Today's Image of the Day from the <a href="https://www.eso.org/public/">European Southern Observatory</a> (ESO) features a stunning view of the Sculptor Galaxy, one of the brightest spiral galaxies visible from Earth.



The ultra-detailed image, which was captured using ESO’s Very Large Telescope, reveals features in the Sculptor Galaxy that have never been seen before.&nbsp;



ESO researcher Enrico Congiu led a new study on the Sculptor Galaxy that is published in the journal Astronomy &amp; Astrophysics.&nbsp;



<h2 class="wp-block-heading" id="h-a-galaxy-wide-view-of-sculptor-nbsp">A galaxy-wide view of Sculptor&nbsp;</h2>



The team observed the galaxy in thousands of wavelengths at once, collecting an immense amount of data from every point across its structure. This allowed them to build a comprehensive, galaxy-wide view of how <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/">stars</a> live and evolve within Sculptor.



"Galaxies are incredibly complex systems that we are still struggling to understand," said Congiu.



“The Sculptor Galaxy is in a sweet spot. It is close enough that we can resolve its internal structure and study its building blocks with incredible detail, but at the same time, big enough that we can still see it as a whole system.”



<h2 class="wp-block-heading" id="h-thousands-of-distinct-colors-nbsp">Thousands of distinct colors&nbsp;</h2>



<a href="https://www.earth.com/news/oxygen-detected-in-the-most-distant-and-primitive-galaxy-ever-analyzed/">Galaxies</a> span hundreds of thousands of light-years, yet their evolution is shaped by processes unfolding on much smaller scales.&nbsp;



The fundamental components of a galaxy - stars, gas, and dust - each emit light in distinct colors. The more shades of color captured in an image, the deeper the insight into a galaxy’s internal structure.&nbsp;



Traditional images typically contain only a few colors, but the new map of the Sculptor Galaxy includes thousands.&nbsp;



This rich spectrum provides astronomers with detailed information about the galaxy’s stars, gas, and dust - from their ages and chemical makeup to how they’re moving through space.



<h2 class="wp-block-heading" id="h-mapping-the-sculptor-galaxy-nbsp">Mapping the Sculptor Galaxy&nbsp;</h2>



The research team spent more than 50 hours observing the Sculptor Galaxy using the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope.&nbsp;



To capture the full view - spanning roughly 65,000 light-years - they combined over 100 separate exposures into a single, detailed mosaic.&nbsp;



According to study co-author Kathryn Kreckel from Heidelberg University, Germany, this makes the map a potent tool.&nbsp;



“We can zoom in to study individual regions where stars form at nearly the scale of individual stars, but we can also zoom out to study the galaxy as a whole,” said Kreckel.&nbsp;



<h2 class="wp-block-heading" id="h-hundreds-of-planetary-nebulae-nbsp">Hundreds of planetary nebulae&nbsp;</h2>



In their initial analysis of the data, the team identified around 500 planetary <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/">nebulae</a> scattered throughout the Sculptor Galaxy.



Study co-author Fabian Scheuermann, a doctoral student at Heidelberg University, emphasized the significance of the discovery.&nbsp;



Scheuermann noted that when astronomers study galaxies outside of our own cosmic neighborhood, they normally detect fewer than 100 planetary nebulae in each one.&nbsp;



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



The Sculptor Galaxy, also known as NGC 253, is located about 11.4 million light-years away in the constellation Sculptor. It’s classified as a starburst galaxy, meaning it’s undergoing an exceptionally high rate of <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/">star formation</a>.&nbsp;



This vigorous star-making activity is especially intense in its central regions, where dense clouds of gas and dust feed the birth of new stars.&nbsp;



The galaxy is tilted at a steep angle from our perspective, which gives it a striking, elongated appearance when viewed through telescopes.



<h2 class="wp-block-heading" id="h-notable-features-of-the-sculptor-galaxy-nbsp">Notable features of the Sculptor Galaxy&nbsp;</h2>



Discovered in 1783 by Caroline Herschel, the Sculptor Galaxy has become a popular target for both professional astronomers and amateur skywatchers due to its brightness and relative proximity.&nbsp;



It’s part of the Sculptor Group, one of the nearest groups of galaxies to our Local Group. Despite being rich in star-forming regions, much of its inner structure is veiled by thick dust lanes.&nbsp;



However, infrared and X-ray observations have helped scientists peer through the obscuring material to study the galaxy’s core, revealing a wealth of activity including supernova remnants and a possible central <a href="https://www.earth.com/news/largest-ultramassive-black-hole-ever-seen-cosmic-horseshoe-lrg-3-757/">black hole</a>.



The Sculptor Galaxy is also notable for its extended halo of stars and gas, which suggests past interactions or mergers with smaller galaxies.&nbsp;



This halo, along with its active central region, makes NGC 253 a valuable subject for understanding how galaxies evolve, form stars, and recycle gas over time. Its combination of beauty and scientific richness continues to make it a focus of galactic studies.



Image Credit: European Southern Observatory&nbsp;



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Thousands of colors in the Sculptor Galaxy

Today's Image of the Day from the European Southern Observatory (ESO) features a stunning view of the Sculptor Galaxy, one of the brightest spiral galaxies visible from Earth. The ultra-detailed image, which was captured using ESO’s Very Large Telescope, reveals features in the Sculptor Galaxy that have never been seen before.&nbsp; ESO researcher Enrico Congiu led a new study on the Sculptor Galaxy that is published in the journal Astronomy &amp; Astrophysics.&nbsp; A galaxy-wide view of Sculptor&nbsp; The team observed the galaxy in...

Today's Image of the Day from the European Space Agency features a stunning reflection nebula known as GN 04.32.8 in the constellation Taurus.



Reflection nebulae are cosmic clouds of fine dust that become visible not by producing their own light, but by reflecting the light of nearby stars.&nbsp;



Unlike emission <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/">nebulae</a>, which glow due to ionized gases radiating light, reflection nebulae shine more subtly.&nbsp;



The light from nearby stars strikes the dust particles within the cloud and scatters in many directions - especially shorter, bluer wavelengths. This scattering effect, similar to the way Earth’s sky appears blue, often gives reflection nebulae their characteristic bluish hue.



<h2 class="wp-block-heading" id="h-the-taurus-molecular-cloud">The Taurus Molecular Cloud</h2>



“GN 04.32.8 is a small part of the stellar nursery known as the Taurus Molecular Cloud. At only roughly 480 light-years from Earth in the constellation Taurus, it's one of the best locations for studying newly forming stars,” noted <a href="https://www.esa.int/ESA_Multimedia/Images">ESA</a>.



The Taurus Molecular Cloud is one of the closest and most extensively studied regions for low-mass star formation.&nbsp;



Unlike larger star-forming regions like <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/">Orion</a> that produce many high-mass stars, the TMC is dominated by the formation of Sun-like and smaller stars, making it a prime analog for understanding the conditions that led to the birth of our own solar system.



<h2 class="wp-block-heading" id="h-energetic-stars-in-the-constellation-taurus-nbsp">Energetic stars in the constellation Taurus&nbsp;</h2>



“This reflection nebula is illuminated by the system of three bright stars in the center of this image, mainly the variable star V1025 Tauri in the very center.”&nbsp;



“One of those stars overlaps with part of the nebula: this is another variable star that is named HP Tauri, but is classified as a T Tauri star, for its similarity to yet another variable star elsewhere in the Taurus Molecular Complex.”&nbsp;



T Tauri stars are young, energetic stars in the earliest stages of stellar evolution, just beginning their journey toward becoming stable main sequence stars like our <a href="https://www.earth.com/news/discovery-sun-like-stars-with-secret-companions/">Sun</a>.&nbsp;



These stars are highly variable and surrounded by dense clouds of gas and dust, often exhibiting strong stellar winds and flares as they settle into equilibrium.&nbsp;



<h2 class="wp-block-heading" id="h-a-dynamic-star-system">A dynamic star system</h2>



In this case, the trio of T Tauri stars - named HP Tau, HP Tau G2, and HP Tau G3 - are believed to be gravitationally bound, forming a dynamic triple star system.



“Eagle-eyed viewers might notice the small, squashed, orange spot, just left of center below the clouds of the nebula, that’s crossed by a dark line. This is a newly-formed protostar, hidden in a <a href="https://www.earth.com/news/planet-forming-disks-surrounding-stars-often-last-much-longer-than-expected/">protoplanetary disc</a> that obstructs some of its light,” explained ESA.



