Looking at the Farallones today, it is easy to understand why early colonists might have given them a wide berth. Named after the Spanish word for cliff, they loom out of the entrance to San Francisco Bay, creating an ominous shadow on the horizon. And the islands don’t just look spooky, either – they’re guarding a number of dark secrets that have kept humans away for generations. Photo Credit: Thomas Winz/Getty Images

Ominous presence

Today's Image of the Day from the European Space Agency features NGC 6744 - a large, barred spiral galaxy located approximately 30 million light-years away in the constellation Pavo.&nbsp;



The galaxy is often considered a close analog to the <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a> due to its similar structure and size, spanning about 175,000 light-years across.&nbsp;



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



The image was captured by the <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid</a> space telescope. NGC 6744 stands out as a prime example of the galaxies currently forming the majority of stars in the nearby universe, making it an ideal subject for study with the Euclid mission.&nbsp;



Euclid’s extensive field-of-view allows it to capture the entire galaxy, showcasing not only its large-scale spiral structure but also revealing intricate details on smaller scales across various wavelengths. These details include feather-like dust lanes, known as “spurs,” emerging from the spiral arms.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-6744">Star formation in NGC 6744</h2>



Euclid's observations enable scientists to count individual stars within NGC 6744, trace the distribution of stars and dust throughout the galaxy, and map the dust associated with the gas that fuels the development of new stars. 



<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> is a key process in the growth of galaxies, making these studies crucial for understanding galaxy evolution.



Researchers are utilizing Euclid’s data to explore the relationship between dust, gas, and star formation; to map the distribution of different stellar populations and identify regions of active star formation; and to investigate the underlying physics of spiral galaxy structures.&nbsp;



Spiral arms play a significant role in star formation by compressing gas, yet the precise mechanisms behind this process are still unclear. The presence of “spurs” along NGC 6744’s spiral arms offers valuable insights into the dynamics of star formation within these structures.



<h2 class="wp-block-heading" id="h-discovering-new-dwarf-galaxies-nbsp">Discovering new dwarf galaxies&nbsp;</h2>



Additionally, Euclid's dataset will help scientists identify clusters of old stars (globular clusters) and discover new dwarf galaxies around NGC 6744. Remarkably, Euclid has already identified a new dwarf satellite galaxy of NGC 6744 - a surprising discovery given that the galaxy has been studied extensively.



With Euclid’s detailed observations, scientists are gaining a deeper understanding of the processes shaping galaxies, providing essential clues to the evolution and appearance of the <a href="https://www.earth.com/news/universes-expansion-rate-hubble-tension-puzzles-astronomers/" target="_blank" rel="noreferrer noopener">universe</a>.



<h2 class="wp-block-heading" id="h-more-about-ngc-6744">More about NGC 6744</h2>



NGC 6744's disk is rich in star-forming regions and contains numerous young, bright blue stars. The galaxy's nucleus is slightly elongated and has a bar structure, which influences the motion of the stars and gas within it.&nbsp;



The spiral arms of NGC 6744 are well-defined and extend outward, wrapping around the central bar. Additionally, NGC 6744 has a smaller companion galaxy, NGC 6744A, which is interacting with it, adding to the complexity and interest of this distant system.&nbsp;



<h2 class="wp-block-heading" id="h-spiral-galaxies">Spiral galaxies</h2>



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are one of the most common types of galaxies in the universe, characterized by their distinct, spiral-shaped structure.&nbsp;



The galaxies typically consist of a flat, rotating disk containing stars, gas, and dust, along with a central concentration of stars known as the bulge. This bulge is often surrounded by a halo of older stars.&nbsp;



The spiral arms, which extend from the central bulge, are regions of active star formation and are rich in young, hot stars, giving them a bright, bluish appearance.&nbsp;



These arms are also sites where interstellar gas and dust are concentrated, leading to the formation of new stars.&nbsp;



Spiral galaxies are classified into different types based on the tightness of their spirals and the size of their central bulge, with classifications ranging from tightly wound arms in Sa galaxies to more loosely wound arms in Sc galaxies. The <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our home galaxy, is a prime example of a spiral galaxy.



<h2 class="wp-block-heading" id="h-the-constellation-pavo">The constellation Pavo</h2>



Pavo, which means "peacock" in Latin, is a constellation in the southern sky. It was named by the Dutch astronomer Petrus Plancius in the late 16th century, based on observations made during the Dutch explorations of the southern hemisphere. 



Pavo is one of the 12 constellations created by Plancius from the records of explorers Pieter Dirkszoon Keyser and Frederick de Houtman. 



The constellation is known for its distinctive shape, resembling a peacock with a long, curved tail. Pavo is not visible from most of the northern hemisphere, but it can be seen from the southern hemisphere, particularly during the winter months.



The constellation contains several interesting celestial objects, including the star Peacock, also known as Alpha Pavonis, which is the brightest star in the constellation. This star is a blue-white subgiant located about 179 light-years from Earth.



Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Euclid/Euclid Consortium/NASA&nbsp;



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Spiral galaxy NGC 6744 in the constellation Pavo

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

Today's Image of the Day from NASA Earth Observatory features an active landslide zone that has been shifting for decades on the Palos Verdes Peninsula in Los Angeles County.



This area, particularly in Portuguese Bend, experiences ongoing ground movement, with land sliding toward the ocean at varying rates - sometimes moving several feet per year.&nbsp;



The instability is largely due to weak, water-saturated bedrock and the effects of <a href="https://www.earth.com/news/rising-seas-sinking-cities-land-subsidence-on-the-east-coast/">human activity</a>, including road construction and irrigation, which have exacerbated the natural movement.



<h2 class="wp-block-heading" id="h-analysis-of-the-landslide-zone">Analysis of the landslide zone</h2>



According to a recent report from NASA, the landslide zone on the Palos Verdes Peninsula has expanded.&nbsp;



“Researchers at NASA’s Jet Propulsion Laboratory in Southern California used data from an airborne radar to measure the movement of the slow-moving landslides on the Palos Verdes Peninsula in Los Angeles County,” the <a href="https://earthobservatory.nasa.gov/images/153893/los-angeles-area-landslide-expands">report</a> stated.



“The analysis determined that, during a four-week period in the fall of 2024, land in the residential area slid toward the ocean by as much as 4 inches (10 centimeters) per week."



“Portions of the peninsula, which juts into the Pacific Ocean just south of the city of Los Angeles, are part of an ancient complex of landslides that has been moving for at least the past six decades, affecting hundreds of buildings in local communities.”&nbsp;



NASA noted that the motion accelerated and the active area expanded following record-breaking rainfall in Southern California in 2023 and heavy <a href="https://www.earth.com/news/rainfall-is-increasingly-unpredictable-due-to-climate-change/" target="_blank" rel="noreferrer noopener">precipitation</a> in early 2024.



<h2 class="wp-block-heading" id="h-visualization-of-the-landslide-zone">Visualization of the landslide zone</h2>



To create the image, the Advanced Rapid Imaging and Analysis (ARIA) team used data from four flights of NASA’s Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) collected between September 18 and October 17, 2024.&nbsp;



“The UAVSAR instrument was mounted to a Gulfstream III jet flown out of NASA’s Armstrong Flight Research Center in Edwards, California, and the four flights were planned to estimate the speed and direction of the landslides in three dimensions,” explained NASA.



“In the image above, colors indicate how fast parts of the landslide complex were moving in late September and October, with the darkest reds indicating the highest speeds." 



"The arrows represent the direction of horizontal motion. The white solid lines are the boundaries of the active landslide area as defined in 2007 by the California Geological Survey.”



<h2 class="wp-block-heading" id="h-accelerating-land-movement-and-risks">Accelerating land movement and risks</h2>



Alexander Handwerger is a landslide scientist at the Jet Propulsion Laboratory who performed the analysis. “In effect, we’re seeing that the footprint of land experiencing significant impacts has expanded, and the speed is more than enough to put human life and infrastructure at risk,” said Handwerger. 



