Today's Image of the Day from the European Space Agency features the Southern Ring Nebula, also known as NGC 3132.



The nebula is located about 2,000 light-years away from Earth in the constellation Vela. This remarkably detailed image was created using data from Webb’s Near-Infrared Camera (NIRCam).



The Southern Ring Nebula is one of the more famous examples of planetary nebulae. It is often studied for its beauty and valuable insights into the end stages of stellar evolution.



<h2 class="wp-block-heading" id="h-stars-power-the-southern-ring-nebula-nbsp">Stars power the Southern Ring Nebula&nbsp;</h2>



The <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a> is powered by two central stars in a binary system. The brighter star is actually a less massive companion. The fainter, dimmer star is the dying, hot central star that has shed its outer layers to form the nebula. 



The dimmer star is a white dwarf and is responsible for the ionization of the gas in the nebula, causing it to glow.



“The bright star at the center of NGC 3132, while prominent when viewed by NASA’s Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"A second star, barely visible at lower left along one of the bright star’s diffraction spikes, is the nebula’s source. It has ejected at least eight layers of gas and dust over thousands of years.” 



“But the bright central star visible here has helped ‘stir’ the pot, changing the shape of this planetary nebula’s highly intricate rings by creating turbulence." 



ESA explained that the pair of stars are locked in a tight orbit, which leads the dimmer star to spray ejected material in a range of directions as they orbit one another, resulting in these jagged rings.



<h2 class="wp-block-heading" id="h-key-characteristics-of-the-southern-ring-nebula-nbsp">Key characteristics of the Southern Ring Nebula&nbsp;</h2>



The Southern Ring Nebula displays a complex structure with multiple layers of gas and dust. 



The outer shells of the nebula consist of hydrogen and other elements that were ejected from the dying star in previous stages of its <a href="https://www.earth.com/news/young-stellar-objects-observing-the-early-lives-of-stars/" target="_blank" rel="noreferrer noopener">evolution</a>. These layers are illuminated by ultraviolet radiation from the central white dwarf.



<h3 class="wp-block-heading" id="h-coloration">Coloration</h3>



The colors seen in the Southern Ring Nebula come from the different gases present. For example, hydrogen emits red light, while oxygen emits blue-green light. 



These colors help astronomers study the composition and dynamics of the nebula.



<h3 class="wp-block-heading" id="h-size-and-shape">Size and shape</h3>



The nebula spans about half a light-year in diameter. Its intricate, symmetrical structure provides valuable insights into the late stages of <a href="https://www.earth.com/news/star-collapse-black-hole-instead-of-supernova-vanish-from-sky/" target="_blank" rel="noreferrer noopener">stellar evolution</a>, especially the processes involved in the shedding of outer layers by dying stars.



<h2 class="wp-block-heading" id="h-spotlights-from-the-bright-star">Spotlights from the bright star</h2>



ESA noted that hundreds of straight, brightly-lit lines pierce through the rings of gas and dust. “These ‘spotlights’ emanate from the bright star and stream through holes in the nebula like sunlight through gaps in a cloud."



“But not all of the starlight can escape. The density of the central region, set off in teal, is reflected by how transparent or opaque it is. Areas that are a deeper teal indicate that the gas and dust are denser - and light is unable to break free.”



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



According to ESA, this is not only a crisp image of a planetary nebula - it also shows us objects in the vast distances of space behind it. The transparent red sections of the nebula are filled with distant <a href="https://www.earth.com/news/galaxies-have-hearts-and-lungs-that-help-them-live-longer/" target="_blank" rel="noreferrer noopener">galaxies</a>.



“Look for the bright angled line at the upper left. It is not starlight - it is a faraway galaxy seen edge-on. Distant spirals, of many shapes and colors, also dot the scene. Those that are farthest away - or very dusty - are small and red,” said ESA.



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



Vela is a southern constellation that represents the sails of a ship. It was once part of a larger constellation called Argo Navis, which depicted the ship of the mythological hero Jason and the Argonauts. 



In the 18th century, Argo Navis was divided into three separate constellations: Vela (the sails), Carina (the keel), and Puppis (the stern).



