on its surface.
The exoplanet in question is the rocky lava planet TOI-561 b, located around 280 light-years away, which was discovered by NASA's exoplanet-hunting spacecraft TESS (Transiting Exoplanet Survey Satellite) in 2020. The planet is located so close to its star, TOI-561, that not only does it complete an orbit every 11 hours, but its surface temperatures reach in excess of 3,000 degrees Fahrenheit (1,800 degrees Celsius).
That is so hot that astronomers once believed that TOI-561 b couldn't possibly possess an atmosphere. With 37 hours of JWST observations covering nearly four full orbits of TOI-561, scientists have now found this horrific planet is buried in a reflective layer of vaporized silicate mineral clouds, the same family of compounds that make up quartz and sand.
"We measured how the planet's brightness and heat changed throughout its orbit," team member Lisa Dang of the University of Waterloo said in a statement. "This technique, known as a phase curve, revealed that the planet reflects a significant amount of light from its star, and that heat is being redistributed around the planet instead of only on the sunlit side. Together, these point to the presence of an atmosphere."
The hemispheres of lava super-Earth are day and night
The proximity of TOI-561 b to its star has another consequence. The planet is tidally locked, meaning it doesn't turn like Earth. Thus, TOI-561 b has one blisteringly hot "dayside" permanently facing its star, and a cooler "nightside" facing out into space in perpetuity.
Dang and colleagues investigated the fact that the bare rock of the dayside seemed to be cooler than should be expected. They theorized that missing heat could be carried around to the night side or the heat may be reflected away before TOI-561 b can absorb it.
By using the JWST to observe full orbits of TOI-561 b, the team was able to observe the planet's nightside for the first time. They found it isn't warm enough to account for all the heat missing from the dayside.
That means TOI-561 b must reflect roughly three-quarters of the starlight that hits it. That is comparable to the most reflective planet in the solar system, Venus, which reflects around 75% of incident sunlight compared to the 30% reflected by Earth.
The team determined that this high reflectivity is the result of clouds of silicate minerals, including silicon dioxide and magnesium silicate, forming on the planet's dayside and acting like sunscreen. These clouds could also help TOI-561 b hang on to an atmosphere.
A diagram shows that TOI-561 b and its two exoplanet siblings would fit well within the orbit of Mercury around the sun (Image credit: NASA)
Of course, the team can't yet be sure what this atmosphere is composed of. It could be a dense carbon dioxide fog like that seen on Venus, or it could be a blanket of sulfur dioxide like that of the most volcanic body in the solar system, Jupiter's moon Io. That would be the case if, like on Io, volcanic activity is replenishing the atmosphere of TOI-561 b.
"The next big question we will seek to answer is whether TOI-561 b's atmosphere resembles Venus or an extreme version of Io," Dang said. "Observing the planet at longer wavelengths with JWST could give us insights and help explain how a planet this hot has held on to an atmosphere for billions of years."
"Sometimes dead is better." Who can forget the immortal words of Jud Crandall, delivered by the incomparable Fred Gwynne in the 1989 film adaptation of Stephen King's Pet Sematary? Turns out Crandall could have been talking about somewhere just as otherworldly as the cursed Chumash burial ground at the heart of one of King's most terrifying works of fiction.
That's because astronomers have discovered two husks of two zombie planets shuffling through the gory remains of what was once their planetary neighbors around a long-deceased star, or white dwarf. The shattered planets were revealed by a clear gap in the debris around the white dwarf J1328−1450, located around 1,600 light-years away from Earth. One of the remnants is estimated to be no larger than the size of the average solar system asteroid, while the other is estimated to be between the size of the moon and the dwarf planet Pluto.
If this wasn't creepy enough, this haunting planetary system could be a grisly warning about the future of our own solar system after the inevitable death of the sun.
White dwarfs like the one at the heart of this system are formed when stars around the same mass as the sun run out of hydrogen in their cores. This means they can no longer fuse hydrogen into helium, the nuclear fusion process that provides the outward push that supports a star against the inward push of its own gravity.
