When the <a href="https://www.earth.com/news/dna-confirms-ancient-hybridization-of-polar-bears-and-brown-bears/">DNA</a> test results were in, it was revealed that the Ulukhaktok pizzly was a unique blend. Its mother was exactly 50% grizzly and 50% polar, while its father was a pure grizzly. This confirmed that the pizzly bears are in fact fertile mammalians. Photo Credit: Valkiyare/Reddit

Half And Half

Today's Image of the Day from the European Southern Observatory (ESO) features the Dark Wolf Nebula, located around 5,300 light-years from Earth in the constellation Scorpius.



According to ESO, this image of the dark <a href="https://www.earth.com/news/scientists-reveal-the-ring-nebula-as-it-has-never-been-seen-before/" target="_blank" rel="noreferrer noopener">nebula</a> creates the illusion of a wolf-like silhouette against a colorful cosmic backdrop.&nbsp;



“This image takes up an area in the sky equivalent to four full Moons, but is actually part of an even larger nebula called Gum 55. If you look closely, the wolf could even be a werewolf, its hands ready to grab unsuspecting bystanders,” noted <a href="https://www.eso.org/public/" target="_blank" rel="noreferrer noopener">ESO</a>.



<h2 class="wp-block-heading" id="h-observing-dark-nebulae">Observing dark nebulae </h2>



Dark nebulae are dense regions in space filled with gas and dust that absorb visible light, making them appear as dark patches against brighter backgrounds.&nbsp;



Unlike emission or reflection nebulae, dark nebulae do not glow on their own. Instead, they obstruct and obscure the light from stars and other objects lying behind them.&nbsp;



This characteristic makes them challenging to observe using visible-light telescopes, as they absorb and scatter light rather than reflecting or emitting it.&nbsp;



However, when viewed in infrared, where their obscuring effect is reduced, dark nebulae reveal intricate details about the <a href="https://www.earth.com/news/building-blocks-of-life-found-in-the-perseus-cloud/" target="_blank" rel="noreferrer noopener">molecular clouds</a> they contain.



According to ESO, astronomers study these clouds of frozen dust because they often contain new stars in the making.



<h2 class="wp-block-heading" id="h-dark-wolf-nebula-nbsp">Dark Wolf Nebula&nbsp;</h2>



The Dark Wolf Nebula is part of a larger complex known as the Lupus Molecular Cloud, one of several significant star-forming regions close to Earth.&nbsp;



Inside of dark nebulae, the conditions are prime for star formation. The dense gas and dust clump together under gravitational forces. As these clouds contract, they heat up, eventually igniting nuclear fusion and forming <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">new stars</a>.



The Dark Wolf Nebula is known for revealing young, low-mass stars - or T Tauri stars - which are in the early stages of their evolution. These stars are still surrounded by disks of material that may eventually form new planets.



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



Scorpius is one of the most recognizable constellations in the sky. It resembles a scorpion with a long, curved tail and stinger.&nbsp;



Located in the southern sky, Scorpius is especially visible during the summer months in the Northern Hemisphere and during the winter months in the Southern Hemisphere. 



The constellation is often associated with the story of Orion in Greek mythology. According to legend, the scorpion was sent by the goddess Artemis to kill Orion, the great hunter, either as punishment for his arrogance or to protect her animals, depending on the version of the tale.&nbsp;



The gods later placed both <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a> and Scorpius in the sky, but in opposite parts of the heavens so they would never be seen together - as Scorpius rises in the east and Orion sets in the west.



Scorpius contains several notable stars and deep-sky objects. Its brightest star, Antares, is a red supergiant often referred to as the "heart of the scorpion" due to its reddish hue and central position. 



Antares is one of the largest visible stars in the sky and has a luminosity that is tens of thousands of times greater than that of our Sun. 



Scorpius is located close to the core of the Milky Way, making it a rich region for star clusters and nebulae. Among these are the Butterfly Cluster and the Ptolemy Cluster - both of which are visible to the naked eye under dark skies.



<h2 class="wp-block-heading" id="h-image-of-the-dark-wolf-nebula">Image of the Dark Wolf Nebula </h2>



“This image shows in spectacular detail how the dark wolf stands out against the glowing star-forming clouds behind it,” noted ESO.



“The colorful clouds are built up mostly of hydrogen gas and glow in reddish tones excited by the intense UV radiation from the newborn stars within them.”



The picture was created from images taken at different times. Each of the images has a filter that makes a different color of light visible.&nbsp;



Observations of the Dark Wolf Nebula provide astronomers with valuable information about the <a href="https://www.earth.com/news/massive-star-redefines-our-understanding-of-stellar-evolution/" target="_blank" rel="noreferrer noopener">evolution of stars</a> and the environments in which they form.



The image was captured by the VLT Survey Telescope (VST) at ESO’s Paranal Observatory in Chile.



Image Credit: ESO/VPHAS+ team



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Dark Wolf Nebula in the constellation Scorpius

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.&nbsp;



"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 9.5-mile section of Pangong Lake on the western end of the Tibetan Plateau. The image was captured by a crew member onboard the International Space Station.&nbsp;



“In this winter scene, a sheet of cracked ice tops part of the lake,” noted <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>. “On the left side, open water appears blue. Shallow water offshore of a delta, formed by a small, winding river, appears green."



"Parallel lines along the coastlines of bays are visible in the high-resolution version of this image. These lines indicate raised beaches, which formed in the past when lake levels were higher.”



NASA pointed out that several roads cut across the landscape, including one with switchbacks that ascends a steep slope. "These roads facilitate tourist travel from both India and China.”&nbsp;



<h2 class="wp-block-heading" id="h-migratory-birds-at-pangong-lake-nbsp">Migratory birds at Pangong Lake&nbsp;</h2>



Pangong Lake and its surroundings are home to numerous bird species, particularly <a href="https://www.earth.com/news/migratory-birds-burn-unexpected-amounts-of-protein/" target="_blank" rel="noreferrer noopener">migratory birds</a>. Visitors can spot various waterfowl and waders that are rarely seen elsewhere.



“During the summer, species such as bar-headed geese and Brahminy ducks attract bird watchers to the lake, which is a major breeding ground for migrating birds,” said NASA.



Pangong Lake is one of the few places in India where the endangered black-necked crane is found during its breeding season. 



Ruddy shelduck and brown-headed <a href="https://www.earth.com/news/gulls-are-shifting-their-habitats-to-urban-areas/" target="_blank" rel="noreferrer noopener">gulls</a> are also frequently spotted around the lake. The ruddy shelduck is known for its striking orange-brown body and creamy white head, while the brown-headed gulls are often seen flying or swimming in the lake.



<h2 class="wp-block-heading" id="h-features-of-pangong-lake">Features of Pangong Lake </h2>



Pangong Lake is a stunning high-altitude lake situated in the <a href="https://www.earth.com/news/temperatures-are-rising-unexpectedly-fast-on-the-tibetan-plateau/" target="_blank" rel="noreferrer noopener">Himalayas</a>, extending from India to the Tibetan Autonomous Region of China. It is renowned for its mesmerizing beauty and dramatic setting, with the lake lying at an elevation of about 4,350 meters.



One of the most distinctive features of Pangong Lake is its changing colors, ranging from shades of blue to green and even red, influenced by the sky's reflection and the lake's mineral content.



This saline water lake is approximately 134 kilometers long and 5 kilometers wide at its broadest point. Despite its considerable size, Pangong Lake is relatively shallow.&nbsp;



The lake gained additional popularity after being featured in several Indian films - most notably the Bollywood hit "3 Idiots." Its remote location requires a permit for visitors, especially due to its proximity to the Line of Actual Control between India and China.



Despite the geopolitical sensitivities surrounding its location, Pangong Lake remains a favorite among tourists for its unparalleled natural beauty and serene environment.



<h2 class="wp-block-heading" id="h-high-altitude-lakes">High-altitude lakes</h2>



High-altitude lakes are unique bodies of water found at elevations typically above 3,000 meters (about 10,000 feet) in mountain ranges like the <a href="https://www.earth.com/news/himalayan-glaciers-retreating-threat-is-much-worse-than-previously-believed/" target="_blank" rel="noreferrer noopener">Himalayas</a>, Andes, and Rockies. 



These lakes are formed either by glacial activity, where glaciers erode the earth to create depressions that fill with melted snow and rainwater, or when natural dams created by landslides or moraines trap water in valleys.



<h3 class="wp-block-heading" id="h-extreme-environments">Extreme environments</h3>



The conditions at high altitudes make these lakes distinct in several ways. The climate is typically colder and harsher, with significant temperature variations between day and night. 



