Today's Image of the Day from the <a href="https://www.eso.org/public/">European Southern Observatory</a> (ESO) features a stunning view of the Sculptor Galaxy, one of the brightest spiral galaxies visible from Earth.



The ultra-detailed image, which was captured using ESO’s Very Large Telescope, reveals features in the Sculptor Galaxy that have never been seen before.&nbsp;



ESO researcher Enrico Congiu led a new study on the Sculptor Galaxy that is published in the journal Astronomy &amp; Astrophysics.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-wide-view-of-sculptor-nbsp">A galaxy-wide view of Sculptor&nbsp;</h2>



The team observed the galaxy in thousands of wavelengths at once, collecting an immense amount of data from every point across its structure. This allowed them to build a comprehensive, galaxy-wide view of how <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/">stars</a> live and evolve within Sculptor.



"Galaxies are incredibly complex systems that we are still struggling to understand," said Congiu.



“The Sculptor Galaxy is in a sweet spot. It is close enough that we can resolve its internal structure and study its building blocks with incredible detail, but at the same time, big enough that we can still see it as a whole system.”



<h2 class="wp-block-heading" id="h-thousands-of-distinct-colors-nbsp">Thousands of distinct colors&nbsp;</h2>



<a href="https://www.earth.com/news/oxygen-detected-in-the-most-distant-and-primitive-galaxy-ever-analyzed/">Galaxies</a> span hundreds of thousands of light-years, yet their evolution is shaped by processes unfolding on much smaller scales.&nbsp;



The fundamental components of a galaxy - stars, gas, and dust - each emit light in distinct colors. The more shades of color captured in an image, the deeper the insight into a galaxy’s internal structure.&nbsp;



Traditional images typically contain only a few colors, but the new map of the Sculptor Galaxy includes thousands.&nbsp;



This rich spectrum provides astronomers with detailed information about the galaxy’s stars, gas, and dust - from their ages and chemical makeup to how they’re moving through space.



<h2 class="wp-block-heading" id="h-mapping-the-sculptor-galaxy-nbsp">Mapping the Sculptor Galaxy&nbsp;</h2>



The research team spent more than 50 hours observing the Sculptor Galaxy using the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope.&nbsp;



To capture the full view - spanning roughly 65,000 light-years - they combined over 100 separate exposures into a single, detailed mosaic.&nbsp;



According to study co-author Kathryn Kreckel from Heidelberg University, Germany, this makes the map a potent tool.&nbsp;



“We can zoom in to study individual regions where stars form at nearly the scale of individual stars, but we can also zoom out to study the galaxy as a whole,” said Kreckel.&nbsp;



<h2 class="wp-block-heading" id="h-hundreds-of-planetary-nebulae-nbsp">Hundreds of planetary nebulae&nbsp;</h2>



In their initial analysis of the data, the team identified around 500 planetary <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/">nebulae</a> scattered throughout the Sculptor Galaxy.



Study co-author Fabian Scheuermann, a doctoral student at Heidelberg University, emphasized the significance of the discovery.&nbsp;



Scheuermann noted that when astronomers study galaxies outside of our own cosmic neighborhood, they normally detect fewer than 100 planetary nebulae in each one.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-of-extremes">A galaxy of extremes</h2>



The Sculptor Galaxy, also known as NGC 253, is located about 11.4 million light-years away in the constellation Sculptor. It’s classified as a starburst galaxy, meaning it’s undergoing an exceptionally high rate of <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/">star formation</a>.&nbsp;



This vigorous star-making activity is especially intense in its central regions, where dense clouds of gas and dust feed the birth of new stars.&nbsp;



The galaxy is tilted at a steep angle from our perspective, which gives it a striking, elongated appearance when viewed through telescopes.



<h2 class="wp-block-heading" id="h-notable-features-of-the-sculptor-galaxy-nbsp">Notable features of the Sculptor Galaxy&nbsp;</h2>



Discovered in 1783 by Caroline Herschel, the Sculptor Galaxy has become a popular target for both professional astronomers and amateur skywatchers due to its brightness and relative proximity.&nbsp;



It’s part of the Sculptor Group, one of the nearest groups of galaxies to our Local Group. Despite being rich in star-forming regions, much of its inner structure is veiled by thick dust lanes.&nbsp;



However, infrared and X-ray observations have helped scientists peer through the obscuring material to study the galaxy’s core, revealing a wealth of activity including supernova remnants and a possible central <a href="https://www.earth.com/news/largest-ultramassive-black-hole-ever-seen-cosmic-horseshoe-lrg-3-757/">black hole</a>.



The Sculptor Galaxy is also notable for its extended halo of stars and gas, which suggests past interactions or mergers with smaller galaxies.&nbsp;



This halo, along with its active central region, makes NGC 253 a valuable subject for understanding how galaxies evolve, form stars, and recycle gas over time. Its combination of beauty and scientific richness continues to make it a focus of galactic studies.



Image Credit: European Southern Observatory&nbsp;



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Thousands of colors in the Sculptor Galaxy

Today's Image of the Day from the European Southern Observatory...

Today's Image of the Day from the European Space Agency features Messier 82, a starburst galaxy located in the constellation Ursa Major. This galaxy is actively forming new stars at a rate ten times that of the Milky Way.



In a study using the <a href="https://webb.nasa.gov/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> (JWST), an international team of astronomers has taken an unprecedented look at Messier 82 (M82), revealing intricate details about its frenzied star formation.&nbsp;



<h2 class="wp-block-heading" id="h-the-power-of-nircam">The power of NIRCam</h2>



The study, led by Alberto Bolatto, utilized Webb’s Near-Infrared Camera (NIRCam) to penetrate the thick dust and gas covering the galaxy's core, a region critical to understanding <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>.&nbsp;



"M82 has garnered a variety of observations over the years because it can be considered as the prototypical starburst galaxy," noted Bolatto. “With Webb’s size and resolution, we can look at this star-forming galaxy and see all of this beautiful new detail.”



Webb's NIRCam has proven crucial for observing areas like M82’s center, where layers of dust typically obscure the view in other wavelengths. The camera's ability to capture infrared light allows it to reveal the galaxy's core and its dynamic processes.&nbsp;



<h2 class="wp-block-heading" id="h-messier-82-image">Messier 82 image </h2>



“This image shows the power of Webb. Every single white dot in this image is either a star or a star cluster. We can start to distinguish all of these tiny point sources, which enables us to acquire an accurate count of all the star clusters in this galaxy,” noted study co-author Rebecca Levy from the University of Arizona.



One of the NIRCam's innovative features is its mode that prevents bright sources from overwhelming the detector, which was particularly useful in studying the intensely active center of Messier 82.&nbsp;



In the image, dark brown tendrils of dust weave through the galaxy's glowing white core, interspersed with small green specks that represent concentrated areas of iron from <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> remnants. Red patches highlight regions where molecular hydrogen is illuminated by the radiation from nearby young stars.



<h2 class="wp-block-heading" id="h-insights-into-galactic-winds">Insights into galactic winds</h2>



The study also focused on understanding how <a href="https://www.earth.com/news/spin-of-a-new-black-hole-is-unlocking-galactic-mysteries/" target="_blank" rel="noreferrer noopener">galactic wind</a>, driven by the rapid rate of star formation and subsequent supernovae, influences M82’s environment. 



The NIRCam images showed clumpy streams of gas, appearing in red, which extend above and below the galaxy's plane, marking the path of this wind rushing out from the starburst's core.



A key revelation came from the NIRCam’s tracing of polycyclic aromatic hydrocarbons (PAHs), sooty chemical molecules that map out the structure of the galactic wind. 



To the surprise of researchers, the PAH emissions closely resembled the patterns of the hot, ionized gas, suggesting a more complex interaction within the wind than previously understood. 



"It was unexpected to see the PAH emission resemble ionised gas," said Bolatto. "PAHs are not supposed to live very long when exposed to such a strong radiation field, so perhaps they are being replenished all the time. It challenges our theories and shows us that further investigation is required."



<h2 class="wp-block-heading" id="h-future-observations-of-messier-82">Future observations of Messier 82</h2>



The findings from Webb are just the beginning. The team plans to further analyze Messier 82 with additional data, including spectroscopic observations, to determine the ages of the <a href="https://www.earth.com/news/galaxy-collisions-hubble-spots-a-string-of-pearls-star-cluster/" target="_blank" rel="noreferrer noopener">star clusters</a> and the duration of each star formation phase within the starburst environment.&nbsp;



These observations will also assist in a broader understanding of similar processes in early <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a>, which were common in the young universe.



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



Study co-author Torsten Böker of the <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a> emphasized the broader implications of these findings.&nbsp;



“With these amazing Webb images, and our upcoming spectra, we can study how exactly the strong winds and shock fronts from young stars and supernovae can remove the very gas and dust from which new stars are forming,” explained Böker.&nbsp;



“A detailed understanding of this ‘feedback’ cycle is important for theories of how the early universe evolved, because compact starbursts such as the one in M82 were very common at high redshift.”