Vela is notable for containing several interesting astronomical features. One of its most prominent stars is Gamma Velorum, also known as Suhail or Regor, which is a bright, massive star system consisting of multiple stars.&nbsp;



The constellation also hosts the Vela Supernova Remnant, the remains of a <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> explosion that occurred about 11,000 years ago. 



This remnant is associated with the Vela Pulsar, a neutron star that formed during the supernova explosion, which is one of the brightest pulsars in the sky.



Vela is best observed in the Southern Hemisphere, where it can be seen in the summer months. Its position along the Milky Way makes it a popular region for both amateur and professional astronomers to explore.



Image Credit: NASA, ESA, CSA, STScI



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Southern Ring Nebula in the constellation Vela 

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

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



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



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



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



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



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



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



<a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">Star formation</a> is a key process in the growth of galaxies, making these studies crucial for understanding galaxy evolution.



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Spiral galaxy NGC 6744 in the constellation Pavo

Today's Image of the Day from the European Space Agency features the Little Dumbbell Nebula, also known as Messier 76, located in the constellation Perseus 3,400 light-years away from Earth.



Astronomers captured this image of the Little Dumbbell Nebula to commemorate the 34th anniversary of the Hubble Space Telescope, a joint venture between NASA and the European Space Agency (<a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>).



The snapshot provides not only a breathtaking view but also deep insights into the life cycle of <a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">stars</a> and the dynamic processes within nebulae.



<h2 class="wp-block-heading" id="h-understanding-messier-76">Understanding Messier 76</h2>



Messier 76 is categorized as a planetary nebula - a term which refers to its round, planet-like appearance when viewed through early, low-power telescopes. 



However, the term is somewhat misleading as planetary nebulae have no connection to actual <a href="https://www.earth.com/news/nasa-finds-17-exoplanets-that-have-oceans-and-possibly-alien-life/" target="_blank" rel="noreferrer noopener">planets</a>. 



Instead, they represent an expansive shell of luminous gases expelled by a dying red giant star, which subsequently collapses into a dense, hot white dwarf. 



This transformation marks the late stages of stellar evolution for medium to low-mass stars.



<h2 class="wp-block-heading" id="h-structure-of-messier-76">Structure of Messier 76</h2>



The structure of Messier 76 is particularly notable. It includes a central ring, giving the appearance of a bar-like feature, with two distinct lobes emanating from either side. 



This formation is believed to be the result of materials ejected by the star during its red giant phase, possibly sculpted by interactions with a companion star. 



Although this binary companion is not visible in current Hubble images, its presence is inferred from the thick disk of dust and gas aligned with its orbital plane. 



The phenomenon of the companion star potentially being absorbed by the primary star, a process akin to stellar cannibalism, is a captivating aspect of the nebula's history.



<h2 class="wp-block-heading" id="h-the-dynamic-environment-of-the-nebula">The dynamic environment of the nebula</h2>



At the core of the nebula, the primary star, now collapsing into a <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/" target="_blank" rel="noreferrer noopener">white dwarf</a>, reaches extreme temperatures. This heat is estimated to be 120,000 degrees Celsius - about 24 times hotter than the surface of our Sun. 



This intensely hot remnant is visible as a small, bright point at the center of the nebula. Directly below this, another star can be seen; however, it is merely aligned with the nebula by chance and is not a part of it.



<h2 class="wp-block-heading" id="h-powerful-glow-of-messier-76">Powerful glow of Messier 76</h2>



The dynamics within Messier 76 are driven by powerful forces. The central disk seems to constrict the material, creating two lobes of gas escaping along the rotational axis of the star, perpendicular to the disk.&nbsp;



The lobes are propelled outward by a potent stellar wind, moving at a staggering two million miles per hour. This rapid movement is sufficient to travel the distance from Earth to the <a href="https://www.earth.com/news/timeless-mystery-solved-scientists-uncover-what-is-inside-the-moons-core/" target="_blank" rel="noreferrer noopener">Moon</a> in just over seven minutes.&nbsp;



The collision of the fast-moving gas with older, slower-moving material ejected during the star’s red giant phase results in the stunning glowing effect seen in the nebula. 