This extreme environment affects both the physical characteristics of 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">lakes</a> and the types of ecosystems they support. For example, due to lower atmospheric pressure, the boiling point of water is reduced, which can affect the type of life that can survive in these regions.



<h3 class="wp-block-heading" id="h-critical-habitats">Critical habitats</h3>



Biologically, high-altitude lakes often have limited biodiversity because only certain types of plants and animals can tolerate the cold temperatures and lower oxygen levels in the water. 



Despite this, these lakes are crucial habitats for some unique species of fish, birds, and other wildlife. They also serve as important indicators of climate change, as variations in their water levels and temperatures can reflect environmental shifts.



<h3 class="wp-block-heading" id="h-significance-of-high-altitude-lakes">Significance of high-altitude lakes </h3>



Lakes at high altitudes are often clear and pristine, due to the low density of human populations in these areas and minimal industrial activity, making them significant for ecological studies and attractive for tourism. 



However, they are sensitive ecosystems, and increased tourist activity brings challenges like pollution and habitat disruption.



High-altitude lakes are not only beautiful and scientifically significant but also hold cultural importance for local communities, often considered sacred and associated with historical and spiritual significance.



Image Credit: NASA Earth Observatory&nbsp;



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Pangong Lake on the Tibetan Plateau

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

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 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 control measure to regulate the floodwaters of the Euphrates River.&nbsp;



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.&nbsp;



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 the Rüppell's fox, golden jackal, Indian grey mongoose, jungle cat, and the wildcat. 



<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 wildlife. 



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 the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba about 43 million light-years away from Earth. 



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. This high rate of star formation 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-galaxy-evolution">Galaxy evolution</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>



These early galaxies were small and irregular, 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 - their 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

Today's Image of the Day from the European Space Agency features the galaxy ESO 300-16, which is located 28.7 million light-years from Earth in the constellation Eridanus. 



The galaxy is part of the ESO (European Southern Observatory) catalog, which includes a vast collection of galaxies observed in the southern hemisphere.



ESO 300-16 is notable for its chaotic structure, lacking the well-defined <a href="https://www.earth.com/image/hubble-captures-a-collection-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">spiral arms</a> or elliptical shape seen in many other galaxies.



<h2 class="wp-block-heading" id="h-ghostly-assemblage-of-stars">Ghostly assemblage of stars</h2>



According to <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>, ESO 300-16 is a ghostly assemblage of stars which resembles a sparkling cloud.&nbsp;



"A rogue’s gallery of distant galaxies and foreground stars complete this astronomical portrait, which was captured by the Advanced Camera for Surveys," said ESA.



"This observation is one of a series which aims to get to know our galactic neighbors; around three quarters of the known galaxies suspected to lie within 10 megaparsecs of Earth have been observed by Hubble in enough detail to resolve their brightest stars and establish the distances to these galaxies."



<h2 class="wp-block-heading" id="h-irregular-galaxy-structure">Irregular galaxy structure </h2>



ESO 300-16 lies at a relatively close distance to Earth compared to many other extragalactic objects, making it an interesting target for studies on galaxy formation and <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">evolution</a>. 



The galaxy's irregular structure suggests that it may have undergone past interactions with other galaxies or is in a stage of dynamic evolution.



One of the most striking features of ESO 300-16 is its wispy, diffuse appearance, with scattered patches of bright star-forming regions embedded within a fainter background. This indicates ongoing star formation, which is a common characteristic of irregular galaxies. 



Unlike large <a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">spiral galaxies</a>, where star formation is often concentrated in well-organized arms, ESO 300-16's active regions are more randomly distributed.



<h2 class="wp-block-heading" id="h-raw-material-for-star-formation">Raw material for star formation</h2>



Due to its irregular nature, the galaxy does not have a well-defined nucleus. Instead, it appears as a loose collection of stars, gas, and dust, which astronomers can study to understand the processes shaping such galaxies. 



Irregular galaxies like ESO 300-16 are often rich in gas and dust, providing the raw material for new stars to form. 



Observations in different wavelengths, such as infrared and ultraviolet, can help reveal the presence of young, hot stars and cooler dust clouds that might be sites of future <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">star formation</a>.



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



Hubble observations of ESO 300-16 provide insight into the structure and stellar populations of the galaxy, helping astronomers piece together its history and evolutionary path. 



The study of galaxies like ESO 300-16 contributes to our broader understanding of how galaxies form and evolve, especially those that do not fit into the traditional classifications of spirals and ellipticals.



Because irregular galaxies are often shaped by gravitational interactions or past mergers, ESO 300-16 may have had a turbulent past. 



It could have once been part of a larger system before being disrupted, or it might have formed in an environment where gravitational influences from nearby galaxies prevented it from developing a more regular shape. 



Studying its motion and the distribution of its stars can provide clues about any past interactions it may have experienced.



<h2 class="wp-block-heading" id="h-a-glimpse-into-the-early-universe">A glimpse into the early universe </h2>



ESO 300-16 also provides a glimpse into what some galaxies in the early <a href="https://www.earth.com/news/universe-is-expanding-faster-than-science-can-explain-hubble-tension-physics-crisis/" target="_blank" rel="noreferrer noopener">universe</a> might have looked like. 



Many early galaxies were irregular in shape before evolving into more structured forms over time. As a result, studying nearby irregular galaxies like ESO 300-16 can offer valuable analogs for understanding galaxy formation in the distant past.



Although ESO 300-16 is not one of the most famous galaxies, it remains an important object for astronomers studying irregular galaxies, star formation, and the role of interactions in shaping galactic structures. 



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

Today's Image of the Day from NASA Earth Observatory features dust plumes streaming over West Texas, after a storm system developed in the Central Plains of the United States. 



The low-pressure storm system produced a destructive series of severe weather events across the country.



“A powerful mid-latitude cyclone delivered a potpourri of weather hazards as it worked its way across the United States in March 2025,” said NASA.



“Beginning on March 3, the low-pressure system fanned wildfires and blinding dust storms in the Southwest, spawned severe thunderstorms and tornadoes in the Southeast, fueled blizzards in the Great Plains and Midwest, and dropped heavy rain in the Northeast.”



<h2 class="wp-block-heading" id="h-massive-dust-storms">Massive dust storms</h2>



In New Mexico and Texas, the storm generated massive <a href="https://www.earth.com/news/sand-and-dust-storms-have-become-unpredictable-and-dangerous/" target="_blank" rel="noreferrer noopener">dust storms</a>, known as "haboobs," characterized by walls of dust stretching miles wide and thousands of feet high. These dust storms led to near-zero visibility, causing hazardous driving conditions and road closures.&nbsp;



The National Weather Service issued dust storm warnings, advising residents to stay indoors and drivers to pull over safely until conditions improved



NASA elaborated on the details captured in the image. “Clouds of dust appear to originate from arid landscapes in northern Mexico and West Texas, a region that spans the Chihuahuan Desert, cattle ranches and cotton farms, and gas and oil fields.”



“Exceptional drought has gripped West Texas for the past several months, according to the U.S. Drought Monitor. The lack of rain has parched vegetation and dried the land surface, making the region particularly susceptible to erosion and dust storms.”



<h2 class="wp-block-heading" id="h-dust-storms-are-intensifying-in-the-u-s">Dust storms are intensifying in the U.S.</h2>



Santiago Gassó, an atmospheric scientist at NASA’s Goddard Space Flight Center, noted that dust storms are typical in this region at this time of year. “Unfortunately, we’re seeing longer <a href="https://www.earth.com/news/droughts-and-extreme-weather-events-are-escalating/" target="_blank" rel="noreferrer noopener">droughts</a> in the southwestern U.S. and northern Mexico, so we can expect more of this type of (larger) event.”



NASA noted that fierce winds and thick plumes of blowing dust led to traffic accidents, flight disruptions, school closures, power outages, and red and orange skies throughout the state and region.&nbsp;



“One particularly severe dust storm on March 3 sharply reduced visibility and contributed to a 21-car accident near Roswell, New Mexico.”



<h2 class="wp-block-heading" id="h-blizzards-tornadoes-and-fire-weather">Blizzards, tornadoes, and fire weather</h2>



The storm also produced blizzard conditions in parts of the Rockies and the Plains, with heavy snowfall and strong winds making travel difficult and increasing the risk of power outages.&nbsp;



Major cities like Chicago and Milwaukee were expected to experience record low-pressure readings due to the storm's intensity.



