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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA/ESA Hubble Space Telescope



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Cat's Eye Nebula in the constellation Draco

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

Today's Image of the Day from NASA Earth Observatory features Klinaklini Glacier, located in the Coast Mountains of British Columbia, Canada.



Klinaklini Glacier is notable for its size and the role it plays in the regional environment. It is part of a larger system of glaciers and ice fields in the area, which are critical for their contribution to <a href="https://www.earth.com/news/satellites-reveal-a-sudden-drop-in-global-freshwater-levels/" target="_blank" rel="noreferrer noopener">freshwater</a> resources and their influence on local climate conditions.



<h2 class="wp-block-heading" id="h-klinaklini-glacier-and-climate-change">Klinaklini Glacier and climate change</h2>



Klinaklini is particularly interesting due to its dynamics and response to climate change. Like many <a href="https://www.earth.com/news/melting-glaciers-pose-great-threat-to-biodiversity-in-mountain-ranges/" target="_blank" rel="noreferrer noopener">glaciers</a> around the world, it is being closely monitored for changes in its size, flow, and overall health. 



Glaciers in the Coast Mountains, including Klinaklini, have been studied for their response to global warming, with many showing signs of retreat and reduced ice mass.



"Decades of satellite images of western Canada make it clear that the region’s glaciers are shrinking and that the rate of ice loss is accelerating," said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"In 1984, there were 14,329 glaciers in British Columbia and Alberta that were large enough to detect with sensors on the Landsat 5 satellite."



"By 2020, nearly 8 percent of them - 1,141 glaciers - had shrunk so much that newer Landsat sensors could no longer distinguish them, according to research conducted by University of Northern British Columbia glaciologists Alexandre Bevington and Brian Menounos."



<h2 class="wp-block-heading" id="h-ecological-role-of-the-klinaklini-glacier">Ecological role of the Klinaklini Glacier </h2>



Klinaklini Glacier also plays a crucial role in the local ecosystem. It feeds into the Klinaklini River, which is an important waterway for the region. 



The river supports a variety of wildlife, including salmon populations that are vital both ecologically and economically for local communities.



Studies conducted on and around the Klinaklini Glacier contribute to the understanding of glaciology, <a href="https://www.earth.com/news/alpine-glaciers-will-lose-half-of-their-volume-by-2050/" target="_blank" rel="noreferrer noopener">climate change</a>, and hydrology. 



This research is essential for predicting future changes in the glacier and for understanding the broader impacts of climate change on glacial systems globally.



<h2 class="wp-block-heading" id="h-coast-mountains-of-british-columbia">Coast Mountains of British Columbia </h2>



The Coast Mountains of British Columbia are a striking and expansive mountain range forming part of the Pacific Coast Ranges in western North America. 



Stretching approximately 1,600 kilometers from the Fraser River near Vancouver in the south to the Yukon Territory in the north, the range is known for its rugged beauty and significant ecological and cultural importance.



<h3 class="wp-block-heading" id="h-geography-of-the-mountains">Geography of the mountains</h3>



Geographically, the Coast Mountains are flanked by the Pacific Ocean to the west and the Interior Plateau to the east. 



They are divided into three main sections: the Pacific Ranges in the south, the Kitimat Ranges in the central region, and the Boundary Ranges in the north, which extend into Alaska and Yukon. 



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



The range's dramatic landscapes include steep peaks, fjords, and valleys carved by ancient <a href="https://www.earth.com/news/melting-glaciers-release-vast-quantities-of-unknown-microbes/" target="_blank" rel="noreferrer noopener">glaciers</a>, showcasing the lasting influence of glaciation on the region.



Geologically, the Coast Mountains are part of the Pacific Ring of Fire, formed by volcanic and tectonic activity. 



Their granitic composition is a result of millions of years of geological processes. Mount Waddington, the highest peak in the range at 4,019 meters, stands as a formidable landmark in the Pacific Ranges.



<h3 class="wp-block-heading" id="h-climate-and-wildlife">Climate and wildlife</h3>



The climate of the Coast Mountains varies significantly depending on location. The western slopes are characterized by a temperate rainforest climate, with high levels of precipitation brought by moist Pacific air. 



In contrast, the eastern slopes are drier, with semi-arid conditions in some areas. This climatic diversity supports a wide range of ecosystems, from lush coastal rainforests to alpine tundra. 