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



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Messier 82: Unlocking the mysteries of star formation

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

Today's Image of the Day from NASA Earth Observatory features a blanket of dust over the Tarim Basin - a vast, arid region in northwestern China. 



Mountain peaks are visible through a break in the dust. These peaks are part of Tekilik Shan, a subrange of the Kunlun Mountains.



Though not as widely known as some other mountain ranges in the area, Tekilik Shan plays a significant role in shaping local <a href="https://www.earth.com/news/extreme-weather-is-pushing-nature-toward-a-breaking-point/" target="_blank" rel="noreferrer noopener">weather</a> patterns and geography.



Its snow-covered peaks can rise above 13,000 feet, contributing to the dramatic elevation differences that define the basin’s borders.



<h2 class="wp-block-heading" id="h-dust-storms-in-the-tarim-basin-nbsp">Dust storms in the Tarim Basin&nbsp;</h2>



Spring marks the height of <a href="https://www.earth.com/news/sahara-desert-dust-storms-carry-harmful-bacteria-and-fungi-around-the-globe/" target="_blank" rel="noreferrer noopener">dust storm</a> activity in the Tarim Basin, particularly in its southern region.&nbsp;



“It’s a time of year when regional wind patterns shift in ways that cause winds and storm systems to sweep in from the northwest,” noted <a href="https://earthobservatory.nasa.gov/images/154126/a-curtain-of-dust-over-the-tarim-basin" target="_blank" rel="noreferrer noopener">NASA</a>.



“In early spring, when landscapes in this region are especially dry and have minimal vegetation, land surfaces warm rapidly under the Sun’s heat every morning, fueling convection that can help loft dust upward by the afternoon.”



<h2 class="wp-block-heading" id="h-fingerlike-dust-formations-nbsp">Fingerlike dust formations&nbsp;</h2>



Satellite images revealed dust formations with fingerlike shapes that mirrored the landscape below. These projections aligned with valleys, which channeled and directed the airborne dust.&nbsp;



Ralph Kahn is an atmospheric scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder and scientist emeritus at NASA’s Goddard Space Flight Center.



According to Kahn, the dust may have been “self-lofting.” In this process, sunlight heats recently stirred-up surface dust, creating pockets of convection that lift it even higher into the air.



This interpretation is supported by hourly observations from Japan’s Himawari-9 geostationary satellite, which showed dust gradually rising into the Tekilik Shan throughout the day. By late afternoon, the storm had grown dense enough to obscure the mountains.&nbsp;



<h2 class="wp-block-heading" id="h-decline-in-atmospheric-dust">Decline in atmospheric dust</h2>



Long-term satellite data from MODIS suggest that <a href="https://www.earth.com/news/dust-storms-in-the-gulf-of-alaska-help-shape-the-global-climate/" target="_blank" rel="noreferrer noopener">atmospheric dust</a> levels in this region have declined by about 1.5 percent each year since the early 2000s.&nbsp;



NASA researcher Hongbin Yu attributes this trend mainly to springtime changes - such as altered wind speeds, <a href="https://www.earth.com/news/how-soil-moisture-can-predict-severe-storms/" target="_blank" rel="noreferrer noopener">soil moisture</a>, or vegetation cover - rather than shifts in other seasons.



<h2 class="wp-block-heading" id="h-rainfall-in-the-tarim-basin-nbsp">Rainfall in the Tarim Basin&nbsp;</h2>



“The <a href="https://www.britannica.com/place/Takla-Makan-Desert" target="_blank" rel="noreferrer noopener">Takla Makan Desert</a> is one of the driest, most barren expanses on Earth. Flanked by mountain ranges on three sides and parched by the resulting <a href="https://glossary.ametsoc.org/wiki/Rain_shadow" target="_blank" rel="noreferrer noopener">rain shadow</a>, parts of the Tarim Basin receive no more than 10 millimeters (0.4 inches) of rain per year,” noted NASA.



“Dust storms can lead to public health problems in populated areas downwind by transporting small particles, bacteria, and viruses that infiltrate human respiratory systems.”&nbsp;



NASA added that dust storms can also affect Earth’s climate by scattering and absorbing incoming solar radiation and changing the properties of clouds.



<h2 class="wp-block-heading" id="h-landscape-of-the-tarim-basin-nbsp">Landscape of the Tarim Basin&nbsp;</h2>



The Tarim Basin is one of the largest endorheic basins in the world, meaning that its rivers do not drain into the sea but instead flow into interior lakes or evaporate.&nbsp;



The basin is encircled by three mountain ranges: the Tien Shan to the north, the Kunlun Mountains to the south, and the Pamirs to the west. These ranges create a powerful rain shadow effect, making the region exceptionally dry.



At the heart of the Tarim Basin lies the Taklamakan Desert, one of the most extreme deserts on Earth. The desert is known for its high dunes, intense temperature swings, and minimal <a href="https://www.earth.com/news/extreme-rainfall-will-wreak-havoc-on-mountain-ranges-as-warming-climate-turns-snow-to-rain/" target="_blank" rel="noreferrer noopener">rainfall</a>.



<h2 class="wp-block-heading" id="h-history-and-geology">History and geology</h2>



Despite its harsh environment, the basin has been historically significant. It was a key section of the ancient Silk Road, with several oases such as Kashgar, Khotan, and Loulan serving as vital trading and cultural centers for centuries.



Geologically, the basin is rich in natural resources, particularly oil and natural gas, and has become a focal point for China's energy exploration and development.&nbsp;



The region’s challenging climate and remote location, however, make infrastructure development and human habitation difficult.&nbsp;



The image was captured on March 27, 2025 by the Operational Land Imager instrument on Landsat 8.



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Blanket of dust covers China’s Tarim Basin

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

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



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



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



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



Messier 78 is a dynamic region of star formation that is obscured by cosmic dust in this high-resolution image captured by the Euclid space telescope.



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



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



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



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



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



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



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



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



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



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



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> and interstellar matter.&nbsp;



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: European Space Agency&nbsp;



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Young stars shine through dense dust

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



By studying regions like NGC 604, astronomers can gain insights into the complex interactions between stars and the interstellar medium, as well as the conditions that lead to the birth of stars. This, in turn, helps in understanding the evolution of <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxies</a> and the universe as a whole.



<h2 class="wp-block-heading" id="h-massive-stars-of-ngc-604">Massive stars of NGC 604</h2>



"Sheltered among NGC 604’s dusty envelopes of gas are more than 200 of the hottest, most massive kinds of stars, all in the early stages of their lives," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"These types of stars are known as B-types and O-types, the latter of which can be more than 100 times the mass of our own Sun. It’s quite rare to find this concentration of them in the nearby universe. In fact, there’s no similar region within our own Milky Way galaxy."



According to ESA, this concentration of massive stars, combined with its relatively close distance, means that NGC 604 gives astronomers an opportunity to study these objects at a fascinating time early in their life.



<h2 class="wp-block-heading" id="h-gigantic-region-of-ionized-hydrogen">Gigantic region of ionized hydrogen</h2>



NGC 604 is one of the largest known regions of ionized hydrogen, also known as an H II region. This nebula is significantly larger than the Orion Nebula, which is one of the most well-known H II regions in our own <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way galaxy</a>.&nbsp;



NGC 604 spans about 1,500 light-years across, making it one of the largest H II regions in the Local Group of galaxies. This group includes the Milky Way, the Andromeda Galaxy, and about 54 other smaller galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-ngc-604-starburst-phenomenon">NGC 604 starburst phenomenon </h2>



Within NGC 604, there are hundreds of young, hot, massive <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">stars</a>. These stars have ionized the surrounding gas, causing it to glow and creating the nebula. The region is a prime example of a starburst phenomenon, where stars form at a much higher rate than in typical galactic conditions.



“The bright orange streaks in this image signify the presence of carbon-based molecules known as polycyclic aromatic hydrocarbons, or PAHs," explained ESA.



"As you travel further from the immediate cavities of dust where the star is forming, the deeper red signifies molecular hydrogen. This cooler gas is a prime environment for star formation. Ionized hydrogen from ultraviolet radiation appears as a white and blue ghostly glow."



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



Star formation is crucial for the evolution of galaxies and the synthesis of heavy elements. In the cores of stars, elements heavier than helium are created.



The elements are spread throughout the <a href="https://www.earth.com/news/ancient-stars-shakti-shiva-shaped-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">galaxy</a> when stars reach the end of their lives and expel their material - either gently through winds or violently via supernova explosions. 



This enriching process allows for the formation of new stars and planets, and ultimately, the potential for life.



<h3 class="wp-block-heading">Cloud collapse</h3>



The process begins when part of a molecular cloud becomes unstable and starts to collapse under its own gravity. This can be triggered by events like shock waves from nearby <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, galactic collisions, or the influence of other massive stars.



<h3 class="wp-block-heading">Formation of a protostar</h3>



As the cloud collapses, it fragments into smaller clumps. Each clump will eventually form one or more stars. 



The material within these clumps continues to fall inward, heating up as it does so, eventually forming a warm core called a protostar. At this stage, the protostar is not yet hot enough for nuclear fusion (the process that powers stars) to occur.



