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

Today's Image of the Day from NASA Earth Observatory features ice on Lake Michigan in late January 2025, when extreme cold settled into the Chicago area.



“Between January 19 and 24, 2025, a brutal cold snap hit Chicago. This satellite image captured a glimpse of the wintry aftermath,” noted <a href="https://earthobservatory.nasa.gov/images/153885/a-chill-over-chicagoland" target="_blank" rel="noreferrer noopener">NASA</a>.



According to the National Weather Service (NWS), the first half of the cold spell was the most intense.&nbsp;



<h2 class="wp-block-heading" id="h-cold-spells-and-snowfall">Cold spells and snowfall</h2>



Cold spells in the Chicago area are often accompanied by strong winds and significant <a href="https://www.earth.com/news/snow-cover-has-decreased-in-recent-decades/" target="_blank" rel="noreferrer noopener">snowfall</a>.



“On January 21, the air temperature in Chicago reached as low as minus 15 degrees Fahrenheit (minus 26 degrees Celsius). At the time, little to no snow covered the ground in Chicago, which NWS noted is uncommon amid sub-zero temperatures,” said NASA.



“Snowflakes returned toward the end of the cold spell. Between the mornings of January 22 and 23, several waves of snowfall produced the blanket of white across the Chicago area visible in this image.”



“Another expanse of white is visible atop Lake Michigan. This is lake ice, which grows on the Great Lakes each winter, though its extent and timing can be highly variable. Ice coverage on the Great Lakes typically reaches its annual peak in late February or early March.”



<h2 class="wp-block-heading" id="h-visible-ice-patterns">Visible ice patterns</h2>



Jia Wang, an ice climatologist at NOAA’s Great Lakes Environmental Research Laboratory (GLERL), noted that on January 24, winds were blowing offshore and pushing ice away from the coastline.



In the photo, areas of dark, thin ice can be seen close to the shore, while patchy areas of bright white ice are visible away from shore. According to Wang, the whiter areas might be due to ice that has piled up and formed a very rough surface.



<h2 class="wp-block-heading" id="h-ice-cover-on-lake-michigan-nbsp">Ice cover on Lake Michigan&nbsp;</h2>



“The area of Lake Michigan covered with ice in late January 2025 hovered around the historical average (1973-2024) for the time of year, according to data from GLERL. When the image was acquired, ice covered about 20 percent of the lake,” noted NASA.



“Meanwhile, several hundred miles to the east, ice on Lake Erie spiked well above average in late January, according to GLERL, with ice spanning around 80 percent of the lake. The ice was thick enough to temporarily immobilize a Canadian cargo freighter, according to news reports.”



To calculate the thickness of ice on the Great Lakes, experts are investigating ways to use altimetry data from NASA’s ICESat-2 (Ice, Cloud and land Elevation Satellite-2).



Eric Anderson, a researcher at the Colorado School of Mines, noted that such measurements could improve ice and weather <a href="https://www.earth.com/news/new-era-in-forecasting-ai-will-improve-extreme-weather-warnings/" target="_blank" rel="noreferrer noopener">forecasting</a> as well as help us understand changes in Earth’s surface freshwater.



<h2 class="wp-block-heading" id="h-ice-on-the-great-lakes">Ice on the Great Lakes</h2>



Ice formation on the <a href="https://www.earth.com/news/mysterious-craters-found-in-the-bottom-of-lake-michigan/" target="_blank" rel="noreferrer noopener">Great Lakes</a> is a dynamic process influenced by seasonal temperatures, wind patterns, and climate variability.&nbsp;



Each year, ice begins to develop in late fall and early winter, typically forming first in sheltered bays and shallow areas before extending over deeper waters.&nbsp;



The extent and duration of ice cover vary significantly, with some years experiencing widespread freezing while others see only partial coverage due to warmer conditions.



<h2 class="wp-block-heading" id="h-fluctuations-in-ice-coverage">Fluctuations in ice coverage</h2>



Historically, ice coverage on the Great Lakes has fluctuated, with long-term records showing a decline in ice extent due to rising global temperatures.&nbsp;



The lakes act as vast heat reservoirs, meaning their large thermal mass can delay freezing, especially in milder winters.&nbsp;



When ice does form, it affects local weather patterns, contributing to lake-effect <a href="https://www.earth.com/news/sea-ice-loss-increases-snowfall-over-west-antarctica/" target="_blank" rel="noreferrer noopener">snow</a> in surrounding regions. It also impacts ecosystems, as ice cover influences fish spawning, winter survival of aquatic organisms, and shoreline <a href="https://www.earth.com/news/fighting-coastal-erosion-electricity-turns-sand-into-a-sea-wall/" target="_blank" rel="noreferrer noopener">erosion</a>.



<h2 class="wp-block-heading" id="h-increasing-variability-in-ice-cover-nbsp">Increasing variability in ice cover&nbsp;</h2>



In recent decades, scientists have observed increasing variability in ice cover, with some years experiencing near-record lows. 