In addition to dust storms and blizzards, the system brought severe weather to the Southern United States, including threats of <a href="https://www.earth.com/news/u-s-tornado-outbreak-100-storms-touched-down-in-a-week/" target="_blank" rel="noreferrer noopener">tornadoes</a>, large hail, and strong winds.&nbsp;



North Texas, particularly the Dallas-Fort Worth area, faced significant impacts, with over 400,000 people experiencing power outages. An EF1 tornado struck Irving, Texas, leading to evacuations from damaged apartment complexes.



The storm's strong winds and low humidity levels also heightened fire risks in regions like Central Texas and Alabama. Red Flag Warnings were issued due to the increased potential for rapid and intense wildfires.&nbsp;



<h2 class="wp-block-heading" id="h-panhandle-hook-storms-in-the-u-s">Panhandle hook storms in the U.S.</h2>



A panhandle hook is a type of low-pressure storm system that originates in the Texas and Oklahoma panhandle regions and then moves northeast across the central United States.&nbsp;



These systems are named for their characteristic "hook-shaped" track, as they often travel from the southern Plains into the Midwest and Great Lakes region.



The storms typically begin as low-pressure systems in the semi-arid regions of Texas, Oklahoma, and eastern New Mexico, where warm, moist air from the Gulf of Mexico meets cold, dry air from the Rockies and the northern Plains.



As the system strengthens, it moves northeastward, often following a curved path that resembles a "hook" when mapped. This movement is influenced by the jet stream, which steers the storm across the central U.S.



Panhandle hook <a href="https://www.earth.com/news/record-heat-fueled-unexpected-and-deadly-storms-in-2023/" target="_blank" rel="noreferrer noopener">storms</a> are particularly dangerous because they develop quickly and can intensify rapidly. They often occur in late winter and early spring, when temperature contrasts are strongest.



The image was captured on March 4, 2025 by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite.&nbsp;



Image Credit: NASA Earth Observatory&nbsp;



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Monster storm spawns severe weather across the U.S. 

The MODIS instrument, short for Moderate Resolution Imaging Spectroradiometer, is a key instrument aboard the Terra and Aqua satellites. MODIS is playing a vital role in the development of Earth ecosystem models, able to predict global changes, which then assist policy makers in making informed decisions about the protection of the global environment.

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

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

Aqua is a NASA scientific research satellite that studies precipitation, evaporation, and water cycles. Terra and Aura make up the Earth Observing System. It's the second component of the system.

A frozen Lake Erie in February Today’s Image of the Day comes from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a frozen <a href="https://www.earth.com/image/icy-lake-erie/">Lake Erie</a>, which is currently 93.3 percent iced over. A frozen Lake Erie in February
This false-color image was created using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Aqua satellite to differentiate between snow, ice, and clouds.
Lake Erie /ˈɪəri/ (French: Lac Érié) is the fourth-largest lake (by surface area) of the five Great Lakes in North America, and the eleventh-largest globally if measured in terms of surface area.It is the southernmost, shallowest, and smallest by volume of the Great Lakes and therefore also has the shortest average water residence time. At its deepest point Lake Erie is 210 feet (64 metres) deep. 
Situated on the International Boundary between Canada and the United States, Lake Erie&#8217;s northern shore is the Canadian province of Ontario, specifically the Ontario Peninsula, with the U.S. states of Michigan, Ohio, Pennsylvania, and New York on its western, southern, and eastern shores. These jurisdictions divide the surface area of the lake with water boundaries. 
The lake was named by the Erie people, a Native American people who lived along its southern shore. The tribal name &#8220;erie&#8221; is a shortened form of the Iroquoian word erielhonan, meaning long tail
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Image Credit: <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>

A frozen Lake Erie in February

Aqua Earth Observing Satellite

This beautiful photo gallery contains 50 incredible images of Earth from Space. These images were taken by astronauts onboard the International Space Station, as well as by a multitude of NASA satellites orbiting the earth.

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a> and features a look at Super Typhoon Noru in the Pacific Ocean just south of <a href="https://www.earth.com/news/first-blue-chrysanthemums-created/">Japan</a>.
This image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite on July 31, 2017. 
At the time the photo was taken, Typhoon Noru was located just 250 kilometers south of Iwo Jima. Maximum sustained winds hit 150 miles per hour.
The storm briefly became a category 5 on July 30, before being downgraded to a category 4 one day later.
&#8211;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

Photos from the International Space Station are found in this awesome Earth.com image gallery. Flat-earthers won't agree, but these incredible photos of the Earth were taken by astronauts onboard the International Space Station. The International Space Station is a modular space station in low Earth orbit.

Northern Italy from the space station is seen here in this Image of the Day from the <a href="http://www.esa.int/">European Space Agency</a> (ESA). The view includes the top half of the Italian Peninsula, along with <a href="https://www.earth.com/image/wildfires-burn-northern-corsica/">Corsica</a> and Sardinia off the coast. This image was captured by ESA astronaut Paolo Nespoli on his third and final mission to the Space Station.

Northern Italy from the Space Station

Photos from the International Space Station

A new report reveals that more than one-third of all U.S. bird species stand in high or moderate conservation danger. Additionally, there are 112 “tipping point” species that have seen half or more of their populations vanish in the past 50 years.



The tipping point groups identified in the report include 42 red-alert species such as Allen’s Hummingbird, Tricolored Blackbird, and Saltmarsh Sparrow. These species are facing a high risk of <a href="https://www.earth.com/news/hundreds-of-bird-species-face-extinction-risks-in-the-neotropics/" target="_blank" rel="noreferrer noopener">extinction</a> unless swift interventions are made.



“Birds tell us that we have a full-on emergency across all habitats,” said Marshall Johnson, chief conservation officer at the <a href="https://www.audubon.org/" target="_blank" rel="noreferrer noopener">National Audubon Society</a>.



<h2 class="wp-block-heading" id="h-state-of-the-birds-report-nbsp">State of the Birds report&nbsp;</h2>



The 2025 U.S. State of the Birds report was unveiled at the 90th annual North American Wildlife and Natural Resources Conference in Louisville, Kentucky.&nbsp;



Compiled by a coalition of top science and conservation organizations, the report documents sustained widespread losses in American bird populations across mainland and marine habitats, highlighting 229 species requiring urgent conservation measures.&nbsp;



The findings follow on from the influential 2019 study that found the loss of three billion birds in North America over five decades.



<h2 class="wp-block-heading" id="h-significance-of-america-s-birds">Significance of America's birds</h2>



In defending birds, the report emphasizes not just the ecological arguments but also the financial rewards for local economies. 



Nearly 100 million Americans take part in bird-related activities, from casual backyard birding to dedicated expeditions. 



The total economic output connected to bird watching activities is $279 billion, while birding related activities support 1.4 million jobs, the experts argued, referencing the latest <a href="https://www.fws.gov/program/national-survey-fishing-hunting-and-wildlife-associated-recreation-fhwar" target="_blank" rel="noreferrer noopener">National Survey of Fishing, Hunting, and Wildlife-Associated Recreation</a> data.



The study emphasizes that birds are also central to <a href="https://www.earth.com/news/millions-of-americans-have-lost-years-of-time-to-poor-mental-health/" target="_blank" rel="noreferrer noopener">mental health</a> benefits. By citing existing research, the authors explain that daily or weekly encounters with birds and nature help relieve stress and diminish symptoms of anxiety and depression - an added incentive to strengthen conservation programs.



<h2 class="wp-block-heading" id="h-disturbing-trends-in-bird-habitats">Disturbing trends in bird habitats</h2>



In analyzing bird populations across America, the authors warn that nearly every type of ecosystem is witnessing declines. Even ducks, which had been a bright spot in past reports, are trending downward in more recent tallies.



“The rapid declines in birds signal the intensifying stressors that wildlife and people alike are experiencing around the world because of habitat loss, environmental degradation, and extreme weather events,” noted Amanda Rodewald, faculty director of the <a href="https://www.birds.cornell.edu/home/" target="_blank" rel="noreferrer noopener">Cornell Lab of Ornithology</a>’s Center for Avian Population Studies.&nbsp;



“When we see declines like those outlined in the report, we need to remember that if conditions are not healthy for birds, they’re unlikely to be healthy for us.”



<h2 class="wp-block-heading" id="h-cause-for-both-alarm-and-hope">Cause for both alarm and hope</h2>



“There is no doubt that the 2025 State of the Birds report is cause for alarm, but it is also cause for hope. Public interest in birds and the economic benefits from birding are at unprecedented levels, as is the information available about the status of each and every one of our bird species,” said Jeff Walters, conservation committee co-chair at the <a href="https://americanornithology.org/" target="_blank" rel="noreferrer noopener">American Ornithological Society</a>.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/bird-populations_united-states_rapid-decline_graph_credit-Cornell_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/bird-populations_united-states_rapid-decline_graph_credit-Cornell_1s.webp" alt="Long-term population trends for America's birds. Credit: State of the Birds long-term population trends, the Cornell Lab of Ornithology." class="wp-image-1962322"/></a><figcaption class="wp-element-caption">Long-term population trends for America's birds. Credit: State of the Birds long-term population trends, the Cornell Lab of Ornithology.</figcaption></figure>



Strategies for reversing these declines emerge throughout the document. The authors highlight conservation success stories and methods that have proven effective for waterfowl, waterbirds, and other avian groups, indicating that more robust action could yield results on a larger scale.



