<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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Young, massive stars in the Triangulum Galaxy

<p>Uranus has long captivated scientists with its mysteries, particularly those that remain hidden within our solar system. </p>



<p>Decades-old data from Voyager 2, a NASA spacecraft, has now breathed new life into our understanding of this distant, enigmatic planet, settling age-old questions that have puzzled researchers for years.</p>



<h2 class="wp-block-heading" id="h-basics-of-planet-uranus">Basics of planet Uranus</h2>



<p>Uranus is the seventh planet from the Sun, and it has this wild tilt -- it's basically spinning on its side with an axis tilt of about 98 degrees. </p>



<p>This unique tilt leads to some extreme seasons that last over 20 Earth years each. The planet's blue-green hue comes from methane in its atmosphere, which absorbs red light and reflects blue, giving it that cool color.</p>



<p>Uranus has a set of rings and 27 known moons, most of which are named after characters from Shakespeare's plays. While its rings aren't as flashy as Saturn's, they're still pretty interesting.</p>



<p> And talk about cold -- Uranus has the coldest planetary atmosphere in the solar system, dipping down to -224 degrees Celsius (-371 Fahrenheit). </p>



<p>Finally, it takes about 84 Earth years to complete one orbit around the Sun, so a single year on Uranus is basically a lifetime for the average human.</p>



<h2 class="wp-block-heading" id="h-voyager-2-meets-uranus">Voyager 2 meets Uranus</h2>



<p>In 1986, Voyager 2 embarked on a momentous journey that brought it into close proximity with Uranus, providing the first -- and so far, only -- detailed examination of this unique, sideways-rotating planet.</p>



<p>This flyby not only unveiled new moons and rings but also introduced perplexing enigmas that challenged the scientific community. </p>



<p>Solving these mysteries and understanding their broader implications is akin to piecing together a cosmic puzzle.</p>



<h2 class="wp-block-heading" id="h-unexplained-oddities-of-uranus">Unexplained oddities of Uranus</h2>



<p>The presence of energized particles around Uranus was a conundrum. Here was a planet, rotating on its side and challenging the established understanding of how <a href="https://www.earth.com/news/milky-way-galaxy-is-surrounded-by-massive-magnetic-fields/" target="_blank" rel="noreferrer noopener">magnetic fields</a> trap particle radiation. </p>



<p>Uranus, known for its unusual properties, was once again surprising the experts.</p>



<p>Scientists re-analyzed data from the notable flyby a few decades ago and, in an exciting twist, identified that an unexpected, cosmic occurrence had thrown this distant planet a curveball.</p>



<p>The experts discovered that, just before the spacecraft’s flyby, <a href="https://www.earth.com/news/space-weather-poses-significant-risks-to-railway-safety/" target="_blank" rel="noreferrer noopener">space weather</a> had peculiarly squashed the planet’s magnetic field, leading to a dramatic compression of Uranus' magnetosphere.</p>



<h2 class="wp-block-heading" id="h-the-importance-of-timing">The importance of timing</h2>



<p>“The spacecraft saw Uranus in conditions that only occur about 4% of the time,” stated Jamie Jasinski, a scientist based at <a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA’s Jet Propulsion Laboratory</a> in Southern California and the lead author of a new study published in <a href="https://www.nature.com/articles/s41550-024-02389-3"><em>Nature Astronomy</em></a>.</p>



<p>Imagine the odds. Had Voyager 2 arrived just a few days earlier, it would have recorded a completely different magnetosphere around Uranus.</p>



<h2 class="wp-block-heading" id="h-mysteries-of-the-magnetosphere">Mysteries of the magnetosphere</h2>



<p>Earth's <a href="https://www.earth.com/news/mysterious-solar-shockwave-has-cracked-earths-magnetosphere/" target="_blank" rel="noreferrer noopener">magnetosphere</a> plays a crucial role in maintaining life on our planet by protecting us from the ionized gas jets that the Sun releases.</p>



<p>Comprehending how magnetospheres operate carries immense significance not just for us, but for understanding the distant, less-explored planets in our solar system.</p>



