Mars isn’t dead — recent volcanic activity reveals it’s just sleeping

Scientists have long suspected that Mars is geologically "dead," but new spacecraft observations suggest the Red Planet's volcanoes are merely sleeping.

That means that Olympus Mons, the extinct Martian volcano that at around 16 miles (26 kilometers) above the surrounding Martian plains is the largest mountain in the solar system, may in fact be a slumbering giant.

The observations were made with the European Space Agency (ESA) mission ExoMars Trace Gas Orbiter (TGO) as it studied volcanic fissures along the Alba Mons region of the Red Planet. Alba Mons is in the Tharsis region of Mars, the same area that is home to Olympus Mons. While the latter is the tallest volcano in the solar system, at 374 miles (600 km) across, about the size of Arizona, the Alba Mons region is the largest volcano when considering surface area.

TGO detected gas containing hydrogen chloride making its way to the surface of Mars through the Alba Mons fissures. The same gas is commonly found escaping from magmatic vents on Earth, with the compound coming from hot magma beneath the surface. Detecting it on Mars is a sign of dormant Martian volcanism.

Orbital imagery had previously shown some volcanoes appear to have been active within the last few million years, and seismometers have detected the rumbling of "marsquakes," both implying the Red Planet is volcanically active. However, eruptions and lava flows have been conspicuous by their absence.

"Our findings suggest that Mars has retained enough internal heat to support volcanic activity until recently, and possibly still does," team co-leader and scientist at the Space Research Centre of the Polish Academy of Sciences, Daniel Mège, said in a statement sent to Space.com via email. "The TGO was able to find the smoking gun. It was like looking for a needle in a haystack."

Evidence of dormant Martian volcanism is rising

Mège and colleagues were first alerted to something strange happening on Mars when they noticed spikes of hydrogen chloride during Martian summer and on the northern hemisphere of the Red Planet. That is both a time and place at which hydrogen chloride shouldn't be detected.

The gas usually peaks in the northern hemisphere during winter on Mars, disappearing in the summer. This variation is connected to the water and dust cycle on Mars. An exception to the rule occurs over volcanic fissures on the flanks of the Alba Mons volcano, in early summer.

The TGO followed up on this by detecting fresh and narrow fissures, in some cases hundreds of feet long, in the Alba Mons region. A clear sign of volcanism.

"It's truly amazing that it spotted a handful of molecules from a perhaps intermittent source, whilst moving continuously along its orbit to monitor the whole Martian atmosphere," Mège said.

An animated gif of the Arsia Mons Elongated Cloud emerging from the morning terminator.

An animated gif of an Elongated Cloud over the Alba Mons. (Image credit: ESA/GCP/UVP/EHU Bilbao.)

The team thinks that these gases have been rising from the interior of Mars during the Martian winter, becoming blocked by ice. When this ice sublimates, changes directly from solid to gas, during summer, the gas is released, prompting spikes in hydrogen chloride seen by the TGO.

"Looking at the spatial distribution of the seeping, it became instantly obvious to me that there was something volcanic behind it, but it had to be demonstrated," said Mège. "A huge part of the work consisted of examining all the possible chemical processes going on in the Martian atmosphere.

"We needed to be rigorous, critical and creative to explain the presence of hydrogen chloride. The data were complex, but also excellent brain food."

Implications for life on Mars?

Mège and colleagues theorize that the gas is connected to "volcanic plumbing" in the form of a dormant magma chamber under the surface of Mars.

Regions like this could become hotspots (pun not intended) in the search for life on Mars. That is because magmatic gases like hydrogen chloride would have been more abundant in the past, creating a thicker Martian atmosphere and warmer climate.

Not only would this have led to liquid water covering much of the Martian surface, but when lava bubbled through the Martian crust and met groundwater, warm habitable niches ideal for microbial life could have been forged.

"Looking for Martian life in the seeping fissures of the Alba Mons region would make a lot of sense. If hydrothermal systems are active, they could contain the ingredients and energy needed for microorganisms to develop, and shield microorganisms from the hostile and changing environment above the surface," Mège concluded.

