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 the European Space Agency...

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



The <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lake</a> was created in the late 1970s as a 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 members of theTriatominae are also known as conenose bugs, kissing bugs (so-called from their habit of feeding from around the mouths of people), or vampire bugs. In areas where Changas disease occurs (from the southern United States to northern Argentina), all triatomine species are potential vectors of the Chagas disease parasite Trypanosoma cruzi. Also, proteins released from their bites have been known to induce anaphylaxis in sensitive and sensitized individuals.  Photo Credit: Vanessa Becker-Miller

Kissing Bugs

A new study suggests that children who consumed the least seafood at age seven exhibited lower prosocial behavior at both seven and nine years old. Prosocial behavior - such as friendliness, sharing, and altruism - appeared to be positively linked to fish consumption.



Seafood provides key nutrients, including omega-3 fatty acids, selenium, iodine, vitamin D, and choline. These nutrients contribute to a balanced diet and support brain development. 



Experts recommend children eat at least two servings of <a href="https://www.earth.com/news/boosting-seafood-production-while-protecting-biodiversity/" target="_blank" rel="noreferrer noopener">fish</a> weekly, with one serving from oily fish like salmon or mackerel.



<h2 class="wp-block-heading" id="h-seafood-consumption-and-child-behavior">Seafood consumption and child behavior</h2>



Researchers from the <a href="https://www.bristol.ac.uk">University of Bristol</a> analyzed data from 5,969 participants in the Children of the 90s study. This long-term research received £5.2 million ($6.6 million) in new funding. The study adjusted data for social and demographic factors, ensuring accurate results.



Previous research was primarily focused on fish consumption during pregnancy. The effects were examined on babies rather than children’s ongoing development. 



However, the current study highlights the importance of research on fish intake during childhood.



The findings showed that children who did not eat <a href="https://www.earth.com/news/shrimp-crisis-alarming-virus-threatens-global-seafood-supplies/" target="_blank" rel="noreferrer noopener">seafood</a> had a 35% higher risk of developing lower prosocial behavior at age seven and a 43% higher risk at age nine.



Those who consumed between 1-190g of seafood per week still had a 25-30% higher risk compared to those who met the NHS recommendation of at least 190g per week.



<h2 class="wp-block-heading" id="h-concerns-about-seafood-consumption">Concerns about seafood consumption</h2>



Many children in the study ate less seafood than NHS recommendations. One reason may be concerns about pollutants like mercury. 



Parents often receive mixed messages about seafood safety, making dietary choices difficult. However, experts note that the benefits of <a href="https://www.earth.com/news/why-eating-farmed-fish-may-be-safer-than-eating-fish-caught-in-the-wild/" target="_blank" rel="noreferrer noopener">fish</a> consumption outweigh potential risks when intake follows guidelines.



Prosocial behavior develops between ages one and two. It becomes more complex as children grow. Encouraging these behaviors early supports social development and overall well-being. Good nutrition plays a vital role in this process.



<h2 class="wp-block-heading" id="h-essential-nutrients-in-brain-development">Essential nutrients in brain development</h2>



Seafood is a primary source of omega-3 fatty acids like DHA and EPA, which support brain function and emotional well-being. While the body can produce small amounts of DHA from other sources, dietary intake is necessary to maintain optimal levels.



Iodine and selenium also contribute to neurodevelopment. Iodine plays a crucial role in thyroid hormone production, which regulates brain growth. 



Selenium supports antioxidant functions and helps with thyroid hormone metabolism. Choline aids in neurotransmitter production, which impacts memory and cognitive function. Vitamin D supports calcium absorption and immune function, contributing to overall <a href="https://www.earth.com/news/microplastics-are-widespread-in-the-seafood-we-eat/" target="_blank" rel="noreferrer noopener">health</a>.



The study measured prosocial behavior using questionnaires. Parents reported their child’s social interactions at ages seven and nine. The results showed that children who ate more seafood displayed better social behavior.



The researchers also investigated a possible link between seafood intake and IQ. However, they found no significant connection between fish consumption and intelligence.



<h2 class="wp-block-heading" id="h-seafood-and-child-development">Seafood and child development</h2>



"When there’s conflicting advice, it can be difficult to know what the best course of action is. Our previous studies have shown that eating fish during pregnancy in the UK can have a positive effect on child development," noted Dr. Caroline Taylor, associate professor of nutrition at the University of Bristol.



"This has also been found in countries where fish intakes are higher than they are here, so encouraging fish consumption is likely to have a positive effect on child development."



Dr. Taylor said the evidence to link fish consumption in children with the best behavioral development is clear, and that her team strongly recommends for parents to provide at least two portions of <a href="https://www.earth.com/news/plastic-particles-found-in-99-of-tested-seafood-samples/" target="_blank" rel="noreferrer noopener">fish</a> a week in accordance with NHS guidelines. 



"We hope these research findings empower parents with the knowledge to give their children the best start in life.”



<h2 class="wp-block-heading" id="h-public-health-considerations">Public health considerations</h2>



The <a href="https://www.nhs.uk" target="_blank" rel="noreferrer noopener">NHS</a> advises that children should consume two portions of seafood per week, including one portion of oily fish. However, girls should have no more than two portions of oily fish per week due to concerns about dioxins and PCBs, which can accumulate in the body over time.



The FAO/WHO has acknowledged the benefits of seafood at all life stages. However, they also stress the need for region-specific guidelines based on local fish contamination levels, nutrient content, and dietary patterns.



Data from the <a href="https://www.gov.uk/government/collections/national-diet-and-nutrition-survey" target="_blank" rel="noreferrer noopener">UK National Diet and Nutrition Survey</a> show that children consume less than the recommended amount of seafood. Many factors contribute to this, including concerns about mercury, taste preferences, cost, and limited availability. 



Addressing these barriers through public health campaigns could help improve childhood nutrition.



