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...

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

Today's Image of the Day from the European Space Agency features NGC 1333, a reflection nebula located in the Perseus molecular cloud about 960 light-years away from Earth. The photo is a mosaic of images captured by the James Webb Space Telescope.



<h2 class="wp-block-heading" id="h-the-power-of-webb-nbsp-nbsp">The power of Webb&nbsp;&nbsp;</h2>



“Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. Some of the faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



The same cluster was featured as the 33rd anniversary image of the Hubble Space Telescope in April 2023.&nbsp;



According to ESA, Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. 



"Observing with larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects."



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc1333">Webb’s view of NGC1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC1333 cloud.&nbsp;



“Across the image we see large patches of orange, which represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation."



The disks of gas and dust that surround the <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">stars</a> in this image may eventually produce planetary systems.&nbsp;



<h2 class="wp-block-heading" id="h-formation-of-the-sun">Formation of the Sun</h2>



“Similar to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster, which was perhaps even more massive than NGC 1333,” explained ESA.



Over time, the stars in the Sun's birth cluster would have drifted apart due to gravitational interactions and the dispersion of gas in the region.



Astronomers have been studying certain clues, such as isotopic signatures in meteorites, that hint the Sun may have formed near massive stars. These stars likely produced supernovae, which could have influenced the early <a href="https://www.earth.com/news/mysterious-objects-spotted-in-the-outer-solar-system-beyond-pluto/" target="_blank" rel="noreferrer noopener">solar system</a> by injecting heavy elements like iron-60.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1333">Star formation in NGC 1333</h2>



NGC 1333 is a vibrant example of a stellar nursery, where active <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 ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



Within NGC 1333, astronomers have observed a high level of turbulence, which makes the region dynamic and complex. 



These disturbances are caused by the outflows of young stars as they eject material into their surroundings, creating shock waves and influencing further star formation.&nbsp;



These outflows are often seen as jets, which are visible in multiple wavelengths of light, especially infrared, as the surrounding dust absorbs visible light.



<h2 class="wp-block-heading" id="h-significance-of-ngc-1333">Significance of NGC 1333</h2>



NGC 1333 is also an area of interest for studying the early stages of star and <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planet formation</a>, as many of the stars within the cluster are in their infancy, still in the process of gathering material and developing protoplanetary disks.&nbsp;



In images, NGC 1333 is marked by bright patches of blue and red, representing reflection <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebulae</a> and the ionized gas created by energetic young stars.&nbsp;



<h2 class="wp-block-heading" id="h-the-perseus-molecular-cloud-nbsp">The Perseus molecular cloud&nbsp;</h2>



The Perseus molecular cloud is a vast region of cold gas and dust located about 600 light-years away from Earth in the constellation <a href="https://www.earth.com/news/1500-billion-orphan-stars-discovered-in-the-perseus-galaxy-cluster/" target="_blank" rel="noreferrer noopener">Perseus</a>.&nbsp;



It is one of the most studied star-forming regions in our galaxy due to its relative proximity and the diversity of its young stellar objects. This cloud spans several hundred light-years and contains dense pockets of gas where new stars are actively forming.&nbsp;



These areas are often enshrouded in thick dust, which obscures them in visible light but allows astronomers to study them using infrared and radio wavelengths.



The Perseus molecular cloud is particularly interesting because of the chemistry taking place within it, including the formation of complex organic molecules that could be precursors to life.&nbsp;



Image Credit: ESA/Webb, NASA &amp; CSA



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Stellar nursery shines in the Perseus cloud

Today's Image of the Day from the European Space Agency features the colors of fall across the continent of Europe. 



“This compilation of images, captured by the Copernicus Sentinel-2 mission, showcases the characteristic hues of autumn in different European countries,” noted <a href="https://www.esa.int/Applications/Observing_the_Earth/Copernicus/Sentinel-2/Earth_from_Space_Autumn_foliage_across_Europe" target="_blank" rel="noreferrer noopener">ESA</a>.



“Autumn foliage is one of nature's most stunning displays, turning deciduous forests into landscapes painted with vibrant colors. As temperatures cool and daylight shortens, deciduous trees cease producing chlorophyll so that leaves turn yellow, orange and red – the colors of autumn.”



<h2 class="wp-block-heading" id="h-colors-of-fall-in-europe-nbsp">Colors of fall in Europe&nbsp;</h2>



The colors of <a href="https://www.earth.com/news/fall-will-be-unusually-warm-across-most-us-states/" target="_blank" rel="noreferrer noopener">fall</a> vary across regions due to the diversity of tree species and the climate.



<h3 class="wp-block-heading" id="h-northern-europe">Northern Europe</h3>



In countries like Norway, Sweden, and Finland, vibrant yellows and golds dominate, especially in forests of birch and aspen. Deep red hues come from the native rowan and some types of maple.



<h3 class="wp-block-heading" id="h-western-and-central-europe">Western and Central Europe</h3>



The landscapes of France, Germany, and Switzerland showcase golden and copper tones. Beech, oak, and chestnut trees create waves of yellow and bronze, while occasional maples provide shades of bright red.



<h3 class="wp-block-heading" id="h-eastern-europe">Eastern Europe</h3>



Countries like Poland, Ukraine, and Hungary experience a full mix of autumn colors, with maple and <a href="https://www.earth.com/news/should-we-cut-down-all-oak-trees-isoprene-emissions-air-pollution-climate-change/" target="_blank" rel="noreferrer noopener">oak forests</a> turning red and orange. The Carpathian Mountains are especially vibrant during this season.



<h3 class="wp-block-heading" id="h-southern-europe">Southern Europe</h3>



In Mediterranean areas like Italy, Spain, and Greece, fall colors are more subtle but still beautiful. Although many <a href="https://www.earth.com/news/trees-struggling-to-breathe-store-co2-hotter-climate/" target="_blank" rel="noreferrer noopener">trees</a> are evergreen, higher elevations display patches of golden-yellow and rusty tones from poplars, chestnuts, and maples.



The European fall color season typically peaks in October, depending on altitude and latitude. The dramatic landscapes of Europe - mountains, lakes, and historic villages - further enhance the stunning display of autumn colors across the continent.



