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



<h2 class="wp-block-heading" id="h-fuel-for-star-formation">Fuel for star formation </h2>



<p>"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>.</p>



<p>"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 ionised nebulae around young stars."</p>



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



<p>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;</p>



<p>"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."</p>



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



<p>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.</p>



<p>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.</p>



<p>"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."</p>



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



<p>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 studying stellar evolution and the lifecycle of stars.</p>



<p>The structure of NGC 1559 includes well-defined spiral arms that are rich in 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>.</p>



<p>The galaxy’s central bar is believed to play a role in driving gas towards the core, fueling both the star formation and the activity around its nucleus.</p>



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



<p>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.</p>



<p>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.</p>



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



<p>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.</p>



<p>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. </p>



<p>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.</p>



<p>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. </p>



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



<p>The Reticulum constellation 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. </p>



<p>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.</p>



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



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Spiral galaxy NGC 1559 is a loner in outer space

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

<p>Today's <strong>Image of the Day</strong> from the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba, about 43 million light-years away from Earth.&nbsp;</p>



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



<p>Image Credit<strong>:</strong> ESA/Hubble &amp; NASA, J. Lee</p>



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NGC 1792: A galactic powerhouse 

<p>Today's Image of the Day from NASA Earth Observatory features the Fedchenko Glacier in the Pamir Mountains of Tajikistan. It is one of the world's longest glaciers outside of the polar regions.&nbsp;</p>



<p>“An astronaut aboard the International Space Station took this photo of glaciers in the high-elevation valleys of the Pamir Mountains of Central Asia. The upper portion of Fedchenko Glacier crosses the center of the scene.”</p>



<p>NASA noted that most of the larger glaciers in the image show a prominent pattern of light- and dark-brown parallel lines.&nbsp;</p>



<p>“The darker ‘streamlines,’ known as medial moraines, give a sense of the direction of flow of the ice down the valleys. These are concentrations of debris that has been eroded by the glacier from the adjacent mountainsides or a rocky outcrop,” said NASA.</p>



<h2 class="wp-block-heading" id="h-fedchenko-a-high-altitude-glacier">Fedchenko: A high-altitude glacier</h2>



<p>Fedchenko Glacier stretches for approximately 48 miles and covers an area of around 270 square miles. This massive glacier is a critical source of <a href="https://www.earth.com/news/satellites-reveal-a-sudden-drop-in-global-freshwater-levels/" target="_blank" rel="noreferrer noopener">freshwater</a>, feeding several rivers and influencing the region's hydrology.</p>



<p>Fedchenko Glacier lies at high altitudes, with its origins in the high peaks of the Pamirs, where snow accumulates heavily. Despite being situated in a relatively arid region, the glacier's significant size and volume are maintained by substantial snowfall.&nbsp;</p>



<p>Named after Alexei Pavlovich Fedchenko, a Russian explorer and naturalist, the glacier was first surveyed in 1928 during Soviet-era expeditions. It plays a crucial role in climate studies, as changes in its length and mass provide insights into the effects of global warming in Central Asia.&nbsp;</p>



<p>The glacier is also part of a spectacular and remote landscape, surrounded by towering <a href="https://www.earth.com/news/early-humans-preferred-the-mountains-and-it-changed-our-evolution/" target="_blank" rel="noreferrer noopener">mountains</a> and rugged terrain, making it a key feature of the Pamirs' natural beauty.&nbsp;</p>



<h2 class="wp-block-heading" id="h-threats-to-glaciers-worldwide">Threats to glaciers worldwide</h2>



<p>Like many glaciers worldwide, Fedchenko faces the threat of retreat due to <a href="https://www.earth.com/news/peru-has-lost-over-half-of-its-glaciers-in-six-decades/" target="_blank" rel="noreferrer noopener">global warming</a>, raising concerns about water availability and ecosystem changes in the region.</p>



<p>Rising global temperatures caused by greenhouse gas emissions are the primary driver of glacier melting. Warmer temperatures not only melt glacier surfaces but also increase the flow of meltwater beneath them, accelerating their disintegration.</p>



