Today's Image of the Day from the European Space Agency features NGC 5335 - a barred spiral galaxy located in the constellation Virgo. 



The photo was captured by the Hubble Space Telescope. According to <a href="https://www.esa.int/ESA_Multimedia/Images/2025/04/Barred_Spiral_Galaxy_NGC_5335" target="_blank" rel="noreferrer noopener">ESA</a>, thousands of distant galaxies are speckled throughout the image in a variety of colors.&nbsp;



Hubble is revealing how <a href="https://www.earth.com/news/hidden-galaxies-discovery-would-upend-current-understanding-of-universe/" target="_blank" rel="noreferrer noopener">galaxies</a> form, grow, and evolve over cosmic time by capturing detailed images of galaxies at various stages of development, from the nearby universe to billions of light-years away. 



Hubble images have shown us that galaxies collide and merge, that star formation varies across different types of galaxies, and that supermassive black holes often lie at their centers.



<h2 class="wp-block-heading" id="h-studying-ngc-5335">Studying NGC 5335</h2>



The galaxy NGC 5335 lies approximately 160 million light-years from Earth. It is classified as an SB(s)bc type galaxy, indicating a well-defined bar structure across its center with less distinct spiral arms. The galaxy was discovered by astronomer William Herschel on May 13, 1793. 



Like many galaxies of its type, NGC 5335 features active <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">star formation</a>, especially in its spiral arms, where interstellar gas and dust provide the raw material for new stars. 



Observations in different wavelengths, including infrared and ultraviolet, help astronomers study its stellar population and the dynamics of its central bar.



<h2 class="wp-block-heading" id="h-hubble-s-view-of-the-spiral-galaxy-nbsp">Hubble’s view of the spiral galaxy&nbsp;</h2>



“NGC 5335 is categorized as a flocculent spiral galaxy with patchy streamers of star formation across its disk. There is a striking lack of well-defined spiral arms that are commonly found among galaxies, including our Milky Way,” noted ESA.



“A notable bar structure slices across the center of the galaxy. The bar channels gas inwards toward the galactic center, fueling star formation.”&nbsp;



“Such bars are dynamic in galaxies and may come and go over two-billion-year intervals. They appear in about 30 percent of observed galaxies, including our Milky Way.”



<h2 class="wp-block-heading" id="h-galactic-bar-in-the-milky-way-nbsp">Galactic bar in the Milky Way&nbsp;</h2>



The bar in the <a href="https://www.earth.com/news/astronomers-found-something-strange-at-core-of-milky-way-galaxy-webb-meerkat/" target="_blank" rel="noreferrer noopener">Milky Way</a> is a vast, elongated structure composed mostly of stars, stretching across the galaxy’s central region. It is a key feature of our galaxy’s architecture, spanning about 27,000 light-years and oriented at an angle relative to the galaxy’s spiral arms.&nbsp;



Astronomers believe it plays a crucial role in the dynamics and evolution of the Milky Way by funneling gas inward toward the galactic center, which can feed star formation and fuel the supermassive black hole at the core.&nbsp;



The bar is thought to have formed from instabilities in the galactic disk and continues to influence the motion of stars and the overall gravitational balance of the galaxy.&nbsp;



Observations in infrared and radio wavelengths, which can pierce through the dust in the galactic plane, have helped scientists map the bar’s size, shape, and orientation.



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



Virgo is one of the most prominent and well-known constellations in the night sky, both astronomically and mythologically. It is the second-largest constellation by area and lies along the zodiac, making it one of the twelve constellations through which the <a href="https://www.earth.com/news/team-creates-video-showing-the-sun-in-gamma-rays-over-a-14-year-period/" target="_blank" rel="noreferrer noopener">Sun</a> appears to move during the year. 



Virgo is most visible in the evening sky in the Northern Hemisphere during spring, particularly in April and May. Its name means “virgin” in Latin.



Virgo is traditionally associated with various fertility and agriculture goddesses across different cultures, including the Greek goddess Demeter and her daughter Persephone, as well as the Roman goddess Ceres. 



In some myths, Virgo represents Astraea, the virgin goddess of justice who fled to the heavens during the corruption of mankind.



<h2 class="wp-block-heading" id="h-astronomical-significance-of-virgo">Astronomical significance of Virgo</h2>



Astronomically, Virgo is situated between Leo to the west and Libra to the east. One of its most notable stars is Spica, the brightest star in Virgo and one of the brightest in the night sky.&nbsp;



Spica is a blue-white giant, located approximately 250 light-years from <a href="https://www.earth.com/news/was-early-earth-a-purple-planet-scientists-say-its-possible/" target="_blank" rel="noreferrer noopener">Earth</a>. It has been important for navigation and agriculture for centuries, marking planting and harvest times in ancient calendars.



Virgo is also of great interest to astronomers because it hosts the Virgo Cluster, a massive cluster of galaxies about 65 million light-years away.&nbsp;



This cluster contains more than 1,000 galaxies, and it's part of the larger Virgo Supercluster, which also includes our own Local Group of galaxies. This makes Virgo a key area for studying large-scale structures in the universe.