The team's research was published in the journal Science Advances on Wednesday (Nov. 4).

James Webb Space Telescope uncovers new clues about the origins of ‘interstellar invader’ comet 3I/ATLAS

Using the James Webb Space Telescope (JWST), scientists have found that the interstellar comet 3I/ATLAS was built from tiny grains of ice mixed with dust that are quite different from the solar system’s comets.

These ice grains do, however, bear striking similarities to some icy bodies located at the edge of the solar system, beyond the orbit of Neptune, so-called trans-Neptunian objects (TNOs).

3I/ATLAS was discovered entering the solar system in the summer of 2025. It was only the third object found entering the solar system from farther afield in the Milky Way after 1I/'Oumuamua, seen in 2017, and 2I/Borisov, detected in 2019. This meant the interstellar comet offered a rare chance to glimpse the conditions under which such bodies form in other star systems. Thus, the JWST was quickly on the trail of 3I/ATLAS.

"We designed [JWST] to be ready the moment an active interstellar comet was found and to follow it over time," Martin Cordiner of NASA’s Goddard Space Flight Center and the Catholic University of America said in a statement.

Cordiner leads the JWST program to study objects such as 3I/ATLAS, and he is a co-author on a new research paper describing some of the findings.

The unclear origins of 3I/ATLAS

Researchers know that 3I/ATLAS wasn't born in the solar system, but nobody knows around which star 3I/ATLAS formed. What scientists are more sure of is the fact that this interstellar comet was produced within a planet-forming disk of gas and dust around a young star, possibly as long ago as 10 to 12 billion years. That's over twice the age of our solar system. It was then ejected from its home system somehow and left to wander interstellar space before encountering our solar system.

Like the familiar comets in our solar system, 3I/ATLAS is composed of grains of ice less than a micron – a millionth of a meter – in size. When the surface of the comet is warmed by the sun, gas erupts outwards, carrying ice grains into the cloud of ice and dust surrounding the comet, its coma, and its tail, where JWST can detect them.

When viewed spectroscopically, the water-ice in comets native to our solar system creates a strong absorption line in a comet’s spectrum at a wavelength of three microns, as well as less-prominent absorption lines at 1.5 and two microns.

Comparison between ice in the interstellar invader comet 3I/Atlas and icy bodies in our solar system.

Comparison between ice in the interstellar invader comet 3I/Atlas and icy bodies in our solar system. (Image credit: SwRI/Silvia Protopapa/NASA/ESA/CSA JWST)

Yet when the JWST’s Near-Infrared spectrograph (NIRSpec) instrument viewed 3I/ATLAS three times between August 2025, before its closest approach to the sun, and after closest approach in April 2026, scientists found the 1.5- and two micron absorption lines were missing, though the three-micron line remained strong.

"That combination was a puzzle," research lead author Silvia Protopapa of the South-west Research Institute said. "The strong three-micron band points to water-ice in the coma, but the weak or absent shorter-wavelength bands suggest the ice is not in the form we usually see in solar system comets."

The JWST's muddy 3I/ATLAS findings

Whenever presented with an unusual observational signature such the JWST delievered for 3I/ATLAS researchers turn to modeling to find the physical characteristics that best fit the spectrum.

The modeling suggested to Protopapa’s team that 3I/ATLAS was composed of sub-micron grains of dirty water-ice, rich in dust. In comparison, the grains from the solar system’s indigenous comets are much cleaner, with almost pure water-ice relatively uncontaminated by dust.

"What seems to set [3I/ATLAS’ grains] apart is how much dust is mixed into the ice," said Protopapa. "Those grains hold clues to the conditions where the comet was born."

Three boxes contain a glowing center that in the left box is blue, the middle box is yellow, and the right box is red.

The chemical composition of 3I/ATLAS (Image credit: NASA, ESA, CSA, STScI, Martin Cordiner (CUA, NASA-GSFC); Image Processing: Alyssa Pagan (STScI))

Comets are made of primordial material found in the planet-forming disk of gas and dust that surrounds a young star, and therefore the composition of comets can provide a window into the conditions in which planets form.