<h3 class="wp-block-heading" id="h-human-activities-and-pollution-nbsp">Human activities and pollution&nbsp;</h3>



<p>Deforestation and urbanization exacerbate these effects by reducing reflective snow cover and increasing heat absorption in nearby areas.&nbsp;</p>



<p>Airborne pollutants like soot and black carbon darken glacier surfaces, reducing their ability to reflect sunlight and speeding up the rate of melting. </p>



<p>Industrial activities and tourism in glacier regions add physical stress and pollution, further degrading these fragile ecosystems.</p>



<h3 class="wp-block-heading" id="h-water-supplies">Water supplies</h3>



<p>The loss of glaciers has far-reaching consequences. It disrupts freshwater supplies for millions of people who depend on glacial runoff for drinking water, agriculture, and hydropower.&nbsp;</p>



<h3 class="wp-block-heading" id="h-rising-sea-levels">Rising sea levels</h3>



<p><a href="https://www.earth.com/news/melting-glaciers-unleash-invasive-species-into-unexpected-areas/" target="_blank" rel="noreferrer noopener">Melting glaciers</a> contribute to rising sea levels, threatening coastal communities and ecosystems worldwide. Additionally, the loss of glaciers impacts biodiversity, as many species rely on cold, glacial habitats for survival.</p>



<h3 class="wp-block-heading" id="h-protecting-glaciers">Protecting glaciers</h3>



<p>Efforts to mitigate these threats focus on reducing <a href="https://www.earth.com/news/melting-glaciers-are-hidden-sources-of-greenhouse-gases/" target="_blank" rel="noreferrer noopener">greenhouse gas</a> emissions, protecting glacier regions from industrial exploitation, and promoting sustainable tourism practices.&nbsp;</p>



<p>However, without urgent action, the continued decline of glaciers will have profound implications for the planet's climate, water systems, and ecosystems.</p>



<h2 class="wp-block-heading" id="h-the-pamir-mountains-nbsp">The Pamir Mountains&nbsp;</h2>



<p>The Pamir Mountains, often called the "Roof of the World," are a vast and rugged mountain range located in Central Asia.&nbsp;</p>



<p>They span across Tajikistan, Afghanistan, China, and Kyrgyzstan, forming a vital part of the junction where the Himalayas, the Tian Shan, the Karakoram, the Kunlun, and the Hindu Kush converge.&nbsp;</p>



<p>With peaks soaring over 7,000 meters, including Ismoil Somoni Peak, the range is home to some of the highest altitudes on Earth.</p>



<p>The Pamir Mountains have been central to trade and cultural exchange for centuries, serving as a critical segment of the ancient Silk Road.&nbsp;</p>



<p>Today, the mountains are a popular destination for trekkers and explorers drawn by their breathtaking beauty and challenging terrain.</p>



<p>The Pamirs are not only a natural wonder but also a biological treasure trove, supporting unique wildlife that is adapted to extreme altitudes.&nbsp;</p>



<p>Culturally, the mountains are home to diverse communities, each with its unique traditions and ways of life, shaped by the harsh but majestic environment.</p>



<p>Image Credit: NASA Earth Observatory</p>



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Fedchenko Glacier in the Pamir Mountains

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

<p>Today's <strong>Image of the Day</strong> from the European Space Agency features the spiral galaxy IC 5332, which is located over 29 million light-years away from Earth.</p>



<p>The galaxy spans approximately 66,000 light-years in diameter. This makes it notably smaller than our <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>, which is just over 100,000 light-years in diameter. </p>



<h2 class="wp-block-heading" id="h-unprecedented-look-at-ic-5332">Unprecedented look at IC 5332</h2>



<p>In a stunning photo release by NASA and ESA in 2022, the spiral galaxy IC 5332 was presented in an unprecedented level of detail. The images were captured by the <a href="https://www.earth.com/news/james-webb-captures-incredible-new-image-of-uranus/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a>.</p>



<p>This feat was made possible through the use of the Mid-InfraRed Instrument (MIRI), which captures images in the mid-infrared spectrum.</p>



<h2 class="wp-block-heading" id="h-unique-perspective-from-earth">Unique perspective from Earth</h2>



