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...

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 the European Space Agency...

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...

Today's Image of the Day from the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba about 43 million light-years away from Earth.&nbsp;



This galaxy, discovered by British astronomer James Dunlop in 1826, is part of the larger NGC 1808 group of galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-intimate-view-of-ngc-1792">Intimate view of NGC 1792</h2>



“An orange glow radiates from the center of NGC 1792, the heart of this stellar forge. Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The vast swathes of tell-tale blue seen throughout the galaxy indicate areas that are full of young, hot stars, and it is in the shades of orange, seen nearer the center, that the older, cooler stars reside.”



<h2 class="wp-block-heading" id="h-vigorous-star-formation-nbsp">Vigorous star formation&nbsp;</h2>



NGC 1792 is notable for its vigorous star formation, classifying it as a starburst galaxy. This high rate of star formation is thought to be triggered by gravitational interactions with neighboring galaxies, though the exact cause is still under study.



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. 



“Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



<h2 class="wp-block-heading" id="h-fierce-bursts-of-star-formation">Fierce bursts of star formation</h2>



ESA noted that when galaxies have a large reservoir of gas, like NGC 1792, these short-lived starburst phases can be sparked by galactic events such as mergers and tidal interactions.&nbsp;



“One might think that these starburst galaxies would easily consume all of their gas in a large forming event. However, supernova explosions and intense stellar winds produced in these powerful starbursts can inject energy into the gas and disperse it.”&nbsp;



“This halts the star formation before it can completely deplete the galaxy of all its fuel. Scientists are actively working to understand this complex interplay between the dynamics that drive and quench these fierce bursts of star formation.”



Due to its distance and brightness, NGC 1792 can be observed with medium-sized telescopes under favorable conditions.



<h2 class="wp-block-heading" id="h-the-evolution-of-galaxies">The evolution of galaxies </h2>



Galaxy evolution refers to the process by which galaxies form and change over time. It begins in the early universe, shortly after the <a href="https://www.earth.com/news/new-observations-disprove-big-bang-theory-universe-began-tired-light-theory/" target="_blank" rel="noreferrer noopener">Big Bang</a>, when small density fluctuations in the primordial gas led to the collapse of matter into the first galaxies.&nbsp;



<h3 class="wp-block-heading" id="h-galaxy-mergers">Galaxy mergers</h3>



Early galaxies were small and irregular, and were composed mostly of gas and dark matter. Over billions of years, galaxies grew larger by merging with one another and by accreting gas from the surrounding space. 



These interactions often triggered bursts of star formation, and collisions between galaxies sometimes led to the creation of new, more massive galaxies.



<h3 class="wp-block-heading" id="h-structural-changes">Structural changes</h3>



As galaxies evolve, their morphology - shape and structure - can change. Early galaxies were often irregular or disk-shaped, but over time, many galaxies formed into the elliptical or spiral shapes we see today. 



<h3 class="wp-block-heading" id="h-star-formation">Star formation</h3>



Star formation is a key driver of galaxy evolution, but it gradually slows down as galaxies age. 



The gas that fuels <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a> can be used up, or it can be heated and pushed out of galaxies by supernovae or black holes, reducing the galaxy's ability to form new stars.



<h3 class="wp-block-heading" id="h-galaxy-environment-nbsp">Galaxy environment&nbsp;</h3>



The environment in which a galaxy resides also plays a role in its evolution. Galaxies in dense clusters are more likely to interact with their neighbors, which can alter their shape or trigger bursts of star formation.&nbsp;



In contrast, galaxies in more isolated regions of space evolve more slowly and without as many dramatic interactions.



<h3 class="wp-block-heading" id="h-dark-matter">Dark matter</h3>



Dark matter also plays a crucial role in galaxy evolution. It provides the gravitational framework that holds galaxies together and influences their interactions with one another.&nbsp;



Supermassive <a href="https://www.earth.com/search-results/?search=Galaxies%20merge&amp;start=0" target="_blank" rel="noreferrer noopener">black holes</a>, found at the centers of most large galaxies, can also affect their evolution by releasing energy that impacts star formation and the movement of gas within the galaxy.



Overall, galaxy evolution is a complex and ongoing process driven by interactions between stars, gas, <a href="https://www.earth.com/news/study-dark-matter-does-not-exist-and-the-universe-is-27-billion-years-old/" target="_blank" rel="noreferrer noopener">dark matter</a>, and black holes, and shaped by both internal processes and external influences.



Image Credit: ESA/Hubble &amp; NASA, J. Lee



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Starburst galaxy in the constellation Columba

As anyone old enough to have witnessed the monumental event will be able to remember, Aldrin, Armstrong and Mike Collins were launched into space in July 1969. The trio departed Earth from the Kennedy Space Center in Florida in a Saturn V rocket. As Aldrin recalled at a 50th anniversary gala, the initial journey was also a surprisingly smooth one. Photo Credit: Project Apollo Archive/Flickr

Apollo 11 liftoff - July 16, 1969

The noises of everyday life might be stirring more than just your eardrums. Recent findings suggest that certain vibrations affect living cells in unexpected ways. 



In an effort to see if cells truly respond to sound, researchers developed specialized setups that send mild pressure waves into cell cultures.



After extensive tests, Masahiro Kumeta from <a href="https://www.kyoto-u.ac.jp/en" target="_blank" rel="noreferrer noopener">Kyoto University</a> emerged as a leading voice in this field.



<h2 class="wp-block-heading" id="h-cells-detect-and-respond-to-sound">Cells detect and respond to sound</h2>



Cells typically rely on chemical signals and mechanical <a href="https://www.earth.com/news/some-people-are-born-to-enjoy-music-more-than-others/" target="_blank" rel="noreferrer noopener">cues</a> to regulate their growth. The notion that <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4659753/" target="_blank" rel="noreferrer noopener">audible frequencies</a> might play a role in shaping cell functions has intrigued scientists for years.



“To investigate the effect of sound on cellular activities, we designed a system to bathe cultured cells in acoustic waves,” said Kumeta. 



The researchers noted that subtle compressions could alter how cells communicate and function.



<h2 class="wp-block-heading" id="h-when-cells-sense-pressure">When cells sense pressure</h2>



One pivotal outcome was the identification of over 100 genes that seemed sensitive to specific sound conditions. 



Different frequencies and intensities triggered varied <a href="https://www.earth.com/news/music-has-the-power-to-change-the-mood-of-our-memories/" target="_blank" rel="noreferrer noopener">responses</a>, hinting at a surprisingly sophisticated cellular awareness.



“Since sound is non-material, acoustic stimulation is a tool that is non-invasive, safe, and immediate, and will likely benefit medicine and healthcare,” said Kumeta. 



Observations <a href="https://pubmed.ncbi.nlm.nih.gov/11089525/" target="_blank" rel="noreferrer noopener">suggested</a> that mechanical receptors on cell surfaces might be picking up sound-related pressure changes.



