Los Glaciares National Park is located in the Santa Cruz Province of <a href="https://www.earth.com/image/tectonic-forces-alter-the-landscape-in-argentina/">Argentina</a>. It lies on top of the Patagonian Andes &#8212; an area filled with mountains, lakes, forests and glaciers. It has a total surface area of about 600,000 hectares and was declared a UNESCO World Heritage Site in 1981. Los Glaciares National Park takes its name from the numerous glaciers which cover about half of the property, many of which are fed by the massive South Patagonia Ice Field.
The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard <a href="https://en.wikipedia.org/wiki/NASA">NASA’s</a> Aqua satellite acquire this true-color image on November 20, 2016. Also Los Glaciares National Park is a beautiful destination spot.
Over time the melting of glaciers have formed the three lakes seen in this image. From north to south they are Lago San Martin, Lago Viedma, and Lago Argentino. The Upsala, Onelli, and Perito Moreno Glaciers calve into Lago Argentino. Perito Moreno is famous for its unusual behavior. The front of the massive glacier rises up to 60 meters (197 feet) high continuously moves forward, eventually blocking a narrow channel formed by Lago Argentino. Eventually, the pressure increases on the glacial tongue until it ruptures dramatically, calving icebergs into the waters of the lake.
&#8212;
Credit: <a href="http://www.nasa.gov" target="_blank" rel="noopener noreferrer">NASA</a>

Los Glaciares National Park

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



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



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



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



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



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



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



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. “Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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NGC 1792: A galactic powerhouse 

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 the European Space Agency features the spiral galaxy IC 5332, which is located over 29 million light-years away from Earth.



The galaxy spans approximately 66,000 light-years in diameter. This makes it notably smaller than our <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>, which is just over 100,000 light-years in diameter. 



<h2 class="wp-block-heading" id="h-unprecedented-look-at-ic-5332">Unprecedented look at IC 5332</h2>



In a stunning photo release by NASA and ESA in 2022, the spiral galaxy IC 5332 was presented in an unprecedented level of detail. The images were captured by the <a href="https://www.earth.com/news/james-webb-captures-incredible-new-image-of-uranus/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a>.



This feat was made possible through the use of the Mid-InfraRed Instrument (MIRI), which captures images in the mid-infrared spectrum.



<h2 class="wp-block-heading" id="h-unique-perspective-from-earth">Unique perspective from Earth</h2>



One of the most striking features of IC 5332, as revealed by these observations, is its almost perfect face-on orientation relative to Earth.&nbsp;



This unique perspective allows astronomers to clearly observe and admire the symmetrical arrangement of its spiral arms.



<h2 class="wp-block-heading" id="h-webb-unveils-ic-5332-in-new-light">Webb unveils IC 5332 in new light</h2>



The clarity of these images represents a significant advancement over previous observations made by the Hubble Space Telescope, which imaged IC 5332 in ultraviolet and visible light.&nbsp;



While Hubble’s images revealed the galaxy’s symmetrical spiral arms, James Webb’s MIRI has unveiled these structures as a complex web of gas that emits infrared light at various temperatures.



<h2 class="wp-block-heading" id="h-the-miri-instrument-on-james-webb-nbsp">The MIRI instrument on James Webb&nbsp;</h2>



Capturing this range of infrared light is no simple task. It requires highly specialized instruments that must be maintained at extremely cold temperatures.&nbsp;



The MIRI instrument on the James Webb Space Telescope is specifically designed for this purpose and performs exceptionally well. Its capabilities allow astronomers to see aspects of <a href="https://www.earth.com/news/james-webb-captures-galaxies-that-are-too-old-to-exist/" target="_blank" rel="noreferrer noopener">galaxies</a> that are otherwise hidden in other wavelengths.



The detailed images provided by MIRI offer more than just a visual spectacle; they provide valuable data about the composition and temperature of the gases that make up the spiral arms of IC 5332. 



This can help scientists understand the processes of star formation within the galaxy and how these processes compare to those in our own <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>.



<h2 class="wp-block-heading" id="h-webb-finds-hidden-features-of-the-universe-nbsp">Webb finds hidden features of the universe&nbsp;</h2>



The images of IC 5332 served as a critical test of the James Webb Space Telescope’s capabilities in observing the universe in infrared light. 



As astronomers continue to explore with Webb’s full suite of instruments, many more hidden features of the universe will be revealed.



The information provided by the <a href="https://www.earth.com/news/webb-telescope-discovers-second-most-distant-galaxy-in-pandoras-cluster/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> not only expands our understanding of the cosmos but also enhances our appreciation for the complex and beautiful structures that exist in our universe.&nbsp;



<h2 class="wp-block-heading" id="h-spiral-galaxies-like-ic-5332">Spiral galaxies like IC 5332</h2>



Spiral galaxies are some of the most visually striking objects in the universe, characterized by their rotating arms that extend from a central nucleus, giving them a distinct spiral appearance.&nbsp;



These galaxies are primarily made up of a flat, rotating disk containing stars, gas, and dust, and a central concentration of stars known as the bulge. These are often surrounded by a much fainter halo of stars, many of which reside in globular clusters.



Spiral galaxies differ from other galaxy types, such as elliptical and irregular galaxies, in their structure and content. 



The spiral arms are sites of ongoing star formation and are brighter than the rest of the disk because of the young, hot stars that are typically found there. The arms appear distinct because of their density waves, which compress the gas and dust, leading to star formation.



The rotation of the spiral arms also contributes to the galaxy's flat shape due to the centrifugal forces acting on the disk. The central bulge can vary in size and often contains older, red stars.&nbsp;



<h2 class="wp-block-heading" id="h-barred-spiral-galaxies-nbsp">Barred spiral galaxies&nbsp;</h2>



Some spiral galaxies have a bar-shaped structure that extends from the central bulge, making them barred spirals. This bar affects the motion of stars and gas within the galaxy and can influence star formation activity.



Spiral galaxies are an important focus of study because they contain a significant amount of visible matter and play a crucial role in understanding the formation and evolution of galaxies.&nbsp;



Their distinct features also make them particularly useful for studying the laws of physics under extreme conditions, such as high densities and velocities.



Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Webb, NASA &amp; CSA, J. Lee and the PHANGS-JWST and PHANGS-HST Teams



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Spiral galaxy IC 5332: A complex web of gas and light

Today's Image of the Day from the European Space Agency features the star-forming region NGC 604, which is located 2.73 million light-years away from Earth in the Triangulum Galaxy (M33). The image was captured by the James Webb Space Telescope.



By studying regions like NGC 604, astronomers can gain insights into the complex interactions between stars and the interstellar medium, as well as the conditions that lead to the birth of stars. This, in turn, helps in understanding the evolution of <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxies</a> and the universe as a whole.



<h2 class="wp-block-heading" id="h-massive-stars-of-ngc-604">Massive stars of NGC 604</h2>



"Sheltered among NGC 604’s dusty envelopes of gas are more than 200 of the hottest, most massive kinds of stars, all in the early stages of their lives," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"These types of stars are known as B-types and O-types, the latter of which can be more than 100 times the mass of our own Sun. It’s quite rare to find this concentration of them in the nearby universe. In fact, there’s no similar region within our own Milky Way galaxy."



According to ESA, this concentration of massive stars, combined with its relatively close distance, means NGC 604 gives astronomers an opportunity to study these objects at a fascinating time early in their life.



<h2 class="wp-block-heading" id="h-gigantic-region-of-ionized-hydrogen">Gigantic region of ionized hydrogen</h2>



NGC 604 is one of the largest known regions of ionized hydrogen, also known as an H II region. This nebula is significantly larger than the Orion Nebula, which is one of the most well-known H II regions in our own <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 galaxy</a>.&nbsp;



NGC 604 spans about 1,500 light-years across, making it one of the largest H II regions in the Local Group of galaxies. This group includes the Milky Way, the Andromeda Galaxy, and about 54 other smaller galaxies. 



<h2 class="wp-block-heading" id="h-ngc-604-starburst-phenomenon">NGC 604 starburst phenomenon </h2>



Within NGC 604, there are hundreds of young, hot, massive <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">stars</a>. These stars have ionized the surrounding gas, causing it to glow and creating the nebula. The region is a prime example of a starburst phenomenon, where stars form at a much higher rate than in typical galactic conditions.



