Photo Credit: Win McNamee/Getty Images

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

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...

Today's Image of the Day from the European Space Agency features the star-forming region NGC 604. The nebula is located 2.73 million light-years away from Earth in the Triangulum Galaxy (M33). 



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 that 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.&nbsp;



<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 the European Space Agency features a stunningly beautiful photo of the Hainan Strait. The image was captured by the Copernicus Sentinel-2 satellite as it orbited over southern China.



“The Hainan Strait, or Qiongzhou Strait, separates Guangdong's Leizhou Peninsula on China’s mainland to the north and the island province of Hainan to the south. It also connects the Gulf of Tonkin on the west to the South China Sea on the east,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



<h2 class="wp-block-heading" id="h-hainan-strait-nbsp">Hainan Strait&nbsp;</h2>



The Hainan Strait is narrow and shallow. At its narrowest point, the strait is about 19 miles wide. Despite this, the Hainan Strait is a busy route for shipping and transportation. It's also vital to local <a href="https://www.earth.com/news/dark-fleets-hidden-industrial-fishing-activity-exposed/" target="_blank" rel="noreferrer noopener">fishing</a> industries.



ESA pointed out that in the image, the water along the coasts is light brown due to sediment runoff. 



“The curved Leizhou Peninsula juts southward into the South China Sea. The largest island on the east coast, Donghai, forms two bays: Leizhou Bay to its south and Zhanjiang Bay to its north," noted ESA.



“Facing both bays are cities with the same names: Zhanjiang, the largest city on the peninsula, and Leizhou, which gave the peninsula its name." 



"Hainan Island dominates the bottom part of the image. The name Hainan means ‘south of the sea,’ reflecting the island's position south of the strait.”



<h2 class="wp-block-heading" id="h-history-of-hainan-island">History of Hainan Island </h2>



During the Mesozoic Era about 100 million years ago, Hainan Island was actually part of a larger landmass connected to <a href="https://www.earth.com/news/denisovan-tooth-suggests-southeast-asia-was-a-human-diversity-hotspot/" target="_blank" rel="noreferrer noopener">Southeast Asia</a>. 



<h3 class="wp-block-heading" id="h-geological-features">Geological features</h3>



Over time, the movements of Earth's plates caused this landmass to break apart and drift. Hainan separated from the continental shelf near Vietnam and moved to its current position.



This tectonic activity not only shaped the island's current location but also influenced its geological features. Hainan's landscape is characterized by <a href="https://www.earth.com/news/how-and-why-do-mountains-form-new-theories-for-an-age-old-mystery/" target="_blank" rel="noreferrer noopener">mountains</a>, volcanic formations, and rich mineral deposits, which are direct results of these ancient geological processes.



Understanding this geological history helps explain why Hainan Island has such unique and diverse natural features compared to the mainland of China and nearby regions. The island's distinct wildlife and terrain make it a fascinating subject for geologists and natural historians alike.



<h3 class="wp-block-heading" id="h-cultural-diversity-nbsp">Cultural diversity&nbsp;</h3>



Hainan was once a remote and undeveloped part of China. It was used as a place of exile for disgraced officials during imperial times. 



However, it was also a place where diverse <a href="https://www.earth.com/news/humans-are-not-the-only-animals-that-create-their-own-culture/" target="_blank" rel="noreferrer noopener">cultures</a> met, as evidenced by the many ethnic groups that live there, including the Li people, who are indigenous to the island.



The island really started to change in the 20th century. During the Second Sino-Japanese War, Hainan was occupied by Japanese forces, which had a significant impact on its development. After the war, it became a part of the People’s Republic of China in 1950.&nbsp;



<h3 class="wp-block-heading" id="h-rapid-development-nbsp">Rapid development&nbsp;</h3>



In the 1980s, Hainan was designated a Special Economic Zone (SEZ), which marked the beginning of its transformation into a major economic and tourist hub. 



The SEZ status attracted significant investment and spurred rapid development, particularly in the capital city of Haikou and the resort city of Sanya.



Today, Hainan is known for its lush landscapes, tropical <a href="https://www.earth.com/news/caribbean-salt-affects-global-climate-study-reveals/" target="_blank" rel="noreferrer noopener">climate</a>, and booming tourism industry. It's also becoming a key player in China's efforts to develop its free trade zones, aiming to become a major center for trade and commerce in the region.



Image Credit: ESA/ Copernicus Sentinel-2&nbsp;



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Hainan Strait in southern China

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. 



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.&nbsp;



<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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Starburst galaxy in the constellation Columba

Today's Image of the Day from the European Space Agency features Messier 78 (M78), a reflection nebula located in the constellation Orion about 1,350 light-years away from Earth. 



This image was released as part of the initial series of observations from ESA's <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid space mission</a>.&nbsp;



All data collected during these early observations, including a series of incredible <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid/Euclid_s_first_images_the_dazzling_edge_of_darkness" target="_blank" rel="noreferrer noopener">new views</a> of the nearby universe, is available to the public. 



<h2 class="wp-block-heading" id="h-image-of-messier-78">Image of Messier 78</h2>



Featured here is a high-resolution, detailed segment of a larger image showcasing Messier 78, a dynamic region of star formation obscured by cosmic dust.&nbsp;



This specific view highlights how young stars generate winds of charged particles, carving out “cavities” in the molecular clouds around them.&nbsp;



The blue hues in the image represent ionized atomic hydrogen, which is a primary component of the cloud, while the red indicates the absorption and scattering of light by dust particles.



The image captures hundreds of stars varying in brightness, illuminating their nebulous, purple surroundings. A dark, arch-like structure stretches from the upper left to the bottom right of the frame, merging into the densest, darkest clouds at the image’s base.



<h2 class="wp-block-heading" id="h-active-site-of-star-formation-nbsp">Active site of star formation&nbsp;</h2>



Messier 78 is not just a single nebula but part of a larger complex of stars and nebulous regions in <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a>, which includes various other objects like dark nebulae that are visible as patches blocking light from behind.



This region is an active site of star formation, featuring many young stars and protostars, which are stars in the early stages of formation.&nbsp;



<h2 class="wp-block-heading" id="h-viewing-messier-78">Viewing Messier 78</h2>



M78 is easily observable with small telescopes, and it appears as a hazy patch of light with two prominent stars near its center, which illuminate the surrounding dust.&nbsp;



The nebula is also a favorite among amateur astronomers for its beauty and relatively bright appearance.



<h2 class="wp-block-heading" id="h-subject-of-scientific-interest-nbsp">Subject of scientific interest&nbsp;</h2>



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <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> and interstellar matter.&nbsp;



The nebula consists of dense, cold gas and dust, which are essential ingredients for the birth of new stars.&nbsp;



The intense blue light that characterizes M78 is due to the reflection of starlight off these dust particles, a process known as scattering.



<h2 class="wp-block-heading" id="h-region-surrounding-messier-78-nbsp">Region surrounding Messier 78&nbsp;</h2>



The region surrounding M78 includes several other interesting features. For instance, there are Herbig-Haro objects within it, which are small patches of nebulosity associated with <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">newly born stars</a>.&nbsp;



These objects are formed when gas ejected by young stars collides with clouds of gas and dust at high speeds, creating shock waves that glow brightly.



<h2 class="wp-block-heading" id="h-earliest-stages-of-star-development-nbsp">Earliest stages of star development&nbsp;</h2>



Additionally, infrared observations of M78 have revealed much about the dust and colder objects in the area, which are not visible in optical light.&nbsp;



The observations have helped astronomers identify numerous young stars and brown dwarfs (objects that are too large to be planets and too small to be stars) within the nebula. 



This makes M78 a critical area for studying the earliest stages of star development and the properties of the interstellar medium.



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp-0">Euclid space mission&nbsp;</h2>



The <a href="https://www.earth.com/news/new-batch-of-brilliant-images-from-the-euclid-mission-live-up-to-the-hype/" target="_blank" rel="noreferrer noopener">Euclid space mission</a> is a European Space Agency (ESA) mission designed to study the dark universe, particularly focusing on dark energy and dark matter, which are fundamental components that are believed to drive the accelerating expansion of the universe and shape its large-scale structure.&nbsp;



The mission aims to map the geometry of the dark universe and better understand the physics of the cosmos.



<h3 class="wp-block-heading" id="h-observing-billions-of-galaxies-nbsp">Observing billions of galaxies&nbsp;</h3>



Euclid uses two primary scientific instruments: a visible light camera (VIS) and a near-infrared spectrometer and photometer (NISP).&nbsp;



These instruments will allow Euclid to measure the shapes and redshifts of galaxies at distances of up to 10 billion light-years. By surveying more than a third of the sky, the mission is expected to observe several billion galaxies.



