Today's Image of the Day from the European Space Agency features Messier 78 (M78), a reflection nebula located in the constellation Orion about 1,350 light-years away from Earth. 



This image was released as part of the initial series of observations from ESA's <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid space mission</a>.&nbsp;



All data collected during these early observations, including a series of incredible <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid/Euclid_s_first_images_the_dazzling_edge_of_darkness" target="_blank" rel="noreferrer noopener">new views</a> of the nearby universe, is available to the public. 



<h2 class="wp-block-heading" id="h-image-of-messier-78">Image of Messier 78</h2>



Featured here is a high-resolution, detailed segment of a larger image showcasing Messier 78, a dynamic region of star formation obscured by cosmic dust.&nbsp;



This specific view highlights how young stars generate winds of charged particles, carving out “cavities” in the molecular clouds around them.&nbsp;



The blue hues in the image represent ionized atomic hydrogen, which is a primary component of the cloud, while the red indicates the absorption and scattering of light by dust particles.



The image captures hundreds of stars varying in brightness, illuminating their nebulous, purple surroundings. A dark, arch-like structure stretches from the upper left to the bottom right of the frame, merging into the densest, darkest clouds at the image’s base.



<h2 class="wp-block-heading" id="h-active-site-of-star-formation-nbsp">Active site of star formation&nbsp;</h2>



Messier 78 is not just a single nebula but part of a larger complex of stars and nebulous regions in <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a>, which includes various other objects like dark nebulae that are visible as patches blocking light from behind.



This region is an active site of star formation, featuring many young stars and protostars, which are stars in the early stages of formation.&nbsp;



<h2 class="wp-block-heading" id="h-viewing-messier-78">Viewing Messier 78</h2>



M78 is easily observable with small telescopes, and it appears as a hazy patch of light with two prominent stars near its center, which illuminate the surrounding dust.&nbsp;



The nebula is also a favorite among amateur astronomers for its beauty and relatively bright appearance.



<h2 class="wp-block-heading" id="h-subject-of-scientific-interest-nbsp">Subject of scientific interest&nbsp;</h2>



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <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> and interstellar matter.&nbsp;



The nebula consists of dense, cold gas and dust, which are essential ingredients for the birth of new stars.&nbsp;



The intense blue light that characterizes M78 is due to the reflection of starlight off these dust particles, a process known as scattering.



<h2 class="wp-block-heading" id="h-region-surrounding-messier-78-nbsp">Region surrounding Messier 78&nbsp;</h2>



The region surrounding M78 includes several other interesting features. For instance, there are Herbig-Haro objects within it, which are small patches of nebulosity associated with <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">newly born stars</a>.&nbsp;



These objects are formed when gas ejected by young stars collides with clouds of gas and dust at high speeds, creating shock waves that glow brightly.



<h2 class="wp-block-heading" id="h-earliest-stages-of-star-development-nbsp">Earliest stages of star development&nbsp;</h2>



Additionally, infrared observations of M78 have revealed much about the dust and colder objects in the area, which are not visible in optical light.&nbsp;



The observations have helped astronomers identify numerous young stars and brown dwarfs (objects that are too large to be planets and too small to be stars) within the nebula. 



This makes M78 a critical area for studying the earliest stages of star development and the properties of the interstellar medium.



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp-0">Euclid space mission&nbsp;</h2>



The <a href="https://www.earth.com/news/new-batch-of-brilliant-images-from-the-euclid-mission-live-up-to-the-hype/" target="_blank" rel="noreferrer noopener">Euclid space mission</a> is a European Space Agency (ESA) mission designed to study the dark universe, particularly focusing on dark energy and dark matter, which are fundamental components that are believed to drive the accelerating expansion of the universe and shape its large-scale structure.&nbsp;



The mission aims to map the geometry of the dark universe and better understand the physics of the cosmos.



<h3 class="wp-block-heading" id="h-observing-billions-of-galaxies-nbsp">Observing billions of galaxies&nbsp;</h3>



Euclid uses two primary scientific instruments: a visible light camera (VIS) and a near-infrared spectrometer and photometer (NISP).&nbsp;



These instruments will allow Euclid to measure the shapes and redshifts of galaxies at distances of up to 10 billion light-years. By surveying more than a third of the sky, the mission is expected to observe several billion galaxies.