<p>In their quest to understand Uranus' magnetosphere, scientists were confused by what they witnessed in the <a href="https://www.earth.com/news/nasa-lost-contact-with-voyager-2-spacecraft-12-billion-miles-away/" target="_blank" rel="noreferrer noopener">Voyager 2</a> data. </p>



<p>Despite a marked absence of plasma, the planet's magnetosphere boasted electron radiation belts with an intensity second only to the notorious radiation belts of Jupiter. </p>



<p>This posed an enigma, as the Uranian moons, which should have been a significant source of water ions, were believed to be inactive.</p>



<h2 class="wp-block-heading" id="h-unexpected-solar-wind-event">Unexpected solar wind event</h2>



<p>The latest data analysis suggests that the solar wind, a flow of charged particles released from the Sun's upper atmosphere, could be the key to solving this puzzle.</p>



<p>It is possible that, as the solar wind compressed the planet's magnetosphere, it also drove the plasma out of the system.</p>



<p>The intensity of the solar wind event could have increased the magnetosphere's dynamics, thereby providing a source for the radiation belts.</p>



<p>This discovery has led researchers to speculate that the five major moons of Uranus might be geologically active, contradicting previous beliefs. </p>



<p>They suggest that these moons could have been continually spewing ions into the surrounding magnetosphere.</p>



<h2 class="wp-block-heading" id="h-renewed-focus-on-uranus-and-future-exploration">Renewed focus on Uranus and future exploration</h2>



<p>The National Academies’ 2023 Planetary Science and Astrobiology Decadal Survey has highlighted the study of Uranus as a key objective for future NASA missions.</p>



<p>Linda Spilker from the JPL, who was involved in the Voyager 2 mission, elaborated on the findings.</p>



<p>“The flyby was packed with surprises, and we were searching for an explanation of its unusual behavior. The magnetosphere Voyager 2 measured was only a snapshot in time," said Spilker.</p>



<p>"This new work explains some of the apparent contradictions and will once again change our view of Uranus." </p>



<h2 class="wp-block-heading" id="h-the-legacy-of-voyager-2">The legacy of Voyager 2</h2>



<p>Despite being billions of miles away, Voyager 2 continues to communicate with Earth using NASA's Deep Space Network, specifically via the antenna in Canberra, Australia. </p>



<p>It is still operational, collecting data on the interstellar medium and is expected to continue transmitting data until at least 2025​​​​​​.</p>



<p>Decades after it was launched, Voyager 2 continues to serve as a cornerstone for scientific discovery, offering invaluable insights into the mysteries of our solar system.</p>



<p>The study is published in the journal <em><a href="https://www.nature.com/articles/s41550-024-02389-3" target="_blank" rel="noreferrer noopener">Nature Astronomy</a></em>.</p>



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



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<p></p>

Uranus mystery finally solved almost 40 years after flyby from Voyager 2 spacecraft

Uranus has long captivated scientists with its mysteries, particularly those...

<p>We all know that the winds bring in rain, but have you ever heard of them bringing in microbes? In a significant scientific discovery, a team of atmospheric, health, and climate specialists from Spain and Japan have found a diverse range of fungi, bacteria, and viruses riding on the winds high up in Earth's atmosphere.</p>



<p>By collecting and testing air samples from 1,000 to 3,000 meters up in the sky, these researchers have assessed the possibility of these microorganisms surviving in extreme atmospheric conditions and hitching a ride on winds across continents.</p>



<h2 class="wp-block-heading" id="h-journey-of-winds-dust-and-microbes">Journey of winds, dust and microbes</h2>



<p>Dust, as we know, isn't a homebody. It loves to travel. Scientists have known for a while that dust can journey thousands of miles in the atmosphere. </p>



<p>Dust from Africa finds its way to both North and South America. But what's new and even more intriguing is the fuller picture of what this <a href="https://www.earth.com/news/microbes-laid-the-foundation-for-early-life-on-earth/" target="_blank" rel="noreferrer noopener">dust</a> carries with it.</p>



<h2 class="wp-block-heading" id="h-inside-the-airborne-microbial-world">Inside the airborne microbial world</h2>



<p>Researchers took to the skies over Japan in a small charter plane to collect wind samples, hoping to discover the heights at which <a href="https://www.earth.com/news/microbes-have-emerged-as-major-source-of-methane-emissions/" target="_blank" rel="noreferrer noopener">microbes</a> could survive.</p>