“The bright orange streaks in this image signify the presence of carbon-based molecules known as polycyclic aromatic hydrocarbons, or PAHs," explained ESA.



"As you travel further from the immediate cavities of dust where the star is forming, the deeper red signifies molecular hydrogen. This cooler gas is a prime environment for star formation. Ionized hydrogen from ultraviolet radiation appears as a white and blue ghostly glow."



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



Star formation is crucial for the evolution of galaxies and the synthesis of heavy elements. In the cores of stars, elements heavier than helium are created.



The elements are spread throughout the <a href="https://www.earth.com/news/ancient-stars-shakti-shiva-shaped-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">galaxy</a> when stars reach the end of their lives and expel their material - either gently through winds or violently via supernova explosions. This enriching process allows for the formation of new stars and planets, and ultimately, the potential for life.



<h3 class="wp-block-heading">Cloud collapse</h3>



The process begins when part of a molecular cloud becomes unstable and starts to collapse under its own gravity. This can be triggered by events like shock waves from nearby <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, galactic collisions, or the influence of other massive stars.



<h3 class="wp-block-heading">Formation of a protostar</h3>



As the cloud collapses, it fragments into smaller clumps. Each clump will eventually form one or more stars. 



The material within these clumps continues to fall inward, heating up as it does so, eventually forming a warm core called a protostar. At this stage, the protostar is not yet hot enough for nuclear fusion (the process that powers stars) to occur.



<h3 class="wp-block-heading">Accretion disk</h3>



Around the protostar, material from the surrounding cloud continues to fall inward, forming a rotating disk. This material slowly accretes onto the protostar, increasing its mass.



<h3 class="wp-block-heading">Nuclear fusion begins</h3>



Once the core of the protostar reaches a high enough temperature and pressure, hydrogen atoms begin to fuse into helium, releasing energy in the process. This marks the transition from a protostar to a main sequence star, like our sun.



<h3 class="wp-block-heading">Main sequence and beyond</h3>



The star will spend the majority of its life in the main sequence stage, where it balances the gravitational forces trying to collapse it and the outward pressure from nuclear fusion. 



Eventually, the star will exhaust its hydrogen fuel. Its subsequent evolution will depend on its initial mass, leading to various end stages such as red giants, supernovae, neutron stars, or black holes.



Image Credit: NASA/ESA/CSA James Webb Space Telescope



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Young, massive stars in the Triangulum Galaxy

Today's Image of the Day from NASA Earth Observatory features the Ruki River in the Democratic Republic of the Congo (DRC). It is a tributary of the Congo River, one of the largest rivers in the world by discharge and depth.&nbsp;



The Ruki River, previously known as the Busira, merges with the Momboyo River near the town of Basankusu to become the Lulonga River, which eventually flows into the Congo River at the town of Lisala.



<h2 class="wp-block-heading" id="h-dark-waters-of-the-ruki-river">Dark waters of the Ruki River</h2>



"If the appearance of the muddy Amazon River evokes a coffee cut with cream, the Ruki River, coursing gently through the Congo Basin, is like a dark tea," said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"On its slow path through mostly untouched lowland rainforest in the Democratic Republic of Congo (DRC), the water leaches organic material from vegetation, prompting some researchers to think it is one of the darkest blackwater rivers on Earth."



According to NASA, scientists are finding that the dissolved material in this distinctive water offers clues about the carbon cycle of tropical forests.



<h2 class="wp-block-heading" id="h-organic-compounds-in-the-ruki-river">Organic compounds in the Ruki River</h2>



In a recent study, researchers measured the chemical <a href="https://www.earth.com/news/warmer-rivers-keep-antimicrobial-resistant-genes-at-bay/" target="_blank" rel="noreferrer noopener">composition</a> and flow of the Ruki for the first time.&nbsp;



"The study reported that, as the water color suggests, the Ruki is rich in dissolved organic carbon compounds," said NASA.



"It contains four times as much organic carbon as the Congo River and 1.5 times as much as the Rio Negro, the world’s largest blackwater river and a major tributary of the Amazon."



Due to this heavy carbon load, the researchers concluded that tropical forests like those around the Ruki might not accumulate quite as much carbon as we once thought.



<h2 class="wp-block-heading" id="h-significance-of-the-river">Significance of the river </h2>



The river is vital for the livelihoods of local communities. <a href="https://www.earth.com/news/fishing-communities-cooperate-to-survive-climate-change/" target="_blank" rel="noreferrer noopener">Fishing</a> is a crucial activity, with many people depending on it for sustenance and income. The river also supports agriculture along its banks, where communities grow crops.



In many parts of the DRC, <a href="https://www.earth.com/news/rivers-are-warming-up-and-losing-oxygen-faster-than-oceans/" target="_blank" rel="noreferrer noopener">rivers</a> like the Ruki are crucial transportation corridors due to the challenging and often nonexistent road infrastructure. 



The river enables the movement of people and goods, facilitating trade and access to markets, health care, and education.



<h2 class="wp-block-heading" id="h-wildlife-of-the-ruki-river">Wildlife of the Ruki River </h2>



The region around the Ruki River is home to diverse wildlife. It is part of the Congo Basin, the second-largest tropical rainforest area in the world, which is a critical habitat for endangered species.



Among the most notable species are elephants and <a href="https://www.earth.com/news/study-mean-chimpanzees-fare-better-in-life-than-nice-ones/" target="_blank" rel="noreferrer noopener">chimpanzees</a>, whose populations thrive in the surrounding forests. Other primates such as bonobos also live in this region, making it a critical area for primate conservation.



The river itself is home to various species of fish that are crucial to local livelihoods. Hippopotamuses and crocodiles are often found in the water.



Birds like kingfishers, herons, and egrets frequent the riverbanks - making it a haven for birdwatchers.



The Ruki River also supports several species of reptiles and amphibians - some of which are unique to the region.



<h2 class="wp-block-heading" id="h-managing-the-river-s-resources">Managing the river's resources </h2>



The region faces several challenges, including <a href="https://www.earth.com/news/global-deforestation-directly-linked-to-atmospheric-mercury-emissions/" target="_blank" rel="noreferrer noopener">deforestation</a>, overfishing, and environmental degradation, which threaten its ecological balance and the livelihoods of people who depend on it. 



Efforts to manage and conserve the river's resources are vital for sustainable development.



Understanding and protecting the Ruki River and its surroundings are crucial for the DRC's environmental sustainability, economic development, and the well-being of its communities.



<h2 class="wp-block-heading" id="h-landscapes-of-the-drc">Landscapes of the DRC</h2>



The Democratic Republic of Congo (DRC) boasts some of the most diverse and breathtaking landscapes in Africa, reflecting its vast size and ecological richness. Dominated by the Congo Basin, the country is a haven for biodiversity.



Beyond its rainforests, the DRC's landscapes shift dramatically. In the east, the terrain rises into rugged mountains, including the Virunga and Rwenzori ranges, where snow-capped peaks like Mount Stanley pierce the sky. 



This region is also marked by active volcanoes such as Mount Nyiragongo, which harbors one of the world’s largest lava lakes, creating a dramatic and otherworldly spectacle.



To the south and west, the country transitions to expansive savannas with rolling grasslands and scattered trees. These areas contrast sharply with the lushness of the forests, providing vital habitats for species like lions and antelope. 



Rivers like the Ruki are a dominant feature, with the mighty Congo River coursing through the heart of the country. Its tributaries shape the lives of millions.



The image was captured by the OLI (Operational Land Imager) on Landsat 8.



Image Credit: NASA Earth Observatory&nbsp;



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Ruki River in the Democratic Republic of the Congo

Today's Image of the Day from the European Space Agency features a brilliant stellar nursery located about 163,000 light-years away.



According to ESA, the image is one of the most photogenic examples of the many stellar nurseries observed by the NASA/ESA Hubble Space Telescope during its 30-year lifetime. 



