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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA Earth Observatory&nbsp;



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Ksudach: A volcano shaped by explosive forces

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA&nbsp;



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Hubble spots a supernova in the constellation Gemini 

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

Today's Image of the Day from NASA Earth Observatory features a satellite view of retreating glaciers in Alaska, where meltwater is rapidly expanding glacial lakes. 



“In parts of Alaska, water is replacing ice. As glaciers thin and <a href="https://www.earth.com/news/satellite-images-reveal-hidden-retreat-of-arctic-glaciers/" target="_blank" rel="noreferrer noopener">retreat</a>, meltwater collects at their fronts, forming proglacial lakes. According to an analysis by Mauri Pelto, a glaciologist at Nichols College, three such lakes in the southeastern part of the state have grown rapidly in recent decades,” said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-retreating-glaciers-in-alaska">Retreating glaciers in Alaska</h2>



“A trio of glaciers - Yakutat, Alsek, and Grand Plateau - descend from inland mountains and flow onto the coastal plain southeast of Yakutat borough, ending at Harlequin Lake, Alsek Lake, and Grand Plateau Lake,” noted NASA.&nbsp;



The retreat of the glaciers, as well as the growth of the lakes, are visible in the image. When compared to an <a href="https://eoimages.gsfc.nasa.gov/images/imagerecords/153000/153638/fastestlake_tm5_19840705_lrg.jpg" target="_blank" rel="noreferrer noopener">image</a> captured by Landsat 5 in the summer of 1984, the changes are even more evident.



NASA elaborated on the extent of the glacier retreat from 1984 to 2024. “During this period, Yakutat Glacier’s main arm retreated 4.3 miles, while Alsek Glacier’s northern and southern arms retreated 3.3 miles and 3.4 miles, respectively. Grand Plateau Glacier’s northern arm lost the most, retreating 4.8 miles.”



<h2 class="wp-block-heading" id="h-glacial-lakes-doubled-in-size-nbsp">Glacial lakes doubled in size&nbsp;</h2>



“Collectively, the three lakes more than doubled in size over 40 years. In 1984, they covered about 50 square miles. By 2024, they spanned 90 square miles. That’s an area larger than Seneca Lake (67 square miles) - one of the Finger Lakes in New York, which also have a glacial origin,” said NASA.



Pelto noted that the lakes forming in this region are immense - starting at the mountains and spreading toward the coast - making this a new lake district that is unique in our nation.



“Millions of other lakes, named and unnamed, dot the state. But this system has grown fast, so much so that Pelto thinks it might represent the fastest lake growth in the United States this century,” said NASA.



<h2 class="wp-block-heading" id="h-understanding-glacier-retreat-nbsp">Understanding glacier retreat&nbsp;</h2>



Glacier retreat is a significant phenomenon driven primarily by global warming the results from rising greenhouse gas <a href="https://www.earth.com/news/global-carbon-dioxide-emissions-hit-a-record-high-in-2023/" target="_blank" rel="noreferrer noopener">emissions</a>.&nbsp;



As temperatures rise, glaciers lose more ice during the summer melt than they can regain in winter snowfall, causing them to shrink over time. This process has profound implications for ecosystems, water resources, and global sea levels.



<h3 class="wp-block-heading" id="h-glacial-lakes">Glacial lakes</h3>



When glaciers retreat, they often leave behind depressions in the landscape that can fill with meltwater, forming glacial lakes. These lakes are typically bounded by natural dams made of rock, ice, or moraine - accumulations of debris left behind by the glacier's movement.&nbsp;



Over the past century, the number and size of glacial lakes worldwide have increased significantly due to the accelerating pace of <a href="https://www.earth.com/news/tropical-glaciers-offer-a-glimpse-of-our-harsh-climate-reality/" target="_blank" rel="noreferrer noopener">glacier</a> retreat. This trend is especially evident in high-altitude regions like the Himalayas, the Andes, and the Alps, as well as in polar areas such as Alaska and Greenland.



<h3 class="wp-block-heading" id="h-positive-and-negative-impacts-nbsp">Positive and negative impacts&nbsp;</h3>



Glacial lakes can have both positive and negative impacts. They provide critical water sources for downstream communities, support biodiversity, and sometimes offer opportunities for hydropower development or tourism.&nbsp;



However, they also pose serious risks. The dams holding back these lakes can fail suddenly, causing glacial lake outburst floods (GLOFs). These catastrophic events can devastate downstream areas, destroying infrastructure, agricultural lands, and habitats while endangering human lives.



<h3 class="wp-block-heading" id="h-monitoring-changes">Monitoring changes</h3>



Understanding glacier retreat and glacial lake formation requires a multidisciplinary approach, combining climate science, hydrology, and geology.&nbsp;



Monitoring these changes is essential to mitigate associated risks and adapt to the evolving landscape shaped by a <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fperu-has-lost-over-half-of-its-glaciers-in-six-decades%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">warming planet</a>.



<h2 class="wp-block-heading" id="h-glacier-retreat-worldwide">Glacier retreat worldwide</h2>



Studies and satellite observations show that most glaciers in almost all regions of the world are shrinking.&nbsp;



Melting glaciers contribute significantly to global <a href="https://www.earth.com/news/emergency-meeting-reveals-the-alarming-extent-of-antarcticas-ice-loss/" target="_blank" rel="noreferrer noopener">sea level rise</a>, which threatens coastal communities and ecosystems.



The retreat of glaciers is considered one of the clearest indicators of climate change.&nbsp;Some glaciers are retreating at unprecedented rates, indicating accelerating climate impacts.



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



Image Credit: NASA Earth Observatory



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Retreating glaciers and expanding meltwater lakes in Alaska

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



“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 in the 33rd anniversary image of the Hubble Space Telescope in April 2023. 



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-ngc-1333">Webb’s view of NGC 1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC 1333 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-stars-in-the-sun-s-birth-cluster">Stars in the Sun's birth cluster</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-early-stages-of-planet-formation">Early stages of planet formation </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.



These stars are still in the process of gathering material and developing protoplanetary disks. 



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 NASA features the spiral galaxy NGC 2566, which is located 76 million light-years away in the constellation Puppis. The image was captured by the NASA/ESA Hubble Space Telescope.



“A prominent bar of stars stretches across the center of this galaxy, and spiral arms emerge from each end of the bar. Because NGC 2566 appears tilted from our perspective, its disk takes on an almond shape, giving the galaxy the appearance of a cosmic eye,” said <a href="https://phys.org/news/2024-12-hubble-spies-spiral-galaxy-ngc.html" target="_blank" rel="noreferrer noopener">NASA</a>.



“As NGC 2566 appears to gaze at us, astronomers gaze right back, using Hubble to survey the galaxy's star clusters and star-forming regions.”



<h2 class="wp-block-heading" id="h-complex-appearance-of-ngc-2566">Complex appearance of NGC 2566</h2>



NGC 2566 lies at a considerable distance from Earth, making it a challenging object for amateur astronomers to observe in detail without powerful telescopes.&nbsp;



It can be seen in the Southern Hemisphere sky and is better observed from locations with minimal <a href="https://www.earth.com/news/how-light-pollution-influences-interest-in-astronomy/" target="_blank" rel="noreferrer noopener">light pollution</a>.&nbsp;



The galaxy's arms are populated with young, bright stars, regions of active star formation, and interstellar gas and dust - giving it a dynamic and complex appearance.