“Because the disc is edge-on to us, it’s an ideal candidate for study. Astronomers are using Hubble here to examine it closely, seeking to learn about the kinds of exoplanets that might be formed in discs like it.”



<h2 class="wp-block-heading" id="h-the-light-of-hot-young-stars">The light of hot, young stars</h2>



Reflection nebulae are usually found in regions where new <a href="https://www.earth.com/news/10-billion-white-dwarf-stars-in-milky-way-galaxy-might-have-habitable-planets/">stars</a> are forming, often near or within dense molecular clouds.&nbsp;



Some reflection nebulae can span light-years across and serve as markers of stellar nurseries - places where future generations of stars are taking shape.



Reflection nebulae offer astronomers a valuable glimpse into the structure and composition of the interstellar medium and help trace the life cycles of stars from birth to maturity.



<h2 class="wp-block-heading" id="h-examples-of-reflection-nebulae-nbsp">Examples of reflection nebulae&nbsp;</h2>



One well-known example is the reflection nebula surrounding the Pleiades star cluster, also called the Seven Sisters.&nbsp;



The Iris Nebula, located in the constellation Cepheus about 1,300 light-years from Earth, is a striking reflection nebula illuminated by the young star SAO 19158.



This Nebula is a popular target for astrophotographers due to its vivid colors and intricate structure.



Found about 1,600 light-years away, M78 is the brightest reflection nebula in the Orion constellation and one of the easiest to observe with amateur telescopes. It’s illuminated by two young stars, HD 38563A and HD 38563B.&nbsp;



M78 is part of a larger complex of gas and dust that includes many other star-forming regions within the Orion Molecular Cloud.



Image Credit: ESA&nbsp;



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Young stars illuminate a reflection nebula in Taurus 

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

Today's Image of the Day from the European Space Agency features Messier 82, a starburst galaxy located in the constellation Ursa Major. This galaxy is actively forming new stars at a rate ten times that of the Milky Way.



In a study using the <a href="https://webb.nasa.gov/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> (JWST), an international team of astronomers has taken an unprecedented look at Messier 82 (M82), revealing intricate details about its frenzied star formation.&nbsp;



<h2 class="wp-block-heading" id="h-the-power-of-nircam">The power of NIRCam</h2>



The study, led by Alberto Bolatto, utilized Webb’s Near-Infrared Camera (NIRCam) to penetrate the thick dust and gas covering the galaxy's core, a region critical to understanding <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>.&nbsp;



"M82 has garnered a variety of observations over the years because it can be considered as the prototypical starburst galaxy," noted Bolatto. “With Webb’s size and resolution, we can look at this star-forming galaxy and see all of this beautiful new detail.”



Webb's NIRCam has proven crucial for observing areas like M82’s center, where layers of dust typically obscure the view in other wavelengths. The camera's ability to capture infrared light allows it to reveal the galaxy's core and its dynamic processes.&nbsp;



<h2 class="wp-block-heading" id="h-messier-82-image">Messier 82 image </h2>



“This image shows the power of Webb. Every single white dot in this image is either a star or a star cluster. We can start to distinguish all of these tiny point sources, which enables us to acquire an accurate count of all the star clusters in this galaxy,” noted study co-author Rebecca Levy from the University of Arizona.



One of the NIRCam's innovative features is its mode that prevents bright sources from overwhelming the detector, which was particularly useful in studying the intensely active center of Messier 82.&nbsp;



In the image, dark brown tendrils of dust weave through the galaxy's glowing white core, interspersed with small green specks that represent concentrated areas of iron from <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> remnants. Red patches highlight regions where molecular hydrogen is illuminated by the radiation from nearby young stars.



<h2 class="wp-block-heading" id="h-insights-into-galactic-winds">Insights into galactic winds</h2>



The study also focused on understanding how <a href="https://www.earth.com/news/spin-of-a-new-black-hole-is-unlocking-galactic-mysteries/" target="_blank" rel="noreferrer noopener">galactic wind</a>, driven by the rapid rate of star formation and subsequent supernovae, influences M82’s environment. 



The NIRCam images showed clumpy streams of gas, appearing in red, which extend above and below the galaxy's plane, marking the path of this wind rushing out from the starburst's core.



A key revelation came from the NIRCam’s tracing of polycyclic aromatic hydrocarbons (PAHs), sooty chemical molecules that map out the structure of the galactic wind. 



To the surprise of researchers, the PAH emissions closely resembled the patterns of the hot, ionized gas, suggesting a more complex interaction within the wind than previously understood. 



"It was unexpected to see the PAH emission resemble ionised gas," said Bolatto. "PAHs are not supposed to live very long when exposed to such a strong radiation field, so perhaps they are being replenished all the time. It challenges our theories and shows us that further investigation is required."



<h2 class="wp-block-heading" id="h-future-observations-of-messier-82">Future observations of Messier 82</h2>



The findings from Webb are just the beginning. The team plans to further analyze Messier 82 with additional data, including spectroscopic observations, to determine the ages of the <a href="https://www.earth.com/news/galaxy-collisions-hubble-spots-a-string-of-pearls-star-cluster/" target="_blank" rel="noreferrer noopener">star clusters</a> and the duration of each star formation phase within the starburst environment.&nbsp;



These observations will also assist in a broader understanding of similar processes in early <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a>, which were common in the young universe.



<h2 class="wp-block-heading" id="h-broader-implications-of-the-study">Broader implications of the study</h2>



Study co-author Torsten Böker of the <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a> emphasized the broader implications of these findings.&nbsp;



“With these amazing Webb images, and our upcoming spectra, we can study how exactly the strong winds and shock fronts from young stars and supernovae can remove the very gas and dust from which new stars are forming,” explained Böker.&nbsp;



“A detailed understanding of this ‘feedback’ cycle is important for theories of how the early universe evolved, because compact starbursts such as the one in M82 were very common at high redshift.”



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



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Messier 82: Unlocking the mysteries of star formation

Today's Image of the Day from NASA Earth Observatory features a blanket of dust over the Tarim Basin - a vast, arid region in northwestern China. 



Mountain peaks are visible through a break in the dust. These peaks are part of Tekilik Shan, a subrange of the Kunlun Mountains.



Though not as widely known as some other mountain ranges in the area, Tekilik Shan plays a significant role in shaping local <a href="https://www.earth.com/news/extreme-weather-is-pushing-nature-toward-a-breaking-point/" target="_blank" rel="noreferrer noopener">weather</a> patterns and geography.



Its snow-covered peaks can rise above 13,000 feet, contributing to the dramatic elevation differences that define the basin’s borders.



<h2 class="wp-block-heading" id="h-dust-storms-in-the-tarim-basin-nbsp">Dust storms in the Tarim Basin&nbsp;</h2>



Spring marks the height of <a href="https://www.earth.com/news/sahara-desert-dust-storms-carry-harmful-bacteria-and-fungi-around-the-globe/" target="_blank" rel="noreferrer noopener">dust storm</a> activity in the Tarim Basin, particularly in its southern region.&nbsp;



“It’s a time of year when regional wind patterns shift in ways that cause winds and storm systems to sweep in from the northwest,” noted <a href="https://earthobservatory.nasa.gov/images/154126/a-curtain-of-dust-over-the-tarim-basin" target="_blank" rel="noreferrer noopener">NASA</a>.



“In early spring, when landscapes in this region are especially dry and have minimal vegetation, land surfaces warm rapidly under the Sun’s heat every morning, fueling convection that can help loft dust upward by the afternoon.”



<h2 class="wp-block-heading" id="h-fingerlike-dust-formations-nbsp">Fingerlike dust formations&nbsp;</h2>



Satellite images revealed dust formations with fingerlike shapes that mirrored the landscape below. These projections aligned with valleys, which channeled and directed the airborne dust.&nbsp;



Ralph Kahn is an atmospheric scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder and scientist emeritus at NASA’s Goddard Space Flight Center.



According to Kahn, the dust may have been “self-lofting.” In this process, sunlight heats recently stirred-up surface dust, creating pockets of convection that lift it even higher into the air.



