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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA Earth Observatory&nbsp;



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Ruki River in the Democratic Republic of the Congo

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

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 Southern Ring Nebula, also known as NGC 3132.



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA, ESA, CSA, STScI



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Southern Ring Nebula in the constellation Vela 

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Spiral galaxy NGC 6744 in the constellation Pavo

Today's Image of the Day from the European Space Agency features the Little Dumbbell Nebula, also known as Messier 76, located in the constellation Perseus 3,400 light-years away from Earth.



Astronomers captured this image of the Little Dumbbell Nebula to commemorate the 34th anniversary of the Hubble Space Telescope, a joint venture between NASA and the European Space Agency (<a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>).



The snapshot provides not only a breathtaking view but also deep insights into the life cycle of <a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">stars</a> and the dynamic processes within nebulae.



<h2 class="wp-block-heading" id="h-understanding-messier-76">Understanding Messier 76</h2>



Messier 76 is categorized as a planetary nebula - a term which refers to its round, planet-like appearance when viewed through early, low-power telescopes. 



However, the term is somewhat misleading as planetary nebulae have no connection to actual <a href="https://www.earth.com/news/nasa-finds-17-exoplanets-that-have-oceans-and-possibly-alien-life/" target="_blank" rel="noreferrer noopener">planets</a>. 



Instead, they represent an expansive shell of luminous gases expelled by a dying red giant star, which subsequently collapses into a dense, hot white dwarf. 



This transformation marks the late stages of stellar evolution for medium to low-mass stars.



<h2 class="wp-block-heading" id="h-structure-of-messier-76">Structure of Messier 76</h2>



The structure of Messier 76 is particularly notable. It includes a central ring, giving the appearance of a bar-like feature, with two distinct lobes emanating from either side. 



This formation is believed to be the result of materials ejected by the star during its red giant phase, possibly sculpted by interactions with a companion star. 



Although this binary companion is not visible in current Hubble images, its presence is inferred from the thick disk of dust and gas aligned with its orbital plane. 



The phenomenon of the companion star potentially being absorbed by the primary star, a process akin to stellar cannibalism, is a captivating aspect of the nebula's history.



<h2 class="wp-block-heading" id="h-the-dynamic-environment-of-the-nebula">The dynamic environment of the nebula</h2>



At the core of the nebula, the primary star, now collapsing into 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>, reaches extreme temperatures. This heat is estimated to be 120,000 degrees Celsius - about 24 times hotter than the surface of our Sun. 



This intensely hot remnant is visible as a small, bright point at the center of the nebula. Directly below this, another star can be seen; however, it is merely aligned with the nebula by chance and is not a part of it.



<h2 class="wp-block-heading" id="h-powerful-glow-of-messier-76">Powerful glow of Messier 76</h2>



The dynamics within Messier 76 are driven by powerful forces. The central disk seems to constrict the material, creating two lobes of gas escaping along the rotational axis of the star, perpendicular to the disk.&nbsp;



The lobes are propelled outward by a potent stellar wind, moving at a staggering two million miles per hour. This rapid movement is sufficient to travel the distance from Earth to the <a href="https://www.earth.com/news/timeless-mystery-solved-scientists-uncover-what-is-inside-the-moons-core/" target="_blank" rel="noreferrer noopener">Moon</a> in just over seven minutes.&nbsp;



The collision of the fast-moving gas with older, slower-moving material ejected during the star’s red giant phase results in the stunning glowing effect seen in the nebula. 



The glow, ignited by the ultraviolet radiation from the white dwarf, is a spectacle of colors with red emanating from nitrogen and blue from oxygen.



<h2 class="wp-block-heading" id="h-a-cosmic-moment-in-time">A cosmic moment in time</h2>



Despite its current brilliance, the existence of the Little Dumbbell Nebula is fleeting on a cosmological scale. It is expected to last only about 15,000 years - a mere moment in the lifespan of the <a href="https://www.earth.com/news/dark-energy-is-ripping-the-universe-apart-but-we-arent-sure-how/" target="_blank" rel="noreferrer noopener">universe</a>. 



This brief period highlights the transient nature of such cosmic phenomena, which, while short-lived, provide crucial insights into the mechanics of stellar evolution and the complex interactions within these celestial sculptures.



<h2 class="wp-block-heading" id="h-more-about-messier-76">More about Messier 76</h2>



Messier 76 was discovered by Pierre Méchain in 1780. It was later cataloged by Charles Messier, who included it in his famous list of nebulous objects.



The nebula's faintness and small size require a good telescope to be observed effectively, with larger telescopes able to reveal more of its fine details and structure.



Studying Messier 76 helps astronomers understand the life cycle of stars and the processes that occur during the late stages of stellar evolution. 



The materials expelled by planetary nebulae like Messier 76 eventually contribute to the interstellar medium, from which new stars and planetary systems may form.



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

Today's Image of the Day from the European Space Agency features the galaxy I Zwicky 18, which was captured in remarkable detail by the James Webb Space Telescope.



I Zwicky 18 is a blue compact dwarf <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">galaxy</a> located approximately 59 million light-years away in the constellation Ursa Major.&nbsp;



<h2 class="wp-block-heading" id="h-star-formation-in-i-zwicky-18">Star formation in I Zwicky 18</h2>



The galaxy is notable for its relatively young appearance and the fact that it contains very few heavy elements. These characteristics indicate that it has experienced little <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> compared to other galaxies of similar age.



“The galaxy was first identified by Swiss astronomer Fritz Zwicky in the 1930’s and resides roughly 59 million light-years from Earth,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>. “This galaxy has gone through several sudden bursts of star formation.”&nbsp;



According to ESA, I Zwicky 18 is typical of the kinds of galaxies that inhabited the early universe and is much smaller than our <a href="https://www.earth.com/news/runaway-star-j1249-36-spotted-trying-to-escape-our-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



<h2 class="wp-block-heading" id="h-webb-telescope-image-of-the-galaxy">Webb telescope image of the galaxy</h2>



“Two major starburst regions are embedded in the heart of the galaxy. The wispy brown filaments surrounding the central starburst region are bubbles of gas that have been heated by stellar winds and intense ultraviolet radiation unleashed by hot, young stars,” noted ESA.



“A companion galaxy resides nearby to the dwarf galaxy, which can be seen at the bottom of the wider-field image. The companion may be interacting with the dwarf galaxy and may have triggered that galaxy's recent star formation.”&nbsp;



ESA explained that the “orange blobs” surrounding the galaxy are the dim glow from ancient fully formed galaxies at much larger distances.



<h2 class="wp-block-heading" id="h-key-characteristics-of-i-zwicky-18">Key characteristics of I Zwicky 18</h2>



As previously mentioned, the galaxy has a very low abundance of elements heavier than hydrogen and helium, suggesting that it has not undergone significant stellar processing.



