Today's Image of the Day from NASA Earth Observatory features an explosive eruption of Mount Etna, the most active volcano in Europe. The photo was captured on February 13 by the OLI (Operational Land Imager) on the Landsat 8 satellite.



<a href="https://earthobservatory.nasa.gov/images/153962/river-of-fire-on-mount-etna" target="_blank" rel="noreferrer noopener">NASA</a> noted that the natural-color scene is overlaid with an infrared signal to distinguish the lava’s heat signature on the mountain's snowy slopes.



<h2 class="wp-block-heading" id="h-signs-of-unrest">Signs of unrest</h2>



“On February 8, 2025, Italy’s National Institute of Geophysics and Volcanology (INGV) reported that Mount Etna had begun exhibiting ‘signs of unrest above its background level,’” said NASA.



“That’s unsurprising for the frequently unruly Sicilian peak, one of the most active stratovolcanoes in the world. But the fiery explosions, disruptive ash clouds, and long lava flows that ensued stood out as being unusually spectacular to many Etna watchers.”



<h2 class="wp-block-heading" id="h-intensifying-eruptions-on-mount-etna">Intensifying eruptions on Mount Etna </h2>



The activity intensified on February 10th, with lava flowing from the Bocca Nuova crater at an altitude of approximately 3,000 meters above sea level.&nbsp;



According to news reports, the eruption created a striking visual as molten lava traversed the snow-covered slopes, producing rivers of lava up to 3 kilometers long and emitting ash plumes visible from several kilometers away.



The volcanic activity attracted thousands of tourists eager to witness the spectacle. However, the influx of visitors led to traffic congestion, obstructing emergency services and prompting warnings from local authorities about the potential dangers of approaching the active volcano.



<h2 class="wp-block-heading" id="h-impacts-of-mount-etna-eruptions">Impacts of Mount Etna eruptions </h2>



Despite the dramatic displays, there were no reports of injuries or significant property damage, though experts continue to closely monitor the situation.



Satellite imagery has provided detailed views of the active lava flow cutting through the snow-covered slopes, with ash plumes dispersing from the summit.



“The presence of ash prompted authorities to raise the aviation color code to orange on February 13. On other days during this eruption, it was elevated to red, the highest level of concern. The airport in nearby Catania diverted flights amid hazardous conditions, according to news reports,” said NASA.



“Since Etna stirred to life this time around, crowds of hikers and even some skiers flocked to its slopes to witness the fiery displays and lava flows melting through snow. The eruption was ongoing as of February 18, with weak ash emissions and decreasing explosive activity.”



<h2 class="wp-block-heading" id="h-a-volcano-with-a-long-history">A volcano with a long history </h2>



Mount Etna has a history stretching back hundreds of thousands of years. Located on the east coast of Sicily, near Catania, the volcano has shaped the landscape and influenced human civilization.



The volcano’s activity dates back at least 500,000 years, with its earliest eruptions occurring beneath the sea before the landmass emerged. Over time, lava flows, eruptions, and collapses have sculpted the towering stratovolcano seen today.



Ancient civilizations were well aware of Etna’s power. Greek mythology depicted it as the forge of Hephaestus, the god of fire, while the poet Pindar described its violent eruptions. The philosopher Empedocles was even said to have perished in its fiery depths.&nbsp;



Etna’s eruptions were documented throughout Roman history, including a major event in 122 BC that devastated Catania.



During the Middle Ages and Renaissance periods, Etna continued its eruptions, frequently altering its landscape and affecting nearby settlements.&nbsp;



<h2 class="wp-block-heading" id="h-monitoring-the-activity-of-mount-etna">Monitoring the activity of Mount Etna </h2>



One of the most devastating eruptions occurred in 1669, when lava flows destroyed several villages and overwhelmed parts of Catania’s city walls. Despite these dangers, people continued to live and farm on Etna’s fertile slopes, taking advantage of its rich volcanic soil.



Scientific study of Mount Etna began in the 19th and 20th centuries, as researchers sought to understand its behavior and mitigate its risks. Advances in monitoring technology have since helped track its activity, though eruptions remain unpredictable.&nbsp;



In modern times, Etna continues to be one of the most closely watched volcanoes in the world, with frequent eruptions, ash clouds, and lava flows affecting air travel and local communities.



Mount Etna was designated a UNESCO World Heritage Site in 2013 due to its geological significance and cultural history. 



Today, the volcano attracts tourists, scientists, and locals alike, serving as both a reminder of nature’s power and a source of economic and scientific interest.



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Fiery eruption of Mount Etna captured from space

Today's Image of the Day from NASA Earth Observatory features...

Today's Image of the Day from the European Space Agency features NGC 1333, a reflection nebula located in the Perseus molecular cloud about 960 light-years away from Earth. The photo is a mosaic of images captured by the James Webb Space Telescope.



<h2 class="wp-block-heading" id="h-the-power-of-webb-nbsp-nbsp">The power of Webb&nbsp;&nbsp;</h2>



“Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. Some of the faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



The same cluster was featured as the 33rd anniversary image of the Hubble Space Telescope in April 2023.&nbsp;



According to ESA, Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. 



"Observing with larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects."



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc-1333">Webb’s view of NGC 1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC 1333 cloud. 



“Across the image we see large patches of orange, which represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation."



The disks of gas and dust that surround the <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">stars</a> in this image may eventually produce planetary systems.&nbsp;



<h2 class="wp-block-heading" id="h-formation-of-the-sun">Formation of the Sun</h2>



“Similar to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster, which was perhaps even more massive than NGC 1333,” explained ESA.



Over time, the stars in the Sun's birth cluster would have drifted apart due to gravitational interactions and the dispersion of gas in the region.



