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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a> and interstellar matter.&nbsp;



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: European Space Agency&nbsp;



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Messier 78: Young stars shine through dense dust

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

Today's Image of the Day from NASA Earth Observatory features the remnants of Lake Razzaza, an artificial lake situated a few miles west of Karbala, Iraq.



The <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lake</a> was created in the late 1970s as a flood control measure to regulate the floodwaters of the Euphrates River. 



Razzaza covers an area of approximately 1,562 square kilometers and is located in a depression where excess water from Lake Habbaniyah is diverted through a controlled escape channel or canal.&nbsp;



<h2 class="wp-block-heading" id="h-the-colors-of-lake-razzaza">The colors of Lake Razzaza</h2>



“The lake, also known as Baḩr al-Milḩ (‘Sea of Salt’ in Arabic), is fed by overflow from Habbaniyah Lake, which lies just outside the top left corner of the image,” noted <a href="https://earthobservatory.nasa.gov/images/153756/iraqs-sea-of-salt" target="_blank" rel="noreferrer noopener">NASA</a>.



“The difference in water color results from the various communities of algae that thrive in the lake depending on the water temperature and salinity.”



“Green areas contain lower salt concentrations than red areas. At times when the lake receives no overflow from Habbaniyah Lake, as shown in this image, most of the lakebed is exposed.”



<h2 class="wp-block-heading" id="h-salinity-of-lake-razzaza">Salinity of Lake Razzaza</h2>



Over the years, the salinity of Lake Razzaza has been increasing due to inadequate water supply from the linked canal and high evaporation rates during Iraq's hot summers.&nbsp;



This rise in <a href="https://www.earth.com/news/salt-pollution-threatens-freshwater-ecosystems/" target="_blank" rel="noreferrer noopener">salinity</a> has led to a decline in fish populations, adversely affecting local fishermen who once relied on the lake for their livelihoods. 



By 2008, only the fish species locally known as "al-Shanik" (Acanthopagrus arabicus), of marine origin and stocked by the government, was reported to survive in the lake.&nbsp;



The lake's fluctuating water levels and increasing salinity have also impacted its recreational appeal, with few recreational areas existing around the lake.&nbsp;



Additionally, the surrounding desert landscape and low cliff shores contribute to its limited accessibility for leisure activities.&nbsp;



<h2 class="wp-block-heading" id="h-wildlife-of-lake-razzaza">Wildlife of Lake Razzaza</h2>



Despite these challenges, Lake Razzaza remains an important habitat for various bird species. It has been designated an Important Bird Area (IBA) by BirdLife International, supporting significant numbers of wintering waterfowl and serving as a breeding ground for species such as the marbled duck.&nbsp;



The lake's mudflats attract large numbers of waders and shorebirds during migration periods.&nbsp;



The surrounding area features vegetation such as Phragmites australis, Juncus acutus, Aeluropus lagopoides, Salicornia herbacea, and Schoenoplectus litoralis, along with desert shrublands including Tamarix aucherana, Prosopis farcta, and Haloxylon salicornicum.&nbsp;



Mammals reported in this region include Rüppell's fox, golden jackal, Indian grey mongoose, jungle cat, and wildcat.&nbsp;



In recent years, the <a href="https://www.earth.com/news/lakes-are-warming-toward-the-point-of-no-return/" target="_blank" rel="noreferrer noopener">lake</a> has faced environmental challenges due to reduced water inflows and increased evaporation, leading to higher salinity levels and a decline in biodiversity. 



Efforts to address these issues are essential to preserve the ecological and economic significance of Lake Razzaza.



<h2 class="wp-block-heading" id="h-the-euphrates-river-nbsp">The Euphrates River&nbsp;</h2>



The Euphrates River is one of the most significant rivers in the Middle East and holds immense historical, cultural, and ecological importance.&nbsp;



Stretching approximately 2,800 kilometers (1,740 miles), it originates in the mountains of eastern Turkey and flows through Syria and Iraq before merging with the Tigris River to form the Shatt al-Arab, which empties into the Persian Gulf.&nbsp;



The <a href="https://www.earth.com/news/major-plastic-pollution-lurks-beneath-the-surface-of-rivers/" target="_blank" rel="noreferrer noopener">river</a> has been a cradle of civilization for thousands of years, supporting ancient Mesopotamian societies, including Sumer, Akkad, Babylon, and Assyria.