This trend impacts commercial shipping in two key ways: reduced ice cover can extend the navigational season, but unpredictable freeze-thaw cycles make ice-breaking operations more challenging.



Additionally, ice conditions influence recreational activities such as ice fishing, skating, and snowmobiling - all of which depend on stable and thick ice.



Overall, ice on the Great Lakes is a key indicator of changing <a href="https://www.earth.com/news/climate-change-earth-energy-imbalance-temperature-rise/" target="_blank" rel="noreferrer noopener">climate patterns</a>, with its variability providing insights into broader environmental shifts.&nbsp;



The image was captured on January 24, 2025 with the OLI (Operational Land Imager) on Landsat 8.



Image Credit: NASA Earth Observatory&nbsp;



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Chicago cold spell brings ice to Lake Michigan 

As humanity strives to establish communities on the Moon, Mars, and beyond, the fundamental problem of how to maintain life remains paramount. The solutions revolve around supplying oxygen, food, and water. 



While it has been established that water exists on the Moon, pinpointing its precise locations presents a formidable challenge. Could it be within craters, permanently shadowed areas, or near the poles?



Answering these questions is essential for ensuring that astronauts can successfully inhabit the Moon.



A recent study by researchers at the <a href="https://ucsd.edu/" target="_blank" rel="noreferrer noopener">University of California San Diego</a> (UC San Diego) might help transform this vision into reality by guiding upcoming space missions, including <a href="https://www.nasa.gov/humans-in-space/artemis/" target="_blank" rel="noreferrer noopener">NASA’s Artemis program</a>, which aims to thoroughly explore and ultimately settle on the <a href="https://www.earth.com/news/lunar-anthropocene-how-humans-have-impacted-the-moon/" target="_blank" rel="noreferrer noopener">Moon</a>.&nbsp;



<h2 class="wp-block-heading" id="h-a-legacy-rooted-in-lunar-analysis">A legacy rooted in lunar analysis</h2>



Study lead author Maxwell Thiemens is a research fellow at <a href="https://www.vub.be/nl" target="_blank" rel="noreferrer noopener">Vrije Universiteit Brussel</a> and an alumnus of the <a href="https://scripps.ucsd.edu/" target="_blank" rel="noreferrer noopener">Scripps Institution of Oceanography</a>. He conducted the study with his father, Mark Thiemens, a professor of chemistry and biochemistry at UC San Diego.



Their contributions build upon UC San Diego’s historical connections to lunar research. In 1967, Nobel Laureate Harold Urey and James Arnold, both at UC San Diego’s Department of Chemistry, were among the earliest scientists to receive Apollo 11 lunar samples.&nbsp;



Urey was one of the first to theorize the presence of <a href="https://www.earth.com/news/moons-entire-surface-is-covered-with-water-and-hydroxyl-not-just-the-poles/" target="_blank" rel="noreferrer noopener">lunar water</a>, particularly within the permanently shadowed polar regions.&nbsp;



<h2 class="wp-block-heading" id="h-where-did-the-moon-get-its-water">Where did the Moon get its water?</h2>



Contemporary scientific understanding suggests that lunar water could stem from one of three primary origins. First, it may be indigenous to the Moon.



Another theory is that lunar water was created by <a href="https://www.earth.com/news/the-solar-wind-which-creates-beautiful-auroras-on-earth-is-now-less-mysterious/" target="_blank" rel="noreferrer noopener">solar winds</a>, where hydrogen from the Sun reacts with lunar oxygen under high energy. The third possibility is that the water was deposited by icy comets that crashed onto the lunar surface.



Just as civilizations on Earth have historically settled near dependable water supplies, any permanent lunar presence will hinge on identifying and understanding the Moon’s water sources.



<h2 class="wp-block-heading" id="h-extracting-water-from-lunar-rocks">Extracting water from lunar rocks</h2>



Seeking to clarify where and how lunar water forms, Morgan Nunn Martinez (formerly a UC San Diego graduate student) conducted an analysis of small <a href="https://www.earth.com/news/mysterious-rocks-may-unlock-secrets-of-the-moons-magnetic-history/" target="_blank" rel="noreferrer noopener">rock samples</a> obtained during the Apollo 9 mission in 1969.&nbsp;



While it might seem improbable for rocks to host measurable amounts of water, a process called thermal release makes it possible. During this process, lunar specimens are heated to three temperature levels - 50°C, 150°C, and 1,000°C - to free water molecules embedded within the rock.



In the case of low-temperature releases (50°C, 150°C), lightly bound water molecules that are loosely attached to the rock are able to escape. 



On the other hand, in a high-temperature release (1,000°C), tightly bound water molecules, lodged deep within the rock’s structure, are liberated. Surprisingly, the rock samples were found to be relatively “wet.” 



After the molecules are driven off as water vapor, they are collected and purified until only oxygen remains. 



