While Shepard and Mitchell were bouncing over the lunar surface during their two moonwalks, Roosa had stayed behind on board the command module. He wasn’t sitting idly, though: he had his own job to do. He took lots of high-quality photos of the Moon, which ultimately went on to help with future missions. Photo Credit: NASA

Today's Image of the Day from NASA Earth Observatory features Ksudach, a remarkable volcanic complex located on Russia's Kamchatka Peninsula.



“The peninsula is one of the world’s most active volcanic arcs due to tectonic plate movement, with the Pacific Plate subducting under the Eurasian Plate,” noted <a href="https://earthobservatory.nasa.gov/images/153779/ksudachs-nested-calderas-and-craters" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-explosive-eruptions-of-ksudach">Explosive eruptions of Ksudach</h2>



Ksudach is classified as a shield <a href="https://www.earth.com/news/new-camera-helps-scientists-forecast-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">volcano</a> due to the gentle slopes formed by its extensive lava flows. The combination of its shield-like structure and the prominent caldera system makes Ksudach a unique volcanic feature on the Kamchatka Peninsula.



“Several overlapping calderas and craters comprise the volcano. Calderas are large, bowl-shaped depressions created by the collapse of overlying material into an emptied subsurface magma chamber,” explained NASA.



“Craters are circular depressions created by volcanic activity, surface impacts, or explosions.”



This volcanic system has a fascinating geological history shaped by multiple explosive eruptions.&nbsp;



The most significant of these occurred around 240 AD, leaving behind a prominent caldera that now hosts scenic crater lakes, such as Lake Ksudach. 



“Lakes within the volcanic region are primarily recharged by rain and snowmelt from the winter season. This photo shows the water’s contrasting blue hues surrounded by green vegetation,” noted NASA.



“Traces of snow fill valleys within and outside the volcano’s caldera complex. These snow-covered areas highlight the drainage patterns from higher to lower elevations. Water that flows through these erosional pathways and into the caldera supports its vegetation and lakes.”



<h2 class="wp-block-heading" id="h-unique-landscape-of-ksudach-nbsp">Unique landscape of Ksudach&nbsp;</h2>



Ksudach's landscape also features pyroclastic deposits, lava flows, and hydrothermal features like fumaroles.&nbsp;



The surrounding environment - which is part of the UNESCO-listed Kamchatka Volcanoes - supports a diverse ecosystem with unique wildlife. 



Despite its remote location, Ksudach has drawn the attention of geologists, offering insights into <a href="https://www.earth.com/news/underwater-volcanic-eruptions-are-more-harmful-than-previously-believed/" target="_blank" rel="noreferrer noopener">volcanic processes</a> and the dynamics of caldera formation.



<h2 class="wp-block-heading" id="h-dynamic-nature-of-earth-s-geology-nbsp">Dynamic nature of Earth's geology&nbsp;</h2>



The most well-documented eruption of Ksudach occurred in March 1907. This eruption ranks as one of the largest in Kamchatka in the 20th century, with a Volcanic Explosivity Index (VEI) of 5.



The eruption produced a colossal ash column that soared into the stratosphere, dispersing fine particles over vast distances and contributing to global atmospheric changes.&nbsp;



The sheer force of the <a href="https://www.earth.com/news/icelands-volcanic-eruptions-may-continue-for-decades/" target="_blank" rel="noreferrer noopener">eruption</a> unleashed pyroclastic flows - fast-moving avalanches of hot gas, ash, and volcanic debris - that raced down the volcano's slopes, obliterating everything in their path.&nbsp;



These flows, capable of reaching temperatures over 1,000°C, decimated vegetation and altered the topography of the surrounding region.&nbsp;



Simultaneously, tephra deposits blanketed the landscape in layers of thick volcanic material, smothering ecosystems and creating a barren wasteland.&nbsp;



Today, Ksudach is considered an active <a href="https://www.earth.com/news/axial-seamount-large-underwater-volcano-off-us-coast-will-likely-erupt-in-2025/" target="_blank" rel="noreferrer noopener">volcano</a> but remains dormant. The region is closely monitored due to its potential for renewed <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">activity</a>.



<h2 class="wp-block-heading" id="h-pacific-ring-of-fire-nbsp">Pacific Ring of Fire&nbsp;</h2>



The Kamchatka Peninsula lies along the Pacific Ring of Fire, a horseshoe-shaped zone encircling the Pacific Ocean where tectonic activity is highly concentrated.&nbsp;



This geologically dynamic area features numerous volcanoes, hot springs, geysers, and frequent seismic activity - making it a hotspot for both natural beauty and scientific study. 



Kamchatka is home to over 160 volcanoes, with about 30 considered active, including Klyuchevskaya Sopka, the highest and one of the most active in the region.



<h3 class="wp-block-heading" id="h-volcanic-activity-nbsp">Volcanic activity&nbsp;</h3>



As the Pacific Plate dives into the Earth's mantle, it melts and generates magma that feeds Kamchatka’s volcanic systems.&nbsp;



This ongoing tectonic interaction also contributes to the broader activity of the Pacific Ring of Fire, which accounts for approximately 75% of the world's active and dormant <a href="https://www.earth.com/news/supervolcano-italy-solfatara-crater-phlegraean-fields-shows-signs-of-waking-up/" target="_blank" rel="noreferrer noopener">volcanoes</a> and about 90% of its earthquakes.



<h3 class="wp-block-heading" id="h-broader-significance-nbsp">Broader significance&nbsp;</h3>



Beyond its geological significance, the Kamchatka Peninsula boasts a diverse ecosystem that is home to animals such as snow sheep, brown bears, red foxes, and unique plants that are adapted to its harsh environment. 



The coastal waters surrounding the peninsula support various fish species, including abundant salmon, as well as sea lions and killer whales.



The interplay of volcanic landscapes and pristine wilderness makes it a natural laboratory for understanding Earth's dynamic processes.



The image was captured by an astronaut aboard the International Space Station.



Image Credit: NASA Earth Observatory&nbsp;



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Ksudach: A volcano shaped by explosive forces

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

Today's Image of the Day from NASA Earth Observatory features a blanket of dust over the Tarim Basin - a vast, arid region in northwestern China. 



Mountain peaks are visible through a break in the dust. These peaks are part of Tekilik Shan, a subrange of the Kunlun Mountains.



Though not as widely known as some other mountain ranges in the area, Tekilik Shan plays a significant role in shaping local <a href="https://www.earth.com/news/extreme-weather-is-pushing-nature-toward-a-breaking-point/" target="_blank" rel="noreferrer noopener">weather</a> patterns and geography.



Its snow-covered peaks can rise above 13,000 feet, contributing to the dramatic elevation differences that define the basin’s borders.



<h2 class="wp-block-heading" id="h-dust-storms-in-the-tarim-basin-nbsp">Dust storms in the Tarim Basin&nbsp;</h2>



Spring marks the height of <a href="https://www.earth.com/news/sahara-desert-dust-storms-carry-harmful-bacteria-and-fungi-around-the-globe/" target="_blank" rel="noreferrer noopener">dust storm</a> activity in the Tarim Basin, particularly in its southern region.&nbsp;



“It’s a time of year when regional wind patterns shift in ways that cause winds and storm systems to sweep in from the northwest,” noted <a href="https://earthobservatory.nasa.gov/images/154126/a-curtain-of-dust-over-the-tarim-basin" target="_blank" rel="noreferrer noopener">NASA</a>.



“In early spring, when landscapes in this region are especially dry and have minimal vegetation, land surfaces warm rapidly under the Sun’s heat every morning, fueling convection that can help loft dust upward by the afternoon.”



<h2 class="wp-block-heading" id="h-fingerlike-dust-formations-nbsp">Fingerlike dust formations&nbsp;</h2>



Satellite images revealed dust formations with fingerlike shapes that mirrored the landscape below. These projections aligned with valleys, which channeled and directed the airborne dust.&nbsp;



Ralph Kahn is an atmospheric scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder and scientist emeritus at NASA’s Goddard Space Flight Center.



According to Kahn, the dust may have been “self-lofting.” In this process, sunlight heats recently stirred-up surface dust, creating pockets of convection that lift it even higher into the air.



This interpretation is supported by hourly observations from Japan’s Himawari-9 geostationary satellite, which showed dust gradually rising into the Tekilik Shan throughout the day. By late afternoon, the storm had grown dense enough to obscure the mountains.&nbsp;



<h2 class="wp-block-heading" id="h-decline-in-atmospheric-dust">Decline in atmospheric dust</h2>



Long-term satellite data from MODIS suggest that <a href="https://www.earth.com/news/dust-storms-in-the-gulf-of-alaska-help-shape-the-global-climate/" target="_blank" rel="noreferrer noopener">atmospheric dust</a> levels in this region have declined by about 1.5 percent each year since the early 2000s.&nbsp;



NASA researcher Hongbin Yu attributes this trend mainly to springtime changes - such as altered wind speeds, <a href="https://www.earth.com/news/how-soil-moisture-can-predict-severe-storms/" target="_blank" rel="noreferrer noopener">soil moisture</a>, or vegetation cover - rather than shifts in other seasons.



<h2 class="wp-block-heading" id="h-rainfall-in-the-tarim-basin-nbsp">Rainfall in the Tarim Basin&nbsp;</h2>



“The <a href="https://www.britannica.com/place/Takla-Makan-Desert" target="_blank" rel="noreferrer noopener">Takla Makan Desert</a> is one of the driest, most barren expanses on Earth. Flanked by mountain ranges on three sides and parched by the resulting <a href="https://glossary.ametsoc.org/wiki/Rain_shadow" target="_blank" rel="noreferrer noopener">rain shadow</a>, parts of the Tarim Basin receive no more than 10 millimeters (0.4 inches) of rain per year,” noted NASA.



“Dust storms can lead to public health problems in populated areas downwind by transporting small particles, bacteria, and viruses that infiltrate human respiratory systems.”&nbsp;



NASA added that dust storms can also affect Earth’s climate by scattering and absorbing incoming solar radiation and changing the properties of clouds.



<h2 class="wp-block-heading" id="h-landscape-of-the-tarim-basin-nbsp">Landscape of the Tarim Basin&nbsp;</h2>



The Tarim Basin is one of the largest endorheic basins in the world, meaning that its rivers do not drain into the sea but instead flow into interior lakes or evaporate.&nbsp;



The basin is encircled by three mountain ranges: the Tien Shan to the north, the Kunlun Mountains to the south, and the Pamirs to the west. These ranges create a powerful rain shadow effect, making the region exceptionally dry.



At the heart of the Tarim Basin lies the Taklamakan Desert, one of the most extreme deserts on Earth. The desert is known for its high dunes, intense temperature swings, and minimal <a href="https://www.earth.com/news/extreme-rainfall-will-wreak-havoc-on-mountain-ranges-as-warming-climate-turns-snow-to-rain/" target="_blank" rel="noreferrer noopener">rainfall</a>.



<h2 class="wp-block-heading" id="h-history-and-geology">History and geology</h2>



Despite its harsh environment, the basin has been historically significant. It was a key section of the ancient Silk Road, with several oases such as Kashgar, Khotan, and Loulan serving as vital trading and cultural centers for centuries.



Geologically, the basin is rich in natural resources, particularly oil and natural gas, and has become a focal point for China's energy exploration and development.&nbsp;



The region’s challenging climate and remote location, however, make infrastructure development and human habitation difficult.&nbsp;



The image was captured on March 27, 2025 by the Operational Land Imager instrument on Landsat 8.



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Blanket of dust covers China’s Tarim Basin

Today's Image of the Day from the European Space Agency features a Copernicus Sentinel-2 photograph of Lake Maracaibo, located in the northwestern part of Venezuela. The lake is a significant geographical and ecological feature of South America. 



Lake Maracaibo is often considered more of a tidal bay due to its direct connection to the Caribbean Sea through the Tablazo Strait. It is one of the oldest lakes on Earth, formed approximately 36 million years ago.



"With an area of over 13,000 sq km, Lake Maracaibo is generally considered the largest lake in South America, although by some estimates it should be considered an inlet of the Caribbean Sea since much of its water is brought in by its direct connection to the ocean," explained <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"As a result, the water in the northern part of the lake is rather brackish, while the southern waters are fresh, owing to the many rivers that flow into the lake. The biggest, the Catatumbo River, can be seen entering the lake from southwest, where a large amount of sediment carried by the river appears as a yellowish plume."



<h2 class="wp-block-heading" id="h-the-catatumbo-lightning">The Catatumbo lightning</h2>



The lake is renowned for a unique weather phenomenon - the Catatumbo lightning. This natural spectacle occurs primarily where the Catatumbo River meets the <a href="https://www.earth.com/news/wildfire-smoke-has-affected-almost-every-lake-in-north-america/" target="_blank" rel="noreferrer noopener">lake</a>.



Known as the most persistent lightning storm in the world, it produces frequent and dramatic flashes of lightning, illuminating the night sky for an average of 260 nights per year.



These storms generate thousands of lightning strikes in a single night, making the region one of the most electrified places on the planet. 