The region is home to diverse <a href="https://www.earth.com/news/outdoor-recreation-noise-triggers-fear-response-in-wildlife/" target="_blank" rel="noreferrer noopener">wildlife</a>, including black bears, grizzly bears, mountain goats, and numerous bird species.



<h3 class="wp-block-heading" id="h-recreation-and-culture">Recreation and culture</h3>



The Coast Mountains are a popular destination for recreation and tourism. Activities such as hiking, skiing, snowboarding, and mountaineering draw visitors from around the world - particularly to destinations like Whistler, a renowned resort town in the Pacific Ranges. 



The fjords and valleys of the range provide opportunities for kayaking, fishing, and scenic exploration.



Indigenous peoples, including the Tlingit, Tsimshian, Haida, and Squamish, have lived in and around the Coast Mountains for millennia. 



These groups maintain a deep connection to the land, reflected in their stories, traditions, and art. The mountains are not only a physical presence but also a vital cultural and spiritual landscape.



Image Credit: NASA Earth Observatory&nbsp;



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Klinaklini Glacier in the Coast Mountains of British Columbia

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

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 NASA Earth Observatory features South Korea, where a November storm set a new record for daily snowfall in Seoul.



“Wintry weather arrived in full force in South Korea. In the last week of November 2024, a storm brought record-breaking accumulations of snow to Seoul. The heavy snow disrupted travel and damaged structures in the nation’s capital and surrounding areas,” said <a href="https://earthobservatory.nasa.gov/images/153649/heavy-snows-in-korea" target="_blank" rel="noreferrer noopener">NASA</a>.



“On the morning of November 27, residents of Seoul awoke to 16.5 centimeters (6.5 inches) of new snow. That amount already surpassed the previous daily snowfall record for Seoul in November since records began in 1907, according to news reports.”



<h2 class="wp-block-heading" id="h-snowfall-across-the-korean-peninsula-nbsp">Snowfall across the Korean Peninsula&nbsp;</h2>



Yet, as NASA noted, the <a href="https://www.earth.com/news/secrets-of-snow-complexity-can-improve-winter-safety/">snow</a> kept flying. By the morning of November 28, Seoul had accumulated a total of 11.3 inches. About 22 miles to the south, the city of Suwon received 17 inches of snow.&nbsp;



“When clouds cleared the following day, the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite captured this image, revealing a broad coating of white across the Korean Peninsula,” said NASA.



<h2 class="wp-block-heading" id="h-rare-snowfall-event-in-south-korea-nbsp">Rare snowfall event in South Korea&nbsp;</h2>



Meteorologists attributed this rare event to a sharp contrast between cold northern air and the warmer surface of the Yellow Sea.



Officials said that the temperature difference between the air and the <a href="https://www.earth.com/news/pacific-ocean-temperatures-highest-in-650-years-greatly-harming-coral-reefs/" target="_blank" rel="noreferrer noopener">sea surface</a> was more profound than normal due to unusual warmth in recent weeks, which likely contributed to the storm’s intensity.



<h2 class="wp-block-heading" id="h-impacts-of-the-snowfall">Impacts of the snowfall</h2>



“Those who braved the weather around Seoul witnessed landmarks transformed into a winter wonderland. However, the storm grounded hundreds of flights across the country, kept dozens of ferries in port, and snarled traffic,” said NASA.&nbsp;



“The weight of the snow also toppled trees and damaged greenhouses and other agricultural facilities in areas surrounding Seoul, according to reports.”



<h2 class="wp-block-heading" id="h-snowfall-in-seoul-south-korea-nbsp">Snowfall in Seoul, South Korea&nbsp;</h2>



Snowfall is not unusual in Seoul, but its frequency and accumulation levels are typically moderate. 



Seoul has a temperate climate with cold, dry winters, and snow is a normal part of the season from December to February. However, heavy snowfall is rare, with most snowfalls being light to moderate.&nbsp;



The city averages about 25-30 days of snow per year, with a total accumulation that is far less than what is seen in colder regions of the world.



<h2 class="wp-block-heading" id="h-climate-change-and-snowfall-patterns-nbsp">Climate change and snowfall patterns&nbsp;</h2>



<a href="https://www.earth.com/news/ski-resorts-face-snow-scarcity-due-to-climate-change/" target="_blank" rel="noreferrer noopener">Climate change</a> is altering snowfall patterns globally, with variations in both frequency and intensity - depending on the region. 



