The Curious Case of the Kidnapped Howlers: Capuchin Monkeys Exhibit New Cultural Behavior

Researchers document young male capuchins on a Panamanian island abducting baby howler monkeys in a first-ever case of non-adaptive primate cultural behavior.

On a remote island in Panama’s Coiba National Park, researchers have recorded white-faced capuchin monkeys engaging in an unusual form of social behavior that has not previously been documented in any primate species. Over a 15-month period, five immature male capuchins were observed carrying infant howler monkeys for multiple days at a time.

A study published in the May 2025 issue of Current Biology describes the behavior as a “non-adaptive cultural tradition.” According to the authors, the capuchins repeatedly abducted and transported at least eleven individual howler monkey infants between January 2022 and March 2023. The scientists concluded that the behavior provided no clear benefit to the carriers and was not motivated by food acquisition, parental care, or play.

“This is the first known documentation of a cultural tradition in which animals repeatedly abduct and carry infants of another species—without any clear benefit to themselves,” said lead author Zoë Goldsborough, a researcher with the Max Planck Institute of Animal Behavior.

Capuchins are a genus of New World monkeys known for their cognitive flexibility, complex social lives, and frequent use of tools. They are part of the Cebinae subfamily, whose members have demonstrated some of the most sophisticated learned behaviors observed among non-human primates. In the wild, capuchins have been recorded using sticks to extract insects from cavities, smashing fruits and snails against hard surfaces, and even fashioning probing tools for termite fishing.

Social learning is central to capuchin societies. Young individuals often acquire behaviors by watching others, and juveniles have been documented imitating older group members in tasks such as food processing and grooming rituals. Tool use, play-fighting, cooperative alliances, and certain vocalizations are among the behaviors known to be passed down through observation rather than instinct.

The capuchin group studied on Jicarón Island has previously been identified for its habitual use of stone tools to crack nuts and shell Terminalia seeds. To monitor the group’s behavior over time, researchers deployed 86 motion-triggered cameras across the monkeys’ home range. These cameras captured 131 separate instances in which capuchins were seen carrying howler infants. These infants, according to the study, were estimated to be between one and four weeks old.

The researchers traced the behavior’s origin to January 2022, when a juvenile male nicknamed “Joker” was first recorded carrying a howler infant. He later carried three additional howler monkeys. By September 2022, the behavior had spread to four other immature males. The carriers transported the infants on their backs and stomachs during normal activities such as foraging and resting. Some infants were carried for as long as nine consecutive days.

“Most howler infants appeared healthy in initial sightings, but deteriorated over time. At least four howler infants died, seemingly from malnourishment,” the authors wrote. There was no evidence of wounding, consumption, or predation. In one recorded encounter, several capuchins prevented an adult howler from recovering her infant by posturing and issuing threat displays.

The press release issued by the Max Planck Institute emphasized that “the males don’t eat the infants, they don’t play with them, and they don’t receive more attention from their group mates while carrying an infant.” The study’s authors found no indication that the behavior conferred status or reproductive advantages on the carriers. “Capuchins appear to carry howler infants solely for carrying’s sake,” the paper states.

Later adopters of the behavior were recorded engaging in actions that increased risk to the infants, including opening nuts with stones while carrying them. In one case, a howler infant fell from the carrier’s back during such activity. The authors describe the behavior as a potential “fashion trend,” referencing earlier findings from chimpanzee groups in which individuals placed grass in their ears despite the absence of any clear function.

While reports of cross-species caregiving exist in the animal kingdom, they are rare and often limited to isolated cases. Domestic dogs have been known to nurse kittens or piglets. Some dolphins have been seen assisting injured members of other cetacean species. However, systematic and socially transmitted interspecies caregiving behaviors are not well documented outside of primates. In particular, repeated, non-functional interspecies infant carrying, such as that reported by the Jicarón study, has not been previously confirmed in any non-primate animal population under natural conditions.

The howler monkeys involved in the study belong to the subspecies Alouatta palliata coibensis, which is endemic to Coiba National Park and classified as endangered. The authors note the potential implications of this behavior for conservation. “If this tradition of infant abduction persists, it poses a serious conservation risk,” the paper concludes.

The findings expand the scope of research into primate behavioral traditions. They also raise questions about the emergence of behaviors that spread through imitation without yielding clear evolutionary advantages. As Goldsborough and her colleagues suggest, under certain ecological conditions, including low predator pressure and minimal social disruption, primate societies may create cultural behaviors that are not directly tied to survival or reproduction.

The behavior recorded on Jicarón Island illustrates how social learning can produce unexpected outcomes in the animal world. It also reinforces the importance of long-term behavioral monitoring in understanding the dynamics of wildlife populations and the cultural traits that may influence their future.

Goldsborough, Zoë, et al. “Rise and Spread of a Social Tradition of Interspecies Abduction.” Current Biology, vol. 35, no. 10, 2025, pp. R375–R376.

April 2025 Was Earth’s Second-Warmest April on Record, Reports Confirm

April 2025 was Earth’s second-warmest April on record, with temperatures staying more than 1.5°C above pre-industrial levels, according to NOAA and Copernicus.

Global temperatures in April 2025 remained alarmingly high, registering as the second-warmest April since global record-keeping began in the mid-19th century, according to data released by both the European Union’s Copernicus Climate Change Service and the U.S. National Oceanic and Atmospheric Administration.

