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



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



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



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



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



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



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



There are two main types of supernovae, classified based on their causes. Type I supernovae occur when a <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/" target="_blank" rel="noreferrer noopener">white dwarf</a> in a binary system accretes material from its companion star, eventually reaching a critical mass and triggering a runaway nuclear reaction.&nbsp;



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA&nbsp;



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Hubble spots a supernova in the constellation Gemini 

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

Today's Image of the Day from NASA Earth Observatory features a satellite view of retreating glaciers in Alaska, where meltwater is rapidly expanding glacial lakes. 



“In parts of Alaska, water is replacing ice. As glaciers thin and <a href="https://www.earth.com/news/satellite-images-reveal-hidden-retreat-of-arctic-glaciers/" target="_blank" rel="noreferrer noopener">retreat</a>, meltwater collects at their fronts, forming proglacial lakes. According to an analysis by Mauri Pelto, a glaciologist at Nichols College, three such lakes in the southeastern part of the state have grown rapidly in recent decades,” said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



<h2 class="wp-block-heading" id="h-retreating-glaciers-in-alaska">Retreating glaciers in Alaska</h2>



“A trio of glaciers - Yakutat, Alsek, and Grand Plateau - descend from inland mountains and flow onto the coastal plain southeast of Yakutat borough, ending at Harlequin Lake, Alsek Lake, and Grand Plateau Lake,” noted NASA.&nbsp;



The retreat of the glaciers, as well as the growth of the lakes, are visible in the image. When compared to an <a href="https://eoimages.gsfc.nasa.gov/images/imagerecords/153000/153638/fastestlake_tm5_19840705_lrg.jpg" target="_blank" rel="noreferrer noopener">image</a> captured by Landsat 5 in the summer of 1984, the changes are even more evident.



NASA elaborated on the extent of the glacier retreat from 1984 to 2024. “During this period, Yakutat Glacier’s main arm retreated 4.3 miles, while Alsek Glacier’s northern and southern arms retreated 3.3 miles and 3.4 miles, respectively. Grand Plateau Glacier’s northern arm lost the most, retreating 4.8 miles.”



<h2 class="wp-block-heading" id="h-glacial-lakes-doubled-in-size-nbsp">Glacial lakes doubled in size&nbsp;</h2>



“Collectively, the three lakes more than doubled in size over 40 years. In 1984, they covered about 50 square miles. By 2024, they spanned 90 square miles. That’s an area larger than Seneca Lake (67 square miles) - one of the Finger Lakes in New York, which also have a glacial origin,” said NASA.



Pelto noted that the lakes forming in this region are immense - starting at the mountains and spreading toward the coast - making this a new lake district that is unique in our nation.



“Millions of other lakes, named and unnamed, dot the state. But this system has grown fast, so much so that Pelto thinks it might represent the fastest lake growth in the United States this century,” said NASA.



<h2 class="wp-block-heading" id="h-understanding-glacier-retreat-nbsp">Understanding glacier retreat&nbsp;</h2>



Glacier retreat is a significant phenomenon driven primarily by global warming the results from rising greenhouse gas <a href="https://www.earth.com/news/global-carbon-dioxide-emissions-hit-a-record-high-in-2023/" target="_blank" rel="noreferrer noopener">emissions</a>.&nbsp;



As temperatures rise, glaciers lose more ice during the summer melt than they can regain in winter snowfall, causing them to shrink over time. This process has profound implications for ecosystems, water resources, and global sea levels.



<h3 class="wp-block-heading" id="h-glacial-lakes">Glacial lakes</h3>



When glaciers retreat, they often leave behind depressions in the landscape that can fill with meltwater, forming glacial lakes. These lakes are typically bounded by natural dams made of rock, ice, or moraine - accumulations of debris left behind by the glacier's movement.&nbsp;



Over the past century, the number and size of glacial lakes worldwide have increased significantly due to the accelerating pace of <a href="https://www.earth.com/news/tropical-glaciers-offer-a-glimpse-of-our-harsh-climate-reality/" target="_blank" rel="noreferrer noopener">glacier</a> retreat. This trend is especially evident in high-altitude regions like the Himalayas, the Andes, and the Alps, as well as in polar areas such as Alaska and Greenland.



