Webb Discovers Surprising Hydrocarbon Abundance in Mysterious Core of Nearby Luminous Galaxy

Astronomers utilizing the NASA/ESA/CSA James Webb Space Telescope have identified an extraordinary presence of small gas-phase hydrocarbons—such as benzene, triacetylene, diacetylene, acetylene, methane, and methyl radicals—within the concealed core of the ultra-bright infrared galaxy IRAS 07251-0248.



Hydrocarbons are influential in shaping the chemistry of the interstellar medium. However, definite observational constraints on their enrichment and relationship with carbonaceous particles and polycyclic aromatic hydrocarbons remain elusive. García Bernete et al. report Webb infrared observations of the Local Ultraluminous Infrared Galaxy (ULIRG) IRAS 07251-0248, revealing extragalactic detections of small gas-phase hydrocarbons. Image credit: García-Bernete et al., doi: 10.1038/s41550-025-02750-0.

The core of IRAS 07251-0248 (also known as 2MASS J07273756-0254540) is obscured by significant amounts of gas and dust.

This dense material absorbs most radiation emitted by the central supermassive black hole, complicating studies with traditional telescopes.

However, the infrared spectrum can penetrate this dust, providing unique insights about these regions and illuminating vital chemical processes in this heavily obscured core.

Dr. Ismael García Bernete and his team employed spectroscopic observations using Webb’s NIRSpec and MIRI instruments, covering wavelengths from 3 to 28 microns.

These observations reveal chemical signatures of gas-phase molecules alongside signatures from ice and dust particles.

These data empowered astronomers to characterize the abundance and temperature of various chemical species within the core of this concealed galaxy.

Remarkably, they discovered an exceptionally high abundance of small organic molecules such as benzene, methane, acetylene, diacetylene, and triacetylene—the first such detections outside our Milky Way, including the methyl radical.

Additionally, substantial amounts of solid molecular materials, including carbonaceous particles and water ice, were identified.

“We uncovered unexpected chemical complexity, showcasing abundances far exceeding current theoretical models,” stated Dr. García Bernete, an astronomer at the Astrobiology Center.

“This suggests a continuous source of carbon within these galactic nuclei, fueling this rich chemical network.”

“These molecules may serve as vital building blocks for complex organic chemistry, relevant to processes that pertain to life.”

Professor Dimitra Rigopoulou from the University of Oxford remarked, “Small organic molecules may not exist in living cells, yet they could play a pivotal role in prebiotic chemistry—a crucial step toward forming amino acids and nucleotides.”

These findings were published in a recent issue of Nature Astronomy.

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I. Garcia-Bernete et al. Abundant hydrocarbons within buried galactic nuclei with evidence of processing of carbonaceous particles and polycyclic aromatic hydrocarbons. Nat Astron, published online on February 8, 2026. doi: 10.1038/s41550-025-02750-0

Source: www.sci.news

New Study Reveals Surprising Abundance of Ceratopsians in Europe’s Cretaceous Fauna

Paleontologists have made significant strides in understanding Europe’s elusive ceratopsians through newly discovered fossils and advanced imaging techniques. Notably, the iguanodon has been reclassified as a true member of the ceratopsian clade.



Possible restoration of Aikaceratops kosmai. Image credit: Matthew Dempsey.

Ceratopsians are a fascinating group of herbivorous ornithischian dinosaurs recognized for their unique parrot-like beaks, bony frills, and distinctive horns.

These remarkable creatures thrived primarily during the Late Cretaceous period, approximately 100 to 66 million years ago.

While ceratopsian fossils are plentiful in Asia and North America, they are notably scarce in Europe.

Previously, evidence in Europe consisted of only a few incomplete and contentious specimens.

The recent discovery of new, well-preserved fossils of Aikaceratops from the Late Cretaceous in Hungary has sparked new research employing CT scans and thorough evolutionary analysis.