<h2 class="wp-block-heading" id="h-why-do-the-leaves-change-colors">Why do the leaves change colors?</h2>



Leaves change color in the fall due to changes in daylight, temperature, and the chemical processes within the leaves.&nbsp;



During spring and summer, leaves are green because they contain chlorophyll, a pigment that allows them to absorb sunlight and produce food through photosynthesis.&nbsp;



However, as the days get shorter and temperatures drop in the fall, trees begin preparing for winter by slowing down their food production.



<h3 class="wp-block-heading" id="h-decrease-in-chlorophyll">Decrease in chlorophyll</h3>



With less sunlight, trees stop producing chlorophyll, which is highly sensitive to light and temperature. As chlorophyll breaks down, the green color fades, revealing other pigments in the leaves.



<h3 class="wp-block-heading" id="h-other-pigments-emerge-nbsp">Other pigments emerge&nbsp;</h3>



There are always other pigments in the leaves, but they’re hidden by the green chlorophyll during the growing season. In fall, these pigments become visible.



Carotenoids produce yellow and orange hues, which we see in trees like birch, beech, and aspen.



Anthocyanins are pigments that create reds, purples, and deep oranges. They form in the fall when sugars get trapped in the leaves. Trees like maple and sumac are known for their red and purple leaves.



Tannins produce brown colors and are especially visible in oaks.



<h3 class="wp-block-heading" id="h-weather-and-climate-influence">Weather and climate influence</h3>



Temperature, sunlight, and soil moisture also affect the intensity and duration of fall colors.&nbsp;



Sunny days and cool nights help produce more vibrant reds and purples. Wet or cloudy weather, on the other hand, can lead to more muted colors.



Ultimately, the color change is a part of the tree’s preparation for winter dormancy. By shedding <a href="https://www.earth.com/news/secrets-of-aging-discovered-in-plant-leaves/">leaves</a>, trees conserve water and energy, improving their chances of surviving the winter months.



<h2 class="wp-block-heading" id="h-how-do-the-fall-colors-affect-us">How do the fall colors affect us?</h2>



Fall colors can have a significant impact on us emotionally, mentally, and even physically. They provide us with a sense of warmth, nostalgia, and comfort.&nbsp;



<h3 class="wp-block-heading" id="h-emotional-uplift-nbsp">Emotional uplift&nbsp;</h3>



The vibrant colors of fall can evoke positive emotions and improve our mood. Studies show that exposure to natural landscapes with diverse colors can reduce stress, enhance feelings of happiness, and promote a sense of well-being.



Nature’s changing colors have a calming effect on our minds, providing mental clarity and relaxation. The natural beauty of fall landscapes can encourage mindfulness, allowing us to be present and appreciate our surroundings, which is beneficial for mental health and focus.



<h3 class="wp-block-heading" id="h-connection-to-nature">Connection to nature</h3>



Autumn’s beauty encourages people to go outside, whether it’s hiking through colorful forests, driving along scenic routes, or simply taking a walk in the park.&nbsp;



This connection with <a href="https://www.earth.com/news/nature-walking-quantifiably-improves-brain-health-and-functioning/" target="_blank" rel="noreferrer noopener">nature</a> has benefits for physical health, improving immunity and reducing blood pressure, and it also strengthens our environmental appreciation.



<h3 class="wp-block-heading" id="h-seasonal-reflection-nbsp">Seasonal reflection&nbsp;</h3>



The cycle of fall reminds us of change, letting go, and renewal. For many, fall is a time for introspection and resetting goals, as the season symbolizes transformation and the approach of a new chapter in life.



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Fall colors transform Europe's landscape 

Swirling sediment in the Caspian Sea is seen here in this Image of the Day from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> . It features a look at colorful sediment in the <a href="https://www.earth.com/image/phytoplankton-blooms-caspian-sea/">Caspian Sea</a> off the coast of Turkmenistan.

Swirling sediment in the Caspian Sea

Recent research highlights the link between air pollution and an increased risk of autism spectrum disorder (ASD) in children, particularly those with a genetic predisposition.&nbsp;



The study explores the role of nitric oxide (NO) and other pollutants in triggering complex biological responses that can impact neurodevelopment.



The research was led by Dr. Haitham Amal, head of the Laboratory of Neuromics, Cell Signaling, and Translational Medicine at the <a href="https://en.huji.ac.il/" target="_blank" rel="noreferrer noopener">Hebrew University</a> of Jerusalem.



“Meeting families and children with <a href="https://www.earth.com/news/autism-diagnoses-have-almost-tripled-in-the-us-over-the-past-ten-years/" target="_blank" rel="noreferrer noopener">autism</a> in Boston during my time at MIT inspired me to focus on a single goal: to help develop biological diagnostics and treatment for autism spectrum disorder,” Amal said.&nbsp;



This encounter shaped his career, leading him to investigate the ways environmental and genetic factors combine to influence ASD risk.



<h2 class="wp-block-heading" id="h-pollution-s-impact-on-neurodevelopment">Pollution’s impact on neurodevelopment</h2>



<a href="https://www.earth.com/news/understanding-how-air-pollution-forms-may-help-us-prevent-it/" target="_blank" rel="noreferrer noopener">Air pollution</a> contains several harmful elements, including particulate matter, nitrogen oxides, sulfur dioxide, and ozone. 



These pollutants, when inhaled, can bypass the blood-brain barrier, leading to inflammation and changes in neural functioning. 



The research emphasizes how particles such as PM2.5 - microscopic particles from sources like construction and car exhaust - and NO products can cross the placenta, directly impacting fetal brain development.&nbsp;



“My lab has shown that nitric oxide plays a major role in ASD,” Amal said, highlighting NO’s key role in brain health.



The review notes how urban areas with high pollution levels, such as Phoenix, San Jose, and Eugene, expose residents, particularly expectant mothers, to levels of pollution that may impact early childhood development.&nbsp;



A report from the <a href="https://www.lung.org/" target="_blank" rel="noreferrer noopener">American Lung Association</a> shows that 39 percent of the U.S. population lives in areas with concerning air quality, which, combined with genetic predispositions, could be a driving factor behind rising autism rates.



<h2 class="wp-block-heading" id="h-pollution-exposure-and-biological-pathways">Pollution exposure and biological pathways</h2>



The review presents evidence of several biological pathways that may link pollution exposure to increased autism risk.



<h3 class="wp-block-heading" id="h-nitrosative-stress-and-nitric-oxide">Nitrosative stress and nitric oxide</h3>



Nitrosative stress caused by NO has been shown to affect neurological development. This was one of Dr. Amal’s foundational discoveries.