<h2 class="wp-block-heading" id="h-long-term-study-continues-nbsp">Long-term study continues&nbsp;</h2>



<a href="https://www.bristol.ac.uk/alspac/" target="_blank" rel="noreferrer noopener">Children of the 90s</a> study has played a major role in health research for over three decades. Founded by Professor Jean Golding in the early 1990s, the study has contributed to more than 3,000 research papers.



With the recent £5.2 million funding boost, the study will continue its research. The focus will now extend to the third generation of participants. These efforts will provide valuable insights into child health and development for years to come.



The study is published in the <a href="https://link.springer.com/article/10.1007/s00394-025-03636-7" target="_blank" rel="noreferrer noopener">European Journal of Nutrition</a>.



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Eating seafood helps children develop better social behaviors

A new study suggests that children who consumed the least...

Human societies often focus on dangers that exist here on Earth, but there are moments when the threats might come from much farther away.



Scientists have long wondered about cosmic events that can affect our planet’s biology. Some have been exploring whether powerful stellar explosions could be tied to catastrophic shifts in Earth’s distant past.



The idea that blasts from massive stars might have influenced global conditions is catching attention. 



Two large-scale losses of life have drawn renewed interest from researchers who see a pattern in the timing of star explosions and severe changes in Earth’s environment.



In a new study from <a href="https://www.keele.ac.uk/" target="_blank" rel="noreferrer noopener">Keele University</a>, lead author Dr. Alexis Quintana, formerly of Keele and now at the <a href="https://www.ua.es/en/" target="_blank" rel="noreferrer noopener">University of Alicante</a>, worked with Dr. Nick Wright from Keele to examine the distribution of massive stars in our region of the galaxy.



The study found that the rate of these stars going supernova near Earth appears to match two large ancient losses of life that happened 372 million years ago and 445 million years ago.



<h2 class="wp-block-heading" id="h-past-mass-extinctions">Past mass extinctions</h2>



Scientists refer to these moments in Earth’s past as the late <a href="https://www.earth.com/news/worlds-newest-oldest-forest-recently-discovered-is-full-of-calamophyton-trees/" target="_blank" rel="noreferrer noopener">Devonian</a> and <a href="https://www.earth.com/news/tiny-worms-sparked-explosive-evolutionary-period-of-life-on-earth/" target="_blank" rel="noreferrer noopener">Ordovician</a> events. 



The first occurred about 372 million years ago and led to the disappearance of around 70 percent of all species, shifting the balance of aquatic life.



The second happened 445 million years ago, removing 60 percent of marine invertebrates at a time when life mostly existed in the sea.



Researchers have struggled to nail down a clear spark for those events, though many have pointed to an erosion of the <a href="https://www.earth.com/news/the-ozone-layer-is-healing-will-the-hole-disappear-for-good/" target="_blank" rel="noreferrer noopener">ozone layer</a>. 



Some now propose that cosmic detonations may have stripped away that protective layer, allowing intense ultraviolet light to reach Earth’s surface.



<h2 class="wp-block-heading" id="h-supernovas-within-earth-s-reach">Supernovas within Earth's reach</h2>



The authors say it is "a great illustration for how massive stars can act as both creators and destructors of life". 



These stars generate heavy elements that make planets possible, but their demise can <a href="https://www.earth.com/news/t-coronae-borealis-nova-explosion-nearby-star-light-up-earths-skies/" target="_blank" rel="noreferrer noopener">produce bursts of radiation</a>.



The team embarked on what they call a “census” of nearby massive stars, known as OB stars, within around 3,260 light-years of the Sun.



OB stars are giants that can collapse under gravity when they run out of fuel, leading to an explosion that releases <a href="https://www.earth.com/news/star-collapse-black-hole-instead-of-supernova-vanish-from-sky/" target="_blank" rel="noreferrer noopener">intense waves of energy</a>.



The researchers then calculated how often these explosions might happen within 65 light-years of Earth, which is about 20 parsecs.



By comparing those estimates with the frequency of major losses of life linked to external triggers, they found a match that points to a nearby supernova as a likely suspect in the late Devonian and Ordovician events.



“We calculated the supernova rate close to Earth and found it to be consistent with the rate of mass extinction events on our planet that have been linked to external forces such as supernovae,” Dr Wright explained.



<h2 class="wp-block-heading" id="h-what-would-a-supernova-do-to-earth">What would a supernova do to Earth</h2>



The study suggests that a supernova near Earth might erode the ozone layer, spark chemical reactions that produce acid rain, and expose organisms to harmful solar radiation.



“Supernova explosions bring heavy chemical elements into the <a href="https://www.earth.com/news/astronomers-reveal-the-first-detailed-image-of-a-dying-star/" target="_blank" rel="noreferrer noopener">interstellar medium</a>, which are then used to form new stars and planets. Dr. Quintana explained. 



"But if a planet, including the Earth, is located too close to this kind of event, this can have devastating effects."



If enough shielding is lost, regions of the planet might become biologically hazardous. This could halt the growth of some organisms while allowing others to take over previously occupied niches.



Dr Wright added, “Supernova explosions are some of the <a href="https://www.earth.com/news/kilonova-explosion-light-years-away-would-devastate-earth/" target="_blank" rel="noreferrer noopener">most energetic explosions in the universe</a>. If a massive star were to explode as a supernova close to the Earth, the results would be devastating for life on Earth. This research suggests that this may have already happened.”



He and his colleagues see the new data as helpful for understanding how elements move around the galaxy and form the basis for new celestial objects.



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



Supernova events are believed to happen at a rate of about one or two per century in galaxies such as the Milky Way. The chance of one erupting in our immediate neighborhood is low, though not impossible.



The researchers note that stars like Antares and <a href="https://www.earth.com/news/supergiant-star-betelgeuse-may-have-a-buddy-causing-it-to-flicker/" target="_blank" rel="noreferrer noopener">Betelgeuse</a> might run out of fuel in the next million years or so, yet they sit far enough away that the effects on Earth are likely limited.



The project’s census of massive stars also aids in studying black holes and neutron stars, which arise from the aftermath of stellar collapses.



The data can support improvements to gravitational wave detectors, which help scientists pinpoint the origins and structure of cosmic events.