Initially described in 2010, Aikaceratops has faced controversy, with some experts regarding it as a horned dinosaur and others viewing it as a distant relative of the ceratopsians, particularly the iguanodon. Despite the debate, it exhibits traits that suggest ceratopsian characteristics.

Utilizing new skull material, Professor Susannah Maidment from the Natural History Museum and the University of Birmingham, along with her colleagues, determined that the dinosaur is not only a ceratopsian but also part of the previously identified rhabdodontid family, which includes Moclodon.

The analysis revealed that several previously misclassified dinosaurs assumed to be rhabdodontids were in fact ceratopsians.

“Although iguanodon and triceratops appear distinctly different, they share a common ancestor, inheriting certain traits,” Professor Maidment stated.

“Both groups uniquely evolved four legs, complex chewing mechanisms, and large body sizes.”

“This shared history makes their teeth and limbs quite similar, complicating classification based on partial skeletons.”

This study confirms the presence of ceratopsians in Europe, addressing a long-standing gap in our understanding of these dinosaurs’ migration across the Northern Hemisphere.

“The initial fossil of Aikaceratops was so incomplete that many scientists doubted its classification as a ceratopsian,” noted Professor Richard Butler from the University of Birmingham.

“What’s fascinating about the new findings regarding Aikaceratops is that they validate the existence of horned dinosaurs in Cretaceous Europe and challenge us to rethink our understanding of ancient ecosystems.”

The earliest ceratopsians, such as Yinlong, originated in Asia and migrated multiple times to North America, leading to the evolution of frilled species like triceratops and Torosaurus.

The most plausible route for this dispersal would have been through Europe, though the scarcity of fossils has posed challenges.

“We know that dinosaurs were capable of crossing the Atlantic Ocean, which was just starting to form during the Cretaceous,” explained Professor Maidment.

“Dinosaurs like Allosaurus have been discovered in both Portugal and the United States, suggesting some level of intercontinental travel was possible.”

“Many dinosaurs could swim, and the islands within the Central European Basin were relatively close, making island-hopping a likely scenario.”

“While triceratops is one of the most recognized horned dinosaurs, most species are native to North America, and many were once misidentified as other types, leading to their obscured presence in Europe,” remarked Professor Steve Brusatte from the University of Edinburgh.

The findings are detailed in a study published in the journal Nature.

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SCR Maidment et al. Hidden diversity of ceratopsians in Late Cretaceous Europe. Nature published online on January 7, 2026. doi: 10.1038/s41586-025-09897-w

Source: www.sci.news

The abundance of ice deposits on the Moon is greater than initially believed

Previous studies have found signs of ice in permanently shadowed regions near the moon’s south pole, including areas within the Cabeus, Howarth, Shoemaker, and Faustini craters. A new analysis of data from NASA’s Lunar Reconnaissance Orbiter (LRO) shows there is widespread evidence of water ice outside Antarctica, at least within a permanently shadowed region toward 77 degrees south latitude. Ta.

This figure shows the distribution of permanently shadowed regions (blue) toward the moon’s poles at 80 degrees south latitude. They are overlaid on a digital elevation map of the lunar surface (gray) from the Lunar Orbiter Laser Altimeter Instrument aboard NASA’s Lunar Reconnaissance Orbiter. Image credit: NASA / GSFC / Timothy P. McClanahan.

Ice may have been embedded in the lunar regolith by comet or meteor impacts, emitted as steam (gas) from the moon’s interior, or formed by chemical reactions between hydrogen in the solar wind and oxygen in the regolith. there is.

Permanently shadowed regions (PSRs) typically occur in topographic depressions near the moon’s poles.

Due to the low angle of the sun, these regions have not seen sunlight for billions of years and are constantly in extremely cold conditions.

Ice molecules are thought to be repeatedly stripped from the regolith by meteorites, cosmic radiation, or sunlight, traveling across the lunar surface and landing on the PSR, where they become trapped in the extreme cold.