<h3 class="wp-block-heading" id="h-neuroinflammation-and-oxidative-stress">Neuroinflammation and oxidative stress</h3>



Inhaled pollutants can prompt inflammation within the brain, which interferes with nerve development, potentially contributing to the behavioral symptoms associated with autism.



<h3 class="wp-block-heading" id="h-neurotransmitter-disruption">Neurotransmitter disruption</h3>



Pollutants may interrupt the balance of crucial brain chemicals like <a href="https://www.earth.com/news/dopamine-helps-us-learn-from-positive-and-negative-experiences/" target="_blank" rel="noreferrer noopener">dopamine</a> and norepinephrine, which play a role in decision-making and overall cognitive development.



The experts reviewed studies on both human and animal models to examine these biological effects, linking the presence of certain pollutants to changes in neural functioning. 



The findings show that pollutants, particularly NO, can cross the placenta and directly affect the fetus.&nbsp;



This sensitivity during prenatal and early childhood development stages, when the brain is rapidly growing, makes the body especially vulnerable to external factors.



<h2 class="wp-block-heading" id="h-convergence-of-genetics-and-environment">Convergence of genetics and environment</h2>



Autism has a strong genetic component, with estimates suggesting that 40-80% of cases may have a genetic basis. However, the scientists argue that genetics alone cannot explain the condition’s rising prevalence.&nbsp;



“The timing of exposure appears crucial, with heightened vulnerability during prenatal development and early childhood,” Amal explained.&nbsp;



The review suggests that while a genetic predisposition to autism can increase sensitivity to pollutants, environmental triggers -- especially air pollution -- may interact with genetics to further elevate autism risk.



A separate Harvard study showed that exposure to fine particulate matter early in life may increase the risk of autism by up to 64 percent, and prenatal exposure may elevate risk by 31 percent. 



This interaction between genes and environment presents a new model for understanding autism’s etiology.



<h2 class="wp-block-heading" id="h-early-interventions-for-at-risk-populations-nbsp">Early interventions for at-risk populations&nbsp;</h2>



As air quality deteriorates with urban expansion, there is an urgent need to assess pollution’s impact on vulnerable populations.&nbsp;



Amal’s findings suggest that governments may need to adjust urban planning and pollution monitoring to safeguard <a href="https://www.earth.com/news/prenatal-pollution-exposure-linked-to-cognitive-impairment/" target="_blank" rel="noreferrer noopener">prenatal</a> health.



The study also points to future research opportunities, particularly in developing biomarkers for early ASD detection.&nbsp;



By identifying specific indicators of pollution-related neurological stress, doctors may one day be able to screen infants and at-risk populations with greater accuracy.



“Different kinds of neurological disorders, including autism spectrum disorder, can be associated with this environmental factor,” Amal said.&nbsp;



His team is examining whether combining genetic and environmental data can improve diagnostics, which could enable earlier intervention for at-risk populations.



<h2 class="wp-block-heading" id="h-pollution-and-autism-prevalence">Pollution and autism prevalence </h2>



The study calls for extensive research to explore how various pollutants impact brain development.&nbsp;



“The research suggests that individuals with genetic predisposition to ASD may be more vulnerable to the harmful effects of air pollution exposure,” Amal said.&nbsp;



As ASD prevalence rises worldwide, this research may drive the development of preventive policies, such as targeted air quality monitoring in cities.



In addition, Amal’s work highlights the need for preventive strategies in communities facing heightened pollution levels.&nbsp;



His insights may prompt city planners, healthcare providers, and families to prioritize air quality improvements, especially in high-risk areas.



<h2 class="wp-block-heading" id="h-pollution-and-neurological-disorders">Pollution and neurological disorders</h2>



Amal’s pioneering work not only contributes to autism research but has implications for other neurological conditions.&nbsp;



The connections he draws between nitric oxide, ASD, and <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> suggest shared molecular pathways. By addressing NO-related neuroinflammation, treatments may eventually target multiple brain conditions.



The study ultimately underscores the power of interdisciplinary research in addressing complex conditions like autism.&nbsp;



As Amal concludes, his laboratory’s commitment to examining environmental factors alongside genetic predispositions could significantly impact the landscape of neurological disorder treatment, benefiting both current and future generations.



The study is published in the journal <a href="https://bm.genomicpress.com/wp-content/uploads/2024/11/BM0115-Amal-2024.pdf" target="_blank" rel="noreferrer noopener">Brain Medicine</a>.



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Air pollution discovered to be a "critical risk factor" for autism

Recent research highlights the link between air pollution and an...

Earworms - those persistent tunes that play in our heads unbidden - can be more than a minor annoyance.



Imagine going about your day when, without warning, a song loops repeatedly in your mind. 



While these spontaneous musical memories can feel intrusive, earworms offer a fascinating glimpse into the precision of our musical recall.



<h2 class="wp-block-heading" id="h-unveiling-the-mystery-of-earworms">Unveiling the mystery of earworms</h2>



A recent study has shed light on the surprising accuracy of earworms.



Published in the journal Attention, Perception, &amp; Psychophysics, the study revealed that nearly half of participants' renditions of earworms matched the original <a href="https://www.earth.com/news/most-people-have-a-hidden-musical-talent-for-singing-on-pitch/" target="_blank" rel="noreferrer noopener">pitch</a> of the songs.



This finding challenges prior beliefs about the limitations of musical memory, suggesting that our brains may preserve detailed “absolute pitch” memories even without formal pitch recognition skills.



Earworms, experienced by over 90% of people, are involuntary musical memories that spontaneously play in our minds. 



This study indicates that our recall of <a href="https://www.earth.com/news/song-melodies-have-become-much-simpler-since-1950/" target="_blank" rel="noreferrer noopener">melodies</a> may be more precise than previously thought, even without external references.



<h2 class="wp-block-heading" id="h-encountering-music-in-a-new-light">Encountering music in a new light</h2>



Matthew G. Evans, PhD candidate at <a href="https://admissions.ucsc.edu/" target="_blank" rel="noreferrer noopener">UC Santa Cruz</a>, said he first learned about the field of <a href="https://www.earth.com/news/music-can-prevent-brain-aging-and-cognitive-decline/" target="_blank" rel="noreferrer noopener">music</a> cognition from Daniel Levitin’s book&nbsp;This Is Your Brain On Music. 