Astronomers have been studying certain clues, such as isotopic signatures in meteorites, that hint the Sun may have formed near massive stars. These stars likely produced supernovae, which could have influenced the early <a href="https://www.earth.com/news/mysterious-objects-spotted-in-the-outer-solar-system-beyond-pluto/" target="_blank" rel="noreferrer noopener">solar system</a> by injecting heavy elements like iron-60.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1333">Star formation in NGC 1333</h2>



NGC 1333 is a vibrant example of a stellar nursery, where active <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> is ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



Within NGC 1333, astronomers have observed a high level of turbulence, which makes the region dynamic and complex. 



These disturbances are caused by the outflows of young stars as they eject material into their surroundings, creating shock waves and influencing further star formation.&nbsp;



These outflows are often seen as jets, which are visible in multiple wavelengths of light, especially infrared, as the surrounding dust absorbs visible light.



<h2 class="wp-block-heading" id="h-significance-of-ngc-1333">Significance of NGC 1333</h2>



NGC 1333 is also an area of interest for studying the early stages of star and <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planet formation</a>, as many of the stars within the cluster are in their infancy, still in the process of gathering material and developing protoplanetary disks.&nbsp;



In images, NGC 1333 is marked by bright patches of blue and red, representing reflection <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebulae</a> and the ionized gas created by energetic young stars.&nbsp;



<h2 class="wp-block-heading" id="h-the-perseus-molecular-cloud-nbsp">The Perseus molecular cloud&nbsp;</h2>



The Perseus molecular cloud is a vast region of cold gas and dust located about 600 light-years away from Earth in the constellation <a href="https://www.earth.com/news/1500-billion-orphan-stars-discovered-in-the-perseus-galaxy-cluster/" target="_blank" rel="noreferrer noopener">Perseus</a>.&nbsp;



It is one of the most studied star-forming regions in our galaxy due to its relative proximity and the diversity of its young stellar objects. This cloud spans several hundred light-years and contains dense pockets of gas where new stars are actively forming.&nbsp;



These areas are often enshrouded in thick dust, which obscures them in visible light but allows astronomers to study them using infrared and radio wavelengths.



The Perseus molecular cloud is particularly interesting because of the chemistry taking place within it, including the formation of complex organic molecules that could be precursors to life.&nbsp;



Image Credit: ESA/Webb, NASA &amp; CSA



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Stellar nursery shines in the Perseus cloud

Today's Image of the Day from the European Space Agency...

Today's Image of the Day from NASA Earth Observatory features smoke streaming from Tasmania, where bushfires were ignited by dry lightning strikes earlier this month.&nbsp;



By February 5, more than a dozen fires were burning in the state's remote central and western regions.



<h2 class="wp-block-heading" id="h-bushfires-fueled-by-challenging-conditions">Bushfires fueled by challenging conditions </h2>



Communities such as Zeehan, Corinna, and Pieman Heads have been threatened, leading to evacuations and significant disruptions during the peak tourism season.



“In early February 2025, bushfires ignited in northwestern Tasmania, where they have continued to burn on the island for more than a week amid windy, warm, and dry conditions,” said <a href="https://earthobservatory.nasa.gov/images/153933/smoke-billows-from-bushfires-in-tasmania" target="_blank" rel="noreferrer noopener">NASA</a>.



“Smoke from the fires is visible in this image, acquired at about 4 p.m. local time on February 12, 2025, by the MODIS (Moderate Resolution Imaging Spectroradiometer) instrument on NASA’s Aqua satellite.”



<h2 class="wp-block-heading" id="h-impacts-of-the-tasmania-bushfires">Impacts of the Tasmania bushfires</h2>



The <a href="https://www.earth.com/news/wildfires-threaten-the-recovery-of-the-ozone-layer/" target="_blank" rel="noreferrer noopener">fires</a> have burned over 90,000 hectares, with a combined perimeter exceeding 1,200 kilometers.



The fires are expected to continue burning for several more weeks. Due to the region's remote and challenging terrain, authorities report that significant effort is still needed to gain control over the blazes.



“According to a heatwave warning from Australia’s Bureau of Meteorology (BoM), much of the state’s west coast saw severe heatwave conditions on several days during the week of February 10,” noted NASA.



“The region has also been exceptionally dry. For example, the past 12-month period has been the driest on record (since 1900) along the coastal areas near Sandy Cape.”



<h2 class="wp-block-heading" id="h-cultural-and-heritage-sites">Cultural and heritage sites</h2>



One significant area under threat is the takayna/Tarkine region in northwest Tasmania. This region is home to a grove of ancient Huon pine trees, including one estimated to be between 2,500 and 3,000 years old, making it the oldest known Huon pine.&nbsp;



The Yellowband Plain fire has burned perilously close to this grove, coming within meters of these irreplaceable trees.



Firefighters from Tasmania, interstate, and New Zealand are collaborating to control the blazes and help protect the Huon pine trees, as well as Indigenous heritage sites. 



Efforts to assess and mitigate the damage have been hampered by challenging weather conditions, including low cloud cover that restricts aerial surveys. Strong winds of up to 50 miles per hour have also complicated efforts to contain the bushfires.&nbsp;



<h2 class="wp-block-heading" id="h-climate-change-is-intensifying-bushfires-nbsp">Climate change is intensifying bushfires&nbsp;</h2>



Climate change and bushfires are deeply interconnected, with rising global temperatures intensifying the frequency and severity of wildfires in many regions.&nbsp;



Warmer temperatures lead to drier conditions, reducing moisture in vegetation and making it more susceptible to ignition. Prolonged droughts - which are becoming more common due to climate change - further dry out forests and grasslands, creating an abundance of flammable material.



Extreme heat waves increase the likelihood of fires starting and spreading rapidly. Higher temperatures also contribute to stronger winds, which can fan flames and carry embers over long distances, igniting new fires. 



Additionally, shifting <a href="https://www.earth.com/news/ultrafine-particles-in-wildfire-smoke-change-weather-patterns/" target="_blank" rel="noreferrer noopener">weather patterns</a> are altering fire seasons, making them longer and more unpredictable. Some areas that previously had clear fire seasons are now experiencing fires year-round.