<h3 class="wp-block-heading" id="h-studying-the-dark-universe-nbsp">Studying the dark universe&nbsp;</h3>



The data collected will help astronomers in studying the effects of dark matter and dark energy in depth, testing cosmological models, and exploring new theories about the nature of the universe.&nbsp;



The mission, named after the ancient Greek mathematician Euclid, seeks to address key questions related to the structure of the universe and the fundamental laws of physics governing its evolution and expansion.



Image Credit: European Space Agency&nbsp;



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Messier 78: Young stars shine through dense dust

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

Today's Image of the Day from the European Space Agency features a galaxy that is located about 600 million light-years away in the constellation Gemini. The Hubble Space Telescope observed a supernova in this galaxy - which appears as a bright blue dot in the photograph.



“This picture was taken roughly two months after a supernova named SN 2022aajn was discovered in this galaxy. The supernova is visible as a blue dot at the center of the image, brightening the hazy body of the galaxy,” noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



<h2 class="wp-block-heading" id="h-what-is-a-supernova">What is a supernova?</h2>



Supernovae are spectacular explosions marking the violent deaths of stars. These cosmic events are so luminous they can briefly outshine entire <a href="https://www.earth.com/news/galaxies-are-much-bigger-than-we-originally-believed-gas-clouds/" target="_blank" rel="noreferrer noopener">galaxies</a> and radiate more energy in a few weeks than our Sun will in its entire lifetime.&nbsp;



Supernovae explosions release heavy elements like carbon, oxygen, and iron into the interstellar medium. This stellar debris becomes the building blocks for new stars, planets, and even life itself. 



Supernovae also produce neutron stars or black holes, depending on the remaining core’s mass after the explosion.



<h2 class="wp-block-heading" id="h-types-of-supernovae-nbsp">Types of supernovae&nbsp;</h2>



There are two main types of supernovae, classified based on their causes. Type I supernovae occur when 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> in a binary system accretes material from its companion star, eventually reaching a critical mass and triggering a runaway nuclear reaction.&nbsp;



Type II supernovae happen when a massive star, at least eight times the mass of the Sun, exhausts its nuclear fuel. Unable to support its own gravity, the core collapses, resulting in a massive explosion that ejects the outer layers into space.



<h2 class="wp-block-heading" id="h-measuring-the-distance-to-faraway-galaxies-nbsp">Measuring the distance to faraway galaxies&nbsp;</h2>



According to ESA, SN 2022aajn is a Type Ia supernova. “Supernovae of this type help astronomers measure the distance to faraway galaxies. This is possible because Type Ia supernovae are thought to be of the same intrinsic luminosity - no matter how bright they seem from Earth, they put out the same amount of light as other Type Ia supernovae.”



This means that researchers can calculate the distance to the supernova and its host galaxy by comparing the observed brightness to the expected brightness.



“This seemingly simple measurement method is complicated by cosmic dust. The farther away a supernova is, the fainter and redder it will appear - but intergalactic dust can make a supernova appear fainter and redder as well,” explained ESA.



“To understand this complication, researchers will use Hubble to survey a total of 100 Type Ia supernovae in seven wavelength bands from the ultraviolet to the near-infrared.”



By analyzing the brightness of supernovae across multiple wavelengths, researchers can distinguish between the influences of dust and distance, refining our measurements of galaxies that exist billions of light-years away.



<h2 class="wp-block-heading" id="h-how-many-galaxies-exist">How many galaxies exist?</h2>



The number of galaxies in the universe is estimated to be around two trillion, based on observations from Hubble and more recent data from the James Webb Space Telescope. 



This estimate is derived from deep-field surveys that reveal countless galaxies, each containing billions to trillions of <a href="https://www.earth.com/news/interstellar-tunnel-found-that-connects-our-solar-system-to-other-stars/" target="_blank" rel="noreferrer noopener">stars</a>.&nbsp;



However, because our observations are limited by current technology and the vastness of the cosmos, the actual number could be even higher.&nbsp;



Many <a href="https://www.earth.com/news/ancient-galaxies-formed-from-the-earliest-elements-in-the-universe/" target="_blank" rel="noreferrer noopener">galaxies</a> remain unseen due to their extreme distances, faintness, or obstruction by cosmic dust.



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



Gemini is one of the 12 zodiac constellations and is best known for representing the mythological twins Castor and Pollux. It is located in the northern celestial hemisphere and is most visible during winter in the Northern Hemisphere.&nbsp;



The constellation is bordered by Taurus to the west, Cancer to the east, and Orion to the south.



The two brightest stars in Gemini - Castor and Pollux - represent the heads of the twins and are easy to spot. Pollux, the brighter of the two, is an orange giant star about 34 light-years from Earth, while Castor is a more complex system made up of six stars. 