The glow, ignited by the ultraviolet radiation from the white dwarf, is a spectacle of colors with red emanating from nitrogen and blue from oxygen.



<h2 class="wp-block-heading" id="h-a-cosmic-moment-in-time">A cosmic moment in time</h2>



Despite its current brilliance, the existence of the Little Dumbbell Nebula is fleeting on a cosmological scale. It is expected to last only about 15,000 years - a mere moment in the lifespan of the <a href="https://www.earth.com/news/dark-energy-is-ripping-the-universe-apart-but-we-arent-sure-how/" target="_blank" rel="noreferrer noopener">universe</a>. 



This brief period highlights the transient nature of such cosmic phenomena, which, while short-lived, provide crucial insights into the mechanics of stellar evolution and the complex interactions within these celestial sculptures.



<h2 class="wp-block-heading" id="h-more-about-messier-76">More about Messier 76</h2>



Messier 76 was discovered by Pierre Méchain in 1780. It was later cataloged by Charles Messier, who included it in his famous list of nebulous objects.



The nebula's faintness and small size require a good telescope to be observed effectively, with larger telescopes able to reveal more of its fine details and structure.



Studying Messier 76 helps astronomers understand the life cycle of stars and the processes that occur during the late stages of stellar evolution. 



The materials expelled by planetary nebulae like Messier 76 eventually contribute to the interstellar medium, from which new stars and planetary systems may form.



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

Today's Image of the Day from the European Space Agency features the galaxy I Zwicky 18, which was captured in remarkable detail by the James Webb Space Telescope.



I Zwicky 18 is a blue compact dwarf <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">galaxy</a> located approximately 59 million light-years away in the constellation Ursa Major.&nbsp;



<h2 class="wp-block-heading" id="h-star-formation-in-i-zwicky-18">Star formation in I Zwicky 18</h2>



The galaxy is notable for its relatively young appearance and the fact that it contains very few heavy elements. These characteristics indicate that it has experienced little <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> compared to other galaxies of similar age.



“The galaxy was first identified by Swiss astronomer Fritz Zwicky in the 1930’s and resides roughly 59 million light-years from Earth,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>. “This galaxy has gone through several sudden bursts of star formation.”&nbsp;



According to ESA, I Zwicky 18 is typical of the kinds of galaxies that inhabited the early universe and is much smaller than our <a href="https://www.earth.com/news/runaway-star-j1249-36-spotted-trying-to-escape-our-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



<h2 class="wp-block-heading" id="h-webb-telescope-image-of-the-galaxy">Webb telescope image of the galaxy</h2>



“Two major starburst regions are embedded in the heart of the galaxy. The wispy brown filaments surrounding the central starburst region are bubbles of gas that have been heated by stellar winds and intense ultraviolet radiation unleashed by hot, young stars,” noted ESA.



“A companion galaxy resides nearby to the dwarf galaxy, which can be seen at the bottom of the wider-field image. The companion may be interacting with the dwarf galaxy and may have triggered that galaxy's recent star formation.”&nbsp;



ESA explained that the “orange blobs” surrounding the galaxy are the dim glow from ancient fully formed galaxies at much larger distances.



<h2 class="wp-block-heading" id="h-key-characteristics-of-i-zwicky-18">Key characteristics of I Zwicky 18</h2>



As previously mentioned, the galaxy has a very low abundance of elements heavier than hydrogen and helium, suggesting that it has not undergone significant stellar processing.



<h3 class="wp-block-heading" id="h-young-stellar-population-nbsp">Young stellar population&nbsp;</h3>



Despite its old age, I Zwicky 18 contains many young, hot stars. This suggests that it might have experienced a burst of <a href="https://www.earth.com/news/hubble-detects-awe-inspiring-newborn-star/" target="_blank" rel="noreferrer noopener">star formation</a> relatively recently in its history.



<h3 class="wp-block-heading" id="h-interstellar-medium-nbsp">Interstellar medium&nbsp;</h3>



The galaxy has a high density of gas, which is a prime ingredient for star formation. This gas is mostly in the form of hydrogen.



<h3 class="wp-block-heading" id="h-unusual-characteristics">Unusual characteristics</h3>



Its characteristics are more typical of primordial galaxies found in the early universe, making it a valuable object of study for understanding galaxy formation and evolution.



