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

Black Widow Spider -Female, male and egg sac Photo Credit: Mark_Kostich

Black Widow Spider

In the heart of the Lighthouse Reef Atoll, off the coast of Belize in the Caribbean, lies a fascinating geological wonder - the Great Blue Hole. This vast, circular sinkhole bears an uncanny resemblance to a giant oceanic eye gazing up at the sky.



Nestled in the turquoise waters of the atoll, about 43 miles from the coast of Belize, this dark circular pit is surrounded by coral and contains sediments that tell a story about centuries of storms.



The Great Blue Hole began as a limestone cave on a dry island. During the last ice age, its roof collapsed, leaving it open to the elements. Today, this underwater cave plunges to a depth of 410 feet, spans 980 feet, and is one of the most fascinating places to scuba dive.



As glaciers melted and sea levels rose, the cave filled with water, turning it into a natural vault of sediment that has quietly recorded the passage of time.



In the summer of 2022, a team of scientists from <a href="https://www.goethe-university-frankfurt.de/en" target="_blank" rel="noreferrer noopener">Goethe University Frankfurt</a> led a mission to explore this hidden archive. Funded by the German Research Foundation, the researchers brought a drilling platform out to sea and extracted a 30-meter-long sediment core from the bottom of the Great Blue Hole.



The analysis, carried out by researchers from the universities of Frankfurt, Cologne, Göttingen, Hamburg, and Bern, has given new insight into storm history and climate change in the southwestern Caribbean.



<h2 class="wp-block-heading" id="h-storm-record-written-in-sediment">Storm record written in sediment</h2>



Roughly 7,200 years ago, the limestone island that once held the Great Blue Hole was overtaken by the sea. Since then, layers of sediment have quietly accumulated at the bottom of the underwater cave.



These layers act like a natural time capsule, offering a window into 5,700 years of storm activity. Each layer records the passing of time, just as is found in <a href="https://www.earth.com/news/californias-weather-extremes-found-in-600-year-old-tree-rings/" target="_blank" rel="noreferrer noopener">tree rings</a>.



“Due to the unique environmental conditions – including oxygen-free bottom water and several stratified water layers – fine marine sediments could settle largely undisturbed in the Great Blue Hole,” said Dr. Dominik Schmitt, a researcher in the Biosedimentology Research Group at Goethe University Frankfurt.



“Inside the sediment core, they look a bit like tree rings, with the annual layers alternating in color between gray-green and light green depending on organic content.”



But not all layers are the same. Some are made up of coarser, lighter-colored particles. 



These event layers, called tempestites, formed when powerful waves from hurricanes and tropical storms swept coarse material from the atoll’s outer reef into the hole. 



“The tempestites stand out from the fair-weather gray-green sediments in terms of grain size, composition, and color, which ranges from beige to white,” Schmitt added.



<h2 class="wp-block-heading" id="h-long-term-climate-patterns">Long-term climate patterns </h2>



The team identified and dated 574 individual storm events that were preserved in the sediment core. This detailed storm record stretches far beyond the reach of written or instrumental history, which only covers about 175 years. 



The results offer a unique look into long-term climate patterns and <a href="https://www.earth.com/news/scientists-propose-adding-a-category-6-to-the-current-hurricane-intensity-scale/" target="_blank" rel="noreferrer noopener">hurricane</a> behavior in the region.



The data paints a clear picture: storm activity in the southwestern Caribbean has steadily risen over the past 6,000 years.



“A key factor has been the southward shift of the equatorial low-pressure zone. Known as the <a href="https://www.earth.com/news/tropical-rains-will-shift-northward-in-the-coming-decades/" target="_blank" rel="noreferrer noopener">Intertropical Convergence Zone</a>, this zone influences the location of major storm formation areas in the Atlantic and determines how tropical storms and hurricanes move and where they make landfall in the Caribbean,” Schmitt said.



The researchers also discovered a connection between sea surface temperatures and storm frequency. Warmer waters matched up with periods of increased storm activity. 



“These shorter-term fluctuations align with five distinct warm and cold climate periods, which also impacted water temperatures in the tropical Atlantic,” Schmitt noted.



<h2 class="wp-block-heading" id="h-a-warning-from-the-storm-record">A warning from the storm record</h2>



Historical averages suggest that the Great Blue Hole experienced between four and sixteen major storms per century. However, the sediment record shows that nine storms have already occurred in just the past 20 years.



“Our results suggest that some 45 tropical <a href="https://www.earth.com/news/record-heat-fueled-unexpected-and-deadly-storms-in-2023/" target="_blank" rel="noreferrer noopener">storms</a> and hurricanes could pass over this region in our century alone. This would far exceed the natural variability of the past millennia,” said Prof. Eberhard Gischler of Goethe University Frankfurt.



The team emphasizes that natural climate changes alone cannot explain this dramatic increase. Instead, they point to human-driven global warming. 



The rise in ocean temperatures and the growing strength of La Niña events are creating the perfect conditions for more frequent and more intense storms.



<h2 class="wp-block-heading" id="h-a-sediment-core-with-a-message">A sediment core with a message</h2>



The Great Blue Hole, once thought to be a quiet underwater marvel, is now telling a louder story - one of climate shifts and increasing storm risk.



As the sediment layers continue to build, so does the urgency to address the accelerating pace of extreme weather. 



This research reminds us that history, especially the kind written in mud and sand, still has much to teach us.



The full study was published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.ads5624" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Sediment in the Great Blue Hole reveals an alarming storm record

In the heart of the Lighthouse Reef Atoll, off the...