The constellation also contains several notable deep-sky objects, including the open cluster Messier 35, which is a beautiful collection of young stars located near Gemini’s western border.



Image Credit: ESA&nbsp;



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Hubble spots a supernova in the constellation Gemini 

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



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



<h2 class="wp-block-heading" id="h-complex-planetary-nebula">Complex planetary nebula </h2>



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA/ESA Hubble Space Telescope



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Cat's Eye Nebula in the constellation Draco

Today's Image of the Day from NASA Earth Observatory features Ksudach, a remarkable volcanic complex located on Russia's Kamchatka Peninsula.



“The peninsula is one of the world’s most active volcanic arcs due to tectonic plate movement, with the Pacific Plate subducting under the Eurasian Plate,” noted <a href="https://earthobservatory.nasa.gov/images/153779/ksudachs-nested-calderas-and-craters" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-explosive-eruptions-of-ksudach">Explosive eruptions of Ksudach</h2>



Ksudach is classified as a shield <a href="https://www.earth.com/news/new-camera-helps-scientists-forecast-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">volcano</a> due to the gentle slopes formed by its extensive lava flows. The combination of its shield-like structure and the prominent caldera system makes Ksudach a unique volcanic feature on the Kamchatka Peninsula.



“Several overlapping calderas and craters comprise the volcano. Calderas are large, bowl-shaped depressions created by the collapse of overlying material into an emptied subsurface magma chamber,” explained NASA.



“Craters are circular depressions created by volcanic activity, surface impacts, or explosions.”



This volcanic system has a fascinating geological history shaped by multiple explosive eruptions.&nbsp;



The most significant of these occurred around 240 AD, leaving behind a prominent caldera that now hosts scenic crater lakes, such as Lake Ksudach. 



“Lakes within the volcanic region are primarily recharged by rain and snowmelt from the winter season. This photo shows the water’s contrasting blue hues surrounded by green vegetation,” noted NASA.



“Traces of snow fill valleys within and outside the volcano’s caldera complex. These snow-covered areas highlight the drainage patterns from higher to lower elevations. Water that flows through these erosional pathways and into the caldera supports its vegetation and lakes.”



<h2 class="wp-block-heading" id="h-unique-landscape-of-ksudach-nbsp">Unique landscape of Ksudach&nbsp;</h2>



Ksudach's landscape also features pyroclastic deposits, lava flows, and hydrothermal features like fumaroles.&nbsp;



The surrounding environment - which is part of the UNESCO-listed Kamchatka Volcanoes - supports a diverse ecosystem with unique wildlife. 



Despite its remote location, Ksudach has drawn the attention of geologists, offering insights into <a href="https://www.earth.com/news/underwater-volcanic-eruptions-are-more-harmful-than-previously-believed/" target="_blank" rel="noreferrer noopener">volcanic processes</a> and the dynamics of caldera formation.



<h2 class="wp-block-heading" id="h-dynamic-nature-of-earth-s-geology-nbsp">Dynamic nature of Earth's geology&nbsp;</h2>



The most well-documented eruption of Ksudach occurred in March 1907. This eruption ranks as one of the largest in Kamchatka in the 20th century, with a Volcanic Explosivity Index (VEI) of 5.



The eruption produced a colossal ash column that soared into the stratosphere, dispersing fine particles over vast distances and contributing to global atmospheric changes.&nbsp;



The sheer force of the <a href="https://www.earth.com/news/icelands-volcanic-eruptions-may-continue-for-decades/" target="_blank" rel="noreferrer noopener">eruption</a> unleashed pyroclastic flows - fast-moving avalanches of hot gas, ash, and volcanic debris - that raced down the volcano's slopes, obliterating everything in their path.&nbsp;



These flows, capable of reaching temperatures over 1,000°C, decimated vegetation and altered the topography of the surrounding region.&nbsp;



Simultaneously, tephra deposits blanketed the landscape in layers of thick volcanic material, smothering ecosystems and creating a barren wasteland.&nbsp;



Today, Ksudach is considered an active <a href="https://www.earth.com/news/axial-seamount-large-underwater-volcano-off-us-coast-will-likely-erupt-in-2025/" target="_blank" rel="noreferrer noopener">volcano</a> but remains dormant. The region is closely monitored due to its potential for renewed <a href="https://www.earth.com/news/new-research-enhances-predictions-on-volcanic-eruptions/" target="_blank" rel="noreferrer noopener">activity</a>.