"In that book, he describes a study where they found evidence for absolute pitch recall in voluntarily-recalled musical imagery - and I tried it myself, and it worked, and I’ve been hooked on the topic of musical memory ever since.”



Evans set out to investigate whether this accurate recall extended to spontaneous earworms or was limited only to songs that people purposefully tried to remember.



<h2 class="wp-block-heading" id="h-earworms-more-than-just-random-tunes">Earworms: More than just random tunes</h2>



The study involved 30 undergraduate students who participated in a two-week research period aimed at exploring the accuracy of spontaneous musical recall. 



Using the experience sampling method, the researchers documented these involuntary musical memories in real time by sending participants random text prompts throughout the day.



Students were asked to record any song playing in their minds, capturing the natural occurrence of earworms outside of a controlled laboratory setting.



While most participants had some familiarity with music, none reported having perfect pitch or formal training that would give them an advantage in recalling exact musical notes. 



Each recording was analyzed against the original <a href="https://www.earth.com/news/the-evolution-of-song-lyrics-less-complexity-and-more-emotion/" target="_blank" rel="noreferrer noopener">song</a> to determine how closely the pitch matched the song’s actual key. 



The findings were striking: 44.7% of the earworms matched the original song’s pitch exactly. When the range was expanded to include recordings within one semitone of the original pitch, nearly 69% of the renditions met this criterion - far surpassing what could be attributed to random chance.



<h2 class="wp-block-heading" id="h-the-melodic-imprint-of-our-brains">The melodic imprint of our brains</h2>



The study also found that pitch accuracy was not significantly affected by recent exposure to a song.



Some participants noted that their earworm was triggered by recently hearing the song, but their ability to match the original pitch remained similar to those whose earworms were not influenced by recent listening.



"When we divided our data into responses where participants said they had recently heard the song and those where they hadn’t, we saw absolutely no difference in absolute pitch accuracy," noted Evans. 



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



While this study provides valuable insights into how we recall music, it also highlights the need for further research to validate and expand upon these findings. 



To gain a broader understanding of how earworms and pitch recall function across different populations, future studies should incorporate a larger and more diverse participant pool, including individuals with no musical background and participants from varied age groups and cultural settings.



By expanding the scope of the research, scientists could explore questions such as whether musical memory accuracy varies by age, cultural exposure to music, or training. 



It may also be valuable to investigate whether factors such as musical genres or personal attachment to specific songs influence pitch accuracy in earworms.



This research marks an early step in unraveling the complex mechanisms of our brain's musical memory. 



As future studies build on this foundational work, we may discover more about the intricate ways in which our minds store and retrieve musical information, shedding light on the intersection of <a href="https://www.earth.com/news/memory-is-shaped-by-both-past-and-future-experience-and-events/" target="_blank" rel="noreferrer noopener">memory</a>, perception, and cognitive processes.



The study is published in the journal <a href="https://link.springer.com/article/10.3758/s13414-024-02936-0" target="_blank" rel="noreferrer noopener">Attention, Perception, &amp; Psychophysics</a>.



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Earworms: The surprising accuracy of our musical memory

Earworms - those persistent tunes that play in our heads...

Imagine Earth, our blue planet, not with sparkling blue oceans and sweeping green terrains, but as a giant chunk of ice. This "Snowball Earth" scenario might not be just a figment of our imagination. Rather, it could very well have been Earth's reality millions of years ago.



In an intriguing new study conducted by the University of Colorado Boulder, researchers have provided compelling evidence indicating that giant glaciers cloaked our Earth all the way to its equator hundreds of millions of years ago. This icy makeover would have turned our beautiful planet into a celestial icicle.



<h2 class="wp-block-heading" id="h-ice-age-and-snowball-earth">Ice Age and Snowball Earth</h2>



This study comes as a major breakthrough for supporters of an <a href="https://www.earth.com/news/snowball-earth-event-set-the-stage-for-complex-life/" target="_blank" rel="noreferrer noopener">enduring theory</a> known as Snowball Earth. 



According to this theory, from around 720 to 635 million years ago, an array of events radically altered the climate of our planet. The temperatures plummeted and huge ice sheets, possibly several miles thick, enveloped our planet from pole to pole.



"This study presents the first physical evidence that Snowball Earth reached the heart of continents at the equator," noted Liam Courtney-Davies, the lead author of the new study and a postdoctoral researcher in the Department of Geological Sciences at <a href="https://www.colorado.edu" target="_blank" rel="noreferrer noopener">CU Boulder</a>.



The team of co-authors included Rebecca Flowers, a professor of geological sciences at CU Boulder, and researchers from Colorado College, <a href="https://www.universityofcalifornia.edu" target="_blank" rel="noreferrer noopener">University of California</a>, Santa Barbara, and University of California, Berkeley.



<h2 class="wp-block-heading" id="h-rocky-mountains-hold-the-key">Rocky mountains hold the key</h2>



The researchers centered their focus on the Front Range of Colorado's Rocky Mountains. A charming array of rocks, lovingly nicknamed the Tavakaiv or "Tava" sandstones, reside here. According to Courtney-Davies, these rocks hold the coveted key to our <a href="https://www.earth.com/news/earth-had-massive-rapid-melting-period-that-left-the-surface-slushy/" target="_blank" rel="noreferrer noopener">planet's frigid past</a>.



The geologists utilized a dating technique known as laser ablation mass spectrometry. This is a method that frees some of the atoms inside the minerals by zapping them with lasers.



Through this process, the scientists discovered that these rocks were forced underground between about 690 to 660 million years ago, most likely due to the immense weight of the overlying glaciers.



<h2 class="wp-block-heading" id="h-snowball-earth-beyond-geology">Snowball Earth beyond geology</h2>



But the implications of this study are not restricted to the realm of geology. 



Courtney-Davies noted that the findings also have profound implications for understanding a critical phase in the evolution of life on Earth. The theory goes that the first multicellular organisms possibly made their appearance in our oceans right after Snowball Earth thawed out.



“You have the climate evolving, and you have life evolving with it. All of these things happened during Snowball Earth upheaval,” explained Courtney-Davies. “We have to better characterize this entire time period to understand how we and the planet evolved together.”



<h2 class="wp-block-heading" id="h-snowball-earth-theory">Snowball Earth theory</h2>



Ever since the term “Snowball Earth” was first proposed in a 1992 paper by American geologist Joseph Kirschvink, it has prompted substantial debate among scientists.



