Fused Fragments You see, the Moon’s surface has been exposed to numerous impacts over time. Astronomical objects have frequently smashed into the natural satellite – breaking down many rocks in the process. Then, the pressure and high temperatures causes the fragments to fuse together and form breccias.

29. Fused Fragments

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



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



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



The study, led by Alberto Bolatto, utilized Webb’s Near-Infrared Camera (NIRCam) to penetrate the thick dust and gas covering the galaxy's core, a region critical to understanding <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a>.&nbsp;



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



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



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



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



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



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



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



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



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



A key revelation came from the NIRCam’s tracing of polycyclic aromatic hydrocarbons (PAHs), sooty chemical molecules that map out the structure of the galactic wind. To the surprise of researchers, the PAH emissions closely resembled the patterns of the hot, ionized gas, suggesting a more complex interaction within the wind than previously understood.&nbsp;



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



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



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



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



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



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



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



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



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



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Messier 82: Unlocking the mysteries of star formation

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

Today's Image of the Day from NASA Earth Observatory features a 9.5-mile section of Pangong Lake on the western end of the Tibetan Plateau. The image was captured by a crew member onboard the International Space Station.&nbsp;



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



This extreme environment affects both the physical characteristics of the <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lakes</a> and the types of ecosystems they support. For example, due to lower atmospheric pressure, the boiling point of water is reduced, which can affect the type of life that can survive in these regions.



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



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



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



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



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



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



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



Image Credit: NASA Earth Observatory&nbsp;



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Pangong Lake on the Tibetan Plateau

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Ecologically, the Euphrates supports a range of habitats, from wetlands to desert ecosystems, making it home to diverse wildlife. 



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



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



Image Credit: NASA



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Lake Razzaza: A shrinking oasis shaped by salinity

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



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



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



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



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



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



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



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. “Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



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



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



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



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



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



<h2 class="wp-block-heading" id="h-galaxy-evolution">Galaxy evolution</h2>



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Starburst galaxy in the constellation Columba

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA Earth Observatory&nbsp;



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Monster storm spawns severe weather across the U.S. 

Today's Image of the Day from the European Space Agency (ESA) features the distant galaxy LEDA 22057, which is located about 650 million light-years away in the constellation Gemini. 



Within the galaxy lies a pale blue dot - SN 2024PI, a supernova explosion that was discovered by an automated survey in January 2024.



“The survey covers the entire northern half of the night sky every two days and has cataloged more than 10,000 supernovae,” noted <a href="https://www.esa.int/ESA_Multimedia/Images/2025/01/Pale_blue_supernova_dot" target="_blank" rel="noreferrer noopener">ESA</a>.



“The supernova is visible in this image: located just down and to the right of the galactic nucleus, the pale blue dot of SN 2024PI stands out against the galaxy’s ghostly spiral arms.”



<h2 class="wp-block-heading" id="h-the-remnants-of-a-supernova-nbsp">The remnants of a supernova&nbsp;</h2>



ESA noted that the image was taken about a month and a half after the <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">supernova</a> was discovered, so it appears many times fainter than its maximum brilliance.



“SN 2024PI is classified as a Type Ia supernova. This type of supernova requires a remarkable object called a white dwarf, the crystallized core of a star with a mass less than about eight times the mass of the Sun,” explained ESA.



“When a star of this size uses up the supply of hydrogen in its core, it balloons into a red giant, becoming cool, puffy and luminous. Over time, pulsations and stellar winds cause the star to shed its outer layers, leaving behind a white dwarf and a colorful planetary nebula.”&nbsp;



<h2 class="wp-block-heading" id="h-the-fate-of-white-dwarfs">The fate of white dwarfs</h2>



Most stars in the <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">Milky Way</a> will eventually transition to white dwarfs after their death. Whether or not a star becomes a white dwarf depends on its mass. 



Stars that are significantly more massive will end their lives differently. Stars that exceed the critical mass threshold of eight times the Sun undergo more violent deaths. 



After exhausting their nuclear fuel, they collapse under their immense gravity and trigger a supernova explosion. Depending on the remaining core mass, they may leave behind either a neutron star or a black hole, rather than a <a href="https://www.earth.com/news/hungry-white-dwarf-stars-eat-heavy-metals/" target="_blank" rel="noreferrer noopener">white dwarf</a>. 



These remnants represent extreme outcomes of stellar evolution and are fundamentally different from white dwarfs.



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



Gemini is one of the twelve zodiac constellations located in the northern celestial hemisphere.&nbsp;



Its name means "twins" in Latin, reflecting its representation of the mythological twins Castor and Pollux from Greek and Roman mythology.&nbsp;



<h3 class="wp-block-heading" id="h-stars-of-gemini">Stars of Gemini</h3>



The stars Castor and Pollux, which form the heads of the twins, are the brightest stars in Gemini and are key to its identification.&nbsp;



Pollux is a bright orange giant star, while Castor is a multiple <a href="https://www.earth.com/news/exoplanet-found-in-the-habitable-zone-of-a-binary-star-system/" target="_blank" rel="noreferrer noopener">star system</a> made up of six stars.



<h3 class="wp-block-heading" id="h-neighboring-constellations">Neighboring constellations</h3>



Gemini lies between Taurus to the west and Cancer to the east, and it is bordered by several other constellations, including Orion to the south.



It is most visible in the night sky during the winter months in the Northern Hemisphere, particularly in January and February.&nbsp;



<h3 class="wp-block-heading" id="h-significance-of-gemini">Significance of Gemini</h3>



The constellation is part of the ecliptic, the path that the Sun appears to take through the sky, making it significant in both astronomy and astrology.



Astronomically, Gemini is home to several interesting deep-sky objects, including the open star cluster M35, which is easily visible with binoculars or a small telescope.&nbsp;



The constellation also contains several stars and stellar systems of interest, such as variable stars and binary systems.



<h3 class="wp-block-heading" id="h-greek-mythology-nbsp">Greek mythology&nbsp;</h3>



In Greek mythology, Castor and Pollux were the sons of Leda, but they had different fathers - Castor was mortal, while Pollux was divine, being the son of Zeus.&nbsp;



Their story is one of loyalty and brotherhood, as Pollux begged Zeus to share his immortality with Castor after his brother's death. As a result, Zeus placed them in the sky as the constellation Gemini, symbolizing their eternal bond.



<h3 class="wp-block-heading" id="h-modern-culture">Modern culture</h3>



In modern culture, Gemini continues to be associated with duality, adaptability, and communication in astrology.&nbsp;



The constellation also holds significance in space science, lending its name to NASA's Gemini program in the 1960s. This program conducted critical missions that paved the way for the Apollo moon landings.