<h2 class="wp-block-heading" id="h-shifting-behavior-of-wildfires-nbsp">Shifting behavior of wildfires&nbsp;</h2>



Climate change is also affecting the way bushfires behave. Many recent wildfires have been more intense, burning hotter and <a href="https://www.earth.com/news/fast-wildfires-are-gaining-even-more-speed/" target="_blank" rel="noreferrer noopener">spreading faster</a> than historical fires. This makes them harder to control and increases their impact on communities, ecosystems, and wildlife. 



The destruction of forests not only contributes to immediate carbon emissions but also reduces the planet’s ability to absorb carbon dioxide, creating a feedback loop that worsens climate change.



<h2 class="wp-block-heading" id="h-consequences-of-increased-fire-activity">Consequences of increased fire activity</h2>



Beyond the direct effects on landscapes and air quality, increased bushfire activity has severe consequences for <a href="https://www.earth.com/news/wildfire-smoke-is-an-underestimated-threat-to-public-health/" target="_blank" rel="noreferrer noopener">human health</a>, economies, and biodiversity. 



Smoke from large wildfires contains fine particles that can cause respiratory problems and other health issues, even for people far from the fire zones.&nbsp;



Wildlife struggles to escape or recover from habitat destruction, sometimes pushing species closer to extinction.



<h2 class="wp-block-heading" id="h-mitigating-the-risks">Mitigating the risks</h2>



Efforts to mitigate these risks include better fire management strategies, improved early <a href="https://www.earth.com/news/bushfires-are-detected-500-times-faster-with-ai-satellites/" target="_blank" rel="noreferrer noopener">warning systems</a>, and sustainable land-use practices. 



However, long-term solutions require addressing the root cause - reducing greenhouse gas emissions to slow down global warming.&nbsp;



Without significant action, climate change will continue to fuel more extreme and destructive bushfires, with devastating consequences for both nature and society.



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Tasmania bushfires: A growing crisis in an era of climate change

Today's Image of the Day from NASA Earth Observatory features an astronaut view of Mount Nemrut, a volcano located in eastern Turkey near Lake Van.



Mount Nemrut is notable for its immense caldera, which was formed through a series of <a href="https://www.earth.com/news/volcanic-eruptions-play-an-overlooked-role-in-earths-climate/" target="_blank" rel="noreferrer noopener">eruptions</a>. The caldera, one of the largest in the world, now contains several lakes such as Lake Nemrut.&nbsp;



"The eastern half of the caldera is partially filled by solidified lava flows from past eruptions. Snow cover present at the time of this photo accentuates pressure ridges that formed as the lava was flowing and cooling," noted <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"These pressure ridges vary in size, thickness, and orientation due to the varying viscosity and flow direction of the lavas during eruptions."



<h2 class="wp-block-heading" id="h-formation-of-lake-nemrut">Formation of Lake Nemrut</h2>



"Lake Nemrut (Nemrut Gölü) occupies the western half of the caldera, creating a rough crescent shape that partially submerges the old lava flows," said NASA.



"This freshwater lake, reaching up to 176 meters deep, is accompanied by a smaller lake at the upper-center of the caldera."



The lake was formed after the collapse of the Nemrut volcano's summit. This collapse created a massive crater, which gradually filled with water over time, forming the <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lake</a>.



<h2 class="wp-block-heading" id="h-unesco-world-heritage-site">UNESCO World Heritage Site </h2>



Mount Nemrut and its surroundings are part of a protected UNESCO World Heritage Site due to their ecological and geological significance.



The site is home to diverse wildlife, including various bird species that use the lake as a stopover during migration. The caldera also contains smaller lakes and wetlands, adding to the area's biodiversity.



Lake Nemrut is a popular destination for tourists, hikers, and nature enthusiasts, offering stunning views of the volcanic landscape.



Despite its popularity, the lake remains relatively remote and unspoiled, contributing to its appeal as a natural wonder.



<h2 class="wp-block-heading" id="h-mount-nemrut-has-shaped-the-landscape">Mount Nemrut has shaped the landscape</h2>



Geologically, Mount Nemrut is interesting because its <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">eruptions</a> have played a key role in shaping the local landscape. 



Its last major eruption occurred around 1441 AD, which indicates that it's not currently active.



The area around Nemrut is known for its geothermal activity, including hot springs and fumaroles, suggesting that there is still significant heat beneath the surface.



<h2 class="wp-block-heading" id="h-tribute-to-a-king">Tribute to a king</h2>



Over thousands of years, various civilizations have inhabited the region around Nemrut, leaving behind a wealth of archaeological sites.



The summit of Mount Nemrut is dominated by a vast funerary mound constructed by King Antiochus I Theos, who ruled the Kingdom of Commagene in the 1st century BCE. 



The site was intended to serve as his tomb sanctuary and a place to commemorate the king's vision of divine kingship and unity between Eastern and Western cultures.



The mound, made of loose crushed stones, measures about 50 meters (164 feet) in height and spans a diameter of 150 meters (492 feet), creating an imposing feature visible from afar.



Surrounding the mound are terraces on the eastern, western, and northern sides, each adorned with colossal statues and reliefs. The statues, ranging in height from 8 to 10 meters (26 to 33 feet), represent various deities, including Zeus, Apollo, Hercules, and the goddess Tyche, alongside King Antiochus himself. 



The heads of the statues, many of which have toppled over due to <a href="https://www.earth.com/news/new-map-shows-75-percent-of-the-u-s-at-risk-of-damaging-earthquakes/" target="_blank" rel="noreferrer noopener">earthquakes</a> and erosion, lie scattered around the site.



<h2 class="wp-block-heading" id="h-spiritual-and-religious-practices">Spiritual and religious practices</h2>



In addition to the statues, inscriptions at Mount Nemrut provide valuable historical information about the kingdom, the king's lineage, and the religious practices of the time.