While geologists have indeed discovered the signs of thick ice from this era in ancient coastal areas, evidence within the interior of continents near the equator has been conspicuously absent.



Enter Colorado. Hundreds of millions of years ago, Colorado was not positioned at the northern latitudes where it is today.



In fact, it was snugly placed over the equator as an integral part of the ancient supercontinent Laurentia. If glaciers did indeed form here, it implies they could have formed just about anywhere.



<h2 class="wp-block-heading" id="h-unearthing-the-past">Unearthing the past</h2>



Eager to uncover this elusive missing piece of the Snowball Earth puzzle, Courtney-Davies and his team turned to the Tava sandstones. These sandstones, predominantly visible around Pikes Peak, may appear as average yellow-brown rocks to an untrained eye. But to a geologist, they tell an extraordinary tale.



These features likely began as sands at Colorado's surface. However, certain forces pushed them underground, akin to claws digging into the Earth's crust. Courtney-Davies wanted to determine whether these sandstones were also linked to the presence of ice sheets.



To do so, the scientists calculated the ages of mineral veins traversing these features. They collected minute samples of the minerals, rich in iron oxide (essentially rust), and zapped them with a laser.



Consequently, the minerals released small quantities of the radioactive element uranium. Since uranium atoms decay into lead at a constant rate, the team used them as a timekeeper to determine the age of these rocks.



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



The findings implied that the Tava sandstone had indeed been forced underground during the Snowball Earth period. The team suspects that thick ice sheets formed over Colorado at the time, subjecting the sands to tremendous pressure, and ultimately, pushing them into the bedrock below.



"We're excited that we had the opportunity to unravel the story of the only Snowball Earth deposits that have so far been identified in Colorado," said Flowers.



The entrepreneurial researchers are not ones to rest on their laurels, though. If such features formed in Colorado during Snowball Earth, they could very well have formed in other parts of North America. 



“We want to get the word out so that others try and find these features and help us build a more complete picture of Snowball Earth," noted Courtney-Davies.



So, next time you find yourself staring at an ice cube, consider this: once upon a time, our entire planet might have <a href="https://www.earth.com/news/earth-was-a-giant-snowball-700-million-years-ago-and-now-scientists-know-why/" target="_blank" rel="noreferrer noopener">looked just like that</a>. A tiny, frozen ball suspended in the vast expanse of space. Sounds like a chilling tale, doesn't it?



The study is published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2410759121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Ancient rocks suggest that Earth was once a 'snowball'

Imagine Earth, our blue planet, not with sparkling blue oceans...

We often hear about the insidious creep of climate change and the warming that's altering landscapes around the world. Well, the Arctic and its plants aren't immune to this silent invasion.



New evidence suggests that it's not just the temperature change we should be monitoring, but also our hoofed friends out on the tundra. Arctic greening, as it is often called, might be more about caribou and muskoxen than we ever realized.



<h2 class="wp-block-heading" id="h-greening-of-the-arctic-landscape">Greening of the Arctic landscape </h2>



Research released from the University of California, Davis (<a href="https://www.ucdavis.edu/academics/graduate" target="_blank" rel="noreferrer noopener">UC Davis</a>) indicates that the large grazers of the Arctic landscape - the caribou and muskoxen - have a direct effect on the timing and abundance of Arctic plants.



This correlation reveals significant implications for the <a href="https://www.earth.com/news/why-planting-trees-in-the-arctic-is-not-a-good-climate-solution/" target="_blank" rel="noreferrer noopener">overall Arctic ecosystem</a>. 



The findings were recently detailed in a study published in the journal PNAS Nexus and illuminate the vital role that these large herbivores play in our understanding of the Arctic ecosystem.



The focus of the narrative so far has been climate change and the increasing temperatures, but there seems to be more to it than that.



<h2 class="wp-block-heading" id="h-plants-emerging-in-the-arctic">Plants emerging in the Arctic</h2>



To fully appreciate the impact of this discovery, it's essential that we first understand phenology- the study of timing and patterns in nature.



It's what alerts us when birds are migrating, or when a plant first bursts to life or bursts into bloom. Within the context of a rapidly warming <a href="https://www.earth.com/news/how-melting-arctic-sea-ice-could-disrupt-earths-climate/" target="_blank" rel="noreferrer noopener">Arctic</a>, understanding these patterns becomes critical.



“Caribou and muskoxen play a key role in how soon plants emerge and this translates to how abundant they become,” said lead author Eric Post, a professor and arctic ecologist in the UC Davis Department of Wildlife, Fish and Conservation Biology. 



“This is an important, and overlooked, factor we need to consider as we seek to more fully understand climate change impacts on tundra vegetation in the Arctic.”



<h2 class="wp-block-heading" id="h-herbivores-and-plant-growth">Herbivores and plant growth </h2>



The research that led to these insights was conducted over a period of 22 years near Kangerlussuaq, Greenland. Here, Post and his team designed an exclusion experiment to understand the effect of herbivores on the timing of plant growth and abundance.



The researchers compared the timing of spring green-up of nine plant species with and without the grazing animals, from 2009 to 2017.



The overall conclusion was that plants where caribou or muskoxen were present underwent earlier green-up and enjoyed greater abundance later into the growing season.



However, not all plants responded equally to the grazing. While about two-thirds of plants greened up earlier, and three-quarters thrived more effectively later in the season with grazing animals present, some species such as dwarf birch and harebell emerged later when grazers were present.



<h2 class="wp-block-heading" id="h-impact-of-herbivore-grazing">Impact of herbivore grazing</h2>



While it's still unclear why Arctic plants respond this way to the presence of grazers, what is clear is that there is a connection.



“We’re used to thinking of the timing of plant availability as impacting the productivity of grazing animals, but not the reverse,” Post said. “The absence or presence of herbivores can also impact the timing of plant growth and their productivity.”



This understanding becomes increasingly important in light of the <a href="https://www.earth.com/news/arctic-ocean-warming-four-times-faster-than-global-average/" target="_blank" rel="noreferrer noopener">current decline</a> of many caribou populations in the Arctic. According to the IUCN Red List, migratory tundra caribou are now considered vulnerable, having lost more than half of their total abundance since the 1990s.



<h2 class="wp-block-heading" id="h-planting-trees-in-the-arctic">Planting trees in the Arctic</h2>



In a related study, Post suggested that supporting sustainable populations of herbivores in the Arctic could be a more effective nature-based solution to climate change in the region than planting trees there. The findings of the PNAS Nexus study lend credence to this suggestion.