<h2 class="wp-block-heading" id="h-measuring-the-ages-of-stars">Measuring the ages of stars</h2>



According to NASA, data from Hubble is especially valuable for studying stars that are just a few million years old. “These stars are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive.”



“Using these data, researchers can measure the ages of NGC 2566's stars, which helps piece together the timeline of the galaxy's star formation and the exchange of gas between star-forming clouds and the stars themselves.”



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



Star formation in <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> is a fascinating and complex process that unfolds over millions of years. It begins in vast clouds of gas and dust, known as molecular clouds, which are often found in the spiral arms of galaxies or in regions of irregular or starburst galaxies.&nbsp;



These clouds provide the raw material for star formation, consisting primarily of hydrogen and helium, with trace amounts of heavier elements.



As the molecular clouds collapse under their own gravity, regions within them begin to condense and fragment, forming dense clumps. Within these clumps, protostars emerge. Their formation is driven by the gravitational pull drawing in surrounding gas.&nbsp;



During this process, the gas heats up due to increasing pressure, eventually igniting nuclear fusion in the core, signaling the birth of a new star.



<h2 class="wp-block-heading" id="h-rate-of-star-formation-nbsp-across-galaxies">Rate of star formation&nbsp;across galaxies</h2>



The rate of star formation varies across galaxies is influenced by numerous factors. In spiral galaxies like the Milky Way, star formation is most active in the spiral arms, where density waves compress gas and dust, triggering the collapse of molecular clouds.&nbsp;



Elliptical galaxies, which often have little cold gas and dust, typically exhibit low rates of star formation or none at all.



Starburst galaxies, on the other hand, experience episodes of exceptionally high star formation, often triggered by <a href="https://www.earth.com/news/webb-captures-a-galaxy-collision-with-a-radiant-smile/">galactic collisions</a> or interactions. 



These events can funnel large amounts of gas into central regions, leading to intense star-forming activity. However, such bursts are usually short-lived on cosmic timescales, exhausting the available gas quickly.



The environment within a galaxy also plays a significant role. Stellar winds and supernova explosions from existing stars can both inhibit and promote star formation. They may disperse gas, preventing further collapse, or compress nearby clouds, triggering new star formation.&nbsp;



Over time, as galaxies evolve, the availability of gas diminishes, leading to a gradual decline in star formation activity.



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



The Puppis constellation in the southern sky represents the stern of a ship. It was once part of a larger constellation known as Argo Navis, which depicted the mythical ship of Jason and the Argonauts.&nbsp;



However, Argo Navis was later divided into three separate constellations: Puppis, Carina (the keel), and Vela (the sails). Puppis is the largest of these three and contains many notable celestial objects.



This constellation is home to several bright stars, including Naos (Zeta Puppis), a hot, massive star that emits intense ultraviolet radiation. Puppis also hosts a wide variety of deep-sky objects, such as open <a href="https://www.earth.com/news/stunning-star-clusters-captured-in-the-extreme-outskirts-of-the-milky-way/" target="_blank" rel="noreferrer noopener">star clusters</a> and nebulae.&nbsp;



Among these, Messier 46 and Messier 47 stand out. Both are beautiful star clusters that are visible through binoculars or small telescopes. The region is dense with stars because it lies along the <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>, making it a prime area for stargazing and astrophotography. 



Image Credit: NASA



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A cosmic eye in the Puppis constellation

Today's Image of the Day from NASA features the spiral...

Today's Image of the Day from the European Space Agency features UGC 5460, a spiral galaxy that is located about 60 million light-years away in the constellation Ursa Major.&nbsp;



“This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms and bright blue star clusters. Also captured in the upper left-hand corner of this image is a far closer object: a star just 577 light-years away in our own galaxy,” said <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“UGC 5460 has hosted two recent supernovae named SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programmes that aim to study various kinds of supernovae.”&nbsp;



<h2 class="wp-block-heading" id="h-a-core-collapse-supernova-nbsp">A core-collapse supernova&nbsp;</h2>



SN 2015as is an example of a core-collapse supernova. This type of <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> occurs when the core of a massive star - typically with more than 8 times the mass of the sun - can no longer support its own gravity after exhausting its nuclear fuel. 



This causes the core to collapse under its own weight, leading to an extremely violent explosion. The collapse triggers the release of an enormous amount of energy, expelling the outer layers of the star into space.



In the aftermath of the explosion, a dense <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">remnant</a> is created. This is often a neutron star or black hole, depending on the mass of the original star. Core-collapse supernovae are some of the most powerful events in the universe.



According to ESA, Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a <a href="https://www.earth.com/news/supernova-dandelion-year-1181-leaves-behind-zombie-star-defying-death/" target="_blank" rel="noreferrer noopener">supernova</a> collides with the gas that surrounds the exploded star.



<h2 class="wp-block-heading" id="h-rare-stars-with-large-eruptions-nbsp">Rare stars with large eruptions&nbsp;</h2>



“SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae,” noted ESA.



“Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location, and the explosion’s identity may be revealed at last.”



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



Spiral galaxies are some of the most recognizable and beautiful structures in the universe. They are known for their distinctive arms that spiral outward from a central bulge.&nbsp;



These galaxies are typically composed of stars, gas, dust, and dark matter. The arms are often sites of intense <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star formation</a>, where clouds of gas collapse to form new stars. 



In the center of a spiral galaxy lies a dense concentration of older stars and, often, a supermassive black hole.



<h2 class="wp-block-heading" id="h-structure-of-a-spiral-galaxy-nbsp">Structure of a spiral galaxy&nbsp;</h2>



The structure of a spiral galaxy is generally divided into three main components: the disk, the bulge, and the halo.&nbsp;



The disk is where the spiral arms are located and contains most of the galaxy's visible stars and interstellar medium.&nbsp;



The bulge is a tightly packed region of older stars at the core, and the halo consists of a sparse collection of stars and globular clusters that surround the galaxy.&nbsp;



Spiral galaxies can be classified into different types based on the tightness and number of their spiral arms, as well as the size of their central bulge.



<h2 class="wp-block-heading" id="h-the-milky-way-galaxy">The Milky Way galaxy</h2>



Our solar system is located within a large spiral galaxy known as the Milky Way. The name refers to its appearance as a dim, milky band of light stretching across the night sky.&nbsp;



The term "Milky Way" comes from ancient Greek mythology, where it was associated the goddess Hera's milk spilling into the sky. In Greek, it was called "Galaxias Kyklos," meaning "milky circle."&nbsp;



Spanning about 100,000 light-years in diameter, the Milky Way is composed of stars, gas, dust, and dark matter. The galaxy has a distinct disk shape with spiral arms that wind outward from a central bulge, which houses a supermassive <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/" target="_blank" rel="noreferrer noopener">black hole</a>. 



Our sun is located in one of the spiral arms - known as the Orion Arm - positioned roughly halfway from the center to the outer edge.&nbsp;



The Milky Way is part of a small group of galaxies called the Local Group, which includes the Andromeda Galaxy and several smaller galaxies.



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Hubble views a spiral galaxy with stellar explosions

Northern Lights in Canada, also known as <a href="https://www.earth.com/image/a-beautiful-aurora-borealis-seen-from-the-space-station/">Aurora Borealis</a>, are produced when the magnetosphere is disrupted by solar wind, causing charged particles to precipitate. Today’s Image of the Day comes courtesy of <a href="https://www.nasa.gov/">NASA</a> and features a look at the Northern Lights glowing over Canada.