Warmer average temperatures are shifting precipitation from snow to rain in many areas, particularly in low-lying regions and mid-latitudes. This trend reduces the duration and extent of <a href="https://www.earth.com/news/snow-cover-has-decreased-in-recent-decades/" target="_blank" rel="noreferrer noopener">snow cover</a>, especially at lower elevations. 



However, paradoxically, some regions experience heavier snowstorms due to increased atmospheric moisture. Warmer air can hold more water vapor, leading to intense snowfall under the right conditions.



<h3 class="wp-block-heading" id="h-complex-climate-impacts">Complex climate impacts</h3>



In high-altitude and polar regions, the impact is more complex. Some areas, like the Himalayas and the Arctic, see diminished snowfall because of warmer conditions and melting ice.&nbsp;



Conversely, parts of the Arctic and Antarctica may experience <a href="https://www.earth.com/news/sea-ice-loss-increases-snowfall-over-west-antarctica/" target="_blank" rel="noreferrer noopener">increased snowfall</a> due to changes in wind patterns and enhanced evaporation over open waters caused by sea ice loss. 



For example, in recent years, storms fueled by unusual temperature differentials have resulted in historic snowfalls in some areas, like the U.S. Northeast and parts of East Asia, as warmer oceans supply more moisture to cold air masses.



<h3 class="wp-block-heading" id="h-shifts-in-the-seasons">Shifts in the seasons</h3>



Seasonal timing is also shifting, with snowfalls occurring later in fall and ending earlier in spring. 



These changes disrupt ecosystems that rely on consistent snowpacks, affect water resources dependent on snowmelt, and complicate winter activities such as agriculture and tourism.



Overall, the effects of climate change on snowfall are not uniform but are instead influenced by local geography, altitude, and changing weather systems.&nbsp;



As global temperatures continue to rise, these shifts are expected to intensify, requiring adaptation in water management, infrastructure, and disaster preparedness.



Image Credit: NASA Earth Observatory&nbsp;



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Winter storm set a new snowfall record in Seoul, South Korea

Today's Image of the Day from the European Space Agency features NGC 1333, a reflection nebula located in the Perseus molecular cloud about 960 light-years away from Earth. The photo is a mosaic of images captured by the James Webb Space Telescope.



<h2 class="wp-block-heading" id="h-the-power-of-webb-nbsp-nbsp">The power of Webb&nbsp;&nbsp;</h2>



“Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. Some of the faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



The same cluster was featured as the 33rd anniversary image of the Hubble Space Telescope in April 2023.&nbsp;



According to ESA, Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. 



"Observing with larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects."



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc1333">Webb’s view of NGC1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC1333 cloud.&nbsp;



“Across the image we see large patches of orange, which represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation."



The disks of gas and dust that surround the <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">stars</a> in this image may eventually produce planetary systems.&nbsp;



<h2 class="wp-block-heading" id="h-formation-of-the-sun">Formation of the Sun</h2>



“Similar to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster, which was perhaps even more massive than NGC 1333,” explained ESA.



Over time, the stars in the Sun's birth cluster would have drifted apart due to gravitational interactions and the dispersion of gas in the region.



Astronomers have been studying certain clues, such as isotopic signatures in meteorites, that hint the Sun may have formed near massive stars. These stars likely produced supernovae, which could have influenced the early <a href="https://www.earth.com/news/mysterious-objects-spotted-in-the-outer-solar-system-beyond-pluto/" target="_blank" rel="noreferrer noopener">solar system</a> by injecting heavy elements like iron-60.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1333">Star formation in NGC 1333</h2>



NGC 1333 is a vibrant example of a stellar nursery, where active <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 ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



Within NGC 1333, astronomers have observed a high level of turbulence, which makes the region dynamic and complex. 



These disturbances are caused by the outflows of young stars as they eject material into their surroundings, creating shock waves and influencing further star formation.&nbsp;



These outflows are often seen as jets, which are visible in multiple wavelengths of light, especially infrared, as the surrounding dust absorbs visible light.