The April report, released by C3S on May 7, found that Earth’s average surface air temperature reached 14.96 degrees Celsius, or 0.60 degrees above the 1991–2020 average for the month. That temperature remains more than 1.5 degrees Celsius above the estimated pre-industrial norm, marking the eleventh consecutive month at or above that threshold. These global readings are based on the ERA5 reanalysis dataset, maintained by the European Centre for Medium-Range Weather Forecasts and publicly available at climate.copernicus.eu.

NOAA, in its April global climate summary published on May 14, corroborated these findings. Using its own global land and ocean database, NOAA reported that Earth’s average temperature in April was 1.22 degrees Celsius above the 20th-century average. That made it the second-warmest April in NOAA’s 175-year record. NOAA observed that “[t]emperatures were above normal across much of the globe in April,” with notable warmth in “eastern Europe, the Russian Far East, western North America, and much of Africa,” while temperatures in “parts of Australia, Greenland, and Antarctica” were below average. NOAA’s full report is available at ncei.noaa.gov.

For scientists tracking long-term climate change, monthly reports such as these provide high-resolution insight into a warming trend driven by human emissions of greenhouse gases. While year-to-year and month-to-month variability can be influenced by factors such as volcanic activity or the El Niño–Southern Oscillation, sustained monthly anomalies above historical norms are strong indicators of systemic climate warming. According to both C3S and NOAA, the April data confirm this persistent pattern.

Sea surface temperatures, another indicator of climate health, also remained exceptionally high in April. Copernicus reported that the average SST between latitudes 60°S and 60°N reached 20.89 degrees Celsius, which was 0.39 degrees above the 1991–2020 average and nearly matched the all-time high recorded in 2024.

NOAA, using a similar 60°S–60°N SST dataset, confirmed that April 2025 recorded the second-warmest global ocean temperature for the month. This follows a streak of record- or near-record-high SSTs dating back to May 2023. Warming oceans contribute to coral bleaching, sea level rise, and stronger tropical storms, and they reduce the ocean’s capacity to absorb atmospheric carbon.

In the cryosphere, sea ice extent remained below average in both hemispheres. Arctic sea ice at the end of April measured 13.6 million square kilometers, which C3S identified as the sixth lowest April extent in the 47-year satellite record. NOAA data further indicated that Arctic sea ice extent was 160,000 square miles below the 1991–2020 average, particularly in the Barents, Okhotsk, Bering, and Labrador Seas.

In the Southern Hemisphere, Antarctic sea ice remained far below normal, continuing a long-term decline that began in 2017. “In April, the Antarctic region recorded its 10th lowest sea ice extent in the satellite record at about 10% below the 1991–2020 average,” according to the Copernicus report. NOAA reported a shortfall of 320,000 square miles in Antarctic sea ice, with below-average extent in most sectors except the Weddell and Amundsen Seas.

Snow cover also receded dramatically. NOAA observed that the Northern Hemisphere’s snow cover extent tied with April 2024 as the smallest in the satellite record, which began in 1967. North America, Eurasia, and Greenland all exhibited below-average snow coverage.

Precipitation patterns showed major regional anomalies. NOAA reported unusually dry conditions in much of the Northern Hemisphere, but record-setting rainfall and flooding occurred in central Asia and parts of Africa. “Flooding and landslides occurred in Brazil, Congo, and western Somalia due to heavy rains,” the agency stated.

Oceanic and atmospheric circulation patterns continued to reflect the lingering influence of the El Niño phase that began in 2023. While forecasters expect a transition to neutral conditions by summer 2025, global sea surface temperatures have remained historically high even as El Niño weakens.

Despite April’s record warmth, NOAA noted that tropical cyclone activity remained average. Four named storms developed globally during the month. These included Severe Tropical Cyclone Courtney in the southwest Indian Ocean, two storms in the Australian region, and one in the southwest Pacific basin.

Together, the April reports from NOAA and Copernicus underscore what climate scientists describe as a broad-based and accelerating warming trend. Their findings reflect the compounding impacts of long-term greenhouse gas accumulation, regional feedbacks such as sea ice loss, and global-scale ocean warming.

Scientists and climate policy experts will continue to watch these monthly anomalies as preparations begin for the United Nations Framework Convention on Climate Change COP30 summit, scheduled for November 2025 in Belém, Brazil.

Both the Copernicus report and NOAA’s full April analysis are available online.

RESOURCES

Copernicus Climate Change Service. “2nd Warmest April Globally Remains 1.5°C Above the Pre-Industrial Level.” Copernicus Climate Change Service, 7 May 2025, https://climate.copernicus.eu/2nd-warmest-april-globally-remains-15degc-above-pre-industrial-level.Copernicus Climate Change Service.

Copernicus Climate Change Service. “Surface Air Temperature for April 2025.” Copernicus Climate Change Service, 7 May 2025, https://climate.copernicus.eu/surface-air-temperature-april-2025.Copernicus Climate Change Service.

NOAA National Centers for Environmental Information. “Assessing the Global Climate in April 2025.” NOAA National Centers for Environmental Information, 12 May 2025, https://www.ncei.noaa.gov/news/global-climate-202504.

NOAA National Centers for Environmental Information. “Global Climate Report for April 2025.” NOAA National Centers for Environmental Information, May 2025, https://www.ncei.noaa.gov/access/monitoring/monthly-report/global/202504.

Urban Trees and the Climate Equation: New Research Underscores the Need for Tailored Urban Forestry Strategies

A new USGS study shows urban trees cool cities unevenly, offering stronger relief in arid zones than in humid climates and reshaping urban heat planning.