<h2 class="wp-block-heading" id="h-sound-affects-fat-development">Sound affects fat development</h2>



The research also uncovered a link between vibrations and <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/adipocyte" target="_blank" rel="noreferrer noopener">adipocyte</a> development. Cells destined to become fat cells showed reduced differentiation when exposed to tailored sound signals.



This effect was partly explained by increased levels of <a href="https://www.sciencedirect.com/topics/neuroscience/prostaglandin-e2" target="_blank" rel="noreferrer noopener">PGE2</a>, a molecule known to influence fat cell growth. The findings add weight to ongoing discussions about non-invasive ways to manage tissue health.



<h2 class="wp-block-heading" id="h-everyday-noise-impacts-cell-health">Everyday noise impacts cell health</h2>



These discoveries raise questions about the relationship between environmental <a href="https://www.earth.com/news/live-music-connects-people-emotionally-and-physically/" target="_blank" rel="noreferrer noopener">noise</a> and cellular health. Future investigations might shed light on whether day-to-day soundscapes carry hidden effects for humans.



Such possibilities could open new therapeutic avenues to address metabolic issues or support tissue regeneration. 



Learning more about how cells detect acoustic cues might guide clinicians toward safer treatment strategies.



<h2 class="wp-block-heading" id="h-sound-can-control-cell-activity">Sound can control cell activity</h2>



Researchers are keen to explore how mechanical waves can be tuned to different cell types. This tuning could help maintain specific cell behaviors without using invasive procedures.



Understanding these mechanisms might also improve regenerative medicine by providing a <a href="https://www.earth.com/news/upright-walking-may-have-sparked-human-creativity-and-music/" target="_blank" rel="noreferrer noopener">tool</a> that supports healing tissues. 



Though the science is still expanding, the conversation around everyday sound’s potential influence on cellular well-being is gaining traction.



The idea that your cells respond to invisible shifts in pressure challenges traditional views of sensory biology. Investigations promise to reveal more about how we can harness acoustic signals in gentle yet meaningful ways.



<h2 class="wp-block-heading" id="h-vibrations-shift-gene-activity">Vibrations shift gene activity</h2>



Mechanobiology extends to how tissues interpret various physical forces. <a href="https://pubmed.ncbi.nlm.nih.gov/5763187/" target="_blank" rel="noreferrer noopener">Studies</a> suggest that subtle vibrations might shift gene expression in skeletal and smooth muscle.



Research into <a href="https://www.ncbi.nlm.nih.gov/books/NBK234245/" target="_blank" rel="noreferrer noopener">neurotoxins</a> and other complex biological processes also shows that cells often respond to unexpected sound cues in their environment. 



Low-intensity pulses can trigger molecular changes that were once thought impossible through conventional means.



<h2 class="wp-block-heading" id="h-noise-pollution-may-harm-cells">Noise pollution may harm cells</h2>



Efforts are underway to design experiments that separate normal mechanical stress from sound-induced signals. If those tests confirm unique responses, the results could open new doors in cell therapy.



Scientists are also curious about whether long-term exposure to mild acoustic environments might steer cells toward different fates.



Communities around the globe deal with noise pollution daily, so these results could change how we think about public health. It raises the possibility certain sound frequencies might either help or hinder basic cellular functions.



Finding a balance between beneficial and disruptive sound levels could become an unexpected health frontier. Communities might one day explore acoustic monitoring alongside typical environmental checks.



The study is published in the journal <a href="https://www.nature.com/articles/s42003-025-07969-1" target="_blank" rel="noreferrer noopener">Communications Biology</a>.



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Our cells react to sounds we can't even hear

The noises of everyday life might be stirring more than...

Greenland’s ice-covered landscape looks like an immovable block on satellite maps. Yet the story locked beneath its center suggests a very different past, one that places future coastal cities in a tight spot. 



During the <a href="https://www.earth.com/news/humans-were-likely-the-leading-cause-of-megafauna-extinctions/" target="_blank" rel="noreferrer noopener">Pleistocene</a> - the geologic chapter that began about 2.7 million years ago and ran through innumerable swings between cold and mild - the island’s ice waxed and waned in tune with global climate. 



New evidence hints that those swings were more dramatic than scientists once believed.



In 1993, drillers hauled a two‑mile‑deep ice core up from the island’s highest point and stowed the entire column in a Colorado freezer. 



The surprise awaited in the bottom three inches of sediment: perfectly preserved traces of a tundra ecosystem. 



That sliver of soil, shielded for ages by roughly 1.9 miles (3 km) of ice, now refocuses the conversation about future sea level and the stability of polar ice in a warming world.



<h2 class="wp-block-heading" id="h-tundra-hidden-beneath-greenland-s-ice">Tundra hidden beneath Greenland's ice</h2>



Once the drill broke through that 1.9‑mile roof of ice, the researchers retrieved those three inches of till. 



“These fossils are beautiful,” says Paul Bierman, a scientist at the <a href="https://www.uvm.edu/" target="_blank" rel="noreferrer noopener">University of Vermont</a> who co‑led the new study with UVM graduate student Halley Mastro and nine other researchers.



“But, yes, we go from bad to worse,” Bierman added, referring to what this finding implies about the impact of <a href="https://www.earth.com/news/indisputable-evidence-of-human-caused-climate-change/" target="_blank" rel="noreferrer noopener">human‑caused climate change</a> on melting of the Greenland ice sheet.



The till holds poppy, spike‑moss, woody willow tissue, fungal sclerotia, insect parts, and a band of soil capped by about 16 inches of erratic boulders. 



This is clear evidence that <a href="https://www.earth.com/news/drones-reveal-hidden-details-about-greenlands-melting-ice/" target="_blank" rel="noreferrer noopener">central Greenland</a> once lay ice‑free under a cold, dry sky where late‑lying snow lingered through early summer.



Because the material sits undisturbed, the team is confident it was not swept in from elsewhere as ice advanced.



<h2 class="wp-block-heading" id="h-inside-a-deep-greenland-ice-core">Inside a deep Greenland ice core</h2>



“Once we made the discovery at Camp Century, we thought, ‘Hey, what's at the bottom of GISP2?’” Bierman recalled.



High‑energy isotope ratios show that the summit last saw open air within the past 1.1 million years, while argon trapped in overlying clear ice indicates at least 250,000 years of continuous cover since then. Basal ice at another drilling site about 19 miles away is roughly 1 million years old. 



A separate core from Camp Century <a href="https://www.earth.com/news/city-under-the-ice-secret-base-camp-found-in-greenland/" target="_blank" rel="noreferrer noopener">near the coast</a> yielded plant remains no older than 416,000 years, underscoring the ice sheet’s flickering presence across the Pleistocene. 



These findings draw on material that had been stored at the National Science Foundation <a href="https://icecores.org/" target="_blank" rel="noreferrer noopener">Ice Core Facility</a> in Lakewood, Colorado, for three decades.



<h2 class="wp-block-heading" id="h-fossils-divulge-a-warmer-greenland">Fossils divulge a warmer Greenland</h2>



Under the microscope, what had looked like no more than specks floating on the surface of the melted core sample was, in fact, a window into a <a href="https://www.earth.com/news/greenland-transformation-ice-melt-plant-growth-vegetation-cascading-effects/" target="_blank" rel="noreferrer noopener">tundra landscape</a>. 