The landslide activity in this region dates back to the 1950s, when road construction projects disturbed the already <a href="https://www.earth.com/news/two-billion-people-are-threatened-by-land-subsidence/">unstable terrain</a>, accelerating movement.&nbsp;



Since then, shifting ground has led to significant damage to infrastructure, including cracked roads, broken utility lines, and distorted buildings. The instability has made it difficult for the city to maintain roads and essential services in the affected areas.



Despite efforts to slow the movement, including drainage improvements and engineering solutions, the land continues to shift. Homeowners and city officials have had to adapt, with some structures built to withstand slow movement, while others have been abandoned.&nbsp;



The situation remains a challenge, with scientists monitoring the landslide to better understand its <a href="https://www.earth.com/news/landslide-predictions-could-become-94-percent-more-accurate/">behavior</a> and explore potential mitigation strategies.



Portuguese Bend is a well-known example of a continuously active landslide, highlighting the complex interaction between geology, human development, and environmental forces.



Image Credit: NASA Earth Observatory&nbsp;



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Landslide zone in Los Angeles County is expanding

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA 



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

Today's Image of the Day from the European Space Agency features a brilliant stellar nursery located about 163,000 light-years away.



According to ESA, the image is one of the most photogenic examples of the many stellar nurseries observed by the NASA/ESA Hubble Space Telescope during its 30-year lifetime. 



“The portrait features the giant nebula NGC 2014 and its neighbor NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



<h2 class="wp-block-heading" id="h-what-is-a-stellar-nursery">What is a stellar nursery?</h2>



Stellar nurseries are regions in space where new stars are <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">born</a> - often within vast clouds of gas and dust called molecular clouds.&nbsp;



These areas are fascinating because they are cradles of stellar evolution, where gravity causes clumps of gas to collapse, eventually forming protostars.&nbsp;



Over time, the protostars will heat up and start the nuclear fusion process that powers a star.



One of the most well-known stellar nurseries is the Orion Nebula, which is visible to the naked eye and located about 1,350 light-years from Earth.&nbsp;



<h2 class="wp-block-heading" id="h-dynamic-nature-of-a-stellar-nursery-nbsp">Dynamic nature of a stellar nursery&nbsp;</h2>



Within these nurseries, the balance between gravity and pressure determines the types of stars that form, from massive, luminous stars to smaller, cooler ones like our Sun.&nbsp;



The environment is incredibly dynamic, with powerful winds from young stars shaping the clouds and triggering the birth of even more stars.



These regions are often illuminated by the light from massive newborn stars - creating stunning, colorful displays. The light reveals the intricate structure of the dust and gas, sculpted by the energy of young stars.&nbsp;



<h2 class="wp-block-heading" id="h-significance-of-stellar-nurseries-nbsp">Significance of stellar nurseries&nbsp;</h2>



Stellar nurseries are essential for understanding the early stages of planetary formation, as protoplanetary disks (the material from which <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planets form</a>) are often found around young stars in these regions.



Stellar nurseries play a crucial role in the ongoing evolution of <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">galaxies</a>. They are responsible for the continuous birth of new stars that enrich the interstellar medium with heavier elements. This constant recycling of material is key to the development of future generations of stars and planets.&nbsp;



Furthermore, the study of these regions helps astronomers understand the fundamental processes that govern the life cycles of stars and the overall dynamics of the universe.



<h2 class="wp-block-heading" id="h-the-local-group">The Local Group</h2>



The Local Group is a collection of over 80 galaxies that includes the Milky Way, the Andromeda Galaxy, and the Triangulum Galaxy, along with numerous smaller dwarf galaxies. These galaxies are bound together by gravity and span a region roughly 10 million light-years across.&nbsp;



The <a href="https://www.earth.com/news/milky-ways-thin-disk-is-billions-of-years-older-than-we-thought/" target="_blank" rel="noreferrer noopener">Milky Way</a> and Andromeda are the dominant members, with their respective satellite galaxies orbiting them.&nbsp;



The Local Group is part of a larger structure known as the Virgo Supercluster, and its galaxies are moving toward the gravitational center of the Local Group, contributing to its dynamic nature.&nbsp;



<h2 class="wp-block-heading" id="h-large-magellanic-cloud">Large Magellanic Cloud</h2>



The Large Magellanic Cloud (LMC) is the fourth largest galaxy in the Local Group and can be seen with the naked eye from the Southern Hemisphere.&nbsp;



This irregular dwarf galaxy is home to the Tarantula Nebula, one of the most active star-forming regions in our cosmic neighborhood.&nbsp;



The Large Magellanic Cloud played a key role in astronomical history, particularly when the supernova SN 1987A was observed, providing valuable insights into stellar evolution.&nbsp;



The LMC's interaction with the Milky Way, along with its own companion, the Small Magellanic Cloud, is believed to influence its shape and star formation activity. Its proximity and unique properties make it a crucial object of study for understanding <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>, star formation, and the dynamics of interacting galaxies.



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young, massive stars in the Triangulum Galaxy

Today's Image of the Day from the European Space Agency features a stunningly beautiful photo of the Hainan Strait. The image was captured by the Copernicus Sentinel-2 satellite as it orbited over southern China.



“The Hainan Strait, or Qiongzhou Strait, separates Guangdong's Leizhou Peninsula on China’s mainland to the north and the island province of Hainan to the south. It also connects the Gulf of Tonkin on the west to the South China Sea on the east,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



<h2 class="wp-block-heading" id="h-hainan-strait-nbsp">Hainan Strait&nbsp;</h2>



The Hainan Strait is narrow and shallow. At its narrowest point, the strait is about 19 miles wide. Despite this, the Hainan Strait is a busy route for shipping and transportation. It's also vital to local <a href="https://www.earth.com/news/dark-fleets-hidden-industrial-fishing-activity-exposed/" target="_blank" rel="noreferrer noopener">fishing</a> industries.



ESA pointed out that in the image, the water along the coasts is light brown due to sediment runoff. 



“The curved Leizhou Peninsula juts southward into the South China Sea. The largest island on the east coast, Donghai, forms two bays: Leizhou Bay to its south and Zhanjiang Bay to its north," noted ESA.



“Facing both bays are cities with the same names: Zhanjiang, the largest city on the peninsula, and Leizhou, which gave the peninsula its name." 



"Hainan Island dominates the bottom part of the image. The name Hainan means ‘south of the sea,’ reflecting the island's position south of the strait.”



<h2 class="wp-block-heading" id="h-history-of-hainan-island">History of Hainan Island </h2>



During the Mesozoic Era about 100 million years ago, Hainan Island was actually part of a larger landmass connected to <a href="https://www.earth.com/news/denisovan-tooth-suggests-southeast-asia-was-a-human-diversity-hotspot/" target="_blank" rel="noreferrer noopener">Southeast Asia</a>. 



<h3 class="wp-block-heading" id="h-geological-features">Geological features</h3>



Over time, the movements of Earth's plates caused this landmass to break apart and drift. Hainan separated from the continental shelf near Vietnam and moved to its current position.



This tectonic activity not only shaped the island's current location but also influenced its geological features. Hainan's landscape is characterized by <a href="https://www.earth.com/news/how-and-why-do-mountains-form-new-theories-for-an-age-old-mystery/" target="_blank" rel="noreferrer noopener">mountains</a>, volcanic formations, and rich mineral deposits, which are direct results of these ancient geological processes.



Understanding this geological history helps explain why Hainan Island has such unique and diverse natural features compared to the mainland of China and nearby regions. The island's distinct wildlife and terrain make it a fascinating subject for geologists and natural historians alike.