<h2 class="wp-block-heading" id="h-effective-conservation-approaches">Effective conservation approaches</h2>



“Many bird populations are struggling. But a proven blueprint for success is science-based planning and collaborative investment in <a href="https://www.earth.com/news/habitat-and-evolution-shape-the-unique-sounds-of-birds/" target="_blank" rel="noreferrer noopener">habitat</a> conservation,” said Steve Adair, Ducks Unlimited chief scientist.



Beyond this, practical measures - like private lands programs, ranching partnerships, forest renewal projects, coastal restoration efforts, and seabird translocation - have all shown promise in reviving bird populations under stress.&nbsp;



Adair cited the strong cooperation among hunters, landowners, agencies, and corporations as having historically benefited waterfowl numbers, at least where suitable weather conditions apply.



“Decades of strategic and aggressive wetland habitat conservation from hunters, landowners, state and federal agencies, and corporations has boosted numerous waterfowl and waterbird species when weather conditions are favorable. We’ve shown it works. And we must do more,” Adair said.



<h2 class="wp-block-heading" id="h-protecting-america-s-bird-life">Protecting America's bird life</h2>



At the same time, the report makes clear that bird conservation has ripple effects for human communities and broader ecosystems.



“Fortunately, many of the actions that are good for birds are good for us. When we protect the habitats that birds rely upon, we also protect the ecosystem services that sustain us,” Rodewald said.



In other words, robust protections for wetlands, coasts, <a href="https://www.earth.com/news/every-bird-song-can-help-scientists-make-smarter-forest-decisions/" target="_blank" rel="noreferrer noopener">forests</a>, and other key habitats not only safeguard bird life, but also maintain carbon storage, preserve water quality, and buffer cities and towns against natural disasters.



<h2 class="wp-block-heading" id="h-looking-toward-effective-solutions">Looking toward effective solutions</h2>



Michael J. Parr, President of <a href="https://abcbirds.org/" target="_blank" rel="noreferrer noopener">American Bird Conservancy</a>, praised ongoing research but emphasized that more support is crucial:



“We have clear evidence that conservation works in halting declines,” said Parr. “What we now need more than ever are programs and funding that match the scale of the greatest challenges birds face today. The science is solid on how to reverse the damage done, but to succeed, these issues need to be taken seriously.”



Marshall Johnson of the National Audubon Society reinforced this need for prompt and inclusive measures. 



“Birds unite us across the hemisphere and across the political spectrum - there should be no hesitation as we move to protect them today and in the future,” he said.



Ultimately, the 2025 U.S. State of the Birds report highlights a stark warning but also underscores the possibility for saving countless bird species if deliberate policies and robust support meet the urgency of the crisis.&nbsp;



Humans stand to benefit economically and culturally from an environment where bird populations thrive, reminding all stakeholders of the vital connections between <a href="https://www.earth.com/news/new-era-in-wildlife-conservation-how-ai-will-help-protect-elephants/" target="_blank" rel="noreferrer noopener">wildlife conservation</a> and broader social well-being.



The report can be found <a href="https://www.stateofthebirds.org/2025/" target="_blank" rel="noreferrer noopener">here</a>.



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Saving America's birds: Scientists declare a 'full-on emergency' in the US

A new report reveals that more than one-third of all...

When astronomers observe distant objects, there is a potential pitfall: does a particular star truly appear reddish because of its intrinsic characteristics, or is it merely taking on a red hue due to intervening cosmic dust?&nbsp;



For astronomers, dust is not just an observational inconvenience - it also provides crucial insights into the composition and local conditions within interstellar space.&nbsp;



Two researchers at the <a href="https://www.mpia.de/en" target="_blank" rel="noreferrer noopener">Max Planck Institute for Astronomy</a> (MPIA) have now created the most detailed three-dimensional map to date, tracking dust in our galaxy and explaining how it alters light along our line of sight.



<h2 class="wp-block-heading" id="h-why-dust-matters-for-observations">Why dust matters for observations</h2>



The <a href="https://www.earth.com/news/how-dust-becomes-planets-in-the-shadows-of-hh-30/" target="_blank" rel="noreferrer noopener">dust</a> spread across the Milky Way dims and reddens the light from distant stars. When light from a star travels to us, the tiny dust particles more strongly absorb and scatter bluer wavelengths, while allowing redder wavelengths to pass more easily.&nbsp;



This wavelength-dependent phenomenon is referred to as extinction (the star appears fainter than it is) and reddening (the star takes on a redder hue).&nbsp;



Accurately disentangling the effect of dust is vital for astronomers, who need a precise picture of distant objects’ actual brightness and color to glean information about their properties.



As Xiangyu Zhang, a doctoral candidate at MPIA, and his advisor Gregory Green explain, cosmic dust particles don’t absorb and scatter light evenly across all wavelengths, but rather they absorb light more strongly at shorter wavelengths, towards the blue end of the spectrum, and less strongly at longer wavelengths, towards the red end.&nbsp;



Studying these dust properties can shed light on the composition and evolution of the interstellar medium.



<h2 class="wp-block-heading" id="h-mapping-dust-across-a-galaxy">Mapping dust across a galaxy</h2>



Previous efforts at mapping dust on a galaxy-wide level were limited, mainly due to incomplete data. 



The <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a>’s <a href="https://www.earth.com/news/gaia-reveals-moons-around-hundreds-of-asteroids/" target="_blank" rel="noreferrer noopener">Gaia mission</a> - devoted to tracking positions, motions, and physical traits for over one billion stars - now offers a treasure trove of new information. 



Gaia’s third data release (DR3), published in June 2022, contains 220 million spectra. Zhang and Green identified 130 million of them as suitable for their study of dust’s effects.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/milky-way-dust_map_wavelength_credit-MPIA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/milky-way-dust_map_wavelength_credit-MPIA_1s.webp" alt="Red indicates regions where extinction falls off more rapidly at long wavelengths (the red end of the spectrum), while blue indicates that extinction is less dependent on wavelength. Regions with insufficient data are shown in white. The gray contours enclose regions of high dust density. Credit: X. Zhang/G. Green, MPIA" class="wp-image-1962319"/></a><figcaption class="wp-element-caption">Red indicates regions where extinction falls off more rapidly at long wavelengths (the red end of the spectrum), while blue indicates that extinction is less dependent on wavelength. Regions with insufficient data are shown in white. The gray contours enclose regions of high dust density. Credit: X. Zhang/G. Green, MPIA</figcaption></figure>



Gaia’s spectra, however, are low-resolution, meaning they only separate incoming light into broad wavelength bins. 



To improve accuracy, the researchers turned to high-resolution data from the <a href="https://www.lamost.org/public/?locale=en" target="_blank" rel="noreferrer noopener">LAMOST survey</a> for approximately 1% of the stars in their sample. 



These extra details helped them determine each star’s surface temperature and other properties, crucial for untangling the effects of dust from the star’s own attributes.



<h2 class="wp-block-heading" id="h-building-a-3d-dust-map-nbsp">Building a 3D dust map&nbsp;</h2>



Zhang and Green employed <a href="https://www.earth.com/news/machine-learning-could-revolutionize-drug-discovery/" target="_blank" rel="noreferrer noopener">machine learning</a> techniques - specifically, a neural network - to synthesize model spectra that incorporate both known stellar properties and dust parameters. 



The researchers compared these model-generated spectra with the observed Gaia data, all while ensuring the results followed certain established laws of physics.



In doing so, they derived new constitutive models detailing how dust in different parts of the galaxy dims and reddens starlight (often represented by an “extinction curve”).&nbsp;



Through statistical analyses, the experts could reconstruct the properties of dust along each star’s line of sight, culminating in the most finely detailed 3D map of dust across the <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">Milky Way</a> yet produced.