<h3 class="wp-block-heading" id="h-young-stellar-population-nbsp">Young stellar population&nbsp;</h3>



Despite its old age, I Zwicky 18 contains many young, hot stars. This suggests that it might have experienced a burst of <a href="https://www.earth.com/news/hubble-detects-awe-inspiring-newborn-star/" target="_blank" rel="noreferrer noopener">star formation</a> relatively recently in its history.



<h3 class="wp-block-heading" id="h-interstellar-medium-nbsp">Interstellar medium&nbsp;</h3>



The galaxy has a high density of gas, which is a prime ingredient for star formation. This gas is mostly in the form of hydrogen.



<h3 class="wp-block-heading" id="h-unusual-characteristics">Unusual characteristics</h3>



Its characteristics are more typical of primordial galaxies found in the early universe, making it a valuable object of study for understanding galaxy formation and evolution.



Ultimately, I Zwicky 18 provides insights into the conditions and processes that might have been prevalent in the early universe.



<h3 class="wp-block-heading" id="h-life-cycles-of-stars-and-dust">Life cycles of stars and dust</h3>



The image was captured as part of a Webb program to study the life cycle of dust in I Zw 18.&nbsp;



“Scientists are now building off of previous research with Hubble obtained at optical wavelengths, studying individual dusty stars in detail with Webb’s equivalent spatial resolution and sensitivity at infrared wavelengths.”&nbsp;



ESA noted that this galaxy is of particular interest as its content of elements heavier than helium is one of the lowest of all known <a href="https://www.earth.com/news/early-galaxy-formation-occurred-much-faster-than-we-thought/" target="_blank" rel="noreferrer noopener">galaxies</a> in the local universe.&nbsp;



“Such conditions are thought to be similar to those in some of the first star-forming galaxies at high redshift, so the Webb study of I Zw 18 should shed light on the life-cycle of stars and dust in the early universe.”



<h2 class="wp-block-heading" id="h-the-constellation-ursa-major">The constellation Ursa Major </h2>



Ursa Major, also known as the Great Bear, is one of the most prominent and easily recognizable constellations in the northern sky. 



Its name, "Ursa Major," means "Great Bear" in Latin, and it has been a significant part of various mythologies and star lore across cultures for thousands of years. 



One of the most famous asterisms within Ursa Major is the Big Dipper, a group of seven bright stars that form a shape resembling a ladle or dipper. The Big Dipper is often used as a navigation tool because it points to Polaris, the North Star, located in the nearby constellation Ursa Minor.



Ursa Major is best viewed in the northern hemisphere and is circumpolar, meaning it is visible year-round for much of the Northern Hemisphere. Its position changes with the seasons, rotating around Polaris, the North Star.



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



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Dwarf galaxy provides a window into the early universe

Building the GPM Microwave Imager (GMI). A test technician completes the final electrical integration of the GPM Microwave Imager (GMI) at Ball Aerospace. Therefore Engineers at NASA Goddard will integrate both the GMI and the Dual-frequency Precipitation Radar. And onto the main body of the Global Precipitation Measurement (GPM) mission's core satellite. After extensive testing, the satellite will then be shipped to <a href="http://www.earth.com/news/japan-commercial-whaling/">Japan</a> for launch in 2014.

The GPM mission is a joint effort between NASA. And the Japan Aerospace Exploration Agency (JAXA) and other international partners. Therefore GPM mission will improve climate, weather and hydrological predictions by providing more accurate precipitation measurements from space.

Credit: <a href="https://www.nasa.gov/mission_pages/GPM/multimedia/gmi_integration.html">Ball Aerospace</a>

Building the GPM Microwave Imager (GMI)

When we think of oxytocin, the image of a warm embrace or the deep connection between a mother and her child often comes to mind. 



This hormone, often dubbed the "love hormone" or "cuddle hormone," is famous for its role in fostering emotional bonds and promoting feelings of trust and empathy. 



But recent studies suggest that oxytocin might be doing much more behind the scenes, especially when it comes to how we learn and remember. And more surprisingly, it may also help cure addiction.



Leading this exciting exploration are Professor Akiyoshi Saitoh and researcher Junpei Takahashi from the <a href="https://www.tus.ac.jp/en/" target="_blank" rel="noreferrer noopener">Tokyo University of Science</a>, and Meredith Berry, Ph.D. from the <a href="http://www.ufl.edu/" target="_blank" rel="noreferrer noopener">University of Florida</a>. 



They have been delving into the intricate ways oxytocin influences our brains, potentially paving the way for new treatments for conditions like dementia and <a href="https://www.earth.com/news/brain-discovery-offers-hope-for-tackling-opioid-addiction/" target="_blank" rel="noreferrer noopener">opioid addiction</a>.



<h2 class="wp-block-heading" id="h-oxytocin-s-role-in-memory">Oxytocin's role in memory</h2>



While oxytocin is well-known for its impact on social behaviors, its role in cognitive functions is less understood. 



Professor Saitoh's team wanted to uncover whether oxytocin could be a key player in <a href="https://www.earth.com/news/how-does-our-brain-form-long-term-memories/" target="_blank" rel="noreferrer noopener">how memories are formed</a> and retained. 



“Previously we had suggested that oxytocin may be a new therapeutic candidate for dementia based on studies using a mouse model of <a href="https://www.earth.com/news/alzheimers-disease-attacks-the-brain-in-two-separate-phases/" target="_blank" rel="noreferrer noopener">Alzheimer’s disease</a>,” he shared. 



“To investigate this further, in this study, we examined the role of endogenous oxytocin in mouse cognitive function.”



Using advanced techniques, the researchers specifically activated oxytocin neurons in certain brain regions of mice. 



They then evaluated the mice's memory using tasks designed to test recognition and recall, like the <a href="https://www.sciencedirect.com/topics/biochemistry-genetics-and-molecular-biology/novel-object-recognition-test" target="_blank" rel="noreferrer noopener">Novel Object Recognition Task</a>. 



This method helps scientists determine how well an animal can recognize a new object compared to one they've seen before.



<h2 class="wp-block-heading" id="h-peering-into-the-brain-s-memory-centers">Peering into the brain's memory centers</h2>



The brain is a complex network, and understanding how different areas interact is crucial. 



The team noticed that when they stimulated oxytocin neurons in the paraventricular hypothalamic nucleus (PVN), there was increased activity not only there but also in the supramammillary nucleus (SuM). 



These regions are connected and play roles in memory and <a href="https://www.earth.com/news/music-causes-similar-emotional-experiences-and-sensations-in-all-cultures/" target="_blank" rel="noreferrer noopener">emotional responses</a>.



By observing markers that indicate neuron activation, they confirmed that these areas were more active following their interventions. 



Interestingly, while the mice didn't show significant changes in short-term memory tasks, there was a noticeable improvement in long-term memory, particularly in recognizing new objects.