By refining how often massive stars explode, astronomers can hone their forecasts for how often <a href="https://www.earth.com/news/matter-spacetime-gravitational-waves-fabric-of-the-universe/" target="_blank" rel="noreferrer noopener">gravitational waves</a> ripple through space.



<h2 class="wp-block-heading" id="h-earth-supernovas-and-future-study">Earth, supernovas, and future study</h2>



Plenty of questions remain about the ways in which these explosions can set off harmful changes in Earth’s environment.



Some experts wonder how quickly the atmosphere recovers if solar radiation spikes. Others are curious if life on land reacts differently from life at sea when <a href="https://www.earth.com/news/extreme-particle-acceleration-new-source-of-cosmic-rays-discovered/" target="_blank" rel="noreferrer noopener">cosmic rays</a> increase.



Although researchers highlight a connection between supernovae and serious biological upheavals, there could be additional processes at work.



These blasts may seed the universe with valuable ingredients while also posing potential dangers when they happen too close for comfort.



The evidence is still coming together, but it points to a story where Earth’s ancient tragedies may have a cosmic explanation. Scientists plan to keep tracking massive stars in our galaxy to see what more can be learned.



The full study was published in the journal <a href="https://academic.oup.com/mnras/article/537/4/3332/8038277" target="_blank" rel="noreferrer noopener">Monthly Notices of the Royal Astronomical Society</a>.



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Two of Earth's mass extinctions were caused by something much worse than asteroids

Human societies often focus on dangers that exist here on...

Black holes have baffled and fascinated both scientists and the public for decades. Their enormous gravity and mysterious interiors have led to endless debates, movies and books feeding our curiosity about what might be hidden inside these cosmic objects.



Now, recent findings from the University of Sheffield point to surprising possibilities linked to time and dark energy.



Researchers suggest that black holes might shift into what they are calling “white holes,” which could throw matter and even time back out into our universe.



In simpler terms, this study proposes a revolutionary link between time and dark energy, suggesting that the mysterious force driving the universe's expansion may be used to measure time



This idea <a href="https://www.earth.com/news/radical-theory-unites-gravity-spacetime-and-the-quantum-realm/" target="_blank" rel="noreferrer noopener">challenges standard views</a> of how black holes function and basically upends everything we thought we knew about the Universe.



<h2 class="wp-block-heading" id="h-quantum-mechanics-and-the-singularity">Quantum mechanics and the singularity</h2>



Dr. Steffen Gielen, from the University of Sheffield’s School of Mathematical and Physical Sciences (<a href="https://www.sheffield.ac.uk/mps" target="_blank" rel="noreferrer noopener">MPS</a>), has long studied the interplay between <a href="https://www.earth.com/news/central-theory-of-quantum-gravity-is-modeled-in-the-laboratory/" target="_blank" rel="noreferrer noopener">quantum mechanics and gravity</a>.



His latest collaboration, entitled ‘Black Hole Singularity Resolution in Unimodular Gravity from Unitarity,’ is now published in Physical Review Letters.



In it, the authors explore how conventional knowledge breaks down at a black hole’s central point, known as the singularity.



“It has long been a question as to whether quantum mechanics can change our understanding of black holes and give us insights into their true nature,” said Dr. Gielen. 



“In <a href="https://www.earth.com/news/impossibility-paradox-calculating-incalculable-quantum-realm-particles/" target="_blank" rel="noreferrer noopener">quantum mechanics</a>, time as we understand it cannot end as systems perpetually change and evolve.”



<h2 class="wp-block-heading" id="h-linking-time-and-dark-energy">Linking time and dark energy</h2>



In this theoretical framework, the team positions dark energy as a potential measuring stick for time. 



They propose that <a href="https://www.earth.com/news/timescape-dark-energy-doesnt-exist-causing-lumpy-universe-expansion-cmbr/" target="_blank" rel="noreferrer noopener">dark energy</a>, thought to power the universe’s expansion, might function as a reference for temporal progression.



“While time is, in general, thought to be relative to the observer, in our research time is derived from the mysterious dark energy which permeates the entire universe,” Dr. Gielen continued.



“We propose that time is measured by the dark energy that is everywhere in the Universe, and responsible for its current expansion. This is the pivotal new idea that allows us to grasp the phenomena occurring within a black hole.”



By framing time through dark energy, the researchers open fresh avenues for interpreting how <a href="https://www.earth.com/news/new-evidence-suggests-that-dark-energy-comes-from-black-holes/" target="_blank" rel="noreferrer noopener">black holes could evolve</a>.



<h2 class="wp-block-heading" id="h-white-holes-as-a-new-phase">White holes as a new phase</h2>



White holes are often portrayed as the reverse of black holes. Instead of trapping matter forever, they are thought to expel energy, matter, and even time back into cosmic space.



In the Sheffield study, co-written with Lucía Menéndez-Pidal from <a href="https://www.ucm.es/english" target="_blank" rel="noreferrer noopener">Complutense University</a> of Madrid, this transformation from black hole to white hole occurs when quantum effects become significant at the singularity, replacing a terminal point with a new phase.



“Hypothetically you could have <a href="https://www.earth.com/news/schrodingers-cat-survives-in-quantum-superposition-for-a-record-shattering-23-minutes/" target="_blank" rel="noreferrer noopener">an observer</a> - a hypothetical entity - go through the black hole, through what we think of as a singularity and emerge on the other side of the white hole. It’s a highly abstract notion of an observer but it could happen, in theory,” Dr. Gielen added.



This scenario, though speculative, underscores the <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">evolving insights</a> into how physics might handle extreme conditions.



<h2 class="wp-block-heading" id="h-planar-vs-conventional-black-holes">Planar vs. conventional black holes</h2>



Their work relies on a simplified model known as a planar black hole. This version differs from conventional black holes, which are spherical, by featuring a flat boundary.



Despite the differences, the team believes that similar processes may apply to the black holes observed throughout space.



Any departure from the usual view of a singularity raises big questions about how time, space, and quantum effects unite.