“It was amazing,” Mastro exclaimed. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/greenland_soil-sample_fossils_recently-melted-ice_credit-UVermont_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/greenland_soil-sample_fossils_recently-melted-ice_credit-UVermont_1s.webp" alt="Willow bud scale, arctic poppy seed, fungal bodies, and rock spikemoss megaspores found in the GISP2 soil sample viewed under a microscope at the University of Vermont. Credit: Halley Mastro/University of Vermont" class="wp-image-1966471"/></a><figcaption class="wp-element-caption">Willow bud scale, arctic poppy seed, fungal bodies, and rock spikemoss megaspores found in the GISP2 soil sample viewed under a microscope at the University of Vermont. Click image to enlarge. Credit: Halley Mastro/University of Vermont</figcaption></figure>



Mastro and colleagues picked out spores of spike‑moss, the bud scale of a young willow, and the compound eye of an insect - life‑forms adapted to chilly air and long summer daylight.



“And then we found Arctic poppy - just one seed of it. That is a tiny flower that's really good at adapting to the cold. It lets us know that Greenland's ice melted and there was soil, because poppies don't grow on top of miles of ice,” Mastro continued.



<h2 class="wp-block-heading" id="h-sea-level-risks-for-global-coasts">Sea‑level risks for global coasts</h2>



Sea level today is rising more than an inch each decade. “And it's getting faster and faster,” said&nbsp;Bierman. The extra water comes from a warming ocean that expands as well as from melting glaciers worldwide.



Near‑complete melting of Greenland’s ice over the next centuries to a few millennia would lead to some 23 feet of sea‑level rise. 



“Look at Boston, New York, Miami, Mumbai, or any other coastal city around the world, and add 20‑plus feet of sea level. It goes underwater. Don't buy a beach house," Bierman advised.



<a href="https://www.earth.com/news/how-much-did-sea-levels-rise-after-the-last-ice-age-alarming-new-clues-revealed/" target="_blank" rel="noreferrer noopener">Sea level</a> is likely to be several feet higher by the end of this century, when today’s children are grandparents.



<h2 class="wp-block-heading" id="h-greenland-s-fragile-ice-fortress">Greenland's fragile ice fortress</h2>



Richard Alley, a leading climate scientist at Penn State, reviewed the new research.



“This new study confirms, and expands upon earlier evidence, that significant sea‑level rise occurred at a time when the causes of warming were not especially extreme, providing a warning of the damage we might cause if we continue to warm the climate," Alley noted.



“We now have direct evidence that not only was the ice gone, but that plants and insects were living there,” Bierman concluded. “And that's unassailable. You don't have to rely on calculations or models.” 



The fossil soil at Greenland’s summit, locked beneath nearly two miles of ice, speaks plainly: polar ice sheets can retreat far and fast when the climate tips, and the coastlines of the future will trace that story in real time. 



Whether that warning is heeded remains a decision for policy makers and citizens alike.



The full study was published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2407465121#supplementary-materials" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Greenland fossil discovery stuns and worries scientists: "Don't buy a beach house"

Greenland’s ice-covered landscape looks like an immovable block on satellite...

Researchers have long studied quantum entanglement to understand how photons appear to influence each other instantaneously.



This peculiar link first emerged when Albert Einstein pointed to what he called “spooky action at a distance,” suggesting that this peculiar behavior contradicted intuitive <a href="https://www.earth.com/news/google-claims-commercial-quantum-computing-is-just-five-years-away/" target="_blank" rel="noreferrer noopener">views</a> of cause and effect.



The conversation around these phenomena has evolved through the decades. 



Ph.D. student <a href="https://phys.technion.ac.il/en/component/adm/person/1189" target="_blank" rel="noreferrer noopener">Amit Kam</a> and <a href="https://scholar.google.co.il/citations?user=Jf5cMM8AAAAJ&amp;hl=en" target="_blank" rel="noreferrer noopener">Dr. Shai Tsesses</a> from <a href="https://www.technion.ac.il/en/" target="_blank" rel="noreferrer noopener">Technion</a> are now adding a twist to this story by exploring surprising effects in photons that occupy incredibly tight spaces.



<h2 class="wp-block-heading" id="h-understanding-quantum-entanglement">Understanding quantum entanglement</h2>



Quantum entanglement is a strange but very real phenomenon where two particles become linked in such a way that their states depend on each other, even when separated by huge distances. 



Imagine you take a pair of gloves, put one in a box, and send it to the other side of the universe. The moment you open the box and see a left glove, you instantly know the other box has the right one. 



With entangled particles, it’s like that, but much weirder. The twist is, unlike gloves that had a clear identity from the start, <a href="https://www.earth.com/news/quantum-entanglement-speed-is-measured-first-time-too-fast-for-humans-minds/" target="_blank" rel="noreferrer noopener">entangled particles</a> don’t “decide” their state until someone measures them. And once one does, the other reacts instantly, no matter how far away it is.



Einstein was never fully onboard with quantum entanglement because it seems to break the rule that nothing can travel faster than light. 



But time and again, experiments have shown it’s real. No hidden signals. No delay. Just instant correlation. 



<h2 class="wp-block-heading" id="h-the-origins-of-entanglement">The origins of entanglement</h2>



Einstein’s <a href="https://plato.stanford.edu/entries/qt-epr/" target="_blank" rel="noreferrer noopener">collaboration</a> with Boris Podolsky and Nathan Rosen produced a classic puzzle that challenged existing ideas. 



Their EPR paper helped spark deeper inquiries into how one <a href="https://www.earth.com/news/microsoft-announces-giant-leap-in-quantum-computing-majorana-1/" target="_blank" rel="noreferrer noopener">particle</a> can instantly affect another across vast distances, a phenomenon that puzzled even seasoned physicists.



Years later, the idea reached practical horizons with <a href="https://doi.org/10.1103/PhysRevLett.70.1895" target="_blank" rel="noreferrer noopener">quantum teleportation</a>, which was conceptualized by Charles Bennett, Gilles Brassard, and Asher Peres. 



This opened the door to quantum communication protocols that rely on bizarre correlations only possible in the quantum world.



<h2 class="wp-block-heading" id="h-tiny-photon-spaces-are-revealing">Tiny photon spaces are revealing</h2>



The push to miniaturize devices is not just about saving space. Scaling down light-based components can strengthen the <a href="https://www.earth.com/news/baffling-quantum-entanglement-statistics-puzzle-finally-solved-advanced-technologies/" target="_blank" rel="noreferrer noopener">interaction</a> between photons and nearby materials, which may lead to applications that larger-scale systems cannot achieve.



Photons in <a href="https://pubs.acs.org/doi/abs/10.1021/acsanm.3c04950" target="_blank" rel="noreferrer noopener">nanoscale</a> environments showcase new combinations of properties. Instead of seeing separate spin and orbital components, scientists are dealing with <a href="https://faculty.washington.edu/seattle/physics541/12text.pdf" target="_blank" rel="noreferrer noopener">total angular momentum</a>, which merges these features into one quantity.