The phenomenon is so intense that it has been recognized by the Guinness World Records as the place with the highest <a href="https://www.earth.com/news/lightning-on-earth-can-influence-the-weather-in-space/" target="_blank" rel="noreferrer noopener">lightning</a> activity.



Scientists believe the lightning is influenced by the area's geography and climate, including the warm air rising from the lake and its surrounding mountains.



<h2 class="wp-block-heading" id="h-economical-significance-of-lake-maracaibo">Economical significance of Lake Maracaibo </h2>



Home to one of the world's largest oil and gas reserves, Lake Maracaibo plays an important role in Venezuela’s economy.



The discovery of petroleum in the early 20th century transformed the region into a major oil-producing area, leading to the establishment of numerous oil rigs and platforms. 



However, this economic activity has come at a cost. <a href="https://www.earth.com/news/half-of-the-worlds-largest-lakes-are-losing-their-resilience/" target="_blank" rel="noreferrer noopener">Pollution</a> from oil spills, industrial waste, and agricultural runoff has significantly degraded the lake's ecosystem.



The appearance of a green, slimy algae known as Lemna has further exacerbated environmental concerns, threatening marine life and the livelihoods of local communities.



<h2 class="wp-block-heading" id="h-cultural-ties-to-lake-maracaibo">Cultural ties to Lake Maracaibo </h2>



The cultural significance of Lake Maracaibo is deeply rooted in the traditions and lifestyle of the Indigenous Añu people, who have inhabited its shores for centuries. The Añu, also known as Paraujano, are known for their distinctive stilt houses, called palafitos.



These wooden structures are built directly over the water, connected by walkways or small boats, allowing the Añu to live harmoniously with their aquatic environment. The architectural style of these stilt houses inspired the early Spanish explorers to nickname the region "The Venice of the Americas."



The Añu's way of life is closely tied to the lake. They rely on <a href="https://www.earth.com/news/sustainable-fishing-must-be-redefined-to-halt-ocean-destruction/" target="_blank" rel="noreferrer noopener">fishing</a> as a primary source of food and income, using traditional methods passed down through generations.



For the Añu, the <a href="https://www.earth.com/news/wildfire-smoke-significantly-impacts-lake-ecosystems/" target="_blank" rel="noreferrer noopener">lake</a> is more than a resource - it is the spiritual and cultural foundation of their identity and daily lives. However, modernization and environmental challenges have disrupted this traditional lifestyle. 



The oil industry’s expansion around Lake Maracaibo has led to significant environmental degradation, which threaten the lake's biodiversity and the Añu’s primary sources of sustenance.



<h2 class="wp-block-heading" id="h-lake-maracaibo-and-venezuelan-history">Lake Maracaibo and Venezuelan history</h2>



Lake Maracaibo also played a pivotal role in Venezuelan history, particularly during the Battle of Lake Maracaibo in 1823. 



This naval battle was a decisive conflict in Venezuela’s war for independence from Spain and marked one of the final military engagements of the South American liberation movements led by figures like Simón Bolívar.



Today, the lake represents a remarkable blend of natural beauty, industrial significance, and cultural heritage. 



<h2 class="wp-block-heading" id="h-ongoing-conservation-efforts">Ongoing conservation efforts </h2>



The need to protect the extraordinary environment of Lake Maracaibo is widely acknowledged. Ongoing efforts aim to harmonize ecological conservation with economic development.



Efforts to preserve the Añu culture and the lake's ecosystem have been initiated by local and international organizations. These initiatives focus on promoting sustainable development, preserving Indigenous languages and traditions, and mitigating the environmental damage caused by industrial activities. 



Despite these challenges, the Añu have shown remarkable resilience, maintaining their cultural identity and advocating for their rights and the health of their ancestral lands.



Image Credit: ESA



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Lake Maracaibo: The lightning capital of the world

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

Today's Image of the Day from NASA Earth Observatory features a satellite view of retreating glaciers in Alaska, where meltwater is rapidly expanding glacial lakes. 



“In parts of Alaska, water is replacing ice. As glaciers thin and <a href="https://www.earth.com/news/satellite-images-reveal-hidden-retreat-of-arctic-glaciers/" target="_blank" rel="noreferrer noopener">retreat</a>, meltwater collects at their fronts, forming proglacial lakes. According to an analysis by Mauri Pelto, a glaciologist at Nichols College, three such lakes in the southeastern part of the state have grown rapidly in recent decades,” said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-retreating-glaciers-in-alaska">Retreating glaciers in Alaska</h2>



“A trio of glaciers - Yakutat, Alsek, and Grand Plateau - descend from inland mountains and flow onto the coastal plain southeast of Yakutat borough, ending at Harlequin Lake, Alsek Lake, and Grand Plateau Lake,” noted NASA.&nbsp;



The retreat of the glaciers, as well as the growth of the lakes, are visible in the image. When compared to an <a href="https://eoimages.gsfc.nasa.gov/images/imagerecords/153000/153638/fastestlake_tm5_19840705_lrg.jpg" target="_blank" rel="noreferrer noopener">image</a> captured by Landsat 5 in the summer of 1984, the changes are even more evident.



NASA elaborated on the extent of the glacier retreat from 1984 to 2024. “During this period, Yakutat Glacier’s main arm retreated 4.3 miles, while Alsek Glacier’s northern and southern arms retreated 3.3 miles and 3.4 miles, respectively. Grand Plateau Glacier’s northern arm lost the most, retreating 4.8 miles.”



<h2 class="wp-block-heading" id="h-glacial-lakes-doubled-in-size-nbsp">Glacial lakes doubled in size&nbsp;</h2>



“Collectively, the three lakes more than doubled in size over 40 years. In 1984, they covered about 50 square miles. By 2024, they spanned 90 square miles. That’s an area larger than Seneca Lake (67 square miles) - one of the Finger Lakes in New York, which also have a glacial origin,” said NASA.



Pelto noted that the lakes forming in this region are immense - starting at the mountains and spreading toward the coast - making this a new lake district that is unique in our nation.



“Millions of other lakes, named and unnamed, dot the state. But this system has grown fast, so much so that Pelto thinks it might represent the fastest lake growth in the United States this century,” said NASA.



<h2 class="wp-block-heading" id="h-understanding-glacier-retreat-nbsp">Understanding glacier retreat&nbsp;</h2>



Glacier retreat is a significant phenomenon driven primarily by global warming the results from rising greenhouse gas <a href="https://www.earth.com/news/global-carbon-dioxide-emissions-hit-a-record-high-in-2023/" target="_blank" rel="noreferrer noopener">emissions</a>.&nbsp;



As temperatures rise, glaciers lose more ice during the summer melt than they can regain in winter snowfall, causing them to shrink over time. This process has profound implications for ecosystems, water resources, and global sea levels.



<h3 class="wp-block-heading" id="h-glacial-lakes">Glacial lakes</h3>



When glaciers retreat, they often leave behind depressions in the landscape that can fill with meltwater, forming glacial lakes. These lakes are typically bounded by natural dams made of rock, ice, or moraine - accumulations of debris left behind by the glacier's movement.&nbsp;



Over the past century, the number and size of glacial lakes worldwide have increased significantly due to the accelerating pace of <a href="https://www.earth.com/news/tropical-glaciers-offer-a-glimpse-of-our-harsh-climate-reality/" target="_blank" rel="noreferrer noopener">glacier</a> retreat. This trend is especially evident in high-altitude regions like the Himalayas, the Andes, and the Alps, as well as in polar areas such as Alaska and Greenland.



<h3 class="wp-block-heading" id="h-positive-and-negative-impacts-nbsp">Positive and negative impacts&nbsp;</h3>



Glacial lakes can have both positive and negative impacts. They provide critical water sources for downstream communities, support biodiversity, and sometimes offer opportunities for hydropower development or tourism.&nbsp;



However, they also pose serious risks. The dams holding back these lakes can fail suddenly, causing glacial lake outburst floods (GLOFs). These catastrophic events can devastate downstream areas, destroying infrastructure, agricultural lands, and habitats while endangering human lives.



<h3 class="wp-block-heading" id="h-monitoring-changes">Monitoring changes</h3>



Understanding glacier retreat and glacial lake formation requires a multidisciplinary approach, combining climate science, hydrology, and geology.&nbsp;



Monitoring these changes is essential to mitigate associated risks and adapt to the evolving landscape shaped by a <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fperu-has-lost-over-half-of-its-glaciers-in-six-decades%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">warming planet</a>.



<h2 class="wp-block-heading" id="h-glacier-retreat-worldwide">Glacier retreat worldwide</h2>



Studies and satellite observations show that most glaciers in almost all regions of the world are shrinking.&nbsp;



Melting glaciers contribute significantly to global <a href="https://www.earth.com/news/emergency-meeting-reveals-the-alarming-extent-of-antarcticas-ice-loss/" target="_blank" rel="noreferrer noopener">sea level rise</a>, which threatens coastal communities and ecosystems.



The retreat of glaciers is considered one of the clearest indicators of climate change.&nbsp;Some glaciers are retreating at unprecedented rates, indicating accelerating climate impacts.



The image was captured on August 4, 2024 by the Landsat 8 satellite.



Image Credit: NASA Earth Observatory



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Retreating glaciers and expanding meltwater lakes in Alaska

Today's Image of the Day from NASA Earth Observatory features dust streaming off the coast of Iran in January 2025.



“Some of the desert dust was carried across the Gulf of Oman to the Arabian Peninsula, degrading air quality for those in its path,” noted <a href="https://earthobservatory.nasa.gov/images/153859/desert-dust-streams-from-iran" target="_blank" rel="noreferrer noopener">NASA</a>.



“The airborne material appears to primarily originate in the dried bed of the intermittent lake known as Hamun-e Jazmurian (Hamun-e Jaz Murian), while some may be blown from coastal areas." 



"Along with arid regions such as the Garagum and Lut deserts and the Sistan Basin, the lakebed is a major source of dust in southwest Asia.”



<h2 class="wp-block-heading" id="h-precipitation-in-the-jazmurian-basin">Precipitation in the Jazmurian Basin</h2>



According to NASA, some areas of the Jazmurian Basin receive less than four inches of rain annually, on average, and evaporation rates are high. During wet times, however, parts of the basin may be covered by an intermittent lake, marshland, or other vegetation.&nbsp;



“Terra’s MODIS sensor has previously captured images of the area when water is present in Hamun-e Jazmurian and when green vegetation fringes the lakebed,” said NASA.



“In early 2025, the land was dry enough for winds to blow dust plumes south-southwest over the Gulf of Oman. Dust traveled across the water to the coast of the United Arab Emirates, where the haze reduced visibility in places, according to news reports.”



<h2 class="wp-block-heading" id="h-particles-in-dust-storms">Particles in dust storms</h2>



In addition to disrupting transportation and other daily activities, the suspended particles in dust storms can pose significant health risks. 



Recent research has revealed that dust from the Jazmurian Basin often contains heavy metals and other potentially harmful substances, such as silica and organic pollutants, which can negatively impact both human and ecosystem health.&nbsp;



Prolonged exposure to these particles has been linked to respiratory and cardiovascular issues, as well as the exacerbation of pre-existing health conditions like asthma and bronchitis.



<h2 class="wp-block-heading" id="h-environmental-impact-of-dust-storms">Environmental impact of dust storms</h2>



The <a href="https://www.earth.com/news/dust-is-an-understudied-contributor-to-climate-change/" target="_blank" rel="noreferrer noopener">environmental impact</a> of dust storms extends beyond human health. The fine particles can settle on vegetation, reducing photosynthesis and agricultural productivity.&nbsp;



Dust deposition can also alter soil composition by introducing heavy metals and changing nutrient balances, which may affect crop growth and soil microbial communities. 



Such changes can lead to long-term degradation of arable land and disrupt local food security.



<h2 class="wp-block-heading" id="h-dust-in-the-jazmurian-basin-nbsp">Dust in the Jazmurian Basin&nbsp;</h2>



Communities near the Jazmurian Basin are particularly vulnerable to the effects of dust storms due to limited access to healthcare and mitigation resources.



Seasonal changes and climate conditions, including prolonged droughts and desertification, further intensify the frequency and severity of dust storms in the region.&nbsp;



This creates a cycle of environmental and health challenges, making it imperative to develop strategies for prevention and adaptation.



Potential measures include reforestation and soil stabilization projects to reduce dust emissions, stricter regulations to limit activities that contribute to desertification, and public health initiatives to educate communities on protective measures during dust events.&nbsp;



Investing in early warning systems and <a href="https://www.earth.com/news/climate-driven-wildfires-worsen-u-s-air-quality-and-health/" target="_blank" rel="noreferrer noopener">air quality</a> monitoring can also help minimize exposure and protect both human populations and the environment.



<h2 class="wp-block-heading" id="h-significance-of-the-jazmurian-basin">Significance of the Jazmurian Basin</h2>



The Jazmurian Basin is a prominent endorheic basin located in southeastern Iran, spanning parts of the provinces of Sistan and Baluchestan as well as Kerman. It lies at the heart of an arid region characterized by sparse vegetation, high temperatures, and limited rainfall.&nbsp;



The basin is primarily fed by the Halil and Bampur rivers, which provide seasonal water flow to the basin's low-lying areas. At its center lies the Jazmurian Depression, which forms a seasonal playa or shallow lake, though it often dries up during extended dry periods.&nbsp;



The area holds geological and archaeological significance, offering insights into ancient human settlements and environmental changes over time.&nbsp;



Despite its harsh climate, the basin supports small-scale agriculture and serves as a critical habitat for certain desert-adapted wildlife. 