A comprehensive study conducted by researchers at the U.S. Geological Survey (USGS) and published in Sustainable Cities and Society has sharpened scientific understanding of how urban tree cover influences heat reduction in American cities. The research confirms what many planners and scientists have long observed in practice: trees can help cool urban environments, but their effects are not uniform and depend heavily on a city’s prevailing climate.

Urban heat islands, which occur when built surfaces absorb and re-emit the sun’s heat, present an increasingly urgent public health and environmental challenge. In cities dominated by asphalt, concrete, and limited vegetation, elevated temperatures can intensify the risk of heat-related illness, drive up electricity demand, and reduce overall livability. As the frequency and intensity of heat waves rise, urban planners and policymakers are under growing pressure to identify strategies that reduce these impacts while making efficient use of public resources.

“All trees have a cooling effect, but trees in hot, dry areas can have a greater impact than in humid cities,” said Peter Ibsen, a research biologist at the USGS and lead author of the study. “Trees in areas like Las Vegas, Phoenix, and Tucson are particularly effective at reducing heat.”

The study analyzed detailed satellite and land cover data from more than one hundred U.S. cities. Drawing from seventeen distinct climate zones, the research team used machine learning to isolate the impact of tree canopy on urban temperatures. They evaluated those effects across both typical summer days and periods of extreme heat.

In dry, arid regions, tree cover was consistently associated with substantial reductions in air temperature. The analysis found that tree canopy in these environments can lower daytime temperatures by as much as 4.2 degrees Celsius. At night, those reductions remained significant, with cooling effects reaching 3.4 degrees Celsius. The presence of trees had its most pronounced impact during heat waves, when built environments typically radiate heat back into the air at the end of the day.

By contrast, the data from humid cities revealed more mixed results. In metropolitan areas such as Miami, the presence of tree canopy was not always associated with clear reductions in heat. In some cases, tree-covered areas retained warmth overnight, likely due to a combination of higher atmospheric moisture, dense vegetation, and restricted airflow. These findings suggest that tree canopy, while valuable, may not produce consistent cooling across all climatic settings.

Prior studies have long documented the cooling and ecological benefits of urban tree cover. Research published in Landscape and Urban Planning in 2010 found that tree canopy can reduce daytime air temperatures in temperate cities by up to two degrees Celsius. Similarly, a 2019 study in the Proceedings of the National Academy of Sciences concluded that tree cover significantly reduces surface temperatures in urban neighborhoods dominated by impervious materials. These findings have informed years of investment in tree planting and greening initiatives. What distinguishes the new study by the USGS is its emphasis on variation across climate zones. Rather than assuming uniform performance, the USGS team shows that trees cool more effectively in arid regions than in humid ones, where nighttime heat retention can complicate their impact. That insight suggests that planners should not only continue to expand urban tree canopy but also design these investments with local climate conditions in mind.

The authors of the USGS study emphasized that “the effectiveness of urban tree canopy in cooling is strongly linked to the region’s climate characteristics.” That conclusion directly challenges the idea that tree planting alone can serve as a universal solution to urban heat. Instead, the researchers encourage city officials to match green infrastructure investments with the specific ecological and meteorological realities of each location.

For cities located in dry climates, the policy implications are relatively straightforward. Strategic investment in urban tree cover can provide measurable and significant reductions in heat, particularly if the species selected are drought-tolerant and well-suited to local water constraints. Expanding canopy coverage in these areas offers a viable and evidence-based adaptation tool.

In more humid regions, municipal governments and urban designers may need to consider a broader range of solutions. While trees remain a valuable part of the landscape, other strategies such as reflective building materials, improved ventilation corridors, and more effective stormwater infrastructure may need to be deployed in parallel to achieve meaningful reductions in heat exposure.

The study represents a growing body of climate-focused research that calls for nuance and specificity in urban adaptation planning. As cities continue to grapple with the consequences of climate change, including more frequent and intense heat events, relying on generalized interventions may not be sufficient. Instead, targeted, data-informed strategies that reflect the environmental complexity of each community will be essential to making cities cooler, healthier, and more resilient.

NOTE: This story was updated on May 22, 2025.


Further Information

  • Bowler, Diana E., et al. “Urban Greening to Cool Towns and Cities: A Systematic Review of the Empirical Evidence.” Landscape and Urban Planning, vol. 97, no. 3, 2010, pp. 147–155. https://doi.org/10.1016/j.landurbplan.2010.05.006
  • Gill, Susannah E., et al. “Adapting Cities for Climate Change: The Role of the Green Infrastructure.” Built Environment, vol. 33, no. 1, 2007, pp. 115–133. https://doi.org/10.2148/benv.33.1.115
  • Ibsen, Peter, et al. “Urban Tree Cover Provides Consistent Mitigation of Extreme Heat in Arid but Not Humid Cities.” Sustainable Cities and Society, 2024. https://doi.org/10.1016/j.scs.2024.105135
  • Nowak, David J., and John F. Dwyer. “Understanding the Benefits and Costs of Urban Forest Ecosystems.” Urban and Community Forestry in the Northeast, edited by John E. Kuser, Springer, 2007, pp. 25–46. https://doi.org/10.1007/978-1-4020-4289-8_2
  • Voskamp, Ilse M., and Frans H. M. van de Ven. “Planning Support System for Climate Adaptation: Composing Effective Sets of Blue–Green Measures to Reduce Urban Vulnerability to Extreme Weather Events.” Building and Environment, vol. 83, 2015, pp. 159–167. https://doi.org/10.1016/j.buildenv.2014.07.018
  • Ziter, Carly D., et al. “Scale-Dependent Interactions Between Tree Canopy Cover and Impervious Surfaces Reduce Daytime Urban Heat During Summer.” Proceedings of the National Academy of Sciences, vol. 116, no. 15, 2019, pp. 7575–7580. https://doi.org/10.1073/pnas.1817561116

Berkeley Lab Demonstrates New Livermorium Synthesis Method, Paving Way for Element 120

Berkeley Lab scientists used a titanium-50 beam to create livermorium, opening a new path to synthesizing superheavy elements like element 120.