The PSR’s continuously cold surface could store ice molecules near the surface for perhaps billions of years, accumulating in sediments large enough for mining.

“Our models and analysis show that the largest ice concentrations are near the coldest parts of the PSR below 75 Kelvin (minus 198 degrees Celsius, or minus 325 degrees Fahrenheit) and on poleward-facing slopes of the PSR. It is expected to occur near the base of the Dr. Timothy McClanahan, researcher at NASA Goddard Space Flight Center.

“It is not possible to accurately measure the volume of ice deposits in the PSR or determine whether they are buried beneath a dry layer of regolith.”

“However, we expect it to be 1 m for each surface.2 If present above these deposits, there should be at least about 5 liters of ice within the top meter of the surface compared to the surrounding area. ”

McClanahan and his colleagues used LRO’s Lunar Exploration Neutron Detector (LEND) instrument to detect signs of ice deposits by measuring moderately energetic “exothermal” neutrons.

Specifically, they used LEND’s Collimating Sensor for Exothermal Neutrons (CSETN), which has a fixed field of view of 30 km (18.6 miles) in diameter.

Neutrons are produced by high-energy galactic cosmic rays that come from powerful deep space events, such as exploding stars, and impact the moon’s surface, destroying regolith atoms and scattering subatomic particles called neutrons.

Neutrons originate from depths of up to about 1 meter (3.3 feet) and ping-pong through the regolith, colliding with other atoms. Some are guided into space and detected by LEND.

Since hydrogen has approximately the same mass as a neutron, neutrons lose relatively more energy in collisions with hydrogen than in collisions with the most common regolith elements.

Therefore, if hydrogen is present in the regolith, its concentration will correspondingly reduce the number of medium-energy neutrons observed.

“We hypothesized that if all PSRs had the same hydrogen concentration, CSETN should detect hydrogen concentrations proportionally depending on their area,” Dr. McClanahan said.

“Therefore, more hydrogen should be observed towards the larger area of the PSR.”

of findings this week, Planetary Science Journal.

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TP McClanahan others. 2024. Evidence of widespread hydrogen sequestration within the lunar south pole cold trap. planet. Science. J 5, 217; doi: 10.3847/PSJ/ad5b55

This article has been adapted from the original release by NASA.

Source: www.sci.news

Amazing Discovery: JWST Uncovers Abundance of Supernovae in Early Universe

Many of the circled objects represent previously unknown supernovae.

Collaboration between NASA, ESA, CSA, STScI and JADES

Astronomers using the James Webb Space Telescope (JWST) have discovered a surprising number of supernovae in the distant universe, including some of the most distant yet seen. Their discoveries increase the number of known supernovae in the early universe by a factor of ten.

The researchers imaged the same small patch of sky twice, in 2022 and 2023, and found 79 new supernovae. “It’s actually very small, about the size of a grain of rice held at arm’s length,” the researchers said. Christa DeCourcy “We’ve spent more than 100 hours on JWST,” said Dr. [observing] I took my time with each image, which gives them a lot of depth.”

Astronomers then compared the two images with each other and with previous photos of the same area taken by the Hubble Space Telescope, looking for bright spots that appear in one image but not the other.

These specks are relatively faint stars that shone brightly before fading in bright supernova explosions. Some of them are candidates for the most distant supernovae ever found, although their distances have yet to be confirmed. And one of them is definitely the most distant one ever seen. This star exploded when the universe was only about 1.8 billion years old.

Such supernovae would have produced the heavy elements that are now widespread throughout the universe, so they would have had lower concentrations of these elements than modern supernovae. “The universe at this early stage was fundamentally different from what has been explored in the past by the Hubble Space Telescope and especially ground-based surveys,” he said. Justin Pierre “This is really new territory that JWST is breaking into,” he said during a presentation at the Space Telescope Science Institute in Maryland, where observations could help shed light on what the first stars were like.

topic:

  • Performer/
  • James Webb Space Telescope

Source: www.newscientist.com