Ultimately, I Zwicky 18 provides insights into the conditions and processes that might have been prevalent in the early universe.



<h3 class="wp-block-heading" id="h-life-cycles-of-stars-and-dust">Life cycles of stars and dust</h3>



The image was captured as part of a Webb program to study the life cycle of dust in I Zw 18.&nbsp;



“Scientists are now building off of previous research with Hubble obtained at optical wavelengths, studying individual dusty stars in detail with Webb’s equivalent spatial resolution and sensitivity at infrared wavelengths.”&nbsp;



ESA noted that this galaxy is of particular interest as its content of elements heavier than helium is one of the lowest of all known <a href="https://www.earth.com/news/early-galaxy-formation-occurred-much-faster-than-we-thought/" target="_blank" rel="noreferrer noopener">galaxies</a> in the local universe.&nbsp;



“Such conditions are thought to be similar to those in some of the first star-forming galaxies at high redshift, so the Webb study of I Zw 18 should shed light on the life-cycle of stars and dust in the early universe.”



<h2 class="wp-block-heading" id="h-the-constellation-ursa-major">The constellation Ursa Major </h2>



Ursa Major, also known as the Great Bear, is one of the most prominent and easily recognizable constellations in the northern sky. 



Its name, "Ursa Major," means "Great Bear" in Latin, and it has been a significant part of various mythologies and star lore across cultures for thousands of years. 



One of the most famous asterisms within Ursa Major is the Big Dipper, a group of seven bright stars that form a shape resembling a ladle or dipper. The Big Dipper is often used as a navigation tool because it points to Polaris, the North Star, located in the nearby constellation Ursa Minor.



Ursa Major is best viewed in the northern hemisphere and is circumpolar, meaning it is visible year-round for much of the Northern Hemisphere. Its position changes with the seasons, rotating around Polaris, the North Star.



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



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Dwarf galaxy provides a window into the early universe

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



NGC 1333 is a vibrant example of a stellar nursery, where active <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> is ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



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



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



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



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



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



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



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



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



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



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



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



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



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Stellar nursery shines in the Perseus cloud

In a quiet and picturesque corner of southern Brazil known as Paraíso do Sul, an extraordinary treasure was uncovered -- a fossil so ancient and well-preserved that it may potentially rewrite the narrative of dinosaur evolution.



This remarkable fossil belonged to a dog-sized reptile named Gondwanax paraisensis that roamed the region approximately 237 million years ago. 



This was during the Triassic period -- a time when Earth’s ecosystems were teeming with evolutionary experiments.



As a newly identified species, this fossil holds tremendous potential as a key to unraveling the mysteries surrounding the origin and early development of the oldest dinosaurs.



Although this fascinating discovery has sparked significant intrigue and excitement among paleontologists, the exact position of the fossil in the complex evolutionary tree of life still remains a subject of debate and careful scientific scrutiny.



<h2 class="wp-block-heading" id="h-dinosaur-history-written-in-stone">Dinosaur history written in stone</h2>



In the realms of science, every fossil discovery is like a puzzle piece that can help us better understand our past. And when it comes to the world of paleontology, there are still many puzzles waiting to be solved.



Gondwanax paraisensis walked on four legs and was 39 inches in length, with a long tail. It belonged to an extinct group of <a href="https://www.earth.com/news/past-climate-change-drove-the-rapid-evolution-of-reptiles/" target="_blank" rel="noreferrer noopener">reptiles</a> known as silesaurids. These were not true dinosaurs, but are considered a closely related sister group to the dinosaurs. 



However, this newly discovered fossil is one of the oldest silesaurids found anywhere in the world, and it may lead scientists to challenge currently accepted theories about the lineage and early <a href="https://www.earth.com/news/dinosaurs-may-have-become-warm-blooded-180-million-years-ago/" target="_blank" rel="noreferrer noopener">evolution of dinosaurs</a>.



"The most important part of this finding is its age,” said Rodrigo Temp Müller, the sole author of the study and a paleontologist at <a href="https://www.ufsm.br/orgaos-de-apoio/sai/welcome-to-ufsm" target="_blank" rel="noreferrer noopener">Federal University of Santa Maria</a> in Brazil. “Because it's so old, it gives us clues as to how dinosaurs came to be."