<h3 class="wp-block-heading" id="h-studying-the-dark-universe-nbsp">Studying the dark universe&nbsp;</h3>



The data collected will help astronomers in studying the effects of dark matter and dark energy in depth, testing cosmological models, and exploring new theories about the nature of the universe.&nbsp;



The mission, named after the ancient Greek mathematician Euclid, seeks to address key questions related to the structure of the universe and the fundamental laws of physics governing its evolution and expansion.



Image Credit: European Space Agency&nbsp;



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Messier 78: Young stars shine through dense dust

Today's Image of the Day from the European Space Agency features a galaxy that is located about 600 million light-years away in the constellation Gemini. The Hubble Space Telescope observed a supernova in this galaxy - which appears as a bright blue dot in the photograph.



“This picture was taken roughly two months after a supernova named SN 2022aajn was discovered in this galaxy. The supernova is visible as a blue dot at the center of the image, brightening the hazy body of the galaxy,” noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



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



Supernovae are spectacular explosions marking the violent deaths of stars. These cosmic events are so luminous they can briefly outshine entire <a href="https://www.earth.com/news/galaxies-are-much-bigger-than-we-originally-believed-gas-clouds/" target="_blank" rel="noreferrer noopener">galaxies</a> and radiate more energy in a few weeks than our Sun will in its entire lifetime.&nbsp;



Supernovae explosions release heavy elements like carbon, oxygen, and iron into the interstellar medium. This stellar debris becomes the building blocks for new stars, planets, and even life itself. 



Supernovae also produce neutron stars or black holes, depending on the remaining core’s mass after the explosion.



<h2 class="wp-block-heading" id="h-types-of-supernovae-nbsp">Types of supernovae&nbsp;</h2>



There are two main types of supernovae, classified based on their causes. Type I supernovae occur when a <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/" target="_blank" rel="noreferrer noopener">white dwarf</a> in a binary system accretes material from its companion star, eventually reaching a critical mass and triggering a runaway nuclear reaction.&nbsp;



Type II supernovae happen when a massive star, at least eight times the mass of the Sun, exhausts its nuclear fuel. Unable to support its own gravity, the core collapses, resulting in a massive explosion that ejects the outer layers into space.



<h2 class="wp-block-heading" id="h-measuring-the-distance-to-faraway-galaxies-nbsp">Measuring the distance to faraway galaxies&nbsp;</h2>



According to ESA, SN 2022aajn is a Type Ia supernova. “Supernovae of this type help astronomers measure the distance to faraway galaxies. This is possible because Type Ia supernovae are thought to be of the same intrinsic luminosity - no matter how bright they seem from Earth, they put out the same amount of light as other Type Ia supernovae.”



This means that researchers can calculate the distance to the supernova and its host galaxy by comparing the observed brightness to the expected brightness.



“This seemingly simple measurement method is complicated by cosmic dust. The farther away a supernova is, the fainter and redder it will appear - but intergalactic dust can make a supernova appear fainter and redder as well,” explained ESA.



“To understand this complication, researchers will use Hubble to survey a total of 100 Type Ia supernovae in seven wavelength bands from the ultraviolet to the near-infrared.”



By analyzing the brightness of supernovae across multiple wavelengths, researchers can distinguish between the influences of dust and distance, refining our measurements of galaxies that exist billions of light-years away.



<h2 class="wp-block-heading" id="h-how-many-galaxies-exist">How many galaxies exist?</h2>



The number of galaxies in the universe is estimated to be around two trillion, based on observations from Hubble and more recent data from the James Webb Space Telescope. 



This estimate is derived from deep-field surveys that reveal countless galaxies, each containing billions to trillions of <a href="https://www.earth.com/news/interstellar-tunnel-found-that-connects-our-solar-system-to-other-stars/" target="_blank" rel="noreferrer noopener">stars</a>.&nbsp;



However, because our observations are limited by current technology and the vastness of the cosmos, the actual number could be even higher.&nbsp;



Many <a href="https://www.earth.com/news/ancient-galaxies-formed-from-the-earliest-elements-in-the-universe/" target="_blank" rel="noreferrer noopener">galaxies</a> remain unseen due to their extreme distances, faintness, or obstruction by cosmic dust.



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



Gemini is one of the 12 zodiac constellations and is best known for representing the mythological twins Castor and Pollux. It is located in the northern celestial hemisphere and is most visible during winter in the Northern Hemisphere.&nbsp;



The constellation is bordered by Taurus to the west, Cancer to the east, and Orion to the south.



The two brightest stars in Gemini - Castor and Pollux - represent the heads of the twins and are easy to spot. Pollux, the brighter of the two, is an orange giant star about 34 light-years from Earth, while Castor is a more complex system made up of six stars. 



The constellation also contains several notable deep-sky objects, including the open cluster Messier 35, which is a beautiful collection of young stars located near Gemini’s western border.



Image Credit: ESA&nbsp;



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Hubble spots a supernova in the constellation Gemini 

Today's Image of the Day from the European Space Agency features the Cat's Eye Nebula (NGC 6543), located about 3,300 light-years from Earth in the constellation Draco.&nbsp;



The nebula's name comes from its eye-like appearance when viewed through a telescope. This particular image, which reveals the <a href="https://www.earth.com/news/horsehead-nebula-webb-telescope-captured-unprecedented-detail/" target="_blank" rel="noreferrer noopener">nebula</a> in stunning detail, was captured by the NASA/ESA Hubble Space Telescope.



<h2 class="wp-block-heading" id="h-complex-planetary-nebula">Complex planetary nebula </h2>



According to ESA, the Cat's Eye Nebula is one of the most complex planetary nebulae that has ever been discovered.



“A planetary nebula forms when Sun-like stars gently eject their outer gaseous layers to form bright nebulae with amazing twisted shapes," explained <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Until recently, it was thought that shells around planetary nebulae were a rare phenomenon. However, astronomers have instead shown that these rings are likely to be the rule rather than the exception."



<h2 class="wp-block-heading" id="h-appearance-of-the-cat-s-eye-nebula-nbsp">Appearance of the Cat's Eye Nebula&nbsp;</h2>



The central focus of the Cat's Eye is a hot, dying star that has shed its outer layers to form 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>. It is surrounded by concentric gas shells, jets of high-speed gas, and unusual shock-induced knots of gas.



“Although the rings may be the key to explaining the final ‘gasp’ of the dying central star, the mystery behind the Cat’s Eye Nebula’s nested ‘Russian doll’ structure remains largely unsolved,” noted ESA.



<h2 class="wp-block-heading" id="h-rings-around-the-cat-s-eye">Rings around the cat’s eye</h2>



“This image, taken with Hubble's Advanced Camera for Surveys (ACS), reveals the full pattern of eleven or more concentric rings, or shells, around the Cat’s Eye. Each ‘ring’ is actually the edge of a spherical bubble seen projected onto the sky - which is why it appears bright along its outer edge.”



According to ESA, observations suggest that the star ejected its mass in a series of pulses at 1,500-year intervals. “These convulsions created dust shells that each contains as much mass as all of the planets in our solar system combined.”



Several explanations have been proposed for this phenomenon, including cycles of magnetic activity similar to our Sun's sunspot cycle, the influence of companion stars orbiting the <a href="https://www.earth.com/news/dying-stars-may-be-a-source-of-gravitational-waves/" target="_blank" rel="noreferrer noopener">dying star</a>, or stellar pulsations.&nbsp;



Another theory suggests that the material is ejected smoothly from the star, with the rings forming later due to the creation of waves in the outflowing material.



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



<a href="https://www.earth.com/news/extrasolar-ocean-planet-discovered-in-the-draco-constellation/" target="_blank" rel="noreferrer noopener">Draco</a> is a constellation in the northern sky that represents a dragon. It's one of the largest constellations, winding between the Big and Little Dippers.&nbsp;



In Greek mythology, Draco is often identified as the dragon Ladon, who guarded the golden apples in the garden of the Hesperides.



Draco is a circumpolar constellation for most northern hemisphere observers, meaning it never sets below the horizon and can be seen all year round.



