Today's Image of the Day from the European Space Agency features NGC 6744 - a large, barred spiral galaxy located approximately 30 million light-years away in the constellation Pavo.&nbsp;



The galaxy is often considered a close analog to the <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a> due to its similar structure and size, spanning about 175,000 light-years across.&nbsp;



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp">Euclid space mission&nbsp;</h2>



The image was captured by the <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid</a> space telescope. NGC 6744 stands out as a prime example of the galaxies currently forming the majority of stars in the nearby universe, making it an ideal subject for study with the Euclid mission.&nbsp;



Euclid’s extensive field-of-view allows it to capture the entire galaxy, showcasing not only its large-scale spiral structure but also revealing intricate details on smaller scales across various wavelengths. These details include feather-like dust lanes, known as “spurs,” emerging from the spiral arms.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-6744">Star formation in NGC 6744</h2>



Euclid's observations enable scientists to count individual stars within NGC 6744, trace the distribution of stars and dust throughout the galaxy, and map the dust associated with the gas that fuels the development of new stars. 



<a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">Star formation</a> is a key process in the growth of galaxies, making these studies crucial for understanding galaxy evolution.



Researchers are utilizing Euclid’s data to explore the relationship between dust, gas, and star formation; to map the distribution of different stellar populations and identify regions of active star formation; and to investigate the underlying physics of spiral galaxy structures.&nbsp;



Spiral arms play a significant role in star formation by compressing gas, yet the precise mechanisms behind this process are still unclear. The presence of “spurs” along NGC 6744’s spiral arms offers valuable insights into the dynamics of star formation within these structures.



<h2 class="wp-block-heading" id="h-discovering-new-dwarf-galaxies-nbsp">Discovering new dwarf galaxies&nbsp;</h2>



Additionally, Euclid's dataset will help scientists identify clusters of old stars (globular clusters) and discover new dwarf galaxies around NGC 6744. Remarkably, Euclid has already identified a new dwarf satellite galaxy of NGC 6744 - a surprising discovery given that the galaxy has been studied extensively.



With Euclid’s detailed observations, scientists are gaining a deeper understanding of the processes shaping galaxies, providing essential clues to the evolution and appearance of the <a href="https://www.earth.com/news/universes-expansion-rate-hubble-tension-puzzles-astronomers/" target="_blank" rel="noreferrer noopener">universe</a>.



<h2 class="wp-block-heading" id="h-more-about-ngc-6744">More about NGC 6744</h2>



NGC 6744's disk is rich in star-forming regions and contains numerous young, bright blue stars. The galaxy's nucleus is slightly elongated and has a bar structure, which influences the motion of the stars and gas within it.&nbsp;



The spiral arms of NGC 6744 are well-defined and extend outward, wrapping around the central bar. Additionally, NGC 6744 has a smaller companion galaxy, NGC 6744A, which is interacting with it, adding to the complexity and interest of this distant system.&nbsp;



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



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are one of the most common types of galaxies in the universe, characterized by their distinct, spiral-shaped structure.&nbsp;



The galaxies typically consist of a flat, rotating disk containing stars, gas, and dust, along with a central concentration of stars known as the bulge. This bulge is often surrounded by a halo of older stars.&nbsp;



The spiral arms, which extend from the central bulge, are regions of active star formation and are rich in young, hot stars, giving them a bright, bluish appearance.&nbsp;



These arms are also sites where interstellar gas and dust are concentrated, leading to the formation of new stars.&nbsp;



Spiral galaxies are classified into different types based on the tightness of their spirals and the size of their central bulge, with classifications ranging from tightly wound arms in Sa galaxies to more loosely wound arms in Sc galaxies. The <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our home galaxy, is a prime example of a spiral galaxy.



<h2 class="wp-block-heading" id="h-the-constellation-pavo">The constellation Pavo</h2>



Pavo, which means "peacock" in Latin, is a constellation in the southern sky. It was named by the Dutch astronomer Petrus Plancius in the late 16th century, based on observations made during the Dutch explorations of the southern hemisphere. 



Pavo is one of the 12 constellations created by Plancius from the records of explorers Pieter Dirkszoon Keyser and Frederick de Houtman. 



The constellation is known for its distinctive shape, resembling a peacock with a long, curved tail. Pavo is not visible from most of the northern hemisphere, but it can be seen from the southern hemisphere, particularly during the winter months.



The constellation contains several interesting celestial objects, including the star Peacock, also known as Alpha Pavonis, which is the brightest star in the constellation. This star is a blue-white subgiant located about 179 light-years from Earth.



Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Euclid/Euclid Consortium/NASA&nbsp;



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Spiral galaxy NGC 6744 in the constellation Pavo

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

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 Glacier 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.&nbsp;



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. 



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 NASA Earth Observatory features...

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



“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.



Image Credit: NASA Earth Observatory



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Retreating glaciers and expanding meltwater lakes in Alaska

Today's Image of the Day from the European Space Agency (ESA) features the distant galaxy LEDA 22057, which is located about 650 million light-years away in the constellation Gemini. 



Within the galaxy lies a pale blue dot - SN 2024PI, a supernova explosion that was discovered by an automated survey in January 2024.



“The survey covers the entire northern half of the night sky every two days and has cataloged more than 10,000 supernovae,” noted <a href="https://www.esa.int/ESA_Multimedia/Images/2025/01/Pale_blue_supernova_dot" target="_blank" rel="noreferrer noopener">ESA</a>.



“The supernova is visible in this image: located just down and to the right of the galactic nucleus, the pale blue dot of SN 2024PI stands out against the galaxy’s ghostly spiral arms.”



<h2 class="wp-block-heading" id="h-the-remnants-of-a-supernova-nbsp">The remnants of a supernova&nbsp;</h2>



ESA noted that the image was taken about a month and a half after the <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">supernova</a> was discovered, so it appears many times fainter than its maximum brilliance.



“SN 2024PI is classified as a Type Ia supernova. This type of supernova requires a remarkable object called a white dwarf, the crystallized core of a star with a mass less than about eight times the mass of the Sun,” explained ESA.



“When a star of this size uses up the supply of hydrogen in its core, it balloons into a red giant, becoming cool, puffy and luminous. Over time, pulsations and stellar winds cause the star to shed its outer layers, leaving behind a white dwarf and a colorful planetary nebula.”&nbsp;



<h2 class="wp-block-heading" id="h-the-fate-of-white-dwarfs">The fate of white dwarfs</h2>



Most stars in the <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">Milky Way</a> will eventually end their lives as white dwarfs. Whether a star becomes a white dwarf depends on its mass.&nbsp;



Stars that are significantly more massive will end their lives differently. Massive stars - which exceed the critical mass threshold of eight times the <a href="https://www.earth.com/news/team-creates-video-showing-the-sun-in-gamma-rays-over-a-14-year-period/">Sun</a> - undergo more violent deaths.&nbsp;



After exhausting their nuclear fuel, they can collapse under their immense gravity and trigger a supernova explosion. Depending on the remaining core mass, they may leave behind either a neutron star or a black hole, rather than a <a href="https://www.earth.com/news/hungry-white-dwarf-stars-eat-heavy-metals/" target="_blank" rel="noreferrer noopener">white dwarf</a>.&nbsp;



These remnants represent extreme outcomes of stellar evolution and are fundamentally different from white dwarfs.



<h2 class="wp-block-heading" id="h-the-constellation-gemini-nbsp">The constellation Gemini&nbsp;</h2>



Gemini is one of the twelve zodiac constellations located in the northern celestial hemisphere.&nbsp;



Its name means "twins" in Latin, reflecting its representation of the mythological twins Castor and Pollux from Greek and Roman mythology.&nbsp;



<h3 class="wp-block-heading" id="h-stars-of-gemini">Stars of Gemini</h3>



The stars Castor and Pollux, which form the heads of the twins, are the brightest stars in Gemini and are key to its identification.&nbsp;



Pollux is a bright orange giant star, while Castor is a multiple <a href="https://www.earth.com/news/exoplanet-found-in-the-habitable-zone-of-a-binary-star-system/" target="_blank" rel="noreferrer noopener">star system</a> made up of six stars.



<h3 class="wp-block-heading" id="h-neighboring-constellations">Neighboring constellations</h3>



Gemini lies between Taurus to the west and Cancer to the east, and it is bordered by several other constellations, including Orion to the south.



It is most visible in the night sky during the winter months in the Northern Hemisphere, particularly in January and February.&nbsp;



<h3 class="wp-block-heading" id="h-significance-of-gemini">Significance of Gemini</h3>



The constellation is part of the ecliptic, the path that the Sun appears to take through the sky, making it significant in both astronomy and astrology.