<h3 class="wp-block-heading" id="h-cultural-diversity-nbsp">Cultural diversity&nbsp;</h3>



Hainan was once a remote and undeveloped part of China. It was used as a place of exile for disgraced officials during imperial times. 



However, it was also a place where diverse <a href="https://www.earth.com/news/humans-are-not-the-only-animals-that-create-their-own-culture/" target="_blank" rel="noreferrer noopener">cultures</a> met, as evidenced by the many ethnic groups that live there, including the Li people, who are indigenous to the island.



The island really started to change in the 20th century. During the Second Sino-Japanese War, Hainan was occupied by Japanese forces, which had a significant impact on its development. After the war, it became a part of the People’s Republic of China in 1950.&nbsp;



<h3 class="wp-block-heading" id="h-rapid-development-nbsp">Rapid development&nbsp;</h3>



In the 1980s, Hainan was designated a Special Economic Zone (SEZ), which marked the beginning of its transformation into a major economic and tourist hub. 



The SEZ status attracted significant investment and spurred rapid development, particularly in the capital city of Haikou and the resort city of Sanya.



Today, Hainan is known for its lush landscapes, tropical <a href="https://www.earth.com/news/caribbean-salt-affects-global-climate-study-reveals/" target="_blank" rel="noreferrer noopener">climate</a>, and booming tourism industry. It's also becoming a key player in China's efforts to develop its free trade zones, aiming to become a major center for trade and commerce in the region.



Image Credit: ESA/ Copernicus Sentinel-2&nbsp;



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Hainan Strait in southern China

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 Messier 78 (M78), a reflection nebula located in the constellation Orion about 1,350 light-years away from Earth. 



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



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



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



Featured here is a high-resolution, detailed segment of a larger image showcasing Messier 78, a dynamic region of star formation obscured by cosmic dust.&nbsp;



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp-0">Euclid space mission&nbsp;</h2>



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



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



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



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



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



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



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



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



Image Credit: European Space Agency&nbsp;



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Messier 78: Young stars shine through dense dust

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

Plant lovers have experimented with everything from eggshell powder to coffee grounds to help their greenery thrive. While some of these methods are effective, a homemade, chlorophyll-rich fertilizer known as "green gold" is gaining attention among gardening enthusiasts.



Dr. Cristhian Josue Cedeno from the <a href="https://www.utm.edu.ec/" target="_blank" rel="noreferrer noopener">Technical University of Manabí</a> has shared new insights on how nutrient-rich preparations can influence plant growth and vitality.



This knowledge aligns with the idea that plants are more than decorations: they are complex organisms that respond well to science-backed care.



<h2 class="wp-block-heading" id="h-chlorophyll-rich-fertilizer">Chlorophyll-rich fertilizer </h2>



Bold, bright leaves are full of <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC10384064/" target="_blank" rel="noreferrer noopener">chlorophyll</a>, the natural pigment responsible for a plant’s green shade. When leaves appear pale or lifeless, it can signal a nutrient deficiency that basic watering cannot fix. Chlorophyll-rich fertilizers may fill that gap by boosting a plant’s photosynthetic process. One promising organic option is LVEB (bovine manure vermicompost leachate), a liquid derived from composted cattle manure that has been processed by earthworms.&nbsp;



This nutrient-rich solution enhances soil quality, promotes <a href="https://www.earth.com/news/beneficial-plant-bacteria-likely-to-decline-due-to-climate-change/">beneficial microbes</a>, and provides essential minerals like magnesium, which directly support chlorophyll production. 



Unlike synthetic fertilizers, LVEB improves plant health naturally, making it a sustainable choice for home gardeners and farmers alike.



“The 1:30 dilution of the LVEB stood out above the remaining ones, showing significantly greater increases than chemical fertilization for plant height, stem diameter, leaf quantity, total chlorophyll content, and increasing yield by 1,28 t/ha compared to plants that received chemical fertilizer,” said study co-author Cedeno Solorzano.



<h2 class="wp-block-heading" id="h-hidden-power-of-magnesium">Hidden power of magnesium</h2>



“Magnesium plays a critical role in plant metabolism as it is the central atom in chlorophyll molecules,” explained Shaul O, from <a href="https://www.biu.ac.il/en" target="_blank" rel="noreferrer noopener">Bar-Ilan University</a>.



Anyone frustrated with sickly plants might consider the importance of <a href="https://ods.od.nih.gov/factsheets/Magnesium-HealthProfessional/" target="_blank" rel="noreferrer noopener">magnesium</a>, which is a crucial mineral in every chlorophyll molecule.&nbsp;



If leaves appear yellow or growth seems sluggish, magnesium deficiency could be an underlying factor. Dark, leafy material used in homemade fertilizer solutions may add a direct supply of this nutrient.



<h2 class="wp-block-heading" id="h-supporting-healthy-soil-with-chlorophyll-fertilizer">Supporting healthy soil with chlorophyll fertilizer </h2>



Adequate <a href="https://bioenergy.asu.edu/why-study-photosynthesis" target="_blank" rel="noreferrer noopener">photosynthesis</a> is important, but roots and soil also deserve attention. Healthy soil provides the foundation for strong plant growth, influencing nutrient absorption, moisture retention, and resistance to disease.



“Organic amendments supply readily available carbon and nutrients that stimulate soil microbial biomass and activity," stated H. J. McGovern from the <a href="https://scri.webarchive.hutton.ac.uk/" target="_blank" rel="noreferrer noopener">Scottish Crop Research Institute</a>.



"This microbial stimulation not only accelerates the decomposition of organic matter but also enhances the availability of essential nutrients to plants, ultimately leading to improved plant growth and soil health."



Homemade chlorophyll fertilizer functions like other organic solutions by feeding beneficial microbes. Healthier soil creates a better environment for roots to access water and nutrients.



<h2 class="wp-block-heading" id="h-preparing-chlorophyll-fertilizer">Preparing chlorophyll fertilizer</h2>



Gardeners often harvest the greenest leaves from shrubs that hold onto their color year-round. These leaves are placed in a blender with around one quart of water to form a rich, dark mixture.



Straining the blend removes chunky bits, and a brief bain-marie heating for about 5 to 10 minutes helps release the essential pigments. This simple recipe is then used in place of typical watering routines every couple of weeks.



<h2 class="wp-block-heading" id="h-maintaining-steady-progress">Maintaining steady progress</h2>



Tracking improvement can be as simple as checking leaves for a vibrant hue. <a href="https://www.earth.com/news/plants-with-wilting-flowers-arent-dying-they-are-saving-energy/">Wilted or droopy plants</a> often show renewed structure after consistent application of the chlorophyll-rich brew.



It pays to stay mindful of the soil’s moisture content and drainage status so that excess water does not cause roots to suffocate. The combination of appropriate watering, sunlight, and nutrient balance keeps plants in good shape.



<h2 class="wp-block-heading" id="h-a-greener-approach">A greener approach</h2>



“The application of organic amendments improves soil physical properties such as structure, porosity, and water retention," noted the Food and Agriculture Organization (<a href="https://www.fao.org/home/en" target="_blank" rel="noreferrer noopener">FAO</a>).



"In turn, these improvements support a more active microbial community that enhances nutrient cycling and overall soil fertility.” 



Sustainability is a crucial point for many who prefer organic methods.&nbsp;



Homemade chlorophyll solutions fit this mindset by reducing dependence on chemical fertilizers. The steps rely on easily available plant material, which makes the process affordable and eco-friendly.



Using the green gold approach can be an encouraging way to nurse neglected houseplants back to health. The steps are quick, and the benefits become visible in the form of stronger leaves and sturdier stems.



The study is published in the journal <a href="https://dialnet.unirioja.es/descarga/articulo/8232839.pdf?utm_source=chatgpt.com" target="_blank" rel="noreferrer noopener">La Técnica</a>.