“The portrait features the giant nebula NGC 2014 and its neighbor NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



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



Stellar nurseries are regions in space where new stars are <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">born</a> - often within vast clouds of gas and dust called molecular clouds.&nbsp;



These areas are fascinating because they are cradles of stellar evolution, where gravity causes clumps of gas to collapse, eventually forming protostars.&nbsp;



Over time, the protostars will heat up and start the nuclear fusion process that powers a star.



One of the most well-known stellar nurseries is the Orion Nebula, which is visible to the naked eye and located about 1,350 light-years from Earth.&nbsp;



<h2 class="wp-block-heading" id="h-dynamic-nature-of-a-stellar-nursery-nbsp">Dynamic nature of a stellar nursery&nbsp;</h2>



Within these nurseries, the balance between gravity and pressure determines the types of stars that form, from massive, luminous stars to smaller, cooler ones like our Sun.&nbsp;



The environment is incredibly dynamic, with powerful winds from young stars shaping the clouds and triggering the birth of even more stars.



These regions are often illuminated by the light from massive newborn stars - creating stunning, colorful displays. The light reveals the intricate structure of the dust and gas, sculpted by the energy of young stars.&nbsp;



<h2 class="wp-block-heading" id="h-significance-of-stellar-nurseries-nbsp">Significance of stellar nurseries&nbsp;</h2>



Stellar nurseries are essential for understanding the early stages of planetary formation, as protoplanetary disks (the material from which <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planets form</a>) are often found around young stars in these regions.



Stellar nurseries play a crucial role in the ongoing evolution of <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">galaxies</a>. They are responsible for the continuous birth of new stars that enrich the interstellar medium with heavier elements. This constant recycling of material is key to the development of future generations of stars and planets.&nbsp;



Furthermore, the study of these regions helps astronomers understand the fundamental processes that govern the life cycles of stars and the overall dynamics of the universe.



<h2 class="wp-block-heading" id="h-the-local-group">The Local Group</h2>



The Local Group is a collection of over 80 galaxies that includes the Milky Way, the Andromeda Galaxy, and the Triangulum Galaxy, along with numerous smaller dwarf galaxies. These galaxies are bound together by gravity and span a region roughly 10 million light-years across.&nbsp;



The <a href="https://www.earth.com/news/milky-ways-thin-disk-is-billions-of-years-older-than-we-thought/" target="_blank" rel="noreferrer noopener">Milky Way</a> and Andromeda are the dominant members, with their respective satellite galaxies orbiting them.&nbsp;



The Local Group is part of a larger structure known as the Virgo Supercluster, and its galaxies are moving toward the gravitational center of the Local Group, contributing to its dynamic nature.&nbsp;



<h2 class="wp-block-heading" id="h-large-magellanic-cloud">Large Magellanic Cloud</h2>



The Large Magellanic Cloud (LMC) is the fourth largest galaxy in the Local Group and can be seen with the naked eye from the Southern Hemisphere.&nbsp;



This irregular dwarf galaxy is home to the Tarantula Nebula, one of the most active star-forming regions in our cosmic neighborhood.&nbsp;



The Large Magellanic Cloud played a key role in astronomical history, particularly when the supernova SN 1987A was observed, providing valuable insights into stellar evolution.&nbsp;



The LMC's interaction with the Milky Way, along with its own companion, the Small Magellanic Cloud, is believed to influence its shape and star formation activity. Its proximity and unique properties make it a crucial object of study for understanding <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>, star formation, and the dynamics of interacting galaxies.



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

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 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

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

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

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

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

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

A frozen Lake Erie in February

Aqua Earth Observing Satellite

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

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

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

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

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

Northern Italy from the Space Station

Photos from the International Space Station

We think about the foods we consume daily and the impact of our diets on our health, but how often do we consider the broader implications of these choices on the health of our planet?



Can shifting to more sustainable diets simultaneously tackle climate change and global food insecurity? This is a delicate balance to strike, but the answer is a resounding "yes."



Before diving into this, though, we ought to remember the words of Joe DeCesaro, a data analyst at <a href="https://www.ucsb.edu/" target="_blank" rel="noreferrer noopener">UC Santa Barbara</a>’s National Center for Ecological Analysis &amp; Synthesis (NCEAS).



“Changes in food demand in one part of the world can have cascading environmental and human welfare implications for people around the world,” he cautioned.



DeCesaro and his team at the NCEAS have conducted a fascinating study that aimed to understand the environmental implications of a major shift towards four distinct types of diets, globally.



<h2 class="wp-block-heading" id="h-environmental-impact-of-global-diet-shifts">Environmental impact of global diet shifts</h2>



The <a href="https://www.earth.com/news/global-food-system-is-unsustainable-and-must-be-transformed/" target="_blank" rel="noreferrer noopener">food system</a> is one of the largest contributors to environmental degradation worldwide, accounting for about a third of global greenhouse gas emissions and using more than 70% of freshwater resources.



Apart from this, agriculture causes significant land degradation and contributes to nutrient pollution in water bodies. 



One way to alleviate environmental pressure is to move towards more sustainable diets that reduce the consumption of resource-intensive food items, such as red meat, and increase the intake of nutrient-dense foods like vegetables and legumes.



Yet, DeCesaro's study reveals that diet change is only part of the solution. 



“We wanted to know who would actually be feeling the change from the food production if these shifts occur,” explained Ben Halpern, NCEAS director and a coauthor on the study.



The team, therefore, focused on understanding where and how environmental pressures might shift if global diets changed significantly.



<h2 class="wp-block-heading" id="h-strengths-and-weaknesses-of-different-diets">Strengths and weaknesses of different diets</h2>



The study analyzed the global impact of shifting to four types of diets: Indian, <a href="https://www.earth.com/news/mediterranean-diet-can-lead-to-longer-life/" target="_blank" rel="noreferrer noopener">Mediterranean</a>, EAT-Lancet (largely plant-based or "flexitarian"), and average government-recommended Food-Based Dietary Guidelines (FBDGs).



The Indian diet emerged as the most beneficial, potentially leading to a 20.9% reduction in food production-based environmental pressure. In contrast, following FBDGs could result in a 35.2% increase in global environmental pressure.



The researchers utilized extensive data, including each country's average diets, trade flows, and the environmental pressures of food production worldwide.



“The research was motivated originally by the question: Who’s consumption is generating the pressures of food production that are being felt by people and places around the world?” explained DeCesaro.



“Are poorer countries paying the environmental price of producing higher pressure foods that are being eaten by richer countries, or vice versa?" 



"Our methods allow us to track changes in the environmental pressures from the producer to the consumer, and vice versa, in a standardized format across four pressures. Our work is quite novel in this space.”



The study found that the Indian diet - primarily due to its recommendation of zero <a href="https://www.earth.com/news/wild-seafood-has-one-sixth-the-carbon-footprint-of-red-meat/" target="_blank" rel="noreferrer noopener">red meat</a> - was the most effective in reducing global cumulative pressure on environments.



This sharply contrasted with FBDGs, which typically recommend more red meat than what many countries currently consume.



<h2 class="wp-block-heading" id="h-learning-from-high-income-countries">Learning from high-income countries</h2>



Interestingly, the study revealed that the majority of the reductions in global environmental pressure would come from high-income countries. 



“Higher-income countries’ average current diets have higher consumption quantities of most food categories than the recommended quantities in our diet scenarios,” said DeCesaro. 



This indicates that these countries are over-consuming, suggesting the potential for significant reductions in environmental pressure through <a href="https://www.earth.com/news/healthy-dietary-shifts-could-keep-global-climate-goals-within-reach/" target="_blank" rel="noreferrer noopener">dietary shifts</a>.



<h2 class="wp-block-heading" id="h-sharing-sustainable-practices">Sharing sustainable practices</h2>



The research also revealed that a shift towards more sustainable, plant-forward diets could increase food-production-related environmental pressures in lower-income countries. 



However, DeCesaro noted, this increase is primarily due to these diets meeting more of the people's daily needs.



To ensure food security and equitable access to nutrition, he suggested that wealthier countries support by providing access to efficiently produced food imports and encouraging economic development to improve dietary health. This support could also include reducing environmental pressures from food production, promoting innovation and sharing sustainable food production practices.



In conclusion, the message, as summarized by Halpern, is clear: “The decisions we make about <a href="https://www.earth.com/news/hundreds-of-genes-identified-that-directly-influence-what-we-eat/" target="_blank" rel="noreferrer noopener">what we eat</a> are important for reducing our environmental footprint, but other people may pay the price for those decisions.”