Scientists have taken a critical step toward extending the periodic table, successfully using a novel reaction to create atoms of livermorium—an element so unstable it vanishes in a fraction of a second. The experiment, conducted at Lawrence Berkeley National Laboratory, paves the way for attempts to synthesize element 120, a candidate for the long-hypothesized “island of stability.”

What Makes Superheavy Elements Special?

Superheavy elements are artificially created atoms with atomic numbers greater than 104. These elements do not occur naturally and must be produced in laboratories through nuclear fusion reactions. Located at the far end of the periodic table beyond the actinide series, superheavy elements belong to the transactinide group. Because of the intense repulsion between the large number of protons in their nuclei, these elements tend to be highly unstable and decay quickly.

Radioactive decay, particularly alpha decay, is the dominant mechanism by which these elements lose energy. In alpha decay, the nucleus emits a particle composed of two protons and two neutrons. This process rapidly alters the identity of the atom and limits how long scientists can observe its behavior. For example, livermorium-293, one of the most stable known isotopes of element 116, has a half-life of just 53 milliseconds.

A New Reaction Pathway

The experiment was conducted using Berkeley Lab’s 88-Inch Cyclotron, a particle accelerator capable of producing high-energy ion beams. In this case, a beam of titanium-50 ions was directed at a plutonium-244 target. Under extreme conditions, the two nuclei fused to form livermorium atoms. These atoms were detected and analyzed using the SHREC (Super Heavy RECoil) detector, a position-sensitive, time-of-flight-enabled system designed to isolate and capture the brief decay sequences of superheavy nuclei.

“This reaction had never been demonstrated before, and it was essential to prove it was possible before embarking on our attempt to make 120,” said Jacklyn Gates, a nuclear scientist at Berkeley Lab. “Creation of a new element is an extremely rare feat. It’s exciting to be a part of the process and to have a promising path forward.”

The experiment yielded four decay chains attributed to livermorium-293, confirming that the reaction pathway using titanium-50 and plutonium-244 is viable, though extraordinarily rare.

Why Scientists Are Targeting Element 120

Although element 119 might seem like the next logical target, Berkeley Lab researchers are prioritizing element 120. The reason lies in the nuclear physics that governs fusion reactions. Superheavy element synthesis has extremely low production cross-sections, meaning the odds of successful fusion are tiny. Prior theoretical research has indicated that a reaction involving titanium-50 and californium-249 may offer a more promising path toward creating element 120.

While livermorium was first synthesized in 2000 by a Dubna–Livermore collaboration using calcium-48 and curium-248, the present experiment introduces a new reaction channel with different beam and target nuclei. This kind of exploratory synthesis is essential for mapping the best paths forward to even heavier elements.

One challenge is the availability of target materials. Californium-249 is rare and must be produced at specialized facilities such as Oak Ridge National Laboratory. Logistical considerations, including isotope handling, safety protocols, and regulatory controls, influence the choice of which element to pursue and when.

Toward the Island of Stability

The so-called “island of stability” refers to a hypothesized region in the periodic table where certain superheavy elements might have longer half-lives due to favorable combinations of protons and neutrons forming closed nuclear shells. Element 120 is thought to lie near this region, offering the potential for longer-lived isotopes than those currently known.

“We think it will take about 10 times longer to make 120 than 116,” said Reiner Kruecken, director of Berkeley Lab’s Nuclear Science Division. “It’s not easy, but it seems feasible now.”

Overcoming Challenges to Reach Element 120

The experiment required advances in beam production technology. Titanium is reactive with many gases, posing challenges for generating a high-current, stable beam. Damon Todd, an accelerator physicist at Berkeley Lab, explained that the team developed an inductive oven capable of maintaining a constant temperature over several days to stabilize titanium output.

The lab expects to begin its attempt to synthesize element 120 in 2025, pending successful target preparation and installation of additional safety and engineering controls. Collaborations with national labs and international institutions will play a critical role in the next phase.

“We’ve shown that we have a facility capable of doing this project, and that the physics seems to make it feasible,” Kruecken said. “Once we get our target, shielding, and engineering controls in place, we will be ready to take on this challenging experiment.”

Gates framed the broader importance of the work in conceptual terms. “We want to figure out the limits of the atom, and the limits of the periodic table. The superheavy elements we know so far don’t live long enough to be useful for practical purposes, but we don’t know what the future holds. Maybe it’s a better understanding of how the nucleus works, or maybe it’s something more.”

NOTE: This story was updated on May 22, 2025.

Reference

Gates, J. M., et al. “Towards the Discovery of New Elements: Production of Livermorium (Z=116) with 50Ti.” Physical Review Letters, vol. 133, no. 17, 2024, article 172502.

October 2024: Unprecedented Heat and Drought Across the U.S.

In October 2024, the contiguous United States experienced its second-warmest October since records began in 1895, with an average temperature of 59.0°F—4.9°F above the 20th-century average. This exceptional warmth was surpassed only by October 1963.

Record-Breaking State Temperatures

Several states reported unprecedented heat:

  • Arizona, New Mexico, Texas, and Utah each recorded their warmest October on record.
  • California, Colorado, Montana, and Wyoming experienced their second-warmest October.
  • An additional ten states ranked within their top ten warmest Octobers.