Whereas solar system comets tell us about the birth of Earth, an interstellar comet can tell us about conditions in which planets formed around another star, and how similar or dissimilar those conditions were to the birth of the solar system.

Yet comets are not the only icy remnants that date back to such primordial times. There are various families of bodies in the outer solar system, and 3I/ATLAS’ spectrum bears a resemblance to the spectrum of some medium-sized TNOs that are rich in carbon-dioxide ice and organic compounds (organic meaning containing carbon atoms). Indeed, in a separate 2025 study led by Cordiner, the JWST found 3I/ATLAS to have one of the greatest abundances of carbon dioxide ever seen in a comet.

TNOs are sizable bodies that are located far beyond the orbit of Neptune, The TNOs in question would have formed in a different part of the Sun’s protoplanetary disk than most comets and their composition reflects that.

A purple and blue disk composed of rough concentric circles

Artist's illustration of a planetary disk, a region of dust and gas where planets form. The zoom-in insert displays carbon monoxide molecules in the ice phase. (Image credit: M.Weiss/Center for Astrophysics | Harvard & Smithsonian)

On the other hand, the results imply that 3I/ATLAS was formed around its star of origin from similar icy material to that which produced some of the TNOs in our solar system, showing that the building blocks of planets around other stars share a common range of properties with the building blocks that formed our solar system. Indeed, 3I/ATLAS could even be a fragment of a TNO-like body that was shattered in a collision.

"At first glance, 3I/ATLAS looks different from the icy comets we know," said Protopapa. "But when we placed it alongside distant icy worlds in our own solar system, it no longer looked out of place.

"This suggests that the icy building block of planets, here and around other stars, may share ice in the form of tiny, micron-scale grains, ranging from relatively pure ice to ice mixed with dust, with 3I/ATLAS toward the dusty end."

What this tells us is that these sub-micron-sized icy grains must form first in planet-forming disks, to then be incorporated into large bodies such as comets and protoplanets.

The team's findings were published on Monday (Oct. 26) in The Astrophysical Journal Letters.

A rainbow of ancient rocks on Mars | Space photo of the day for Nov. 2, 2026

Rocks on Mars

In this image, we can see a colorful view of an ancient, rocky Martian hill. (Image credit: NASA/JPL-Caltech/UArizona)

This rainbow-hued rocky plain looks like the landscape of an alien world. And, it turns out, it is.

What is it?

In this image, we can see an ancient, rocky hill on Mars. In the Red Planet's Southern Highlands, this alien terrain is chock-full of minerals, which we can see clearly defined in this color-enhanced view of the region.

This image was snapped by the HiRISE camera aboard NASA's Mars Reconnaissance Orbiter (MRO), which has been studying the planet's surface, atmosphere and climate since arriving in Martian orbit in March 2006.

But this isn't exactly what the surface of the planet would look like through our eyes; the image is color-enhanced. Why would scientists take a natural-color image and turn it rainbow? Doing so enhances the slight color differences in these rocks, allowing researchers to pick out the different minerals.

Why is it incredible?

As pointed to above, enhancing colors in scientific images can be an incredibly useful tool for exploration.

For instance, in this image, the blue- and green-toned rocks could be full of minerals like pyroxenes and olivine, according to scientists analyzing the image. And they think that the yellow, orange and red patches may contain minerals formed by past interactions with liquid water.

By exploring the mineral content of rocks like this, researchers can peel back the layers of history within the Martian bedrock. The discovery of certain minerals, for example, can show that water flowed on Mars long ago, pointing to potentially habitable conditions.

So, as we can see, this striking rainbow image isn't just a beautiful landscape; it's also hiding serious clues to Mars' history.

Satellites watch an escaping Antarctic iceberg | Space photo of the day for Oct. 28, 2026

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.