We now have a better understanding of the crucial role our hoofed friends play in the Arctic ecosystem, but it is clear that more research is needed.



The challenge is enormous, yet with every bit of new knowledge, we get one step closer to a comprehensive understanding of the <a href="https://www.earth.com/news/air-pollution-alters-the-atmosphere-in-the-remote-arctic/" target="_blank" rel="noreferrer noopener">Arctic ecosystem</a> and how we can best protect it against the backdrop of climate change.



The study is published in the journal <a href="https://dx.doi.org/10.1093/PNASNEXUS-2024-00279RR" target="_blank" rel="noreferrer noopener">PNAS Nexus</a>.



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Arctic grazers secretly shape plant growth and survival

We often hear about the insidious creep of climate change...

Psilocybin, a compound at the forefront of psychedelic research, has sparked new hope in the perennial quest for an effective cure for psychiatric ailments, particularly anorexia nervosa. 



A clinical trial conducted by researchers at the University of California, San Diego (UCSD) highlights how this compound could potentially revolutionize treatment methods and result in improved clinical outcomes.



<h2 class="wp-block-heading" id="h-psilocybin-s-effect-on-anorexia-patients">Psilocybin’s effect on anorexia patients</h2>



<a href="https://www.earth.com/news/mental-disorders-can-be-contagious-among-teens/" target="_blank" rel="noreferrer noopener">Anorexia nervosa</a> is a psychiatric disorder that has resisted conventional treatments and currently has no effective medications approved by the US Food and Drug Administration. It is also the psychiatric illness that holds the record for having the highest mortality rate.



The <a href="https://ucsd.edu/" target="_blank" rel="noreferrer noopener">UCSD</a> research explores the effect of psilocybin treatment on this condition and provides a first-hand account of its consequences.



“Our findings suggest that psilocybin may be helpful in supporting meaningful psychological change in a subset of people with anorexia nervosa," explained Dr. Stephanie Knatz Peck, lead author of the study.



"What's particularly interesting is that 60% of participants reported a reduction in the importance of physical appearance, while 70% noted quality-of-life improvements and shifts in personal identity."



<h2 class="wp-block-heading" id="h-psilocybin-treatment-outcomes">Psilocybin treatment outcomes </h2>



The clinical trial revealed some fascinating outcomes. An overwhelming 90% of participants described their psilocybin session as one of the top five most meaningful experiences of their lives.



Additionally, 40% of the subjects showed clinically significant reductions in eating disorder psychopathology.



However, despite these positive results, the study notes that improvements in psychological outlook did not necessarily translate to weight restoration. 



Furthermore, psilocybin treatment appeared to work very effectively for some individuals while others showed minimal improvements. 



These discrepancies highlight the need for further research, particularly into how genetic variations in serotonin receptors might influence treatment outcomes.



<h2 class="wp-block-heading" id="h-transformative-experience-for-some-patients">Transformative experience for some patients </h2>



The impact of this treatment transcends the scientific data and filters into the personal lives of the subjects. 



As one participant shared: “You are able to act in a way that maybe had felt unachievable before, if you set the right intention.”



Another participant echoed similar sentiments, stating: “Things might not look that different from the outside, but they feel completely different from the inside.”



<h2 class="wp-block-heading" id="h-further-research-is-needed">Further research is needed</h2>



The study employed a single 25mg dose of psilocybin alongside specialized <a href="https://www.earth.com/news/overweight-depression/" target="_blank" rel="noreferrer noopener">psychological</a> support before, during, and after administration. 



Despite showcasing potential, the results also highlight the intricacy of treating anorexia nervosa and suggest a synergistic approach might be the most effective.



Dr. Walter H. Kaye, the study's senior author and UCSD Eating Disorders Treatment Center director, maintains that while the findings are promising, they need to be backed by larger, well-controlled studies. 



This includes the use of <a href="https://www.earth.com/news/brain-imaging-method-will-unravel-mysteries-of-neural-processes/" target="_blank" rel="noreferrer noopener">brain imaging</a> and genetic analysis to ascertain who might benefit most from this innovative treatment approach.



<h2 class="wp-block-heading" id="h-personalized-medicine-for-eating-disorders">Personalized medicine for eating disorders </h2>



The fascinating findings of the clinical trial initiated new trajectories for personalized medicine for eating disorders. 



However, it also sparked a flurry of questions around optimizing therapeutic protocols for this vulnerable demographic. 



Surely, it's a profound addition to the current discourse around non-traditional treatment methods.



<h2 class="wp-block-heading" id="h-challenges-of-psilocybin-therapy">Challenges of psilocybin therapy</h2>



The promise of psilocybin as a treatment for anorexia nervosa comes with its share of challenges. One major concern is ensuring that the therapy takes place in a safe, supportive environment. 



Psychedelic experiences can be intense and unpredictable, making it crucial to have professional guidance in place to support patients before, during, and after treatment.



This guidance helps maximize the benefits while minimizing any potential risks or adverse reactions.



There are also questions about how psilocybin therapy could fit into existing treatment plans. Researchers are looking at how it might complement traditional methods like <a href="https://www.earth.com/search-results/?search=cognitive-behavioral%20therapy&amp;start=0" target="_blank" rel="noreferrer noopener">cognitive-behavioral therapy</a> to boost long-term recovery. 



As more studies are conducted, it will be vital to address these challenges and questions. Only then can psilocybin potentially become a reliable, safe, and effective treatment option for those battling the complexities of anorexia nervosa.



The journey forward is one of thorough research, careful observation, and continued exploration to bring the best possible outcome to patients who need it most.



The study is published in the journal <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC10427429/" target="_blank" rel="noreferrer noopener">Nature Medicine</a>.



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Psilocybin shows promise for treating anorexia

Psilocybin, a compound at the forefront of psychedelic research, has...

The mystery of the moon and its origins has Intrigued scientists for centuries. During the Kona Conference of Hawaii in 1984, a group of moonstruck scientists analyzed approximately 363 kg of lunar material brought back by NASA's Apollo missions.



The experts found that the moon's chemical composition is strikingly similar, but not identical, to Earth's.



A conclusion was drawn that perhaps the moon was born from the debris cast off during a heavy impact between a <a href="https://www.earth.com/news/how-did-earth-get-its-moon-a-new-theory-has-emerged/" target="_blank" rel="noreferrer noopener">celestial body</a> and a young Earth.