<h2 class="wp-block-heading" id="h-pacific-ring-of-fire-nbsp">Pacific Ring of Fire&nbsp;</h2>



The Kamchatka Peninsula lies along the Pacific Ring of Fire, a horseshoe-shaped zone encircling the Pacific Ocean where tectonic activity is highly concentrated.&nbsp;



This geologically dynamic area features numerous volcanoes, hot springs, geysers, and frequent seismic activity - making it a hotspot for both natural beauty and scientific study. 



Kamchatka is home to over 160 volcanoes, with about 30 considered active, including Klyuchevskaya Sopka, the highest and one of the most active in the region.



<h3 class="wp-block-heading" id="h-volcanic-activity-nbsp">Volcanic activity&nbsp;</h3>



As the Pacific Plate dives into the Earth's mantle, it melts and generates magma that feeds Kamchatka’s volcanic systems.&nbsp;



This ongoing tectonic interaction also contributes to the broader activity of the Pacific Ring of Fire, which accounts for approximately 75% of the world's active and dormant <a href="https://www.earth.com/news/supervolcano-italy-solfatara-crater-phlegraean-fields-shows-signs-of-waking-up/" target="_blank" rel="noreferrer noopener">volcanoes</a> and about 90% of its earthquakes.



<h3 class="wp-block-heading" id="h-broader-significance-nbsp">Broader significance&nbsp;</h3>



Beyond its geological significance, the Kamchatka Peninsula boasts a diverse ecosystem that is home to animals such as snow sheep, brown bears, red foxes, and unique plants that are adapted to its harsh environment. 



The coastal waters surrounding the peninsula support various fish species, including abundant salmon, as well as sea lions and killer whales.



The interplay of volcanic landscapes and pristine wilderness makes it a natural laboratory for understanding Earth's dynamic processes.



The image was captured by an astronaut aboard the International Space Station.



Image Credit: NASA Earth Observatory&nbsp;



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Ksudach: A volcano shaped by explosive forces

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

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,” said 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

Earth, the only known planet to support life, owes much of its habitability to water. Understanding when and how water arrived on Earth is crucial for piecing together the story of life’s origins. 



Scientists have long debated whether water was present from the planet’s formation or if it arrived later through external sources. 



A recent study led by a Rutgers-New Brunswick scientist challenges existing theories, suggesting that water arrived much later than <a href="https://www.earth.com/news/water-cycles-through-plants-with-unexpected-speed/" target="_blank" rel="noreferrer noopener">previously believed</a>.



The findings indicate that Earth received water toward the final stages of its formation. This discovery could reshape scientific understanding of the conditions necessary for life.



By examining isotopes in Earth’s rocks and comparing them with meteorites, researchers have provided new insights into the timing and process of water’s arrival on our planet.



<h2 class="wp-block-heading" id="h-timing-of-life-s-origins">Timing of life’s origins</h2>



Scientists seek to pinpoint when key <a href="https://www.earth.com/news/comets-may-have-delivered-water-to-earth/" target="_blank" rel="noreferrer noopener">ingredients for life</a> first appeared on Earth. Water, energy, and a mix of organic chemicals known as CHNOPS - carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur - are essential for life to emerge. 



Determining when these components arrived can offer clues about the timing of life’s formation.



Katherine Bermingham is an associate professor in the <a href="https://eps.rutgers.edu" target="_blank" rel="noreferrer noopener">Department of Earth and Planetary Sciences</a> at Rutgers and lead author of the study.



“When water was delivered to the planet is a major unanswered question in planetary science,” said Bermingham. “If we know the answer, we can better constrain when and how life developed.”



Her research suggests that water was not present during the early phases of Earth’s formation, as some theories propose. Instead, the planet acquired it much later through a process known as late accretion, when additional material from space continued to shape Earth.



<h2 class="wp-block-heading" id="h-examining-the-building-blocks-of-planets">Examining the building blocks of planets</h2>



Bermingham specializes in cosmogeochemistry, a field that examines the chemical composition of planetary materials to understand their origins. 



By analyzing Earth rocks and extraterrestrial materials such as meteorites, she investigates how rocky planets, including Earth, formed and evolved.



In this study, Bermingham’s team used thermal ionization mass spectrometry, a precise method for measuring isotopic compositions. 



They developed a new analytical approach to examine isotopes of molybdenum, an element found in both Earth’s crust and meteorites.