<h3 class="wp-block-heading">Accretion disk</h3>



Around the protostar, material from the surrounding cloud continues to fall inward, forming a rotating disk. This material slowly accretes onto the protostar, increasing its mass.



<h3 class="wp-block-heading">Nuclear fusion begins</h3>



Once the core of the protostar reaches a high enough temperature and pressure, hydrogen atoms begin to fuse into helium, releasing energy in the process. This marks the transition from a protostar to a main sequence star, like our sun.



<h3 class="wp-block-heading">Main sequence and beyond</h3>



The star will spend the majority of its life in the main sequence stage, where it balances the gravitational forces trying to collapse it and the outward pressure from nuclear fusion. 



Eventually, the star will exhaust its hydrogen fuel. Its subsequent evolution will depend on its initial mass, leading to various end stages such as red giants, supernovae, neutron stars, or black holes.



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



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Young, massive stars in the Triangulum Galaxy

Today's Image of the Day from the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba about 43 million light-years away from Earth.&nbsp;



This galaxy, discovered by British astronomer James Dunlop in 1826, is part of the larger NGC 1808 group of galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-intimate-view-of-ngc-1792">Intimate view of NGC 1792</h2>



“An orange glow radiates from the center of NGC 1792, the heart of this stellar forge. Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The vast swathes of tell-tale blue seen throughout the galaxy indicate areas that are full of young, hot stars, and it is in the shades of orange, seen nearer the center, that the older, cooler stars reside.”



<h2 class="wp-block-heading" id="h-vigorous-star-formation-nbsp">Vigorous star formation&nbsp;</h2>



NGC 1792 is notable for its vigorous star formation, classifying it as a starburst galaxy. The high rate of star birth is thought to be triggered by gravitational interactions with neighboring galaxies, though the exact cause is still under study.



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. 



“Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



<h2 class="wp-block-heading" id="h-fierce-bursts-of-star-formation">Fierce bursts of star formation</h2>



ESA noted that when galaxies have a large reservoir of gas, like NGC 1792, these short-lived starburst phases can be sparked by galactic events such as mergers and tidal interactions.&nbsp;



“One might think that these starburst galaxies would easily consume all of their gas in a large forming event. However, supernova explosions and intense stellar winds produced in these powerful starbursts can inject energy into the gas and disperse it.”&nbsp;



“This halts the star formation before it can completely deplete the galaxy of all its fuel. Scientists are actively working to understand this complex interplay between the dynamics that drive and quench these fierce bursts of star formation.”



Due to its distance and brightness, NGC 1792 can be observed with medium-sized telescopes under favorable conditions.



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



Galaxy evolution refers to the process by which galaxies form and change over time. It begins in the early universe, shortly after the <a href="https://www.earth.com/news/new-observations-disprove-big-bang-theory-universe-began-tired-light-theory/" target="_blank" rel="noreferrer noopener">Big Bang</a>, when small density fluctuations in the primordial gas led to the collapse of matter into the first galaxies.&nbsp;



<h3 class="wp-block-heading" id="h-galaxy-mergers">Galaxy mergers</h3>



Early galaxies were small and irregular, and were composed mostly of gas and dark matter. Over billions of years, galaxies grew larger by merging with one another and by accreting gas from the surrounding space.&nbsp;



These interactions often triggered bursts of star formation, and collisions between galaxies sometimes led to the creation of new, more massive galaxies.



<h3 class="wp-block-heading" id="h-structural-changes">Structural changes</h3>



As galaxies evolve, their morphology - shape and structure - can change. Early galaxies were often irregular or disk-shaped, but over time, many galaxies formed into the elliptical or spiral shapes we see today.&nbsp;



<h3 class="wp-block-heading" id="h-star-formation">Star formation</h3>



Star formation is a key driver of galaxy evolution, but it gradually slows down as galaxies age. 



The gas that fuels <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a> can be used up, or it can be heated and pushed out of galaxies by supernovae or black holes, reducing the galaxy's ability to form new stars.



<h3 class="wp-block-heading" id="h-galaxy-environment-nbsp">Galaxy environment&nbsp;</h3>



The environment in which a galaxy resides also plays a role in its evolution. Galaxies in dense clusters are more likely to interact with their neighbors, which can alter their shape or trigger bursts of star formation.&nbsp;



In contrast, galaxies in more isolated regions of space evolve more slowly and without as many dramatic interactions.



<h3 class="wp-block-heading" id="h-dark-matter">Dark matter</h3>



Dark matter also plays a crucial role in galaxy evolution. It provides the gravitational framework that holds galaxies together and influences their interactions with one another.&nbsp;



Supermassive <a href="https://www.earth.com/search-results/?search=Galaxies%20merge&amp;start=0" target="_blank" rel="noreferrer noopener">black holes</a>, found at the centers of most large galaxies, can also affect their evolution by releasing energy that impacts star formation and the movement of gas within the galaxy.



Overall, galaxy evolution is a complex and ongoing process driven by interactions between stars, gas, <a href="https://www.earth.com/news/study-dark-matter-does-not-exist-and-the-universe-is-27-billion-years-old/" target="_blank" rel="noreferrer noopener">dark matter</a>, and black holes, and shaped by both internal processes and external influences.



Image Credit: ESA/Hubble &amp; NASA, J. Lee



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Starburst galaxy in the constellation Columba

Diseño sin título - 1

The fossil of Ferruaspis brocksi lay unnoticed inside a small slab of rust‑colored rock from a newly discovered exceptional fossil site in central New South Wales, Australia until a curious researcher split the stone in early March. 



“It was a complete fluke,” exclaimed <a href="https://earthsciences.anu.edu.au/people/professor-jochen-j-brocks" target="_blank" rel="noreferrer noopener">Prof. Jochen Brocks</a> of the <a href="https://www.anu.edu.au/" target="_blank" rel="noreferrer noopener">Australian National University</a> after realizing what he had found. 



That single break exposed a two‑inch fish so complete that even its stomach contents and color cells were still visible.



During the <a href="https://ucmp.berkeley.edu/tertiary/miocene.php" target="_blank" rel="noreferrer noopener">Miocene epoch</a>, central New South Wales was covered by temperate rainforest and freshwater oxbow lakes rather than today’s dusty paddocks. 



The new species belongs to the <a href="https://www.inaturalist.org/taxa/49887-Osmeriformes" target="_blank" rel="noreferrer noopener">Osmeriformes order</a>, a group better known for modern graylings and smelts but never before recorded in Australia’s fossil record.



Researchers led by <a href="https://australian.museum/get-involved/staff-profiles/matthew-mccurry/" target="_blank" rel="noreferrer noopener">Dr. Matthew McCurry</a> at the Australian Museum and <a href="https://researchprofiles.canberra.edu.au/en/persons/michael-frese" target="_blank" rel="noreferrer noopener">Dr. Michael Frese</a> at the University of Canberra compared dozens of specimens ranging from 2.1 to 3 inches long, confirming a healthy resident population rather than scattered migrants.



<h2 class="wp-block-heading" id="h-rainforest-lake-that-turned-to-rust">Rainforest lake that turned to rust</h2>



The <a href="https://www.earth.com/news/fish-like-rainbow-trout-suffer-extreme-pain-when-killed-by-air/">fish</a> and many plants and insects were entombed in <a href="https://pubchem.ncbi.nlm.nih.gov/compound/Goethite" target="_blank" rel="noreferrer noopener">goethite</a>, an <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC3866414/" target="_blank" rel="noreferrer noopener">iron‑oxide</a> mineral that precipitated rapidly in the stagnant lake water. 



Iron’s ability to lock soft tissue in place is now recognized as a key factor in deep‑time preservation of cells and proteins. 



Geochemists <a href="https://www.sciencedirect.com/science/article/pii/S0012825223000569" target="_blank" rel="noreferrer noopener">note</a> that goethite’s fine crystals can replicate sub‑micron features before decay destroys the originals, explaining why pigment cells survived here while bones often did not.



McGraths Flat is classed as a <a href="https://www.cambridge.org/core/journals/paleobiology/article/abs/konservatlagerstatten-cause-and-classification/40A5D354B2DB79EFB6D654BC77421A33" target="_blank" rel="noreferrer noopener">Konservat‑Lagerstätte</a>, a sedimentary deposit famous for extraordinary detail, and its ferric layers sit just three feet below the surface near Gulgong. 



The discovery encourages field crews to re‑examine iron‑rich outcrops worldwide that were once dismissed as fossil‑poor.



<h2 class="wp-block-heading" id="h-fish-fossil-was-a-two-inch-hunter">Fish fossil was a two‑inch hunter</h2>



Under a scanning electron microscope, the team identified packed groups of <a href="https://www.nature.com/articles/ncomms1819" target="_blank" rel="noreferrer noopener">melanosomes</a> that once sat inside pigment cells called melanophores. 



Their distribution shows a dark back, pale belly, and two lateral racing stripes, classic countershading that helps living fish blend into sunlit water.