The Euphrates has provided water for irrigation, enabling the development of agriculture in an otherwise arid region. Its floodplains have been vital for sustaining life and fostering the growth of cities along its course.&nbsp;



However, the river also plays a key geopolitical role, as disputes over water usage and dam construction among Turkey, Syria, and Iraq have emerged over the years, impacting water availability downstream.



Ecologically, the Euphrates supports a range of habitats, from wetlands to desert ecosystems, making it home to diverse flora and fauna.&nbsp;



However, modern challenges such as damming, pollution, and climate change threaten its flow and ecological balance. Despite these challenges, the Euphrates remains a symbol of life and resilience in the heart of the Middle East.



The image was captured by an astronaut on the International Space Station (ISS) on September 23, 2024.



Image Credit: NASA



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Lake Razzaza: A shrinking oasis shaped by salinity

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

Today's Image of the Day from NASA features the spiral galaxy NGC 2566, which is located 76 million light-years away in the constellation Puppis. The image was captured by the NASA/ESA Hubble Space Telescope.



“A prominent bar of stars stretches across the center of this galaxy, and spiral arms emerge from each end of the bar. Because NGC 2566 appears tilted from our perspective, its disk takes on an almond shape, giving the galaxy the appearance of a cosmic eye,” said <a href="https://phys.org/news/2024-12-hubble-spies-spiral-galaxy-ngc.html" target="_blank" rel="noreferrer noopener">NASA</a>.



“As NGC 2566 appears to gaze at us, astronomers gaze right back, using Hubble to survey the galaxy's star clusters and star-forming regions.”



<h2 class="wp-block-heading" id="h-complex-appearance-of-ngc-2566">Complex appearance of NGC 2566</h2>



NGC 2566 lies at a considerable distance from Earth, making it a challenging object for amateur astronomers to observe in detail without powerful telescopes.&nbsp;



It can be seen in the Southern Hemisphere sky and is better observed from locations with minimal <a href="https://www.earth.com/news/how-light-pollution-influences-interest-in-astronomy/" target="_blank" rel="noreferrer noopener">light pollution</a>.&nbsp;



The galaxy's arms are populated with young, bright stars, regions of active star formation, and interstellar gas and dust - giving it a dynamic and complex appearance.



<h2 class="wp-block-heading" id="h-measuring-the-ages-of-stars">Measuring the ages of stars</h2>



According to NASA, data from Hubble is especially valuable for studying stars that are just a few million years old. “These stars are bright at the ultraviolet and visible wavelengths to which Hubble is sensitive.”



“Using these data, researchers can measure the ages of NGC 2566's stars, which helps piece together the timeline of the galaxy's star formation and the exchange of gas between star-forming clouds and the stars themselves.”



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



Star formation in <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> is a fascinating and complex process that unfolds over millions of years. It begins in vast clouds of gas and dust, known as molecular clouds, which are often found in the spiral arms of galaxies or in regions of irregular or starburst galaxies.&nbsp;



These clouds provide the raw material for star formation, consisting primarily of hydrogen and helium, with trace amounts of heavier elements.



As the molecular clouds collapse under their own gravity, regions within them begin to condense and fragment, forming dense clumps. Within these clumps, protostars emerge. Their formation is driven by the gravitational pull drawing in surrounding gas. 



During this process, the gas heats up due to increasing pressure, eventually igniting nuclear fusion in the core, signaling the birth of a new star.



<h2 class="wp-block-heading" id="h-rate-of-star-formation-nbsp-across-galaxies">Rate of star formation&nbsp;across galaxies</h2>



The rate of star formation varies across galaxies is influenced by numerous factors. In spiral galaxies like the Milky Way, star formation is most active in the spiral arms, where density waves compress gas and dust, triggering the collapse of molecular clouds. 



In contrast, elliptical galaxies, which often have little cold gas and dust, typically exhibit low rates of star formation or none at all.



Starburst galaxies, on the other hand, experience episodes of exceptionally high star formation, often triggered by <a href="https://www.earth.com/news/webb-captures-a-galaxy-collision-with-a-radiant-smile/">galactic collisions</a> or interactions. 



These events can funnel large amounts of gas into central regions, leading to intense star-forming activity. However, such bursts are usually short-lived on cosmic timescales, exhausting the available gas quickly.



The environment within a galaxy also plays a significant role. Stellar winds and supernova explosions from existing stars can both inhibit and promote star formation. They may disperse gas, preventing further collapse, or compress nearby clouds, triggering new star formation.&nbsp;



Over time, as galaxies evolve, the availability of gas diminishes, leading to a gradual decline in star formation activity.