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Hubble spotlights galaxies in the constellation Virgo

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

Today's Image of the Day from the European Space Agency features the galaxy ESO 300-16, which is located 28.7 million light-years from Earth in the constellation Eridanus. 



The galaxy is part of the ESO (European Southern Observatory) catalog, which includes a vast collection of galaxies observed in the southern hemisphere.



ESO 300-16 is notable for its chaotic structure, lacking the well-defined <a href="https://www.earth.com/image/hubble-captures-a-collection-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">spiral arms</a> or elliptical shape seen in many other galaxies.



<h2 class="wp-block-heading" id="h-ghostly-assemblage-of-stars">Ghostly assemblage of stars</h2>



According to <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>, ESO 300-16 is a ghostly assemblage of stars which resembles a sparkling cloud.&nbsp;



"A rogue’s gallery of distant galaxies and foreground stars complete this astronomical portrait, which was captured by the Advanced Camera for Surveys," said ESA.



"This observation is one of a series which aims to get to know our galactic neighbors; around three quarters of the known galaxies suspected to lie within 10 megaparsecs of Earth have been observed by Hubble in enough detail to resolve their brightest stars and establish the distances to these galaxies."



<h2 class="wp-block-heading" id="h-irregular-galaxy-structure">Irregular galaxy structure </h2>



ESO 300-16 lies at a relatively close distance to Earth compared to many other extragalactic objects, making it an interesting target for studies on galaxy formation and <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">evolution</a>. 



The galaxy's irregular structure suggests that it may have undergone past interactions with other galaxies or is in a stage of dynamic evolution.



One of the most striking features of ESO 300-16 is its wispy, diffuse appearance, with scattered patches of bright star-forming regions embedded within a fainter background. This indicates ongoing star formation, which is a common characteristic of irregular galaxies. 



Unlike large <a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">spiral galaxies</a>, where star formation is often concentrated in well-organized arms, ESO 300-16's active regions are more randomly distributed.



<h2 class="wp-block-heading" id="h-raw-material-for-star-formation">Raw material for star formation</h2>



Due to its irregular nature, the galaxy does not have a well-defined nucleus. Instead, it appears as a loose collection of stars, gas, and dust, which astronomers can study to understand the processes shaping such galaxies. 



Irregular galaxies like ESO 300-16 are often rich in gas and dust, providing the raw material for new stars to form. 



Observations in different wavelengths, such as infrared and ultraviolet, can help reveal the presence of young, hot stars and cooler dust clouds that might be sites of future <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">star formation</a>.



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



Hubble observations of ESO 300-16 provide insight into the structure and stellar populations of the galaxy, helping astronomers piece together its history and evolutionary path. 



The study of galaxies like ESO 300-16 contributes to our broader understanding of how galaxies form and evolve, especially those that do not fit into the traditional classifications of spirals and ellipticals.



Because irregular galaxies are often shaped by gravitational interactions or past mergers, ESO 300-16 may have had a turbulent past. 



It could have once been part of a larger system before being disrupted, or it might have formed in an environment where gravitational influences from nearby galaxies prevented it from developing a more regular shape. 



Studying its motion and the distribution of its stars can provide clues about any past interactions it may have experienced.



<h2 class="wp-block-heading" id="h-a-glimpse-into-the-early-universe">A glimpse into the early universe </h2>



ESO 300-16 also provides a glimpse into what some galaxies in the early <a href="https://www.earth.com/news/universe-is-expanding-faster-than-science-can-explain-hubble-tension-physics-crisis/" target="_blank" rel="noreferrer noopener">universe</a> might have looked like. 



Many early galaxies were irregular in shape before evolving into more structured forms over time. As a result, studying nearby irregular galaxies like ESO 300-16 can offer valuable analogs for understanding galaxy formation in the distant past.



Although ESO 300-16 is not one of the most famous galaxies, it remains an important object for astronomers studying irregular galaxies, star formation, and the role of interactions in shaping galactic structures. 



Image Credit: ESA



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Ghostly galaxy in the constellation Eridanus

Today's Image of the Day from the European Space Agency features a portion of the Rosetta Nebula, captured by the Hubble Space Telescope.



The Rosetta Nebula is a vast cloud of gas and dust located in the constellation Monoceros, also known as the Unicorn. Shaped like a blooming rose in deep space, it lies about 5,200 light-years from Earth and spans roughly 100 light-years in diameter.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-the-rosetta-nebula-nbsp">Image of the Rosetta Nebula&nbsp;</h2>



“<a href="https://www.earth.com/news/35-years-of-hubble-the-telescope-that-changed-our-view-of-the-universe/" target="_blank" rel="noreferrer noopener">Hubble</a> zooms into a small portion of the nebula that is only four light-years across (the approximate distance between our Sun and the neighboring Alpha Centauri star system),” noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“Dark clouds of hydrogen gas laced with dust are silhouetted across the image. The clouds are being eroded and shaped by the seething radiation from the cluster of larger stars in the center of the nebula.”&nbsp;



“An embedded star seen at the tip of a dark cloud in the upper right portion of the image is launching jets of plasma that are crashing into the cold cloud around it. The resulting shock wave is causing a red glow. The colors come from the presence of hydrogen, oxygen, and nitrogen.”