By using quantum mechanics to show that a singularity could be replaced by fluctuating regions, the authors hint at a richer description of where <a href="https://www.earth.com/news/physicists-make-bold-claims-that-time-is-an-illusion-question-its-existence/" target="_blank" rel="noreferrer noopener">physics and time</a> continue to operate.



<h2 class="wp-block-heading" id="h-einstein-unimodular-gravity-and-spacetime">Einstein, unimodular gravity, and spacetime</h2>



Unimodular gravity, a version of Einstein’s theory that treats certain variables as fixed, plays a key role in this research.



In standard general relativity, the cosmological constant is an extra piece that can shape the universe’s expansion.



In unimodular gravity, this constant is partly integrated into how the theory sets up space and time.



Some physicists see it as a simpler way to handle <a href="https://www.earth.com/news/universe-expansion-rate-dark-energy-measured-11-billion-years-ago/" target="_blank" rel="noreferrer noopener">dark energy</a> because it can separate how gravity affects geometry from how energy drives cosmic growth.



In this study, unimodular gravity underpins the argument that <a href="https://www.earth.com/news/why-the-universe-remains-predictable-insights-from-quantum-mechanics/" target="_blank" rel="noreferrer noopener">black hole singularities</a> might not mark the end of time.



By adjusting the underlying equations, the approach provides a path to include quantum effects that keep space and time going.



This aligns with the hypothesis that matter and time could be released as a white hole forms.



Though questions remain about how these mathematical insights translate to actual observations, this framework adds another dimension to discussions of <a href="https://www.earth.com/news/powerful-forces-have-made-the-structure-of-the-universe-messier/" target="_blank" rel="noreferrer noopener">cosmic evolution</a>.



<h2 class="wp-block-heading" id="h-white-holes-and-new-textbooks">White holes and new textbooks</h2>



To sum it all up in a tidy package, these researchers are suggesting that black holes may transform into white holes that release matter and time, overturning old ideas and hinting at a new link between dark energy and our measure of time. 



They present a model where black holes don’t end in singularities but shift into regions of quantum fluctuations, and they believe this perspective could unify quantum mechanics and gravity.



From this theory, the scientists see potential for connecting these ideas with efforts to merge gravity and quantum mechanics.



Such approaches could reshape our understanding of how cosmic expansion, dark energy, and black holes fit together in a single theoretical picture.



The new research also suggests novel approaches to reconciling gravity and quantum mechanics, potentially paving the way for transformative new fundamental theories and breakthroughs in our understanding of the universe.



As these ideas progress, scientists will continue testing how dark energy and quantum processes might shed light on the puzzle at the heart of these powerful cosmic objects.



May the force be with us all.



The full study was published in the journal <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.134.101501" target="_blank" rel="noreferrer noopener">Physical Review Letters</a>.



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'White holes' change everything: Don't just rewrite the textbooks, throw them away

Black holes have baffled and fascinated both scientists and the...

Barnard’s Star has long been a focus of interest for people who study worlds beyond our solar system. It sits about six light-years from Earth and is known for its quick motion across our sky.



For years, astronomers have wondered whether it might harbor planets that could help us understand how planetary systems form.



Now, they seem to have gotten their wish. Recent observations suggest there may be four miniature planets orbiting Barnard’s Star.



Each is calculated to be just 20 to 30% the mass of Earth and completes one full trip around the star in only a few days.



These findings have caught many people’s attention because they point to greater precision in detecting smaller, more elusive planets.



“It’s a really exciting find - Barnard’s Star is our cosmic neighbor, and yet we know so little about it,” said Ritvik Basant, Ph.D. student at the <a href="https://www.uchicago.edu/en" target="_blank" rel="noreferrer noopener">University of Chicago</a> and first author on the study. “It’s signaling a breakthrough with the precision of these new instruments from previous generations.”



<h2 class="wp-block-heading" id="h-understanding-barnard-s-star-the-basics">Understanding Barnard’s Star - the basics</h2>



Barnard’s Star first came to light in 1916, thanks to astronomer E. E. Barnard at <a href="https://yerkesobservatory.org/" target="_blank" rel="noreferrer noopener">Yerkes Observatory</a>. Ever since, scientists have been keeping an eye on it.



They nicknamed it a “great white whale” because people have often claimed to see planets there, only to be disappointed later. This time, the work is featured in The Astrophysical Journal Letters, dated March 11.



Observers used to rely on less sensitive equipment, which sometimes produced conflicting signals. That is one reason the star became such a legend among planet hunters, who occasionally thought they had proof but eventually realized their results were inconclusive.



Experts point out that Barnard’s Star is the closest single-star system after the Sun. In contrast, the nearest star system overall, <a href="https://www.earth.com/news/new-telescopes-can-directly-detect-signs-of-alien-life-in-exoplanet-atmospheres/" target="_blank" rel="noreferrer noopener">Proxima Centauri</a>, has three stars in a gravitational dance.



The difference matters because multiple stars complicate how planets might form, so an M dwarf star with just one companion star suggests a different environment for potential worlds.



<h2 class="wp-block-heading" id="h-hunting-planets-with-maroon-x">Hunting planets with MAROON-X</h2>



Astronomers cannot directly see tiny planets close to bright stars. Instead, they track the gentle pull each planet exerts on its star. 



A specialized instrument called <a href="https://www.gemini.edu/instrumentation/maroon-x" target="_blank" rel="noreferrer noopener">MAROON-X</a>, installed on the Gemini Telescope in Hawaii, can detect faint wobbles in a star’s light signal. With this approach, the group detected three planets around Barnard’s Star. 



The fourth emerged when they combined their work with data from an earlier observation, taken by an instrument called ESPRESSO in Chile.



“We observed at different times of night on different days. They’re in Chile; we’re in Hawaii. Our teams didn’t coordinate with each other at all,” said Basant. “That gives us a lot of assurance that these aren’t phantoms in the data.”



<h2 class="wp-block-heading" id="h-barnard-s-star-s-planets">Barnard's Star's planets</h2>



Scientists suspect the new finds are small, rocky worlds, though exact compositions are hard to confirm. 