<h2 class="wp-block-heading" id="h-strange-photon-actions-in-small-spaces">Strange photon actions in small spaces</h2>



Most people imagine light beams spreading out freely, but these experiments <a href="https://www.earth.com/news/quantum-dance-entangled-photons-wave-functions-captured-real-time/" target="_blank" rel="noreferrer noopener">confine photons</a> into structures tinier than a thousandth the thickness of a human hair.



That restriction forces angular components of light to overlap in unexpected ways, altering how each photon can carry information.



These observations may hold promise for new kinds of <a href="https://www.earth.com/news/radical-theory-unites-gravity-spacetime-and-the-quantum-realm/" target="_blank" rel="noreferrer noopener">quantum</a> devices. 



Researchers propose that total angular momentum entanglement might enable more compact hardware for quantum computing or communication links than previously thought possible.



<h2 class="wp-block-heading" id="h-different-kind-of-quantum-entanglement">Different kind of quantum entanglement</h2>



Several forms of entanglement in photons involve separate characteristics such as direction, frequency, or polarization. In contrast, total angular momentum combines many properties into a single description.



Evidence for this new structure only surfaced when <a href="https://www.nature.com/articles/s41586-025-08761-1" target="_blank" rel="noreferrer noopener">researchers</a> tested how photon pairs behave once they pass through carefully designed nanoscale channels. 



The outcomes hinted at correlations that do not resemble conventional entanglement structures in larger settings.



<h2 class="wp-block-heading" id="h-why-does-this-matter">Why does this matter?</h2>



Those studying photon-based technologies aim to construct more efficient equipment that harnesses quantum <a href="https://www.earth.com/news/quantum-phase-superradiant-phase-transition-srpt-observed-in-lab/" target="_blank" rel="noreferrer noopener">effects</a> for faster computations or stealthy message exchanges. 



Smaller components can pack more operations onto a single chip, much like the ongoing trend in electronics.



While some quantum methods focus on established particle attributes, this work suggests that total angular momentum could be an untapped resource. 



The miniature systems explored by Technion scientists might offer fresh ways to encode and process data without taking up a lot of space.



<h2 class="wp-block-heading" id="h-photon-control-and-next-steps">Photon control and next steps</h2>



Entangled photons, even in conventional systems, are notoriously sensitive to environmental disturbances. 



Confining light in tiny spaces can amplify those effects, so the engineering behind these setups must address potential losses or interference.



Researchers also want to confirm whether total angular momentum entanglement behaves reliably in real-world conditions. 



Investigations into materials and device architectures are underway, guided by the new data from these nanoscale experiments.



<h2 class="wp-block-heading" id="h-how-this-links-back-to-einstein">How this links back to Einstein</h2>



Einstein’s skepticism about instant influence did not stop the scientific community from uncovering new frontiers in quantum theory. 



The <a href="https://www.nobelprize.org/prizes/physics/2022/summary/" target="_blank" rel="noreferrer noopener">2022 Nobel Prize in Physics</a> recognized key contributions that shaped how we measure and interpret entanglement.



Today, the focus has turned toward next-generation experiments that push these correlations into ever-smaller spaces. 



By compressing photons into structures below their typical wavelength, scientists hope to uncover possibilities beyond familiar optical behaviors.



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



Each step in quantum research sparks questions about how nature encodes information. 



The notion of merging spin and orbit into a single total angular momentum points to a shift in the thinking about light, especially when devices must stay small.



Further studies may translate these findings into commercial products. 



Many experts foresee a path where photons replace electrons in computing tasks, leading to faster speeds and less heat dissipation. This new entanglement feature could become an essential piece of that puzzle.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-025-08761-1" target="_blank" rel="noreferrer noopener">Nature</a>.



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New type of quantum entanglement will transform real-world technology

Researchers have long studied quantum entanglement to understand how photons appear...

For centuries, the universe has offered humanity glimpses of unimaginable galaxies and structures. Some shine brightly, others hide behind veils of gas and dust.



The Southern Pinwheel Galaxy, or Messier 83 (M83), seemed like one of the latter. Its vibrant spiral arms and starburst activity have dazzled astronomers. Yet, deep in its luminous center, something powerful remained unseen - until now.



Recent observations from the James Webb Space Telescope (<a href="https://science.nasa.gov/mission/webb/" target="_blank" rel="noreferrer noopener">JWST</a>) may have uncovered long-sought evidence of a supermassive <a href="https://www.earth.com/news/evidence-of-massive-early-universe-black-hole-stuns-astronomers/" target="_blank" rel="noreferrer noopener">black hole</a> at the galaxy's core.



This finding, driven by the telescope’s Mid-Infrared Instrument (MIRI), marks a major shift in our understanding of M83 and other galaxies that were once thought to be starburst-only systems. The results open a new chapter in extragalactic astronomy.



<h2 class="wp-block-heading" id="h-black-hole-hiding-in-a-starburst-galaxy">Black hole hiding in a starburst galaxy</h2>



M83 lies just 4.6 million parsecs away - relatively close on the cosmic scale. Its classification as a barred spiral galaxy with intense star-forming activity placed it under frequent scrutiny.



Yet, despite decades of detailed study, researchers failed to detect signs of a central <a href="https://www.earth.com/news/monster-in-the-shadows-giant-black-hole-emerges-from-cosmic-dust/" target="_blank" rel="noreferrer noopener">active galactic nucleus</a> (AGN), which is typically expected in galaxies of its size and structure.



Older optical and near-infrared observations suggested a complex nuclear region. Past efforts even revealed multiple candidate centers - each differing slightly in location and properties.



Still, none of these zones produced evidence strong enough to confirm AGN activity. If the galaxy held a supermassive black hole, it had to be dormant, hidden, or incredibly faint.



Astronomers suspected that thick dust may obscure faint AGN signals, especially in the galaxy’s nuclear starburst zone. Webb’s mid-infrared sensitivity changed that. With MIRI, researchers now see what previous instruments could not.



<h2 class="wp-block-heading" id="h-neon-signals-point-to-mystery">Neon signals point to mystery</h2>



The new study, led by Svea Hernandez, reported clear detections of highly ionized [Ne v] (14.3 μm) and [Ne vi] (7.7 μm) emission in the nucleus of M83.



These lines require photon energies of 97 and 126 electron volts, respectively, which are far higher than typical stellar processes can generate.



“Our discovery of highly ionized neon <a href="https://www.earth.com/news/thousands-of-active-black-holes-discovered-where-it-was-believed-they-couldnt-exist/" target="_blank" rel="noreferrer noopener">emission</a> in the nucleus of M83 was unexpected,” said Hernandez. “These signatures require large amounts of energy to be produced - more than what normal stars can generate. This strongly suggests the presence of an AGN that has been elusive until now.”



The emission appeared in distinct regions, including a point-like structure about 140 parsecs south of the optical nucleus, named P3. The structure measures less than 18 parsecs across and shows low obscuration, contrasting with the highly dust-shrouded core. This difference adds weight to the AGN scenario.