<h2 class="wp-block-heading" id="h-oxytocin-connection-to-dementia">Oxytocin connection to dementia</h2>



These findings have significant implications. <a href="https://www.earth.com/news/herbal-medicine-shows-potential-to-treat-and-prevent-dementia/" target="_blank" rel="noreferrer noopener">Dementia</a>, including Alzheimer's disease, affects millions worldwide, leading to memory loss and cognitive decline. 



Understanding how oxytocin influences memory could lead to new therapies that slow down or mitigate these effects.



There's also a broader social context. Many believe that loneliness and lack of social interaction can worsen <a href="https://www.earth.com/news/dementia-was-extremely-rare-in-ancient-times-so-why-is-it-now-so-prevalent/" target="_blank" rel="noreferrer noopener">dementia symptoms</a>. 



“There is a widely acknowledged belief that dementia tends to advance more rapidly in settings where individuals experience loneliness or limited social engagement. However, the scientific underpinnings of this phenomenon have remained largely elusive," Professor Saitoh pointed out.



By highlighting oxytocin's role, the research suggests that stimulating social interactions -- or even directly targeting oxytocin pathways -- might help in <a href="https://www.earth.com/news/diabetes-drugs-may-protect-against-dementia/" target="_blank" rel="noreferrer noopener">managing dementia</a>.



<h2 class="wp-block-heading" id="h-oxytocin-and-opioid-addiction">Oxytocin and opioid addiction</h2>



Across the globe, another team is exploring oxytocin's potential in a different arena. 



At the University of Florida, researchers are investigating whether a synthetic version of oxytocin can help curb opioid addictions, a pressing issue affecting many communities.



“The idea is that physicians could potentially prescribe, in combination, an opioid and oxytocin as an acute <a href="https://www.earth.com/news/mindfulness-meditation-is-a-powerful-weapon-against-chronic-pain/" target="_blank" rel="noreferrer noopener">pain management</a> option, while at the same time lessening the likelihood of developing an addiction to opioids,” explained Dr. Meredith Berry.



Working alongside Dr. Yenisel Cruz-Almeida and Dr. Natalie Ebner, Dr. Berry is examining whether oxytocin can reduce pain effectively while also decreasing the desire for prolonged opioid use.



<h2 class="wp-block-heading" id="h-opioids-are-still-a-huge-problem">Opioids are still a huge problem</h2>



Opioid addiction has become a significant public health concern, particularly in the United States. 



Prescription opioids, while effective for managing pain, carry a high risk of addiction. Older adults, who often require pain management, can be particularly vulnerable.



By exploring alternatives that reduce pain without the same addictive potential, researchers hope to offer safer options for patients. 



Oxytocin's natural role in promoting well-being might counteract some of the addictive properties of opioids.



<h2 class="wp-block-heading" id="h-healing-addiction-with-oxytocin">Healing addiction with oxytocin</h2>



In their carefully designed study, the University of Florida team is working with participants aged 55 to 85 who have some history of opioid use. 



In a controlled setting, these participants will receive synthetic oxytocin via a nasal spray or a placebo after taking oral <a href="https://www.earth.com/news/experts-identify-a-route-to-safer-painkillers/" target="_blank" rel="noreferrer noopener">oxycodone</a>.



The researchers will collect data on how much the participants enjoy the drugs, as well as monitor physical responses like heart rate and breathing. 



They'll also assess cognitive and emotional reactions. To measure pain responses, they will apply mild mechanical pressure to the thighs and expose the hands to varying temperatures.



Dr. Ebner will analyze mood changes and cognitive effects, while Dr. Cruz-Almeida will examine how the drugs affect pain responses. 



Dr. Berry will evaluate the potential for reduced opioid addiction based on these findings. Physicians from the university's College of Medicine are involved to ensure participant safety.



<h2 class="wp-block-heading" id="h-is-oxytocin-the-wonder-drug-of-the-future">Is oxytocin the "wonder drug" of the future?</h2>



The combined efforts of these research teams highlight the versatility of oxytocin, putting the "love hormone" on the radar of scientists of all disciplines around the world.



From potentially enhancing memory and combating dementia to offering new strategies for pain management without the high risk of addiction, oxytocin's benefits could be far-reaching.



These studies underscore the importance of looking beyond traditional uses of well-known substances. Sometimes, the key to solving complex health issues lies in re-examining what we thought we knew.



The journey of oxytocin from a simple "love hormone" to a potential powerhouse in medical treatment is a testament to the ever-evolving nature of science. 



As researchers like Professor Saitoh and Dr. Berry continue their work, we can look forward to new discoveries that might improve the quality of life for many.



The full study was published in the journal <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0294113" target="_blank" rel="noreferrer noopener">PLOS One</a>.



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'Cuddle hormone' fosters love, boosts memory, and now also cures addiction

When we think of oxytocin, the image of a warm...

Scientists have uncovered a disturbing twist in how climate change affects our oceans, revealing that tiny changes at the bottom of the food chain can have massive impacts on most fish populations.



The findings of a recent study highlight the intricate workings of the ocean's food web and how it's more vulnerable to warming temperatures than previously thought.



<h2 class="wp-block-heading" id="h-tiny-ocean-creatures-big-fish-impact">Tiny ocean creatures, big fish impact</h2>



<a href="https://www.earth.com/news/arctic-heatwaves-have-complex-effects-on-phytoplankton-food-web/" target="_blank" rel="noreferrer noopener">Phytoplankton</a> are tiny, plant-like organisms that float around in oceans, seas, and lakes. Even though you can't see them without a microscope, they're incredibly important. 



They use sunlight to make their own food through photosynthesis, just like plants do on land. In the process, they produce a huge amount of the Earth's oxygen -- some estimates say up to half of it. 



These little guys are the starting point of the food chain in aquatic environments, feeding small fish, shrimp, and other marine creatures.



<a href="https://www.earth.com/news/dust-from-africa-sparked-a-massive-phytoplankton-bloom/" target="_blank" rel="noreferrer noopener">Phytoplankton</a> also play a big role in absorbing carbon dioxide from the atmosphere, helping to regulate our planet's climate. But they're sensitive to changes in their environment, like warming waters.



When climate models predict that warming oceans will reduce phytoplankton levels by 16% to 26% in regions like the North Atlantic, it's a cause for concern.



But here's where it gets alarming: the study found that this seemingly modest drop in phytoplankton could slash the ocean's capacity to support fish by a staggering 38% to 55%. That's more than double the initial decrease in phytoplankton.



<h2 class="wp-block-heading" id="h-phytoplankton-and-the-hidden-amplifier">Phytoplankton and the hidden amplifier</h2>



Dr. Angus Atkinson from the <a href="https://pml.ac.uk/" target="_blank" rel="noreferrer noopener">Plymouth Marine Laboratory</a> and Dr. Axel Rossberg of <a href="https://www.qmul.ac.uk/" target="_blank" rel="noreferrer noopener">Queen Mary University</a> of London led the research team behind this discovery.