Isotopes are variations of an element with the same number of protons but different numbers of neutrons, which gives them slightly different atomic masses while maintaining identical <a href="https://www.earth.com/news/distress-signals-earths-water-cycle-is-becoming-more-erratic/" target="_blank" rel="noreferrer noopener">chemical properties</a>.



“The molybdenum isotopic composition of Earth rocks provides us with a special window into events occurring around the time of Earth’s final core formation, when the last 10% to 20% of material was being assembled by the planet. This period is thought to coincide with the Moon’s formation,” explained Bermingham.



<h2 class="wp-block-heading" id="h-comparing-meteorites-and-earth-rocks">Comparing meteorites and Earth rocks</h2>



To track Earth’s early chemical history, the team examined meteorite samples from the National Museum of Natural History at the Smithsonian Institution. Scientists classify meteorites into two main groups based on their place of origin in the solar system.



The first group, known as “CC” meteorites, likely formed in the outer solar system, where conditions were wetter. The second group, “NC” meteorites, originated in the inner solar system, where conditions were much drier. 



This study focused on meteorites from the NC group to compare their chemical composition with Earth rocks.



The researchers analyzed molybdenum isotopes in rocks from Greenland, South Africa, Canada, the United States, and Japan. 



These rocks date back to the time of the Moon’s formation and are believed to contain elements added to <a href="https://www.earth.com/news/earth-other-planets-collected-first-water-from-unexpected-source-planetesimals/" target="_blank" rel="noreferrer noopener">Earth</a> during this period.



By comparing the isotopic signatures of meteorites and Earth rocks, the team sought to determine whether the Moon-forming event delivered a significant amount of water to Earth.



<h2 class="wp-block-heading" id="h-earth-s-water-may-have-arrived-late">Earth’s water may have arrived late</h2>



“Once we gathered the different samples and measured their isotopic compositions, we compared the meteorites’ signatures with the rock signatures to see if there was a similarity or a difference,” Bermingham said. “And from there, we drew inferences.”



The analysis revealed that the molybdenum composition of Earth rocks closely matched that of NC meteorites, which originated in the drier inner solar system. 



This finding suggests that Earth’s building blocks primarily came from a region of the solar system where water was scarce.



This contradicts a popular theory that a significant amount of Earth’s water arrived during the Moon-forming event. 



Instead, the study indicates that water was delivered in smaller amounts long after the Moon formed, during the later stages of planetary development.



<h2 class="wp-block-heading" id="h-rethinking-the-source-of-earth-s-water">Rethinking the source of Earth’s water</h2>



“We have to figure out from where in our solar system Earth's <a href="https://www.earth.com/news/stunning-discovery-earths-building-blocks-contained-water/" target="_blank" rel="noreferrer noopener">building blocks</a> - the dust and the gas - came and around when that happened,” Bermingham said. “That’s the information needed to understand when the stage was set for life to begin.”



If most of Earth’s original material came from the drier inner solar system, then the Moon-forming event was likely not a major contributor of water. Instead, water must have arrived in smaller portions later. 



This conclusion challenges the idea that a single event provided Earth with the majority of its water. 



The study supports the view that water accumulated gradually over time, arriving through a combination of asteroid impacts and other processes occurring well after the planet had taken shape.



<h2 class="wp-block-heading" id="h-questions-about-life-s-early-conditions">Questions about life’s early conditions</h2>



“Our results suggest that the Moon-forming event was not a major supplier of water, unlike what has been thought previously,” Bermingham said. “These findings, however, permit a small amount of water to be added after final core formation, during what is called late accretion.”



This discovery raises new questions about how long it took for Earth to become habitable. If water arrived later than previously thought, then life may have taken longer to emerge. 



This could also have implications for understanding other planets, particularly those that scientists consider candidates for life.



By refining the timeline of Earth’s water history, this study contributes to a broader effort to understand planetary evolution. If water arrived late on Earth, then other planets might have followed a similar pattern. 



This could mean that life-supporting conditions take longer to develop than scientists once assumed.



<h2 class="wp-block-heading" id="h-what-s-next-in-the-search-for-earth-s-water">What’s next in the search for Earth’s water?</h2>



The study represents a step forward in unraveling Earth’s past, but it also highlights the many unanswered questions about the origins of water and life. 



Future research will likely focus on refining models of planetary accretion, analyzing additional meteorite samples, and exploring other isotopic markers that could provide further insights.



Other Rutgers contributors to the study include Linda Godfrey, an assistant research professor, and Hope Tornebene, a laboratory researcher in the Department of Earth and Planetary Sciences. 