As a result, the stars' cores collapse while the outer layers, where nuclear fusion is still proceeding, puff out. This so-called red giant phase can see stars increase their radius by many 100s of times. When it happens to the sun in around 5 billion years, our star will expand to consume the inner planets, including Earth.
The red giant phase ends when the outer layers disperse along with the wreckage of consumed planets, leaving a smoldering stellar core, now a white dwarf, surrounded by the disk-shaped remains of its outer layers and cannibalized planetary children. But this may not be the final death of all the planets that once orbited the now-dead star.
"We have known for some time that planets may survive beyond the transformation of their central star, but this is the first example of a complex system with a double debris disc and potentially two surviving planetesimals," research leader Nicola Gentille Fusillo, an astronomer at the Università degli Studi di Trieste, Italy, said in a statement.
Violent stellar death can't kill these two planetary Jason Voorhees
This system differs from others seen because of the large gap between the remarkably stable inner and outer rings. All previously known debris discs around white dwarfs have been surrounded by single, flat, rotating disks, not a double structure like this.
"The system is a rare glimpse of the violent, chaotic process by which a planetary system meets its end, and it hints that dead stars can have disc structures far more complex than previously realized," team member Gentle Fusillo of the Astronomical Observatory of Trieste said.
The team thinks that this unique double structure is evidence of planets that weren't completely vaporized during this white dwarf's red giant phase.
That means just like the residents and campers of Crystal Lake couldn't finish off Pamela Voorhees' baby boy, even an expanding star couldn't finish these two planets.
An illustration shows a massive black hole seed next to a standard stellar mass black hole (Image credit: Fortuna and Gentile Fusillo)
The team's observations, made with the Very Large Telescope (VLT), revealed the presence of calcium, oxygen, magnesium, and iron in the disk around the white dwarf. This indicates the destroyed planets had a composition similar to the rocky planets of the inner solar system.
The researchers also found evidence of a diversity of composition in the destroyed planets. The chemistry of the outer rings deviated from that of the inner rings, indicating that at least two of the consumed planets had very different compositions.
"The system therefore offers a remarkable glimpse of what the future of planetary systems, including systems like our own, might look like," Lagos-Vilches explained.
The team's research was published on Monday (Oct. 26) in the journal Nature Astronomy.
Iceberg A-81 escaping the Weddell Sea and drifting near the edge of South Georgia's underwater shelf. The image was captured on Oct. 20, 2026. (Image credit: NASA Earth Observatory/Michala Garrison)
An iceberg has quickly escaped from the Weddell Sea in Antarctica, on its way to an icy new destination.
What is it?
As captured by a satellite in orbit, the Antarctic iceberg A-81 has quite quickly (for an iceberg) parted ways from its icy home, breaking off to drift toward a shallow underwater shelf in Georgia.
The 600-square-mile (1,550-square-kilometer) iceberg first broke off from the Brunt Ice Shelf in January of 2023. Now, generally speaking, giant icebergs don't travel that fast. But In just three years, this massive iceberg has traveled 1,400 miles (2,300 kilometers) north of the Brunt Ice Shelf. For an iceberg, that's really fast.
Over this time period, the iceberg drifted through the Weddell Sea in Antarctica's Southern Ocean before reaching the tip of the Antarctic Peninsula, floating further into the Scotia Sea and then finally now reaching the edge of a remote island in South Georgia.
In this satellite snapshot captured on Oct. 20, 2026, we can see the iceberg in its current location near an underwater shelf off the coast of South Georgia. While it isn't abnormal for icebergs like A-81 to break off from larger ice shelves, Brunt has recently had multiple large icebergs break off one quickly after the other, according to a statement from NASA.
Why is it incredible?
This image was captured by the MODIS (Moderate Resolution Imaging Spectroradiometer), an instrument on board NASA's Terra satellite.
