Named Beta Pictoris d, the newly-discovered world is 100 times fainter than Beta Pictoris b -- the first planet discovered around the A5-type star Beta Pictoris -- and is among the lightest exoplanets ever to be imaged from the ground.
The post Astronomers Discover and Directly Image Third Planet in Beta Pictoris System appeared first on Sci.News: Breaking Science News.
Using the upgraded GRAVITY+ instrument on ESO’s Very Large Telescope Interferometer (VLTI), astronomers have measured the ratio of carbon isotopes in the atmosphere of the young exoplanet Beta Pictoris, offering new insights into how giant planets form.
The post Astronomers Probe Chemistry of Giant Exoplanet Beta Pictoris b appeared first on Sci.News: Breaking Science News.
Researchers have discovered a potentially habitable exoplanet just 25 light-years from Earth—but is its precarious location on the cosmic shore too dangerous to make it a home for extraterrestrial life?
In a recent paper in The Astrophysical Journal, researchers at the University of California, Irvine, revealed their discovery of GJ 3378b, an exoplanet that resides in the habitable zone, sometimes referred to as the “Goldilocks zone,” a distance from the host star ideal for liquid surface water.
The habitable zone is a key focus in the search for extraterrestrial life, as planets any closer would have their atmospheres and surface waters burned off, while those any further from their host star would be completely frozen.
“This one’s exciting,” said lead author Paul Robertson, a UC Irvine assistant professor of astronomy and lead author of the new study. “It’s one of our closest cosmic neighbors. 25 light-years sounds like a long way, but the Milky Way is about 100,000 light-years across, so in that respect it’s our next-door neighbor.”
Robertson led the team in the exoplanet discovery, using the Habitable-zone Planet Finder on the Hobby-Eberly Telescope at McDonald Observatory in Texas, and the NEID Spectrometer on the WIYN Telescope at Kitt Peak National Observatory in Arizona.
GJ 3378b is about twice the size of Earth, making it what astronomers call a “super-Earth” for its increased size. Additionally, this potentially habitable exoplanet likely receives a comparable amount of stellar radiation to our planet.
“This super-Earth gets about 90 percent of the radiation from its host star as Earth gets from its sun, so it’s right in the sweet spot,” said Robertson.
While GJ 3378b resides within its star’s habitable zone, it does so only barely. This fringe area astronomers refer to as “the cosmic shoreline,” a distance just outside of which the stellar radiation would become so intense that its atmosphere would be ripped away, and any potential surface water along with it.
Straddling this shoreline, researchers are uncertain whether GJ 3378b has an atmosphere or is still a victim of excessive stellar radiation, as its larger size relative to Earth may make it more susceptible.
Our own solar system also offers an excellent example of this: the planet Mars, which researchers suspect once had an Earth-like atmosphere, and potentially even life. However, intense solar radiation bombardment destroyed that atmosphere, taking the surface water with it, leaving a desolate wasteland.
“If you scale the Earth down to the size of an apple, its atmosphere would be about as thick as the skin of the apple,” said Robertson. “That’s just enough to maintain the kinds of surface pressures where you can have liquid water. It’s enough that there’ll be breathable air, and it provides maybe a little bit of protection from the harsh radiation environment of space.”
Although GJ 3377b is relatively close to Earth on a cosmic scale, current equipment cannot determine whether the planet harbors an atmosphere. To do so, advanced future observation platforms will be required, and just such work is on the horizon.
“If a planet in the habitable zone has a proper atmosphere, we can justify further research looking for biosignatures, liquid water, or other signs of life that require both an atmosphere and the right amount of heating from the host star,” said co-author Gogod James, a UC Irvine student in Robertson’s group who worked to characterize the size of GJ 3378b.
NASA plans to take a closer look at these potentially habitable worlds in about two decades with its upcoming Habitable Worlds Observatory (HWO). Launching in the 2020s, HWO will be a large infrared/optical/ultraviolet space telescope designed to confirm whether exoplanets have atmospheres, and then seek biosignatures within those atmospheres, which could indicate the presence of extraterrestrial life.