<p>One of the most striking features of IC 5332, as revealed by these observations, is its almost perfect face-on orientation relative to Earth.&nbsp;</p>



<p>This unique perspective allows astronomers to clearly observe and admire the symmetrical arrangement of its spiral arms.</p>



<h2 class="wp-block-heading" id="h-webb-unveils-ic-5332-in-new-light">Webb unveils IC 5332 in new light</h2>



<p>The clarity of these images represents a significant advancement over previous observations made by the Hubble Space Telescope, which imaged IC 5332 in ultraviolet and visible light.&nbsp;</p>



<p>While Hubble’s images revealed the galaxy’s symmetrical spiral arms, James Webb’s MIRI has unveiled these structures as a complex web of gas that emits infrared light at various temperatures.</p>



<h2 class="wp-block-heading" id="h-the-miri-instrument-on-james-webb-nbsp">The MIRI instrument on James Webb&nbsp;</h2>



<p>Capturing this range of infrared light is no simple task. It requires highly specialized instruments that must be maintained at extremely cold temperatures.&nbsp;</p>



<p>The MIRI instrument on the James Webb Space Telescope is specifically designed for this purpose and performs exceptionally well. Its capabilities allow astronomers to see aspects of <a href="https://www.earth.com/news/james-webb-captures-galaxies-that-are-too-old-to-exist/" target="_blank" rel="noreferrer noopener">galaxies</a> that are otherwise hidden in other wavelengths.</p>



<p>The detailed images provided by MIRI offer more than just a visual spectacle; they provide valuable data about the composition and temperature of the gases that make up the spiral arms of IC 5332. </p>



<p>This can help scientists understand the processes of star formation within the galaxy and how these processes compare to those in our own <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">Milky Way</a>.</p>



<h2 class="wp-block-heading" id="h-webb-finds-hidden-features-of-the-universe-nbsp">Webb finds hidden features of the universe&nbsp;</h2>



<p>The images of IC 5332 served as a critical test of the James Webb Space Telescope’s capabilities in observing the universe in infrared light. </p>



<p>As astronomers continue to explore with Webb’s full suite of instruments, many more hidden features of the universe will be revealed.</p>



<p>The information provided by the <a href="https://www.earth.com/news/webb-telescope-discovers-second-most-distant-galaxy-in-pandoras-cluster/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> not only expands our understanding of the cosmos but also enhances our appreciation for the complex and beautiful structures that exist in our universe.&nbsp;</p>



<h2 class="wp-block-heading" id="h-spiral-galaxies-like-ic-5332">Spiral galaxies like IC 5332</h2>



<p>Spiral galaxies are some of the most visually striking objects in the universe, characterized by their rotating arms that extend from a central nucleus, giving them a distinct spiral appearance.&nbsp;</p>



<p>These galaxies are primarily made up of a flat, rotating disk containing stars, gas, and dust, and a central concentration of stars known as the bulge. These are often surrounded by a much fainter halo of stars, many of which reside in globular clusters.</p>



<p>Spiral galaxies differ from other galaxy types, such as elliptical and irregular galaxies, in their structure and content. </p>



<p>The spiral arms are sites of ongoing star formation and are brighter than the rest of the disk because of the young, hot stars that are typically found there. The arms appear distinct because of their density waves, which compress the gas and dust, leading to star formation.</p>



<p>The rotation of the spiral arms also contributes to the galaxy's flat shape due to the centrifugal forces acting on the disk. The central bulge can vary in size and often contains older, red stars.&nbsp;</p>



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



<p>Some spiral galaxies have a bar-shaped structure that extends from the central bulge, making them barred spirals. This bar affects the motion of stars and gas within the galaxy and can influence star formation activity.</p>



<p>Spiral galaxies are an important focus of study because they contain a significant amount of visible matter and play a crucial role in understanding the formation and evolution of galaxies.&nbsp;</p>



<p>Their distinct features also make them particularly useful for studying the laws of physics under extreme conditions, such as high densities and velocities.</p>



<p>Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Webb, NASA &amp; CSA, J. Lee and the PHANGS-JWST and PHANGS-HST Teams</p>



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Spiral galaxy IC 5332: A complex web of gas and light