<h3 class="wp-block-heading" id="h-positive-and-negative-impacts-nbsp">Positive and negative impacts&nbsp;</h3>



Glacial lakes can have both positive and negative impacts. They provide critical water sources for downstream communities, support biodiversity, and sometimes offer opportunities for hydropower development or tourism.&nbsp;



However, they also pose serious risks. The dams holding back these lakes can fail suddenly, causing glacial lake outburst floods (GLOFs). These catastrophic events can devastate downstream areas, destroying infrastructure, agricultural lands, and habitats while endangering human lives.



<h3 class="wp-block-heading" id="h-monitoring-changes">Monitoring changes</h3>



Understanding glacier retreat and glacial lake formation requires a multidisciplinary approach, combining climate science, hydrology, and geology.&nbsp;



Monitoring these changes is essential to mitigate associated risks and adapt to the evolving landscape shaped by a <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fperu-has-lost-over-half-of-its-glaciers-in-six-decades%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">warming planet</a>.



<h2 class="wp-block-heading" id="h-glacier-retreat-worldwide">Glacier retreat worldwide</h2>



Studies and satellite observations show that most glaciers in almost all regions of the world are shrinking.&nbsp;



Melting glaciers contribute significantly to global <a href="https://www.earth.com/news/emergency-meeting-reveals-the-alarming-extent-of-antarcticas-ice-loss/" target="_blank" rel="noreferrer noopener">sea level rise</a>, which threatens coastal communities and ecosystems.



The retreat of glaciers is considered one of the clearest indicators of climate change.&nbsp;Some glaciers are retreating at unprecedented rates, indicating accelerating climate impacts.



The image was captured on August 4, 2024 by the Landsat 8 satellite.



Image Credit: NASA Earth Observatory



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Retreating glaciers and expanding meltwater lakes in Alaska

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

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

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.&nbsp;



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.&nbsp;



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.&nbsp;



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.&nbsp;



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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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 UGC 5460, a spiral galaxy that is located about 60 million light-years away in the constellation Ursa Major.&nbsp;



“This image combines four different wavelengths of light to reveal UGC 5460’s central bar of stars, winding spiral arms and bright blue star clusters. Also captured in the upper left-hand corner of this image is a far closer object: a star just 577 light-years away in our own galaxy,” said <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“UGC 5460 has hosted two recent supernovae named SN 2011ht and SN 2015as. It’s because of these two stellar explosions that Hubble targeted this galaxy, collecting data for three observing programmes that aim to study various kinds of supernovae.”&nbsp;



<h2 class="wp-block-heading" id="h-a-core-collapse-supernova-nbsp">A core-collapse supernova&nbsp;</h2>



SN 2015as is an example of a core-collapse supernova. This type of <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> occurs when the core of a massive star - typically with more than 8 times the mass of the sun - can no longer support its own gravity after exhausting its nuclear fuel. 



This causes the core to collapse under its own weight, leading to an extremely violent explosion. The collapse triggers the release of an enormous amount of energy, expelling the outer layers of the star into space.



In the aftermath of the explosion, a dense <a href="https://www.earth.com/news/shockingly-bright-carbon-monoxide-detected-in-supernova-remnant/" target="_blank" rel="noreferrer noopener">remnant</a> is created. This is often a neutron star or black hole, depending on the mass of the original star. Core-collapse supernovae are some of the most powerful events in the universe.



According to ESA, Hubble observations of SN 2015as will help researchers understand what happens when the expanding shockwave of a <a href="https://www.earth.com/news/supernova-dandelion-year-1181-leaves-behind-zombie-star-defying-death/" target="_blank" rel="noreferrer noopener">supernova</a> collides with the gas that surrounds the exploded star.



<h2 class="wp-block-heading" id="h-rare-stars-with-large-eruptions-nbsp">Rare stars with large eruptions&nbsp;</h2>



“SN 2011ht might have been a core-collapse supernova as well, but it could also be an impostor called a luminous blue variable. Luminous blue variables are rare stars that experience eruptions so large that they can mimic supernovae,” noted ESA.