<h2 class="wp-block-heading" id="h-distinct-appearance-of-rosetta">Distinct appearance of Rosetta</h2>



Stellar winds and ultraviolet light are gradually carving out a cavity in the nebula’s center while simultaneously triggering new waves of <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star formation</a> along its dense edges.&nbsp;



The Rosetta Nebula is often studied to understand the life cycle of stars and the complex interactions between radiation and interstellar material.&nbsp;



Its intricate structure and visual appeal have made it a favorite target for both professional astronomers and astrophotographers.



<h2 class="wp-block-heading" id="h-nebulae-that-are-similar-to-rosetta-nbsp">Nebulae that are similar to Rosetta&nbsp;</h2>



Compared to other famous nebulae, the Rosetta Nebula stands out for its symmetry and floral appearance, which give it a distinct, iconic look. It's often compared to the Orion Nebula, which is much closer to Earth at about 1,300 light-years away and far brighter in the night sky.&nbsp;



The <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion Nebula</a> is a bustling stellar nursery visible even to the naked eye, while the Rosetta requires a telescope and is more diffuse and fainter despite being larger in actual size.



The Eagle Nebula, home to the famous "Pillars of Creation," shares a similar process of star formation and sculpting by radiation, but the Eagle has more dramatic, finger-like structures.&nbsp;



<h2 class="wp-block-heading" id="h-stellar-feedback-and-cosmic-evolution">Stellar feedback and cosmic evolution</h2>



The Lagoon Nebula and the Trifid Nebula, both in the constellation Sagittarius, also resemble the Rosetta in that they are active star-forming regions, but they lie in a denser part of the <a href="https://www.earth.com/news/astronomers-found-something-strange-at-core-of-milky-way-galaxy-webb-meerkat/" target="_blank" rel="noreferrer noopener">Milky Way</a> and are often surrounded by a rich starfield.



What makes the Rosetta Nebula particularly interesting scientifically is the clear interaction between its central star cluster and the surrounding gas, offering a textbook example of how massive stars influence their environment.&nbsp;



It may not be as visually iconic as the Orion or as dynamic as the Eagle, but it's a beautiful and instructive example of stellar feedback and cosmic evolution.



<h2 class="wp-block-heading" id="h-history-of-the-rosetta-nebula-nbsp">History of the Rosetta Nebula&nbsp;</h2>



The history of the Rosetta Nebula, like many deep-sky objects, is a blend of observational discovery and increasing scientific understanding over time.&nbsp;



Although it was likely spotted by earlier astronomers, its first documented observation was in the late 17th century by John Flamsteed, the first Astronomer Royal of England.&nbsp;



However, the <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebula</a> itself was not fully recognized as a distinct object until the advent of astrophotography and improved telescopes in the 19th and 20th centuries.



<h2 class="wp-block-heading" id="h-star-clusters-of-the-enormous-cloud">Star clusters of the enormous cloud</h2>



The central star cluster, NGC 2244, was cataloged separately by William Herschel in the 18th century. Over time, astronomers realized that this cluster was embedded in a much larger, complex nebular structure.&nbsp;



As telescope technology advanced, astronomers identified several parts of the Rosetta Nebula and gave them separate designations, including NGC 2237, NGC 2238, NGC 2239, and NGC 2246 - essentially referring to different regions of the same enormous cloud.



Observations from space-based telescopes like Chandra (X-rays) and Spitzer (infrared) helped map the energetic processes inside the nebula, revealing how radiation and stellar winds from NGC 2244 are triggering the birth of new stars in its surrounding regions.



Image Credit: ESA



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Rosetta Nebula: Sculpted by starlight over millions of years

Today's Image of the Day from the European Space Agency features the spiral galaxy NGC 5643, which is located roughly 40 million light-years away in the constellation Lupus.&nbsp;



NGC 5643 belongs to the Hubble classification SBc, indicating that it is a barred spiral galaxy with loosely wound arms.&nbsp;



Its orientation, nearly face-on to Earth, provides astronomers with an exceptional view of its detailed spiral structure and central bar.



<h2 class="wp-block-heading" id="h-ngc-5643-a-grand-design-spiral-nbsp">NGC 5643: A grand design spiral&nbsp;</h2>



“NGC 5643 is what’s known as a grand design spiral, referring to how the galaxy’s two large, winding spiral arms are clear to see,” noted <a href="https://www.esa.int/ESA_Multimedia/Images">ESA</a>. “The spiral arms are defined by bright blue stars, lacy reddish-brown dust clouds and pink star-forming regions.”