This interpretation is supported by hourly observations from Japan’s Himawari-9 geostationary satellite, which showed dust gradually rising into the Tekilik Shan throughout the day. By late afternoon, the storm had grown dense enough to obscure the mountains.&nbsp;



<h2 class="wp-block-heading" id="h-decline-in-atmospheric-dust">Decline in atmospheric dust</h2>



Long-term satellite data from MODIS suggest that <a href="https://www.earth.com/news/dust-storms-in-the-gulf-of-alaska-help-shape-the-global-climate/" target="_blank" rel="noreferrer noopener">atmospheric dust</a> levels in this region have declined by about 1.5 percent each year since the early 2000s.&nbsp;



NASA researcher Hongbin Yu attributes this trend mainly to springtime changes - such as altered wind speeds, <a href="https://www.earth.com/news/how-soil-moisture-can-predict-severe-storms/" target="_blank" rel="noreferrer noopener">soil moisture</a>, or vegetation cover - rather than shifts in other seasons.



<h2 class="wp-block-heading" id="h-rainfall-in-the-tarim-basin-nbsp">Rainfall in the Tarim Basin&nbsp;</h2>



“The <a href="https://www.britannica.com/place/Takla-Makan-Desert" target="_blank" rel="noreferrer noopener">Takla Makan Desert</a> is one of the driest, most barren expanses on Earth. Flanked by mountain ranges on three sides and parched by the resulting <a href="https://glossary.ametsoc.org/wiki/Rain_shadow" target="_blank" rel="noreferrer noopener">rain shadow</a>, parts of the Tarim Basin receive no more than 10 millimeters (0.4 inches) of rain per year,” noted NASA.



“Dust storms can lead to public health problems in populated areas downwind by transporting small particles, bacteria, and viruses that infiltrate human respiratory systems.”&nbsp;



NASA added that dust storms can also affect Earth’s climate by scattering and absorbing incoming solar radiation and changing the properties of clouds.



<h2 class="wp-block-heading" id="h-landscape-of-the-tarim-basin-nbsp">Landscape of the Tarim Basin&nbsp;</h2>



The Tarim Basin is one of the largest endorheic basins in the world, meaning that its rivers do not drain into the sea but instead flow into interior lakes or evaporate.&nbsp;



The basin is encircled by three mountain ranges: the Tien Shan to the north, the Kunlun Mountains to the south, and the Pamirs to the west. These ranges create a powerful rain shadow effect, making the region exceptionally dry.



At the heart of the Tarim Basin lies the Taklamakan Desert, one of the most extreme deserts on Earth. The desert is known for its high dunes, intense temperature swings, and minimal <a href="https://www.earth.com/news/extreme-rainfall-will-wreak-havoc-on-mountain-ranges-as-warming-climate-turns-snow-to-rain/" target="_blank" rel="noreferrer noopener">rainfall</a>.



<h2 class="wp-block-heading" id="h-history-and-geology">History and geology</h2>



Despite its harsh environment, the basin has been historically significant. It was a key section of the ancient Silk Road, with several oases such as Kashgar, Khotan, and Loulan serving as vital trading and cultural centers for centuries.



Geologically, the basin is rich in natural resources, particularly oil and natural gas, and has become a focal point for China's energy exploration and development.&nbsp;



The region’s challenging climate and remote location, however, make infrastructure development and human habitation difficult.&nbsp;



The image was captured on March 27, 2025 by the Operational Land Imager instrument on Landsat 8.



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Blanket of dust covers China’s Tarim Basin

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

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.&nbsp;



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.&nbsp;



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



Messier 78 is a dynamic region of star formation that is obscured by cosmic dust in this high-resolution image captured by the Euclid space telescope.



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.&nbsp;



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">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 designed to study the dark universe, particularly focusing on dark energy and dark matter. These components are believed to drive the accelerating expansion of the universe and shape its large-scale structure. 



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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Young stars shine through dense dust

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



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



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



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



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



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



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



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. 



“Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA, J. Lee



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Starburst galaxy in the constellation Columba

Today's Image of the Day from the European Space Agency features a brilliant stellar nursery located about 163,000 light-years away.



According to ESA, the image is one of the most photogenic examples of the many stellar nurseries observed by the NASA/ESA Hubble Space Telescope during its 30-year lifetime. 



“The portrait features the giant nebula NGC 2014 and its neighbor NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



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



Stellar nurseries are regions in space where new stars are <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">born</a> - often within vast clouds of gas and dust called molecular clouds.&nbsp;



These areas are fascinating because they are cradles of stellar evolution, where gravity causes clumps of gas to collapse, eventually forming protostars.&nbsp;



Over time, the protostars will heat up and start the nuclear fusion process that powers a star.



One of the most well-known stellar nurseries is the Orion Nebula, which is visible to the naked eye and located about 1,350 light-years from Earth.&nbsp;



<h2 class="wp-block-heading" id="h-dynamic-nature-of-a-stellar-nursery-nbsp">Dynamic nature of a stellar nursery&nbsp;</h2>



Within these nurseries, the balance between gravity and pressure determines the types of stars that form, from massive, luminous stars to smaller, cooler ones like our Sun.&nbsp;



The environment is incredibly dynamic, with powerful winds from young stars shaping the clouds and triggering the birth of even more stars.



These regions are often illuminated by the light from massive newborn stars - creating stunning, colorful displays. The light reveals the intricate structure of the dust and gas, sculpted by the energy of young stars.&nbsp;



<h2 class="wp-block-heading" id="h-significance-of-stellar-nurseries-nbsp">Significance of stellar nurseries&nbsp;</h2>



Stellar nurseries are essential for understanding the early stages of planetary formation, as protoplanetary disks (the material from which <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planets form</a>) are often found around young stars in these regions.



Stellar nurseries play a crucial role in the ongoing evolution of <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">galaxies</a>. They are responsible for the continuous birth of new stars that enrich the interstellar medium with heavier elements. This constant recycling of material is key to the development of future generations of stars and planets.&nbsp;



Furthermore, the study of these regions helps astronomers understand the fundamental processes that govern the life cycles of stars and the overall dynamics of the universe.



<h2 class="wp-block-heading" id="h-the-local-group">The Local Group</h2>



The Local Group is a collection of over 80 galaxies that includes the Milky Way, the Andromeda Galaxy, and the Triangulum Galaxy, along with numerous smaller dwarf galaxies. These galaxies are bound together by gravity and span a region roughly 10 million light-years across.&nbsp;



The <a href="https://www.earth.com/news/milky-ways-thin-disk-is-billions-of-years-older-than-we-thought/" target="_blank" rel="noreferrer noopener">Milky Way</a> and Andromeda are the dominant members, with their respective satellite galaxies orbiting them.&nbsp;



The Local Group is part of a larger structure known as the Virgo Supercluster, and its galaxies are moving toward the gravitational center of the Local Group, contributing to its dynamic nature.&nbsp;



<h2 class="wp-block-heading" id="h-large-magellanic-cloud">Large Magellanic Cloud</h2>



The Large Magellanic Cloud (LMC) is the fourth largest galaxy in the Local Group and can be seen with the naked eye from the Southern Hemisphere.&nbsp;



This irregular dwarf galaxy is home to the Tarantula Nebula, one of the most active star-forming regions in our cosmic neighborhood.&nbsp;



The Large Magellanic Cloud played a key role in astronomical history, particularly when the supernova SN 1987A was observed, providing valuable insights into stellar evolution.&nbsp;



The LMC's interaction with the Milky Way, along with its own companion, the Small Magellanic Cloud, is believed to influence its shape and star formation activity. Its proximity and unique properties make it a crucial object of study for understanding <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>, star formation, and the dynamics of interacting galaxies.



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

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



"The data featured in this portrait make use of two of Webb’s instruments: the Mid-InfraRed Instrument (MIRI) and Near-InfraRed Camera (NIRCam)," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"Here MIRI captures the glow of interstellar dust grains, which trace out the interstellar medium, the fuel for future star formation. NIRCam shows the light from stars, even young stars hidden behind prodigious amounts of dust. NIRCam also captures emission from ionized nebulae around young stars."



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



According to ESA, the data was collected by the <a href="https://sites.google.com/view/phangs/home">PHANGS team</a> as part of a program in which Webb will observe 55 <a href="https://www.earth.com/news/james-webb-captures-galaxies-that-are-too-old-to-exist/">galaxies</a> that have also been mapped by the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope, the Hubble Space Telescope, and more.&nbsp;



"By combining Webb’s unprecedented view of the dust and stars with data from these other facilities, the team aims to obtain a new, highly detailed view of how stars are born, live, and die in galaxies across the Universe."



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



Although NGC 1559 appears to sit close to one of our nearest neighbors in the sky - the Large Magellanic Cloud (LMC) - this is just a trick of perspective, noted ESA.



While it is part of the Reticulum constellation, NGC 1559 is not part of the Local Group of galaxies but instead resides in a more distant region of space.