Scientists then measure the composition of the three oxygen isotopes in the sample - valuable for identifying both the origin and the time frame of the water.



<h2 class="wp-block-heading" id="h-origins-of-water-molecules-nbsp">Origins of water molecules&nbsp;</h2>



In much the same way that every person has a distinct fingerprint, celestial bodies like comets and the Sun possess characteristic isotopic signatures.



By comparing the oxygen isotope ratios against those known signatures, researchers can pinpoint where the water molecules came from.



The results of the rock analysis indicate that most of the Moon’s water likely formed within the Moon itself or arrived through comet collisions, not primarily via the solar wind. This challenges earlier assumptions that solar wind interactions might be a dominant water source.



<h2 class="wp-block-heading" id="h-human-presence-on-the-moon">Human presence on the Moon</h2>



The findings offer critical insights to agencies such as NASA, which intends to establish a sustained human presence on the Moon through the Artemis program.&nbsp;



Determining water’s precise locations and its most likely origins will help mission planners decide where best to set up long-term habitation.



“This kind of work hasn’t been done before and we think it can provide NASA with some valuable clues about where water is located on the moon,” Mark Thiemens said. “The real goal of Artemis is to get to <a href="https://www.earth.com/news/wave-ripples-discovered-mars-surface-indicate-liquid-water-present-4-billion-years-ago/" target="_blank" rel="noreferrer noopener">Mars</a>. Our research shows that there is likely at least as much water on Mars as on the moon, if not more.”



<h2 class="wp-block-heading" id="h-practical-challenges-and-future-innovations">Practical challenges and future innovations</h2>



Although finding and analyzing lunar water sources marks a major step, effectively extracting and utilizing water to support human communities on the Moon is another challenge entirely.&nbsp;



Researchers will need to develop robust technology for large-scale water extraction, as well as systems to ensure that the water is potable or otherwise suitable for use in life support.



Questions such as whether the water requires purification and how to store it in sufficient quantities remain to be addressed. These solutions will be pivotal for enabling off-planet growth, ultimately extending beyond the Moon to Mars and other parts of the solar system.



<h2 class="wp-block-heading" id="h-significance-of-the-study">Significance of the study</h2>



By identifying the potential locations and likely origins of lunar water, this study paves the way toward human settlements on the Moon, an idea once confined to science fiction.&nbsp;



Through the synergy of advanced isotopic measurements, decades of lunar rock analysis, and forward-looking mission planning, researchers and space agencies are inching closer to making lunar colonization a reality.



Armed with fresh scientific data and improved extraction techniques, future explorers may soon find themselves sustainably living on the Moon.



The study is detailed in a special issue of the journal <a href="http://dx.doi.org/10.1073/pnas.2321069121" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a> (PNAS) under the theme “Water on the Moon and Mars.”&nbsp;



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Experts are searching for viable sources of water on the Moon

As humanity strives to establish communities on the Moon, Mars,...

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....

Chlorella vulgaris is a small species of microalga that is rapidly becoming the new champion in superfoods. It combines high nutritional power with sustainable production methods and may represent a game-changer in terms of global food security.



Could this little green powerhouse be the future of sustainable nutrition? Science is starting to say yes.



<h2 class="wp-block-heading" id="h-chlorella-vulgaris-is-a-nutritional-powerhouse">Chlorella vulgaris is a nutritional powerhouse</h2>



This tiny <a href="https://www.earth.com/news/arctic-microalgae-show-photosynthesis-is-possible-in-near-darkness/" target="_blank" rel="noreferrer noopener">microalga</a> is abundant in freshwater habitats and uses sunlight and carbon dioxide to manufacture its own food, even though its entire body consists of only a single cell. 



Previous <a href="https://www.jstor.org/stable/3106856?origin=crossref">research</a> has found that Chlorella vulgaris cells contain almost 50% protein, along with a healthy supply of fats, carbohydrates, and various vitamins and minerals.



This makes algae a go-to <a href="https://www.earth.com/news/algae-may-be-the-future-of-sustainable-superfoods/" target="_blank" rel="noreferrer noopener">superfood</a> for our increasingly health-conscious society. Not only is it rich in nutrients, but its cultivation requires minimal land and water use. 



Thus, it is a way to reduce our environmental footprint while eating without concerns about animal cruelty or damage to the planet.



<h2 class="wp-block-heading" id="h-healthy-for-body-and-environment">Healthy for body and environment</h2>



Its environmental friendliness is not the end of its superpowers - it also has antioxidant properties and supports immune function, making it an attractive, nutrient-dense addition to food products.



It is currently marketed on a small scale in tablet and powder form, as a food supplement.



In this current wave of health and eco-conscious awakening, a team of scientists from the <a href="https://www.birmingham.ac.uk/" target="_blank" rel="noreferrer noopener">University of Birmingham</a> have investigated the potential of Chlorella vulgaris as a large-scale source of nutrients for humans.