The study is published in the journal <a href="https://iopscience.iop.org/article/10.1088/1748-9326/ad8509">Environmental Research Letters</a>.



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Global diet shifts: The hidden costs of what we eat

We think about the foods we consume daily and the...

For a very long time, we have been under the impression that memory and learning are solely the brain's forte. Central to this belief is the fact that our brains, particularly our brain cells, store memories.



However, an innovative team of researchers begs to differ, suggesting that cells in other parts of the body partake in this memory function too.



The ability of non-brain cells to learn and form memories is a riveting discovery. 



This thought-provoking study provides us with a new understanding of memory's mechanisms and paves the way for potential advancements in learning and memory-related afflictions treatment.



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



Memory is like your brain’s personal filing system. When you experience something new -- like meeting a friend or learning a fact -- your brain encodes that information by turning it into patterns of neural activity. 



These patterns get stored in different parts of your brain, depending on what type of information it is. For example, <a href="https://www.earth.com/news/how-human-brain-decides-which-memories-to-remember/" target="_blank" rel="noreferrer noopener">visual memories</a> might be stored in areas responsible for processing images, while facts and numbers find their way into regions that handle language and logic.



Retrieving memories happens when your brain needs to access those stored patterns. It’s similar to searching for a file on your computer. 



If you want to remember your friend’s birthday, your brain activates the relevant neural pathways to bring that information back into your <a href="https://www.earth.com/news/consciousness-may-stem-from-unseen-dimensions-beyond-our-reality/" target="_blank" rel="noreferrer noopener">conscious mind</a>. 



Sometimes, this process is seamless, but other times memories can be a bit fuzzy or mixed up, especially if they’re not accessed frequently. That’s why you might struggle to recall something you haven’t thought about in a while.



Your memory isn’t perfect, and it can change over time. Each time you recall a memory, your brain might update it with new <a href="https://www.earth.com/news/unlocking-memories-with-scents-may-help-treat-depression/" target="_blank" rel="noreferrer noopener">information or emotions</a>, which can make the memory stronger or slightly different from the original event. Factors like sleep, stress, and even nutrition can influence how well your memory works.



<h2 class="wp-block-heading" id="h-memory-formation-and-cells">Memory formation and cells</h2>



“Learning and memory are generally associated with brains and brain cells alone, but our study shows that other cells in the body can learn and <a href="https://www.earth.com/news/memory-is-shaped-by-both-past-and-future-experience-and-events/" target="_blank" rel="noreferrer noopener">form memories</a>, too,” explains New York University’s&nbsp;<a href="https://liberalstudies.nyu.edu/about/faculty-listing/nikolay-kukushkin.html" target="_blank" rel="noreferrer noopener">Nikolay V. Kukushkin</a>, the lead author of the&nbsp;study.&nbsp;



The goal of the research was straightforward -- to investigate if non-brain cells contribute to memory. To do this, the scientists deployed the time-honored neurological property, known as the massed-space effect.



This principle asserts that our retention capacity is better when information is studied in spaced intervals rather than crammed into a single, intensive session.



Does this strike a chord? We have all experienced the futility of last-minute cramming before tests.



<h2 class="wp-block-heading" id="h-memory-test-in-non-brain-cells">Memory test in non-brain cells</h2>



In this study, the scientists simulated the process of spaced learning by examining two types of non-brain human cells -- one from nerve tissue and one from kidney tissue -- in a laboratory setting.



These cells were exposed to varying patterns of chemical signals, akin to the exposure of brain cells to neurotransmitter patterns when we learn new information.



The intriguing part? These non-brain cells also switched on a "memory gene" - the same gene that brain cells activate when they detect information patterns and reorganize their connections to form memories.



So, how exactly did the scientists gauge the memory and learning process? 



They ingeniously engineered the non-brain cells to generate a glowing protein, which indicated whether the memory gene was active or dormant.



<h2 class="wp-block-heading" id="h-memory-cells-learning-and-pulses">Memory cells, learning, and pulses</h2>



The results of this innovative research were nothing short of astounding. 



It turned out that these cells were able to discern when the chemical pulses (simulating bursts of neurotransmitters in the brain) were repeated rather than simply prolonged -- much like neurons in our own brains when we opt for break-filled studying instead of continuous cramming.



When the pulses were delivered at intervals, they activated the "<a href="https://www.earth.com/news/sleep-is-essential-for-memory-formation/" target="_blank" rel="noreferrer noopener">memory</a> gene" more intensely and for a longer duration than when the same treatment was administered all at once - a perfect demonstration of the massed-space effect.



“This reflects the massed-space effect in action,” says Kukushkin, a clinical associate professor of life science at NYU Liberal Studies and a research fellow at NYU’s Center for Neural Science. 



“It shows that the ability to learn from spaced repetition isn't unique to brain cells, but, in fact, might be a fundamental property of all cells.”



<h2 class="wp-block-heading" id="h-understanding-how-memory-works">Understanding how memory works</h2>



Not only does this research on non-brain cells introduce fresh perspectives to study memory, but it also holds promise for potential health-related benefits.



“This discovery opens new doors for understanding how <a href="https://www.earth.com/news/how-does-our-brain-form-long-term-memories/" target="_blank" rel="noreferrer noopener">memory</a> works and could lead to better ways to enhance learning and treat memory problems,” notes Kukushkin.



“At the same time, it suggests that in the future, we will need to treat our body more like the brain -- for example, consider what our pancreas remembers about the pattern of our past meals to maintain healthy levels of blood glucose or consider what a cancer cell remembers about the pattern of chemotherapy.”



<h2 class="wp-block-heading" id="h-implications-of-this-research">Implications of this research</h2>



As we explore this fascinating new research on non-brain cells, the pressing question remains - how will this impact our <a href="https://www.earth.com/news/human-brains-create-three-copies-of-every-memory-we-make/" target="_blank" rel="noreferrer noopener">understanding of memory formation</a>?



What implications does this discovery hold for the future of learning and memory-related treatments? Only time will tell. 



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The research team also included Thomas Carew, a professor in NYU’s Center for Neural Science; Tasnim Tabassum, an NYU researcher; and Robert Carney, an NYU undergraduate researcher. The study was funded by a grant from the National Institutes of Health (R01-MH120300-01A1).



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-53922-x" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Memory is stored in cells throughout the body, not just the brain

For a very long time, we have been under the...

It's no secret that the global health community has been grappling with the catastrophic impacts of the COVID-19 pandemic since it arose in 2019. This disease has presented unprecedented challenges in treatment and prevention, and we still do not fully understand the behavior of the SARS-CoV-2 virus.



As of today, the World Health Organization has documented over 770 million COVID-19 cases worldwide, indicating the extensive reach and impact that this virus has had on global populations.



<h2 class="wp-block-heading" id="h-the-mystery-of-how-covid-19-travels">The mystery of how COVID-19 travels</h2>



While we have decent knowledge about how the <a href="https://www.earth.com/news/covid-19-virus-lingers-body-two-years-after-infection/" target="_blank" rel="noreferrer noopener">virus</a> enters our bodies - by attaching onto healthy cells in our nose and throat - there remains a level of mystery about how COVID-19 further travels and spreads once inside an airway, and how it contributes to severe illness and long-term complications.



But recently, thanks to extensive research efforts and collaborative studies, a new piece of the puzzle has been identified. The findings offer fresh insights that may inform future treatment strategies and preventive measures.



Scientists at <a href="https://www.nm.org/" target="_blank" rel="noreferrer noopener">Northwestern Medicine</a> embarked on a mission to uncover the mysteries of SARS-CoV-2 's proliferation in our bodies.



One of their most significant findings was that the virus uses our body's own mucus as its personal highway into the lower lungs.



<h2 class="wp-block-heading" id="h-mucus-the-unexpected-accomplice">Mucus: The unexpected accomplice</h2>



In their study, which was published recently in Nature Communications, the researchers performed live imaging on human bronchial epithelium cells after they were exposed to SARS-CoV-2 virus.