This protoplanet, given the name "Theia," is believed to have caused an explosive aftermath that led to the formation of our moon. 



<h2 class="wp-block-heading" id="h-binary-exchange-capture-theory">Binary-exchange capture theory</h2>



Not all scientists are onboard with the theory of Theia. Some, like experts at Penn State University, suggest a different origin story for our moon. 



The researchers propose that Earth may have swooped the <a href="https://www.earth.com/news/2024-pt5-mini-moon-say-goodbye-to-earths-second-moon-we-barely-got-to-know-you/" target="_blank" rel="noreferrer noopener">moon</a> into its orbit during a process called "binary-exchange capture."



Just like plucking an apple from a tree, the Earth may have captured one satellite from a pair of rocky bodies orbiting each other.



"No one knows how the moon was formed. For the last four decades, we have had one possibility for how it got there. Now, we have two," noted Professor Darren Williams, the lead researcher from <a href="https://www.psu.edu" target="_blank" rel="noreferrer noopener">Penn State University</a>.



<h2 class="wp-block-heading" id="h-did-earth-capture-its-moon">Did Earth capture its moon?</h2>



The proponents of the binary-exchange capture theory argue that if the <a href="https://www.earth.com/news/its-official-earth-now-has-two-moons-captured-asteroid-2024-pt5/" target="_blank" rel="noreferrer noopener">moon</a> was born out of a ring of debris, it should orbit above our equator. However, the moon's orbit is tilted at about seven degrees from the equatorial plane.



This tilt could be explained by the binary-exchange capture theory. Could it be that the Earth ensnared one of a pair of passing rocky bodies to make it into its satellite while the other was flung into oblivion?



The plausibility of this theory is backed by previous research on Triton, Neptune's largest moon. 



Triton, like our moon, orbits its planet at an unusual angle, hinting that it was once part of a binary pulled into Neptune's orbit from the Kuiper Belt.



<h2 class="wp-block-heading" id="h-how-could-the-moon-capture-happen">How could the moon capture happen?</h2>



Mathematically speaking, capturing the moon is entirely possible. 



According to the research, Earth could have seized an object between one and 10 percent of its total mass. At 1.2 percent of Earth's mass, the moon fits this criterion neatly.



The only condition is that the binary pair would have to pass within 80,000 miles of Earth at a speed below 6,700 miles per hour. 



If everything fell into place, the moon's initial orbit would have been quite erratic, possibly resembling a comet's journey around the sun. However, over time, tidal forces would have rounded this orbit.



"Today, the Earth tide is ahead of the <a href="https://www.earth.com/news/this-weekends-strawberry-moon-is-the-sweetest-of-the-year/" target="_blank" rel="noreferrer noopener">Moon</a>, high tide accelerates the orbit. Over time, the moon drifts a bit farther away," noted Williams.



<h2 class="wp-block-heading" id="h-complexity-of-the-moon-s-origin-story">Complexity of the moon's origin story </h2>



A deeper geochemical analysis of lunar samples continues to add layers of complexity to the moon's origin story. Recent studies examining the carbon content of these samples have revealed intriguing discrepancies that challenge the established narratives. 



The discrepancies suggest that there might have been different environments or events that contributed to the moon’s current composition, further complicating the binary-exchange capture theory and the protoplanet collision model. 



"The carbon anomalies in lunar rocks open new doors to understanding the processes that shaped our moon," noted Dr. Lisa Simpson, a prominent geochemist.



<h2 class="wp-block-heading" id="h-the-prospect-of-future-lunar-missions">The prospect of future lunar missions</h2>



As we advance technologically, the prospect of future <a href="https://www.earth.com/news/scientists-learn-composition-of-moons-interior-core-its-not-green-cheese/" target="_blank" rel="noreferrer noopener">lunar missions</a> grows ever more promising, offering unparalleled opportunities to unravel the moon’s enigmatic past. 



These missions aim to employ state-of-the-art equipment to gather more data, testing existing theories and potentially offering fresh insights. 



For instance, plans to analyze deeper strata of lunar material might hold the key to uncover epochal events that are hidden beneath the surface.



Coupled with advancements in artificial intelligence, these ventures will help us simulate the moon’s geological history with unprecedented accuracy. 



<h2 class="wp-block-heading" id="h-mystery-of-the-moon-s-origin">Mystery of the moon's origin</h2>



"With each mission, we peel back a layer of mystery, inching closer to a comprehensive understanding of our closest cosmic companion," said Professor John Carter, who is leading the upcoming lunar exploration project.



It's safe to say that the mystery of the moon's origin isn't entirely solved. After all, Williams himself noted that the binary-exchange capture theory relies on several "implausible events." However, it opens up exciting avenues for future scientific exploration.



The study is published in <a href="https://search.app?link=https%3A%2F%2Fiopscience.iop.org%2Farticle%2F10.3847%2FPSJ%2Fad5a9a&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">The Planetary Science Journal</a>.



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Earth may have 'captured' the moon from space

The mystery of the moon and its origins has Intrigued...

Researchers have discovered that mangrove forests - a shield against destructive storms across many coastlines - are now suffocating underwater in the Maldives.



The data shows that the combination of an escalating sea level and a shift in Indian Ocean conditions has caused some Maldivian islands to lose more than half of their mangrove <a href="https://www.earth.com/news/mangroves-and-saltmarshes-are-much-better-at-storing-carbon-than-previously-believed/" target="_blank" rel="noreferrer noopener">cover</a> since 2020.



The researchers, led by Lucy Carruthers and Dr. Vasile Ersek of Northumbria University, noted that this isn't a singular incident affecting only the Maldives. 



The experts said that extreme climate events represent an emerging threat to mangroves and coastal ecosystems worldwide.



<h2 class="wp-block-heading" id="h-slowly-deteriorating-mangroves">Slowly deteriorating mangroves</h2>



In 2020, the mangroves on more than a quarter of the Maldives islands started showing signs of slow deterioration, sliding into a state known as dieback, before bidding the world adieu. 



The intensity of this mangrove loss phenomenon was captured by satellite imagery. The experts found that some islands had lost more than half of their mangrove cover.



For their investigation of mangrove dieback, the researchers combined evidence from sea level, climate data, and remote sensing. Field observations of sediment geochemistry and dendrology were also taken into consideration.