Severe Drought Conditions

The month also marked significant drought expansion:

  • The average precipitation across the contiguous U.S. was 0.95 inches—1.21 inches below average—tying with October 1963 as the second-driest October on record.
  • Delaware and New Jersey each had their driest October on record.
  • Nineteen additional states from Texas to the Northeast experienced their top ten driest Octobers.

By October 29, 2024, 87.16% of the contiguous U.S. was experiencing abnormally dry to exceptional drought conditions—the highest percentage in the 25-year history of the U.S. Drought Monitor.

Year-to-Date Climate Overview

From January through October 2024, the average U.S. temperature was 58.3°F, ranking as the second-warmest such period on record. States including Maine, Michigan, New Hampshire, New Mexico, New York, Ohio, Pennsylvania, Vermont, Virginia, West Virginia, and Wisconsin each experienced their warmest January–October on record.

Global Context

Globally, October 2024 was the second-warmest October in NOAA’s 175-year record, with temperatures 2.38°F (1.32°C) above the 20th-century average. North America experienced its warmest October on record, while South America and Oceania each had their second-warmest October.

Implications and Future Outlook

The combination of record-breaking heat and expanding drought conditions underscores the increasing variability and extremity of the U.S. climate. These patterns have profound implications for agriculture, water resources, and energy consumption, necessitating proactive measures to mitigate and adapt to these evolving climate challenges.

For a comprehensive analysis, refer to NOAA’s full reports:

Heat-Driven Droughts: A Paradigm Shift in Western U.S. Climate Dynamics

In recent years, the Western United States has experienced droughts of unprecedented severity. Traditionally, these droughts were attributed to a lack of precipitation. But a groundbreaking study published Nov. 6 in Science Advances reveals a significant shift: temperature-induced high evaporative demand, rather than precipitation deficits, has become the primary driver of droughts since 2000. This change underscores the profound impact of anthropogenic warming on regional climate patterns.

The study, led by Yizhou Zhuang of the Department of Atmospheric and Oceanic Sciences at UCLA, utilized observational data and climate model simulations to assess the contributions of precipitation and potential evapotranspiration to drought severity. Historically, precipitation deficits were the main culprits behind drought conditions. The analysis included in the new study indicates that since the turn of the century, PET—which represents the atmosphere’s demand for moisture—has played an increasingly dominant role. This shift is particularly evident in the 2020–2022 drought, where evaporative demand accounted for 61% of its severity, marking a departure from previous drought dynamics.

The implications of these findings are profound. As temperatures continue to rise due to human activities, the atmosphere’s capacity to extract moisture from the land increases, exacerbating drought conditions even in the absence of significant precipitation deficits. This paradigm shift necessitates a reevaluation of water management strategies, agricultural practices, and urban planning to mitigate the impacts of heat-driven droughts.

Moreover, climate projections under high-emission scenarios suggest that droughts of similar severity to the 2020–2022 event could become more frequent by the late 21st century. This underscores the urgency of addressing greenhouse gas emissions to curb future warming and its associated impacts on drought frequency and intensity.

The study highlights a critical transition in the drivers of drought in the Western United States, with temperature-induced evaporative demand now playing a central role. This shift calls for immediate attention to climate mitigation and adaptation strategies to safeguard water resources and ensure the resilience of ecosystems and human communities in the face of evolving climate dynamics.

The paper is here.

Photo of Lake Oroville, 2014. Courtesy NOAA.

Scientists Record Fastest Neutron Star Spin Rate, Challenging Limits of Stellar Physics

An international team of astronomers, led by Dr. Gaurava Jaisawal from the Technical University of Denmark (DTU), may have observed the fastest-spinning neutron star on record, potentially challenging established limits on stellar stability. Using NASA’s Neutron Star Interior Composition Explorer (NICER) aboard the International Space Station, the team recorded a rotation rate of 716 times per second in the neutron star 4U 1820–30, located about 26,000 light-years away in the Milky Way’s globular cluster NGC 6624. Published in The Astrophysical Journal, these findings could push the boundaries of neutron star physics, testing theories about how such stars can withstand rapid spin without breaking apart.

“Our findings show the neutron star’s rotation rate as among the fastest ever observed,” stated Dr. Jaisawal. “This challenges previously accepted models of neutron star stability.”

Understanding Neutron Stars and Their Extreme Nature

Neutron stars, the remnants of massive stars that collapse under intense gravitational force, are some of the densest objects in the universe. A single teaspoon of neutron star material would weigh about a billion tons on Earth, comparable to a skyscraper compacted into the size of a marble. Known for their rapid spin and powerful gravitational pull, neutron stars in binary systems can increase their spin rates over time by accreting material from a nearby companion star. The neutron star 4U 1820–30 orbits a white dwarf companion in a remarkably short 11.4-minute orbit, allowing it to pull in helium-rich material from its companion and generate periodic bursts of X-rays.

Precision Observations with NICER

The NICER team collected five years of data on 15 thermonuclear X-ray bursts emitted by 4U 1820–30. These bursts occur when material from the companion star ignites in nuclear fusion on the neutron star’s surface, producing intense bursts of radiation. NICER’s sensitive X-ray timing capabilities allowed the team to capture detailed data, revealing “photospheric radius expansion” (PRE) in each burst. This phenomenon occurs when radiation pressure from the burst pushes the neutron star’s outer layer outward, providing a clear measure of the star’s rapid spin.