The image was captured on January 22 by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite.&nbsp;



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Dust rises from the Jazmurian Basin in Iran

Today's Image of the Day from NASA Earth Observatory features the Fedchenko Glacier in the Pamir Mountains of Tajikistan. It is one of the world's longest glaciers outside of the polar regions.&nbsp;



“An astronaut aboard the International Space Station took this photo of glaciers in the high-elevation valleys of the Pamir Mountains of Central Asia. The upper portion of Fedchenko Glacier crosses the center of the scene.”



NASA noted that most of the larger glaciers in the image show a prominent pattern of light- and dark-brown parallel lines.&nbsp;



“The darker ‘streamlines,’ known as medial moraines, give a sense of the direction of flow of the ice down the valleys. These are concentrations of debris that has been eroded by the glacier from the adjacent mountainsides or a rocky outcrop,” said NASA.



<h2 class="wp-block-heading" id="h-fedchenko-a-high-altitude-glacier">Fedchenko: A high-altitude glacier</h2>



Fedchenko Glacier stretches for approximately 48 miles and covers an area of around 270 square miles. This massive glacier is a critical source of <a href="https://www.earth.com/news/satellites-reveal-a-sudden-drop-in-global-freshwater-levels/" target="_blank" rel="noreferrer noopener">freshwater</a>, feeding several rivers and influencing the region's hydrology.



Fedchenko lies at high altitudes, with its origins in the high peaks of the Pamirs, where snow accumulates heavily. Despite being situated in a relatively arid region, the glacier's significant size and volume are maintained by substantial snowfall. 



Named after Alexei Pavlovich Fedchenko, a Russian explorer and naturalist, the glacier was first surveyed in 1928 during Soviet-era expeditions. It plays a crucial role in climate studies, as changes in its length and mass provide insights into the effects of global warming in Central Asia.&nbsp;



The glacier is also part of a spectacular and remote landscape, surrounded by towering <a href="https://www.earth.com/news/early-humans-preferred-the-mountains-and-it-changed-our-evolution/" target="_blank" rel="noreferrer noopener">mountains</a> and rugged terrain, making it a key feature of the Pamirs' natural beauty.&nbsp;



<h2 class="wp-block-heading" id="h-threats-to-glaciers-worldwide">Threats to glaciers worldwide</h2>



Like many glaciers worldwide, Fedchenko faces the threat of retreat due to <a href="https://www.earth.com/news/peru-has-lost-over-half-of-its-glaciers-in-six-decades/" target="_blank" rel="noreferrer noopener">global warming</a>, raising concerns about water availability and ecosystem changes in the region.



Rising global temperatures caused by greenhouse gas emissions are the primary driver of glacier melting. Warmer temperatures not only melt glacier surfaces but also increase the flow of meltwater beneath them, accelerating their disintegration.



<h3 class="wp-block-heading" id="h-human-activities-and-pollution-nbsp">Human activities and pollution&nbsp;</h3>



Deforestation and urbanization exacerbate these effects by reducing reflective snow cover and increasing heat absorption in nearby areas.&nbsp;



Airborne pollutants like soot and black carbon darken glacier surfaces, reducing their ability to reflect sunlight and speeding up the rate of melting.&nbsp;



Industrial activities and tourism in glacier regions add physical stress and pollution, further degrading these fragile ecosystems.



<h3 class="wp-block-heading" id="h-water-supplies">Water supplies</h3>



The loss of glaciers has far-reaching consequences. It disrupts freshwater supplies for millions of people who depend on glacial runoff for drinking water, agriculture, and hydropower.&nbsp;



<h3 class="wp-block-heading" id="h-rising-sea-levels">Rising sea levels</h3>



<a href="https://www.earth.com/news/melting-glaciers-unleash-invasive-species-into-unexpected-areas/" target="_blank" rel="noreferrer noopener">Melting glaciers</a> contribute to rising sea levels, threatening coastal communities and ecosystems worldwide. Additionally, the loss of glaciers impacts biodiversity, as many species rely on cold, glacial habitats for survival.



<h3 class="wp-block-heading" id="h-protecting-glaciers">Protecting glaciers</h3>



Efforts to mitigate these threats focus on reducing <a href="https://www.earth.com/news/melting-glaciers-are-hidden-sources-of-greenhouse-gases/" target="_blank" rel="noreferrer noopener">greenhouse gas</a> emissions, protecting glacier regions from industrial exploitation, and promoting sustainable tourism practices.&nbsp;



However, without urgent action, the continued decline of glaciers will have profound implications for the planet's climate, water systems, and ecosystems.



<h2 class="wp-block-heading" id="h-the-pamir-mountains-nbsp">The Pamir Mountains&nbsp;</h2>



The Pamir Mountains, often called the "Roof of the World," are a vast and rugged mountain range located in Central Asia.&nbsp;



They span across Tajikistan, Afghanistan, China, and Kyrgyzstan, forming a vital part of the junction where the Himalayas, the Tian Shan, the Karakoram, the Kunlun, and the Hindu Kush converge.&nbsp;



With peaks soaring over 7,000 meters, including Ismoil Somoni Peak, the range is home to some of the highest altitudes on Earth.



The Pamir Mountains have been central to trade and cultural exchange for centuries, serving as a critical segment of the ancient Silk Road.&nbsp;



Today, the mountains are a popular destination for trekkers and explorers drawn by their breathtaking beauty and challenging terrain.



The Pamirs are not only a natural wonder but also a biological treasure trove, supporting unique wildlife that is adapted to extreme altitudes.&nbsp;



Culturally, the mountains are home to diverse communities, each with its unique traditions and ways of life, shaped by the harsh but majestic environment.



Image Credit: NASA Earth Observatory



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Fedchenko Glacier in the Pamir Mountains

Today's Image of the Day from the European Space Agency features UGC 5460, a spiral galaxy that is located about 60 million light-years away in the constellation Ursa Major.&nbsp;



“This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms and bright blue star clusters. Also captured in the upper left-hand corner of this image is a far closer object: a star just 577 light-years away in our own galaxy,” said <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“UGC 5460 has hosted two recent supernovae named SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programmes that aim to study various kinds of supernovae.”&nbsp;



<h2 class="wp-block-heading" id="h-a-core-collapse-supernova-nbsp">A core-collapse supernova&nbsp;</h2>



SN 2015as is an example of a core-collapse supernova. This type of <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> occurs when the core of a massive star - typically with more than 8 times the mass of the sun - can no longer support its own gravity after exhausting its nuclear fuel. 



This causes the core to collapse under its own weight, leading to an extremely violent explosion. The collapse triggers the release of an enormous amount of energy, expelling the outer layers of the star into space.



In the aftermath of the explosion, a dense <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">remnant</a> is created. This is often a neutron star or black hole, depending on the mass of the original star. Core-collapse supernovae are some of the most powerful events in the universe.



According to ESA, Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a <a href="https://www.earth.com/news/supernova-dandelion-year-1181-leaves-behind-zombie-star-defying-death/" target="_blank" rel="noreferrer noopener">supernova</a> collides with the gas that surrounds the exploded star.



<h2 class="wp-block-heading" id="h-rare-stars-with-large-eruptions-nbsp">Rare stars with large eruptions&nbsp;</h2>



“SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae,” noted ESA.



“Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location, and the explosion’s identity may be revealed at last.”



<h2 class="wp-block-heading" id="h-what-is-a-spiral-galaxy">What is a spiral galaxy?</h2>



Spiral galaxies are some of the most recognizable and beautiful structures in the universe. They are known for their distinctive arms that spiral outward from a central bulge.&nbsp;



These galaxies are typically composed of stars, gas, dust, and dark matter. The arms are often sites of intense <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star formation</a>, where clouds of gas collapse to form new stars. 



In the center of a spiral galaxy lies a dense concentration of older stars and, often, a supermassive black hole.



<h2 class="wp-block-heading" id="h-structure-of-a-spiral-galaxy-nbsp">Structure of a spiral galaxy&nbsp;</h2>



The structure of a spiral galaxy is generally divided into three main components: the disk, the bulge, and the halo.&nbsp;



The disk is where the spiral arms are located and contains most of the galaxy's visible stars and interstellar medium.&nbsp;



The bulge is a tightly packed region of older stars at the core, and the halo consists of a sparse collection of stars and globular clusters that surround the galaxy.&nbsp;



Spiral galaxies can be classified into different types based on the tightness and number of their spiral arms, as well as the size of their central bulge.



<h2 class="wp-block-heading" id="h-the-milky-way-galaxy">The Milky Way galaxy</h2>



Our solar system is located within a large spiral galaxy known as the Milky Way. The name refers to its appearance as a dim, milky band of light stretching across the night sky.&nbsp;



The term "Milky Way" comes from ancient Greek mythology, where it was associated the goddess Hera's milk spilling into the sky. In Greek, it was called "Galaxias Kyklos," meaning "milky circle."&nbsp;



Spanning about 100,000 light-years in diameter, the Milky Way is composed of stars, gas, dust, and dark matter. The galaxy has a distinct disk shape with spiral arms that wind outward from a central bulge, which houses a supermassive <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/" target="_blank" rel="noreferrer noopener">black hole</a>. 



Our sun is located in one of the spiral arms - known as the Orion Arm - positioned roughly halfway from the center to the outer edge.&nbsp;



The Milky Way is part of a small group of galaxies called the Local Group, which includes the Andromeda Galaxy and several smaller galaxies.



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Hubble views a spiral galaxy with stellar explosions

Today's Image of the Day from NASA features an extraordinary view of Uranus, the seventh planet from the sun in our solar system. 



The photo reveals the rings, moons, and extreme seasons of the ice giant Uranus in unprecedented detail.&nbsp;



<h2 class="wp-block-heading" id="h-dynamic-north-polar-cap-nbsp">Dynamic north polar cap&nbsp;</h2>



“The Webb image exquisitely captures Uranus’s seasonal north polar cap, including the bright, white, inner cap and the dark lane in the bottom of the polar cap,” noted NASA.



Unlike Earth, where polar ice caps are formed by the freezing of water, Uranus's polar caps are thought to be primarily composed of a dense concentration of haze in the atmosphere.&nbsp;



The polar cap's haze is likely composed of methane particles. Methane in Uranus's atmosphere condenses into ice particles, which then create a thick haze that scatters sunlight, giving the polar cap its distinct bright appearance in visible and infrared light.



The polar cap is dynamic and changes over time. It becomes more prominent during the summer season of each pole. 



As Uranus moves along its orbit, the cap's appearance transforms, with the haze becoming thicker and brighter when the pole is in continuous sunlight.



<h2 class="wp-block-heading" id="h-the-zeta-ring-nbsp">The Zeta ring&nbsp;</h2>



The inner and outer rings of Uranus are visible in the image, including Zeta - the innermost ring which is the faintest and most difficult to observe.



The <a href="https://www.earth.com/news/stunning-photo-of-uranus-and-its-rings-and-moons-captured-by-the-webb-telescope/" target="_blank" rel="noreferrer noopener">rings of Uranus</a> are primarily composed of narrow bands of particles, likely made of water ice mixed with a dark material. These rings are distinct from those of Saturn in that they are much darker and narrower.



The faintness and characteristics of the Zeta ring make it a subject of interest in studies related to the dynamics and composition of planetary ring systems.



<h2 class="wp-block-heading" id="h-moons-of-uranus-nbsp">Moons of Uranus&nbsp;</h2>



The <a href="https://science.nasa.gov/mission/webb/multimedia/images/" target="_blank" rel="noreferrer noopener">Webb</a> photo also features nine of the planet’s <a href="https://www.earth.com/news/nasa-four-uranus-moons-may-have-oceans-that-are-miles-deep/" target="_blank" rel="noreferrer noopener">moons</a>, which appear as blue dots surrounding the rings.&nbsp;



“Clockwise starting at 2 o’clock, they are: Rosalind, Puck, Belinda, Desdemona, Cressida, Bianca, Portia, Juliet, and Perdita. The orbits of these moons share the 98-degree tilt of their parent planet relative to the plane of the solar system,” noted NASA.



Uranus has 27 known moons, and they are divided into three main groups based on their orbits: the inner moons, the major moons, and the irregular moons.



The <a href="https://www.earth.com/news/uranus-moon-ariel-may-have-a-hidden-ocean/" target="_blank" rel="noreferrer noopener">moons</a> of Uranus are unique because they are named after characters from the works of William Shakespeare and Alexander Pope, rather than being named after figures from classical mythology, as is common for the moons of other planets.



<h2 class="wp-block-heading" id="h-the-ice-giant-uranus-nbsp">The ice giant Uranus&nbsp;</h2>



Uranus is classified as an "ice giant" because, unlike the gas giants Jupiter and Saturn, which are primarily composed of hydrogen and helium, Uranus has a significant proportion of "ices" in its composition.&nbsp;



In astronomical terms, ices refer to volatile substances like water, ammonia, and methane, which exist in solid or liquid forms at the low temperatures found in the outer solar system.