Earth-observing satellites like Terra keep a close eye on changes on our home planet. In addition to this image, observations from Terra have showed how the iceberg has traveled over the last few years.
With satellites like Terra, scientists can keep a close eye on these changes in Antarctic ice, which is becoming increasingly important as climate change continues to progress across the globe, affecting everything from Arctic ice to sea levels rising, worsening natural disasters and more.
The powerful Vera Rubin Observatory has spotted what seems to be a dwarf planet circling the sun in the frigid depths beyond Neptune.
The icy object, known as 2026 ED138, is likely between 600 and 1500 kilometers (373 to 972 miles) wide, scientists say. It's therefore probably big enough to be sculpted into a sphere by its own gravity — a key characteristic that separates dwarf planets from asteroids and other small space rocks.
And if 2026 ED138 is indeed a dwarf planet, that's a pretty big deal, as astronomers have confirmed just five of them to date: Pluto, Ceres, Eris, Haumea and Makemake.
An illustration of the solar system showing the orbital pathway of newly discovered dwarf planet candidate 2026 ED138 (ED138). (Image credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA/R. ProctorImage Processing: M. Zamani (NSF NOIRLab)Orbit data provided by the IAU Minor Planet Center (MPCorb catalog), funded by NASA PDCO and the Tamkin Foundation.Star map: NASA/Goddard Space Flight Center Scientific Visualization Studio. Gaia DR2: ESA/Gaia/DPAC)
2026 ED138 was discovered by Matthew Holman, who works at the Center for Astrophysics | Harvard & Smithsonian (CfA). The big moment came on Oct. 13, when Holman was running previously collected Rubin data through a search code that he developed with his CfA colleague Kevin Napier.
That search revealed a mysterious object beyond Neptune's orbit. Despite its immense distance from the sun, this body was relatively bright, suggesting that it's larger than the average trans-Neptunian object.
"My first reaction was one of excited disbelief," Holman said in a statement on Tuesday (Oct. 27), the day the discovery of 2026 ED138 was announced. "Objects like this are very rare, so I immediately started checking whether I or the code had done something wrong."
Those checks involved a thorough search through Rubin's catalog. And that catalog is pretty heft, even though Rubin is a pretty new scope.
This image shows the orbital pathway of the newly discovered dwarf planet candidate 2026 ED138, as observed by the NSF-DOE Vera C. Rubin Observatory. This image is a composite of multiple images captured by Rubin between March 4 and July 11, 2026 at intervals indicated by the teal circles. ED138 is visible at the center of each circle. (Image credit: NSF-DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA. Acknowledgement: Image Processing: M. Jurić (UW), D. de Martin & M. Zamani (NSF NOIRLab))
The Vera Rubin Observatory sits atop Cerro Pachón, an 8,799-foot-tall (2,682 meters) mountain in northern Chile, and features a primary mirror 28 feet (8.4 m) wide. The scope achieved first light in April 2025 and began its main project, the 10-year-long Legacy Survey of Space and Time (LSST), in June of this year.
During the LSST, Rubin images the entire southern sky every few days using a 3.2-gigapixel camera, the largest digital camera ever built for astronomy. This work creates a high-resolution time-lapse "movie" that can reveal a great deal about the cosmos.
For example, astronomers think Rubin will shed light on dark energy and dark matter, the mysterious stuff that together makes up most of the universe's mass-energy budget. Its observations will also serve as a solar system inventory, helping scientists map out our cosmic backyard like never before. Rubin has already discovered more than 11,000 new asteroids, for example, with many more surely to come.
The LSST inventory will likely include a number of new dwarf planets as well — including, possibly, 2026 ED138. For the object definitely exists: Holman and his colleague Mario Jurić, who works at the University of Washington and serves as Rubin Solar System Lead Scientist, found that Rubin spotted 2026 ED138 30 separate times on 20 nights between March 4 and July 11 of this year.
And further digging revealed that the Dark Energy Camera (DEC), an instrument on the Víctor M. Blanco 4-meter Telescope at the Cerro Tololo Inter-American Observatory in Chile, also spotted 2026 ED138. Indeed, DEC observations of the object go all the way back to 2016.
