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



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



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



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



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



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



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



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



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



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



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



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



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



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



At the core of the nebula, the primary star, now collapsing into a <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/" target="_blank" rel="noreferrer noopener">white dwarf</a>, reaches extreme temperatures. This heat is estimated to be 120,000 degrees Celsius - about 24 times hotter than the surface of our Sun.&nbsp;



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

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

Today's Image of the Day from NASA Earth Observatory features the remnants of Lake Razzaza, an artificial lake situated a few miles west of Karbala, Iraq.



The <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lake</a> was created in the late 1970s as a flood control measure to regulate the floodwaters of the Euphrates River. 



Razzaza covers an area of approximately 1,562 square kilometers and is located in a depression where excess water from Lake Habbaniyah is diverted through a controlled escape channel or canal.&nbsp;



<h2 class="wp-block-heading" id="h-the-colors-of-lake-razzaza">The colors of Lake Razzaza</h2>



“The lake, also known as Baḩr al-Milḩ (‘Sea of Salt’ in Arabic), is fed by overflow from Habbaniyah Lake, which lies just outside the top left corner of the image,” noted <a href="https://earthobservatory.nasa.gov/images/153756/iraqs-sea-of-salt" target="_blank" rel="noreferrer noopener">NASA</a>.



“The difference in water color results from the various communities of algae that thrive in the lake depending on the water temperature and salinity.”



“Green areas contain lower salt concentrations than red areas. At times when the lake receives no overflow from Habbaniyah Lake, as shown in this image, most of the lakebed is exposed.”



<h2 class="wp-block-heading" id="h-salinity-of-lake-razzaza">Salinity of Lake Razzaza</h2>



Over the years, the salinity of Lake Razzaza has been increasing due to inadequate water supply from the linked canal and high evaporation rates during Iraq's hot summers.&nbsp;



This rise in <a href="https://www.earth.com/news/salt-pollution-threatens-freshwater-ecosystems/" target="_blank" rel="noreferrer noopener">salinity</a> has led to a decline in fish populations, adversely affecting local fishermen who once relied on the lake for their livelihoods. 



By 2008, only the fish species locally known as "al-Shanik" (Acanthopagrus arabicus), of marine origin and stocked by the government, was reported to survive in the lake.&nbsp;



The lake's fluctuating water levels and increasing salinity have also impacted its recreational appeal, with few recreational areas existing around the lake.&nbsp;



Additionally, the surrounding desert landscape and low cliff shores contribute to its limited accessibility for leisure activities.&nbsp;



<h2 class="wp-block-heading" id="h-wildlife-of-lake-razzaza">Wildlife of Lake Razzaza</h2>



Despite these challenges, Lake Razzaza remains an important habitat for various bird species. It has been designated an Important Bird Area (IBA) by BirdLife International, supporting significant numbers of wintering waterfowl and serving as a breeding ground for species such as the marbled duck.&nbsp;



The lake's mudflats attract large numbers of waders and shorebirds during migration periods.&nbsp;



The surrounding area features vegetation such as Phragmites australis, Juncus acutus, Aeluropus lagopoides, Salicornia herbacea, and Schoenoplectus litoralis, along with desert shrublands including Tamarix aucherana, Prosopis farcta, and Haloxylon salicornicum.&nbsp;



Mammals reported in this region include Rüppell's fox, golden jackal, Indian grey mongoose, jungle cat, and wildcat.&nbsp;



In recent years, the <a href="https://www.earth.com/news/lakes-are-warming-toward-the-point-of-no-return/" target="_blank" rel="noreferrer noopener">lake</a> has faced environmental challenges due to reduced water inflows and increased evaporation, leading to higher salinity levels and a decline in biodiversity. 



Efforts to address these issues are essential to preserve the ecological and economic significance of Lake Razzaza.



<h2 class="wp-block-heading" id="h-the-euphrates-river-nbsp">The Euphrates River&nbsp;</h2>



The Euphrates River is one of the most significant rivers in the Middle East and holds immense historical, cultural, and ecological importance.&nbsp;



Stretching approximately 2,800 kilometers (1,740 miles), it originates in the mountains of eastern Turkey and flows through Syria and Iraq before merging with the Tigris River to form the Shatt al-Arab, which empties into the Persian Gulf.&nbsp;



The <a href="https://www.earth.com/news/major-plastic-pollution-lurks-beneath-the-surface-of-rivers/" target="_blank" rel="noreferrer noopener">river</a> has been a cradle of civilization for thousands of years, supporting ancient Mesopotamian societies, including Sumer, Akkad, Babylon, and Assyria.



The Euphrates has provided water for irrigation, enabling the development of agriculture in an otherwise arid region. Its floodplains have been vital for sustaining life and fostering the growth of cities along its course.&nbsp;



However, the river also plays a key geopolitical role, as disputes over water usage and dam construction among Turkey, Syria, and Iraq have emerged over the years, impacting water availability downstream.