<p>Today's <strong>Image of the Day</strong> from the European Space Agency features the star-forming region NGC 604, which is located 2.73 million light-years away from Earth in the Triangulum Galaxy (M33). The image was captured by the James Webb Space Telescope.</p>



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



<p>Image Credit: NASA/ESA/CSA James Webb Space Telescope</p>



<p>-----</p>



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<p>-----</p>

Young, massive stars in the Triangulum Galaxy

<p>An asteroid impact on Mars about 11 million years ago, sending fragments of the Red Planet hurtling through space. One of these pieces eventually crashed into Earth and somehow made its way into a drawer of an old desk at Purdue University. </p>



<p>This rare find, now known as the Lafayette Meteorite, has been instrumental in unlocking secrets of <a href="https://www.earth.com/news/manganese-discovery-ancient-mars-earth-like-water-lake-habitable/" target="_blank" rel="noreferrer noopener">Mars</a>’ watery past, with new research recently published in the journal <a href="http://dx.doi.org/10.7185/geochemlet.2443" target="_blank" rel="noreferrer noopener"><em>Geochemical Perspective Letters</em></a> that provides insight into the timing and nature of Mars’ ancient water activity.</p>



<h2 class="wp-block-heading" id="h-tracing-mars-watery-past">Tracing Mars’ watery past</h2>



<p>Scientists have long known that the Lafayette Meteorite interacted with liquid water on Mars, but the exact timing of this event was uncertain.&nbsp;</p>



<p>Dr. Marissa Tremblay, an assistant professor at Purdue University’s <a href="https://www.eaps.purdue.edu/" target="_blank" rel="noreferrer noopener">Department of Earth, Atmospheric, and Planetary Sciences</a> (EAPS), led an international research team to determine the age of the water-altered minerals in the meteorite, pinpointing it to 742 million years ago.</p>



<p>“Dating these minerals can therefore tell us when there was liquid water at or near the surface of Mars in the planet's geologic past,” Tremblay explained.&nbsp;</p>



<p>The findings suggest that while liquid water wasn’t abundant on the surface at this time, it likely came from melting subsurface ice, or permafrost, caused by intermittent volcanic activity -- a phenomenon still observed on Mars today.</p>



<h2 class="wp-block-heading" id="h-preserving-a-moment-in-mars-geological-timeline">Preserving a moment in Mars’ geological timeline</h2>



<p>The study not only identified when water interacted with the meteorite but also established that the dating was unaffected by events after the meteorite left Mars.&nbsp;</p>



<p>“The age could have been affected by the impact that ejected the Lafayette Meteorite from Mars, the heating it experienced during the 11 million years it was floating in space, or the heating when it fell to Earth,” Tremblay said.&nbsp;</p>



<p>However, the team confirmed that none of these factors altered the age, validating the timeline of <a href="https://www.earth.com/news/mars-lost-most-of-its-water-but-where-did-it-go/" target="_blank" rel="noreferrer noopener">water</a> interaction.</p>



<p>Study co-author and Purdue EAPS researcher Ryan Ickert applied heavy isotope analysis to further verify that previous data on the meteorite’s water-rock interaction had likely been skewed by other geological processes.&nbsp;&nbsp;</p>



<p>“This meteorite uniquely has evidence that it has reacted with water. The exact date of this was controversial, and our publication dates when water was present,” said Ickert.</p>



<h2 class="wp-block-heading" id="h-mysterious-journey-of-the-meteorite">Mysterious journey of the meteorite </h2>



<p>The Lafayette Meteorite’s journey to Purdue is something of a mystery. It was found in a university drawer in 1931, though how it got there remains unknown.&nbsp;</p>



<p>In previous research, Tremblay and her team used crop disease markers from organic contaminants found on the meteorite to narrow down when it might have fallen to Earth.</p>



<p>Once the meteorite was ejected from Mars, it endured constant cosmic ray bombardment in space, which produced certain isotopes, offering clues to its time of impact on Earth.&nbsp;</p>



<p>“Many meteoroids are produced by impacts on Mars and other planetary bodies, but only a handful will eventually fall to Earth,” Tremblay said.</p>