The angle from Earth means these planets do not appear to pass in front of their star, so the usual tests to identify rock or gas are out of reach. 



However, these orbits are probably far too close to the star for comfortable conditions.



“We worked on this data really intensely at the end of December, and I was thinking about it all the time," reflected Jacob Bean, a professor at the University of Chicago.



“It was like, suddenly we know something that no one else does about the universe. We just couldn’t wait to get this secret out," Bean added.



A sense of excitement fueled the entire project. 



“A lot of what we do can be incremental, and it’s sometimes hard to see the bigger picture,” Bean enthused. “But we found something that humanity will hopefully know forever. That sense of discovery is incredible.”



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



Barnard’s Star’s four worlds rank among the tiniest bodies confirmed with such radial velocity tools. 



Many <a href="https://www.earth.com/news/exotic-worlds-tess-unveils-126-new-exoplanets/" target="_blank" rel="noreferrer noopener">rocky exoplanets</a> discovered so far tend to be larger than Earth, and patterns among them appear consistent across the galaxy. 



Astronomers want to see if smaller ones show diverse compositions that might hint at how they form. 



M dwarfs, which are abundant in the universe, are known to have intense magnetic activity, and that may affect how planets develop. 



<h2 class="wp-block-heading" id="h-why-barnard-s-star-s-planets-are-important">Why Barnard's Star's planets are important</h2>



Understanding these processes could unlock clues about which stars are most likely to host stable surfaces.



Some hope these insights will guide future searches for life, even though these particular worlds lie in scorching territory. 



Researchers will keep refining their techniques to look for planets in more temperate zones. Each fresh advance in instrumentation increases the odds of uncovering new surprises. 



Additional surveys may also shed light on whether tiny planets form more often around cooler stars, or if conditions for habitability vary in unexpected ways. 



With every improved telescope, the possibility of spotting something remarkable grows.



The full study was published in <a href="https://iopscience.iop.org/article/10.3847/2041-8213/adb8d5" target="_blank" rel="noreferrer noopener">The Astrophysical Journal Letters</a>.



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Earth has new neighbors: Four new planets found orbiting a star just 6 light years away

Barnard’s Star has long been a focus of interest for...

Bacterial neighbors can be fierce rivals in their daily scuffle for resources. Some Pseudomonas bacteria species use specialized microscopic membrane devices to fight back against competing bacteria.



According to new research, these <a href="https://www.earth.com/news/bacteria-strain-identified-that-can-eat-forever-chemicals/" target="_blank" rel="noreferrer noopener">cells</a> react to threats by assembling a precise injection tool inside their outer shell. 



This work comes from the lab of <a href="https://www.biozentrum.unibas.ch/about/administration/administration-a-z/overview/unit/research-group-marek-basler" target="_blank" rel="noreferrer noopener">Professor Marek Basler</a> at the Biozentrum, <a href="https://www.unibas.ch/en.html" target="_blank" rel="noreferrer noopener">University of Basel</a>.



<h2 class="wp-block-heading" id="h-pseudomonas-bacteria-and-nano-spearguns">Pseudomonas bacteria and nano-spearguns</h2>



These weapon-like structures are known as the type VI secretion system (<a href="https://asm.org/articles/2023/april/type-vi-secretion-systems-weapons-of-bacterial-des" target="_blank" rel="noreferrer noopener">T6SS</a>), and they allow bacteria to inject harmful molecules into rivals. 



They have been studied extensively because of their importance in bacterial <a href="https://www.earth.com/news/bacteria-and-imprint-new-era-dna-transformation/" target="_blank" rel="noreferrer noopener">competition</a> and survival.



“We knew that Pseudomonas aeruginosa bacteria uses its T6SS to fire back when attacked,” said Basler. Scientists had long <a href="https://pubmed.ncbi.nlm.nih.gov/18289922/" target="_blank" rel="noreferrer noopener">suspected</a> that external stress might activate these devices in <a href="https://my.clevelandclinic.org/health/diseases/25164-pseudomonas-infection" target="_blank" rel="noreferrer noopener">Pseudomonas aeruginosa</a>. 



One survey showed that T6SS genes occur in about a quarter of <a href="https://www.ncbi.nlm.nih.gov/books/NBK538213/" target="_blank" rel="noreferrer noopener">gram-negative species</a>, highlighting their prevalence as a competitive strategy.



Some bacteria also direct T6SS at eukaryotic targets, affecting plant and animal hosts. This flexibility helps them adapt to diverse situations.



<h2 class="wp-block-heading" id="h-understanding-t6ss-genes-the-basics">Understanding T6SS genes - the basics</h2>



T6SS genes control the Type VI Secretion System (T6SS), an impressive molecular weapon that bacteria use to fight each other and sometimes even mess with host cells. 



Think of it as a microscopic harpoon gun - bacteria literally shoot toxic proteins into rival microbes to kill them or weaken their defenses. 



Some bacteria also use T6SS to interact with host organisms, either to establish infections or to outcompete other microbes in a shared environment. 



This system gives bacteria a serious advantage in the <a href="https://www.earth.com/news/viruses-that-love-to-kill-bacteria-could-help-fight-deadly-infections/" target="_blank" rel="noreferrer noopener">microscopic battlefield</a>, whether they're battling it out in soil, water, or even inside a host’s gut.



Scientists are fascinated by T6SS because it plays a huge role in bacterial survival, competition, and even virulence. 



Some nasty pathogens, like Vibrio cholerae (which causes cholera) and Pseudomonas aeruginosa (a major threat in hospitals), use T6SS to dominate their environments.



<h2 class="wp-block-heading" id="h-mechanical-force-as-a-trigger">Mechanical force as a trigger</h2>



“Using AFM, we have been able to mimic a bacterial T6SS attack,” said Yves F Dufrêne, a doctoral researcher at the <a href="https://pubmed.ncbi.nlm.nih.gov/17661630/" target="_blank" rel="noreferrer noopener">Swiss Nanoscience Institute</a>. 