A mosaic of images captured by the NSF-DOE Vera C. Rubin Observatory of the newly discovered dwarf planet candidate 2026 ED138. Its distance from the sun places it beyond the orbit of Pluto, and initial analysis indicates that it may be among the largest and brightest bodies scientists have discovered in this region of the solar system. (Image credit: NSF-DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA. Image Processing: M. Jurić (UW), D. de Martin & M. Zamani (NSF NOIRLab))
The data show that 2026 ED138's orbit is tilted by about 25 degrees relative to the plane of the solar system. It therefore likely had a gravitational interaction with Neptune, which knocked it off kilter, scientists say.
2026 ED138 currently lies about 46 astronomical units (AU) from the sun. (One AU is the Earth-sun distance — about 93 million miles, or 150 million kilometers). This puts it beyond Pluto's average distance from the sun, which is roughly 40 AU.
There is still much to learn about the object, however. For example, we won't know whether or not it's a dwarf planet until astronomers nail down its size. And that will require observations in infrared light, the range of wavelengths that NASA's James Webb Space Telescope is optimized for.
So stay tuned: There's doubtless more news about 2026 ED138 coming, and Rubin could turn up more worlds like it in the coming months and years.
"If confirmed as a dwarf planet, ED138 would join a very small family of worlds," Holman said. "Rubin will image the whole southern sky again and again for 10 years, so any others hiding in the places earlier surveys skipped are now within reach."
Scientists have long known that when two black holes collide, they merge to create a more massive black hole. These events are so violent that they set the very fabric of space ringing with ripples called gravitational waves.
Now, new research suggests that the opposite may happen, too: single black holes may be able to split in two. But this can only happen if that progenitor black hole is spinning at maximum possible speed. That speed prevents the black holes from immediately falling back on each other.
There are physical laws in place that would usually prevent black holes from splitting in two; the team behind this research investigated whether there are conditions in which these laws can be temporarily bypassed.
One of the key aspects of physics that prevents black holes from bifurcating comes from thermodynamics. Black holes possess a characteristic called "entropy," which is essentially a measure of disorder within a system.
Imagine a toddler's crayon box. When entropy is low, the crayons are neatly arranged by color. As entropy is increased, the crayons are scattered and no longer in order. To get the crayons back in order, it requires a parent to put energy into the system and neatly reorder the crayons. In other words, the entropy of a system can't be reduced without some intervention and energy being added from outside that system. Parenting would be a little easier if it could.
A black hole splitting in two would represent a decrease in entropy, strongly disfavored by the laws of thermodynamics, but only if the black hole is not rotating. The situation could be different for a rapidly rotating black hole.
This team of scientists found that a loophole exists for such a black hole.
"The two resulting black holes must also be able to separate rather than immediately fall back together," team member Francesco Sannino of the University of Naples Federico II in Italy said in a statement. "When we include this requirement, the window largely closes again, except possibly for black holes rotating close to their maximum possible rate."
Black hole trousers?
The team calculated just how such a black hole split could occur, finding that the division of the black hole's outer boundary, or "event horizon," proceeds in an oddly trouser-like shape, with one resulting black hole slipping down each "leg."
They termed this "pair-of-pants topologies."
The researchers also determined that a split is more likely to take place if one of the resultant black holes is considerably smaller than its newly born twin.
An illustration of a black hole splitting in two, creating the shape of pants. (Image credit: Francesco Sannino)
"We cannot yet give a single probability for a black hole to split. It depends on how gravity behaves beyond Einstein's theory, and we are working to quantify this," Sannino said. "We expect small primordial black holes to be more prone to splitting than much larger astrophysical black holes."
Sannino added that such black hole splits may be detectable in high-energy light called gamma-rays.
"We may detect a split indirectly: gamma-ray telescopes such as Fermi-LAT can search for signals from tiny black-hole fragments that might form during mergers," the researcher concluded.