Astronomers found a mysterious object beyond Neptune, and it could be a new dwarf planet

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.

concentric white lines on a starry background. the outermost circle has a label that reads

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.

image of star-filled sky with the orbit of a distant newfound object superimposed over it in greenish-blue

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.

mosaic of 10 images showing closeups of patches of a starry sky, which is seen in an image on the left

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."

What causes mysterious long delayed radio echoes in Earth’s atmosphere?

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. Crawford conducted 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 calls magnetospherically 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."

yellow gases swirl near a blue orb surrounded by a blue, wispy cloud

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, who was the first to propose the idea that autonomous interstellar probes 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 Boötes as it might have looked 15,000 years ago — right around the time the suspected space probe would have been dispatched to Earth.

a spacecraft shaped like a three-pronged star above a striped planet

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 echoes was 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.

Australia’s bizarre ‘Spider Crater’ seen from orbit | Space photo of the day for Oct. 22, 2026

An image from space of spider crater on Earth.

A satellite image of "Spider Crater" in Western Australia. (Image credit: NASA Earth Observatory image by Michala Garrison, using Landsat data from the U.S. Geological Survey)

From the dangerous Sydney funnel-web to the common huntsman, Australia is home to its fair share of spiders. It even has a crater shaped like one.

What is it?

One stretch of the vast Western Australia wilderness is imprinted with a curious crater, which likely formed after a meteor impact hundreds of millions of years ago. Geologists think the spider-like pattern in the crater's center was created when its floor rebounded following the initial impact, NASA has said.

In the hundreds of millions of years since the initial impact, erosion has continued to carve this formation into its current, signature shape. Complete with "legs," the planetary imprint has earned its name Spider Crater.

This image shows the impact structure in its entirety, which stretches 8 by 7 miles (13 by 11 kilometers) in full, with the central "spider" piece measuring 2.5 miles (4 km).

Why is it incredible?

In this image, we can see this "spider" from space. This snapshot shows the geologic feature as captured by the OLI (Operational Land Imager) aboard the Landsat 9 satellite, an Earth-observing craft that launched back in 2021.

The satellite, a collaborative effort between NASA and the U.S. Geological Survey, is the ninth in the Landsat Earth-observing series, which goes all the way back to the launch of Landsat 1 in 1972. On a near-weekly basis, Landsat 9 delivers observations of everything from deforestation to water quality and crop growth.

The series of Landsat satellites have been a critical piece in the modern understanding of how our planet continues to change. Whether it's the repercussions of climate change or fluctuations in agriculture, observations from orbit do more than provide interesting photos of our home world; they also capture critical data.

NASA closes the book on epic OSIRIS-REx asteroid-sampling mission: ‘I am immensely proud of what we did’

On Sept. 30, NASA formally concluded OSIRIS-REx, the historic first U.S. mission to pluck a pristine piece of an asteroid and deliver it safely back to Earth.

The van-sized OSIRIS-REx spacecraft — whose name is short for Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer — visited and sampled Bennu, an ancient space rock holding pristine remnants from the dawn of our solar system more than 4.5 billion years ago. Among those cosmic relics are raw organic building blocks, the kind that may have seeded life on Earth.

"I have known this day was coming for a long time, but it is still difficult to see it arrive," OSIRIS-REx Principal Investigator Dante Lauretta, who's based at the University of Arizona, said in a post on LinkedIn. "I feel enormous pride in what we accomplished together, and real sadness that this journey has come to an end."

For the mission team, the farewell capped a decade of high-stakes engineering, on-the-fly troubleshooting and nail-biting close calls that ultimately delivered to Earth the largest asteroid sample ever collected in space, one that held secrets from the early solar system.

Long before launch, the team faced obstacles that nearly thwarted the endeavor — chiefly, two rejections from NASA — before finally securing the green light for the $1 billion project under the New Frontiers Program in 2011.

When OSIRIS-REx launched on Sept. 8, 2016, on a two-year journey across the inner solar system, Bennu was little more than a point of light in telescopes. Scientists expected the asteroid’s surface to be a smooth, sandy sphere where OSIRIS-REx could seamlessly touch down. Much to their surprise, however, when the probe arrived at the asteroid in late 2018, it revealed Bennu to be a treacherous, loosely bound amalgamation of jagged boulders.