“As fascinating as the galaxy appears at visible wavelengths, some of NGC 5643’s most interesting features are invisible to the human eye.”&nbsp;



<h2 class="wp-block-heading" id="h-intense-activity-in-ngc-5643">Intense activity in NGC 5643</h2>



This galaxy is notable for its Seyfert 2 nucleus, a type of active galactic nucleus (AGN). The intense activity in its core is powered by a supermassive <a href="https://www.earth.com/news/awakening-of-a-black-hole-witnessed-for-the-first-time/">black hole</a> that accretes surrounding material, emitting energy across a wide range of wavelengths.&nbsp;



“When a supermassive black hole ensnares gas from its surroundings, the gas collects in a disc that heats up to hundreds of thousands of degrees. The superheated gas shines brightly across the electromagnetic spectrum, but especially at X-ray wavelengths,” said ESA.



Observations have revealed jets and outflows of material emanating from the nucleus, likely driven by the black hole’s activity.&nbsp;



NGC 5643’s AGN has been studied extensively for its role in galactic evolution, particularly in how its energetic processes interact with the galaxy’s interstellar medium.



<h2 class="wp-block-heading" id="h-the-mystery-of-ngc-5643-x-1">The mystery of NGC 5643 X-1</h2>



ESA pointed out that NGC 5643’s active galactic nucleus isn’t the brightest source of X-rays in the galaxy. 



“Researchers using ESA’s XMM-Newton discovered an even brighter X-ray-emitting object, called NGC 5643 X-1, on the galaxy’s outskirts. What could be a more powerful source of X-rays than a <a href="https://www.earth.com/news/how-do-black-holes-become-supermassive/">supermassive black hole</a>?”&nbsp;



“Surprisingly, the answer appears to be a much smaller black hole! While the exact identity of NGC 5643 X-1 is not yet known, evidence points to a black hole that is about 30 times more massive than the Sun.”&nbsp;



“Locked in an orbital dance with a companion star, the black hole ensnares gas from its stellar companion, creating a superheated disc that outshines the galactic center,” said ESA.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-5643">Star formation in NGC 5643</h2>



NGC 5643 also exhibits prominent regions of <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/">star formation</a> within its spiral arms. These areas are rich in gas and dust - the raw materials for birthing new stars - and glow brightly in ultraviolet and infrared light.&nbsp;



Observations from the Hubble Space Telescope and the Very Large Telescope (VLT) have helped uncover the complex interplay between star formation and the galaxy's central activity.



<h2 class="wp-block-heading" id="h-extended-ionized-gas-regions-nbsp">Extended ionized gas regions&nbsp;</h2>



A defining feature of NGC 5643 is the presence of its extended ionized gas regions, which are shaped by the galaxy's AGN activity and star-forming regions.&nbsp;



These structures have been mapped through optical spectroscopy, revealing intricate patterns that help astronomers understand the physical conditions of the gas, such as density, temperature, and composition.



The galaxy also has a dust lane that crosses its nucleus, partially obscuring direct observations of the central region in visible light.&nbsp;



Overall, NGC 5643 offers a fascinating glimpse into the dynamics of barred <a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/">spiral galaxies</a> with active nuclei, serving as a valuable resource for studying the interactions between supermassive black holes, star formation, and galactic evolution.



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



Lupus is a constellation located in the southern sky, its name meaning "wolf" in Latin. It has been known since antiquity and was cataloged by the Greek astronomer Ptolemy.&nbsp;



Once part of the larger constellation Centaurus, Lupus was later recognized as a distinct constellation. It is relatively faint but holds historical significance in mythology, often associated with a sacrificial wolf in ancient stories.



Lupus is bordered by other constellations like Scorpius, Centaurus, and Libra. Its stars do not form a particularly striking pattern, but it contains a variety of interesting astronomical features. Among them are numerous double stars, globular clusters, and other deep-sky objects, visible through telescopes.&nbsp;



For observers in the Southern Hemisphere, Lupus is best seen in the winter and spring months, while it appears closer to the horizon for those in northern latitudes.



This constellation also lies along the <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/">Milky Way</a>, offering a rich field of stars and nebulae for stargazers. Despite its modest brightness, Lupus holds a special place in the science of astronomy.



Image Credit: NASA/ESA Hubble Space Telescope



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Secrets of a spiraling galactic powerhouse

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



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



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



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



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



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc-1333">Webb’s view of NGC 1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC 1333 cloud.&nbsp;



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



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



<h2 class="wp-block-heading" id="h-stars-in-the-sun-s-birth-cluster">Stars in the Sun's birth cluster</h2>



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



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



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



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



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



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



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



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



<h2 class="wp-block-heading" id="h-early-stages-of-planet-formation">Early stages of planet formation </h2>



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



These stars are still in the process of gathering material and developing protoplanetary disks. 



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



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



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



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



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



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



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



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Stellar nursery shines in the Perseus cloud

An octopus taking a piggyback ride on a shark might sound like a tall tale. Yet a surprising video from the waters near New Zealand has given ocean-watchers cause to scratch their heads.