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Gardening hack called 'green gold' works like magic for houseplants

Plant lovers have experimented with everything from eggshell powder to...

New research reveals that subtle shifts in land elevation can considerably increase or decrease the local impacts of sea level rise along coastlines.&nbsp;



Even though these changes usually amount to fractions of an inch per year, they may alter flood risk, wave exposure, and saltwater intrusion for nearby communities.



<h2 class="wp-block-heading" id="h-looking-beyond-ocean-heights">Looking beyond ocean heights</h2>



Accurately predicting future <a href="https://www.earth.com/news/global-sea-levels-spiked-dramatically-in-2023/" target="_blank" rel="noreferrer noopener">sea level rise</a> involves more than measuring how high the oceans climb. It also requires determining whether coastal lands are subsiding or uplifting.&nbsp;



A <a href="https://www.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>-led study focused on California demonstrates how slow vertical movement of the land could have serious implications for areas already dealing with the challenges of a warming planet.



Sea levels along California’s coastline are projected to rise by 6 to 14.5 inches (15 to 37 centimeters) above year 2000 levels by 2050, mainly due to <a href="https://www.earth.com/news/melting-glaciers-are-reshaping-landscapes-and-national-borders-around-the-world/" target="_blank" rel="noreferrer noopener">melting glaciers</a> and ice sheets, as well as the thermal expansion of warming ocean waters. 



However, the recent study emphasizes that a better grasp of land elevation trends is crucial for refining local sea level forecasts.



“In many parts of the world, like the reclaimed ground beneath San Francisco, the land is moving down faster than the sea itself is going up,” said lead author Marin Govorcin, a remote sensing scientist at <a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA’s Jet Propulsion Laboratory</a> in Southern California.



<h2 class="wp-block-heading" id="h-tracking-land-motion-in-detail">Tracking land motion in detail</h2>



The new research also highlights that the pace and scale of vertical land motion vary widely, shaped by both natural processes - such as tectonic activity - and human endeavors like <a href="https://www.earth.com/news/pumping-too-much-groundwater-affects-earths-spin/" target="_blank" rel="noreferrer noopener">groundwater pumping</a> or wastewater injection.&nbsp;



Previous regional models relying on tide gauges cannot capture all these dynamic changes or produce the detailed local picture that direct satellite observations now enable.



Scientists from NASA’s Jet Propulsion Laboratory (JPL) and the <a href="https://www.noaa.gov/" target="_blank" rel="noreferrer noopener">National Oceanic and Atmospheric Administration</a> (NOAA) used satellite radar to study over a thousand miles of California’s coastline.&nbsp;



The experts identified multiple “hotspots,” including urban centers, beaches, and aquifers, where the sinking or rising of land could interact with ongoing sea level rise in significant ways.



<h2 class="wp-block-heading" id="h-shifting-land-and-rising-sea-levels">Shifting land and rising sea levels</h2>



By analyzing radar measurements from <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a>’s Sentinel-1 satellites and velocity data from ground-based Global Navigation Satellite System stations, the researchers pinpointed areas experiencing subsidence of more than 0.4 inches (10 millimeters) per year.



Regions like San Rafael, Corte Madera, Foster City, and Bay Farm Island in the San Francisco Bay Area are gradually sinking due to sediment compaction, among other factors.&nbsp;



As a result, projected sea levels in these localities could exceed 17 inches (45 centimeters) by 2050 - over twice the general regional estimate of 7.4 inches (19 centimeters) indicated by tide gauge data.



Certain areas, however, are rising. The Santa Barbara groundwater basin has been slowly lifting since 2018 thanks to aquifer replenishment, while Long Beach exhibited uplift driven by fluid extraction and injection linked to oil and gas activities.



In parts of Los Angeles and San Diego Counties, human-driven changes in land motion increase sea level projections by as much as 15 inches (40 centimeters). Groundwater use, hydrocarbon extraction, and other unpredictable land-use practices raise uncertainties that demand vigilant, real-time monitoring.



<h2 class="wp-block-heading" id="h-dowmward-drifting-terrain">Dowmward-drifting terrain</h2>



Farther inland, the Central Valley experiences rapid sinking - sometimes up to 8 inches (20 centimeters) annually - because of widespread groundwater withdrawals.&nbsp;



Scientists also recorded cyclical patterns of rising and falling land in Santa Clara, Santa Ana, and Chula Vista, correlated with fluctuations in <a href="https://www.earth.com/news/how-changing-rainfall-patterns-impact-plants-worldwide/" target="_blank" rel="noreferrer noopener">rainfall</a> and drought.&nbsp;



In geologically active coastal regions like Big Sur and Palos Verdes, slow-moving landslides are causing portions of terrain to drift downward. Around San Francisco and Monterey bays, subsiding marshes and lagoons highlight erosion’s role in land changes.



<h2 class="wp-block-heading" id="h-changes-in-the-coming-decades">Changes in the coming decades</h2>



Policymakers, the public, and scientists can keep an eye on coastal land motion through the <a href="https://www.jpl.nasa.gov/go/opera/" target="_blank" rel="noreferrer noopener">OPERA</a> (Observational Products for End-Users from Remote Sensing Analysis) initiative, led by JPL.&nbsp;



This project details surface elevation changes across North America, including subsidence zones, tectonic shifts, and landslide-prone areas.&nbsp;



The data will become even more precise once the next-generation <a href="https://nisar.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">NISAR</a> (NASA-Indian Space Research Organization Synthetic Aperture Radar) mission is launched in the coming months.



By incorporating satellite-based measurements of land elevation changes into broader sea level rise models, researchers hope to provide more accurate and actionable forecasts. The goal is to help coastal communities develop more robust strategies for coping with climate change in the decades to come.



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Sinking land will intensify the effects of rising sea levels

New research reveals that subtle shifts in land elevation can...

Who is most vulnerable to online misinformation and why? A new study offers a revealing look at how different demographic and psychological factors - such as age, education, political identity, and analytical thinking - shape individuals’ ability to assess the accuracy of news.&nbsp;



Researchers at the Max Planck Institute for Human Development analyzed data from 31 experiments conducted in the United States between 2006 and 2023.



Surprisingly, the findings do not align with many long-held assumptions about who is more likely to be duped by fake news.



<h2 class="wp-block-heading" id="h-demographics-psychological-factors-and-fake-news">Demographics, psychological factors, and fake news</h2>



The study was led by Mubashir Sultan, a doctoral candidate at the <a href="https://www.mpib-berlin.mpg.de/en" target="_blank" rel="noreferrer noopener">Max Planck Institute for Human Development</a>’s Center for Adaptive Rationality.&nbsp;



Sultan and his colleagues performed an individual participant data meta-analysis, often considered the gold standard because it compiles and re-examines raw data from multiple studies rather than simply aggregating previously reported effect sizes.&nbsp;



This approach allowed the team to analyze 256,337 individual decisions made by 11,561 participants, whose ages ranged from 18 to 88 years.&nbsp;



Participants were asked to judge whether headlines covering politics, health, and other topics were true or false. 



The researchers then connected participants’ responses to four demographic factors (age, gender, education, and political identity) and four psychological factors (analytical thinking, partisan bias, motivated reflection, and familiarity with the news).



<h2 class="wp-block-heading" id="h-common-assumptions-about-education">Common assumptions about education</h2>



Education emerged as one of the most surprising factors. Higher education is often presumed to protect against misinformation - under the assumption that college and advanced degrees teach critical thinking.



However, the meta-analysis found no significant difference in susceptibility between those with higher and lower educational attainment. 



In other words, a four-year degree or postgraduate study did not predict better performance in distinguishing real from fake headlines. This finding runs counter to the conventional wisdom that more education automatically translates into greater immunity to misinformation.



