This image shows the aftermath of <a href="https://www.earth.com/video/puerto-rico-after-hurricane-maria/">Hurricane Maria</a> in Puerto Rico and was captured by the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>. This landscape usually appears as a lush and vibrant green, but now looks like a dark brown after Maria destroyed vegetation and kicked up sediment and mud.

Aftermath of Hurricane Maria in Puerto Rico

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

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Blanket of dust covers China’s Tarim Basin

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

Today's Image of the Day from the European Space Agency features 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 NASA Earth Observatory features dust streaming off the coast of Iran in January 2025.



“Some of the desert dust was carried across the Gulf of Oman to the Arabian Peninsula, degrading air quality for those in its path,” noted <a href="https://earthobservatory.nasa.gov/images/153859/desert-dust-streams-from-iran" target="_blank" rel="noreferrer noopener">NASA</a>.



“The airborne material appears to primarily originate in the dried bed of the intermittent lake known as Hamun-e Jazmurian (Hamun-e Jaz Murian), while some may be blown from coastal areas." 



"Along with arid regions such as the Garagum and Lut deserts and the Sistan Basin, the lakebed is a major source of dust in southwest Asia.”



<h2 class="wp-block-heading" id="h-precipitation-in-the-jazmurian-basin">Precipitation in the Jazmurian Basin</h2>



According to NASA, some areas of the Jazmurian Basin receive less than four inches of rain annually, on average, and evaporation rates are high. During wet times, however, parts of the basin may be covered by an intermittent lake, marshland, or other vegetation.&nbsp;



“Terra’s MODIS sensor has previously captured images of the area when water is present in Hamun-e Jazmurian and when green vegetation fringes the lakebed,” said NASA.



“In early 2025, the land was dry enough for winds to blow dust plumes south-southwest over the Gulf of Oman. Dust traveled across the water to the coast of the United Arab Emirates, where the haze reduced visibility in places, according to news reports.”



<h2 class="wp-block-heading" id="h-particles-in-dust-storms">Particles in dust storms</h2>



In addition to disrupting transportation and other daily activities, the suspended particles in dust storms can pose significant health risks. 



Recent research has revealed that dust from the Jazmurian Basin often contains heavy metals and other potentially harmful substances, such as silica and organic pollutants, which can negatively impact both human and ecosystem health.&nbsp;



Prolonged exposure to these particles has been linked to respiratory and cardiovascular issues, as well as the exacerbation of pre-existing health conditions like asthma and bronchitis.



<h2 class="wp-block-heading" id="h-environmental-impact-of-dust-storms">Environmental impact of dust storms</h2>



The <a href="https://www.earth.com/news/dust-is-an-understudied-contributor-to-climate-change/" target="_blank" rel="noreferrer noopener">environmental impact</a> of dust storms extends beyond human health. The fine particles can settle on vegetation, reducing photosynthesis and agricultural productivity.&nbsp;



Dust deposition can also alter soil composition by introducing heavy metals and changing nutrient balances, which may affect crop growth and soil microbial communities. 



Such changes can lead to long-term degradation of arable land and disrupt local food security.



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



Communities near the Jazmurian Basin are particularly vulnerable to the effects of dust storms due to limited access to healthcare and mitigation resources.



Seasonal changes and climate conditions, including prolonged droughts and desertification, further intensify the frequency and severity of dust storms in the region.&nbsp;



This creates a cycle of environmental and health challenges, making it imperative to develop strategies for prevention and adaptation.



Potential measures include reforestation and soil stabilization projects to reduce dust emissions, stricter regulations to limit activities that contribute to desertification, and public health initiatives to educate communities on protective measures during dust events.&nbsp;



Investing in early warning systems and <a href="https://www.earth.com/news/climate-driven-wildfires-worsen-u-s-air-quality-and-health/" target="_blank" rel="noreferrer noopener">air quality</a> monitoring can also help minimize exposure and protect both human populations and the environment.



<h2 class="wp-block-heading" id="h-significance-of-the-jazmurian-basin">Significance of the Jazmurian Basin</h2>



The Jazmurian Basin is a prominent endorheic basin located in southeastern Iran, spanning parts of the provinces of Sistan and Baluchestan as well as Kerman. It lies at the heart of an arid region characterized by sparse vegetation, high temperatures, and limited rainfall.&nbsp;



The basin is primarily fed by the Halil and Bampur rivers, which provide seasonal water flow to the basin's low-lying areas. At its center lies the Jazmurian Depression, which forms a seasonal playa or shallow lake, though it often dries up during extended dry periods.&nbsp;



The area holds geological and archaeological significance, offering insights into ancient human settlements and environmental changes over time.&nbsp;



Despite its harsh climate, the basin supports small-scale agriculture and serves as a critical habitat for certain desert-adapted wildlife. 



The image was captured on January 22 by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite.&nbsp;



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Dust rises from the Jazmurian Basin in Iran

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA&nbsp;



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Hubble spots a supernova in the constellation Gemini 

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Spiral galaxy glows with young stars and interstellar dust

Today's Image of the Day from 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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Cosmic eye in the Puppis constellation

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

The MODIS instrument, short for Moderate Resolution Imaging Spectroradiometer, is a key instrument aboard the Terra and Aqua satellites. MODIS is playing a vital role in the development of Earth ecosystem models, able to predict global changes, which then assist policy makers in making informed decisions about the protection of the global environment.

Heavy snow and cloud cover in the Alps are seen in this Image of the day&nbsp;from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at heavy snow and low clouds in the Alps. Wildlife such as ibex live in the higher peaks to elevations of 3,400 m (11,155 ft), and plants such as Edelweiss grow in rocky areas in lower elevations as well as in higher elevations.

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

Aqua is a NASA scientific research satellite that studies precipitation, evaporation, and water cycles. Terra and Aura make up the Earth Observing System. It's the second component of the system.

A frozen Lake Erie in February Today’s Image of the Day comes from the <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> and features a look at a frozen <a href="https://www.earth.com/image/icy-lake-erie/">Lake Erie</a>, which is currently 93.3 percent iced over. A frozen Lake Erie in February
This false-color image was created using data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Aqua satellite to differentiate between snow, ice, and clouds.
Lake Erie /ˈɪəri/ (French: Lac Érié) is the fourth-largest lake (by surface area) of the five Great Lakes in North America, and the eleventh-largest globally if measured in terms of surface area.It is the southernmost, shallowest, and smallest by volume of the Great Lakes and therefore also has the shortest average water residence time. At its deepest point Lake Erie is 210 feet (64 metres) deep. 
Situated on the International Boundary between Canada and the United States, Lake Erie&#8217;s northern shore is the Canadian province of Ontario, specifically the Ontario Peninsula, with the U.S. states of Michigan, Ohio, Pennsylvania, and New York on its western, southern, and eastern shores. These jurisdictions divide the surface area of the lake with water boundaries. 
The lake was named by the Erie people, a Native American people who lived along its southern shore. The tribal name &#8220;erie&#8221; is a shortened form of the Iroquoian word erielhonan, meaning long tail
&#8212;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Image Credit: <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a>

A frozen Lake Erie in February

Aqua Earth Observing Satellite

This beautiful photo gallery contains 50 incredible images of Earth from Space. These images were taken by astronauts onboard the International Space Station, as well as by a multitude of NASA satellites orbiting the earth.