<h2 class="wp-block-heading" id="h-significance-of-ngc-1333">Significance of NGC 1333</h2>



NGC 1333 is also an area of interest for studying the early stages of star and <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planet formation</a>, as many of the stars within the cluster are in their infancy, still in the process of gathering material and developing protoplanetary disks.&nbsp;



In images, NGC 1333 is marked by bright patches of blue and red, representing reflection <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebulae</a> and the ionized gas created by energetic young stars.&nbsp;



<h2 class="wp-block-heading" id="h-the-perseus-molecular-cloud-nbsp">The Perseus molecular cloud&nbsp;</h2>



The Perseus molecular cloud is a vast region of cold gas and dust located about 600 light-years away from Earth in the constellation <a href="https://www.earth.com/news/1500-billion-orphan-stars-discovered-in-the-perseus-galaxy-cluster/" target="_blank" rel="noreferrer noopener">Perseus</a>.&nbsp;



It is one of the most studied star-forming regions in our galaxy due to its relative proximity and the diversity of its young stellar objects. This cloud spans several hundred light-years and contains dense pockets of gas where new stars are actively forming.&nbsp;



These areas are often enshrouded in thick dust, which obscures them in visible light but allows astronomers to study them using infrared and radio wavelengths.



The Perseus molecular cloud is particularly interesting because of the chemistry taking place within it, including the formation of complex organic molecules that could be precursors to life.&nbsp;



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



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Stellar nursery shines in the Perseus cloud

The combined effects of sea level rise, permafrost thaw subsidence, and coastal retreat threaten to reshape Arctic coastal regions on an unprecedented scale, surpassing the impact of any single climate hazard.&nbsp;



According to scientists, this compounding set of factors will lead to drastic land loss, posing significant challenges for Arctic communities.



<h2 class="wp-block-heading" id="h-overlapping-hazards-magnify-coastal-retreat-nbsp">Overlapping hazards magnify coastal retreat&nbsp;</h2>



While decades of research have documented the growing threat of <a href="https://www.earth.com/news/fighting-coastal-erosion-electricity-turns-sand-into-a-sea-wall/" target="_blank" rel="noreferrer noopener">coastal erosion</a> in the Arctic, the additional roles of sea level rise and permafrost thaw subsidence have been less explored.&nbsp;



This gap in understanding has limited the ability to evaluate the full extent of these combined processes and their impacts on Arctic landscapes.



A new study by researchers from the <a href="https://www.whoi.edu/who-we-are/" target="_blank" rel="noreferrer noopener">Woods Hole Oceanographic Institution</a> (WHOI) and other institutions, focuses on the Alaska Arctic Coastal Plain (ACP). Spanning more than 60,000 square kilometers, this low-lying, ice-rich region experiences some of the Arctic’s most extreme rates of erosion and <a href="https://www.earth.com/news/sea-level-warnings-what-coastal-cities-must-prepare-for/" target="_blank" rel="noreferrer noopener">sea-level rise</a>.



“Our findings highlight the risks that compounding climate hazards pose to coastal communities and underscore the need for adaptive planning for Arctic communities within zones of 21st-century land loss,” the experts wrote.



<h2 class="wp-block-heading" id="h-a-stark-forecast-for-arctic-shorelines">A stark forecast for Arctic shorelines</h2>



The study presents a stark forecast for the North Slope shoreline, predicting a dramatic inland retreat by 2100 due to the interplay of these three hazards.



“Compound <a href="https://www.earth.com/news/arctic-warming-permafrost-melt-devastating-role-accelerating-global-climate-change/" target="_blank" rel="noreferrer noopener">climate</a> impacts accelerate coastal change,” said lead author Roger Creel, a postdoctoral scholar in WHOI’s Department of Physical Oceanography. “There is this nonlinear acceleration in coastal impacts that we should be expecting will happen in places like Northern Alaska.”



The shoreline is expected to retreat farther inland than it has been in over 100,000 years, during the last interglacial period.&nbsp;



“By 2100, the combined effects of coastal erosion, sea level rise, and permafrost thaw subsidence will likely push the North Slope shoreline inland to a location it hasn't reached since the last interglacial period over 100,000 years ago,” explained co-author Benjamin Jones of the <a href="https://www.uaf.edu/uaf/" target="_blank" rel="noreferrer noopener">University of Alaska Fairbanks</a>.