The site is not only a marvel of ancient engineering but also a spiritual and astronomical center. Scholars believe the terraces were aligned with celestial events, serving as an observatory for solstices and equinoxes.



In addition to its natural and historical significance, the Nemrut volcano has been the subject of scientific study, as researchers aim to understand more about <a href="https://www.earth.com/news/volcanic-eruptions-play-an-overlooked-role-in-earths-climate/" target="_blank" rel="noreferrer noopener">volcanic activity</a> in the region, the history of its eruptions, and the potential risks it may pose in the future.



Image Credit: NASA Earth Observatory



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Mount Nemrut: Ancient mysteries and natural marvels 

Today's Image of the Day from NASA Earth Observatory features La Niña, a global climate event that is expected to be short-lived.



The map represents sea surface height anomalies on January 13, 2025 across the central and eastern Pacific Ocean.&nbsp;



“Shades of blue indicate sea levels that were lower than average, while shades of red indicate areas where the ocean stood higher than normal. Normal sea level conditions appear in white,” noted <a href="https://earthobservatory.nasa.gov/images/153917/la-nina-is-here" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-the-onset-of-la-nina-nbsp">The onset of La Niña&nbsp;</h2>



According to the National Oceanic and Atmospheric Administration (NOAA), sea surface temperatures in the east-central equatorial Pacific dropped below average in December 2024, marking the onset of La Niña. This cooling pattern has persisted into early 2025.



NOAA's Climate Prediction Center indicates a 59% chance that La Niña conditions will continue through February-April 2025, with a likely transition to ENSO-neutral conditions during March-May 2025.



“After seven months of waiting, La Niña - the cooler sister of El Niño - finally showed up in the eastern Pacific Ocean in early December 2024. La Niña may not stick around long, though,” said NASA.



<h2 class="wp-block-heading" id="h-what-is-la-nina">What is La Niña?</h2>



La Niña is a phase of the El Niño-Southern Oscillation (ENSO) cycle that occurs when strengthened easterly trade winds enhance the upwelling of cooler water from the depths of the eastern tropical Pacific.&nbsp;



This process leads to a significant cooling of surface waters in the central and eastern Pacific near the equator. The intensified trade winds also drive warm equatorial waters westward toward Asia and Australia.&nbsp;



“This dramatic cooling of the ocean’s surface layers affects the atmosphere by modifying the moisture content across the Pacific,” explained NASA.



“In a report published on January 9, 2025, the NOAA Climate Prediction Center confirmed that La Niña conditions were present. They measured sea surface temperatures 0.7 degrees Celsius (1.3 degrees Fahrenheit) below average in an area of the tropical Pacific, from 170° to 120° West longitude, known as the Niño 3.4 region.”



“The signature of La Niña is also visible in the central and eastern Pacific Ocean as areas of lower-than-average water levels. That’s because cooler water contracts, lowering sea levels. (Conversely, warmer water expands, raising them).”&nbsp;



<h2 class="wp-block-heading" id="h-la-nina-forecast-nbsp">La Niña forecast&nbsp;</h2>



Josh Willis, an oceanographer and Sentinel-6 Michael Freilich project scientist at JPL, pointed out that although La Niña is here, it’s not a particularly strong one.



Willis noted that during an especially strong La Niña in 2010-2011, temperatures in the tropical Pacific were about 1.6°C (2.9°F) below average in January 2011, compared to just 0.7°C (1.3°F) below average in January 2025.&nbsp;



NOAA predicts that this La Niña will remain weak and is unlikely to drop below -1°C from the average - the threshold for a moderate-strength event. Neutral conditions are expected to return during the meteorological spring.



La Niña’s interaction between the ocean and atmosphere alters global atmospheric circulation, shifting mid-latitude jet streams in ways that can intensify rainfall in some regions and cause drought in others.&nbsp;



In the western Pacific, Indonesia and Australia may experience increased rainfall. The central and eastern Pacific is expected to experience reduced cloud cover and precipitation, leading to drier conditions in Brazil, Argentina, and other parts of South America. Meanwhile, Central America may see wetter conditions.&nbsp;



<h2 class="wp-block-heading" id="h-"></h2>



In North America, La Niña typically brings cooler, stormier weather to the Pacific Northwest, while the southern United States and northern Mexico tend to experience warmer, drier conditions.



<h2 class="wp-block-heading" id="h-natural-source-of-variability">Natural source of variability</h2>



“ENSO adds a natural source of year-to-year variability in global temperatures. Because such a wide swath of the Pacific is cold, La Niña tends to keep a lid on the average global surface temperature,” explained NASA.



“But even the cool water in the Pacific does not completely offset long-term warming trends; some of the hottest years on record have coincided with La Niña, such as in 2010 and 2020.”



The map is based on data that was acquired by the Sentinel-6 Michael Freilich satellite and processed by scientists at NASA’s Jet Propulsion Laboratory (JPL).&nbsp;



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La Niña has arrived - but it may not stay for long

Scientists have developed an AI-powered modeling method that mimics how birds produce songs, similar to how large language models like ChatGPT generate human sentences.&nbsp;



By training on birdsong recordings, the model successfully recreates sequences of Bengalese <a href="https://www.earth.com/news/finch-beaks-and-bird-songs-a-new-story-of-evolution/" target="_blank" rel="noreferrer noopener">finch</a> songs, revealing important insights into how birds structure their vocalizations.&nbsp;



The research, published in <a href="http://dx.doi.org/10.1523/JNEUROSCI.0522-24.2024" target="_blank" rel="noreferrer noopener">The Journal of Neuroscience</a>, could enhance understanding of the neurobiology behind language processing and how humans and animals form complex vocal patterns.



<h2 class="wp-block-heading" id="h-birdsongs-and-human-language">Birdsongs and human language</h2>



Both birds and humans arrange their vocal expressions in structured ways. In human speech, words follow specific grammatical rules, while birds sing in organized syllabic patterns.