Northern Lights in Canada

In many Western countries today, the number of dogs is increasing, but the number of children is not. This striking shift raises big questions. Are people choosing dogs instead of kids? Or is something deeper going on?



Professor Enikő Kubinyi from <a href="https://www.elte.hu/en/" target="_blank" rel="noreferrer noopener">Eötvös Loránd University</a> believes she has found the answer. Her theory connects the rise of dog ownership to falling birth rates - but not in a simple, cause-and-effect way.



Kubinyi explains that many see their dogs not just as pets, but as full <a href="https://www.earth.com/news/national-puppy-day-2025-where-happiness-meets-responsibility/" target="_blank" rel="noreferrer noopener">family members</a>. Some even place their relationships with their dogs above those that they have with humans.



<h2 class="wp-block-heading" id="h-dogs-as-emotional-anchors">Dogs as emotional anchors</h2>



Recent surveys in Hungary show a surprising trend. Nineteen percent of childless adults, and ten percent of parents, value their dog more than any human.



Kubinyi’s theory explores why this emotional shift is happening.



"Some say dogs are the new children, while others find this idea outrageous. Pope Francis, for example, has called it selfish for childless people to pamper pets," noted Kubinyi.



She points to studies suggesting that dog owners often feel more negatively about motherhood. Some mothers with <a href="https://www.earth.com/news/lost-in-translation-how-we-misread-our-dogs-emotions/" target="_blank" rel="noreferrer noopener">dogs</a> feel parenting becomes more burdensome, reducing their desire for more children. In some cases, dogs even create distance in romantic relationships.



<h2 class="wp-block-heading" id="h-dogs-as-a-step-before-having-a-child">Dogs as a step before having a child</h2>



But the picture isn’t one-sided. Kubinyi highlights another argument: dog ownership may actually support family life.



"Families with children are more likely to own dogs, and some couples see their pet as a 'practice child,' a preparatory step toward starting a family. Women also tend to find men with <a href="https://www.earth.com/news/dogs-focus-more-when-humans-use-eye-contact-and-gestures/" target="_blank" rel="noreferrer noopener">dogs</a> more attractive, which could increase the chances of fatherhood."



In this view, dogs don’t replace children. They support and sometimes lead to parenthood.



<h2 class="wp-block-heading" id="h-dogs-build-social-ties-too">Dogs build social ties too</h2>



<a href="https://www.earth.com/news/humans-and-dogs-share-genes-linked-to-obesity/" target="_blank" rel="noreferrer noopener">Dog ownership</a> doesn’t just affect families. It also shapes social life. Dog walking often leads to more human interaction. 



Kubinyi explains that dogs serve as "social glue" in modern life. They help build relationships.



But there’s a flip side. If someone&nbsp;leans only on dogs for emotional needs,&nbsp;<a href="https://www.sciencedirect.com/science/article/pii/S1558787820300356" target="_blank" rel="noreferrer noopener">behavior issues</a> like barking or aggression can isolate them further, instead of connecting them to other people.



<h2 class="wp-block-heading" id="h-emotional-bonds-now-shift-to-dogs">Emotional bonds now shift to dogs</h2>



"The number of children is not declining because the number of dogs is increasing, but the same trend lies behind both phenomena: the transformation of social networks," said Kubinyi.



She calls this the&nbsp;<a href="https://www.x-mol.com/paper/1900939840006262784">companion dog runaway theory</a>.&nbsp;It ties the rise of dog ownership to both biology and culture.&nbsp;Humans have an innate need to care and connect.&nbsp;When bonds between humans weaken, these instincts shift to dogs.



<h2 class="wp-block-heading" id="h-what-changed-in-society">What changed in society?</h2>



Nearly 90% of Hungarian adults don’t spend even an hour a week with children. That’s unusual for a species built around cooperative childcare.



Kubinyi points out that modern support networks have eroded. People feel alone. Some have lost faith in human relationships altogether. <a href="https://www.earth.com/news/rewards-of-dog-ownership-outweigh-the-challenges/" target="_blank" rel="noreferrer noopener">Dogs</a> that offer loyalty and comfort fill that space.



Cultural shifts support this trend.&nbsp;Memes joke about dog-parent life, and&nbsp;<a href="https://www.sciencedirect.com/science/article/pii/S1558787824000819" target="_blank" rel="noreferrer noopener">pet businesses are booming</a>. People call themselves "dog moms" and "dog dads." These aren’t just trends - they reflect emotional truths.



<h2 class="wp-block-heading" id="h-dogs-are-treated-like-children">Dogs are treated like children</h2>



Dogs aren’t just pets anymore. For many, they’re the most important companion a person has. Their loyalty, shaped by thousands of years beside humans, fits perfectly in the role of substitute family.



Even breeding reflects this change.&nbsp;<a href="https://www.earth.com/news/flat-faced-dogs-have-childlike-traits-that-humans-cannot-resist/" target="_blank" rel="noreferrer noopener">Small, baby-faced dogs</a> are now wildly popular. Their “cuteness” triggers our nurturing instincts. But these breeds also suffer from many health issues. Owners care for them intensely - and feel deeply needed.



Sometimes, though, over-caring causes confusion and behavior problems. Dogs have needs, but they aren’t children. Misreading these needs can cause stress - for both pet and owner.



<h2 class="wp-block-heading" id="h-people-substitute-caregivers-with-dogs">People substitute caregivers with dogs</h2>



"The changing role of dog ownership suggests that people in Western societies experience a significant lack of caregiving and social support - and they try to compensate for this, at least in part, with dogs and likely cats as well," said Kubinyi.



She urges stronger support systems for families and better ways to fight loneliness. Dog ownership should help people connect - not push them further apart.



Other experts agree. Researcher Hal Herzog refers to Kubinyi’s theory as "an important new perspective" on how dogs fit into our social and emotional world.



In the end, keeping dogs reflects our deepest human needs - for love, connection, and care.



The study is published in the journal <a href="https://journals.sagepub.com/doi/10.1177/09637214251318284" target="_blank" rel="noreferrer noopener">Current Directions in Psychological Science</a>.



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Are dogs replacing children? How modern society is changing

In many Western countries today, the number of dogs is...

Have you ever noticed how memories from the same day seem to blend together, while events that happened weeks apart feel like they exist in totally separate mental files? 



A new study sheds light on why this happens - and it’s not because of what’s happening in the main body of brain cells. Instead, the secret lies in the tiny branches called dendrites.



In a recent study, scientists from <a href="https://www.osu.edu/" target="_blank" rel="noreferrer noopener">The Ohio State University</a> used advanced imaging tools, including miniaturized microscopes, to track how mice formed memories in real time. 



The team focused on a lesser-known part of the brain cell - dendrites, the slender projections that stretch out from neurons. These branches are known for receiving information, but they’re much more active than previously thought.



<h2 class="wp-block-heading" id="h-small-branches-big-role">Small branches, big role</h2>



The researchers zeroed in on the retrosplenial cortex (RSC), a brain area involved in spatial and contextual memory.



When mice were introduced to two different environments close together in time, something remarkable happened: the memories of those places became linked. 