The feeling of fullness after a nice meal usually prevents us from eating more. This is a familiar experience for humans, but we are not alone. We share this with starfish and many other organisms as well.



New research indicates that the same message instructing us to eat no more has existed for more than 500 million years. The same molecule affecting our feeding behavior in this way also acts on starfish and other sea animals.



Researchers at <a href="https://www.qmul.ac.uk/" target="_blank" rel="noreferrer noopener">Queen Mary University of London</a> have followed the evolutionary trail of a neurohormone named bombesin, which regulates appetite in humans. 



Collaborating with colleagues at the Institut Pasteur in Paris and the University of Warwick, the researchers discovered that this satiety-inducing peptide is much older than was thought, and is found in animals that lived before the first <a href="https://www.earth.com/news/over-half-of-the-worlds-vertebrates-reside-in-the-tropics/" target="_blank" rel="noreferrer noopener">vertebrates</a> set foot on Earth.



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



Bombesin is a small peptide that helps regulate appetite by sending a message when it's <a href="https://www.earth.com/news/neurons-discovered-that-tell-us-when-to-stop-eating/" target="_blank" rel="noreferrer noopener">time to stop eating</a>. While it’s been studied in humans and other mammals, its origins were less understood - until now. 



Researchers discovered that a bombesin-like molecule is present in echinoderms like starfish, sea urchins, and sea cucumbers.



If you’re wondering about the unusual name, bombesin isn’t explosive. It’s named after the fire-bellied toad, Bombina bombina, where it was first identified in 1971. 



Scientists noticed that injecting this compound into <a href="https://www.earth.com/news/evolutionary-mystery-why-are-mammals-the-only-vertebrates-to-have-only-one-lower-jawbone/" target="_blank" rel="noreferrer noopener">mammals</a> caused them to eat less and take longer between meals. This led to the idea that bombesin-like neurohormones are part of the body’s natural appetite control system.



Today, compounds that mimic bombesin are being explored as potential treatments for obesity, alongside well-known medications like Ozempic.



<h2 class="wp-block-heading" id="h-a-needle-in-a-haystack">A needle in a haystack</h2>



The research team began by searching for bombesin-like genes in <a href="https://www.earth.com/news/ocean-noise-can-be-fatal-to-marine-invertebrates/" target="_blank" rel="noreferrer noopener">marine invertebrates</a>. 



“It was a bit like looking for a needle in a haystack,” said Professor Maurice Elphick. “But eventually we discovered genes encoding a bombesin-like neurohormone in the genomes of starfish and their relatives.”



Once the gene was identified in the common starfish (Asterias rubens), scientists named the molecule ArBN. 



Collaborators at the University of Warwick used mass spectrometry to determine the exact structure of ArBN, which allowed the molecule to be synthesized for lab testing.



<h2 class="wp-block-heading" id="h-watching-starfish-eat-or-not-eat">Watching starfish eat - or not eat</h2>



<a href="https://www.earth.com/news/starfish-break-off-their-arms-to-evade-danger-and-regenerate-them-later/" target="_blank" rel="noreferrer noopener">Starfish</a> feed in a bizarre and fascinating way: they push their stomachs out through their mouths to digest prey like mussels. The team wanted to know how ArBN affected this feeding behavior.



“When I tested ArBN, I saw that it caused contraction of the starfish stomach. This suggested that ArBN might be involved in stimulating stomach retraction when starfish stop feeding. And this is exactly what I found," explained Dr. Weiling Huang, who conducted the behavioral tests. 



"When I injected ArBN into starfish with their stomachs everted, it triggered the stomach to retract back into the mouth. What’s more, ArBN also delayed the initiation of feeding, as starfish injected with ArBN took longer to enclose a mussel compared to those injected with water.”



<h2 class="wp-block-heading" id="h-a-molecule-older-than-starfish">A molecule older than starfish</h2>



Understanding that bombesin-like molecules have been regulating feeding behavior since before the rise of vertebrates adds an important piece to the puzzle of how appetite evolved. 



“We can infer that this function extends back half-a-billion years to the common ancestor of starfish, humans, and other vertebrates,” said Professor Elphick.



But the implications go beyond biology textbooks. Some species of starfish are moving into new habitats due to climate change. In particular, these species are seeking cooler waters where shellfish farms are located, and may threaten aquaculture operations.



“One of the consequences of climate change is that some starfish species are invading cooler waters where shellfish are cultivated for human consumption,” said Professor Elphick.



“Discovering molecules that inhibit feeding in starfish could be useful in managing these invasions.”



<h2 class="wp-block-heading" id="h-more-than-just-an-ancient-molecule">More than just an ancient molecule</h2>



This study connects two very different worlds: the sophisticated brain-gut interactions in humans and the slow, alien feeding behavior of starfish. Yet both rely on the same ancient molecule to know when it's time to stop eating.



As scientific discoveries reveal the biological links between species, the deep interconnectedness of all life becomes ever more apparent.



The full study was published in the journal <a href="https://dx.doi.org/10.1073/pnas.2420966122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Ancient molecule tells starfish and humans when to stop eating

The feeling of fullness after a nice meal usually prevents...

Humans are good at using the things that the natural world has to offer. Trees are used for their timber and fruits, bees and other insects pollinate our crops, and mountains bring us peace. But what happens when nature is pushed too far? 



As the planet heats up and extreme weather becomes more frequent, we may soon find ourselves counting the real cost - not just in lost trees or damaged trails, but in disappearing livelihoods and shaken communities.