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



The Puppis constellation in the southern sky represents the stern of a ship. It was once part of a larger constellation known as Argo Navis, which depicted the mythical ship of Jason and the Argonauts. 



However, Argo Navis was later divided into three separate constellations: Puppis, Carina (the keel), and Vela (the sails). Puppis is the largest of these three and contains many notable celestial objects.



This constellation is home to several bright stars, including Naos (Zeta Puppis), a hot, massive star that emits intense ultraviolet radiation. Puppis also hosts a wide variety of deep-sky objects, such as open <a href="https://www.earth.com/news/stunning-star-clusters-captured-in-the-extreme-outskirts-of-the-milky-way/" target="_blank" rel="noreferrer noopener">star clusters</a> and nebulae. 



Among these, Messier 46 and Messier 47 stand out. Both are beautiful star clusters that are visible through binoculars or small telescopes. The region is dense with stars because it lies along the <a href="https://www.earth.com/news/milky-way-collision-may-change-everything-we-know-about-our-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>, making it a prime area for stargazing and astrophotography. 



Image Credit: NASA



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NGC 2566: A cosmic eye in the Puppis constellation

Today's Image of the Day from NASA features the spiral...

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-planetary-nebulae-nbsp">Planetary nebulae&nbsp;</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. 



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

On December 16, Henry, the world’s oldest known crocodile, marked his 124th birthday at a conservation center in South Africa. He has attracted attention for his extraordinary lifespan and remains a prime example of how a well-protected environment may support <a href="https://www.earth.com/news/social-aging-what-animals-can-teach-us-about-getting-older/">healthy aging in animals</a>.



<h2 class="wp-block-heading" id="h-henry-s-timeless-presence">Henry’s timeless presence</h2>



He has resided at the <a href="https://crocworld.co.za/" target="_blank" rel="noreferrer noopener">Crocworld Conservation Centre</a> in Scottburgh, South Africa, since 1985 and arrived with a history reaching back to his capture in the Okavango Delta in 1903. 



According to the center, <a href="https://crocworld.co.za/news/detail/friends-of-henry-can-rest-assured-this-crocodile-is-still-rocking-at-crocworld" target="_blank" rel="noreferrer noopener">Henry</a> has fathered over <a href="https://crocworld.co.za/news/detail/friends-of-henry-can-rest-assured-this-crocodile-is-still-rocking-at-crocworld">10,000 offspring</a>, illustrating his sustained vitality and robust biological functions.



“An age of 124 is not inconceivable for a crocodile,” said <a href="https://www.uab.edu/cas/biology/people/faculty/steven-n-austad" target="_blank" rel="noreferrer noopener">Steven Austad</a> from the <a href="https://www.ua.edu/" target="_blank" rel="noreferrer noopener">University of Alabama</a>. This commentary adds weight to Henry’s reputation and has prompted curiosity about the factors that support crocodile resilience.



<h2 class="wp-block-heading" id="h-growth-and-metabolism">Growth and metabolism</h2>



Many reptiles grow throughout their lives, and Henry is no exception at an estimated 1,540 pounds (700 kg) in mass and 16.4 feet (5 meters) in length. 



This hefty size, combined with a slow metabolism, helps him conserve energy and may also give him an edge against external threats.



Crocodiles rely on heat from the sun and surrounding environment instead of generating warmth <a href="https://www.earth.com/news/world-croc-day-embracing-the-mighty-reptile/" target="_blank" rel="noreferrer noopener">within their bodies</a>. 



This trait appears to reduce the rate at which their tissues wear out, and adds to their ability to maintain a high level of functioning for years.



Life in captivity has limited Henry’s exposure to food shortages or conflicts with other crocodiles. Such stability shields him from hazards that might cut short a more vulnerable reptile’s life in the wild.



<h2 class="wp-block-heading" id="h-observations-on-crocodile-aging">Observations on crocodile aging</h2>



Scientists have found <a href="https://www.nih.gov/news-events/nih-research-matters/aging-insights-reptiles-amphibians" target="_blank" rel="noreferrer noopener">evidence</a> that reptiles in good living conditions show minimal deterioration in muscles, bones, and even immune response. 