“Crucially, luminous blue variables emerge from these eruptions unscathed, while stars that go supernova do not. Hubble will search for a stellar survivor at SN 2011ht’s location, and the explosion’s identity may be revealed at last.”



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



Spiral galaxies are some of the most recognizable and beautiful structures in the universe. They are known for their distinctive arms that spiral outward from a central bulge.&nbsp;



These galaxies are typically composed of stars, gas, dust, and dark matter. The arms are often sites of intense <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>, where clouds of gas collapse to form new stars. 



In the center of a spiral galaxy lies a dense concentration of older stars and, often, a supermassive black hole.



<h2 class="wp-block-heading" id="h-structure-of-a-spiral-galaxy-nbsp">Structure of a spiral galaxy&nbsp;</h2>



The structure of a spiral galaxy is generally divided into three main components: the disk, the bulge, and the halo.&nbsp;



The disk is where the spiral arms are located and contains most of the galaxy's visible stars and interstellar medium.&nbsp;



The bulge is a tightly packed region of older stars at the core, and the halo consists of a sparse collection of stars and globular clusters that surround the galaxy.&nbsp;



Spiral galaxies can be classified into different types based on the tightness and number of their spiral arms, as well as the size of their central bulge.



<h2 class="wp-block-heading" id="h-the-milky-way-galaxy">The Milky Way galaxy</h2>



Our solar system is located within a large spiral galaxy known as the Milky Way. The name refers to its appearance as a dim, milky band of light stretching across the night sky.&nbsp;



The term "Milky Way" comes from ancient Greek mythology, where it was associated the goddess Hera's milk spilling into the sky. In Greek, it was called "Galaxias Kyklos," meaning "milky circle."&nbsp;



Spanning about 100,000 light-years in diameter, the Milky Way is composed of stars, gas, dust, and dark matter. The galaxy has a distinct disk shape with spiral arms that wind outward from a central bulge, which houses a supermassive <a href="https://www.earth.com/news/milky-ways-black-hole-unleashes-mysterious-flares/" target="_blank" rel="noreferrer noopener">black hole</a>. 



Our sun is located in one of the spiral arms - known as the Orion Arm - positioned roughly halfway from the center to the outer edge.&nbsp;



The Milky Way is part of a small group of galaxies called the Local Group, which includes the Andromeda Galaxy and several smaller galaxies.



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Hubble views a spiral galaxy with stellar explosions

The blue lotus, a captivating water lily entwined with Egyptian mythology, has long dazzled archaeologists and historians. Its petals were famously found adorning King Tutankhamun’s mummy, and its image flourishes in ancient scrolls and temple art.&nbsp;



For decades, scholars have speculated that the flower held powerful psychedelic properties - used in wine-soaked rituals steeped in ecstasy and divine visions.



Today, a plant bearing the same name is sold widely online, promising everything from tranquility to heightened awareness. But according to <a href="https://www.berkeley.edu/" target="_blank" rel="noreferrer noopener">UC Berkeley</a> anthropology student Liam McEvoy, those modern offerings have little in common with the true blue <a href="https://www.earth.com/earthpedia-articles/how-does-a-lotus-flower-grow/" target="_blank" rel="noreferrer noopener">lotus</a> of antiquity.



McEvoy has spent years tracing the story of Nymphaea caerulea, the authentic Egyptian blue lotus. With a minor in Egyptology and support from the UC Berkeley Center for the Science of Psychedelics, he’s dug into ancient texts, collaborated with chemists, and even turned to Reddit to track down specimens.&nbsp;



McEvoy’s findings reveal that the plant revered in ancient Egypt is not the same as the water lilies currently sold in online marketplaces - and that both the species and its supposed effects have been widely misunderstood.



<h2 class="wp-block-heading" id="h-the-story-of-the-egyptian-blue-lotus-nbsp">The story of the Egyptian blue lotus&nbsp;</h2>



McEvoy’s journey began unexpectedly during high school when he stumbled upon an old BBC documentary called Sacred Weeds. In it, researchers gave participants wine infused with lotus petals and watched to see if they entered a <a href="https://www.earth.com/news/magic-mushrooms-are-the-most-popular-psychedelic-drug/" target="_blank" rel="noreferrer noopener">psychedelic</a> state. The footage, complete with dated special effects and questionable methodology, left a lasting impression.