Imagine Colorado’s wildflower meadows scorched by wildfire, or a strawberry field yielding less because heat drives away pollinators. These aren’t just <a href="https://www.earth.com/news/world-wildlife-day-2025-a-global-call-to-protect-nature/" target="_blank" rel="noreferrer noopener">environmental losses</a>; they impact economies, families, and entire ways of life. 



As extreme weather becomes more frequent, scientists are asking a new kind of question: How do we measure what we’re about to lose? A recent study led by <a href="https://www.colorado.edu" target="_blank" rel="noreferrer noopener">CU Boulder</a> researchers brings new tools to that conversation.



<h2 class="wp-block-heading" id="h-how-extreme-weather-harms-nature">How extreme weather harms nature</h2>



In a paper published in Nature Ecology &amp; Evolution, ecologist Laura Dee and her team introduced a computer model that looks at extreme weather with a fresh perspective.



The model connects environmental damage with economic and social consequences. It’s designed to predict what could happen if violent storms, fires, or floods hit ecosystems that people depend on.



The study’s example is striking: a forest in Minnesota could lose up to 50% of its timber income if a severe windstorm strikes.



“With climate change, there’s an urgent need to incorporate the impacts [that] extreme <a href="https://www.earth.com/news/people-must-reconnect-with-nature-now-to-save-biodiversity/" target="_blank" rel="noreferrer noopener">events</a> like mega-fires and hurricanes have on the benefits nature provides,” said Laura Dee, the paper’s first author and associate professor in the Department of Ecology and Evolutionary Biology.



“This research is an important step toward anticipating impacts to ecosystem services so that we can adapt management strategies accordingly.”



<h2 class="wp-block-heading" id="h-understanding-ecosystem-services">Understanding ecosystem services</h2>



The model focuses on what scientists call “ecosystem services,” which are the direct and indirect benefits that people derive from natural processes.



These include water purification by tree roots, crop pollination by insects, and carbon storage in <a href="https://www.earth.com/news/natures-grip-on-co2-is-slipping-what-it-means-for-us-all/" target="_blank" rel="noreferrer noopener">forests</a>. They also include less obvious values, like the joy of hiking or the cultural significance of a mountain lake.



Traditionally, climate models have treated environmental changes as gradual - things that happen slowly over time. But extreme weather doesn’t follow a smooth path. Wildfires, hurricanes, and floods hit fast and hard, causing damage that lingers long after the skies clear.



Dee’s model fills this gap by focusing on sudden disturbances and how they ripple through both ecosystems and economies. It doesn’t just track what gets damaged - it also accounts for how people value what is lost.



<h2 class="wp-block-heading" id="h-a-forest-put-to-the-test">A forest put to the test</h2>



To demonstrate how the model works, the researchers applied it to a mixed <a href="https://www.earth.com/news/we-must-live-in-harmony-with-nature-to-create-a-sustainable-future/" target="_blank" rel="noreferrer noopener">forest</a> in northern Minnesota. They studied how various tree species - each with different levels of wind resistance and market value - respond to intense windstorms.



For instance, white cedar trees are sturdy against strong winds but bring in less profit. Balsam firs are weaker but sell at a higher price.



The simulation showed a striking result: depending on storm strength, timber value could drop by between 23% and 50%. And timber isn’t the only thing at risk. Hiking, birdwatching, and camping opportunities also take a hit after such damage, further reducing the forest’s value to surrounding communities.



Dee said that researchers and land management officials could use the model to evaluate the impacts of any disturbances, from drought to invasive species.



<h2 class="wp-block-heading" id="h-reducing-extreme-weather-to-protect-nature">Reducing extreme weather to protect nature</h2>



Dee’s work doesn’t stop with predicting wind damage. Her research group at CU Boulder also looks at fire management. Specifically, they study how prescribed burns - intentional fires set under controlled conditions - can reduce wildfire <a href="https://www.earth.com/news/tackling-the-dual-crises-of-climate-and-nature/" target="_blank" rel="noreferrer noopener">risks</a>.



The new model supports these efforts by identifying areas where controlled burns could offer the greatest benefits. This includes not only reducing the risk of massive wildfires but also protecting other ecosystem services like clean water and carbon removal.



“Nature’s contributions to people have not typically been valued and are usually left out of key decision-making processes when developing land management policies and strategies,” Dee said.



By offering a clearer picture of what’s at stake, this model helps planners make smarter choices about which lands to protect and how.



<h2 class="wp-block-heading" id="h-a-wake-up-call-for-economic-systems">A wake-up call for economic systems</h2>



This isn’t just about trees and trails. It’s about how we prepare for a future where nature’s disruptions affect jobs, housing, and national economies. 



On March 5, the United Nations’ World Meteorological Organization reported that over 150 record-breaking weather events occurred across the globe last year. The pattern is not only repeating - it’s accelerating.



Dee believes our economic models must change to reflect this new reality. Traditional indicators like Gross Domestic Product don’t account for the value of clean air, stable forests, or functioning watersheds. But as these systems grow more vulnerable, leaving them out of the equation could become a costly mistake.



“If we fail to consider the growing risks from extreme weather events, we could lose more than we realize,” she said.



<h2 class="wp-block-heading" id="h-the-value-of-nature">The value of nature </h2>



What if planning for the future required not just spreadsheets and projections, but listening more closely to forests, rivers, and skies? Dee’s model is a reminder that nature’s value goes far beyond dollars. 