The paper, “A Revised Mass and Period for the Habitable Zone Super-Earth GJ 3378 b: A Planet Straddling the Cosmic Shoreline,” appeared in The Astrophysical Journal on June 30, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
James Webb Space Telescope (JWST) observations have revealed that the fate of planets after the death of their host star may be surprisingly warm, according to new research from the University of St Andrews.
The JWST observations offer a possible glimpse into what our solar system will be like billions of years from now, particularly for gas giants like Jupiter. In a recent paper published in Nature, the St Andrew researchers describe JWST observations of WD 1856 b, a Jupiter-sized exoplanet much warmer than would be expected for orbiting a dead white dwarf star.
A collaboration between NASA, the European Space Agency, and the Canadian Space Agency, the JWST has provided an unprecedented view of the distant edges of the universe, revealing many unexpected finds. Among these surprises was WD 1856 b, whose mass, temperature, and atmosphere readings reveal a surprisingly intact planet after the death of its star.
Our own Sun is projected to exhaust its supply of hydrogen in roughly five billion years, after which it will expand into a red giant star about 100 times larger than it is today, before shedding mass in its final transformation into a white dwarf star.
In the distant future, the Sun’s transformations will likely someday obliterate Mercury, Venus, and even Earth, yet scientists have remained uncertain about how more distant planets will fare. Only by observing real-world examples of planets orbiting dead stars can scientists gather more data on how these scenarios play out for the remaining planets, as with JWST’s observations of WD 1856 b.
Discovered in 2020 by the TESS survey and the Spitzer space telescope, WD 1856 b orbits the white dwarf star WD 1856+534 at a distance of around 80 light-years from Earth.
“The planet is quite the oddball. It’s about the size of Jupiter, but the white dwarf it orbits is the size of Earth, so the planet is seven times larger than its star,” said lead author Dr. Ryan MacDonald from the University of St Andrews.
Perhaps the most confounding element of this system is how close the exoplanet is to its host star. At a distance of 50 times closer than the Earth is to the Sun, the planet is at a distance at which the star’s red giant phase should have destroyed it. How the planet managed to escape the destruction while ultimately ending up so close to its star intrigued the St. Andrews team.
As WD 1856 b performed a grazing transit, where just its top edge passed in front of the host star, JWST observations allowed the researchers to crucially measure mass and temperature data, allowing them to estimate its mass at between four and eleven times that of Jupiter.
“We’re used to looking back in time when we use telescopes, but this is the first time we have been able to look forward to what might happen to the outer planets around the remnant of a Sun-like star,” MacDonald said, adding that “it’s like using a time machine to peer into the distant future of our Solar System.”
Infrared light emitted by the planet’s own heat showed a surprising temperature of 126°C, which is 240°C hotter than it would be from the white dwarf’s heat alone.
As the team worked on the problem, the temperature mystery proved to be the answer to the distance issue.
“The big question is how WD 1856 b ended up where it is today, and there are two theories. One is that the planet was swallowed by the host star as it was dying, and managed to survive on the inside,” said Dr. Christopher O’Connor of Northwestern University. “The other is that the migration took place due to the gravitational effect of other objects in the system. The white dwarf is part of a triple star system, and the outer companion stars could have influenced WD 1856 b’s orbit.”
Since no present source of energy should be capable of generating this much heat on the exoplanet, the researchers suggest that it represents heat left over from being engulfed by the red giant or possibly through an inward migration. Cooling models the team analyzed indicated that the planet likely first captured heat about 3 to 3.5 billion years ago, then cooled to its present temperature and migrated closer to its host star.
“This is just the beginning of our exploration of planets orbiting dead stars with Webb, and the search for further planets orbiting white dwarfs is ongoing,” Dr. MacDonald concluded. “Our results show that stellar death is not the end – some planets experience a vibrant and lively future after the death of their star.”
