Today's Image of the Day from the European Space Agency features the Cat's Paw Nebula - a massive, active star-forming region in the constellation Scorpius. Also known as NGC 6334, the nebula is located about 4,000 light-years away from Earth.



The nebula’s name comes from its appearance. When viewed in visible or infrared light, it resembles a cat’s paw with bright lobes that look like giant toe beans.



“To celebrate the NASA/ESA/CSA James Webb Space Telescope’s third year of highly productive science, astronomers used the telescope to scratch beyond the surface of the Cat’s Paw Nebula (NGC 6334), a massive, local star-forming region,” said <a href="https://www.esa.int/ESA_Multimedia/Images">ESA</a>.



“This area is of great interest to scientists, having been subject to previous study by NASA/ESA’s Hubble and retired NASA Spitzer Space telescopes, as they seek to understand the multiple steps required for a turbulent molecular cloud to transition to stars.”



<h2 class="wp-block-heading" id="h-activity-in-the-cat-s-paw-nebula-nbsp">Activity in the Cat’s Paw Nebula&nbsp;</h2>



The Cat’s Paw Nebula is a <a href="https://www.earth.com/news/80-million-pixels-reveal-the-brilliance-of-a-star-cluster/">stellar nursery</a>, teeming with young, hot stars that are still forming from clouds of gas and dust. It spans roughly 50 light-years across and glows red, primarily due to the presence of ionized hydrogen gas illuminated by ultraviolet radiation from the newborn stars.&nbsp;



Much of the star formation remains hidden in visible light because of dense dust clouds, but observations in infrared and radio wavelengths have revealed an incredible amount of ongoing activity beneath the surface.



NGC 6334 is particularly rich in massive <a href="https://www.earth.com/news/planet-forming-disks-surrounding-stars-often-last-much-longer-than-expected/">stars</a>, including some that are over ten times the mass of the Sun.&nbsp;



Because of this, it's often used by astronomers to study the early stages of high-mass star formation, which are less understood than the processes that form lower-mass stars.&nbsp;



The region is also home to a number of protostars and clusters still wrapped in dusty cocoons, making it a dynamic and evolving part of our galaxy.



<h2 class="wp-block-heading" id="h-new-details-in-the-cat-s-paw-nebula-nbsp">New details in the Cat’s Paw Nebula&nbsp;</h2>



“With its near-infrared capabilities and sharp resolution, the telescope 'clawed' back a portion of a singular 'toe bean,' revealing a subset of mini toe bean-reminiscent structures composed of gas, dust, and young stars,” noted ESA.



“Webb’s view reveals a chaotic scene still in development: massive young stars are carving away at nearby gas and dust, while their bright starlight is producing a bright nebulous glow represented in blue.”&nbsp;



Although only recently recognized in modern astronomy, the Cat’s Paw Nebula has become iconic - not just for its curious shape, but also for the insight it offers into how massive stars form in the <a href="https://www.earth.com/news/milky-ways-thin-disk-is-billions-of-years-older-than-we-thought/">Milky Way</a>.



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



Scorpius is one of the most striking constellations in the night sky, especially visible during the summer months in the Southern Hemisphere and lower latitudes of the Northern Hemisphere.&nbsp;



Its shape is unusually recognizable, forming a long, curving line that resembles a scorpion with a curled tail and extended claws.&nbsp;



In mythology, Scorpius is often associated with the story of Orion, the great hunter. According to one version of the myth, Orion boasted that he could kill all the animals on Earth, which angered the goddess Artemis. To punish him, she sent a giant scorpion to defeat him.&nbsp;



After a fierce battle, both <a href="https://www.earth.com/news/our-solar-system-once-drifted-through-orions-star-forming-region/">Orion</a> and the scorpion were placed among the stars on opposite sides of the sky. To this day, Orion sets as Scorpius rises, as if the hunter is still fleeing from the celestial scorpion.



Antares, the brightest star in the constellation Scorpius, is a red supergiant whose name means "rival of Mars" due to its reddish hue and brightness. Antares serves as the scorpion's heart and is one of the most prominent stars in the night sky.&nbsp;



Because Scorpius lies along the plane of the <a href="https://www.earth.com/news/cosmic-map-reveals-that-the-milky-ways-dust-has-very-unusual-properties/">Milky Way</a>, it is filled with dense star fields and deep-sky objects. This part of the sky is exceptionally rich in detail, offering a glimpse into the crowded heart of our galaxy.



Image Credit: ESA



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Webb reveals the Cat's Paw Nebula in stunning detail

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

Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 1559, located around 35 million light-years away in the southern constellation Reticulum. The image was captured by the James Webb Space Telescope.&nbsp;



"The data featured in this portrait make use of two of Webb’s instruments: the Mid-InfraRed Instrument (MIRI) and Near-InfraRed Camera (NIRCam)," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Here MIRI captures the glow of interstellar dust grains, which trace out the interstellar medium, the fuel for future star formation. NIRCam shows the light from stars, even young stars hidden behind prodigious amounts of dust. NIRCam also captures emission from ionized nebulae around young stars."



<h2 class="wp-block-heading" id="h-webb-reveals-galaxies-in-new-light">Webb reveals galaxies in new light</h2>



According to ESA, the data was collected by the <a href="https://sites.google.com/view/phangs/home">PHANGS team</a> as part of a program in which Webb will observe 55 <a href="https://www.earth.com/news/james-webb-captures-galaxies-that-are-too-old-to-exist/">galaxies</a> that have also been mapped by the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope, the Hubble Space Telescope, and more.&nbsp;



"By combining Webb’s unprecedented view of the dust and stars with data from these other facilities, the team aims to obtain a new, highly detailed view of how stars are born, live, and die in galaxies across the Universe."