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



There is an ongoing debate among paleontologists about where silesaurids fit in terms of dinosaur evolution. Were they actual dinosaurs or were they just closely related ancestors?



The answer to this question is not straightforward. Some scientists believe that silesaurids are a sister group to dinosaurs, implying that they share a common ancestor but evolved separately.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/11/Gondwanax-paraisensis_history-of-dinosaurs_illustration_credit-Gondwana-research_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/Gondwanax-paraisensis_history-of-dinosaurs_illustration_credit-Gondwana-research_1s.webp" alt="Illustration showing the evolution of dinosaurs on the Gondwana continent of ancient Earth. Credit: Gondwana research" class="wp-image-1950311"/></a><figcaption class="wp-element-caption">Illustration showing the evolution of dinosaurs on the Gondwana continent of ancient Earth. Credit: Gondwana research</figcaption></figure>



Others, however, hypothesize that some silesaurids may have evolved into ornithischians - <a href="https://www.earth.com/news/isle-of-wight-fossils-suggest-that-europe-had-unique-plant-eating-dinosaurs/" target="_blank" rel="noreferrer noopener">herbivorous dinosaurs</a>, such as the Stegosaurus and Triceratops, that possessed a bird-like pelvic structure.



Understanding silesaurids could potentially lead to a better understanding of what physical traits contributed to the success of early dinosaurs.



However, solving this puzzle has not been an easy task as many fossils of silesaurids are found incomplete or fragmented, making it difficult for scientists to reach consensus regarding the position of silesaurids in the evolutionary tree of dinosaurs. 



<h2 class="wp-block-heading" id="h-new-clues-about-the-history-of-dinosaurs">New clues about the history of dinosaurs </h2>



Physician Pedro Lucas Porcela Aurélio, who discovered the new fossil in 2014, was hit by an indescribable feeling. "Being the first human to touch something from 237 million years ago is extraordinary," he remarked.



When Aurélio handed over the fossil to the paleontologists in 2021, it was encased in hard rock with only the vertebrae visible. 



Surprisingly, Gondwanax was found to have three vertebrae in its hips, unlike its relatives who only had two. This difference suggested that this reptile may have been more dinosaur-like than previously assumed.



If this hypothesis is confirmed, it would not only extend the history of <a href="https://www.earth.com/news/how-did-bird-hipped-dinosaurs-evolve/" target="_blank" rel="noreferrer noopener">ornithischians</a> (bird-like dinosaurs) by up to ten million years, but it would also significantly alter our understanding of dinosaur origin.



<h2 class="wp-block-heading" id="h-the-quest-for-more-evidence-continues">The quest for more evidence continues</h2>



Despite the enthusiasm around the discovery, scientists still need more fossil evidence to confirm this theory. 



Steve Brusatte, a paleontologist from the University of Edinburgh, highlighted this need for further exploration. "I wish I could say that this new silesaurid fossil solves the riddle once and for all," he said. "But for me, it is still an open question."



In the upcoming chapters of this extraordinary journey of scientific exploration, we will be waiting eagerly for more pieces of this ancient puzzle to surface. 



Until then, the mystery of the dog-sized reptile continues to linger in our minds, reminding us that every stone turned may be a step closer to unravelling the <a href="https://www.earth.com/news/ancient-ocean-water-discovery-is-unlocking-secrets-of-earths-past/" target="_blank" rel="noreferrer noopener">secrets of the past</a>.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/abs/pii/S1342937X24002764">Gondwana Research</a>.



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Rare Triassic fossil discovery may rewrite the history of dinosaurs

In a quiet and picturesque corner of southern Brazil known...

Recent research highlights the link between air pollution and an increased risk of autism spectrum disorder (ASD) in children, particularly those with a genetic predisposition.&nbsp;



The study explores the role of nitric oxide (NO) and other pollutants in triggering complex biological responses that can impact neurodevelopment.