Marine biology professor <a href="https://profiles.auckland.ac.nz/r-constantine" target="_blank" rel="noreferrer noopener">Rochelle Constantine</a> from the <a href="https://www.auckland.ac.nz/en.html" target="_blank" rel="noreferrer noopener">University of Auckland</a> was on hand to document this unusual sight. 



She spotted a <a href="https://www.earth.com/news/blue-ringed-octopus-a-master-of-deception-inspires-new-technology/" target="_blank" rel="noreferrer noopener">bright octopus</a> clinging to a powerful <a href="https://oceana.org/marine-life/shortfin-mako-shark/" target="_blank" rel="noreferrer noopener">shortfin mako</a> shark, the fastest of its kind in open ocean waters.



<h2 class="wp-block-heading" id="h-sharks-and-octopuses-aren-t-typically-friends">Sharks and octopuses aren't typically friends</h2>



This get-together was no mild meeting of acquaintances. The shark was swimming along without appearing bothered by its unusual passenger, while the octopus held on with all of its eight arms.



"The ocean is filled with unexpected things," stated Constantine, in a <a href="https://www.auckland.ac.nz/en/news/2025/03/11/sharks-.html" target="_blank" rel="noreferrer noopener">note</a> shared after the research trip. Reports suggest the creature stuck close to the shark’s dorsal area.&nbsp;



<h2 class="wp-block-heading" id="h-technology-helped-catch-the-octopus-ride">Technology helped catch the octopus ride</h2>



Without modern tools, this strange event would’ve gone unnoticed. The research team launched a drone and used a GoPro to get a clear view of what was really on the shark’s back.



Drones and waterproof cameras have become essential equipment for marine science. They let researchers monitor wildlife safely and document rare behaviors without disturbing the animals.



<h2 class="wp-block-heading" id="h-shortfin-mako-s-swift-reputation">Shortfin mako’s swift reputation</h2>



Many people find the shortfin <a href="https://www.earth.com/news/first-global-photos-of-killer-whales-attacking-the-enigmatic-prickly-shark/">mako</a> shark intriguing. It holds the title for the highest speed among all sharks, clocking more than 40 miles (64 kilometers) per hour.



These sharks grow to impressive sizes, often stretching nearly 12 feet (3.7 meters). Their streamlined bodies and aerodynamic fins help them chase swift prey like tuna and even other sharks.



<h2 class="wp-block-heading" id="h-how-the-octopus-got-on-the-shark">How the octopus got on the shark</h2>



While sharks command plenty of attention, the octopus is no <a href="https://www.earth.com/news/turquets-octopus-dna-tells-scientists-that-west-antarctic-ice-sheet-collapse-is-close/">minor figure</a>. Octopuses are known for their flexible bodies, color-changing abilities, and knack for staying out of harm’s way.



Scientists believe <a href="https://www.earth.com/news/world-octopus-day-the-intelligent-creatures-of-the-sea/" target="_blank" rel="noreferrer noopener">octopuses sense vibrations</a> through the water, making them skilled at evading predators. 



Their soft tissues allow them to slip through narrow spaces, which raises questions about how one ended up on the back of a large shark.



Encounter stories like these usually come from hidden pockets of the ocean. This unexpected duo popped up near the northern coast of New Zealand’s North Island.



"Incredible moments like this remind us there is more we don’t know than we do," remarked Constantine. She and her team observed the hitchhiking octopus for a short while before it continued onward.



<h2 class="wp-block-heading" id="h-what-might-the-octopus-be-thinking">What might the octopus be thinking?</h2>



Octopuses have been seen using tools, escaping tight spots, and even unscrewing the lids of jars from the inside. 



Some <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC8499036/" target="_blank" rel="noreferrer noopener">scientists</a> believe they have short-term memory and a basic sense of planning, which might suggest that this hitchhiking event wasn’t purely accidental.



Could the octopus have been hiding from a predator, or trying to explore a new environment? Researchers don’t yet know. 



But holding tight to a moving shark might have offered camouflage, faster travel, or just a brief break from danger in open waters.



<h2 class="wp-block-heading" id="h-why-does-any-of-this-matter">Why does any of this matter?</h2>



Shortfin mako sharks face threats from commercial fishing and the global fin trade. They are listed as <a href="https://www.iucnredlist.org/species/39341/2903170" target="_blank" rel="noreferrer noopener">endangered</a> by the International Union for Conservation of Nature.



Although efforts to regulate shark fishing exist, bycatch remains a major concern. Mako sharks reproduce slowly, so their numbers can’t easily recover after heavy fishing pressure.



Odd encounters can teach scientists new things about predator-prey behaviors. Sharks usually swim near the surface, while octopuses often stick to the <a href="https://www.earth.com/news/the-octopus-has-mastered-the-art-of-multispecies-hunting/">seafloor</a>, which makes the partnership puzzling.