When we account for it properly, we make better decisions - not just for the environment, but for ourselves.



Extreme weather doesn’t wait. It strikes hard and fast. And with tools like this new simulation, we can at least be ready to measure the fallout and prepare. Because in the age of climate uncertainty, knowing what we stand to lose is the first step in making sure we don’t lose it.



The study is published in the journal <a href="https://www.nature.com/articles/s41559-024-02626-y" target="_blank" rel="noreferrer noopener">Nature Ecology &amp; Evolution</a>.



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Extreme weather is pushing nature toward a breaking point

Humans are good at using the things that the natural...

In a major scientific milestone, a team of researchers has captured the first continuous, real-time footage of cellulose being synthesized and self-assembled into the intricate scaffolding that gives plant cells their structure.&nbsp;



Using advanced microscopy techniques and a custom-built imaging system, the team recorded 24 hours of this cellular construction process in living plant cells, revealing surprising new details about how plant cell walls are built.



The study, led by <a href="https://newbrunswick.rutgers.edu/" target="_blank" rel="noreferrer noopener">Rutgers University–New Brunswick</a>, provides an unprecedented look into the behavior of cellulose - the most abundant biopolymer on Earth.



The research also offers insights that could lead to stronger, more resilient <a href="https://www.earth.com/news/nanoparticles-unlock-a-new-way-to-genetically-modify-plants/" target="_blank" rel="noreferrer noopener">crops</a>, cheaper biofuels, biodegradable plastics, and other sustainable products.



<h2 class="wp-block-heading" id="h-closer-look-at-plant-cells">Closer look at plant cells</h2>



Cellulose is a key component of plant cell walls and plays a vital role in maintaining plant structure. It’s also a valuable resource used in countless everyday products, from paper and clothing to food thickeners and filtration materials.



Sang-Hyuk Lee is an associate professor in the Department of Physics and Astronomy at Rutgers and a co-author of the study.&nbsp;



“This work is the first direct visualization of how cellulose synthesizes and self-assembles into a dense fibril network on a plant cell surface, since Robert Hook’s first microscopic observation of cell walls in 1667,” said Lee.



“This study also provides entirely new insights into how simple, basic physical mechanisms such as diffusion and self-organization may lead to the formation of complex cellulose networks in cells.”



The <a href="https://www.eurekalert.org/multimedia/1064673" target="_blank" rel="noreferrer noopener">videos</a> produced by Lee’s team show protoplasts - plant cells with their outer walls removed - from Arabidopsis, a relative of cabbage, as they spontaneously begin forming cellulose filaments.



These filaments grow outward from the cell surface in seemingly chaotic patterns, gradually coalescing into the highly organized structure of a new cell wall.



“I was very surprised by the emergence of ordered structures out of the chaotic dance of molecules when I first saw these video images,” Lee said. “I thought plant cellulose would be made in a lot more of an organized fashion, as depicted in classical biology textbooks.”



<h2 class="wp-block-heading" id="h-a-team-effort-across-disciplines">A team effort across disciplines</h2>



The breakthrough is the result of more than six years of collaboration between three Rutgers laboratories representing physics, engineering, and plant biology. Each group played a vital role in bringing the project to life.



When standard laboratory microscopes proved too limited to observe the fine detail of cellulose formation, Lee developed a specialized system based on total internal reflection fluorescence microscopy. 



This method allowed the researchers to image the cell’s underside with high resolution over long periods without damaging the samples.



Meanwhile, Shishir Chundawat, an associate professor in the Department of Chemical and Biochemical Engineering at Rutgers, led the development of a fluorescent probe system that tagged cellulose molecules so they could be visualized under the microscope. 



<h2 class="wp-block-heading" id="h-how-to-watch-plants-build-cell-walls">How to watch plants build cell walls</h2>



His team used a modified bacterial enzyme that binds specifically to cellulose to create the tagging system.



“I have always been fascinated by plants and how they capture sunlight via leaves into reduced carbon forms like cellulose that form cell walls,” said Chundawat, who is also focused on biofuel and bioproduct development. 



“I was inspired by collecting leaves as a middle school student. That early curiosity led me to delve deeper into biomass and its potential to create valuable, sustainable products.”



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/plant-cellulose_microfibril-network_illustration_credit-Ehsan-Faridi_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/plant-cellulose_microfibril-network_illustration_credit-Ehsan-Faridi_1s.webp" alt="Artistic rendering of cellulose regenerating on a plant protoplast cell surface with zoomed out view. Cellulose is synthesized by plasma membrane-bound enzyme complexes (green) and assembles into a microfibril network (brown), forming the main scaffold for the cell wall. Credit: Ehsan Faridi/ Inmywork Studio/ Chundawat, Lee and Lam Labs" class="wp-image-1963291"/></a><figcaption class="wp-element-caption">Artistic rendering of cellulose regenerating on a plant protoplast cell surface with zoomed out view. Cellulose is synthesized by plasma membrane-bound enzyme complexes (green) and assembles into a microfibril network (brown), forming the main scaffold for the cell wall. Credit: Ehsan Faridi/ Inmywork Studio/ Chundawat, Lee and Lam Labs</figcaption></figure>



Eric Lam, a professor in the Department of Plant Biology, and his team developed the protocol to isolate protoplasts - cells stripped of their original walls. 



This provided a clean slate on which new cellulose fibers could be tracked as they formed in real time.



“This provided little to no background cellulose to confound our visualization and tracking of newly synthesized cellulose under optimized conditions,” Lam explained.