<h2 class="wp-block-heading" id="h-famous-planetary-nebulae">Famous planetary nebulae </h2>



Planetary nebulae are some of the most beautiful and intriguing objects in the universe.&nbsp;



One of the most famous is the Ring Nebula, or M57, located in the constellation Lyra. This nebula is renowned for its nearly perfect ring shape, which is the result of a dying star shedding its outer layers.&nbsp;



Another well-known planetary nebula is the Helix Nebula, or NGC 7293, often referred to as the "Eye of God" due to its eye-like appearance. The Helix Nebula is one of the closest planetary nebulae to Earth, making it a popular target for amateur astronomers.&nbsp;



The Dumbbell Nebula, or M27, in the constellation Vulpecula, is another striking example. It is named for its resemblance to a dumbbell and is notable for being the first planetary nebula ever discovered, by Charles Messier in 1764.&nbsp;



The Butterfly Nebula, or NGC 6302, is located in the constellation Scorpius. Its name comes from its distinctive bipolar structure, resembling the wings of a butterfly. The nebula's central star is one of the hottest known, with a surface temperature of around 250,000 degrees Celsius.&nbsp;



The Eskimo Nebula, or NGC 2392, in the constellation Gemini, is known for its resemblance to a face surrounded by a fur parka, which gives it its name. Its intricate structure, including filaments and bubble-like shapes, makes it a fascinating object of study.&nbsp;



These nebulae not only captivate us with their beauty but also provide valuable insights into the life cycles of stars and the processes that shape our galaxy.



Image Credit: NASA/ESA Hubble Space Telescope



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Cat's Eye Nebula in the constellation Draco

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA Earth Observatory&nbsp;



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Ksudach: A volcano shaped by explosive forces

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

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

Glp-1,Receptor,,Inactivated,And,Surrounded,By,An,Agonist,(semaglutide,,Red)

Sugar holds a strong place in many people’s diets, especially when stress runs high or snacks are within easy reach. While sugar’s appeal may feel irresistible, excessive consumption can increase the risk of type 2 diabetes. 



Scientists may have discovered a natural way to regulate blood sugar and curb cravings, <a href="https://www.earth.com/news/weight-loss-drugs-could-save-an-enormous-number-of-lives/" target="_blank" rel="noreferrer noopener">akin to drugs like Ozempic</a>. They've been investigating the relationship between sugar intake, gut signals, and hormones that help control appetite.



Reducing sugar intake can be challenging, but experts emphasize that managing blood sugar lowers the risk of diabetes complications. 



Health guidelines suggest limiting added sugars to 9 teaspoons per day for men and 6 teaspoons per day for women. 



Though this might seem difficult, research points to gut microbes as a potential secret weapon against persistent <a href="https://www.earth.com/news/americas-tide-of-obesity-is-rising-with-75-already-impacted/" target="_blank" rel="noreferrer noopener">cravings and obesity</a>.



<h2 class="wp-block-heading" id="h-understanding-glp-1-the-basics">Understanding GLP-1 - the basics</h2>



GLP-1, or glucagon-like peptide-1, is a hormone your body naturally produces in the gut. It plays a big role in managing blood sugar and appetite. 



After you eat, your intestines release GLP-1, which signals your pancreas to pump out insulin. At the same time, it tells your liver to slow down glucose production, keeping blood sugar levels steady. 



But GLP-1 doesn’t stop there - it also slows digestion and sends signals to your brain that make you feel full, which helps prevent overeating.



Drugs like <a href="https://www.ozempic.com/" target="_blank" rel="noreferrer noopener">Ozempic</a>, <a href="https://www.wegovy.com/" target="_blank" rel="noreferrer noopener">Wegovy</a>, and <a href="https://www.victoza.com/" target="_blank" rel="noreferrer noopener">Victoza</a> mimic GLP-1’s natural actions, helping control blood sugar and curb cravings.



<h2 class="wp-block-heading" id="h-gut-signals-and-sugary-foods">Gut signals and sugary foods</h2>



Dr. Li from <a href="https://english.jiangnan.edu.cn/" target="_blank" rel="noreferrer noopener">Jiangnan University</a> in China has been examining how gut signals might shape a person’s preference for sugary foods. 



In a recent publication, the authors state, “A growing body of research has revealed that our cravings for dietary components originate from signals sent from the gut, a key organ in transmitting dietary preferences.” 



This highlights the dynamic interaction between diet and gut microbes.



They also note, “However, which genes, gut flora, and metabolites in the gut microenvironment are involved in the regulation of sugar preference is currently unclear.” 



To understand this better, some studies have explored the role of hormones in sugar cravings, especially in individuals with <a href="https://www.earth.com/news/type-2-diabetes-heightens-alzheimers-risk/" target="_blank" rel="noreferrer noopener">type 2 diabetes</a>. 



There is also evidence suggesting that those with certain genetic variations tied to FGF21 are about 20% more likely to consume high amounts of sweet foods.



<h2 class="wp-block-heading" id="h-glp-1-and-gut-microbiota">GLP-1 and gut microbiota</h2>



One surprising discovery involves Ffar4, a receptor that influences gut microbiota composition. When Ffar4 levels decrease, the abundance of a gut microbe, Bacteroides vulgatus, may shift. 



Researchers at Jiangnan University have found that increasing this microbe in diabetic mice can “orchestrate the secretion of <a href="https://www.earth.com/news/weight-loss-drugs-could-save-an-enormous-number-of-lives/" target="_blank" rel="noreferrer noopener">glucagon-like peptide-1</a> (GLP-1).” 



This microbe produces metabolic compounds that send signals linked to sugar cravings and energy balance.



Bacteroides vulgatus is known to produce pantothenate, a form of vitamin B5. Scientists report that pantothenate helps release GLP-1, a hormone tied to satiety and blood sugar regulation. 



GLP-1, in turn, triggers the release of another hormone, FGF21. When these signals function properly, the body manages sugar more effectively, ultimately reducing the urge for sweet foods.



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



People with type 2 diabetes often have impaired GLP-1 function, prompting researchers to explore ways to improve or <a href="https://www.earth.com/news/olives-may-be-a-powerful-weapon-in-the-fight-against-obesity/" target="_blank" rel="noreferrer noopener">mimic its activity</a>. 



GLP-1 agonist drugs, such as semaglutide, have proven effective in lowering blood sugar and controlling appetite. 



While these medications work, some scientists are investigating whether natural methods can stimulate the same hormonal pathways. The authors suggest their study “provides a strategy for diabetes prevention.”



This approach brings the gut microbiome into focus, as small changes in microbial makeup might have broader implications. 



If further research confirms similar outcomes in humans, it could influence how doctors approach <a href="https://www.earth.com/news/neurons-discovered-that-tell-us-when-to-stop-eating/" target="_blank" rel="noreferrer noopener">sugar cravings</a> and early diabetes management. 



Emerging studies indicate potential benefits in boosting beneficial gut microbes, but it remains unclear how soon this concept will translate into practical medical solutions.



<h2 class="wp-block-heading" id="h-glp-1-microbiomes-and-the-future">GLP-1, microbiomes, and the future</h2>



Many questions remain about how gut microbes shape individual dietary choices. Researchers continue exploring whether manipulating these microbes could regulate sugar intake without drastic measures. 



Adjustments in <a href="https://www.earth.com/news/your-microbiome-trillions-of-bacteria-unique-like-your-fingerprint/" target="_blank" rel="noreferrer noopener">gut microbe populations</a> might not only help balance blood sugar but also support overall health.



Evidence linking intestinal bacteria to hunger-regulating hormones is growing, raising hopes that these discoveries may curb sugar cravings before diabetes develops. 



Some might compare this to a helpful chain reaction: the gut microbe produces specific compounds, those compounds activate the body’s natural signals, and the result is steadier blood sugar control. 



While the future direction of this research is uncertain, ongoing discoveries about microbes and hormones provide valuable insights into maintaining health - and possibly preserving a sweet tooth in moderation.



The full study was published in the journal <a href="https://www.nature.com/articles/s41564-024-01902-8" target="_blank" rel="noreferrer noopener">Nature Microbiology</a>.



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Natural alternative to Ozempic may soon be available for humans

Sugar holds a strong place in many people’s diets, especially...

Researchers in Sweden have reported control over a new kind of magnetism with the potential to boost electronic performance. Their work shows that this new class of magnetism, called altermagnetism, can increase memory device operation speeds by up to a thousand times. 



Scientists say it stands apart from the two widely known forms of magnetic order and may open doors to faster, more efficient technologies.



Scientists from the University of Nottingham's <a href="https://www.nottingham.ac.uk/physics/" target="_blank" rel="noreferrer noopener">School of Physics and Astronomy</a> have confirmed this third category in microscopic devices, and their findings have been published in Nature. Professor Peter Wadley from the same institution led the research.



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



Materials that exhibit altermagnetism contain <a href="https://www.earth.com/news/strong-magnetic-fields-leave-marks-on-nuclear-matter/" target="_blank" rel="noreferrer noopener">magnetic building blocks</a> that point antiparallel to one another, yet their crystal structure is rotated slightly relative to these neighboring units. 