<h2 class="wp-block-heading" id="h-ngc-1559-a-loner-in-space">NGC 1559: A loner in space</h2>



Although NGC 1559 appears to sit close to one of our nearest neighbors in the sky - the Large Magellanic Cloud (LMC) - this is just a trick of perspective, noted ESA.



While it is part of the Reticulum constellation, NGC 1559 is not part of the Local Group of galaxies but instead resides in a more distant region of space.



"In reality, NGC 1559 is physically nowhere near the LMC in space; in fact it truly is a loner, lacking the company of any nearby galaxies or membership of any galaxy cluster," said ESA.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1559">Star formation in NGC 1559</h2>



NGC 1559 is notable for its active star formation and strong magnetic fields. It has also been the site of several <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, making it of particular interest to astronomers who study stellar evolution and the life cycle of stars.



The structure of NGC 1559 includes well-defined spiral arms that contain young, hot stars and regions of ionized gas, indicative of ongoing <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>.



<h2 class="wp-block-heading" id="h-an-extragalactic-wonder">An extragalactic wonder</h2>



Despite being relatively small compared to larger galaxies like the Milky Way, NGC 1559 is an important object for understanding how barred spiral galaxies evolve and the processes that trigger supernovae.



The galaxy’s remote location and active nature make it a fascinating subject of study in the field of extragalactic astronomy. 



The isolation of NGC 1559 allows for a clearer view of its structure without much interference from neighboring galaxies.



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



Barred spiral galaxies are a type of spiral galaxy characterized by a central bar-shaped structure composed of stars. This bar extends out from the core and connects to the galaxy's spiral arms, which swirl outward in a graceful pattern.



Scientists believe that the bar plays a crucial role in the evolution of the galaxy, funneling gas towards the core and potentially triggering star formation or feeding a central black hole. 



The <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our own galaxy, is an example of a barred spiral. These galaxies are quite common in the universe, making up about two-thirds of all observed spiral galaxies.



The bar itself is thought to be a temporary feature, developing as the galaxy matures and possibly disappearing over time as the dynamics of the stars change. 



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



Reticulum is a small, faint constellation in the southern sky. Its name means "the reticle" in Latin, which refers to the crosshairs in an eyepiece of a telescope.



The constellation was named in the 18th century by the French astronomer Nicolas Louis de Lacaille to honor the reticle he used in his scientific instruments. It is one of the 88 modern constellations recognized by the International Astronomical Union.



Image Credit: ESA/Webb, NASA &amp; CSA, A. Leroy, J. Lee and the PHANGS Team



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Spiral galaxy glows with young stars and interstellar dust

Today's Image of the Day from the <a href="https://www.eso.org/public/">European Southern Observatory</a> (ESO) features a stunning view of the Sculptor Galaxy, one of the brightest spiral galaxies visible from Earth.



The ultra-detailed image, which was captured using ESO’s Very Large Telescope, reveals features in the Sculptor Galaxy that have never been seen before.&nbsp;



ESO researcher Enrico Congiu led a new study on the Sculptor Galaxy that is published in the journal Astronomy &amp; Astrophysics.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-wide-view-of-sculptor-nbsp">A galaxy-wide view of Sculptor&nbsp;</h2>



The team observed the galaxy in thousands of wavelengths at once, collecting an immense amount of data from every point across its structure. This allowed them to build a comprehensive, galaxy-wide view of how <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/">stars</a> live and evolve within Sculptor.



"Galaxies are incredibly complex systems that we are still struggling to understand," said Congiu.



“The Sculptor Galaxy is in a sweet spot. It is close enough that we can resolve its internal structure and study its building blocks with incredible detail, but at the same time, big enough that we can still see it as a whole system.”



<h2 class="wp-block-heading" id="h-thousands-of-distinct-colors-nbsp">Thousands of distinct colors&nbsp;</h2>



<a href="https://www.earth.com/news/oxygen-detected-in-the-most-distant-and-primitive-galaxy-ever-analyzed/">Galaxies</a> span hundreds of thousands of light-years, yet their evolution is shaped by processes unfolding on much smaller scales.&nbsp;



The fundamental components of a galaxy - stars, gas, and dust - each emit light in distinct colors. The more shades of color captured in an image, the deeper the insight into a galaxy’s internal structure.&nbsp;



Traditional images typically contain only a few colors, but the new map of the Sculptor Galaxy includes thousands.&nbsp;



This rich spectrum provides astronomers with detailed information about the galaxy’s stars, gas, and dust - from their ages and chemical makeup to how they’re moving through space.



<h2 class="wp-block-heading" id="h-mapping-the-sculptor-galaxy-nbsp">Mapping the Sculptor Galaxy&nbsp;</h2>



The research team spent more than 50 hours observing the Sculptor Galaxy using the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope.&nbsp;



To capture the full view - spanning roughly 65,000 light-years - they combined over 100 separate exposures into a single, detailed mosaic.&nbsp;



According to study co-author Kathryn Kreckel from Heidelberg University, Germany, this makes the map a potent tool.&nbsp;



“We can zoom in to study individual regions where stars form at nearly the scale of individual stars, but we can also zoom out to study the galaxy as a whole,” said Kreckel.&nbsp;



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



In their initial analysis of the data, the team identified around 500 planetary <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/">nebulae</a> scattered throughout the Sculptor Galaxy.