The research was led by Dr. Haitham Amal, head of the Laboratory of Neuromics, Cell Signaling, and Translational Medicine at the <a href="https://en.huji.ac.il/" target="_blank" rel="noreferrer noopener">Hebrew University</a> of Jerusalem.



“Meeting families and children with <a href="https://www.earth.com/news/autism-diagnoses-have-almost-tripled-in-the-us-over-the-past-ten-years/" target="_blank" rel="noreferrer noopener">autism</a> in Boston during my time at MIT inspired me to focus on a single goal: to help develop biological diagnostics and treatment for autism spectrum disorder,” Amal said.&nbsp;



This encounter shaped his career, leading him to investigate the ways environmental and genetic factors combine to influence ASD risk.



<h2 class="wp-block-heading" id="h-pollution-s-impact-on-neurodevelopment">Pollution’s impact on neurodevelopment</h2>



<a href="https://www.earth.com/news/understanding-how-air-pollution-forms-may-help-us-prevent-it/" target="_blank" rel="noreferrer noopener">Air pollution</a> contains several harmful elements, including particulate matter, nitrogen oxides, sulfur dioxide, and ozone. 



These pollutants, when inhaled, can bypass the blood-brain barrier, leading to inflammation and changes in neural functioning. 



The research emphasizes how particles such as PM2.5 - microscopic particles from sources like construction and car exhaust - and NO products can cross the placenta, directly impacting fetal brain development.&nbsp;



“My lab has shown that nitric oxide plays a major role in ASD,” Amal said, highlighting NO’s key role in brain health.



The review notes how urban areas with high pollution levels, such as Phoenix, San Jose, and Eugene, expose residents, particularly expectant mothers, to levels of pollution that may impact early childhood development.&nbsp;



A report from the <a href="https://www.lung.org/" target="_blank" rel="noreferrer noopener">American Lung Association</a> shows that 39 percent of the U.S. population lives in areas with concerning air quality, which, combined with genetic predispositions, could be a driving factor behind rising autism rates.



<h2 class="wp-block-heading" id="h-pollution-exposure-and-biological-pathways">Pollution exposure and biological pathways</h2>



The review presents evidence of several biological pathways that may link pollution exposure to increased autism risk.



<h3 class="wp-block-heading" id="h-nitrosative-stress-and-nitric-oxide">Nitrosative stress and nitric oxide</h3>



Nitrosative stress caused by NO has been shown to affect neurological development. This was one of Dr. Amal’s foundational discoveries.



<h3 class="wp-block-heading" id="h-neuroinflammation-and-oxidative-stress">Neuroinflammation and oxidative stress</h3>



Inhaled pollutants can prompt inflammation within the brain, which interferes with nerve development, potentially contributing to the behavioral symptoms associated with autism.



<h3 class="wp-block-heading" id="h-neurotransmitter-disruption">Neurotransmitter disruption</h3>



Pollutants may interrupt the balance of crucial brain chemicals like <a href="https://www.earth.com/news/dopamine-helps-us-learn-from-positive-and-negative-experiences/" target="_blank" rel="noreferrer noopener">dopamine</a> and norepinephrine, which play a role in decision-making and overall cognitive development.



The experts reviewed studies on both human and animal models to examine these biological effects, linking the presence of certain pollutants to changes in neural functioning. 



The findings show that pollutants, particularly NO, can cross the placenta and directly affect the fetus.&nbsp;



This sensitivity during prenatal and early childhood development stages, when the brain is rapidly growing, makes the body especially vulnerable to external factors.



<h2 class="wp-block-heading" id="h-convergence-of-genetics-and-environment">Convergence of genetics and environment</h2>



Autism has a strong genetic component, with estimates suggesting that 40-80% of cases may have a genetic basis. However, the scientists argue that genetics alone cannot explain the condition’s rising prevalence.&nbsp;



“The timing of exposure appears crucial, with heightened vulnerability during prenatal development and early childhood,” Amal explained.&nbsp;



The review suggests that while a genetic predisposition to autism can increase sensitivity to pollutants, environmental triggers -- especially air pollution -- may interact with genetics to further elevate autism risk.



A separate Harvard study showed that exposure to fine particulate matter early in life may increase the risk of autism by up to 64 percent, and prenatal exposure may elevate risk by 31 percent. 