"Altermagnets consist of magnetic moments that point antiparallel to their neighbors," Professor Wadley explains.



"However, each part of the crystal hosting these tiny moments is rotated with respect to its adjacent block. This is like <a href="https://www.sciencedirect.com/topics/physics-and-astronomy/antiferromagnetism#:~:text=Antiferromagnetism%20refers%20to%20the%20phenomenon,variation%20in%20susceptibility%20with%20temperature." target="_blank" rel="noreferrer noopener">antiferromagnetism</a> with a twist. But this subtle difference has huge ramifications."



<h2 class="wp-block-heading" id="h-bridging-magnetic-properties">Bridging magnetic properties</h2>



Altermagnets combine the favorable properties of ferromagnets and antiferromagnets in one material. 



Conventional magnets, such as iron, nickel, and cobalt, rely on aligned spins to deliver the familiar push-and-pull force of everyday magnets. 



In contrast, typical antiferromagnets cancel these forces, producing effects that are less noticeable from a distance. 



This new type links those features in a configuration that appears inactive from afar yet exhibits unique characteristics on a <a href="https://www.earth.com/news/transmitting-quantum-information-using-electron-spin/" target="_blank" rel="noreferrer noopener">nanoscopic scale</a>.



<h2 class="wp-block-heading" id="h-altermagnetism-and-synchrotrons">Altermagnetism and synchrotrons</h2>



A specialized synchrotron experiment at the <a href="https://www.maxiv.lu.se/" target="_blank" rel="noreferrer noopener">MAX IV</a> international facility in Sweden helped confirm these properties. The facility produces X-rays by accelerating electrons to near-light speeds. 



An ultra-thin wafer of manganese telluride was bathed in X-rays of different polarizations to reveal patterns reflecting previously unobserved magnetic activity. 



"Our experimental work has provided a bridge between theoretical concepts and real-life realization, which hopefully illuminates a path to developing altermagnetic materials for practical applications," explained Senior Research Fellow Oliver Amin, who led the experiment.



<h2 class="wp-block-heading" id="h-capturing-nanoscale-magnetic-patterns">Capturing nanoscale magnetic patterns</h2>



The synchrotron facility - a circular structure sometimes described as a giant metal doughnut - can generate high-intensity X-rays. 



Scientists used a specialized microscope to detect electrons emitted from the material's surface under X-ray illumination. 



This process created images of magnetism with nanoscale resolution. The direct view of altermagnetic features revealed a distinctive twist in the arrangement of magnetic moments.



<h2 class="wp-block-heading" id="h-revolutionizing-memory-technology">Revolutionizing memory technology</h2>



Industry experts note that magnetic materials represent a large and important part of current memory technology. 



Many <a href="https://www.earth.com/news/new-memory-crystal-data-storage-will-preserve-information-for-billions-of-years/" target="_blank" rel="noreferrer noopener">data-storage systems</a> rely on ferromagnets, which constitute an enormous global business and are also a significant source of energy consumption. 



Swapping conventional materials for altermagnets could significantly reduce reliance on heavy elements while cutting carbon emissions. 



The researchers believe this approach might allow speeds up to a thousand times faster than those of some existing microelectronic components.



Ph.D. student Alfred Dal Din has participated in experiments to explore how altermagnets can be applied in modern technology. 



"To be among the first to observe the effects and properties of this promising new class of magnetic materials during my Ph.D. has been an immensely rewarding and challenging privilege," Din enthused.



The group hopes that these findings will encourage broader investigations into how altermagnets operate under different conditions.



<h2 class="wp-block-heading" id="h-altermagnetism-and-large-scale-fields">Altermagnetism and large-scale fields</h2>



Engineers are already considering how to harness these special effects. Many existing designs rely on ferromagnets for long-term data storage because they offer a strong, consistent magnetic signal. 



Materials with a hidden magnetism that emerges on the nanoscale could be used in faster electronic switching or more <a href="https://www.earth.com/news/new-quantum-device-uses-crystal-layers-to-generate-entangled-photons/" target="_blank" rel="noreferrer noopener">compact memory</a> devices. 



Altermagnetism allows for the creation of structures that cancel large-scale fields while retaining a usable internal order.



<h2 class="wp-block-heading" id="h-environmental-and-economic-benefits">Environmental and economic benefits</h2>



This discovery may have implications for a wide range of products. In microelectronics, every extra bit of speed helps reduce lag and energy usage. 



Altermagnets show promise as a new platform for addressing the twin challenges of efficiency and performance. 



Because these materials can be grown in thin films, it becomes easier to integrate them into existing device architectures. 



They do not require the same rare resources used by many strong ferromagnets - a factor that could help lower costs and lessen the overall environmental impact of tech manufacturing.



The next phase of this work involves refining the methods used to control altermagnetism. Some experts note that many discoveries in magnetism take years to become standard in electronics. 



Whether altermagnets soon make their way into everyday devices or not, the findings highlight the importance of exploring new paths in physics to address modern challenges.



-----



Image -- Mapping an altermagnetic vortex pair in MnTe. The six colors, with arrows overlayed, show the direction of the altermagnetic ordering within the material. The size of the region shown is 1μm2. Credit: Oliver Amin, University of Nottingham



The full study was published in the journal <a href="https://www.nature.com/articles/s41586-024-08234-x" target="_blank" rel="noreferrer noopener">Nature</a>.



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Third form of magnetism, recently confirmed, could transform electronics

Researchers in Sweden have reported control over a new kind...

Out of all the planets in our solar system beyond Earth, most consider Saturn's beauty to be the most spectacular, with a set of rings that have inspired curiosity for hundreds of years. 



In the 17th century, Italian astronomer Galileo Galilei described this distant world as having "ears," showing how limited his view was at the time. 



Even with basic tools, he sensed something unusual about the planet’s appearance, although he could not fully explain it.



<h2 class="wp-block-heading" id="h-saturn-s-rings-steal-the-show">Saturn's rings steal the show</h2>



Modern telescopes and worldwide observatories have transformed our <a href="https://www.earth.com/news/massive-energy-imbalance-discovered-on-saturn/" target="_blank" rel="noreferrer noopener">understanding of Saturn</a>. They reveal swirling collections of ice and rocks orbiting the massive planet in broad arcs that we call rings. 



These ribbons of debris are more than a mere celestial decoration for us humans to admire; they shed light on the gravitational forces at work in our solar system.



By studying Saturn's rings, astronomers gain a better understanding of how cosmic particles behave when bound by gravity, and why their appearance changes when viewed from Earth. 



Jonah Peter, a doctoral student at Harvard-Smithsonian Center for Astrophysics (<a href="https://www.cfa.harvard.edu/" target="_blank" rel="noreferrer noopener">CfA</a>), has focused on how Saturn’s moons affect the <a href="https://www.earth.com/news/new-image-of-saturn-and-its-ring-spokes-from-the-hubble-space-telescope/" target="_blank" rel="noreferrer noopener">ring environment</a>.



His work connects the motions of this ring material to the broader story of our cosmic neighborhood, all of which is driven by a process known as orbital mechanics, or celestial mechanics. 



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



Orbital mechanics describes how bodies move under the pull of gravity. Planets circle the Sun, moons circle planets, and satellites stay in orbit around Earth. 



These paths depend on factors like velocity and orbital shape, all of which keep objects traveling in predictable loops.



Saturn’s tilt plays a role in how we see the rings. As the planet continues on its journey, our viewpoint changes over time. 



In some phases, the rings show off their full width. In others, they line up edge-on, turning into a thin band that seems ready to vanish.



<h2 class="wp-block-heading" id="h-how-saturn-s-rings-will-disappear">How Saturn's rings will disappear</h2>



A striking event called a "ring plane crossing" will occur on March 23, 2025. The rings will appear to have completely vanished because their thin edges will be aimed at Earth. 



This alignment happens when Saturn’s tilt and location match up so that we no longer see the bright swath of particles head-on. Once the rings vanish from easy sight in March 2025, Saturn will look like a pale yellow sphere through most telescopes. A subtle line may be visible around the planet’s middle, but only through the most powerful telescopes.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/01/saturn_rings_viewed-from-earth_orbital-mechanics_nasa_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/01/saturn_rings_viewed-from-earth_orbital-mechanics_nasa_1s.webp" alt="Rings A, B, C. You notice a large gap between the A and B rings. This is called the &quot;Cassini division&quot;. (See attached picture, where I've labeled the A, B, and C rings, along with the Cassini division.) There are other gaps in the rings at other places, but this one is the largest. the Cassini division (Hubble Space Telescope picture). Credit: NASA" class="wp-image-1956187"/></a><figcaption class="wp-element-caption">Rings A, B, C. You notice a large gap between the A and B rings. This is called the "Cassini division". (See attached picture, where I've labeled the A, B, and C rings, along with the Cassini division.) There are other gaps in the rings at other places, but this one is the largest. the Cassini division (Hubble Space Telescope picture). Credit: NASA</figcaption></figure>



Some enthusiasts might miss the typical glow, yet there is a certain thrill in waiting for that grand display to reappear.



