Saturday, February 14, 2026

Archival Data From NASA’s NEOWISE Tracks Star Turning Into Black Hole - UNIVERSE - The Latest in NASA Science News

This artist’s concept shows a thick shell of gas and dust that has been expelled from a massive star’s outer layers as its core collapses after running out of fuel. At the center, a hot, dense ball of gas continues to fall inward, feeding the newly formed black hole.

Keith Miller, Caltech/IPAC – SELab

Massive stars are often known to go out with a bang: The core collapses, and a wave of subatomic particles called neutrinos erupt outward, causing the star to explode as a supernova that can outshine an entire galaxy. But 2.5 million light-years away from Earth, in the Andromeda galaxy, a dying star named M31-2014-DS1 did something unusual and it was captured by a NASA telescope. Rather than exploding, the star blinked out, leaving behind a shroud of hot gas and dust — and something else.

Using archival data from NASA’s NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer) mission along with data from other space and ground-based observatories from 2005 to 2023, astronomers pieced together the mystery of this “failed” supernova, providing the most intimate look yet at how a black hole can be born from a fizz instead of fireworks. The research, which was supported by NASA’s Astrophysics Data Analysis Program, is described in a study published Thursday in the journal Science.

The archival data revealed the star suddenly brightened in infrared light in 2014, but by 2023, M31-2014-DS1 dimmed in visible light by more than a factor of 10,000. The researchers concluded that the infrared brightening was caused by the star shedding its outermost layers as its inner core ran out of fuel at the end of its life. Unable to be pushed outward by a weak shockwave, most of the stellar material collapsed under its immense gravity, turning into a black hole.

The team has now identified another massive star that may have met the same fate as M31-2014-DS1, so this work could help uncover a common mechanism for black holes to form from dying stars that fade quietly into a cloud of hot gas and dust. 

Source: Archival Data From NASA’s NEOWISE Tracks Star Turning Into Black Hole - NASA Science 

Climate-friendly diet yields unexpectedly strong nutritional outcomes - medicalxpress

Credit: CC0 Public Domain

That eating plenty of vegetables, wholegrains and legumes is beneficial for health is well known. More surprising, however, is that people who eat in an environmentally-friendly way also display nutritional values that are better than researchers had expected. This is shown in a new study from Lund University.

The EAT–Lancet diet is a global dietary guideline developed to promote both human health and a sustainable planet. It is based on plant-based foods rich in wholegrains, legumes, fruit and vegetables, with small amounts of animal products—above all, considerably lower meat consumption than what the Swedish Food Agency recommends.

"There have been concerns that a diet with less meat and other animal products would increase the risk of nutrient deficiencies. But we did not see that. On the contrary, most of those who ate in line with the planetary dietary guidelines had good nutritional status," says Anna Stubbendorff, who was a doctoral student at the Faculty of Medicine at Lund University and part of the Agenda 2030 Graduate School.

The study has just been published in The Lancet Planetary Health and forms part of the doctoral thesis on the health effects of the planetary dietary recommendations, which she defended on 16 January this year.

The results of the current study show that the nutrient intake among those who ate a climate‑friendly diet was fully comparable to those who ate the same amount of a "typical" diet with a larger share of animal products. Put differently: the majority of those who ate in a way similar to the new recommendations obtained sufficient amounts of key vitamins and minerals, despite the EAT–Lancet diet containing less meat.

Blood-based measures of nutritional status were also comparable. The researchers are not entirely certain about the reasons, but one explanation may be that the human body adapts its uptake of nutrients to the levels present in the body and therefore absorbs more when needed, she explains.

A couple of deviations were noted among those who ate more climate‑friendly diets. First, levels of the B vitamin folate (folic acid) were higher among them than among the other participants—something that was unexpected and positive. Second, there was an increased risk of anemia (iron deficiency) among female participants. The difference was small—4.6% instead of 3.3%—but Stubbendorff nonetheless suggests that foods could be fortified, or that at‑risk groups receive supplements to achieve good blood values.