If the mice were later given a small shock in just one of the environments, they reacted with fear in both. Their brains treated the two places as connected - even though only one was associated with the unpleasant experience.



“If you think of a <a href="https://www.earth.com/news/first-complete-map-of-every-neuron-in-the-brain-revealed/" target="_blank" rel="noreferrer noopener">neuron</a> as a computer, dendrites are like tiny computers inside it, each performing its own calculations,” said study lead author Megha Sehgal.



“This discovery shows that our brains can link information arriving close in time to the same dendritic location, expanding our understanding of how memories are organized.”



<h2 class="wp-block-heading" id="h-communication-between-neurons">Communication between neurons </h2>



The researchers studied how dendrites change during the process of learning and storing information. On the surface of these branches are small bumps called spines - tiny hubs where communication between neurons happens.



When a new memory was formed, they saw clusters of these spines pop up. Then, if another memory formed shortly after, those same spots were more likely to attract additional spines.



This physical clustering of connections appears to be how the brain binds related <a href="https://www.earth.com/news/we-often-undervalue-the-most-meaningful-experiences-in-life/" target="_blank" rel="noreferrer noopener">experiences</a> together.



“The idea is that we don’t form memories in isolation. You don’t form a single memory. You use that memory, make a framework of memories, and then pull from that framework when you need to make adaptive decisions,” said Sehgal.



<h2 class="wp-block-heading" id="h-critical-role-of-dendrites">Critical role of dendrites</h2>



To test whether these dendritic branches were really causing the linking effect, the team used a method called optogenetics. This technique lets scientists control <a href="https://www.earth.com/news/mixed-emotions-linked-to-unique-brain-activity/" target="_blank" rel="noreferrer noopener">brain activity</a> using light. 



The experts reactivated the exact dendritic branches that had been used during one memory and found that doing so could link it to another, unrelated memory.



This confirmed the critical role that dendrites play in how memories are joined together in our brains.



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



This discovery not only changes how we think about memory - it also opens the door to new ways of understanding <a href="https://www.earth.com/news/dementia-was-extremely-rare-in-ancient-times-so-why-is-it-now-so-prevalent/" target="_blank" rel="noreferrer noopener">memory-related disorders</a>.



If scientists can learn to influence how dendrites work, they may be able to treat conditions where memory formation or linking is impaired.



“Our work not only expands our understanding of how memories are formed but also suggests exciting new possibilities for manipulating higher order memory processes,” said Sehgal. “This could have implications for developing therapies for memory-related conditions such as <a href="https://www.earth.com/news/stopping-alzheimers-before-it-starts-early-treatment-shows-potential/" target="_blank" rel="noreferrer noopener">Alzheimer’s disease</a>.”



The research marks an important step in decoding the physical structure of memory -and it all starts with the tiny, busy branches inside each brain cell.



<h2 class="wp-block-heading" id="h-rethinking-memory-storage">Rethinking memory storage</h2>



This study encourages us to rethink how we view memory storage. Instead of seeing each experience as a separate snapshot, it may be more accurate to picture them as parts of a timeline - physically tied together through shared dendritic changes.



This could explain why certain days feel like a continuous stream of events, while others stand alone. 



The findings also suggest that how we mentally group events may depend more on timing than emotional weight. 



With a clearer picture of how the brain organizes information, scientists can better understand what happens when that system begins to fail, such as in age-related cognitive decline.



The full study was published in the journal <a href="https://www.nature.com/articles/s41593-025-01876-8" target="_blank" rel="noreferrer noopener">Nature Neuroscience</a>.



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Why memories close in time feel connected

Have you ever noticed how memories from the same day...

Climate change has long threatened species living in extreme habitats. Emperor penguins, iconic residents of Antarctica, now face a sharper edge of that threat. 



​A team led by scientists at the&nbsp;Woods Hole Oceanographic Institution (<a href="https://www.whoi.edu/press-room/news-release/new-study-finds-emperor-penguins-increasingly-threatened-by-climate-change/" target="_blank" rel="noreferrer noopener">WHOI</a>), along with global collaborators, has revealed new evidence that these birds are more at risk than previously believed.​



The study suggests emperor penguins should no longer be considered “Near Threatened.” Instead, the team recommends reclassifying them as&nbsp;<a href="https://www.sciencedirect.com/science/article/pii/S0006320719309899?" target="_blank" rel="noreferrer noopener">“Vulnerable” or even “Endangered”</a>. This shift, based on&nbsp;<a href="https://www.iucnredlist.org/species/22697752/132600320?" target="_blank" rel="noreferrer noopener">updated IUCN criteria</a>, highlights an urgent need to reconsider current conservation strategies.



The researchers tailored their study to match the <a href="https://www.earth.com/news/just-a-whiff-of-penguin-poop-can-send-krill-into-a-frenzy/" target="_blank" rel="noreferrer noopener">penguins</a>’ deep dependence on stable sea ice and predictable Antarctic conditions. The changing environment now places them on unstable ground.



<h2 class="wp-block-heading" id="h-climate-threats-to-emperor-penguins">Climate threats to emperor penguins </h2>



Emperor penguins are at significant risk of extinction due to climate change, particularly the rapid loss of Antarctic sea ice, which they depend on for breeding and raising their chicks. 



Studies suggest that if current warming trends continue, more than 90% of emperor penguin colonies could be gone by the end of the century. 



Some projections indicate that major population declines could happen much sooner, potentially within our lifetime.



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



Published in Biological Conservation, the paper titled Living with Uncertainty presents new tools to predict future risks. The researchers used a cutting-edge method: the Multi-Model Large Ensemble (MMLE) framework.



This approach combines numerous Earth system simulations to capture a fuller picture of possible <a href="https://www.earth.com/news/enhanced-monitoring-of-emperor-penguins-can-help-us-save-them/" target="_blank" rel="noreferrer noopener">environmental futures</a>.



“This is the first study to integrate natural variability in physical and biological processes and employ a wide range of Earth system and ecological models to account for numerous sources of uncertainty in projecting assessments of future population trajectories,” said Stéphanie Jenouvrier, lead author and senior scientist at WHOI.



“Improved methods for accounting for uncertainties are urgently needed to strengthen assessments of extinction and inform conservation efforts in an uncertain world.”



The framework improves how scientists handle uncertainty in environmental modeling. Instead of relying on a single future scenario, the MMLE considers many outcomes. This change offers deeper insight into extinction risks.



<h2 class="wp-block-heading" id="h-the-world-is-changing-for-emperor-penguins">The world is changing for emperor penguins</h2>



To build their models, the team used a wide variety of data. These included satellite images of 50 <a href="https://www.earth.com/news/african-penguins-have-lost-97-percent-of-their-population/" target="_blank" rel="noreferrer noopener">penguin colonies</a>, long-term monitoring of chicks and adults, and over a decade of observations of individual birds. The researchers also factored in how colonies move, drawn from genetic and population data.



“There are quantifiable uncertainties in projections of future environmental conditions,” said Jenouvrier. “Incorporating this uncertainty in ecosystem projections allows for a more complete and robust assessment of potential extinction risk.”



This approach blends fieldwork, satellite technology, and ecological theory. It gives conservationists a more grounded look at future risks. Such forecasts help shape stronger policies - especially when dealing with species that live in remote or harsh environments.