In one particularly intense burst, described as a “superexpansion,” NICER recorded the outer layer expanding to nearly 900 kilometers—comparable to the radius of Earth’s largest moon—before collapsing back. NICER’s precision enabled the researchers to detect oscillations that suggested a rotation rate of 716 Hz, which, if confirmed, would set a new record for neutron star spin rates.

“NICER’s advanced timing technology, designed for capturing rapid oscillations down to the nanosecond, has provided us with unprecedented insights into neutron star behaviors,” Dr. Jaisawal said.

Implications for Neutron Star Stability

The recorded spin rate of 4U 1820–30 surpasses the theoretical limit of 600 rotations per second predicted by early models, which suggested that faster spins would destabilize the star. Exceeding this limit implies that neutron stars may maintain structural integrity even under extreme conditions, particularly in binary systems where they draw material from a companion. The accreted material adds angular momentum to the neutron star, accelerating its spin rate over time.

Accretion Disk Interactions and Stellar Dynamics

Beyond rotation rates, the NICER data revealed how bursts affect the neutron star’s surrounding accretion disk—a ring of gas drawn in from its companion. During the bursts, the team observed that radiation from the neutron star temporarily altered the accretion disk’s structure and ionization levels, suggesting a real-time interaction between the neutron star’s intense radiation and the surrounding matter. This phenomenon is akin to the way solar flares impact the magnetic fields around the Sun, creating ripple effects that alter the structure and behavior of nearby matter.

“Each burst showed changes in ionization at the peak, influenced by reflection modeling of the burst spectra,” the research team noted, underscoring NICER’s ability to document these complex interactions.

Setting New Standards in Astrophysics

The record-breaking spin rate of 4U 1820–30 could redefine how fast neutron stars can spin, setting a new benchmark for astrophysicists studying the limits of neutron star stability. According to the DTU press release, the findings are likely to prompt revisions to existing models of neutron star structure, stability, and formation. Neutron stars, with their extreme density and rotation, offer unique insights into the fundamental limits of matter under intense gravitational forces.

Future research aims to confirm the 716 rotations-per-second spin rate and explore what these findings reveal about neutron stars’ ability to endure high spin rates. NICER’s technology will continue to play a key role in advancing this field, providing insights into one of the universe’s most extreme phenomena. If confirmed, these observations may lead to a new understanding of how neutron stars withstand such high speeds and could prompt updated models of how these dense objects resist destabilization even under extreme conditions.

References
  1. Jaisawal, G., et al. (2024). “A Comprehensive Study of Thermonuclear X-Ray Bursts from 4U 1820–30 with NICER: Accretion Disk Interactions and a Candidate Burst Oscillation.” The Astrophysical Journal, 975(67).
  2. Hartman, J. M., Galloway, D. K., & Chakrabarty, D. (2003). “Burst Oscillations in the X-Ray Burster 4U 1608–52.” The Astrophysical Journal, 582(1), 11-14.
  3. Galloway, D. K., & Keek, L. (2021). “Thermonuclear (Type I) X-ray Bursts: An Observer’s Guide to the Universe’s Strongest Thermonuclear Explosions.” Annual Review of Astronomy and Astrophysics, 59, 59-98.
  4. Hessels, J. W. T., Ransom, S. M., Stairs, I. H., Kaspi, V. M., & Freire, P. C. C. (2006). “A Radio Pulsar Spinning at 716 Hz.” Science, 311(5769), 1901-1904.
  5. Degenaar, N., et al. (2018). “A Reflection Model for Thermonuclear X-Ray Bursts on Accreting Neutron Stars.” Monthly Notices of the Royal Astronomical Society, 478(4), 1661-1667.
  6. Kuulkers, E., & den Hartog, P. R. (2003). “Photospheric Radius Expansion Bursts and Eddington Luminosity.” Astronomy and Astrophysics, 399, 663-666.
  7. Watts, A. L. (2012). “Thermonuclear Burst Oscillations.” Annual Review of Astronomy and Astrophysics, 50, 609-640.

NASA’s Webb and Hubble Reveal a Stunning, Star-Forming Galaxy Collision

NASA’s Webb and Hubble telescopes have captured an extraordinary galaxy collision in IC 1623, revealing intense star formation fueled by cosmic dust. This rare look at galactic evolution offers insights into the powerful forces that shape our universe and the lifecycle of galaxies.

NASA’s Webb and Hubble telescopes have captured a galaxy collision happening 500 million light-years away. The new images show IC 1623, a galaxy pair, as it undergoes intense star formation fueled by dust and cosmic gas, offering scientists new insights into galactic evolution.


NASA’s James Webb Space Telescope and the Hubble Space Telescope have turned their advanced optics on a galaxy pair known as IC 1623. Located about 500 million light-years away in the constellation Cetus, this galaxy pair is in the midst of a collision that has ignited a high rate of star formation, or “starburst” activity. With the ability to capture visible, ultraviolet, and infrared wavelengths, Webb and Hubble reveal this merging galaxy’s unique red glow, which scientists say resembles “blood-soaked eyes.”

The intense red color seen in IC 1623 is caused by a combination of thick cosmic dust and rapid star formation. This interaction produces a high volume of infrared light, which Webb’s infrared capabilities capture in detail. Hubble’s ultraviolet sensitivity, in turn, shows how light escapes the dense dust regions, offering a fuller picture of the processes fueling star formation. These observations allow scientists to look deeper into the galaxy, providing unprecedented data on how galaxies like IC 1623 form new stars at extraordinary rates.