Her findings are based on analyses of the extensive Malmö Diet and Cancer Study, in which 26,000 people reported their eating habits and were followed for several decades.

Stubbendorff's answer to the question of whether the EAT–Lancet diet is sustainable for both humans and the environment is therefore a clear yes.

"It is possible to combine an environmentally sustainable diet with good health. The studies show that such dietary patterns can reduce the risk of disease and premature death without compromising nutrient intake among the majority of the population. There are positive synergies between health and sustainability," says Stubbendorff.

More wholegrains—substantially less meat

Stubbendorff, a trained dietitian, began her doctoral position at the Faculty of Medicine and the Agenda 2030 Graduate School at Lund University in 2019. That same year, the first version of the EAT–Lancet diet was published, and she decided to examine how sustainable the new diet was from a health perspective.

"With the EAT–Lancet dietary advice, two strands were tied together—a diet intended to be sustainable for both humans and the planet. It opened up a completely new field of research. Would what was sustainable for the planet increase or decrease the risk of disease and nutrient deficiencies for those who followed the diet?"

Since then, she has published five scientific articles included in the doctoral thesis Environmentally sustainable diets and human health—Nutritional adequacy, disease risk, and mortality. In addition, during her doctoral studies, she has authored and co-authored a further 23 articles related to food and health.

Swedish dietary habits far from sustainable

So how do Swedish eating habits fare from a climate and sustainability perspective? In a global comparison of climate impact, not well. In a ranking of 156 countries, Sweden is 13th from the bottom—just after traditional high‑meat nations such as the U.S. and New Zealand. The explanation is clear: Swedish consumers eat a lot of meat and dairy products, which drives emissions upward. Today, meat consumption is about 680 grams per person per week.

For Sweden to approach the EAT–Lancet recommended diet, a sharp reduction in both meat and dairy consumption is required. The Nordic Nutrition Recommendations, on which the Swedish Food Agency bases its advice, now take some climate considerations into account.

But the differences are notable. According to the Nordic advice, 350–400 grams of red meat per week is acceptable—several times higher than the EAT–Lancet ceiling of 90 grams. At the same time, Sweden lacks guidelines for dairy and poultry consumption, areas where EAT–Lancet specifies a maximum of 250 grams of dairy and 30 grams of chicken per day.

"There is a lot of focus on meat, but other things we can also influence in our part of the world are not eating more than we need and stopping food waste—overproduction of food also depletes the planet's resources. We can also talk more about what we ought to eat more of, such as wholegrains and legumes. There is great potential for public health there," says Stubbendorff.

Links between health and environmental impact

Her doctoral thesis also comprises earlier studies, and one of the most important findings was that the people who ate most in line with the EAT–Lancet diet had approximately a 33% lower relative risk of dying from cardiovascular disease compared with those who adhered least to the diet. This does not mean that one third fewer people died, but rather that the probability of dying from cardiovascular disease was about one third lower in the group that followed the dietary pattern most closely.

At the same time, the overall relative risk of premature death was around 25% lower, and cancer-related mortality decreased by nearly as much. The results are based on observational data and show associations between dietary patterns and mortality, but they cannot establish direct causal relationships.

Are there uncertainties in the results? Yes—measuring what people eat is generally difficult. "But the Malmö Diet and Cancer Study that we analyzed used an unusually advanced method with a food diary, questionnaire and interviews. The study also followed a large group over a long time. So even though there is uncertainty in the material, I consider the results robust," she says.

She now hopes that experts and decision‑makers will dare to address the issue of our dietary habits, even though it is sensitive. Today, food production globally accounts for about one third of total greenhouse‑gas emissions, uses around 70% of the world's freshwater and is the single largest driver of biodiversity loss, with agriculture identified as a threat to the majority of species at risk of extinction.