He was hooked. “I wanted to let the plant tell its story and contribute to a discussion where there's all this pseudoscience floating around - pseudoscience that makes some people a lot of money.”



Once at Berkeley, McEvoy dove deeper. Through coursework and work at the <a href="https://hearstmuseum.berkeley.edu/" target="_blank" rel="noreferrer noopener">Phoebe A. Hearst Museum of Anthropology</a>, he learned to read hieroglyphs and came to recognize the true Egyptian blue lotus by its distinctive spotted sepals and consistent petal count.&nbsp;



It appeared again and again in scrolls and religious festivals, most notably in the Hathoric Festival of Drunkenness - an event where celebrants drank themselves into a stupor and awoke, if only briefly, to see the face of the goddess Hathor.



<h2 class="wp-block-heading" id="h-flowers-sold-as-blue-lotus">Flowers sold as blue lotus</h2>



The more McEvoy studied, the more he questioned whether the flowers sold online as “blue lotus” were the real thing.&nbsp;



Many of these products, often marketed as calming or aphrodisiacal, are used in teas, vapes, or essential oils. They claim effects ranging from spiritual insight to improved sleep. But were they really Nymphaea caerulea?



To find out, McEvoy needed a legitimate sample. With wild populations now rare - dam construction and habitat loss have pushed the species to the edge of endangerment - he turned to the internet.&nbsp;



On Reddit, he connected with a user in Arizona who claimed to grow authentic blue lotus. The stranger agreed to send a live plant, which botanists at UC Berkeley confirmed as genuine.



That plant now resides in the <a href="https://botanicalgarden.berkeley.edu/" target="_blank" rel="noreferrer noopener">UC Botanical Garden</a>’s Virginia Haldan Tropical House, making it the only known living Egyptian blue lotus in a U.S. university collection.



McEvoy also ordered petals from Etsy to compare. Partnering with Berkeley chemistry professor Evan Williams and scientist Anthony Iavarone, he used mass spectrometry to analyze both samples.&nbsp;



The results were clear: the authentic flower contained significantly higher levels of the alkaloid nuciferine, thought to be responsible for its psychoactive effects. The Etsy sample, by contrast, likely came from a common non-psychoactive <a href="https://www.earth.com/news/japanese-lily-species-discovered-after-over-a-century/" target="_blank" rel="noreferrer noopener">lily</a>.



<h2 class="wp-block-heading" id="h-a-new-take-on-ancient-rituals">A new take on ancient rituals</h2>



In ancient Egypt, it’s often assumed that people steeped the blue lotus directly in <a href="https://www.earth.com/news/wine-production-in-a-warming-world-the-winners-and-losers/" target="_blank" rel="noreferrer noopener">wine</a> to unlock its effects. But McEvoy’s chemical analysis suggests that’s unlikely.&nbsp;



While pure nuciferine dissolves in alcohol, the waxy petals of the flower do not release it so easily. Instead, a fatty substance - similar to olive oil - may have been used to extract the compound before mixing it into wine.



“We're beginning to think the ancient Egyptians didn't just put it into wine,” McEvoy said. “We hypothesize they actually created an infused oil, which was later added to wine.”



This revised understanding reframes centuries of assumptions about ancient Egyptian ceremonial practices and raises new questions about how they engaged with plant-based compounds.



<h2 class="wp-block-heading" id="h-searching-for-molecular-remnants">Searching for molecular remnants </h2>



McEvoy’s next steps include a chemical analysis of a 3,000-year-old Egyptian goblet housed in the Hearst Museum. He hopes to detect trace amounts of fats that would support his theory about infused oils - and perhaps even find molecular remnants of the lotus itself.



Together with Williams and Ph.D. candidate Veena Avadhani, he also plans to use liquid chromatography to break down the flower’s chemical makeup even further.&nbsp;



This advanced method will allow them to isolate individual compounds and gain a clearer understanding of what makes the true blue lotus unique.