Today’s Image of the Day comes thanks to the <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a> and features a look at Super Typhoon Noru in the Pacific Ocean just south of <a href="https://www.earth.com/news/first-blue-chrysanthemums-created/">Japan</a>.
This image was captured by the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite on July 31, 2017. 
At the time the photo was taken, Typhoon Noru was located just 250 kilometers south of Iwo Jima. Maximum sustained winds hit 150 miles per hour.
The storm briefly became a category 5 on July 30, before being downgraded to a category 4 one day later.
&#8211;
By <a href="mailto:rarnold@earth.com">Rory Arnold</a>, <a href="https://www.earth.com/staff">Earth.com</a> Staff Writer
Source: <a href="https://earthobservatory.nasa.gov/IOTD/view.php?id=90654&amp;eocn=home&amp;eoci=iotd_readmore">NASA Earth Observatory</a>

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

Photos from the International Space Station are found in this awesome Earth.com image gallery. Flat-earthers won't agree, but these incredible photos of the Earth were taken by astronauts onboard the International Space Station. The International Space Station is a modular space station in low Earth orbit.

Northern Italy from the space station is seen here in this Image of the Day from the <a href="http://www.esa.int/">European Space Agency</a> (ESA). The view includes the top half of the Italian Peninsula, along with <a href="https://www.earth.com/image/wildfires-burn-northern-corsica/">Corsica</a> and Sardinia off the coast. This image was captured by ESA astronaut Paolo Nespoli on his third and final mission to the Space Station.

Northern Italy from the Space Station

Photos from the International Space Station

A growing body of scientific work is revealing a remarkable feature of certain microbes. They can “breathe” in a way that produces electricity instead of relying on oxygen, suggesting unusual survival strategies that could inspire future clean energy solutions.



This <a href="https://linkinghub.elsevier.com/retrieve/pii/S0092867425002892" target="_blank" rel="noreferrer noopener">discovery</a> came to light when researchers noticed that some <a href="https://www.earth.com/news/previously-overlooked-viruses-may-secretly-shape-bacterial-populations/" target="_blank" rel="noreferrer noopener">bacteria</a> thrive in conditions with little or no oxygen by sending out electrons into their environment.



Soon after, they found a key detail: these bacteria hand off electrons through certain molecular carriers, enabling them to keep growing while essentially “exhaling” electric current. Caroline Ajo-Franklin of <a href="https://www.rice.edu" target="_blank" rel="noreferrer noopener">Rice University</a> helped guide this project.



<h2 class="wp-block-heading" id="h-bacteria-produce-electricity">Bacteria produce electricity</h2>



Some species, including <a href="https://pmc.ncbi.nlm.nih.gov/articles/PMC9481105/" target="_blank" rel="noreferrer noopener">Shewanella</a> and <a href="https://www.sciencedirect.com/topics/agricultural-and-biological-sciences/geobacter" target="_blank" rel="noreferrer noopener">Geobacter</a>, have long been <a href="https://www.nature.com/articles/nrmicro2113" target="_blank" rel="noreferrer noopener">known</a> to transfer electrons to external surfaces, even metal oxides, while growing in oxygen-limited zones. 



Scientists realized these organisms produce a small but steady electric current through this process.



Biki Bapi Kundu is a Rice doctoral student and first author of the study who took a closer look at an everyday bacterium and figured out the mechanism behind its power output.&nbsp;



“This newly discovered mechanism of respiration is a simple and ingenious way to get the job done,” said Bapi Kundu.



<h2 class="wp-block-heading" id="h-microbes-generate-energy-without-oxygen">Microbes generate energy without oxygen</h2>



These electricity-generating <a href="https://www.earth.com/news/bacteria-recreate-an-ancient-war-trick-to-defeat-viruses/" target="_blank" rel="noreferrer noopener">microbes</a> do not rely on the usual electron acceptors, like oxygen. Instead, they latch onto conductive surfaces. 



By pushing electrons onto external materials, they gain energy to keep going in oxygen-deprived spots. 



Researchers now know that certain bacteria use a special molecule known as <a href="https://www.sciencedirect.com/science/article/pii/S0092867425002892" target="_blank" rel="noreferrer noopener">naphthoquinone</a> to help pass electrons to their outside world.



Once those electrons move out, the cells generate energy in a self-sustained system. The process bears similarities to how a battery releases current.



<h2 class="wp-block-heading" id="h-microbes-transfer-electrons-like-a-battery">Microbes transfer electrons like a battery</h2>



These <a href="https://www.earth.com/news/new-type-of-microbes-found-earths-deep-soil-critical-zone/" target="_blank" rel="noreferrer noopener">bacteria</a> gain an advantage by freeing up electrons they would otherwise hold onto. Through that exit pathway, they can break down carbon sources more efficiently than in standard fermentation processes.



It seems that this feature might be lurking in a wider range of microbes than previously thought. One research group discovered that these electricity-making strategies are not limited to organisms specifically adapted to extreme habitats.



“Our research not only solves a long-standing scientific mystery, but it also points to a new and potentially widespread survival strategy in nature,” said Ajo-Franklin.



<h2 class="wp-block-heading" id="h-uses-for-electricity-producing-bacteria">Uses for electricity-producing bacteria</h2>



Because electricity-producing <a href="https://www.earth.com/news/bacteria-pass-down-their-memories-to-fight-viruses/" target="_blank" rel="noreferrer noopener">bacteria</a> can relieve the buildup of electrons, they have potential uses in various industrial applications. 



Some scientists foresee improved wastewater treatment, where these microbes might help remove pollutants while sending out an electric signal.



This line of work could also help with biomanufacturing. While certain processes bog down from electron imbalances, electricity-generating organisms might balance the system by shuttling electrons away in real time.



<h2 class="wp-block-heading" id="h-long-term-vision-for-clean-energy">Long-term vision for clean energy</h2>



With a bit of engineering, these cells might even harness carbon dioxide through renewable power. The concept mimics photosynthesis in plants, but here, bacteria could rely on external electricity in a controlled setting.



In the future, we may see specialized microbial <a href="https://www.earth.com/news/23-new-marine-bacteria-species-discovered-that-influence-global-ocean-cycles/" target="_blank" rel="noreferrer noopener">communities</a> that maintain their own flow of electrons, feeding into sensors and energy devices. 