<h2 class="wp-block-heading" id="h-a-model-for-future-conservation">A model for future conservation</h2>



Professor Phil Trathan, one of the study’s authors and formerly Head of Conservation Biology at the <a href="https://www.bas.ac.uk/" target="_blank" rel="noreferrer noopener">British Antarctic Survey</a>, emphasized the broader meaning of this research.



“Emperor <a href="https://www.earth.com/news/emperor-penguins-are-struggling-to-survive-as-sea-ice-vanishes/" target="_blank" rel="noreferrer noopener">penguins</a> are vital indicators of ecosystem health in the Antarctic, they also help inform us about wider changes in the earth system. Therefore, harnessing robust models that increase our understanding about uncertainty and risk are vital, if we are to better conserve and protect this and other species.”



“Ultimately, humans depend upon the natural world, so developing better projections of the future earth system are essential for ensuring human health and well-being. The tools used in this study should now help us all.”



The combination of modeling tools and diverse data points may set a precedent for future work. Other species in similarly vulnerable habitats may also benefit from these techniques.



<h2 class="wp-block-heading" id="h-protecting-emperor-penguins">Protecting emperor penguins</h2>



The IUCN plays a central role in shaping how species like the emperor penguin are protected. The Red List guides many conservation decisions, often influencing discussions at international levels.



These include forums like the&nbsp;Antarctic Treaty Consultative Meeting (<a href="https://www.ats.aq/e/atcm.html" target="_blank" rel="noreferrer noopener">ATCM</a>)&nbsp;and the&nbsp;Convention on the Conservation of Antarctic Marine Living Resources (<a href="https://www.ccamlr.org/" target="_blank" rel="noreferrer noopener">CCAMLR</a>).​



“The Antarctic Treaty Consultative Meeting serves as a key forum for decision-making on Antarctic conservation. This new IUCN Red List assessment provides critical scientific support for strengthening protections for emperor penguins under the Antarctic Treaty System,” noted Jenouvrier.



”It also strengthens the case for establishing Marine Protected Areas (MPAs) under the Convention on the Conservation of Antarctic Marine Living Resources, particularly in vital regions like the Ross Sea and the Weddell Sea, which could serve as crucial refugia for emperor penguins.” 



With the scientific foundation now laid, the next step lies with policymakers. If taken seriously, this reassessment may not only protect emperor penguins but also influence how we respond to global climate threats across species and continents.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0006320725000746" target="_blank" rel="noreferrer noopener">Biological Conservation</a>.



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Emperor penguins may disappear in our lifetime

Climate change has long threatened species living in extreme habitats....

In every classroom, on every street, there are teenagers quietly battling depression. It’s a growing crisis, one that does not treat everyone equally. Around the world, depression strikes women twice as often as men. 



This disparity begins not in adulthood but during adolescence. While hormones, social pressure, and life events all play roles, new science is pointing to something deeper - something biological.



A new study published in&nbsp;Biological Psychiatry&nbsp;explores how <a href="https://www.earth.com/news/people-with-chronic-pain-have-high-rates-of-depression-and-anxiety/" target="_blank" rel="noreferrer noopener">brain chemistry</a> may drive this gender divide. It focuses on a lesser-known series of chemical reactions in the brain called the "kynurenine pathway."



This pathway has long been studied in adults with depression, but for the first time, scientists have turned their attention to teenagers. The goal was to find out whether differences in this brain chemistry could explain why depression takes root more strongly in adolescent girls.



<h2 class="wp-block-heading" id="h-biological-drivers-for-depression">Biological drivers for depression </h2>



Tryptophan breaks into two key products. Kynurenic acid protects the <a href="https://www.earth.com/news/stress-related-brain-inflammation-linked-to-depression/" target="_blank" rel="noreferrer noopener">brain</a>. Quinolinic acid harms it. These chemicals may influence how depression develops. 



The researchers focused on this pathway in teenagers, examining how these brain chemicals differ between boys and girls.​



“Adolescence is a time when many <a href="https://www.earth.com/news/young-adult-depression-linked-to-worse-memory-skills/" target="_blank" rel="noreferrer noopener">changes occur in the brain</a> and body but we still know very little about the possible biological drivers for depression and how this might affect the difference between teenage boys and girls,“ said Professor Valeria Mondelli from King’s IoPPN.



“Our study indicates the ‘kynurenine pathway’ plays a role in development of depression during the teenage years which may help us to understand why there is a higher incidence amongst girls."



“During adolescence there are a wide range of social and individual factors that influence mental health and by identifying the biological pathways involved we hope we can help build a clearer picture of how we can help teenagers manage depression.”



<h2 class="wp-block-heading" id="h-teen-girls-with-a-chemical-imbalance">Teen girls with a chemical imbalance </h2>



The teenagers, aged between 14 and 16, were placed into three distinct groups based on their <a href="https://www.earth.com/news/teens-with-problematic-smartphone-use-suffer-from-depression/" target="_blank" rel="noreferrer noopener">mental health</a> profiles: those with low risk of depression, those considered high risk, and those already diagnosed with depression. 



Each group included 50 adolescents, with an equal number of boys and girls. To determine risk levels, the researchers used an assessment developed as part of the IDEA project, which evaluates various psychological and social factors.



The participants were then tracked over a period of three years to observe whether their symptoms improved or remained.



The findings revealed that teens with a high risk of depression or a current diagnosis had lower levels of kynurenic acid, a chemical known to protect the brain. 



This decrease was especially evident among girls, suggesting that an imbalance in the kynurenine pathway may affect them more severely during adolescence.



<h2 class="wp-block-heading" id="h-inflammation-and-its-role-in-depression">Inflammation and its role in depression</h2>



The experts also measured proteins that show inflammation. These markers rise during infection or stress. 



The researchers found high inflammation levels linked to more quinolinic acid. This means inflammation could push the kynurenine pathway toward damage.



This pattern appeared only in high-risk or depressed teens. Low-risk teens did not show the same chemical changes. That points to inflammation as a driver of depression’s deeper roots in the brain.



<h2 class="wp-block-heading" id="h-persistent-depression-in-teen-girls">Persistent depression in teen girls</h2>



Three years later, the researchers checked back in. Girls with ongoing depression had more neurotoxic chemicals in their blood. Those who improved had lower levels, suggesting that a long-term <a href="https://www.earth.com/news/psilocybin-therapy-offers-hope-for-millions-with-depression/" target="_blank" rel="noreferrer noopener">chemical imbalance</a> might slow recovery.



“Our study indicates that the measurement of chemicals involved in the kynurenine pathway could potentially help identify those who at risk of persistent depression, particularly amongst females, as well as inform the approaches we take to providing support,“ said Dr. Naghmeh Nikkheslat, the study’s first author.



“This insight could help develop more targeted support for teenagers with depression through interventions that work in a range of ways on the kynurenine pathway from medication to lifestyle changes such as diet and exercise.”



<h2 class="wp-block-heading" id="h-personalized-support-is-needed">Personalized support is needed</h2>



This research could change how we detect and treat teen depression. Measuring brain-related chemicals may help flag those most at risk. With more data, doctors might offer depression support earlier, especially to girls.



By linking biology to <a href="https://www.earth.com/news/millions-of-americans-have-lost-years-of-time-to-poor-mental-health/" target="_blank" rel="noreferrer noopener">mental health</a>, the study brings new options to the table. It offers hope for more effective, personal care in the teenage years.