“It pushed the boundaries of what can be preserved,” noted Dr. Frese. Similar spherical and rod‑shaped melanosomes had been recorded earlier in an Eocene fish eye from Denmark, providing a useful comparison for the Australian material. 



The stripes also hint at schooling behavior, because bold horizontal bands are common in small modern smelts that rely on group camouflage.



<h2 class="wp-block-heading" id="h-what-a-final-snack-reveals">What a final snack reveals</h2>



Each fossil gut contained antennae from <a href="https://aslopubs.onlinelibrary.wiley.com/doi/pdf/10.4319/lo.1990.35.7.1631" target="_blank" rel="noreferrer noopener">Chaoborus larvae</a>, better known as phantom midge young, along with fragments of insect wings and an occasional bivalve shell. 



Modern Chaoborus sink into mud by day and rise at night to avoid fish, a strategy documented in laboratory and field studies.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/06/fossilized-fish-15-million-years-ago-last-meal-intact-stomach_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/06/fossilized-fish-15-million-years-ago-last-meal-intact-stomach_1s.webp" alt="Chromatophores and melanosomes in F. brocksi. Light microscopy photographs (A–F, AM F.155048) and scanning electron micrographs (G–L, AM F.146748). A, overview image showing the distribution pattern of melanophores in the fish’s skin. B–F, melanophores in the flank and the anal fin showing variation in size, form, and color. G–I, melanosomes in melanophores in an area of skin near the pectoral fin; single melanophore (G); edge of a single melanophore (H); center of a single melanophore (I). J–L, melanosomes in retinal pigment epithelial cells of the eye. Dashed lines mark areas that are depicted at higher magnifications in other panels. Credit: Australian National University" class="wp-image-1974319"/></a><figcaption class="wp-element-caption">Chromatophores and melanosomes in F. brocksi. Light microscopy photographs (A–F, AM F.155048) and scanning electron micrographs (G–L, AM F.146748). A, overview image showing the distribution pattern of melanophores in the fish’s skin. B–F, melanophores in the flank and the anal fin showing variation in size, form, and color. G–I, melanosomes in melanophores in an area of skin near the pectoral fin; single melanophore (G); edge of a single melanophore (H); center of a single melanophore (I). J–L, melanosomes in retinal pigment epithelial cells of the eye. Dashed lines mark areas that are depicted at higher magnifications in other panels. Click image to enlarge. Credit: Australian National University</figcaption></figure>



The heavy reliance on pelagic prey suggests F. brocksi hunted in open water after dusk rather than picking along the bottom. 



Because several size classes died together, scientists infer the lake provided year‑round habitat, unlike many living smelts that migrate between rivers and the sea.



<h2 class="wp-block-heading" id="h-a-parasite-hitchhiker">A parasite hitchhiker</h2>



One specimen shows a juvenile freshwater mussel, or glochidium, clamped to its tail fin. This is the oldest direct <a href="https://www.earth.com/news/why-some-animals-become-fossils-while-others-just-disappear/">fossil record</a> of such parasitism and implies the lake was periodically connected to a river where adult unionid mussels spawned.



Another <a href="https://www.earth.com/news/small-fish-provide-climate-resilient-nutrition-for-a-warming-world/">fish</a> swallowed a similar mussel, meaning it likely ventured near the river mouth shortly before dying. 



These clues help reconstruct seasonal flooding patterns in Miocene Australia without relying solely on sedimentology.



<h2 class="wp-block-heading" id="h-why-iron-fish-fossils-matter">Why iron fish fossils matter</h2>



Palaeontologist <a href="https://staffportal.curtin.edu.au/staff/profile/view/kate-trinajstic-f0dcf6b1/" target="_blank" rel="noreferrer noopener">Kate Trinajstic</a>, Curtin University, observed that iron deposits “open up a new area for people to investigate.” 



Her point is underscored by experimental decay work showing that early iron infiltration can arrest bacterial breakdown within days.



Goethite <a href="https://www.earth.com/news/fossil-euarthropod-youti-yuanshi-lived-520-million-years-ago-insect-evolution/">fossils</a> therefore extend the window for studying fragile tissues like eyes, muscles, and even viral particles that normally vanish. 



They also capture ecological interactions, predation, parasitism, pigmentation, that skeletons alone cannot.



<h2 class="wp-block-heading" id="h-rethinking-australia-s-fossil-record">Rethinking Australia's fossil record</h2>



The discovery of Ferruaspis brocksi challenges the long-held notion that Australia’s freshwater fish fossil record is too sparse for meaningful evolutionary study. 



Until now, no complete body fossils of <a href="https://www.sciencedirect.com/topics/agricultural-and-biological-sciences/osmeriformes" target="_blank" rel="noreferrer noopener">Osmeriformes</a> had been found on the continent, leaving major gaps in understanding their arrival and development.



With dozens of specimens at a single site, paleontologists now have a rare opportunity to study not just anatomy, but behavior, ecology, and population structure. 



This level of detail is nearly unheard of in Miocene freshwater <a href="https://www.earth.com/news/fish-are-quietly-battling-climate-change-on-the-seabed/">fish</a> fossils from the Southern Hemisphere.



The team’s phylogenetic analysis places F. brocksi near the base of the southern Osmeriformes radiation, pushing the group’s Australian arrival to at least 15 million years ago. 



That timeline aligns with molecular studies indicating a mid‑Miocene split between Australian and New Zealand graylings. Fieldwork will resume next dry season, targeting deeper layers that may hold older relatives or their predators.&nbsp;



The study is published in the <a href="https://www.tandfonline.com/doi/full/10.1080/02724634.2024.2445684" target="_blank" rel="noreferrer noopener">Journal of Vertebrate Paleontology</a>.



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Fossilized fish that lived 15 million years ago still has preserved food in its stomach

The fossil of Ferruaspis brocksi lay unnoticed inside a small...

New research reveals how the brain assigns emotional value to smells - and why it matters for health and happiness.



If you've ever recoiled from the smell of microwaved fish or smiled at the scent of fresh bread, you’ve experienced just how powerfully odors can stir emotions. But what makes our brains decide that a smell is pleasant - or downright awful?



A new study from researchers at the <a href="https://ufhealth.org/" target="_blank" rel="noreferrer noopener">University of Florida Health</a> reveals the neural pathways that give odors their emotional charge.



The findings provide the first detailed insight into how the brain categorizes smells as good or bad. This sheds light on why certain odors evoke such visceral reactions - and how that knowledge could eventually improve health outcomes.



<h2 class="wp-block-heading" id="h-smell-s-path-to-the-brain">Smell's path to the brain</h2>



Dan Wesson is senior author of the study and a professor of pharmacology and therapeutics. He's also the interim director of the <a href="https://fcs.institute.ufl.edu/" target="_blank" rel="noreferrer noopener">Florida Chemical Senses Institute</a>.



“Odors are powerful at driving <a href="https://www.earth.com/news/how-emotions-build-in-the-brain-and-why-they-linger/" target="_blank" rel="noreferrer noopener">emotions</a>," he said. "It’s long been thought that the sense of smell is just as powerful, if not more powerful, at driving an emotional response as a picture, a song, or any other sensory stimulus.” 



The research focused on the amygdala - the brain’s emotional command center - which interacts with all of our senses. It has especially close ties to smell. In fact, the olfactory system has a more direct route to the <a href="https://www.earth.com/news/lizard-brain-shapes-social-abilities-in-humans/" target="_blank" rel="noreferrer noopener">amygdala</a> than any other sense.



“This is, in part, what we mean when we say your sense of smell is your most emotional sense,” said first author Sarah Sniffen, a graduate research fellow.



“Yes, smells evoke strong, emotional memories, but the brain’s smell centers are more closely connected with emotional centers like the amygdala.”



<h2 class="wp-block-heading" id="h-good-vs-bad-smells">Good vs. bad smells</h2>



To understand how this connection works, researchers studied <a href="https://www.earth.com/news/mice-use-scent-to-determine-whos-the-boss/" target="_blank" rel="noreferrer noopener">mice</a> - animals whose brains share many neurochemical similarities with humans. Like us, mice can learn to associate smells with positive or negative experiences.



By analyzing the mice’s brain activity, the researchers identified two genetically distinct types of brain cells in the amygdala that play a key role in determining the emotional value of a smell.



Surprisingly, they found that both cell types could be involved in generating either positive or negative responses. It all depended on where those cells were sending signals.



“It can make an odor positive or negative to you,” Wesson said. “And it all depends upon where that cell type projects in your brain and how it engages with structures in your brain.”



In other words, the same type of <a href="https://www.earth.com/news/brain-cell-origins-traced-to-creatures-that-lived-800-million-years-ago/">brain cell</a> could contribute to opposite emotional outcomes depending on its connections.



<h2 class="wp-block-heading" id="h-odors-shape-daily-experience">Odors shape daily experience</h2>



Understanding smell responses may seem niche, but it has big implications - especially for those with heightened sensory sensitivity.



“We’re constantly breathing in and out and that means that we’re constantly receiving olfactory input,” Sniffen said.