<h2 class="wp-block-heading" id="h-signs-of-salinity-stress-in-mangroves">Signs of salinity stress in mangroves </h2>



According to the results, the dead trees exhibited increased signs of salinity stress when compared to their living counterparts.



This stress gives us a clue that the tree roots were having a tough time dealing with the heightened salt levels, which played a key role in their demise.



The scientists concluded that sea levels around the Maldives had risen at an escalated rate of over 30mm per year from 2017 to 2020. 



Adding fuel to the fire, there was a particularly intense shift in the Indian Ocean Dipole during this period. This brought along warmer sea surface temperatures and a sea-level increase in the Western Indian Ocean.



<h2 class="wp-block-heading" id="h-limited-tidal-movement">Limited tidal movement </h2>



While mangroves do have a way to cope with slow and steady rising seas by building up sediment, they found the pace of sea level rise over the past few years too fast to keep up with. 



Due to limited tidal movements in the basin areas where many <a href="https://www.earth.com/news/mangroves-and-saltmarshes-are-much-better-at-storing-carbon-than-previously-believed/" target="_blank" rel="noreferrer noopener">mangrove forests</a> grow, the rising sea levels essentially drowned them. 



The lack of tidal movement and the consequent flooding obstructed the mangroves from building the sediment they needed to stay above water.



<h2 class="wp-block-heading" id="h-extreme-magnitude-of-forest-dieback">Extreme magnitude of forest dieback</h2>



Dr. Vasile Ersek is an associate professor in Northumbria University’s <a href="https://www.northumbria.ac.uk/about-us/academic-departments/geography-and-environmental-sciences/" target="_blank" rel="noreferrer noopener">Department of Geography and Environmental Sciences</a>.



"Dieback was first observed in the center of low-lying basin areas before gradually spreading outwards," said Dr. Ersek.



"As these basin areas have something we call limited tidal flushing we saw evidence of the rising sea level inundating the forests with seawater. This prolonged exposure created higher concentrations of salt."



“As the mangroves’ build-up of sediment slowed down due to the pace of the rising sea level, the soil salinity increased beyond what even these salt-tolerant trees could handle. Essentially, the mangroves were drowning."



Dr. Ersek noted that the extreme magnitude of dieback seen in the Maldives is a vivid illustration of how climate change may push natural systems past their limits, with cascading consequences for both nature and people.



<h2 class="wp-block-heading" id="h-future-of-mangroves-in-a-warning-climate">Future of mangroves in a warning climate</h2>



Lucy Carruthers, the study's lead author, is now a postdoctoral scholar in <a href="https://coastal.ecu.edu/faculty/" target="_blank" rel="noreferrer noopener">East Carolina University’s Department of Coastal Studies</a>.



“Sea level in the region reached its highest point on tide gauge records when the dieback occurred in 2020. This coincided with an intense positive phase in the Indian Ocean Dipole which can induce climate extremes for countries within the Indian Ocean," said Carruthers. 



“As our planet continues to warm, we can expect to see the Indian Ocean Dipole occurring more frequently and at higher magnitude, meaning events like this mangrove die-off may become more common."



“These remarkable forests have thrived at the interface of land and sea for many centuries. Whether they can survive the rapid changes of the coming decades will depend largely on our actions in managing the climate crisis today.”



The study is published in the journal <a href="https://www.nature.com/articles/s41598-024-73776-z" target="_blank" rel="noreferrer noopener">Scientific Reports</a>.



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Drowning mangroves: Climate change is pushing nature past its limits

Researchers have discovered that mangrove forests - a shield against...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Lake Trasimeno, which is located west of Perugia in central Italy. It is the fourth largest lake in the country. While Trasimeno’s water level varies, it has a maximum depth of approximately six meters.&nbsp;



"In this Copernicus Sentinel-2 image, captured on 6 August 2022, the lake’s emerald green colour is likely due to the presence of phytoplankton. Streaks in the water, particularly visible in the west, indicate the presence of soil and sediments which have been stirred up by winds. Dark colored waters in the southern part of the lake indicate a presence of submerged and floating macrophytes (aquatic plants) as well as algae," says ESA.



"Surrounded by hills on three sides, Trasimeno is subject to heavy storms created by winds, especially from the north and west. There are three islets in the lake: Maggiore, Minore and Polvese (the largest). The lake’s shores are sparsely inhabited with only two popular villages: Castiglione del Lago and Passignano sul Trasimeno."



"Italy is experiencing its worst drought in 70 years which has affected drinking water supplies, hydroelectric power and agricultural production. High temperatures, hot winds and lack of rainfall are the main causes of drought in the Umbrian region which saw Lake Trasimeno’s drop 1.3 m, reaching the limit of the hydrometric zero in July 2022."



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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Detecting mercury contamination with the tap of a finger

[sendtonews key="LvS8v8bp9z-2564889-12187" type="single"] Today's Video of the Day from the...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Kainji Lake, a reservoir on the Niger River.



In 1968, Kainji Lake was created by the construction of the Kainji Dam. The Niger River, the third longest in Africa, enters the lake in the north.&nbsp;



According to <a href="https://www.earth.com/news/rivers-in-the-american-west-are-a-lifesaving-resource-for-birds/">ESA</a>, the creation of the lake submerged Foge Island and the town of Bussa and permanently flooded other riverine settlements, leaving around 50,000 people displaced.&nbsp;



Large parts of Foge Island are temporarily exposed during low water tides, and the land is often used by migrating fishermen. Kainji Dam is a dam across the Niger River in Niger State of Central Nigeria. 



Wild mammals occur at relatively low densities due to illegal hunting. Lake Kainji has suffered a dramatic decline as a fishery due to the high numbers of artisanal and subsistence fisherfolk using the lake. It has been suggested that a period of closure, together with controlled fishing rights may help improve fish stocks.



Kainji Lake National Park is the oldest of its kind in Nigeria. The park contains three distinct areas: a part of the Kainji Lake, the Borgu Game Reserve to the west of the lake, and the Zugurma Game Reserve to the southeast. The park is home to around 65 mammal species, 350 bird species, and 30 species of reptiles and amphibians. 



Video/ Image Credit: European Space Agency&nbsp;



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



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Kainji Lake in north central Nigeria

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

<div class="wp-block-sendtonews-playerselector">[sendtonews key="QGPzYnXEtN-1712599-12187" type="single"]</div>



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...

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