Ecologically, the Euphrates supports a range of habitats, from wetlands to desert ecosystems, making it home to diverse flora and fauna.&nbsp;



However, modern challenges such as damming, pollution, and climate change threaten its flow and ecological balance. Despite these challenges, the Euphrates remains a symbol of life and resilience in the heart of the Middle East.



The image was captured by an astronaut on the International Space Station (ISS) on September 23, 2024.



Image Credit: NASA



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Lake Razzaza: A shrinking oasis shaped by salinity

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA



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NGC 2566: A cosmic eye in the Puppis constellation

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

Today's Image of the Day from the European Space Agency features the Cat's Eye Nebula (NGC 6543), located about 3,300 light-years from Earth in the constellation Draco.&nbsp;



The nebula's name comes from its eye-like appearance when viewed through a telescope. This particular image, which reveals the <a href="https://www.earth.com/news/horsehead-nebula-webb-telescope-captured-unprecedented-detail/" target="_blank" rel="noreferrer noopener">nebula</a> in stunning detail, was captured by the NASA/ESA Hubble Space Telescope.



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



According to ESA, the Cat's Eye Nebula is one of the most complex planetary nebulae that has ever been discovered.



“A planetary nebula forms when Sun-like stars gently eject their outer gaseous layers to form bright nebulae with amazing twisted shapes," explained <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Until recently, it was thought that shells around planetary nebulae were a rare phenomenon. However, astronomers have instead shown that these rings are likely to be the rule rather than the exception."



<h2 class="wp-block-heading" id="h-appearance-of-the-cat-s-eye-nebula-nbsp">Appearance of the Cat's Eye Nebula&nbsp;</h2>



The central focus of the Cat's Eye is a hot, dying star that has shed its outer layers to form the <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a>. It is surrounded by concentric gas shells, jets of high-speed gas, and unusual shock-induced knots of gas.



“Although the rings may be the key to explaining the final ‘gasp’ of the dying central star, the mystery behind the Cat’s Eye Nebula’s nested ‘Russian doll’ structure remains largely unsolved,” noted ESA.



<h2 class="wp-block-heading" id="h-rings-around-the-cat-s-eye">Rings around the Cat’s Eye</h2>



“This image, taken with Hubble's Advanced Camera for Surveys (ACS), reveals the full pattern of eleven or more concentric rings, or shells, around the Cat’s Eye. Each ‘ring’ is actually the edge of a spherical bubble seen projected onto the sky - which is why it appears bright along its outer edge.”



According to ESA, observations suggest that the star ejected its mass in a series of pulses at 1,500-year intervals. “These convulsions created dust shells that each contains as much mass as all of the planets in our solar system combined.”



Several explanations have been proposed for this phenomenon, including cycles of magnetic activity similar to our Sun's sunspot cycle, the influence of companion stars orbiting the <a href="https://www.earth.com/news/dying-stars-may-be-a-source-of-gravitational-waves/" target="_blank" rel="noreferrer noopener">dying star</a>, or stellar pulsations.&nbsp;



Another theory suggests that the material is ejected smoothly from the star, with the rings forming later due to the creation of waves in the outflowing material.



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



<a href="https://www.earth.com/news/extrasolar-ocean-planet-discovered-in-the-draco-constellation/" target="_blank" rel="noreferrer noopener">Draco</a> is a constellation in the northern sky that represents a dragon. It's one of the largest constellations, winding between the Big and Little Dippers.&nbsp;



In Greek mythology, Draco is often identified as the dragon Ladon, who guarded the golden apples in the garden of the Hesperides.



Draco is a circumpolar constellation for most northern hemisphere observers, meaning it never sets below the horizon and can be seen all year round.



<h2 class="wp-block-heading" id="h-famous-planetary-nebulae">Famous planetary nebulae </h2>



Planetary nebulae are some of the most beautiful and intriguing objects in the universe.&nbsp;



One of the most famous is the Ring Nebula, or M57, located in the constellation Lyra. This nebula is renowned for its nearly perfect ring shape, which is the result of a dying star shedding its outer layers.&nbsp;



Another well-known planetary nebula is the Helix Nebula, or NGC 7293, often referred to as the "Eye of God" due to its eye-like appearance. The Helix Nebula is one of the closest planetary nebulae to Earth, making it a popular target for amateur astronomers.&nbsp;



The Dumbbell Nebula, or M27, in the constellation Vulpecula, is another striking example. It is named for its resemblance to a dumbbell and is notable for being the first planetary nebula ever discovered, by Charles Messier in 1764.&nbsp;



The Butterfly Nebula, or NGC 6302, is located in the constellation Scorpius. Its name comes from its distinctive bipolar structure, resembling the wings of a butterfly. The nebula's central star is one of the hottest known, with a surface temperature of around 250,000 degrees Celsius.&nbsp;



The Eskimo Nebula, or NGC 2392, in the constellation Gemini, is known for its resemblance to a face surrounded by a fur parka, which gives it its name. Its intricate structure, including filaments and bubble-like shapes, makes it a fascinating object of study. 