The paper, “Aerosol and Hydrocarbons in the Atmosphere of a White Dwarf Planet,” appeared in Nature on July 1, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
An exoplanet is exerting a magnetic influence on its host star in a manner opposite to what astronomers normally observe, according to researchers at the Institute of Astrophysics of Andalusia (IAA-CSIC).
In a recent paper published in Science, IAA-CSIC researchers revealed how the exoplanet GJ 436 b is affecting its host star’s behavior in a never-before-seen way. In their work, the team developed a novel method to estimate an exoplanet‘s magnetic field strength, an important factor in determining habitability.
“Until recently it was thought that it was mainly the star that influenced the planet,” said Rafael Luque, an IAA-CSIC researcher and one of the new study’s co-authors.
Luque adds that his team’s results now offer “the clearest evidence to date of something that had already been suspected: that the opposite can also happen and that a nearby planet can alter the environment of its star.”
While the most obvious ingredients for a habitable planet are water and a breathable atmosphere, other elements are less apparent to us based on our human experience. Our planet’s invisible magnetic field protects us from the solar wind and holds the atmosphere together.
While Earth’s magnetic field guided the evolution of its atmosphere, Mars provides an example of what the loss of a magnetic field can do to an otherwise potentially habitable planet. When the Martian magnetic field disappeared four billion years ago as the planet’s core rapidly cooled, the atmosphere dissipated, followed by the loss of surface water.
As shown by the fates of two cosmic neighbors like Earth and Mars, a stable magnetic field is a key element of habitability.
Detecting magnetic fields on distant exoplanets has proven more challenging for astronomers than other observations, such as atmospheric composition. In their new paper, the IAA-CSIC team provides the first conclusive evidence of an exoplanet’s magnetic field, observed through its impact on the host star.
“In particular, we have observed that GJ 436 b, an exoplanet similar to Neptune that orbits very close to its star, causes regular changes in the brightness and energy emitted by the star at certain wavelengths,” explained lead author Daniel Revilla, an IAA-CSIC researcher who led the study as part of his doctoral thesis.
GJ 436 b provided the team with measurable signals that allowed them to infer that the exoplanet had a magnetic field and estimate its strength. The IAA-CSIC team analyzed sixteen years of spectroscopic observations of the GJ-436 system for their research, collected by the CARMENES instrument at the Calar Alto Observatory.
“Despite its smaller size, GJ 436 b would have a magnetic field between 2.33 and 27 times more intense than that of Jupiter,” said co-author Pedro J. Beloved, a researcher at the IAA-CSIC.
In the paper, the researchers demonstrate how, in a very close orbit, a planet can flip the normal planet-star relationship, with the planet controlling the influence of gravity, radiation, and magnetic fields between the two. As the exoplanet interacts with its host star, it injects energy into the star’s chromosphere to produce a phenomenon like a stellar aurora.
This strange interaction has only been measured periodically, occurring in eight-year cycles, with observations in 2008, 2016, and 2024. Intriguingly, these years correlate to phases of the host star’s magnetic cycle, which the researchers believe affects the intensity.
“Until now, measuring the magnetic field of an exoplanet was extremely difficult,” Devilla concluded. “This property is key to knowing if a planet can protect its atmosphere and, ultimately, if it could harbor life.”
The paper, “Constraining an Exoplanet’s Magnetic Field Using Star-Planet Interactions,” appeared in Science on June 25, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
A tiny green dot appearing in an image taken by NASA’s Mars Reconnaissance Orbiter (MRO) captures a historic tale of Red Planet exploration by one of its first Earthling visitors.
That visitor—a robotic rover named Perseverance—has been conducting investigations on Mars since February 18, 2021, and the new aerial images reveal its current location in an area that mission specialists have dubbed “Arbot.”
While Perseverance’s latest appearance reveals little more than a greenish spec on the planet’s rust-colored surface, also visible in the new images are the long path its formidable tires have left in the Martian soil as the robotic explorer has trekked west of its initial landing site.
The new images, captured on June 13, 2026, were taken just one day before Perseverance broke the previous distance record held by a robotic explorer on Mars: NASA’s Opportunity rover.