"Our expectations about the asteroid's surface were completely wrong," Lauretta said in an Oct. 7 statement from the University of Arizona. "There was no obvious place to collect a sample anywhere."

When OSIRIS-REx touched down on a small crater named Nightingale, Bennu offered so little structural resistance that scientists said its surface reacted more like fluid than a hard, rocky shell. The spacecraft's sampling head sank directly into the asteroid, stopping after burrowing 20 inches (51 centimeters) deep by firing its thrusters at the right time to pull away, with the precious sample in hand.

A spacecraft's arm above a moving ground. It's black and white and the ground looks pebbled and rocky.

NASA's OSIRIS-REx spacecraft captured this series of images of asteroid Bennu on April 14, 2020, during the first rehearsal of the mission's sample collection event. The actual sample retrieval was extremely close to the way this looks. (Image credit: NASA/Goddard/University of Arizona)

Then came another nail-biting moment: The sample collector lid got jammed in a partially open position because so much material was scooped up, allowing fragments of the precious cargo to escape. In a race against time to prevent further loss, the mission team quickly stowed the sampler head directly inside the return capsule, securing the cosmic treasure for its journey back to Earth.

Even the final return to Earth, on Sept. 24, 2023, kept the team on edge: A parachute failed to deploy properly during reentry, forcing a tense but ultimately safe landing in the Utah desert.

"Successful exploration missions are not those that avoid surprises; they are those that are deliberately designed to adapt to them," Lauretta said in the statement, quoting a line from the mission's final report to NASA.

"That certainly describes OSIRIS-REx," he said. "Again and again, the mission presented us with circumstances we had not expected, and again and again, this team found a way forward."

The mission's triumphs began long before the samples reached Earth. For example, the probe set a Guinness World Record when it slid into orbit around the 1,610-foot-wide (490 meters) Bennu, which became the smallest object ever circled by a spacecraft.

The scientific payoff that followed included remote-sensing work that confirmed Bennu's surface is coated in carbon-bearing compounds. Those observations also revealed that Bennu was once part of a much larger, water-rich parent asteroid that shattered in a catastrophic collision in the main asteroid belt between Mars and Jupiter.

The returned sample — which weighs 4.29 ounces (121.6 grams) here on Earth, more than twice the mission's requirement — continues to thrill and occupy scientists.

A wave of research papers, now topping 200, continues to piece together the composition and history of the ancient space rock. Among other findings, Bennu's pristine material has revealed amino acids and sugars that, on Earth, are essential for life, alongside a history of exposure to liquid water that could have served as the "broth" for these compounds to interact.

More discoveries are likely to come. Most of the returned Bennu sample is being preserved for future generations of scientists, who will study it "with questions and instruments we cannot yet anticipate," Lauretta said in the statement.

Though its OSIRIS-REx chapter is closed, the spacecraft itself is far from retired. Renamed OSIRIS-APEX (OSIRIS-APophis EXplorer), the probe is using its remaining propellant to head toward Apophis, another near-Earth asteroid and a different type of space rock from Bennu. It is scheduled to arrive in 2029.

The moon is shrinking. 10,000 cracks on the lunar surface reveal by how much

The moon is shrinking, and scientists are narrowing in on exactly how much our natural satellite has dwindled over the years.

The moon is thought to have formed from a violent collision between a massive object and our young Earth roughly 4.5 billion years ago, and its interior is still gradually cooling off from this ancient collision. As it cools, the moon contracts, leading to a long, slow shrinking process. Now, in a new study, scientists think that they have figured out how much smaller the moon is actually getting.

In this new study, scientists analyzing images snapped by the Lunar Reconnaissance Orbiter Camera (LROC) have spotted over 10,000 young faults, or cracks across the moon's surface. This helped them to figure out how much the moon has contracted over time, and they now estimate that the moon's radius has decreased by about 148 feet (45 meters) over the past 400 to 800 million years.