Astronomically, Gemini is home to several interesting deep-sky objects, including the open star cluster M35, which is easily visible with binoculars or a small telescope.&nbsp;



The constellation also contains several stars and stellar systems of interest, such as variable stars and binary systems.



<h3 class="wp-block-heading" id="h-greek-mythology-nbsp">Greek mythology&nbsp;</h3>



In Greek mythology, Castor and Pollux were the sons of Leda, but they had different fathers - Castor was mortal, while Pollux was divine, being the son of Zeus.&nbsp;



Their story is one of loyalty and brotherhood, as Pollux begged Zeus to share his immortality with Castor after his brother's death. As a result, Zeus placed them in the sky as the constellation Gemini, symbolizing their eternal bond.



<h3 class="wp-block-heading" id="h-modern-culture">Modern culture</h3>



In modern culture, Gemini continues to be associated with duality, adaptability, and communication in astrology.&nbsp;



The constellation also holds significance in space science, lending its name to NASA's Gemini program in the 1960s. This program conducted critical missions that paved the way for the Apollo moon landings.



Image Credit: ESA&nbsp;



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Supernova explosion captured in the constellation Gemini 

Today's Image of the Day from the European Space Agency features the Southern Ring Nebula, also known as NGC 3132.



The nebula is located about 2,000 light-years away from Earth in the constellation Vela. This remarkably detailed image was created using data from Webb’s Near-Infrared Camera (NIRCam).



The Southern Ring Nebula is one of the more famous examples of planetary nebulae. It is often studied for its beauty and valuable insights into the end stages of stellar evolution.



<h2 class="wp-block-heading" id="h-stars-power-the-southern-ring-nebula-nbsp">Stars power the Southern Ring Nebula&nbsp;</h2>



The <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a> is powered by two central stars in a binary system. The brighter star is actually a less massive companion. The fainter, dimmer star is the dying, hot central star that has shed its outer layers to form the nebula. 



The dimmer star is a white dwarf and is responsible for the ionization of the gas in the nebula, causing it to glow.



“The bright star at the center of NGC 3132, while prominent when viewed by NASA’s Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"A second star, barely visible at lower left along one of the bright star’s diffraction spikes, is the nebula’s source. It has ejected at least eight layers of gas and dust over thousands of years.” 



“But the bright central star visible here has helped ‘stir’ the pot, changing the shape of this planetary nebula’s highly intricate rings by creating turbulence." 



ESA explained that the pair of stars are locked in a tight orbit, which leads the dimmer star to spray ejected material in a range of directions as they orbit one another, resulting in these jagged rings.



<h2 class="wp-block-heading" id="h-key-characteristics-of-the-southern-ring-nebula-nbsp">Key characteristics of the Southern Ring Nebula&nbsp;</h2>



The Southern Ring Nebula displays a complex structure with multiple layers of gas and dust. 



The outer shells of the nebula consist of hydrogen and other elements that were ejected from the dying star in previous stages of its <a href="https://www.earth.com/news/young-stellar-objects-observing-the-early-lives-of-stars/" target="_blank" rel="noreferrer noopener">evolution</a>. These layers are illuminated by ultraviolet radiation from the central white dwarf.



<h3 class="wp-block-heading" id="h-coloration">Coloration</h3>



The colors seen in the Southern Ring Nebula come from the different gases present. For example, hydrogen emits red light, while oxygen emits blue-green light. 



These colors help astronomers study the composition and dynamics of the nebula.



<h3 class="wp-block-heading" id="h-size-and-shape">Size and shape</h3>



The nebula spans about half a light-year in diameter. Its intricate, symmetrical structure provides valuable insights into the late stages of <a href="https://www.earth.com/news/star-collapse-black-hole-instead-of-supernova-vanish-from-sky/" target="_blank" rel="noreferrer noopener">stellar evolution</a>, especially the processes involved in the shedding of outer layers by dying stars.



<h2 class="wp-block-heading" id="h-spotlights-from-the-bright-star">Spotlights from the bright star</h2>



ESA noted that hundreds of straight, brightly-lit lines pierce through the rings of gas and dust. “These ‘spotlights’ emanate from the bright star and stream through holes in the nebula like sunlight through gaps in a cloud."



“But not all of the starlight can escape. The density of the central region, set off in teal, is reflected by how transparent or opaque it is. Areas that are a deeper teal indicate that the gas and dust are denser - and light is unable to break free.”



<h2 class="wp-block-heading" id="h-more-about-the-image">More about the image</h2>



According to ESA, this is not only a crisp image of a planetary nebula - it also shows us objects in the vast distances of space behind it. The transparent red sections of the nebula are filled with distant <a href="https://www.earth.com/news/galaxies-have-hearts-and-lungs-that-help-them-live-longer/" target="_blank" rel="noreferrer noopener">galaxies</a>.



“Look for the bright angled line at the upper left. It is not starlight - it is a faraway galaxy seen edge-on. Distant spirals, of many shapes and colors, also dot the scene. Those that are farthest away - or very dusty - are small and red,” said ESA.



<h2 class="wp-block-heading" id="h-the-constellation-vela-nbsp">The constellation Vela&nbsp;</h2>



Vela is a southern constellation that represents the sails of a ship. It was once part of a larger constellation called Argo Navis, which depicted the ship of the mythological hero Jason and the Argonauts. 



In the 18th century, Argo Navis was divided into three separate constellations: Vela (the sails), Carina (the keel), and Puppis (the stern).



Vela is notable for containing several interesting astronomical features. One of its most prominent stars is Gamma Velorum, also known as Suhail or Regor, which is a bright, massive star system consisting of multiple stars.&nbsp;



The constellation also hosts the Vela Supernova Remnant, the remains of a <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> explosion that occurred about 11,000 years ago. 



This remnant is associated with the Vela Pulsar, a neutron star that formed during the supernova explosion, which is one of the brightest pulsars in the sky.



Vela is best observed in the Southern Hemisphere, where it can be seen in the summer months. Its position along the Milky Way makes it a popular region for both amateur and professional astronomers to explore.



Image Credit: NASA, ESA, CSA, STScI



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Southern Ring Nebula in the constellation Vela 

Today's Image of the Day from the European Space Agency features the galaxy NGC 2090, located approximately 40 million light-years away in the constellation Columba.



NGC 2090 is a stunning spiral galaxy that is notable for its well-defined structure, featuring a bright central core surrounded by tightly wound spiral arms.&nbsp;



These arms are filled with young, hot stars and interstellar gas, indicating active star formation.&nbsp;



Captured by the Webb Telescope’s MIRI and NIRCam instruments, the image reveals the galaxy's winding spiral arms and the swirling gas and dust of its disc in magnificent and unique detail, noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>. 



<h2 class="wp-block-heading" id="h-observations-of-ngc-2090">Observations of NGC 2090</h2>



The galaxy’s spiral pattern is relatively symmetrical, making it a fascinating object of study for astronomers interested in galactic evolution and dynamics.&nbsp;



Observations of NGC 2090, including those conducted by the <a href="https://www.earth.com/news/hubble-helps-solve-the-mystery-of-a-young-eruptive-star/" target="_blank" rel="noreferrer noopener">Hubble</a> Space Telescope, have provided valuable insights into the properties of its stellar populations, gas content, and the nature of its spiral structure.



“NGC 2090 was one of many galaxies studied by the NASA/ESA Hubble Space Telescope to refine the measurement of the Universe’s expansion rate, or ‘Hubble constant,’” said ESA.&nbsp;



“This can be done by observing a special type of variable stars named ‘Cepheids’ in relatively nearby galaxies.”



<h2 class="wp-block-heading" id="h-new-insights-into-ngc-2090">New insights into NGC 2090</h2>



A Cepheid-based measurement from 1998 indicated that NGC 2090 is 37 million light-years away from Earth. However, the latest measurements suggest that the galaxy is 40 million light-years away.