<h2 class="wp-block-heading" id="h-projections-of-coastal-retreat-nbsp">Projections of coastal retreat&nbsp;</h2>



The researchers utilized advanced tools to assess future land loss, including 5-meter topography, satellite-derived lake depth measurements, and empirical data on permafrost thaw subsidence.&nbsp;



The team incorporated these with projections of coastal erosion and sea level rise under medium- and high-emission scenarios from the <a href="https://www.ipcc.ch/assessment-report/ar6/" target="_blank" rel="noreferrer noopener">IPCC’s 6th Assessment Report</a>.



“This research highlights the value of working across disciplinary boundaries for more robust projections of coastal Arctic evolution in the coming century,” said co-author Julia Guimond, an assistant scientist at WHOI.&nbsp;



“Our work shows that by 2100, total land loss will exceed erosional losses by up to eight times. Here we focus on processes affecting Alaska's Arctic Coastal Plain, but a key takeaway is the compounding effects of multiple hazards and that applies to coastal resilience planning across the globe.”



<h2 class="wp-block-heading" id="h-permafrost-thaw-a-hidden-dominator">Permafrost thaw: A hidden dominator</h2>



The study emphasizes that <a href="https://www.earth.com/news/rapid-permafrost-thaw-in-alaska-threatens-global-climate-balance/" target="_blank" rel="noreferrer noopener">permafrost thaw</a> subsidence will be the dominant factor driving land loss, surpassing even sea level rise and coastal erosion in its long-term impacts.



“Along ice-rich permafrost coastlines, the land surface is falling faster than the sea levels are rising,” noted co-author Pier Paul Overduin from the <a href="https://www.awi.de/en/" target="_blank" rel="noreferrer noopener">Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research</a>.&nbsp;



“Over the coming decades, permafrost thaw subsidence will move the coastline farther inland than coastal erosion or sea level rise alone will move it, and this subsidence will dominate Arctic coastal change over the long term.”



Creel highlighted the need for greater awareness among decision-making agencies, such as the <a href="https://www.usace.army.mil/" target="_blank" rel="noreferrer noopener">U.S. Army Corps of Engineers</a> and <a href="https://www.fema.gov/" target="_blank" rel="noreferrer noopener">FEMA</a>, to allocate resources more effectively.&nbsp;



“These sorts of bodies with a lot of resources may have not been paying enough attention to permafrost thaw subsidence as an agent of coastal change. This study is a wake-up call to expand the conversation.”



<h2 class="wp-block-heading" id="h-communities-on-the-frontline-of-change">Communities on the frontline of change</h2>



An Arctic coastline shaped by inundation will create unprecedented challenges for the communities that call this region home. These include the loss of infrastructure, hunting grounds, subsistence routes, and cultural heritage sites.



“Future research on Arctic shoreline evolution should be motivated by the needs of these communities, who will need support to respond to the paradigm shift in 21st-century Arctic coastal change that we project here,” the authors concluded.



The study is published in <a href="http://dx.doi.org/10.1073/pnas.2409411121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



Image Credit: Photo by: Benjamin M. Jones, Institute of Northern Engineering, University of Alaska Fairbanks



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Accelerating coastal retreat in Alaska: The triple threat

The combined effects of sea level rise, permafrost thaw subsidence,...

In the pursuit of innovation, a group of scientists has achieved something remarkable: they've found a way to create "real" diamonds at normal room temperature and pressure.



This breakthrough not only eliminates the need for a starter gem but also drastically simplifies the process of producing lab-grown diamonds, making it more efficient and potentially more accessible. 



By challenging conventional methods, this discovery paves the way for a new era in diamond synthesis.



<h2 class="wp-block-heading" id="h-how-nature-makes-diamonds">How nature makes diamonds</h2>



Most diamonds start their journey about 90 to 150 miles beneath the surface, in a part of the <a href="https://www.earth.com/news/record-breaking-hole-drilled-into-earths-mantle-scientific-goldmine-magma-life/" target="_blank" rel="noreferrer noopener">Earth's mantle</a> where temperatures soar to around 2,000 degrees Fahrenheit, and pressures are mind-bogglingly high. 



Under these extreme conditions, <a href="https://www.earth.com/news/graphite-in-2-5-billion-year-old-ruby-linked-to-early-life/" target="_blank" rel="noreferrer noopener">carbon atoms</a> bond together in a unique crystal structure, creating the hard, shiny gems we know and love.