Henry’s lifestyle suggests that an environment with the right temperature, healthy nutrition, and reliable care can delay many common issues that come <a href="https://www.earth.com/news/social-aging-what-animals-can-teach-us-about-getting-older/" target="_blank" rel="noreferrer noopener">with advanced age</a>.



Research on crocodiles reveals remarkable immune features. One <a href="https://www.sciencedirect.com/science/article/pii/S2405844024006145" target="_blank" rel="noreferrer noopener">study</a> demonstrated that Nile crocodile blood contains proteins that help ward off infections and boost healing by increasing white blood cell production.



<h2 class="wp-block-heading" id="h-insights-from-infection-studies">Insights from infection studies</h2>



In one investigation, experts observed a spike in white blood cells within a single hour after a crocodile was exposed to a common bacterial threat. 



Those findings highlight the speed and strength of crocodiles’ defenses, which may keep them healthy across the decades.



Antibacterial qualities in crocodile blood have been shown to limit the spread of harmful pathogens. 



This may explain how these animals survive wounds in habitats that teem with microbes, while comparable injuries might be life-threatening for other creatures.



Scientists have also examined the <a href="https://www.sciencedirect.com/science/article/pii/S2405844021026979" target="_blank" rel="noreferrer noopener">gut microbiome</a> in crocodiles, suspecting that their intestinal microbes support a stronger immune system. 



This microbial harmony might protect against infections, thus promoting longevity and resilience in harsh conditions.



<h2 class="wp-block-heading" id="h-historical-resilience">Historical resilience</h2>



Crocodilians have been around for many millions of years, according to the <a href="https://www.floridamuseum.ufl.edu/science/crocodile-evolution/" target="_blank" rel="noreferrer noopener">Florida Museum of Natural History</a>. 



They endured drastic climate changes and lived through mass extinction events that eradicated many other large reptiles.



<h2 class="wp-block-heading" id="h-crocodile-aging-studies">Crocodile aging studies</h2>



Researchers aim to unravel more details about crocodiles’ <a href="https://www.earth.com/news/crocodile-evolution-was-influenced-by-environmental-factors/" target="_blank" rel="noreferrer noopener">immune functions</a>, as these might inspire new treatments for infections and inflammatory conditions. 



Unlocking these biological pathways could offer significant benefits for human health.



Advances in technology will allow teams to study crocodile genes, proteins, and microbial interactions more thoroughly. 



This focus may lead to safer approaches in fighting antibiotic-resistant bacteria or managing wound recovery, thereby improving people’s quality of life in underserved areas.



<h2 class="wp-block-heading" id="h-community-level-gains">Community-level gains</h2>



Neighboring communities can use knowledge from this research to protect their natural surroundings. 



Preserving habitats for crocodiles, while observing how these animals regulate their health, might lead to conservation and biomedical breakthroughs.



Henry’s case highlights the importance of safeguarding older animals that can teach us about longevity. 



Facilities that promote coexistence between people and wildlife help preserve irreplaceable genetic resources that might one day turn into lifesaving innovations.



<h2 class="wp-block-heading" id="h-improved-public-awareness">Improved public awareness</h2>



Experts believe this research can spark interest in reptile welfare and the crucial role these species play in ecosystems. 



Encouraging broader conservation efforts, in turn, fosters a stronger appreciation of biodiversity and its benefits.



Representatives from conservation groups outside of Crocworld have remarked that aging crocodiles sometimes exhibit unusual levels of disease resistance. 



This input aligns with what researchers are finding about <a href="https://www.earth.com/news/ancient-crocodile-had-dolphin-like-flippers-and-smooth-skin/" target="_blank" rel="noreferrer noopener">reptile biology</a>, emphasizing the value of long-term study in controlled environments.



Gathering data on crocodiles from hatchling to old age remains difficult, given these animals’ lifespans. 



Studies require a long window of monitoring, and continuity can be hard to maintain as scientists change institutions or move on to other projects.



<h2 class="wp-block-heading" id="h-crocodiles-aging-and-the-future">Crocodiles, aging, and the future</h2>



Henry’s enduring presence offers a chance to learn more about life at the extreme upper range of crocodile longevity. 



By exploring the intersection of genetics, environment, and microbial symbiosis, scientists may find pathways to boost disease prevention for both animals and humans.



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124-year-old crocodile challenges everything we know about aging

On December 16, Henry, the world’s oldest known crocodile, marked...