Uranus has a thick atmosphere of hydrogen and helium, but beneath that, it contains a large, dense mantle composed of these ices, along with rock and other heavier elements.&nbsp;



The term <a href="https://www.earth.com/news/diamond-rain-may-be-common-on-giant-icy-planets/" target="_blank" rel="noreferrer noopener">ice giant</a> differentiates Uranus (and Neptune, the other ice giant) from the larger gas giants, emphasizing the different chemical compositions and internal structures of these planets.



<h2 class="wp-block-heading" id="h-climate-of-uranus-nbsp">Climate of Uranus&nbsp;</h2>



Uranus has a unique and extreme climate, largely influenced by its unusual tilt, which causes the planet to rotate almost on its side. This tilt leads to extreme seasonal variations, with each pole experiencing 42 years of continuous sunlight followed by 42 years of darkness.&nbsp;



Even though it is closer to the sun than Neptune, Uranus is the coldest planet in the solar system, with temperatures plunging to as low as -224°C (-371°F). The reason for this is not fully understood, but it might be due to an internal heat distribution anomaly.



Despite these frigid conditions, Uranus experiences intense weather patterns, including powerful storms and winds that can reach speeds of up to 900 kilometers per hour. These winds blow in the same direction as the planet’s rotation and are some of the fastest in the solar system.



Storms on Uranus are driven by its internal heat and the interaction of its <a href="https://www.earth.com/news/uranus-is-more-gassy-less-icy-than-we-ever-imagined/" target="_blank" rel="noreferrer noopener">atmospheric gases</a>. Observations have shown that these storms can be quite large, sometimes comparable in size to the Earth, and can last for several years.&nbsp;



The planet’s extreme axial tilt also means that the storms and weather patterns are highly variable, depending on the season. During equinoxes, when the Sun is directly over the equator, Uranus exhibits more storm activity compared to when the poles are pointed towards the Sun or away from it.



<h2 class="wp-block-heading" id="h-observations-of-uranus">Observations of Uranus</h2>



“One day on Uranus is about 17 hours, so the planet’s rotation is relatively quick. This makes it supremely difficult for observatories with a sharp eye like Webb to capture one simple image of the entire planet - storms and other atmospheric features, and the planet’s moons, move visibly within minutes,” explained NASA.



“This image combines several longer and shorter exposures of this dynamic system to correct for those slight changes throughout the observing time.”



The first recorded observations of Uranus were made by John Flamsteed on December 13, 1690. However, Flamsteed mistakenly identified the planet as a star, which he named “34 Tauri."&nbsp;



It wasn't until March 13, 1781, that Uranus was officially identified as a planet by William Herschel. He initially thought he had discovered a comet, but further observations and calculations by other astronomers confirmed that it was a new planet, making Uranus the first planet discovered in modern history with the aid of a telescope.



Image Credit: NASA, ESA, CSA, STScI



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The ice giant Uranus in stunning detail

Today's Image of the Day from NASA features an extraordinary...

The MODIS instrument, short for Moderate Resolution Imaging Spectroradiometer, is a key instrument aboard the Terra and Aqua satellites. MODIS is playing a vital role in the development of Earth ecosystem models, able to predict global changes, which then assist policy makers in making informed decisions about the protection of the global environment.

Heavy snow and cloud cover in the Alps are seen in this Image of the day&nbsp;from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at heavy snow and low clouds in the Alps. Wildlife such as ibex live in the higher peaks to elevations of 3,400 m (11,155 ft), and plants such as Edelweiss grow in rocky areas in lower elevations as well as in higher elevations.

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

Aqua is a NASA scientific research satellite that studies precipitation, evaporation, and water cycles. Terra and Aura make up the Earth Observing System. It's the second component of the system.

A frozen Lake Erie in February Today’s Image of the Day comes from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a frozen <a href="https://www.earth.com/image/icy-lake-erie/">Lake Erie</a>, which is currently 93.3 percent iced over. A frozen Lake Erie in February
This false-color image was created using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Aqua satellite to differentiate between snow, ice, and clouds.
Lake Erie /ˈɪəri/ (French: Lac Érié) is the fourth-largest lake (by surface area) of the five Great Lakes in North America, and the eleventh-largest globally if measured in terms of surface area.It is the southernmost, shallowest, and smallest by volume of the Great Lakes and therefore also has the shortest average water residence time. At its deepest point Lake Erie is 210 feet (64 metres) deep. 
Situated on the International Boundary between Canada and the United States, Lake Erie&#8217;s northern shore is the Canadian province of Ontario, specifically the Ontario Peninsula, with the U.S. states of Michigan, Ohio, Pennsylvania, and New York on its western, southern, and eastern shores. These jurisdictions divide the surface area of the lake with water boundaries. 
The lake was named by the Erie people, a Native American people who lived along its southern shore. The tribal name &#8220;erie&#8221; is a shortened form of the Iroquoian word erielhonan, meaning long tail
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Image Credit: <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>

A frozen Lake Erie in February

Aqua Earth Observing Satellite

This beautiful photo gallery contains 50 incredible images of Earth from Space. These images were taken by astronauts onboard the International Space Station, as well as by a multitude of NASA satellites orbiting the earth.

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a> and features a look at Super Typhoon Noru in the Pacific Ocean just south of <a href="https://www.earth.com/news/first-blue-chrysanthemums-created/">Japan</a>.
This image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite on July 31, 2017. 
At the time the photo was taken, Typhoon Noru was located just 250 kilometers south of Iwo Jima. Maximum sustained winds hit 150 miles per hour.
The storm briefly became a category 5 on July 30, before being downgraded to a category 4 one day later.
&#8211;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

Photos from the International Space Station are found in this awesome Earth.com image gallery. Flat-earthers won't agree, but these incredible photos of the Earth were taken by astronauts onboard the International Space Station. The International Space Station is a modular space station in low Earth orbit.

Northern Italy from the space station is seen here in this Image of the Day from the <a href="http://www.esa.int/">European Space Agency</a> (ESA). The view includes the top half of the Italian Peninsula, along with <a href="https://www.earth.com/image/wildfires-burn-northern-corsica/">Corsica</a> and Sardinia off the coast. This image was captured by ESA astronaut Paolo Nespoli on his third and final mission to the Space Station.

Northern Italy from the Space Station

Photos from the International Space Station

Conservation scientists often reassure themselves with a simple rule of thumb: species that live over huge swaths of territory and boast large populations are usually safer from extinction than creatures confined to small patches of habitat. 



However, a new global analysis of roughly 1,500 bird species has revealed that there's no comfortable rule when it comes to climate change.



The study, led by the <a href="https://www.utexas.edu/" target="_blank" rel="noreferrer noopener">University of Texas at Austin</a>, shows that a wide geographic footprint can hide an unexpectedly narrow dependence on climate. In a warming world, that hidden fragility could make certain familiar birds surprisingly vulnerable.



“Because that region is so big, species that occupy it tend to have large populations and large geographic range sizes - two characteristics that are often associated with lower <a href="https://www.earth.com/news/bird-extinctions-shatter-the-harmonious-balance-of-nature/" target="_blank" rel="noreferrer noopener">extinction</a> risks,” explained Carlos Botero, an associate professor of integrative biology and senior author of the study.



“The problem here is that because many of those species are adapted to a very narrow range of climates, those seemingly large populations can be quite <a href="https://www.earth.com/news/hundreds-of-bird-species-face-extinction-risks-in-the-neotropics/" target="_blank" rel="noreferrer noopener">susceptible</a> to collapse when climate patterns begin to change.”



<h2 class="wp-block-heading" id="h-a-paradox-from-the-arctic"><a></a>A paradox from the Arctic</h2>



One of the clearest examples comes from the Arctic, where a single broad climatic regime stretches across thousands of miles. The Bohemian waxwing is emblematic: its breeding distribution spans an immense arc from Scandinavia to Alaska.



Yet the Arctic’s uniform environment means that the waxwing’s entire life cycle is tied to cold temperatures and consistent snow cover. Even minor warming or shifts in precipitation could push the species outside its comfort zone - no matter how far it can fly within that chilly belt.



In their analysis, Botero’s team contrasted the waxwing with the chestnut-crowned laughingthrush. The laughingthrush is restricted to a sliver of montane forest in Nepal, Bhutan, and neighboring parts of Asia - an area a fraction of the waxwing’s extent.



But the Himalayan foothills expose that small-ranged bird to a wider palette of temperatures and <a href="https://www.earth.com/news/extreme-rainfall-increases-as-a-direct-result-of-global-warming/" target="_blank" rel="noreferrer noopener">rainfall</a> patterns throughout the year. The laughingthrush therefore occupies a broader “climate niche,” potentially giving it more room to maneuver as conditions shift.



<h2 class="wp-block-heading" id="h-bird-brains-and-climate-specialization">Bird brains and climate specialization</h2>



The surprises did not stop with range maps. Analyses also revealed an unexpected relationship between brain size and climate flexibility. 



Larger-brained birds, long celebrated for their resourcefulness, tended to be the very species most tightly wedded to specific climate regimes. “Larger brain sizes correlate with more flexible behavior, so `big-brained birds are usually expected to be more adaptable,” Botero said. 



“However, it turns out that many big-brained birds are climate specialists - meaning that they have evolved to thrive in very particular climate types and may therefore also be more <a href="https://www.earth.com/news/some-birds-are-more-at-risk-from-climate-change-than-others/" target="_blank" rel="noreferrer noopener">vulnerable</a> to climate change than we expected.”



Why would an animal capable of problem-solving and tool use paint itself into a narrow climatic corner? Botero and coauthor João Fabrício Mota Rodrigues (now at <a href="https://unicamp.br/" target="_blank" rel="noreferrer noopener">Brazil’s University of Campinas</a>) suspect that cognitive prowess helps species exploit highly specific environments with great efficiency. 



Over evolutionary time, that specialization can lead to tight physiological tolerances - exactly the trait that becomes risky when the planet’s thermostat creeps upward.



<h2 class="wp-block-heading" id="h-building-a-two-dimensional-climate-map"><a></a>Building a two-dimensional climate map</h2>



To quantify each species’ niche, the team merged two huge datasets. First came detailed range maps created from hundreds of thousands of sightings submitted by volunteer birders to the <a href="https://ebird.org/home" target="_blank" rel="noreferrer noopener">eBird</a> platform. 



Second, the researchers developed a simplified, yet powerful, climate classification that captures two axes of environmental hardship. The first axis - “temperature harshness” - rises as places become colder, more variable, and less predictable. 



The second - “xeric harshness” - ratchets upward with drier, more erratic rainfall. Plotting Earth’s land areas across those twin axes produced a two-dimensional climate space. 



Points near the center represent benign zones: warm, moist, and seasonally steady. Farther out lie the extremes: parched deserts, storm-prone tropics, or frigid <a href="https://www.earth.com/news/how-will-changing-tundra-landscapes-affect-earths-climate/" target="_blank" rel="noreferrer noopener">tundra</a>. 



By overlaying each bird’s distribution onto that grid, the researchers measured how much of the climate space the species actually uses. A small ellipse located at one edge of the diagram signals trouble. 



Birds confined to that limited set of conditions may find it hard to track shifting isotherms or precipitation belts. Conversely, a large swath cutting across multiple quadrants suggests climatic breadth and, potentially, resilience.



<h2 class="wp-block-heading" id="h-hidden-interactions-hidden-risks"><a></a>Hidden interactions, hidden risks</h2>



The latest study adds to a growing chorus urging conservation planners to reconsider single-factor threat lists. 



“We need to stop looking at individual risk factors in isolation, but evaluate how these complex factors combine,” Botero emphasized. “Sometimes, it is the unexpected interactions that matter most.”



Indeed, a species can check all the traditional “safe” boxes - huge range, big population, high intelligence - yet still sit on a climatic knife-edge. Arctic breeders are just one illustration. 



Tropical forest birds with large brains and tight humidity requirements could face similar hazards if droughts intensify. Even desert specialists might falter if rainfall becomes too unpredictable for reliable breeding.



<h2 class="wp-block-heading" id="h-citizen-science-and-big-picture-insights">Citizen science and big-picture insights</h2>



According to Rodrigues, the analysis was made possible by citizen scientists. Data derived from eBird gave the experts an unprecedented global snapshot.



Without hundreds of thousands of observers recording where they saw even the most common species, they couldn’t have mapped climate niches with this precision. Such an approach is quickly becoming a backbone of ecological forecasting. 



By harnessing real-time, geo-tagged records from amateurs, researchers can update models as species ranges expand, contract, or fragment - often faster than traditional field surveys could manage.



<h2 class="wp-block-heading" id="h-smarter-species-conservation">Smarter species conservation</h2>



Recognizing climate specialization where none was suspected may reshape conservation priorities. Agencies often triage limited funds toward charismatic, range-restricted species. 