“For some people that’s fine, and it doesn’t impact their day-to-day life. They might even think, ‘Oh, odors don’t matter that much.’ But for people who have a heightened response to sensory stimuli, like those with PTSD or <a href="https://www.earth.com/news/gut-microbes-have-an-unexpected-link-to-anxiety/" target="_blank" rel="noreferrer noopener">anxiety</a> or autism, it’s a really important factor for their day-to-day life.”



Scents associated with trauma, illness, or discomfort can trigger disproportionately strong responses in certain individuals. These reactions can sometimes interfere with routine activities or medical treatment.



Wesson noted how a patient’s negative association with the smell of a clinic - tied to previous transfusions - could cause intense distress.



<h2 class="wp-block-heading" id="h-future-scent-based-therapies">Future scent-based therapies</h2>



Understanding the specific brain circuits behind these reactions may open the door to targeted therapies. According to the researchers, it may one day be possible to modulate the activity of these odor-processing pathways with medications.



This could either dampen distressing responses or help restore emotional enjoyment in cases like appetite loss.



“Emotions in part dictate our quality of life, and we’re learning more about how they arise in our brain,” Wesson said. “Understanding more about how our surroundings can impact our feelings can help us become happier, healthier humans.”



By demystifying the deep link between scent and emotion, this research not only advances neuroscience - it also offers a potential path toward better mental and physical <a href="https://www.earth.com/news/world-environment-day-the-critical-role-of-nature-in-human-well-being/" target="_blank" rel="noreferrer noopener">well-being</a>.



The study is published in the journal <a href="https://www.nature.com/articles/s41380-025-03075-0" target="_blank" rel="noreferrer noopener">Nature: Molecular Psychiatry</a>.



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How your brain decides what smells good or bad

New research reveals how the brain assigns emotional value to...

Plants are far more adventurous underground than scientists once believed. A new study reports that many species extend a second, hidden network of roots more than a meter below the surface.



This discovery could ultimately reshape how researchers model nutrient cycling, water use, and the planet’s carbon budget.



Mingzhen Lu, an assistant professor in <a href="https://as.nyu.edu/departments/environment.html" target="_blank" rel="noreferrer noopener">New York University’s Department of Environmental Studies</a>, led this multi-institutional project.



“Understanding where plants grow roots is vital, as deeper roots could mean safer and longer-term carbon storage," she said. "Harsher conditions at depth may prevent detritus-feeding microbes from releasing carbon back to the atmosphere."



The findings suggest that plant roots may already be storing climate-warming carbon well below areas tracked by most ecological surveys.



<h2 class="wp-block-heading" id="h-data-goes-deeper">Data goes deeper</h2>



Traditional root research stops at roughly 30 centimeters, the depth that shovels and corers reach most easily.



Lu and her colleagues pushed past that limit by tapping into the <a href="https://www.neonscience.org/" target="_blank" rel="noreferrer noopener">National Ecological Observatory Network</a> (NEON), which collects samples down to two meters at dozens of U.S. sites.



From Alaskan tundra to Puerto Rican rainforest, the database provided thousands of soil cores reaching 6.5 feet - deep enough to chart root presence in realms seldom studied.



With those records in hand, the team set out to answer three intertwined questions: How does root density shift as soil gets deeper? Which environmental factors govern that distribution? And are subterranean nutrients being tapped as thoroughly as surface nutrients?



<h2 class="wp-block-heading" id="h-roots-defy-expectations">Roots defy expectations</h2>



The most eye-opening pattern was “bimodality.” Nearly one-fifth of the ecosystems examined showed two separate peaks in root abundance with depth: one in familiar shallow layers and another much farther down, often aligning with deposits of <a href="https://www.earth.com/news/nitrogen-was-plentiful-for-early-life-on-earth/" target="_blank" rel="noreferrer noopener">nitrogen</a>, phosphorus, or moisture.



In other words, plants were quietly plumbing secondary resource pockets, countering the long-held assumption that root activity simply dwindles the deeper one goes.



“The current understanding of roots is literally too shallow. Aboveground, we have eagle vision - thanks to satellites and remote sensing. But belowground, we have mole vision,” Lu said.



That “mole vision,” she argues, has left major gaps in Earth system models that guide climate policy and land-management decisions.



<h2 class="wp-block-heading" id="h-carbon-storage-or-carbon-release"><a></a>Carbon storage - or carbon release?</h2>



The presence of deep roots raises a crucial follow-up: What happens to the carbon that plants ferry into those depths? Avni Malhotra, a co-author and lead investigator on a <a href="https://www.biorxiv.org/content/10.1101/2025.04.07.647629v1" target="_blank" rel="noreferrer noopener">companion paper</a>, notes that outcomes could diverge.



“Deep plant roots may cause increased <a href="https://www.earth.com/news/organic-farming-practices-boost-soil-carbon-storage/" target="_blank" rel="noreferrer noopener">soil carbon storage</a> in one condition or lead to losses in other conditions due to a stimulation of soil microbes,” she said.



Cool, compacted subsoil tends to slow microbial digestion, potentially locking carbon away for centuries.



Yet in some settings, added root exudates might energize buried microbes, accelerating decomposition. Deciding which scenario dominates will require the kind of stratified sampling that NEON has only begun to provide.



<h2 class="wp-block-heading" id="h-deep-roots-defy-models">Deep roots defy models</h2>



Global climate models often assume that most biologically relevant actions - plant root growth, microbial decay, nutrient turnover - occur in the topsoil.



Lu’s study indicates that a significant share of plant activity, including carbon allocation, happens far below that zone.



If roots can chase nutrients downward during <a href="https://www.earth.com/news/droughts-and-extreme-weather-events-are-escalating/" target="_blank" rel="noreferrer noopener">droughts</a> or warming events, they may confer more resilience than current simulations capture. Conversely, land-use changes that compact or strip deep horizons could hamper an unseen but vital layer of carbon storage.



<h2 class="wp-block-heading" id="h-putting-root-data-to-work">Putting root data to work</h2>



These subterranean discoveries matter for forestry, agriculture, and conservation. Crop breeders might select varieties with deeper, bimodal rooting patterns to better capture water in arid regions.



Restoration ecologists could prioritize species that drive carbon into stable subsoil pools. 



Policymakers aiming to offset emissions through <a href="https://www.earth.com/news/reforestation-cannot-offset-carbon-emissions-from-harvesting-wood/" target="_blank" rel="noreferrer noopener">reforestation</a> or soil-carbon credits will need estimates grounded in full-profile measurements rather than the customary shallow cores.



<h2 class="wp-block-heading" id="h-plant-roots-store-climate-secrets">Plant roots store climate secrets</h2>



“Scientists and policymakers need to look deeper beneath the Earth’s surface as these overlooked deep soil layers may hold critical keys for understanding and managing ecosystems in a rapidly changing climate,” Lu said. The team envisions denser networks of deep cores, advanced imaging, and sensor arrays able to watch roots grow in real time.



While many unknowns remain - How universal is bimodality? Which soil chemistries foster it? How stable is deep-buried carbon? - the message is cautiously optimistic.



“The good news is plants may already be naturally mitigating climate change more actively than we’ve realized - we just need to dig deeper to fully understand their potential,” Lu concluded.



By illuminating a hidden architecture beneath our feet, the study invites scientists and citizens alike to rethink what lies between the surface and bedrock - and to recognize that the battle against rising CO2 might have powerful, unseen allies in the dark below.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-60055-2" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Plant roots could be key to fighting climate change

Plants are far more adventurous underground than scientists once believed....

Vultures cruising high above a savanna or hyenas crunching bones in the night are more than cinematic symbols of death - they are the planet’s front-line sanitation crew. By devouring carcasses quickly and completely, large scavengers deny dangerous microbes a foothold.



A wide-ranging study from <a href="https://www.stanford.edu/" target="_blank" rel="noreferrer noopener">Stanford University</a> shows that these underappreciated scavengers are declining at an alarming pace.



The work draws on population assessments for more than 1,300 vertebrate <a href="https://www.earth.com/news/scavengers-clean-up-wetlands-and-boost-their-health/" target="_blank" rel="noreferrer noopener">scavenger</a> species and reveals a worrisome pattern.



The steepest rates of scavenger decline were found among the biggest, most specialized carrion eaters, while adaptable opportunists such as rats and feral dogs surge in their absence.



“The evidence we found is very clear,” said senior author Rodolfo Dirzo, a professor of biology and environmental science at Stanford. "Scavengers are in decline, but it’s not homogeneous. It is particularly the large and specialized ones.”



“At the same time, this allows space for the smaller scavengers, which are problematic because they are themselves sources of zoonotic diseases.”



<h2 class="wp-block-heading" id="h-from-cleaners-to-contaminators">From cleaners to contaminators</h2>



The researchers cataloged everything from famous scavengers - Old World <a href="https://www.earth.com/news/vanishing-vultures-may-threaten-public-health/" target="_blank" rel="noreferrer noopener">vultures</a>, spotted hyenas, condors - to less obvious diners such as pond turtles, catfish, even great white sharks.



Cross-referencing each species against the <a href="https://www.iucnredlist.org/" target="_blank" rel="noreferrer noopener">International Union for Conservation of Nature’s Red List</a> and regional studies, they found that 36 percent of the world’s scavenger populations are threatened or already shrinking.