These nebulae not only captivate us with their beauty but also provide valuable insights into the life cycles of stars and the processes that shape our galaxy.



Image Credit: NASA/ESA Hubble Space Telescope



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Cat's Eye Nebula in the constellation Draco

Today's Image of the Day from the European Space Agency features a Copernicus Sentinel-2 photograph of South Georgia, a remote and rugged island located in the southern Atlantic Ocean. 



"Linked with the South Sandwich Islands to form a British Overseas Territory, this southern Atlantic island is a haven for a vast array of wildlife," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Around five million seals call the islands home, as well as 65 million birds of 30 different species. Migrating whales and various fish species populate the surrounding waters and there is a large penguin population."



<h2 class="wp-block-heading" id="h-climate-and-wildlife-of-south-georgia">Climate and wildlife of South Georgia </h2>



The island is dominated by mountains, glaciers, and fjords. Its highest peak, Mount Paget, rises to 2,935 meters, making it one of the tallest in the region.



South Georgia’s location within the Antarctic Convergence gives it a cold, maritime climate. Although not part of the Antarctic Treaty System, its environment and <a href="https://www.earth.com/news/conservation-efforts-are-not-enough-to-save-antarctic-wildlife/" target="_blank" rel="noreferrer noopener">wildlife</a> are closely linked to Antarctica. 



The island is home to vast colonies of penguins, seals, and seabirds. The surrounding waters are rich with krill, providing an abundant food source for marine life.



<h2 class="wp-block-heading" id="h-penguins-adapted-to-harsh-environments">Penguins adapted to harsh environments </h2>



The most notable species found here are the king penguins, which are the second-largest penguin species in the world. South Georgia also hosts large populations of <a href="https://www.earth.com/news/what-makes-the-gentoo-penguin-the-worlds-fastest-swimming-bird/" target="_blank" rel="noreferrer noopener">gentoo</a> and macaroni penguins. 



The island's harsh climate, characterized by strong winds, snow, and cold temperatures, makes it a tough environment, but the penguins have adapted well. 



Their colonies - some of which number in the hundreds of thousands - can be found along the island's rugged coasts and beaches. 



The island’s isolation, combined with its plentiful food supply, makes it a critical breeding ground for these penguins.



<h2 class="wp-block-heading" id="h-history-of-south-georgia">History of South Georgia </h2>



The island has a history of exploration and exploitation. Captain James Cook first claimed South Georgia for Britain in 1775. 



During the late 19th and early 20th centuries, it became a hub for the <a href="https://www.earth.com/news/echoes-of-the-past-whalings-long-term-impact-on-genetic-diversity/" target="_blank" rel="noreferrer noopener">whaling</a> industry, with stations like Grytviken serving as operational centers. These stations have since been abandoned, and the island is now a haven for scientific research and ecotourism.



South Georgia is also notable for its role in Ernest Shackleton’s famed Endurance expedition. His crew reached the island in 1916 after an extraordinary open-boat journey from Elephant Island. Shackleton later died on South Georgia in 1922 and is buried in Grytviken.



<h2 class="wp-block-heading" id="h-pristine-nature-of-the-island">Pristine nature of the island</h2>



Today, South Georgia is a focus of conservation efforts. The eradication of invasive species, such as rats and reindeer, has been a significant success, allowing native wildlife to recover. 



Rats and mice were responsible for the decline of ground-nesting birds, including the South Georgia pipit, the island's only endemic bird. 



<a href="https://www.earth.com/news/reindeer-use-ultraviolet-vision-to-find-food-in-the-winter/" target="_blank" rel="noreferrer noopener">Reindeer</a>, which had been introduced for farming in the 19th century, caused extensive damage to the island’s vegetation, disrupting the habitat for native species.



South Georgia is uninhabited except for a small number of scientists and staff working at research stations and administrative facilities, emphasizing its role as a protected wilderness area and an essential site for understanding global environmental changes.



Its uninhabited status has helped preserve its pristine nature. Visitors to South Georgia must follow strict environmental guidelines to minimize human impact on this extraordinary island.



<h2 class="wp-block-heading" id="h-scientific-significance-of-remote-islands">Scientific significance of remote islands </h2>



Remote <a href="https://www.earth.com/news/plant-life-on-islands-loses-diversity-when-humans-arrive/" target="_blank" rel="noreferrer noopener">islands</a> are scientifically significant for several reasons. They often serve as unique ecosystems that can provide insights into evolutionary processes, biodiversity, and adaptation. 



Due to their isolation, species on remote islands may evolve differently from their mainland counterparts, resulting in the development of endemic species that exist nowhere else in the world. 



These islands also act as natural laboratories for studying the effects of climate change, human activity, and ecological interactions, as they are more vulnerable to disturbances. 



Moreover, remote islands can offer valuable information on the health of marine and terrestrial ecosystems, as their ecosystems are often less impacted by human-induced factors. This makes them ideal for studying natural processes in relatively undisturbed environments. 