Researchers note that these bacteria may also prove handy in areas where oxygen is scarce, like underground or potentially even in space technology.



<h2 class="wp-block-heading" id="h-bacteria-as-real-time-sensors">Bacteria as real-time sensors</h2>



Experts believe electricity-making cells could bring improvements to environmental monitoring. Their electrical signals change when toxins are present, so they can provide real-time alerts about pollution or water quality.



Some hope that such systems might open the door to new diagnostic tools as well. The natural inclination of these microbes to shuttle electrons might allow them to perform tasks that previously demanded more complex instruments.



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



These findings expand our perspective on microbial metabolism. Once thought to be limited to fermentation under oxygen-free conditions, many ordinary bacteria may hold hidden skills for electron transfer. 



The implications extend across fields from bioengineering to synthetic biology. Researchers are optimistic that this work will encourage a deeper examination of how microbes manage energy in their native habitats. 



By understanding these strategies, scientists can look for ways to steer or optimize electron transfer on a larger scale.



Academics point out that an improved knowledge of microbial electron flow could open new doors in sustainable technology. 



If cultivated in controlled bioreactors, these organisms might help curtail industrial waste and boost the output of valuable chemicals.



At the same time, study authors are cautious about the next steps. They say that scaling up these systems requires more data and design know-how, but they remain confident about the future.



The study is published in the journal <a href="https://linkinghub.elsevier.com/retrieve/pii/S0092867425002892" target="_blank" rel="noreferrer noopener">Cell</a>.



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Life finds a way: Some bacteria "breathe" by producing electricity instead of relying on oxygen

A growing body of scientific work is revealing a remarkable...

Astronomers have spotted something that appears to stretch around ten billion light years across. This so-called Hercules–Corona Borealis Great Wall is being reevaluated, and it might be more extensive and nearer to Earth than earlier calculations suggested.



Its immense size has fueled discussions about how matter spreads out in the cosmos. Some see it as an oddity that cannot be explained by standard maps of the universe, while others say more data will shed light on its nature.



One person at the center of these efforts is <a href="https://www.uah.edu/announcements/16621-welcome-dr-jon-hakkila-new-associate-provost" target="_blank" rel="noreferrer noopener">Dr. Jon Hakkila</a> from the <a href="https://www.uah.edu/" target="_blank" rel="noreferrer noopener">University of Alabama in Huntsville</a>. He and his team have examined the way <a href="https://www.mdpi.com/2075-4434/13/2/16" target="_blank" rel="noreferrer noopener">gamma-ray bursts</a> signal the edges of this structure.



<h2 class="wp-block-heading" id="h-hercules-corona-borealis-supercluster">Hercules–Corona Borealis supercluster</h2>



Researchers label this structure a supercluster because of how it gathers countless galaxies in one region. 



They rely on <a href="https://www.esa.int/Science_Exploration/Space_Science/What_is_red_shift" target="_blank" rel="noreferrer noopener">redshifts</a> to estimate distances and found that multiple galaxies, linked by these bursts, cluster in an area bigger than anything else known.



“It is larger than the size of most anything to which it might be compared,” said Dr. Hakkila at the end of a discussion featured in recent observations. 



His remark highlights how standard theories about universal uniformity cannot fully account for this sprawling arrangement.



<h2 class="wp-block-heading" id="h-why-bursts-matter">Why bursts matter</h2>



<a href="https://www.earth.com/news/astronomers-confirm-lone-black-hole-wandering-through-our-galaxy/">Astronomers</a> use gamma-ray bursts to measure cosmic distances because these bursts shine more brightly than typical stellar processes. 



They can be powered by supernova events or by merging neutron stars and are detectable across vast stretches of space.



Since these bursts come from catastrophic stellar endings, they appear wherever stars exist in large numbers. 



By tracking them, observers gain a glimpse of how far matter extends, even in places that defy straightforward study.



<h2 class="wp-block-heading" id="h-how-hercules-corona-borealis-compares">How Hercules–Corona Borealis compares</h2>



This wall isn’t the only oversized feature that’s caused a stir. 



Structures like the <a href="https://www.aanda.org/articles/aa/full_html/2016/11/aa28567-16/aa28567-16.html" target="_blank" rel="noreferrer noopener">Sloan Great Wall</a>, the <a href="https://ui.adsabs.harvard.edu/abs/2014RMxAC..44..201C/abstract" target="_blank" rel="noreferrer noopener">Huge Large Quasar Group</a>, and the <a href="https://www.aanda.org/articles/aa/full_html/2016/11/aa28567-16/aa28567-16.html" target="_blank" rel="noreferrer noopener">Giant Quasar Arc</a> have all pushed against the expected boundaries of cosmic uniformity.



Still, the Hercules–Corona Borealis Great Wall dwarfs them. 



At around ten billion light years long, it’s nearly twenty-five times the size of the Sloan Great Wall, which was already thought to be massive when it was discovered in 2003.



<h2 class="wp-block-heading" id="h-why-scientists-still-have-doubts">Why scientists still have doubts</h2>



Some astronomers caution that the current GRB dataset might not be complete enough to draw final conclusions. 



The precision of burst positions and redshifts isn’t always high, and small errors can create the illusion of larger structures than what actually exists.



There’s also the issue of sampling bias, since parts of the sky are harder to observe due to dust or <a href="https://www.earth.com/news/35-years-of-hubble-the-telescope-that-changed-our-view-of-the-universe/">telescope</a> access. Until more consistent coverage is available, there’s always the chance that what looks like a wall might just be a trick of patchy data.



Any structure beyond about 1.2 billion light years in size is generally viewed with caution by theorists, because the <a href="https://astro.wku.edu/astr106/structure/cosmologicalprinciple.html" target="_blank" rel="noreferrer noopener">cosmological principle</a> implies matter should look uniform at enormous distances. Yet this giant wall sits right at the limit of what current models can handle without adjustments.



“The jury is still out on what it all means,” said Dr. Hakkila during a recent briefing. Some models can accommodate something so grand, but others fall short.



<h2 class="wp-block-heading" id="h-hercules-corona-borealis-not-fully-mapped">Hercules–Corona Borealis not fully mapped</h2>



One of the biggest hurdles in confirming the wall’s full outline is the limited number of gamma-ray bursts (GRBs) available with known distances. 



The team used <a href="https://arxiv.org/abs/2312.10050" target="_blank" rel="noreferrer noopener">542 GRBs</a> in their study, and only about half of those were in the right part of the sky to trace this particular structure.



Because the detection of GRBs depends on many factors - like the brightness of the event, telescope availability, and even sky conditions - the data is naturally uneven. 



That unevenness makes it harder to rule out random clustering or signal confusion without more coverage from upcoming missions.



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



Astronomers are eager to figure out exactly where this wall starts and ends. 