<h2 class="wp-block-heading" id="h-planetary-time-capsules">Planetary time capsules</h2>



<p>Meteorites like Lafayette serve as planetary time capsules, offering invaluable data on the geological and environmental history of their <a href="https://www.earth.com/news/most-meteorites-can-be-traced-to-three-asteroid-families/" target="_blank" rel="noreferrer noopener">home worlds</a>. With their dense structure, metallic content, and magnetic properties, meteorites are often distinguishable from Earth rocks.&nbsp;</p>



<p>“We can identify meteorites by studying what minerals are present in them, their mineral relationships, and by checking for a fusion crust formed during entry into Earth’s atmosphere,” Tremblay explained.&nbsp;</p>



<p>By analyzing these traits and their chemical signatures, scientists can often determine a meteorite’s planetary origin.</p>



<h2 class="wp-block-heading" id="h-complex-history-of-meteorites">Complex history of meteorites</h2>



<p>This research marks a significant milestone for the team, which included scientists from institutions across the globe, such as the Scottish Universities Environmental Research Center (SUERC), the University of St. Andrews, the University of Glasgow, the University of Bristol, and London’s <a href="https://www.nhm.ac.uk/" target="_blank" rel="noreferrer noopener">Natural History Museum</a>.&nbsp;</p>



<p>“Before moving to Purdue, Ryan and I were both based at SUERC, where the argon-argon isotopic analyses of the alteration minerals in Lafayette took place,” Tremblay said.&nbsp;</p>



<p>Their partners at SUERC and the Natural History Museum have long contributed to studying Lafayette’s complex history.</p>



<h2 class="wp-block-heading" id="h-dating-minerals-in-meteorites">Dating minerals in meteorites</h2>



<p>Dating the water-altered minerals in Lafayette, and others in its class of Martian meteorites called nakhlites, has been a central focus in planetary science, as they uniquely capture moments when liquid water was present on Mars.&nbsp;</p>



<p>Due to complex alterations over time, previous attempts to date these minerals were plagued with uncertainties.&nbsp;</p>



<p>However, the team has now developed a robust dating method that could be applied to other meteorites, enhancing our understanding of when water might have been present on Mars and other planetary bodies.</p>



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



<p>Thanks to the Stahura Undergraduate Meteorite Fund, Tremblay and Ickert’s research on the Lafayette Meteorite will continue, with the involvement of undergraduate students in Purdue EAPS.&nbsp;</p>



<p>This opportunity allows students to engage in real-world planetary science, helping to reveal the intricate histories of meteoritic samples.</p>



<p>Tremblay and her team’s work on the Lafayette Meteorite highlights its scientific significance, revealing a complex history that ties it to Mars’ geological past.&nbsp;</p>



<p>Their findings not only deepen our understanding of Mars but also set a precedent for future studies that might unveil even more about the red planet’s climate history, water activity, and potential for supporting <a href="https://www.earth.com/news/some-mars-rocks-contain-signs-of-life-scientists-call-to-bring-them-back-to-earth/" target="_blank" rel="noreferrer noopener">life</a>.</p>



<p>-----</p>



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<p></p>

Meteorite found in an old desk shows Mars had water about 700 million years ago

An asteroid impact on Mars about 11 million years ago,...

<p>Have you ever wondered how your internet and browsing habits impact your mental health? The relationship between internet use and happiness, it turns out, isn't as simple as you might think. </p>



<p>For those crossing the 50-year mark, the internet could be a portal to a more contented life. However, for the younger crowd, losing themselves in the world of online activities might not be so rosy.</p>



<h2 class="wp-block-heading" id="h-mental-health-and-internet-use">Mental health and internet use</h2>



<p>An intriguing new study reveals that people over 50 who regularly navigate the <a href="https://www.earth.com/news/internet-addiction-impairs-brain-function-in-teenagers/" target="_blank" rel="noreferrer noopener">digital landscape</a> of emails, online shopping, or information seeking tend to feel happier and less blue. Eugenia Cheng of the <a href="https://www.hku.hk" target="_blank" rel="noreferrer noopener">University of Hong Kong</a> led the team behind this research.</p>