<h2 class="wp-block-heading" id="h-stellar-birth-and-planet-formation-nbsp">Stellar birth and planet formation&nbsp;</h2>



Dust is sometimes seen as “the astronomer’s enemy,” as it confounds easy measurements of stellar brightness and color. Yet it also lies at the core of stellar birth and planet formation.&nbsp;



Stars emerge from massive <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">molecular clouds</a>, which are shielded from harsh external radiation by dust. Newly formed stars are surrounded by disks of gas and dust that seed planetary systems.&nbsp;



Moreover, much of the chemical richness in our galaxy, especially elements heavier than hydrogen and helium, remain locked in dust grains.



<h2 class="wp-block-heading" id="h-surprising-dust-behavior">Surprising dust behavior</h2>



One of the map’s key findings contradicts earlier expectations. Astronomers once assumed that in regions of higher dust density, dust growth would flatten the extinction curve, making it less sensitive to wavelength.&nbsp;



Instead, Zhang and Green found that in areas of intermediate density, the extinction curve steepens, with shorter wavelengths more readily absorbed than longer ones.



“Higher density,” they note, is still extremely low by human standards - roughly ten billionth billionth grams of dust per cubic meter. 



One plausible explanation is that certain molecules, especially polycyclic aromatic hydrocarbons (PAHs), might flourish in these conditions, causing the steeper wavelength dependency. 



PAHs, which are the most widespread hydrocarbons in space, have even been proposed as a possible precursor to life.



<h2 class="wp-block-heading" id="h-first-3d-map-of-dust-in-the-milky-way-nbsp">First 3D map of dust in the Milky Way&nbsp;</h2>



Zhang and Green’s work constitutes the first detailed, three-dimensional map of the extinction curve of dust in the Milky Way, relying on 130 million measurements compared to around one million in past studies.&nbsp;



The success of this research demonstrates how advanced techniques - merging big data and rigorous physics - can unearth new insights.



Though their results provide an unprecedented view of dust’s large-scale distribution and properties, questions linger about how dust forms and evolves in different parts of the galaxy, and how these changes might influence the births of stars and planetary systems.&nbsp;



Zhang and Green intend to test their PAH hypothesis with future observations, refining the model to capture finer structural details and verifying the presence of specific molecular signatures.



In a broader sense, the study’s methodology promises to refine how astronomers correct for dust’s interference in both local and cosmological observations. 



It may also help interpret new data from upcoming missions that probe the Milky Way’s structure and chemical makeup. 



Consequently, the refined 3D dust map offers a clearer, dust-corrected view of our galaxy’s layout - an essential foundation for everything from measuring star distances to unraveling the riddle of how cosmic matter is assembled into complex, life-enabling systems.



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Cosmic map reveals that the Milky Way's dust has very unusual properties

When astronomers observe distant objects, there is a potential pitfall:...

Tiny microplastic fragments, often smaller than a grain of rice, are turning up in surprising places. From city streets to remote oceans, they persist in the air, water, and soil. 



Scientists have learned that these particles can also invade the human body, showing up in organs that keep us alive. 



For years, researchers have warned us about the possible dangers microplastics pose to animals, our food sources, and human health. Now a fresh study suggests even plants are feeling the pressure.



<h2 class="wp-block-heading" id="h-plants-photosynthesis-and-microplastics">Plants, photosynthesis, and microplastics</h2>



This new research from <a href="https://www.5gyres.org/" target="_blank" rel="noreferrer noopener">5 Gyres Institute</a> offers new clues about how these plastic particles affect photosynthesis. 



The team gathered over 3,200 records from across the globe, focusing on how tiny bits of microplastics alter photosynthesis by changing the way <a href="https://www.earth.com/news/details-photosynthesis-water-viewed-atomic-level-cryo-microscope/" target="_blank" rel="noreferrer noopener">plants use sunlight</a> to produce energy. 



Their analysis spans common food crops and aquatic species, highlighting concerns about weakened growth. 



For communities that rely on healthy harvests and marine resources, these findings add a fresh dimension to the worldwide plastic conversation.



“It’s really scary,” says Marcus Eriksen, a marine scientist at the 5 Gyres Institute, a nonprofit plastic pollution research organization, who was not involved in the study.



<h2 class="wp-block-heading" id="h-how-microplastics-spread-far-and-wide">How microplastics spread far and wide</h2>



Most microplastics come from everyday sources. Plastic bottles, packaging, and synthetic clothing shed fibers that break into smaller pieces. Rain and wind carry these particles into rivers, and eventually they end up in oceans. 



In agricultural fields, plastic mulch or irrigation systems contribute fragments that seep into the soil. Over time, these bits degrade further, leading to a steady accumulation in places we least expect. 



This constant spread worries experts because smaller sizes mean they can slip into living organisms more easily.



Researchers have found these particles in fish, shellfish, and even table salt. In recent years, labs have also identified plastic remnants in bottled water and tap supplies. 



While ongoing investigations continue to measure how widespread they are, one thing is clear: once plastic breaks down, it does not disappear. That lingering presence has potential consequences for all life on Earth.



<h2 class="wp-block-heading" id="h-microplastics-impede-photosynthesis">Microplastics impede photosynthesis</h2>



In this new analysis, researchers show that microplastics reduce photosynthesis by 7 to 12% across different plant species. 



A computer model backs this up, indicating that plastic particles can <a href="https://www.earth.com/news/artificial-photosynthesis-could-transform-power-generation/" target="_blank" rel="noreferrer noopener">lower chlorophyll</a> levels by 11 to 13%. 



<a href="https://www.earth.com/news/gardening-hack-called-green-gold-chlorophyll-works-like-magic-for-houseplants/" target="_blank" rel="noreferrer noopener">Chlorophyll</a> is the green pigment that helps plants capture sunlight for food production, so any dip in its presence can affect overall growth.



Every year, this pollution could cause a loss of 109 to 361 million metric tons of crops and 1 to 24 million metric tons of seafood, according to the study. 



Because of microplastic buildup, global harvests may drop by 4 to 13% yearly, and food from the ocean could decline by up to 7%. 



Even minor disruptions to plant growth may have ripple effects on human nutrition and economies that rely on farming.



<h2 class="wp-block-heading" id="h-challenges-for-the-food-supply">Challenges for the food supply</h2>



Beyond plants, these particles also affect marine life, which many communities rely on for protein. Scientists report that if <a href="https://www.earth.com/news/microplastic-pollution-is-everywhere-even-in-newborns-and-getting-worse/" target="_blank" rel="noreferrer noopener">microplastic pollution</a> continues unchecked, seafood yields could suffer even further. 



They are associated with an increase in people’s risk of heart attack and stroke, and they have been found to hamper growth and reproduction in multiple species. 



Worries about <a href="https://www.earth.com/news/we-are-in-a-race-against-time-to-save-our-food-supply-from-climate-change/" target="_blank" rel="noreferrer noopener">food safety and supply</a> also arise when these pollutants accumulate in organisms that people eat.



Researchers suggest that a modest 13% reduction in these particles could prevent the loss of up to 47 million metric tons of crops and 3 million metric<a href="https://www.earth.com/news/plastic-particles-found-in-99-of-tested-seafood-samples/" target="_blank" rel="noreferrer noopener"> tons of seafood</a> each year, translating to a 30% cut in overall harm. 



This projection highlights the importance of tightening plastic regulations and improving waste management to protect food resources.



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



Reduced photosynthesis does not only <a href="https://www.earth.com/news/microbial-awakening-arctic-food-webs-are-transforming-from-green-to-brown/" target="_blank" rel="noreferrer noopener">disrupt food webs</a>. When plants capture less carbon dioxide, there is less natural removal of this greenhouse gas from the atmosphere. 



In many climate strategies, forests and marine algae are expected to absorb significant amounts of carbon in the coming decades. If plastic particles undermine that process, climate models may need to be revised.



Most projections assume stable plant performance over time. Any drop in growth or carbon uptake could make <a href="https://www.earth.com/news/un-the-world-is-on-track-for-a-catastrophic-level-of-global-warming/" target="_blank" rel="noreferrer noopener">global warming</a> harder to control. 



With ecosystems already under stress, additional strain from microscopic plastic fragments raises concerns about future carbon storage in forests, grasslands, and kelp beds.



<h2 class="wp-block-heading" id="h-sounding-the-alarm">Sounding the alarm</h2>



The study’s authors emphasize the need for international efforts to address plastic waste, pointing out that large pieces eventually degrade into smaller and more invasive forms.



A global treaty on plastic issues has been in discussion since 2017, yet recent negotiations concluded without a formal agreement.



Marine biologist Richard Thompson, who specializes in microplastic pollution at the <a href="https://www.plymouth.ac.uk/" target="_blank" rel="noreferrer noopener">University of Plymouth</a> in England and was not involved in the study, notes that delaying action only increases the risks.



“If we don’t take action now,” he adds, “within the next 70 to 100 years, we’ll see much wide-scale ecological harm.”