Data on these interspecies moments can hint at changes in ocean conditions, habitats, or species movements. <a href="https://www.earth.com/news/warming-seas-impair-octopus-vision-to-a-critical-extent/" target="_blank" rel="noreferrer noopener">Spotting an octopus</a> in open water might be a signal about local currents or unusual feeding patterns.



<h2 class="wp-block-heading" id="h-sharks-and-octopuses-grab-attention">Sharks and octopuses grab attention</h2>



When species behave in ways that don’t match typical patterns, it forces scientists to recheck assumptions. 



An octopus <a href="https://www.earth.com/news/unprovoked-shark-attacks-dropped-to-record-low-in-2024/">riding</a> a shark may seem like a one-off event, but it raises deeper questions about movement, interaction, and adaptability in marine life.



Unusual pairings like this one can highlight stressors in the ecosystem, such as food scarcity, habitat shifts, or climate-related disruption. 



Even a short encounter, captured by chance, might help piece together a larger puzzle about how animals are adjusting to human-altered oceans.



<h2 class="wp-block-heading" id="h-what-happens-next">What happens next?</h2>



People sometimes label sharks as dangerous. Videos showing a calm mako might reshape how some view these agile hunters.



Similarly, an octopus is no simple <a href="https://videos.fisheries.noaa.gov/detail/videos/b-roll-packages---all/video/5231307735001/b-roll:-octopus-giant-pacific-research-in-alaska">creature</a>. Researchers have found them to be quite intelligent, capable of short-term problem-solving and playful exploration.



There is still much to learn about how often such hitchhikes happen or why they occur. Marine experts encourage curious minds to support healthy ecosystems by reducing pollution and changing harmful fishing methods.



"One of the best things about being a marine scientist is that you never know what you might see next in the sea," wrote Constantine. When wild animals surprise us, it can spark fresh interest in protecting them and their homes.



Click here to <a href="https://youtu.be/3cYlBarkmDY?si=-NlGKY3j2HeJieCC" target="_blank" rel="noreferrer noopener">watch the video of an octopus riding a shark...</a>



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Octopus caught riding on the back of the world's fastest shark in the open ocean

An octopus taking a piggyback ride on a shark might...

When was the last time you sat quietly in a garden, and let your eyes wander without a goal? Observation gardens are built for moments like these. They give people space to simply look, breathe, and feel present.



But beyond offering a peaceful break, these green spaces may do something even more valuable - they could help us manage <a href="https://www.earth.com/news/stress-eats-away-our-brains-cognitive-defenses/" target="_blank" rel="noreferrer noopener">stress</a>.



<h2 class="wp-block-heading" id="h-some-gardens-are-more-relaxing">Some gardens are more relaxing </h2>



A group of scientists recently explored why some gardens are more calming and relaxing than others. The research was focused on Kyoto’s Murin-an garden, a famous example of Japanese design, and compared it to a less carefully maintained university garden.



The team’s findings reveal why these special <a href="https://www.earth.com/news/green-spaces-near-homes-reduce-emotional-problems-in-children/" target="_blank" rel="noreferrer noopener">green spaces</a> soothe the mind. The study was a joint effort by <a href="https://en.nagasaki-u.ac.jp/" target="_blank" rel="noreferrer noopener">Nagasaki University</a> and the University of Pittsburgh. 



"Unlike most gardens where a visitor is expected to move through its space and appreciate its elements from many different visual perspectives, an observation garden is designed to be viewed while seated at a single vantage point," noted the researchers.



"Indeed, the location of this vantage point is a critical design feature that is carefully chosen to maximize the impact of the visual scene."



<h2 class="wp-block-heading" id="h-studying-the-calming-effect-of-gardens">Studying the calming effect of gardens</h2>



The research team set out to investigate how the design of a garden affects our stress levels.



The scientists brought 16 students to two different gardens in Kyoto. One was Murin-an, known for its meticulous design and care. The other was a university garden that was more ordinary and less groomed.



Each participant spent seven minutes in each setting, observing the scenery. During this time, researchers tracked their eye movements and heart rates. They also asked about their mood before and after each visit.



“Well-designed Japanese gardens have evocative and abstract sceneries designed in great detail. These sceneries encourage the viewer to observe longer to understand the composition and meaning of the <a href="https://www.earth.com/news/sunsets-have-a-wow-factor-that-adds-value-to-landscapes/" target="_blank" rel="noreferrer noopener">scenery</a>, while the gaze wanders more and faster,” said Professor Seiko Goto of Nagasaki University, who specializes in landscape architecture.



<h2 class="wp-block-heading" id="h-gaze-patterns-that-ease-the-mind">Gaze patterns that ease the mind</h2>



The results showed clear differences. In the Murin-an garden, people’s eyes moved more quickly across the scene. Their gazes shifted from one detail to another, covering a wider area. This was not the case in the university garden, where people mostly stared at the central features.