“Already before that Hubble project in 1998, NGC 2090 had been well studied as a very prominent nearby example of star formation,” noted ESA.&nbsp;



“Described as a ‘flocculent’ spiral, this galaxy has a patchy, dusty disc and arms that are flaky or not visible at all. We can see those patterns well in Hubble's visible-light images. However, Webb’s NIRCam near-infrared data reveal the spiral arms with remarkable clarity.”&nbsp;



<h2 class="wp-block-heading" id="h-what-are-spiral-galaxies">What are spiral galaxies?</h2>



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are among the most common and visually striking types of galaxies in the universe.&nbsp;



They are characterized by their flat, disk-like shape with a bright central bulge surrounded by sweeping spiral arms.&nbsp;



<h3 class="wp-block-heading" id="h-spiral-arms-and-central-bulge-nbsp">Spiral arms and central bulge&nbsp;</h3>



The arms of a spiral galaxy are regions where stars, gas, and dust are concentrated, often glowing brightly with the light of young, hot stars that form within them.&nbsp;



The central bulge typically contains older stars and can host a supermassive black hole at its core.&nbsp;



<h3 class="wp-block-heading" id="h-types-of-spiral-galaxies-nbsp">Types of spiral galaxies&nbsp;</h3>



Spiral galaxies are classified into different types based on how tightly their arms are wound and the size of their central bulge, ranging from tightly wound "Sa" galaxies to loosely wound "Sc" types.



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



The structure of spiral galaxies is maintained by the interplay of gravity and angular momentum, with a rotating disk of stars and gas giving rise to their iconic shape.&nbsp;



They are active sites of <a href="https://www.earth.com/news/massive-star-redefines-our-understanding-of-stellar-evolution/" target="_blank" rel="noreferrer noopener">star formation</a> due to the abundance of gas in their arms.&nbsp;



Spiral galaxies often have a halo of older stars and globular clusters surrounding their disks, which provides clues about their formation and evolution.&nbsp;



<h3 class="wp-block-heading" id="h-barred-spiral-galaxy">Barred spiral galaxy</h3>



The <a href="https://www.earth.com/news/milky-way-galaxy-is-surrounded-by-massive-magnetic-fields/" target="_blank" rel="noreferrer noopener">Milky Way</a>, the galaxy that contains our Solar System, is a prime example of a barred spiral galaxy, a subtype where a bar-shaped structure of stars extends from the central bulge.&nbsp;



<h2 class="wp-block-heading" id="h-the-constellation-columba-nbsp">The constellation Columba&nbsp;</h2>



Columba is a small and relatively faint constellation in the southern sky, whose name means "dove" in Latin. It was introduced in the late 16th century by the Dutch astronomer Petrus Plancius and first appeared in a celestial atlas by Johann Bayer in 1603.&nbsp;



The <a href="https://www.earth.com/news/super-jupiter-discovered-in-the-great-bear-constellation/" target="_blank" rel="noreferrer noopener">constellation</a> is said to represent the dove sent out by Noah during the biblical flood, tying it to themes of hope and peace.



Columba lies near the larger constellation Canis Major and is bordered by others such as Lepus and Puppis.&nbsp;



Although it lacks particularly bright stars, its most notable star, Alpha Columbae (also called Phact), shines at a magnitude of approximately 2.6 and is a hot blue-white star. Beta Columbae, another prominent star in the constellation, is a slightly cooler, yellow-white star.



The constellation is best viewed from the Southern Hemisphere during the summer months, though it can also be seen from lower latitudes in the Northern Hemisphere.&nbsp;



Image Credit: NASA/ESA/CSA James Webb Space Telescope&nbsp;



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Webb unveils spiral galaxy NGC 2090 in magnificent detail

One day, however, Luna started feeling strange. While she had spent most of her life in captivity, she still had inescapable bear urges. There was something that she needed to do.

Bear Urges

Narcan, the nasal spray form of the opioid overdose-reversing drug naloxone, is now available over the counter in the United States. However, many people still don’t realize they can get it without a prescription. 



This simple spray, capable of restoring normal breathing in a matter of minutes, has become an essential tool in the fight against a rising tide of <a href="https://www.earth.com/news/brain-discovery-offers-hope-for-tackling-opioid-addiction/">opioid</a> overdoses. 



Yet, even with new efforts to boost awareness, polls indicate that a large portion of Americans remain uninformed about the updated, easier availability of naxolone.



<h2 class="wp-block-heading" id="h-a-source-of-real-world-guidance">A source of real-world guidance </h2>



TikTok’s rapid rise as a place to find health information has shifted how younger audiences learn about critical topics, including substance use and harm reduction.&nbsp;



A recent <a href="https://www.pewresearch.org/short-reads/2024/09/17/more-americans-regularly-get-news-on-tiktok-especially-young-adults/" target="_blank" rel="noreferrer noopener">study</a> found that roughly one in five adults in the United States now turns to TikTok for news and information on a variety of issues. This number has more than quadrupled in the last four years. 



As a result, the platform has transformed into more than a casual entertainment hub. It’s also a key source of real-world guidance that can influence behavior.



<h2 class="wp-block-heading" id="h-tiktok-and-opioid-overdose-prevention">TikTok and opioid overdose prevention</h2>



Led by Dr. Kelli Boling, assistant professor of advertising at the <a href="https://www.unl.edu/" target="_blank" rel="noreferrer noopener">University of Nebraska–Lincoln</a>, a team of researchers analyzed hundreds of TikTok posts to see how people talk about naloxone and its brand name Narcan online. 



The study was focused on videos featuring popular hashtags linked to opioid safety messages. The researchers narrowed their search to a time when opioid fatalities were climbing, and more people were scrolling through social media. 



The findings highlight TikTok’s potential for quick, high-impact communication about overdose prevention, addiction support, and news on treatment options.



<h2 class="wp-block-heading" id="h-tiktok-videos-on-narcan-access">TikTok videos on Narcan access</h2>



The researchers found that the most consistent topic across the videos was education about opioid risks, Narcan access, and the reality of recovery. 



In each video, creators used text, audio, and captions to clarify how to use naloxone and where to find it. The team also noticed a supportive group dynamic. 



“There was a strong ‘collective voice’ among the harm reduction creators that is ‘de-stigmatizing opioid harm reduction and sharing resources and information helpful to others,’” noted the researchers.



Similar trends emerged in a separate scholarly investigation that focused on the top opioid-related content under the #opioids hashtag, demonstrating that <a href="https://www.earth.com/news/growing-up-in-a-digital-world-tiktok-makes-teenagers-happy/">TikTok</a> discussions often revolve around safe medication practices, overdose risks, and pain management.&nbsp;



Across these studies, the short-video format proved to be an unexpected stage for candid personal stories and urgent calls to action.



<h2 class="wp-block-heading" id="h-implications-of-the-tiktok-ban">Implications of the TikTok ban </h2>



Despite TikTok’s growing impact on <a href="https://www.earth.com/news/longer-lifespan-strongly-linked-to-higher-education/">health education</a>, the Supreme Court recently upheld a federal law that effectively bans new downloads of the app unless it is sold by its current parent company. The court cited national security concerns as the main reason for its decision.&nbsp;



No matter where one stands on the ruling, the ban threatens to interrupt the steady flow of harm reduction content that is reaching individuals who might otherwise not seek out such information.



Existing users may still access TikTok, but fresh downloads and updates for new users will be blocked. This limit on functionality could reduce the platform’s reach and eventually affect creators who regularly upload videos about opioid safety.&nbsp;



For individuals in rural or underserved communities, losing easy access to these short but informative clips could make a real difference in whether they learn about new ways to manage opioid-related emergencies.



<h2 class="wp-block-heading" id="h-tiktok-and-opioid-safety-messages">TikTok and opioid safety messages</h2>



Educators and content creators on TikTok have long embraced the app’s simplicity. <a href="https://www.earth.com/news/scrolling-online-videos-is-not-a-good-cure-for-boredom/">Videos</a> showing how to administer Narcan, how to watch for overdose warnings, or where to find naloxone kits can be filmed in a matter of minutes.&nbsp;



This approach keeps instructions clear and relatable. Their style relies less on complicated jargon and more on straightforward guidance, which encourages viewers to ask questions and share personal experiences.



At a time when stigma still clings to discussions of addiction, these snippets of community-led education are often a lifeline. Many participants share struggles with pain or recovery, offering mutual support in the comments.&nbsp;



Such interactions highlight a practical form of outreach that appeals to younger audiences. That sense of openness can break down shame, encouraging people to seek professional help or pick up a naloxone kit at a local pharmacy.



<h2 class="wp-block-heading" id="h-life-saving-opioid-information-on-tiktok">Life-saving opioid information on TikTok </h2>



The recent legal development creates uncertainty. Some worry about a drop in new creators who tackle opioid safety messages. Others point out that alternative platforms exist, though none match TikTok’s unique way of combining brief, entertaining videos with a vast user base.&nbsp;



Conversations about harm reduction may end up scattered across multiple sites, making it harder for people to find consistent, trustworthy guidance.