"It is important that this issue is allowed to rest on a scientific foundation. We have a fantastic opportunity if we succeed with these important changes," she says. 

Source: Climate-friendly diet yields unexpectedly strong nutritional outcomes 

A new framework could transform national flood prediction - Earth - Environment

Conceptual model showing the relative size of the parameter space required (brown band) and resulting predictability (green band) for modeling stormflow generation as a function of land surface-, soil-, and groundwater-dominated mechanisms. This conceptual model considers infiltration–excess and saturation–excess storm flow generation mechanisms as highly predictable end members. Credit: JAWRA Journal of the American Water Resources Association (2026). DOI: 10.1111/1752-1688.70089

When severe weather strikes, the National Weather Service's (NWS) Office of Water Prediction (OWP) makes critical flood forecasts with the National Water Model. Despite improvements over time, the model's performance has plateaued in recent years, leaving researchers from the federal government, academia, and private industry searching for a better solution.

Now a new set of software tools, the Next Generation Water Resources Modeling framework (NextGen), will help develop better predictions. As detailed in a new study led by OWP and the University of Vermont (UVM), with collaborators from nine other institutions, NextGen is a novel framework that allows OWP to make more accurate, representative flood forecasts; and allows researchers, students, and practitioners to experiment with and develop more advanced hydrologic models.

The paper is published in the JAWRA Journal of the American Water Resources Association.

"This paper represents years of close collaboration between scientists and software engineers at the National Weather Service, other federal agencies, the private sector, and universities across the country," said Dr. Keith Jennings, the Director of Research at UVM's Water Resources Institute. "The ultimate goal is to create more accurate, timely flood forecasts with the National Water Model to save lives during severe weather events. The NextGen framework is the software platform we created to do just that."

Complex challenges in water prediction

In addition to improving flood forecasts, NextGen work was also inspired by some of the biggest challenges facing hydrologists.

Water moves through the landscape in complex ways, traversing terrain at varying rates and across different routes. This unpredictability causes numerous challenges for researchers, developers, water managers, and operational forecasters when it comes to water prediction.

There are sizable gaps in understanding water processes from streamflow to rainfall and snowmelt. Hydrologists and water resources engineers complement field studies by employing or developing computational models to understand this hard-to-observe phenomenon. These models can overcome shortcomings in measurements, process understanding, and forecasting.

But computational models, with their variety of formulations, programming languages, compilers, data models, and required inputs, require considerable effort to understand and apply. So researchers and practitioners tend to choose models based on familiarity instead of the model that is most appropriate for their study and objectives.

There is no one perfect model.

How the NextGen framework works

To support water prediction needs and enable greater flexibility to use the right model in the right place at the right time, NextGen is "model-agnostic." It uses common standards, and is user-friendly and open-source.

The framework enables scientific evaluation of water prediction models that simulate diverse hydrologic and hydraulic processes. Its design supports models written in multiple programming languages, and runs on laptops, cloud, and supercomputers.

These capabilities will advance hydrologic science and help OWP make better forecasts. The National Water Model, which is slated to use the NextGen framework for its next operational version, needs to provide accurate water resources modeling for a variety of purposes, including flood forecasting, reservoir operations, and drought prediction.

However, the current operational National Water Model, like all computer models, suffers biases and errors that affect its predictive capabilities. Its performance also varies, working best in the Pacific Northwest and northern Rocky Mountains. These challenges, combined with the ever-present need for improving hydrologic forecast accuracy, created a need for a new modeling framework.

Key capabilities and future impact

NextGen has a wide range of capabilities that will enhance the next National Water Model. These include 1) the use of user-defined, not model-specific, geospatial data to define model domains, initialize parameter values and model states, and to build stream networks for flow routing, 2) the execution of various models and modules in the same framework using the same configuration system and execution commands, and 3) the production of model outputs in a standardized format over a consistent domain regardless of the chosen model.