“Although much simpler, the sequences of a bird’s song syllables are organized in a similar way to human language, so birds provide a good model to explore the neurobiology of language,” said Dezhe Jin, an associate professor of physics at <a href="https://www.psu.edu/" target="_blank" rel="noreferrer noopener">Penn State</a>’s Eberly College of Science and lead author of the study.



One key aspect of both birdsong and <a href="https://www.earth.com/news/bird-songs-human-speech-common-vocal-genetic-origin-syrinx/" target="_blank" rel="noreferrer noopener">human language</a> is context dependence - where previous sounds influence what comes next. In English, for example, the phrase “flies like” can have different meanings depending on what follows.&nbsp;



For instance, while “time flies like an arrow” is a statement about time, “fruit flies like bananas” is one about insects and food. If we mix these up - “time flies like bananas” - the meaning becomes nonsensical.&nbsp;



The same principle applies to birds: the order of their syllables is not random but follows specific patterns that make their songs recognizable.



“We know from our previous work that the songs of Bengalese finches also have context dependence,” Jin said. “In this study, we developed a new statistical method to better quantify context dependence in individual birds and start to understand how it is wired in the brain.”



<h2 class="wp-block-heading" id="h-training-a-generative-birdsong-model">Training a generative birdsong model</h2>



The research team analyzed previously recorded songs from six Bengalese finches, each of which sings 7 to 15 syllables per sequence. Their <a href="https://www.earth.com/news/ai-can-monitor-biodiversity-through-animal-sounds/" target="_blank" rel="noreferrer noopener">AI</a> model, similar to large language models, learns the probability of different syllables appearing in sequences - akin to how ChatGPT predicts words based on past text.



The model is built using Markov models, a method that maps sequences of events by tracking what comes next based on past occurrences. Imagine a flowchart where each syllable leads to a range of possible next syllables, with probabilities assigned to each transition.



“Basic Markov models are quite simple, but they tend to overgeneralize, meaning they might result in sequences that don’t actually exist,” Jin explained.&nbsp;



“Here, we used a specific type of model called a Partially Observable Markov Model that allowed us to incorporate context dependence, adding more connections to what syllables typically go together. The added complexity allows for more accurate models.”



Using their approach, the team generated a range of possible models for each bird’s song, gradually refining them to ensure they only produced sequences that actually exist in the bird’s natural repertoire.&nbsp;



The final models accurately reflected each bird’s real singing patterns while identifying which syllables were context-dependent.



<h2 class="wp-block-heading" id="h-what-the-birdsong-model-revealed">What the birdsong model revealed</h2>



The results showed that all six birds displayed context dependence in their songs, meaning they carefully structured their syllable sequences rather than singing randomly. However, the degree of context dependence varied between individuals.



“This could be due to several factors, including aspects of the birds’ brains,” Jin explained. “Or, because these songs are learned, this could be related to the amount of context dependence in their tutor’s songs.”



To explore this further, the researchers studied birds that could not hear their own songs. The results were striking. These birds showed a dramatic reduction in context-dependent syllables, suggesting that auditory feedback is crucial in shaping how birds refine their songs.



This finding supports the idea that birds listen to themselves and adjust their vocal patterns based on what they hear, much like how humans refine speech and grammar while learning a language.



“The birds are listening to themselves and adjusting their song based on what they hear, and the related machinery in the brain likely plays a role in context dependence,” Jin said.&nbsp;



“In the future, we would also like to map neuron states to specific syllables. Our study suggests that, even when a bird is singing the same syllable, different sets of neurons might be active.”



<h2 class="wp-block-heading" id="h-broader-applications-of-the-research">Broader applications of the research </h2>



The researchers emphasize that this new AI-based modeling technique could be applied not just to birdsong, but to other animal vocalizations and behavioral patterns.



“We actually used this method with the English language and were able to generate text that is mostly grammatical,” Jin said. “Of course, we’re not trying to create a new generative language model, but it is interesting that the same kind of model can handle both birdsong and <a href="https://www.earth.com/news/whale-songs-share-very-similar-patterns-with-human-language/" target="_blank" rel="noreferrer noopener">human language</a>.”



This suggests that the neural mechanisms behind birdsong and human language may share deeper similarities than previously thought.&nbsp;



Some philosophers argue that human grammar is a uniquely complex feature of cognition, but this study raises questions about how truly unique human language is if birds follow similar rules.



<h2 class="wp-block-heading" id="h-understanding-human-language-and-communication">Understanding human language and communication </h2>



This research opens up new possibilities for understanding how brains - both bird and human - encode language and communication. In the future, scientists hope to map neuronal activity during song production to see which brain circuits control context dependence.



The experts would also like to apply AI models to other vocal species - such as whales, dolphins, and primates - to identify common patterns in communication.



Furthermore, the goal is to develop better speech-related AI systems based on how real biological brains organize vocalization sequences.



Ultimately, this work bridges the gap between neuroscience, AI, and linguistics, offering new clues about how brains generate structured communication across species.&nbsp;



As AI technology continues to evolve, models trained on birdsongs could help us better understand how our own brains process language and adapt speech over time.



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AI-generated birdsongs may shed new light on human language

Scientists have developed an AI-powered modeling method that mimics how...

A recent study has unveiled how chemical elements and powerful winds shape the atmosphere of a planet far beyond our solar system.&nbsp;



By examining separate layers of the planet’s atmosphere in 3D, the researchers have revealed an intricate system of jet streams and temperature contrasts.