<p>The experts classified 87,000 people aged 50 and older from 23 countries into four groups based on their internet usage: non-users, sporadic users (those using the internet less than once a week), weekly users, and daily users.</p>



<p>Over six years, these "silver surfers" painted a picture showing that more internet use correlated with more life satisfaction and improved health.</p>



<h2 class="wp-block-heading" id="h-dark-side-of-the-internet">Dark side of the internet</h2>



<p>Before anyone decides to glue themselves to their screens, it's important to remember that the internet can be a source of poor mental health and distress for our younger counterparts.</p>



<p>Earlier research suggested that <a href="https://www.earth.com/news/the-shocking-reality-of-website-emissions/" target="_blank" rel="noreferrer noopener">internet</a> use among those under 50 could exacerbate anxiety, self-esteem issues, eating disorders, and exposure to online harassment.</p>



<h2 class="wp-block-heading" id="h-geography-and-age">Geography and age</h2>



<p>Turning to England, the researchers discovered that only daily <a href="https://www.earth.com/news/study-the-internet-is-not-bad-for-your-mental-health/" target="_blank" rel="noreferrer noopener">internet</a> users reported fewer depressive symptoms compared to the other groups.</p>



<p>The difference in happiness seems more pronounced for those aged 65 and above - especially for those who were unmarried, physically inactive, and not as financially comfortable.</p>



<h2 class="wp-block-heading" id="h-sociability-and-support">Sociability and support</h2>



<p>Cheng's team believes that for those aged 50 and above, the internet could promote social interaction and help combat loneliness.</p>



<p>Beyond the social aspect, it lends a helping hand in accessing valuable information and services that offer emotional support and medical advice. But while the internet may be a tool for boosting mental health, it's not without its perils.</p>



<h2 class="wp-block-heading" id="h-internet-and-mental-health-connection">Internet and mental health connection</h2>



<p>Remember that old saying about having too much of a good thing? It perfectly applies to the internet, especially for older populations. </p>



<p>Excessive internet use could cut into time for sleep, physical activity, and face-to-face socializing - the very factors important for good mental health. Moreover, there's the tricky business of <a href="https://www.earth.com/news/internet-addiction-impairs-brain-function-in-teenagers/" target="_blank" rel="noreferrer noopener">online</a> fraud and misinformation. </p>



<h2 class="wp-block-heading" id="h-internet-boosts-mental-health">Internet boosts mental health</h2>



<p>According to the researchers, their study highlights the potential of internet use as an effective strategy to bolster overall mental health in middle-aged and older populations.</p>



<p>After all, the internet serves as a lifeline for people in their twilight years, allowing them to access health-related information, build social connections, and find entertainment - all contributing positively to their mental health.</p>



<h2 class="wp-block-heading" id="h-little-internet-goes-a-long-way">Little internet goes a long way</h2>



<p>Let's not forget another noteworthy finding. "Silver surfers" who keep using the internet cut their risk of developing dementia in half compared to their less digital savvy peers.</p>



<p>"Online engagement may help to develop and maintain cognitive reserve, which can in turn compensate for brain aging and reduce the risk of dementia," explained Dr. Virginia Chang, a professor at NYU School of Global Public Health.</p>



<h2 class="wp-block-heading" id="h-informed-decisions-about-our-digital-habits">Informed decisions about our digital habits</h2>



<p>The internet, like many things in life, can be a boon or a bane for mental health, depending on how we use it and, interestingly, how old we are. </p>



<p>While older adults surf their way towards a healthier and happier life, our younger generations might need to tread the online waters more carefully. Either way, it seems clear that the world wide web continues to weave its complex threads into the fabric of our lives.</p>



<p>Within this digital maze we <a href="https://www.earth.com/news/your-brain-literally-changes-based-on-daily-activities-and-lifestyle/" target="_blank" rel="noreferrer noopener">navigate</a> daily, let's continue to explore and learn the best ways to use it for our advantage.</p>



<p>As our lives become increasingly entwined with technology, studies like these offer valuable insights. They help us to question, reflect, and make informed decisions about our digital habits. In what ways can we all strike a balance in our internet use to improve our quality of life?</p>



<p>-----</p>



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Mental health and the internet: Who benefits and who suffers?