Image Credit: ESA&nbsp;



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Supernova explosion captured in the constellation Gemini 

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

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

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

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

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

A frozen Lake Erie in February

Aqua Earth Observing Satellite

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

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

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

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

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

Northern Italy from the Space Station

Photos from the International Space Station

Human litter has now infiltrated the deepest parts of Earth's oceans and seas. Debris and trash produced by human activity was spotted at a depth of 5,112 meters (3.2 miles) in the Mediterranean Sea. 



The site, which is the deepest point in the Mediterranean, is known as Calypso Deep, and is located off the south-western coast of Greece in the Ionian Sea.



In a new study, researchers have identified 167 objects at the bottom. Of these, 148 were clearly marine debris, while 19 were believed to be of human origin, though less definitively.



According to the authors, this represents one of the highest concentrations of litter documented at great depths in any sea.



<h2 class="wp-block-heading" id="h-debris-in-the-bottom-of-the-sea">Debris in the bottom of the sea </h2>



To investigate the Calypso Deep, scientists used a crewed submersible called the Limiting Factor, a deep-submergence vehicle capable of withstanding extreme pressure.



Images captured by the Limiting Factor confirm that besides accumulating on coasts, surface waters and shallower bottoms, <a href="https://www.earth.com/news/is-it-still-possible-to-save-the-ocean-from-plastic-pollution/" target="_blank" rel="noreferrer noopener">marine waste</a> also reaches the deepest, most remote points of the Mediterranean Sea.&nbsp;



Given the heavy impact of human activities on this nearly enclosed sea, the discovery emphasizes the urgency of global actions to reduce marine debris and a need for lifestyle changes that cut waste and protect marine environments worldwide.



<h2 class="wp-block-heading" id="h-the-calypso-deep-as-a-debris-trap">The Calypso Deep as a debris trap</h2>



Located about 60 kilometers (37 miles) south west of the Peloponnese coast in Greece, the Calypso Deep is a depression within the Hellenic Trench system. 



Surrounded by steep terrain in an area with active faults, it has slopes measuring thousands of meters and a mostly flat floor at its lowest point. 



Its deeper, kidney-shaped portion extends over approximately 20 by 5 kilometers (12 by 3 miles) at depths surpassing 5,000 meters (3 miles).



<h2 class="wp-block-heading" id="h-litter-s-journey-to-the-bottom">Litter's journey to the bottom</h2>



But how does rubbish collect so far down?



According to Miquel Canals from the University of Barcelona’s <a href="https://www.ub.edu/portal/web/earth-sciences" target="_blank" rel="noreferrer noopener">Faculty of Earth Sciences</a>, the debris comes from various sources, both terrestrial and marine. 



It could have arrived by various routes, including both long-distance transport by <a href="https://www.earth.com/news/weakening-ocean-currents-could-cost-trillions-of-dollars/" target="_blank" rel="noreferrer noopener">ocean currents</a> and direct dumping. 



Canals explains that plastic items, for instance, can drift from coastal waters. 



Some light waste, such as plastics, comes from the coast, from where it escapes to the Calypso Deep, just 60 kilometers [37 miles] away. 



Some plastics, such as bags, drift just above the bottom until they are partially or completely buried, or disintegrate into smaller fragments.



“We have also found evidence of the boats’ dumping of bags full of rubbish, as revealed by the pile-up of different types of waste followed by an almost rectilinear furrow," Canals continued.



"Unfortunately, as far as the Mediterranean is concerned, it would not be wrong to say that ‘not a single inch of it is clean.'"



<h2 class="wp-block-heading" id="h-debris-transport-across-the-sea">Debris transport across the sea</h2>



Canals noted that the Calypso Deep is a closed depression, which favors the accumulation of debris inside it. He pointed out that the weak currents in the trench also facilitate the deposition of light debris at the bottom.



Floating debris originates mostly in the southern Ionian Sea or further south, and drifting eddies bring it toward the Calypso Deep.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-litter-debris_bottom-seafloor_Mediterranean-Sea_montage_credit-Caladan-Oceanic_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-litter-debris_bottom-seafloor_Mediterranean-Sea_montage_credit-Caladan-Oceanic_1s.webp" alt="The debris identified by the international team in the Calypso Deep warns of the need to implement global policy actions to reduce ocean waste, as well as to encourage changes in citizens’ consumption habits and waste reduction in order to protect seas and oceans around the world. Credit: Caladan Oceanic" class="wp-image-1962233"/></a><figcaption class="wp-element-caption">The debris identified by the international team in the Calypso Deep warns of the need to implement global policy actions to reduce ocean waste, as well as to encourage changes in citizens’ consumption habits and waste reduction in order to protect seas and oceans around the world. Credit: Caladan Oceanic</figcaption></figure>



“When these eddies are located over the Calypso Trench, some debris tends to fall slowly to the bottom, aided by degradation mechanisms and ballasting processes that increase its density," explained Canals 



"Surface currents can also transport debris from the Adriatic Sea to the north, through the Strait of Otranto, and from the waters off north-western Greece."



<h2 class="wp-block-heading" id="h-technology-to-explore-the-abyss">Technology to explore the abyss</h2>



Investigating such extreme depths demands cutting-edge tools. In this case, the Limiting Factor submarine, built by Triton Submarines, allowed a small crew of two to descend. 



Moving at about 1.8 kilometers (1.1 miles) per hour to obtain clear images, the Limiting Factor covered roughly 650 meters (0.4 miles) in a straight line over a 43-minute window on the bottom.&nbsp;



“On each dive, more time is usually spent descending and ascending the vehicle back to the surface than inspecting the bottom. Each complete dive usually takes a few hours,” Canals noted.



The expedition revealed no substantial impact on local marine life, likely due to the area’s low biodiversity. 



Only a few species - namely, the fish Coryphaenoides mediterraneus and the crustacean Acanthephyra eximia - appeared in the footage. 



“However, in places with more <a href="https://www.earth.com/news/world-ocean-day-a-unified-approach-to-protect-biodiversity/" target="_blank" rel="noreferrer noopener">biodiversity</a>, there are different types of interaction between the debris deposited on the bottom and the organisms, such as ghost fishing, burial, hooking or ingestion, but also the use of debris as a substrate where animals can grow, hide or lay their eggs,” Canals said.



<h2 class="wp-block-heading" id="h-mediterranean-s-pollution-problem">Mediterranean’s pollution problem</h2>



Scientists first documented trash on the ocean floor in 1975, in the North Atlantic’s Skagerrak Strait. Areas like canyons and seamounts are especially prone to accumulating garbage, either from settling, burial, or erosion processes. 



Now, the Mediterranean ranks among the worst-affected seas. In 2021, research identified the Strait of Messina as the global hot spot for seafloor litter. 



This highlights broader concerns about intensifying human influence on an enclosed region subject to heavy maritime traffic and fishing.



“The Mediterranean is an enclosed sea, surrounded by humanity, with intense maritime traffic and widespread fishing activity," noted Canals. 