“Since the most distant extent of the Hercules–Corona Borealis Great Wall is hard to verify, the most interesting finding is that the closest parts of it lie closer to us than had previously been identified,” said Dr. Hakkila.



<a href="https://www.earth.com/news/space-debris-now-threatens-working-satellites/">New satellites</a> under development may sharpen the data needed to sort out lingering unknowns. 



In the meantime, scientists see the current findings as a reason to reevaluate large-scale structures and how they might push the boundaries of our cosmic road maps.



A proposed European mission called <a href="https://arxiv.org/abs/1907.00616" target="_blank" rel="noreferrer noopener">THESEUS</a> (Transient High Energy Sky and Early Universe Surveyor) could change everything. 



With its wide field of view and heightened sensitivity, it may detect thousands of new gamma-ray bursts, especially from very distant or faint sources.



If launched, THESEUS would give researchers the dense data they need to finally outline the full size of the Hercules–Corona Borealis Great Wall—or prove that it doesn’t stretch quite as far as it seems.



The study is published in <a href="https://www.aanda.org/articles/aa/full_html/2015/12/aa24829-14/aa24829-14.html" target="_blank" rel="noreferrer noopener">Universe 2025</a>.



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'Largest structure in the universe' is even bigger than astronomers imagined and still a huge mystery

Astronomers have spotted something that appears to stretch around ten...

A new investigation at a high‑Andean temple reveals that the distant ancestors of the Inca wielded psychoactive plants as a political tool. 



Archaeologists have uncovered bone tubes still coated with traces of mind‑altering snuff, showing that Chavín lords used controlled visions to cement their rule almost three millennia ago.



The discovery comes from a project led by researchers at the <a href="https://www.ufl.edu/">University of Florida</a>, <a href="https://www.stanford.edu/">Stanford University</a>, and partner institutions across South America. 



The experts analyzed artifacts from Chavín de Huántar, a vast ceremonial center that sits 10,000 feet above sea level in the Peruvian Andes.



<h2 class="wp-block-heading" id="h-ancient-use-of-psychoactive-plants">Ancient use of psychoactive plants</h2>



Inside narrow passageways and hidden rooms, the team found small hollow bones carved into elegant inhalation tubes. 



Chemical testing detected nicotine from wild tobacco relatives and residue from vilca beans, whose potent compounds are related to DMT.



Microscopic work confirmed plant particles embedded in the ancient surfaces. The date of the deposits makes this the oldest direct evidence for psychoactive plant use yet known in the high Andes.



<h2 class="wp-block-heading" id="h-rituals-shaped-social-order">Rituals shaped social order</h2>



The placement of the tubes mattered. They were sealed within private chambers that could hold only a handful of people. That setting implies exclusive ceremonies, not widespread communal feasts.



The evidence matches a broader pattern of Chavín architecture, which funnels visitors through labyrinths toward dimly lit sanctuaries where sights, sounds, and fragrances overwhelm the senses.



“Taking psychoactives was not just about seeing visions. It was part of a tightly controlled ritual, likely reserved for a select few, reinforcing the social hierarchy,” said Daniel Contreras, an anthropological archaeologist at the University of Florida and a co‑author of the study.



<h2 class="wp-block-heading" id="h-chavin-rituals-meant-to-stun">Chavín rituals meant to stun</h2>



Stone corridors at Chavín already distort light and echo footsteps. Researchers have also recovered giant trumpets fashioned from imported conch shells. 



The deep blasts of those horns, amplified by the tunnels, would have rattled bone. Add intense <a href="https://www.earth.com/news/understanding-presence-hallucinations-impact-on-social-perception/">hallucinations</a>, and followers might have felt a raw presence of gods or spirits.



“The supernatural world isn’t necessarily friendly, but it’s powerful,” Contreras said. “These rituals, often enhanced by psychoactives, were compelling, transformative experiences that reinforced belief systems and social structures.”



By staging such events, leaders wrapped their authority in cosmic mystery. Participants emerged convinced that rank and building labor served a higher design. 



Craftspeople who carved the monumental granite slabs and farmers who fed the workforce likely saw themselves as part of a living myth, not as servants under duress.



<h2 class="wp-block-heading" id="h-belief-used-for-power">Belief used for power</h2>



“One of the ways that <a href="https://www.earth.com/news/wealth-inequality-began-shaping-human-societies-10000-years-ago/">inequality</a> was justified or naturalized was through ideology - through the creation of impressive ceremonial experiences that made people believe this whole project was a good idea,” Contreras said.



The snuff tubes thus fit a larger strategy. Earlier Andean settlements show few signs of strict hierarchy. By Chavín times, around 800 BCE, society had acquired priests, skilled artisans, and regional trade routes. 



Control over sacred knowledge, including plant lore, helped elites turn soft power into hard architecture and coordinated labor.



<h2 class="wp-block-heading" id="h-psychoactive-plant-mixture">Psychoactive plant mixture</h2>



Vilca beans grow in lowland forests far from Chavín’s icy heights. Their presence points to long‑distance exchange networks and to careful botanical skill.



When roasted, mixed with lime, and inhaled, the powder produces vivid visions, rapid heartbeat, and disorientation. 



Wild tobaccos add <a href="https://www.earth.com/news/nicotine-pouches-are-a-new-dangerous-trend-among-teens/">nicotine</a>’s stimulant rush and sharp aroma. Combined, these plants could propel users into what seemed another realm.



<h2 class="wp-block-heading" id="h-bringing-invisible-details-to-light">Bringing invisible details to light</h2>



Contreras has worked at the site for nearly 30 years in a project directed by Stanford archaeologist John Rick.



Their excavations have mapped hidden galleries, sculpted stone icons, and water channels that once gurgled beneath temple floors. The new chemical analyses bring invisible details to light, showing not only what people did but also what they felt.



“It’s exciting that ongoing excavations can be combined with cutting‑edge archaeological science techniques to get us closer to understanding what it was like to live at this site,” Contreras said.



<h2 class="wp-block-heading" id="h-from-vision-to-empire">From vision to empire</h2>



The Chavín phenomenon spread a shared artistic style and worldview up and down the Peruvian coast and sierra. Later Andean states inherited its taste for grand plazas, stone imagery, and elite ritual.



By demonstrating the intentional use of psychoactive plants in tightly managed settings, the study bridges the gap between small egalitarian hamlets and the vast empires that eventually ruled the Cordillera.



<h2 class="wp-block-heading" id="h-a-modern-glimpse-of-ancient-minds">A modern glimpse of ancient minds</h2>



Today, visitors to Chavín de Huántar walk through restored corridors where carved fangs and staring eyes still pierce the dim light. 



Knowing that select priests once knelt here, inhaled potent smoke, and proclaimed cosmic truths changes how we read those walls.