"In reality, NGC 1559 is physically nowhere near the LMC in space; in fact it truly is a loner, lacking the company of any nearby galaxies or membership of any galaxy cluster," said ESA.



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



NGC 1559 is notable for its active star formation and strong magnetic fields. It has also been the site of several <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, making it of particular interest to astronomers who study stellar evolution and the life cycle of stars.



The structure of NGC 1559 includes well-defined spiral arms that contain young, hot stars and regions of ionized gas, indicative of ongoing <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a>.



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



Despite being relatively small compared to larger galaxies like the Milky Way, NGC 1559 is an important object for understanding how barred spiral galaxies evolve and the processes that trigger supernovae.



The galaxy’s remote location and active nature make it a fascinating subject of study in the field of extragalactic astronomy. 



The isolation of NGC 1559 allows for a clearer view of its structure without much interference from neighboring galaxies.



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



Barred spiral galaxies are a type of spiral galaxy characterized by a central bar-shaped structure composed of stars. This bar extends out from the core and connects to the galaxy's spiral arms, which swirl outward in a graceful pattern.



Scientists believe that the bar plays a crucial role in the evolution of the galaxy, funneling gas towards the core and potentially triggering star formation or feeding a central black hole. 



The <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">Milky Way</a>, our own galaxy, is an example of a barred spiral. These galaxies are quite common in the universe, making up about two-thirds of all observed spiral galaxies.



The bar itself is thought to be a temporary feature, developing as the galaxy matures and possibly disappearing over time as the dynamics of the stars change. 



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



Reticulum is a small, faint constellation in the southern sky. Its name means "the reticle" in Latin, which refers to the crosshairs in an eyepiece of a telescope.



The constellation was named in the 18th century by the French astronomer Nicolas Louis de Lacaille to honor the reticle he used in his scientific instruments. It is one of the 88 modern constellations recognized by the International Astronomical Union.



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



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Spiral galaxy glows with young stars and interstellar dust

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



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



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



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



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



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



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



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



Researchers are utilizing Euclid’s data to explore the relationship between dust, gas, and star formation. The data can also be used to map the distribution of different stellar populations and identify regions of active star formation.



Spiral arms play a significant role in star formation by compressing gas, yet the precise mechanisms behind this process are still unclear. 



The presence of “spurs” along NGC 6744’s spiral arms offers valuable insights into the dynamics of star formation within these structures.



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



Additionally, Euclid's dataset will help scientists identify clusters of old stars (globular clusters) and discover new dwarf galaxies around NGC 6744. 



Remarkably, Euclid has already identified a new dwarf satellite galaxy of NGC 6744 - a surprising discovery given that the galaxy has been studied extensively.



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



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



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



The spiral arms of NGC 6744 are well-defined and extend outward, wrapping around the central bar. 



Additionally, NGC 6744 has a smaller companion galaxy, NGC 6744A, which is interacting with it, adding to the complexity and interest of this distant system.&nbsp;



<h2 class="wp-block-heading" id="h-types-of-spiral-galaxies">Types of spiral galaxies</h2>



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



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



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



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



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



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



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



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



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



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



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



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Young stars illuminate a spiral galaxy in the constellation Pavo

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

While age may bring wisdom for people, it appears to bring peril for white-lined sphinx moths. A recent field study shows that birds, rodents, and other predators are far more likely to peck, bite, or maul these insects once they emerge from the pupal stage and spread their wings.



Led by the <a href="https://www.utep.edu/">University of Texas at El Paso</a> (UTEP), the research lends experimental weight to a long-standing evolutionary idea. Complete metamorphosis may protect youthful stages from predation, allowing individuals to reach reproductive maturity before facing the most dangerous chapter of life.



<h2 class="wp-block-heading" id="h-caterpillars-versus-adult-moths">Caterpillars versus adult moths</h2>



Biologist Brett Seymoure, principal investigator and assistant professor at UTEP, studies holometabolous insects - species that pass through egg, larva, pupa, and adult phases.



The prevailing theory suggests that <a href="https://www.earth.com/news/dragonfly-larvae-expose-climates-hidden-influence-on-biology/">larvae</a> enjoy a relative sanctuary from predators, giving them a chance to grow before adulthood brings mobility, exposure, and heightened risk.



“There are multiple hypotheses about why these insects go through so many stages before reaching adulthood,” Seymoure said.



“Our research set out to test the prediction that caterpillars are less likely to be attacked by predators, enabling the insect to survive to adulthood and reproduce before it has to face the most dangerous part of its life.”



<h2 class="wp-block-heading" id="h-creating-life-sized-decoys">Creating life-sized decoys</h2>



Directly observing countless <a href="https://www.earth.com/news/largest-predator-prey-feast-ever-seen-in-the-ocean-enormous-quickly-altered-food-chain/">predator attacks</a> on real moths would be impractical. Instead, graduate student and lead author Braulio Alexis Sanchez created convincing clay replicas of both caterpillars and adult moths.



To mimic the wing patterns of Hyles lineata accurately, he printed photographs on special paper calibrated for precise color matching, then attached the wings to the clay bodies. 



Because clay records punctures and impressions, each model would serve as a forensic logbook, revealing encounters with sharp beaks or probing mandibles.



<h2 class="wp-block-heading" id="h-moths-meet-predators-in-texas">Moths meet predators in Texas</h2>



The team installed pairs of decoys - one caterpillar, one adult - on creosote bushes scattered across the rugged Indio Mountains Research Station in West Texas, a property managed by UTEP. 



Spacing the models closely ensured they faced identical environmental conditions. Over three consecutive days, researchers visited sites at dawn and dusk, inspecting every replica for new damage, counting beak marks, tooth gouges, or missing segments.



“Out of 70 replicas that were attacked, 50 were adults and 20 were caterpillars, and most of the attack marks were consistent with birds,” noted Sanchez.



In other words, adult-shaped models were assaulted two and a half times more often than larval shapes. Because both forms were equally available to predators, the data point toward active selection: visually oriented hunters seemed to prefer the adult silhouette.



<h2 class="wp-block-heading" id="h-predators-prefer-winged-moths">Predators prefer winged moths</h2>



The results bolster the notion that larval life provides a safer developmental window. If predation focused primarily on caterpillars, populations might struggle to produce enough breeding adults.



“If moths in the <a href="https://www.earth.com/news/caterpillars-inherit-food-preferences-through-their-blood/">caterpillar</a> stage were more heavily attacked, it would be much more difficult for moths to reach adulthood and reproduce,” Seymoure noted. 



Instead, the danger spikes only when the moth takes wing - precisely when reproduction becomes possible.



<h2 class="wp-block-heading" id="h-a-reminder-of-insect-importance"><a></a>A reminder of insect importance</h2>



Beyond theoretical interest, the study highlights insects’ ecological centrality. As Sanchez put it, “Without insects, there are no humans, trees, or plants.”



<a href="https://www.earth.com/news/insects-are-still-disappearing-and-there-are-hundreds-of-reasons-why/">Insects</a> pollinate crops, decompose organic matter, seed food webs, and cycle nutrients. Yet global surveys report worrying declines. 



Understanding at what life stage insects are most vulnerable can inform habitat management, pesticide timing, and conservation priorities.



<h2 class="wp-block-heading" id="h-identifying-the-moth-s-predators">Identifying the moth's predators</h2>



While bite impressions suggested birds were the main culprits, the researchers plan to broaden their surveillance.



Nocturnal moth predators - <a href="https://www.earth.com/news/frog-mating-calls-teach-bats-which-prey-to-avoid/">bats</a>, rodents, even wandering spiders - might attack under cover of darkness. 



Motion-activated cameras, night-vision optics, and ultrasonic detectors could capture real-time predation events and complement the static clay evidence.



The Chihuahuan Desert hosts unique avian assemblages and sparse vegetation, potentially exaggerating visual hunting cues. To test generality, Seymoure’s team hopes to replicate experiments in woodland, grassland, and urban settings, and with different moth species.



If adult-biased predation proves universal, it would underscore metamorphosis as a widespread risk-management strategy in insects.



<h2 class="wp-block-heading" id="h-maturity-invites-greater-danger">Maturity invites greater danger</h2>



Complete metamorphosis remains one of evolution’s most ingenious inventions, separating growth and reproduction into distinct anatomical phases.



The new findings suggest an additional benefit: by bottling youth within a relatively inconspicuous caterpillar, nature minimizes early-life losses. 