But Botero’s work suggests that some cosmopolitan birds deserve equal attention, precisely because their “bigness” masks a slender climatic lifeline. Future investigations will probe whether similar patterns hold for mammals, reptiles, or <a href="https://www.earth.com/news/amphibians-are-being-pushed-beyond-their-heat-limits/" target="_blank" rel="noreferrer noopener">amphibians</a>. 



For now, the message is clear: size - of range, of population, of brain - does not guarantee safety. In a rapidly changing climate, ecological nuance matters. 



Understanding that nuance could spell the difference between proactive protection and costly rescue missions when numbers suddenly plummet. As policymakers craft strategies for the coming decades, studies like this remind us that vulnerability isn’t always where we expect it. 



Sometimes it hides beneath vast northern skies, in flocks that seem abundant - until the weather shifts just a little too far, and the invisible boundaries of their climate niches close in.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-58815-1" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Big brains and wide ranges can't save birds from climate change

Conservation scientists often reassure themselves with a simple rule of...

For decades, astronomers have searched for the universe’s missing matter - the normal matter that should exist according to the Big Bang theory, but can’t be fully seen.



This isn’t about dark matter, which constitutes most of the universe’s mass. It’s about ordinary, visible matter like stars, gas, and galaxies. Even after accounting for everything that can be observed through telescopes, more than half of this matter seemed to be missing.



But new research might have solved the mystery. Scientists believe they’ve found the missing matter in a form that’s been hiding in plain sight - very diffuse, invisible hydrogen gas floating far beyond what we once thought was the edge of galaxies.



<h2 class="wp-block-heading" id="h-faint-gas-solves-the-mystery">Faint gas solves the mystery</h2>



The discovery comes from a team of researchers at the <a href="https://www.berkeley.edu/" target="_blank" rel="noreferrer noopener">University of California, Berkeley</a>, in collaboration with the Lawrence Berkeley National Laboratory. 



The experts believe the missing matter is in a faint, expanded halo of ionized <a href="https://www.earth.com/news/hydrothermal-vents-earths-first-living-beings-hydrogen-gas-energy/" target="_blank" rel="noreferrer noopener">hydrogen</a> that surrounds galaxies and stretches much farther than previously assumed - about five times farther, in fact.



This gas doesn’t glow or shine. It's nearly impossible to detect with traditional tools. But its presence helps fix a major inconsistency between what we see in the sky and what our models of the <a href="https://www.earth.com/news/if-the-big-bang-theory-is-correct-what-exactly-happened/" target="_blank" rel="noreferrer noopener">Big Bang</a> predict.



"We think that, once we go farther away from the galaxy, we recover all of the missing gas," said Boryana Hadzhiyska, a Miller Postdoctoral Fellow at UC Berkeley and lead author of the study.



"To be more accurate, we have to do a careful analysis with simulations, which we haven't done. We want to do a careful job."



"The measurements are certainly consistent with finding all of the gas," noted Simone Ferraro, a senior scientist at Berkeley Lab and UC Berkeley.



<h2 class="wp-block-heading" id="h-the-cosmic-microwave-background">The cosmic microwave background </h2>



To find this gas, the team used a technique that involved "stacking" images of roughly 7 million <a href="https://www.earth.com/news/galaxies-are-much-bigger-than-we-originally-believed-gas-clouds/" target="_blank" rel="noreferrer noopener">galaxies</a>. All of these galaxies lie within 8 billion light-years from Earth. 



By studying how these galaxies slightly dim or brighten the cosmic microwave background - the oldest light in the universe - they were able to detect the scattering effect from free electrons in the ionized gas. This phenomenon is called the kinematic Sunyaev-Zel'dovich effect.



"The cosmic microwave background is in the back of everything we see in the universe. It's the edge of the observable universe," Ferraro explained. "So you can use that as a backlight to see where the gas is."



The galaxy images used in the study were taken using the Dark Energy Spectroscopic Instrument (DESI) on the Mayall Telescope in Arizona. DESI, built by a Berkeley Lab-led collaboration, is working on a massive 3D <a href="https://www.earth.com/news/largest-ever-3d-map-of-the-universe-lets-us-travel-back-11-billion-years/" target="_blank" rel="noreferrer noopener">map of the universe</a>. 



For background light, the team relied on data from the Atacama Cosmology Telescope in Chile, which produced the most accurate measurements of the cosmic microwave background before its retirement in 2022.



<h2 class="wp-block-heading" id="h-gas-expelled-from-black-holes">Gas expelled from black holes</h2>



The discovery has bigger implications than just solving the missing matter problem. It also sheds light on what’s happening at the center of galaxies - specifically, around the enormous black holes that lie at their cores.



Traditionally, scientists believed these black holes only shot out jets of gas and radiation early in their life, when they were feeding on surrounding material. But this new research suggests that the black holes might not be so quiet during their middle years after all.



"One problem we don't understand is about AGNs, and one of the hypotheses is that they turn on and off occasionally in what is called a duty cycle," said Hadzhiyska.



This process - called feedback - involves gas being expelled far from the galaxy and then falling back into the galactic disk. It plays a key role in regulating how new stars are formed. Earlier work in 2020 by Ferraro and his colleagues had already hinted at this extended feedback mechanism.



Graduate student Bernardita Ried Guachalla from Stanford University later confirmed the findings using a more nearby galaxy sample. Her work also revealed that the gas isn't evenly spread around galaxies but rather follows the "cosmic filaments"- long strands of matter that connect galaxies across the universe.



<h2 class="wp-block-heading" id="h-rethinking-our-universe-models">Rethinking our universe models</h2>



The findings suggest that galaxy evolution models need a serious upgrade. Simulations of how galaxies form and change over time often don’t account for this much gas being pushed so far out by central <a href="https://www.earth.com/news/black-holes-shaped-the-universe-before-galaxies-existed/" target="_blank" rel="noreferrer noopener">black holes</a>.



Some researchers are already adapting their models to better match this new evidence. The results also help clarify other long-standing puzzles in cosmology.



"Knowing where the gas is has become one of the most serious limiting factors in trying to get cosmology out of current and future surveys," Ferraro said. "We've kind of hit this wall, and this is the right time to address these questions." 



"Once you know where the gas is, you can ask, 'What's the consequence for cosmological problems?'"



For instance, some assumptions suggest that gas follows dark matter. But if large amounts of gas are being blown out of galaxies, that idea needs to be re-evaluated. If not corrected, this can lead to inaccuracies in cosmological calculations. Now, this research might help resolve those issues.



"There are a huge number of people interested in using our measurements to do a very thorough analysis that includes this gas," said Hadzhiyska. "People in astronomy care a lot about it for understanding galaxy formation and evolution."



<h2 class="wp-block-heading" id="h-from-missing-matter-to-cosmic-insights">From missing matter to cosmic insights</h2>



Beyond helping explain current galaxies, this approach may open a new window into the early universe. 



By using the same kinematic Sunyaev-Zel'dovich effect, scientists might be able to study large-scale structures that formed just after the Big Bang. It could even help test major theories about gravity and general relativity.



While there’s still work to be done, this research offers a promising step forward in answering some of cosmology’s biggest questions - starting with where half the universe’s matter has been hiding all along.



The full study was published in the journal <a href="https://arxiv.org/abs/2407.07152" target="_blank" rel="noreferrer noopener">arXiv</a>.



Image Credit: NASA/CXC/M.Weiss; NASA/CXC/Ohio State/A Gupta et al



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'Ghost gas' may solve the mystery of the universe’s missing matter

For decades, astronomers have searched for the universe’s missing matter...

Water on the Moon has long fascinated scientists, not just because it's crucial for future lunar missions, but also because it raises a big question: where did it come from? Since the 1960s, researchers have proposed that water might be forming thanks to the sun.



The idea is simple yet powerful: when charged particles from the Sun hit the Moon’s surface, they might spark a chemical reaction that produces water. That theory now has strong experimental support.



<h2 class="wp-block-heading" id="h-is-the-sun-creating-the-moon-s-water">Is the Sun creating the Moon's water?</h2>



Researchers at NASA's Goddard Space Flight Center and their collaborators have confirmed this process in the lab. They used one of the most realistic simulations of solar wind hitting <a href="https://www.earth.com/news/astronauts-will-melt-lunar-dust-to-build-roads-on-the-moon/" target="_blank" rel="noreferrer noopener">lunar dust</a> to date.



The findings could have a big impact on how NASA plans future missions, especially to the <a href="https://www.earth.com/news/two-spacecraft-set-out-to-drill-for-water-on-the-moons-south-pole/" target="_blank" rel="noreferrer noopener">Moon's South Pole</a> - where frozen water may lie in shadowed craters, a potential goldmine for exploration.



<blockquote class="wp-block-quote">
“The exciting thing here is that with only lunar soil and a basic ingredient from the Sun, which is always spitting out hydrogen, there’s a possibility of creating water. That’s incredible to think about," said Li Hsia Yeo, a research scientist at <a href="https://www.nasa.gov/goddard/" target="_blank" rel="noreferrer noopener">NASA's Goddard Space Flight Center in Greenbelt, Maryland</a> who led the study.
</blockquote>



<h2 class="wp-block-heading" id="h-solar-wind-and-water-formation">Solar wind and water formation</h2>



The Sun constantly blasts the solar system with a stream of particles called the solar wind. These particles travel at over one million miles per hour and are mostly made of hydrogen protons.



Earth has a magnetic field and an atmosphere that protect it from this bombardment, but the Moon doesn't. With no protection, its dusty surface - made of a gritty, rocky material called regolith - is fully exposed.



When solar wind protons hit this regolith, they can pick up electrons, becoming hydrogen atoms. These atoms then move through the lunar surface and bond with oxygen in minerals like silica. 



The result? Molecules of hydroxyl (OH) and, sometimes, actual <a href="https://www.earth.com/news/moons-entire-surface-is-covered-with-water-and-hydroxyl-not-just-the-poles/" target="_blank" rel="noreferrer noopener">water</a> (H₂O). Evidence of both hydroxyl and water has been found in the Moon’s uppermost surface - just a few millimeters deep.



Scientists detect these molecules through their chemical "fingerprint" using light analysis. But distinguishing between hydroxyl and water is tricky, so researchers often use “water” as a catch-all term.



<h2 class="wp-block-heading" id="h-the-moon-s-dynamic-water-signature">The Moon’s dynamic water signature </h2>



Previous spacecraft observations hinted that <a href="https://www.earth.com/news/silent-storms-experts-identify-the-mysterious-source-of-solar-wind/" target="_blank" rel="noreferrer noopener">solar wind</a> might be actively generating this water. One major clue is that the Moon’s water signature changes over the course of a day.



In some places, the signal is stronger in the cooler morning and weakens in the heat of the afternoon. Then it returns at night. This suggests the water isn't static - it’s dynamic, possibly being made and lost on a daily basis.



<h2 class="wp-block-heading" id="h-bringing-the-moon-to-the-lab">Bringing the Moon to the lab</h2>



To test the solar wind theory, Yeo and her colleague, Jason McLain, built a unique lab setup. It was the first of its kind to keep lunar samples sealed in a vacuum during testing - eliminating the risk of contamination from Earth’s moisture.



<blockquote class="wp-block-quote">
“It took a long time and many iterations to design the apparatus components and get them all to fit inside,” said McLain. “But it was worth it, because once we eliminated all possible sources of contamination, we learned that this decades-old idea about the solar wind turns out to be true.”
</blockquote>



The team used lunar dust from Apollo 17 - collected back in 1972 - and baked it to remove any trace water it might have picked up since. Then they bombarded the samples with high doses of mock solar wind using a tiny particle accelerator. This simulated about 80,000 years of lunar exposure.



<h2 class="wp-block-heading" id="h-detecting-a-molecular-signal">Detecting a molecular signal</h2>



To track changes, the researchers used a spectrometer - a tool that measures how light reflects off materials. They spotted a very specific dip in the light signal, right near the infrared wavelength where water usually absorbs energy. 



This dip is the telltale sign that something like water had formed. Although they can't say for sure whether it was hydroxyl or full water molecules, the signal strongly suggests both were produced. 



The results support the idea that the Sun plays a <a href="https://www.earth.com/news/experts-are-searching-for-viable-sources-of-water-on-the-moon/" target="_blank" rel="noreferrer noopener">major role</a> in forming water on the Moon through solar wind.



<h2 class="wp-block-heading" id="h-water-creation-by-the-sun">Water creation by the Sun</h2>



Understanding where and how water forms on the moon isn’t just a scientific curiosity. It could shape how future astronauts explore the lunar surface. 



If solar wind really is making water, even in tiny amounts, then lunar soil itself could become a resource - potentially useful for drinking water, breathable oxygen, or even rocket fuel.



And now, thanks to one carefully sealed chamber and a bit of lunar dust from the past, that possibility looks a lot more real.



The full study was published in the journal <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JE008334" target="_blank" rel="noreferrer noopener">Journal of Geophysical Research: Planets</a>.



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How the Sun might be making water on the Moon

Water on the Moon has long fascinated scientists, not just...

In a world shaped by virtual interactions, avatars are now the new face of communication. In games, work, shopping, or therapy, they act like real people - showing expressions and emotions, and even changing how we feel about taking risks.



But what happens when our brains start treating these digital stand-ins differently than real humans?