Funded by <a href="https://www.mqmentalhealth.org/" target="_blank" rel="noreferrer noopener">MQ Mental Health Research</a>, the research received support from the <a href="https://www.maudsleybrc.nihr.ac.uk/" target="_blank" rel="noreferrer noopener">NIHR Maudsley Biomedical Research Centre</a>. 



The study is published in the journal <a href="https://www.biologicalpsychiatryjournal.com/article/S0006-3223(24)01789-X/fulltext" target="_blank" rel="noreferrer noopener">Biological Psychiatry</a>.



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Why teen girls struggle more with depression

In every classroom, on every street, there are teenagers quietly...

Antibiotic resistance is rising. Infections spread unchecked as old treatments fail. The next solution may come not from labs, but from swamps and forests. Frogs - ancient survivors of earth’s changing ecosystems - have evolved powerful natural defenses. These defenses may hold the key to future antibiotics.



Frogs thrive in environments teeming with microbes. Yet, they rarely suffer <a href="https://www.earth.com/news/bacteria-pass-down-their-memories-to-fight-viruses/" target="_blank" rel="noreferrer noopener">infections</a>. That mystery has long intrigued researchers. Could frogs be carrying biological secrets that might save human lives?



​A new study led by&nbsp;Professor Cesar de la Fuente&nbsp;at the&nbsp;<a href="https://www.upenn.edu/" target="_blank" rel="noreferrer noopener">University of Pennsylvania</a>&nbsp;believes the answer is yes.&nbsp;His team is tapping into the molecular defenses of frogs to design synthetic antibiotics that may defeat drug-resistant bacteria.​



<h2 class="wp-block-heading" id="h-frog-evolution-shaped-powerful-antibiotics">Frog evolution shaped powerful antibiotics</h2>



Frogs have existed for over 200 million years. They have spread across continents and climates, adapting to jungles, rivers, deserts, and subarctic forests. Living in moist, microbe-rich environments, frogs constantly face bacterial threats. 



To survive, many species evolved antimicrobial peptides in their skin. These natural compounds kill harmful bacteria on contact. Unlike traditional antibiotics, they do not easily trigger resistance.



One frog species, Odorrana andersonii, has become the focus of research. It produces a peptide known as Andersonnin-D1. Chinese scientists first identified it in 2012. 



Despite its strength against bacteria, the peptide clumps together, making it less effective and more toxic. Because of this flaw, it cannot be used in clinical medicine without modification.



<h2 class="wp-block-heading" id="h-mission-to-rebuild-nature-s-blueprints">Mission to rebuild nature’s blueprints</h2>



Professor Cesar de la Fuente’s lab works at the intersection of biology, engineering, and synthetic chemistry. His team looks for inspiration in nature’s forgotten corners. 



Their earlier work explored ancient DNA from extinct animals like the woolly mammoth and Neanderthals. They also investigated the human gut microbiome, home to countless natural compounds.



“Each study is motivated by imagining environments where evolution would spur the creation of antibiotics,” said de la Fuente.



“Amphibians live in very microbe-rich environments. They very rarely get infected despite being surrounded by microbes, so they must produce antimicrobial compounds.”



Inspired by this evolutionary logic, the team set out to redesign Andersonnin-D1. The goal was to remove its dangerous tendencies while keeping its bacterial-fighting power.



<h2 class="wp-block-heading" id="h-improving-frog-antibiotics-in-the-lab">Improving frog antibiotics in the lab</h2>



Using structure-guided design, the researchers altered the chemical structure of Andersonnin-D1. This approach allows experts to make small, deliberate changes to a molecule’s sequence and observe the effects.



Marcelo Torres is a research associate in the de la Fuente lab and co-author of the paper.



“With structure-guided design, we change the sequence of the molecule. And then we see how those mutations affect the function that we are trying to improve," said Torres.



This method generated several synthetic peptides. These versions kept the strong <a href="https://www.earth.com/news/cigarette-waste-fuels-antibiotic-resistance/" target="_blank" rel="noreferrer noopener">antimicrobial effect</a> but avoided the clumping that caused toxicity in the original. 



Each design aimed for maximum precision, producing molecules more suitable for real-world use.



<h2 class="wp-block-heading" id="h-putting-the-molecules-to-the-test">Putting the molecules to the test</h2>



Designing new&nbsp;frog-based&nbsp;antibiotics is only the beginning. To prove their value, the synthetic peptides had to succeed in rigorous lab tests. 



The team exposed the molecules to a range of harmful <a href="https://www.earth.com/news/antibiotic-resistance-could-cause-a-health-crisis-globally/" target="_blank" rel="noreferrer noopener">bacteria</a>. The results were promising. In preclinical models, the peptides matched the strength of polymyxin B - a last-resort drug used when others fail.



More importantly, these synthetic antibiotics showed low toxicity. They left human cells unharmed and did not disrupt beneficial gut bacteria. This makes them more targeted and less harmful than many existing drugs. The lab tested the peptides in both simple and complex bacterial communities.



“Those experiments are very difficult to set up because you need to grow different bacteria at once,” says de la Fuente. “We had to come up with the specific ratio of each bacterium to have a sustained community.”



These community-based models better reflect the conditions of real <a href="https://www.earth.com/news/antimicrobial-resistance-could-cause-39-million-deaths-by-2050/" target="_blank" rel="noreferrer noopener">infections</a> in the human body.



<h2 class="wp-block-heading" id="h-steps-toward-clinical-use">Steps toward clinical use</h2>



If additional studies continue to show strong results, the team will prepare for Investigational New Drug (IND) enabling studies. 



These tests assess safety and efficacy before a drug can be submitted to the U.S. Food and Drug Administration. Only after passing these stages can the peptides move into clinical trials involving human patients.



“We are excited that frogs - and nature in general - can inspire new molecules that could be developed into antibiotics,” said de la Fuente. “Thanks to the power of engineering, we can take those natural molecules and turn them into something more useful for humanity.”



This line of research represents a fusion of <a href="https://www.earth.com/news/soil-plays-an-overlooked-role-in-antibiotic-resistance/" target="_blank" rel="noreferrer noopener">evolutionary biology</a> and advanced engineering. It shows how careful study of nature’s own defenses can guide the creation of life-saving medicines.



<h2 class="wp-block-heading" id="h-nature-s-role-in-innovation">Nature’s role in innovation</h2>



The research was conducted at the University of Pennsylvania’s <a href="https://www.seas.upenn.edu/" target="_blank" rel="noreferrer noopener">School of Engineering and Applied Science</a>. It was supported by funding from organizations such as the National Institutes of Health (<a href="https://www.nih.gov/" target="_blank" rel="noreferrer noopener">NIH</a>), the Defense Threat Reduction Agency (<a href="https://www.dtra.mil/" target="_blank" rel="noreferrer noopener">DTRA</a>), <a href="https://us.pg.com/" target="_blank" rel="noreferrer noopener">Procter &amp; Gamble</a>, and the <a href="https://www.aiche.org/giving" target="_blank" rel="noreferrer noopener">AIChE Foundation</a>.



The study is not just about frogs or antibiotics. It reflects a larger movement in science. Instead of only inventing new molecules from scratch, researchers are increasingly exploring the solutions that evolution already tested over millions of years.