Study co-author Fabian Scheuermann, a doctoral student at Heidelberg University, emphasized the significance of the discovery.&nbsp;



Scheuermann noted that when astronomers study galaxies outside of our own cosmic neighborhood, they normally detect fewer than 100 planetary nebulae in each one.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-of-extremes">A galaxy of extremes</h2>



The Sculptor Galaxy, also known as NGC 253, is located about 11.4 million light-years away in the constellation Sculptor. It’s classified as a starburst galaxy, meaning it’s undergoing an exceptionally high rate of <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/">star formation</a>.&nbsp;



This vigorous star-making activity is especially intense in its central regions, where dense clouds of gas and dust feed the birth of new stars.&nbsp;



The galaxy is tilted at a steep angle from our perspective, which gives it a striking, elongated appearance when viewed through telescopes.



<h2 class="wp-block-heading" id="h-notable-features-of-the-sculptor-galaxy-nbsp">Notable features of the Sculptor Galaxy&nbsp;</h2>



Discovered in 1783 by Caroline Herschel, the Sculptor Galaxy has become a popular target for both professional astronomers and amateur skywatchers due to its brightness and relative proximity.&nbsp;



It’s part of the Sculptor Group, one of the nearest groups of galaxies to our Local Group. Despite being rich in star-forming regions, much of its inner structure is veiled by thick dust lanes.&nbsp;



However, infrared and X-ray observations have helped scientists peer through the obscuring material to study the galaxy’s core, revealing a wealth of activity including supernova remnants and a possible central <a href="https://www.earth.com/news/largest-ultramassive-black-hole-ever-seen-cosmic-horseshoe-lrg-3-757/">black hole</a>.



The Sculptor Galaxy is also notable for its extended halo of stars and gas, which suggests past interactions or mergers with smaller galaxies.&nbsp;



This halo, along with its active central region, makes NGC 253 a valuable subject for understanding how galaxies evolve, form stars, and recycle gas over time. Its combination of beauty and scientific richness continues to make it a focus of galactic studies.



Image Credit: European Southern Observatory&nbsp;



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Thousands of colors in the Sculptor Galaxy

Today's Image of the Day from the European Southern Observatory...

Today's Image of the Day from the European Space Agency features a stunning reflection nebula known as GN 04.32.8 in the constellation Taurus.



Reflection nebulae are cosmic clouds of fine dust that become visible not by producing their own light, but by reflecting the light of nearby stars.&nbsp;



Unlike emission <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/">nebulae</a>, which glow due to ionized gases radiating light, reflection nebulae shine more subtly.&nbsp;



The light from nearby stars strikes the dust particles within the cloud and scatters in many directions - especially shorter, bluer wavelengths. This scattering effect, similar to the way Earth’s sky appears blue, often gives reflection nebulae their characteristic bluish hue.



<h2 class="wp-block-heading" id="h-the-taurus-molecular-cloud">The Taurus Molecular Cloud</h2>



“GN 04.32.8 is a small part of the stellar nursery known as the Taurus Molecular Cloud. At only roughly 480 light-years from Earth in the constellation Taurus, it's one of the best locations for studying newly forming stars,” noted <a href="https://www.esa.int/ESA_Multimedia/Images">ESA</a>.



The Taurus Molecular Cloud is one of the closest and most extensively studied regions for low-mass star formation.&nbsp;



Unlike larger star-forming regions like <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/">Orion</a> that produce many high-mass stars, the TMC is dominated by the formation of Sun-like and smaller stars, making it a prime analog for understanding the conditions that led to the birth of our own solar system.



<h2 class="wp-block-heading" id="h-energetic-stars-in-the-constellation-taurus-nbsp">Energetic stars in the constellation Taurus&nbsp;</h2>



“This reflection nebula is illuminated by the system of three bright stars in the center of this image, mainly the variable star V1025 Tauri in the very center.”&nbsp;



“One of those stars overlaps with part of the nebula: this is another variable star that is named HP Tauri, but is classified as a T Tauri star, for its similarity to yet another variable star elsewhere in the Taurus Molecular Complex.”&nbsp;



T Tauri stars are young, energetic stars in the earliest stages of stellar evolution, just beginning their journey toward becoming stable main sequence stars like our <a href="https://www.earth.com/news/discovery-sun-like-stars-with-secret-companions/">Sun</a>.&nbsp;



These stars are highly variable and surrounded by dense clouds of gas and dust, often exhibiting strong stellar winds and flares as they settle into equilibrium.&nbsp;



<h2 class="wp-block-heading" id="h-a-dynamic-star-system">A dynamic star system</h2>



In this case, the trio of T Tauri stars - named HP Tau, HP Tau G2, and HP Tau G3 - are believed to be gravitationally bound, forming a dynamic triple star system.



“Eagle-eyed viewers might notice the small, squashed, orange spot, just left of center below the clouds of the nebula, that’s crossed by a dark line. This is a newly-formed protostar, hidden in a <a href="https://www.earth.com/news/planet-forming-disks-surrounding-stars-often-last-much-longer-than-expected/">protoplanetary disc</a> that obstructs some of its light,” explained ESA.



“Because the disc is edge-on to us, it’s an ideal candidate for study. Astronomers are using Hubble here to examine it closely, seeking to learn about the kinds of exoplanets that might be formed in discs like it.”