They took a straightforward approach by examining real-world data on plankton sizes from oceans, seas, and lakes around the globe. 



By looking at the sizes of plankton, they could determine how efficiently energy moves up the food chain -- from tiny phytoplankton to the fish we rely on.



This amplification effect hinges on a surprising twist: temperature, often blamed for food web disruptions, appears to play a secondary role. 



Instead, the key driver is the overall amount of phytoplankton, which governs how efficiently energy flows from tiny plankton to larger fish.



"Our global analysis sheds light on a hidden vulnerability," explained Dr. Atkinson. "We were surprised to find temperature didn't directly affect food web efficiency. Instead, we see ecosystems <a href="https://www.earth.com/news/invisible-forest-of-phytoplankton-thrives-in-a-warming-climate/" target="_blank" rel="noreferrer noopener">adapting to warming</a> by changing plankton size. "



<h2 class="wp-block-heading" id="h-nutrients-the-unsung-hero">Nutrients: The unsung hero</h2>



In the open ocean, nutrients come from deeper waters. As the surface warms, it becomes more layered, making it harder for these nutrients to reach the <a href="https://www.earth.com/image/spectacular-phytoplankton-bloom-in-the-north-atlantic/" target="_blank" rel="noreferrer noopener">phytoplankton at the top</a>.



"Close to shore or in lakes, excess nutrients from land can cause imbalances like harmful algal blooms," notes Dr. Rossberg. 



"But at the vast scales relevant to climate change, it's the lack of nutrients from deeper waters that becomes the major bottleneck."



To clarify, warming oceans, seas, and lakes impact fish indirectly by reducing nutrient supply from <a href="https://www.earth.com/news/toxic-legacy-decades-old-ddt-found-in-deep-sea-fish/" target="_blank" rel="noreferrer noopener">deeper waters</a>, ultimately shrinking phytoplankton size and hindering energy transfer throughout the food web.



<h2 class="wp-block-heading" id="h-real-world-impact-for-ocean-fish">Real world impact for ocean fish</h2>



When phytoplankton numbers change, the impact can ripple through the entire <a href="https://www.earth.com/news/oceans-twilight-zone-stabilizes-the-marine-food-chain/" target="_blank" rel="noreferrer noopener">marine ecosystem</a>, impacting everything from water quality to the abundance of fish.



This isn't just a problem for the fish; it's a problem the planet. Many communities around the world depend on fishing for food and livelihood. 



The study highlights the need to consider climate change impacts when managing fisheries.



"Global averages can mask the true picture," explains Dr. Atkinson. "Some of the most significant projected declines are in areas with concentrated <a href="https://www.earth.com/news/fish-stocks-are-collapsing-globally-as-overfishing-continues/" target="_blank" rel="noreferrer noopener">fishing activities</a>."



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



So, what can we do about it? The researchers suggest a multi-pronged approach to ensure sustainable fisheries in the face of climate change. 



"We need a combination of data on plankton size structure and sophisticated computer simulation models to design truly 'climate-smart' ocean protection strategies," concludes Dr. Rossberg. 



"By understanding the hidden amplifiers within the food web, we can better safeguard the future of our oceans and the vital resources they provide."



<h2 class="wp-block-heading" id="h-oceans-fish-and-the-global-food-chain">Oceans, fish, and the global food chain</h2>



To sum it all up, these scientists found that even a small drop in phytoplankton levels due to warming oceans can massively reduce fish populations. 



They discovered that it's not just the temperature rise itself causing problems, but the decrease in nutrients reaching these tiny organisms. 



This leads to smaller plankton and less efficient energy transfer <a href="https://www.earth.com/news/microbial-awakening-arctic-food-webs-are-transforming-from-green-to-brown/" target="_blank" rel="noreferrer noopener">up the food chain</a>, which is bad news for fish and, by extension, us.



This study underscores underscores the interconnectedness of Earth's ecosystem. Tiny changes at the bottom can have huge impacts at the top. 



It's a reminder that we need to pay attention to even the smallest players in the ecosystem if we want to protect the health of our planet. 



By understanding these hidden mechanisms, we can work towards smarter strategies to safeguard our oceans and the communities that rely on them.



The full study was published in the journal <a href="https://www.nature.com/articles/s41467-023-44406-5" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Oceans and lakes are quickly losing their ability to keep fish alive

Scientists have uncovered a disturbing twist in how climate change...

The development of a big brain in humans and its connection to social bonding has been a hot topic of debate, and secrets found in fossil teeth may hold the answers.



Researchers have been studying the fossilized teeth of an early Homo from Georgia, dating back approximately 1.77 million years. The research was made possible by the European Synchrotron in Grenoble, France.



The findings suggest that despite having a small brain and reaching adulthood at a similar pace to great apes, these early humans had a prolonged childhood. 



This could mean that the large brain of modern humans resulted from an extended childhood along with cultural transmission across generations instead of vice versa.



<h2 class="wp-block-heading" id="h-long-childhood-big-brains">Long childhood, big brains</h2>



A team of researchers - including specialists from Switzerland's <a href="https://www.uzh.ch/en.html" target="_blank" rel="noreferrer noopener">University of Zurich</a>, the European Synchrotron Radiation Facility and Georgia's National Museum - have challenged the theory that modern humans' extended childhood is directly linked to their large brains.



The team analyzed dental development in an early Homo that was almost an adult. The results suggest that though these early humans reached adulthood at a similar age as <a href="https://www.earth.com/news/buronius-manfredschmidi-tiny-great-ape-species-lived-11-million-years-ago/" target="_blank" rel="noreferrer noopener">great apes</a>, their tooth development followed a longer timeline similar to modern humans.



This proposes the distinct possibility of a longer dependency on adults and an elongated childhood for these early humans.



Remarkably, the brain size of these early Homo specimens was only marginally larger than that of a chimpanzee. This made the researchers question the link between the prolonged development and cultural transmission across generations.



An extended childhood within a three-generation context might have allowed the immature members of the group to effectively assimilate growing amounts of knowledge. 



Eventually, this led to the development of larger brains and longer life spans, traits characteristic of modern humans.



<h2 class="wp-block-heading" id="h-dental-development-in-early-homo">Dental development in early Homo</h2>



An enduring assumption has been that humans' extended growth period is a consequence of <a href="https://www.earth.com/news/our-brain-sizes-are-growing-possibly-lowering-dementia-risk/" target="_blank" rel="noreferrer noopener">increased brain volume</a> since a larger organ requires more energy resources to grow. But analysis of the fossil's dental growth has caused researchers to question this hypothesis.



The research team used synchrotron imaging to study the dental development of a near-adult fossil of early Homo from the Dmanisi site in Georgia, dated to around 1.77 million years ago. 