A study by Toshiko Tanaka and Masahiko Haruno of the National Institute of Information and Communications Technology (<a href="https://www.nict.go.jp/en/" target="_blank" rel="noreferrer noopener">NICT</a>) in Japan has brought this question into sharp focus.



The research explores how avatars influence <a href="https://www.earth.com/news/rethinking-vision-the-brain-sees-what-it-wants-to-see/" target="_blank" rel="noreferrer noopener">human behavior</a>, particularly when it comes to taking risks, and it offers a deeper look at the neural mechanics behind this shift.



<h2 class="wp-block-heading" id="h-more-risks-with-avatar-feedback">More risks with avatar feedback</h2>



Tanaka and Haruno designed a study that places human decision-making under the microscope in virtual environments. 



Participants engaged in a gambling task, where they had to choose between a guaranteed small reward and a risky option with a larger potential payout. Their choices were followed by dynamic facial feedback from either a real human face or an avatar presenting the same expressions.



What the researchers found was striking: people made more risky <a href="https://www.earth.com/news/your-brain-literally-changes-based-on-daily-activities-and-lifestyle/" target="_blank" rel="noreferrer noopener">choices</a> when they expected to receive feedback from an avatar rather than a real face. 



The difference was not subtle. It persisted across both behavioral and neuroimaging experiments, revealing that avatar interactions fundamentally altered the way people assessed the value of risk.



<h2 class="wp-block-heading" id="h-the-brain-s-reaction-to-avatars">The brain’s reaction to avatars</h2>



The answer lies in how our brain interprets uncertainty, especially in social situations. The researchers discovered that avatars shift our emotional processing of risk. 



Participants perceived facial feedback from avatars - be it admiring or contemptuous - as less emotionally charged than the same expressions from real humans. This led to a more favorable valuation of feedback uncertainty.



That means when participants weren’t quite sure what kind of response they’d receive, the ambiguity felt less threatening if it came from an avatar. This change in emotional <a href="https://www.earth.com/news/how-does-the-human-brain-create-retrieve-memories-engram-cells-connections/" target="_blank" rel="noreferrer noopener">processing</a> allowed them to focus more on potential gains, encouraging riskier choices.



<h2 class="wp-block-heading" id="h-quieting-the-brain-s-emotional-alarm">Quieting the brain’s emotional alarm</h2>



To understand the brain’s role in this behavior, the researchers used functional magnetic resonance imaging (fMRI) scans. 



The experts found that a key emotional processing center in the brain - the amygdala - was deeply involved. Specifically, activity in the central amygdala (CM) decreased when feedback uncertainty was delivered through avatars.



This reduction in amygdala response reflected a lower emotional cost attached to avatar feedback. In essence, avatars made the stakes feel lower, even when the actual risk remained the same. 



This neural response was not random. It tracked closely with how individuals evaluated feedback uncertainty and how often they chose the risky option.



<h2 class="wp-block-heading" id="h-empathetic-people-are-more-affected">Empathetic people are more affected</h2>



Not everyone responded the same way to avatar feedback. The researchers included psychological assessments that measured traits like empathy and anxiety. 



They found that people who scored high on empathetic concern - those more emotionally attuned to others - were especially likely to show reduced amygdala responses and increased risk-taking in the avatar condition.



The central amygdala response to feedback uncertainty also correlated specifically with these empathy scores. It wasn’t general anxiety or social avoidance that shaped the brain’s behavior - it was the emotional consideration of others’ internal states.



According to the study, this pattern was not observed in participants with higher scores for social anxiety. That distinction suggests that avatars reduce emotional burden without diminishing the social component of the interaction.



<h2 class="wp-block-heading" id="h-other-brain-areas-that-responded">Other brain areas that responded</h2>



Though the amygdala played the primary role, other brain regions also responded. The ventral striatum (vSTR) and ventral anterior cingulate cortex (vACC) showed activity linked to feedback uncertainty, though their involvement was less direct. 



These areas processed reward-related and emotional information, but they didn’t show the same predictive power as the amygdala when it came to actual behavior changes.



Participants who took more risks with avatars had amygdala activity patterns that clearly differed from those who remained cautious. The vSTR and vACC supported these shifts but did not appear to drive them.



<h2 class="wp-block-heading" id="h-how-avatar-influence-was-measured">How avatar influence was measured </h2>



The strength of these conclusions rests in a meticulous experimental design. Participants interacted with a same-gender observer whom they believed was monitoring and evaluating their gambling behavior.



Unbeknownst to them, feedback expressions were pre-recorded, and observer appearances alternated between avatar and real-face conditions.



Each trial in the experiment involved choosing between a safe and risky option, followed by feedback in the form of facial expressions. The researchers recorded behavioral data and brain activity, allowing them to model the valuation process mathematically and neurologically.



Computational modeling confirmed that feedback uncertainty carried more weight in decision-making under avatar conditions. The best-fitting models showed that only this parameter needed to vary between avatar and human feedback to explain participants' risk behavior.



<h2 class="wp-block-heading" id="h-tests-confirm-risk-taking-boost">Tests confirm risk-taking boost</h2>



To ensure their findings were not due to a simple lack of <a href="https://www.earth.com/news/digital-misinformation-rumors-spread-like-nuclear-reactions/" target="_blank" rel="noreferrer noopener">engagement</a>, the team ran pilot tests. These included a no-observer condition, in which participants received no feedback at all. 



Risk-taking rates in this condition were significantly lower than those seen with avatar feedback. This helped eliminate the possibility that participants were simply ignoring avatar responses.



Even when compared to human feedback, avatars elicited more risk-taking. This demonstrated that it wasn’t just the presence of feedback but the form of the feedback that mattered.



<h2 class="wp-block-heading" id="h-real-world-implications">Real-world implications</h2>



“We found that people tend to take more risks when their partner responds through an avatar rather than showing their real face. This seems to be driven by a change in how they process uncertainty - and interestingly, that change is reflected in the amygdala," said Haruno.



“Using the same confederate and having them pass as just another participant every time wasn’t easy - it took a lot of effort to keep things feeling real for each new person,” added Tanaka.



These findings extend far beyond the lab. In virtual workspaces, therapy sessions, and customer service interactions, avatars may unintentionally nudge users toward riskier behavior. This could be a double-edged sword - boosting confidence in some cases while increasing impulsivity in others.



<h2 class="wp-block-heading" id="h-next-steps-in-avatar-research">Next steps in avatar research</h2>



Future investigations will likely explore how avatar characteristics - age, gender, realism - affect user responses.



Researchers are also interested in whether these findings apply to other kinds of decision-making, such as moral choices or long-term planning.



The study suggests that more human-like avatars could deepen emotional engagement, potentially altering the balance between empathy and risk even further. As avatar technology becomes more lifelike and widespread, these questions will become increasingly important.



<h2 class="wp-block-heading" id="h-new-era-of-virtual-world-risk">New era of virtual world risk</h2>



Tanaka and Haruno’s study offers a timely look at how digital interactions shape human behavior. By revealing that avatars influence our emotional evaluation of uncertainty, they uncover a hidden driver of risk in the virtual world.



The amygdala, a structure tied to emotional memory and fear, emerges as a key player in how we navigate the unfamiliar terrain of avatar communication. 



As we spend more time in these environments, we must learn how these subtle shifts in perception can shape the choices we make - online and off.



The study is published in the journal <a href="https://journals.plos.org/plosbiology/article?id=10.1371/journal.pbio.3003122" target="_blank" rel="noreferrer noopener">PLOS Biology</a>.



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How avatars are making people take more risks

In a world shaped by virtual interactions, avatars are now...

Ask any parent of a teenager, and they will confirm that young people rarely go to bed early. Smartphones glow into the night, homework drags past midnight, and weekend sleep-ins feel like catch-up sessions rather than luxury.&nbsp;



Yet a large international study led by researchers at the <a href="https://www.cam.ac.uk/" target="_blank" rel="noreferrer noopener">University of Cambridge</a> and <a href="https://www.fudan.edu.cn/en/" target="_blank" rel="noreferrer noopener">Fudan University</a> suggests that even small shifts toward longer, earlier sleep may deliver measurable benefits for adolescents’ brains.



<h2 class="wp-block-heading" id="h-sleep-patterns-and-adolescent-brains">Sleep patterns and adolescent brains </h2>



The investigation is one of the most comprehensive attempts to link real-world <a href="https://www.earth.com/news/sleep-quality-could-be-the-key-to-better-metabolic-health/" target="_blank" rel="noreferrer noopener">sleep patterns</a> with brain imaging and cognitive testing in early adolescence. 



Drawing on data from the <a href="https://abcdstudy.org/" target="_blank" rel="noreferrer noopener">Adolescent Brain Cognitive Development (ABCD) Study</a> in the United States, the research tracked nightly rest in more than 3,200 children aged 11–12 by using Fitbit wearables rather than relying on self-reported bedtimes. The scientists then compared those objective sleep metrics with MRI scans, heart-rate data, and a battery of tasks that measure attention, vocabulary, <a href="https://www.earth.com/news/sleep-rewires-the-brain-to-strengthen-memories/" target="_blank" rel="noreferrer noopener">memory</a>, and reasoning.



“Regularly getting a good night’s sleep is important in helping us function properly, but while we know a lot about sleep in adulthood and later life, we know surprisingly little about sleep in adolescence, even though this is a crucial time in our development,” said Professor Barbara Sahakian of Cambridge’s Department of Psychiatry, one of the senior authors.&nbsp;



“How long do young people sleep for, for example, and what impact does this have on their brain function and cognitive performance?”



<h2 class="wp-block-heading" id="h-three-distinct-sleep-profiles">Three distinct sleep profiles</h2>



When the team clustered the teenagers’ nightly patterns, three broad groups emerged.&nbsp;



The first group, labeled "late-to-bed, early-to-rise sleepers," made up about 39 percent of the sample. These adolescents started their slumber the latest and woke the earliest, averaging just seven hours and ten minutes of sleep - the least rest of all.&nbsp;



The second group, comprising just under a quarter of the participants, were considered "average sleepers." They managed roughly seven hours and twenty-one minutes, with bedtimes, wake times, and sleep efficiency all falling in the mid-range.&nbsp;



The final group, the "early-to-bed sleepers," accounted for the remaining 37 percent. These teens consistently shut down earlier in the evening and clocked in at about seven hours and twenty-five minutes of sleep. Notably, they exhibited the lowest overnight <a href="https://www.earth.com/news/sleeping-more-on-weekends-can-reduce-heart-disease-risk/" target="_blank" rel="noreferrer noopener">heart</a> rates - a well-known marker of deeper, more restorative sleep.



At first glance, the difference between the most-rested and least-rested teens seems negligible: barely fifteen minutes. Yet those extra minutes translated into meaningful neurological and cognitive distinctions.



<h2 class="wp-block-heading" id="h-adolescent-brains-built-on-sleep">Adolescent brains built on sleep</h2>



MRI scans revealed that Group Three, the earliest and longest sleepers, possessed the greatest overall brain volume and showed healthier patterns of functional connectivity - the way distinct neural hubs communicate. Group One, in contrast, had the smallest volumes and weakest functional links.



Cognitive testing echoed the brain-imaging results. In tasks involving reading comprehension, vocabulary recognition, sustained <a href="https://www.earth.com/news/our-brain-stops-paying-attention-to-repeated-distractions/" target="_blank" rel="noreferrer noopener">attention</a>, and problem-solving speed, Group Three consistently outperformed Group Two, which in turn outperformed Group One.&nbsp;



No significant gaps appeared in standard school grades, perhaps because grades involve numerous external factors such as teacher support or parental involvement. Nevertheless, the neuro-cognitive edge associated with slightly better sleep was unmistakable.



“Even though the differences in the amount of sleep that each group got was relatively small, at just over a quarter-of-an-hour between the best and worst sleepers, we could still see differences in brain structure and activity and in how well they did at tasks,” Sahakian noted. “This drives home to us just how important it is to have a good night’s sleep at this important time in life.”



<h2 class="wp-block-heading" id="h-reinforcing-the-link-over-time">Reinforcing the link over time</h2>



Because the ABCD project is longitudinal, following participants for a decade or more, the team could examine sleep and brain metrics two years earlier and two years later for overlapping subsets of youths.&nbsp;



The researchers discovered that sleep habits and associated cognitive advantages or disadvantages tended to persist. Children who were short sleepers at nine and ten were likely still short sleepers at thirteen and fourteen. Likewise, the adolescents' relative brain volumes and task scores stayed aligned with sleep duration.



First author Qing Ma of Fudan University emphasized that the study cannot prove unequivocally that longer sleep causes enhanced cognition, but it dovetails with a broad literature.



“Although our study can’t answer conclusively whether young people have better brain function and perform better at tests because they sleep better, there are a number of studies that would support this idea,” Ma said.&nbsp;



“For example, research has shown the benefits of sleep on memory, especially on memory consolidation, which is important for learning.”