<h2 class="wp-block-heading" id="h-ancient-magic-and-modern-science-nbsp">Ancient magic and modern science&nbsp;</h2>



As McEvoy prepares to graduate and pursue a career in intellectual property law, he sees his work as a model for how science and the humanities can illuminate each other.&nbsp;



“There should be someone at the table who has studied people - not just economics, money or political science,” he said. “Someone who sees people as human beings and sees communities as interconnected webs of meaning.”



For now, he’s focused on finishing his research. But in doing so, he’s already redefined the story of a flower once believed to be mythic. His project not only separates fact from fiction in today’s lotus-laced health products - it reopens a window into the lived experience of an ancient civilization.



“This is a rare example of how ancient magic and modern science can come together to deepen our understanding of the nature that has always surrounded us,” he concluded.



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Blue lotus: Unraveling an Egyptian psychedelic mystery

The blue lotus, a captivating water lily entwined with Egyptian...

A recent discovery by an international team of astronomers has revealed an enormous, spiral galaxy unlike any other yet observed in the Universe.



Led by researchers from <a href="https://christuniversity.in" target="_blank" rel="noreferrer noopener">Christ University</a> in Bangalore, this team found something strange and unsettling. 



A massive, well-structured galaxy nearly a billion light-years away seems to defy everything we thought we knew about galactic behavior.



At its core lies a supermassive black hole. What’s shocking is that this black hole is producing enormous jets of energy, six million light-years long. These kinds of jets usually only come from elliptical <a href="https://www.earth.com/news/strange-signals-from-the-center-of-our-galaxy-hint-at-a-new-kind-of-dark-matter/" target="_blank" rel="noreferrer noopener">galaxies</a>. 



But this galaxy, a spiral like our Milky Way, is somehow managing to survive - and even remain stable - under extreme cosmic stress.



<h2 class="wp-block-heading" id="h-spiral-galaxy-that-shouldn-t-exist">Spiral galaxy that shouldn't exist</h2>



The galaxy, known as 2MASX J23453268−0449256, is not just a bit bigger than the Milky Way - it is three times the size. 



Its structure remains beautifully intact, with sweeping spiral arms and a glowing central bar. Yet, it's producing some of the largest radio jets ever seen in a spiral galaxy.



Powerful radio jets usually rip apart the delicate structure of spirals. They disrupt star formation, break the balance of matter, and change how galaxies grow. 



But this one breaks that rule. It continues to exist as a peaceful spiral, even while ejecting energy into space on a stunning scale.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/galaxy-spiral-J23453268−0449256_massive_credit-GMRT_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/galaxy-spiral-J23453268−0449256_massive_credit-GMRT_1s.webp" alt="The giant radio jets stretching six million light-years across and an enormous supermassive black hole at the heart of spiral galaxy J23453268−0449256, as imaged by the Giant Metrewave Radio Telescope. Credit: Bagchi and Ray et al/Giant Metrewave Radio Telescope" class="wp-image-1963256"/></a><figcaption class="wp-element-caption">The giant radio jets stretching six million light-years across and an enormous supermassive black hole at the heart of spiral galaxy J23453268−0449256, as imaged by the Giant Metrewave Radio Telescope. Credit: Bagchi and Ray et al/Giant Metrewave Radio Telescope</figcaption></figure>



"This discovery is more than just an oddity - it forces us to rethink how <a href="https://www.earth.com/news/euclid-captures-26-million-galaxies-in-vivid-deep-field-photos/" target="_blank" rel="noreferrer noopener">galaxies</a> evolve, and how supermassive black holes grow in them and shape their environments," said lead author Professor Joydeep Bagchi of Christ University, Bangalore.



"If a spiral galaxy can not only survive but thrive under such extreme conditions, what does this mean for the future of galaxies like our own Milky Way? 



"Could our galaxy one day experience similar high-energy phenomena that will have serious consequences for the survival of precious life in it?" 