However, Perseverance completed this phase of its journey in record time compared to its predecessor, which took more than 11 years to traverse a similar distance. Perseverance, by contrast, covered the same distance in less than half that time, with just five years and four months of travel now behind it.
The images were made possible by the MROs’ High-Resolution Imaging Science Experiment (HiRISE) camera, which also captured surface features in the Arbot area that include ridges and windswept areas along Mars’ rugged exterior.
Built and operated by the University of Arizona, HiRISE captures images with resolutions as fine as about 25 centimeters (10 inches) per pixel, allowing researchers to distinguish features roughly the size of a kitchen table from orbit. The camera has returned hundreds of thousands of detailed images since the MRO arrived at Mars two decades ago, contributing to a growing data set that has transformed scientists’ understanding of the Red Planet.
Documenting everything from active dust avalanches and shifting dunes to fresh impact craters, the unprecedented resolution its imagery provides has made HiRISE one of the most powerful planetary imaging instruments ever deployed.
Last year, the MRO’s HiRISE camera also successfully captured images of the interstellar comet 3I/ATLAS as it made its way past Mars during its trip through our Solar System. Although the HiRISE images weren’t the clearest images of the interstellar visitor obtained during its visit, they did help demonstrate just how formidable NASA’s MRO and its suite of instruments are.
Additional details about Perseverance and its mission can be found at NASA’s official web page, and information about the MRO can be found here.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached at micah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
The first direct measurements of exoplanet magnetic fields reveal that ultra-hot Jupiters possess strong magnetism that shapes their atmospheres and may provide new insights into planetary habitability. Astronomers have achieved a major advance in the study of worlds beyond our Solar System by estimating the strength of the magnetic fields surrounding seven ultra-hot Jupiters. The [...]HD 80606b has one of the most extreme orbits of any known exoplanet and the NASA/ESA/CSA James Webb Space Telescope just caught it getting flash-fried as it whipped past its star.
The post Webb Sees Jupiter-Size Exoplanet Being Roasted by Its Star appeared first on Sci.News: Breaking Science News.
James Webb Space Telescope (JWST) observations have revealed the colorful secret of the Pink Planet, the coldest object of its type ever directly observed.
A team of astronomers led by Northwestern University has revealed their findings in a recent paper published in The Astronomical Journal, finally describing the rose-colored haze covering the planetary-mass companion GJ504b, thanks to JWST data.
For over a decade, researchers have speculated that atmospheric salt clouds may create the pink planet’s strange hue, but this is the first concrete evidence for the hypothesis.
Since its discovery in 2013, GJ504b, commonly known as “The Pink Planet,” has been a bit of an astronomical mystery. Even the object’s description is imprecise: a “planetary-mass companion,” a nebulous category teetering between the size of a large planet and a brown dwarf, at roughly 25 times Jupiter’s mass. Residing 57 light-years from Earth, the object’s host star is similar to our Sun.
Faint due to extremely cold temperatures, astronomers cannot obtain clear enough observations with ground-based telescopes to perform spectroscopic analysis. However, from its vantage point beyond our atmosphere, the JWST’s advanced instruments have finally provided the necessary data to make sense of the object’s strange pink atmosphere.
The exoplanets most clearly observed are much hotter than our world, with temperatures between 1,000 and 2,000°F, creating a brilliance which can be seen across the gulf of space and through Earth’s atmosphere.
This giant planet is a mere 550°F, still hot by Earth standards, but far cooler than is normal for its type. According to the new study, GJ504b is an ancient world, some 2.5 to 4billion years old, with a slow cooling over time accounting for its decreased temperature.
In addition to providing the first evidence for The Pink Planet’s elusive salt clouds, the team’s research has broader implications for studying cold objects, laying the groundwork for future JWST observations of such faint glows, too dim for ground-based telescopes.
“The Pink Planet is the coldest companion ever discovered using ground-based instruments,” according to Aneesh Baburaj, the study’s lead author. “Many teams all around the world performed follow-up observations to study its light, but it was too faint for ground-based instruments. That made it a perfect target for JWST. When we finally obtained its spectrum, it immediately looked interesting. But once we started digging deeper into the data, we realized it was not like anything we have analyzed before.”