The team's research was published on Oct. 22 in the journal Physical Review D.
Scientists are still learning about a cosmic "string of pearls," a unique celestial relic left by a supernova explosion that humanity witnessed around 850 years ago.
That is thanks to the most detailed observation of the dandelion-shaped chains of gas and supernova debris that comprise Pa 30, the only supernova remnant of its type observed in the Milky Way. What makes Pa 30 even more unique is that it has a rare "zombie star" at its heart.
Supernovas like the one that created Pa 30 are called Type Ia supernovas; they happen when a dead star called a white dwarf overfeeds on a companion star like a cosmic vampire. This overfeeding triggers a runaway nuclear explosion that usually destroys the white dwarf. But on rare occasions, the supernova doesn't completely destroy the star, and a shattered stellar body remains, called a zombie star. These events are called Type Iax supernovas.
Pa 30 was first identified in 2013 by a citizen scientist in 2013, but scientists soon linked it to a cosmic explosion recorded independently in the year 1181 in Japanese, Chinese, and Arabic historical documentation. That makes this one of only five supernovas seen before the invention of the telescope.
"Reliable historical records of stellar explosions extend back only about a thousand years. For all we know, there might well be similar remnants still lurking in the dark in our own galaxy," team member Ilaria Caiazzo, assistant professor at the Institute of Science and Technology Austria (ISTA), said in a statement.
"Today, we are lucky to study an intriguing object we know was observed by astronomers who made three independent historical records of the event centuries before the invention of the telescope."
Solar system-sized pearls
Pa 30 is a good laboratory to study supernovas because, at around 7,500 light-years away, it is relatively close to Earth on cosmic scales. For instance, the heart of our galaxy is around 26,000 light-years away. "We can see this much detail because of Pa 30's proximity to Earth," said Caiazzo. "This proximity makes Pa 30 uniquely valuable for study."
It is also an important subject of study because it is the only supernova remnant in which we can see a zombie star.
Using the Gemini North telescope, Caiazzo and colleagues zoomed in on Pa 30, discovering knots along the strands of gas radiating out from the site of the cosmic explosion, like pearls on a string.
These pearls are each wide enough to encompass the orbit of Neptune, the most distant planet from the sun, ten times over.
"The planetary region of our solar system could fit in each knot about ten times with room to spare," said Caiazzo. "The knots are quite strikingly uniform. We are excited to try to model them."
The team also discovered that the zombie star sits almost perfectly at the heart of Pa 30. When these cosmic explosions happen, they should provide any debris, including zombie stars, with a kick. The fact that this "living dead" star still sits dead center of this wreckage suggests that when this explosion happened, it was roughly symmetrical and the kick was relatively light.
"Explosions conserve momentum. If the explosion itself was perfectly symmetric, the ejecta should also be symmetric, and the surviving star should not receive a substantial kick," Caiazzo said. "We were able to measure a precise upper limit of the remnant star's transverse kick speed, showing that it was surprisingly small. We practically don't see the star moving away at all."
An image of the nebula Pa 30. (Image credit: Robert Fesen)
While there are still many mysteries surrounding Pa 30 and its zombie occupant, one of the most exciting prospects emerging from this research is the possibility it will help identify the wreckage of other Type Iax supernovas in our galaxy.
"While we can see Type Iax supernovas in distant galaxies as point sources of light, resolving the remnants of such explosions is only possible in our own galaxy and in very few nearby ones," Caiazzo concluded. "Eventually, we plan to use Pa 30's distinctive properties to search the Milky Way and nearby galaxies for similar objects."
In 1927, Norwegian civil engineer and amateur radio operator Jørgen Hals made an unusual discovery: while monitoring transmissions from a shortwave radio station in Eindhoven, The Netherlands, he began hearing odd, "delayed" radio echoes, arriving approximately three seconds after the original transmissions, that sometimes accompanied the station's signals.