Their observations revealed the virus' cunning tactic - the movement of our own mucus helps the virus to travel inside the respiratory tract.



This eventually leads to the formation of <a href="https://www.earth.com/news/how-covid-19-is-transmitted-through-aerosols/" target="_blank" rel="noreferrer noopener">infectious aerosols</a>, which can further affect other individuals.



"The virus goes where the mucus goes," said Mark Becker, the leading student author of the study.



We generally understand mucus as a protective shield against infection, that traps viruses and other harmful particles before they can enter the tissues. Our own ciliated cells help to "sweep" dirty mucus upwards towards the throat, thus keeping the respiratory surfaces clean.



Ironically, when exploited by the SARS-CoV-2 virus , this protective defense becomes an accomplice that aids the spread after <a href="https://www.earth.com/news/covid-impacts-the-brain-through-inflammation-not-infection/" target="_blank" rel="noreferrer noopener">infection</a>.



<h2 class="wp-block-heading" id="h-covid-19-insights-and-future-research">COVID-19 insights and future research</h2>



While funding for COVID-19 related research has started to decrease, the experts remain hopeful. 



They believe their discovery of how COVID-19 travels could have substantial applications in the context of other viral diseases as well, specifically <a href="https://www.earth.com/news/genetic-variant-linked-to-both-covid-risk-and-hiv-protection/" target="_blank" rel="noreferrer noopener">HIV</a>.



"The mucosal environment most similar to the lungs is the upper female reproductive tract," noted study senior author Dr. Thomas Hope.



Perhaps, then, this understanding of how the virus that causes COVID-19 manoeuvres through the respiratory tract can open doors to new research on other diseases that may similarly exploit the supply of mucus.



<h2 class="wp-block-heading" id="h-a-story-of-scientific-innovation">A story of scientific innovation </h2>



The success of this study is also a reflection of the robust infrastructure and commitment at Northwestern Medicine.



"The university really supported us and that is a testament to what a great environment Northwestern Medicine is," noted Dr. Hope.



It's a story of scientific innovation, pushing the boundaries of our understanding of the virus that has turned our world upside down. And above all, it's about teamwork - because that's how scientific breakthroughs happen.



This research contributes to the ever-growing body of knowledge about COVID-19. It demonstrates the virus's surprisingly strategic use of our <a href="https://www.earth.com/news/reprogramming-the-immune-system-to-attack-cancer-cells/" target="_blank" rel="noreferrer noopener">body's own defenses</a>.



<h2 class="wp-block-heading" id="h-covid-19-insights-and-innovative-treatments">COVID-19 insights and innovative treatments</h2>



The newfound understanding of SARS-CoV-2's behavior in the mucosal environment has sparked interest in developing innovative treatment approaches.



Researchers are now looking at how this knowledge could be applied to create therapies that reinforce mucosal barriers, potentially preventing viral entry and spread. 



This type of preventive treatment could revolutionize how viral diseases are managed, particularly for infections that target mucosal tissues.



By focusing on fortifying the body’s first line of defense, scientists hope to reduce the severity and transmission of certain viral diseases.



Beyond COVID-19, these strategies could offer hope for combating other viruses that similarly exploit mucosal pathways, such as influenza and respiratory syncytial virus (RSV). 



The potential for cross-applicability means that advancements made now could lay the groundwork for a more resilient response to future viral outbreaks, and create a broad-spectrum approach to viral prevention and treatment.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-53791-4" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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How the COVID-19 virus travels deep inside our lungs

It's no secret that the global health community has been...

A prescription medication that has been available in the U.S. since 1992, which many people recognize for treating hair loss and enlarged prostate, seems to have another significant health benefit.



Recent research suggests that a drug called finasteride could lower cholesterol levels and reduce the risk of heart disease. That's a surprising twist for a drug that's been around for decades.



Curiosity led <a href="https://fshn.illinois.edu/directory/jaume6" target="_blank" rel="noreferrer noopener">Dr. Jaume Amengual</a>, an assistant professor in the Department of Food Science and Human Nutrition at the <a href="https://fshn.illinois.edu/" target="_blank" rel="noreferrer noopener">University of Illinois</a>, to explore this unexpected connection. 



After noticing something unusual in a national survey, he decided to dig deeper. 



"When we looked at the men taking finasteride in the survey, their <a href="https://www.earth.com/news/the-power-of-fish-oil-in-combating-high-cholesterol/" target="_blank" rel="noreferrer noopener">cholesterol levels</a> averaged 30 points lower than men not taking the drug. I thought we'd see the opposite pattern, so it was very interesting," Dr. Amengual enthused.



<h2 class="wp-block-heading" id="h-lowering-cholesterol-with-finasteride">Lowering cholesterol with finasteride?</h2>



The initial clue came from the <a href="https://www.cdc.gov/nchs/nhanes/index.htm" target="_blank" rel="noreferrer noopener">National Health and Nutrition Examination Survey</a> conducted between 2009 and 2016. 



This survey collects health information from thousands of Americans. In this data, men using finasteride as a <a href="https://www.earth.com/news/new-natural-cure-male-baldness-highly-effective-sugar-2-deoxy-d-ribose/" target="_blank" rel="noreferrer noopener">hair loss treatment</a> had significantly lower cholesterol levels compared to those who weren't on the medication. 



A 30-point difference is substantial and caught the researchers' attention. But observational studies have limitations. The sample size of men over 50 using finasteride was small. 



"This was not a clinical study in which you can control everything perfectly," Amengual noted. "It was more of an observation that led us to say, 'Okay, now we've seen this in people. Let's see what happens in mice.'"



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



To get a clearer picture, the team turned to laboratory mice. Doctoral student <a href="https://www.linkedin.com/in/donald-molina-ba3099197/?locale=es_ES" target="_blank" rel="noreferrer noopener">Donald Molina Chaves</a> conducted experiments on mice predisposed to <a href="https://www.earth.com/news/fathers-diets-impact-the-heart-health-of-their-daughters/" target="_blank" rel="noreferrer noopener">atherosclerosis</a> -- a condition where arteries narrow due to plaque buildup. 



The mice were fed different doses of finasteride along with a high-fat, high-cholesterol diet.



"Mice that were given a high dose of finasteride showed lower <a href="https://www.earth.com/news/certain-gut-bacteria-lower-cholesterol-and-the-risk-of-heart-disease/" target="_blank" rel="noreferrer noopener">cholesterol levels</a> within the plasma as well as in the arteries," Molina Chaves said. "There were also fewer lipids and inflammatory markers in the liver." 



These findings suggested that finasteride doesn't just lower cholesterol in the blood but might also <a href="https://www.earth.com/news/lifestyle-choices-in-young-adulthood-impact-cognitive-ability-in-midlife/" target="_blank" rel="noreferrer noopener">reduce inflammation</a> and plaque formation in arteries.



While the highest dose had significant effects, it's not a dose humans would take. 



"It's an incredibly high level of the drug. But we use mice as a model, and they are extremely resistant to things that would kill any of us," Amengual explained. "So it is not that wild when you think about it that way." 



The results in mice provide a direction for future human studies.



<h2 class="wp-block-heading" id="h-finasteride-testosterone-and-heart-disease">Finasteride, testosterone, and heart disease</h2>



So why would a hair loss drug affect <a href="https://www.earth.com/news/new-study-eating-eggs-is-not-bad-for-your-health-despite-years-of-warnings/" target="_blank" rel="noreferrer noopener">cholesterol levels</a>? It comes down to hormones. 



Finasteride works by blocking a protein that activates testosterone, specifically reducing levels of <a href="https://www.earth.com/news/men-with-low-testosterone-have-a-higher-risk-of-mortality/" target="_blank" rel="noreferrer noopener">dihydrotestosterone (DHT)</a>. DHT is linked to hair loss, prostate enlargement, and, as it turns out, possibly heart disease.



"I was reading about this medication one day, and I started to notice that there were not many long-term studies of the implications of the drug," Amengual said. 



"Initially, it was just my own curiosity, based on the fact that hormone levels are known to have an effect on atherosclerosis, hair loss, and prostate issues. So, we decided to dig into it."