The <a href="https://www.earth.com/news/archaeologists-find-hallucinogenic-seeds-in-ancient-bones-black-henbane/">bone</a> tubes, simple yet sophisticated, remind us that chemistry, belief, and social order have long been intertwined. In the high Andes, <a href="https://www.earth.com/news/meditation-reveals-common-altered-states-of-consciousness/">altered consciousness</a> was more than a personal journey - it was statecraft written in breath and stone.



The study is published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2425125122">Proceedings of the National Academy of Sciences</a>.



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How psychoactive plants helped build an ancient empire

A new investigation at a high‑Andean temple reveals that the...

Happy,Mature,Female,Teacher,Educator,Helping,African,American,Junior,School

Grading student work can take up countless hours for teachers, especially when assignments call for deep thinking, explanations, or scientific modeling. However, a new study suggests that artificial intelligence (AI) could help ease that burden - but only if used carefully and alongside human input.



The research was led by Xiaoming Zhai, associate professor and director of the <a href="https://coe.uga.edu/research/labs/ai4stem/" target="_blank" rel="noreferrer noopener">AI4STEM Education Center </a>at <a href="https://www.uga.edu/" target="_blank" rel="noreferrer noopener">University of Georgia</a>’s Mary Frances Early College of Education. The study explores how well Large Language Models (LLMs) can assess student work compared to human graders.



“Asking kids to draw a model, to write an explanation, to argue with each other are very complex tasks,” Zhai said. “<a href="https://www.earth.com/news/robots-teaching-other-robots-its-no-longer-science-fiction/" target="_blank" rel="noreferrer noopener">Teachers</a> often don’t have enough time to score all the students’ responses, which means students will not be able to receive timely feedback.”



<h2 class="wp-block-heading" id="h-ai-grading-vs-human-judgment">AI grading vs. human judgment</h2>



The study focused on middle school students’ responses to science questions aligned with the Next Generation Science Standards. One question, for example, asked students to create a model showing how particles behave when heat energy is added. 



The correct answer would explain that molecules speed up as they heat and slow down when cooled. The research team fed student answers into an LLM called Mixtral and asked it to grade them. 



But unlike most AI grading studies, where the AI is trained using examples of human‑scored answers, this study took a different approach. Here, the LLM had to create its own grading rubric and apply it to student work.



<h2 class="wp-block-heading" id="h-trading-accuracy-for-speed">Trading accuracy for speed</h2>



The researchers found that Mixtral could grade responses very quickly. However, it tended to rely on shortcuts, such as looking for specific keywords, rather than assessing the actual depth of the students’ understanding.



“Students could mention a temperature increase, and the large language model interprets that all students understand the particles are moving faster when temperatures rise,” Zhai explained.



“But based upon the student writing, as a human, we’re not able to infer whether the students know whether the particles will move faster or not.”



In other words, the AI might give points to a student simply for mentioning the right terms, even if the <a href="https://www.earth.com/news/where-logic-lives-experts-identify-the-brain-region-responsible-for-reasoning/" target="_blank" rel="noreferrer noopener">reasoning</a> behind the answer is unclear or incorrect.



<h2 class="wp-block-heading" id="h-improving-ai-with-human-standards">Improving AI with human standards</h2>



The study suggests that LLMs need better guidelines to match human grading standards. Specifically, AI models perform better when they use detailed rubrics created by teachers, which outline exactly what to look for in a good response.



Without these rubrics, the AI only reached about 33.5% accuracy when compared to human grading. With access to human‑created rubrics, that accuracy jumped to just over 50%.



“The train has left the station, but it has just left the station,” Zhai said. “It means we still have a long way to go when it comes to using AI, and we still need to figure out which direction to go in.”



<h2 class="wp-block-heading" id="h-why-human-reasoning-still-matters"><a></a>Why human reasoning still matters</h2>



One key difference between human graders and LLMs is how they handle complex or incomplete answers. 



According to the researchers, while LLMs will mark a student’s response as correct if it includes certain keywords,. However, it cannot evaluate the logic the student is using.



This happens because LLMs tend to “over‑infer,” assuming a student understands a concept based on surface clues. Human teachers, though, look for evidence of clear thinking and accurate reasoning. 



Without explanations for why certain answers earned specific grades, the AI lacks the context to make fine‑tuned decisions.



<h2 class="wp-block-heading" id="h-teachers-want-help-not-replacement"><a></a>Teachers want help, not replacement</h2>



Despite these limitations, many teachers are interested in using AI <a href="https://www.earth.com/news/man-vs-machine-why-students-still-write-better-than-ai/" target="_blank" rel="noreferrer noopener">tools</a> to speed up routine grading.



“Many teachers told me, ‘I had to spend my weekend giving feedback, but by using automatic scoring, I do not have to do that. Now, I have more time to focus on more meaningful work instead of some labor‑intensive work,’” Zhai said. “That’s very encouraging for me.”



Rather than fully replacing human graders, the researchers suggest that AI systems should serve as assistants. This way, it frees teachers to concentrate on tasks that require human judgment, <a href="https://www.earth.com/news/creativity-improves-life-satisfaction-and-overall-well-being/" target="_blank" rel="noreferrer noopener">creativity</a>, and connection.



<h2 class="wp-block-heading" id="h-what-comes-next-for-ai-grading"><a></a>What comes next for AI grading</h2>



The research highlights both the promise and the challenges of using AI in classrooms. While current LLMs can process large batches of student work quickly, they still need better instructions, oversight, and refinement to deliver meaningful feedback. 



Teachers remain essential for guiding the use of these tools, setting expectations, and ensuring fairness. As AI technologies continue to evolve, the hope is that future models will become more adept at understanding not just keywords but the quality of student reasoning.



With thoughtful design and <a href="https://www.earth.com/news/do-humans-and-ai-work-better-together/" target="_blank" rel="noreferrer noopener">human‑AI collaboration</a>, these tools could become powerful allies in helping teachers support student learning - without sacrificing weekends to piles of ungraded papers.



The study is published in the journal <a href="https://link.springer.com/article/10.1007/s10758-025-09836-8" target="_blank" rel="noreferrer noopener">Technology, Knowledge and Learning</a>.



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Grading with AI: Faster than teachers, but not smarter

Grading student work can take up countless hours for teachers,...

Scientists have come up with a new high-resolution map of the ocean floor. The newly released findings show nearly 100,000 underwater mountains that were previously unknown.



<a href="https://scripps.ucsd.edu/profiles/dsandwell" target="_blank" rel="noreferrer noopener">David Sandwell</a> from Scripps Institution of Oceanography contributed to this research and credits advanced satellite observations for the detailed results. 



<a href="https://scripps.ucsd.edu/profiles/dsandwell" target="_blank" rel="noreferrer noopener">The SWOT mission</a>, launched in December 2022, is central to collecting the critical data that enabled this mapping effort.