When those dominant consumers disappear, their ecological niche is rapidly filled by smaller generalists in a process ecologists label “ecological release.” In temperate suburbs, that might mean raccoons and crows; in tropical villages, perhaps <a href="https://www.earth.com/news/rats-are-spreading-a-deadly-disease-across-cities/" target="_blank" rel="noreferrer noopener">rats</a> and village dogs.



These newcomers rarely match the efficiency of an eagle or a vulture, leaving more rotting flesh on the landscape. Worse, many thrive near humans, turning carcasses into pathways for diseases to jump from wildlife to people.



<h2 class="wp-block-heading" id="h-effects-of-scavenger-decline-in-india">Effects of scavenger decline in India</h2>



Few episodes capture the stakes so vividly as India’s vulture crisis in the 1990s. Veterinary use of the anti-inflammatory drug diclofenac proved fatal to vultures that scavenged treated cattle. Populations plummeted, opening a niche for free-roaming dogs.



With vultures gone, feral dog populations surged, leading to an estimated 39 million extra dog bites and 48,000 human deaths from <a href="https://www.earth.com/news/rabies-is-spreading-among-marine-animals-for-the-first-time/" target="_blank" rel="noreferrer noopener">rabies</a> between 1992 and 2006.



Once India banned diclofenac in 2006, vulture numbers began to inch upward. This reminded scientists and policymakers that timely intervention can halt or even reverse a downward spiral.



<h2 class="wp-block-heading" id="h-scavengers-quietly-protect-health">Scavengers quietly protect health</h2>



The study emphasizes that these issues are not confined to the Global South. In the Greater Yellowstone Ecosystem of the United States, eagles and ravens consume elk carcasses and even aborted fetuses.



By removing potential bacterial incubators within hours, scavengers help curb brucellosis, a livestock disease that can spill over to ranchers. A drop in scavengers there could raise veterinary costs and public-health risks despite the region’s strong infrastructure.



Lead author Chinmay Sonawane, a doctoral student in Dirzo’s lab, underscored humanity’s reliance on species most of us rarely notice: “We’re starting to understand exactly how we depend on each individual species.”



“As we become more aware of these connections, we're going to be more inclined to protect these species, because we are ultimately protecting our health.”



<h2 class="wp-block-heading" id="h-factors-driving-scavenger-decline">Factors driving scavenger decline</h2>



Three forces repeatedly surfaced in the team’s analysis. Expanding agriculture and <a href="https://www.earth.com/news/urbanization-is-a-threat-to-78-of-the-worlds-bird-species/" target="_blank" rel="noreferrer noopener">urbanization</a> fragment habitats, making it harder for wide-ranging birds and mammals to find carcasses or safe nesting sites.



Intensive livestock production brings direct conflict when ranchers poison or shoot scavengers they suspect of killing calves. At the same time, wildlife trade and trophy hunting remove lions, eagles, and other predators that double as high-capacity scavengers.



These pressures often overlap. Clearing forest for pasture, for instance, strips vultures of roosting trees while putting them nearer cattle treated with toxic veterinary drugs.



<h2 class="wp-block-heading" id="h-ecosystem-function-and-human-well-being">Ecosystem function and human well-being </h2>



Public suspicion of scavengers compounds their plight. “There is this prejudice that these scavengers are nasty animals and that we should get rid of them, but they are important for the functioning of ecosystems, also for human well-being,” Dirzo said.



The authors call for multi-layered solutions. Conservationists must protect nesting cliffs and den sites and enforce tighter regulation of pharmaceuticals known to poison birds.



Outreach programs can dispel myths, showing local communities how vultures actually protect livestock by removing disease hotspots. Financial incentives or livestock-guarding measures could reduce retaliatory killings of <a href="https://www.earth.com/news/spotted-hyena-returns-to-egypt-after-5000-years/" target="_blank" rel="noreferrer noopener">hyenas</a> and jackals.



<h2 class="wp-block-heading" id="h-scavengers-are-public-health-allies">Scavengers are public health allies</h2>



Rather than tracking a handful of charismatic species, the Stanford team focused on a functional group - animals bound by what they do rather than by taxonomic labels.



That lens, they argue, reveals how losing one slice of biodiversity can disrupt entire healthcare networks in nature. If carcasses linger, fly populations balloon, dog packs expand, and viruses gain new hosts.



Scavengers may lack the appeal of pandas or coral reefs, yet their economic and public-health value is immense. The world’s oldest waste-management system runs on wings, paws, and powerful stomach acids.



Letting it collapse means footing a growing medical bill - one paid in outbreaks, veterinary losses, and human lives. Protecting vultures in India reduced rabies deaths; hyenas curb anthrax in Africa; condors help keep Americas’ pastures cleaner.



Ultimately, the study offers a simple equation: conserve the big eaters of the dead, and you safeguard the living. Ignore them, and the costs arrive on hospital ledgers and in destabilized ecosystems. The choice is clear - and action is urgently needed to halt scavenger decline. 



The study is published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2417328122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Scavenger decline is a threat to ecosystems  - and human health

Vultures cruising high above a savanna or hyenas crunching bones...

Woman,Hand,Holding,Pre-rolled,Cones,For,Smoking,Cannabis,With,Cannabis

Cannabis is everywhere now. It’s in pharmacies, parties, pain clinics, and political speeches. Many use it to sleep better, relax, or deal with pain. Some cannabis users even see it as a natural alternative to pills.



However, while the world embraced cannabis, heart doctors started noticing something else. A new study published in the journal Heart, based on data from over 432 million people, has revealed a clear <a href="https://www.earth.com/news/cannabis-extract-cbd-proven-highly-effective-at-killing-mosquitoes/">connection</a>. 



People who use cannabis have a much higher risk of heart attacks, strokes, and even dying from heart disease. That’s not fear-mongering - it’s data from .



<h2 class="wp-block-heading" id="h-more-people-are-using-stronger-cannabis">More people are using stronger cannabis </h2>



In over half of the states in the U.S., and in some countries in Europe, like France, doctors can give cannabis to patients as medicine, but using it just for fun is still illegal. 



Even though it's not allowed for fun, many young people in France still use it a lot. Germany recently changed its laws and now lets people use cannabis recreationally, starting in April 2024.



Now more people use cannabis, and the products they’re using are stronger than before. Today’s cannabis has more <a href="https://www.earth.com/news/scientists-reveal-the-most-complete-cannabis-genome-yet/">THC</a>. That means stronger effects on the brain and body - especially the heart.



<h2 class="wp-block-heading" id="h-cannabis-linked-to-heart-problems">Cannabis linked to heart problems</h2>



The researchers looked at 3,012 studies. Among them, 24 studies were focused on the link between cannabis and major heart problems.



An analysis of the research showed that people who use <a href="https://www.earth.com/news/cbd-reduces-the-unwanted-side-effects-of-thc/">cannabis</a> have a 29 percent higher risk of heart attack, a 20 percent higher risk of stroke, and more than double the risk of dying from heart disease.



<h2 class="wp-block-heading" id="h-regular-use-raises-stroke-risk">Regular use raises stroke risk</h2>



Stroke risk didn’t look the same in every study. A few didn’t find strong links, especially in people who used cannabis once or twice. But when the researchers zoomed in on heavy users or younger adults, the risk became clearer.



In Australia, one study found that people who used <a href="https://www.earth.com/news/cannabis-use-in-any-form-directly-linked-to-significant-risk-of-heart-damage/">cannabis</a> weekly were nearly five times more likely to suffer a stroke or mini-stroke. A U.S. hospital database also found increased risk, especially in people aged 25 to 34.



These results suggest that occasional cannabis use may not be a red flag. But regular use, especially while young, is when things start looking risky.



<h2 class="wp-block-heading" id="h-cannabis-linked-to-more-heart-attacks">Cannabis linked to more heart attacks</h2>



One study showed that cannabis users aged 15 to 22 were 36 percent more likely to have a heart attack. Another found that people using cannabis <a href="https://www.earth.com/news/cannabis-use-directly-linked-to-head-and-neck-cancer/">more than once a week</a> had more than double the odds.



That’s after adjusting for tobacco, cocaine, and other drugs. Cannabis came out as the strongest predictor in a French hospital study - even stronger than <a href="https://www.earth.com/news/how-cocaine-tricks-and-hijacks-the-brain/">cocaine</a>.



That’s not the story we usually hear about cannabis. But these numbers speak louder than opinions.



<h2 class="wp-block-heading" id="h-higher-death-risk-from-heart-disease">Higher death risk from heart disease</h2>



The risk of fatal cardiovascular events was also investigated. In one study, young patients who had heart attacks and also used cannabis were far more likely to die. The link remained consistent even after controlling for smoking and other conditions.



Another study conducted in the United States confirmed that cannabis users had a much higher chance of dying from heart-related causes. 



In the UK, a 2024 study revealed an unexpected twist. Women, not men, faced higher risks of heart-related death from heavy cannabis use.