Still, the drive to curb opioid overdoses carries on. <a href="https://www.earth.com/news/living-alone-in-america-an-escalating-public-health-crisis/">Public health</a> groups and grassroots advocates continue to emphasize naloxone training in schools, libraries, and community centers.&nbsp;



Experts at academic institutions are studying how best to deliver clear, effective instructions that cut through noise and misconceptions. 



The top priority is reversing rising overdose figures, and many believe that social media (no matter which platform ends up in the spotlight) will remain an essential tool for sharing life-saving information.



The study is published in the <a href="https://pubmed.ncbi.nlm.nih.gov/39727094/" target="_blank" rel="noreferrer noopener">Journal of Studies on Alcohol and Drugs</a>.



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TikTok videos provide a lifeline to prevent opioid overdoses

Narcan, the nasal spray form of the opioid overdose-reversing drug...

Scientists have been fascinated with solar flares for years. These fierce flashes of light from the Sun release a storm of charged particles into space, creating a breathtaking cosmic phenomenon.



But as awe-inspiring as these solar eruptions are, they also carry potential dangers for technology and astronauts in space - and even here on Earth.



<h2 class="wp-block-heading" id="h-flickering-clues-ahead-of-solar-flares">Flickering clues ahead of solar flares</h2>



A group of dedicated researchers has made a significant breakthrough in understanding solar flares. The team has been using NASA's Solar Dynamics Observatory to observe the <a href="https://www.earth.com/news/why-is-the-suns-corona-hotter-than-its-surface/" target="_blank" rel="noreferrer noopener">Sun's corona</a>, or outer atmosphere.



The experts focused their attention on a peculiar phenomenon: loops of light flickering in the Sun's corona. According to their observations, these flickering loops seem to serve as a lighted beacon signaling the onset of a massive solar flare.



This discovery holds enormous potential. It could assist NASA, along with other organizations involved in space and technology, to anticipate and protect against the harmful effects of <a href="https://www.earth.com/news/space-weather-poses-significant-risks-to-railway-safety/" target="_blank" rel="noreferrer noopener">space weather</a>.



<h2 class="wp-block-heading" id="h-coronal-loops-and-solar-flares">Coronal loops and solar flares</h2>



The research was led by Emily Mason, a heliophysicist at <a href="https://www.predsci.com/portal/home.php" target="_blank" rel="noreferrer noopener">Predictive Sciences Inc</a>.



The team examined structures known as <a href="https://www.earth.com/news/sun-covered-with-moss-peculiar-structure-sunspot-groups/" target="_blank" rel="noreferrer noopener">coronal loops</a>, which are arching, shimmering waves of light that jet out from magnetically charged areas of the Sun. It's in these active regions that solar flares find their birthplace.



The researchers analyzed coronal loops in close proximity to 50 strong solar flares. They observed the fluctuation in brightness of these loops in the hours leading up to the flare, and compared them to loops above areas of the Sun where no flares occurred.



The findings were intriguing: the loops above flare-active regions showed significantly more variations, serving as a kind of cosmic warning system.



"We found that some of the extreme ultraviolet light above active regions flickers erratically for a few hours before a solar flare. The results are really important for understanding flares and may improve our ability to predict dangerous space weather,” said Mason.



<h2 class="wp-block-heading" id="h-building-on-previous-research">Building on previous research</h2>



The experts noted that more research is needed to strengthen the correlation, especially concerning stronger flares from the Sun where the flickering seems to peak earlier.



Various other groups of scientists have turned to different methods to predict solar flares, such as studying <a href="https://www.earth.com/news/solar-dynamo-sun-magnetic-field-origin-generated-near-surface/" target="_blank" rel="noreferrer noopener">magnetic fields on the Sun</a> or searching for consistent patterns in other coronal loop features. 



However, Mason and her colleagues propose that monitoring the brightness variations in coronal loops might offer a more accurate warning, as they predict incoming flares 2 to 6 hours in advance with a 60 to 80 percent accuracy rate.



“A lot of the predictive schemes that have been developed are still predicting the likelihood of flares in a given time period and not necessarily exact timing," explained Seth Garland, a team member from the <a href="https://www.afit.edu/ABOUT/" target="_blank" rel="noreferrer noopener">Air Force Institute of Technology</a>.



<h2 class="wp-block-heading" id="h-towards-a-safer-space">Towards a safer space</h2>



The researchers believe their observations about coronal loops could significantly boost safety measures in space and on Earth, as they could protect astronauts, spacecraft, electrical grids, and other assets from harmful <a href="https://www.earth.com/news/scientist-sun-umbrella-tethered-to-an-asteroid-will-mitigate-climate-change/" target="_blank" rel="noreferrer noopener">solar radiation</a>.



An automated system could potentially monitor real-time images of coronal loop brightness shifts from the Solar Dynamics Observatory, thus enabling scientists to issue timely alerts.



“We could build on this and come up with a well-tested and, ideally, simpler indicator ready for the leap from research to operations," said Vadim Uritsky, an expert in space physics at NASA’s Goddard Space Flight Center and the Catholic University of Washington.



<h2 class="wp-block-heading" id="h-flickering-loops-on-the-sun">Flickering loops on the Sun</h2>



The discovery of flickering coronal loops as a precursor to solar flares opens up transformative possibilities in both research and technology. 



By incorporating these findings into predictive algorithms, researchers hope to see the development of automated systems capable of monitoring solar activity in real-time.



Such systems could alert satellite operators and power grid managers to potential disruptions, minimizing economic losses and enhancing global preparedness.



Moreover, this breakthrough has implications for deep space exploration. As human missions to the Moon, Mars, and beyond become more ambitious, the ability to predict solar flares with precision could be a vital tool for astronaut safety. 



Protective measures, such as temporary shielding or adjustments to mission schedules, could be implemented based on timely warnings, which would ensure that missions proceed with minimal risk.



Ultimately, this research could serve as a foundation for the integration of solar weather data into everyday life, influencing decisions ranging from airline route planning to GPS optimization.



The team presented their findings at the 245th meeting of the American Astronomical Society. The full study is published in the journal <a href="https://iopscience.iop.org/article/10.3847/2041-8213/ad94dd" target="_blank" rel="noreferrer noopener">The Astrophysical Journal Letters</a>.



Image Credit: NASA/Solar Dynamics Observatory



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Flickering loops appear on the Sun before it erupts

Scientists have been fascinated with solar flares for years. These...

Adding green tea and green smoothies to the traditional Mediterranean diet could slow brain aging more effectively, according to a new study by researchers at BGU University in Israel.



“This <a href="https://heart.bmj.com/content/107/13/1054" target="_blank" rel="noreferrer noopener">research</a> points towards the value of plant chemicals, called polyphenols, in the diet,” explained Laura Clark, a dietitian.



“These compounds, abundant in green vegetables, have anti-inflammatory properties and seem to be amongst the most potent for reducing our risk of brain degeneration as we age.”



While the study was focused specifically on green tea and smoothies, eating a variety of <a href="https://www.earth.com/news/mediterranean-diet-boosts-brain-power-by-altering-the-gut/" target="_blank" rel="noreferrer noopener">green vegetables</a> can offer similar benefits. 



In a recent report for The Telegraph, Sam Rice shared a list of five powerhouse greens and easy ways to enjoy them.



<h3 class="wp-block-heading" id="h-sauteed-kale-antioxidants-for-cell-protection">Sautéed Kale: Antioxidants for cell protection</h3>



Kale is rich in&nbsp;flavonols, antioxidants that help protect cells from damage and inflammation. It also contains&nbsp;glucosinolates, which convert to sulforaphane in the gut - a compound known for its anti-cancer properties.



<h4 class="wp-block-heading" id="h-how-to-enjoy-it">How to enjoy it</h4>



Since raw kale can be tough, try sautéing it. Heat&nbsp;olive oil&nbsp;in a pan, add&nbsp;grated garlic&nbsp;and a sprinkle of&nbsp;red pepper flakes, then toss in&nbsp;chopped kale. Cook until wilted, finish with&nbsp;lemon juice&nbsp;and&nbsp;black pepper, and serve warm.



<h3 class="wp-block-heading" id="h-leek-soup-prebiotics-for-gut-and-brain">Leek soup: Prebiotics for gut and brain</h3>



Leeks are a fantastic source of&nbsp;resistant starch, a type of fiber that feeds gut bacteria. The gut-brain connection plays a crucial role in&nbsp;cognitive function and insulin sensitivity.