NextGen has capabilities that promise to advance hydrologic and hydraulic modeling. By providing a common operating environment, collaboration will be increased between the research community and federal agencies. This will speed up operational implementation, initiate an increased pace of discovery, create more accurate and less redundant modeling, and ultimately, provide more effective water resource forecasts and predictions. 

Source: A new framework could transform national flood prediction    

Ariane 6: more boosters, more power - European Space Agency, ESA


 

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Short Film - Natalie Portman - Hotel Chevalier (2007) - Drama - Romance - Short Film directed by Wes Anderson

A prologue of one heart-breaking history of love and the prologue of the travel told in Darjeeling Limited (2007).




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Friday, February 13, 2026

NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles - UNIVERSE

For the first time, astronomers using NASA’s Fermi Gamma-ray Space Telescope have traced a budding outflow of gas from a cluster of young stars in our galaxy — insights that help us understand how the universe has evolved as NASA explores the secrets of the cosmos for the benefit of all.

The cluster, called Westerlund 1, is located about 12,000 light-years away in the southern constellation Ara. It’s the closest, most massive, and most luminous super star cluster in the Milky Way. The only reason Westerlund 1 isn’t visible to the unaided eye is because it’s surrounded by thick clouds of dust. Its outflow extends below the plane of the galaxy and is filled with high-speed, hard-to-study particles called cosmic rays.

“Understanding cosmic ray outflows is crucial to better comprehending the long-term evolution of the Milky Way,” said Marianne Lemoine-Goumard, an astrophysicist at the University of Bordeaux in France. “We think these particles carry a large amount of the energy released within clusters. They could help drive galactic winds, regulate star formation, and distribute chemical elements within the galaxy.”

paper detailing the results published Dec. 9 in Nature Communications. Lemoine-Goumard led the research with Lucia Härer and Lars Mohrmann, both at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany.

This image of super star cluster Westerlund 1 was captured with the Near-InfraRed Camera on NASA’s James Webb’s Space Telescope. The cluster is largely hidden at visible wavelengths by dust clouds, which infrared light penetrates. Westerlund 1’s large, dense, and diverse stellar population of massive stars has no other known counterpart in the Milky Way.

ESA/Webb, NASA & CSA, M. Zamani (ESA/Webb), M. G. Guarcello (INAF-OAPA) and the EWOCS team

Super star clusters like Westerlund 1 contain more than 10,000 times our Sun’s mass. They are also more luminous and contain higher numbers of rare, massive stars than other clusters.

Scientists think that supernova explosions and stellar winds within star clusters push ambient gas outward, propelling cosmic rays to near light speed. About 90% of these particles are hydrogen nuclei, or protons, and the remainder are electrons and the nuclei of heavier elements.

Because cosmic ray particles are electrically charged, they change course when they encounter magnetic fields. This means scientists can’t trace them back to their sources. Gamma rays, however, travel in a straight line. Gamma rays are the highest-energy form of light, and cosmic rays produce gamma rays when they interact with matter in their environment.

Most gamma-ray observations of stellar clusters have limited resolution, so astronomers effectively see them as indistinct areas of emission. Because Westerlund 1 is so close and bright, however, it’s easier to study.

In 2022, scientists using a group of telescopes in Namibia operated by the Max Planck Institute called the High Energy Spectroscopic System detected a distinct ring of gamma rays around Westerlund 1 with energies trillions of times higher than visible light.

Lemoine-Goumard, Härer, and Mohrmann wondered if the cluster’s unique properties might allow them to see other details by looking back through nearly two decades of Fermi data at slightly lower energies — millions to billions of times the energy of visible light.

Fermi’s sensitivity and resolution allowed the researchers to filter out other gamma-ray sources like rapidly spinning stellar remnants called pulsars, background radiation, and Westerlund 1 itself.

What was left was a bubble of gamma rays extending over 650 light-years from the cluster below the plane of the Milky Way. That means the outflow is about 200 times larger than Westerlund 1 itself.