<h2 class="wp-block-heading" id="h-gas-flows-hinted-at-a-black-hole">Gas flows hinted at a black hole</h2>



Velocity maps from JWST show [Ne v] distributed in a clumpy, north-to-south alignment, with different regions exhibiting distinct kinematic signatures. 



P3’s [Ne vi] emission, for instance, shows a velocity of +80 km/s, slightly offset from the local [Ne v] velocity. Other zones closer to the nucleus display negative velocity offsets, hinting at motion that may trace outflow or turbulence.



The researchers compared the profiles of various ionized lines, from low to high energy. At P3, the high-ionization lines like [Ne v] and [Ne vi] are narrower than the lower-ionization lines.



This suggests that the gas producing these emissions may originate from a different physical process, possibly linked to AGN activity or compact shock-driven regions.



“Before Webb, we simply did not have the tools to detect such faint and highly ionised gas signatures in M83’s nucleus,” Svea added. “Now, with its incredible mid-infrared sensitivity, we are finally able to explore these hidden depths of the galaxy and uncover what was once invisible.”



<h2 class="wp-block-heading" id="h-are-radiative-shocks-the-culprit">Are radiative shocks the culprit?</h2>



To explain the origin of these extreme neon lines, the researchers tested several scenarios. Fast radiative shocks were one possibility.



These shocks occur when turbulent gas, such as that from a supernova or stellar wind, moves at supersonic speeds and compresses surrounding material. The resulting heat can produce high-energy radiation.



Shock models did reproduce the observed line ratios - but only under extreme assumptions. Specifically, the preshock density had to be a mere 0.01 cm⁻³, which is much lower than what is typically found in star-forming galaxies.



The observed postshock densities were also much higher, exceeding 1000 cm⁻³. This discrepancy challenges the idea that shocks alone could explain the data.



Energetic shocks are also known to destroy PAH molecules. Interestingly, P3 - the only region with [Ne vi] - shows the weakest PAH features in its spectrum. This matches the shock hypothesis, yet the unusual density mismatch casts doubt on this explanation.



<h2 class="wp-block-heading" id="h-black-hole-models-explain-galaxy-emissions">Black hole models explain galaxy emissions</h2>



The researchers then tested tailored photoionization models built around a low-luminosity AGN.



The models used a two-zone structure: one zone optically thin to ionizing radiation to generate high-energy lines like [Ne v], and another zone optically thick to generate lower-ionisation lines. This method reproduced the observed line strengths and ratios well.



The models assumed hydrogen column densities and metallicities consistent with M83’s central environment. They also used realistic ionisation parameters and densities. The best-fitting model places P3’s emission well within AGN-dominated zones on classic diagnostic plots.



“Webb is revolutionizing our understanding of galaxies,” said study co-author Linda Smith. “For years, astronomers have searched for a black hole in M83 without success. Now, we finally have a compelling clue that suggests one may be present.”



<h2 class="wp-block-heading" id="h-ruling-out-other-extreme-sources">Ruling out other extreme sources</h2>



Could other compact objects be responsible? High-mass X-ray binaries (HMXBs) can produce hard radiation, though usually at lower levels. 



Past X-ray surveys of M83 revealed several sources, including a bright object coinciding with the optical nucleus. But P3, where [Ne vi] was detected, shows no corresponding X-ray source.



Starburst activity alone cannot easily explain these ionized lines either. Models based on massive stars, including Wolf–Rayet populations, typically fail to reproduce the observed [Ne v] and [Ne vi] strengths. These limitations, combined with the success of the AGN models, make the AGN scenario more likely.



“This discovery showcases how Webb is making unexpected breakthroughs,” noted Smith. “Astronomers thought they had ruled out an AGN in M83, but now we have fresh evidence that challenges past assumptions and opens new avenues for exploration.”



<h2 class="wp-block-heading" id="h-m83-may-not-be-so-pure-after-all">M83 may not be so pure after all</h2>



For decades, M83 stood as a textbook example of a starburst galaxy. Optical data showed little hint of a central <a href="https://www.earth.com/news/black-holes-turn-into-white-holes-and-blast-out-matter-and-time-runs-backwards/" target="_blank" rel="noreferrer noopener">black hole</a>, but the discovery of high-ionization neon lines shifts this picture. Mid-infrared diagnostics, less hindered by dust, reveal what optical instruments missed.



Line ratio plots now place M83’s nuclear regions alongside hybrid AGN-starburst systems. In particular, P3 falls between the domains of purely star-forming galaxies and low-luminosity AGNs. This blend suggests that more such “pure” galaxies may indeed harbor faint AGNs.



The study urges astronomers to rethink what defines a starburst galaxy. With JWST, similar hidden cores may soon be uncovered in other nearby systems.



<h2 class="wp-block-heading" id="h-confirming-the-galaxy-s-black-hole">Confirming the galaxy’s black hole</h2>



The Webb team has laid the groundwork, but the mystery isn't solved yet. Future observations with ALMA and the Very Large Telescope will help test whether the neon emission truly comes from an AGN or another exotic source. These studies will probe gas motion, composition, and geometry more precisely.



Simulations with more complex geometries may also provide better answers. For now, M83’s hidden giant remains a strong candidate - but not a confirmed one.



Still, this work shows the power of <a href="https://www.earth.com/news/exoplanet-k2-18b-strongest-evidence-yet-of-extraterrestrial-life-discovered-webb/" target="_blank" rel="noreferrer noopener">Webb</a>. Where previous telescopes saw only dust and star formation in some galaxies, JWST has potentially opened a new window into spotting black holes and other hidden structures.



The study is published in <a href="https://iopscience.iop.org/article/10.3847/1538-4357/adba5d" target="_blank" rel="noreferrer noopener">The Astrophysical Journal</a>. 



Image Credit: ESA



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Black hole found hiding in a 'pure' starburst galaxy

For centuries, the universe has offered humanity glimpses of unimaginable...

River deltas hold a record of climate history. On Earth, coastlines mark where land and sea constantly interact. Here, rivers meet oceans. Materials from land gather in deltas. These areas store vital clues about tectonics, climate, and planetary evolution.



Scientists apply that same logic to Titan, Saturn’s <a href="https://www.earth.com/news/titan-may-harbor-life-but-it-will-be-difficult-to-find/" target="_blank" rel="noreferrer noopener">largest moon</a>. Titan has active rivers and vast seas, but its coastlines don’t behave like those on Earth.



<h2 class="wp-block-heading" id="h-titan-has-rivers-with-no-deltas">Titan has rivers with no deltas</h2>



Titan is the only body in the solar system, besides Earth, known to have stable liquid on its <a href="https://www.earth.com/news/cosmic-disturbance-the-mystery-of-titans-shifting-orbit/" target="_blank" rel="noreferrer noopener">surface</a>. 



Titan has clouds, rain, rivers, lakes, and seas. But the liquid is not water. It is replaced by methane and ethane, which remain liquid under Titan’s frigid atmospheric conditions. These features make it a rare and valuable analog to Earth.