The discovery was made by astronomers at the <a href="https://www.eso.org/public/" target="_blank" rel="noreferrer noopener">European Southern Observatory</a> (ESO) in Chile and other institutions, who combined multiple telescope units to obtain a detailed view.&nbsp;



<h2 class="wp-block-heading" id="h-weather-conditions-on-a-distant-world">Weather conditions on a distant world</h2>



The research focused on WASP-121b (also called Tylos), a so-called “ultra-hot Jupiter” about 900 light-years away in the constellation Puppis. The results offer an unprecedented glimpse into the weather conditions of a distant world.&nbsp;



“This planet’s atmosphere behaves in ways that challenge our understanding of how <a href="http://dx.doi.org/10.1038/s41586-025-08664-1" target="_blank" rel="noreferrer noopener">weather</a> works - not just on Earth, but on all planets. It feels like something out of science fiction,” said Julia Victoria Seidel, a researcher at the European Southern Observatory (<a href="https://www.eso.org" target="_blank" rel="noreferrer noopener">ESO</a>) in Chile and lead author of the study.



WASP-121b completes an orbit around its host star in roughly 30 hours, hugging it so closely that one side is perpetually scorched while the opposite side remains significantly cooler. 



This extreme temperature difference results in what scientists describe as a violent and highly unusual climate. 



<h2 class="wp-block-heading" id="h-distinct-layers-of-the-exoplanet-s-atmosphere-nbsp">Distinct layers of the exoplanet’s atmosphere&nbsp;</h2>



The research team used high-resolution observations of starlight passing through the exoplanet’s atmosphere to deduce how distinct layers move and mix.



“What we found was surprising: a <a href="https://www.earth.com/news/jupiters-turbulent-atmosphere-includes-a-high-speed-jet-stream/" target="_blank" rel="noreferrer noopener">jet stream</a> rotates material around the planet’s equator, while a separate flow at lower levels of the atmosphere moves gas from the hot side to the cooler side. This kind of climate has never been seen before on any planet,” Seidel explained.&nbsp;



By tracing iron and other gases at different heights, the scientists identified powerful winds racing across Tylos’s skies. “Even the strongest hurricanes in the Solar System seem calm in comparison,” she added.



<h2 class="wp-block-heading" id="h-viewing-the-planet-in-3d">Viewing the planet in 3D</h2>



To map out these winds and their distribution of elements, the astronomers made use of the Very Large Telescope (VLT), merging the light from four of its units into a single signal via a specialized instrument.&nbsp;



The goal was to capture enough detail to distinguish chemical signatures at various altitudes - all within a single transit of WASP-121b in front of its host star.



“The VLT enabled us to probe three different layers of the exoplanet’s atmosphere in one fell swoop,” said study co-author Leonardo A. dos Santos, an assistant astronomer at the <a href="https://www.stsci.edu/home" target="_blank" rel="noreferrer noopener">Space Telescope Science Institute</a> in Baltimore, United States.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/exoplanet-Tylos_atmospheric-structure_3d-view_illustration_ESO_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/exoplanet-Tylos_atmospheric-structure_3d-view_illustration_ESO_1s.webp" alt="This diagram shows the structure and motion of the atmosphere of the exoplanet Tylos (WASP-121b). The exoplanet is shown from above in this figure, looking at one of its poles. The planet rotates counter-clockwise, in such a way that it always shows the same side to its parent star, so it's always day on one half of the planet and night on the other. The transition between night and day is the &quot;morning side&quot; while the &quot;evening side&quot; represents the transition between day and night; its morning side is to the right and its evening side to the left. Credit: ESO" class="wp-image-1960368"/></a><figcaption class="wp-element-caption">This diagram shows the structure and motion of the atmosphere of the exoplanet Tylos (WASP-121b). The exoplanet is shown from above in this figure, looking at one of its poles. The planet rotates counter-clockwise, in such a way that it always shows the same side to its parent star, so it's always day on one half of the planet and night on the other. The transition between night and day is the "morning side" while the "evening side" represents the transition between day and night; its morning side is to the right and its evening side to the left. Credit: ESO</figcaption></figure>



By monitoring how iron, sodium, and hydrogen moved within these layers, the team reconstructed the flow of material from the planet’s deep interior to its outermost atmospheric regions.&nbsp;



“It’s the kind of observation that is very challenging to do with space telescopes, highlighting the importance of ground-based observations of <a href="https://www.earth.com/news/exoplanet-discovery-nasa-identifies-over-5500-distant-worlds/" target="_blank" rel="noreferrer noopener">exoplanets</a>,” noted dos Santos.



<h2 class="wp-block-heading" id="h-metals-and-other-compounds">Metals and other compounds</h2>



The deeper parts of WASP-121b’s atmosphere feature intense heat, while the upper layers experience a dynamic interplay between cooler regions and strong winds.&nbsp;



The combined data indicate that metals and other compounds are shuttled around by swift jets, leading to the unfamiliar climate patterns seen on Tylos.



Alongside iron, sodium, and hydrogen, the researchers uncovered titanium in levels just beneath the high-altitude jet stream - an unexpected finding, given that previous attempts to locate titanium in WASP-121b’s atmosphere had come up short.&nbsp;



“It’s truly mind-blowing that we’re able to study details like the chemical makeup and weather patterns of a planet at such a vast distance,” said Bibiana Prinoth, a PhD student at Lund University, Sweden, and ESO.



Prinoth led a companion study published in the journal <a href="http://aanda.org/10.1051/0004-6361/202452405" target="_blank" rel="noreferrer noopener">Astronomy &amp; Astrophysics</a> and co-authored the Nature paper.



The newly detected titanium, hidden at lower altitudes, indicates the planet’s <a href="https://www.earth.com/news/hubble-finds-a-water-rich-planet-with-a-steamy-atmosphere-named-gj-9827d/" target="_blank" rel="noreferrer noopener">atmosphere</a> is even more complex than once thought.&nbsp;



While it remains unclear exactly how these metals form and move around Tylos, one possibility is that temperature gradients and the planet’s day-night contrast help determine where certain elements accumulate.