<h2 class="wp-block-heading" id="h-implications-for-agriculture-and-biofuels">Implications for agriculture and biofuels</h2>



The new findings are expected to inform future genetic and biotechnological efforts to enhance cellulose production in crops - improving traits like <a href="https://www.earth.com/news/droughts-and-extreme-weather-events-are-escalating/" target="_blank" rel="noreferrer noopener">drought</a> resistance, <a href="https://www.earth.com/news/turning-plants-into-carbon-capture-machines-with-cyanobacteria/" target="_blank" rel="noreferrer noopener">carbon capture</a>, and the efficiency of biomass conversion to fuel.



“This discovery opens the door for researchers to begin dissecting the genes that could play various roles for cellulose biosynthesis in the plant,” Lam said.&nbsp;



“The knowledge gained from these future studies will provide new clues for approaches to design better plants for carbon capture, improve tolerance to all kinds of environmental stresses, from drought to disease, and optimize second-generation cellulosic biofuels production.”



<h2 class="wp-block-heading" id="h-a-new-chapter-in-plant-biology">A new chapter in plant biology</h2>



The Rutgers team’s work challenges the traditional textbook narrative of orderly cellulose assembly, showing that what appears initially as disordered movement eventually organizes into the essential structure of the cell wall. 



This finding adds complexity to our understanding of plant biology and could inspire future scientists to take a closer look - literally and figuratively - at the hidden processes that sustain life on Earth.



Animations aimed at young students often simplify how plant cell walls are made, but the Rutgers team’s research reveals that the real process is far more intricate - and far more beautiful.



The study is published in the journal <a href="http://dx.doi.org/10.1126/sciadv.ads6312" target="_blank" rel="noreferrer noopener">Science Advances</a>.



Image Credit: Ehsan Faridi/ Inmywork Studio/ Chundawat, Lee and Lam Labs



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How plants build their cell walls is seen by scientists for the first time ever

In a major scientific milestone, a team of researchers has...

It's easy to think that older forests, with their diverse and well established trees, are better at storing carbon. Many assume that, as trees grow and ecosystems mature, they naturally become more effective at soaking up carbon from the atmosphere. 



A new study from scientists at the <a href="https://umich.edu/" target="_blank" rel="noreferrer noopener">University of Michigan</a> Biological Station challenges this assumption, however, and suggests that the reality is much more complicated.



The research team, which included more than 100 scientists over several decades, found that <a href="https://www.earth.com/news/mixed-forests-with-many-tree-species-are-more-effective-at-carbon-storage/" target="_blank" rel="noreferrer noopener">carbon storage in forests</a> depends more on what's happening within the ecosystem than how old it is. 



Factors like the structure of the forest canopy, the types of trees and fungi present, and how nutrients move through the soil all play a bigger role than previously thought.



<h2 class="wp-block-heading" id="h-looking-at-two-centuries-of-change">Looking at two centuries of change</h2>



The research was conducted at the U-M Biological Station in Pellston, Michigan. This historic field site, founded in 1909, spans over 10,000 acres and has long served as a hub for studying northern <a href="https://www.earth.com/news/forests-rich-tree-diversity-adapt-better-changing-climate/" target="_blank" rel="noreferrer noopener">forest ecosystems</a>. 



Scientists used data from a wide range of forest stands on the property. Some were untouched remnants from the 1800s, while others had been logged or burned at different points in the 20th century.



At the heart of the study was a massive dataset that had been built over decades. It included information from the station’s 150-foot AmeriFlux tower, which tracks carbon dioxide, water, and energy flows between forests and the atmosphere.



Additional data covered everything from soil respiration and microbial activity to leaf litter, root growth, and nutrient cycling.



Luke Nave was the study's lead researcher and a faculty member at Michigan Technological University.



"Time is not what drives <a href="https://www.earth.com/news/plants-release-carbon-faster-than-we-expected/" target="_blank" rel="noreferrer noopener">carbon cycling</a>," said Nave. "Time is more of a playing field, and the rules of the game on that field are things like canopy structure, tree and microbial community composition, and soil nitrogen availability."



"That means that changes in things like structure, composition and soil nitrogen are what control forest carbon trajectories, whether those changes happen quickly or slowly, and whether we are influencing those changes through management or letting them happen on their own terms."



<h2 class="wp-block-heading" id="h-the-power-of-long-term-carbon-research">The power of long-term carbon research</h2>



One of the study’s strengths lies in its use of both historical and current data. 



With so much emphasis on real-time monitoring, the researchers were able to paint a detailed picture of how carbon moves through forest ecosystems - and how that movement has changed over time.



"It's exciting to see the results of this study. It was a lot of work and many years in the making," said Jason Tallant, data manager and research specialist at the University of Michigan Biological Station.



"At the U-M Biological Station, we put a lot of effort into data curation and digitization. It's nice to see the carbon synthesis research team leverage our historic data sets and crunch real-time <a href="https://www.earth.com/news/forest-modeling-study-reveals-new-insights-into-carbon-sequestration/" target="_blank" rel="noreferrer noopener">carbon sequestration</a> information to illuminate what's happening in our forests and inform future management."



The project brought together a wide range of measurements, including fungal community studies, root production, carbon pool tracking, and soil enzyme activity. All of these factors helped the team understand how different pieces of the ecosystem influence carbon storage.



<h2 class="wp-block-heading" id="h-rethinking-forest-management">Rethinking forest management</h2>



The takeaway from this study is clear: managing forests means more than just letting them grow old. 