<h2 class="wp-block-heading" id="h-the-light-of-hot-young-stars">The light of hot, young stars</h2>



Reflection nebulae are usually found in regions where new <a href="https://www.earth.com/news/10-billion-white-dwarf-stars-in-milky-way-galaxy-might-have-habitable-planets/">stars</a> are forming, often near or within dense molecular clouds.&nbsp;



Some reflection nebulae can span light-years across and serve as markers of stellar nurseries - places where future generations of stars are taking shape.



Reflection nebulae offer astronomers a valuable glimpse into the structure and composition of the interstellar medium and help trace the life cycles of stars from birth to maturity.



<h2 class="wp-block-heading" id="h-examples-of-reflection-nebulae-nbsp">Examples of reflection nebulae&nbsp;</h2>



One well-known example is the reflection nebula surrounding the Pleiades star cluster, also called the Seven Sisters.&nbsp;



The Iris Nebula, located in the constellation Cepheus about 1,300 light-years from Earth, is a striking reflection nebula illuminated by the young star SAO 19158.



This Nebula is a popular target for astrophotographers due to its vivid colors and intricate structure.



Found about 1,600 light-years away, M78 is the brightest reflection nebula in the Orion constellation and one of the easiest to observe with amateur telescopes. It’s illuminated by two young stars, HD 38563A and HD 38563B.&nbsp;



M78 is part of a larger complex of gas and dust that includes many other star-forming regions within the Orion Molecular Cloud.



Image Credit: ESA&nbsp;



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Young stars illuminate a reflection nebula in Taurus 

Today's Image of the Day from the European Space Agency features the spiral galaxy UGC 11397 in the constellation Lyra (The Lyre).



The light captured in this striking image traveled for 250 million years before reaching the NASA/ESA <a href="https://www.earth.com/news/35-years-of-hubble-the-telescope-that-changed-our-view-of-the-universe/">Hubble Space Telescope</a>.



“At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust,” noted ESA.



“What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of the Sun is growing.”&nbsp;



<h2 class="wp-block-heading" id="h-a-hidden-powerhouse">A hidden powerhouse</h2>



As the <a href="https://www.earth.com/news/largest-oldest-black-hole-jet-ever-seen-is-size-of-three-milky-ways-j1601-3102/">black hole</a> consumes gas, dust, and even entire stars from its surroundings, the infalling material heats up dramatically, producing a dazzling display of energy.&nbsp;



These emissions span the electromagnetic spectrum - from gamma rays to radio waves - and can flare or fade unpredictably.&nbsp;



“But in some galaxies, including UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light,” explained ESA.



“Despite this, UGC 11397's actively growing black hole was revealed through its bright X-ray emission - high-energy light that can pierce the surrounding dust.”&nbsp;



Its distinctive signature has earned UGC 11397 the classification of a Type 2 Seyfert galaxy. This category describes active galaxies whose central regions are obscured in visible light by a doughnut-shaped cloud of dust and gas.



<h2 class="wp-block-heading" id="h-galaxy-and-black-hole-growth">Galaxy and black hole growth</h2>



“Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass,” noted ESA.&nbsp;



“The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.”



Studying <a href="https://www.earth.com/news/hidden-galaxies-discovery-would-upend-current-understanding-of-universe/">galaxies</a> like UGC 11397 also offers insight into the mysterious relationship between supermassive black holes and their host galaxies.&nbsp;



Despite residing at the heart of galaxies, these black holes influence their surroundings on a much larger scale, often regulating the formation of stars and even shaping the structure of the galaxy itself.



<h2 class="wp-block-heading" id="h-tracing-black-hole-origins">Tracing black hole origins</h2>



One of the key questions astronomers hope to answer is how these black holes grow so massive in the first place.&nbsp;



While some appear to have formed gradually over billions of years, others - especially those in the early universe - seem to have reached enormous sizes much more quickly. 



Observations of galaxies such as UGC 11397 provide crucial data to test different growth scenarios.



<h2 class="wp-block-heading" id="h-a-clearer-picture-of-cosmic-evolution">A clearer picture of cosmic evolution</h2>



By combining Hubble’s observations with data from other telescopes, including those that detect X-rays and radio waves, researchers can build a more complete picture of how matter behaves around black holes.&nbsp;



This multi-wavelength approach is essential for studying objects obscured by dust, like Type 2 Seyfert galaxies, where optical views alone can be misleading.



Hubble’s sharp vision also allows astronomers to examine the surrounding galactic disk and spiral arms in high detail. 



These structures hold clues about recent star formation, galactic dynamics, and how gas flows toward the center - fueling both star birth and black hole growth.



<h2 class="wp-block-heading" id="h-black-hole-energy-in-active-galaxies">Black hole energy in active galaxies</h2>



In many active <a href="https://www.earth.com/news/thousands-of-galaxies-revealed-in-a-single-webb-image/">galaxies</a>, the energy released by the central black hole can blast out powerful winds or jets that affect star formation. These feedback processes can either shut down or stimulate the creation of new stars, depending on the conditions.&nbsp;



Understanding when and how this feedback occurs is another major goal of Hubble’s ongoing studies.



UGC 11397 is just one of many galaxies being surveyed as part of broader efforts to trace the cosmic history of <a href="https://www.earth.com/news/black-holes-turn-into-white-holes-and-blast-out-matter-and-time-runs-backwards/">black hole</a> activity.&nbsp;



Projects such as these are helping scientists map how common active galactic nuclei are, how their properties evolve over time, and how they relate to galaxy mergers and other large-scale events.



The wealth of information gathered from galaxies like UGC 11397 is not only deepening our understanding of black holes but also refining models of galaxy formation and evolution.&nbsp;



With each new observation, astronomers are piecing together the vast and complex puzzle of how galaxies and their central engines co-evolve across cosmic time.