Testosterone and its derivatives can influence the development of atherosclerosis. By altering these hormone levels, finasteride might indirectly impact cholesterol metabolism and inflammation, leading to improved <a href="https://www.earth.com/news/social-expectations-of-men-are-bad-for-their-heart-health/" target="_blank" rel="noreferrer noopener">heart health</a>.



<h2 class="wp-block-heading" id="h-more-surprises-from-finasteride">More surprises from finasteride</h2>



Interestingly, these findings might benefit more than just men dealing with hair loss or prostate issues. 



Transgender individuals undergoing hormone therapy often face a higher risk of heart disease due to hormonal changes. 



Finasteride is sometimes prescribed during gender transitions to manage hair loss triggered by hormone treatments.



"Over the past decade, doctors have started prescribing this drug for individuals transitioning either from male to female or female to male. In both cases, the hormonal changes can trigger hair loss," Amengual said. 



"The interesting thing is that transgender people are also at a higher risk of <a href="https://www.earth.com/news/depression-and-cardiovascular-diseases-are-genetically-linked/" target="_blank" rel="noreferrer noopener">cardiovascular diseases</a>. So this drug could have a potential beneficial effect to prevent cardiovascular disease not only in cis men, but also in transgender individuals."



This opens up the possibility that finasteride could serve a dual purpose for transgender patients, helping with hair loss while also reducing heart disease risk.



<h2 class="wp-block-heading" id="h-what-s-the-catch-understanding-finasteride-risks">What's the catch? Understanding finasteride risks</h2>



Of course, no medication is without risks. Finasteride can cause side effects, and it's important to consider them. 



Some users experience <a href="https://www.earth.com/news/men-exhibit-better-sexual-health-eating-a-plant-based-vegan-diet/" target="_blank" rel="noreferrer noopener">sexual side effects</a> like decreased libido, erectile dysfunction, and reduced ejaculate volume. These effects happen because finasteride reduces DHT, which plays a role in sexual function.



There have also been reports of psychological effects such as depression, anxiety, and mood changes. While not everyone experiences these, they're important to monitor. 



Physical side effects can include breast tenderness or enlargement, rashes, and swelling in the hands or feet. Rarely, finasteride can affect liver enzymes, so regular medical check-ups are recommended.



A small percentage of users report persistent side effects even after stopping the medication, a condition referred to as Post-Finasteride Syndrome (PFS). 



Symptoms can include ongoing sexual dysfunction and psychological issues. Research is ongoing to understand and address these concerns.



<h2 class="wp-block-heading" id="h-what-the-future-holds-for-finasteride">What the future holds for finasteride</h2>



These discoveries suggest that finasteride could have a role in heart health beyond its current uses. More research is needed, though. 



Clinical trials involving people would help determine if the cholesterol-lowering effects seen in mice also occur in humans at practical doses.



"This was not a clinical study in which you can control everything perfectly," Amengual emphasized. "It was more of an observation that led us to say, 'Okay, now we've seen this in people. Let's see what happens in mice.'"



If future studies confirm these benefits, finasteride could become part of a strategy to prevent <a href="https://www.earth.com/news/artificial-sweetener-erythritol-sugar-substitute-linked-to-blood-clots-heart-disease/" target="_blank" rel="noreferrer noopener">heart disease</a>, especially in populations at higher risk.



<h2 class="wp-block-heading" id="h-a-new-hope-proceed-with-eyes-wide-open">A new hope? Proceed with eyes wide open</h2>



Finasteride has been around for a while, helping many with hair loss and prostate issues. Now, it might have a new role to play in promoting heart health. 



This could be significant not just for men but also for the transgender community and others at risk of cardiovascular disease.



As with any medical treatment, it's crucial to consult healthcare providers before making changes. Finasteride's potential benefits must be balanced with its risks. But this research opens up exciting possibilities.



The full study was published in the&nbsp;<a href="https://www.jlr.org/article/S0022-2275(24)00012-9/fulltext" target="_blank" rel="noreferrer noopener">Journal of Lipid Research</a>.



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Old drug now called a "magic pill" because it regrows hair and improves heart health

A prescription medication that has been available in the U.S....

Color,Laser,Beams,Fantail,In,A,Haze

Can light itself, perhaps from a laser, cast a shadow? It might seem like a trick, but under certain conditions, the answer to this paradoxical question is "yes." 



Researchers have discovered that a laser beam can act like an opaque object, blocking another beam of light and creating a visible shadow. 



This finding challenges our traditional understanding of how light behaves.



"Laser light casting a shadow was previously thought impossible since light usually passes through other light without interacting," said Raphael A. Abrahao, the research team leader from <a href="https://www.bnl.gov/world/" target="_blank" rel="noreferrer noopener">Brookhaven National Laboratory</a> and the <a href="https://www.uottawa.ca/en" target="_blank" rel="noreferrer noopener">University of Ottawa</a>.



His team has opened the door to new ways of thinking about light and its interactions, pushing the boundaries of optics and could lead to innovative technologies that harness light in unexpected ways.



<h2 class="wp-block-heading" id="h-lasers-lights-and-lunch">Lasers, lights, and lunch</h2>



The idea started over a lunch conversation. 



Some scientists noticed that experimental schematics made with 3D visualization software depicted the shadow of a <a href="https://www.earth.com/news/earth-received-laser-communication-from-10-million-miles-away/" target="_blank" rel="noreferrer noopener">laser beam</a>, treating it as a solid cylinder rather than accounting for the physics of light. 



This sparked a lively discussion. 



"What started as a funny discussion over lunch led to a conversation on the physics of lasers and the nonlinear optical response of materials," remembered Abrahao. 



"From there, we decided to conduct an experiment to demonstrate the shadow of a <a href="https://www.earth.com/news/impossible-quantum-effects-observed-atoms-positioned-closely-together/" target="_blank" rel="noreferrer noopener">laser beam</a>."



<h2 class="wp-block-heading" id="h-making-laser-light-cast-a-shadow">Making laser light cast a shadow</h2>



To explore this curious idea, the team set up an experiment using a high-power green laser directed through a cube made of standard ruby crystal. 



At the same time, they illuminated the cube with a blue laser from the side. When the green laser entered the ruby, it changed the material's response to the <a href="https://www.earth.com/news/long-term-effects-of-artificial-blue-light-remain-unknown/" target="_blank" rel="noreferrer noopener">blue wavelength</a>. 



The interaction between the two light sources created a shadow on a screen -- a dark area where the green laser blocked the blue light.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/11/laser-beam-light_casing-shadow_credit-Optica_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/laser-beam-light_casing-shadow_credit-Optica_1s.webp" alt="Researchers showed that a laser beam can sometimes act like a solid object and cast a shadow that is visible to the naked eye. In the picture, the shadow appears as the horizontal line traversing the blue background. Credit: R. A. Abrahao, H. P. N. Morin, J. T. R. Pagé, A. Safari, R. W. Boyd, J. S. Lundeen" class="wp-image-1950880"/></a><figcaption class="wp-element-caption">Researchers showed that a laser beam can sometimes act like a solid object and cast a shadow that is visible to the naked eye. In the picture, the shadow appears as the horizontal line traversing the blue background. Credit: R. A. Abrahao, H. P. N. Morin, J. T. R. Pagé, A. Safari, R. W. Boyd, J. S. Lundeen</figcaption></figure>



The effect occurs due to a nonlinear optical process. Nonlinear optics involves light interacting with a material in an intensity-dependent way, allowing one light beam to influence another. 



"Our demonstration of a very counter-intuitive optical effect invites us to reconsider our notion of shadow," Abrahao explained. 



In this case, the green laser increased the optical absorption of the blue laser in the ruby crystal, creating a region where less blue light passed through -- essentially, a shadow.



<h2 class="wp-block-heading" id="h-very-cool-but-why-does-it-matter">Very cool, but why does it matter?</h2>



Nonlinear optics is a field that studies how light behaves in materials under high-intensity conditions. 



When light is intense enough, it can change the properties of the material it passes through, affecting how other light waves move through that material. 



This is different from linear optics, where light beams pass through each other without interaction.



"Our understanding of shadows has developed hand-in-hand with our understanding of light and optics," Abrahao noted. 