<h2 class="wp-block-heading" id="h-how-satellites-outpace-ships">How satellites outpace ships</h2>



Mapping the ocean floor with ships takes time, fuel, and money. Even with sonar, a single vessel might only cover a narrow strip of seafloor each day.



Satellites like SWOT cover about 90% of the Earth every 21 days. They don’t match the detail of sonar, but they make up for it with speed, scale, and frequency of observation.



<h2 class="wp-block-heading" id="h-why-seafloor-maps-matter">Why seafloor maps matter</h2>



Ships equipped <a href="https://www.earth.com/news/nasa-swot-satellite-mission-maps-earths-ocean-floors-from-space-in-stunning-detail/">with sonar instruments can survey the ocean</a> bottom directly, but only about one-quarter of the seafloor has been charted in this way. That knowledge gap spurred scientists to turn to satellite-based data for a bigger picture.



“Seafloor mapping is key in both established and emerging economic opportunities, including rare-mineral seabed mining, optimizing shipping routes, hazard detection, and seabed warfare operations,” said <a href="https://science.nasa.gov/people/nadya-vinogradova-shiffer-physical-oceanography-program/" target="_blank" rel="noreferrer noopener">Nadya Vinogradova Shiffer</a> at the end of a NASA statement. 



Accurate mapping has practical uses for navigation and cable-laying, and it also shapes our understanding of ocean processes.&nbsp;



<h2 class="wp-block-heading" id="h-hidden-ocean-mountains">Hidden ocean mountains</h2>



<a href="https://oceanexplorer.noaa.gov/facts/seamounts.html" target="_blank" rel="noreferrer noopener">Seamounts</a> are underwater mountains that rise from the ocean floor but do not break the surface. These features were once hard to detect if they measured less than about 3,300 feet in height.



The new satellite map can sense seamounts less than half that tall. By zeroing in on tiny gravitational “bumps” on the water’s surface, the data predict the position of these newly discovered peaks, boosting known seamount counts from 44,000 to nearly 100,000.



The technique behind the map depends on gravity - not cameras. Since seamounts and abyssal hills have more mass than the surrounding seafloor, they tug slightly more on the ocean above them.



That tug creates tiny rises in the water’s surface, sometimes only a few centimeters high. The SWOT satellite detects those subtle changes and translates them into detailed maps that outline what’s below.



<h2 class="wp-block-heading" id="h-influence-of-abyssal-hills">Influence of abyssal hills</h2>



“Abyssal hills are the most abundant landform on Earth, covering about 70% of the ocean floor,” said <a href="https://yaoyu9404.github.io/" target="_blank" rel="noreferrer noopener">Yao Yu</a> at the end of a recent study. Scientists also looked at <a href="https://www.sciencedirect.com/science/article/pii/S0079661115001391" target="_blank" rel="noreferrer noopener">abyssal hills</a>, which are smaller mounds covering much of the deep sea.&nbsp;



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/nasa_SWOT-mission_seamounts_Abyssal-hills_NASA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/nasa_SWOT-mission_seamounts_Abyssal-hills_NASA_1s.webp" alt="The joint NASA–CNES (Centre National d’Etudes Spatiales) Surface Water and Ocean Topography (SWOT) mission uses phase-coherent, wide-swath radar altimetry to measure ocean surface heights at high precision. Credit: NASA" class="wp-image-1968742"/></a><figcaption class="wp-element-caption">The joint NASA–CNES (Centre National d’Etudes Spatiales) Surface Water and Ocean Topography (SWOT) mission uses phase-coherent, wide-swath radar altimetry to measure ocean surface heights at high precision. Credit: NASA</figcaption></figure>



These rolling ridges can be just a few miles wide, making them difficult to observe from previous satellites. Any shifts in tectonic plates over time leave patterns on these hills, creating a geological record that is now clearer than ever.



<h2 class="wp-block-heading" id="h-ocean-mountains-currents-and-tides">Ocean mountains, currents, and tides</h2>



Seafloor structures direct deep-sea currents that move heat and nutrients across the globe. Currents flowing over steep slopes can drive pockets of marine life to gather near the slopes, forming biodiversity hotspots.



Understanding these dynamics leads to better insights about how ocean patterns impact climate and <a href="https://www.earth.com/news/fishing-removes-key-nutrients-from-marine-ecosystems/">marine ecosystems</a>. 



Oceanographers look at everything from tidal movements to nutrient exchange in these areas and plan to refine that analysis further with ongoing data collection.



<h2 class="wp-block-heading" id="h-life-thrives-in-hidden-places">Life thrives in hidden places</h2>



Underwater mountains and hills create slopes where currents slow down just enough to drop nutrients. These nutrient-rich zones become gathering spots for plankton, fish, and deep-sea corals.



Even in the darkest parts of the ocean, these formations act like magnets for life. Mapping them helps scientists locate fragile ecosystems that may need protection from deep-sea mining and trawling.



<h2 class="wp-block-heading" id="h-bridging-the-knowledge-gap">Bridging the knowledge gap</h2>



Mapping isn’t the main purpose of the SWOT satellite, but its radar altimeter collects precise measurements of water heights. 



That information can be converted into a topographic map of the sea surface, which mirrors the contours of the bottom.



This helps researchers chart terrain in places where ship-based sonar data remain sparse. It also complements efforts by the <a href="https://seabed2030.org/" target="_blank" rel="noreferrer noopener">Seabed 2030</a> project to fully survey the global seafloor by the end of this decade.



<h2 class="wp-block-heading" id="h-unexpected-military-and-climate-benefits">Unexpected military and climate benefits</h2>



Improved seafloor maps don’t just help scientists and sailors. Defense agencies use them to detect submarines, design sonar strategies, and assess undersea terrain for stealth operations.



The same data also play a role in climate modeling. Accurate bathymetry helps researchers trace heat flow in the <a href="https://www.earth.com/news/oceans-hidden-skin-could-protect-us-from-climate-change/">ocean</a>, a major factor in predicting long-term weather patterns and identifying areas vulnerable to sea level changes.



<h2 class="wp-block-heading" id="h-what-s-next-for-these-ocean-mountains">What's next for these ocean mountains?</h2>



Scientists plan to measure the depth of each feature more precisely next. They have squeezed out nearly all possible details about seafloor shapes from the first year of SWOT data, which could revolutionize future marine research.



Even with the best technology, complete sonar-based coverage of Earth’s ocean will still take time. However, satellite missions like SWOT will speed up progress and ensure more sections of the ocean floor are understood.



The study is published in <a href="https://www.science.org/doi/10.1126/science.ads4472" target="_blank" rel="noreferrer noopener">Science</a>.



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NASA's new underwater map reveals nearly 100,000 hidden mountains beneath the ocean

Scientists have come up with a new high-resolution map of...

Science has been chasing a single rulebook for nature ever since people realized the same laws that guide apples also steer planets. Three of the four known forces - electromagnetism, the strong force, and the weak force - comfortably share pages in that quantum physics manual. 