Image Credit: ESA/Hubble &amp; NASA, M. J. Koss, A. J. Barth



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Graceful spiral galaxy hides a dark secret

A global team of researchers has delivered new evidence that public backing for climate measures rises when people connect extreme weather with climate change.



The findings also reveal a nuanced picture. Certain hazards, such as <a href="https://www.earth.com/news/mapping-marine-heatwaves-to-understand-their-impacts/">heatwaves</a> and tropical cyclones, appear to shift attitudes more than others - and the size of this shift varies widely across regions.



The study gauged support for a suite of government policy measures. These included higher taxes on carbon-intensive foods, steeper levies on fossil fuels, expanded public transport infrastructure, wider deployment of <a href="https://www.earth.com/news/tapping-into-the-natural-power-of-plants-for-renewable-energy/">renewable energy</a>, and stronger protection of forests and other natural land.



<h2 class="wp-block-heading" id="h-disaster-blame-shapes-climate-views">Disaster blame shapes climate views</h2>



Using a dataset that blended satellite-derived records of natural disasters including storms, floods, fires, and droughts with survey responses from 68 countries, the authors estimated how many citizens had faced each hazard in recent years. They then compared that exposure to stated policy preferences.



The results highlight the psychological weight of attribution - the extent to which respondents believe climate change has intensified local disasters.&nbsp;



“Our data suggest that if individuals attribute extreme weather events to climate change, support for climate policies is higher regardless of whether the events are more frequent,” the scientists explained.



They also conceded that reverse causality is possible: environmentally minded citizens may be more inclined to blame climate change for a <a href="https://www.earth.com/news/can-we-outrun-the-flood-risks-of-climate-change/">flood</a> or heatwave.



<h2 class="wp-block-heading" id="h-biggest-supporters-of-climate-policies">Biggest supporters of climate policies</h2>



Taxation remains a tough sell. “Increasing carbon taxes received the lowest support, with only 22 percent and 29 percent of people, respectively, indicating they very much supported increased taxes on carbon-intensive foods and <a href="https://www.earth.com/news/more-warnings-fossil-fuels-are-causing-climate-health-and-biodiversity-crises/">fossil fuels</a>,” the authors wrote.



“Protecting forested and land areas, by contrast, was a popular policy option. Eighty-two percent supported it very much and only three percent not supporting it at all.” 



Renewables ranked second, drawing strong approval from three in four respondents. Demographic factors moderated these views. 



“Participants who identified as men, were younger, more religious, had higher education, higher income, left-leaning politics, and who lived in urban areas were more likely to support climate policies,” the researchers explained.



Such patterns echo earlier work on environmental attitudes but gain statistical heft when paired with hard numbers on disaster exposure.



<h2 class="wp-block-heading" id="h-some-disasters-matter-more">Some disasters matter more</h2>



Support was highest across Africa and Asia, middle of the pack in Australia, Costa Rica, and the United Kingdom, and below average in parts of Europe such as Czechia, Finland, and Norway.



To better understand why some disasters sway opinion more than others, the team examined the “management potential” of each event type.



Heatwaves and <a href="https://www.earth.com/news/are-bomb-cyclones-increasing-due-to-climate-change/">cyclones</a>, they argue, lend themselves to engineering solutions - irrigation or seawalls - so citizens may associate them more closely with concrete policy interventions.



“One possible explanation is that these types of extreme weather events allow for management strategies that can directly reduce the hazard itself,” the scientists noted, listing measures like “flood protections, irrigation systems, prescribed burn-offs, and land-use policies.”



<h2 class="wp-block-heading" id="h-perception-shapes-climate-response">Perception shapes climate response</h2>



Another key takeaway: simply living through a disaster does not automatically translate into greener voting habits. For most hazard categories, raw exposure showed little correlation with climate policy support unless people also perceived a climate link.



The authors pointed out that attribution varies dramatically around the world. In South America - particularly Brazil and Colombia - people overwhelmingly agree that storms and heatwaves are climate-driven. 



Northern Europe and much of Africa report lower attribution levels, mirroring polls that find limited awareness of anthropogenic climate change in those regions.



<h2 class="wp-block-heading" id="h-disasters-demand-climate-framing">Disasters demand climate framing</h2>



The paper suggests that effective climate messaging should draw explicit connections between local disasters and broader warming trends, especially in places where that mental bridge is weak. 



At the same time, communication campaigns must navigate skepticism toward carbon pricing by highlighting co-benefits of renewables or ecosystem protection.



The authors caution that their results do not prove causation in a strict sense, but the statistical associations are robust across thousands of survey responses and multiple modeling approaches.



They call for follow-up studies focused on how to communicate about lesser-known hazards. These include prolonged droughts and slow-onset sea level rise, which citizens may not instinctively link to climate change.



Finally, the experts stress that policy design must account for demographic and cultural nuances. For officials drafting climate plans after a devastating storm, the lesson is clear. 



The public’s willingness to pay for mitigation will hinge not only on their lived experience but also on whether they see that storm as another symptom of a warming planet.



The study is published in the journal <a href="https://www.nature.com/articles/s41558-025-02372-4">Nature Climate Change</a>.



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Connecting disasters to climate change drives public action

A global team of researchers has delivered new evidence that...

Ozempic,Insulin,Injection,Pen,Or,Insulin,Cartridge,Pen,For,Diabetics.