"The evidence provided by our research should shake up global efforts, and in particular in the Mediterranean, to mitigate waste dumping, especially plastics, in the natural environment and ultimately in the sea, in line with the <a href="https://www.unep.org/inc-plastic-pollution" target="_blank" rel="noreferrer noopener">UN Global Plastics Treaty</a> against plastic pollution, which is still pending approval."



Canals emphasized that the ocean floor is still largely unknown to society as a whole, which makes it difficult to raise social and political awareness about the conservation of these spaces. 



"It is necessary to make a joint effort between scientists, communicators, journalists, the media, influencers and other people with social impact. The problem is there, and it has an enormous scope, even if it is not directly visible. We should not forget about it."



Details of the study are published in the <a href="https://www.sciencedirect.com/science/article/pii/S0025326X25000852?via%3Dihub" target="_blank" rel="noreferrer noopener">Marine Pollution Bulletin</a>.



Image Credit: Caladan Oceanic



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Human trash has found its way to the deepest parts of Earth's seas and oceans

Human litter has now infiltrated the deepest parts of Earth's...

The tapestry of human evolution is adorned with fascinating episodes and, among them, the story of Paranthropus robustus from the Cradle of Humankind in South Africa stands out as a testament to survival, adaptation, and dominance.



This ancient hominin species, also referred to as Australopithecus robustus, inhabited the terrains of South Africa approximately 2 million years ago. It shared this region with Homo ergaster, which is believed to be a direct forerunner of modern humans.



The Swartkrans Cave, that is nestled halfway between Johannesburg and Pretoria, is a treasure trove of Paranthropus robustus fossils. 



Archaeological pursuits at this site since 1948 have helped unearth a multitude of insightful details about the extinct species' dietary patterns and social arrangements.



But a recent groundbreaking discovery is now reshaping what we know about the physical traits and way of life of these early hominins, offering a rare glimpse into how they moved, survived, and interacted in a prehistoric landscape.



<h2 class="wp-block-heading" id="h-life-and-traits-of-paranthropus-robustus">Life and traits of Paranthropus robustus</h2>



Paranthropus robustus was equipped with extraordinarily heavy jaws and thickly coated teeth – an adaptation for enduring lean times by when individuals would have needed to consume low-grade, tough foods. 



Fossilized skulls and teeth of this species have been excavated in several different locations in the Cradle of Humankind.



The skulls and teeth provide fascinating insights into the social structure of these hominins. Some are exceptionally large, suggesting that they were probably males, while others are smaller and likely to have been females.



This physical difference suggests that Paranthropus robustus probably engaged in <a href="https://www.earth.com/news/polygynous-male-mammals-may-have-more-sexual-aggression/" target="_blank" rel="noreferrer noopener">polygyny</a> – a system of mating where one dominant male mates with several females.



But until now, the scarcity of fossilized bones from the rest of the post-cranial skeleton has impeded our knowledge of their body type, posture, and locomotion – key&nbsp;characteristics&nbsp;associated&nbsp;with their diet and mate searching behavior.



A recent groundbreaking find in the Swartkrans Cave is, however, poised to reverse this paradigm.



<h2 class="wp-block-heading" id="h-discoveries-at-swartkrans-cave">Discoveries at Swartkrans cave</h2>



Recently, an international team of researchers based at the Evolutionary Studies Institute at the <a href="https://www.wits.ac.za/esi/" target="_blank" rel="noreferrer noopener">University of the Witwatersrand</a> in South Africa made a fascinating discovery.



Their dig resulted in the exposure of the very first articulating hipbone, thigh bone, and shin bone of a Paranthropus robustus individual.



This groundbreaking discovery provides us with valuable information regarding the existence and features of this <a href="https://www.earth.com/news/homo-juluensis-new-human-species-vanished-just-fifty-thousand-years-ago/" target="_blank" rel="noreferrer noopener">prehistoric hominin species</a>.



The newly discovered fossil not only illustrates that Paranthropus robustus primarily moved around by walking upright (similar to the locomotion of <a href="https://www.earth.com/news/modern-humans-are-separated-from-neanderthals-by-one-gene/" target="_blank" rel="noreferrer noopener">modern humans</a>), but also reveals their surprisingly petite size.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/hominin_human-ancestor_Paranthropus-robustus_thigh-bone_walked-upright_credit-Jason-Heaton_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/hominin_human-ancestor_Paranthropus-robustus_thigh-bone_walked-upright_credit-Jason-Heaton_1s.webp" alt="The new Paranthropus robustus thigh and shin bones, articulated at the knee joint. Credit: Jason Heaton" class="wp-image-1962225"/></a><figcaption class="wp-element-caption">The new Paranthropus robustus thigh and shin bones, articulated at the knee joint. Credit: Jason Heaton</figcaption></figure>



"It is estimated that this individual, probably a female, was only about a meter tall (3.3 feet) and 27 kg (60 pounds) when it died, making it even smaller than adults from other diminutive early human species, including those represented by the famous '<a href="https://www.earth.com/news/lucy-could-barely-run-what-does-that-say-about-our-ancestors/" target="_blank" rel="noreferrer noopener">Lucy</a>' (Australopithecus afarensis; about 3.2 million years old) and 'Hobbit' (Homo floresiensis; about 90,000 years old) skeletons, from Ethiopia and Indonesia, respectively," explained Professor Pickering from the University of Wisconsin–Madison, who spearheaded the research.



<h2 class="wp-block-heading" id="h-predators-prey-and-survival-instincts">Predators, prey, and survival instincts</h2>



The compact size of the prehistoric Prananthropus robustus rendered them vulnerable to predators, such as <a href="https://www.earth.com/news/two-new-species-of-sabertooth-cat-discovered-in-south-africa/" target="_blank" rel="noreferrer noopener">sabertooth cats</a> and giant hyenas, who roamed the areas surrounding Swartkrans Cave.



This hypothesis is supported by the team's identification of tooth marks and chewing damage on fossilized P. robustus bones. These marks are identical to those made by leopards when they chew on their prey.



Yet, their small size didn’t necessarily hinder their survival. 



"Although it seems that this particular Paranthropus robustus individual was the unfortunate victim of predation, that conclusion does not mean that the entire species was inept," Pickering stresses.



Their existence in South Africa for over a million years attests to their endurance, and the presence of <a href="https://www.earth.com/news/first-tools-ever-made-on-earth-hominins-3-million-years-ago-cradle-of-humankind/" target="_blank" rel="noreferrer noopener">stone and bone tools</a> near their fossils suggests a degree of intelligence.