Once it stockpiles resources and unfurls its wings, the adult embarks on the perilous business of mating and dispersal. For Hyles lineata, growing older quite literally means stepping into the firing line.



<h2 class="wp-block-heading" id="h-focusing-on-climate-and-scent">Focusing on climate and scent</h2>



Future studies may integrate chemical cues - some predators use scent rather than sight - or assess how <a href="https://www.earth.com/news/danger-zones-climate-change-is-altering-predator-prey-dynamics/">climate change</a> alters predator-prey dynamics.



For now, the clay decoys at Indio Mountains recount a simple story: in the desert sky, an adult moth is a conspicuous, protein-rich morsel, while a plump caterpillar clinging to creosote is more likely to pass unnoticed. 



Age, it seems, is more than just a number for these shapeshifting insects; it marks the difference between relative safety and a sudden, predatory strike.



The study is published in the journal <a href="https://www.mdpi.com/2075-4450/16/4/347">Insects</a>.



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Why predators attack adult moths instead of caterpillars

While age may bring wisdom for people, it appears to...

Wheat is a major part of our diet, especially in the form of bread. But not all wheat is the same - and the way in which it’s grown, processed, and baked affects the nutrients that are present in it.



Until now, the wheat industry has mostly focused on boosting yields, reducing inputs like fertilizers and pesticides, and ensuring good baking quality. 



What often gets overlooked, however, is that wheat can also be a valuable source of nutrients. In fact, it contributes over 20% to the global supply of fiber, minerals, and trace elements, according to the Food and Agriculture Organization.



But getting more nutrition out of wheat isn’t just about planting a different variety. It involves the entire chain - all the way from the field to the oven.



<h2 class="wp-block-heading" id="h-characteristics-of-wheat-varieties">Characteristics of wheat varieties </h2>



Scientists at the <a href="https://www.uni-hohenheim.de/en" target="_blank" rel="noreferrer noopener">University of Hohenheim</a> and the University Medical Center at the University of Mainz teamed up with four wheat breeding companies to study how wheat’s nutritional value can be improved across the whole value chain. 



Over five years, they recorded more than 6,000 traits across 282 wheat varieties and 400 breeding lines.



Dr. Friedrich Longin is director of the Wheat Department at the <a href="https://lsa.uni-hohenheim.de/" target="_blank" rel="noreferrer noopener">State Plant Breeding Institute</a> and coordinator of the <a href="https://lsa.uni-hohenheim.de/en/betterwheat_en" target="_blank" rel="noreferrer noopener">Betterwheat project</a>.



“The unique thing about the project was the holistic view of variety characteristics along the entire value chain,” explained Dr. Longin.



“In addition to important characteristics for successful cultivation, several dozen processing characteristics for bakeries were considered, as well as important ingredients and proteins that could be important for <a href="https://www.earth.com/news/proper-nutrition-in-the-first-1000-days-of-life-is-crucial/">human</a> nutrition.”



<h2 class="wp-block-heading" id="h-some-wheat-just-has-more-nutrients">Some wheat just has more nutrients</h2>



The wheat varieties were tested in different environments across Europe to measure how both breeding and growing conditions influence the traits of the wheat.



“This allows us to estimate the extent of the influence of breeding, but also that of the growing environment, on these many traits,” noted Dr. Johannes Schacht, senior wheat breeder at <a href="https://www.limagrain.com/en">Limagrain</a> GmbH.



One of the team's main goals was to understand how nutrient levels vary between wheat types. They tested about 800 wheat samples for 13 key minerals and trace elements like iron and <a href="https://www.earth.com/news/calcium-zinc-are-keys-to-healthier-pregnancy/">zinc</a> - nutrients that are important for immunity, metabolism, and cell health.



“We were able to determine that the nutrient content in different wheat varieties varies greatly - and can fluctuate by up to 50%,” stated Dr. Longin.



“Our trials also show that the nutrients in wheat can be combined well with the required baking qualities in terms of breeding. These correlated positively with the protein content and dough properties.”



<h2 class="wp-block-heading" id="h-measuring-wheat-nutrient-content">Measuring wheat nutrient content</h2>



To apply this research practically, the scientists explored how to quickly measure nutrient content in wheat. 



One method, x-ray fluorescence (XRF) spectrometry, could be a game changer. It scans wheat with X-rays and, based on prior calibrations, provides fast, reliable nutrient readings.



“In order to use this knowledge in practice, xrf fluorescence spectrometry is a method that can be used to measure the nutrient content in wheat quickly and reliably,” explained Dr. Longin.



But using this technology widely would require investment. “This is only possible if the additional work is also paid for,” he added.



And there’s another catch: boosting wheat’s nutrition only makes a difference if people eat more <a href="https://www.earth.com/news/refined-grains-increase-the-risk-of-heart-disease/">whole grains</a> or at least <a href="https://www.earth.com/news/chocolate-with-less-sugar-still-tastes-great-with-a-secret-ingredient/">flours</a> with high type numbers (1050 and up). That’s because most nutrients are in the outer layers of the grain, which are lost in refined flours like types 405, 550, and 812.



<h2 class="wp-block-heading" id="h-bakers-make-wheat-digestible">Bakers make wheat digestible</h2>



Even if wheat is nutrient-rich, our bodies might not absorb those nutrients unless the bread is <a href="https://www.earth.com/news/freezing-bread-could-make-it-healthier/">baked</a> the right way.



“The healthy ingredients in wheat are bound in phytic acid. However, this acid cannot be digested and is excreted along with the beneficial nutrients,” said Dr. Longin.



So the researchers partnered with artisan bakers to test four common baking methods. One technique stood out: combining a long dough cycle with sourdough. 



“We found that the phytic acid is almost completely broken down during this baking process, making the ingredients available to the body,” he said.



<h2 class="wp-block-heading" id="h-better-bread-starts-with-better-choices">Better bread starts with better choices</h2>



From field to bakery, everyone involved in wheat production can help improve the nutritional value of bread. But it starts with us.



“All partners in the wheat value chain can influence the nutritional content of bread,” said Dr. Longin. "However, clear priorities must be set: first of all, we consumers should eat more whole grains." 



"This should then be baked with a long leavening process, and only then does breeding and targeted grain trading make sense in order to further optimize the nutrient profile."



Wheat offers more than just <a href="https://www.earth.com/news/eating-almonds-can-help-you-cut-calories/">calories</a>. With the right science, baking methods, and consumer choices, it can play a much bigger role in a healthy diet.



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Bread reinvented: Maximizing the nutrient potential of wheat

Wheat is a major part of our diet, especially in...

The Mediterranean has long been a crossroads of trade and tourism, yet its deepest pocket, the Calypso Deep, seemed beyond the reach of day-to-day pollution. 



That hope ended earlier this year when researchers reported plastic bags, glass shards, and crumpled cans resting 16,770 feet beneath the waves in the <a href="https://en.wikipedia.org/wiki/Ionian_Sea" target="_blank" rel="noreferrer noopener">Ionian Sea</a>.



Their survey logged hundreds of items on the trench floor. By any measure, it is one of the densest concentrations of trash ever recorded in the <a href="https://www.earth.com/news/deep-ocean-buffet-big-fish-are-surprisingly-reliant-on-the-twilight-zone/">dark zone</a> of the ocean.



The discovery arrives as global attention continues to focus on <a href="https://www.earth.com/news/surprise-study-some-scientists-call-for-halting-ocean-plastic-cleanup-efforts/">plastic waste</a>. 



Videos of snagged sea turtles and bottle-strewn beaches have already ignited public concern, but those images barely hint at what sinks far below the reach of sunlight.



Now evidence from Calypso Deep shows that even the <a href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/calypso" target="_blank" rel="noreferrer noopener">Mediterranean’s farthest recesses</a> are filling up.



<h2 class="wp-block-heading" id="h-calypso-deep-is-full-of-plastic-waste">Calypso Deep is full of plastic waste</h2>



The team used the submersible <a href="https://en.wikipedia.org/wiki/DSV_Limiting_Factor" target="_blank" rel="noreferrer noopener">Limiting Factor</a> to reach the bottom of a kidney-shaped trench roughly 12.4 miles long and 3.1 miles across. 



During a 43-minute trek near the seafloor of the Calypso Deep, cameras captured thousands of objects per square mile, mostly plastic waste discarded by humans.