Researchers say that lowering even a small amount of microplastic pollution could help protect crops, preserve marine life, and support our climate goals.



Taking action now can guard our health and ensure a healthier environment for generations to come, which doesn’t seem like too much to ask of humanity.



The full study was published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2423957122">Proceedings of the National Academy of Sciences</a>.



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Sounding the alarm: Microplastics are disrupting  photosynthesis around the world

Tiny microplastic fragments, often smaller than a grain of rice,...

When thinking about why animals look the way they do, color is often front and center. However, humans are mostly limited to seeing a certain slice of the spectrum, ignoring the ultraviolet (UV) range that many animals use in their daily lives.&nbsp;



A recent study by scientists at the <a href="https://umich.edu/" target="_blank" rel="noreferrer noopener">University of Michigan</a> (U-M) highlights the importance of UV coloration in <a href="https://www.earth.com/news/diverse-group-of-snakes-has-a-new-evolutionary-tree/" target="_blank" rel="noreferrer noopener">snakes</a>, showing that UV patterns are widespread and may play a significant role in evading predators such as birds.



The findings point to a broader issue in the study of color evolution: researchers tend to focus on colors we humans can detect.&nbsp;



“A lot of UV color work is done in systems that we consider traditionally bright and colorful, like birds, flowers and butterflies, but a lot of this color research is really biased by the human perception of color,” said Hayley Crowell, a doctoral student in the U-M Department of Ecology and Evolutionary Biology.



<h2 class="wp-block-heading" id="h-hidden-signals-in-the-uv-spectrum">Hidden signals in the UV spectrum</h2>



Crowell notes that much of the past work on UV color has concentrated on reproductive behaviors - things like UV ‘nectar guides’ in flowers that help steer insects to the part of the flower necessary for pollination.



In snakes, the team suspected UV coloration might be used for different reasons. Because snakes don’t typically rely on bright <a href="https://www.earth.com/news/new-camera-system-takes-photos-in-the-same-colors-that-different-animals-see/" target="_blank" rel="noreferrer noopener">colors</a> to find mates, the scientists hypothesized that UV might be associated more with camouflage or environmental signaling.



The researchers analyzed 110 snake species, collected in various regions ranging from Colorado to Peru. Many of the species examined in the study can see UV light in ways that humans cannot.&nbsp;



Using a specialized camera lens and filters, they captured images of the snakes, searching for ultraviolet reflection patterns. Importantly, they did not rely on black lights to observe fluorescence; instead, they looked at the UV color that the snakes naturally reflect - colors invisible to the human eye.



<h2 class="wp-block-heading" id="h-the-hidden-colors-of-snakes">The hidden colors of snakes</h2>



Next, the researchers tested how different factors - such as a snake’s age, sex, habitat, evolutionary background, and how visible the snake was to predators - might correlate with having more or less UV color.&nbsp;



To their surprise, the biggest driver of UV coloration turned out to be where and how the snakes live. Arboreal snakes that spend most of their time in trees and are active at night had the highest levels of UV reflection.



“<a href="https://www.earth.com/news/some-birds-use-snake-skins-in-their-nests-to-deter-predators/" target="_blank" rel="noreferrer noopener">Birds</a>, which can also see UV color, are one of snakes’ biggest predators,” Crowell explained.&nbsp;



For a nocturnal, tree-dwelling snake, sporting a heavy UV reflection might be inconsequential at night - but can provide camouflage during the day, when birds are actively hunting.&nbsp;



Leaves, lichens, and other vegetation are all known to reflect UV light. Thus, a snake displaying UV patterns could blend seamlessly into its sunlit habitat.



<h2 class="wp-block-heading" id="h-surprising-lack-of-sex-differences">Surprising lack of sex differences</h2>



One unexpected finding was that UV patterns did not differ substantially between male and female snakes.&nbsp;



“Because reproduction drives UV color evolution in so many other species, the lack of sexual differences in snakes was a surprise,” said study co-author Alison Davis Rabosky, an associate professor of ecology and evolutionary biology at U-M.&nbsp;



“But I don’t think snakes are actually some kind of outlier doing color ‘differently’ than other animals. I think we scientists have simply overlooked a lot of UV coloration in cryptically colored species, especially in insects. They are the next frontier.”



Snakes are closely related to <a href="https://www.earth.com/news/lizards-take-bigger-risks-when-they-are-hungry/" target="_blank" rel="noreferrer noopener">lizards</a>, and lizard species are known for strong sexual dimorphism - males often have flashier colors or bigger ornaments than females.&nbsp;



In contrast, the lack of color contrast between male and female snakes suggests that sexual selection may not drive color differences as much in snakes as it does in their lizard relatives.



<h2 class="wp-block-heading" id="h-intriguing-individual-variations">Intriguing individual variations</h2>



The researchers also found that some snakes of the same species, same sex, and from the same location could differ dramatically in UV reflectance levels.&nbsp;



Two individuals might look nearly identical in the visible color spectrum, but one reflects UV strongly and the other does not. This highlights the complexity of color usage - humans simply cannot see it, so the reasons behind these differences remain obscure.



Similarly, evolutionary relationships among snakes didn’t always predict UV usage: some closely related species varied significantly in the presence or intensity of UV reflectance.&nbsp;



Even within the same genus, the team found both strongly UV-reflective and barely UV-reflective species or populations.



<h2 class="wp-block-heading" id="h-reassessing-our-vision-of-animal-color">Reassessing our vision of animal color</h2>



The new research underscores the concept that just focusing on colors visible to humans could hide a great deal of evolutionary strategy.&nbsp;



By revealing that snakes employ UV coloration widely - often for camouflage and not for sex-based selection - this study challenges assumptions about how color is used throughout the animal kingdom.&nbsp;



“I think what’s so exceptional about this study is that we got to look at patterns of UV color across so many species and individuals,” said co-author Hannah Weller, a postdoctoral research fellow at the <a href="https://www.helsinki.fi/en" target="_blank" rel="noreferrer noopener">University of Helsinki</a>. 



“This amazing dataset really helped us start to understand just how variable a trait like this is, even in a group where we wouldn’t expect it.”



Ultimately, the researchers hope to inspire further investigations of UV coloration in other less-studied animal groups, especially among those perceived by humans as drab or colorless.



The study is published in the journal <a href="https://dx.doi.org/10.1038/s41467-024-49506-4" target="_blank" rel="noreferrer noopener">Nature Communications</a>.&nbsp;



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Snakes use invisible colors to outsmart predators

When thinking about why animals look the way they do,...

As the planet heats up and Antarctica’s ice sheet melts at a faster pace, scientists warn of a steady rise in sea levels that could put coastal communities at risk.&nbsp;



Home to enough frozen water to increase global sea levels by 190 feet if completely melted, Antarctica remains a focus of intense scientific scrutiny.&nbsp;



Yet most climate models struggle to capture the complexities of its ice movement due to limited direct observations and the interplay between ocean currents, atmospheric conditions, and the frozen surface.



In a paper published in the journal <a href="http://dx.doi.org/10.1126/science.adp3300" target="_blank" rel="noreferrer noopener">Science</a>, a team from <a href="https://www.stanford.edu/" target="_blank" rel="noreferrer noopener">Stanford University</a> utilized machine learning to analyze high-resolution remote-sensing data of Antarctic ice movements.&nbsp;



<h2 class="wp-block-heading" id="h-insights-into-the-behavior-of-ice-nbsp">Insights into the behavior of ice&nbsp;</h2>



By combining large volumes of satellite imagery with established physical principles, their approach identifies fundamental processes governing the large-scale flow of ice on the continent. 



The resulting insights could help refine how existing models estimate Antarctica’s future and the associated threat of accelerating <a href="https://www.earth.com/news/coastal-cities-will-spend-over-3-trillion-dollars-damages-from-sea-level-rise/" target="_blank" rel="noreferrer noopener">sea-level rise</a>.



Ching-Yao Lai is an assistant professor of geophysics at the Stanford Doerr School of Sustainability and senior author of the study.&nbsp;



“A vast amount of observational data has become widely available in the satellite age,” said Professor Lai. “We combined that extensive observational dataset with physics-informed deep learning to gain new insights about the behavior of ice in its natural environment.”



<h2 class="wp-block-heading" id="h-a-critical-component-of-global-climate">A critical component of global climate</h2>



Antarctica’s <a href="https://www.earth.com/news/antarctic-ice-sheet-past-present-and-future/" target="_blank" rel="noreferrer noopener">ice sheet</a> is Earth’s largest reservoir of frozen water, nearly twice the size of Australia. Acting like a vast sponge for the planet, it plays a pivotal role in regulating global sea levels. 