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



In order to learn more about the growth and developmental patterns of Paranthropus robustus, as well as their locomotion behaviors, the team is currently doing research that includes CT-scan examinations of internal bone structures.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/hominin_human-ancestor_Paranthropus-robustus_skull_walked-upright_credit-Jason-Heaton_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/hominin_human-ancestor_Paranthropus-robustus_skull_walked-upright_credit-Jason-Heaton_1s.webp" alt="A fossil leopard lower jawbone next to a skull fragment of a juvenile Paranthropus robustus. Note the two punctures in the skull, which match the spacing of the tips of the leopard's fangs—implying that this unfortunate hominin was killed and eaten by a leopard. Credit: Jason Heaton" class="wp-image-1962223"/></a><figcaption class="wp-element-caption">A fossil leopard lower jawbone next to a skull fragment of a juvenile Paranthropus robustus. Note the two punctures in the skull, which match the spacing of the tips of the leopard's fangs—implying that this unfortunate hominin was killed and eaten by a leopard. Credit: Jason Heaton</figcaption></figure>



This study has the potential to advance our knowledge of human evolution and add fresh chapters to the intriguing story of Paranthropus robustus.



<h2 class="wp-block-heading" id="h-daily-lives-of-paranthropus-robustus">Daily lives of Paranthropus robustus</h2>



Outside of their skeletal system and survival habits, knowledge of the daily existence of Paranthropus robustus gives greater insight into what they were like.



Scientists surmise that the early hominins lived in small groups and most likely scavenged in groups in the woodland and open savannas that surrounded the Swartkrans Cave. 



They ate largely tough plant matter, such as roots, tubers, and seeds, to which their heavy-duty jaws and heavily enamel-coated teeth were best suited.



Proof of stone and bone tools alongside their fossils evokes intriguing questions regarding their level of cognitive skills. 



Although not as sophisticated a tool maker as the subsequent hominin species, P. robustus might have utilized basic tools to assist with food preparation and tuber excavation.



Such resourcefulness implies that Paranthropus robustus was more cunning than previously realized, and was potentially able to manipulate its surroundings in order to enhance survival prospects.



As scientists go on to examine fossilized bones and related artifacts, every finding is a step towards piecing together the complicated world of Paranthropus robustus, a species that flourished under difficult prehistoric conditions.



The full study was published in the journal <a href="https://linkinghub.elsevier.com/retrieve/pii/S0047248424001556" target="_blank" rel="noreferrer noopener">Journal of Human Evolution</a>.



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Discovery: These human ancestors walked upright over 2 million years ago

The tapestry of human evolution is adorned with fascinating episodes...

Millions of years from now, the remnants of today’s world will be buried beneath layers of rock and sediment. While fossils of ancient creatures have long fascinated scientists, we are likely to leave behind a new kind of fossil in the future - one shaped by human activity. 



These "technofossils" include everything from plastic bottles and old mobile phones to the most unexpected of all - the blades of wind turbines.



The idea that everyday objects could become <a href="https://www.earth.com/news/neanderthal-fossils-reveal-signs-of-a-population-collapse/" target="_blank" rel="noreferrer noopener">fossils</a> may seem strange. People associate fossils with dinosaur bones, ancient trees, and primitive sea creatures - not with discarded technology.



However, researchers have started to realize that the impact of human-made materials will last far longer than many natural formations. The structures we build and the items we use daily will leave a lasting imprint on the Earth’s geological record, creating a new chapter in the history of fossilization.



<h2 class="wp-block-heading" id="h-how-human-made-objects-become-fossils">How human-made objects become fossils</h2>



Fossilization is a slow and selective process. For an object to become a fossil, it must be buried under sediment, shielded from decay, and eventually mineralized over time. 



Most organic materials decompose before they have a chance to fossilize, but some artificial materials resist natural breakdown.



Plastics, synthetic fabrics, and certain composites are particularly durable. They do not degrade easily, which makes them prime candidates for future <a href="https://www.earth.com/news/north-americas-oldest-dinosaur-is-completely-rewriting-history/" target="_blank" rel="noreferrer noopener">fossils</a>.



The layers of waste accumulating in landfills today could, under the right conditions, transform into well-preserved remnants of the Anthropocene epoch - the age of human influence on Earth.



<a href="https://le.ac.uk" target="_blank" rel="noreferrer noopener">University of Leicester</a> paleontologists Professor Sarah Gabbott and Professor Jan Zalasiewicz have explored this idea in depth. 



In their book <a href="https://global.oup.com/academic/product/discarded-9780192869333?cc=gb&amp;lang=en&amp;" target="_blank" rel="noreferrer noopener">Discarded: How Technofossils Will be Our Ultimate Legacy</a>, they examine how the products of modern life will be preserved for millennia. These objects will tell the story of a civilization defined by industry, technology, and mass consumption.



<h2 class="wp-block-heading" id="h-fossilized-wind-turbine-blades">Fossilized wind turbine blades </h2>



Among all the potential technofossils, wind turbine blades stand out as among the most surprising. These towering structures symbolize clean energy, yet their long-term environmental fate remains uncertain.



Unlike the metal towers that hold them aloft, turbine blades are produced from materials that are difficult to recycle, making them far more likely to persist in the geological record.



“The fossils won’t be of the towers, by and large – those are made of metal, which can be recycled. The enormous wind turbine blades, though, are made of materials like fibreglass and epoxy resin and carbon fibres, which are terribly hard to recycle - but easy to fossilize,“ explained Professor Zalasiewicz.



“As wind turbines reach end-of-life and are decommissioned, huge landfills of the 50 meter-long-plus blades, sliced into truck-length segments and neatly stacked side by side, are appearing and growing."



“Some will stay buried for millions of years – and, if finally erosion-revealed and stumbled upon by some curious far-future palaeontologist, will be an amazing sight, like a graveyard of gigantic, hollow, sawn-up bones."



"Some may be squashed and crumpled by earth movements, and others may be filled with mineral growths, but their striking shape and enormous size will shine out of the strata.”



<h2 class="wp-block-heading" id="h-piecing-together-the-past">Piecing together the past</h2>



Future scientists may one day stumble upon these massive fossils and wonder about their origins. 



Just as modern paleontologists reconstruct dinosaur skeletons from fragmented bones, these wind turbine fossils could present a mystery for researchers in the distant future. Their aerodynamic design might hint at their original purpose, but without historical records, their function could remain uncertain.



“For our far-future explorers, they will be a huge puzzle – will they be able to tell that they were built to catch the wind, and to provide energy that is clean and renewable? Perhaps they will, if they can piece them together – like we reconstruct huge dinosaur skeletons today – to see their aerodynamic shapes,” said Professor Zalasiewicz.



These fossils will not be alone. They will be part of a vast and complex geological archive of human activity. Alongside them, future scientists may uncover the remains of other everyday objects, from metal wires and plastic containers to microchips and industrial pollutants.



<h2 class="wp-block-heading" id="h-growing-impact-of-human-waste">Growing impact of human waste</h2>



While wind turbine blades are one of the more dramatic examples, they are not the only evidence of human impact on the planet. 