If coastlines on Earth can store records of climate and tectonic change, then Titan’s might hold the same promise - offering a chance to study an alien hydrological system that’s still active today.



Yet there’s a mystery at Titan’s shores. Even though Titan has broad rivers and large lakes, river deltas appear to be almost entirely missing. This caught the attention of Sam Birch, an assistant professor at <a href="https://www.brown.edu" target="_blank" rel="noreferrer noopener">Brown University</a>.



“It’s kind of disappointing as a geomorphologist because deltas should preserve so much of Titan’s history,” Birch said.



<h2 class="wp-block-heading" id="h-are-deltas-just-hidden-from-view">Are deltas just hidden from view?</h2>



Back in 2006, NASA’s <a href="https://science.nasa.gov/mission/cassini/" target="_blank" rel="noreferrer noopener">Cassini</a> spacecraft gave scientists their first clear view of Titan’s <a href="https://www.earth.com/news/saturns-moon-titan-has-shorelines-shaped-by-waves/" target="_blank" rel="noreferrer noopener">surface</a>. Its Synthetic Aperture Radar (SAR) pierced Titan’s thick, hazy atmosphere and revealed flowing channels and dark, flat seas. 



But even at the mouths of Titan’s largest rivers, Cassini’s radar showed no clear signs of deltas. Scientists wondered - were these deltas hidden or missing altogether?



To answer that question, Birch and his team created a model. They simulated what Earth’s coastlines would look like through Titan’s radar conditions. In their model, Earth’s water was swapped for methane, mimicking Titan’s fluids, which absorb and reflect radar differently. 



The idea was simple: if Earth’s large deltas remain visible in these synthetic SAR images, then Cassini should have seen Titan’s deltas - if they existed.



“We basically made synthetic SAR images of Earth that assume properties of Titan’s liquid instead of Earth’s,” Birch explained.



<h2 class="wp-block-heading" id="h-cassini-should-detect-titan-s-deltas">Cassini should detect Titan's deltas</h2>



The model worked. Earth’s major coastal features - like the Mississippi River delta and barrier islands along the Gulf Coast - remained visible in the altered radar images.



This proved that Cassini should have been capable of detecting large deltas on <a href="https://www.earth.com/news/dragonfly-space-mission-saturn-moon-titan-gets-greenlight/" target="_blank" rel="noreferrer noopener">Titan</a>. With this in mind, the researchers returned to Titan’s SAR data and re-examined its coastlines.



“If there are deltas the size of the one at the mouth of the Mississippi River, we should be able to see it,” Birch said.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/titan_cassini-radar_earth-deltas_credit-Brown-University_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/titan_cassini-radar_earth-deltas_credit-Brown-University_1s.webp" alt="Earth, as seen by Cassini's radar. In order to understand what landforms on Titan could be seen by Cassini's radar, researchers looked at well-known Earth landforms through Cassini's perspective. The bottom image is how the U.S. Gulf Coast would have looked to Cassini. Credit: Birch Lab / Brown University" class="wp-image-1966464"/></a><figcaption class="wp-element-caption">Earth, as seen by Cassini's radar. In order to understand what landforms on Titan could be seen by Cassini's radar, researchers looked at well-known Earth landforms through Cassini's perspective. The bottom image is how the U.S. Gulf Coast would have looked to Cassini. Click image to enlarge. Credit: Birch Lab / Brown University</figcaption></figure>



But after carefully reviewing the data, they found that deltas were indeed rare. Aside from two likely deltas near the south pole, most large rivers on Titan showed no signs of delta formation. 



Only about 1.3% of the moon’s coastal rivers ended in deltas. By comparison, nearly every major river on Earth forms a delta at its mouth.



<h2 class="wp-block-heading" id="h-shifting-seas-may-erase-titan-s-river-deltas">Shifting seas may erase Titan's river deltas</h2>



On Earth, coastlines are dynamic boundaries. Materials eroded from mountains travel down rivers and settle into sedimentary structures. 



These interactions produce a range of landforms that help scientists trace environmental evolution. Coastal areas are also shaped by tides, storms, and long-term sea-level changes. 



Titan, with its unique climate system, is no exception. It too hosts coastlines where energy and materials interact - just with different ingredients and under different rules.



But Titan’s liquids are transparent to microwave radiation. This means Cassini’s radar can’t always distinguish where the coastline ends and where the sea floor begins. 



While that poses challenges, the team’s modeling showed that large features are still detectable - provided there is enough contrast between land and submerged surfaces.



The findings confirmed what many had suspected: Titan truly lacks deltas, and it’s not because of poor visibility. Something else is preventing these sediment-rich features from forming or surviving.



<h2 class="wp-block-heading" id="h-hidden-clues-beneath-titan-s-seas">Hidden clues beneath Titan’s seas</h2>



The new radar analysis also uncovered something unexpected. On Titan’s sea floors, the team found submerged river channels and deep pits of unknown origin.



These features suggest that sea levels may rise and fall frequently, eroding or dispersing any deltas before they have time to build up. 



The researchers also suspect that winds and underwater flows might redistribute sediment, flattening coastlines before deltas can grow.



These discoveries hint at a much more dynamic Titan than previously assumed. Active coastal processes - shaped by tides, climate shifts, and even currents beneath the seas - may constantly reshape the landscape.



“It’s a playground for studying processes we thought we understood,” said Birch.



<h2 class="wp-block-heading" id="h-a-dynamic-alien-coastline">A dynamic alien coastline</h2>



The absence of deltas and presence of submerged features offer a new window into Titan’s climate and geological behavior. Birch and his colleagues have proposed several preliminary hypotheses.



Sea-level cycling, strong coastal winds, and sub-aqueous flows could all contribute to the vanishing deltas. But more data is needed to understand these interactions fully.



“This is really not what we expected,” Birch said. “But Titan does this to us a lot. I think that’s what makes it such an engaging place to study.”



The study also reinforces the value of improving future instruments. A better imaging system could reveal Titan’s river networks and coasts in greater detail, uncovering hidden patterns and explaining current mysteries.



Such improvements wouldn’t just benefit research on Titan. They could also refine how scientists observe Earth’s own changing coasts in the face of sea-level rise and erosion.



The study is published in the <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JE008737" target="_blank" rel="noreferrer noopener">Journal of Geophysical Research Planets</a>. 



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Why does Saturn's moon, Titan, have rivers but not deltas? Scientists have an idea

River deltas hold a record of climate history. On Earth,...

For most of Earth’s first three billion years, oceans brimmed with single‑celled microbes that shuffled along at a slow biochemical pace -- life, but not complex. 



It lacked ample phosphorus, the nutrient every cell needs for DNA assembly, membrane stability, and ATP energy swaps. Rivers dripped only trace amounts of phosphorus into seawater, holding biology to pint‑size proportions and throttling evolutionary experiments in body size.



Evidence for that long famine sits in ancient mudstones, which contain scant phosphate minerals compared with younger rocks. 