“Chlorella vulgaris could be one of the superfoods that redefine the future of food innovation,” they state. However, they caution that realizing this potential food revolution will not be without hurdles.



<h2 class="wp-block-heading" id="h-overcoming-challenges-for-widespread-adoption">Overcoming challenges for widespread adoption</h2>



The researchers acknowledge the need for further development in various areas. 



From refining cultivation techniques to processing methods that can enhance its appeal to the average consumer's palate, the future is ripe with opportunities for growth. 



“Our study underscores the critical role of applied research in addressing <a href="https://www.earth.com/news/vaccinating-plants-could-boost-global-food-security/" target="_blank" rel="noreferrer noopener">global food security</a> challenges while promoting environmental sustainability,” shared Dr. Helen Onyeaka, a co-author of the study.



The bright future of this microalga is dependent on continued technological advances, which can improve the efficiency of production and broaden its adoption among food producers.



The researchers note that the key to success involves enhancing strains of C. vulgaris using genetic modification and improving cultivation systems. They propose that the development of new culture systems could increase yields and cut costs.



Furthermore, they recommend the use of diverse bioreactors that allow for the tweaking of light and nutrient parameters in order to maximize yield in sterile conditions.



<h2 class="wp-block-heading" id="h-innovations-for-a-better-future">Innovations for a better future</h2>



In order to unlock the full potential of Chlorella vulgaris as a <a href="https://www.earth.com/news/study-confirms-that-broccoli-is-a-superfood/" target="_blank" rel="noreferrer noopener">mainstream superfood</a>, significant advances in processing and cultivation are essential.



Various techniques, such as mechanical milling and ultrasonication, can significantly increase nutrient accessibility, making this micro-organism's rich protein and vitamin content more bioavailable.



Additionally, advanced techniques such as pulsed electric fields can improve digestibility while retaining the production costs within economically acceptable limits. 



Sensory evaluations and consumer testing play a crucial role in refining the taste and texture of the final products, so that it is palatable and appealing to a wide audience.



As scientists continue to refine these processes, Chlorella vulgaris is poised to transition from a niche supplement to a widely accepted dietary staple that merges nutrition, sustainability, and food security into a single, green solution.



<h2 class="wp-block-heading" id="h-chlorella-vulgaris-a-superfood-with-far-reaching-benefits">Chlorella vulgaris: A superfood with far-reaching benefits</h2>



Chlorella vulgaris is not only a promising addition to the food industry but also a powerful tool in <a href="https://www.earth.com/news/increasing-plant-extinction-threatens-the-future-of-medicine-and-human-health/" target="_blank" rel="noreferrer noopener">medicine</a> and environmental sustainability.



Studies suggest it may aid in cholesterol reduction, cancer prevention, and neuroprotection against some diseases, including Alzheimer’s.



Its antioxidant and immune-boosting properties make it a compelling candidate for future medical research.



Additionally, this microalga contributes to sustainability by absorbing carbon dioxide, supporting carbon sequestration, and helping to purify wastewater through its ability to remove heavy metals and toxins. 



With continued research and technological advances, Chlorella vulgaris could become a cornerstone of health, industry, and environmental solutions, paving the way for a more <a href="https://www.earth.com/news/nature-inspires-solutions-for-a-sustainable-future/" target="_blank" rel="noreferrer noopener">sustainable future</a>.



The full study was published in the <a href="https://research.birmingham.ac.uk/en/publications/ichlorella-vulgarisi-as-a-food-substitute-applications-and-benefi" target="_blank" rel="noreferrer noopener">Journal of Food Science</a>.



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This nutritional powerhouse is shaping up to be the next big 'superfood'

Chlorella vulgaris is a small species of microalga that is...

Octopuses have long fascinated scientists with their intelligence, camouflage abilities, and unique biology. 



These remarkable creatures continue to surprise researchers, revealing new secrets about their evolutionary past. One of the most intriguing mysteries has been the question of how octopuses determine their sex.



Scientists at the University of Oregon recently identified a sex chromosome in the California two-spot octopus. This discovery confirms that cephalopods, a group that includes squid and nautiluses, rely on chromosomes for sex determination. 



The research also suggests that this chromosome has existed for at least 480 million years, making it one of the oldest known sex chromosomes in the <a href="https://www.earth.com/news/turquets-octopus-dna-tells-scientists-that-west-antarctic-ice-sheet-collapse-is-close/" target="_blank" rel="noreferrer noopener">animal kingdom</a>.



<h2 class="wp-block-heading" id="h-sex-chromosome-in-octopuses">Sex chromosome in octopuses</h2>



“Cephalopods are already such interesting creatures, and there are so many things we’re still learning about them, especially in neuroscience,” said Gabby Coffing, a doctoral student at the <a href="https://www.uoregon.edu" target="_blank" rel="noreferrer noopener">University of Oregon</a>. 



“This is just showing one more interesting thing about them: They have really ancient sex chromosomes.”