As Earth and Saturn shift positions, the rings will come back into full view around November 2025. The planet’s looping debris will stand out again, along with glimpses of its many moons. 



<a href="https://www.earth.com/news/megastorms-on-saturn-are-larger-than-the-earth-and-last-for-hundreds-of-years/" target="_blank" rel="noreferrer noopener">This recurring pattern</a> reminds observers that our perspective can change, even when Saturn itself remains the same majestic world it has always been.



<h2 class="wp-block-heading" id="h-composition-and-structure-of-saturn-s-rings">Composition and structure of Saturn's rings</h2>



The rings are <a href="https://www.earth.com/news/saturns-rings-may-have-formed-after-two-icy-moons-collided/" target="_blank" rel="noreferrer noopener">divided into sections</a> called the A, B, and C rings, plus a few fainter ones labeled D, E, F, and G. Between the A and B rings lies the Cassini Division, measuring around 2,982 miles wide. 



Scientists note that spaces like this can form when orbital motions and gravitational tugs clear out certain pathways.



These rings are not solid sheets. They're made of pieces that range from dust-size grains to lumps as large as buses. 



Some researchers think the rings sprang from a moon ripped apart by Saturn’s gravity. Others propose that leftover material from the planet’s formation helped craft <a href="https://www.earth.com/news/we-now-know-the-age-of-saturns-rings-and-the-number-might-surprise-you/" target="_blank" rel="noreferrer noopener">these looping bands</a> more than four billion years ago.



<h2 class="wp-block-heading" id="h-moons-and-their-gravitational-pull">Moons and their gravitational pull</h2>



Saturn hosts <a href="https://www.earth.com/news/saturn-now-leads-the-solar-system-moon-race-with-145/" target="_blank" rel="noreferrer noopener">at least 145 moons</a>. Some are called shepherd moons, and they drift near the ring edges. 



Their gravity holds ring particles in place, preventing them from scattering too far in one direction or another. This process helps the rings maintain their recognizable gaps and bands.



Beyond those shepherds, Saturn’s system includes larger bodies that have unique properties. <a href="https://www.earth.com/news/saturns-moon-titan-has-shorelines-shaped-by-waves/" target="_blank" rel="noreferrer noopener">The biggest, Titan</a>, is a place of ongoing study. It has an atmosphere mostly made of nitrogen. 



Scientists have also measured a magnetic field around Titan that, while weaker than Jupiter’s, surpasses Earth’s field in relative strength.



<h2 class="wp-block-heading" id="h-titan-and-the-dragonfly">Titan and the Dragonfly</h2>



<a href="https://www.earth.com/news/dragonfly-space-mission-saturn-moon-titan-gets-greenlight/" target="_blank" rel="noreferrer noopener">NASA’s Dragonfly mission</a> plans to send an exploratory craft to Titan. Researchers are keen to learn more about its lakes of liquid hydrocarbons and the thick orange haze that hides much of its surface. 



These features hint at a landscape shaped by chemistry unlike anything on our planet.



Radio signals from Titan indicate bright auroras at the poles. These signals prove that electric and magnetic forces act in that moon’s environment. 



This unusual blend of ingredients prompts questions about how life might appear elsewhere, if it appears at all.



<h2 class="wp-block-heading" id="h-enceladus-may-harbor-life">Enceladus may harbor life</h2>



<a href="https://www.earth.com/news/life-on-saturns-moon-enceladus-massive-water-plume-has-scientists-wondering/" target="_blank" rel="noreferrer noopener">Enceladus</a>, another of Saturn’s moons, has drawn attention because of icy plumes venting from near its south pole. 



Observations from the Cassini mission revealed water vapor and possible chemical building blocks for living organisms. 



That discovery turned Enceladus into a point of interest for people searching for life in the solar system.



"Not only does Enceladus seem to meet the basic <a href="https://www.earth.com/news/life-sparking-energy-source-found-on-saturns-moon-enceladus/" target="_blank" rel="noreferrer noopener">requirements for habitability</a>, we now have an idea about how complex biomolecules could form there, and what sort of chemical pathways might be involved," explains Jonah Peter. These findings stir hope about discovering microbial life beyond Earth.



<h2 class="wp-block-heading" id="h-saturn-s-mystery-and-majesty">Saturn's mystery and majesty</h2>



Galileo’s old remark about Saturn’s "ears" underscores how far we have come. Early astronomers had limited tools, yet they still glimpsed something remarkable. 



Modern instruments add detail, but the sense of wonder remains. Saturn shows how our solar system is filled with surprises that motivate fresh discoveries.



As amateurs and experts keep pointing their lenses skyward, they continue to find reasons to appreciate this planet’s evolving appearance. 



The rings may fade from view temporarily, but people know they will return. Each phase allows us to learn a little more about how cosmic objects behave and how life might emerge under new conditions.



The full study was published in the journal <a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2023JE008236" target="_blank" rel="noreferrer noopener">JGR Planets</a>.



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Saturn's beautiful rings will vanish in about six weeks from now

Out of all the planets in our solar system beyond...

The Arctic, long considered a remote and icy wilderness, is becoming&nbsp;warmer&nbsp;and undergoing dramatic changes. Once a symbol of resilience against the forces of nature, it now stands as one of the most vulnerable regions on Earth. 



The rising global temperatures are not only reshaping its physical landscape but also threatening the delicate ecosystems and communities that depend on it. 



The future of the <a href="https://www.earth.com/news/permafrost-is-no-longer-permanent-arctic-communities-in-danger/" target="_blank" rel="noreferrer noopener">Arctic</a> is not a distant concern - it is unfolding now, and the consequences will be felt worldwide.



In 2024, the world crossed a sobering threshold. For the first time, global air temperatures averaged more than 1.5 degrees Celsius (2.7 degrees Fahrenheit) above pre-industrial levels.



This milestone set off a chain reaction of extreme weather events, including unprecedented rainfall and flooding in the Sahara Desert and brutal heat waves across multiple continents. 



Despite years of warnings from scientists, the reality of climate change is becoming impossible to ignore.



<h2 class="wp-block-heading" id="h-future-of-a-warming-planet">Future of a warming planet</h2>



Surpassing 1.5 degrees Celsius (2.7 degrees Fahrenheit) was never meant to be a stopping point. Scientists have long cautioned that without aggressive action, temperatures would continue to rise.



Based on the current commitments made by governments to limit greenhouse gas emissions, the planet is projected to warm by 2.7 degrees Celsius (4.9 degrees Fahrenheit) above pre-industrial levels by the end of the century.



This level of warming would have devastating consequences, with no place on Earth experiencing them as profoundly as the Arctic.



The Arctic is warming faster than any other region on the planet. Ice that has existed for thousands of years is vanishing. 



Permafrost, which has locked away vast amounts of carbon, is beginning to thaw. The effects of these changes will not remain confined to the polar regions.



The impacts will ripple outward, influencing global weather patterns, sea levels, and ecosystems in ways that are still being fully understood.



<h2 class="wp-block-heading" id="h-the-arctic-s-fate-in-a-warming-world">The Arctic’s fate in a warming world</h2>



In a review paper published in the journal Science, researchers examined the rapid changes taking place in the Arctic.



The study was led by Julienne Stroeve, a senior research scientist at the National Snow and Ice Data Center (NSIDC) and professor at the Centre for Earth Observation Science at the <a href="https://umanitoba.ca" target="_blank" rel="noreferrer noopener">University of Manitoba</a>.



The research provides a comprehensive look at how continued warming will reshape the Arctic landscape and what that means for the planet as a whole.



“The Arctic is warming at four times the rate of the rest of the planet,” said Stroeve. 



“At 2.7 degrees Celsius of global warming, we will see more extreme and cascading impacts in this region than elsewhere, including sea-ice-free Arctic summers, accelerated melting of the Greenland Ice Sheet, widespread permafrost loss, and more extreme air temperatures."



"These changes will devastate infrastructure, ecosystems, vulnerable communities, and wildlife.”