<h2 class="wp-block-heading" id="h-quiet-galaxy-with-inner-chaos">Quiet galaxy with inner chaos</h2>



The team used several powerful tools to study this unusual galaxy. These included the&nbsp;<a href="https://hubblesite.org/" target="_blank" rel="noreferrer noopener">Hubble Space Telescope</a>, the&nbsp;<a href="https://www.gmrt.ncra.tifr.res.in/" target="_blank" rel="noreferrer noopener">Giant Metrewave Radio Telescope</a>, and the&nbsp;Atacama Large Millimeter/submillimeter Array (<a href="https://www.almaobservatory.org/en/home/" target="_blank" rel="noreferrer noopener">ALMA</a>).&nbsp;



The experts analyzed the galaxy in many wavelengths, building a detailed picture of its internal dynamics.​



At the center of J23453268−0449256 lies a supermassive black hole that’s billions of times more massive than the Sun. 



The jets coming from this black hole stretch out across six million light-years of space. That’s about sixty times the diameter of the Milky Way.



Incredibly, even with such intense activity, the galaxy’s structure remains untouched. The spiral arms remain well-shaped. 



A bright bar stretches through the center. A peaceful ring of stars surrounds it. This calm appearance hides the violent energy pulsing from its core.



Adding to the mystery is a huge halo of hot gas that surrounds the <a href="https://www.earth.com/news/largest-ever-3d-map-of-the-universe-lets-us-travel-back-11-billion-years/" target="_blank" rel="noreferrer noopener">galaxy</a>. This gas glows in X-ray light, indicating extremely high temperatures. 



Over time, this halo would normally cool and allow stars to form. But the black hole jets keep it too hot for that, acting like a cosmic furnace that stops star birth.



<h2 class="wp-block-heading" id="h-could-our-own-galaxy-behave-like-this">Could our own galaxy behave like this?</h2>



Could the Milky Way one day look like this galaxy? Right now, the black hole at our center - called Sagittarius A* - is quiet. It has a mass of four million Suns and shows no signs of powerful activity. But that could change.



If a gas cloud, star, or even a small galaxy falls into Sagittarius A*, it could trigger a violent reaction. This is known as a tidal disruption event (TDE). 



TDEs have been seen in other <a href="https://www.earth.com/news/galaxy-found-in-the-early-universe-that-shouldnt-exist/" target="_blank" rel="noreferrer noopener">galaxies</a>, but not yet in our own. If such an event were to occur, Sagittarius A* might awaken and produce high-energy jets. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/03/galaxy-J23453268-0449256_Milky-Way_comparison_Hubble_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/03/galaxy-J23453268-0449256_Milky-Way_comparison_Hubble_1s.webp" alt="Colour image of J23453268-0449256, which is 300,000 light-years across, as captured by the Hubble Space Telescope. It is shown alongside a depiction of our own Milky Way galaxy, which is three times smaller. Credit: Bagchi and Ray et al/Hubble Space Telescope" class="wp-image-1963254"/></a><figcaption class="wp-element-caption">Color image of J23453268-0449256, which is 300,000 light-years across, as captured by the Hubble Space Telescope. It is shown alongside a depiction of our own Milky Way galaxy, which is three times smaller. Credit: Bagchi and Ray et al/Hubble Space Telescope</figcaption></figure>



The danger lies in their direction and strength. If a TDE were aimed near Earth, it could damage our atmosphere, harm DNA, and raise mutation rates. In the worst-case scenario, it could erode the ozone layer and trigger mass extinction.



Even if no extinction follows, these jets could still affect the <a href="https://www.earth.com/news/oldest-known-galaxy-contains-surprising-oxygen-levels/" target="_blank" rel="noreferrer noopener">galaxy</a>. They might halt star formation in some areas or reshape the interstellar medium. That’s what seems to have happened in the case of J23453268−0449256.



<h2 class="wp-block-heading" id="h-why-is-this-spiral-galaxy-so-stable">Why is this spiral galaxy so stable?</h2>



Another piece of the puzzle is dark matter. The research team found that J23453268−0449256 has ten times more dark matter than the Milky Way. This likely helps keep the galaxy’s disc stable, even with massive forces trying to tear it apart.



Dark matter is invisible but exerts gravitational pull. It holds galaxies together. In this case, it may be the key that allows the galaxy to survive such violent internal processes without falling apart.