Productivity lagged; oxygen production stayed low; food chains hid in microscopic layers. When phosphorus finally surged, life gained the <a href="https://www.earth.com/news/key-ingredients-building-blocks-of-life-found-in-asteroid-bennu-dust-sample/" target="_blank" rel="noreferrer noopener">building blocks</a> to try larger, more complex designs.



<h2 class="wp-block-heading" id="h-volcanic-chaos-and-complex-life">Volcanic chaos and complex life</h2>



About 2.1 billion years ago, the Congo and São Francisco continental blocks slammed together. 



Their collision squeezed faults, stirred magma, and unleashed underwater volcanoes across a shallow inland sea now preserved as the <a href="https://en.wikipedia.org/wiki/Franceville_basin" target="_blank" rel="noreferrer noopener">Francevillian sub‑basin</a> in Gabon. 



Eruptions pumped phosphorus‑rich fluids straight into the water and walled the basin off from the wider ocean.



<a href="https://www.earth.com/news/light-pollution-fuels-toxic-algae-and-alters-carbon-cycling-in-lakes/" target="_blank" rel="noreferrer noopener">Cyanobacteria</a> thrived in this enclosed lagoon, releasing oxygen and burying carbon as fast as nutrients arrived. 



The chemical bloom raised local energy budgets many times over, creating conditions that favored bigger bodies and cooperative cell assemblies rather than lone bacterial drifters.



<h2 class="wp-block-heading" id="h-fossil-discovery-challenges-timeline">Fossil discovery challenges timeline</h2>



Black shales from the basin hold disc‑shaped, ribbon‑shaped, and leaf‑shaped impressions up to six inches long - giants for their day. 



Their regular outlines and clustering hint at biological growth rather than odd mineral concretions. They appear in the same sedimentary layers that show the phosphorus spike, linking anatomy to chemistry.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/08/earth_complex-life_began-much-earlier_lobate-macrofossils_credit-UPoitiers_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/08/earth_complex-life_began-much-earlier_lobate-macrofossils_credit-UPoitiers_1s.webp" alt="The team’s research provides strong validation for the biological affinity of the lobate macrofossils whose validity has been widely debated in the scientific community. Credit: Professor Abderrazzak El Albani of the University of Poitiers, France" class="wp-image-1966454"/></a><figcaption class="wp-element-caption">The team’s research provides strong validation for the biological affinity of the lobate macrofossils whose validity has been widely debated in the scientific community. Click image to enlarge. Credit: Professor Abderrazzak El Albani of the University of Poitiers, France</figcaption></figure>



If these forms truly represent multicellular life, they push the arrival of complex organisms back by roughly 1.5 billion years. 



That jump rewrites the <a href="https://www.earth.com/news/timeline-of-life-ice-ages-gave-evolution-a-kick-start/" target="_blank" rel="noreferrer noopener">evolutionary timeline</a>, showing that animals were not the first to test large size; earlier prototypes surfaced when nutrients and oxygen briefly aligned.



<h2 class="wp-block-heading" id="h-chemistry-meets-biology">Chemistry meets biology</h2>



The new work, led by <a href="https://www.cardiff.ac.uk/" target="_blank" rel="noreferrer noopener">Cardiff University</a> geobiologist Dr. Ernest Chi Fru, pairs detailed rock chemistry with fossil mapping. 



“The availability of phosphorus in the environment is thought to be a key component in the evolution of life on Earth, especially in the transition from simple single‑celled organisms to complex organisms like animals and plants," Dr. Chi Fru explained.



“We already know that increases in marine phosphorus and seawater oxygen concentrations are linked to an episode of biological evolution around 635 million years ago. Our study adds another, much earlier episode into the record, 2.1 billion years ago.”



Digging into the basin’s history, Dr. Chi Fru explained that the volcanic activity following the collision of continental blocks likely isolated the basin from the global ocean, creating a nutrient-rich inland sea. 



This stable environment supported abundant <a href="https://www.earth.com/news/earth-was-once-a-green-marble-before-its-oceans-turned-blue/" target="_blank" rel="noreferrer noopener">cyanobacterial photosynthesis</a>, which in turn oxygenated the water and generated enough energy to support larger, more complex life forms like those seen in the fossils from the period.



<h2 class="wp-block-heading" id="h-why-the-complex-life-experiment-stalled">Why the complex life experiment stalled</h2>



Outside the Francevillian lagoon, oceans still lacked phosphorus and carried little oxygen. Larger creatures would have struggled in those harsh surroundings. 



The basin’s shoreline barrier turned the ecosystem into a biological bubble; when volcanic vents cooled and nutrient flow faded, conditions reverted and the macro‑organisms vanished.



Their failure to spread shows that evolution tests possibilities whenever resources allow, but those trials can fizzle if the wider planet remains hostile. 



Complexity needs both innovation and the freedom to roam - something the early <a href="https://www.earth.com/news/timeline-of-lifes-evolution-extended-by-nearly-1-5-billion-years/" target="_blank" rel="noreferrer noopener">Proterozoic world</a> could not yet provide.



<h2 class="wp-block-heading" id="h-two-steps-to-modern-animals">Two steps to modern animals</h2>



Researchers see a “two‑step” path. The Francevillian pulse marks step one, following the first known rise in atmospheric oxygen. 



Step two arrived nearly <a href="https://www.earth.com/news/luca-last-universal-common-ancestor-progenitor-all-life-on-earth/" target="_blank" rel="noreferrer noopener">1.5 billion years later</a>, when another oxygen surge met a more sustained supply of nutrients during the Ediacaran period. 



That tandem lifted complex life beyond isolated pockets, setting the stage for the Cambrian explosion and the diverse animals that populate Earth now.



The record hints that ample phosphorus may be as critical as oxygen for forging ecosystems full of active, energy‑demanding organisms. Without both factors in play, biology tends to stay microscopic.



<h2 class="wp-block-heading" id="h-why-does-any-of-this-matter">Why does any of this matter?</h2>



Astrobiologists comb <a href="https://www.earth.com/news/building-blocks-of-life-found-on-the-dwarf-planet-ceres/" target="_blank" rel="noreferrer noopener">exoplanet atmospheres</a> for oxygen because it signals possible photosynthesis. The Francevillian story suggests they should also weigh a planet’s phosphorus cycle. 



A world awash in oxygen but starved of phosphate could linger in a microbial phase for eons. Conversely, tectonic quirks that sprinkle oceans with phosphate might jump‑start evolutionary leaps.



Phosphorus, then, is more than fertilizer for terrestrial crops. It is a potential cosmic throttle on complexity, deciding whether life remains small or reaches for new biological heights.



-----



The full study was published in the journal <a href="https://www.sciencedirect.com/science/article/abs/pii/S0301926824001669?via%3Dihub" target="_blank" rel="noreferrer noopener">Precambrian Research</a>.



Image Credit: Professor Abderrazzak El Albani of the University of Poitiers, France



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Is this a fossil? If so, complex life on Earth emerged 1.5 billion years earlier

For most of Earth’s first three billion years, oceans brimmed...