This new finding could prove useful in various applications such as <a href="https://www.earth.com/news/bose-einstein-condensate-bec-rare-form-quantum-matter-created-with-molecules/" target="_blank" rel="noreferrer noopener">optical switching</a> -- devices in which light controls the presence of another light -- or technologies that require precise control of light transmission, like high-power lasers. 



It could also impact the development of optical computing, where light is used instead of electricity to process information.



<h2 class="wp-block-heading" id="h-measuring-laser-light-s-shadow">Measuring laser light's shadow</h2>



The researchers measured the shadow's contrast based on the laser beam's power, finding a maximum contrast of approximately 22%. 



That's similar to the contrast of a tree's shadow on a sunny day. They also developed a theoretical model that accurately predicted the shadow contrast. 



This alignment between experiment and theory strengthens the validity of their findings.



The ability to control one light beam with another could lead to advances in <a href="https://www.earth.com/news/new-data-transmission-speed-record-set-by-scientists-using-optical-cables/" target="_blank" rel="noreferrer noopener">optical communication</a> and signal processing. 



For instance, optical switches that use light instead of electronic signals could operate at much higher speeds and with less energy loss. 



This discovery might also contribute to the development of new types of lasers with adjustable properties for use in medicine, manufacturing, or scientific research.



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



"This discovery expands our understanding of light-matter interactions and opens up new possibilities for utilizing light in ways we hadn’t considered before," Abrahao concluded. 



The team plans to investigate other materials and laser wavelengths that can produce similar effects. They are curious to see how different combinations might enhance or alter the shadow effect.



The notion that light can cast a shadow on light challenges fundamental ideas in physics. It invites scientists and engineers to rethink how we can manipulate light for advanced technologies. 



This discovery is a reminder that even well-established concepts can be revisited and that curiosity can lead to surprising insights.



From a casual conversation to a laboratory breakthrough, the journey of this discovery highlights the importance of questioning assumptions. The shadow of a laser beam is just one example of how much more there is to learn.



The full study was published in the journal <a href="https://opg.optica.org/optica/fulltext.cfm?uri=optica-11-11-1549&amp;id=563468" target="_blank" rel="noreferrer noopener">Optica</a>.



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If shadows are created by light, how can light cast its own shadow?

Can light itself, perhaps from a laser, cast a shadow?...

Ever pondered the extraordinary migratory journeys of birds? 



These feathered wanderers traverse thousands of kilometers, exhibiting an incredible knack for endurance and navigation that almost seems magical. 



In past research, the stars, the Sun and the Earth's magnetic field have all been implicated as means by which birds find their way to faraway places.



A recent study has shed new light on how birds use the magnetic field to navigate, and the findings challenge previously held beliefs.



<h2 class="wp-block-heading" id="h-the-science-behind-bird-migration">The science behind bird migration</h2>



The research was conducted by scientists from <a href="https://www.bangor.ac.uk/" target="_blank" rel="noreferrer noopener">Bangor University</a> in Wales, and focused on the migratory behavior of Eurasian reed warblers, which are small songbirds.



The study presents an intriguing hypothesis: these birds employ only the Earth's magnetic dip and variation to identify their position and set their direction.



This revelation is a significant stride away from the conventional belief that all aspects of the <a href="https://www.earth.com/news/earths-magnetic-field-is-shifting-and-putting-navigation-at-risk/" target="_blank" rel="noreferrer noopener">Earth's magnetic field</a>, particularly total intensity, are essential to precise navigation. 



For years, it was believed that birds carry a 'map-and-compass' navigation system. They identify their location using this "map," and the "<a href="https://www.earth.com/news/migratory-bats-use-earths-magnetic-field-as-a-compass/" target="_blank" rel="noreferrer noopener">compass</a>" aids in maintaining the correct direction towards their destination.



However, the precise nature of this 'map' has always been a topic of debate.



<h2 class="wp-block-heading" id="h-how-birds-respond-to-virtual-displacement">How birds respond to virtual displacement </h2>



The experiment involved subjecting the warblers to "virtual displacement."



The birds experienced artificially adjusted values of magnetic inclination (the dip angle of the field lines) and declination&nbsp;(the difference between the direction to the geographic and magnetic poles).



This simulation created the illusion of a geographic relocation while maintaining a consistent total magnetic intensity.



<h2 class="wp-block-heading" id="h-birds-use-certain-cues-to-navigate">Birds use certain cues to navigate</h2>



The results were nothing short of astonishing. Despite the simulated relocation, the birds recalibrated and redirected their <a href="https://www.earth.com/news/arctic-geese-adapt-by-finding-a-new-migratory-route/" target="_blank" rel="noreferrer noopener">migratory routes</a> as though they were in an entirely different location. 



This behavior suggests that birds can determine their position and direction using only certain magnetic cues, even if other aspects of the magnetic field, such as total intensity, remain unchanged.



"What's interesting is that these findings reveal that the birds don't necessarily need all components of the Earth's magnetic field to determine their position. They can rely solely on inclination and declination, which are also used in compass orientation, to extract their location," explained Professor Richard Holland, the study's leader, who specializes in animal behavior. 



<h2 class="wp-block-heading" id="h-new-understanding-of-how-birds-navigate">New understanding of how birds navigate</h2>



These findings indicate that birds are equipped with a sophisticated and adaptable internal navigation system.



This system allows them to adjust to environmental changes, even in situations they've never encountered before.



"It remains to be seen whether birds use the total intensity of the Earth's magnetic field for navigation in other contexts, but what we've shown is that these two components - magnetic <a href="https://www.earth.com/news/how-do-birds-know-when-its-time-to-stop-migrating/" target="_blank" rel="noreferrer noopener">inclination</a> and declination - are enough to provide positional information," stated Prof. Holland.



This study carves out exciting avenues for further research into animal navigation. It sets a solid foundation for broader biological studies, including into how animals decipher and interact with their environment.



<h2 class="wp-block-heading" id="h-evolutionary-advantage-of-magnetic-navigation">Evolutionary advantage of magnetic navigation</h2>



This newfound understanding of <a href="https://www.earth.com/news/bird-migration-is-influenced-by-social-relationships/" target="_blank" rel="noreferrer noopener">bird migration</a> and navigation raises questions about how these magnetic cues evolved and why they became central to avian migration.



The ability to rely on magnetic dip and variation could provide birds with a reliable, all-weather navigation system that ensures their survival across vast distances.



Unlike visual landmarks or celestial cues, magnetic fields are constant and unaffected by weather, providing an advantage in conditions where other methods might fail.



The evolutionary benefits of this specialized navigation system are immense. Birds that migrate successfully are better equipped to find food, suitable climates, and breeding grounds, thereby enhancing their chances of survival and reproduction.



This adaptability suggests that magnetic navigation may have been a critical trait for birds that traverse unpredictable environments, such as oceans or dense forests, where visual or auditory landmarks are scarce.



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



Moreover, understanding the mechanics behind this capability opens doors to potential applications in biomimicry and navigation technologies. 



Researchers may one day harness the principles behind avian magnetic navigation to develop new, eco-friendly navigation tools or improve current systems used in aviation and marine transport. 



This study highlights how much we still have to learn from nature's most seasoned travelers.



The full study was published in the journal <a href="https://royalsocietypublishing.org/doi/10.1098/rspb.2024.1363" target="_blank" rel="noreferrer noopener">Proceedings of the Royal Society B: Biological Sciences</a>.



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Birds navigate using clues from Earth's magnetic field

Ever pondered the extraordinary migratory journeys of birds? These feathered...

Beautiful,Night,Landscape,,Old,Volcano,,Crater,Lake.,The,Colorful,Star

From the tiniest fluctuations after the Big Bang, gravity has orchestrated the formation of galaxies, stars, and planets, creating the vast cosmic web we see today.



Gravity isn't just what keeps us grounded -- it's been shaping the universe since its earliest days. Recent studies have provided the most precise tests of gravity on the grandest scales imaginable. 



By examining how cosmic structures have grown over the past 11 billion years, scientists have confirmed that gravity behaves just as <a href="https://www.earth.com/news/cosmic-glitch-in-gravity-expands-the-theory-of-general-relativity/" target="_blank" rel="noreferrer noopener">Einstein's theory</a> of general relativity predicts, even across billions of light-years.