<h2 class="wp-block-heading" id="h-why-aren-t-teens-sleeping-enough">Why aren’t teens sleeping enough?</h2>



Despite the brighter outlook for early-to-bed sleepers, none of the groups met the <a href="https://aasm.org/" target="_blank" rel="noreferrer noopener">American Academy of Sleep Medicine</a>’s recommendation that adolescents log eight to ten hours nightly. On average the entire sample fell short by at least forty-five minutes, highlighting a systemic sleep deficit.



Senior author Wei Cheng of Fudan University believes the next challenge is diagnosing the reasons. 



“Given the importance of sleep, we now need to look at why some children go to bed later and sleep less than others. Is it because of playing videogames or smartphones, for example, or is [it] just that their body clocks do not tell them it’s time to sleep until later?”



Biological shifts during puberty cause a natural delay in <a href="https://www.earth.com/news/colors-of-sunset-and-sunrise-reset-our-circadian-rhythms/" target="_blank" rel="noreferrer noopener">circadian rhythm</a> - essentially rewiring teens to feel sleepy later - but social factors exacerbate the problem. Homework loads, extracurricular activities, social media, and screen glare all encroach on bedtime.&nbsp;



Some school districts have responded by pushing start times later, aligning schedules more closely with adolescent biology. Evidence from this large-scale study lends weight to such policy interventions and to household rules that prioritize sleep hygiene.



<h2 class="wp-block-heading" id="h-small-changes-lasting-gains">Small changes, lasting gains</h2>



While eight to ten hours may remain a lofty goal, the study indicates that trimming bedtimes even by fifteen or twenty minutes could yield tangible brain benefits.&nbsp;



Modest shifts toward earlier lights-out routines, consistent wake-up times, and device curfews might help teens move from the most deprived category to the middle or top tier.



Ma, Sahakian, Cheng, and colleagues plan further analyses as the ABCD Study matures, including investigations into emotional regulation, mental-health trajectories, and risk-taking behavior.&nbsp;



For now, their findings deliver a clear message to parents, educators, and policymakers alike: sleep matters - not just by the hour but by the minute - and adolescence is no time to skimp on it.



The study is published in the journal <a href="https://www.cell.com/cell-reports/fulltext/S2211-1247(25)00336-5" target="_blank" rel="noreferrer noopener">Cell Reports</a>.



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Sleeping smarter: Just 15 extra minutes can boost adolescent brains

Ask any parent of a teenager, and they will confirm...

Strolling a familiar beach and stumbling upon a relic from the age of dinosaurs sounds like pure fantasy, yet that is exactly what happened on England’s west coast. 



A stretch of shoreline below Somerset’s crumbling cliffs yielded a bone so large that it challenged everything we thought we knew about prehistoric marine reptiles. 



The fossil - a lower jaw more than 6½ feet long - promised a creature leagues beyond anything alive today. The find dated to around 202 million years ago, slotting it into the turbulent final chapter of the <a href="https://www.earth.com/news/triassic-fossils-shed-new-light-on-ancient-ecosystems/" target="_blank" rel="noreferrer noopener">Triassic Period</a>.



At that time, much of what is now Britain lay beneath a warm, shallow sea patrolled by meat‑eating giants. Their reign ended in a mass extinction, leaving only scattered bones to whisper their stories - until now.



<h2 class="wp-block-heading" id="h-ruby-and-ichthyotitan-severnensis">Ruby and Ichthyotitan severnensis</h2>



Back in late&nbsp;May&nbsp;2020, 11‑year‑old Ruby&nbsp;Reynolds and her father, Justin, headed for the mudflats of Blue&nbsp;Anchor, looking for fossils. 



Justin spotted a four‑inch scrap of bone, “bigger than any piece of bone I'd ever found before,” he recalls. 



Ruby wandered on and unearthed a second fragment twice that size. “It was just sort of lying there,” she says. “I was just happy, really.” Their excitement would soon ripple far beyond the shoreline.



Word reached paleontologist Dean&nbsp;Lomax, who holds posts at both the <a href="https://www.bristol.ac.uk/" target="_blank" rel="noreferrer noopener">University of Bristol</a> and the <a href="https://www.manchester.ac.uk/" target="_blank" rel="noreferrer noopener">University of Manchester</a>. He recognized echoes of another Somerset specimen lifted in&nbsp;2016 by local collector Paul&nbsp;de&nbsp;la&nbsp;Salle. 



That earlier jaw fragment, called a surangular, came together from several chunks that, Lomax remembers, “fit together perfectly like an ancient prehistoric jigsaw puzzle.”



Ruby's discovery was eventually named Ichthyotitan severnensis, which literally translates to “giant fish lizard from the Severn.” 



<h2 class="wp-block-heading" id="h-ichthyotitan-severnensis-was-a-true-monster">Ichthyotitan severnensis was a true monster</h2>



The first bone’s eroded edges left scientists yearning for more. “It suggests that it was from something unusual and exceedingly large,”&nbsp;Lomax says. 



He and colleagues published a cautious description, but could not pin down the creature’s identity. “What we'd hoped for - we kept our fingers crossed - we hoped that maybe more specimens would come to light in the future,” he admits.



Ruby and Justin’s beachside haul delivered exactly that. After they emailed photographs - “Hey, Dr.&nbsp;Lomax - we think we've found another one of your giant ichthyosaur jawbones”&nbsp;-&nbsp;the research team raced to Somerset. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/Ichthyotitan-severnensis_largest-marine-reptile_jawbone-comparison_credit-Dean-Lomax_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/Ichthyotitan-severnensis_largest-marine-reptile_jawbone-comparison_credit-Dean-Lomax_1s.webp" alt="Photograph of the nearly complete giant jawbone, along with a comparison with the 2018 bone (middle and bottom) found by Paul de la Salle. Credit: Dr. Dean Lomax" class="wp-image-1966376"/></a><figcaption class="wp-element-caption">Photograph of the nearly complete giant jawbone, along with a comparison with the 2018 bone (middle and bottom) found by Paul de la Salle. Click image to enlarge. Credit: Dr. Dean Lomax</figcaption></figure>



“Of course, they were quite right,” Lomax says. “They correctly identified these sections of bone as belonging to an ichthyosaur.” 



Fresh collecting trips recovered still more pieces, leaving nearly two‑thirds of the jaw intact and in excellent shape.



<h2 class="wp-block-heading" id="h-matching-two-huge-jawbones">Matching two huge jawbones</h2>



Comparison of the two Somerset jaws revealed striking similarities. Because both turned up in the same rock layer and displayed uncommon internal bone textures, the team concluded they belonged to one new species. 



In a paper published in PLOS&nbsp;ONE, they proposed that the full animal stretched roughly&nbsp;82&nbsp;feet - “genuinely enormous, about the length of a blue whale,” Lomax says.



Scale alone does not grant a place in the record books; scientists also scrutinized microscopic structures inside the bone. 



These matched the odd pattern seen in other <a href="https://www.earth.com/news/fiona-the-ichthyosaur-was-preserved-for-millions-of-years-after-a-landslide/" target="_blank" rel="noreferrer noopener">super‑sized ichthyosaurs</a>, nudging researchers to suggest these reptiles grew in a way unlike most of their scaly kin.



Whether Ichthyotitan severnensis belonged to the shastasaur group - the clade that once produced Triassic leviathans across the globe - remains uncertain until a complete skeleton surfaces.



<h2 class="wp-block-heading" id="h-sizing-up-ichthyotitan">Sizing up Ichthyotitan</h2>



The Somerset titan likely carried a lighter, more streamlined frame suited for open‑ocean cruising. Its jawbone alone outsizes a grown person by several feet. 



If its proportions followed relatives such as Shonisaurus, the skull may have spanned over&nbsp;10&nbsp;feet, with paddle‑shaped flippers stretching wider than a living‑room couch.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/Ichthyotitan-severnensis_largest-marine-reptile_illustration_credit-Gabriel-Ugueto_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/Ichthyotitan-severnensis_largest-marine-reptile_illustration_credit-Gabriel-Ugueto_1s.webp" alt="A giant pair of swimming Ichthyotitan severnensis. Credit: Gabriel Ugueto" class="wp-image-1966374"/></a><figcaption class="wp-element-caption">A giant pair of swimming Ichthyotitan severnensis. Click image to enlarge. Credit: Gabriel Ugueto</figcaption></figure>



Growth to such dimensions suggests a sea rich in food and free of bigger predators. Massive schools of squid‑like cephalopods thrived in Triassic waters, offering a banquet to long‑roaming hunters. 



Stable‑isotope evidence from other ichthyosaur bones hints at warm‑blooded metabolisms, which, paired with live birth and sleek bodies, let them fill whale‑like niches long before mammals took the plunge.



<h2 class="wp-block-heading" id="h-life-in-the-triassic-was-incredible">Life in the Triassic was incredible</h2>



The Triassic often flies under the radar next to the Jurassic’s celebrity dinosaurs, yet biomechanist Kelsey&nbsp;Stilson calls it “a really weird time.” 



Continents had only just fused into <a href="https://www.earth.com/earthpedia-articles/supercontinents-101-pannotia-gondwana-and-pangea/" target="_blank" rel="noreferrer noopener">Pangaea</a>, monsoon‑driven climates swung from drought to deluge, and both early dinosaurs and mammals were fresh on the scene. 



“There were things that we can't even possibly imagine in the past,”&nbsp;Stilson adds. “But we can get little hints, and this is one little hint at this larger picture of evolution on Earth.”



That broader picture shows ichthyosaurs rising fast after the end‑Permian mass extinction, then peaking in size just before the next cataclysm. 



“No marine reptile ever reached such gigantic sizes ever again,”&nbsp;Lomax notes. Later Jurassic and Cretaceous ichthyosaurs shrank, perhaps pushed aside by changing oceans and by the emergence of other reptilian predators such as <a href="https://www.earth.com/news/dinosaurs-were-not-the-only-animals-that-grew-fast-during-the-mesozoic/" target="_blank" rel="noreferrer noopener">pliosaurs</a> and <a href="https://www.earth.com/news/mosasaurs-had-fierce-survival-strategies-including-cannibalism/" target="_blank" rel="noreferrer noopener">mosasaurs</a>.



<h2 class="wp-block-heading" id="h-whales-replaced-ichthyotitan-severnensis">Whales replaced Ichthyotitan severnensis</h2>



The last ichthyosaurs disappeared about&nbsp;94&nbsp;million&nbsp;years ago, vacating the top spot in marine food webs. 



That gap lingered until hoofed mammals ventured back to sea some&nbsp;50&nbsp;million&nbsp;years ago, setting whales on their own path to titanic proportions. 



The repeat story - big fish‑shaped predators evolving from land‑going ancestors - highlights how evolutionary solutions recur when similar ecological opportunities arise.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/Ichthyotitan-severnensis_largest-marine-reptile_beached_credit-Sergey-Krasovskiy_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/Ichthyotitan-severnensis_largest-marine-reptile_beached_credit-Sergey-Krasovskiy_1s.webp" alt="A washed-up Ichthyotitan severnensis carcass on the beach. Credit: Sergey Krasovskiy." class="wp-image-1966372"/></a><figcaption class="wp-element-caption">A washed-up Ichthyotitan severnensis carcass on the beach. Click image to enlarge. Credit: Sergey Krasovskiy.</figcaption></figure>



Modern blue whales now stretch beyond&nbsp;100&nbsp;feet and can weigh&nbsp;180&nbsp;tons, yet, length for length, they share the open ocean’s realm with Ichthyotitan in the fossil archives. 



Their stories highlight the ocean’s capacity to <a href="https://www.earth.com/news/trachelosaurus-fischeri-worlds-oldest-long-necked-marine-reptile-rediscovered/" target="_blank" rel="noreferrer noopener">nurture behemoths</a> when food is ample and competition sparse.



<h2 class="wp-block-heading" id="h-what-happens-next">What happens next?</h2>



Somerset’s cliffs erode a little more each winter. Storms tear at ancient mudstones, exposing new fossils overnight. 



“This research has been ongoing for almost eight years. It is quite remarkable to think that gigantic, blue whale‑sized ichthyosaurs were swimming in the oceans around what was the UK during the Triassic Period," Lomax concluded.



"These jawbones provide tantalizing evidence that perhaps one day a complete skull or skeleton of one of these giants might be found. You never know.”



Beachcombers like Ruby and Justin now scan those shores with renewed purpose. Their lucky strike reminds us that scientific breakthroughs sometimes hide in plain sight, waiting for curious eyes and a little persistence. 



The sea claimed Ichthyotitan severnensis long before humans walked Europe, yet its story shows that even after millions of years, a coast‑side ramble can rewrite natural history.



The full study was published in the journal <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0300289" target="_blank" rel="noreferrer noopener">PLOS ONE</a>.



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Largest marine reptile ever known to exist was discovered by an 11-year-old girl

Strolling a familiar beach and stumbling upon a relic from...

Antarctica’s winter sea ice usually forms a bright lid over millions of square miles. So when a massive, black patch was spotted by NASA scientists for the first time, satellite operators were taken aback, to say the least.



Then roughly a year later, the situation got even stranger. The gap, called a polynya, swelled to the size of Switzerland and stayed open for weeks.



Only after it refroze did researchers start piecing together how such an enormous opening in the ice could appear hundreds of miles from the nearest shoreline - right above a submerged plateau named Maud Rise.