But getting those diamonds to the surface is another story. Volcanic eruptions, millions of years ago, brought diamonds closer to the Earth’s crust in <a href="https://www.earth.com/news/diamond-fountain-eruption-from-volcanoes-when-earth-continents-shift/" target="_blank" rel="noreferrer noopener">rocks called kimberlite</a> or lamproite. 



These eruptions were like express elevators, moving the diamonds upward quickly enough to keep them intact under lower-pressure conditions. 



Today, miners find these ancient gems in volcanic pipes or riverbeds where erosion has carried them. 



<h2 class="wp-block-heading" id="h-mimicking-extreme-conditions-in-the-lab">Mimicking extreme conditions in the lab</h2>



To mimic these natural conditions in the lab, scientists have been using a method called high-pressure, high-temperature (HPHT) growth. 



With this method, they have been simulating the same extreme conditions in order to coerce dissolved carbon, in liquid metals like iron, to convert into diamond around a starter <a href="https://www.earth.com/news/worlds-second-largest-diamond-found-in-botswana/" target="_blank" rel="noreferrer noopener">gem</a>.



<h2 class="wp-block-heading" id="h-challenges-of-growing-diamonds">Challenges of growing diamonds</h2>



This approach has its limitations. Incredible pressure and heat aren't easy to achieve or maintain in a lab setting. And, the size of the lab-made gems leaves a bit to be desired.



The largest ones only reach about the size of a blueberry, and the process is time-consuming.



Alternative methods, such as chemical vapor deposition, attempt to eliminate some of HPHT's limitations, such as the need for high pressures, but the requirement for a starter diamond remains.



The new technique, developed by a team led by Rodney Ruoff, a physical chemist at the <a href="https://www.ibs.re.kr/eng.do" target="_blank" rel="noreferrer noopener">Institute for Basic Science</a> in South Korea, eliminates some of the disadvantages of the above-mentioned synthesis processes. 



According to Ruoff, he has been pondering new ways to grow diamonds for over a decade now, challenging conventional thinking.



<h2 class="wp-block-heading" id="h-secret-to-growing-diamonds">Secret to growing diamonds</h2>



The team's method began with electrically heated gallium with a little bit of silicon in a graphite crucible. 



While gallium may sound exotic, it was actually chosen based on a previous unrelated study that identified its ability to catalyze the formation of <a href="https://www.earth.com/news/graphene-new-wonder-material-earth-technology-found-moon-soil/" target="_blank" rel="noreferrer noopener">graphene</a>, a carbon cousin to diamond.



The team also invented a special chamber containing a 2.4-gallon crucible where the gallium-silicon mix awaited. 



This crucible chamber, designed to be at sea-level atmospheric pressure, was ready to experiment in just 15 minutes. It allowed the experimental gas mixtures to be changed rapidly and easily to determine the optimal blend.



After numerous trials, the scientists found that an optimal mixture of gallium-nickel-iron, with a smattering of silicon, catalyzed the <a href="https://www.earth.com/news/diamonds-can-be-grown-in-a-lab-in-less-than-3-hours/" target="_blank" rel="noreferrer noopener">growth</a> of diamonds most efficiently.



Even more impressive was that diamonds appeared at the base of the crucible within 15 minutes, and a more complete diamond film formed within two and a half hours.



<h2 class="wp-block-heading" id="h-mystery-of-diamond-formation">Mystery of diamond formation</h2>



The actual mechanism that leads to diamond formation deep within the Earth isn't yet completely understood.



However, the researchers believe that a decrease in temperature helps drive the carbon from the methane towards the center of the crucible, where it coalesces into a diamond.



The process seems reliant on silicon. Without it, no diamonds could be formed, indicating the crucial role it plays as a seed for the carbon to crystallize around.



<h2 class="wp-block-heading" id="h-limitations-of-the-new-technique">Limitations of the new technique</h2>



Despite these thrilling advancements, the new technique isn't without its own limitations. 



The diamonds produced using this method are minuscule, hundreds of thousands of times smaller than those grown with the HPHT method. Hence, these diamonds are far too small for <a href="https://www.earth.com/news/revolutionary-process-turns-carbon-emissions-into-diamonds/" target="_blank" rel="noreferrer noopener">jewelry</a> applications.



However, their use in technological applications, such as drilling or polishing, is a possibility. Due to the low pressure involved in the new method, it might be feasible to significantly scale up diamond synthesis.