The isolation of these islands can also help scientists study the patterns of species migration, colonization, and extinction.



Image Credit: ESA 



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South Georgia: One of the most remote islands in the world

Axial Seamount sits under the Pacific Ocean about 300 miles from the U.S. coast. Since 1997, scientists have kept a careful eye on it using instruments that measure pressure on the ocean floor. 



Data shows that the volcano has been swelling, with changing rates that hint at an upcoming eruption.



Its activity caught the attention of experts because it shows a pattern of erupting after reaching a particular level of inflation. 



Observers have noted that the volcano’s swelling slowed from 2015 to 2023, then sped up again in late 2023. By mid-2024, that rate hit 10 inches per year, while daily earthquakes soared into the hundreds.



Mark Zumberge, a geophysicist at <a href="https://scripps.ucsd.edu/" target="_blank" rel="noreferrer noopener">Scripps Institution of Oceanography</a>, has described it this way: “It’s the most well-instrumented submarine volcano on the planet.” 



He and others use pressure sensors and AI-driven analysis to gauge shifts in earthquake patterns. William Chadwick of <a href="https://oregonstate.edu/" target="_blank" rel="noreferrer noopener">Oregon State University</a> once referred to a 2015 eruption forecast as their “best forecasting success.”



<h2 class="wp-block-heading" id="h-where-continental-plates-pull-apart">Where continental plates pull apart</h2>



Axial Seamount rises from the <a href="https://www.usgs.gov/media/images/subduction-juan-de-fuca-plate-beneath-north-american-pla" target="_blank" rel="noreferrer noopener">Juan de Fuca Ridge</a>, an underwater mountain range in the northeastern Pacific. 



At this ridge, the Earth’s crust pulls apart due to the motion of tectonic plates, allowing molten rock to rise up and shape new crust. 



Plates moving apart have built a chain of peaks called a mid-ocean ridge. These ridges rarely capture the public’s imagination, yet they form one of Earth’s largest continuous geological features.



The ridge separates the Pacific Plate and the <a href="https://www.earth.com/news/claim-earth-has-six-continents-not-seven-north-america-europe-connected/" target="_blank" rel="noreferrer noopener">North American Plate</a>. When those plates drift away from each other, magma surfaces and hardens. 



<a href="https://www.earth.com/news/supervolcano-italy-solfatara-crater-phlegraean-fields-shows-signs-of-waking-up/" target="_blank" rel="noreferrer noopener">Volcanic and seismic events</a> dot this region, including those at Axial. Repeated eruptions at this particular volcano have given researchers a real-time window into volcanic processes that most can only study from old rocks on land.



<h2 class="wp-block-heading" id="h-axial-seamount-eruptions">Axial Seamount eruptions</h2>



Because Axial Seamount experiences frequent eruptions, it provides chances to fine-tune eruption predictions. 



Its swelling has reached levels that match those seen before past eruptions, prompting discussions about the next event possibly coming by the end of 2025.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/01/axial-seamount_underground-magma-system_credit-OregonStateU_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/01/axial-seamount_underground-magma-system_credit-OregonStateU_1s.webp" alt="A schematic model of the magmatic system below Axial Seamount. Green, blue, and cyan polygons on the seafloor indicate 1998, 2011, and 2015 lava flows, respectively. The red star indicates the location of a revised prolate-spheroid inflation source for the 2015 eruption52, and the magenta cycles denote the hydrothermal vents. Black lines denote eruptive fissures identified during 2011 and 2015 eruptions. A thermally controlled permeability boundary layer separates the MMR from hydrothermal fluid circulation (cyan dashed lines with arrows) in the dike and lava section above13. White dashed lines denote the isotherms. Credit: Nature" class="wp-image-1955438"/></a><figcaption class="wp-element-caption">A schematic model of the magmatic system below Axial Seamount. Green, blue, and cyan polygons on the seafloor indicate 1998, 2011, and 2015 lava flows, respectively. The red star indicates the location of a revised prolate-spheroid inflation source for the 2015 eruption52, and the magenta cycles denote the hydrothermal vents. Black lines denote eruptive fissures identified during 2011 and 2015 eruptions. A thermally controlled permeability boundary layer separates the MMR from hydrothermal fluid circulation (cyan dashed lines with arrows) in the dike and lava section above13. White dashed lines denote the isotherms. Credit: Nature</figcaption></figure>



Since these eruptions have been fairly similar each time, scientists are learning which signs point to magma movement and what those signals might mean for future activity.



<a href="https://www.earth.com/news/hydrothermal-vents-earths-blueprint-for-finding-alien-life/" target="_blank" rel="noreferrer noopener">Hydrothermal vents</a> play a role in shaping local marine ecosystems. Lava flows and bursts of heated fluid feed specialized life, such as tube worms and clams, that flourish in dark, high-pressure environments. 



This small spot of deep-sea life is a reminder of how volcanic activity can spur biological communities in unexpected places.