Have you ever wondered how your internet and browsing habits...

<p>The Northern Lights have been visible much farther south than usual this year, filing social media with stunning images of colorful skies. Now, imagine an aurora so intense that it would instantly render smartphones useless as particles from the sun overwhelm electronic devices.&nbsp;</p>



<p>Such <a href="https://www.earth.com/news/ancient-tree-rings-help-predict-extreme-solar-storms/" target="_blank" rel="noreferrer noopener">extreme solar storms</a> are incredibly rare - only six have left their traces on Earth in the past 14,500 years, and none have been observed since the height of the Assyrian Empire nearly 2,700 years ago.</p>



<h2 class="wp-block-heading" id="h-a-cosmic-event-from-664-b-c">A cosmic event from 664 B.C.</h2>



<p>A research team led by Irina Panyushkina of the <a href="https://www.arizona.edu/" target="_blank" rel="noreferrer noopener">University of Arizona</a>'s Laboratory for Tree-Ring Research and Timothy Jull from the Department of Geosciences has identified the last time Earth experienced such a powerful burst of cosmic radiation.&nbsp;</p>



<p>Their findings, published in the journal <a href="http://dx.doi.org/10.1038/s43247-024-01618-x" target="_blank" rel="noreferrer noopener"><em>Communications Earth &amp; Environment</em></a>, reveal a spike in carbon-14 dating to the year 664 B.C., pinpointing the timing of this elusive extreme solar storm.</p>



<h2 class="wp-block-heading" id="h-what-are-solar-storms">What are solar storms?</h2>



<p>Solar storms occur when the Sun releases massive amounts of energy in the form of solar flares or coronal mass ejections (CMEs). These events send high-energy particles and magnetic fields hurtling toward Earth at incredible speeds.</p>



<p>When these charged particles interact with Earth's magnetic field, they can create dramatic and far-reaching effects.</p>



<h2 class="wp-block-heading" id="h-tracing-solar-storms-through-carbon-14">Tracing solar storms through carbon-14</h2>



<p>“After a few months, carbon-14 will have traveled from the stratosphere to the lower atmosphere, where it is taken up by trees and becomes part of the wood as they grow,” Panyushkina said.&nbsp;</p>



<p>By analyzing <a href="https://www.earth.com/news/earths-largest-ever-solar-storm-discovered-through-tree-rings/" target="_blank" rel="noreferrer noopener">tree rings</a> for carbon-14, a naturally occurring radioactive variant of carbon, the team detected this ancient solar storm.&nbsp;</p>



<p>Determining the precise timing of such massive solar eruptions provides important data for scientists who study and develop models of the sun's activity over time.</p>



<h2 class="wp-block-heading" id="h-signature-of-extreme-solar-storms">Signature of extreme solar storms</h2>



<p>It wasn't until 2012 that scientists recognized extreme solar storms known as Miyake events. </p>



<p>That year, Fusa Miyake, a Japanese physicist and collaborator with Panyushkina's team, published a paper reporting the storms' telltale signature: spikes in radioactive carbon isotopes in the growth rings of trees. </p>



<p>Miyake events occur when the sun's electromagnetic field weakens, allowing plasma from the sun's surface to escape into space.&nbsp;</p>



<p>Increased <a href="https://www.earth.com/news/sunspot-sketches-from-1607-unlock-secrets-of-solar-activity/" target="_blank" rel="noreferrer noopener">solar activity</a> leads to protons bombarding Earth's atmosphere, triggering chemical reactions that result in spikes of radioactive isotopes.</p>



<p>“Thanks to radiocarbon in tree-rings, we now know that six Miyake events happened over the last 14,500 years,” Panyushkina said. “If they happened today, they would have cataclysmic effects on communication technology.”</p>



<h2 class="wp-block-heading" id="h-methodology-tree-rings-and-ice-cores">Methodology: Tree rings and ice cores</h2>



<p>The research team used surgical knives to dissect individual tree rings from ancient wood samples, including those from dead trees buried in riverbanks and timbers excavated during archaeological digs.&nbsp;</p>