"In about a year or two, the world might have a clearer picture of things like possible commercial impact," Rodney Ruoff predicts optimistically. 



This breakthrough is a remarkable reflection of the unceasing quest for innovation that pushes the boundaries, and redefines the possible.



The intriguing discovery may even hint at an exciting new chapter in the evolving story of synthetic gems, one that could reshape their production and applications. Only time will tell how far this innovation will take us.



The full study was published in the journal <a href="https://www.nature.com/articles/s41586-024-07339-7" target="_blank" rel="noreferrer noopener">Nature</a>.



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Real diamonds can now be created from scratch in the lab in just 15 minutes

In the pursuit of innovation, a group of scientists has...

At first glance, hummingbird bills look like straws -- long and thin, perfect for sipping nectar. But a new study reveals that this comparison is far from accurate. 



These tiny birds have evolved intricate adaptations for drinking nectar, turning their bills into incredibly sophisticated tools.



In a recent study, a team led by Alejandro Rico-Guevara from the University of Washington discovered that hummingbird bills do much more than we thought. 



The bills aren't passive tools; they actively and flexibly engage with the bird's tongue to help it drink nectar with lightning speed.



The team showed that, contrary to what you might expect, a hummingbird’s bill works in concert with its tongue, opening and closing in various sections while drinking. 



This rapid coordination allows the bird to extract nectar quickly, helping it conserve energy while hovering mid-air.



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



These little birds, found mostly in the Americas, are famous for their incredible ability to hover in place, thanks to their unique wing structure. 



Their wings beat at mind-blowing speeds -- up to 80 beats per second in some species -- which creates the signature humming sound that gives them their name. 



They also <a href="https://www.earth.com/news/how-hummingbirds-deal-with-their-need-for-flight-speed/" target="_blank" rel="noreferrer noopener">have extraordinary agility</a>, flying not just forward but backward, sideways, and even upside down. What really sets hummingbirds apart is their insanely high metabolism. 



To fuel their constant movement, they feed on nectar from flowers, using their long, specialized beaks and tongues to reach deep into blooms. They also eat insects and spiders for protein, keeping their diet balanced. 



Hummingbirds are small -- some, like the bee hummingbird, are just 2 inches long -- but they pack a visual punch. 



Their iridescent feathers shimmer in the sunlight, changing colors depending on the angle, making them one of nature’s most <a href="https://www.earth.com/news/giants-hummingbirds-are-not-just-one-two-species/" target="_blank" rel="noreferrer noopener">eye-catching creatures</a>. 



Plus, their energy and tenacity are unmatched, with some species migrating thousands of miles to escape the cold.



<h2 class="wp-block-heading" id="h-complexities-of-drinking-nectar">Complexities of drinking nectar</h2>



“Most <a href="https://www.earth.com/news/hummingbirds-have-an-amazing-sense-of-touch-for-precise-navigation/" target="_blank" rel="noreferrer noopener">hummingbirds</a> drink while they’re hovering mid-flight,” said Rico-Guevara, who is also curator of ornithology at the UW’s&nbsp;<a href="https://www.burkemuseum.org/" target="_blank" rel="noreferrer noopener">Burke Museum of Natural History and Culture</a>. 



“Energetically, that is very expensive. Flying straight at commuting speeds uses up less energy than hovering to drink. So, hummingbirds are trying to minimize energy and drink as fast as they can -- all from these hard-to-reach spaces -- which requires special adaptations for speed and efficiency.”



Until now, scientists knew that hummingbirds use their long, intricate tongues to gather nectar. But how their bills contributed to this task remained a mystery. 



<h2 class="wp-block-heading" id="h-essential-role-of-hummingbird-bill">Essential role of hummingbird bill</h2>



By filming hummingbirds in slow motion at field sites across Colombia, Ecuador, and the U.S., the researchers discovered the bill plays an essential role:



<ul class="wp-block-list">
<li>The hummingbird opens just the tip of its bill to extend its tongue. </li>



<li>After the tongue gathers nectar, the bill tip closes. </li>



<li>To draw the nectar further, the midsection of the bill stays closed while the base opens slightly. </li>



<li>The tip opens again for the next round, repeating 10-15 times each second. </li>
</ul>



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Hummingbirds have highly specialized tongues -- some even resembling intricate origami -- to gather nectar. But this study highlights the often-overlooked importance of the bill.