Every year, billions of discarded items accumulate in landfills and oceans. Over time, many of these objects will become buried beneath layers of sediment, preserving them for future generations to discover.



“They will be only one puzzle among the millions we leave behind in our daily lives (and we suspect they would also find the more sinister fossils left by fossil fuel burning). There’s been nothing like this emerging new fossil cornucopia in the Earth’s four and a half billion-year history,“ noted Professor Zalasiewicz.



“And right now, we should begin to understand this amazing, if often toxic, legacy that we are leaving for the planet. Knowing how our myriad discarded objects will fossilise into the far future can help us deal with the growing mountains of trash we live among today.”



Understanding how our waste fossilizes is not just an academic pursuit. It provides insight into the long-term effects of human consumption and pollution. 



This knowledge could encourage more sustainable practices and better waste management strategies to reduce the environmental footprint of future generations.



<h2 class="wp-block-heading" id="h-unexpected-relics-of-modern-life">Unexpected relics of modern life</h2>



The idea of human-made fossils, including turbine blades, invites some unusual questions.



What will be the strangest objects that survive millions of years into the future? Which everyday items will become the most unexpected relics of modern life?



“It’s been a real adventure to use our understanding of how fossils form in the past and now apply it to the very new world of what we call technofossils,“ Professor Sarah Gabbott noted.



“But then we were asked a really tricky question. What will the most surprising technofossil that we leave behind, millions (or billions) of years from now?



“There are so many candidates to rival wind turbines for the ‘weirdest human-made fossil of all time.' There are, for instance, the myriad different shapes that a pair of Y-fronts can take when pressed within strata (and yes, we do explore that very particular question in the book)."



“There are the tiny, but very distinctive – and very hard-wearing – fossil smoke particles that come out of our power stations. There are the strange stories of tea-bags, and of chicken feathers, non-stick pans, the minute patterns on silicon chips, the copper wires that wrap around the globe, and much more,” explained Professor Gabbott.



From fabric pressed into rock to microscopic patterns on electronic chips, these objects will provide a unique record of human civilization. Their presence in the geological archive will serve as evidence of a world driven by innovation, industry, and material consumption.



<h2 class="wp-block-heading" id="h-future-research-on-wind-turbine-blades">Future research on wind turbine blades</h2>



The study of technofossils is more than just a curiosity - it forces us to reconsider our relationship with waste and <a href="https://www.earth.com/news/global-warming-is-accelerating-beyond-control-as-co2-levels-rise/" target="_blank" rel="noreferrer noopener">long-term environmental impact</a>. If everyday objects will outlast entire civilizations, what responsibilities do we have in managing what we leave behind?



Gabbott and Zalasiewicz’s research challenges us to think beyond the present moment. The choices we make today will shape how future generations understand our era. 



By studying how human-made materials fossilize, we gain a new perspective on sustainability, history, and the consequences of our actions over deep time .



As we continue to innovate and build, it is worth remembering that the fossils of the future will not just be ancient bones and shells. Everything we discard has the potential to become a lasting mark on the planet. 



This is what will tell the story of a world transformed by humanity.



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What modern fossils will be the 'most surprising' to future explorers?

Millions of years from now, the remnants of today’s world...

Teen pregnancy remains a significant public health concern around the world, especially in West Virginia where the rate is notably higher than the national average.



A recent study highlights the challenges associated with teenage pregnancies, particularly regarding birth outcomes and access to prenatal care. 



Researchers found that infants born to teenage mothers in the state tend to have lower birth weights and are smaller for their gestational age compared to those born to adult mothers.



<h2 class="wp-block-heading" id="h-teen-pregnancy-rates-in-west-virginia">Teen pregnancy rates in West Virginia</h2>



Researchers at <a href="https://www.wvu.edu/" target="_blank" rel="noreferrer noopener">West Virginia University</a> analyzed data from Project Watch, a system that tracks all births in hospitals across the state. 



The study examined 86,447 live births between 2018 and 2023, and found that 5,310 of these infants - about 6.15% - were born to teenage mothers.



By comparison, the national teen birth rate in 2022 stood at 1.36%. Rural counties had the highest rates, with Pendleton County reaching 14.38% and Boone, Mercer, and Hardy counties all surpassing 10%. The lowest rate, 2.76%, was recorded in Monongalia County.



According to Amna Umer, associate professor in the WVU School of Medicine's Department of Pediatrics, the findings emphasize an urgent issue.



“We used the most current data and the findings underscore a significant issue in the state. The risk of teen birth is multifactorial," Umer explained.



"This study highlights the role of social, geographical and educational factors offering crucial insights for policymakers to expand comprehensive, evidence-based teen pregnancy prevention education and <a href="https://www.earth.com/news/male-birth-control-scientists-develop-a-non-hormonal-pill-for-men/" target="_blank" rel="noreferrer noopener">birth control</a> access for at-risk teens.”



<h2 class="wp-block-heading" id="h-barriers-to-prenatal-care">Barriers to prenatal care</h2>



Teenage mothers are less likely to receive adequate <a href="https://www.earth.com/news/why-are-pregnancy-related-deaths-in-the-u-s-skyrocketing/" target="_blank" rel="noreferrer noopener">prenatal care</a>, a concern that has been confirmed by this study. Access to health services is a significant hurdle, especially for those in rural communities where medical facilities are scarce.



“Teenage mothers are a vulnerable population and there really isn’t a lot of research out there, especially on those living in rural areas,” said Rylee Childers, a third-year medical student from Morgantown, and the study's corresponding author.



“Our research identifies the hurdles that come with being a teenage mom and that’s important to not just people in rural areas, but also their primary care physicians and people in the medical field.”



Many factors contribute to this lack of care. Geographic distance and transportation barriers make it difficult for <a href="https://www.earth.com/news/nearly-half-of-u-s-teens-have-been-harassed-by-a-partner/" target="_blank" rel="noreferrer noopener">teens</a> to attend regular checkups.



“There are some people in rural areas that have to drive three to four hours to see their obstetrician,” Childers confirmed.



“Additionally, a lot of teenage moms can’t drive yet. So, another adult would have to take off work which might be difficult if they work two jobs. There are a lot of different factors that maybe not everybody realizes because they’re not familiar with that population.”



<h2 class="wp-block-heading" id="h-addressing-teen-pregnancy">Addressing teen pregnancy</h2>



Since most teen pregnancies are unintended, health care professionals have an opportunity to support prevention efforts. 



The study suggests that providers could play a critical role in <a href="https://www.earth.com/news/sales-of-morning-after-pills-soar-after-new-years-day/" target="_blank" rel="noreferrer noopener">contraception</a> counseling, navigating health care options, and ensuring confidentiality in patient care.