<p>Next, the researchers burned the cellulose - the main component of wood - to determine the radiocarbon content.&nbsp;</p>



<p>To confirm whether solar storms caused the radiocarbon spikes, the researchers compared their tree ring data to spikes found in a different isotope, beryllium-10, locked in <a href="https://www.earth.com/news/ice-cores-from-highest-tropical-peak-reveal-new-climate-clues/" target="_blank" rel="noreferrer noopener">ice cores</a> from glaciers and ice sheets.&nbsp;</p>



<p>Like carbon-14, beryllium-10 forms in the atmosphere due to solar particles and becomes trapped in ice through rain and snow.</p>



<p>“If ice cores from both the North Pole and South Pole show a spike in the isotope beryllium-10 for a particular year corresponding to increased radiocarbon in tree rings, we know there was a solar storm,” Panyushkina said.</p>



<h2 class="wp-block-heading" id="h-can-we-predict-extreme-solar-storms">Can we predict extreme solar storms?</h2>



<p>Although tree rings act as “archivists” recording Miyake events, researchers have not yet found evidence of a pattern in these occurrences.&nbsp;</p>



<p>According to Panyushkina, tree rings give us an idea of the magnitude of these massive storms, but we can't detect any type of pattern, so it is unlikely we will ever be able to predict when such an event is going to happen.</p>



<p>“Still, we believe our paper will transform how we search and understand the carbon-14 spike signal of extreme solar proton events in tree rings,” said Panyushkina.</p>



<p>“The energy from this type of event not only changes the atmosphere's radiocarbon content but also the atmosphere's chemistry. We are trying to figure out how those short-lived and powerful events affect the Earth system as a whole.”</p>



<p>Image Credit: NASA/SDO and the AIA, EVE, and HMI science teams</p>



<p>-----</p>



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Trees hold evidence of one of Earth's most extreme solar storms

The Northern Lights have been visible much farther south than...

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<p><span style="font-weight: 400;">Why is chocolate so bad for dogs? Today’s </span><b>Video of the Day</b><span style="font-weight: 400;"> comes from the </span><a href="https://www.acs.org/"><span style="font-weight: 400;">American Chemical Society’s</span></a> <i><span style="font-weight: 400;">Reactions</span></i><span style="font-weight: 400;"> series and answers the question: why is chocolate so bad for <a href="https://www.earth.com/news/dogs-sniffing-cancer-cells/">dogs</a>?</span></p>
<p><span style="font-weight: 400;">Actually, it’s the molecule theobromine that’s found in chocolate that is toxic to dogs. Dogs have a very hard time metabolizing theobromine, as it attacks their central nervous system. Warning signs of theobromine poisoning include high temperature, diarrhea, seizures, vomiting and rapid breathing.</span></p>
<p><span style="font-weight: 400;">Different types of chocolate contain differing levels of theobromine. Milk chocolate typically only has 60 mg per 1 oz, but dark chocolate has 400 mg per 1 oz.  </span></p>
<p><span style="font-weight: 400;">Chocolate is poisonous to dogs mostly because of its theobromine content, which dogs are unable to metabolize effectively. Find out which foods that can be toxic and poisonous to cats and dogs. Discover the people foods that can be extremely poisonous if eaten by cats and dogs. Chocolate is bad for dogs because it contains theobromine and caffeine. Theobromine and caffeine is dangerous because of how slowly it breaks down in dogs bodies.</span></p>
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<p><span style="font-weight: 400;">&#8212;</span></p>
<p><i><span style="font-weight: 400;">By </span></i><a href="mailto:rarnold@earth.com"><i><span style="font-weight: 400;">Rory Arnold</span></i></a><i><span style="font-weight: 400;">, </span></i><a href="https://www.earth.com/staff"><i><span style="font-weight: 400;">Earth.com</span></i></a></p>
<p><i><span style="font-weight: 400;">Source: </span></i><a href="https://www.youtube.com/watch?v=X86co4E1NvE&amp;index=25&amp;list=PLtLT74crQcwXo6laaF7C0DUkaa974KRkR"><i><span style="font-weight: 400;">American Chemical Society</span></i></a></p>


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