Nature, shaped by survival, often creates molecules more elegant and efficient than anything built by human hands.



In this case, one frog’s molecular defense may lead to a major medical breakthrough. As the world searches for new antibiotics, it may be ancient animals - and the researchers who study them - that help protect our future.



The study is published in the journal <a href="https://dx.doi.org/10.1016/j.tibtech.2025.02.007" target="_blank" rel="noreferrer noopener">Trends in Biotechnology</a>.



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-----

Frogs lead the way in developing new antibiotics

Antibiotic resistance is rising. Infections spread unchecked as old treatments...

We often think parenting begins after birth - diapers, lullabies, and sleepless nights. But what if a mother’s bond with her baby starts much earlier, long before the baby is born?



A recent study led by Dr. Nora Medina from <a href="https://www.jefferson.edu/" target="_blank" rel="noreferrer noopener">Thomas Jefferson University</a> suggests just that. 



Dr. Medina and her colleagues at the <a href="https://www.uchicago.edu/" target="_blank" rel="noreferrer noopener">University of Chicago</a> have shed light on how the emotional connection between mother and child during pregnancy lays the groundwork for future relationships.



This work goes beyond traditional research, which often begins after the child is born. By tracing bonds from the prenatal stage, Medina reveals new insight into how early experiences influence <a href="https://www.earth.com/news/moms-health-shapes-how-well-an-embryo-develops/" target="_blank" rel="noreferrer noopener">parenthood</a>. 



Her study focuses on a group often overlooked or misjudged - young, low-income, racially diverse mothers - and highlights their emotional resilience and strength. In doing so, she challenges long-held assumptions about who makes a good parent.



<h2 class="wp-block-heading" id="h-mother-child-bond-begins-before-birth">Mother-child bond begins before birth</h2>



Dr. Medina and her team followed 160 women from pregnancy through their children’s toddler years. The mothers came from racially diverse backgrounds and faced economic challenges. Yet within this group, the researchers discovered powerful stories of connection, <a href="https://www.earth.com/news/mothers-care-linked-to-the-evolution-of-longer-lifespans/" target="_blank" rel="noreferrer noopener">emotion, and care</a>.



Mothers who reported feeling emotionally connected to their babies during pregnancy later had stronger, more positive relationships with them. They interacted with greater sensitivity and warmth. These bonds weren’t fleeting emotions - they predicted lasting patterns in how mothers related to their toddlers over time.



On the other hand, mothers who had difficult experiences with their own parents struggled more to connect prenatally. 



These women often expressed frustration and anger in their early <a href="https://www.earth.com/news/eating-chili-during-pregnancy-may-actually-be-a-good-idea/" target="_blank" rel="noreferrer noopener">parenting</a>. The study reveals how cycles of emotional distance can repeat — but also how they can be identified and changed.



<h2 class="wp-block-heading" id="h-bonding-shapes-how-motherhood-begins">Bonding shapes how motherhood begins</h2>



Most parenting studies begin after childbirth. They examine how parents behave, what support systems they use, and how children respond. But Medina’s work shifts that focus to pregnancy itself - a time often treated as purely medical.



Her research fills a critical gap. The prenatal period isn’t just about physical development. It’s also an emotional window, where a parent begins forming their sense of identity and <a href="https://www.earth.com/news/all-of-your-energy-comes-from-mom-not-dad/" target="_blank" rel="noreferrer noopener">connection</a>. 



When that early bond feels strong, it can shape everything that comes after - from how a mother soothes her baby to how she sees herself in the role of a parent.



These findings suggest we need to rethink when parenting really begins. Pregnancy isn’t just preparation - it’s the beginning of a relationship.



<h2 class="wp-block-heading" id="h-young-mothers-can-build-strong-early-bonds">Young mothers can build strong early bonds</h2>



In addition to emotional insights, Dr. Medina’s study takes on harmful cultural stereotypes. Young, low-income mothers often carry the burden of negative assumptions. They are seen as disengaged or incapable. Medina wanted to counter that image with data from real lives.



“Parenting is challenging, and young, low-income mothers face additional stressors,” said Dr. Medina. “I focused on studying mother-infant relationships within this population to produce findings that may inform parenting support programs more closely aligned with the lived experiences of young, low-income mothers.”



The results contradict common misconceptions. The majority of participants reported strong prenatal connections. They continued to show care, attentiveness, and love as their children grew. 



This group, often painted in broad and negative strokes, revealed themselves as thoughtful, emotionally aware parents - navigating hardship with strength.



<h2 class="wp-block-heading" id="h-early-support-and-the-mother-baby-bond">Early support and the mother-baby bond</h2>



Dr. Medina believes our systems need to support mothers earlier in the journey. Too often, interventions wait until problems appear. Instead, she proposes we begin during pregnancy, when emotional connections are forming.



Dr. Medina suggests that support to promote strong parent-child relationships should begin during pregnancy. Interventions should help young mothers explore their past relationship experiences and recognize how they shape their expectations of parenthood. 



Programs that incorporate perinatal social workers or doulas could help facilitate these discussions and encourage healthier attachment patterns.



Support during pregnancy allows mothers to reflect on their own emotional histories. It also helps them build a sense of confidence and preparedness. 



Early conversations about relationships, expectations, and past trauma can have lasting effects on parenting style and connection.



<h2 class="wp-block-heading" id="h-access-remains-the-greatest-challenge">Access remains the greatest challenge</h2>



While the research offers clear solutions, one problem remains - access. Despite the promising insights, Dr. Medina says funding remains a key barrier to accessibility of such support programs.



Moving forward, she hopes to further investigate how familial and community-based support can help strengthen early mother-child bonds and improve long-term outcomes for young mothers and their children.



Her hope lies in community support networks - systems already embedded in many families’ lives. These local connections may offer flexible, culturally grounded ways to support young mothers. 



Medina’s future research will explore how family structures and neighborhood ties can reinforce early attachment.



Dr. Medina’s study invites us to expand our understanding of what it means to parent. Parenthood doesn’t begin with birth - it begins with emotion, intention, and connection. Her work reminds us that even in challenging circumstances, strong relationships can take root early.



The study is published in the journal <a href="https://onlinelibrary.wiley.com/doi/epdf/10.1002/imhj.22162" target="_blank" rel="noreferrer noopener">Infant Mental Health Journal Infancy and Early Childhood</a>.



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Mothers start bonding with their baby before delivery

We often think parenting begins after birth - diapers, lullabies,...

Ever heard of a rule that's been around for so long, everyone just assumes it's unbreakable? Well, a team of scientists is turning that notion on its head by proving wrong a key rule of organic chemistry.



Neil Garg, a distinguished professor of chemistry and biochemistry, is leading the charge to rewrite a fundamental principle that's been part of organic chemistry for the past hundred years.



In a recent study published in Science, Garg and his colleagues at <a href="https://www.ucla.edu" target="_blank" rel="noreferrer noopener">UCLA</a> revealed that Bredt's rule - a staple in chemistry textbooks since 1924 - might not be as ironclad as we've been led to believe.



But before we get into how they're shaking things up, let's take a step back and understand what this rule is all about.



<h2 class="wp-block-heading" id="h-what-exactly-is-bredt-s-rule">What exactly is Bredt's rule?</h2>



According to Bredt's rule, you can't have a double bond at the bridgehead position of a small, bridged ring system -- a kind of molecular structure that looks like two rings sharing some atoms. 