How Galaxies Collide and Create New Stars

Galactic collisions are a relatively common but impactful event in the universe. When two galaxies collide, their gravitational pull distorts their structures, forcing gas and dust into dense, compact regions. These areas serve as fertile grounds for star formation, which in IC 1623 is happening at a rate about 20 times faster than in the Milky Way. The energy released by new stars fuels the surrounding dust and gas, creating a feedback loop that can sustain star formation for millions of years.

In this particular starburst galaxy, scientists estimate that IC 1623 could one day stabilize and form a more typical elliptical galaxy. However, before reaching that point, the galaxy must first undergo a phase of intense activity marked by supernovae, radiation, and rapid star production, which could last several hundred million years.

Why Infrared and Ultraviolet Observations Matter

The Webb Telescope’s infrared sensitivity has been crucial to uncovering IC 1623’s unique red glow. Unlike Hubble, which operates primarily in visible and ultraviolet wavelengths, Webb’s infrared imaging can capture the heat and light emitted by young stars shrouded in thick cosmic dust. This combination of observations allows scientists to track the formation and evolution of galaxies even when they are hidden by dust clouds.

By combining data from Webb’s infrared and Hubble’s ultraviolet observations, scientists can see beyond the dust-obscured star-forming regions and gather detailed information about galactic structure. This makes IC 1623 an ideal case for studying galactic evolution and the lifecycle of starburst galaxies, which, according to astronomers, can contribute to our understanding of how the earliest galaxies might have formed.

What the Future Holds for Galaxy IC 1623

The insights from IC 1623 show that the violent collision of galaxies can lead to intense but short-lived periods of star formation. This “starburst” phase could eventually slow as radiation and stellar winds from massive stars push gas away from the galaxy core, creating a more stable environment.

NASA plans to continue observing IC 1623, tracking its development in the coming years. By studying how starburst galaxies transform into stable galaxies, astronomers hope to unlock key details about galactic history, evolution, and the forces shaping our own Milky Way.

NASA’s Mission to Uncover the Secrets of Galactic Evolution

These findings from NASA’s Hubble and Webb telescopes remind us that the universe is constantly evolving. Each new galaxy observation adds to the scientific understanding of how galaxies collide, form new stars, and transform. Webb and Hubble’s observations of IC 1623 provide a vivid look at the forces of cosmic creation and evolution, offering a glimpse into our universe’s dynamic history.

NASA’s combined observations mark a leap forward in how we understand the galactic processes that lead to star formation and change, emphasizing the continued role of telescopes in exploring the cosmos.


Resources for Further Exploration

Online Articles

Books

  • Sparke, Linda S., and John S. Gallagher III. Galaxies in the Universe: An Introduction. 2nd ed., Cambridge University Press, 2007.
    An introduction to galaxy formation and evolution, including topics like galactic collisions and starbursts.
  • Kormendy, John, and R. Bender. Dynamics of Galaxies. Annual Review of Astronomy and Astrophysics, 2013.
    Provides an in-depth look at galactic dynamics, with a focus on the forces driving galactic evolution and star formation.

Scientific Journal Papers

  • Kennicutt, Robert C., Jr. “Star Formation in Galaxies Along the Hubble Sequence.” The Astrophysical Journal, vol. 498, no. 2, 1998, pp. 541-552.
    Analyzes star formation across different types of galaxies, with special focus on starburst galaxies.
  • Hernquist, Lars, and N. Katz. “Simulations of Galaxy Mergers.” The Astrophysical Journal Supplement Series, vol. 70, 1989, pp. 419-446.
    A foundational paper on the role of gravitational dynamics in galactic collisions.

Videos

  • “What Happens When Galaxies Collide?” PBS Space Time, YouTube, 5 June 2019, https://www.youtube.com/watch?v=rzzQQuMqa7U.
    This video discusses galactic collisions and the changes they bring to star formation and galactic structure.
  • NASA Goddard. “Hubble’s Panoramic View of the Universe.” NASA Goddard Space Flight Center, 6 Feb. 2023, https://www.youtube.com/watch?v=Z1Gg9_O24nM.
    A detailed look at Hubble’s observations, including images of galactic mergers and other cosmic phenomena.

Additional Resources

Earth Records Hottest Day Ever on July 22, 2024: NASA and Copernicus Confirm Rising Global Temperatures

Earth experienced the highest average temperature in its recorded history last month.

Data from NASA indicates that the global average temperature reached an unprecedented level on July 22. The milestone underscores the escalating impacts of climate change.

The measurement is based on analysis from NASA’s Modern-Era Retrospective Analysis for Research and Applications, Version 2 (MERRA-2), and the Goddard Earth Observing System Forward Processing (GEOS-FP) systems. These systems integrate millions of observations from instruments on land, sea, air, and satellites using sophisticated atmospheric models.

The unprecedented heatwave was not an isolated incident. July 21 and July 23 also recorded temperatures surpassing previous highs, indicating a persistent and dangerous trend.

NASA’s findings are consistent with long-term data from the agency’s Goddard Institute for Space Studies (GISS), which has observed a consistent increase in global temperatures over the past several decades.

NASA administrator Bill Nelson emphasized the gravity of these findings.

“In a year that has been the hottest on record to date, these past two weeks have been particularly brutal,” said Nelson in a July 29 statement.

The European Union’s Copernicus Climate Change Service (C3S) also confirmed that July 2024 was shaping up to be the warmest month ever recorded globally.

C3S reported that the global average temperature on July 22 was 17.34°C (63.21°F), which surpassed the previous record set in August 2023.