<p>The samples were then brought down to Earth for some lab-based sleuthing. A detailed DNA analysis of the samples revealed that these high-altitude hitchhikers were quite diverse, including a range of fungi, bacteria, and viruses.</p>



<p>And the little creatures weren't just surviving; they were thriving. In lab dishes, many of the microbes were still viable, which means that they could reproduce and continue to grow.</p>



<p>In total, the air samples contained 266 different types of fungi and 305 types of bacteria. Many of these microorganisms are commonly found in soil or plants, which clearly indicates their likely origins.</p>



<h2 class="wp-block-heading" id="h-atmospheric-pathways-the-invisible-highways">Atmospheric pathways: The invisible highways</h2>



<p>Now, where did these microbes come from? The researchers believe that most of them came from China, which means they had traveled at least 2,000 kilometers.</p>



<p>The high-altitude winds, it seems, can carry these microbes over significant distances.</p>



<p>This has fascinating implications because, if microorganisms can travel thousands of kilometers and survive high up in the atmosphere, they could potentially spread diseases worldwide. This is exactly what the current research proposes.</p>



<h2 class="wp-block-heading" id="h-pathogens-high-in-the-sky">Pathogens high in the sky</h2>



<p>The thought of airborne pathogens crossing continents is quite unsettling. While we knew that winds and dust particles could carry microbes over long distances, this study takes things up a notch.</p>



<p>The researchers found many airborne microbes that are known to inhabit the human body, particularly in the mouth and intestines.</p>



<p>While they caution that this doesn't necessarily prove a direct link between these microbes and health effects, it does open up the possibility of a new route for disease transmission.</p>



<p>Intriguingly, some of these sky-high microbes could be linked to soil or plants, suggesting that they might have been swept up into the atmosphere from land sources. Does this mean that poor sewage or waste disposal could supply pathogens for such a skyward journey?</p>



<h2 class="wp-block-heading" id="h-blowing-microbes-in-the-wind">Blowing microbes in the wind</h2>



<p>The study shows that microbes can be lifted by pressure systems, such as the Siberian High, and transported from agricultural regions in northeast China to other parts of the world. This also highlights the potential for insects to spread over large areas through these atmospheric conveyer belts.</p>



<p>But it's not just about human health. Think about the potential impact on ecosystems worldwide. Pathogens that are known to us, like <em>E. coli</em> and various <em>Staphylococcus</em> species, could be floating up there in the sky, ready to descend on unsuspecting habitats.</p>



<p>So where do we go from here?</p>



<h2 class="wp-block-heading" id="h-future-directions-on-wind-and-microbes">Future directions on wind and microbes</h2>



<p>Understanding how these <a href="https://www.earth.com/news/humans-are-walking-ecosystems-and-microbes-rule-their-evolution/">microorganisms</a> endure and prosper in such harsh conditions could help scientists develop better strategies for mitigating disease spread.</p>



<p>There's a whole new field of research now focusing on the upper atmosphere and how it might harbor and transport microbes across different regions and seasons.</p>



<p>"This study confirms the long-distance transport of microbial pathogens, which has important implications for public health, and environmental protection," said study co-author Xavier Rodó.</p>



<p>So, the next time you look up at the sky, just remember - there is more up there than meets the eye. And while this reality might seem a little unsettling, it also represents a vast new field of scientific discovery.</p>



<p>The study is published in the journal <em><a href="https://www.pnas.org/doi/10.1073/pnas.2404191121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a></em>.</p>



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



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Microbes hitch rides on winds across continents

We all know that the winds bring in rain, but...