A single straight-line pass of 2,130 feet was enough to confirm that human trash blankets large stretches of the basin. Most pieces were flexible plastics; glass, metal, and paper rounded out the list. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_study-map_UBarcelona_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_study-map_UBarcelona_1s.webp" alt="(A) General location of the Calypso Deep (box) in the Ionian Sea. PP: Peloponnese Peninsula. (B) Close up and general bathymetry of Calypso Deep (box) and surrounding area. For depth ranges, see color scale. (C) Detailed bathymetry of Calypso Deep with depth contours in meters. The position of the deepest point is indicated by the white dot, while the dive area is indicated by the red dot. Credit: University of Barcelona" class="wp-image-1976573"/></a><figcaption class="wp-element-caption">(A) General location of the Calypso Deep (box) in the Ionian Sea. PP: Peloponnese Peninsula. (B) Close up and general bathymetry of Calypso Deep (box) and surrounding area. For depth ranges, see color scale. (C) Detailed bathymetry of Calypso Deep with depth contours in meters. The position of the deepest point is indicated by the white dot, while the dive area is indicated by the red dot. Click image to enlarge. Credit: University of Barcelona</figcaption></figure>



Even without animals caught on camera, the piles raise alarms because deep-sea communities recover slowly from disturbance.



Calypso Deep lies about 37 miles west of the Peloponnese coast inside the Hellenic Trench, a zone of steep, stepped walls prone to earthquakes. 



<h2 class="wp-block-heading" id="h-plastic-waste-rides-currents">Plastic waste rides currents</h2>



Weak currents, usually under 0.8 inches per second and rarely reaching 7 inches per second, let debris settle instead of sweeping it away.



“It comes from various sources, both terrestrial and marine. It could have arrived by various routes, including long-distance transport by ocean currents or direct dumping,” explains <a href="https://web.ub.edu/en/web/directori/?accio=SEL&amp;id=v759w8s35bo5v72r&amp;lang=ca" target="_blank" rel="noreferrer noopener">Miquel Canals</a>, professor at the Department of Earth and Ocean Dynamics at the University of Barcelona.



“Some light waste, such as plastics, comes from the coast and escapes to Calypso Deep, just about 37 miles away. Certain plastics, <a href="https://www.earth.com/news/plastic-bag-bans-have-drastically-reduced-ocean-pollution/">like bags</a>, drift just above the seabed until they are partially or completely buried or break down into smaller fragments," Canals continued.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_litter-photos_UBarcelona_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_litter-photos_UBarcelona_1s.webp" alt="Examples of identified litter items with category attribution per material type (cf. Table 2). (A) Plastic bag, J3. (B) Plastic heavy-duty sack, J36. (C) Plastic sheet, J67. (D) Plastic food container made of hard plastic, J225. (E) Plastic heavy-duty sack, J36. (F) Plastic bag, J3 (G) Cups and lids of hard plastic, J227. (H) Plastic rope &gt; 1 cm in diameter, J49. (I) Paper cartons/Tetrapak (non-milk), J151. (J) Metal drink can, J175. (K) Glass bottle. Note sediment shadow with side scouring downwards of the bottle J200. (L) Plastic drink bottle. Credit: University of Barcelona" class="wp-image-1976569"/></a><figcaption class="wp-element-caption">Examples of identified litter items with category attribution per material type. (A) Plastic bag, J3. (B) Plastic heavy-duty sack, J36. (C) Plastic sheet, J67. (D) Plastic food container made of hard plastic, J225. (E) Plastic heavy-duty sack, J36. (F) Plastic bag, J3 (G) Cups and lids of hard plastic, J227. (H) Plastic rope &gt; 1 cm in diameter, J49. (I) Paper cartons/Tetrapak (non-milk), J151. (J) Metal drink can, J175. (K) Glass bottle. Note sediment shadow with side scouring downwards of the bottle J200. (L) Plastic drink bottle. Click image to enlarge. Credit: University of Barcelona</figcaption></figure>



Rivers, wind, and ship traffic all feed the stream of refuse heading offshore. As algae and other organisms cling to floating polymers, the added weight turns buoyant scraps into sinking hazards. The trench’s closed shape then locks the pieces in place.



<h2 class="wp-block-heading" id="h-calypso-deep-as-a-plastic-graveyard">Calypso Deep as a plastic graveyard</h2>



Surface eddies often corral floating trash into the trench. When these eddies form over the Calypso Trench, some debris slowly falls to the bottom, aided by degradation and ballasting processes that increase its density. 



Surface currents can also carry debris northward from the Adriatic Sea through the Strait of Otranto and from waters off northwestern Greece. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_3D-model_UBarcelona_1m.jpg"><img src="https://www.earth.com/wp-content/uploads/2025/03/marine-trash_Calypso-Deep-region_Mediterranean_3D-model_UBarcelona_1s.webp" alt="(A) 3D model generated from a subset of video frames by reference to a litter item of known size shown in B. The white dashed line in A represents the camera frames along the Deep Submergence Vehicle (DSV) Limiting Factor moving path, whereas the red dashed line represents the frames counted between two items identified on the seabed. (B) Accumulation of litter items in the inner Calypso Deep with a litter item of known size (12 cm) used as a reference for 3D model generation. Credit: University of Barcelona" class="wp-image-1976567"/></a><figcaption class="wp-element-caption">(A) 3D model generated from a subset of video frames by reference to a litter item of known size shown in B. The white dashed line in A represents the camera frames along the Deep Submergence Vehicle (DSV) Limiting Factor moving path, whereas the red dashed line represents the frames counted between two items identified on the seabed. (B) Accumulation of litter items in the inner Calypso Deep with a litter item of known size (12 cm) used as a reference for 3D model generation. Click image to enlarge. Credit: University of Barcelona</figcaption></figure>



The same circular flows that drive marine life cycles are now channeling waste into permanent graveyards at the very bottom of Earth's deepest bodies of water.



<a href="https://web.ub.edu/ca/web/actualitat/w/a-sea-of-rubbish-ocean-floor-landfills-?" target="_blank" rel="noreferrer noopener">Earlier work in 2021</a> showed the Strait of Messina carrying the world’s heaviest load of undersea garbage, confirming that the Mediterranean is especially at risk.



“We have also found evidence of boats dumping bags of rubbish, indicated by piles of assorted waste followed by an almost straight furrow," said Canals, expressing his frustration.



That is why the bottom of the Calypso Deep is littered with humans' plastic waste, and also why the problem will do nothing but continue to worsen.



"Unfortunately, when it comes to the Mediterranean, it is fair to say that ‘not a single inch of it is clean.’”



<h2 class="wp-block-heading" id="h-where-do-we-go-from-here">Where do we go from here?</h2>



Unlike beaches and coastlines, the <a href="https://www.earth.com/news/99-percent-of-the-deep-ocean-floor-has-still-never-been-seen-by-humans/">ocean floor</a> remains largely out of sight, making it difficult to build social and political momentum for its conservation. 



Yet what settles at the bottom can influence marine life, food webs, fisheries, climate feedback loops, and even geological stability.



<a href="https://www.earth.com/news/the-mediterranean-nearly-lost-all-of-its-water-6-million-years-ago/">The Mediterranean</a> is an enclosed sea, surrounded by humanity, with intense maritime traffic and widespread fishing activity.



“Scientists, communicators, journalists, influencers - everyone with a platform - must work together. The problem is vast, even if it is not directly visible, and we cannot ignore it," Canals implored.



The trail of refuse from shorelines to Calypso Deep underlines a plain truth: plastics and other debris do not vanish once tossed aside. They ride currents, sink in stages, and ultimately collect in the planet’s most secluded hollows. 



The evidence provided by this research should galvanize global efforts - especially in the Mediterranean - to curb dumping, particularly of plastics, in line with the pending <a href="https://www.globalplasticlaws.org/un-global-plastics-treaty" target="_blank" rel="noreferrer noopener">UN Global Plastics Treaty</a>.



From the North Atlantic’s first recorded litter in 1975 to the record densities documented across the Mediterranean today, the pattern remains the same - human waste reaches everywhere water flows.



We must do more, we must do better, and we must do it now.



-----



Thanks to the leaders of this research team - Miquel Canals of the <a href="https://web.ub.edu/en/" target="_blank" rel="noreferrer noopener">University of Barcelona</a>, Georg Hanke of the European Commission’s <a href="https://commission.europa.eu/about/departments-and-executive-agencies/joint-research-centre_en" target="_blank" rel="noreferrer noopener">Joint Research Centre</a>, François Galgani of <a href="https://www.ifremer.fr/en" target="_blank" rel="noreferrer noopener">IFREMER</a>, and Victor Vescovo of <a href="https://caladanoceanic.com/" target="_blank" rel="noreferrer noopener">Caladan Oceanic</a>



The full study was published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0025326X25000852">Marine Pollution Bulletin</a>.