<h4 class="wp-block-heading" id="h-comforting-winter-recipe">Comforting winter recipe</h4>



Melt&nbsp;1 tsp of butter&nbsp;in a saucepan, add&nbsp;finely sliced leek, and sauté for a few minutes. Add&nbsp;a diced potato&nbsp;and&nbsp;a bag of watercress, cooking for five more minutes. Pour in&nbsp;500ml vegetable stock&nbsp;and a sprinkle of&nbsp;nutmeg. Simmer for 20 minutes, then blend until smooth.



<h3 class="wp-block-heading" id="h-stir-fried-savoy-cabbage-a-fiber-powerhouse">Stir-fried savoy cabbage: A fiber powerhouse</h3>



Fiber is essential for digestion, heart health, and weight management. Savoy cabbage offers&nbsp;3g of fiber per 100g, making it a delicious alternative to bland bran cereals.



<h4 class="wp-block-heading" id="h-quick-stir-fry-method">Quick stir-fry method</h4>



Heat&nbsp;1 tbsp of oil&nbsp;in a wok, add&nbsp;grated garlic, fresh ginger, and diced red chili, and stir-fry for a minute. Toss in&nbsp;shredded Savoy cabbage&nbsp;and cook for three more minutes. Drizzle with&nbsp;sesame oil&nbsp;before serving.



<h3 class="wp-block-heading" id="h-green-peas-in-diet-a-plant-based-brain-boost">Green peas in diet: A plant-based brain boost</h3>



Unlike most <a href="https://www.earth.com/news/mediterranean-diet-a-delicious-way-to-manage-stress/" target="_blank" rel="noreferrer noopener">vegetables</a>, peas are rich in&nbsp;plant-based protein, offering&nbsp;5.5g per 100g&nbsp;without the saturated fat found in animal protein.



<h4 class="wp-block-heading" id="h-how-to-add-them-to-your-diet">How to add them to your diet</h4>



Blanch&nbsp;peas, mangetout, and green beans&nbsp;in boiling water for a few minutes. Make a dressing with&nbsp;lemon juice, orange juice, cumin, olive oil, salt, and pepper. Toss the veggies while warm and enjoy as a hearty winter salad.



<h3 class="wp-block-heading" id="h-swiss-chard-with-quinoa-strengthen-your-bones">Swiss chard with quinoa: Strengthen your bones</h3>



Most people know that calcium and vitamin D are essential for bone health, but&nbsp;vitamin K&nbsp;is just as crucial.&nbsp;It takes just 100g of Swiss chard&nbsp;to provide the daily recommended amount of vitamin K.



<h4 class="wp-block-heading" id="h-simple-side-dish">Simple side dish</h4>



Sauté&nbsp;mushrooms&nbsp;in&nbsp;butter and olive oil. Add&nbsp;pre-cooked quinoa,&nbsp;chopped Swiss chard, and fresh&nbsp;herbs&nbsp;(like mint or parsley). Let the leaves wilt, then finish with&nbsp;lemon juice, Parmesan shavings, and black pepper.



<h2 class="wp-block-heading" id="h-focus-of-the-mediterranean-diet">Focus of the Mediterranean diet </h2>



The Mediterranean diet draws inspiration from the&nbsp;traditional cuisines&nbsp;of Mediterranean countries like Greece, Italy, and Spain. It focuses on whole, nutrient-rich foods and prioritizes healthy fats, with olive oil serving as the main source.



The diet includes abundant vegetables, fruits, whole grains, nuts, and seeds, along with lean proteins like fish and seafood, and moderate amounts of poultry, eggs, and dairy.



Red meat and processed foods are consumed sparingly, while meals are rich in fiber from plant-based sources such as legumes and whole grains. Herbs and spices are used to flavor dishes, reducing the reliance on salt.



<h2 class="wp-block-heading" id="h-green-diet-for-brain-health">Green diet for brain health</h2>



The latest research shows that adding more&nbsp;green vegetables to this diet&nbsp;can help support&nbsp;brain function, improve memory, and enhance overall health. 



These greens contain&nbsp;powerful plant compounds, such as&nbsp;polyphenols and antioxidants, which help reduce&nbsp;inflammation and protect brain cells from age-related damage.



By adding extra greens to your diet, you can provide your brain with essential vitamins, minerals, and fiber that support cognitive function and gut health. These nutrients play a key role in reducing the risk of memory decline.



Regular consumption of these&nbsp;green Mediterranean staples&nbsp;may help maintain long-term brain health, keeping you mentally sharp for years to come.



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Brain benefits of the Mediterranean diet can be boosted with more greens

Adding green tea and green smoothies to the traditional Mediterranean diet could...

Galaxies come in many shapes and sizes, from massive spiral galaxies like the Milky Way to tiny, faint dwarf galaxies. While larger galaxies often steal the spotlight, small galaxies can also provide crucial insights into the history of the universe.



Researchers led by Kristen McQuinn of the Space Telescope Science Institute (STScI) have used the James Webb Space Telescope (JWST) to investigate Leo P, an isolated dwarf galaxy located 5.3 million light-years from Earth.



Their study has revealed surprising patterns in star formation that could reshape our understanding of how galaxies evolve over cosmic time.



<h2 class="wp-block-heading" id="h-leo-p-a-galactic-time-capsule">Leo P: A galactic time capsule</h2>



Leo P is unique among dwarf <a href="https://www.earth.com/news/spiral-galaxy-with-quasar-jet-surprises-astronomers/" target="_blank" rel="noreferrer noopener">galaxies</a>. Unlike many of its counterparts, it sits relatively isolated, away from the gravitational influence of larger galaxies like the Milky Way and Andromeda. This makes it a pristine laboratory for studying galaxy evolution without the complications of external interference.



The “P” in Leo P stands for “pristine,” a reference to its low metal content. In astronomy, "metals" refer to elements heavier than hydrogen and helium, which are produced by stars over time.



Leo P contains just&nbsp;3% of the Sun’s heavy elements, making it&nbsp;one of the most metal-poor galaxies known. This means Leo P resembles&nbsp;some of the earliest galaxies that formed in the universe, offering a rare glimpse into what galaxies looked like billions of years ago.



“Leo P provides a unique laboratory to explore the early evolution of a low-mass galaxy in detail,” said McQuinn, who also leads the <a href="https://www.stsci.edu/roman" target="_blank" rel="noreferrer noopener">Nancy Grace Roman Space Telescope</a>’s Science Operations Center.



<h2 class="wp-block-heading" id="h-a-start-stop-history-of-star-formation">A start-stop history of star formation</h2>



Astronomers have long studied&nbsp;how and when small <a href="https://www.earth.com/news/galaxies-are-much-bigger-than-we-originally-believed-gas-clouds/" target="_blank" rel="noreferrer noopener">galaxies</a> form stars. 



In most cases, dwarf galaxies begin forming stars early in their history. However, many of them stop producing stars after a few billion years - often permanently. The new observations of Leo P challenge that assumption.



Using&nbsp;JWST’s Near-Infrared Camera (<a href="https://science.nasa.gov/mission/webb/nircam/" target="_blank" rel="noreferrer noopener">NIRCam</a>), McQuinn’s team measured the&nbsp;brightness and colors of thousands of individual stars in Leo P. This data allowed them to reconstruct the&nbsp;star formation history&nbsp;of the galaxy in great detail.



They discovered that Leo P formed stars early in <a href="https://www.earth.com/news/universe-is-expanding-faster-than-science-can-explain-hubble-tension-physics-crisis/" target="_blank" rel="noreferrer noopener">cosmic history</a> but then&nbsp;abruptly stopped forming new stars shortly after a period known as the Epoch of Reionization. 



This was a key phase in the early universe when radiation from the first galaxies ionized the remaining neutral hydrogen gas, ending the universe’s “dark ages.” Many small galaxies&nbsp;lost their ability to form stars during this period and never recovered.



But Leo P was different. After a long dormancy, the galaxy reignited its star formation billions of years later - something rarely seen in other dwarf galaxies.



“We have a measurement like this for only three other galaxies that are all isolated from the Milky Way, and they all show a similar pattern,”&nbsp;McQuinn explained.



<h2 class="wp-block-heading" id="h-what-makes-leo-p-different">What makes Leo P different? </h2>



This discovery challenges long-held assumptions about why some <a href="https://www.earth.com/news/andromeda-galaxy-the-violent-history-of-our-closest-cosmic-neighbor/" target="_blank" rel="noreferrer noopener">galaxies</a> stop forming stars while others continue. 