<h2 class="wp-block-heading" id="h-understanding-polynyas-the-basics">Understanding polynyas - the basics</h2>



<a href="https://www.earth.com/news/carbon-storage-mystery-emerges-in-the-southern-ocean/" target="_blank" rel="noreferrer noopener">The Southern Ocean</a> is normally a layer cake. A thin cap of cold, relatively fresh water floats over saltier, warmer layers, and that slight density difference keeps the column from churning. 



A mid‑ocean polynya needs the cake to collapse. Salt must slip into the surface, make the top layer heavier, and flip the stack. 



Once that happens, convection kicks in, the lid fractures, heat pours skyward, and the ocean “breathes” gases.



Coastal versions manage something similar each year because fierce winds shove ice away from land. Out on the high seas, though, the phenomenon is much less common.



<a href="https://en.wikipedia.org/wiki/Maud_Rise" target="_blank" rel="noreferrer noopener">Maud Rise</a>, a 4,600‑foot‑tall seamount, may provide the missing ingredient by diverting currents and trapping water in tight spirals.



<h2 class="wp-block-heading" id="h-stubborn-patch-over-maud-rise">Stubborn patch over Maud Rise</h2>



History backs that hunch. Between 1974 and 1976, a much larger hole lingered over Maud Rise each winter. 



The Maud Rise polynya was discovered in the 1970s, when remote‑sensing satellites capable of observing <a href="https://www.earth.com/news/rapid-antarctic-sea-ice-loss-is-causing-severe-storms-around-the-world/" target="_blank" rel="noreferrer noopener">sea ice</a> over the Southern Ocean were first launched. 



It persisted through consecutive winters from 1974 to 1976, and oceanographers at the time assumed it would become an annual occurrence. But since the 1970s, it has occurred only sporadically and for brief intervals.



<figure class="wp-block-image aligncenter size-full is-resized"><a href="https://www.earth.com/wp-content/uploads/2025/04/antarctica_sea-ice-hole_Maud-Rise-polynya_switzerland-size_blue-ice_credit-NASA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/antarctica_sea-ice-hole_Maud-Rise-polynya_switzerland-size_blue-ice_credit-NASA_1s.webp" alt="An arial view of the Maud Rise polynya. Scientists were baffled as to how this formed but now have an explanation. Credit: NASA Earth Observatory" class="wp-image-1966649" style="width:300px;height:auto"/></a><figcaption class="wp-element-caption">An arial view of the Maud Rise polynya. Scientists were baffled as to how this formed but now have an explanation. Click image to enlarge. Credit: NASA Earth Observatory</figcaption></figure>



“2017 was the first time that we've had such a large and long‑lived polynya in the Weddell Sea since the 1970s,” said Aditya Narayanan of the <a href="https://www.southampton.ac.uk/" target="_blank" rel="noreferrer noopener">University of Southampton</a>, lead author of the study in Science Advances. 



He joined colleagues to probe the comeback with robotic floats, tagged elephant seals, and a high‑resolution <a href="https://www.earth.com/news/shrinking-sea-ice-what-record-lows-tell-us-about-the-future/" target="_blank" rel="noreferrer noopener">ocean model</a>.



<h2 class="wp-block-heading" id="h-salt-storms-and-a-hidden-conveyor">Salt, storms, and a hidden conveyor</h2>



During those winters, the clockwise Weddell Gyre sped up. That spin drew a deep layer of warm, salty water nearer the surface, softening ice from below. Yet the meltwater should have freshened the lid and shut down mixing.



"This upwelling helps to explain how the sea ice might melt. But as sea ice melts this leads to a freshening of the surface water, which should in turn put a stop to the mixing," explained Fabien Roquet, a Professor in Physical Oceanography at the <a href="https://www.gu.se/en" target="_blank" rel="noreferrer noopener">University of Gothenburg</a> and co-author of the research. 



"So, another process must be happening for the polynya to persist. There must be an additional input of salt from somewhere."



Roaring extratropical storms supplied part of that punch. Their swirling winds flung sea ice outward and dragged briny water toward Maud Rise. 



Atmospheric rivers - plumes of moist air stretching a thousand miles - added warmth from above, helping strip away stratification.



<h2 class="wp-block-heading" id="h-ekman-transport-as-the-missing-shove">"Ekman transport" as the missing shove</h2>



A final push came from physics first described a century ago. When wind blows across the ocean, Earth’s rotation deflects the surface flow roughly 90 degrees, a process called <a href="https://oceanservice.noaa.gov/education/tutorial_currents/04currents4.html" target="_blank" rel="noreferrer noopener">Ekman transport</a>. 



The model showed this flow steering salt‑laden water onto the northern flank of Maud Rise, exactly where the 2017 hole opened. 



“Ekman transport was the essential missing ingredient that was necessary to increase the balance of salt and sustain the mixing of salt and heat towards the surface water,” said co‑author Alberto Naveira Garabato, also from the University of Southampton.



The storms didn’t just move ice; they herded the right water into the right spot, letting convection roar. By late September, the opening had vented more than twenty times the heat that normally seeps through unbroken ice before finally freezing again.



<h2 class="wp-block-heading" id="h-polynyas-have-a-global-impact">Polynyas have a global impact</h2>



A hole in the <a href="https://www.earth.com/news/southern-ocean-absorbs-more-co2-than-previously-thought/" target="_blank" rel="noreferrer noopener">Southern Ocean</a> sea ice may look local, yet its fingerprints show up far away. 



“The imprint of polynyas can remain in the water for multiple years after they've formed," noted Professor Sarah Gille from University of California San Diego (<a href="https://www.ucsd.edu" target="_blank" rel="noreferrer noopener">UCSD</a>), another co-author of the research



"They can change how water moves around and how currents carry heat toward the continent. The dense waters that form here can spread across the global ocean.” 



Deep convection hauls carbon‑rich water upward, where it can release CO₂, and sends newly formed, oxygen‑rich brine sliding along the seafloor.



<h2 class="wp-block-heading" id="h-what-happens-next">What happens next?</h2>



That heavy brine eventually feeds the global conveyor belt of currents that helps regulate climate. Because the Maud&nbsp;Rise mechanism hinges on a stronger gyre and stormier skies, its future frequency could ride on winds already shifting as the planet warms.



“For the first time since observations began in the 1970s, there's a <a href="https://www.earth.com/news/record-low-antarctic-sea-ice-and-rapid-melting-pace-stuns-climate-scientists/" target="_blank" rel="noreferrer noopener">negative trend in sea ice</a> in the Southern Ocean, which began around 2016. Before then, it had remained somewhat stable," Professor Gille concluded.



The same rise of warm, salty water that primed the 2017 hole now seems to be thinning ice across Antarctica’s fringe.



Scientists will watch the next few winters closely. Whether the polynya returns or not, its story shows that the frozen edge of the world can still spring surprises - and that what happens far south seldom stays there, for the wider planet.



The full study was published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adj0777" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Massive hole the size of Switzerland appeared in the Antarctica sea ice, now we know why

Antarctica’s winter sea ice usually forms a bright lid over...

Scientists are transforming chocolate into a functional food by infusing it with probiotics and prebiotics, aiming to create a treat that satisfies cravings while supporting gut health. 



The challenge lies in maintaining chocolate's beloved texture and flavor while adding health benefits.



<figure class="wp-block-embed aligncenter is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio"><div class="wp-block-embed__wrapper">
https://youtu.be/Ug657J67iEo?si=w96YjGMsg939LD_3
</div></figure>



Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



Prebiotics act as food for these microbes, helping them thrive. Together, they form "synbiotics," a powerful health combination.



Researchers Smriti Gaur and Shubhi Singh from India's Jaypee Institute of Information Technology took an innovative approach, using natural prebiotics like corn and honey instead of complex processing methods. 



They created five chocolate varieties: a control and four synbiotic versions containing different combinations of prebiotics, probiotics (Lactobacillus strains), and flavor enhancers (cinnamon or orange).



Laboratory simulations of human digestion showed the probiotics remained viable for over five hours, suggesting they could survive long enough to benefit gut health.



Taste tests were positive, with researchers particularly enjoying the orange-flavored variety, describing it as having "vibrant citrus notes" complementing the "rich cocoa" with a "luxurious" texture.



This research represents just the beginning. With further refinement of strains, textures, and flavors, chocolate could evolve beyond mere indulgence to become a functional food that nourishes while it delights.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acsfoodscitech.4c00741" target="_blank" rel="noreferrer noopener">ACS Food Science &amp; Technology</a>.

Is chocolate the next nutritional powerhouse?

Scientists are transforming chocolate into a functional food by infusing...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Nushagak Bay, a large estuary in southwest Alaska. Nushagak runs mainly north to south and exits in Bristol Bay, a large body of water in the Bering Sea.



"The bay is primarily fed by the Nushagak River, which begins in the Alaska Range and flows southwest approximately 450 km. The bay is also fed by several additional rivers including the Wood, Igushik, Snake and Weary rivers," says ESA.



"The dark colors of the Nushagak River are most likely due to tannins or lignins (chemical substances found in plants). Tannins and lignins from roots, leaves, seeds, bark and soil can leach into the water and give it a brown or even black colour. The sediments then flow southwards where it is mixed with the bluer waters of the bay."



Video/ Image Credit: ESA



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Nushagak Bay in southwest Alaska

[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"] Today’s Video of the Day from the...

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> (ACS) reveals that proteins on flu viruses are actually flexible, tilting and waving in a “breath-like” motion. According to the experts, these proteins could be used to better defend against the flu.



"The main antigenic targets of influenza virus are two surface glycoproteins, hemagglutinin (HA) and neuraminidase (NA). Whereas the structural and dynamical properties of both glycoproteins have been studied previously, the understanding of their plasticity in the whole-virion context is fragmented," wrote the researchers.



To investigate, the team conducted detailed simulations of the influenza A H1N1 virion, or the swine flu. The experts concluded that the visualizations show many new vulnerable states of flu viruses, which could improve future vaccines and antiviral drugs.



Video/ Image Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Flu viruses are more flexible than expected

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Lake Trasimeno, which is located west of Perugia in central Italy. It is the fourth largest lake in the country. While Trasimeno’s water level varies, it has a maximum depth of approximately six meters.&nbsp;



"In this Copernicus Sentinel-2 image, captured on 6 August 2022, the lake’s emerald green colour is likely due to the presence of phytoplankton. Streaks in the water, particularly visible in the west, indicate the presence of soil and sediments which have been stirred up by winds. Dark colored waters in the southern part of the lake indicate a presence of submerged and floating macrophytes (aquatic plants) as well as algae," says ESA.



"Surrounded by hills on three sides, Trasimeno is subject to heavy storms created by winds, especially from the north and west. There are three islets in the lake: Maggiore, Minore and Polvese (the largest). The lake’s shores are sparsely inhabited with only two popular villages: Castiglione del Lago and Passignano sul Trasimeno."



"Italy is experiencing its worst drought in 70 years which has affected drinking water supplies, hydroelectric power and agricultural production. High temperatures, hot winds and lack of rainfall are the main causes of drought in the Umbrian region which saw Lake Trasimeno’s drop 1.3 m, reaching the limit of the hydrometric zero in July 2022."



Video/Image Credit: ESA&nbsp;



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Lake Trasimeno in Central Italy

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> describes a new self-powered nanosensor that can instantly detect mercury contamination with the tap of a finger.&nbsp;



The oxidized form of mercury can be harmful when it is ingested through contaminated water or food. This makes it necessary for experts to develop sensors that can quickly and accurately detect the presence of mercury.&nbsp;



Zong-Hong Lin and colleagues have now created a triboelectric nanosensor (TENS) that can detect mercury by simply by touching a sample. According to the researchers, their TENS could serve as the basis for similar devices to safely and remotely monitor other pollutants.



Video Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Detecting mercury contamination with the tap of a finger

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Kainji Lake, a reservoir on the Niger River.



In 1968, Kainji Lake was created by the construction of the Kainji Dam. The Niger River, the third longest in Africa, enters the lake in the north.&nbsp;



According to <a href="https://www.earth.com/news/rivers-in-the-american-west-are-a-lifesaving-resource-for-birds/">ESA</a>, the creation of the lake submerged Foge Island and the town of Bussa and permanently flooded other riverine settlements, leaving around 50,000 people displaced.&nbsp;



Large parts of Foge Island are temporarily exposed during low water tides, and the land is often used by migrating fishermen. Kainji Dam is a dam across the Niger River in Niger State of Central Nigeria. 



Wild mammals occur at relatively low densities due to illegal hunting. Lake Kainji has suffered a dramatic decline as a fishery due to the high numbers of artisanal and subsistence fisherfolk using the lake. It has been suggested that a period of closure, together with controlled fishing rights may help improve fish stocks.



Kainji Lake National Park is the oldest of its kind in Nigeria. The park contains three distinct areas: a part of the Kainji Lake, the Borgu Game Reserve to the west of the lake, and the Zugurma Game Reserve to the southeast. The park is home to around 65 mammal species, 350 bird species, and 30 species of reptiles and amphibians. 



Video/ Image Credit: European Space Agency&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Kainji Lake in north central Nigeria

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