By studying the balance between dark matter, the supermassive black hole, and the galaxy’s structure, the researchers have opened up a new window into how galaxies might behave in extreme situations. 



Their findings could shift our entire understanding of cosmic evolution.



"Understanding these rare galaxies could provide vital clues about the unseen forces governing the universe – including the nature of dark matter, the long-term fate of galaxies, and the origin of life," noted study co-author Shankar Ray, a Ph.D. student at Christ University.



"Ultimately, this study brings us one step closer to unraveling the <a href="https://www.earth.com/news/spherex-will-scan-the-galaxy-to-look-for-lifes-ingredients/" target="_blank" rel="noreferrer noopener">mysteries of the cosmos</a>, reminding us that the universe still holds surprises beyond our imagination."



<h2 class="wp-block-heading" id="h-many-questions-remain">Many questions remain</h2>



The mystery is far from solved. Scientists don’t yet know how often such spiral galaxies form. They also don’t know what triggers their black holes to produce jets of this magnitude. 



Every answer leads to more questions.



Could the Milky Way already be preparing for such a phase? Is Sagittarius A* a ticking bomb, just waiting for the right spark? 



These questions don’t have clear answers yet, but discoveries like this one give us important clues.



For now, the Milky Way is calm, as life on Earth continues. But the universe, always changing and never fully known, reminds us that peace in the cosmos is never permanent. Somewhere, just a billion light-years away, a spiral galaxy lives on the edge - and still spins.



The study is published in the <a href="https://academic.oup.com/mnras/article/538/3/1628/8084797" target="_blank" rel="noreferrer noopener">Monthly Notices of the Royal Astronomical Society</a>. 



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Spiral galaxy discovered that defies everything we thought we knew about galaxies

A recent discovery by an international team of astronomers has...

Since the Industrial Revolution, the world has witnessed a sharp increase in noise pollution generated by human activities. Whether it’s the constant hum of traffic, airplanes overhead, or the repetitive clamor of construction, these sounds can obstruct animals’ abilities to give and receive crucial signals - a process that is fundamental to their survival and reproduction.



Now, a team of biologists at the <a href="https://www.unl.edu/" target="_blank" rel="noreferrer noopener">University of Nebraska–Lincoln</a> (UNL) has published one of the first known studies demonstrating how one group of animals can react to human-made noise by adjusting its own method of sensing sounds.&nbsp;



In an article published in the journal <a href="https://dx.doi.org/10.1016/j.cub.2025.02.041" target="_blank" rel="noreferrer noopener">Current Biology</a>, researchers Brandi Pessman and Eileen Hebets show that funnel-weaving <a href="https://www.earth.com/news/spiders-reveal-how-cave-creatures-lose-their-vision-over-time/" target="_blank" rel="noreferrer noopener">spiders</a> alter how their silk webs transmit vibrations in response to local noise. 



This finding suggests that the spiders might deliberately change web structure to cope with the auditory chaos surrounding them, ensuring they receive vital cues from potential mates, prey, or predators.



<h2 class="wp-block-heading" id="h-a-key-discovery-about-web-adjustments">A key discovery about web adjustments</h2>



Drawing on lab experiments, the study uncovered a particularly unexpected insight: the way a spider’s web conveys vibrations varies depending on whether its architect was collected from a rural or urban area. This discrepancy hints at the idea that prior exposure to noise - possibly even inherited across generations - may influence a spider’s malleability when it comes to spinning webs.



“One of the most interesting things that we found is that urban and rural spiders are reacting differently when they're put into a noisy environment,” said Pessman, a postdoctoral researcher in biological sciences and the lead author of the paper. 



“This means that spiders with different experiences with noise - whether they themselves experienced it or their mothers passed it down to them across generations - respond differently.”



<h2 class="wp-block-heading" id="h-spider-webs-as-sensory-extensions">Spider webs as sensory extensions</h2>



It has been well documented that animals such as birds and <a href="https://www.earth.com/news/climate-change-is-altering-the-calls-and-voices-of-frogs-around-the-world/" target="_blank" rel="noreferrer noopener">frogs</a> can change their calls or the timing of their vocalizations in the face of increased human noise. However, little was known about how animals manage to tweak the way they receive acoustic or vibratory signals. 