Though it looks rigid, the bill is surprisingly flexible and essential for efficient nectar drinking.



<h2 class="wp-block-heading" id="h-unique-fluid-collection-of-hummingbird-bills">Unique fluid collection of hummingbird bills</h2>



The <a href="https://www.washington.edu" target="_blank" rel="noreferrer noopener">University of Washington</a> research also uncovered something unique about hummingbird feeding techniques. 



"We already knew that hummingbird bills have some flexibility, for example bending their lower bill while catching insects. But now we know that the bill plays this very active and essential role in drawing up nectar that the tongue collects," Rico-Guevara explained.



Most animals use just one method to collect fluids. Dogs and cats, for instance, lap water using what’s known as Couette flow, while mosquitoes use a suction-based system called Poiseuille flow.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/12/hummingbird-beak_feeder_Chalybura-buffonii_credit-Kristiina-Hurme_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/12/hummingbird-beak_feeder_Chalybura-buffonii_credit-Kristiina-Hurme_1s.webp" alt="Image showing a white-vented plumeleteer (Chalybura buffonii) drinking from a feeder at the Colibrí Gorriazul Research Center in Colombia. Credit: Kristiina Hurme" class="wp-image-1952645"/></a><figcaption class="wp-element-caption">Image showing a white-vented plumeleteer (Chalybura buffonii) drinking from a feeder at the Colibrí Gorriazul Research Center in Colombia. Credit: Kristiina Hurme</figcaption></figure>



Hummingbirds, however, use both approaches. Their bills and tongues work together, first lapping the nectar and then drawing it up through suction. 



This dual method makes hummingbirds truly unique among nectar feeders.



"It makes sense that they would have to use both, given the pressure to reach the nectar deep within the flower and to feed quickly and efficiently," said Rico-Guevara.



<h2 class="wp-block-heading" id="h-evolution-and-future-questions">Evolution and future questions</h2>



The evolution of <a href="https://www.earth.com/news/national-butterfly-and-hummingbird-day-celebrating-the-beauty-of-life/" target="_blank" rel="noreferrer noopener">hummingbird</a> bills is a fascinating example of adaptation. As flowers have evolved different shapes and sizes, hummingbird bills have also adapted, becoming perfectly suited for reaching deep into blossoms.



But with every answer, new questions arise. What muscles control these intricate movements? How does catching insects impact bill flexibility? There’s still much to learn about these tiny avian marvels.



The co-authors of the study include researchers from universities across the U.S. and the U.K., highlighting the international effort to understand these tiny <a href="https://www.earth.com/news/bird-extinctions-shatter-the-harmonious-balance-of-nature/" target="_blank" rel="noreferrer noopener">birds</a>.



In conclusion, hummingbirds, with their delicate beauty and incredible speed, are more than just nectar sippers. 



Their bills, far from being mere straws, are the result of millions of years of evolution, fine-tuned to help these birds survive in a competitive environment.



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The study "Upper bill bending as an adaptation for nectar feeding in hummingbirds" is published in the <a href="https://royalsocietypublishing.org/doi/10.1098/rsif.2024.0286" target="_blank" rel="noreferrer noopener">Journal of the Royal Society Interface</a>.



Video Credit: Alejandro Rico-Guevara



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Hummingbird bills are an evolutionary wonder

At first glance, hummingbird bills look like straws -- long...

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Today&#8217;s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Perth, the capital city of Western Australia. The metropolitan area of Perth is a 125-kilometer region along the coast that stretches from Two Rocks in the north to Singleton in the south.



Prior to European colonization, the area was inhabited by the Whadjuk Noongar people for over 40,000 years. At that time, Perth was called Boorloo by the Aboriginals. The official estimation of the Greater Perth population as of June 2017 is 2,050,138 people. 



West Perth is an inner suburb of the city. Formerly an exclusive suburb for wealthy merchants and politicians, it is now part of the inner mixed zone, and has predominantly office blocks which displaced residential buildings.



Perth is one of the most isolated cities in the world. Brisbane, the nearest city, is about 2,000 kilometers away. It is also the world&#8217;s sunniest capital city &#8211; with almost 8 hours of sunshine a day. 



Video 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

The city of Perth in Western Australia