Front,View,Of,The,Terminus,Of,Hisinger,Glacier,,Dickson,Fiord,

<p>Tsunamis are powerful natural phenomena capable of reshaping entire coastlines. Modern technology is now capable of helping scientists to study them in remarkable detail.  </p>



<p>The ability to monitor and analyze these massive waves in real-time has revolutionized our understanding of their behavior and impact, providing invaluable data that can inform safety protocols and predictive models.</p>



<p>This technological prowess recently helped unravel the nine-day-old reverberations of a tsunami in Greenland, a rare and complex event captured by the International SWOT Satellite. </p>



<p>The satellite's advanced imaging capabilities revealed unprecedented insights into how the tsunami waves moved and persisted within the steep walls of Dickson Fjord, thereby contributing significantly to the field of oceanography.</p>



<h2 class="wp-block-heading" id="h-first-things-first-what-s-a-tsunami">First things first -- what's a tsunami?</h2>



<p>Tsunamis are a massive series of ocean waves that can cause a whole lot of trouble when they hit land. </p>



<p>These waves aren't like the regular ones you surf on -- they're much bigger and can travel very fast across the ocean. </p>



<p>When they reach the shore, they can flood coastal areas and cause serious damage.</p>



<p>Now, what causes tsunamis? Well, they're usually triggered by underwater disturbances like earthquakes, volcanic eruptions, or even landslides. </p>



<p>When the ocean floor suddenly moves, it displaces a huge amount of water, and that energy creates waves that spread out in all directions. Essentially, it's the sudden movement under the sea that sets off these giant waves.</p>



<h2 class="wp-block-heading" id="h-swot-satellite-tsunami-discovery">SWOT satellite tsunami discovery</h2>



<p>At the core of this investigation were scientists from <a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA’s Jet Propulsion Laboratory</a> in Southern California and France’s CNES (Centre National d’Etudes Spatiales).</p>



<p>These dedicated professionals collaborated on the international Surface Water and Ocean Topography (SWOT) satellite mission. </p>



<p>Their joint efforts led to the discovery of unique shapes formed by tsunamis trapped within the steep walls of Greenland's Dickson Fjord.</p>



<h2 class="wp-block-heading" id="h-a-picture-paints-a-thousand-words">A picture paints a thousand words</h2>



<p>On September 17, 2023, the day following a massive rockslide, the <a href="https://www.earth.com/video/nasa-launches-revolutionary-satellite-to-monitor-earths-water/" target="_blank" rel="noreferrer noopener">SWOT satellite</a> was at the right place at the right time, collecting water elevation measurements in the Dickson Fjord. </p>



<p>By comparing these measurements with those recorded a few weeks prior, the scientists got a clear image of the aftermath of the tsunami.</p>



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/11/greenland-tsunami_SWOT-satellite_NASA_1m.webp" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/greenland-tsunami_SWOT-satellite_NASA_1s.webp" alt="A SWOT data visualization shows water on the northern side of Greenland’s Dickson Fjord at higher levels than on the southern side on Sept. 17, 2023. A huge rockslide into the fjord the previous day led to a tsunami lasting nine days that caused seismic rumbling around the world. Credit: NASA Earth Observatory" class="wp-image-1950872"/></a><figcaption class="wp-element-caption"><em>A SWOT data visualization shows water on the northern side of Greenland’s Dickson Fjord at higher levels than on the southern side on Sept. 17, 2023. A huge rockslide into the fjord the previous day led to a tsunami lasting nine days that caused seismic rumbling around the world. Credit: NASA Earth Observatory</em></figcaption></figure>



<p>The SWOT satellite captured a colored data visualization, indicating higher water levels with lighter colors and lower levels with darker tones. </p>



<p>The findings suggested that the northern side of the fjord reached certain points where water levels were almost 4 feet (1.2 meters) higher than on the southern side.</p>



<h2 class="wp-block-heading" id="h-milestone-in-the-field-of-research">Milestone in the field of research</h2>



<p>Astoundingly, this was the first instance where the SWOT satellite had the opportunity to examine the shape of a <a href="https://www.earth.com/news/tsunami-wave-from-tonga-eruption-was-90-meters-tall/" target="_blank" rel="noreferrer noopener">tsunami wave</a>. </p>



<p>“SWOT happened to fly over at a time when the water had piled up pretty high against the north wall of the fjord,” said Josh Willis, a sea level researcher at NASA’s Jet Propulsion Laboratory in Southern California. </p>



<p>“Seeing the shape of the wave - that’s something we could never do before SWOT."</p>



<h2 class="wp-block-heading" id="h-tracing-the-origins-of-the-tsunami">Tracing the origins of the tsunami</h2>