If we want forests to help mitigate climate change, we need to pay close attention to their structure and species makeup, both above and below the ground.



"With the rates of change we're now seeing in things like climate, forest health and disturbance, and tree species composition, management will have to contend with more challenges and constraints all the time. What was true a decade or two ago can't be assumed as truth at this point," Nave commented.



"A good example for folks who know the territory is on the Burn Plots - the 1998 burn is a thriving young stand of post-clearcut aspen, and the 2017 burn is a regeneration failure. You might not think that 19 years is a long time to a tree, but it is in today's world."



"Researchers and managers who take a whole-ecosystem perspective like we did in the paper will have an easier time understanding what has changed over the last few decades and what we can do about it to <a href="https://www.earth.com/news/future-forests-which-tree-species-can-survive-climate-change/" target="_blank" rel="noreferrer noopener">sustain forests</a>."



This study reminds us that forests are dynamic systems, and treating them as such is essential for their health and their ability to store carbon. 



Simply counting the years isn't enough. Understanding what happens within those years is what really matters.



The full study was published in the journal <a href="https://esajournals.onlinelibrary.wiley.com/doi/10.1002/eap.70001">Ecological Applications</a>.



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Older forests do not necessarily store more carbon

It's easy to think that older forests, with their diverse...

Pregnancy often brings with it a mix of anticipation, anxiety, and countless decisions - especially about food. For decades, health experts have promoted beans as a budget-friendly powerhouse food rich in protein, fiber, and complex carbohydrates. 



Now, new research offers an interesting twist: eating chili with beans during pregnancy may reduce the risk of developing gestational diabetes.



This spicy finding comes from a recent study by researchers at the University at Buffalo. Published in the journal Nutrients, the study highlights chili as a possible dietary ally for <a href="https://www.earth.com/news/study-links-teen-pregnancy-to-smaller-newborns/" target="_blank" rel="noreferrer noopener">pregnant individuals</a> - especially those at higher risk for blood sugar complications.



But how did the researchers make this connection? And why chili, specifically? The answers may surprise you.



<h2 class="wp-block-heading" id="h-rising-challenge-of-gestational-diabetes">Rising challenge of gestational diabetes</h2>



Gestational diabetes is a condition diagnosed during pregnancy that affects how the body processes sugar.



If unmanaged, it can lead to complications for both the baby and the mother. While the condition typically resolves after childbirth, it leaves behind a lingering risk - mothers are more likely to develop Type 2 diabetes later in life.



Factors like pre-pregnancy obesity, maternal age, excessive pregnancy weight gain, low physical activity, poor diet, and even COVID-19 have all been linked to this condition. 



​According to recent data from the&nbsp;<a href="https://www.cdc.gov/mmwr/volumes/72/wr/mm7201a4.htm" target="_blank" rel="noreferrer noopener">Centers for Disease Control and Prevention</a>, gestational diabetes in the U.S. increased from 6.0% in 2016 to 8.3% in 2021.​



In response to this rise, researchers are exploring ways to reduce risk - ideally through practical, nutritional choices. That’s where beans come into the picture.



Known for their ability to stabilize blood sugar levels and support digestive health, beans have already earned their place on many healthy-eating lists. But what happens when beans are cooked into a spicy, flavorful bowl of chili?



<h2 class="wp-block-heading" id="h-chili-consumption-during-pregnancy">Chili consumption during pregnancy </h2>



The team at the University at Buffalo wanted to explore this very question. 



Using data from the Infant Feeding Practices Study II, a U.S. national cohort effort by the Food and Drug Administration and the CDC, researchers analyzed eating habits of 1,397 pregnant women. 



Their goal was to see if different forms of bean consumption - chili, dried beans, and bean soup - had any effect on the risk of gestational diabetes during pregnancy.



“Our research aimed to study the roles of bean consumption in gestational diabetes, including chili, dried beans and bean soup,” said Dr.&nbsp;Xiaozhong Wen, first author and associate professor of pediatrics in the Division of Behavioral Medicine in the&nbsp;<a href="https://medicine.buffalo.edu/" target="_blank" rel="noreferrer noopener">Jacobs School of Medicine and Biomedical Sciences</a>.​



“Interestingly, only chili consumption was statistically significantly associated with the risk of gestational diabetes.”



According to the study, <a href="https://www.earth.com/news/how-pregnancy-changes-the-brain/" target="_blank" rel="noreferrer noopener">women</a> who ate chili once per month had a 3.5% risk of developing gestational diabetes. Those who never ate chili had a 7.4% risk. That’s a significant difference for just one serving a month. 



But it also raises a new question: what makes chili so special?



<h2 class="wp-block-heading" id="h-chili-may-help-control-blood-sugar">Chili may help control blood sugar</h2>



Beans alone carry many benefits, including being high in fiber and low on the glycemic index. But chili often includes more than just beans. It typically contains dark beans, chili powder, and sometimes additional spices - all of which might contribute to its unique effects on blood sugar.



The researchers point to two specific components: capsaicin, the compound responsible for chili’s heat, and phenolic compounds found in dark beans. These substances have shown promise in both human and animal studies.



“Both human and animal studies have shown that capsaicin and phenolic compounds have some potential benefits of improving glycemic control through slowing glucose absorption and increasing insulin secretion and/or insulin sensitivity,” said Wen.