“We found a correlation of rapid gaze shifts and a reduction in heart rate and improved <a href="https://www.earth.com/news/sleep-timing-has-a-powerful-effect-on-our-mood/" target="_blank" rel="noreferrer noopener">mood</a>. The reduction in stress experienced by viewers of a well-crafted Japanese garden is largely due to the design features that lead the viewer to engage in frequent, rapid horizontal shifts in gaze,” explained Professor Karl Herrup, a neurobiologist at the University of Pittsburgh.



Maintenance also played a key role. A clean, well-pruned space invites the eye to keep moving. 



“To induce such close attention of the viewer, not only quality of design but also quality of the maintenance is important,” said Goto. “Viewers’ gaze keeps moving to seek more fascination on the well pruned trees and speckless ground.”



<h2 class="wp-block-heading" id="h-gardens-as-everyday-therapy">Gardens as everyday therapy</h2>



Beyond visual tracking, participants reported feeling more relaxed in the Murin-an garden. They liked it more, felt calmer, and expressed a stronger desire to return. Their heart rates also slowed, hinting at a true physiological response.



Interestingly, both gardens had similar features: water elements, stones, trees, and a bridge. But the way these elements were arranged made all the difference. In Murin-an, the design leads the eyes sideways, flowing with the layout. The university garden, by contrast, drew attention to one central spot.



“The Murin-an garden was designed as a viewing garden that should be appreciated from a specific vantage point relative to the design elements,” said Herrup. “It is this attention to detail that coaxes the eyes into the patterns that relieve stress.”



<h2 class="wp-block-heading" id="h-a-simple-pleasure-with-big-potential">A simple pleasure with big potential</h2>



The researchers acknowledge some limitations of their study. They had a short window of access to the gardens, and all of the participants were university students. 



Yet, previous research suggests that the calming effects of gardens apply across different ages, backgrounds, and even cognitive conditions. The experts also see potential for these findings to support people with <a href="https://www.earth.com/news/coffee-grounds-could-help-prevent-neurodegenerative-diseases/" target="_blank" rel="noreferrer noopener">neurodegenerative diseases</a>.



“Gardens are generally seen as a hobby for the wealthy, but if appreciating Japanese gardens can induce a relaxing effect, which intuitively everyone feels, it could be used as a form of therapy in hospitals and welfare facilities,” Goto concluded. 



“I think it would be good if Japanese gardens are built not just as a luxury but as a means of mental care in our aging society.”



The full study was published in the journal <a href="https://www.frontiersin.org/journals/neuroscience/articles/10.3389/fnins.2025.1581080/full" target="_blank" rel="noreferrer noopener">Frontiers in Neuroscience</a>.



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Why some gardens are more calming than others

When was the last time you sat quietly in a...

Headshot,Of,Ant,Orange,In,The,Argentine,Jungle.,(linepithema,Humile)

Ants march across sidewalks and kitchen counters as if they own the place. They cross oceans inside cargo ships, set up vast super-colonies, and push out native species on six continents. 



Once a <a href="https://www.earth.com/news/how-many-ants-live-on-earth-at-any-point-in-time-total-number-is-astounding/" target="_blank" rel="noreferrer noopener">nest of ants</a> settles in, homeowners and farmers often reach for poison baits, yet the insects lose interest before enough of them carry the toxic treat back home. 



A new study suggests that a tiny splash of caffeine could keep the party going - and give pest managers an edge.



The research shows that moderate doses of caffeine sharpen an ant’s memory for the bait’s location. Ants that sipped a caffeinated sugar drop found it again more quickly on later trips, leaving a stronger scent trail for nest-mates. 



The discovery points to a low-cost tweak that might finally turn the <a href="https://www.earth.com/news/ants-perform-life-saving-amputation-surgeries-on-injured-nest-mates/" target="_blank" rel="noreferrer noopener">invader’s own teamwork</a> against it.



<h2 class="wp-block-heading" id="h-tiny-ant-huge-impact">Tiny ant, huge impact</h2>



The Argentine ant (Linepithema humile) is only about one-tenth of an inch long, yet its cooperative spirit builds super-colonies stretching thousands of miles along the Mediterranean coast and the U.S. West Coast. 



Those armies displace local insects, rob hummingbird feeders, and even short-circuit electrical gear. 



Recent economic analyses peg the global cost of <a href="https://www.earth.com/news/ants-are-shifting-to-new-habitats-to-cope-with-climate-change/" target="_blank" rel="noreferrer noopener">invasive ants</a> - including crop losses and control bills - at billions of dollars each year. No wonder pest crews keep searching for smarter tactics.



<h2 class="wp-block-heading" id="h-giving-caffeine-to-ants">Giving caffeine to ants</h2>



To find out, researchers set up a miniature arena: a Lego drawbridge led each ant onto a letter-size acrylic platform where a single sugar drop waited. 



Some drops carried no additive, while others contained 25 parts per million (ppm), 250 ppm, or 2 000 ppm of caffeine. One hundred forty-two ants took part, and each explorer tackled the course four times.