The team used atomic force microscopy (<a href="https://www.nanoscience.com/techniques/atomic-force-microscopy/" target="_blank" rel="noreferrer noopener">AFM</a>) to gently push on the bacterial surface with a very fine tip. 



By applying measured force, they found that the <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC8934262/" target="_blank" rel="noreferrer noopener">outer membrane</a> damage alone could spur this injection tool into action. Once activated, the cells unleashed a burst of toxin-bearing elements to ward off intruders.



Studies from different labs have shown that surfaces with varied stiffness can influence <a href="https://www.earth.com/news/23-new-marine-bacteria-species-discovered-that-influence-global-ocean-cycles/" target="_blank" rel="noreferrer noopener">bacterial</a> attachment. However, it was less clear how direct mechanical stress might activate a defensive tool like T6SS.



Laboratories investigating <a href="https://www.sciencedirect.com/topics/food-science/vibrio" target="_blank" rel="noreferrer noopener">Vibrio species</a> observed T6SS responses to mechanical cues in marine environments. 



These clues paved the way for experiments focusing on Pseudomonas under controlled force measurements.



<h2 class="wp-block-heading" id="h-pseudomonas-bacteria-attack-detection">Pseudomonas bacteria attack detection</h2>



The scientists discovered that the site of membrane rupture guided the T6SS to assemble at the exact spot of assault. This high precision helps reduce wasted energy and ensures toxins only hit the intended target.



“Our work clearly shows that breaking the outer membrane is necessary and sufficient to trigger T6SS assembly,” said Basler.



 Researchers believe this system works thanks to a <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/phosphorylation-cascade" target="_blank" rel="noreferrer noopener">phosphorylation cascade</a> that springs into action upon sensing disruption. 



Pinpointing the exact trigger site allows minimal resource expenditure while maximizing impact on an aggressor. This specificity keeps the <a href="https://www.earth.com/news/bacteria-pass-down-memories-to-future-generations/" target="_blank" rel="noreferrer noopener">bacterial</a> cell from randomly launching costly attacks.



Scientists are interested in finding the molecular components that link physical membrane disturbance to T6SS initiation. These details could open doors for inhibitors designed to neutralize this response.



<h2 class="wp-block-heading" id="h-chemical-assault-on-the-membrane">Chemical assault on the membrane</h2>



Interestingly, certain antibiotics or <a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/peptide-derivative" target="_blank" rel="noreferrer noopener">peptide derivatives</a> also weaken the same barrier. This hints that chemical agents capable of penetrating the membrane can provoke a similar defensive strike.



The findings could be significant when considering <a href="https://www.sciencedirect.com/topics/pharmacology-toxicology-and-pharmaceutical-science/multiple-drug-resistance" target="_blank" rel="noreferrer noopener">multidrug resistance</a> in clinical settings. If a damaged outer membrane leads to a swift T6SS reaction, it might alter how pathogens respond to various medications.



<a href="https://www.sciencedirect.com/topics/medicine-and-dentistry/polymyxin-derivative" target="_blank" rel="noreferrer noopener">Polymyxin derivatives</a>, often reserved for severe infections, disrupt the outer membrane of Gram-negative bacteria. 



This disruption can unintentionally activate T6SS, giving the pathogen a countermeasure against rival organisms.



Understanding this dynamic may help clinicians refine how these drugs are applied in critical care. If T6SS ramps up under partial membrane stress, combination therapies might offer a more thorough strategy.



<h2 class="wp-block-heading" id="h-next-steps-for-pseudomonas-bacteria-study">Next steps for Pseudomonas bacteria study</h2>



Much still needs to be clarified, such as how multiple T6SS assemblies are precisely regulated once the membrane is compromised. Different strains may also vary in how sensitive they are to mechanical or chemical <a href="https://www.earth.com/news/bacteria-in-lake-mendota-keep-evolving-but-never-change/" target="_blank" rel="noreferrer noopener">cues</a>.



The bigger picture could involve a network of signals that prime bacteria to respond rapidly whenever their boundary is breached. 



Exploring these nuances might help researchers develop ways to disrupt this mechanism without harming beneficial microbes.



Researchers suspect that different bacterial species have unique thresholds for activating T6SS when threatened. 



This variation might determine which organisms thrive in complex environments like soil or aquatic habitats.



Experts are also investigating the role of protein partners that reset or limit T6SS after activation. 



Gaining clarity on the shutdown mechanism could lead to ways of blocking these assemblies and tackling antibiotic-resistant infections in the future.



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Featured image: Pseudomonas bacteria deploy their nano-spearguns when damaged by a sharp tip (15,000 x magnification). Credit: University of Basel, Biozentrum/<a href="https://nanoscience.unibas.ch/en/services/nano-imaging-lab/" target="_blank" rel="noreferrer noopener">SNI Nano Imaging Lab</a>



The study is published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adr1713" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Bacteria build tiny 'nano-spearguns' to fight back against attacks

Bacterial neighbors can be fierce rivals in their daily scuffle...

A frog species thought to be missing for well over a century has been spotted again.&nbsp;This startling discovery was announced by a group of Chilean and international researchers.



First described in 1902, the species Alsodes vittatus had not appeared in any scientific records for more than 130 years. 



Despite multiple expeditions attempting to locate the frog in the intervening decades, all efforts ended in vain - until now.



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



Recent fieldwork by researchers from the Laboratory of Systematics and Conservation of Herpetozoa (SyCoH) at the <a href="https://www.udec.cl/pexterno/" target="_blank" rel="noreferrer noopener">University of Concepción</a> has confirmed that the elusive amphibian is, in fact, still alive.&nbsp;



The findings detail the missing frog’s reemergence in the southeastern region of the Hacienda San Ignacio de Pemehue in La Araucanía, Chile.&nbsp;



This rediscovery represents a significant moment for scientists studying South American <a href="https://www.earth.com/news/what-are-the-biggest-drivers-of-biodiversity-loss/" target="_blank" rel="noreferrer noopener">biodiversity</a>, especially in light of the many frog species currently listed as threatened or lacking sufficient data to assess their status.