“I really hope the study starts a conversation about <a href="https://www.earth.com/news/growing-health-gap-between-rural-and-urban-men-around-the-world/" target="_blank" rel="noreferrer noopener">rural health care</a> as a whole and especially about access to care and resources,” Childers said.



The findings also reflect broader disparities. The study found that teenage pregnancies were more common among individuals receiving Medicaid and among racial minority groups. 



These findings align with previous research that points to economic and social inequalities as factors influencing teen birth rates.



<h2 class="wp-block-heading" id="h-moving-forward">Moving forward</h2>



Childers and co-author Alexandra Richmond, a third-year medical student from Beckley, were selected to present their findings at the 2024 West Virginia Rural Health Conference.



For Childers, the research experience has been eye-opening.



“Working on this study opened my eyes to the entire process of research and understanding the health care disparities of the rural population as a whole,” she said. “It makes me think about how I can be a better provider for my patients.”



As discussions on teen pregnancy prevention and access to health care continue, studies like this provide valuable insights for policymakers, medical professionals, and community leaders striving to improve maternal and child health outcomes in West Virginia.



The full study was published in the journal <a href="https://www.jpagonline.org/article/S1083-3188(25)00006-3/abstract" target="_blank" rel="noreferrer noopener">Journal of Pediatric and Adolescent Gynecology</a>.



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Study links teen pregnancy to smaller newborns

Teen pregnancy remains a significant public health concern around the...

Scientists have searched for alien life for years, but space is huge, and technology has limits, making it hard to find answers. Traditionally, researchers have focused on finding planets similar to Earth, believing that conditions mirroring our own would be the best place to look for life.



However, a new study suggests that an entirely different type of planet could provide clearer <a href="https://www.earth.com/news/new-super-earth-hd-20794-found-just-20-light-years-away-is-best-target-yet-for-alien-life/" target="_blank" rel="noreferrer noopener">evidence of living organisms</a>.



Instead of focusing on Earth-like planets, scientists have identified a unique biosignature gas that could reveal life in environments that are vastly different from our own.



This discovery shifts the search toward larger, ocean-covered planets with thick hydrogen atmospheres, known as hycean planets, where certain microbes could potentially thrive.



<h2 class="wp-block-heading" id="h-gases-could-be-key-indicators">Gases could be key indicators</h2>



The recent study, led by researchers from the <a href="https://www.ucr.edu/" target="_blank" rel="noreferrer noopener">University of California, Riverside</a>, explored the unexpected gases that may signify life on exoplanets.



The research was focused on methyl halides, compounds made of a carbon and three hydrogen atoms bonded to a halogen, such as chlorine or bromine. 



On Earth, these gases are produced by bacteria, marine algae, fungi, and certain plants.



<h2 class="wp-block-heading" id="h-hycean-planets-and-extraterrestrial-life">Hycean planets and extraterrestrial life</h2>



Detecting these biosignatures presents challenges. Exoplanets similar to Earth are too small and dim for the James Webb Space Telescope (<a href="https://science.nasa.gov/mission/webb/" target="_blank" rel="noreferrer noopener">JWST</a>) to observe effectively. 



Instead, researchers suggest targeting hycean planets, which are larger and in orbit around small red stars.



These bodies are covered in deep oceans, and enveloped in thick hydrogen atmospheres. Though humans cannot survive on these <a href="https://www.earth.com/news/if-aliens-could-detect-earth-what-would-they-see/" target="_blank" rel="noreferrer noopener">planets</a>, some microbes might.



“Unlike an Earth-like planet, where atmospheric noise and telescope limitations make it difficult to detect biosignatures, hycean planets offer a much clearer signal,” explained Eddie Schwieterman, <a href="https://www.ucr.edu" target="_blank" rel="noreferrer noopener">UCR</a> astrobiologist and co-author of the paper .



<h2 class="wp-block-heading" id="h-practical-approach-to-finding-life">Practical approach to finding life</h2>



Scientists believe looking for methyl halides on hycean planets is a practical strategy, given current technology.



“Oxygen is currently difficult or impossible to detect on an Earth-like planet. However, methyl halides on hycean worlds offer a unique opportunity for detection with existing technology,” said Michaela Leung, UCR planetary scientist and first author of the paper.



Finding these gases could also be more efficient than searching for other <a href="https://www.earth.com/news/finding-alien-life-may-be-as-simple-as-watching-microbes-move/" target="_blank" rel="noreferrer noopener">biosignatures</a>.



“One of the great benefits of looking for methyl halides is you could potentially find them in as few as 13 hours with James Webb. That is similar or lower, by a lot, to how much telescope time you’d need to find gases like oxygen or methane,” Leung said. 



“Less time with the telescope means it’s less expensive.”



<h2 class="wp-block-heading" id="h-detecting-life-from-vast-distances">Detecting life from vast distances</h2>



Methyl halides exist on Earth in small amounts, but hycean planets could have atmospheric conditions that allow these gases to accumulate. This makes detection easier from vast distances.



“These microbes, if we found them, would be anaerobic. They’d be adapted to a very different type of environment, and we can’t really conceive of what that looks like, except to say that these gases are a plausible output from their metabolism,” Schwieterman said.



The study builds on previous research into biosignature gases, including dimethyl sulfide. 



Methyl halides stand out due to their strong absorption of infrared light and their ability to accumulate in hydrogen-rich <a href="https://www.earth.com/news/four-small-planets-discovered-orbiting-the-nearest-single-star-to-earth-barnards-star/" target="_blank" rel="noreferrer noopener">atmospheres</a>.



While JWST is currently the most powerful tool for this search, future missions could enhance detection. 



The proposed <a href="https://eu-life.eu/about/mission-values" target="_blank" rel="noreferrer noopener">European LIFE mission</a>, expected to launch in the 2040s, may confirm these biosignatures in less than a day.



“If we start finding methyl halides on multiple planets, it would suggest that microbial life is common across the universe,” Leung said. 



“That would reshape our understanding of life’s distribution and the processes that lead to the origins of life.”



<h2 class="wp-block-heading" id="h-expanding-the-search-for-extraterrestrial-life">Expanding the search for extraterrestrial life</h2>



Researchers plan to extend their investigations to other planetary types and biosignature gases. 



They have already studied gases from extreme environments on Earth, such as the Salton Sea, which emits halogenated compounds like chloroform.



“We want to get measurements of other things produced in extreme <a href="https://www.earth.com/news/dark-oxygen-in-the-deep-sea-may-hold-clues-about-alien-life/" target="_blank" rel="noreferrer noopener">environments</a> on Earth, which could be more common elsewhere,” Schwieterman said.



Direct sampling of exoplanet atmospheres remains out of reach, but advances in telescope technology and observational techniques could change that.