For years, astronomers believed that a galaxy’s&nbsp;mass&nbsp;played the biggest role in whether it could sustain star formation.&nbsp;Smaller galaxies were thought to be more vulnerable to cosmic events like reionization, which stripped them of their gas and halted star formation.



However, Leo P tells a different story. The team compared its history with that of dwarf galaxies within the Local Group, the collection of galaxies that includes the Milky Way. Many of these galaxies ceased forming stars after the Epoch of Reionization - and never started again.



The difference?&nbsp;Leo P and the three other galaxies that restarted star formation are isolated, while the ones that remained dormant are&nbsp;satellite galaxies orbiting larger galaxies like the Milky Way.



This suggests that a galaxy’s environment, rather than just its mass, plays a crucial role in its ability to form stars over time.&nbsp;Galaxies that remain isolated may have a better chance of recovering and forming stars again, while those near large galaxies may lose their gas permanently.



“If the trend holds, it provides insights about the growth of low-mass structures that are not only a fundamental constraint for structure formation but a benchmark for cosmological simulations,” noted McQuinn.



<h2 class="wp-block-heading" id="h-a-window-into-the-early-universe">A window into the early universe</h2>



Another key finding from the study is that&nbsp;Leo P’s extremely low metal content makes it one of the closest analogs to the earliest <a href="https://www.earth.com/news/young-galaxy-shows-us-what-the-early-milky-way-looked-like/" target="_blank" rel="noreferrer noopener">galaxies</a> in the universe. The first galaxies to form after the Big Bang were extremely metal-poor, composed mainly of&nbsp;hydrogen and helium. 



Studying galaxies like Leo P helps astronomers understand&nbsp;how those first galaxies evolved and produced the heavy elements that make up stars, planets, and even life itself.



<h2 class="wp-block-heading" id="h-what-s-next-expanding-the-study">What’s next? Expanding the study</h2>



Leo P is just one piece of a much larger cosmic puzzle. To confirm whether its unusual star formation history is part of a broader pattern, McQuinn’s team plans to&nbsp;study four more isolated, star-forming dwarf galaxies&nbsp;using JWST. 



If they find similar trends, it could mean that&nbsp;many more galaxies in the early universe experienced multiple bursts of star formation instead of a single continuous phase.



These findings also have implications for&nbsp;cosmological simulations, which attempt to model how galaxies form and evolve over billions of years. If small galaxies like Leo P can reignite their star formation after long dormancies, then existing models may need to be revised to reflect this possibility.



<h2 class="wp-block-heading" id="h-small-galaxies-with-big-secrets">Small galaxies with big secrets</h2>



The&nbsp;<a href="https://science.nasa.gov/mission/webb/?exclude_child_pages=false&amp;order=DESC&amp;orderby=date&amp;layout=list&amp;number_of_items=4&amp;requesting_id=48174&amp;science_only=false&amp;show_content_type_tags=yes&amp;show_excerpts=yes&amp;show_pagination=true&amp;show_readtime=no&amp;show_thumbnails=yes&amp;response_format=html&amp;listing_page=no&amp;listing_page_category_id=2881&amp;post_types=post%2Cpress-release&amp;categories=2881" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a>&nbsp;continues to revolutionize astronomy. Its ability to peer into the past with&nbsp;unprecedented clarity&nbsp;allows astronomers to answer some of the biggest questions about&nbsp;galaxy formation and evolution.



The study of Leo P is just one example of how Webb is uncovering hidden details about the universe, helping scientists piece together the story of how galaxies - and ultimately, life itself - came to be.



Leo P’s&nbsp;unexpectedly complex history&nbsp;serves as a reminder that even the&nbsp;smallest galaxies can hold the biggest secrets.



Image Credit: NASA, ESA, CSA, Kristen McQuinn (STScI)



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Star formation 'reignited' in the galaxy Leo P after billions of years

Galaxies come in many shapes and sizes, from massive spiral...

Big,Cuttlefish,Hanging,In,The,Blue,Water,Close,Up,Photo

Cuttlefish, small marine animals that are masters of disguise, have left researchers wide-eyed by demonstrating high levels of self-control and an innate ability to wait, think, and make smart decisions. 



These highly-intelligent relatives of octopuses and squids have shown they’re capable of pausing for better rewards at a later point in time. 



It’s the same idea behind a popular test originally given to kids to see if they could wait for a bigger treat. Instead of marshmallows, though, these sea critters wait for shrimp.



<h2 class="wp-block-heading" id="h-ability-of-cuttlefish-to-wait">Ability of cuttlefish to wait</h2>



The findings come from a <a href="https://royalsocietypublishing.org/doi/10.1098/rspb.2020.3161" target="_blank" rel="noreferrer noopener">study</a> where scientists adapted <a href="https://www.universityofcalifornia.edu/news/marshmallow-test-revisited" target="_blank" rel="noreferrer noopener">the famous marshmallow test</a> to measure whether cuttlefish would pass on a snack if it meant enjoying tastier food later.



After it was confirmed they could hold out for something better, the team took things a step further. They checked if the same animals that showed self-control would also do well on a learning task. They did.&nbsp;



This is according to behavioral ecologist Alexandra Schnell from the <a href="https://www.cam.ac.uk/" target="_blank" rel="noreferrer noopener">University of Cambridge</a> in the UK, whose team first confirmed that cuttlefish could hold back their impulses.



<h2 class="wp-block-heading" id="h-peeking-inside-clever-minds">Peeking inside clever minds</h2>



Cuttlefish belong to a group of animals known for surprising feats. Certain <a href="https://www.earth.com/news/octopuses-could-dominate-earth-if-humans-vanish/" target="_blank" rel="noreferrer noopener">octopuses</a> have been filmed using coconut shells as portable hideouts.



Some squids communicate with patterns on their bodies. But these findings raised a question for Dr. Schnell’s team: do cuttlefish also show <a href="https://www.earth.com/news/cuttlefish-camouflage-is-much-more-complex-and-mind-boggling-than-initially-thought/" target="_blank" rel="noreferrer noopener">problem-solving skills</a> that appear in large-brained animals like crows and chimpanzees? 



One <a href="https://royalsocietypublishing.org/doi/10.1098/rspb.2020.3161" target="_blank" rel="noreferrer noopener">experiment</a> put that question to the test by letting the cuttlefish choose between a snack they could get right away or an even better snack if they waited. As soon as they picked the immediate option, the better meal disappeared.



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



When kids take part in a marshmallow test, they might look around nervously or cover their eyes so they don’t eat the treat too soon. In dogs, a similar ability to delay reward has been <a href="https://www.nature.com/articles/srep42459" target="_blank" rel="noreferrer noopener">studied</a> using treat tests.



While most of our beloved pets struggle to resist, some can wait longer than others. This skill often suggests a capacity for planning ahead. 



Cuttlefish, though, have never been known to rely on food storing or shared group behavior that might explain why they’d stand to benefit from waiting. So, a patient cuttlefish is a bit of a head-scratcher.



<h2 class="wp-block-heading" id="h-from-food-to-camouflage">From food to camouflage</h2>



The study was carried out in collaboration with senior scientist <a href="https://www.mbl.edu/research/faculty-and-whitman-scientists/Roger%20Hanlon" target="_blank" rel="noreferrer noopener">Roger Hanlon</a> at the Marine Biological Laboratory (<a href="https://www.mbl.edu/" target="_blank" rel="noreferrer noopener">MBL</a>). One theory for this behavior points to the cuttlefish’s defensive strategies. 



They spend a lot of time blending in with their surroundings to avoid being eaten. That means they can’t just dart around all day in search of nibbles. 



In many cases, the <a href="https://www.earth.com/news/cuttlefish-form-false-memories-events-similar-human-brains/" target="_blank" rel="noreferrer noopener">ability to hold out</a> might help cuttlefish wait for better prey, rather than risk revealing themselves for something mediocre. 



“Cuttlefish in the present study were all able to wait for the better reward and tolerated delays for up to 50-130 seconds, which is comparable to what we see in large-brained vertebrates such as chimpanzees, crows, and parrots,” said Dr. Schnell. 



A team of six cuttlefish proved they could hang back for up to about 130 seconds, which is roughly two minutes.&nbsp;



<h2 class="wp-block-heading" id="h-cuttlefish-wait-and-adapt-quickly">Cuttlefish wait and adapt quickly</h2>



Cuttlefish aren’t known to be social, nor do they spend time carrying objects to build complex traps. But <a href="https://www.earth.com/news/how-do-cuttlefish-instantly-change-their-skin-color-based-on-what-they-see-and-feel/" target="_blank" rel="noreferrer noopener">they do learn quickly</a>.