<h2 class="wp-block-heading" id="h-ai-and-new-prediction-methods">AI and new prediction methods</h2>



A recent effort involves analyzing quake patterns prior to 2015. That study leverages machine learning to recognize signals that precede an eruption. 



Experts see these methods as a way to identify shifts in ground motion more quickly than manual approaches. 



As inflation picks up again, this automated tracking could help identify the precise moment when <a href="https://www.earth.com/news/unexpected-molten-rock-layer-discovered-under-earths-crust/" target="_blank" rel="noreferrer noopener">molten rock</a> nears the surface.



Zumberge and others draw on a network of sensors that map every tremor and change in ground tilt. “At Axial, we don’t have to worry about false alarms,” said Chadwick. 



Thanks to these tools, false starts - common in volcano monitoring - have not posed much confusion here.



<h2 class="wp-block-heading" id="h-beyond-axial-seamount-s-slopes">Beyond Axial Seamount's slopes</h2>



Underwater eruptions may seem distant to folks on land, but they have global significance. The 2022 <a href="https://www.earth.com/news/tonga-eruption-had-the-energy-of-five-nuclear-explosions/" target="_blank" rel="noreferrer noopener">Hunga Tonga event</a>, for example, triggered a tsunami that caused an estimated $90 billion in losses. 



Though Axial Seamount itself poses little direct threat - shield volcanoes are less violent, and tremors here lack the force to create large waves - insights gained may aid efforts to forecast other, more hazardous sites.



“There’s no crystal ball,” noted volcanologist Valerio Acocella, from <a href="https://www.uniroma3.it/en/" target="_blank" rel="noreferrer noopener">University Roma Tre</a> in Italy, who studies both submarine and terrestrial volcanoes. 



That simple fact drives efforts to refine predictive science, using a wide range of data: ground deformation, quake frequency, and the chemistry of volcanic gases. 



Any improvement in these forecasts could limit harm in regions where eruptions might strike without warning.



<h2 class="wp-block-heading" id="h-refining-models-with-real-time-data">Refining models with real-time data</h2>



When Axial erupts, molten rock pours out across the seafloor, and new vents appear. These events offer a direct look at how <a href="https://www.earth.com/news/crystals-can-help-predict-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">magma moves underground</a>. 



Instruments feed constant streams of measurements to shore-based labs, revealing changes that happen within hours or even minutes. 



That trove of information helps experts see common threads that tie Axial’s predictable nature to more erratic volcanoes around the world.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/01/axial-seamount_seafloor-uplift_graph_credit-OregonStateU_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/01/axial-seamount_seafloor-uplift_graph_credit-OregonStateU_1s.webp" alt="Cumulative seafloor uplift and detected earthquakes at Axial Seamount underwater volcano. The vertical axis shows the uplift since May 2015, and the horizontal axis shows the cumulative amount of earthquakes detected since May 2015. Credit: Oregon State University" class="wp-image-1955436"/></a><figcaption class="wp-element-caption">Cumulative seafloor uplift and detected earthquakes at Axial Seamount underwater volcano. The vertical axis shows the uplift since May 2015, and the horizontal axis shows the cumulative amount of earthquakes detected since May 2015. Credit: Oregon State University</figcaption></figure>



Each new episode produces extra details, clarifying where magma is stored and how it shifts in the days or weeks before an eruption. 



According to Acocella, “We need these ideal cases to understand how volcanoes work.” 



Because Axial has such robust instrumentation, these “ideal cases” are more complete than anything available from many land-based sites.



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



Even though the undersea location of Axial Seamount means there is minimal risk to nearby shorelines, scientists still keep track of everything that happens beneath the waves. 



If a future <a href="https://www.earth.com/news/underwater-volcanic-eruptions-are-more-harmful-than-previously-believed/" target="_blank" rel="noreferrer noopener">submarine volcano</a> shows similar signals but lies closer to inhabited regions, the same methods could help governments plan. 



Real-time data streams might allow them to evacuate at-risk areas or safeguard critical infrastructure.



At Axial, repeated eruptions give a sense of certainty about what might unfold next. 



Unlike volcanoes that lie dormant for decades, this one reactivates on a cycle, creating a chance to track repeated patterns. That cyclical aspect has turned Axial into a natural classroom for geophysicists.



<h2 class="wp-block-heading" id="h-global-impact-of-axial-seamount">Global impact of Axial Seamount</h2>



To sum it all up, technological advances have made it easier to keep watch on both shallow and deep sections of Earth’s crust. Long cables connect sensors, offering near-instant awareness of quake swarms and ground shifts. 



By combining those tools with AI algorithms, research teams spot subtle shifts that might have gone unnoticed in older data sets.



The anticipation of Axial’s next eruption has galvanized experts who study volcanic forecasting. 



Axial’s shield structure, real-time monitoring, and location on a mid-ocean ridge present a unique scenario where everything lines up for practical research. 



Overall, many specialists see this site as a key test bed for learning about submarine eruptions. 