<h2 class="wp-block-heading" id="h-a-missing-frog-species">A missing frog species</h2>



Alsodes vittatus, originally described by naturalist Rodulfo Amando Philippi, was initially located by French entomologist Philibert Germain in 1893, who provided the three specimens that Philippi used to define the species.&nbsp;



Ever since then, it has disappeared from the record. Between 1995 and 2002, researchers combed the Pemehue area, determined to relocate A. vittatus, but none succeeded.&nbsp;



Efforts resumed in 2015 and 2016, yet the <a href="https://www.earth.com/news/world-frog-day-addressing-environmental-threats-to-frogs/" target="_blank" rel="noreferrer noopener">frog</a> populations identified lacked the characteristic white or yellow dorsal stripe that defines A. vittatus.



<h2 class="wp-block-heading" id="h-south-america-s-frog-species">South America's frog species </h2>



Eventually, over a decade into the investigation, new teams led by Dr. Claudio Correa, engineer in renewable natural resources Edvin Riveros Riffo, and biologist Juan Pablo Donoso focused on a different part of the same region. Their change of venue paid off.&nbsp;



Within the Lolco and Portales river basins at the southeastern end of the former estate, they spotted two populations of a frog that, upon careful examination, was confirmed to be A. vittatus.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/toad-species_Alsodes-vittatus_rediscovered_credit-ZooKeys_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/toad-species_Alsodes-vittatus_rediscovered_credit-ZooKeys_1s.webp" alt="Individuals of Alsodes igneus and A. vittatus from the new populations, syntype of A. vittatus and environment of one of the new locality from underwater Tupuyuntué River at the point where tadpoles and juveniles of A. vittatus were observed. Credit: Edvin Riveros" class="wp-image-1962139"/></a><figcaption class="wp-element-caption">Individuals of Alsodes igneus and A. vittatus from the new populations, syntype of A. vittatus and environment of one of the new locality from underwater Tupuyuntué River at the point where tadpoles and juveniles of A. vittatus were observed. Credit: Edvin Riveros</figcaption></figure>



This unexpected triumph sheds light on important conservation implications for frogs in the southern cone of South America.



“The main challenge in locating it was the lack of precision in the description of its type locality,” the researchers wrote. 



“In Germain's time, the Hacienda San Ignacio de Pemehue was an estate of enormous size, and the naturalist did not specify the exact place where he collected the specimens.”



<h2 class="wp-block-heading" id="h-retracing-old-footsteps">Retracing old footsteps</h2>



While the northwestern section of the old hacienda had been surveyed frequently, there was little information about areas farther to the southeast.&nbsp;



Because Germain never noted his precise collecting site, the modern team resorted to reconstructing his likely path through historical documents and publications.&nbsp;



Armed with this historical context, Correa and Riveros hiked the estate from its southeastern reaches, culminating in the discovery that Alsodes vittatus still exists - albeit in small populations.



<h2 class="wp-block-heading" id="h-significant-risks-to-amphibians-nbsp">Significant risks to amphibians&nbsp;</h2>



More than a century after its scientific description, scientists now have their first biological and ecological data on A. vittatus. The species is found living near streams, as is common among many other Alsodes frogs.&nbsp;



By sampling individuals carefully, the team identified the presence of the distinctive dorsal stripe that sets A. vittatus apart.&nbsp;



Because most Alsodes frogs are extremely local in their habitats and easily disturbed by <a href="https://www.earth.com/news/human-activities-are-weakening-earths-air-circulation/" target="_blank" rel="noreferrer noopener">human activities</a>, the researchers believe A. vittatus faces several immediate threats.&nbsp;



Local land-use changes, logging activities, and climate factors all pose significant risks to amphibians in Chile’s temperate forests.



<h2 class="wp-block-heading" id="h-missing-and-threatened-frog-species">Missing and threatened frog species</h2>



This is a major milestone for South American herpetology and the conservation of biodiversity in the southern region. 



Many frogs in the region are threatened with <a href="https://www.earth.com/news/eu-responsible-for-extinction-of-frog-populations/" target="_blank" rel="noreferrer noopener">extinction</a>, so clarifying the distribution and life history of this one species is a crucial first step toward its protection. 



Field evidence collected by the team indicates that A. vittatus could meet criteria for classification as an endangered species. 



Further studies will be needed to confirm population sizes, any breeding sites, and precise habitat conditions.



“In a broader context, this rediscovery demonstrates the limited biological, evolutionary and biogeographic knowledge of the amphibians that inhabit the southern cone of South America, emphasizing the urgency of their study and conservation,” the scientists wrote.&nbsp;



Since multiple Alsodes species remain poorly understood, the authors encourage additional research and collaboration to fill knowledge gaps.



<h2 class="wp-block-heading" id="h-optimism-for-amphibian-conservation-nbsp">Optimism for amphibian conservation&nbsp;</h2>



The announcement of A. vittatus’ reemergence brings optimism for amphibian conservation worldwide.&nbsp;



By pinpointing the frog’s habitat and conditions, scientists can make targeted recommendations for habitat preservation, enforce measures that mitigate human impact, and explore breeding programs or other forms of support if the animal’s situation proves perilous.&nbsp;



Above all, the reappearance of a species lost to science for 130 years demonstrates that biodiversity can hide in overlooked corners of the Earth and highlights the value of determined research efforts.



The study is published in the journal <a href="http://dx.doi.org/10.3897/zookeys.1230.135523" target="_blank" rel="noreferrer noopener">ZooKeys</a>.



Image Credit: Edvin Riveros



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Missing frog species resurfaces after 130 years

A frog species thought to be missing for well over...

Politicians learned long ago that humor is a powerful asset for capturing public attention and building credibility. Scientists, however, often avoid jokes when presenting their work, worried that a lighthearted tone might reduce their authority and, consequently, the perceived reliability of their research.&nbsp;



Yet a newly published paper appears to contradict this assumption, pointing toward humor’s potential to bolster a scientist’s likability and legitimize their message.