"The number of these young faults revealed in LROC images is much greater than I ever imagined," study lead Thomas Watters, a geologist and scientist emeritus at the Center for Earth and Planetary Studies at the Smithsonian's National Air and Space Museum, said in a statement. "As the interior of the moon continues to cool and contract, it is expected that the growth of existing faults and formation of new faults continues today."

Lobate scarps on the moon.

Lobate scarps on the lunar surface, as seen by LROC. (Image credit: NASA/KARI/ASU/Intuitive Machines/Smithsonian  )

With these LROC observations, researchers in this study saw a variety of different types of cracks and landforms across the lunar surface. This included lobate scarps, or long, curved structures that form when the moon's surface contracts, cracks and is pushed upwards; and small mare ridges, or narrow "wrinkles" in the lunar surface, across the dark plains on the moon.

Lobate scarps on the moon.

Lobate scarps on the moon, as seen by LROC. (Image credit: NASA/KARI/ASU/Intuitive Machines/Smithsonian)

Tectonic activity on the moon looks a lot different than it does on Earth. On our own planet, there are about 15 major tectonic plates. On the moon, there are no tectonic plates at all. Instead, the moon has a single-plate body meaning its outer shell is a single piece only broken by faults or other such cracks created by the moon contracting. This means that instead of faults or cracks appearing at tectonic plate boundaries, they are instead scattered all over the moon.

A global map of lunar faults.

A global map of lunar faults. Red lines indicate over 8,900 lobate scarps while blue lines show over 2,000 small mare ridges. (Image credit: NASA/ASU/Intuitive Machines/Smithsonian)

By mapping these thousands of different features, all created from the moon cooling and contracting over time, the researchers are piecing together lunar history. In addition to finding the extent to which the moon has shrunk over time, they also found that some areas of the moon are covered in many more faults than other areas, and the areas with fewer cracks and faults have thicker moon crust.

This led them to conclude that not only are these areas with thicker crust more stable, but they suggest that a great deal of the widespread cracks in the lunar surface were created later in the moon's history as, in its earlier years, its thick crust would have insulated the moon's warm interior and prevented cooling, contracting and cracking.

This work was described in a study published Oct. 14 in The Planetary Science Journal.

Elephant Island is an icy sight from orbit | Space photo of the day for Oct. 19, 2026

Ice floats by in West Antarctica as winter comes to an end in the Southern Hemisphere. (Image credit: contains modified Copernicus Sentinel data (2026), processed by ESA)

Antarctica is a magnificent sight, and that beauty is visible all the way from space.

What is it?

Orbiting planet Earth, the European Space Agency's (ESA) Copernicus Sentinel-3 mission captured a close-up of West Antarctica.

Winter is ending in the Southern Hemisphere, meaning this is the peak of icy weather and sea ice in the Arctic.

In this image snapped by Sentinel-3, you can see a massive swath of ice which includes Elephant Island on the left-hand side. An ice-covered island off the Antarctic coast, Elephant Island floats in the Southern Ocean. It got its name both from the island's shape, which some liken to that of an elephant's head, and the fact that the island is home to a community of elephant seals.

Why is it incredible?

While a seal-inhabited island on the left floats near the Antarctic coast, across the water is a vast, frozen landscape. In just this snapshot, you can see about between 746 and 1,056 miles (1,200 to 1,700 kilometers) of the icy continent.

This image was captured on Sept. 30, 2026. In the Southern Hemisphere, that was just past the end of winter. The absolute peak for sea ice in Antarctica fell just a couple weeks before, on Sept. 14, according to the National Snow and Ice Data Center, ESA reported.

So in this one snapshot, we can see a near-maximum for sea ice in the Antarctic, spanning hundreds of miles. In observing our own planet from space, we are able to peer across vast landscapes, capturing important observational data. This is especially critical for the Antarctic as, with the progression of climate change, this sea ice continues to dwindle, adding to sea level rise among other serious consequences across the planet.