"From where this echo comes I cannot say for the present," Hals wrote of his peculiar discovery, adding that he could "only confirm that I really heard it."
Almost a century after Hals' discovery, the exact cause of this unusual phenomenon — known today as long delayed echoes, or LDEs — remains unknown. Their baffling nature has prompted a range of potential explanations, most of which focus on a variety of unexplained natural phenomena occurring in Earth's atmosphere. However, a few more far-out possibilities, including potential evidence of extraterrestrial technology, have also been considered.
What do we know?
A curious discovery
The enigma of long-delayed echoes has perplexed scientists since their initial detection by Hals, who at the time reported his odd findings to Norwegian physicist Carl Størmer. This prompted an investigation by Størmer with physicist Balthasar van der Pol, during which the duo was able to reproduce the phenomenon but were unsuccessful in determining its cause.
Since those early observations, ongoing reports of long-delayed echoes have continued to be recorded. Under normal conditions, radio echoes occur whenever a radio signal reflects or "bounces" off an object, although other conditions such as signals traveling through a delayed path can also cause echoes to occur.
Long delayed echoes, by contrast, are generally characterized by radio signals that return after more than 2.7 seconds following their original transmission, although the terminology has sometimes been applied more broadly.
Complicating investigations into this unusual brand of radio phenomena over the years has been their unpredictable nature, along with significant reported variances in the timing and nature of the delays, which has made it difficult for researchers to narrow down a single cause.
Possible explanations
Despite the challenges presented by this unique class of space mysteries, there are several theories that have been put forward over the years about what could cause long-delayed echoes.
In the mid 1980s, researchers R. J. Vidmar and F. W. Crawfordconducted experiments in Alaska that aimed to detect long-delayed echoes, which built on earlier research they published involving possible detections in 1970. According to their findings at the time, Vidmar and Crawford hypothesized that radio signals could be captured between ionized layers in the atmosphere and "guided" over long distances.
More recently, University of Oslo researcher Sverre Holm has advanced a similar concept that he callsmagnetospherically ducted echo (MDE), in which radio waves may become trapped within electrically charged regions of Earth's upper atmosphere and guided along magnetic field lines extending far into the magnetosphere. Under certain conditions, these signals may reach as far away as the opposite hemisphere before they are "bounced" back toward Earth, resulting in the delayed echo effect.
According to Holm, MDE "is the best understood mechanism for long delayed echoes"out of five promising explanations he outlines, adding that based on the MDE model, such long delayed echoes "can be predicted to what seems like about 5 ms accuracy using a simple model for the magnetic field lines."
Still, one problem that arises involves the relatively short delays associated with this mechanism, which may not necessarily account for the much longer, multi-second echoes reported in some historical observations. Since radio waves travel at close to the speed of light, a signal could theoretically cover distances equivalent to the planet's circumference several times in a single second. While this doesn't prove the signals actually followed such paths, it does imply that some of the reported instances of long-delayed echoes might correspond to dozens of journeys around the planet.
Speaking with Space about historical cases involving much lengthier long-delayed echoes, Holm was clear in expressing that the MDE theory also has its limitations.
"In my view," Holm told Space in an email, "Magnetospheric Duct Echoes cannot [account] for those historical LDEs at all."
Earth is surrounded by a giant magnetic bubble called the magnetosphere, which helps protect the planet from radiation released by the sun. (Image credit: NASA)
To illustrate this, Holm points to two primary differences. First, the historical echoes were detected at approximately 9.55 MHz, well above the 1–4 MHz frequency range typically associated with MDEs. Additionally, historical LDEs reportedly exhibited delays ranging from 3 to 30 seconds, whereas MDEs generally produce delays of only a few hundred milliseconds.
By contrast, "MDES are only a few hundred milliseconds," Holm explained, meaning that they cannot account for all the characteristics of the earlier historic observations of long-delayed echoes.