<h2 class="wp-block-heading" id="h-misconceptions-about-age-and-fake-news">Misconceptions about age and fake news</h2>



Age also challenged expectations. Previous studies often blame older adults for being more prone to sharing or believing misinformation.&nbsp;



In contrast, the new analysis showed that older adults were actually better than younger adults at discerning true headlines from false ones. They tended to label more headlines as false, indicating a greater degree of skepticism.&nbsp;



However, these findings exist alongside the well-documented observation that older adults do share more <a href="https://www.earth.com/news/digital-misinformation-rumors-spread-like-nuclear-reactions/" target="_blank" rel="noreferrer noopener">fake content</a> online - suggesting a complex interplay between careful headline scrutiny and actual sharing behavior.



<h2 class="wp-block-heading" id="h-political-identity-and-partisan-bias">Political identity and partisan bias</h2>



<a href="https://www.earth.com/news/people-trust-news-that-matches-their-political-views-even-when-its-fake/" target="_blank" rel="noreferrer noopener">Political identity</a> proved to be another influential factor. The meta-analysis confirmed that Republicans, on average, are more likely to accept news headlines as true, resulting in lower overall accuracy when distinguishing real from false stories.&nbsp;



Democrats, for their part, were more skeptical, labeling more headlines as false. Sultan and his colleagues link these findings to partisan bias, in which people are more willing to believe stories that align with their political affiliations and to reject those that conflict with them.



That said, analytical thinking - the ability to logically evaluate information and solve problems systematically - generally predicted better performance in detecting misinformation.&nbsp;



However, a twist emerged in the form of motivated reflection: individuals who scored higher in analytical thinking were actually more susceptible to partisan bias.&nbsp;



In other words, rather than using their critical skills to transcend personal beliefs, these analytical thinkers often deployed their reasoning faculties to defend their existing political identities. 



This paradox highlights the fact that reasoning can sometimes serve entrenched worldviews instead of open-minded evaluation.



<h2 class="wp-block-heading" id="h-familiarity-as-a-powerful-persuader">Familiarity as a powerful persuader</h2>



One of the strongest indicators of misinformation susceptibility turned out to be familiarity with the news. If participants recognized a headline from having seen it before, they were significantly more likely to accept it as true.&nbsp;



This result highlights the perils of repeated exposure, especially on <a href="https://www.earth.com/news/spending-less-time-on-social-media-improves-your-mental-health/" target="_blank" rel="noreferrer noopener">social media</a> platforms where the same headlines (whether accurate or false) can circulate extensively.&nbsp;



Over time, familiarity can breed acceptance, making misinformation more persuasive simply by virtue of being encountered multiple times.



The findings come at a time of growing concern over how misinformation shapes public opinion and election outcomes.&nbsp;



According to co-author Ralf Kurvers, a senior research scientist at the Max Planck Institute, the study’s relevance is heightened by the rise of right-wing populism and the dire warnings from the <a href="https://www.weforum.org/publications/global-risks-report-2024/" target="_blank" rel="noreferrer noopener">World Economic Forum’s Global Risks Report 2024</a>. This report identifies misinformation as one of the world’s greatest short-term threats.&nbsp;



Kurvers advocates for targeted media literacy efforts, particularly for younger adults, who, despite being “digital natives,” were less able to differentiate between genuine and fake news in the study.



<h2 class="wp-block-heading" id="h-addressing-the-challenges-of-misinformation">Addressing the challenges of misinformation </h2>



Moving forward, the researchers recommend that interventions account for how political bias and repeated exposure can reinforce incorrect beliefs. 



They point to the need for fostering respectful conversations across political divides and designing social media tools that reduce the repeated circulation of false content. 



As part of a broader initiative on online environments at the Max Planck Institute, the team aims to develop strategies for addressing these challenges, including methods that help people become more reflective about the information they encounter.



Ultimately, the study underscores the complexity of combating misinformation. Simply improving education levels does not appear to be a magic bullet, nor does encouraging more analytical thought if that thinking is subverted by partisan motives.&nbsp;



Instead, the research suggests that a multi-pronged approach - combining critical reflection, awareness of <a href="https://www.earth.com/news/quick-decisions-are-often-biased-and-misleading/" target="_blank" rel="noreferrer noopener">bias</a>, and caution about familiar-seeming claims - is needed to help individuals navigate the vast sea of online information.



The study is published in the <a href="https://dx.doi.org/10.1073/pnas.2409329121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Who falls for fake news? New study challenges what we thought

Who is most vulnerable to online misinformation and why? A...

2024 was an exceptionally calm year for shark bites, with only 47 unprovoked attacks recorded around the globe. This number was 22 fewer than the previous year and far below the 10-year average of 70.&nbsp;



Among the shark bites documented, only four resulted in fatalities, marking a clear decrease compared to recent years.



<h2 class="wp-block-heading" id="h-defining-unprovoked-shark-bites-nbsp">Defining unprovoked shark bites&nbsp;</h2>



The <a href="https://www.floridamuseum.ufl.edu/shark-attacks/" target="_blank" rel="noreferrer noopener">International Shark Attack File</a> (ISAF), compiled by the <a href="https://www.floridamuseum.ufl.edu/" target="_blank" rel="noreferrer noopener">Florida Museum of Natural History</a>, serves as a repository for data on what it classifies as unprovoked attacks. These are cases in which a person does not initiate contact with a <a href="https://www.earth.com/news/mediterranean-sharks-face-growing-threats-despite-conservation-efforts/%C3%B9" target="_blank" rel="noreferrer noopener">shark</a>.&nbsp;



Situations in which a person intentionally or unintentionally engages with a shark, such as releasing them from fishing gear or spearfishing, do not appear in these figures.



“We’re interested in the natural patterns of shark behavior so that we can understand why people occasionally get bitten by these animals. Any cue or attribute that modifies an animal’s natural behavior is something that, we as scientists, want to exclude,” said Gavin Naylor, director of the <a href="https://www.floridamuseum.ufl.edu/sharks/" target="_blank" rel="noreferrer noopener">Florida Program for Shark Research</a>.



<h2 class="wp-block-heading" id="h-u-s-leads-in-shark-encounters">U.S. leads in shark encounters</h2>



The United States consistently registers the highest number of <a href="https://www.earth.com/news/unprovoked-shark-attacks-and-fatalities-increased-in-2023/" target="_blank" rel="noreferrer noopener">unprovoked attacks</a>, a pattern that held last year with 28 reported incidents. 



One fatality occurred off the northwest coast of Oahu, Hawaii, caused by an unidentified shark species - the sole unprovoked death in U.S. waters.



With its extensive coastline and warm waters, Florida led the states in unprovoked bites, totaling 14. Of these, eight took place in Volusia County, commonly labeled the shark bite capital of the world.&nbsp;



Although unconfirmed, many of these incidents likely involved juvenile blacktip sharks, which breed in the waters along northeast Florida. The juvenile sharks in this habitat have yet to fully distinguish humans from fish, stingrays, or other sharks, resulting in occasional mistaken bites.



<h2 class="wp-block-heading" id="h-shark-attacks-in-the-florida-panhandle">Shark attacks in the Florida Panhandle</h2>



In June, the Florida Panhandle witnessed a cluster of shark attacks spanning a mere four miles. Three individuals were injured, including a woman at Watersound Beach who was bitten by a bull shark. Present among the bystanders were two nurses and a paramedic who helped stabilize her injuries until first responders arrived. 



In a separate incident less than two hours later, a shark bit two teenagers standing in the shallow waters off Seacrest Beach.



Bull sharks and tiger sharks frequent the northern Florida coastline but rarely enter popular swimming zones.



“You’ll see 20 to 30 of them patrolling the coast about 500 feet offshore, where they mind their own business,” Naylor said.