The findings, published in the journal Current Biology, provide new insights into the genetic history of octopuses and their relatives. Understanding this ancient sex determination system could help scientists uncover more about how these intelligent <a href="https://www.earth.com/news/world-octopus-day-the-intelligent-creatures-of-the-sea/" target="_blank" rel="noreferrer noopener">creatures</a> evolved.



<h2 class="wp-block-heading" id="h-sex-determination-varies-across-species">Sex determination varies across species</h2>



Sex determination is not the same for all animals. While humans and most mammals rely on the X/Y chromosome system, other species follow different methods. 



In turtles, sex depends on the temperature at which the eggs incubate. Some fish determine sex using a single gene rather than a whole chromosome. 



Even in humans, sex chromosomes are not always straightforward. Gene mutations or extra sex chromosomes can lead to biological variations that do not fit into a simple male or female category.



Cephalopods have long posed a challenge for genetic research. They are not standard laboratory animals like mice or fruit flies, making it difficult for scientists to study their genetics in depth. 



Although researchers have sequenced the genomes of some octopus <a href="https://www.earth.com/news/octopus-suckers-the-future-of-underwater-adhesives/" target="_blank" rel="noreferrer noopener">species</a>, they still struggle to link specific genes to particular traits. The discovery of an octopus sex chromosome marks a major breakthrough in understanding how these animals develop and reproduce.



<h2 class="wp-block-heading" id="h-unique-sex-chromosome-in-female-octopuses">Unique sex chromosome in female octopuses</h2>



The research team at the University of Oregon made an unexpected discovery when sequencing the DNA of a female California two-spot octopus. 



Among its 30 chromosomes, one stood out because it contained only half the usual amount of genetic material. This anomaly had not appeared in previous studies of male octopus DNA.



“This particular chromosome had half the amount of sequencing data, which indicated there was only one copy,” Coffing explained. “Then as we explored that more, we reached the conclusion that we must have stumbled upon a sex chromosome.”



This finding suggested that female octopuses carry a unique chromosome that males do not. The scientists needed to confirm their discovery by comparing it with data from other cephalopods. 



If this chromosome appeared in multiple species, it would indicate an ancient and consistent pattern of sex determination.



<h2 class="wp-block-heading" id="h-sex-chromosome-exists-in-other-cephalopods">Sex chromosome exists in other cephalopods</h2>



The team analyzed genomic data from other octopus species and found similar evidence of this unique chromosome. 



The experts also detected the sex chromosome in squid, a species that diverged from octopuses between 248 and 455 million years ago. More surprisingly, they identified traces of it in the nautilus, a mollusk that split from the octopus lineage approximately 480 million years ago.



“This indicates that their common ancestor had this similar sex determination system,” Coffing said.



Most sex chromosomes change rapidly over time because they play a crucial role in reproduction. However, this cephalopod sex chromosome appears to have remained stable for hundreds of millions of years. 



This suggests that octopuses and their relatives have relied on this system without significant evolutionary changes.



<h2 class="wp-block-heading" id="h-comparing-ancient-sex-chromosomes">Comparing ancient sex chromosomes</h2>



While the octopus sex chromosome is one of the oldest known, other ancient sex chromosomes exist in nature. 



Some plants, like mosses and liverworts, evolved their sex chromosomes early in Earth’s history. Insects also have sex chromosomes that date back about 450 million years, though these have changed considerably over time.



The discovery in octopuses challenges the idea that sex chromosomes always evolve quickly. It suggests that some systems remain stable if they continue to work effectively over long periods. Cephalopods seem to have found a genetic formula for sex determination that has stood the test of time.



<h2 class="wp-block-heading" id="h-mystery-of-the-missing-w-chromosome">Mystery of the missing W chromosome</h2>



One question remains unanswered: how exactly does the sex determination system work in octopuses? Scientists initially suspected that octopuses might have a system similar to birds and butterflies, where males have two identical chromosomes (ZZ) and females have one of each (ZW).



Kern and his team searched for a W chromosome in female octopuses but didn't find one. This leaves open the possibility that octopuses follow a different system in which males have two copies of a single chromosome (ZZ), while females have only one (Z).



Researchers still need more evidence to confirm how octopus sex chromosomes function. While this study has solved one piece of the puzzle, many questions remain.



<h2 class="wp-block-heading" id="h-secrets-of-the-octopus">Secrets of the octopus </h2>



Octopuses continue to be one of the most enigmatic creatures in the ocean. Their <a href="https://www.earth.com/news/the-octopus-has-mastered-the-art-of-multispecies-hunting/" target="_blank" rel="noreferrer noopener">intelligence</a>, problem-solving skills, and unique genetics set them apart from most other animals. 