Gravity, though vital to everything from tides to timekeeping, insists on speaking a different dialect inspired by Einstein’s theory of general relativity.



That mismatch keeps physicists up at night. <a href="https://www.earth.com/news/new-form-of-quantum-entanglement-discovered-will-transform-next-gen-technology/" target="_blank" rel="noreferrer noopener">Quantum ideas</a> describe particles and fields in tiny, jumpy packages, while general relativity paints gravity as smooth curves in space‑time. 



Fit those viewpoints together, and the math usually blows up into useless infinities. A fresh effort now claims to tame those infinities without bending the facts we already trust.



<h2 class="wp-block-heading" id="h-bridging-gravity-and-quantum-forces">Bridging gravity and quantum forces</h2>



Researchers Mikko Partanen and Jukka Tulkki at <a href="https://www.aalto.fi/en" target="_blank" rel="noreferrer noopener">Aalto University</a> believe they have found common ground. They place gravity inside a type of gauge theory, the same broad framework that lets photons mediate light and <a href="https://www.earth.com/news/atomic-nucleus-made-of-quarks-and-gluons-reproduced-for-the-first-time/" target="_blank" rel="noreferrer noopener">gluons glue quarks</a>. 



“If this turns out to lead to a complete quantum field theory of gravity, then eventually it will give answers to the very difficult problems of understanding singularities in black holes and the Big Bang,” he says. 



The pair argue that the payoff could stretch far beyond pure curiosity; without <a href="https://www.earth.com/news/cosmic-glitch-in-gravity-expands-the-theory-of-general-relativity/" target="_blank" rel="noreferrer noopener">Einstein’s gravity</a>, for instance, GPS satellites would drift miles off course in a day.



Their proposal, published in Reports on Progress in Physics, introduces an eight‑dimensional mathematical space that hosts gravity alongside the other forces. 



In everyday life we move through three dimensions plus time, yet the extra four directions allow the equations to behave properly. 



By choosing a symmetry that mirrors the Standard Model, they avoid clashing with proven particle physics. The plan looks daring, but the researchers are convinced it keeps both feet on solid ground.



<h2 class="wp-block-heading" id="h-spinors-and-symmetry">Spinors and symmetry</h2>



Inside the eight‑dimensional arena, spinors - exotic objects that keep track of how particles twist - carry gravity’s information. 



“The main idea is to have a gravity gauge theory with a symmetry that is similar to the <a href="https://www.earth.com/news/quantum-entanglement-spooky-action-at-a-distance-persists-between-top-quarks/" target="_blank" rel="noreferrer noopener">Standard Model</a> symmetries, instead of basing the theory on the very different kind of spacetime symmetry of general relativity,” says Partanen, the study’s lead author. 



Using a shared symmetry lets gravity slot into the same style of equations that already explain how electrons interact with light.



That symmetry also dictates a new kind of gravitational field. 



“The most familiar gauge field is the <a href="https://www.earth.com/news/invisible-electric-field-discovered-surrounding-earth-nasa-says-its-as-crucial-as-gravity/" target="_blank" rel="noreferrer noopener">electromagnetic field</a>. When electrically charged particles interact with each other, they interact through the electromagnetic field, which is the pertinent gauge field,” explains Tulkki. 



“So when we have particles which have energy, the interactions they have just because they have energy would happen through the gravitational field.” 



In short, energy - not mass alone - becomes the charge that gravity responds to in this setup.



<h2 class="wp-block-heading" id="h-space-time-dimension-field">Space‑time dimension field</h2>



Extra dimensions sound abstract, yet the theory never asks anyone to live in them. Instead it builds a “space‑time dimension field” that quietly translates eight‑dimensional math into the four‑dimensional universe people occupy. 



That bridge preserves the equivalence principle, the observation that a feather and a hammer fall together in a vacuum, even though the calculations chug away behind the curtain in higher‑dimensional space.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/gravity-quantum-field_theory-of-everything_illustration_credit-Aalto-University_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/gravity-quantum-field_theory-of-everything_illustration_credit-Aalto-University_1s.webp" alt="The gravity quantum field is calculated in flat spacetime. The curved classical metric is calculated using the expectation value of the gravity quantum field. Credit: Aalto University" class="wp-image-1968436"/></a><figcaption class="wp-element-caption">The gravity quantum field is calculated in flat spacetime. The curved classical metric is calculated using the expectation value of the gravity quantum field. Click image to enlarge. Credit: Aalto University</figcaption></figure>



Because the field emerges from strict symmetry rules, the resulting gravity still pulls objects along the familiar paths predicted by Einstein, at least in calm conditions like those near Earth. 



Where things heat up - think black‑hole edges or the newborn universe - the new math starts to reveal effects that classical relativity misses.



<h2 class="wp-block-heading" id="h-quantum-gravity-and-renormalization">Quantum gravity and renormalization</h2>



Previous attempts to quantize gravity ran aground when higher‑order calculations spiraled into infinite answers. The Aalto approach leans on a tool called renormalization, which systematically sweeps those infinities into measurable constants. 



“If renormalization doesn’t work for higher order terms, you’ll get infinite results. So it’s vital to show that this renormalization continues to work,” explains Tulkki. So far, first‑order checks look solid; the team is pushing deeper to prove the pattern holds.



Keeping infinities in line would let physicists compute reliable probabilities for violent cosmic events. It also means gravity can be treated with the same respect as the other forces - in short, no more special exemptions that break the rules when the math gets messy.



<h2 class="wp-block-heading" id="h-black-holes-big-bangs-quantum-gravity">Black holes, big bangs, quantum gravity</h2>



“A quantum theory of gravity is needed to understand what kind of phenomena there are in cases where there’s a <a href="https://www.earth.com/news/unraveling-gravity-quantum-nature-entanglement-mechanics/" target="_blank" rel="noreferrer noopener">gravitational field</a> and high energies,” says Partanen. 



Such conditions prevail near the edges of black holes and during the first instants after the <a href="https://www.earth.com/news/more-than-one-big-bang-may-explain-cosmic-expansion-without-dark-matter/" target="_blank" rel="noreferrer noopener">Big Bang</a>, places where current theories shrug. 



A working quantum gravity model could clarify whether singularities truly exist or whether new physics softens the infinities predicted by Einstein’s equations.



Deeper still, the theory might speak to nagging puzzles about why <a href="https://www.earth.com/news/higgs-boson-god-particle-still-remains-quantum-mystery-after-12-years/" target="_blank" rel="noreferrer noopener">matter outnumbers antimatter</a>. 



“A theory that coherently describes all fundamental forces of nature is often called the Theory of Everything,” says Partanen, although he doesn’t like to use the term himself. 



“Some fundamental questions of physics still remain unanswered. For example, the present theories do not yet explain why there is more matter than antimatter in the observable universe.” Unifying gravity could offer fresh angles on that imbalance.