To accurately analyze the light, Baburaj’s team used an advanced data-processing technique to remove considerable glare from the Pink Planet’s host star, improving the quality of the JWST data. Breaking light into separate colors through spectroscopic analysis allows scientists to determine the elemental composition of exoplanet atmospheres using JWST data.
“In the past, other astronomers observed the companion for an entire night with some of the biggest telescopes in the world to obtain a spectrum,” Baburaj said. “And they could not see the object. With JWST, our entire observation took around two hours, and we were successful.”
The team discovered water vapor, methane, carbon dioxide, ammonia, and other molecules in the object’s atmosphere, but these results conflicted with existing atmospheric models, which only made sense if the object had an extremely unlikely combination of physical features. However, once the team added clouds to the model, the effect of their salty formations on the light made the JWST data much easier to explain.
“We ran simulations with clouds, and the results aligned with what we know about cold planets,” Baburaj said. “We tried three different types of clouds, and salt clouds fit best. When we accounted for salt clouds, it subdued the signature of molecules hidden deeper in the companion’s atmosphere. Then, the results became physically possible.”
In addition to the salty clues, the researchers discovered an abundance of heavy metals. These may have something to do with The Pink Planet’s origins, as it may have originally formed as a star instead of a planet, but astronomers remain uncertain. In any case, the work process developed here will be essential to future JWST investigation of cold objects.
“This is the first time we’ve found that salt clouds are critical to explaining the spectrum of an object,” Baburaj concluded. “It’s a good reminder to account for clouds in our models.”
The paper, “JWST-TST High Contrast: First Direct Spectroscopy of GJ504b Reveals Clouds and Possible Metal Enrichment,” appeared in The Astronomical Journal on June 18, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
Astronomers have discovered an unexpected surprise on the famous “Pink Planet,” a strange world known as GJ504b. Using the powerful James Webb Space Telescope (JWST), scientists found that the object is surrounded by salty clouds and has an atmosphere filled with unusual chemicals. GJ504b was first discovered in 2013. It orbits a sun-like star about […]
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For the first time, astronomers have distinguished between the morning and evening atmospheres of a single planet, revealing two remarkably different environments at its edges. WASP-121 b is a gas giant that orbits extremely close to its star, resulting in one hemisphere exposed to temperatures approaching 2,500 degrees Celsius while the opposite side remains in constant darkness.
A research team from the Max Planck Institute for Astronomy used the James Webb Space Telescope to provide observational evidence for a phenomenon that models had previously predicted. The boundary regions between day and night on tidally locked planets can exhibit distinct temperatures and chemical compositions.
The recent findings appeared in a study published in Nature Astronomy.
WASP-121 b is part of a group of gas giants known as hot Jupiters. These massive planets orbit their stars in just a few days and eventually become locked in place by gravity. Tidal forces keep one side facing the star at all times, while the other side never sees daylight.
“WASP-121 b is particularly extreme,” said co-author Tom Evans-Soma of the University of Newcastle, Australia. “Average temperatures on the dayside hemisphere are around 2,770 Kelvin, while those on the nightside are closer to about 1,000 Kelvin.”
The difference in temperature between the two hemispheres, which is about 1,775 degrees Celsius, makes WASP-121 b one of the most thermally extreme exoplanets known. The regions at the boundary between day and night, called terminators, are where the planet experiences constant morning or evening conditions. Scientists expected these areas to have different atmospheric properties, but only with the precision of JWST could these differences be directly observed.
The researchers used a method based on the planet’s transit across its star to study these differences. As WASP-121 b passes in front of its star, it rotates by about 30 degrees, which means that different parts of its atmosphere can be observed during each transit. By tracking how infrared starlight filters through the atmosphere over time, the team reconstructed how temperature and chemical composition change across different longitudes.