Understanding how this sheet moves and melts is essential as its rate of shrinkage increases every year.



Historically, researchers have relied on laboratory experiments to approximate Antarctic ice’s mechanical properties. However, simulating real Antarctic ice in a lab can be deceptively simplistic, explained Professor Lai.&nbsp;



<h2 class="wp-block-heading" id="h-finding-patterns-in-antarctica-s-ice">Finding patterns in Antarctica’s ice </h2>



Factors such as variations between seawater-derived ice and snow-compacted ice, or the presence of cracks, air voids, and other irregularities, all contribute to ice movement in nature.



“These differences influence the overall mechanical behavior, the so-called constitutive model, of the ice sheet in ways that are not captured in existing models or in a lab setting,” Lai said.



Rather than tackling every variable individually, the Stanford-led team used a <a href="https://www.earth.com/news/how-machine-learning-can-help-us-protect-chimpanzees/" target="_blank" rel="noreferrer noopener">machine learning</a> model to assess large-scale patterns in the movement and thickness of ice. 



This model used satellite images and airplane radar data from 2007 to 2018, while adhering to basic physical laws that regulate ice flow.



<h2 class="wp-block-heading" id="h-variations-in-ice-shelf-dynamics">Variations in ice shelf dynamics</h2>



The researchers examined five Antarctic ice shelves - floating extensions of land-based <a href="https://www.earth.com/news/melting-glaciers-are-reshaping-landscapes-and-national-borders-around-the-world/" target="_blank" rel="noreferrer noopener">glaciers</a>. These shelves maintain stable levels of continental ice by keeping large amounts of it from sliding outright into the ocean.&nbsp;



The experts discovered that areas of the shelves closer to land experience strong compression, a characteristic that aligns with typical lab-derived models for ice dynamics. 



However, ice located farther offshore experiences extension, causing it to respond differently in different directions - a phenomenon known as anisotropy.



Study first author Yongji Wang completed the project as a postdoctoral researcher in Lai’s lab and is now a postdoctoral researcher at <a href="https://www.nyu.edu/" target="_blank" rel="noreferrer noopener">New York University</a>.&nbsp;



“Our study uncovers that most of the ice shelf is anisotropic,” said Wang. “The compression zone - the part near the grounded ice - only accounts for less than 5% of the ice shelf. The other 95% is the extension zone and doesn’t follow the same law.”



This finding undermines a key assumption in many climate models that treat ice as the same in every direction. Real conditions, Wang’s analysis indicates, are considerably more nuanced.



“People thought about this before, but it had never been validated,” Wang added. “Now, based on this new method and the rigorous mathematical thinking behind it, we know that models predicting the future evolution of Antarctica should be anisotropic.”



<h2 class="wp-block-heading" id="h-consequences-for-coastal-areas">Consequences for coastal areas</h2>



Understanding these complex ice dynamics is crucial, especially as polar regions warm rapidly. Rising seas already cause intensifying floods, <a href="https://www.earth.com/news/fighting-coastal-erosion-electricity-turns-sand-into-a-sea-wall/" target="_blank" rel="noreferrer noopener">coastal erosion</a>, and severe storm damage.&nbsp;



Models that overgeneralize the ice’s properties may underestimate or misjudge how fast Antarctica’s ice sheets can collapse or produce icebergs - a process called calving.



Moreover, the scientists note that many existing models have assumed the Antarctic ice sheet’s mechanical behavior is uniform. This oversimplification could translate into significant inaccuracies in projections about melt rates and sea-level rise.



<h2 class="wp-block-heading" id="h-new-understanding-of-earth-processes">New understanding of Earth processes </h2>



This project exemplifies an emerging strategy that merges “big data” with fundamental physics in Earth science research.&nbsp;



Professor Lai emphasized that while machine learning can discover patterns from enormous sets of satellite images, scientists must still ensure the results adhere to the time-tested laws of physics that govern planetary processes.



“We are trying to show that you can actually use AI to learn something new,” Lai said. “It still needs to be bound by some physical laws, but this combined approach allowed us to uncover ice physics beyond what was previously known and could really drive new understanding of Earth and planetary processes in a natural setting.”



Since the data used here extend only to 2018, the team’s next steps include refining their technique with newly available images and radar signals.&nbsp;



The researchers also plan to apply the method to other parts of the Antarctic continent and possibly beyond, gleaning more clues about how these massive frozen landscapes might evolve under accelerating climate change.



<h2 class="wp-block-heading" id="h-guiding-adaptation-strategies-nbsp">Guiding adaptation strategies&nbsp;</h2>



As researchers plug these results into broader climate simulations, the hope is that predictions about rising oceans will incorporate Antarctica’s real-world complexities more faithfully.&nbsp;



Policymakers and coastal communities around the globe stand to benefit from improved forecasts to guide adaptation strategies - from planning dikes to restoring coastal wetlands.



Ultimately, the fusion of machine learning with physical knowledge marks a powerful advance in unraveling how Antarctica’s ice moves and melts.&nbsp;



By better capturing small-scale differences across the continent’s ice shelves, scientists can glean deeper insights into the largest reservoir of freshwater on the planet - and how its future may shape the global coastline in coming decades.



Image Credit: NASA's Goddard Space Flight Center Scientific Visualization Studio



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Antarctica’s hidden ice dynamics will redefine sea level projections

As the planet heats up and Antarctica’s ice sheet melts...

With spring approaching, many people are already considering which flowers to plant. Flowers do more than simply make gardens look nice. They are an important source of food for birds and insects, particularly wild bees.



In cities, the appropriate combination of flowers can be the difference between healthy bee populations and unhealthy ones.



A recent study has explored how the properties of flowers affect urban <a href="https://www.earth.com/news/flower-strips-can-boost-wild-bee-populations/" target="_blank" rel="noreferrer noopener">bee populations</a>. 



The researchers discovered that a diverse range of flower sizes and shapes is crucial for supporting wild bee populations. A more varied floral landscape promotes a richer and more abundant bee community.



<h2 class="wp-block-heading" id="h-why-flower-shape-and-size-matter">Why flower shape and size matter</h2>



Study co-author Carly Ziter is an associate professor in the Department of Biology in the Faculty of Arts and Science at <a href="https://www.concordia.ca/" target="_blank" rel="noreferrer noopener">Concordia University</a>.



"We know that flowers are an important source of nutrition for bees, but not all flowers are created equal," said Professor Ziter.



"Having a high <a href="https://www.earth.com/news/new-secrets-of-flower-diversity-revealed/" target="_blank" rel="noreferrer noopener">diversity of flowers</a> is a key to supporting bee populations, but our research goes one step further to show a possible mechanism: that having a diversity of floral species is important because they have different shapes and sizes."



Flowers store <a href="https://www.earth.com/news/honeybees-carrying-nectar-avoid-overheating-rising-temperatures/" target="_blank" rel="noreferrer noopener">nectar</a> within their corolla - the tube-like structure formed by a ring of <a href="https://www.earth.com/news/plants-engineer-their-petals-to-be-visually-attractive-to-bees/" target="_blank" rel="noreferrer noopener">petals</a>. Different bee species have different tongue lengths, which means some bees can only access nectar from specific flower shapes.



"This follows the idea of size-matching, where corollas are the right size for a certain type of bee’s proboscis or tongue, allowing it to effectively connect to the flower’s nectar," noted Professor Ziter.



"So, whether a bee has a short or longer proboscis, they will be able to access the nutrition they need if there are multiple kinds of flower morphology nearby."



<h2 class="wp-block-heading" id="h-tracking-bees-in-the-city">Tracking bees in the city</h2>



The team collected data in July 2020 from 16 sites across the Island of Montreal, including community gardens, nature parks, and cemeteries.



The researchers recorded nearly 2,000 bee samples and identified 150 different <a href="https://www.earth.com/news/study-reveals-that-90-of-flowering-plant-species-rely-on-animal-pollinators/" target="_blank" rel="noreferrer noopener">species of flowers</a> within small two-by-two-meter plots.



The density of flowers was measured, and the size of each corolla was documented using digital calipers.



A total of 94 different species of bees were observed during the study. While nectar samples were also collected, no firm connection was established between sugar content and bee diversity.



<h2 class="wp-block-heading" id="h-plant-diversity-and-the-food-web">Plant diversity and the food web</h2>



"We wanted to see if there was an optimal value for corolla traits," said Professor Ziter. "Was it better to have small corollas, medium ones, or a diversity of them? The results showed quite strongly that having a diversity of corolla sizes was important."