Data from NASA’s Fermi Gamma-ray Space Telescope reveal the budding gas bubble of star cluster Westerlund 1. Brighter colors indicate a stronger likelihood that gamma rays arise from specific types of point sources, notably two pulsars located at center and in the brightest portion of the image. Pink contours denote steep changes in likelihood. An underlying orange-magenta feature extends down the image, starting from the cluster’s location, and represents the nascent outflow. The grey lines indicate distance below the galactic plane. The bubble is over 650 light-years long and angles slightly away from us. Westerlund 1’s stellar activity more easily pushes gas outward into lower-density regions of the galaxy’s disk.

NASA's Goddard Space Flight Center/Lemoine-Goumard et al. 2025; ESA/Webb, NASA & CSA, M. Zamani (ESA/Webb), M. G. Guarcello (INAF-OAPA) and the EWOCS team

The researchers call this a nascent, or early stage, outflow because it was likely recently produced by massive young stars within the cluster and hasn’t yet had time to break out of the galactic disk. Eventually it will stream into the galactic halo, the hot gas surrounding the Milky Way.

Westerlund 1 is located slightly below the galactic plane, so the researchers think the gas expanded asymmetrically, following the path of least resistance into a zone of lower density below the disk.

“One of the next steps is to model how the cosmic rays travel across this distance and how they create a changing gamma-ray energy spectrum,” Härer said. “We’d also like to look for similar features in other star clusters. We got very lucky with Westerlund 1, though, since it’s so massive, bright, and close. But now we know what to look for, and we might find something even more surprising.”

“Since it started operations 17 years ago, Fermi has continued to advance our understanding of the universe around us,” said Elizabeth Hays, Fermi’s project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “From activity in distant galaxies to lightning storms in our own atmosphere, the gamma-ray sky continues to astound us.”

By Jeanette Kazmierczak
NASA’s 
Goddard Space Flight Center, Greenbelt, Md.
  

Source: NASA’s Fermi Spots Young Star Cluster Blowing Gamma-Ray Bubbles - NASA Science  

Neptunium study yields plutonium insights for space exploration - Energy & Green Tech

Credit: Pixabay/CC0 Public Domain

Researchers at the Department of Energy's Oak Ridge National Laboratory are breathing new life into the scientific understanding of neptunium, a unique, radioactive, metallic element—and a key precursor for production of the plutonium-238, or Pu-238, that fuels exploratory spacecraft.

The ORNL team's research arrives during a period of increased national interest in the use of Pu-238 in radioisotope thermoelectric generators, or RTGs. Often used in space missions such as NASA's Perseverance Rover for long-term power, RTGs convert heat from radioactive decay into electricity. Advancing RTG knowledge and application possibilities also requires the same high-level evaluation of both chemical reactions and structural characterization, two key aspects of the materials science for which ORNL is known.

"When people want to do scientific experiments in space, they need something to power their instruments, and plutonium is typically the power source because things like solar and lithium ion batteries don't withstand deep space," said Kathryn Lawson, radiochemist in ORNL's Fuel Cycle Chemical Technology Group and lead author of the new study.

"Plutonium is the solution, so the more scientific inquiry there is to go on a spacecraft, you need to have these types of batteries," said Lawson. "The demand always exceeds our supply. Hence, we need to have a great understanding of neptunium chemistry to support that production of Pu-238."

The team's findings, which illuminate important chemical and structural aspects of neptunium, were discovered through thermal decomposition—or by breaking down neptunium samples with heat—helping scientists to identify critical intermediate phases and guide more precise thermal treatments to discover additional neptunium insights.

The research is published in the journal Inorganic Chemistry Frontiers.

At ORNL, this and other modern characterization techniques provide useful data on neptunium's chemistry, helping advance the lab's Pu-238 production process. A critical radioisotope for use in space exploration is being produced at ORNL.