The discovery of an ancient sex chromosome adds another layer to their <a href="https://www.earth.com/news/what-animal-will-replace-humans-as-earths-dominant-species-this-scientist-has-an-idea/" target="_blank" rel="noreferrer noopener">evolutionary story</a>. For now, researchers know that this octopus sex chromosome has been around for nearly half a billion years. However, the exact mechanics of how it works remain uncertain.



As scientists continue to explore cephalopod genetics, they will uncover more about how these fascinating animals developed their extraordinary traits.



The octopus has revealed one of its secrets, but it still holds on to many more.



The study is published in the journal <a href="https://www.cell.com/current-biology/fulltext/S0960-9822(25)00005-3" target="_blank" rel="noreferrer noopener">Current Biology</a>.



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Sex chromosome discovered in octopuses is 480 million years old

Octopuses have long fascinated scientists with their intelligence, camouflage abilities,...

Fungi are often overlooked in the grand tapestry of life, yet they play an essential role in ecosystems around the world. From decomposing organic matter to forming symbiotic relationships with plants and animals, fungi are nature’s silent architects. 



Recently, a discovery involving a fungus growing on a spider has added a new layer of understanding to the story of these remarkable organisms.



During this research, scientists identified a previously unknown <a href="https://www.earth.com/news/fungi-can-think-and-make-smart-decisions-without-a-brain/" target="_blank" rel="noreferrer noopener">species of fungus</a> that has been named in honor of a legendary figure in natural history. 



This discovery adds to our knowledge of fungal diversity and is a reminder of how much there is still to learn about the intricate connections between fungi and their hosts.



<h2 class="wp-block-heading" id="h-new-species-gibellula-attenboroughii">New species Gibellula attenboroughii</h2>



Dr. Harry Evans, an Emeritus Fellow at CAB International, led a team of researchers from institutions such as the <a href="https://snm.dk/en" target="_blank" rel="noreferrer noopener">Natural History Museum of Denmark</a> and the <a href="https://www.kew.org" target="_blank" rel="noreferrer noopener">Royal Botanical Gardens Kew</a>. 



The investigation began during the filming of the <a href="https://www.bbc.co.uk/programmes/p012msk2/episodes/guide" target="_blank" rel="noreferrer noopener">BBC Winterwatch series</a> in Northern Ireland, where a peculiar fungus was found growing on a spider.



Using both morphological and molecular evidence, the scientists confirmed that this fungus represented a novel species. 



In recognition of his profound impact on natural history programming, the team decided to name it after Sir David Attenborough.



"[The species is] named after the broadcaster and natural historian Sir David Attenborough, a pioneer of BBC natural history programs, who - in his role as controller of BBC 2 - helped to develop the Natural History Unit," noted Dr. Evans.



This led, indirectly, to the filming of the present nature series, during which the new species was first discovered.



<h2 class="wp-block-heading" id="h-gibellula-attenboroughii-and-spiders">Gibellula attenboroughii and spiders</h2>



The spider that hosted the fungus was later identified as Metellina merianae, an orb-weaving cave spider belonging to the family Tetragnathidae.



With the help of a local speleologist, the researchers extended their search and discovered more specimens of the newly named species, Gibellula attenboroughii, in cave systems across Northern Ireland and the Republic of Ireland. 



Interestingly, the fungus was also found to infect another spider species, Meta menardi, which occupies different ecological niches within the caves. 



Like the original specimen, which was located on the ceiling of a gunpowder store, all of the infected spiders were found on the roof or walls of the caves.



These typically reclusive creatures had abandoned their usual hiding spots or webs, and migrated to exposed areas before dying.



<h2 class="wp-block-heading" id="h-connection-to-zombie-ant-fungi">Connection to zombie-ant fungi</h2>



This behavior mirrors what has been observed in ants that are similarly infected by fungi of the genus Ophiocordyceps in Brazil's Atlantic rainforest. 



In those cases, the fungi manipulated their ant hosts to position themselves in locations ideal for spore dispersal, which led to the use of the term "zombie-ant fungi."



This phenomenon has captured the public's imagination, inspiring books, video games, and even the popular television series The Last of Us. 



Scientists have since identified behavioral-changing metabolites, such as dopamine, in cultures of zombie-ant fungi.



The discovery of similar behaviors in spiders infected by Gibellula attenboroughii suggests that these fungi may employ comparable mechanisms to control their hosts.



<h2 class="wp-block-heading" id="h-fungus-and-spiders-in-the-british-isles">Fungus and spiders in the British Isles</h2>



Published in the journal Fungal Systematics and Evolution, the study went beyond identifying the new species. 



The researchers conducted extensive historical herbarium records and literature searches, and revealed a <a href="https://www.earth.com/news/secrets-of-fungi-diversity-can-be-pulled-out-of-thin-air/" target="_blank" rel="noreferrer noopener">hidden diversity</a> within the genus Gibellula in the British Isles.



The experts also uncovered evidence of widespread disease epidemics among spiders in Norfolk and Wales. 



The findings suggest that fungi like Gibellula attenboroughii may play a significant role in regulating spider populations.