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Disturbing discovery made on the deepest parts of the seafloor: "Not a single inch of it is clean"

The Mediterranean has long been a crossroads of trade and...

Many people toast the end of the day with a five‑ounce glass of wine, hoping that ritual keeps heart trouble at bay. Two new analyses suggest the habit might offer real - if limited - protection for adults already at higher risk of cardiovascular disease.



The latest evidence comes from a Spanish arm of the long‑running <a href="https://pubmed.ncbi.nlm.nih.gov/28684083/" target="_blank" rel="noreferrer noopener">PREDIMED trial</a>. The study tracked 1,232 older adults following a <a href="https://my.clevelandclinic.org/health/articles/16037-mediterranean-diet" target="_blank" rel="noreferrer noopener">Mediterranean diet</a> and found that those who averaged roughly half to one glass per day had significantly lower heart risks. 



After five years, their risk of heart attack, stroke, or cardiac death dropped by nearly half.



Researchers verified intake by measuring wine‑derived tartaric acid in urine instead of relying on memory, a switch that turned vague drink logs into hard numbers. 



The work was led by <a href="https://www.clinicbarcelona.org/en/professionals/ramon-estruch" target="_blank" rel="noreferrer noopener">Professor Ramon Estruch</a> of the <a href="https://web.ub.edu/en/" target="_blank" rel="noreferrer noopener">University of Barcelona</a> and <a href="https://www.clinicbarcelona.org/en" target="_blank" rel="noreferrer noopener">Hospital Clinic Barcelona</a>.



<h2 class="wp-block-heading" id="h-chemical-reveals-true-wine-intake">Chemical reveals true wine intake</h2>



Questionnaires often miss what people actually pour, so scientists struggle to pin down alcohol’s true effects. Using the <a href="https://www.mdpi.com/2311-7524/9/11/1173" target="_blank" rel="noreferrer noopener">grape‑exclusive metabolite tartaric acid</a> makes it possible to see how much wine someone enjoyed over the previous week without asking them to confess.



“By measuring tartaric acid in the urine, alongside food and drink questionnaires, we have been able to make a more accurate measurement of wine consumption,” said Estruch.



The study linked tartaric acid levels to self-reported wine intake, confirming it as a reliable consumption marker.



<h2 class="wp-block-heading" id="h-wine-s-effects-in-mediterranean-diets">Wine's effects in Mediterranean diets</h2>



Adopting such objective tools may help resolve decades of conflicting findings that swing from “red wine is medicine” to “no amount is safe.”



The investigators also adjusted for smoking, exercise, and other <a href="https://www.earth.com/news/to-get-fit-and-stay-healthy-walk-this-exact-distance-every-day/">lifestyle habits</a>, so the reduced risk cannot be written off as a simple marker of healthier living.



Importantly, tartaric acid only captures wine, not beer or spirits, letting researchers isolate how fermented <a href="https://www.earth.com/news/hidden-chemistry-of-wine-what-actually-shapes-its-texture/">grape products</a> behave inside a diet already rich in extra‑virgin olive oil, fish, and vegetables.



That context matters because many of wine’s plant compounds appear to interact with the broader Mediterranean plate, enhancing their <a href="https://www.earth.com/news/healing-chronic-wounds-with-gold-and-red-wine/">antioxidant reach</a>.



<h2 class="wp-block-heading" id="h-benefits-tied-to-small-servings">Benefits tied to small servings</h2>



Participants who logged between three and thirty‑five five‑ounce glasses a month, roughly half to one serving a day, saw their risk of a major cardiac event fall by 50 percent. Light users who stayed below half a glass a day gained a 38 percent cut.



Once intake climbed above one glass each day, the advantage disappeared and, in some analyses, reversed. 



That pattern mirrors American Heart Association <a href="https://www.heart.org/en/health-topics/high-blood-pressure/changes-you-can-make-to-manage-high-blood-pressure" target="_blank" rel="noreferrer noopener">guidance</a>, which caps daily wine at one five‑ounce serving for women and two for men.



Men, who made up just under half the study group, appeared to draw a stronger benefit. However, statisticians caution that the sex difference may fade in larger samples.



Even within the favorable range, nurses warned that pouring size matters because many home glasses hold eight or nine ounces, inadvertently nudging people past the safer ceiling.



<h2 class="wp-block-heading" id="h-what-makes-wine-different">What makes wine different</h2>



Wine carries a mix of polyphenols such as resveratrol, quercetin, and catechins that seem to boost the lining of blood vessels. 



Clinical <a href="https://pubmed.ncbi.nlm.nih.gov/34119624/" target="_blank" rel="noreferrer noopener">reviews</a> report that supplemental resveratrol can improve endothelial function, a key factor in healthy blood pressure and clot prevention.



Red wine has more antioxidants due to skin fermentation, though white wine still provides some. That biochemical cocktail may partly explain why studies often find beer or spirits lack the same signal.



Moderate alcohol itself can raise high-density lipoprotein (<a href="https://www.cdc.gov/cholesterol/about/ldl-and-hdl-cholesterol-and-triglycerides.html" target="_blank" rel="noreferrer noopener">HDL</a>), the so‑called “good” cholesterol, yet ethanol also raises triglycerides and blood pressure at larger doses. Polyphenols may tilt the equation back toward benefit, but only within a narrow window.



<h2 class="wp-block-heading" id="h-too-much-wine-harms-the-heart">Too much wine harms the heart</h2>



A 2023 systematic <a href="https://jamanetwork.com/journals/jamanetworkopen/fullarticle/2802963" target="_blank" rel="noreferrer noopener">review</a> that pooled data from 4.8 million people found no reduction in all‑cause mortality among moderate drinkers once misclassified former drinkers were excluded. 



The authors warned that earlier optimism probably stemmed from comparing social drinkers with people who quit because of illness.



Heavy pouring is indisputably harmful. Even <a href="https://www.heart.org/en/news/2023/07/31/even-just-1-alcoholic-drink-a-day-may-increase-blood-pressure" target="_blank" rel="noreferrer noopener">one extra daily drink</a> can raise systolic blood pressure by two to four millimeters of mercury, a change large enough to push many people into hypertension. Elevated pressure strains arteries, sets the stage for arrhythmias, and accelerates heart failure.



<a href="https://alcoholresearchforum.org/members/giovanni-de-gaetano/" target="_blank" rel="noreferrer noopener">Professor Giovanni de Gaetano</a> noted that the biomarker approach “provides robust evidence that moderate wine consumption is associated with lower CVD risk. He cautioned that the same data “remind us of the risks associated with higher levels of consumption.”



Alcohol also carries addictive potential, and the Centers for Disease Control and Prevention (CDC) estimates that roughly <a href="https://archive.cdc.gov/www_cdc_gov/media/releases/2014/p0626-excessive-drinking.html" target="_blank" rel="noreferrer noopener">one in ten deaths</a> among working‑age adults is tied to excessive drinking. 



That sobering statistic explains why public health agencies repeat that zero is the only completely risk‑free dose.



<h2 class="wp-block-heading" id="h-wine-humans-and-heart-health">Wine, humans, and heart health</h2>



For adults older than about 35 who already follow a <a href="https://my.clevelandclinic.org/health/articles/16037-mediterranean-diet" target="_blank" rel="noreferrer noopener">Mediterranean diet</a>, a small glass of wine with supper may fit comfortably into a heart‑conscious lifestyle.



People who are pregnant, taking interacting medications, or battling addiction should not take the PREDIMED results as a green light.



Nutrients that give wine its appeal, <a href="https://www.earth.com/news/moderate-wine-consumption-reduces-cardiovascular-risks/">including resveratrol</a>, also reside in grapes, blueberries, nuts, and olive oil. Anyone who chooses to skip alcohol can still obtain similar antioxidant support without ethanol’s downsides.



Clinicians emphasize that no one should start drinking for health reasons. Instead, the sensible takeaway is that very modest wine, enjoyed with meals and within established limits, is unlikely to harm. It might even help certain high‑risk adults when paired with vegetables, fish, and extra‑virgin olive oil.



The study is published in the <a href="https://academic.oup.com/eurheartj/article/46/2/161/7920812" target="_blank" rel="noreferrer noopener">European Heart Journal</a>.



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How a glass of wine a day affects your heart, according to doctors

Many people toast the end of the day with a...