The research continues to push the boundaries of planetary science, bringing us closer to understanding how Earth became a world capable of supporting life.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0016703724005751?via%3Dihub" target="_blank" rel="noreferrer noopener">Geochimica et Cosmochimica Acta</a>.



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Water arrived on Earth gradually over time, not in one big event

Earth, the only known planet to support life, owes much...

Childhood malignant brain tumors remain a significant challenge for clinicians and researchers around the world, largely because they are often only discovered after they have already become complex and difficult to treat.&nbsp;



Among these cancers, medulloblastoma stands out as the most common malignant brain tumor in children, frequently leading to devastating outcomes.&nbsp;



Now, a team of scientists at <a href="https://www.sickkids.ca/" target="_blank" rel="noreferrer noopener">The Hospital for Sick Children</a> (SickKids) has made a pivotal finding that could stop a subtype of medulloblastoma - known as sonic hedgehog (SHH) medulloblastoma - from forming at its earliest stages.



<h2 class="wp-block-heading" id="h-detection-of-childhood-brain-cancer">Detection of childhood brain cancer</h2>



Because <a href="https://www.earth.com/news/how-antidepressants-could-help-treat-brain-tumors/" target="_blank" rel="noreferrer noopener">brain tumors</a> typically trigger noticeable symptoms only after considerable growth, crucial details about the cancer’s initial formation can remain hidden. 



By the time a young patient is diagnosed, the tumorous cells may have already undergone numerous mutations. 



In response to this clinical hurdle, a research group led by Dr. Peter Dirks at SickKids focused on the earliest cellular steps of SHH medulloblastoma.&nbsp;



<h2 class="wp-block-heading" id="h-halting-tumor-formation">Halting tumor formation </h2>



The new study, published in the journal <a href="http://dx.doi.org/10.1038/s41467-024-54858-y" target="_blank" rel="noreferrer noopener">Nature Communications</a>, shows that a single protein serves as a critical “on switch,” awakening dormant stem cells that then give rise to a tumor.



“Our findings offer a novel strategy to target cancer stem cells, providing hope for more effective treatments against aggressive brain tumors,” said Dirks, a senior scientist in the Developmental, Stem Cell &amp; Cancer Biology program and Chief of the Division of Neurosurgery.



One of the study’s most significant insights is that by preventing the reactivation of these dormant, cancer-initiating cells, the entire cascade of tumor formation can be intercepted.&nbsp;



SHH medulloblastoma arises in a particular subset of patients, and this discovery suggests that if the first molecular trigger is blocked, the disease may be prevented from taking root in the brain.



<h2 class="wp-block-heading" id="h-an-opportunity-for-intervention-nbsp">An opportunity for intervention&nbsp;</h2>



In the study, the team looked at how SHH medulloblastoma unfolds at the cellular level. They found that the protein OLIG2 plays a central role in “waking up” quiescent stem <a href="https://www.earth.com/news/secrets-of-cancer-cell-death-may-transform-treatment/" target="_blank" rel="noreferrer noopener">cells</a> - cells that are otherwise inactive - and prompting them to divide uncontrollably, eventually forming tumors.&nbsp;



As the scientists dug deeper, they identified the exact window in which this reactivation occurs and recognized it as a prime opportunity for intervention.



“There is order to how the cancer initiating stem cells undergo fate changes to form tumors. We can target an early transition event and intercept the entire process - essentially stopping the cancer in its earliest form,” said study first author Kinjal Desai, a postdoctoral researcher in the Dirks lab.



<h2 class="wp-block-heading" id="h-potential-to-prevent-relapse">Potential to prevent relapse</h2>



By pinpointing OLIG2’s critical role, the researchers tested whether blocking its action could halt tumor initiation and, importantly, prevent relapse in cases that had already undergone conventional treatments.&nbsp;



The experts used a small molecule called CT-179, which disrupts OLIG2 function and stops the dormant stem cells from waking.&nbsp;



When combined with an existing therapeutic approach, this treatment not only blocked SHH medulloblastoma formation in a preclinical model but also effectively prevented residual cancer stem cells from becoming reactivated later on.&nbsp;



This two-pronged effect significantly reduced the chance of tumor regrowth and improved survival outcomes.