Other theories that might be capable of filling some of the gaps in the long-delayed echo mystery include the idea that electromagnetic radio energy could be coupled into slower plasma-wave "modes" while traveling through Earth’s upper atmosphere, which, according to Holm’s review of the earlier work by Vidmar and Crawford, could potentially create much longer delays than ordinary radio propagation would allow.
After this proposed coupling into a plasma-wave mode, the signals may be converted back to ordinary electromagnetic signals and bounced back down to lower levels of Earth's atmosphere. Finally, a similar line of investigation has looked at whether clouds of plasma originating from the sun might also be able to produce the well-characterized echo effect.
What remains unknown?
Extraterrestrial origins?
Although scientific research has identified several promising explanations for long-delayed echoes, the mysterious nature of these events has also inspired more speculative theories over the decades, including some involving the search for extraterrestrial intelligence.
This unique dimension to the LDE mystery has its roots in the theories of Australian physicist Ronald Bracewell, whowas the first to propose the idea that autonomous interstellarprobes might be used by an advanced civilization as a means of establishing contact.
According to Bracewell, the initiators of such a hypothetical contact scenario might choose to reveal their presence by intercepting and re-transmitting radio signals rather than engaging in direct communication. Carl Sagan explored a similar concept in his novel "Contact", in which transmissions from the 1936 Olympics — the earliest broadcast signals to leave Earth's ionosphere — are intercepted and rebroadcast back to Earth as a data-encoded message originating from the Vega system.
However, more than a decade before the publication of Sagan's famous novel, Scottish writer Duncan Lunan attracted international attention for his 1973 article in the journal "Spaceflight"outlining his belief that he had successfully decoded a radio message dispatched from an extraterrestrial probe. According to Lunan, the initial detection of this "hidden" alien signal had taken place decades earlier in 1927, with the famous discovery of long-delayed echoes by Jørgen Hals.
Lunan's theory essentially went like this: an extraterrestrial civilization in the Epsilon Boötis system had deployed a hypothetical autonomous communications probe (known as a Bracewell probe) to Earth in the distant past, which had been comfortably orbiting in one of Earth's gravitationally stable Lagrange points for thousands of years.
Using the original long-delayed echo detections from Hals and Størmer's research decades earlier, Lunan placed the transmitted sequence on a vertical axis, while placing the recorded echo delay time on a horizontal axis, revealing what he believed to be a view of the constellation Boötesas it might have looked 15,000 years ago — right around the time the suspected space probe would have been dispatched to Earth.
A visualization of NASA's Juno probe orbiting Jupiter. Some scientists have proposed that distant alien civilizations might send autonomous interstellar probes to our solar system as a means of establishing contact. (Image credit: NASA/JPL-Caltech)
Despite Lunan's imaginative theory, an alternative hypothesis proposing a natural cause behind long-delayed echoeswas subsequently advanced by Anthony Lawton, which ultimately garnered an award from the British Interplanetary Society. By 1976, Lunan had withdrawn his ideas in an article published in the Journal of the Society of Electronic and Radio Technicians, although he would eventually revisit a version of the theory in the 1990s.
The mystery continues
While few modern researchers seriously consider extraterrestrial hypotheses to explain long-delayed echoes, these obscure phenomena remain intriguing, even as ongoing research sheds light on their possible causes. Explanations such as Sverre Holm's magnetospherically ducted echo model offer promising mechanisms that may account for at least some of these unusual signals, although important questions remain unanswered.
For now, long-delayed echoes serve as a reminder of the challenges of studying electromagnetic phenomena, and how even seemingly familiar aspects of our physical world can harbor mysteries that resist straightforward explanations, even after nearly a century of investigation.
The James Webb Space Telescope's stunning view of the emission nebula N159 in the Large Magellanic Cloud. (Image credit: ESA/Webb, NASA & CSA, E. Sabbi, M. Zamani (ESA/Webb)Acknowledgement: M. H. Özsaraç)
The NASA/ESA James Webb Space Telescope has captured a breathtaking view of a majestic star-forming region shining 161,000 light-years from Earth in a satellite galaxy of the Milky Way known as the Large Magellanic Cloud.