In 2022, the underwater Hunga volcano exploded, blasting ash 37 miles into the sky - the largest volcanic plume ever captured by satellites. What followed offered researchers a rare chance to see how the ocean floor responds to sudden, massive disruption.



Months later, scientists from around the world headed to the location of the eruption on a research vessel.



Onboard the ship, undergraduate student Marcus Chaknova discovered something unexpected: thick layers of <a href="https://www.earth.com/news/fire-and-ice-volcanic-ash-plays-a-surprising-role-in-cloud-formation/">volcanic ash</a> coating the seafloor. The ash had suffocated deep-sea ecosystems that rely on fragile chemical exchanges to survive.



<h2 class="wp-block-heading" id="h-underwater-eruptions-usually-go-unseen">Underwater eruptions usually go unseen</h2>



“This was an extremely rare opportunity,” Chaknova explained. “Observing the mass movement of underwater sediment is something that hasn't been studied much.”



Now a graduate student in Earth Sciences at the <a href="https://www.uoregon.edu/" target="_blank" rel="noreferrer noopener">University of Oregon</a>, Chaknova led a study that analyzed what the underwater eruption left behind.



Working with Professor Thomas Giachetti and 16 other experts from around the world, he became the lead author on a study that looked at how volcanic ash travels - and what it does to life underwater.



“We had scientists from every single time zone you could think of,” Chaknova said. His project needed expertise from the fields of marine biology, geochemistry, and micropaleontology.



<h2 class="wp-block-heading" id="h-tracking-ash-from-the-volcano">Tracking ash from the volcano </h2>



The first step was to confirm that the underwater ash had indeed come from <a href="https://www.earth.com/news/new-clues-about-the-hunga-tonga-hunga-haapai-eruption/">Hunga</a>, located about 40 miles from <a href="https://www.bbc.com/news/world-asia-pacific-16197014" target="_blank" rel="noreferrer noopener">Tonga's</a> main island in the South Pacific. 



After an eruption, it can take weeks or even months for ash to fall through the water and settle on the ocean floor. As it drifts, wind and currents push it farther from the eruption site.



"One grain of sediment will take weeks or months to reach the bottom of the ocean. It's like a leaf falling from a tree. Because of the wind, it might end up somewhere completely different," Giachetti explained.



Back in the lab, Chaknova matched the ash samples to those found near the volcano. The grains were varied - some jagged and sharp, others rounded and smooth. 



In some places, the sediment was more than a meter thick. Most of it was made up of very fine particles, around the width of a human hair.



<h2 class="wp-block-heading" id="h-what-the-eruption-left-behind">What the eruption left behind</h2>



Chaknova discovered that much of the ash came from the volcano’s caldera walls and was carried away by fast-moving underwater flows - something like underwater avalanches.



Those flows were so powerful they damaged submarine cables and carved small canyons into the seafloor. The researchers even used the timing of power loss from those broken cables to calculate how fast the ash surged.



Using computer models, Chaknova plans to simulate how the ash moved and where it went. Giachetti said this research could change how scientists think about sediment movement in the oceans.



<h2 class="wp-block-heading" id="h-deep-sea-life-suffocated">Deep-sea life suffocated</h2>



The underwater <a href="https://www.earth.com/news/tonga-volcanic-eruption-had-a-much-more-devastating-impact-than-we-knew/">eruption</a> didn’t just leave a geological footprint; it disrupted entire ecosystems.



In the deep sea, where sunlight doesn’t reach, life depends on <a href="https://www.earth.com/news/how-can-deep-ocean-microbes-survive-without-sunlight/">chemosynthesis</a> - organisms use chemicals like methane or ammonia from hydrothermal vents, instead of sunlight, to produce energy.



Roughly 90% of marine life lives on the seafloor, according to the <a href="https://www.worldwildlife.org/" target="_blank" rel="noreferrer noopener">World Wide Fund for Nature</a>. After the eruption, much of that life was buried in thick sediment.



Some creatures like worms and anemones can survive brief burials, but this sudden wave of ash was too much. 



Many deep-sea species are suspension feeders. They grab tiny particles of food from the water and filter them through their gills.



"With all the displaced sediment, these organisms are only grabbing sediment," Chaknova continued. "That's going to clog their gills, it's going to clog their intestines, and that's going to have a dramatic effect on their ability to create energy."



<h2 class="wp-block-heading" id="h-fallout-from-the-underwater-eruption">Fallout from the underwater eruption </h2>



Chaknova’s early findings also show that ash made it all the way to Tonga’s coral reefs. At first, it caused a short-lived plankton bloom at the surface. 



But as the ash settled, it threatened coral ecosystems that support larger marine life. When coral suffers, everything above it in the food chain is affected.



On top of the environmental consequences, the eruption of this underwater volcano also affected livelihoods for Tonga residents.



Fishing is a way of life in Tonga. According to the <a href="https://www.worldbank.org/ext/en/home" target="_blank" rel="noreferrer noopener">World Bank</a>, about 82% of households rely on reef fishing in some way for income. Marine tourism accounts for more than 7% of Tonga’s GDP.



“Although this eruption occurred on the seafloor, there is a chain of both positive and negative effects,” Chaknova explained.



“The negative effects go farther than just losing power or Wi-Fi from submarine cables. This is some people’s livelihood. They need fish for food. Fishing is incredibly important for the economic and food security of Tonga.”



<h2 class="wp-block-heading" id="h-warning-for-deep-sea-mining">Warning for deep-sea mining</h2>



The study also has bigger implications. As the world turns toward clean energy, demand is growing for metals like copper and cobalt - many of which sit in potato-sized nodules beneath the ocean floor.



Private companies have approached small Pacific nations, including Tonga, with offers to mine these resources.



"The area where we collected the sediment is within the Kingdom of Tonga, and we found that they are very rich in minerals," Chaknova said. 



"A lot of companies are interested in collecting these minerals, and so this area that belongs to the Kingdom of Tonga will be up for bid, in coming years, for <a href="https://www.earth.com/news/deep-sea-mining-impacts-marine-life-for-decades/">deep-sea mining</a>."



While commercial mining hasn’t started yet, researchers are urging caution. The plumes of sediment created by mining could be just as harmful as those created by volcanic eruptions - clogging gills, burying habitats, and destroying fragile ecosystems.



Chaknova’s work provides some of the only real-world data we have on what that kind of disturbance could look like. 



The research gives scientists and policymakers a better understanding of what’s at stake - and what might be lost if we move forward without enough knowledge.



The full study was published in the journal <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024GC011629" target="_blank" rel="noreferrer noopener">Geochemistry, Geophysics, Geosystems</a>.



Image Credit: <a href="https://www.noaa.gov" target="_blank" rel="noreferrer noopener">NOAA</a>



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Massive underwater eruption layered coral reefs with ash and suffocated marine life

In 2022, the underwater Hunga volcano exploded, blasting ash 37...

Scientists are transforming chocolate into a functional food by infusing it with probiotics and prebiotics, aiming to create a treat that satisfies cravings while supporting gut health. 



The challenge lies in maintaining chocolate's beloved texture and flavor while adding health benefits.



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https://youtu.be/Ug657J67iEo?si=w96YjGMsg939LD_3
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Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



Prebiotics act as food for these microbes, helping them thrive. Together, they form "synbiotics," a powerful health combination.



Researchers Smriti Gaur and Shubhi Singh from India's Jaypee Institute of Information Technology took an innovative approach, using natural prebiotics like corn and honey instead of complex processing methods. 



They created five chocolate varieties: a control and four synbiotic versions containing different combinations of prebiotics, probiotics (Lactobacillus strains), and flavor enhancers (cinnamon or orange).



Laboratory simulations of human digestion showed the probiotics remained viable for over five hours, suggesting they could survive long enough to benefit gut health.



Taste tests were positive, with researchers particularly enjoying the orange-flavored variety, describing it as having "vibrant citrus notes" complementing the "rich cocoa" with a "luxurious" texture.



This research represents just the beginning. With further refinement of strains, textures, and flavors, chocolate could evolve beyond mere indulgence to become a functional food that nourishes while it delights.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acsfoodscitech.4c00741" target="_blank" rel="noreferrer noopener">ACS Food Science &amp; Technology</a>.

Is chocolate the next nutritional powerhouse?

Scientists are transforming chocolate into a functional food by infusing...

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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



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Flu viruses are more flexible than expected

[sendtonews key="G9bUoxcjr4-2511624-12187" type="single"] Today's Video of the Day from the...

Thousands of colors in the Sculptor Galaxy

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