The July 22 record and the late July heat wave follow 13 months of consecutive monthly temperature records. Scientists at NASA’s Goddard Institute for Space Studies in New York determined that year-plus long pattern based on the GISTEMP record, which relies only on data gathered by surface-based instruments. That record also allows for a longer-term view of global temperature changes on a monthly and annual basis dating to the late 19th century.

“The recent temperatures recorded are not just statistics; they are indicative of the drastic changes we are experiencing in our climate system,” said Carlo Buontempo, director of the Copernicus Climate Change Service.

Those changes have significant potential consequences for human health. Heatwaves can lead to increased mortality rates, especially among vulnerable populations such as the elderly, children, and those with pre-existing health conditions. And the stress on agriculture and water resources can exacerbate food and water insecurity, leading to broader social and economic impacts.

Resources

These resources offer valuable information for understanding the complex dynamics of climate change and the necessary steps to mitigate its effects:

  1. NASA Climate Change and Global Warming – Detailed information on the science of climate change, its causes, and impacts. NASA Climate
  2. Goddard Institute for Space Studies (GISS) – In-depth analyses and research findings on climate change. GISS Research
  3. Copernicus Climate Change Service – Monitors and analyzes global climate data. Copernicus Climate
  4. Intergovernmental Panel on Climate Change (IPCC) – Comprehensive reports on climate change science and policy. IPCC Reports
  5. National Oceanic and Atmospheric Administration (NOAA) Climate.gov – Resources on climate science, data, and impacts. NOAA Climate

Red Dwarf Stars Pose New Risks and Opportunities for Exoplanet Habitability

Astronomers have found that red dwarf stars emit far more ultraviolet (UV) radiation during flares than previously believed, posing significant risks to nearby planets’ potential to support life.

A groundbreaking study from the University of Hawaiʻi’s Institute for Astronomy (IfA), published in the Monthly Notices of the Royal Astronomical Society, reveals that these intense UV flares could erode planetary atmospheres, making them less habitable. However, the same radiation could also drive the chemical reactions needed to form the building blocks of life.

“Our findings show that many more stars may generate enough UV radiation through flares to impact planet habitability,” said Vera Berger, the lead author who conducted the study as part of the Research Experiences for Undergraduates program at IfA.

A Dual-Edged Sword

UV radiation from stellar flares has a complex role. While it can strip away a planet’s atmosphere, it can also contribute to the formation of RNA building blocks essential for life. The study analyzed data from 300,000 stars using the GALEX space telescope and discovered that far-UV emissions from these flares are, on average, three times more energetic than previously assumed and can be up to twelve times stronger.

Most studies have assumed a 9000 K blackbody spectrum for stellar flares, which produces more near-UV flux than far-UV flux. However, Berger’s team found the opposite, with excess far-UV reaching ratios roughly three to twelve times higher than expected. This discrepancy has major implications for understanding the true impact of stellar flares on exoplanets.

“A change of three is the same as the difference in UV in the summer from Anchorage, Alaska, to Honolulu,” explained Benjamin J. Shappee, an associate astronomer at IfA who mentored Berger. Such differences highlight the potential for far-UV radiation to significantly alter planetary conditions.

Implications for Habitability

This discovery challenges existing models of stellar flares and their impact on exoplanets. Higher levels of far-UV radiation could erode planetary atmospheres, reducing their ability to support life. This radiation can break down molecules like ozone, which protect planets from harmful UV radiation. The loss of ozone could leave a planet’s surface exposed to damaging radiation, making it less hospitable for life.

On the other hand, these intense flares might also foster prebiotic chemistry, creating RNA building blocks. High levels of UV radiation can drive chemical reactions that form complex organic molecules, essential for the development of life. This dual role of UV radiation from stellar flares makes the study of red dwarf stars particularly intriguing for astronomers searching for habitable exoplanets.

“This study has changed the picture of the environments around stars less massive than our Sun,” said Jason Hinkle, a PhD candidate at IfA and co-author of the study. Stars that were once considered benign may actually pose significant challenges for planetary habitability.

Looking Forward

The exact cause of the stronger far-UV emissions remains unclear, prompting calls for more data from space telescopes. Future missions like the planned Ultraviolet Transient Astronomy Satellite (ULTRASAT) may provide further insights into these emissions and their effects on exoplanetary atmospheres.

ULTRASAT aims to observe over 100,000 flaring and variable stars in the near-UV range. It will help scientists understand the frequency and intensity of UV flares, shedding light on their potential to impact planetary atmospheres. The Monitoring Activity from Nearby Stars with UV Imaging and Spectroscopy (MANTIS) mission will complement these observations by providing detailed UV spectra of cool stars, helping to differentiate between line and continuum emission during flares.

“Combining modern computer power with gigabytes of decades-old observations allowed us to search for flares on thousands of nearby stars,” noted Michael Tucker, a PhD graduate of IfA and now a postdoctoral fellow at Ohio State University. This approach underscores the importance of revisiting and reanalyzing archival data with new tools and perspectives.

Understanding these dynamics is crucial for accurate assessments of exoplanet habitability and the search for life beyond our solar system. The findings highlight the complex interplay between stellar activity and planetary environments, suggesting that planets around red dwarf stars face significant challenges in maintaining atmospheres conducive to life.

As of now, astronomers have identified over 5,000 exoplanets, encompassing a wide variety of types, including gas giants, rocky planets, and ice worlds. Many of these exoplanets orbit red dwarf stars, making the study’s findings particularly relevant. The potential impacts of UV radiation are critical for assessing the habitability of these diverse worlds, emphasizing the need for ongoing research.

For more details, read the full study in the Monthly Notices of the Royal Astronomical Society here.

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