While the exact mechanism isn’t fully understood, the combination of these elements may work together to help the body manage blood sugar more effectively. This makes chili not just a comfort food but potentially a functional food - at least for <a href="https://www.earth.com/news/pregnancy-stress-may-have-lasting-effects-on-fetal-development/" target="_blank" rel="noreferrer noopener">pregnant women</a>.



<h2 class="wp-block-heading" id="h-future-research-on-chili-during-pregnancy">Future research on chili during pregnancy </h2>



It’s important to note that this study was observational. That means the researchers didn’t assign participants to eat chili; they simply studied existing eating patterns and health outcomes. As a result, they cannot prove cause and effect.



Wen acknowledges this and calls for caution when interpreting the findings. He emphasizes the need for further research.



Wen says the research findings need to be replicated in larger cohorts with more diverse populations, detailed measures of bean consumption and dietary intake information collected more frequently and a randomized controlled design.



He adds that given the non-causal nature of observational research, recall bias and selection bias, the findings should be interpreted cautiously.



That said, the results are compelling enough to encourage further investigation. A single monthly serving of chili cutting gestational diabetes risk nearly in half is an idea worth exploring, especially if it can be done safely and inexpensively.



<h2 class="wp-block-heading" id="h-chili-may-support-a-diabetes-safe-diet">Chili may support a diabetes-safe diet</h2>



So what should expecting mothers do with this information? Should chili become a regular part of prenatal nutrition? Wen offers a balanced approach.



“Moderate chili consumption may be incorporated into a balanced diet approach to addressing gestational diabetes, along with other clinical recommendations, such as early screening, diagnosis, exercise and medications as needed,” says Wen.



This means chili should not replace medical care or professional dietary advice, but it may have a place at the table. Especially for <a href="https://www.earth.com/news/moms-health-shapes-how-well-an-embryo-develops/" target="_blank" rel="noreferrer noopener">women</a> at higher risk of gestational diabetes, it could be a simple, delicious way to support their health.



<h2 class="wp-block-heading" id="h-looking-ahead-what-comes-next">Looking ahead: What comes next</h2>



​The study was co-led by Todd C. Rideout, PhD, associate professor of exercise and nutrition sciences in the&nbsp;<a href="https://publichealth.buffalo.edu/" target="_blank" rel="noreferrer noopener">School of Public Health and Health Professions</a>&nbsp;at the&nbsp;<a href="https://www.buffalo.edu/" target="_blank" rel="noreferrer noopener">University at Buffalo</a>.&nbsp;



Other University at Buffalo contributors included Fatima Makama, Ryan Buzby, Jeremy Nguyen, Rose Durnell, Iyobosa Ekhator, and Daren Chan.&nbsp;The&nbsp;<a href="https://www.usda.gov/" target="_blank" rel="noreferrer noopener">U.S. Department of Agriculture</a>&nbsp;funded the research.​



As scientists continue to explore the links between food and <a href="https://www.earth.com/news/cbd-use-during-pregnancy-has-unexpected-consequences/" target="_blank" rel="noreferrer noopener">maternal health</a>, this study opens new possibilities. A bowl of chili may hold more than warmth and flavor — it might also support better blood sugar control during one of life’s most critical periods.



For now, pregnant individuals should focus on balanced eating, regular checkups, and physical activity. But with research like this, even small choices — like what you put in your bowl — could make a meaningful difference.



The study is published in the journal <a href="https://www.mdpi.com/2072-6643/17/6/1025" target="_blank" rel="noreferrer noopener">Nutrients</a>.



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Eating chili during pregnancy may actually be a good idea

Pregnancy often brings with it a mix of anticipation, anxiety,...

In the invisible war between life forms, bacteria constantly fight off threats from viruses. These viruses, known as bacteriophages or simply “phages,” infect bacterial cells the same way human viruses attack our own bodies, leaving behind a memory of the invasion.



But unlike humans, bacteria don’t have white blood cells or antibodies. Instead, they use a genetic system called CRISPR to defend themselves. This ancient defense system is now drawing fresh attention from scientists.



Recent research from Johns Hopkins Medicine shows that <a href="https://www.earth.com/news/bacteria-strain-identified-that-can-eat-forever-chemicals/" target="_blank" rel="noreferrer noopener">bacteria</a> don’t just defend passively. They actively gather pieces of viral code to remember their enemies. They pass these memories to their descendants. 



Understanding this bacterial memory process may help us design new treatments for antibiotic-resistant infections - a growing global concern.



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



Phages get their name from the Greek word meaning “bacteria-eaters.” 



These viruses either destroy their bacterial hosts or hide quietly inside them. That quiet phase is called dormancy. While dormant, the virus does not kill the host. Instead, it lives silently within the bacterial DNA.



Researchers have long wondered how <a href="https://www.earth.com/news/bacteria-pseudomonas-build-tiny-nano-spearguns-to-fight-back-against-attack/" target="_blank" rel="noreferrer noopener">bacteria</a> survive the first wave of viral infection, especially from these temperate phages. The answer may lie in how bacteria collect and store genetic fragments from dormant viruses. 



This behavior is not just survival; it's preparation for the future.



<h2 class="wp-block-heading" id="h-biological-memory-of-viruses">Biological memory of viruses</h2>



In the Johns Hopkins study, researchers focused on Streptococcus pyogenes, the bacteria responsible for strep throat. They found that these bacteria take advantage of temperate phages during their inactive phase. 



The bacteria gather genetic information from the phage while it’s dormant. This material forms a biological “memory” of the invader.