<h2 class="wp-block-heading" id="h-future-insights-on-alien-climates">Future insights on alien climates</h2>



The fact that WASP-121b’s jets and temperature distributions can be traced in such detail from light-years away marks a significant leap in exoplanet science.&nbsp;



Yet, as astronomers look to study smaller, rockier planets with potentially milder climates, even more powerful instruments will be required.&nbsp;



“The ELT will be a game-changer for studying exoplanet atmospheres,” Prinoth said, referring to the <a href="https://elt.eso.org/" target="_blank" rel="noreferrer noopener">Extremely Large Telescope</a> currently under construction in Chile’s Atacama Desert.&nbsp;



“This experience makes me feel like we’re on the verge of uncovering incredible things we can only dream about now.”



<h2 class="wp-block-heading" id="h-probing-the-atmospheres-of-exoplanets">Probing the atmospheres of exoplanets</h2>



Using next-generation telescopes such as the ELT, researchers hope to probe the atmospheres of Earth-like planets and see if they harbor any hints of habitability.&nbsp;



By refining techniques already showcased in this study, astronomers aim to decode the layers, winds, and potentially life-supporting chemistry of still more distant worlds.&nbsp;



The success of this recent work on WASP-121b foreshadows a new era in which entire atmospheric systems - weather, chemical cycles, and beyond - can be revealed in detail, unveiling the dynamic nature of far-off environments that were once the stuff of pure speculation.



The study is published in the journal <a href="http://dx.doi.org/10.1038/s41586-025-08664-1" target="_blank" rel="noreferrer noopener">Nature</a>.



Image Credit: ESO/M. Kornmesser



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First 3D view of an exoplanet's atmosphere reveals alien weather that's "Out of science fiction"

A recent study has unveiled how chemical elements and powerful...

Black holes are among the most mysterious objects in the universe. Their immense gravitational pull can warp space and time, yet they remain invisible unless they interact with their surroundings. 



Understanding black holes is crucial to deciphering the history of the cosmos. Scientists know that supermassive black holes sit at the centers of large galaxies, including the Milky Way. 



However, much remains unknown about <a href="https://www.earth.com/news/evidence-of-massive-early-universe-black-hole-stuns-astronomers/" target="_blank" rel="noreferrer noopener">black holes</a> in smaller galaxies.



Using early data from the Dark Energy Spectroscopic Instrument (<a href="https://www.desi.lbl.gov" target="_blank" rel="noreferrer noopener">DESI</a>), researchers have uncovered an extraordinary population of black holes hiding in dwarf galaxies. 



This discovery includes the largest-ever sample of dwarf galaxies with actively feeding black holes.



The study also presents the most extensive collection of intermediate-mass black hole candidates. These findings push the boundaries of astrophysics and open new avenues for exploring galaxy formation and evolution.



<h2 class="wp-block-heading" id="h-mapping-the-universe">Mapping the Universe</h2>



DESI is one of the most advanced instruments in modern astronomy. It can capture light from 5,000 galaxies at once, allowing scientists to collect vast amounts of data efficiently. 



The instrument operates on the Nicholas U. Mayall 4-meter Telescope at <a href="https://noirlab.edu/public/programs/kitt-peak-national-observatory/" target="_blank" rel="noreferrer noopener">Kitt Peak National Observatory</a> in Arizona. 



The project is funded by the Department of Energy (<a href="https://www.energy.gov" target="_blank" rel="noreferrer noopener">DOE</a>) and the National Science Foundation (<a href="https://www.nsf.gov" target="_blank" rel="noreferrer noopener">NSF</a>), with contributions from international partners.



The DESI survey is in its fourth year and aims to observe 40 million galaxies and quasars. This ambitious project involves over 900 scientists from 70 institutions worldwide. 



DESI’s precision and large-scale capabilities make it a crucial tool in identifying <a href="https://www.earth.com/news/black-hole-draco-1es-1927-654-just-awoke-is-spewing-material-at-incredible-speeds/" target="_blank" rel="noreferrer noopener">hidden black holes</a> across the universe.



<h2 class="wp-block-heading" id="h-hunting-for-black-holes-in-dwarf-galaxies">Hunting for black holes in dwarf galaxies</h2>



Dwarf galaxies are small, faint, and contain fewer stars than massive galaxies. They are difficult to study because their black holes are not as prominent. 



In large galaxies, astronomers can detect black holes by observing the movement of stars and gas around them. However, dwarf galaxies require a different approach.



One way to find <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/" target="_blank" rel="noreferrer noopener">black holes</a> in these galaxies is by identifying active galactic nuclei (AGN). When a black hole consumes surrounding material, it releases a massive amount of energy, making it easier to detect. 



This energy illuminates the surrounding region, acting as a signal for scientists.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/black-holes_dwarf-galaxies_NoirLabs_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/black-holes_dwarf-galaxies_NoirLabs_1s.webp" alt="This mosaic shows a series of images featuring candidate dwarf galaxies hosting an active galactic nucleus, captured with the Subaru Telescope’s Hyper Suprime-Cam. Credit: Legacy Surveys/D. Lang (Perimeter Institute)/NAOJ/HSC Collaboration/D. de Martin (NSF NOIRLab) &amp; M. Zamani (NSF NOIRLab)" class="wp-image-1960353"/></a><figcaption class="wp-element-caption">This mosaic shows a series of images featuring candidate dwarf galaxies hosting an active galactic nucleus, captured with the Subaru Telescope’s Hyper Suprime-Cam. Credit: Legacy Surveys/D. Lang (Perimeter Institute)/NAOJ/HSC Collaboration/D. de Martin (NSF NOIRLab) &amp; M. Zamani (NSF NOIRLab)</figcaption></figure>



“When a black hole at the center of a galaxy starts feeding, it unleashes a tremendous amount of energy into its surroundings, transforming into what we call an active galactic nucleus,” says Ragadeepika Pucha, a postdoctoral researcher at the <a href="https://www.utah.edu" target="_blank" rel="noreferrer noopener">University of Utah</a>.