<h2 class="wp-block-heading" id="h-desi-tracks-gravity-over-11-billion-years">DESI tracks gravity over 11 billion years</h2>



Pauline Zarrouk, a cosmologist at the French National Center for Scientific Research (<a href="https://www.cnrs.fr/en" target="_blank" rel="noreferrer noopener">CNRS</a>) working at the Laboratory of Nuclear and High-Energy Physics (LPNHE), has been exploring this cosmic evolution.



In collaboration with the international team behind the Dark Energy Spectroscopic Instrument (<a href="https://www.desi.lbl.gov/" target="_blank" rel="noreferrer noopener">DESI</a>), Zarrouk and her colleagues have traced how cosmic structures grew over the past 11 billion years.



Using data from DESI, the researchers provided the most precise test to date of gravity on the largest scales. 



"General relativity has been very well tested at the scale of solar systems, but we also needed to test that our assumption works at much larger scales," Zarrouk explained. 



"Studying the rate at which galaxies formed lets us directly test our theories and, so far, we're lining up with what <a href="https://www.earth.com/news/radical-new-theory-finally-unites-gravity-spacetime-and-the-quantum-realm/" target="_blank" rel="noreferrer noopener">general relativity</a> predicts at cosmological scales."



<h2 class="wp-block-heading" id="h-einstein-is-smiling-from-the-grave">Einstein is smiling from the grave</h2>



Their findings confirm that gravity behaves as Einstein's theory of general relativity predicts, even across the immense distances of the universe. 



This validation supports our leading model of the cosmos and narrows down alternative theories of gravity that have been proposed to explain puzzling observations, like the <a href="https://www.earth.com/news/universe-expansion-rate-dark-energy-measured-11-billion-years-ago/" target="_blank" rel="noreferrer noopener">accelerating expansion</a> of the universe often attributed to dark energy.



The study also sheds light on <a href="https://www.earth.com/news/quantum-gravity-search-south-pole-neutrinos-experiment/" target="_blank" rel="noreferrer noopener">neutrinos</a> -- the elusive particles that zip through space almost undetected. 



Previous experiments determined that the combined mass of the three types of neutrinos should be at least 0.059 electron volts (eV/c²). For perspective, an electron has a mass of about 511,000 eV/c². 



DESI's results suggest that the total mass of neutrinos should be less than 0.071 eV/c², tightening the constraints on these mysterious particles.



<h2 class="wp-block-heading" id="h-desi-gravity-and-cosmic-structure">DESI, gravity, and cosmic structure</h2>



"Both our BAO results and the full-shape analysis are spectacular," said Dragan Huterer, a professor at the <a href="https://umich.edu/" target="_blank" rel="noreferrer noopener">University of Michigan</a> and co-lead of DESI's group interpreting the cosmological data. 



"This is the first time that DESI has looked at the growth of cosmic structure. We're showing a tremendous new ability to probe modified gravity and improve constraints on models of <a href="https://www.earth.com/news/dark-energy-is-ripping-the-universe-apart-but-we-arent-sure-how/" target="_blank" rel="noreferrer noopener">dark energy</a>. And it's only the tip of the iceberg."



DESI is no ordinary telescope. Mounted on the Nicholas U. Mayall 4-meter Telescope at <a href="https://kpno.noirlab.edu/" target="_blank" rel="noreferrer noopener">Kitt Peak National Observatory</a>, it's capable of capturing light from 5,000 galaxies at once. 



Funded by the DOE Office of Science, the project is now in its fourth year of surveying the sky and aims to collect data from roughly 40 million galaxies and quasars by the time it's done.



<a href="https://www.earth.com/news/theory-gravity-exists-without-mass-so-dark-matter-does-not-exist/" target="_blank" rel="noreferrer noopener">Testing gravity</a> at cosmic scales is crucial. While Einstein's theory has passed every test within our solar system, there's always the possibility that it might behave differently across the vastness of space. 



By confirming that gravity acts as expected over billions of light-years, scientists can be more confident in their models of how the universe has evolved. 



<h2 class="wp-block-heading" id="h-interpreting-the-desi-data">Interpreting the DESI data</h2>



<a href="https://profiles.utdallas.edu/mishak">Dr. Mustapha Ishak-Boushaki</a>, a professor of physics in the <a href="https://nsm.utdallas.edu/">School of Natural Sciences and Mathematics</a> at UT Dallas, co-led the DESI working group that interpreted the cosmological data.



“For this round of DESI results, I focused my efforts at UT Dallas on conducting a large part of the analysis on gravity, which puts constraints on how matter in the universe moves and how large-scale structures, such as clusters of galaxies, evolve,” explained Ishak-Boushaki. 



“The results from DESI, combined with datasets from other experiments, are consistent with general relativity theory operating at cosmic scales, although they do not completely exclude other theories of <a href="https://www.earth.com/news/central-theory-of-quantum-gravity-is-modeled-in-the-laboratory/" target="_blank" rel="noreferrer noopener">modified gravity</a>.”



The new results provide an extended analysis of <a href="https://news.utdallas.edu/science-technology/desi-findings-2024/" target="_blank" rel="noreferrer noopener">DESI’s first year of data</a>, which in April contributed to the largest 3D map of the universe to date and revealed hints that <a href="https://newscenter.lbl.gov/2024/04/04/desi-first-results-make-most-precise-measurement-of-expanding-universe/" target="_blank" rel="noreferrer noopener">dark energy might be evolving</a> over time.



“The latest analysis is also consistent with our previous findings that give preference to the theory that <a href="https://www.earth.com/news/dark-energy-could-explain-the-rapid-expansion-of-the-early-universe/" target="_blank" rel="noreferrer noopener">dark energy</a> is not constant, but dynamic, which is a very important result for cosmic acceleration,” Ishak-Boushaki said.



<h2 class="wp-block-heading" id="h-how-did-this-happen">How did this happen?</h2>



The collaboration is currently analyzing data from the first three years and expects to present updated measurements of <a href="https://www.earth.com/news/new-evidence-suggests-that-dark-energy-comes-from-black-holes/" target="_blank" rel="noreferrer noopener">dark energy</a> and the universe's expansion history by spring 2025. 



The recent results align with earlier hints that dark energy might be evolving over time, adding to the excitement for what's to come.



"Dark matter makes up about a quarter of the universe, and dark energy makes up another 70 percent, and we don't really know what either one is," said Mark Maus, a PhD student at <a href="https://www.lbl.gov/" target="_blank" rel="noreferrer noopener">Berkeley Lab</a> and UC Berkeley who worked on theory and validation modeling pipelines for the new analysis. 



"The idea that we can take pictures of the universe and tackle these big, fundamental questions is mind-blowing."



The study utilized nearly 6 million <a href="https://www.earth.com/news/lonely-quasars-in-the-early-universe-cannot-be-explained/" target="_blank" rel="noreferrer noopener">galaxies and quasars</a>, allowing researchers to peer up to 11 billion years into the past. 



<h2 class="wp-block-heading" id="h-what-s-next-for-desi-and-gravity">What's next for DESI and gravity?</h2>



To sum it all up, with just one year of data, DESI has made the most precise overall measurement of the growth of cosmic structures, surpassing previous efforts that took decades.



The DESI project is remarkable not just for its technological capabilities but also for its collaborative spirit. 



With over 900 researchers from more than 70 institutions worldwide, it's a testament to what can be achieved when the global scientific community comes together.



As we await the next round of results, one can't help but wonder: What other secrets of the universe are waiting to be uncovered? 



The quest to understand gravity, dark matter, and dark energy continues, and each new discovery brings us a little closer to unraveling the mysteries of the cosmos.



The full study was published in <a href="https://data.desi.lbl.gov/doc/papers/">several scientific journals</a>.



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"Mind-blowing" gravity discovery proves Einstein right again

From the tiniest fluctuations after the Big Bang, gravity has...

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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



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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



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Detecting mercury contamination with the tap of a finger

[sendtonews key="LvS8v8bp9z-2564889-12187" 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 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

[sendtonews key="iuA5mpp3jv-1641775-12187" type="single"] Today’s Video of the Day from the...

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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

[sendtonews key="QGPzYnXEtN-1712599-12187" type="single"] Today’s Video of the Day from Carl...