<div class="wp-block-sendtonews-playerselector">[sendtonews key="CWxiqQg039-4024544-12187" type="single"]</div>



“Childhood and cognition do not fossilize, so we have to rely on indirect information. Teeth are ideal because they fossilize well and produce daily rings, in the same way that trees produce annual rings, which record their development,” noted study first author Christoph Zollikofer from the University of Zurich.



<h2 class="wp-block-heading" id="h-unexpected-findings-and-a-new-perspective">Unexpected findings and a new perspective</h2>



“Dental development is strongly correlated with the development of the rest of the body, including brain development," explained study co-author Paul Tafforeau, scientist at the ESRF.



"Access to the details of a <a href="https://www.earth.com/search-results/?search=fossil%20hominid&amp;start=0" target="_blank" rel="noreferrer noopener">fossil</a> hominid's dental growth therefore provides a great deal of information about its general growth."



After almost two decades of research beginning in 2005, the initial results startled researchers. 



“We expected to find either dental development typical of early hominids, close to that of the great apes, or dental development close to that of <a href="https://www.earth.com/news/neanderthal-genes-still-influence-modern-humans/" target="_blank" rel="noreferrer noopener">modern humans</a>," said Tafforeau.



"When we obtained the first results, we couldn’t believe what we saw, because it was something different that implied faster molar crown growth than in any other fossil hominin or living great ape."



In the following years, the team conducted five series of experiments and completed four full analyses, employing various methods as dental synchrotron imaging technology advanced.



As the consistent results suggested significant implications for the "big brain - long childhood" hypothesis, the scientists needed to think creatively to interpret this fossil's findings.



“It's been a slow maturation, both technically and intellectually, to finally arrive at the hypothesis we are publishing today,” said Tafforeau.



<h2 class="wp-block-heading" id="h-longer-childhood-evolution-s-early-experiment">Longer childhood: Evolution's early experiment?</h2>



The dental development of the studied fossil suggested that milk teeth were used longer than in great apes, implying that early Homo children were dependent on adult care for a longer duration.



This could be the first experiment evolution took towards a prolonged childhood. Despite having brains only slightly larger than australopithecines or great apes, early Homo are believed to have lived longer.



The survival of a very old individual with no teeth for several years indicates that the group sufficiently cared for him. This alludes to a three-generation structure, a key aspect of <a href="https://www.earth.com/news/humans-started-cumulative-culture-around-600000-years-ago/" target="_blank" rel="noreferrer noopener">cultural transmission in humans</a>.



The new hypothesis begins with children's growth slowing down as cultural transmission increased. 



The accumulation of information from older to younger individuals had an advantageous effect on resource utilization and the development of complex behaviors, thus favoring a longer childhood. 



Once this mechanism was established, natural selection acted on cultural transmission, not just biological traits. 



<h2 class="wp-block-heading" id="h-big-brains-and-delayed-adulthood">Big brains and delayed adulthood</h2>



As the volume of transferrable information grew, evolution supported a larger brain and delayed adulthood, enabling a longer learning period in childhood and time to grow a bigger brain despite limited food resources.



The large brain of modern humans could be attributed to an extended childhood and a three-generation structure encouraging bio-cultural evolution. These mechanisms may have led to increased brain size, delayed adulthood, and longer lifespan. 



The study of this exceptional fossil could motivate researchers to rethink the evolutionary mechanisms that led to Homo sapiens.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-024-08205-2" target="_blank" rel="noreferrer noopener">Nature</a>.



Image &amp; Video Credit: ESRF/Paul Tafforeau, Vincent Beyrand



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How did humans get big brains? Fossil teeth reveal new clues

The development of a big brain in humans and its...

Psychedelic substances, once the mainstay of counterculture, are steadily blending into mainstream recreational and therapeutic activities across North America. But are they safe?



A recent in-depth study offers some sobering new insights. The investigation reveals a worrying association between the use of hallucinogens - a category that includes substances such as psilocybin, LSD, DMT (Ayahuasca), and MDMA (Ecstasy) - and a heightened risk of developing schizophrenia.



The comprehensive study was conducted by researchers at ICES, The Ottawa Hospital, the Department of Family Medicine at the <a href="https://www.uottawa.ca/en" target="_blank" rel="noreferrer noopener">University of Ottawa</a>, and Bruyère Health Research Institute.



Although the positive therapeutic potential of psychedelics has garnered significant enthusiasm lately, the research team cautions that usually, such celebration outpaces thorough understanding of the associated risks.



<h2 class="wp-block-heading" id="h-psychedelic-use-and-schizophrenia">Psychedelic use and schizophrenia </h2>



The analytic foundation of the study relied on over a decade's health data of people aged 14 to 65 years living in Ontario, Canada. 



The researchers monitored changes in hallucinogen-related emergency department (ED) visits and ensuing <a href="https://www.earth.com/news/owning-a-cat-before-age-25-doubles-the-risk-of-schizophrenia/" target="_blank" rel="noreferrer noopener">schizophrenia</a> diagnosis rates.



The results were astonishing: Relative to the general population, an individual with a hallucinogen-related visit to the emergency department had a staggering 21-fold increase in the likelihood of developing schizophrenia.



Even after factoring in co-occurring substance use and <a href="https://www.earth.com/news/mental-health-crisis-half-of-the-worlds-population-will-be-affected-by-age-75/" target="_blank" rel="noreferrer noopener">mental health disorders</a>, the risk remained 3.5 times higher.



<h2 class="wp-block-heading" id="h-alarming-data-trends">Alarming data trends</h2>



The data, spanning from 2008 to 2021, also revealed another concerning trend. While the annual rates of ED visits associated with <a href="https://www.earth.com/news/cannabis-and-hallucinogen-use-are-at-historically-high-levels/" target="_blank" rel="noreferrer noopener">hallucinogen use</a> were stable between 2008 and 2012, they saw a sudden 86% spike in the period from 2013 to 2021.



Within three years of an ED visit involving hallucinogens, 4% of individuals were diagnosed with schizophrenia. 



In comparison, the diagnosis rate for the general population was a meager 0.15% within the same timeframe - a difference that equates to an alarming 21 times higher risk for the former group.



When stacked against the risk associated with alcohol and <a href="https://www.earth.com/news/high-potency-cannabis-use-linked-to-epigenetic-changes/" target="_blank" rel="noreferrer noopener">cannabis use</a>, hallucinogens still didn't fare well. 



Individuals with ED visits due to psychedelic use were at 4.7 and 1.5 times higher risk of schizophrenia, respectively, compared to alcohol and cannabis.



<h2 class="wp-block-heading" id="h-risks-of-psychedelic-use">Risks of psychedelic use</h2>



Despite the study’s potentially alarming findings, the study authors emphasized that their findings do not establish a causal link between hallucinogen use and schizophrenia and that much more information is needed about risks associated with different types and use patterns of hallucinogens.