A once‑weekly injection of semaglutide or tirzepatide has become the hottest ticket in obesity care. Pharmacies struggle to keep the GLP-1 pens in stock, and billboards promise effortless appetite control. 



A new analysis out of the <a href="https://www.ox.ac.uk/" target="_blank" rel="noreferrer noopener">University of Oxford</a> shows the scale of the catch: most users are back at their starting weight roughly a year after the last dose of GLP-1.



“These drugs are very effective at helping you lose weight, but when you stop them, weight regain is much faster than after stopping diets,” said <a href="https://www.phc.ox.ac.uk/team/susan-jebb" target="_blank" rel="noreferrer noopener">Susan Jebb</a>, professor of diet and population health at the University of Oxford.



<h2 class="wp-block-heading" id="h-why-glp-1-drugs-work">Why GLP‑1 drugs work</h2>



A class of medicines called <a href="https://my.clevelandclinic.org/health/treatments/13901-glp-1-agonists" target="_blank" rel="noreferrer noopener">GLP‑1 receptor agonists</a> mimics a gut hormone that slows stomach emptying and tells the brain that the tank is full. Semaglutide and tirzepatide also dampen reward signals linked to food, so cravings fade.



Clinical trials report average losses of 15 percent body weight in about 68 weeks when the injections are paired with nutrition counseling. Participants often see blood‑pressure and cholesterol numbers improve alongside the shrinking waistline.



Both drugs amplify insulin release after meals, lowering glucose swings that can drive hunger. At higher doses they carve out a new <a href="https://www.earth.com/news/plant-extracts-may-help-treat-metabolic-syndrome/">metabolic</a> set point, convincing the body that the lighter figure is normal.



<h2 class="wp-block-heading" id="h-what-happens-if-you-stop-glp-1">What happens if you stop GLP-1</h2>



The Oxford team pooled data from 11 studies covering 6,370 adults and found that pounds crept back at roughly 1.5 each month once treatment ended. 



Within ten months the typical participant regained 18 pounds, erasing the 17‑pound loss recorded at the final clinic visit.



In trials of the newer, stronger agents, the bounce‑back was just as swift. The <a href="https://www.nejm.org/doi/full/10.1056/NEJMoa2206038" target="_blank" rel="noreferrer noopener">SURMOUNT‑1 study</a> showed a 21 percent weight drop on tirzepatide, yet follow‑up revealed nearly half of that loss returned in the first year after discontinuation.



Researchers see two forces at work. First, hunger hormones roar back to pre‑treatment levels within weeks, leaving people suddenly ravenous. Second, many patients never practiced portion control while medicated, so they lack habits that cushion the transition.



<h2 class="wp-block-heading" id="h-drug-discontinuation-vs-quitting-a-diet">Drug discontinuation vs. quitting a diet</h2>



Stopping a calorie‑restricted diet is also linked to regain, but the slope is gentler. 



A 2023 <a href="https://pubmed.ncbi.nlm.nih.gov/36974678/" target="_blank" rel="noreferrer noopener">meta‑analysis</a> of behavioral weight‑management programs showed that participants took at least five years to drift back to baseline. Lifestyle plans demand daily choices, and those routines appear to leave a longer‑lasting imprint.



“It shouldn’t surprise anyone if people regain weight having used GLP‑1 drugs without seriously attempting to improve their lifestyle,” said <a href="https://www.elevatearena.com/london/speakers/tam-fry" target="_blank" rel="noreferrer noopener">Tam Fry</a> of the <a href="https://pubmed.ncbi.nlm.nih.gov/27316564/" target="_blank" rel="noreferrer noopener">National Obesity Forum</a>, offering blunt criticism.&nbsp;



“They’re going to need psychological, nutritional, and behavior change support from that moment on to help them sustain healthier behavior,” noted <a href="https://www.surrey.ac.uk/people/jane-ogden" target="_blank" rel="noreferrer noopener">Jane Ogden</a>, a health psychologist at the <a href="https://www.surrey.ac.uk/" target="_blank" rel="noreferrer noopener">University of Surrey</a>, explaining that counseling must start the moment a prescription ends.&nbsp;



<h2 class="wp-block-heading" id="h-policy-dilemma-for-health-systems">Policy dilemma for health systems</h2>



Britain’s National Institute for Health and Care Excellence (<a href="https://www.nice.org.uk/" target="_blank" rel="noreferrer noopener">NICE</a>) limits semaglutide coverage to two years inside specialist services. Payers worry that footing the bill for lifelong injections would bust budgets, yet short courses look futile.



In the United States, employers negotiate steep rebates on GLP-1 medications but still face annual costs exceeding twenty thousand dollars per patient. 



Insurers now debate whether maintenance dosing at a lower level could hold the line without breaking the bank.



Clinicians face ethical questions as well. Should a physician start therapy knowing most users will eventually stop and rebound, or withhold the option until longer‑term answers arrive?



<h2 class="wp-block-heading" id="h-helping-patients-transition-off-glp-1">Helping patients transition off GLP-1</h2>



Obesity specialists increasingly frame GLP‑1 therapy as a bridge rather than a cure. Structured exit plans include gradual dose tapering, monthly check‑ins, and enrollment in digital coaching platforms.



Dietitians encourage a higher protein intake and resistance training to preserve lean mass, which may blunt the metabolic slowdown that follows rapid <a href="https://www.earth.com/news/scientists-identify-two-key-habits-for-losing-weight-without-dieting-meal-timing/">weight</a> loss. 



Simple self‑monitoring tools, such as a weekly step target or photo‑based food diary, add accountability once pharmacologic restraint disappears.