Thriving bee populations play a vital role in <a href="https://www.earth.com/news/robotic-insects-may-be-the-future-of-farming-and-plant-pollination/" target="_blank" rel="noreferrer noopener">pollination</a>, supporting entire ecosystems and sustaining food supplies.



According to Professor Ziter, the study supports the belief that a diversity of flowers impacts the next trophic level, which contributes to an ecosystem’s food web in a way that goes far beyond bees. 



<h2 class="wp-block-heading" id="h-how-to-make-your-garden-bee-friendly">How to make your garden bee-friendly</h2>



City planners, gardeners, and anyone interested in promoting biodiversity can apply these findings in practical ways.



"If you are planting, try to think about what makes these species different. Are they different colors? Are they different sizes? Do they bloom at different times? The more you can think about these different axes of variety in your own garden, the more you are likely to be better off in terms of supporting biodiversity," said Professor Ziter.



By planting a diverse mix of flowers, urban residents can play a small but significant role in sustaining local bee populations and contributing to a healthier environment.



<h2 class="wp-block-heading" id="h-choosing-the-right-flowers-for-bees">Choosing the right flowers for bees</h2>



For a bee-friendly garden, native plants are often the best choice since they have co-evolved with local species and provide the most suitable nectar and pollen.



Flowers with open, accessible petals are ideal for short-tongued bees, while tubular flowers cater to species with longer proboscises.



Bloom timing is another crucial factor. By planting a variety of flowers that bloom at different times throughout the growing season, gardeners can ensure a steady food supply for bees from early spring to late fall. 



Perennial flowers such as coneflowers, milkweed, and goldenrod are excellent choices, as they return each year and require minimal maintenance.



Avoiding pesticide use and opting for organic gardening practices further enhances the bee-friendly environment. 



The full study was published in the journal <a href="https://esajournals.onlinelibrary.wiley.com/doi/10.1002/eap.3067" target="_blank" rel="noreferrer noopener">Ecological Applications</a>.



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Bee-friendly gardening: Why flower diversity is so important

With spring approaching, many people are already considering which flowers...

Physical activity is often linked to a longer life, but a Finnish twin study suggests the connection may not be as direct as previously thought. The findings challenge traditional assumptions about exercise and aging.



Researchers from the University of Jyväskylä examined how long-term physical activity affects mortality and whether it can counteract genetic risks for disease. The team also explored role of exercise in biological aging.



The experts analyzed 22,750 Finnish twins born before 1958. Their leisure-time <a href="https://www.earth.com/news/exercise-reduces-the-risk-of-brain-diseases-by-up-to-54-percent/" target="_blank" rel="noreferrer noopener">physical activity</a> was assessed in 1975, 1981, and 1990. The researchers followed up on mortality data through the end of 2020. 



<h2 class="wp-block-heading" id="h-moderate-activity-yields-maximum-benefits">Moderate activity yields maximum benefits</h2>



The researchers identified four activity groups: sedentary, moderately active, active, and highly active. Over 30 years, the biggest difference was found between the sedentary and moderately active groups.



Moderately active individuals had a 7% lower mortality risk. However, those in the highly active group did not show additional <a href="https://www.earth.com/news/strength-training-may-be-the-best-exercise-for-insomnia/" target="_blank" rel="noreferrer noopener">benefits</a>.



In the short term, more physical activity correlated with lower mortality. However, in the long run, highly active individuals had no advantage over those who were sedentary.



“An underlying pre-disease state can limit physical activity and ultimately lead to death, not the lack of exercise itself,” said Professor Elina Sillanpää from the Faculty of Sports and Health Sciences.



“This can bias the association between <a href="https://www.earth.com/news/small-doses-of-exercise-can-greatly-reduce-dementia-risk/" target="_blank" rel="noreferrer noopener">physical activity</a> and mortality in the short term.”



<h2 class="wp-block-heading" id="h-exercise-guidelines-and-mortality-risk">Exercise guidelines and mortality risk</h2>



The experts also evaluated whether following World Health Organization (<a href="https://www.who.int" target="_blank" rel="noreferrer noopener">WHO</a>) physical activity guidelines influenced mortality and genetic disease risk. The WHO recommends 150–300 minutes of moderate or 75–150 minutes of vigorous activity weekly.



The results of the study showed that meeting these guidelines did not lower mortality risk. Even twins who followed the recommendations for 15 years showed no significant difference in mortality rates compared to their less active siblings.



"The widely observed favorable association between <a href="https://www.earth.com/news/fitness-focused-medicine-physical-activity-reduces-chronic-disease-risk/" target="_blank" rel="noreferrer noopener">physical activity</a> and mortality are based on observational studies that are prone to bias from different sources,” noted postdoctoral researcher Laura Joensuu.



“In our studies, we aimed to account for various sources of biases, and combined with the long follow-up period, we could not confirm that adhering to physical activity guidelines mitigates genetic cardiovascular disease risk or causally reduces mortality.”



<h2 class="wp-block-heading" id="h-exercise-and-biological-aging">Exercise and biological aging</h2>



For a subset of twins, the researchers analyzed biological aging using epigenetic clocks. These clocks estimate biological aging based on chemical markers that regulate gene activity.



The results showed a U-shaped pattern. Both the least and most active individuals experienced accelerated biological aging.



“We found that the association between leisure-time physical activity and biological aging was U-shaped: Biological aging was accelerated in those who exercised the least and the most,” said Sillanpää.



Lifestyle factors like smoking and alcohol use played a major role in the link between <a href="https://www.earth.com/news/fitness-is-far-more-important-than-weight-for-living-a-healthy-life/" target="_blank" rel="noreferrer noopener">physical activity</a> and biological aging. The study also examined genetic susceptibility to coronary artery disease and blood pressure using polygenic risk scores.



<h2 class="wp-block-heading" id="h-more-exercise-does-not-slow-aging">More exercise does not slow aging</h2>



This research challenges the widely held belief that more exercise always leads to a longer life. 



While physical activity is beneficial for overall health, its impact on longevity is more complicated than previously assumed. Moderate exercise appears to offer the best balance, while excessive activity does not necessarily add extra years to life.



The findings also highlight the importance of considering other factors, such as lifestyle habits and genetic predisposition. Exercise alone may not be enough to overcome genetic risks. Other aspects of health, such as diet, stress management, and avoiding harmful habits, play a crucial role in aging and longevity.



Future research may further clarify the relationship between physical activity and lifespan. In the meantime, individuals should aim for a balanced approach to exercise, focusing on overall well-being rather than just lifespan extension.



The study involved researchers from the Faculty of Sport and Health Sciences and the Methodology Centre for Human Sciences at the <a href="https://www.jyu.fi/en" target="_blank" rel="noreferrer noopener">University of Jyväskylä</a>. Experts at the Finnish Institute of Molecular Medicine at the <a href="https://www.helsinki.fi/en" target="_blank" rel="noreferrer noopener">University of Helsinki</a> also contributed.



The findings are published in the <a href="https://link.springer.com/article/10.1007/s10654-024-01200-x" target="_blank" rel="noreferrer noopener">European Journal of Epidemiology</a>.



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Exercise and aging: New study reveals a surprising connection

Physical activity is often linked to a longer life, but...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

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

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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...

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Today’s Video of the Day from <a href="https://www.igb.illinois.edu/">Carl R. Woese Institute for Genomic Biology</a> reveals how scientists can modify common crops like soybean, rice, and wheat to protect them from heat stress.



“We need to double crop production by 2050 to feed a growing global population, and not only are we not on track to do that, but climate change is further complicating things,” said Amanda Cavanagh, a lecturer at the University of Essex. 



The study is part of Realizing Increased Photosynthetic Efficiency (RIPE), an international research project that aims to develop food crops that turn the sun’s energy into food more efficiently.



“Using an engineering approach we designed multiple alternative metabolic pathways to photorespiration. Testing them in the field showed increases in productivity which led Amanda to significantly move the project forward by showing our engineered plants can withstand pretty extreme temperature stress,” said study co-author and RIPE researcher Paul South.&nbsp;



“As the climate changes and temperature stresses increase the pressure on our global food supply, farmers will need every tool available including engineering approaches like the synthetic biology used here to maintain safe and productive harvests.”



The experts tested plants modified to have more efficient photorespiration to see if they were better adapted to warmer temperatures.&nbsp;



The team found that the engineered plants produced 26 percent more biomass than the wild-type plants exposed to the same temperatures, and had 15 percent less yield loss under the higher temperatures.



Video Credit: Amanda Nguyen/University of Illinois



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



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

Designing crops that can beat the heat

[sendtonews key="QGPzYnXEtN-1712599-12187" type="single"] Today’s Video of the Day from Carl...

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