<h2 class="wp-block-heading" id="h-what-about-the-benefits-of-cannabis">What about the benefits of cannabis?</h2>



Cannabis has shown several proven medical benefits, especially when used under a doctor’s guidance. One of its most recognized uses is for managing chronic pain. 



People with conditions like arthritis, multiple sclerosis, or nerve-related injuries often find relief through cannabis-based treatments. 



The plant's compounds - mainly THC and <a href="https://www.earth.com/news/cannabis-extract-cbd-proven-highly-effective-at-killing-mosquitoes/">CBD</a> - can interact with the body’s endocannabinoid system to reduce pain signals and inflammation. 



Medical cannabis also <a href="https://www.earth.com/news/cannabis-may-ease-cancer-symptoms-like-pain-and-nausea/">helps cancer patients</a> by easing nausea and vomiting caused by chemotherapy, and in some cases, it can stimulate appetite for those struggling with weight loss due to illness.



Doctors have also used cannabis to help patients with neurological disorders. In certain forms of epilepsy, especially in children, CBD-based medications have reduced the number and severity of seizures.



These examples reflect how cannabis, when used appropriately, can provide real and sometimes life-changing benefits for patients, making it easier for some to ignore the overall health implications attached to cannabis use.



<h2 class="wp-block-heading" id="h-experts-urge-tobacco-style-warnings">Experts urge tobacco-style warnings</h2>



“Cannabis needs to be incorporated into the framework for prevention of clinical cardiovascular disease. So too must cardiovascular disease prevention be incorporated into the regulation of cannabis markets,” noted Professor Stanton Glantz and Dr. Lynn Silver.



The experts emphasized that today's cannabis is not what it used to be. It now includes potent concentrates, synthetic versions, and a growing variety of edible and inhalable forms. These may carry risks beyond the cannabinoids themselves.



“How these changes affect cardiovascular risk requires clarification, as does the proportion of risk attributable to cannabinoids themselves versus particulate matter, terpenes or other components of the exposure,” the authors noted.



“Specifically, cannabis should be treated like tobacco: not criminalized, but discouraged, with protection of bystanders from secondhand exposure.”



Doctors should ask about cannabis use, particularly when it comes to patients with heart problems. For people using cannabis regularly, it’s time to rethink the idea that it is harmless.



The study is published in the journal <a href="https://heart.bmj.com/content/early/2025/06/10/heartjnl-2024-325429" target="_blank" rel="noreferrer noopener">Heart</a>.



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Cannabis is worse for heart health than cocaine, according to a startling new study

Cannabis is everywhere now. It’s in pharmacies, parties, pain clinics,...

Atom,Anatomy,,Atomic,Model,Or,Structure,,,Electrons,Orbiting,The

Physicists have been searching for ways to link photons and local quantum bits in a single system. One approach that uses quantum dots is particularly appealing. By carefully steering atomic nuclear spins, researchers have found a way to store and retrieve quantum information without sacrificing stability or flexibility.



Recent experiments with <a href="https://www.sciencedirect.com/topics/materials-science/gallium-arsenide" target="_blank" rel="noreferrer noopener">gallium arsenide</a> quantum dots revealed a technique where 13,000 entangled nuclear spins cooperated to form a robust “dark state.” 



This effort was led by <a href="https://www.phy.cam.ac.uk/profile/prof-mete-atature/" target="_blank" rel="noreferrer noopener">Mete Atatüre</a> from the <a href="https://www.phy.cam.ac.uk/" target="_blank" rel="noreferrer noopener">Cavendish Laboratory at the University of Cambridge</a>, working with colleagues at the University of Linz and other partners. 



Together, they have shown how quantum dots can form multi-qubit nodes for advanced communication and computing.



<h2 class="wp-block-heading" id="h-understanding-quantum-nodes">Understanding quantum nodes</h2>



<a href="https://www.nist.gov/pml/productsservices/quantum-networks-nist/connecting-quantum-network-nodes" target="_blank" rel="noreferrer noopener">Quantum networks</a> rely on nodes that can send <a href="https://www.energy.gov/science/doe-explainsphotons" target="_blank" rel="noreferrer noopener">photons</a> and also keep data in local storage. While current systems handle one piece or two of quantum data at a time, new experiments need multiple qubits in each node.



 The community has tested many platforms, but the search for something reliable and user-friendly continues.



The focus turned to <a href="https://www.earth.com/news/scientists-discover-previously-unknown-properties-of-a-very-unusual-metal-gallium/" target="_blank" rel="noreferrer noopener">gallium arsenide</a> quantum dots, which had been criticized for nuclear spin noise. Engineers tried taming those nuclear spins, since stable interactions among them could be repurposed for <a href="https://www.earth.com/news/scientific-surprise-as-turbulence-mixing-dynamics-captured-using-quantum-computing/" target="_blank" rel="noreferrer noopener">quantum data</a> storage. 



They discovered that even though there are thousands of interacting spins, meticulous driving of atomic states can align them into a unified register.



<h2 class="wp-block-heading" id="h-nuclear-spins-as-a-quantum-register">Nuclear spins as a quantum register</h2>



Many quantum dot designs include thousands of nuclei. When first examined, these spins behaved more like an unwanted background that muddied the electron spin signal. 



However, by applying methods inspired by <a href="https://www.cambridge.org/core/books/introduction-to-manybody-physics/B7598FC1FCEE0285F5EC767E835854C8" target="_blank" rel="noreferrer noopener">many-body physics</a>, the research team arranged a collective “dark state” of these nuclei.



The group stored <a href="https://iopscience.iop.org/article/10.1088/1742-6596/2809/1/012028/pdf" target="_blank" rel="noreferrer noopener">electron-based qubits</a> into the spin register, which retained that data reliably. They reported a storage fidelity of nearly 69% and a measured coherence time that exceeded 130 microseconds for certain operations. 



Those figures might seem modest, but they mark a leap in controlling nuclear spins inside a semiconductor device.



<h2 class="wp-block-heading" id="h-entangled-spins-and-the-dark-state">Entangled spins and the dark state</h2>



A dark state is a type of entangled arrangement that avoids regular environmental coupling. 



Because these 13,000 nuclear <a href="https://www.physik.uni-hamburg.de/en/inf/ag-wiesendanger/forschung/atomic-spin.html" target="_blank" rel="noreferrer noopener">spins settled</a> into that quiet configuration, less information was lost to external disturbances. Data could be written, stored, and retrieved without immediate decoherence.



“This breakthrough is a testament to the power many-body physics can have in transforming quantum devices,” said Mete Atatüre. 



By combining advanced feedback loops and carefully tuned magnetic fields, the team significantly improved the performance of <a href="https://www.sciencedirect.com/topics/materials-science/quantum-dot" target="_blank" rel="noreferrer noopener">quantum dots</a>. 



This demonstration highlights a new path for connecting various quantum components into larger systems.



<h2 class="wp-block-heading" id="h-nuclear-spins-and-quantum-communication">Nuclear spins and quantum communication</h2>



Devices that distribute <a href="https://www.earth.com/news/new-form-of-quantum-entanglement-discovered-will-transform-next-gen-technology/" target="_blank" rel="noreferrer noopener">entangled particles</a> over long distances need network nodes that can handle photon signals and keep data safe. 



Many attempts have aimed to achieve that by using <a href="https://www.nature.com/articles/s41467-024-51265-1" target="_blank" rel="noreferrer noopener">artificial atoms</a> that emit single photons. The gallium arsenide approach may accomplish this and provide a register of multiple nuclear spins for holding onto states as needed.



Quantum repeaters that send signals across hundreds of miles often stall because of photon losses in fiber. A <a href="https://news.mit.edu/2023/quantum-repeaters-use-defects-diamond-interconnect-quantum-systems-0927" target="_blank" rel="noreferrer noopener">quantum repeater</a> uses a memory unit as an intermediate station. 



This work points to gallium arsenide quantum dots as a practical candidate for such memory nodes, which could be placed between remote processors to enable secure communication protocols.



<h2 class="wp-block-heading" id="h-many-body-physics-and-dark-states">Many-body physics and dark states</h2>



The success of this experiment depends heavily on the principles of many-body physics, which studies how large numbers of interacting particles behave as a whole. 



Instead of treating each <a href="https://www.earth.com/news/nuclear-fusion-milestone-brings-clean-energy-closer-to-reality/">nuclear</a> spin as a separate bit, the researchers engineered a state where thousands of spins moved and responded collectively, something impossible to predict by simply summing up individual behaviors.



This approach allows scientists to tap into collective phenomena like <a href="https://www.earth.com/news/quantum-entanglement-a-simple-way-to-grasp-this-impossible-concept-carl-kocher/">entanglement</a>, <a href="https://www.anl.gov/article/what-is-quantum-coherence" target="_blank" rel="noreferrer noopener">coherence</a>, and <a href="https://www.cambridge.org/core/books/quantum-phase-transitions/33C1C81500346005E54C1DE4223E5562" target="_blank" rel="noreferrer noopener">quantum phase transition</a><a href="https://www.earth.com/news/quantum-phase-superradiant-phase-transition-srpt-observed-in-lab/">s</a>. 