“Our findings underscore a concerning link between hallucinogen use that requires care in the emergency room and increased risk of schizophrenia,” said Dr. Daniel Myran, a Canada Research Chair in Social Accountability at the University of Ottawa.



“While there is enormous enthusiasm for psychedelic-assisted therapy as a new mental health treatment, we need to remember how early and limited the data remains for both the benefits and the risks,” noted Myran.



This highlights the urgency for more studies and improved public health measures to better comprehend and mitigate these risks.



<h2 class="wp-block-heading" id="h-screening-and-monitoring">Screening and monitoring</h2>



In clinical trials of psychedelic-assisted psychotherapy, experts integrate safeguards like excluding individuals with a personal or family history of schizophrenia and close monitoring,.



However, the study authors warn about the potential risks of hallucinogen use outside of these controlled settings.



The study also highlights the need to identify those at higher risk of developing serious adverse events from hallucinogens, facilitating safe recruitment practices in future trials.



<h2 class="wp-block-heading" id="h-psychedelic-safety-in-clinical-settings">Psychedelic safety in clinical settings</h2>



The implications of this study are very critical both to public health and to policy development. As psychedelics become more accepted for therapeutic and recreational use, understanding the associated risks becomes increasingly crucial.



Initiatives for public health education should include specific education on the dangers of hallucinogen use - particularly in cases where there is known predilection to a mental health disorder.



This awareness can be created with targeted community outreach, evidence-based medical guidelines, and collaboration among healthcare providers and mental health specialists.



Another proactive strategy could be mental health checkups for patients before <a href="https://www.earth.com/news/psychedelic-drug-therapy-could-help-treat-alcoholism/" target="_blank" rel="noreferrer noopener">psychedelic therapy</a>. This would allow experts screen for people with a greater risk of an adverse reaction.



The study is published in the journal <a href="https://jamanetwork.com/journals/jamapsychiatry/article-abstract/2825649" target="_blank" rel="noreferrer noopener">JAMA Psychiatry</a>.



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Psychedelic use linked to higher risk of schizophrenia

Psychedelic substances, once the mainstay of counterculture, are steadily blending...

The scorching heatwaves we experience, the wildfires that rage across nations, and the invisible carbon dioxide that fills the air are severely impacting our planet.



In 2023, the world saw extreme heatwaves that fueled substantial wildfires and induced severe droughts across the globe. 



What's more, these <a href="https://www.earth.com/news/fast-wildfires-are-gaining-even-more-speed/" target="_blank" rel="noreferrer noopener">adverse conditions</a> significantly weakened the land's ability to absorb atmospheric carbon. 



The result? A notable surge in atmospheric carbon dioxide levels, growing the scale of concern about accelerating climate change.



<h2 class="wp-block-heading" id="h-heat-and-atmospheric-carbon">Heat and atmospheric carbon </h2>



Data from Hawaii's <a href="https://gml.noaa.gov/obop/mlo/aboutus/aboutus.html" target="_blank" rel="noreferrer noopener">Mauna Loa Observatory</a> showed that atmospheric carbon concentrations skyrocketed by an alarming 86% in 2023 compared to 2012. This increase sets a new record high since tracking of these levels began in 1958.



Interestingly, the rise in carbon dioxide levels cannot solely be pointed towards fossil fuel emissions. These, it seems, only rose by roughly 0.6 percent.



So, what's the primary culprit behind the spike in emissions? It's likely due to weakened <a href="https://www.earth.com/news/extreme-fire-risk-has-grown-exponentially-in-a-hotter-climate/" target="_blank" rel="noreferrer noopener">carbon absorption</a> by natural ecosystems.



<h2 class="wp-block-heading" id="h-weakened-carbon-sink">Weakened carbon sink </h2>



An international team of scientists backed by the <a href="https://www.esa.int/Applications/Observing_the_Earth/Extreme_heat_weakens_land_s_power_to_absorb_carbon" target="_blank" rel="noreferrer noopener">ESA</a> Science for Society Near-Realtime Carbon Extremes project - along with the Climate Change Initiative RECCAP-2 project - set out to investigate the root causes of this event.



The experts used global vegetation models and satellite data to expedite a carbon budget report for 2023.



Land typically absorbs about one-third of human-generated carbon dioxide emissions. However, in 2023, this absorption capacity fell to a mere one-fifth of its usual level, marking the weakest performance by land carbon sink in two decades.



<h2 class="wp-block-heading" id="h-extreme-heat-and-carbon-storage-capacity">Extreme heat and carbon storage capacity </h2>



“Our research shows that 30% of this decline was driven by the extreme heat of 2023, which fueled massive <a href="https://www.earth.com/news/ultrafine-particles-in-wildfire-smoke-change-weather-patterns/" target="_blank" rel="noreferrer noopener">wildfires</a> that ravaged vast areas of Canadian forest and triggered severe drought across parts of the Amazon rainforest," said Philippe Ciais, a scientist from France’s Laboratory for Climate and Environmental Sciences.



"These fires and droughts led to substantial vegetation loss, weakening the land ecosystem’s ability to absorb carbon dioxide. This was further compounded by a particularly strong El Niño, which historically reduces the carbon absorption capacity in the Tropics." 



The situation was made worse by a particularly potent El Niño, which historically reduces carbon absorption capacity in the tropics.



<h2 class="wp-block-heading" id="h-carbon-emitted-from-wildfires">Carbon emitted from wildfires</h2>



Widespread wildfires across Canada and droughts in the Amazon in 2023 released nearly the same amount of carbon to the atmosphere as North America's total fossil fuel emissions. 



This finding highlights the severe impact of climate change on natural ecosystems.



The Amazon rainforest, one of the planet's most essential carbon sinks, is showing signs of long-term distress. Some regions of the Amazon that no longer absorb carbon have shifted into net sources of carbon emissions.



<h2 class="wp-block-heading" id="h-earth-s-declining-capacity-to-absorb-carbon">Earth's declining capacity to absorb carbon </h2>



The declining capacity of Earth's land ecosystems to absorb carbon dioxide may signify that these natural carbon sinks are nearing their limits. 



They won't be able to continue to provide the mitigation service of absorbing half of human-induced carbon dioxide emissions.



"Consequently, achieving safe global warming limits will require even more ambitious emission reductions than previously anticipated," Ciais adds.



<h2 class="wp-block-heading" id="h-saving-earth-s-carbon-cycle">Saving Earth's carbon cycle</h2>



The study also highlights that <a href="https://www.earth.com/news/climate-models-underestimate-sea-ice-melt-and-global-warming/" target="_blank" rel="noreferrer noopener">current climate models</a> might be underestimating the pace and impact of extreme events such as droughts and fires on the degradation of these crucial carbon reservoirs.