Eruptions at Axial allow researchers to gather immediate, detailed data that refine future warnings and guide planning for potentially dangerous underwater volcanoes elsewhere.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-49188-y" target="_blank" rel="noreferrer noopener">Nature</a>.



Image Credit: <a href="https://www.washington.edu/" target="_blank" rel="noreferrer noopener">University of Washington</a>



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Underwater volcano off the US coast could erupt at any moment

Axial Seamount sits under the Pacific Ocean about 300 miles...

Artificial intelligence (AI) continues to revolutionize the world of art, uncovering details that are invisible to the human eye. 



In a fascinating revelation, an AI neural network has unearthed a long-debated truth about Raphael’s&nbsp;Madonna della Rosa, a painting historically attributed to this Italian Renaissance master.



According to the study, not every brushstroke in the masterpiece is Raphael's.



<h2 class="wp-block-heading" id="h-who-is-raphael">Who is Raphael?</h2>



Raffaello Sanzio da Urbino was one of the most famous artists of the Renaissance. Born on April 6, 1483, in Urbino, Italy, he became known for his beautiful paintings and frescoes. Sadly, he passed away on his 37th birthday, April 6, 1520.



He’s best remembered for works like "The School of Athens," a stunning fresco in the Vatican, "Madonna della Rosa," as discussed here, and "The Transfiguration," which is often seen as his final masterpiece. 



Raphael was known for creating art that felt balanced, clear, and full of beauty, blending emotion with graceful figures. 



He was able to mix the emotional depth of artists like Leonardo da Vinci with the elegant compositions of artists like Michelangelo.



Besides painting, Raphael was also a talented architect. He worked on the design of St. Peter's Basilica in the Vatican and later became the chief architect there. 



His influence shaped both art and architecture during the Renaissance, and he’s still considered one of the greats, alongside Leonardo and Michelangelo.



<h2 class="wp-block-heading" id="h-the-masterpiece-madonna-della-rosa">The masterpiece: Madonna della Rosa</h2>



Madonna della Rosa&nbsp;is a Renaissance painting that was created during the late period of Raphael's career. The artwork portrays the Madonna and Child alongside St. Joseph and St. John, reflecting themes of familial unity and sacred devotion. 



The painting is notable for its vibrant color palette, soft rendering of figures, and the delicate interplay of light and shadow - all of which are hallmarks of Raphael's mature style.



Currently housed in the Museo Nacional del Prado in Madrid, the painting has undergone various restoration efforts over centuries to preserve its details and hues. 



Its title,&nbsp;Madonna della Rosa&nbsp;("Madonna of the Rose"), comes from the symbolic rose depicted in the scene, which has often been interpreted as a reference to the Virgin Mary's purity and suffering.



The painting represents a transitional moment in art history, blending elements of High Renaissance ideals with emerging Mannerist influences. 



Its history is intertwined with debates over authorship and the collaborative nature of Renaissance workshops, which were common at the time.



This has made&nbsp;Madonna della Rosa&nbsp;a subject of <a href="https://www.earth.com/news/worlds-oldest-cave-painting-discovered-in-indonesia/" target="_blank" rel="noreferrer noopener">fascination for art historians</a> and enthusiasts alike.



<h2 class="wp-block-heading" id="h-st-joseph-s-face-in-madonna-della-rosa">St. Joseph’s face in Madonna della Rosa</h2>



The face of St. Joseph, featured in the top-left corner of the famous painting, has sparked centuries of speculation.



While the painting’s authenticity as a Raphael original has been questioned since the mid-1800s, recent AI-powered analysis points to a significant conclusion: St. Joseph’s face was likely painted by another artist.



"Using deep feature analysis, we used pictures of authenticated Raphael paintings to train the computer to recognize his style to a very detailed degree, from the <a href="https://www.earth.com/news/acoustic-echoes-may-have-inspired-prehistoric-rock-art/" target="_blank" rel="noreferrer noopener">brushstrokes</a>, the color palette, the shading, and every aspect of the work," explained Hassan Ugail, mathematician and computer scientist from the <a href="https://www.bradford.ac.uk/external/" target="_blank" rel="noreferrer noopener">University of Bradford</a>.



"The computer sees far more deeply than the human eye, to microscopic level."



<h2 class="wp-block-heading" id="h-using-ai-to-analyze-the-painting">Using AI to analyze the painting</h2>



The researchers designed a specialized algorithm to compare <a href="https://www.earth.com/news/rock-art-reveals-early-human-ties-with-amazon-animals/" target="_blank" rel="noreferrer noopener">elements of the painting</a> to those found in verified Raphael works. 



This AI analysis, grounded in Microsoft’s ResNet50 framework and enhanced with a Support Vector Machine technique, could discern nuances at a microscopic level. The technology had previously demonstrated 98% accuracy in identifying Raphael’s works.



For this study, the team took the innovative step of analyzing individual faces within the painting. While the Madonna, the Child, and St. John showed clear signs of Raphael’s style, St. Joseph’s face stood out as inconsistent.