During the attacks, local dune lakes that usually allow <a href="https://www.earth.com/news/satellites-reveal-a-sudden-drop-in-global-freshwater-levels/" target="_blank" rel="noreferrer noopener">freshwater</a> to flow into the sea were reportedly clogged. This could have let schools of fish, which sharks typically follow, move closer to shore than normal.



<h2 class="wp-block-heading" id="h-holiday-weekend-shark-attacks-nbsp">Holiday weekend shark attacks&nbsp;</h2>



As beaches become busier with both locals and travelers, the risk of encountering sharks goes up. Over the July 4 weekend, six people were bitten by sharks in Texas and Florida. Of those, five were deemed unprovoked.



“The South Padre Island bites were significant, with several incidents on the same day in the same vicinity,” said International Shark Attack File manager Joe Miguez.



Situated near the U.S.–Mexico border, Padre Island is the world’s largest barrier island, attracting considerable tourism. In one incident, a woman was bitten on her calf while swimming in murky conditions near a sandbar, and her husband incurred minor injuries defending her.&nbsp;



Another man was bitten in the same vicinity, and a teenager received a smaller injury when a shark collided with her. Initial conjecture suggested a single shark might be to blame for these attacks, as well as those in the Florida Panhandle. However, experts see limited evidence to support that theory.



“We can’t preclude that it was the same animal, but what’s often overlooked is that the same climatic conditions that bring people into the water are the same conditions that bring sharks closer to shore,” Naylor said, implying that multiple sharks might be present under such conditions.



“This naturally increases the likelihood of human-shark encounters,” Miguez said. “In the case of the Padre Island incidents, it is much more plausible that multiple sharks were present in the area, responding to the same environmental cues.”



<h2 class="wp-block-heading" id="h-surfers-and-other-encounters">Surfers and other encounters</h2>



California experienced three unprovoked bites, including one incident involving a punctured surfboard. Surfers accounted for 33% of all attacks in 2024 on a global scale.



“People surf where there are good waves, and where there are good waves, there’s <a href="https://www.earth.com/news/water-turbidity-helps-protect-coastal-ecosystems/">turbidity</a>, and where there’s turbidity, there are often bait fish that attract sharks. The turbidity also reduces visibility in the water, making it harder for sharks to see. Some of them make mistakes,” Naylor said.



Three further bites were reported in North and South Carolina, rounding out the U.S. total.



<h2 class="wp-block-heading" id="h-international-shark-encounters">International shark encounters</h2>



Australia typically has the second-highest count of shark bites and related fatalities. Of the 13 shark species known to bite humans, all inhabit Australian waters.&nbsp;



White sharks and bull sharks remain especially common, although the white shark populations off Australia’s southwest and southeast shores have fallen from their presumed historical levels. While white and bull sharks inflict potentially severe bites, no fatalities were recorded in Australia in 2019, 2022, or 2024 from unprovoked encounters.



Ten other countries each documented one shark bite last year. In the Red Sea, off Egypt, a man lost his life while swimming outside a designated safety area.&nbsp;



Other nations registering one incident include Belize, Trinidad and Tobago, the Bahamas, the Maldives, Mozambique, French Polynesia, Thailand, and the Turks and Caicos.



An unusual case off Western Sahara represented that region’s first reported shark attack. A German tourist swimming next to a British catamaran was bitten, but it took several hours for a helicopter rescue crew to reach the remote location. She died en route after sustaining severe injuries.



In the Vaitarna River of western India, a medium-sized bull shark bit a man wading through the shallows. Bull sharks can thrive in freshwater settings and have been spotted several hundred miles inland, as pregnant females often travel upriver to avoid predators that might endanger their offspring.



<h2 class="wp-block-heading" id="h-relative-rarity-of-shark-attacks">Relative rarity of shark attacks</h2>



Even with these accounts, the odds of a shark bite remain extremely slim. The <a href="https://www.who.int/" target="_blank" rel="noreferrer noopener">World Health Organization</a> notes that drowning is the third leading cause of accidental death worldwide, while beach hazards like rip tides and strong currents pose a greater threat than sharks.



Ultimately, the 2024 data underscores a reassuring trend: fewer attacks, fewer fatalities, and enhanced insights into shark behavior to help prevent future incidents.



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Unprovoked shark attacks dropped to record low in 2024

2024 was an exceptionally calm year for shark bites, with...

Astronomers may have discovered a star hurtling through the Milky Way with a planet in tow. If confirmed, this could become the fastest-moving exoplanet system ever recorded. 



Moving at nearly twice the speed of our solar system, this phenomenon challenges our understanding of how planets remain bound to their host stars under extreme conditions.



High-speed stars are rare, and even rarer are those dragging a <a href="https://www.earth.com/news/january-2025-stargazing-a-parade-of-bright-planets/" target="_blank" rel="noreferrer noopener">planetary companion</a> along for the ride. 



The system in question is estimated to move at a staggering 1.2 million miles per hour (1.9 million kilometers per hour). This revelation raises new questions about planetary survival and migration in the cosmos.



<h2 class="wp-block-heading" id="h-high-speed-star-with-an-orbiting-planet">High-speed star with an orbiting planet </h2>



The <a href="https://www.earth.com/news/six-planet-system-hd110067-discovered-that-moves-in-perfect-mathematical-harmony/" target="_blank" rel="noreferrer noopener">planet</a> orbiting this star is believed to be a gas giant that is larger than Neptune but smaller than Jupiter. Scientists estimate that it is orbiting relatively close to its central star.



“We think this is a so-called super-Neptune world orbiting a low-mass star at a distance that would lie between the orbits of Venus and Earth if it were in our solar system,” said Sean Terry, a postdoctoral researcher at the <a href="https://umd.edu" target="_blank" rel="noreferrer noopener">University of Maryland</a>, College Park and NASA’s <a href="https://www.nasa.gov/goddard/" target="_blank" rel="noreferrer noopener">Goddard Space Flight Center</a>.



However, the star’s weak brightness places the planet well outside the habitable zone. This means it is unlikely to support life as we know it. 



Despite that, its presence could provide valuable insight into how planetary systems behave when subjected to extreme speeds. If confirmed, this would mark the first time a planet has been found orbiting a hypervelocity star.



<h2 class="wp-block-heading" id="h-detection-using-microlensing">Detection using microlensing</h2>



This extraordinary system was first detected in 2011. Scientists working on the MOA (Microlensing Observations in Astrophysics) project, a collaborative survey based in New Zealand, were searching for distant exoplanets. 



Instead, the team stumbled upon an unusual microlensing event that hinted at a pair of <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">celestial objects</a>.



Microlensing is a phenomenon where gravity bends and magnifies the light from a background star. When an object passes in front of a more distant star, its gravitational pull can act as a natural lens, briefly amplifying the star’s brightness. 



By studying these fluctuations in light, astronomers can infer the presence of unseen objects. In this case, the microlensing event suggested two objects, one significantly more massive than the other. 



<h2 class="wp-block-heading" id="h-objects-with-unknown-masses">Objects with unknown masses</h2>



The scientists calculated their relative masses, but could not determine the exact sizes of the objects without knowing their distance from Earth.



“Determining the mass ratio is easy. It’s much more difficult to calculate their actual masses," said David Bennett, a senior research scientist at NASA Goddard.



The 2011 data suggested two possibilities. Either the system consisted of a low-mass star with a Neptune-like planet in orbit around it, or it was a rogue planet accompanied by a smaller moon. Determining which scenario was correct required further investigation.



<h2 class="wp-block-heading" id="h-is-it-a-star-or-a-moon">Is it a star or a moon?</h2>



To solve this mystery, astronomers turned to data from the <a href="https://keckobservatory.org" target="_blank" rel="noreferrer noopener">Keck Observatory</a> in Hawaii and the European Space Agency’s <a href="https://www.esa.int/Science_Exploration/Space_Science/Gaia" target="_blank" rel="noreferrer noopener">Gaia satellite</a>. If the objects were a rogue planet and moon, they would be extremely difficult to detect. But if a small star were present, its light could be identified.