A shapeless liquid form is something we usually take for granted. We expect fluids to spread and assume the shape of the container in which they are held. But nature sometimes defies our intuition.



In a recent study, a curious liquid refused to remain <a href="https://www.earth.com/news/water-appears-to-have-a-secret-liquid-phase/" target="_blank" rel="noreferrer noopener">chaotic</a> after being shaken and instead settled into a smooth, outlined shape reminiscent of a piece of classic pottery.



This strange finding was uncovered by a team that includes graduate student <a href="https://www.umass.edu/polymer-science/about/directory/anthony-raykh" target="_blank" rel="noreferrer noopener">Anthony Raykh</a> at the <a href="https://www.umass.edu" target="_blank" rel="noreferrer noopener">University of Massachusetts Amherst</a>. The group had been experimenting with oil and water when they noticed a shape they had never seen before.



<h2 class="wp-block-heading" id="h-understanding-shape-recovering-liquids">Understanding shape-recovering liquids</h2>



Some substances pull themselves together in neat ways. Others spread out in a disorderly manner.



For centuries, <a href="https://www.physics.ox.ac.uk/system/files/file_attachments/basic_thermo.pdf" target="_blank" rel="noreferrer noopener">thermodynamics</a> has helped predict these behaviors by setting rules about energy and equilibrium. 



Typically, adding particles to an oil-water mixture encourages the two <a href="https://www.earth.com/news/drones-reveal-hidden-details-about-greenlands-melting-ice/" target="_blank" rel="noreferrer noopener">liquids</a> to combine more readily and form new structures.



This phenomenon is known as <a href="https://www.sciencedirect.com/topics/agricultural-and-biological-sciences/emulsification" target="_blank" rel="noreferrer noopener">emulsification</a>, and it is vital in the production of foods, cosmetics, and many other commercial products. The usual theory says that those particles should lessen the tension between oil and water.



<h2 class="wp-block-heading" id="h-why-magnetism-matters">Why magnetism matters</h2>



Raykh decided to use magnetized nickel particles in his mixture. He shook things up, and something uncanny happened.



“... in a complete surprise, the mixture formed this beautiful, pristine urn-shape,” said Raykh. He tried shaking harder, but the fluid returned to the same outline.



Lab tests hinted that strong magnetic <a href="https://www.earth.com/news/wave-ripples-discovered-mars-surface-indicate-liquid-water-present-4-billion-years-ago/" target="_blank" rel="noreferrer noopener">interactions</a> were the reason. These metallic bits were powerful enough to throw a wrench into the fluid's normal behavior.



<h2 class="wp-block-heading" id="h-magnetic-forces-and-liquid-shape">Magnetic forces and liquid shape</h2>



Scientists often rely on known <a href="https://www.earth.com/news/earths-inner-core-proven-to-be-rapidly-changing-and-now-rotating-backwards/" target="_blank" rel="noreferrer noopener">interactions</a> to guide their experiments. Imposing magnetic forces adds another layer of complexity.



“When you look very closely at the individual nanoparticles of magnetized nickel that form the boundary between the water and oil, you can get extremely detailed information on how different forms assemble,” said <a href="https://www.umass.edu/natural-sciences/about/directory/david-hoagland" target="_blank" rel="noreferrer noopener">David Hoagland</a>, professor of polymer science and engineering at the University of Massachusetts Amherst. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/04/liquid_shape-recovering_breaks-laws-thermodynamics_Credit-UMassAmherst_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/04/liquid_shape-recovering_breaks-laws-thermodynamics_Credit-UMassAmherst_1s.webp" alt="Raykh and his colleagues discovered that strongly magnetized particles can bend the laws of thermodynamics. Credit: Anthony Raykh/UMass Amherst" class="wp-image-1964865"/></a><figcaption class="wp-element-caption">Raykh and his colleagues discovered that strongly magnetized particles can bend the laws of thermodynamics. Click image to enlarge. Credit: Anthony Raykh/UMass Amherst</figcaption></figure>



No one expected this intense attraction to stiffen the boundary so much that the liquids would create a neat form.



Researchers found that these <a href="https://www.sciencedirect.com/science/article/abs/pii/S0143720818304157" target="_blank" rel="noreferrer noopener">dipolar pulls</a> can drive up the tension between oil and water. This stands in contrast to what most textbooks tell us should happen.



<h2 class="wp-block-heading" id="h-why-does-any-of-this-matter">Why does any of this matter?</h2>



A single exception to well-known rules might inspire more questions on these types of liquid forms. The next challenge is figuring out the deeper mechanisms behind these robust fluid contours.



“Imagine your favorite Italian salad dressing. It’s made up of oil, water, and spices, and before you pour it onto your salad, you shake it up so that all the ingredients mix,” said <a href="https://www.umass.edu/polymer-science/about/directory/thomas-russell" target="_blank" rel="noreferrer noopener">Thomas Russell</a>, Silvio O. Conte distinguished professor of polymer science and engineering at the University of Massachusetts Amherst.



He compared his everyday culinary example to the surprising phenomenon in the lab.



The urn-like outline is stable enough to tease scientists with new ideas. Explorations of these forces could lead to fresh theories about soft materials and how they behave under powerful <a href="https://www.wiley.com/en-us/Introduction+to+Magnetic+Materials%2C+2nd+Edition-p-9780471477419" target="_blank" rel="noreferrer noopener">magnetic</a> influences.



<h2 class="wp-block-heading" id="h-what-it-means-for-the-laws-of-physics">What it means for the laws of physics</h2>



This discovery doesn’t mean thermodynamics is broken. But it does suggest that, under specific conditions, there may be edge cases where the traditional models don’t fully apply. 



Scientists call these scenarios “exceptions” rather than violations, and they help sharpen our understanding of how physical laws behave under extreme or unusual circumstances.



It’s a reminder that physical laws are models of reality, not reality itself. They hold true across vast numbers of conditions - but surprises like this urn-shaped liquid reveal that even well-tested theories can be stretched in new and useful ways.



<h2 class="wp-block-heading" id="h-liquid-shape-and-future-applications">Liquid shape and future applications</h2>



This experiment opens the door to unexpected applications in fields that involve finely tuned liquids. 



Medical formulations might someday use this kind of shape control to ensure more precise delivery of components.



Researchers are now looking into how strongly magnetized particles might alter other standard chemical processes.



Scientists remain cautious about declaring any new technology from this peculiar mixture. Even so, this discovery proves that our understanding of fluid behavior can still be surprised by odd twists.



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Click here to <a href="https://youtu.be/H02E7YTTFGQ" target="_blank" rel="noreferrer noopener">watch a video of this phenomenon...</a>



The study is published in <a href="https://www.nature.com/articles/s41567-025-02865-1" target="_blank" rel="noreferrer noopener">Nature Physics</a>.



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'Shape-recovering liquid' accidentally created by student breaks the laws of thermodynamics

A shapeless liquid form is something we usually take for...

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.



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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

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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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Photo Credit: Win McNamee/Getty Images

Buzz Aldrin Shares What Happened To Him After Landing On The Moon

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