The team identified 2,500 dwarf galaxies hosting AGN - the largest sample ever discovered. Previous studies estimated that only 0.5% of dwarf galaxies contained an AGN, but this new research suggests a much higher percentage.



These results indicate that many low-mass black holes have remained undetected until now.



<h2 class="wp-block-heading" id="h-mystery-of-intermediate-mass-black-holes">Mystery of intermediate-mass black holes</h2>



Most known black holes are either stellar-mass or supermassive. Stellar-mass black holes form when massive stars collapse. 



Supermassive black holes exist at the centers of large galaxies, weighing millions to billions of times the mass of the Sun. However, intermediate-mass black holes remain elusive.



Scientists believe these mid-sized black holes could be the remnants of the first black holes formed in the early universe. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/black-holes_intermediate-mass_mosaic_NoirLabs_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/black-holes_intermediate-mass_mosaic_NoirLabs_1s.webp" alt="This mosaic shows a series of images featuring intermediate-mass black hole candidates, arranged in increasing order of stellar mass, captured with the Subaru Telescope’s Hyper Suprime-Cam. Credit: Legacy Surveys/D. Lang (Perimeter Institute)/NAOJ/HSC Collaboration/D. de Martin (NSF NOIRLab) &amp; M. Zamani (NSF NOIRLab)" class="wp-image-1960355"/></a><figcaption class="wp-element-caption">This mosaic shows a series of images featuring intermediate-mass black hole candidates, arranged in increasing order of stellar mass, captured with the Subaru Telescope’s Hyper Suprime-Cam. Credit: Legacy Surveys/D. Lang (Perimeter Institute)/NAOJ/HSC Collaboration/D. de Martin (NSF NOIRLab) &amp; M. Zamani (NSF NOIRLab)</figcaption></figure>



They may also be the seeds that eventually grew into supermassive black holes. Despite their importance, only about 100-150 intermediate-mass black hole candidates had been identified before DESI’s survey.



In their search, researchers found 300 new intermediate-mass black hole candidates, the most extensive collection to date. This dataset provides a powerful tool for studying how these black holes form and evolve.



<h2 class="wp-block-heading" id="h-advancements-in-black-hole-detection">Advancements in black hole detection</h2>



Detecting black holes in dwarf galaxies requires high-precision instruments. DESI’s advanced design played a key role in this discovery. 



The instrument uses small optical fibers to capture light from distant galaxies. This allows researchers to focus on the central regions of <a href="https://www.earth.com/news/many-supermassive-black-holes-are-hidden-by-gas-and-dust/" target="_blank" rel="noreferrer noopener">galaxies</a> without interference from surrounding starlight.



“The technological design of DESI was important for this project, particularly its small fiber size, which allowed us to better zoom in on the center of galaxies and identify the subtle signatures of active black holes,” said Stephanie Juneau, associate astronomer at NSF <a href="https://noirlab.edu/public/" target="_blank" rel="noreferrer noopener">NOIRLab</a>.



Previous instruments had larger optical fibers that collected too much light from the outskirts of galaxies. This extra light diluted the signals scientists were searching for. 



DESI’s small fibers provided a clearer view of black hole activity in dwarf galaxies, leading to a higher detection rate than previous surveys.



<h2 class="wp-block-heading" id="h-unexpected-findings-and-new-questions">Unexpected findings and new questions</h2>



Scientists expected most black holes in dwarf galaxies to be intermediate-mass. However, the study revealed an unexpected result. 



Of the 2,500 dwarf AGN candidates, only 70 overlapped with the 300 intermediate-mass black hole candidates.



This suggests that many of the detected black holes in dwarf galaxies may be more massive than previously thought.



The findings raise new questions about how black holes form and evolve in different types of galaxies. Do different black hole formation processes occur in dwarf and large galaxies? Are some intermediate-mass black holes growing more rapidly than expected?



“For example, is there any relationship between the mechanisms of black hole formation and the types of galaxies they inhabit?” Pucha said. 



“Our wealth of new candidates will help us delve deeper into these mysteries, enriching our understanding of black holes and their pivotal role in galaxy evolution.”



<h2 class="wp-block-heading" id="h-future-of-black-hole-research">Future of black hole research</h2>



DESI’s discoveries mark a turning point in the study of black holes. The new dataset will help scientists explore the early stages of black hole growth and their impact on galaxy evolution. As the DESI survey continues, researchers expect to uncover even more hidden black holes.



By studying these newly identified black holes, scientists hope to answer fundamental questions about the structure and <a href="https://www.earth.com/news/black-holes-seen-creating-their-own-food-gases-x-rays-fascinating-discovery/" target="_blank" rel="noreferrer noopener">history of the universe</a>. 



Future research will focus on confirming the nature of these candidates and examining how they interact with their host galaxies.



Black holes remain one of the greatest mysteries of astrophysics. Thanks to DESI, scientists now have a powerful tool to uncover their secrets, bringing us closer to understanding the forces that shape the cosmos.



The study is published in The Astrophysical Journal and <a href="https://arxiv.org/abs/2411.00091" target="_blank" rel="noreferrer noopener">arXiv</a>.



Image Credit: NOIRLab/NSF/AURA/J. da Silva/M. Zamani



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Thousands of active black holes discovered where it was believed they couldn't exist

Black holes are among the most mysterious objects in the...

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Today&#8217;s Video of the Day from the <a href="http://Nsf.gov">National Science Foundation</a> describes ongoing research which aims to improve the design of prosthetic limbs. 
A team at Stanford University has developed a new tool that makes it possible to try out many different designs without actually having to construct the hardware.
The researchers are experimenting with robotic prosthetic devices that can sense an individual&#8217;s movement and help to correct it based on the surrounding environment.
&#8212;
By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer
Video Credit: Stanford University
&nbsp;

New tool for designing prosthetic limbs

News coming your way