The search led to a promising candidate located about 24,000 light-years away. This placed it within the Milky Way’s galactic bulge, the densely packed central region of the galaxy. By comparing the star’s position in 2011 and 2021, the researchers determined it was moving at incredible speeds.



However, the team needed to confirm whether this star was indeed part of the system detected in 2011. Its measured speed already suggested it was among the fastest-moving stars known, but its full velocity remained uncertain.



“To be certain the newly identified star is part of the system that caused the 2011 signal, we’d like to look again in another year and see if it moves the right amount and in the right direction to confirm it came from the point where we detected the signal,” Bennett explained.



<h2 class="wp-block-heading" id="h-planet-star-system-may-escape-the-galaxy">Planet-star system may escape the galaxy</h2>



If this system includes a hypervelocity star, it could eventually escape the Milky Way. Its true velocity might exceed 1.3 million miles per hour (2 million kilometers per hour), which is faster than the galaxy’s escape velocity. 



If this is the case, the planet and star will drift into intergalactic space over millions of years, joining the ranks of stars that have already been lost to the void.



Scientists are eager to verify this possibility. Observations over the next few years will determine if the identified star is indeed linked to the 2011 microlensing event.



“If high-resolution observations show that the star just stays in the same position, then we can tell for sure that it is not part of the system that caused the signal. That would mean the rogue <a href="https://www.earth.com/news/nasa-finds-a-planet-k2-22b-disintegrating-at-a-speed-never-seen-before/" target="_blank" rel="noreferrer noopener">planet</a> and exomoon model is favored," said Aparna Bhattacharya, a research scientist at NASA Goddard.



<h2 class="wp-block-heading" id="h-the-role-of-future-telescopes">The role of future telescopes</h2>



Upcoming missions will help astronomers find more of these high-speed planetary systems. NASA’s Nancy Grace <a href="https://roman.gsfc.nasa.gov" target="_blank" rel="noreferrer noopener">Roman Space Telescope</a>, set to launch in the near future, will play a crucial role. 



Its advanced capabilities will allow scientists to study the galactic bulge in unprecedented detail, and help them understand how planets form around stars that are moving at extreme speeds.



“In this case we used MOA for its broad field of view and then followed up with Keck and Gaia for their sharper resolution, but thanks to Roman’s powerful view and planned survey strategy, we won’t need to rely on additional telescopes,” said Terry. “Roman will do it all.”



With technology advancing, astronomers are closer than ever to unraveling the mysteries of fast-moving stars and their planets. Whether this system turns out to be a star with a planet or a rogue planet with a moon, it will deepen our knowledge of how <a href="https://www.earth.com/news/star-behavior-can-distort-our-view-of-distant-planets/" target="_blank" rel="noreferrer noopener">celestial bodies</a> travel across the vast reaches of space.



The study is published in <a href="https://iopscience.iop.org/article/10.3847/1538-3881/ad9b0f" target="_blank" rel="noreferrer noopener">The Astronomical Journal</a>. 



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Runaway star may be dragging a planet along with it

Astronomers may have discovered a star hurtling through the Milky...

The natural world is in constant flux, but few changes have been as rapid or as far-reaching as those brought by climate change. Rising temperatures, shifting rainfall patterns, and extreme weather events are transforming ecosystems worldwide. 



Plants, unlike animals, cannot move to escape these changes. Instead, they must adapt where they stand, developing new ways to cope with heat, drought, and unpredictable seasons.



This challenge is particularly urgent for crops, which provide food for billions of people. Agricultural systems depend on <a href="https://www.earth.com/news/saving-earths-most-endangered-plants-from-extinction-proving-difficult-botanic-gardens/" target="_blank" rel="noreferrer noopener">plants</a> that can withstand extreme conditions while maintaining high yields. 



Some species, like Arabidopsis thaliana, already show remarkable adaptability, thriving in vastly different environments such as Sweden and Italy.



By understanding how plants naturally adjust to different climates, scientists can develop stronger, more resilient crops that will sustain future generations in an increasingly unpredictable world.



<h2 class="wp-block-heading" id="h-plants-and-climate-adaptation">Plants and climate adaptation</h2>



Every plant species has a unique way of responding to environmental stress. Some grow deeper roots to access water, while others alter their reproductive cycles to match changing seasons. 



These adaptations do not happen randomly; they are rooted in genetic changes that help <a href="https://www.earth.com/news/new-understanding-of-light-detection-in-plants-may-revolutionize-farming/" target="_blank" rel="noreferrer noopener">plants</a> survive in specific conditions. However, scientists are still working to uncover the exact genetic mechanisms that drive these changes.



A recent study provides new insight into this process. By combining population genetics with global climate data, researchers have identified key genetic variants that help plants adapt to different climates. 



The study focuses on Marchantia polymorpha, a liverwort that grows in diverse environments across Europe, America, and Japan.



The research was conducted by scientists from the Gregor Mendel Institute (<a href="https://www.oeaw.ac.at/gmi/" target="_blank" rel="noreferrer noopener">GMI</a>) of Molecular Plant Biology, the Umeå Plant Science Centre (<a href="https://www.upsc.se" target="_blank" rel="noreferrer noopener">UPSC</a>), and <a href="https://www.hiroshima-u.ac.jp/en" target="_blank" rel="noreferrer noopener">Hiroshima University</a>. The findings reveal important details about how plants evolve in response to climate stress.



<h2 class="wp-block-heading" id="h-plant-genes-for-climate-survival">Plant genes for climate survival</h2>



Scientists have long known that certain genetic traits provide advantages in specific environments. Plants in arid regions tend to develop water-retaining structures, while those in colder climates often produce antifreeze proteins to prevent cell damage. However, pinpointing which genetic variants control these traits remains a major challenge.



To address this, the researchers collected genetic samples from different populations of Marchantia polymorpha across Europe, America, and Japan. 



By integrating this genetic data with a worldwide climate dataset, they analyzed how each subpopulation’s genetic profile corresponded to its local climate.



“Comparing populations in Europe and Japan, we found genetic variants associated with warmer and colder summer temperatures, as well as with the amount of summer precipitation,” noted study co-author Liam Dolan. “These adaptations could be crucial for optimizing reproduction in different conditions.”



The analysis not only highlighted specific genetic changes linked to temperature and precipitation but also revealed broader patterns in how plants <a href="https://www.earth.com/news/plants-defy-climate-change-through-acclimation/" target="_blank" rel="noreferrer noopener">adjust to their surroundings</a>.



<h2 class="wp-block-heading" id="h-regional-differences-in-genetic-adaptation">Regional differences in genetic adaptation</h2>



One of the most striking findings of the study was the difference in genetic diversity among Marchantia polymorpha populations from different regions.



In Europe, populations exhibited high genetic variability among individuals but remained genetically similar across different locations. This suggests that plants in these regions have maintained a wide range of genetic tools to handle diverse <a href="https://www.earth.com/news/predicting-how-climate-change-will-alter-plant-growth-cycles/" target="_blank" rel="noreferrer noopener">environmental conditions</a>.



In contrast, Japanese populations showed a much more uniform genetic structure. Since these populations are geographically isolated, they may have evolved under more consistent environmental pressures, leading to less genetic diversity. These differences suggest that climate adaptation may shape reproductive strategies in unique ways.



Marchantia polymorpha, like many bryophytes, can reproduce both sexually and asexually. This flexibility gives it an advantage in changing environments. While sexually reproducing individuals can generate genetic diversity, asexual reproduction allows plants to rapidly colonize suitable habitats.



Understanding how these strategies vary between populations helps scientists piece together the bigger picture of plant adaptation.