<h2 class="wp-block-heading" id="h-alarming-arctic-transformations">Alarming Arctic transformations</h2>



The findings of the review paper build on the work of the United Nations <a href="https://www.ipcc.ch" target="_blank" rel="noreferrer noopener">Intergovernmental Panel on Climate Change</a>’s Sixth Assessment Report. 



The study updates previous knowledge by focusing on three critical areas of Arctic transformation: sea ice, the Greenland Ice Sheet, and permafrost. 



By analyzing existing research, the study presents a clearer picture of how the Arctic will respond to continued warming.



If global temperatures rise to 2.7 degrees Celsius, <a href="https://www.earth.com/news/the-arctic-may-be-ice-free-sooner-than-we-expected/" target="_blank" rel="noreferrer noopener">Arctic</a> air temperatures will consistently surpass historical extremes. Ice that once covered the Arctic Ocean year-round will disappear for several months each summer. 



The Greenland Ice Sheet, which holds enough ice to raise global sea levels significantly, will see an alarming expansion of areas where surface temperatures remain above freezing for extended periods. 



At the same time, surface permafrost will decline to half of its pre-industrial levels, releasing more carbon into the atmosphere and exacerbating global warming.



<h2 class="wp-block-heading" id="h-global-impact-of-arctic-warming">Global impact of Arctic warming </h2>



The loss of Arctic ice is not just a regional issue. It is a critical factor in regulating the planet’s climate. The Arctic acts as Earth’s refrigerator, reflecting sunlight and helping to cool the atmosphere. 



As ice disappears, the darker ocean absorbs more heat, accelerating the warming process in a cycle that scientists call Arctic amplification.



This shift will have severe consequences beyond the <a href="https://www.earth.com/news/arctic-warming-permafrost-melt-devastating-role-accelerating-global-climate-change/" target="_blank" rel="noreferrer noopener">Arctic</a>. The melting of the Greenland Ice Sheet will contribute to rising sea levels, threatening coastal cities and small island nations. 



Changes in Arctic weather patterns will disrupt global climate systems, leading to more frequent and intense storms, droughts, and extreme temperatures in regions far from the poles. 



The thawing of permafrost will release trapped greenhouse gases, further accelerating global warming and creating additional challenges for efforts to slow climate change.



<h2 class="wp-block-heading" id="h-human-activity-and-arctic-warming">Human activity and Arctic warming</h2>



The study serves as a stark reminder that human activity is the driving force behind these changes. The choices made today will determine the future of the Arctic and the planet as a whole. 



Scientists hope that by presenting a clear picture of what lies ahead, decision-makers will take meaningful action to reduce emissions and slow the pace of warming.



Study co-author Dirk Notz is a professor for polar research at the University of Hamburg.



“Our paper shows that, already today, mankind has the power to wipe out entire landscapes from the surface of our planet,” said Notz. 



“It’d be amazing if we could become more aware of this power and the responsibility that goes with it, as the future of the <a href="https://www.earth.com/news/arctic-industrialization-how-will-it-impact-delicate-ecosystems/" target="_blank" rel="noreferrer noopener">Arctic</a> truly lies in our hands.”



<h2 class="wp-block-heading" id="h-the-time-to-act-is-now">The time to act is now</h2>



The study relied on data from NSIDC’s <a href="https://nsidc.org/sea-ice-today" target="_blank" rel="noreferrer noopener">Sea Ice Today</a> and <a href="https://nsidc.org/ice-sheets-today" target="_blank" rel="noreferrer noopener">Ice Sheets Today</a> projects to analyze changes in Arctic ice conditions. 



The findings add to the growing body of evidence showing that climate change is not a distant threat. It is happening now, and its effects are accelerating.



While the Arctic may seem far removed from the daily lives of many people, the changes occurring there will have far-reaching consequences for the entire planet.



The fate of the <a href="https://www.earth.com/news/first-ice-free-day-in-the-arctic-may-arrive-in-2027/" target="_blank" rel="noreferrer noopener">Arctic</a> is not yet sealed. There is still time to prevent the worst outcomes, but it will require a global effort. 



Governments must commit to stronger emissions reductions, businesses must invest in sustainable practices, and individuals must push for change.



The Arctic has long been a symbol of endurance in the face of harsh conditions. Whether it remains that way will depend on the actions taken today. The findings of this study serve as both a warning and a call to action. 



The choices made in the coming years will determine whether the Arctic continues to exist as we know it or becomes an irreversible casualty of a warming world.



The study is published in the journal <a href="https://www.science.org/doi/10.1126/science.ads1549" target="_blank" rel="noreferrer noopener">Science</a>.



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Drastic warming will transform the Arctic "beyond recognition"

The Arctic, long considered a remote and icy wilderness, is...

Aging is a natural process, but many seek ways to delay its effects. The desire to maintain health and vitality has led researchers to explore different interventions. 



Some studies suggest that reducing calorie intake can slow aging in humans. Others indicate that omega-3 fatty acids and vitamin D may influence biological aging in animals.



However, until recently, it was unclear whether these approaches would have the same <a href="https://www.earth.com/news/muscles-defy-aging-with-remarkable-resilience/" target="_blank" rel="noreferrer noopener">impact on humans</a>.



A team of researchers set out to investigate whether these simple, accessible measures could influence aging at a biological level. 



The findings suggest that certain lifestyle changes might hold the key to slowing down the body’s natural decline.



<h2 class="wp-block-heading" id="h-omega-3-and-aging-in-older-adults">Omega-3 and aging in older adults</h2>



One of the most extensive studies on aging is the DO-HEALTH trial led by Heike Bischoff-Ferrari at the <a href="https://www.uzh.ch/en.html" target="_blank" rel="noreferrer noopener">University of Zurich</a>. The team explored whether vitamin D, omega-3 fatty acids, and regular exercise could impact aging in humans.



Previous research had already demonstrated that these three factors contribute to better health by reducing infections, preventing falls, and lowering cancer risks.



“These results inspired us to measure the direct influence of these three therapies on the biological aging process in the Swiss DO-HEALTH participants,” said Bischoff-Ferrari.



The research team aimed to determine whether these benefits extended beyond general health and actually slowed down the biological <a href="https://www.earth.com/news/scientists-discover-the-cellular-mortality-timer-that-dictates-aging/" target="_blank" rel="noreferrer noopener">markers of aging</a>.



<h2 class="wp-block-heading" id="h-focus-of-the-aging-study">Focus of the aging study</h2>



The trial included 2,157 participants who were randomly divided into eight groups. Each group followed a different combination of vitamin D, omega-3s, exercise, or a placebo to assess aging.



Some received all three interventions, while others took only one or two. The experts monitored participants over three years, conducting follow-up phone calls every three months and in-depth health assessments at yearly intervals.



The DO-HEALTH cohort is the largest European study of healthy adults over 70. Funded by the EU’s Seventh Framework Program for Research, it represents a significant effort to understand how simple interventions can improve <a href="https://www.earth.com/news/secrets-of-aging-discovered-in-plant-leaves/" target="_blank" rel="noreferrer noopener">aging outcomes</a>.



The Swiss National Science Foundation provided additional support for epigenetic measurements.



<h2 class="wp-block-heading" id="h-biological-vs-chronological-aging">Biological vs. chronological aging</h2>



Aging can be measured in different ways. Chronological age is simply the number of years a person has lived, while biological age reflects the body's actual <a href="https://www.earth.com/news/human-bodies-begin-breaking-down-very-precise-age/" target="_blank" rel="noreferrer noopener">condition</a>. 



Some people age faster due to genetic factors, lifestyle choices, or environmental influences. Others remain biologically younger than their chronological years suggest.



To measure biological aging, scientists use a tool called an epigenetic clock. This method tracks DNA modifications, specifically methylation, which can indicate how quickly a body is aging. 



The DO-HEALTH study applied this technique to analyze whether certain interventions influenced biological aging.



<h2 class="wp-block-heading" id="h-role-of-epigenetic-clocks">Role of epigenetic clocks </h2>



The research team collaborated with Steve Horvath, a senior researcher at Altos Labs Cambridge. Horvath is a pioneer in the development of epigenetic clocks, which have become an essential tool for measuring aging at the molecular level.



The study examined 777 individuals over the age of 70. Each participant was assigned one of eight treatment plans, which included taking 2,000 IU of vitamin D daily, consuming 1 gram of omega-3 fatty acids, or engaging in 30 minutes of strength training three times per week. 



Some participants followed a combination of these interventions, while others received a placebo. The goal was to observe whether any of these treatments influenced biological aging over three years.