“The idea with this project was to find some cognitive way of getting the ants to consume more of the poisonous baits we put in the field,” says the study’s first author Henrique Galante, a computational biologist at the <a href="https://www.uni-regensburg.de/en" target="_blank" rel="noreferrer noopener">University of Regensburg</a>. 



Automated cameras tracked every step, logging travel time and the straightness of each path. Without caffeine, the insects wandered, needing the same span to reach the treat on every attempt. Add a modest stimulant, and the story changed.



<h2 class="wp-block-heading" id="h-caffeine-gives-ant-focus-not-speed">Caffeine gives ant focus, not speed</h2>



“We found that intermediate <a href="https://www.earth.com/news/caffeine-evolution-in-plants-the-surprising-story-of-yerba-mate/" target="_blank" rel="noreferrer noopener">doses of caffeine</a> actually boost learning - when you give them a bit of caffeine, it pushes them into having straighter paths and being able to reach the reward faster," Galante explained.



In fact, ants that tasted 25 ppm caffeine shaved 28 percent off their foraging time on every return. Those on 250 ppm cut the clock by 38 percent. 



Picture an individual that spent 300 seconds during its first outing - it would need just 113 seconds after three more trips on the lower dose and 54 seconds on the medium dose.



<a href="https://www.earth.com/news/caffeine-consumption-may-lower-the-risk-of-dementia/" target="_blank" rel="noreferrer noopener">The stimulant</a> did not act like an energy drink. There was no uptick in raw speed. “What we see is that they're not moving faster, they're just being more focused on where they're going,” Galante noted. 



“This suggests that they know where they want to go, therefore, they have learned the locations of the reward.” 



Only path geometry tightened; pace stayed the same. At the heaviest 2 000 ppm dose - the level that kills half of honeybees in tests - the learning advantage disappeared.



<h2 class="wp-block-heading" id="h-sharper-trails-deadlier-bait">Sharper trails, deadlier bait</h2>



Argentine ants rely on <a href="https://www.earth.com/news/ants-are-now-using-cars-to-travel-spread-to-new-locations/" target="_blank" rel="noreferrer noopener">pheromone highways</a>. A worker that discovers food drags its stinger along the ground, laying a chemical breadcrumb trail that guides the next shift. Faster relearning multiplies that effect. 



“We're trying to make them better at finding these baits, because the faster they go and come back to them, the more pheromone trails they lay, the <a href="https://www.earth.com/news/evolutionary-deja-vu-the-symbiotic-relationships-of-trees-and-ants/" target="_blank" rel="noreferrer noopener">more ants will come</a>, and, therefore, the faster they will spread the poison in the colony before they realize it's poison,” Galante continued.



Adding caffeine could also slash the waste that now limits bait stations. In neighborhoods and orchards, technicians often replenish gels every few days because the first wave of foragers gives up. 



A caffeinated lure might stay attractive long enough for queens and larvae to receive a lethal serving.



<h2 class="wp-block-heading" id="h-what-happens-next">What happens next</h2>



The team is already field-testing the recipe at infested sites in Spain. They also plan to check whether caffeine interacts with common active ingredients such as hydramethylnon or spinosad. 



“The lowest dose we used is what you find in natural plants, the intermediate dose is similar to what you would find in some energy drinks, and the highest amount is set to be the LD50 of bees - where half the bees fed this dose die - so it's likely to be quite toxic for them,” Galante notes. 



Selecting a concentration that boosts memory without harming pollinators will be crucial.



Caffeine’s appeal extends beyond Argentine ants. Other <a href="https://www.earth.com/news/dirt-ants-were-once-masters-of-disguise-in-the-caribbean/" target="_blank" rel="noreferrer noopener">invasive species</a> - including fire ants and big-headed ants - share the same food-sharing habits that make baiting tricky. 



If the stimulant nudges their neural circuits in a similar way, managers could deploy a single additive across multiple pest fronts.



<h2 class="wp-block-heading" id="h-what-we-learned-about-ants-and-caffeine">What we learned about ants and caffeine</h2>



To sum it all up, caffeine improves ants' overall focus and learning without increasing speed, allowing them to navigate straighter paths and lay stronger pheromone trails. 



This effect boosts the effectiveness of bait traps, leading more ants to the poison and increasing the chances of it spreading through the colony. 



However, the benefit peaks at moderate doses - very high levels eliminate the learning advantage and can be toxic. So, overall, caffeine makes ants better at foraging and sharing, which ironically makes them more vulnerable to well-designed pest control strategies.



For now, the message is simple: a dash of coffee in the buffet may turn an army’s fabled navigation skills against itself. When the ants get better at remembering dessert, the colony’s days could finally be numbered.



The full study was published in the journal <a href="https://www.cell.com/iscience/fulltext/S2589-0042(24)01157-X" target="_blank" rel="noreferrer noopener">iScience</a>.



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When you give caffeine to ants, many interesting things happen

Ants march across sidewalks and kitchen counters as if they...

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Deconstructing a Mobile Home Chapter 4: Safety

Deconstructing a Mobile Home Chapter 4: Safety

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