"Understanding the knock-on effects of climate change on the carbon cycle is imperative, and the two ESA study projects demonstrate the importance of Earth observation in developing methodologies to provide rapid assessment of these impacts globally," said Stephen Plummer, <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a> Earth Observation Applications Scientist.



"These results are particularly alarming, especially considering the difficulty the world is having limiting warming to 1.5°C, as laid out in the Paris Agreement," noted Clement Albergel, ESA’s Acting Head of the Actionable Climate Information Section.



Given these alarming revelations, it's vital that we ask ourselves: how can we contribute to mitigating these effects? Can we consume less, recycle more, and seek out greener alternatives in our daily lives? The need for climate action could not be more urgent.



The study is published in the journal <a href="https://academic.oup.com/nsr/advance-article/doi/10.1093/nsr/nwae367/7831648?login=false" target="_blank" rel="noreferrer noopener">National Science Review</a>.



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Extreme heat of 2023  weakened Earth's carbon storage capacity

The scorching heatwaves we experience, the wildfires that rage across...

Desolate, arid and virtually lifeless - that's how one would traditionally describe the Atacama Desert. Stretching across the Pacific coast in Chile, this unforgiving territory is known as the driest spot on our planet. It's no surprise that the desert is deemed hostile to most forms of life.



Yet, a closer look at the sandy soil reveals a perfect paradox - a diverse community of resilient microorganisms, thriving in the seeming desolation.



Investigating the function of these microorganisms can be challenging. Modern science tools often hit a wall while trying to separate the genetic material of the living from the dead in this <a href="https://www.earth.com/news/saharan-dust-supports-ocean-life-far-from-the-desert/" target="_blank" rel="noreferrer noopener">microbial community</a>.



But now, a promising solution to this mystery is at hand.



<h2 class="wp-block-heading" id="h-identifying-the-desert-microbes">Identifying the desert microbes </h2>



Presented this week in Applied and Environmental Microbiology, an international team of researchers announces a novel separation technique. 



This innovative method distinguishes extracellular (eDNA) from intracellular (iDNA) genetic material, casting a spotlight on the living members of the elusive microbial community.



The technique is a game-changer in studying microbial life in <a href="https://www.earth.com/news/floods-are-becoming-more-deadly-in-the-desert/" target="_blank" rel="noreferrer noopener">low-biomass environments</a> - an area where conventional DNA extraction methods have been falling short.



The research was led by Dr. Dirk Wagner from the GFZ German Research Centre for Geosciences in Potsdam. He believes this development could usher in a new era in microbial research.



<h2 class="wp-block-heading" id="h-active-life-in-arid-regions-of-desert">Active life in arid regions of desert</h2>



The microbiologists put their novel method to practice on soil samples collected from the Atacama Desert, running along a west-to-east path from the ocean's edge to the foothills of the Andes mountains. 



What they found was intriguing: a variety of potentially active microbes were discovered in the most arid regions of the desert.



"Microbes are the pioneers colonizing this kind of environment and preparing the ground for the next succession of life," said Dr. Wagner. He noted that these processes aren't exclusive to desert lands.



"This could also apply to new terrain that forms after earthquakes or landslides where you have more or less the same situation, a mineral or rock-based substrate."



<h2 class="wp-block-heading" id="h-new-approach-to-dna-extraction">New approach to DNA extraction</h2>



Conventional tools for DNA extraction from <a href="https://www.earth.com/news/desert-grass-survives-by-capturing-moisture-from-fog/" target="_blank" rel="noreferrer noopener">soils</a> often present a blend of living, dormant and dead cells from microorganisms.



“If you extract all the DNA, you have DNA from living organisms and also DNA that can represent organisms that just died or died a long time ago," explained Dr. Wagner.



The formidable challenge, especially in low-biomass environments, is securing sufficient good-quality DNA for metagenomic sequencing to unravel specific microbes and their processes. 



Dr. Wagner and his team have found a way around this by creating a process that filters out intact cells from a mixture, leaving behind eDNA genetic fragments from dead cells.



<h2 class="wp-block-heading" id="h-implications-for-extraterrestrial-life">Implications for extraterrestrial life</h2>



The significance of this research extends far <a href="https://www.earth.com/news/this-desert-moss-might-help-humans-live-on-mars/" target="_blank" rel="noreferrer noopener">beyond Earthly environments</a>. 



The techniques developed for distinguishing living microbial communities in the Atacama Desert could offer a tantalizing approach to astrobiology, a field dedicated to exploring life beyond our planet. 



Mars, with its barren and inhospitable terrain, presents a setting not unlike parts of the Atacama. Here, scientists speculate that if life ever arose, it might have persisted in microbial form beneath the surface. 



By applying this novel genetic separation technique, future missions to Mars could possibly identify signs of life that traditional methods might overlook, thus advancing our understanding of life's potential in the cosmos.



<h2 class="wp-block-heading" id="h-charting-future-research">Charting future research</h2>



The advent of this cutting-edge method represents a paradigm shift in microbial ecology and environmental microbiology. 



It opens up new avenues for research, not only in desolate regions like the Atacama Desert but also in other extreme environments such as Antarctic ice, deep-ocean vents, and arid regions worldwide. 



By accurately categorizing active microorganisms, we can better understand their roles in nutrient cycling, climate change, and biogeochemical processes. 



This refined approach provides a critical tool for scientists aiming to unravel the life forms that have evolved to thrive against the odds. It also lays the groundwork for future discoveries at the intersections of life, earth, and space sciences.



<h2 class="wp-block-heading" id="h-vibrant-life-beneath-atacama-desert">Vibrant life beneath Atacama Desert</h2>



Dr. Wagner plans to extend the study's methodology to other hostile environments. He believes that this technique, which focuses on active microorganisms (iDNA), can provide deeper insights into the active part of the community.



By examining the vibrant life thriving beneath the surface of the Atacama Desert, we are slowly unearthing the secret resilience of microbes in the most <a href="https://www.earth.com/news/oases-grow-by-human-effort-but-face-threats-from-desertification/" target="_blank" rel="noreferrer noopener">arid of environments</a>. 



As we continue to witness the incredible adaptation and survival of life in the harshest of conditions, the lines of possibility for microbial life continue to expand, taking us one step deeper into unraveling the mysteries of life itself.



The study is published in the journal <a href="https://search.app?link=https%3A%2F%2Fjournals.asm.org%2Fdoi%2F10.1128%2Faem.01443-24&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">Applied and Environmental Microbiology</a>.



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Living microbes found in the driest desert on Earth

Desolate, arid and virtually lifeless - that's how one would...

Pando, an extraordinary organism residing in Utah, quietly stands out among the myriad of living beings that inhabit our planet, captivating scientists and nature enthusiasts alike. 