<h2 class="wp-block-heading" id="h-omega-3-slowed-biological-aging">Omega-3 slowed biological aging</h2>



Blood samples from the participants provided valuable insights. Researchers found that taking omega-3 fatty acids slowed down biological aging by up to four months. 



This effect was consistent regardless of gender, age, or body mass index. More significantly, the combination of omega-3s, vitamin D, and strength training yielded even stronger results.



“This result extends our previous findings from the DO-HEALTH study, in which these three factors combined had the greatest impact on reducing the risk of cancer and preventing premature frailty over a three-year period, to slowing down the biological <a href="https://www.earth.com/news/what-25-years-of-research-revealed-about-brain-aging/" target="_blank" rel="noreferrer noopener">aging process</a>,” noted Bischoff-Ferrari.



The findings suggest that each factor works through different mechanisms that complement each other, leading to a greater overall effect when combined.



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



The study provides evidence that simple lifestyle changes, including Omega-3 intake, can influence biological aging.



While the difference of a few months may seem small, slowing down aging on a molecular level could have long-term health benefits. 



A slower aging process might reduce the risk of age-related diseases, improve quality of life, and extend healthy lifespan.



Despite these promising findings, the researchers acknowledge that measuring biological aging remains a challenge. 



“There is no generally accepted gold standard for measuring biological age. However, we analyzed the best currently validated epigenetic clocks, which reflect the state of the art," said Bischoff-Ferrari.



The study contributes to a growing body of research exploring how lifestyle factors influence aging at a biological level.



<h2 class="wp-block-heading" id="h-expanding-to-a-broader-population">Expanding to a broader population</h2>



One of the study’s limitations is its focus on Swiss participants. Biological aging can be influenced by genetics, lifestyle, and environmental factors, which vary across populations. 



To gain a more comprehensive understanding, the researchers plan to expand the study to include participants from Germany, France, Austria, and Portugal. 



This broader dataset will help determine whether the findings apply to a more diverse range of individuals.



The DO-HEALTH study is part of a larger effort to refine methods for measuring and slowing aging. 



Bischoff-Ferrari and her team are working with the <a href="https://healthspanextension.science" target="_blank" rel="noreferrer noopener">Global Health Span Extension</a> Consortium to validate biological clocks and improve the accuracy of aging biomarkers.



<h2 class="wp-block-heading" id="h-future-of-omega-3-and-aging-research">Future of omega-3 and aging research</h2>



The findings from this study reinforce the idea that aging is not entirely out of our control. While there is no single solution to stop aging, certain lifestyle choices may slow its progression. 



The combination of omega-3 fatty acids, vitamin D, and strength training shows measurable benefits, suggesting that simple, accessible interventions can make a real difference.



Future studies will continue refining these approaches and testing new methods to measure biological aging. The hope is that ongoing research will lead to more effective strategies for maintaining health and vitality in later years. 



The study is published in the journal <a href="https://www.nature.com/articles/s43587-024-00793-y" target="_blank" rel="noreferrer noopener">Nature Aging</a>.



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New study confirms three simple ways to slow biological aging

Aging is a natural process, but many seek ways to...

Pregnancy is a time when many expectant mothers seek ways to manage discomfort and stress. With growing interest in natural remedies, cannabidiol (CBD), a compound derived from cannabis, has gained popularity as a perceived safe option for nausea, anxiety, and sleep disturbances. 



Unlike tetrahydrocannabinol (THC), the psychoactive component of cannabis, CBD does not produce a high, leading many to assume it poses little to no risk during pregnancy.



Despite this perception, scientific research on the effects of CBD during pregnancy remains limited. Many previous studies have focused on <a href="https://www.earth.com/news/cannabis-use-impacts-working-memory-and-brain-function/" target="_blank" rel="noreferrer noopener">cannabis smoke</a> or THC exposure, leaving CBD largely unexplored. 



A new study from <a href="https://www.mcmaster.ca" target="_blank" rel="noreferrer noopener">McMaster University</a> challenges these assumptions, revealing concerning links between CBD use and fetal development issues. These findings suggest that CBD, often considered harmless, may have unexpected consequences for both mother and child.



<h2 class="wp-block-heading" id="h-potential-risks-of-cbd-in-pregnancy">Potential risks of CBD in pregnancy</h2>



A team of researchers at McMaster University investigated the effects of cannabis use during pregnancy, specifically focusing on both CBD and THC. 



The findings, published in eBioMedicine, highlight the potential dangers of oral cannabis consumption from early to mid-pregnancy. 



The study revealed that <a href="https://www.earth.com/news/cannabis-use-during-pregnancy-rewires-the-fetal-brain/" target="_blank" rel="noreferrer noopener">cannabis exposure</a> was associated with impaired fetal growth, changes in the placenta, and behavioral alterations in offspring.



Tyrah Ritchie led the study while completing her master’s degree in the Medical Sciences program at McMaster University.



“The use of cannabis during pregnancy is rising in Canada. Most previous studies focus on exposure to cannabis smoke or just the psychoactive component of cannabis (THC), leaving other cannabis ingredients and methods of consumption understudied," noted Ritchie.



"However, consuming cannabis orally or only using other <a href="https://www.earth.com/news/high-potency-cannabis-use-linked-to-epigenetic-changes/" target="_blank" rel="noreferrer noopener">cannabis</a> ingredients like CBD, is often perceived as safer despite this lack of evidence. Our study is shedding light that there's a possibility that CBD might also be harmful in the pregnancy.”



The study challenges the belief that CBD is a safe alternative to THC during pregnancy. While THC has long been linked to developmental concerns, this research suggests that CBD may also have unintended effects.



<h2 class="wp-block-heading" id="h-fetal-growth-and-placental-development">Fetal growth and placental development</h2>



The researchers examined how THC and CBD affect fetal development by administering cannabis oil to pregnant mice. 



Their observations revealed that <a href="https://www.earth.com/news/cannabis-and-hallucinogen-use-are-at-historically-high-levels/" target="_blank" rel="noreferrer noopener">cannabis exposure</a> resulted in smaller fetuses compared to those in the control group. This suggests that cannabis compounds may interfere with normal growth, leading to intrauterine growth restriction.



In addition to reduced fetal size, the study found that cannabis impacted the development of blood vessels that supply nutrients to the placenta. 



The placenta plays a crucial role in providing oxygen and nutrients to the developing baby, and any disruption in this process could have serious consequences.



“We did see that both THC and CBD can disrupt a special type of immune cell called a Uterine NK Cell that is crucial in normal development of the placenta," said Ali Ashkar, professor in McMaster’s Department of Medicine and co-leader of the study.



"We also saw poor development of the arteries that help supply blood to the placenta. We're thinking this is what is possibly disrupting the nutrient and oxygen delivery to the baby and contributing to the intrauterine grow restriction.”



<h2 class="wp-block-heading" id="h-pregnancy-cbd-and-offspring">Pregnancy, CBD, and offspring</h2>



Beyond physical growth, the study also examined how <a href="https://www.earth.com/news/chemical-found-in-cannabis-plants-can-actually-reduce-cannabis-induced-anxiety/" target="_blank" rel="noreferrer noopener">cannabis exposure</a> affects offspring behavior. Researchers monitored the behavior of the mice after birth and discovered changes in aggression, activity levels, and learning ability. 



These findings suggest that exposure to cannabis during pregnancy could have lasting neurological effects on the offspring.



“Oral use of THC and CBD during the pregnancy not only disrupts growth of the baby but seems to have long-term consequences as the babies were found to have changes in their behaviour later in life,” said Ritchie.



Behavioral changes in offspring highlight the possibility of cognitive and emotional challenges that may persist into adulthood. 



The exact mechanisms behind these effects remain unclear, but the findings raise concerns about how cannabis interacts with the developing brain.



<h2 class="wp-block-heading" id="h-need-for-further-investigation">Need for further investigation</h2>



While this study provides critical insights, researchers emphasize the need for further investigation to fully understand the <a href="https://www.earth.com/news/recreational-cannabis-use-protects-against-cognitive-decline/" target="_blank" rel="noreferrer noopener">risks</a> of CBD use during pregnancy. 



The study was conducted on mice, and while animal models offer valuable information, human studies are necessary to confirm these findings.



Ritchie stresses that the growing trend of cannabis use during pregnancy should be met with caution. Many expectant mothers turn to CBD with the belief that it is safe, but without clear scientific evidence, assumptions about its harmlessness may be misleading.



<h2 class="wp-block-heading" id="h-rethinking-cbd-use-during-pregnancy">Rethinking CBD use during pregnancy</h2>



The widespread perception of CBD as a natural and safe remedy has led to its increasing use among pregnant individuals. 