Ebola, a severe hemorrhagic disease caused by a virus endemic in parts of East-Central and West Africa, is generally known to spread through contact with bodily fluids from individuals who have the infection.&nbsp;



<h2 class="wp-block-heading" id="h-ebola-virus-on-the-skin-surface">Ebola virus on the skin surface</h2>



More recent outbreaks, such as the 2013-2016 Ebola epidemic in West Africa, have shown that infectious Ebola virus (EBOV) is also found on the surface of the <a href="https://www.earth.com/news/future-tech-will-track-emotions-through-changes-in-our-skin/" target="_blank" rel="noreferrer noopener">skin</a> of those who have succumbed to infection or at late times during infection.&nbsp;



Although this suggests that the virus can be transmitted from skin contact with someone in the later stages of the disease, researchers have not yet fully understood how the virus exits the body and appears on the skin’s surface.



In a recent study, scientists at <a href="https://uihealthcare.org/" target="_blank" rel="noreferrer noopener">University of Iowa Health Care</a>, working with colleagues at <a href="https://www.txbiomed.org/" target="_blank" rel="noreferrer noopener">Texas Biomedical Research Institute</a> and <a href="https://www.bu.edu/" target="_blank" rel="noreferrer noopener">Boston University</a>, have uncovered a cellular route that EBOV uses to traverse the inner and outer layers of skin and emerge onto the surface.&nbsp;



The researchers identified new cell types within the skin that are targeted by EBOV during infection and confirms that human skin tissues actively sustain EBOV infection.&nbsp;



<h2 class="wp-block-heading" id="h-possible-route-of-ebola-infection">Possible route of Ebola infection</h2>



The results, published in the journal <a href="http://dx.doi.org/10.1126/sciadv.adr6140" target="_blank" rel="noreferrer noopener">Science Advances</a>, suggest that the skin’s surface may be one possible route of person-to-person transmission.



“The skin is the largest organ in the human body yet is woefully understudied compared to most other organs. Interactions of EBOV with skin cells have not previously been extensively examined,” said study senior author Wendy Maury, a professor of microbiology and immunology at the University of Iowa.&nbsp;



“Our work provides evidence for one mechanistic avenue that EBOV uses to exit from the human body. A comprehensive understanding of which cells are targeted during virus infection is critical for rational development of <a href="https://www.earth.com/news/willow-bark-may-contain-life-saving-antiviral-medications/" target="_blank" rel="noreferrer noopener">antiviral</a> approaches.”



<h2 class="wp-block-heading" id="h-human-skin-model-for-tracking-ebola">Human skin model for tracking Ebola</h2>



The research team, guided by Maury and Kelly Messingham, a research professor of dermatology at the University of Iowa, designed a new method for discovering which skin cells are infected by Ebola virus.&nbsp;



They constructed a human skin explant system using full-thickness biopsies from healthy individuals, preserving both the deeper (dermal) and surface (epidermal) layers of skin.



Next, the team placed these explants dermal side down in culture media, adding virus particles to simulate how EBOV would move from the bloodstream outward toward the skin’s exterior.&nbsp;



This setup let the researchers use specialized tracing and labeling techniques to observe how the <a href="https://www.earth.com/news/how-the-covid-19-virus-travels-deep-inside-our-lungs/">virus</a> progressed from one layer of skin to the next, tracking which cells became infected as time passed.



<h2 class="wp-block-heading" id="h-skin-cells-prone-to-ebola-infection">Skin cells prone to Ebola infection</h2>



Prior clinical and animal studies indicated that skin cells could become infected with EBOV, yet they did not identify the particular cells involved.&nbsp;



In this work, the authors showed that EBOV infects several cell types in the skin explant, including macrophages, endothelial cells, fibroblasts, and keratinocytes.&nbsp;



Some of these cells are also infected by EBOV in other tissues, but keratinocytes - particular to skin - had not been previously recognized as an EBOV replication site.



Notably, the virus appeared to replicate more actively in the epidermal layer than in the dermal layer when compared on a per-gram basis. Within three days, infectious virus was detected at the epidermal surface, underscoring the virus’s ability to rapidly move through skin to the surface.



<h2 class="wp-block-heading" id="h-tool-for-exploring-new-therapies">Tool for exploring new therapies </h2>



In addition to mapping how the virus travels through the skin, the scientists demonstrated that human skin explants offer a realistic, three-dimensional model for examining potential antiviral treatments against EBOV. This model could be an economical and valuable tool for exploring new therapies.