This remarkable colony of quaking aspen trees (Populus tremuloides) stretches across 106 acres, and is connected by an extensive underground root system that forms a single, unified organism rather than just a forest of unrelated individuals.



With its remarkable size and age, Pando dwarfs its fellow inhabitants, holding the potential to be not only the oldest living being but also the largest organism on Earth. It is a symbol of nature's resilience and complexity over millennia.



<h2 class="wp-block-heading" id="h-utah-s-pride-the-incredible-pando">Utah's pride: The incredible Pando</h2>



A group of American researchers has suggested that this 106-acre woodland in the heart of Utah could have originated from a single seedling, which sprouted 34,000 years ago, pre-dating the end of the <a href="https://www.earth.com/news/disastrous-climate-changes-of-the-last-ice-age-could-happen-again/" target="_blank" rel="noreferrer noopener">last ice age</a>.



Even bolder estimates propose that this clonal organism, which appears to consist of 47,000 separate trees, might have been present tens of thousands of years earlier.



<h2 class="wp-block-heading" id="h-the-astonishing-life-of-clonal-organisms">The astonishing life of clonal organisms</h2>



Pando (which means "I spread" in Latin) is intriguing because of its massive size, but it also boasts a unique genetic identity shared by all its individual parts that are linked together through one vast network of roots.



This form of asexual reproduction makes Pando a <a href="https://www.earth.com/news/listening-to-the-largest-and-oldest-tree-on-earth-what-does-it-have-to-say/" target="_blank" rel="noreferrer noopener">clonal organism</a>, with each 'tree' being a part of the whole, rooted and growing from the same entity. 



There are other life forms, including fungi and the bristlecone pines on the White Mountains in eastern California, that display similar capabilities. They survive through <a href="https://www.earth.com/news/scientists-have-had-a-breakthrough-in-cloning-coconut-trees/" target="_blank" rel="noreferrer noopener">cloning</a> methods for hundreds, or even thousands of years.



<h2 class="wp-block-heading" id="h-unlocking-pando-s-historical-tales">Unlocking Pando's historical tales</h2>



To discern Pando's true age more accurately, the research team meticulously collected around 500 samples, including root, leaf, and bark, from different parts of this giant organism.



They also obtained specimens from other, unrelated aspens and embarked on a journey to sequence their DNA.



The scientists identified 4,000 genetic variations within these samples, and the mutation patterns narrated a captivating story that dates back potentially between 16,000 and 80,000 years.



<h2 class="wp-block-heading" id="h-unraveling-the-genetic-enigma">Unraveling the genetic enigma</h2>



The researchers, led by Rozenn Pineau of the <a href="https://www.uchicago.edu/en" target="_blank" rel="noreferrer noopener">University of Chicago</a>, noted that they had initially expected a close genetic correlation between trees that are physically near each other.



"You would expect that the trees that are spatially close are also closer genetically," Pineau told Helena Kudiabor at Nature. "But this is not exactly what we find. We found a spatial signal, but that is much weaker than what we expected."



Those trees that were in close proximity did share more similar mutations than those that were far apart - but only slightly more.



This discovery adds a new layer of complexity to understanding Pando's genetic structure and resilience.



Additional research focusing on Pando's mutation history and its genomic protection methods could provide insights into how this plant (and other similar organisms) has managed to survive for millennia.



<h2 class="wp-block-heading" id="h-ensuring-pando-s-enduring-legacy">Ensuring Pando's enduring legacy</h2>



Concerns are mounting over the longevity of Pando. Ensuring its survival will require a deep understanding of this ancient <a href="https://www.earth.com/news/plants-use-dna-duplication-to-increase-their-resilience/" target="_blank" rel="noreferrer noopener">plant's resilience</a> against the assaults of man and nature.



Moreover, similar investigations into other clonal organisms elsewhere may offer Pando competition for its venerable title. 



One competitor lies in a patch of Posidonia oceanica seagrass off the Spanish island of Formentera, which some believe to be more than 200,000 years old.



<h2 class="wp-block-heading" id="h-the-ecological-significance-of-pando">The ecological significance of Pando</h2>



Pando is more than just a marvel of age and size; it plays a crucial role in the local ecosystem. 



This vast network of quaking <a href="https://www.earth.com/news/aspen-forests-could-reverse-biodiversity-loss-in-europe/" target="_blank" rel="noreferrer noopener">aspens</a> supports a diversity of wildlife by providing habitat and food for numerous species, from insects and birds to larger mammals such as deer and elk.



The interconnected root system of Pando also aids in soil stabilization, which prevents erosion and supports the health of the surrounding environment.



However, understanding Pando's ecological contributions has become more urgent than ever, as climate change and human activities threaten its survival. 



Efforts to study and preserve this unique organism are now critical, not only to protect its ancient legacy but also to help maintain the delicate balance of the ecosystem it anchors.



<h2 class="wp-block-heading" id="h-the-enduring-hymns-of-pando">The enduring hymns of Pando</h2>



Pando's survival through the ages is a tribute to time itself. It stands as a constant reminder of the ancient world, sharing with us stories of an era long gone. 



As we continue to unravel the mysteries of Pando, we can only hope that this ancient marvel stands tall and flourishes in the years to come.



The research is published in <a href="https://www.biorxiv.org/content/10.1101/2024.10.19.619233v2">BioRxiv</a>.



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The world's largest living organism consists of 47,000 trees

Pando, an extraordinary organism residing in Utah, quietly stands out...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

[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...

GPM Core Observatory Centrifuge Testing. NASA technicians spun the GPM satellite up to just over 10 RPM at <a href="https://www.earth.com/video/new-magnetic-process/">Goddard Space Flight Center’s.</a>  High-Capacity Centrifuge facility on March 31st, 2011. At that speed, the spin exerted a lateral pressure of 2.4 G’s, or 2.4 times the force of gravity on the satellite.
Spin tests such as these are used to determine whether the forces of launch could adversely affect hardware we put into space. Therefore they test spacecraft chassis design.
In this case, a combination of flight hardware parts and the so-called mass model were spun. The mass model simulates the final size. And shape and weight distribution of the satellite and it’s component sensors, fuel, maneuvering thrusters. Therefore processing and control equipment.

GPM Core Observatory Centrifuge Testing

Engineers Prepare the <a href="http://www.earth.com/image/gpm-tanegashima-space-center/">GPM</a> Solar Array for Testing. The –Y wing prepares to undergo modal testing, a type of vibrational testing. Therefore small squares are 59 accelerometers that measure the movement of the array. Also GPM's two solar array wings that extend to the right (+Y) and left (-Y) of the spacecraft. And are currently undergoing assembly and testing at Goddard Space Flight Center, Greenbelt, Md. The solar arrays provide all the electrical energy for the satellite, and must survive flying in Earth's thin upper atmosphere at an altitude of 407 km (253 miles), where they will be subjected to small drag forces and exposure to corrosive atomic oxygen