As the bacteria multiply, they pass this memory on. That means future generations are born with a built-in recognition system. When the same phage attacks again, the <a href="https://www.earth.com/news/bacteria-pseudomonas-build-tiny-nano-spearguns-to-fight-back-against-attack/" target="_blank" rel="noreferrer noopener">bacterial descendants</a> already know how to defend themselves.



“We essentially wanted to answer the question: If bacterial cells don’t have any memory, or survival skills, to combat a new temperate phage that shows up, how do they buy themselves enough time to establish a new memory, before they succumb to that initial infection?” said Modell.



<h2 class="wp-block-heading" id="h-bacteria-use-crispr-to-store-viral-memory">Bacteria use CRISPR to store viral memory</h2>



Bacteria use the CRISPR-Cas system to deal with phages. This system stores DNA from previous infections. When a known phage tries to re-enter, CRISPR recognizes its genetic material and destroys it.



Johns Hopkins researchers infected <a href="https://www.earth.com/news/bacteria-and-imprint-new-era-dna-transformation/" target="_blank" rel="noreferrer noopener">bacterial cells</a> with both natural phages that go dormant and genetically modified phages that stay active. They wanted to see how the CRISPR system responded under both conditions.



“Our results indicate that the bacteria’s CRISPR system was more effective at using the naturally dormant phage to pull parts of the viral genetic code into their genome,” said Modell. “When we tested phages that could not go dormant, the CRISPR system did not work nearly as well.”



<h2 class="wp-block-heading" id="h-dormant-viruses-boost-bacteria-memory">Dormant viruses boost bacteria memory</h2>



When phages go dormant, bacteria have more time. They use this period to build memory and prepare defenses. Researchers then allowed the surviving bacteria to multiply. They sequenced the DNA of these new generations.



The results were striking. The bacteria had collected hundreds of thousands of genetic “memories.” Each entry in the CRISPR system reflected past encounters with the virus. This memory-building happened mostly during dormancy, when the virus posed no immediate threat.



“This is conceptually similar to a vaccine with an attenuated virus,” said Nicholas Keith, a graduate student and first author of the paper.



“We believe this is the reason why the CRISPR Cas9 system has a unique <a href="https://www.earth.com/news/hungry-bacteria-will-devour-plastic-waste/" target="_blank" rel="noreferrer noopener">relationship</a> with this specific class of temperate phage.”



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



Vaccines train human immune systems by introducing harmless versions of dangerous viruses. The CRISPR system appears to do something similar. Dormant phages act like training tools, helping bacteria prepare without putting their survival at risk.



“We can use these types of experiments to find what elements of the phage, the bacterial host and its CRISPR system are important for all stages of bacterial immunity,” explained Keith.



Researchers are especially interested in why the system works better with dormant viruses than with active ones. This information could shape how scientists use phages to treat bacterial infections in humans.



<h2 class="wp-block-heading" id="h-future-treatments-and-fighting-resistance">Future treatments and fighting resistance</h2>



Antibiotic resistance is a growing problem. Some bacterial infections no longer respond to any known drugs. Phage therapy - using viruses to attack <a href="https://www.earth.com/news/how-bacteria-share-genes-and-defy-defenses/" target="_blank" rel="noreferrer noopener">bacteria</a> - is one potential solution. But this approach only works if we understand how bacteria defend themselves.



“We know CRISPR systems are one of the first lines of defense against the transfer of hazardous genes from phages that turn bacterial cells toxic. Furthermore, our studies will inform the design of ‘phage therapies’ which could be used in clinical cases where a bacterial infection is resistant to all available antibiotics,” noted Modell.



Understanding CRISPR could help scientists fine-tune phage therapies. They could choose or design viruses that bacteria are less able to resist, leading to more effective treatments.



<h2 class="wp-block-heading" id="h-a-collaborative-effort">A collaborative effort</h2>



​The research was supported by multiple institutions, including the&nbsp;<a href="https://www.hopkinsmedicine.org/som/" target="_blank" rel="noreferrer noopener">Johns Hopkins University School of Medicine</a>, the&nbsp;<a href="https://www.nih.gov/" target="_blank" rel="noreferrer noopener">National Institutes of Health</a>, the&nbsp;<a href="https://ritaallen.org/" target="_blank" rel="noreferrer noopener">Rita Allen Foundation</a>, and the&nbsp;<a href="https://www.nsf.gov/" target="_blank" rel="noreferrer noopener">National Science Foundation</a>.​



In addition to Nicholas Keith and Joshua Modell, the team included Rhett Snyder from Johns Hopkins and Chad Euler from <a href="https://hunter.cuny.edu" target="_blank" rel="noreferrer noopener">Hunter College</a>. Their combined efforts push us closer to smarter, safer ways of managing infections that resist current drugs.



In the end, studying bacteria doesn’t just teach us about microbes. It shows us new paths to protect ourselves, using lessons written in the smallest pieces of life.



The study is published in the journal <a href="https://www.cell.com/cell-host-microbe/fulltext/S1931-3128(25)00029-0" target="_blank" rel="noreferrer noopener">Cell Host &amp; Microbe</a>.



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Bacteria pass down their memories to fight viruses

In the invisible war between life forms, bacteria constantly fight...

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...

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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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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Close-up of dangerous horned viper in the sahara Photo Credit: acceptphoto

Horned Viper

A Tarantula Spider a wild native of the Sonoran Desert. This large brown spider was seen on the Pima Canyon trail in the Catalina Mountains north of Tucson, Arizona. Photo Credit: Charles T Peden

Horned Viper

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