Imagine trying to fit a double bond in a tight space - it just doesn't work because the molecule becomes too strained and unstable.



In these small ring systems, the atoms are connected in such a way that there's not enough room for the flat shape of a <a href="https://www.earth.com/news/capturing-carbon-directly-from-the-air-is-now-much-more-efficient-thanks-to-new-material/" target="_blank" rel="noreferrer noopener">double bond</a>. 



The angles get all messed up, and the molecule would be forced into an awkward position. It's kind of like trying to bend a straight stick into a circle without breaking it - it just doesn't work that way.



Bredt's rule has been a guiding principle for chemists studying organic molecules, especially those known as olefins.



Olefins are compounds featuring a double bond between two <a href="https://www.earth.com/news/scientists-detect-molecules-that-store-carbon-in-space/" target="_blank" rel="noreferrer noopener">carbon atoms</a>, and they usually have a flat, planar structure.



<h2 class="wp-block-heading" id="h-turning-bredt-s-rule-upside-down">Turning Bredt's rule upside down</h2>



Garg's team decided to challenge that assumption. 



Instead of accepting the limitations imposed by this long-standing rule, they set out to prove that these molecules, called anti-Bredt olefins (ABOs), can indeed be created and used.



"People aren't exploring anti-Bredt olefins because they think they can't," Garg pointed out.



Using a clever approach, the researchers treated certain molecules known as silyl (pseudo)halides with a <a href="https://www.earth.com/news/is-water-fluoridation-still-effective/" target="_blank" rel="noreferrer noopener">fluoride source</a>. This reaction was designed to produce the elusive ABOs. 



Since these molecules are highly unstable and tend to fall apart quickly, the team included another chemical to "trap" them. 



This way, they could capture the ABOs long enough to study them and even use them to make new, valuable compounds.



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



Anti-Bredt olefins, or ABOs, are a bit of a chemistry oddity. 



Normally, double bonds don’t like to hang out at the bridgehead position of a bicyclic compound - that’s where Bredt’s Rule comes in. 



It says that putting a double bond at a bridgehead is usually too strained, especially in small or medium-sized rings. 



The atoms just can’t line up the way they need to for a stable double bond. But anti-Bredt olefins break that rule. 



They do have a double bond at the bridgehead, and they manage to exist anyway - sometimes even with surprising stability.



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



By showing that ABOs can be generated and utilized, the team is opening up new possibilities for <a href="https://www.earth.com/news/machine-learning-could-revolutionize-drug-discovery/" target="_blank" rel="noreferrer noopener">drug discovery</a>.



"There's a big push in the pharmaceutical industry to develop chemical reactions that give three-dimensional structures like ours because they can be used to discover new medicines," Garg explained. 



The ability to create these unique molecular structures means scientists can explore a whole new realm of compounds that were previously off-limits.



<h2 class="wp-block-heading" id="h-more-rules-need-to-be-challenged">More "rules" need to be challenged</h2>



Garg's work doesn't just break a rule -- it invites the entire scientific community to rethink how we approach long-held beliefs. 



"We shouldn't have rules like this -- or if we have them, they should only exist with the constant reminder that they're guidelines, not rules. It destroys creativity when we have rules that supposedly can't be overcome," he said.



By challenging Bredt's rule, the team is advocating for a more flexible and innovative approach to chemistry. 



They're reminding us that science is always evolving, and what we consider impossible today might just be tomorrow's breakthrough.



<h2 class="wp-block-heading" id="h-science-needs-more-creativity">Science needs more creativity</h2>



What does this mean for budding chemists and researchers? 



It's a call to question assumptions and push boundaries. If a century-old rule can be upended, who knows what other "impossible" feats are within reach?



"What this study shows is that contrary to one hundred years of conventional wisdom, chemists can make and use anti-Bredt olefins to make value-added products," Garg noted. 



It's not just about breaking a rule; it's about expanding the toolkit scientists have to tackle some of the world's most pressing challenges, like developing new medications.



<h2 class="wp-block-heading" id="h-what-s-next-for-garg-and-bredt-s-rule">What's next for Garg and Bredt's rule?</h2>



This discovery is a stepping stone to numerous possibilities in organic chemistry, pharmaceuticals, and basically any other field of study.



By demonstrating that ABOs can be both generated and trapped effectively, Garg's team has laid the groundwork for future research that could lead to significant advancements in medicine.



So, the next time you hear someone say, "You can't do that," remember that sometimes, all it takes is a fresh perspective and a willingness to challenge the status quo. 



Who knows? You might just be the one to rewrite the next chapter in the science books.



The full study was published in the journal <a href="https://www.science.org/doi/10.1126/science.adq3519" target="_blank" rel="noreferrer noopener">Science</a>.



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100-year-old chemistry rule proven false, updating textbooks comes next

Ever heard of a rule that's been around for so...

Scientists are transforming chocolate into a functional food by infusing it with probiotics and prebiotics, aiming to create a treat that satisfies cravings while supporting gut health. 



The challenge lies in maintaining chocolate's beloved texture and flavor while adding health benefits.



<figure class="wp-block-embed aligncenter is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio"><div class="wp-block-embed__wrapper">
https://youtu.be/Ug657J67iEo?si=w96YjGMsg939LD_3
</div></figure>



Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



Prebiotics act as food for these microbes, helping them thrive. Together, they form "synbiotics," a powerful health combination.



Researchers Smriti Gaur and Shubhi Singh from India's Jaypee Institute of Information Technology took an innovative approach, using natural prebiotics like corn and honey instead of complex processing methods. 



They created five chocolate varieties: a control and four synbiotic versions containing different combinations of prebiotics, probiotics (Lactobacillus strains), and flavor enhancers (cinnamon or orange).



Laboratory simulations of human digestion showed the probiotics remained viable for over five hours, suggesting they could survive long enough to benefit gut health.



Taste tests were positive, with researchers particularly enjoying the orange-flavored variety, describing it as having "vibrant citrus notes" complementing the "rich cocoa" with a "luxurious" texture.



This research represents just the beginning. With further refinement of strains, textures, and flavors, chocolate could evolve beyond mere indulgence to become a functional food that nourishes while it delights.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acsfoodscitech.4c00741" target="_blank" rel="noreferrer noopener">ACS Food Science &amp; Technology</a>.

Is chocolate the next nutritional powerhouse?

Scientists are transforming chocolate into a functional food by infusing...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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

<div class="wp-block-sendtonews-playerselector">[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"]</div>



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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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This image shows the aftermath of <a href="https://www.earth.com/video/puerto-rico-after-hurricane-maria/">Hurricane Maria</a> in Puerto Rico and was captured by the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>. This landscape usually appears as a lush and vibrant green, but now looks like a dark brown after Maria destroyed vegetation and kicked up sediment and mud.

Aftermath of Hurricane Maria in Puerto Rico

Fire damage from the Santa Rosa California wildfires is featured in this Image of the Day from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>. Back in October 8, 2017, <a href="https://www.earth.com/news/wildfires-california-wine-country/">wildfires</a> devastated the region, killing at least 29 people and engulfing over 265 square miles of land. According to <a href="http://www.fire.ca.gov/">CalFire</a>, at least 3,500 homes and businesses have been destroyed.

Aftermath of Hurricane Maria in Puerto Rico

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