“Humans are not going to visit an exoplanet anytime soon,” Schwieterman said. “But knowing where to look, and what to look for, could be the first step in finding life beyond Earth.”



The study is published in <a href="https://iopscience.iop.org/article/10.3847/2041-8213/adb558" target="_blank" rel="noreferrer noopener">The Astrophysical Journal Letters</a>. 



Image Credit: NASA, ESA, CSA, Joseph Olmsted/STScI



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Weird planets may be the best place to look for strange alien life, according to new research

Scientists have searched for alien life for years, but space...

Chocolate is a comfort food for many people and a symbol of happiness in countless cultures. For years, farmers and scientists have collaborated to refine this treasured <a href="https://www.earth.com/news/sustainable-farming-could-save-the-future-of-chocolate/" target="_blank" rel="noreferrer noopener">plant</a>, but new evidence shows there is more to its story than meets the eye.



Experts have been analyzing genetic details that trace the cacao tree’s past to a surprising point in time. <a href="https://www.researchgate.net/profile/Daniel-Tineo" target="_blank" rel="noreferrer noopener">Daniel Tineo</a>, from the National University Toribio Rodríguez de Mendoza, led a study that used chloroplast genome data to examine when and how Theobroma cacao diversified.



<h2 class="wp-block-heading" id="h-chocolate-s-place-in-nature">Chocolate’s place in nature</h2>



Cacao belongs to the Malvaceae family, which also includes hibiscus and cotton. This group of plants has a history going back millions of years, and reflecting a long process of <a href="https://www.earth.com/news/chocolate-and-cocoa-prices-have-doubled-in-the-past-year-climate-change/" target="_blank" rel="noreferrer noopener">adaptation</a> and survival.



“It can be inferred that T. cacao diverged at approximately 7.55 Ma, and it is highly likely that T. cacao populations diversified during the Pliocene or Miocene,” explained Tineo. 



Two main factors appear to have played a role in shaping the trees we see today. First, their <a href="https://www.sciencedirect.com/topics/agricultural-and-biological-sciences/chloroplast-genome" target="_blank" rel="noreferrer noopener">chloroplast genomes</a> carry signs of gradual change, which is common in species that extend across tropical regions. Second, environmental pressures likely promoted different genetic traits in various localities.



<h2 class="wp-block-heading" id="h-genetic-insights-to-save-chocolate">Genetic insights to save chocolate </h2>



The chloroplast genome, often called <a href="https://www.sciencedirect.com/topics/agricultural-and-biological-sciences/chloroplast-dna" target="_blank" rel="noreferrer noopener">cpDNA</a>, is inherited in a predictable way in most plants. This trait gives scientists a clear view of family relationships, even within the same species.



One gene, named <a href="https://www.nature.com/articles/srep08348" target="_blank" rel="noreferrer noopener">ycf1</a>, turned out to be important because it showed more differences among cacao plants than other commonly studied genetic regions. By examining these differences, researchers hope to spot unique traits that may improve the flavor, resilience, or productivity of <a href="https://www.earth.com/news/cocoa-production-in-africa-is-under-extreme-climate-pressure/" target="_blank" rel="noreferrer noopener">cacao varieties</a>.



This approach might help breeders develop trees that survive better in changing climates. It may also allow them to detect disease-resistant lines, thus cutting down on the need for chemical treatments and on farm losses.



<h2 class="wp-block-heading" id="h-why-the-past-matters">Why the past matters </h2>



Farmers today face pests, diseases, and market uncertainty. Learning about cacao’s ancient lineage is not just for academic interest; it can also guide solutions that reduce farming risks.



The deeper a plant’s genetic roots, the more variation it hides in its DNA. This variation supplies fresh building blocks for traits like drought tolerance, flavor, and disease resistance.



<h2 class="wp-block-heading" id="h-practical-benefits-for-farmers">Practical benefits for farmers</h2>



Thousands of smallholders grow cacao as a main or side income. When farmers tap into genetically diverse planting materials, their crops can adapt more effectively to different environments.



A broader gene pool also lowers the chance that a single disease outbreak will devastate cacao plants in an entire region. Strengthening genetic tools for farmers promotes stable harvests and consistently better beans.



<h2 class="wp-block-heading" id="h-modern-breeding-methods">Modern breeding methods</h2>



Classic breeding methods rely on observing which trees yield the best crops. Now, molecular tools add a scientific boost by marking the genes that truly matter.



When breeders target specific genes - like ycf1 - they can make more precise matches between strong, disease-tolerant varieties and those with desired flavors. This level of detail speeds up the long process of developing improved trees.



<h2 class="wp-block-heading" id="h-balancing-tradition-with-discovery">Balancing tradition with discovery</h2>



Farmers in Latin America, Africa, and Asia have nurtured cacao for generations. Their local expertise is valuable when it comes to spotting subtle differences among trees.



Collaboration between traditional growers and research institutions bridges technology and cultural wisdom. This approach promotes new partnerships that benefit everyone, from growers to chocolate enthusiasts.



<h2 class="wp-block-heading" id="h-protecting-the-future-of-chocolate">Protecting the future of chocolate </h2>



Scientists still do not fully understand how <a href="https://www.nature.com/articles/s41586-022-05288-7" target="_blank" rel="noreferrer noopener">nuclear or mitochondrial data</a> compare with chloroplast results. More work is needed to fill the gaps left by incomplete samples from various parts of the tropics.



Some lines may carry rare genetic elements waiting to be explored. Locating these hidden genes could reveal new ways to manage diseases and keep farms flourishing.



Cacao stands at a crossroads of heritage, commerce, and science. Studies suggest that this plant’s DNA is more varied and ancient than was once believed, hinting that there may be more secrets in its cells.



Ongoing research may answer questions about how different cacao types emerged and how they can be preserved. The bigger picture promises a future where growers and chocolate lovers share the rewards of knowledge-driven innovation.



The study is published in the journal <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0316148" target="_blank" rel="noreferrer noopener">PLOS One</a>.



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Can chocolate survive? DNA research may help save cacao trees

Chocolate is a comfort food for many people and a...

People on a fishing boat in the Aegean Sea had an unsettling experience when they noticed square waves creating a chessboard-like pattern all around them. This phenomenon, which quickly drew concern, is an unusual sight in the ocean.



Square waves, also known as a cross sea, are caused by two interacting <a href="https://www.earth.com/news/sinking-land-will-intensify-the-effects-of-rising-sea-levels/" target="_blank" rel="noreferrer noopener">wave systems</a> traveling at different speeds and trajectories.



This activity was examined by <a href="https://iris.cnr.it/cris/rp/rp12539" target="_blank" rel="noreferrer noopener">Dr. Silvio Davison</a> from the Consiglio Nazionale delle Ricerche (<a href="https://www.cnr.it/" target="_blank" rel="noreferrer noopener">CNR</a>), Istituto di Scienze Marine (<a href="https://www.ismar.cnr.it/web-content/" target="_blank" rel="noreferrer noopener">ISMAR</a>) in Venice, Italy.