The main challenge is the hidden nature of most animals’ sensory systems, which are located within their bodies. But web-building spiders are unique, as their webs function effectively like external sensory extensions that capture vibrations from the environment.



This distinction makes funnel-weaving spiders, also known as Agelenopsis pennsylvanica, an ideal test group. They rely predominantly on vibratory signals for vital information. Their webs connect to various surfaces - trees, rocks, or buildings - capable of transmitting the vibratory noise created by <a href="https://www.earth.com/news/some-birds-get-road-rage-when-exposed-to-traffic-noise/" target="_blank" rel="noreferrer noopener">traffic</a>, industrial activities, and more.&nbsp;



The research team hypothesized that funnel-weaving spiders might be able to reduce the volume of unwanted or irrelevant vibrations caused by human-related noise, which often shares the frequency range these spiders need for effective communication.



<h2 class="wp-block-heading" id="h-spiders-in-urban-areas">Spiders in urban areas</h2>



Pessman started by collecting a total of 60 funnel-weaving spiders in and around Lincoln, Nebraska - some from city settings and others from out in the countryside. In the lab, the spiders were then placed in controlled environments that were either quiet or noisy as they spun webs over four nights. 



Upon completion, the researchers introduced test vibrations into those webs, measuring how energy moved across the silk in different conditions.



They observed that spiders from urban areas tended to build webs that lost more energy in short-distance vibrations across a broader set of frequencies when placed under noisy conditions. 



Interpreted practically, these webs essentially “muffled” environmental noise. This may prevent sensory overload, giving the spiders a clearer signal from <a href="https://www.earth.com/news/largest-predator-prey-feast-ever-seen-in-the-ocean-enormous-quickly-altered-food-chain/" target="_blank" rel="noreferrer noopener">prey</a> or other relevant vibrations in their immediate vicinity.



<h2 class="wp-block-heading" id="h-spiders-that-are-exposed-to-less-noise">Spiders that are exposed to less noise</h2>



Meanwhile, rural spiders assembled their webs in such a way that energy from biologically important long-distance vibrations was preserved. This indicates they might be amplifying or enhancing certain frequency ranges to pick out meaningful vibrations above the background noise.



“Rural spiders are not used to as much noise in their environment,” Pessman said. “When they suddenly get a lot of noise, they might try to 'turn up' the volume in their webs or amplify what's coming in to better hear certain signals above the noise.”



<h2 class="wp-block-heading" id="h-implications-for-ecology-and-future-studies">Implications for ecology and future studies</h2>



Given the role of funnel webs as external sensory structures, these findings open a new window into how animals can adjust the way they receive signals, a research area that had remained largely unclear until now. 



The ability to alter web structure in response to different noise environments could prove vital as human-made noise continues to escalate across the planet.



In the future, the team plans to investigate precisely how the spiders are changing their webs - whether they adjust the tension of certain silk lines, vary anchor points, or adopt an entirely new shape to filter or boost specific frequencies. 



High-speed video of the web-building process, combined with digital tracking methods, will let them delve deeper into these construction nuances.



<h2 class="wp-block-heading" id="h-spiders-overcoming-environmental-noise">Spiders overcoming environmental noise</h2>



“This study really highlights the role of receivers in overcoming environmental noise,” said Hebets, who is a professor of biological sciences at UNL. 



“It opens up entirely new avenues of research. For example, are receivers placing themselves at certain locations in the environment where signals are going to receive less attenuation or overlap of noise?”



By revealing that some species can modify their “sensor” for hearing, the team hopes to inspire more research on how other animals cope with rising noise levels. 



The funnels built by these little invertebrates may seem inconsequential to an urban passerby, but as the study shows, each strand of silk can be precisely tuned to help the spider thrive in a clamorous world.



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Spiders adapt their webs to filter out human-made noise

Since the Industrial Revolution, the world has witnessed a sharp...

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Sean Sheldrake, a unit dive officer with EPA&#8221;s Region 10, talks about his career at EPA.

EPA Careers: Sean Sheldrake

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