The dark state formed in this experiment is a direct product of that cooperation. 



It gives the system new properties, such as resistance to certain types of noise, and opens the door to scalable designs that treat large atomic ensembles as single programmable units.



<h2 class="wp-block-heading" id="h-nuclear-spins-dark-states-and-the-future">Nuclear spins, dark states, and the future</h2>



The research team intends to extend the storage time by refining their spin-driving techniques. When combined with <a href="https://quantum.yale.edu/nuclear-magnetic-resonance-and-quantum-control" target="_blank" rel="noreferrer noopener">nuclear magnetic resonance controls</a>, some forecasts suggest storage times that may reach tens of milliseconds. 



If that goal is met, it could enable quantum dot setups to function as core parts of repeaters and distributed networks.



The challenge is to further reduce interference among different nuclear species within the dot. Reducing or eliminating isotopes that cause spectral overlap is one strategy.&nbsp;



Additional methods include applying more precise radio-frequency pulses to maintain coherence. 



Every improvement could raise the fidelity for data storage and retrieval, allowing quantum dots to compete with other leading platforms.



The study is published in <a href="https://www.nature.com/articles/s41567-024-02746-z" target="_blank" rel="noreferrer noopener">Nature Physics</a>.



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Physicists entangle 13,000 nuclear spins, unlocking the power of the 'dark state'

Physicists have been searching for ways to link photons and...

The Amazon Basin is no longer following its familiar seasonal rhythm. A new study shows that over the past four decades, the region’s wet months have grown markedly wetter, while its dry months are turning even drier.



The discovery comes from an unlikely archive: the annual growth <a href="https://www.earth.com/news/ancient-tree-rings-help-predict-extreme-solar-storms/" target="_blank" rel="noreferrer noopener">rings</a> of rainforest trees. Their chemistry records the isotopic “fingerprint” of rainwater year by year.



<h2 class="wp-block-heading" id="h-rings-that-remember-rain"><a></a>Rings that remember rain</h2>



Every downpour carries a distinct ratio of oxygen isotopes. Heavy rains flush lighter isotopes out of clouds first, enriching the water in heavier variants.



When a tree absorbs that moisture, the isotope mix becomes locked into its wood. By extracting pencils of core wood from trunks and reading those ratios, scientists can reconstruct past rainfall with month-by-month resolution.



For the new analysis, researchers sampled Cedrela odorata, a mahogany relative that grows on well-drained terra-firme soils, and Macrolobium acaciifolium, a species rooted in seasonally flooded forests.



Those complementary habitats allowed the team to profile both wet- and dry-season water inputs. Their isotope record spans 1980 to 2010.



The verdict is striking: wet-season rainfall in the Amazon has climbed between 15 and 22 percent, while dry-season rainfall has dropped by roughly 6 to 14 percent. The shift is large enough to affect river levels, forest physiology, and regional weather far beyond the Amazon.



<h2 class="wp-block-heading" id="h-oceans-influence-on-rainfall-patterns">Oceans’ influence on rainfall patterns</h2>



What is driving the divergence? The scientists point to changing sea-surface <a href="https://www.earth.com/news/ocean-temperatures-are-rising-faster-than-expected-and-likely-to-accelerate/" target="_blank" rel="noreferrer noopener">temperatures</a> in both the tropical Atlantic and Pacific. 



Warm anomalies in these oceans alter wind belts, convection, and therefore the intensity of rain systems that sweep across South America.



Some of that variability is natural, cycling over decades. But the authors warn that greenhouse warming is very likely amplifying the pattern.



“Our research demonstrates that the Amazon's hydrological cycle is becoming more extreme," said co-authors Roel Brienen and Emanuel Gloor from the <a href="https://www.leeds.ac.uk/" target="_blank" rel="noreferrer noopener">University of Leeds</a>.



"Increased wet season <a href="https://www.earth.com/news/rainfall-is-increasingly-unpredictable-due-to-climate-change/" target="_blank" rel="noreferrer noopener">rainfall</a> can lead to more frequent and severe flooding, while reduced dry season rainfall exacerbates drought conditions, impacting forest health and biodiversity.” 



<h2 class="wp-block-heading" id="h-seeing-deeper-than-standard-datasets"><a></a>Seeing deeper than standard datasets</h2>



Standard rainfall gauges and satellite products often underplay long-term trends because they cover limited areas or short periods. Isotope ratios aggregate the signal over large catchments, providing what the authors call a “basin-integrated” view.



“While traditional climate datasets may underestimate these changes, the tree ring isotope data offer a more integrated, large-scale perspective,” explained co-author Arnoud Boom of the <a href="https://le.ac.uk/" target="_blank" rel="noreferrer noopener">University of Leicester</a>.



By combining upland and floodplain samples, the team isolated changes unique to wet and dry months. That dual approach revealed a previously unrecognized “bimodality” in Amazon rainfall trends.



<h2 class="wp-block-heading" id="h-amazon-s-pulse-grows-more-erratic">Amazon’s pulse grows more erratic</h2>



Seasonal extremes bring real-world consequences. In wetter months, swollen rivers inundate low-lying towns, destroy crops, and erode banks. In drier months, the receding waters limit transport, concentrate pollutants, and leave isolated villages without reliable fish stocks.



The study's co-author is Jochen Schöngart of Brazil’s <a href="https://www.gov.br/inpa/pt-br" target="_blank" rel="noreferrer noopener">National Institute for Amazon Research</a> (INPA).



“These findings highlight that the Amazon is not simply drying or wetting overall but experiencing more extreme seasonal swings,” he said. 



“This is of relevant concern as the intensification of the <a href="https://www.earth.com/news/distress-signals-earths-water-cycle-is-becoming-more-erratic/" target="_blank" rel="noreferrer noopener">hydrological cycle</a> impacts the functioning of ecosystems, water, and food security of millions of traditional and indigenous people.”



<h2 class="wp-block-heading" id="h-changing-amazon-endangers-climate-future">Changing Amazon endangers climate future</h2>



The ramifications go far beyond local hardship. The Amazon acts as a giant <a href="https://www.earth.com/news/earths-carbon-sinks-are-being-pushed-to-their-limits/" target="_blank" rel="noreferrer noopener">carbon sink</a>. Longer and hotter dry seasons stress trees, raising mortality and potentially tipping the forest from absorbing CO2 to emitting it. 



More intense wet seasons, on the other hand, can destabilize soils and release <a href="https://www.earth.com/news/climate-extremes-will-boost-methane-emissions-in-the-amazon/" target="_blank" rel="noreferrer noopener">methane</a> from flooded areas.



“The Amazon is a key component of the Earth's climate system," said lead author Bruno Cintra, a scientist at the <a href="https://www.birmingham.ac.uk/" target="_blank" rel="noreferrer noopener">University of Birmingham</a>. "Understanding how its hydrological cycle is changing is essential for predicting future climate scenarios and developing effective conservation strategies.”



He points to the 2025 UN climate summit in Belém - COP30 - as “a critical opportunity for world leaders to take decisive action.”



<h2 class="wp-block-heading" id="h-tree-rings-reveal-rainfall-trends">Tree rings reveal rainfall trends</h2>



The researchers relied on the <a href="https://www.neonscience.org/" target="_blank" rel="noreferrer noopener">National Ecological Observatory Network</a>’s deep-coring archive to calibrate tree-ring isotopes against rain gauges, reanalysis grids, and atmospheric models.



Sensitivity tests confirmed that temperature or evaporation could not alone explain the isotope trends; rainfall changes in the Amazon were the dominant driver.



Although the record ends in 2010, satellite data suggest the divergence has persisted - and may have accelerated - in recent years. That makes the study a baseline for assessing how future warming, <a href="https://www.earth.com/news/global-deforestation-crisis-how-can-we-stop-massive-forest-losses/" target="_blank" rel="noreferrer noopener">deforestation</a>, and fires will interact with ocean-driven variability.



<h2 class="wp-block-heading" id="h-amazon-stability-demands-urgent-action">Amazon stability demands urgent action</h2>



Policy implications are clear: conserving intact forest buffers against drought by maintaining local moisture recycling, while curbing global emissions limits further ocean-atmosphere shifts.



The experts argue that accurate Amazon rainfall projections will require integrating deep tree-ring records with modern sensor networks.



“Urgent actions to mitigate climate change and simultaneously adapt the livelihood and traditional management of the populations are required,” Schöngart said.



The rings have spoken; the challenge now is to translate their warning into meaningful protection for the world’s largest rainforest - and the climate system it helps stabilize.



The study is published in the journal <a href="https://www.nature.com/articles/s43247-025-02408-9" target="_blank" rel="noreferrer noopener">Nature Communications Earth &amp; Environment</a>.



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Tree rings show Amazon rainfall is getting more extreme

The Amazon Basin is no longer following its familiar seasonal...

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.



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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

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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

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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

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

The local government had issued a warning to everyone in the area – which is why the beach wasn’t very busy that day.
It’s another example of why education and awareness are so important! Photo Credit: YouTube/Animal File Facts

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