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



Ocean waves are nature’s way of keeping the sea in constant motion. Wind blows across the surface, transferring its energy to the water and creating waves that can travel thousands of miles.



The size and strength of a wave depend on three things: wind speed, how long the wind blows, and the distance it travels over open water (also called fetch). The longer and stronger these forces act, the bigger the waves get.



But not all waves come from the wind. Some, like <a href="https://www.earth.com/news/lake-tsunamis-are-an-emerging-climate-linked-hazard/" target="_blank" rel="noreferrer noopener">tsunamis</a>, are triggered by underwater earthquakes, volcanic eruptions, or landslides.



Then there are tidal waves, which are actually caused by the gravitational pull of the Moon and Sun, not wind or sudden underwater events.



Next we have <a href="https://www.earth.com/news/most-extreme-rogue-wave-recorded-in-the-pacific-ocean/" target="_blank" rel="noreferrer noopener">rogue waves</a>, which are are massive, unpredictable walls of water that seem to appear out of nowhere. 



Rogue waves happen due to complex interactions between ocean currents, wind, and smaller waves merging at just the right moment. Some can reach over 100 feet (30 meters) tall, powerful enough to sink even large ships.



Finally, we have square waves, which is the reason that we're all here right now.



<h2 class="wp-block-heading" id="h-causes-behind-the-grid">Causes behind the grid</h2>



Ocean dynamics can sometimes lead to waves from separate storms merging at sharp angles. When that overlap happens, the surface arranges itself into a repeating, square-like shape.



This can vanish quickly if the wind shifts or if one wave set loses energy. On other occasions, the pattern remains long enough for unwary surfers or vessels to run into trouble.



<a href="https://www.frontiersin.org/journals/marine-science/articles/10.3389/fmars.2022.1002806/full" target="_blank" rel="noreferrer noopener">Researchers</a> have noted that such interactions are more common in open waters with multiple strong weather systems. 



Storm tracks crossing each other can spark chaotic <a href="https://www.earth.com/news/ocean-warming-broke-records-for-450-straight-days/" target="_blank" rel="noreferrer noopener">wave</a> fields that keep everyone on edge.



<h2 class="wp-block-heading" id="h-impact-on-maritime-travel">Impact on maritime travel</h2>



Large <a href="https://www.noaa.gov/jetstream/ocean/rip-currents/rip-current-safety" target="_blank" rel="noreferrer noopener">cross seas</a> can reach heights of nearly 10 feet (3 meters), which is problematic for smaller boats. Faced with perpendicular waves, even a ship may roll unpredictably.



According to the <a href="https://business.esa.int/maritime" target="_blank" rel="noreferrer noopener">European Space Agency</a>, data collected between 1995 and 1999 showed that a large proportion of ship accidents occurred in cross seas. This highlights the threat posed by these shifting forces.



Sailors in these conditions report abrupt lurches and sudden veering. Cargo ships can also face cargo shifts when waves slam from two different angles.



<h2 class="wp-block-heading" id="h-swimmers-should-avoid-square-waves">Swimmers should avoid square waves</h2>



“Swimmers are at risk of being swept away, while boaters can experience navigational problems.” This note of caution from <a href="https://nhess.copernicus.org/articles/21/115/2021/nhess-21-115-2021.html" target="_blank" rel="noreferrer noopener">maritime observers</a> is especially relevant in unpredictable waters.



Opposing currents make it hard for people to fight the pull toward deeper areas. Sections of the sea floor can slope in unexpected ways, which compounds the danger.



Checkered wave events have drawn attention in certain tourist destinations. In places where the phenomenon is less intense, onlookers sometimes gather to watch the spectacle.



A noteworthy location is Île de Ré, near France, where visitors sometimes ascend a lighthouse to see the square pattern. They might not recognize that, out in deeper waters, the same sight can be much more powerful.



<h2 class="wp-block-heading" id="h-precautions-and-advice">Precautions and advice</h2>



Maritime authorities suggest that if a grid-like sea surface is spotted, smaller crafts should stay nearer to shore. Rapid changes can make it tough for seafarers to maneuver.



Some wave specialists recommend altering course to avoid perpendicular wave trains entirely, while others suggest that slowing down can minimize the stress on a vessel’s structure.



Swimmers are urged to exit the water if they notice conflicting currents. Strong swimmers often underestimate lateral pushes that can tire them quickly.



<h2 class="wp-block-heading" id="h-new-technology-to-study-square-waves">New technology to study square waves</h2>



Scientists are examining ways to forecast cross seas more accurately. They hope better models will help shipping routes avoid high-risk zones.



Advanced radar networks are collecting data on wave heights, angles, and directions. These tools might enhance warnings about any abrupt formation of intersecting waves.



Some labs now rely on <a href="https://www.baslerweb.com/en/cameras/basler-stereo-camera/?srsltid=AfmBOoojjrrNlPY291861Z4Kfl0bmQMlssog8JwjcqK_fNtpUb4kFR8Q" target="_blank" rel="noreferrer noopener">stereo camera systems</a> to capture wide surface areas. This technology allows them to document the biggest crests in cross <a href="https://www.earth.com/news/north-atlantic-ocean-has-a-memory-that-lasts-up-to-20-years/" target="_blank" rel="noreferrer noopener">seas</a> with more accuracy.



Digital simulations, like the <a href="https://www.sciencedirect.com/science/article/pii/S246801331730044X" target="_blank" rel="noreferrer noopener">High-Order Spectral method</a>, add another layer of understanding. They reveal how separate swells interact in real time, helping experts refine safety recommendations.



<h2 class="wp-block-heading" id="h-visually-intriguing-yet-dangerous">Visually intriguing yet dangerous </h2>



Cross seas are visually intriguing yet dangerous for unaware travelers. They remind us that the <a href="https://www.earth.com/news/earths-oceans-are-rapidly-changing-colors-matching-climate-predictions/" target="_blank" rel="noreferrer noopener">ocean</a>’s complexity sometimes slips under the radar.



Predicting the square waves calls for close attention to wind shifts and storm paths. Such vigilance may keep mariners and beachgoers out of harm’s way.



Researchers continue to emphasize caution when these wave patterns arise, especially in open oceans.



The study is published in <a href="https://www.frontiersin.org/journals/marine-science/articles/10.3389/fmars.2022.1002806/full" target="_blank" rel="noreferrer noopener">Frontiers in Marine Science</a>.



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Square waves: The deadly chessboard pattern threatening sailors

People on a fishing boat in the Aegean Sea had...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

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

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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

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



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



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



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



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



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



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



Video Credit: Amanda Nguyen/University of Illinois



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



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

Designing crops that can beat the heat

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