Neptunium is an important precursor of Pu-238, meaning it participates in a nuclear reaction that eventually results in Pu-238. Unlocking neptunium's complex secrets for a better understanding of its chemistry will enable more efficient, effective Pu-238 production. By improving how we understand and work with neptunium, ORNL is helping to ensure a secure, domestic supply chain for this mission-critical material, while fueling deep space exploration and advancing U.S. energy independence.

In the early 1980s, ORNL designed the original thermal decomposition process for uranium analysis. Today, Lawson and her colleagues across the lab are deploying the method to break down neptunium samples with steadily increasing heat, from 150 to 600 degrees Celsius—302 to 1,112 degrees Fahrenheit—and using multiple measurement techniques to analyze the resulting chemical reactions.

By integrating the results from each categorization and measurement technique—including Raman spectroscopy, which bombards samples with lasers to examine molecular vibrations, and computational modeling, which offers a mathematic comparison point against the team's scaled experiments—the researchers discovered new mechanistic and materials chemistry information. Including the first detailed Raman fingerprint of a key neptunium oxide, these findings help advance a general understanding of neptunium while improving the lab's specific process for Pu-238 production.

"My group and I were looking at this from a structural point of view, to help understand the decomposition mechanism. Essentially, what we do is use Raman spectroscopy to shoot lasers at the sample and excite different vibrations in the structure of the material," said nuclear security scientist Tyler Spano of ORNL's Materials and Chemistry Group, a contributing researcher to the recently published study.

"What comes out is a series of peaks, a spectrum. That tells us something about the current material structure, but what we did was follow the heating pathway that Kathryn [Lawson] uses for the material," said Spano. "We made these measurements as we were heating the material, so we could see how the chemical bonding environments were changing as we increased the temperature."

The study reunited a familiar cohort of early-career staff spanning three research directorates at ORNL, including National Security Sciences, Fusion and Fission Energy and Science, and Isotope Sciences and Enrichment. Now colleagues and collaborators at ORNL, Spano and Lawson met more than a decade ago at the University of Notre Dame, when Spano served as Lawson's graduate teaching assistant, and they worked side by side in the same university research lab. In 2020, they were reunited when Lawson joined Spano at ORNL.

"I had started a couple years before that and was so excited when Kathryn started," said Spano. "Our community is small, and the pool of people who have the expertise that you can work with in this field is so limited. It's exciting to know that someone else who thinks literally about science and the important questions is going to be here."

Lawson, Spano and their ORNL colleagues and collaborators on neptunium research are contributing to the history of understanding radioactive, metallic elements, or actinides, such as uranium, neptunium and plutonium. Meanwhile, they're adding to the resurgence of interest in neptunium's possibilities for advancing Pu-238 science.

"We're already working on our next project. It's again very basic-science-focused, and we're looking at the decomposition of some other neptunium compounds," said Lawson. "Essentially, we've figured out that we have these capabilities, and so we're looking at a number of other poorly understood neptunium compounds that are all going to be potentially of interest for Pu-238 production."

Together, Lawson, Spano and their fellow early-career researchers are helping to reinvigorate the study of neptunium chemistry and contributing to a shared understanding of the natural world, even though naturally occurring neptunium is exceedingly rare.

"It's so fun to get to research with your friends. It's all in the family," said Spano. "There are so few people who do this type of research. We all know each other, and it's just really beneficial to work together and pool our resources and capabilities."

At a place like ORNL, that unique collection of people and capabilities can yield important innovations in energy research and scientific discovery.

"This work is fun because it supports RTGs, and that side of things really captivates people when they talk about space," said Lawson. "That's what I get to tell my family: I make batteries for space. That's the nutshell. Making the best and the most batteries for space, so that we can continue to explore our solar system." 

Provided by Oak Ridge National Laboratory  

Source: Neptunium study yields plutonium insights for space exploration