“This study explores the role of the skin as a potential route of Ebola virus infection and identifies, for the first time, several cell types in the skin that are permissive to infection,” Messingham said.&nbsp;



“In total, these findings elucidate a mechanism by which EBOV traffics to the skin’s surface and may explain person-to-person transmission via skin contact.”



<h2 class="wp-block-heading" id="h-new-insights-into-ebola-infection-nbsp">New insights into Ebola infection&nbsp;</h2>



Beyond its discoveries about the skin, the research also zoomed in on interactions between the Ebola virus and two particular skin cell types, fibroblasts and keratinocytes.&nbsp;



The team found specific receptors on these cells that facilitate the virus’s entry, adding further clarity on how EBOV infects skin on a molecular level.



By clarifying one route the virus may take to exit the body, these findings expand our knowledge of Ebola’s spread and highlight why skin-to-skin contact in advanced cases of infection can pose such a risk.&nbsp;



<h2 class="wp-block-heading" id="h-ongoing-public-health-concern">Ongoing public health concern</h2>



Understanding these pathways, and identifying the cell types that the virus relies on, can influence future efforts to develop effective treatments and prevention measures.



This work also sets the stage for further investigations into how EBOV might exploit other organs or tissues and suggests potential ways to block the virus’s path at the skin level.&nbsp;



With Ebola remaining an ongoing global health concern, insights like these can help scientists target the virus more effectively and better protect those at risk of <a href="https://www.earth.com/news/covid-infection-equips-the-body-to-fight-off-the-flu/" target="_blank" rel="noreferrer noopener">infection</a>.



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Skin may play a hidden role in Ebola infection

Ebola, a severe hemorrhagic disease caused by a virus endemic...

Ground,Coffee,In,Coffee,Maker,Portafilter,On,Coffee,Beans,Background,

Ever wondered if the flavor of your coffee could taste even better? A simple dash of water might hold the secret to a richer, smoother cup. 



New research reveals that adding moisture to coffee beans before grinding can significantly improve brewing flavor while preventing the mess and waste often caused by static electricity.



<h2 class="wp-block-heading" id="h-why-static-electricity-matters">Why static electricity matters</h2>



Grinding <a href="https://www.earth.com/news/drinking-coffee-reduces-the-risk-of-certain-cancers/" target="_blank" rel="noreferrer noopener">coffee</a> beans produces friction as the particles collide, rub together, and break apart. This process causes the ground coffee to develop a charge, which then produces static electricity.



The charged coffee particles stick together, forming clumps that can clog grinders. These clumps make it difficult to achieve a consistent grind, leading to uneven brewing and less flavorful coffee.



Scientists have investigated the impact of this static buildup on the brewing process. Their research revealed a simple yet effective solution: adding water to the beans before grinding. 



This moisture reduces static electricity, prevents clumping, and ensures smoother grinding, which ultimately improves the quality and flavor of the brewed coffee.



"Moisture, whether it's residual moisture inside the roasted coffee or external moisture added during grinding, is what dictates the amount of charge that is formed during grinding," explained Christopher Hendon, a materials chemist at the <a href="https://www.uoregon.edu" target="_blank" rel="noreferrer noopener">University of Oregon</a>.



<h2 class="wp-block-heading" id="h-understanding-static-electricity-the-basics">Understanding static electricity -- the basics</h2>



Static electricity is what happens when there's an imbalance of tiny electric charges on the surface of an object. 



Everything around us is made up of <a href="https://www.earth.com/news/x-ray-single-atom-captured-by-scientists-for-first-time/" target="_blank" rel="noreferrer noopener">tiny particles called atoms</a>, and inside these atoms, there are even smaller particles called electrons. Electrons carry a negative charge, and they can move from one object to another.



For example, when you rub a balloon on your hair, some electrons from your hair move to the balloon, making the balloon negatively charged and your hair positively charged. This is why the balloon can stick to your hair or make your hair stand up - opposite charges attract!



We experience <a href="https://www.earth.com/news/mystery-of-static-electricity-has-finally-been-solved/" target="_blank" rel="noreferrer noopener">static electricity</a> a lot in everyday life. You might have felt it when you touch a metal doorknob and get a little shock, or when your clothes stick together after they come out of the dryer.



These shocks happen when the extra charges suddenly move from one thing to another, often through your body, which feels like a quick zap. 



Static electricity is more common in dry air because moisture in the air helps stop the buildup of charges. That’s why it tends to happen more in the winter when the air is dry.