To measure that, the team placed two distinct shapes in the tank. One symbol signaled a reward if they touched it. 



Later, the scientists switched the meaning. The cuttlefish had to figure out that the “correct” shape now meant something else entirely. 



This is called a reversal-learning task, and it often trips up animals that rely on routine. Oddly enough, the cuttlefish that were better at waiting for a shrimp snack also learned this shape-swapping game in fewer tries.



<h2 class="wp-block-heading" id="h-memories-that-stay-sharp">Memories that stay sharp</h2>



Longer <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0038125" target="_blank" rel="noreferrer noopener">studies</a> on cuttlefish hint they may also have a good handle on remembering past events. 



Researchers have tested whether these animals recall what they ate, when they ate it, and where they found it. Their memory holds up, even when they’re older. 



Other <a href="https://www.cell.com/iscience/fulltext/S2589-0042(24)01547-5" target="_blank" rel="noreferrer noopener">studies</a> show they might sometimes form mistaken memories. That means the way they store events in their minds could be as twisty as it is in humans. 



Cuttlefish may even exhibit different <a href="https://www.earth.com/news/can-three-fish-make-a-school-study-offers-surprising-insights/" target="_blank" rel="noreferrer noopener">responses</a> to misleading cues, suggesting a process much like our own memory reconstruction.



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



Biologists studying big brains in animals often look at <a href="https://www.earth.com/news/bonobos-group-cohesion-common-enemy-effect-do-not-kill-inside-their-species/" target="_blank" rel="noreferrer noopener">primates</a>, <a href="https://www.earth.com/news/animals-care-more-about-unmet-expectations-than-fairness/" target="_blank" rel="noreferrer noopener">corvids</a>, and <a href="https://www.earth.com/news/parrots-have-a-unique-voice-print-similar-to-humans/" target="_blank" rel="noreferrer noopener">parrots</a>, because these groups seem to come up with creative solutions to daily challenges. 



The cuttlefish’s ability to hold back in a waiting game is a strong clue that self-control doesn’t always depend on working in teams or building fancy tools. It could arise from a creature’s environment. 



In this case, it might have grown out of the cuttlefish’s camouflage routine and the need to pick high-quality prey without exposing itself to danger.



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



Cuttlefish might not make complicated gadgets or team up to hunt in packs, yet they handle some tasks as well as animals famous for smarts.&nbsp;



That raises a puzzle about how intelligence evolves in separate branches of the animal kingdom. 



Scientists have speculated that these brainy feats can pop up when a species needs to adapt in special ways, whether to outwit predators or to find hidden meals.



The team's research was published in <a href="http://rspb.royalsocietypublishing.org/lookup/doi/10.1098/rspb.2020.3161" target="_blank" rel="noreferrer noopener">Proceedings of the Royal Society B</a>.



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Cuttlefish show levels of self-control and reasoning that rivals that of primates

Cuttlefish, small marine animals that are masters of disguise, have...

As an embryo grows, its cells engage in a complex conversation, ensuring the proper formation of tissues and organs. These signals come in chemical and mechanical forms, guiding cells like navigational beacons. However, recent research reveals an additional player in this intricate dance: bio-electric fields.



These invisible currents help direct the movement of cells, particularly the neural crest, a crucial population responsible for forming parts of the face, neck, and nervous system.



<h2 class="wp-block-heading" id="h-electric-signals-and-embryo-development">Electric signals and embryo development</h2>



For years, scientists speculated that <a href="https://www.earth.com/news/electric-field-signals-can-help-us-predict-extreme-weather/" target="_blank" rel="noreferrer noopener">electrical signals</a> played a role in embryonic development. Now, a study led by Dr. Elias H. Barriga provides definitive evidence. 



"We have characterized an endogenous bioelectric current pattern, which resembles an electric field during development, and demonstrated that this current can guide migration of a cell population known as the neural crest," noted Dr. Barriga.



His team first began this research at the Gulbenkian Institute of Science (<a href="https://gulbenkian.pt/en/a-new-scientific-era/" target="_blank" rel="noreferrer noopener">IGC</a>) in Portugal before continuing their work in Dresden at the Cluster of Excellence Physics of Life. The findings challenge previous assumptions about how cells coordinate movement within a developing embryo.



<h2 class="wp-block-heading" id="h-electrotaxis-the-traffic-signals-of-development">Electrotaxis: The traffic signals of development</h2>



The concept of electrotaxis, where cells move in response to electric fields, has been studied primarily in artificial lab settings. But Dr. Barriga's work brings this <a href="https://www.earth.com/news/earths-magnetic-field-has-a-dent-and-nasa-is-watching-closely/" target="_blank" rel="noreferrer noopener">phenomenon</a> of electric field response into the realm of live embryos. 



His team observed that neural crest cells naturally migrate by following internal electrical cues, much like drivers obeying traffic lights.



To understand how cells interpret these bioelectric signals, the researchers identified a key enzyme, voltage-sensitive phosphatase 1 (Vsp1), present in neural crest cells. This enzyme appears to act as both a sensor and a translator of electric fields, enabling cells to move in an organized, directional manner.



Dr. Sofia Moreira, a postdoctoral scientist on the study, found great satisfaction in applying genetic tools to explore bioelectricity. "For me, applying tools I developed to target gene expression in the context of bioelectricity was highly rewarding, and I look forward to its potential being fully exploited."



Interestingly, Vsp1 does not influence cell movement directly. Instead, it ensures cells respond correctly to electrical gradients, making it distinct from other enzymes typically linked to cell migration. This insight paves the way for further exploration into bioelectric guidance systems in development.



<h2 class="wp-block-heading" id="h-how-electric-fields-form-in-the-embryo">How electric fields form in the embryo</h2>



The study also sheds light on how these electric fields emerge in the embryo. 



The team proposed that mechanical stretching in a region known as the neural fold activates specific ion channels, generating a voltage gradient. Neural crest cells then detect this gradient, using Vsp1 to decode the signal and move accordingly.



This discovery marks the first experimental proof that electric fields not only guide migrating cells but also arise along their path. These findings add a new dimension to our understanding of embryonic development, offering a deeper appreciation of bioelectricity’s role in shaping life.



<h2 class="wp-block-heading" id="h-a-new-era-in-bio-electricity-research">A new era in bio-electricity research</h2>



The implications of this study extend beyond embryology. 



"This paper bridges an important, decades-old gap in bio-electricity research, and it is deeply rewarding to be part of the ongoing renaissance in developmental bio-electricity," noted postdoctoral scientist Dr. Fernando Ferreira.



According to Dr. Barriga, the next question is, how does this fit into already established frameworks of mechanical and chemical cues during embryogenesis?



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



Beyond embryo development,&nbsp;bioelectric fields may influence wound healing and cancer progression. 



In <a href="https://www.earth.com/news/healing-chronic-wounds-with-gold-and-red-wine/" target="_blank" rel="noreferrer noopener">wound healing</a>, cells migrate to repair tissues, and electric fields may help direct them, just as they do in embryos. Understanding this process could lead to treatments that&nbsp;speed up recovery&nbsp;and improve healing.



<a href="https://www.earth.com/news/secrets-of-cancer-cell-death-may-transform-treatment/" target="_blank" rel="noreferrer noopener">Cancer</a> cells also move in ways similar to embryonic cells. If electric fields influence this migration, researchers could find ways to&nbsp;control cancer spread, leading to potential new therapies.



In&nbsp;regenerative medicine and tissue engineering, scientists aim to rebuild tissues and organs. If electric fields naturally guide cell movement, they could be used to&nbsp;improve lab-grown tissues and nerve regeneration.



This discovery reveals a&nbsp;new layer of biological complexity. Cells respond to bioelectricity, not just chemical and mechanical cues. Further research could&nbsp;unlock new medical breakthroughs, shaping the future of healing, disease treatment, and tissue engineering.



The study is published in the journal <a href="https://www.nature.com/articles/s41563-024-02060-2" target="_blank" rel="noreferrer noopener">Nature Materials</a>.



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Embryo formation is shaped by electric fields

As an embryo grows, its cells engage in a complex...

Physicists have long grouped the most basic building blocks of our universe into two categories. One group consists of fermions, which include matter particles like electrons, protons, and neutrons.&nbsp;



The other group contains bosons, which include particles linked to forces like photons and the <a href="https://www.earth.com/news/higgs-boson-god-particle-still-remains-quantum-mystery-after-12-years/" target="_blank" rel="noreferrer noopener">Higgs particle</a>. These two families differ in their “spin” values and in how many can occupy the same place at once.