"Their role in spider-population dynamics warrants further study, as do the metabolites they produce which enable them to exploit such a highly specific ecological niche," noted the researchers.



<h2 class="wp-block-heading" id="h-how-zombie-fungus-controls-spiders">How zombie fungus controls spiders</h2>



The discovery of Gibellula attenboroughii highlights the importance of studying fungi not only for their ecological roles but also for their potential applications. 



Understanding how these fungi influence spiders could provide insights into broader <a href="https://www.earth.com/news/tipping-point-discovered-in-fungi-evolution-that-impacts-their-shape-and-growth-rate/" target="_blank" rel="noreferrer noopener">ecological dynamics</a>.



For instance, if certain fungi regulate spider numbers, they might indirectly affect other species within the <a href="https://www.earth.com/news/rare-frost-beard-ice-formation-exidiopsis-effusa-fungi-discovered-by-hiker/" target="_blank" rel="noreferrer noopener">ecosystem</a>. 



Additionally, investigating the metabolites produced by these fungi could lead to discoveries with implications beyond ecology. 



Such compounds might have pharmaceutical or industrial uses, which makes this area of research particularly promising.



<h2 class="wp-block-heading" id="h-tribute-to-sir-david-attenborough">Tribute to Sir David Attenborough</h2>



Naming the fungus after <a href="https://www.imdb.com/name/nm0041003/" target="_blank" rel="noreferrer noopener">Sir David Attenborough</a> serves as a fitting tribute to his lifelong dedication to exploring and sharing the wonders of the natural world. 



His work has inspired countless individuals, including the scientists involved in this study, to examine the mysteries of <a href="https://www.earth.com/news/deadly-fungus-found-in-garden-soils-across-america/" target="_blank" rel="noreferrer noopener">nature</a>. 



By honoring Sir Attenborough in this way, the researchers not only celebrate his contributions but also emphasize the interconnectedness of scientific discovery and public engagement. It is a reminder that science thrives when curiosity is shared and nurtured.



<h2 class="wp-block-heading" id="h-why-is-gibellula-attenboroughii-important">Why is Gibellula attenboroughii important?</h2>



The identification of Gibellula attenboroughii opens up numerous avenues for future research. Scientists are eager to explore how these fungi manipulate their hosts and what chemical compounds they produce to achieve such precise control. 



Furthermore, understanding the role of fungi in regulating spider populations could provide valuable insights into ecosystem stability.



In a time when biodiversity is under threat, studies like this remind us of the importance of preserving ecosystems and the species within them. 



The study is published in the journal <a href="https://www.ingentaconnect.com/content/wfbi/fuse/pre-prints/content-f1_fuse_vol15_art7;jsessionid=dd632sclfekn9.x-ic-live-03" target="_blank" rel="noreferrer noopener">Fungal Systematics and Evolution</a>.



Image Credit: CABI



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Newfound fungus infects and controls spiders, turning them into "zombies"

Fungi are often overlooked in the grand tapestry of life,...

<div class="wp-block-sendtonews-playerselector">[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"]</div>



Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Nushagak Bay, a large estuary in southwest Alaska. Nushagak runs mainly north to south and exits in Bristol Bay, a large body of water in the Bering Sea.



"The bay is primarily fed by the Nushagak River, which begins in the Alaska Range and flows southwest approximately 450 km. The bay is also fed by several additional rivers including the Wood, Igushik, Snake and Weary rivers," says ESA.



"The dark colors of the Nushagak River are most likely due to tannins or lignins (chemical substances found in plants). Tannins and lignins from roots, leaves, seeds, bark and soil can leach into the water and give it a brown or even black colour. The sediments then flow southwards where it is mixed with the bluer waters of the bay."



Video/ Image Credit: ESA



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Nushagak Bay in southwest Alaska

[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"] Today’s Video of the Day from the...

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> (ACS) reveals that proteins on flu viruses are actually flexible, tilting and waving in a “breath-like” motion. According to the experts, these proteins could be used to better defend against the flu.



"The main antigenic targets of influenza virus are two surface glycoproteins, hemagglutinin (HA) and neuraminidase (NA). Whereas the structural and dynamical properties of both glycoproteins have been studied previously, the understanding of their plasticity in the whole-virion context is fragmented," wrote the researchers.



To investigate, the team conducted detailed simulations of the influenza A H1N1 virion, or the swine flu. The experts concluded that the visualizations show many new vulnerable states of flu viruses, which could improve future vaccines and antiviral drugs.



Video/ Image Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Flu viruses are more flexible than expected

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Lake Trasimeno, which is located west of Perugia in central Italy. It is the fourth largest lake in the country. While Trasimeno’s water level varies, it has a maximum depth of approximately six meters.&nbsp;



"In this Copernicus Sentinel-2 image, captured on 6 August 2022, the lake’s emerald green colour is likely due to the presence of phytoplankton. Streaks in the water, particularly visible in the west, indicate the presence of soil and sediments which have been stirred up by winds. Dark colored waters in the southern part of the lake indicate a presence of submerged and floating macrophytes (aquatic plants) as well as algae," says ESA.