<p>A paper published recently in <em>Science</em> traced the <a href="https://www.earth.com/news/new-map-shows-75-percent-of-the-u-s-at-risk-of-damaging-earthquakes/" target="_blank" rel="noreferrer noopener">seismic</a> signals of the tsunami back to its roots.</p>



<p>More than 880 million cubic feet of rock and ice, equivalent to 25 million cubic meters, had plummeted into Dickson Fjord, triggering the tsunami that sloshed around within the fjord.</p>



<p>The fjord is a part of a network of channels on Greenland's eastern coast, with the depth of about 1,772 feet (540 meters) and width of 1.7 miles (2.7 kilometers), while its walls tower over 6,000 feet (1,830 meters) high.</p>



<p>Interestingly, because the fjord is far from the open ocean and confined, the energy from the tsunami's motion had limited opportunities to dissipate. </p>



<p>This resulted in the wave moving back and forth approximately every 90 seconds for a surprising duration of nine days.</p>



<p>These findings demonstrate how modern technology can help us unravel nature’s mysteries. The international SWOT satellite, through its unique capabilities, has managed to provide us with a fresh  understanding of tsunamis and their prolonged effects.</p>



<h2 class="wp-block-heading" id="h-satellite-technology-and-monitoring-tsunamis">Satellite technology and monitoring tsunamis</h2>



<p>The SWOT satellite's ability to capture and analyze detailed water elevation data showcases the immense potential of satellite technology in monitoring <a href="https://www.earth.com/news/natural-disasters-are-on-the-rise-but-hazard-plans-are-inadequate/" target="_blank" rel="noreferrer noopener">natural disasters</a>.</p>



<p>Unlike traditional, on-ground sensors, satellites offer a comprehensive view of remote locations, like Greenland’s fjords. This capability is crucial for capturing disaster impacts and building predictive models for better preparedness.</p>



<p>The September 2023 event in Dickson Fjord demonstrated how satellite imaging has evolved to reveal the movement of tsunami waves over nine days, offering insights that were previously unattainable.</p>



<p>Such data enhance our understanding of energy dynamics within confined areas, informing disaster response and risk mitigation efforts.</p>



<p>Beyond <a href="https://www.earth.com/news/machine-learning-may-help-with-earlier-tsunami-detection/" target="_blank" rel="noreferrer noopener">tsunami monitoring</a>, satellites like SWOT play a vital role in observing storm surges, flooding, and sea-level rise. </p>



<p>Integrating satellite data with real-time analytics paves the way for quicker, more effective responses to natural disasters, thereby contributing to safer and more resilient communities.</p>



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NASA records a 650-foot tsunami in Greenland that shook the Earth for 9 days

Tsunamis are powerful natural phenomena capable of reshaping entire coastlines....

<p></p>
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<p><br />
<span style="font-weight: 400;">Today&#8217;s </span><b>Video of the Day </b><span style="font-weight: 400;">from the </span><a href="https://www.esa.int/"><span style="font-weight: 400;">European Space Agency</span></a><span style="font-weight: 400;"> features Sardinia, a large Italian island in the Mediterranean Sea.</span></p>
<p><span style="font-weight: 400;">The island is located west of the Italian Peninsula, north of Tunisia, and just south of the French island of Corsica.</span></p>
<p><span style="font-weight: 400;">The false-color image of Sardinia was processed using the shortwave infrared band and the near infrared band to highlight crops and vegetation, which appear in bright green. </span></p>
<p><span style="font-weight: 400;">Sardinia is a predominantly mountainous region that has over 1,800 kilometers of coastline along the Emerald Coast, or Costa Smeralda, Alghero, and Villasimius.</span></p>
<p><span style="font-weight: 400;">V</span><i><span style="font-weight: 400;">ideo Credit: ESA</span></i></p>
<p><span style="font-weight: 400;">&#8211;</span><span style="font-weight: 400;">&#8212;</span></p>
<p><i><span style="font-weight: 400;">By </span></i><a href="http://csexton@earth.com"><i><span style="font-weight: 400;">Chrissy Sexton</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><i><span style="font-weight: 400;"> Staff Writer</span></i></p>

The island of Sardinia in the Mediterranean Sea