Group programs modeled on cardiac rehabilitation are being piloted in several NHS trusts. Early reports suggest that peer support helps maintain about three‑quarters of the initial loss at the one‑year mark, though results await formal publication.



<h2 class="wp-block-heading" id="h-long-term-treatment-options">Long‑term treatment options</h2>



Pharmaceutical companies are testing oral GLP‑1 combinations that might be taken indefinitely at a lower cost. A once‑monthly antibody fusion is entering phase 2 trials, aiming to smooth appetite signals without daily injections.



Researchers also explore “set point locking,” using brief courses of appetite suppressants alongside neuromodulation to recalibrate weight‑regulating neural circuits. 



Animal data hint that the brain can adopt a lighter normal if changes in intake and expenditure are synchronized.



Until those ideas mature, many experts advocate shared decision‑making. Patients who accept open‑ended therapy may stay on the shots, while others cycle off with an intensive lifestyle package.



The study is published in <a href="https://karger.com/ofa/article-pdf/doi/10.1159/000545547/4375755/000545547.pdf" target="_blank" rel="noreferrer noopener">Obesity Facts</a>.



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How and why health issues arise when people stop using new weight loss treatments

A once‑weekly injection of semaglutide or tirzepatide has become the...

Young trees in large forests are often dismissed as bit players in the fight against climate change, but new evidence shows their importance is anything but small. 



The latest study of <a href="https://www.fao.org/4/j0628e/J0628E16.htm" target="_blank" rel="noreferrer noopener">secondary forest regrowth</a> found that young trees, only a few decades old, can lock away carbon faster than almost any other land based solution.



Researchers mapped carbon removal in regrowing woodlands worldwide and discovered a sweet spot between 20 and 40 years where <a href="https://www.usgs.gov/faqs/what-carbon-sequestration" target="_blank" rel="noreferrer noopener">carbon sequestration</a> peaks, reaching up to eight times the rate recorded in newly sprouting forest patches.



The <a href="https://www.nature.com/articles/s41558-025-02355-5" target="_blank" rel="noreferrer noopener">work</a> was led by ecologist <a href="https://www.birmingham.ac.uk/staff/profiles/gees/muelbert-adriane-esquivel" target="_blank" rel="noreferrer noopener">Adriane Esquivel-Muelbert</a> at the <a href="https://www.birmingham.ac.uk/" target="_blank" rel="noreferrer noopener">University of Birmingham</a>, whose team says protecting these adolescent forests could keep billions of tons of CO2 out of the atmosphere.



<h2 class="wp-block-heading" id="h-young-forests-trap-more-carbon">Young forests trap more carbon</h2>



“Our research underscores the <a href="https://www.earth.com/news/forest-fire-smoke-boosts-ocean-life-but-with-a-hidden-cost/">critical role</a> of young secondary forests in the global fight against climate change,” said Esquivel-Muelbert. 



Overlooking their protection could forfeit the opportunity to capture carbon more quickly and at a larger scale when it's needed most.



The emphasis on youth contrasts with <a href="https://www.earth.com/news/forests-are-lagging-centuries-behind-in-climate-adaptation/">reforestation</a> drives that prioritize planting, then wait decades for stored carbon to accrue. 



Keeping a 25 year old stand standing can deliver as much carbon benefit as planting several acres of new trees because its engines are already running at full speed.



A global <a href="https://www.nature.com/articles/s41586-020-2686-x" target="_blank" rel="noreferrer noopener">synthesis</a> published in 2020 showed that natural forest regrowth could capture 226 gigatons of carbon over the century.



<h2 class="wp-block-heading" id="h-maps-reveal-fastest-carbon-gains">Maps reveal fastest carbon gains</h2>



The new paper applies a random forest model, crunching 109,708 field plots and 66 environmental layers to generate one kilometer growth curves for stands up to 100 years old. 



That computational lift produced the first fine scale map of how fast <a href="https://www.earth.com/news/virtual-forest-bathing-can-reduce-stress-and-improve-mood/">above-ground biomass</a> piles up decade by decade.



Across 800 million hectares of land identified as restorable, starting regeneration in 2025 could remove 20.3 billion metric tons of carbon by 2050. 



Delay the start to 2035 and the budget shrinks by almost half, underscoring the cost of procrastination.



Machine learning also revealed how growth spurts shift with latitude, offering a tool planners can use to rank projects by speed of return. Such spatial precision was impossible a decade ago.



Earlier satellite <a href="https://pubmed.ncbi.nlm.nih.gov/36922608/" target="_blank" rel="noreferrer noopener">work</a> led by Viola Heinrich showed recovering humid tropical forests store an average 3.6 billion tons of carbon but only if they survive interruptions from fire or fresh clearing.



<h2 class="wp-block-heading" id="h-young-forests-left-out-of-climate-plans">Young forests left out of climate plans</h2>



The Intergovernmental Panel on Climate Change (<a href="https://www.wri.org/insights/2023-ipcc-ar6-synthesis-report-climate-change-findings" target="_blank" rel="noreferrer noopener">IPCC</a>) warns that deep emissions cuts alone will not limit warming to 1.5 degrees Celsius above pre industrial levels, making carbon removal essential. 



Yet current market rules rarely pay for preserving forests younger than 20 years, creating a blind spot that could derail mitigation efforts.



Co‑author <a href="https://www.birmingham.ac.uk/staff/profiles/gees/pugh-thomas" target="_blank" rel="noreferrer noopener">Tom Pugh</a>, from the School of Geography, Earth and Environmental Sciences, at the University of Birmingham, notes that young stands “aren’t even on the books” for many offset schemes, despite their outsized impact. 