What is it?
The deep-space image reveals a 230-light-year-wide swathe of the glowing emission nebula N159, threaded with denser filaments of reddish molecular hydrogen that hide countless energetic young stars.
Ghostly blue clouds of ionized hydrogen gas (H II) glow in the center of the image, having been energized by the ultraviolet radiation pouring out from nearby stars, whose winds helped create the chaotic structure of the vast stellar nursery.
N159 is estimated to be less than 3 million years old, making it one of the youngest star-forming regions in the Large Magellanic Cloud. It also has a markedly different composition than the stellar nurseries that spawn stars in our Milky Way, boasting a lower metal content that could mirror environments that existed in the early universe.
By pointing JWST at N159, astronomers open a window to the distant past. They can compare the characteristics of stars at varying stages of evolution, including pre-main-sequence stars that are still in the process of forming, or accreting from the vast interstellar cloud.
Want to know more?
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Black holes more massive than entire galaxies are not a major component of the mysterious dark matter that's thought to make up most of the matter in the cosmos, a new study finds.
For decades, to explain why galaxies do not spin apart at the speeds at which they whirl, scientists have suggested the existence of an unseen substance known as dark matter, whose gravitational pull helps keep galaxies together. Dark matter is thought to make up about five-sixths of all matter in the universe.
Much remains unknown about dark matter, however — including whether or not it actually exists. Black holes make good potential contenders for dark matter, since they are extremely massive and are difficult to spot in the dark depths of space.
In the new study, researchers investigated whether dark matter could be made of "stupendously large black holes," ones with masses greater than 100 billion times the mass of the sun. Stupendously large black holes greater than 1 million billion to 10 million billion suns in mass would be heavier than entire galaxies.
So far, astronomers have not detected any stupendously large black holes — currently, the largest black hole known may weigh about 36 billion suns. Since researchers have not seen any even after looking at many galaxies, the new study noted they cannot make up all of dark matter — but team members wondered if the exotic objects still might constitute a significant portion of the puzzling substance.
Often, dark matter is thought of "as a fine dust spread everywhere," study co-author Christopher Gerlach, a theoretical physicist at the Mainz Institute for Theoretical Physics in Germany, told Space.com. However, if dark matter is packed into a handful of gigantic objects such as stupendously large black holes, "the universe becomes grainy on very large scales. And we can check that."
Specifically, the scientists analyzed the light from the dawn of the universe, study co-author Yann Gouttenoire, a theoretical physicist at the Mainz Institute for Theoretical Physics, told Space.com.
For the first 380,000 years after the Big Bang, the cosmos was filled with a hot plasma in which light was trapped. Eventually, the expansion of the universe let the cosmos cool enough for the plasma to largely dissipate and form atoms. This in turn let light shine freely, "and that light is still arriving today," Gerlach explained. "We call it the cosmic microwave background, a snapshot of the infant universe covering the whole sky."
The temperature of the cosmic microwave background "varies from place to place by about one part in 100,000," study co-author Antonio Iovino, a theoretical physicist at New York University, Abu Dhabi, in the United Arab Emirates, told Space.com. "That pattern tells us how matter was spread back then."
An illustration of a supermassive black hole against a background of dark matter. (Image credit: Robert Lea (created with Canva))
Analyzing the cosmic microwave background revealed it is not grainy the way stupendously black holes would have made it. "So these black holes can't be a significant part of the dark matter," Nicholas Leister, a theoretical physicist at the Mainz Institute for Theoretical Physics, told Space.com.
The researchers cautioned that the new findings do not suggest that stupendously large black holes cannot exist, only that they do not make up a major fraction of dark matter. They added that another candidate for dark matter — relatively tiny black holes the size of asteroids — might potentially exist. They are now investigating whether they can rule out such itty-bitty black holes as a major constituent of dark matter.
The scientists detail their findings in a study that will be published Oct. 26 in the journal Physical Review Letters.