<h2 class="wp-block-heading" id="h-targeting-brain-tumors-in-the-early-stages">Targeting brain tumors in the early stages</h2>



Simultaneously, researchers at <a href="https://www.choa.org/" target="_blank" rel="noreferrer noopener">Children’s Healthcare of Atlanta</a> and the <a href="https://www.qimrberghofer.edu.au/" target="_blank" rel="noreferrer noopener">QIMR Berghofer Medical Research Institute</a> in Australia carried out related experiments, published concurrently in <a href="https://www.nature.com/articles/s41467-024-54861-3" target="_blank" rel="noreferrer noopener">Nature Communications</a>.&nbsp;



Their work corroborates the SickKids findings, hinting that this kind of OLIG2-targeting strategy could go beyond SHH medulloblastoma to combat other pediatric brain tumors, including diffuse intrinsic pontine glioma (DIPG) - an aggressive <a href="https://www.earth.com/news/rising-cancer-rates-in-young-adults-linked-to-accelerated-aging/" target="_blank" rel="noreferrer noopener">cancer</a> that has proven particularly resistant to conventional therapies.



This latest discovery advances previous research from the Dirks Lab on the early stages of brain tumors. While the new findings will require validation in clinical trials, they highlight the advantages of what Dr. Dirks describes as ‘precision biology.’



“At SickKids, we’re already genetically testing every child with cancer to inform their diagnosis and treatments - our study goes beyond genetic testing to precision biology,” Dirks said. “I am excited for a future where this ‘magic bullet’ for early treatment could be combined with diagnostic tests to potentially prevent the cancer from developing at all.”



By intervening at the very root of tumor formation, the team’s approach could offer a transformative path for children with medulloblastoma and other aggressive brain cancers.&nbsp;



If these promising strategies move successfully through clinical trials, early intervention might indeed stop pediatric brain tumors before they can even take hold, heralding a new era in <a href="https://www.earth.com/news/ai-is-the-next-frontier-in-cancer-treatment/" target="_blank" rel="noreferrer noopener">cancer treatment</a>.



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New therapy for childhood brain cancer halts tumor formation

Childhood malignant brain tumors remain a significant challenge for clinicians...

The stereotype that women outtalk men persists across many cultures. Yet, a prominent study in 2007 challenged that notion by finding that men and women each speak around 16,000 words per day, on average.



A new, larger investigation revisits this topic and offers a more nuanced view: women may indeed be more talkative - but only during a specific stage of life.



Study co-lead author Colin Tidwell is a clinical psychology doctoral candidate at the <a href="https://www.arizona.edu/" target="_blank" rel="noreferrer noopener">University of Arizona </a>(U of A).&nbsp;



“There is a strong cross-cultural assumption that women talk a lot more than men,” said Tidwell. “We wanted to see whether or not this assumption holds when empirically tested.”



<h2 class="wp-block-heading" id="h-talking-varies-by-age-and-gender">Talking varies by age and gender</h2>



Analyzing data from nearly 2,200 participants, the researchers found that women aged 25 to 65 speak about 3,000 more words per day than men in the same age bracket.&nbsp;



However, in adolescence (10-17), emerging adulthood (18-24), and older adulthood (65 and up), they observed no notable gender gap in daily word count.



The study also suggests that people overall might be talking less than before, which the researchers suspect could be linked to growing reliance on digital communication.



<h2 class="wp-block-heading" id="h-the-claim-that-women-talk-more">The claim that women talk more</h2>



In 2007, University of Arizona psychologist Matthias Mehl investigated the common claim that women are significantly more talkative than men.&nbsp;



Participants in that study - about 500 men and women - wore a device called the EAR (Electronically Activated Recorder), which periodically recorded brief clips of their everyday <a href="https://www.earth.com/news/scientists-have-20-minute-conversation-with-a-humpback-whale-named-twain/" target="_blank" rel="noreferrer noopener">conversations</a>.



After estimating each participant’s total daily word count, the researchers concluded that no significant gender difference existed - a finding that appeared in the journal <a href="https://www.science.org/doi/10.1126/science.1139940?adobe_mc=MCMID%3D90780648708216300104417575982572668868%7CMCORGID%3D242B6472541199F70A4C98A6%2540AdobeOrg%7CTS%3D1738666255&amp;adobe_mc=MCMID%3D90780648708216300104417575982572668868%7CMCORGID%3D242B6472541199F70A4C98A6%2540AdobeOrg%7CTS%3D1738667536" target="_blank" rel="noreferrer noopener">Science</a> and garnered national headlines.&nbsp;



Nevertheless, critics pointed out that most participants were college-aged and all lived in Austin, Texas, limiting the study’s diversity.