"When we tested the&nbsp;della Rosa&nbsp;as a whole, the results were not conclusive," said Ugail. "So, then we tested the individual parts and while the rest of the picture was confirmed as Raphael, Joseph's face came up as most likely not Raphael."



<h2 class="wp-block-heading" id="h-who-is-the-mystery-artist">Who is the mystery artist?</h2>



Historical evidence suggests Giulio Romano, one of Raphael’s most talented pupils, may have contributed to the <a href="https://www.earth.com/news/how-neanderthals-mastered-adhesive-technology/" target="_blank" rel="noreferrer noopener">painting</a>. 



Art critics have long noted St. Joseph’s face appears less refined compared to the other figures. While the AI analysis strengthens this theory, it does not definitively confirm the identity of the artist responsible for painting St. Joseph.



<h2 class="wp-block-heading" id="h-role-of-ai-in-art-authentication">Role of AI in art authentication</h2>



This revelation demonstrates the potential of AI to complement, not replace, human expertise in art authentication. 



AI’s ability to analyze brushstrokes, shading, and color palette at an unparalleled level provides a new dimension to evaluating artwork.



"This is not a case of AI taking people's jobs," said Ugail. "The process of authenticating a work of art involves looking at many aspects, from its provenance, pigments, condition of the work, and so on."



"However, this sort of software can be used as one tool to assist in the process."



<h2 class="wp-block-heading" id="h-a-masterpiece-with-a-modern-twist">A masterpiece with a modern twist</h2>



Madonna della Rosa, painted between 1518 and 1520, remains a captivating masterpiece. Yet, its history grows richer with this discovery, adding another layer to the narrative of Renaissance art. 



As AI continues to advance, it holds promise for uncovering hidden secrets in centuries-old works, and for enhancing our understanding of artistic legacies while preserving their mystique.



The study is published in the journal <a href="https://heritagesciencejournal.springeropen.com/articles/10.1186/s40494-023-01094-0" target="_blank" rel="noreferrer noopener">Heritage Science</a>.



Image Credit: Museo Nacional del Prado



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AI identifies surprising details about one of the most famous paintings in the world

Artificial intelligence (AI) continues to revolutionize the world of art,...

Micro- and nanoplastics (MNPs), plastic particles and fibers sized from nanometers (≥ 1 nm) to micrometers (≤ 5 mm), have emerged as critical environmental pollutants. While their impact on marine ecosystems has been widely studied, research on the effects of microplastics on terrestrial ecosystems remains underdeveloped.



A recent study&nbsp;by researchers from the Xishuangbanna Tropical Botanical Garden at the Chinese Academy of Sciences sheds light on this overlooked issue.



<h2 class="wp-block-heading" id="h-microplastics-in-terrestrial-ecosystems">Microplastics in terrestrial ecosystems</h2>



Micro- and nanoplastics are ubiquitous in terrestrial ecosystems, bioaccumulating in plants and organisms connected through aboveground (AG) and underground (BG) food webs.



These tiny particles not only impact individual plants but also disrupt multi-trophic interactions, biodiversity patterns, and ecosystem processes.



According to the researchers, MNPs interact with plants and associated AG-BG biota at multiple trophic levels. These interactions include herbivores, pollinators, and mycorrhiza fungi, which are essential for plant health and <a href="https://www.earth.com/news/microplastics-are-steadily-increasing-in-freshwater-environments/" target="_blank" rel="noreferrer noopener">ecosystem</a> stability.



By transferring across trophic levels, MNPs can harm biodiversity and affect ecosystem multifunctionality.



<h2 class="wp-block-heading" id="h-microplastic-transfer-in-terrestrial-ecosystems">Microplastic transfer in terrestrial ecosystems </h2>



The study identifies several trophic and non-trophic pathways for <a href="https://www.earth.com/news/microplastics-linked-to-health-issues-including-cancer-and-infertility/" target="_blank" rel="noreferrer noopener">MNP transfer</a> within and between AG-BG food webs. 



These include:



<ul class="wp-block-list">
<li>Leaves to herbivores: Herbivores that feed on plant leaves inadvertently ingest MNPs present on the surface of these leaves. This exposes them to potential toxic effects of these tiny particles.</li>



<li>Flowers to pollinators: Pollinators, like bees and butterflies, come into contact with MNPs when they land on flowers to collect nectar or pollen. These interactions can impact pollinator health and their role in pollination.</li>



<li>Prey to predators: Predators consume prey that has already ingested MNPs, leading to the transfer of these plastics up the food chain. This can accumulate and potentially harm predator species.</li>



<li>Roots to arbuscular mycorrhizal fungi: Mycorrhizal fungi, which form symbiotic relationships with plant roots to aid in nutrient absorption, can absorb MNPs present in the soil. This impacts the fungi and their role in plant health.</li>



<li>Roots to herbivores: Soil-dwelling herbivores that feed on plant roots may ingest MNPs present in or around the roots, exposing them to the harmful effects of these plastics.</li>