Fixing that oversight, the team argues, would steer finance toward projects that begin sequestering carbon within a single election cycle instead of a generation.



A persistent global forest sink of roughly <a href="https://www.science.org/doi/10.1126/science.1201609" target="_blank" rel="noreferrer noopener">2.4 petagrams</a> of carbon per year from 1990 to 2007 already helps offset emissions, but analysts say ramping up the sink during the decisive 2020s could keep warming targets within reach.



<h2 class="wp-block-heading" id="h-location-changes-forest-carbon-speed">Location changes forest carbon speed</h2>



<a href="https://education.nationalgeographic.org/resource/resource-library-biomes/" target="_blank" rel="noreferrer noopener">Biome</a> type influences when forests hit their peak carbon removal rates. In <a href="https://earthobservatory.nasa.gov/biome/biorainforest.php" target="_blank" rel="noreferrer noopener">warm tropical zones</a>, forests often reach their highest rates in their early 20s, while <a href="https://www.oneearth.org/ecoregions/mediterranean-woodlands-and-forests/" target="_blank" rel="noreferrer noopener">Mediterranean woodlands</a> may not hit that point until they're closer to 50 years old.



Even so, the per hectare advantage of youth appears everywhere. In the Amazon, a forest that is eight years old today would draw 36 percent more carbon by 2030 than a clear cut plot replanted next year.



Similar arithmetic holds in <a href="http://costarica-information.com/nature/ecosystems-of-costa-rica/Lowland%20Rainforest" target="_blank" rel="noreferrer noopener">Costa Rica’s wet lowlands</a>, where a 20 year old stand can outperform seedlings by 65 percent over the same window. That universality makes age tracking as important as area.



Journalist <a href="https://www.reuters.com/sustainability/climate-energy/policymakers-often-ignore-forest-regeneration-fight-against-climate-change-2025-06-24/" target="_blank" rel="noreferrer noopener">data</a> show that fewer than six percent of young forests in the tropics survive long enough to reach their twentieth birthday, often sacrificed to repeat agricultural cycles or burned in accidental fires.



<h2 class="wp-block-heading" id="h-saving-trees-saves-money">Saving trees saves money</h2>



Carbon credits linked to young forest protection could offer investors quicker returns than tree planting programs because monitoring tools can confirm <a href="https://www.earth.com/news/protecting-forests-helps-birds-and-humans-in-many-ways/">biomass gains</a> within a few years. That speed matters to companies racing toward net zero pledges set for 2030.



Maintaining existing young stands is also cheaper for governments. Studies suggest natural regeneration costs a fraction of active planting while delivering side benefits such as better soil structure and wildlife habitat.



A fresh economic <a href="https://www.nature.org/content/dam/tnc/nature/en/documents/N4C_NaturePositiveRecoveryReport_063020.pdf" target="_blank" rel="noreferrer noopener">analysis</a> estimated that every dollar spent on safeguarding regrowth can yield climate returns three to four times higher than planting efforts in the same region.



<h2 class="wp-block-heading" id="h-global-talks-may-boost-forests">Global talks may boost forests</h2>



The study lands months before negotiators gather in Belém, Brazil, for <a href="https://cop30.br/en" target="_blank" rel="noreferrer noopener">COP30</a>. The hosts sit amid the world’s largest tropical forest and also the fastest disappearing, giving added weight to calls for immediate safeguards on regrowth.



“We urge policymakers to prioritize the protection and regeneration of young secondary forests,” said Esquivel‑Muelbert. She wants treaty language that treats young forests as a strategic reserve, not a placeholder. 



Brazilian officials have hinted that regrowth credits could join the country’s voluntary carbon market, a signal observers hope will ripple across the Amazon Basin. If other nations follow, the carbon math suggests the path to net zero could get a much needed boost.



The study is published in <a href="https://www.nature.com/articles/s41558-025-02355-5" target="_blank" rel="noreferrer noopener">Nature Climate Change</a>.



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Young forests, big climate punch: Why 20-year‑old trees matter most

Young trees in large forests are often dismissed as bit...

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<script src="data:image/gif;base64,R0lGODlhAQABAIAAAAAAAP///yH5BAEAAAAALAAAAAABAAEAAAIBRAA7" type="text/javascript"></script></div>
 
Iceland is losing its ice Iceland is losing its ice Today&#8217;s Video of the Day from the <a href="https://www.usgs.gov/">USGS</a> shows the rapid retreat of ice across Iceland over the last five decades. 
For example, the OK Glacier in western Iceland had lost so much of its ice by 2014 that it was no longer considered a glacier. As seen above in the video is Iceland is losing its ice showing the changes of the ice due to climate.
The same year, glaciologists concluded that the current rate of melting will wipe out all of the country&#8217;s ice except its highest elevation glaciers by the year 2200. Icelandic is the national language of Iceland. Many people (nearly 100% below the age of 50) speak very good English. You will also hear Danish, German, and Polish quite often.
The Golden Circle is the most popular sightseeing route in Iceland, and there is no wonder as to why; it&#8217;s accessible all year round, it can be visited in half a day from Reykjavík whether booking a tour or driving yourself, and the sites along it are incredible. Akureyri: Explore the second largest city in Iceland. The second-largest city in Iceland, sitting just behind Reykjavik in terms of population, Akureyri is located in the northern part of the island and has about 20,000 residents.
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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
Video Credit: USGS

Iceland is losing its ice

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