However, this study suggests that CBD may not be as risk-free as commonly thought. The findings indicate that both THC and CBD could interfere with crucial developmental processes, affecting both physical growth and long-term behavior.



Pregnant individuals considering cannabis products should consult healthcare professionals before use. While the study does not provide definitive answers on CBD’s safety for human pregnancies, it does highlight the need for greater awareness and caution.



<h2 class="wp-block-heading" id="h-funding-and-future-research">Funding and future research</h2>



This study was supported by The <a href="https://cannabisresearch.mcmaster.ca" target="_blank" rel="noreferrer noopener">Michael G. DeGroote</a> Centre for Medicinal Cancer Research, the <a href="https://cihr-irsc.gc.ca/e/193.html" target="_blank" rel="noreferrer noopener">Canadian Institutes of Health Research</a>, and the <a href="https://www.innovation.ca" target="_blank" rel="noreferrer noopener">Canadian Foundation for Innovation</a>. 



As research in this field continues, scientists aim to explore the specific mechanisms by which cannabis compounds affect pregnancy outcomes.



With increasing cannabis use worldwide, understanding its full impact on pregnancy is more important than ever. Further studies will help clarify the risks, providing expectant mothers with the information they need to make informed choices.



The study is published in the journal <a href="https://www.thelancet.com/journals/ebiom/article/PIIS2352-3964(25)00016-7/fulltext" target="_blank" rel="noreferrer noopener">EBioMedicine</a>.



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CBD use during pregnancy has unexpected consequences

Pregnancy is a time when many expectant mothers seek ways...

Human height has been evolving over the past century, with both men and women getting taller and heavier across the spectrum. Researchers suggest these shifts are tied to living conditions, broader health measures, and the dynamic ways <a href="https://www.earth.com/news/who-is-happier-being-single-men-or-women/">men and women</a> respond to their environments.



While everyone has seen gains, recent <a href="https://royalsocietypublishing.org/doi/10.1098/rsbl.2024.0565" target="_blank" rel="noreferrer noopener">work</a> points to men making larger strides. There’s more to the story than meets the eye.



<h2 class="wp-block-heading" id="h-evolution-of-height-in-men-and-women">Evolution of height in men and women</h2>



A century ago, <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4961475/" target="_blank" rel="noreferrer noopener">scientists</a> began investigating trends in human stature in different populations. The goal was to see how factors such as nutrition, disease rates, and economic changes might leave lasting marks on adult height and weight.



Some teams uncovered that better diets and improved health care often resulted in taller generations (<a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC4961475/" target="_blank" rel="noreferrer noopener">NCD Risk Factor Collaboration (NCD-RisC</a>), 2016). Their work laid the groundwork for more recent efforts to track how these gains compare between men and women.



More recent research <a href="https://royalsocietypublishing.org/doi/10.1098/rsbl.2024.0565" target="_blank" rel="noreferrer noopener">work</a> from this year builds on that older study. Scientists, such as <a href="https://www.researchgate.net/profile/Lewis-Halsey#:~:text=Lewis%20Halsey%20is%20a%20Professor,and%20adaptations%20for%20energy%20efficiency." target="_blank" rel="noreferrer noopener">Professor Lewis Halsey</a> from the <a href="https://www.roehampton.ac.uk/" target="_blank" rel="noreferrer noopener">University of Roehampton</a>, an environmental physiologist, have focused on what other factors, apart from better diets, might be influencing the weights and heights of adults. 



They also consider evolution and mating preferences to explain why the height gap between men and women might be increasing.



<h2 class="wp-block-heading" id="h-how-living-conditions-affect-height">How living conditions affect height</h2>



When researchers measured differences across countries, they turned to indices that reflect overall well-being. 



One index, the <a href="https://hdr.undp.org/data-center/human-development-index#/indicies/HDI" target="_blank" rel="noreferrer noopener">Human Development Index (HDI)</a>, looks at a nation’s average life expectancy, years of schooling, and income.



In one large-scale <a href="https://royalsocietypublishing.org/doi/10.1098/rsbl.2024.0565" target="_blank" rel="noreferrer noopener">study</a> that examined individuals in dozens of countries, every bump in HDI seemed to bring clear gains in adult size - both height and weight. Yet, men outpaced women in these increases, by more than double.



This pattern was also measured against income inequality through another global indicator. Where inequality was high, the ability to achieve full growth potential decreased.



Researchers found that men’s stature is often more sensitive to environmental stressors, so in tough settings, men’s growth can stall more prominently.



<h2 class="wp-block-heading" id="h-men-women-and-height-differences">Men, women, and height differences</h2>



“On average <a href="https://www.earth.com/news/human-evolution-why-men-are-advancing-faster-than-women/" target="_blank" rel="noreferrer noopener">men are taller</a> and more muscular than women, which confers on them advantages related to female choice,” wrote the authors of the 2025 study. 



Part of this advantage lies in mating preferences: the idea that, over time, taller men have had better odds of passing on their traits.



Researchers believe that, in situations where food is ample and disease burdens are lower, men experience a more pronounced boost in height and weight than women do.



The assumption is that this sex-based difference has deeper evolutionary roots. Larger bodies for men might be linked to strength and competitiveness, which could have historically helped them secure partners more easily.



In modern contexts, these same traits still seem to matter, even if life has changed dramatically since our ancestors roamed the planet.



<h2 class="wp-block-heading" id="h-what-the-2016-research-showed">What the 2016 research showed</h2>



In <a href="https://elifesciences.org/articles/13410" target="_blank" rel="noreferrer noopener">2016</a>, an analysis of adult height suggested that gains were not spread evenly across countries (NCD Risk Factor Collaboration (NCD-RisC). The project found stark differences between various regions.



Europe and parts of East Asia showed big leaps in adult height, while some nations in sub-Saharan Africa and South Asia saw little movement or even declines. 



That earlier work also revealed how American men and women, once near the global top in average height, fell behind countries with steadily improving healthcare and nutrition.



The findings back then hinted that living conditions shape growth, but the focus was not just about getting taller. Being taller was linked to health benefits, fewer birth complications, and even higher income in some populations.



At the same time, experts cautioned that taller stature can come with vulnerabilities like higher rates of certain cancers.



<h2 class="wp-block-heading" id="h-insight-from-the-2025-findings">Insight from the 2025 findings</h2>



More recently, researchers have taken these ideas further by examining both height and body mass over the decades. Their efforts highlight how men’s growth appears to be more “expensive” in terms of energy.



Bigger bodies require more nutrients, so when the environment offers stable healthcare and abundant food, men see a greater surge in these body dimensions.&nbsp;



“We’re seeing insights into how sexual selection has shaped the male and female body and how improved environments, in terms of food and a lower burden of disease, have freed us from our shackles,” commented Professor Halsey from the University of Roehampton.



Looking at historical records from within a single country, like the United Kingdom, backs up the global results. <a href="https://www.earth.com/news/mens-brains-shrink-in-the-evening-and-reset-overnight/">Men</a> show a steeper increase in both height and weight.



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



The disparity might spark questions about health management, especially because men’s size can be more sensitive to setbacks such as infections in early life. Researchers often see men’s height as a useful barometer for overall living conditions.



When disease rates are high and nutrition is poor, men’s measurements respond more sharply. When these factors improve, men’s gains are larger.



Women still make noticeable progress, but they face fewer extreme swings. Some scientists suggest that female bodies, due to their vital role in reproduction, cannot afford as much growth fluctuation.



Others note that cultural preferences for male height have played a part in amplifying certain traits across generations.



<h2 class="wp-block-heading" id="h-future-height-of-men-and-women">Future height of men and women</h2>



By examining <a href="https://www.earth.com/news/why-women-experience-more-chronic-pain-than-men/">sex-based differences</a> in height and weight, public health experts may find new ways to measure progress. 



When looking at improved living conditions, a steep increase in men’s average size can signal better nutrition and fewer childhood illnesses.



Height alone won’t predict every health outcome, though. The research underscores the value of a well-rounded approach to health, one that considers everything from prenatal care to consistent access to nutritious foods.



Size is not the only indicator of well-being, but it does serve as a clear marker of the opportunities and obstacles that define our early years. 



Men may experience these environmental factors more intensely, which makes male growth an especially telling measurement.



The study is published in <a href="https://royalsocietypublishing.org/doi/10.1098/rsbl.2024.0565" target="_blank" rel="noreferrer noopener">Biology Letters</a>.



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Men are getting taller at a much faster rate than women - what’s causing this?

Human height has been evolving over the past century, with...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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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

[sendtonews key="3upvlAaHgO-2256633-12187" type="single"] Today’s Video of the Day from the...

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

[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...