<h2 class="wp-block-heading" id="h-searching-for-paraparticles">Searching for paraparticles</h2>



Recent work suggests a whole new category of quasiparticles called paraparticles might exist. After decades of thinking we had only two options (<a href="https://www.energy.gov/science/doe-explainsbosons-and-fermions" target="_blank" rel="noreferrer noopener">bosons or fermions</a>) scientists discovered a possible third way.&nbsp;



They have only explored these proposed objects in one- and two-dimensional mathematical models, but there is no ironclad reason to dismiss their presence in our three-dimensional world.



<a href="https://profiles.rice.edu/faculty/kaden-hazzard" target="_blank" rel="noreferrer noopener">Dr. Kaden Hazzard</a> at <a href="https://www.rice.edu/" target="_blank" rel="noreferrer noopener">Rice University</a> appears as one of the key researchers behind this study. 



He and his colleague <a href="https://www.mpq.mpg.de/person/127228/4571983" target="_blank" rel="noreferrer noopener">Zhiyuan Wang</a>, now at the <a href="https://www.mpq.mpg.de/en" target="_blank" rel="noreferrer noopener">Max Planck Institute of Quantum Optics</a>, carried out an in-depth analysis to challenge the assumption that no other particle types could exist.



<h2 class="wp-block-heading" id="h-how-paraparticles-might-work">How paraparticles might work</h2>



“<a href="https://www.earth.com/news/particles-are-forming-in-the-atmosphere-in-an-unexpected-way/" target="_blank" rel="noreferrer noopener">Particles</a> aren’t just these fundamental things,” said Hazzard at the end of one of the study’s statements. 



That comment underscores a focus on quasiparticles, which are effective descriptions of how groups of regular particles behave when they interact. 



<a href="https://www.uni-muenster.de/Physik.AP/Demokritov/en/Forschen/Forschungsschwerpunkte/mBECwaqp.html#" target="_blank" rel="noreferrer noopener">Quasiparticles</a> are not original building blocks of matter. Instead, they show up as patterns or disturbances in a larger system.



Hazzard and Wang’s mathematical efforts centered on condensed matter settings, which involve materials like magnets and other densely packed systems. 



They used advanced algebraic methods to handle the exchange of particles within those tight environments. 



Their calculations revealed that paraparticles could develop different rules than either <a href="https://www.energy.gov/science/doe-explainsbosons-and-fermions" target="_blank" rel="noreferrer noopener">fermions or bosons</a> when they switch places.



“We determined that new types of particles we never knew of before are possible,” said Hazzard at the end of another statement. That claim upsets the longstanding idea that quasiparticles always fit into the same old categories.



<h2 class="wp-block-heading" id="h-why-are-paraparticles-important">Why are paraparticles important?</h2>



A person might wonder if these hypothetical particles have any real-world use. In recent years, a type of quasiparticle called <a href="https://www.energy.gov/science/bes/articles/anyons-found-best-evidence-yet-these-long-sought-quasi-particles" target="_blank" rel="noreferrer noopener">anyons</a> has excited <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.53.722" target="_blank" rel="noreferrer noopener">researchers</a> looking into quantum computers. The reason is that anyons could help store and process information in more stable ways.&nbsp;



Paraparticles might offer something equally helpful - or maybe even more unusual. Nobody is sure how far this idea could go.



“This is cross-disciplinary research that involves several areas of theoretical physics and mathematics,” said Wang near the end of the published results.&nbsp;



The range of methods used (such as Lie algebra, Hopf algebra, and group theory) points to serious effort in bridging <a href="https://www.earth.com/news/if-a-monkey-typed-for-infinity-could-it-recreate-shakespeare/" target="_blank" rel="noreferrer noopener">mathematical ideas</a> with physical reality.



<h2 class="wp-block-heading" id="h-could-paraparticles-appear-in-everyday-life">Could paraparticles appear in everyday life?</h2>



Most breakthroughs in <a href="https://www.earth.com/news/quantum-entanglement-spooky-action-at-a-distance-persists-between-top-quarks/" target="_blank" rel="noreferrer noopener">particle physics</a> or condensed matter do not show up on a kitchen table. These paraparticles might appear only under very special conditions. 



Right now, the studies point to their appearance in one and two dimensions, like in tightly controlled experiments or possibly in exotic states of matter. It is not clear how often nature might brew up these odd entities, but the door is open for future tests.



“I don’t know where it will go, but I know it will be exciting to find out,” said Hazzard at the end of another remark, echoing the sentiment that today’s curiosity can become tomorrow’s discovery.&nbsp;



For decades, researchers have questioned whether we were missing something in the particle zoo. Now, fresh models indicate there might be more to the story than we assumed.



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



Hazzard and Wang’s new approach is still at an early stage. It demonstrates that <a href="https://www.earth.com/news/graviton-like-particle-observed-in-quantum-material-for-the-first-time/" target="_blank" rel="noreferrer noopener">condensed matter</a> systems could host paraparticle-like excitations, which means scientists have a place to start searching. 



Efforts to nail down signatures of paraparticles may help confirm that they are not just neat math puzzles. These ideas might also spark a wave of research into exotic phases of matter that never quite fit into existing theories.



“It’s also why you don’t just go through your chair when you sit down,” joked Hazzard in one of his public addresses, emphasizing how particle statistics define the <a href="https://www.earth.com/news/strange-high-energy-cosmic-rays-did-something-outside-our-galaxy-send-them-here/" target="_blank" rel="noreferrer noopener">entire structure</a> of ordinary matter. 



That principle underlies familiar features such as solidity and chemical behavior. If paraparticles lurk anywhere, they might enrich our understanding of why the world is the way it is.



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



Researchers may next try to propose experiments that shine light on paraparticle effects in advanced laboratories. Whether they manage to create these new quasiparticles or see them naturally in materials remains to be seen.&nbsp;



Even small hints that paraparticles are real would give scientists a chance to explore phenomena that previously looked off-limits.



For now, the notion stands as a mathematical proof of possibility. It challenges the assumption that <a href="https://www.earth.com/news/higgs-boson-god-particle-still-remains-quantum-mystery-after-12-years/" target="_blank" rel="noreferrer noopener">bosons</a> and fermions are the only options and leaves the door open for more surprises.&nbsp;



That sense of possibility is enough to keep many scientists energized. They recognize that what seems purely theoretical now can sometimes lead to major leaps down the road.



The study is published in <a href="https://www.nature.com/articles/s41586-024-08262-7" target="_blank" rel="noreferrer noopener">Nature</a>.



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New category of particles discovered in the subatomic realm

Physicists have long grouped the most basic building blocks of...

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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

[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"] Today's Video of the Day from the...

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Today’s Video of the Day from the <a href="https://www.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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Today’s Video of the Day from <a href="https://www.igb.illinois.edu/">Carl R. Woese Institute for Genomic Biology</a> reveals how scientists can modify common crops like soybean, rice, and wheat to protect them from heat stress.



“We need to double crop production by 2050 to feed a growing global population, and not only are we not on track to do that, but climate change is further complicating things,” said Amanda Cavanagh, a lecturer at the University of Essex. 



The study is part of Realizing Increased Photosynthetic Efficiency (RIPE), an international research project that aims to develop food crops that turn the sun’s energy into food more efficiently.



“Using an engineering approach we designed multiple alternative metabolic pathways to photorespiration. Testing them in the field showed increases in productivity which led Amanda to significantly move the project forward by showing our engineered plants can withstand pretty extreme temperature stress,” said study co-author and RIPE researcher Paul South.&nbsp;



“As the climate changes and temperature stresses increase the pressure on our global food supply, farmers will need every tool available including engineering approaches like the synthetic biology used here to maintain safe and productive harvests.”



The experts tested plants modified to have more efficient photorespiration to see if they were better adapted to warmer temperatures.&nbsp;



The team found that the engineered plants produced 26 percent more biomass than the wild-type plants exposed to the same temperatures, and had 15 percent less yield loss under the higher temperatures.



Video Credit: Amanda Nguyen/University of Illinois



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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.

Designing crops that can beat the heat

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Once she realized where she was, Luna immediately settled into her new home. Instinct took over, and, before long, she was running through the grass as if she had never left. Photo Credit: Beverley &amp; Pack/ Flickr

Free At Last

They had taken her to Bear Sanctuary Muritz to live in comfort. After three long years trapped in a cramped, amusement park cage, Luna was returning to nature. Cautiously, she sniffed the air. Photo Credit: Four Paws