<h2 class="wp-block-heading" id="h-science-of-better-coffee-brewing">Science of better coffee brewing</h2>



Hendon and Joshua Méndez Harper, a former volcanologist from the University of Oregon, investigated how moisture affects <a href="https://www.earth.com/news/your-coffee-is-missing-these-five-brain-boosting-spices/" target="_blank" rel="noreferrer noopener">coffee</a> grinding. 



The researchers examined coffee beans from various origins, with different roasting levels and moisture contents. 



They measured key factors such as the static electricity generated during grinding, the size of the resulting particles, and the flavor profiles of the brewed coffee.



The study revealed that darker, drier coffee roasts are more susceptible to static electricity than lighter, moister beans. 



The increased brittleness of darker roasts leads to greater friction during grinding, which causes clumping and uneven grounds.



By adding a small amount of water to the beans before grinding, the researchers showed that static electricity could be reduced. 



This simple adjustment produced a smoother grind and improved consistency, enhancing the quality of the coffee.



<h2 class="wp-block-heading" id="h-stronger-espresso-with-water">Stronger espresso with water</h2>



Harper and his team compared espresso brewed with beans ground with and without added moisture. 



They discovered that a light spritz of water not only reduced clumping but also improved the extraction process. The moist grounds allowed water to flow more evenly, and pulled more flavor from the coffee.



Hendon recommends adding about 20 microliters of water per gram of <a href="https://www.earth.com/news/robusta-coffee-could-save-our-morning-brew-from-climate-change/" target="_blank" rel="noreferrer noopener">coffee</a>, which equals roughly half a milliliter for a single shot of espresso. 



This minor adjustment not only enhances the uniformity of the grind but also ensures a stronger and tastier cup of coffee, making it a simple yet effective technique for coffee enthusiasts.



<h2 class="wp-block-heading" id="h-lessons-from-geophysics">Lessons from geophysics</h2>



The research also connects <a href="https://www.earth.com/news/healthy-aging-drinking-coffee-can-add-years-to-your-life/" target="_blank" rel="noreferrer noopener">coffee</a> science with earth science. 



"There's a lot more to know about how coffee breaks, how it flows as particles, and how it interacts with water," said Harper. 



By studying coffee, scientists hope to gain insights into broader geophysical phenomena like landslides, volcanic eruptions, and soil water flow.



These parallels highlight how everyday activities like brewing coffee can inspire scientific breakthroughs in seemingly unrelated fields.



<h2 class="wp-block-heading" id="h-spritz-your-beans-before-grinding">Spritz your beans before grinding </h2>



For coffee enthusiasts, the study provides an easy and practical tip: spritz your beans before grinding. By preventing clumping, the grinding process becomes smoother and more consistent, which leads to evenly sized grounds.



This consistency enhances the brewing process, allowing water to flow more uniformly through the coffee. 



The result is a richer and more flavorful espresso, making this method an easy way to elevate your coffee experience without requiring additional tools or complex techniques.



"A few simple squirts of water have solved the problems of clumping, channeling, and poor extractions while aiding in the pursuit of attaining the tastiest espresso," Hendon states.



So, the next time you prepare your morning brew, try adding a little water to your <a href="https://www.earth.com/news/is-coffee-good-for-you-it-may-depend-on-your-genes/" target="_blank" rel="noreferrer noopener">beans</a>. It’s a simple step with a big payoff - and who knows, your kitchen experiment might just inspire the next scientific breakthrough.



The study is published in the journal <a href="https://www.cell.com/matter/fulltext/S2590-2385(23)00568-4" target="_blank" rel="noreferrer noopener">Matter</a>.



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Coffee flavor can be greatly improved with a simple trick

Ever wondered if the flavor of your coffee could taste...

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</div>
 
Today’s Video of the Day comes from the <a href="https://www.acs.org/">American Chemical Society’s</a> Earth from Space series and features a look at how hand sanitizers kill germs.
The active ingredient in most hand sanitizers is <a href="https://www.earth.com/news/alcoholic-beverages-emotional-responses/">alcohol</a>, either in the form of ethanol, isopropanol, or n-propanol. The alcohol breaks down the outer coating of bacteria and viruses, which causes the germs to explode. 
This inhibits their ability to infect humans, rendering the germs useless. 
 &#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Video Credit: <a href="https://www.acs.org/">American Chemical Society</a>

How do hand sanitizers kill germs?