"Surrounded by hills on three sides, Trasimeno is subject to heavy storms created by winds, especially from the north and west. There are three islets in the lake: Maggiore, Minore and Polvese (the largest). The lake’s shores are sparsely inhabited with only two popular villages: Castiglione del Lago and Passignano sul Trasimeno."



"Italy is experiencing its worst drought in 70 years which has affected drinking water supplies, hydroelectric power and agricultural production. High temperatures, hot winds and lack of rainfall are the main causes of drought in the Umbrian region which saw Lake Trasimeno’s drop 1.3 m, reaching the limit of the hydrometric zero in July 2022."



Video/Image Credit: ESA&nbsp;



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By <a href="http://csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer

Lake Trasimeno in Central Italy

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Today's Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> describes a new self-powered nanosensor that can instantly detect mercury contamination with the tap of a finger.&nbsp;



The oxidized form of mercury can be harmful when it is ingested through contaminated water or food. This makes it necessary for experts to develop sensors that can quickly and accurately detect the presence of mercury.&nbsp;



Zong-Hong Lin and colleagues have now created a triboelectric nanosensor (TENS) that can detect mercury by simply by touching a sample. According to the researchers, their TENS could serve as the basis for similar devices to safely and remotely monitor other pollutants.



Video Credit: American Chemical Society&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Detecting mercury contamination with the tap of a finger

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Kainji Lake, a reservoir on the Niger River.



In 1968, Kainji Lake was created by the construction of the Kainji Dam. The Niger River, the third longest in Africa, enters the lake in the north.&nbsp;



According to <a href="https://www.earth.com/news/rivers-in-the-american-west-are-a-lifesaving-resource-for-birds/">ESA</a>, the creation of the lake submerged Foge Island and the town of Bussa and permanently flooded other riverine settlements, leaving around 50,000 people displaced.&nbsp;



Large parts of Foge Island are temporarily exposed during low water tides, and the land is often used by migrating fishermen. Kainji Dam is a dam across the Niger River in Niger State of Central Nigeria. 



Wild mammals occur at relatively low densities due to illegal hunting. Lake Kainji has suffered a dramatic decline as a fishery due to the high numbers of artisanal and subsistence fisherfolk using the lake. It has been suggested that a period of closure, together with controlled fishing rights may help improve fish stocks.



Kainji Lake National Park is the oldest of its kind in Nigeria. The park contains three distinct areas: a part of the Kainji Lake, the Borgu Game Reserve to the west of the lake, and the Zugurma Game Reserve to the southeast. The park is home to around 65 mammal species, 350 bird species, and 30 species of reptiles and amphibians. 



Video/ Image Credit: European Space Agency&nbsp;



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Kainji Lake in north central Nigeria

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Today’s Video of the Day from <a href="https://www.igb.illinois.edu/">Carl R. Woese Institute for Genomic Biology</a> reveals how scientists can modify common crops like soybean, rice, and wheat to protect them from heat stress.



“We need to double crop production by 2050 to feed a growing global population, and not only are we not on track to do that, but climate change is further complicating things,” said Amanda Cavanagh, a lecturer at the University of Essex. 



The study is part of Realizing Increased Photosynthetic Efficiency (RIPE), an international research project that aims to develop food crops that turn the sun’s energy into food more efficiently.



“Using an engineering approach we designed multiple alternative metabolic pathways to photorespiration. Testing them in the field showed increases in productivity which led Amanda to significantly move the project forward by showing our engineered plants can withstand pretty extreme temperature stress,” said study co-author and RIPE researcher Paul South.&nbsp;



“As the climate changes and temperature stresses increase the pressure on our global food supply, farmers will need every tool available including engineering approaches like the synthetic biology used here to maintain safe and productive harvests.”



The experts tested plants modified to have more efficient photorespiration to see if they were better adapted to warmer temperatures.&nbsp;



The team found that the engineered plants produced 26 percent more biomass than the wild-type plants exposed to the same temperatures, and had 15 percent less yield loss under the higher temperatures.



Video Credit: Amanda Nguyen/University of Illinois



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By <a href="mailto:csexton@earth.com">Chrissy Sexton</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Editor



Check us out on <a href="https://www.earth.com/earthsnap/">EarthSnap</a>, a free app brought to you by Eric Ralls and Earth.com.

Designing crops that can beat the heat

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Suka was drawn away from the shelter, which bought the workers enough time to grab Laerke. That must have been tense! Once they had the sickly cub, she was then transported to Detroit Zoo’s Ruth Roby Glancy Animal Health Complex. She was given a thorough check-up, before receiving “around-the-clock care.” Photo Credit: ROLF VENNENBERND/DPA/AFP via Getty Images

Around-the-clock care