<h2 class="wp-block-heading" id="h-plant-gene-database-helps-climate-research">Plant gene database helps climate research</h2>



One of the most important outcomes of the study is the creation of a population genomics database for Marchantia polymorpha.



This resource allows scientists to examine genetic variability in greater detail, providing a foundation for future research. It is the first database of its kind for this species and could serve as a model for studying other plants.



“We’re eager to expand this database with samples from around the globe, enhancing the robustness of future research,” said Dolan. "Our platform opens up exciting possibilities for addressing a wide range of biological questions related to plant growth and development.”



By incorporating more samples from different climates, researchers can refine their understanding of how genetic diversity contributes to plant survival. This information may help scientists identify genes that improve drought tolerance, disease resistance, or temperature adaptability in crops.



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



Climate change presents one of the greatest challenges to modern agriculture. Rising temperatures and unpredictable weather patterns threaten global food production, making it more important than ever to develop resilient crops. 



Studies like this one offer a glimpse into how plants naturally cope with environmental stress. By identifying the genetic factors that support adaptation, scientists can apply these insights to crop breeding programs.



Developing climate-resilient crops is not just about improving yield; it is about ensuring that food production remains stable in a changing world. Breeding programs can use the knowledge gained from this research to select for traits that enhance survival under extreme conditions. 



If certain genetic variants help Marchantia polymorpha withstand heat or drought, similar traits could be introduced into staple crops like wheat, rice, and maize.



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



This study is an important step in understanding <a href="https://www.earth.com/news/smarter-climate-models-how-plants-influence-the-water-cycle/" target="_blank" rel="noreferrer noopener">plant</a> adaptation at the genetic level, but it is only the beginning. Expanding the genetic database and conducting further research on different plant species will provide a clearer picture of how plants evolve in response to climate change.



As scientists continue to explore plant genetics, they may uncover even more ways in which plants naturally adjust to their environments. The knowledge gained from these studies could revolutionize agriculture, conservation, and climate resilience strategies.



For now, Marchantia polymorpha serves as a valuable model for studying genetic adaptation. Its ability to thrive in diverse climates offers a powerful example of nature’s capacity for change.



By decoding its genetic secrets, scientists move one step closer to ensuring a stable and sustainable future for plant life on Earth.



The study is published in the journal <a href="https://www.cell.com/current-biology/fulltext/S0960-9822(25)00008-9" target="_blank" rel="noreferrer noopener">Current Biology</a>.



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How plants adapt to survive a changing climate

The natural world is in constant flux, but few changes...

Human activity has profound consequences, including the rising concentration of heavy metals in the environment - a threat that is often overlooked. Few realize that elements like arsenic, lead, and mercury are becoming more prevalent due to human actions.



The seemingly insignificant activities of our everyday lives - like using fertilizers, mining, and even driving our vehicles - contribute to the growing problem of heavy metal pollution.



The issue is amplified by the persistence of these metals in our environment. They can bioaccumulate and cause harm even in small amounts, posing a danger to both humans and wildlife.



<h2 class="wp-block-heading" id="h-heavy-metal-pollution-in-yangshan-port">Heavy metal pollution in Yangshan Port</h2>



A recent study was focused on China's Yangshan Port. Researchers from <a href="http://zjou.admissions.cn/" target="_blank" rel="noreferrer noopener">Zhejiang Ocean University</a> looked at the concentration of seven heavy metals (arsenic, cadmium, chromium, copper, <a href="https://www.earth.com/news/151-million-americans-have-mental-health-disorders-linked-to-leaded-gasoline/" target="_blank" rel="noreferrer noopener">lead</a>, mercury, and zinc) in seawater, sediment samples, and five species of fish and crustaceans thriving on or near the seafloor.



Heavy metals were found to accumulate more in the sediment than in the water column. This, unfortunately, correlated with a higher degree of <a href="https://www.earth.com/news/microplastics-strengthen-the-toxicity-of-pollutants/" target="_blank" rel="noreferrer noopener">toxicity</a> in benthic organisms dwelling close to the seafloor, as they interact more with bottom sediments compared to fish dwelling in the upper water layers.



The situation is further complicated by differences in metabolisms and detoxification mechanisms among marine species living at varying depths.



For instance, fish living at different depths of the water column adapt to different dissolved oxygen levels, which could influence their ability to handle these heavy metals.



<h2 class="wp-block-heading" id="h-biggest-sources-of-heavy-metals">Biggest sources of heavy metals</h2>



The researchers have no doubt that human factors are the primary cause of this growing <a href="https://www.earth.com/news/heavy-metal-pollution-increases-antibiotic-resistance-in-rivers/" target="_blank" rel="noreferrer noopener">pollution</a>, especially in the port area close to the Yangtze River estuary.



"With the acceleration of urbanization and the development rapidly industry in coastal areas, heavy metals circulated continuously in the marine environment through river runoff and atmospheric deposition," wrote the study authors. 



The experts identified the biggest sources of heavy metal contamination, such as household and industrial wastewater.



"Heavy metals entering marine environment were affected by a variety of factors, including domestic sewage, garbage discharge, automobile exhaust and agricultural and fishery wastewater, fertilizer residues, metal mining and smelting, industrial wastewater, etc., as well as antifouling coatings and fuel leaks from ships."



<h2 class="wp-block-heading" id="h-health-risks-of-heavy-metals">Health risks of heavy metals </h2>



"Excessive heavy metal contamination not only impacted the marine environment negatively, but also presented a threat to marine organisms and human health," said the researchers.



They noted that arsenic and <a href="https://www.earth.com/news/mercury-pollution-is-making-its-way-to-the-deepest-parts-of-the-ocean/" target="_blank" rel="noreferrer noopener">mercury</a> pose the greatest threat to the area's marine environment, with arsenic being the highest risk to human health through trace metal poisoning. 



The repercussions could be severe, affecting various body systems and increasing the risk of cancer. The threat is even greater for children due to their developing metabolism, immune systems, and rapid cell growth.



<h2 class="wp-block-heading" id="h-wake-up-call-for-communities">Wake-up call for communities </h2>



Due to the bioaccumulation of heavy metal toxicity in marine organisms, this silent menace moves quietly up the food chain. To limit exposure, the local population may need to reduce their seafood consumption.



The study highlights the increasing need to understand heavy metal toxicity in oceans, its impact on marine ecosystems, and its effects on human health.



The research serves as a wake-up call to communities and policymakers around the world to enforce protective measures to reduce the risks associated with heavy metal pollution.



<h2 class="wp-block-heading" id="h-addressing-toxic-metal-contamination">Addressing toxic metal contamination</h2>



With Yangshan and other ports in different parts of the world undergoing expansion projects, the need to address the issue grows even more urgent.



Regulatory bodies must implement stricter monitoring of industrial discharges, agricultural runoff, and shipping activities to limit the influx of toxic metals into the ocean. 



Additionally, sustainable fishing practices and improved wastewater treatment technologies can help mitigate the long-term effects of contamination.



Public awareness also plays a crucial role. Educating local communities about the risks of heavy metal exposure through seafood consumption can encourage safer dietary choices.



Consumers, policymakers, and industries must collaborate to develop sustainable solutions that protect marine ecosystems while ensuring the safety of global seafood supplies.



The full study was published in the journal <a href="https://www.frontiersin.org/journals/marine-science/articles/10.3389/fmars.2024.1512115/full" target="_blank" rel="noreferrer noopener">Frontiers in Marine Science</a>.



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Heavy metal pollution threatens marine life and human health

Human activity has profound consequences, including the rising concentration of...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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

Detecting mercury contamination with the tap of a finger

[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

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



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



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



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



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



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



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



Video Credit: Amanda Nguyen/University of Illinois



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



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

Designing crops that can beat the heat

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