This interaction between genes and environment presents a new model for understanding autism’s etiology.



<h2 class="wp-block-heading" id="h-early-interventions-for-at-risk-populations-nbsp">Early interventions for at-risk populations&nbsp;</h2>



As air quality deteriorates with urban expansion, there is an urgent need to assess pollution’s impact on vulnerable populations.&nbsp;



Amal’s findings suggest that governments may need to adjust urban planning and pollution monitoring to safeguard <a href="https://www.earth.com/news/prenatal-pollution-exposure-linked-to-cognitive-impairment/" target="_blank" rel="noreferrer noopener">prenatal</a> health.



The study also points to future research opportunities, particularly in developing biomarkers for early ASD detection.&nbsp;



By identifying specific indicators of pollution-related neurological stress, doctors may one day be able to screen infants and at-risk populations with greater accuracy.



“Different kinds of neurological disorders, including autism spectrum disorder, can be associated with this environmental factor,” Amal said.&nbsp;



His team is examining whether combining genetic and environmental data can improve diagnostics, which could enable earlier intervention for at-risk populations.



<h2 class="wp-block-heading" id="h-pollution-and-autism-prevalence">Pollution and autism prevalence </h2>



The study calls for extensive research to explore how various pollutants impact brain development.&nbsp;



“The research suggests that individuals with genetic predisposition to ASD may be more vulnerable to the harmful effects of air pollution exposure,” Amal said.&nbsp;



As ASD prevalence rises worldwide, this research may drive the development of preventive policies, such as targeted air quality monitoring in cities.



In addition, Amal’s work highlights the need for preventive strategies in communities facing heightened pollution levels.&nbsp;



His insights may prompt city planners, healthcare providers, and families to prioritize air quality improvements, especially in high-risk areas.



<h2 class="wp-block-heading" id="h-pollution-and-neurological-disorders">Pollution and neurological disorders</h2>



Amal’s pioneering work not only contributes to autism research but has implications for other neurological conditions.&nbsp;



The connections he draws between nitric oxide, ASD, and <a href="https://www.earth.com/news/alzheimers-disease-attacks-the-brain-in-two-separate-phases/" target="_blank" rel="noreferrer noopener">Alzheimer’s disease</a> suggest shared molecular pathways. By addressing NO-related neuroinflammation, treatments may eventually target multiple brain conditions.



The study ultimately underscores the power of interdisciplinary research in addressing complex conditions like autism.&nbsp;



As Amal concludes, his laboratory’s commitment to examining environmental factors alongside genetic predispositions could significantly impact the landscape of neurological disorder treatment, benefiting both current and future generations.



The study is published in the journal <a href="https://bm.genomicpress.com/wp-content/uploads/2024/11/BM0115-Amal-2024.pdf" target="_blank" rel="noreferrer noopener">Brain Medicine</a>.



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Air pollution discovered to be a "critical risk factor" for autism

Recent research highlights the link between air pollution and an...

Earworms - those persistent tunes that play in our heads unbidden - can be more than a minor annoyance.



Imagine going about your day when, without warning, a song loops repeatedly in your mind. 



While these spontaneous musical memories can feel intrusive, earworms offer a fascinating glimpse into the precision of our musical recall.



<h2 class="wp-block-heading" id="h-unveiling-the-mystery-of-earworms">Unveiling the mystery of earworms</h2>



A recent study has shed light on the surprising accuracy of earworms.



Published in the journal Attention, Perception, &amp; Psychophysics, the study revealed that nearly half of participants' renditions of earworms matched the original <a href="https://www.earth.com/news/most-people-have-a-hidden-musical-talent-for-singing-on-pitch/" target="_blank" rel="noreferrer noopener">pitch</a> of the songs.



This finding challenges prior beliefs about the limitations of musical memory, suggesting that our brains may preserve detailed “absolute pitch” memories even without formal pitch recognition skills.



Earworms, experienced by over 90% of people, are involuntary musical memories that spontaneously play in our minds. 



This study indicates that our recall of <a href="https://www.earth.com/news/song-melodies-have-become-much-simpler-since-1950/" target="_blank" rel="noreferrer noopener">melodies</a> may be more precise than previously thought, even without external references.