“By measuring how starlight absorption changes as WASP-121 b rotates, we probe its atmosphere longitude by longitude,” said lead author Cyril Gapp of MPIA. The observations not only confirmed what models had predicted, but also showed that the differences between the two terminators are even greater than expected.
The evening side of the planet’s terminator absorbs more starlight than the morning side. Powerful eastward winds sweep heat from the scorching dayside toward the nightside, with the evening region getting the first blast of this warmth. This extra heat causes the atmosphere there to puff up, allowing it to absorb even more starlight, as the observations showed.
Chemical measurements backed up these findings. Carbon monoxide absorption increased as the hotter regions of the evening came into view near the end of the transit. Water showed a different pattern. Rather than simply decreasing with higher temperatures, the researchers interpret the result as evidence that water molecules in the upper atmosphere are breaking apart, likely due to the intense heat at the evening terminator. This points to a real chemical change, not just a shift in molecular location.
The morning side shows a different environment. Although models predicted a difference between the two terminators, they did not fully explain why the morning side appears cooler and more opaque. The most likely explanation involves clouds that are unlike those on Earth.
At the morning terminator, air comes in from the cold nightside. Temperatures may be low enough for silicate and mineral compounds to turn into tiny particles, forming clouds that block infrared radiation from below. This makes the atmosphere appear cooler than it really is underneath.
When the team adjusted their models to account for these clouds, the results more closely aligned with their observations. Still, confirming exactly how these clouds form and behave will require more advanced modeling, as cloud formation and evaporation in such extreme environments remain a major puzzle in exoplanet science.
WASP-121 b has been the subject of previous studies, but JWST now enables astronomers to examine its atmosphere in detail, section by section. This approach is now also available for use with other exoplanets.
The team has already found other ultra-hot gas giants with the right temperatures and orbits for similar analysis. Using this method on other planets will help astronomers compare atmospheric conditions and deepen our understanding of extreme planetary environments.
Austin Burgess is a writer and researcher with a background in sales, marketing, and data analytics. He holds an MBA, a Bachelor of Science in Business Administration, and a data analytics certification. His work focuses on breaking scientific developments, with an emphasis on emerging biology, cognitive neuroscience, and archaeological discoveries.
James Webb has revealed that the sunrise and sunset sides of WASP-121 b have surprisingly different atmospheres. Astronomers using the James Webb Space Telescope (JWST) have discovered striking differences between the morning and evening sides of the atmosphere of WASP-121 b, an ultra-hot gas giant located far beyond our solar system. The findings provide the [...]Planetary scientists analyzing a lunar meteorite known as Northwest Africa (NWA) 12593 have uncovered evidence of an asteroid impact that occurred 3.5 billion years ago on the Moon, helping to reconstruct a period of intense bombardment that left lasting marks across the inner Solar System.
The post Lunar Meteorite Preserves Evidence of Colossal Asteroid Strike appeared first on Sci.News: Breaking Science News.
By combining seismic, gravity and topographic data, a team of researchers from Italy, Switzerland, Germany and the United Kingdom found that several well-known subglacial basins in East Antarctica are part of a single fan-shaped province whose origins trace back to ancient continental stretching.
The post Geoscientists Find Vast Fan-Shaped Structure beneath Antarctica’s Ice appeared first on Sci.News: Breaking Science News.
A meteorite discovered in Africa could be evidence of a lost protoplanet that once orbited our Sun, according to researchers at the University of Colorado at Boulder.
In a recent paper published in Earth and Planetary Science Letters, the team revealed evidence of an ancient protoplanet that may have been as large as Mars based on simulations of how the meteorite sample may have formed.
The four-and-a-half-billion-year-old world carried an unexpected geological makeup, which the researchers say casts doubt on common assumptions regarding planetary evolution.
According to the UC Boulder team, the massive protoplanetary body collided with another object four and a half billion years ago, shattering it completely. This is the first definitive evidence of a lost protoplanet in our solar system, based on analysis of the angrite meteorite NWA 12774, a shard of that planetary embryo recovered from the Sahara Desert.