Almost two decades later, Mehl collaborated with Tidwell, Valeria Pfeifer, a postdoctoral researcher at the U of A, and Alexander Danvers, a former U of A postdoctoral fellow, to repeat the experiment on a larger scale.&nbsp;



The new work incorporates 630,000 EAR recordings from 22 separate studies across four countries, covering individuals aged 10 to 94 - a total of 2,197 participants, which is four times the original sample size.



<h2 class="wp-block-heading" id="h-why-do-women-talk-more">Why do women talk more?</h2>



Among all age groups studied, a significant difference between men’s and women’s word counts emerged only in early to middle <a href="https://www.earth.com/news/lifestyle-choices-in-young-adulthood-impact-cognitive-ability-in-midlife/" target="_blank" rel="noreferrer noopener">adulthood</a> (25-64). During these years, women spoke about 21,845 words per day, while men spoke about 18,570.



The researchers remain unsure exactly why women might talk more during this period, but they propose that <a href="https://www.earth.com/news/parent-children-relationships-are-key-to-lifelong-well-being/" target="_blank" rel="noreferrer noopener">parenting</a> responsibilities could be one contributing factor.



“Gender-linked differences in child rearing and family care are one possibility that could account for this difference,” said Mehl, the senior author of the study and a professor in the U of A Department of Psychology.&nbsp;



“If biological factors like hormones were to be the main cause, a sizable gender difference should have also been present among emerging adults. If societal generational changes were to be the driving force, there should have been a gradually increasing gender difference with older participants. Neither, though, was the case.”



<h2 class="wp-block-heading" id="h-talking-trends-across-time">Talking trends across time</h2>



While the data suggest that women do speak more than men during early and middle adulthood, Mehl highlighted that individual differences can overshadow such group patterns.&nbsp;



The least talkative person in the entire study - a man - spoke roughly 100 words a day, while the most talkative participant - also a man - exceeded 120,000 words.



“We humans are so much more different individually than the two genders systematically,” Mehl said.



Another revealing finding was that the average word count across participants has been declining since 2005, slipping from about 16,000 words per day to about 13,000.



“We did a full analysis looking at what year the data were collected and found that, indeed, 300 spoken words on average per year go missing,” noted study co-lead author Pfeifer.



Although the exact cause for this decline is not fully established, researchers suspect that digital technologies - such as texting, <a href="https://www.earth.com/news/spending-less-time-on-social-media-improves-your-mental-health/" target="_blank" rel="noreferrer noopener">social media</a>, and online chats - could be supplanting spoken conversations.



<h2 class="wp-block-heading" id="h-conversation-as-a-health-behavior">Conversation as a health behavior</h2>



Mehl emphasized the need for further inquiry into the effects of talkativeness and social engagement on overall health. He is currently co-developing a device called SocialBit, akin to a Fitbit, that tracks the duration of daily conversations without recording their content. Instead, it relies on an algorithm to detect whether ambient sounds contain speech.



“I'm fascinated by the idea that we know how much we need to sleep, we know how much we need to exercise, and people are wearing Fitbits all the time, but we have no idea how much we're supposed to socialize,” he said.&nbsp;



“The evidence is very strong that socializing is linked to health, at least to the same extent as physical activity and sleep are. It's just another health behavior.”



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



Overall, the follow-up study offers a refined perspective on the question of whether women speak more than men. While the gap exists during early and middle adulthood, no significant difference emerges in adolescence, emerging adulthood, or older age.&nbsp;



Beyond that, both genders may be speaking fewer words over time - possibly due to a shift toward digital forms of communication.



As researchers continue to investigate the intersection between conversation, well-being, and modern technology, novel tools like SocialBit may shed light on just how much human dialogue contributes to <a href="https://www.earth.com/news/social-activity-may-delay-the-onset-of-dementia-by-years/" target="_blank" rel="noreferrer noopener">health</a>, reinforcing the importance of face-to-face interactions in an increasingly digital era.



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Do women really talk more than men? A new look at the debate

The stereotype that women outtalk men persists across many cultures....

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Today&#8217;s Video of the Day from <a href="https://www.stanford.edu/">Stanford University</a> describes how virtual reality can be used to raise awareness about the harmful effects of ocean acidification. 
“I believe virtual reality is a powerful tool that can help the environment in so many ways,” said study co-author Professor Jeremy Bailenson. “Changing the right minds can have a huge impact.”
The experts hope that exposure to a virtual underwater experience will not only educate people about ocean acidification, but will also motivate them to do something about it. 
&#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: Stanford University 
&nbsp;

Using virtual reality to motivate environmental action