<h2 class="wp-block-heading" id="h-encountering-music-in-a-new-light">Encountering music in a new light</h2>



Matthew G. Evans, PhD candidate at <a href="https://admissions.ucsc.edu/" target="_blank" rel="noreferrer noopener">UC Santa Cruz</a>, said he first learned about the field of <a href="https://www.earth.com/news/music-can-prevent-brain-aging-and-cognitive-decline/" target="_blank" rel="noreferrer noopener">music</a> cognition from Daniel Levitin’s book&nbsp;This Is Your Brain On Music. 



"In that book, he describes a study where they found evidence for absolute pitch recall in voluntarily-recalled musical imagery - and I tried it myself, and it worked, and I’ve been hooked on the topic of musical memory ever since.”



Evans set out to investigate whether this accurate recall extended to spontaneous earworms or was limited only to songs that people purposefully tried to remember.



<h2 class="wp-block-heading" id="h-earworms-more-than-just-random-tunes">Earworms: More than just random tunes</h2>



The study involved 30 undergraduate students who participated in a two-week research period aimed at exploring the accuracy of spontaneous musical recall. 



Using the experience sampling method, the researchers documented these involuntary musical memories in real time by sending participants random text prompts throughout the day.



Students were asked to record any song playing in their minds, capturing the natural occurrence of earworms outside of a controlled laboratory setting.



While most participants had some familiarity with music, none reported having perfect pitch or formal training that would give them an advantage in recalling exact musical notes. 



Each recording was analyzed against the original <a href="https://www.earth.com/news/the-evolution-of-song-lyrics-less-complexity-and-more-emotion/" target="_blank" rel="noreferrer noopener">song</a> to determine how closely the pitch matched the song’s actual key. 



The findings were striking: 44.7% of the earworms matched the original song’s pitch exactly. When the range was expanded to include recordings within one semitone of the original pitch, nearly 69% of the renditions met this criterion - far surpassing what could be attributed to random chance.



<h2 class="wp-block-heading" id="h-the-melodic-imprint-of-our-brains">The melodic imprint of our brains</h2>



The study also found that pitch accuracy was not significantly affected by recent exposure to a song.



Some participants noted that their earworm was triggered by recently hearing the song, but their ability to match the original pitch remained similar to those whose earworms were not influenced by recent listening.



"When we divided our data into responses where participants said they had recently heard the song and those where they hadn’t, we saw absolutely no difference in absolute pitch accuracy," noted Evans. 



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



While this study provides valuable insights into how we recall music, it also highlights the need for further research to validate and expand upon these findings. 



To gain a broader understanding of how earworms and pitch recall function across different populations, future studies should incorporate a larger and more diverse participant pool, including individuals with no musical background and participants from varied age groups and cultural settings.



By expanding the scope of the research, scientists could explore questions such as whether musical memory accuracy varies by age, cultural exposure to music, or training. 



It may also be valuable to investigate whether factors such as musical genres or personal attachment to specific songs influence pitch accuracy in earworms.



This research marks an early step in unraveling the complex mechanisms of our brain's musical memory. 



As future studies build on this foundational work, we may discover more about the intricate ways in which our minds store and retrieve musical information, shedding light on the intersection of <a href="https://www.earth.com/news/memory-is-shaped-by-both-past-and-future-experience-and-events/" target="_blank" rel="noreferrer noopener">memory</a>, perception, and cognitive processes.



The study is published in the journal <a href="https://link.springer.com/article/10.3758/s13414-024-02936-0" target="_blank" rel="noreferrer noopener">Attention, Perception, &amp; Psychophysics</a>.



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Earworms: The surprising accuracy of our musical memory

Earworms - those persistent tunes that play in our heads...

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</div>
 
Today&#8217;s Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> describes the different fabrics that make some clothes safe to wash at home while others are dry clean only. 
Clothing fibers are either synthetic, plant based, or animal based. The chemical composition of these fibers will respond to cleaning methods differently, and understanding how these chemicals will react to water is key to safely washing and drying your clothes. 
&#8212;
By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer
Video Credit: American Chemical Society

The chemistry of clothes