<li>Leaf litter to decomposers: When leaves containing MNPs decay, decomposer organisms like fungi, bacteria, and invertebrates break them down, absorbing or ingesting the embedded plastics.</li>



<li>Aboveground litter to belowground decomposers: Plant litter from aboveground, such as fallen leaves or flowers, carries <a href="https://www.earth.com/news/microplastic-pollution-is-everywhere-even-in-newborns-and-getting-worse/" target="_blank" rel="noreferrer noopener">MNPs</a> into the soil, where they are processed by belowground decomposers like earthworms and microbes.</li>



<li>Belowground prey to aboveground predators: MNPs present in soil-dwelling prey (like insects or larvae) transfer to aboveground predators (like birds or spiders) when they consume these organisms.</li>



<li>Belowground larvae to aboveground adults: Insects that spend their larval stages underground and then emerge as adults aboveground may carry microplastics they absorbed in their earlier stages into aboveground ecosystems.</li>
</ul>



These pathways illustrate the complexity of microplastic interactions within ecosystems and highlight their potential to disrupt ecological functions.



<h2 class="wp-block-heading" id="h-ecotoxicological-effects-of-microplastics">Ecotoxicological effects of microplastics </h2>



The study emphasizes that MNPs pose ecotoxicological threats across trophic levels. 



When plants absorb MNPs, these particles can affect the interactions between plants and organisms, leading to cascading effects in food webs. 



The researchers noted significant impacts on biodiversity, ecosystem processes, and multifunctionality. However, the extent of these effects remains uncertain due to limited research.



<h2 class="wp-block-heading" id="h-call-for-urgent-research-and-mitigation">Call for urgent research and mitigation</h2>



The researchers argue that terrestrial ecosystems urgently require more attention to fully assess the ecological impacts of MNPs. 



They emphasize the need for research to identify the long-term effects of <a href="https://www.earth.com/news/how-nanotechnology-is-fighting-microplastic-pollution/" target="_blank" rel="noreferrer noopener">MNPs</a> on plants and food webs, mitigation strategies to reduce MNP exposure in terrestrial ecosystems, and policies to manage MNP pollution effectively.



Such research will be critical to safeguarding plants and the intricate food webs they support.



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



To bridge the knowledge gap, researchers recommend focusing on the following areas:



<ul class="wp-block-list">
<li>MNP detection methods:&nbsp;Developing advanced techniques to identify and measure MNPs in terrestrial environments.</li>



<li>Long-term monitoring:&nbsp;Establishing long-term studies to understand MNP bioaccumulation and ecosystem impacts.</li>



<li>Mitigation strategies:&nbsp;Designing solutions to reduce MNP exposure, such as improved waste management and soil remediation techniques.</li>
</ul>



In sum, micro- and nanoplastics have emerged as a hidden threat to terrestrial ecosystems, affecting plants and interconnected AG-BG food webs. The findings emphasize the urgency of expanding research on this topic to mitigate their ecological <a href="https://www.earth.com/news/hotspots-of-microplastic-pollution-found-in-the-north-sea/" target="_blank" rel="noreferrer noopener">impact</a>.



This study highlights the interconnected nature of ecosystems and the critical role of plants in maintaining balance. Addressing MNP pollution in terrestrial systems will be vital for protecting biodiversity and ensuring ecosystem sustainability.



The study is published in the journal <a href="https://www.cell.com/trends/plant-science/abstract/S1360-1385(24)00335-2" target="_blank" rel="noreferrer noopener">Trends in Plant Science</a>.



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Silent invasion: How microplastics are disrupting land ecosystems

Micro- and nanoplastics (MNPs), plastic particles and fibers sized from...

<div class="vdb_player vdb_58e3ebce955a315103d39bd158d96b98cd4fed198a0d2a49" vdb_params="m.embeded=cms_video_plugin_www.earth.com" data-placeholder="//img.vidible.tv/prod/2017-09/23/59c5b1a785eb422a2d5cc2ad/59c5b23a6174ba154e30a3a7_o_A_v2.jpg?w=1440&#038;h=900">	<script type="text/javascript" src="//delivery.vidible.tv/jsonp/pid=58e3ebce955a315103d39bd1/vid=59c5b1a785eb422a2d5cc2ad/58d96b98cd4fed198a0d2a49.js?m.embeded=cms_video_plugin_www.earth.com"></script></div>
 
In the 1996 film Twister, storm chasers release data-gathering instruments into the funnel of a tornado to learn more about the storm. Today’s Video of the Day features two <a href="http://www.psu.edu/">Penn State</a> professors who are releasing their own instruments into possible tornado storms. The difference, though, is that instead of getting equipment into a <a href="https://www.earth.com/news/six-tornadoes-southeast-louisiana/">tornado</a>, these researchers are focusing on mapping the 3D variations in temperature at the time of the storm to better understand how they form.
 &#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a>
Video Credit: Penn State College of Earth &amp; Mineral Sciences

Using balloon probes to learn more about tornadoes