The research was led by Alexandra Lynn Frank, a doctoral student at the <a href="https://www.uga.edu/" target="_blank" rel="noreferrer noopener">University of Georgia</a>’s Grady College of Mass Communication.



The results showed that <a href="https://www.earth.com/news/parents-who-use-humor-have-better-relationships-with-their-children/" target="_blank" rel="noreferrer noopener">humor</a> - if it genuinely elicits amusement - “can both have positive impacts on the likeability of a communicator, as well as enhancing perceptions that the message is an appropriate and legitimate source of scientific information.”&nbsp;



This conclusion broadens a growing line of inquiry into how comedic strategies in public outreach, such as stand-up performances, might sharpen scientific engagement. Frank’s research team placed their focus on a specific context, examining humor in the context of <a href="https://www.earth.com/news/spending-less-time-on-social-media-improves-your-mental-health/" target="_blank" rel="noreferrer noopener">social media</a> posts from scientists.



“Our study aimed to bridge this gap by enhancing our understanding of how individuals react to anthropomorphism and satire while providing practical insights for scientists and science communicators,” Frank explained.



<h2 class="wp-block-heading" id="h-cartoons-anthropomorphism-and-satire">Cartoons, anthropomorphism, and satire</h2>



The project centered on <a href="https://www.earth.com/news/ai-reveals-hidden-climate-extremes-in-europe/" target="_blank" rel="noreferrer noopener">artificial intelligence</a> (AI) content conveyed via cartoons in social media posts by a fabricated scientist named Dr. Jamie Devon. Three types of humor were tested: mild satire, anthropomorphism, or a mixture of both. Alongside these were control posts that lacked any humorous element.



Frank and her team ran an online survey with an embedded experiment. While participants realized they were completing a survey, they did not know they were part of an experiment.&nbsp;



Carefully selected using quota sampling aligned with U.S. Census data, 2,212 individuals viewed one of eight hypothetical tweets from Dr. Devon. Each tweet addressed AI and contained a cartoon, but the humorous aspect varied by group: no humor, anthropomorphism, satire, or a combination of both.&nbsp;



Survey respondents then rated how amusing the content was, how much they liked the fictional scientist, and how credible they felt the material was as a source of scientific knowledge.



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



“Politicians, entertainers, and advertisers often use humor because people tend to like and connect with people who can make them laugh,” said Frank.&nbsp;



“When people find something funny, they’re usually less likely to argue with or reject the message or the person delivering it. Our research supports this idea. We found that humor can aid scientists’ communication efforts, but only if people think they’re funny.”



In other words, a humorous approach must genuinely provoke amusement in an audience, or it might do more harm than good. The study also warns that certain types of comedy, especially harsh satire, can appear hostile and reduce the speaker’s believability.&nbsp;



“However, it is important to note that recent research conducted by my co-authors indicates that harsh forms of satire can be perceived as aggressive, which may undermine the credibility of the source of scientific information,” noted Frank.



<h2 class="wp-block-heading" id="h-scientists-and-humor-on-social-media">Scientists and humor on social media</h2>



Sarcasm or combative humor is therefore discouraged. Instead, Frank and her co-authors propose that scientists on social media carefully select the tone of their jokes, aiming for content that resonates positively with readers.&nbsp;



The findings raise implications for how scientists might adopt novel and more engaging communication techniques.



“Our research aims to provide valuable insights to aid these professionals in developing public communication strategies,” said Frank, adding that comedic methods used judiciously have the power to establish a warmer connection.



“When used responsibly, humor is a powerful tool that can humanize scientists and create meaningful connections with the public on social media. By leveraging humor, scientists can simplify complex concepts, making them more relatable and easier to understand.”



“This approach not only fosters goodwill but also has the potential to dispel misinformation in a friendly manner. Moreover, humor can spark curiosity, motivating people to seek out additional information on important scientific topics.”



<h2 class="wp-block-heading" id="h-implications-for-future-outreach">Implications for future outreach</h2>



By conveying a scientist’s approachable side while maintaining factual accuracy, humor might help reframe weighty or complicated research subjects in ways that more people can digest.&nbsp;



Meanwhile, the cautionary reminders about harsh satire underline the importance of aligning comedic approaches with the values of trustworthiness and sensitivity to one’s audience.



Although this study revolved around AI-related posts, its results could apply to a wide range of scientific discussions, suggesting that thoughtful use of jokes, cartoons, or playful analogies can enhance both interest and respect for scientific viewpoints.&nbsp;



For scientists venturing into social media - a domain that often shapes public perception - the research offers a signpost for bridging expertise with accessibility, reinforcing the message that a genuine sense of mirth can be an ally rather than a liability in <a href="https://www.earth.com/news/most-people-trust-science-but-want-better-communication/" target="_blank" rel="noreferrer noopener">science communication</a>.



In a digital ecosystem where short attention spans and skepticism can challenge the spread of scientific information, humor stands out as a channel for empathy and engagement.&nbsp;



As Frank’s study indicates, humor and factual accuracy need not be at odds. Instead, a carefully tailored, genuinely amusing approach can make the communicator more likable, the message more credible, and the science more understandable - ultimately helping to broaden support for scientific endeavors.



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Humor helps scientists connect with the public and gain trust

Politicians learned long ago that humor is a powerful asset...

<div class="wp-block-sendtonews-playerselector">[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"]</div>



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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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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

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Micruroides euryxanthus, commonly known as the Sonoran coral snake or the Arizona coral snake, is endemic to northwestern Mexico and the southwestern United States. The venom of M. euryxanthus is neurotoxic and extremely potent. Photo Credit: Alexander Wong

Sonoran Coral Snake

Experienced hunters say that wild boar can be even more dangerous to hunt than a bear. Equipped with thick, razor-sharp tusks, and a razor-sharp mind (hogs are the 4th most intelligent animal in the world) a wild boar can weigh a staggering 660 lbs and exhibit extremely aggressive and unpredictable behavior. Photo Credit: OAnderson

Sonoran Coral Snake

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