“It’s incredible to think there was once a world this large,” said lead author Aaron Bell, an assistant research professor in the Department of Earth Science at CU Boulder. “We only know it existed because a few fragments of it happened to land on Earth. These meteorites preserved evidence of a completely different pathway through which early planets developed.”
Angrites, a rare type of volcanic rock, serve as a record of our solar system’s distant past. These rocks began forming only a few million years after the solar system’s birth, making them valuable evidence of this early era. However, they are extremely rare and difficult to find.
NWA 12774 is one of only 68 angrite samples identified among more than 80,000 meteorites cataloged by scientists. Given its rarity, the discovery could potentially reshape how researchers understand these ancient rocks.
Until now, scientists had assumed that angrites originated from relatively small asteroids less than 124 miles (200 kilometers) wide, based largely on their chemical composition. Large rocky planets such as Earth and Mars contain significant amounts of silicon dioxide, while angrites contain very little of the compound.
Researchers began to reconsider those assumptions when they identified clinopyroxene in the meteorite sample. This mineral, commonly found in Earth’s crust and mantle, appeared unusually rich in aluminum, suggesting that it formed under significant pressure deep within a planetary body.
To investigate this unusual characteristic of NWA 12774, the University of Colorado Boulder team recreated the conditions under which the sample could have formed. Their analysis revealed that pressures of at least 17.5 kilobars were required to produce the aluminum-rich clinopyroxene found in the meteorite. For comparison, one kilobar is roughly equivalent to the pressure at the deepest part of Earth’s oceans, near the bottom of the Mariana Trench.
The researchers’ discovery proved that at least this particular angrite sample could not have formed inside a small meteorite, as a body with a radius of at least 621 miles would be required to generate the pressure needed to produce the crystals.
Additional evidence suggested the parent body may have been even larger. The crystals’ sharp edges and delicate internal structures indicate they likely formed at relatively shallow depths beneath the surface. Reconciling both the high-pressure conditions and the shallow formation depth suggests that the parent body may have ranged in size from the Moon to Mars.
“There are many meteorites sitting in drawers that haven’t been thoroughly studied, so there were likely more of these protoplanets we don’t know about,” Bell said.
Exactly what happened to this ancient world remains uncertain, but researchers believe it was likely destroyed in a massive collision early in the solar system’s history. Fragments of that lost protoplanet may have later contributed material to other bodies, potentially including Earth itself.
“The materials that formed the angrite parent body are fundamentally different from the ingredients of Earth and Mars,” Bell concluded. “It points to a distinct and separate evolutionary path in planetary formation in the early history of our solar system.”
The paper, “High-Pressure Clinopyroxene in Northwest Africa 12774 and New Geobarometric Evidence for a Planetary Embryo-Sized Angrite Parent Body,” appeared in Earth and Planetary Science Letters on July 1, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
The giant planet’s bow shock isn’t just deflecting the solar wind, it’s acting as a powerful particle accelerator, firing electrons to relativistic energies of at least 1 MeV, according to a new analysis of data from NASA’s Juno spacecraft.
The post Jupiter Accelerates Electrons to Near-Light Speed, Offering Clues to Cosmic Ray Origins appeared first on Sci.News: Breaking Science News.
A new Keck Observatory study indicates that giant planets can spin faster than more massive brown dwarfs, revealing important clues about how planetary systems form and evolve. Astronomers have long suspected that a planet’s mass may be linked to how quickly it spins. In our solar system, Jupiter and Saturn rotate especially fast, each completing [...]The Northwest Africa (NWA) 12774, an angrite meteorite discovered in the Sahara Desert, likely in Mauritania, appears to be a fragment of a vanished protoplanet, offering the strongest evidence yet that a large planetary body formed and was later destroyed during the Solar System’s chaotic infancy.
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By tracking fierce winds racing through the atmospheres of seven ultra-hot Jupiters, astronomers have uncovered the strongest evidence yet that magnetic fields shape weather on worlds beyond our Solar System.
The post Astronomers Detect Clearest Signs Yet of Magnetic Fields on Extrasolar Planets appeared first on Sci.News: Breaking Science News.
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