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



Partanen and Tulkki openly admit the work is not finished. They must prove the renormalization machinery survives every level of the calculation and make sure no hidden contradictions lurk in the symmetry choices. 



Independent teams will also test whether the new gravity predicts subtle deviations - tiny shifts in particle behavior or cosmic signals - that future experiments can check.



For now, the duo have invited the wider community to kick the tires. 



“Like quantum mechanics and the theory of relativity before it, we hope our theory will open countless avenues for scientists to explore,” Partanen concludes. 



Success would finally let gravity pull its weight in the quantum club, tightening the threads that tie the universe together.



The full study was published in the journal <a href="https://iopscience.iop.org/article/10.1088/1361-6633/adc82e" target="_blank" rel="noreferrer noopener">Reports on Progress in Physics</a>.



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Gravity discovery brings us one step closer to a unified "Theory of Everything"

Science has been chasing a single rulebook for nature ever...

Many people believe that small skin injuries heal quickly. Recent findings suggest that compared to certain other primates, human skin heals at a much slower pace.



Researchers measured how quickly skin edges moved together after injuries in humans and discovered a rate about one-third of what they saw in non-human primates. 



Their work indicates that humans might have traded rapid recovery for other unique <a href="https://www.earth.com/news/future-tech-will-track-emotions-through-changes-in-our-skin/" target="_blank" rel="noreferrer noopener">characteristics</a>.



Dr. Akiko Matsumoto-Oda, an evolutionary scientist with the <a href="https://www.u-ryukyu.ac.jp/en/" target="_blank" rel="noreferrer noopener">University of the Ryukyus</a>, conducted these investigations with collaborators from the Kyoto University <a href="https://www.wrc.kyoto-u.ac.jp/en/" target="_blank" rel="noreferrer noopener">Wildlife Research Center</a>. 



They studied volunteers undergoing medically required skin procedures, as well as various primates in structured environments.



<h2 class="wp-block-heading" id="h-why-human-skin-heals-slower-than-primates">Why human skin heals slower than primates</h2>



Scientists have long recognized that different species rely on diverse strategies for <a href="https://www.earth.com/news/teen-skin-bacteria-could-hold-the-secret-to-acne-prevention/" target="_blank" rel="noreferrer noopener">tissue</a> repair. Some rely on quick wound contraction, while others regenerate skin through careful layering of new cells.



Hair follicles play a big part in healing because each follicle can hold stem cells that jump into action once the skin is injured. 



Humans, however, lack the dense covering seen in many fur-bearing mammals, which can mean a smaller pool of helpful cells.



<h2 class="wp-block-heading" id="h-sweat-glands-impact-skin-healing-in-humans">Sweat glands impact skin healing in humans</h2>



Sweat glands help <a href="https://www.earth.com/news/human-bodies-begin-breaking-down-two-very-precise-ages/" target="_blank" rel="noreferrer noopener">people</a> stay cool in hot conditions, but they might not support tissue repair as efficiently as follicles. Researchers think that a shift toward more sweat glands and fewer follicles could have slowed healing.



Perspiration lets people remain active for longer in warm regions. This advantage may have outweighed the slower closure of skin wounds, giving humans better odds in harsh environments.



<h2 class="wp-block-heading" id="h-social-structures-compensate-for-slow-healing">Social structures compensate for slow healing</h2>



Reduced healing speed might seem problematic. Yet humans have social systems that can compensate for a delayed rate of repair.



Community care, shelter, and shared resources ensure that a slow recovery does not always threaten survival. 



Archaeological <a href="https://www.nejm.org/doi/full/10.1056/NEJM199909023411006" target="_blank" rel="noreferrer noopener">evidence</a> points to the fact that ancient groups cared for individuals with injuries, allowing them to live despite physical challenges.



<h2 class="wp-block-heading" id="h-human-skin-healing-differs-from-other-primates">Human skin healing differs from other primates</h2>



Chimpanzees showed a wound-closure pace similar to monkeys, suggesting they all share a roughly similar rate. Humans were the clear exception in this investigation.



Experts noted that a thicker epidermis and a more elaborate sweat duct system could be part of the reason. These <a href="https://www.pnas.org/doi/10.1073/pnas.0914628107" target="_blank" rel="noreferrer noopener">traits</a> likely emerged as humans evolved larger brains and better heat management.



<h2 class="wp-block-heading" id="h-what-drives-human-skin-s-structure">What drives human skin’s structure</h2>



Dermatologist teams often examine how genes shape the surface of our bodies. Emerging <a href="https://pubmed.ncbi.nlm.nih.gov/12822721/" target="_blank" rel="noreferrer noopener">research</a> suggests that specific genetic switches influence sweat gland formation, hair density, and wound repair.



Variations in these pathways likely pushed ancient humans toward less body hair. Over time, the result was a distinctive type of <a href="https://www.earth.com/news/skin-may-play-a-hidden-role-in-ebola-infection/" target="_blank" rel="noreferrer noopener">skin</a> that protects us while sacrificing rapid recovery from damage.



<h2 class="wp-block-heading" id="h-why-slow-skin-healing-is-a-concern">Why slow skin healing is a concern</h2>



Slow wound repair remains a challenge in modern clinics. Specialists are searching for therapies that might encourage faster closure, especially in older adults and those with illnesses.



Looking to primates and other mammals could inspire new approaches. If scientists can figure out what helps non-human species regrow skin so effectively, they might adapt those tools for human medicine.



<h2 class="wp-block-heading" id="h-toward-future-solutions">Toward future solutions</h2>



Gene editing, advanced dressings, and novel cell-based treatments hold potential. Combining these discoveries with an understanding of natural healing in primates might shorten recovery times.



Some <a href="https://pubmed.ncbi.nlm.nih.gov/30890574/" target="_blank" rel="noreferrer noopener">researchers</a> hope to replicate the healing strategy of smaller mammals that close cuts quickly. Although it is still experimental, progress in stem cell therapy could transform patient outcomes.



<h2 class="wp-block-heading" id="h-how-doctors-approach-slow-skin-healing">How doctors approach slow skin healing</h2>



Recognizing that human skin mends more slowly can alter how surgeons and doctors manage postoperative care. Extra monitoring of sutures and incisions might prevent complications.



People with chronic wounds could benefit from therapies tailored to overcome certain genetic hurdles. Targeted interventions might address the biology behind slower healing in humans.



<h2 class="wp-block-heading" id="h-modern-medicine-still-lags-behind-nature">Modern medicine still lags behind nature</h2>



Despite advances in medical care, human wound healing often relies on external help like stitches, antibiotics, and dressings to prevent infection and speed recovery. 



These interventions, while effective, highlight how dependent we’ve become on tools to make up for our slower natural response.



In contrast, non-human primates and rodents typically heal without assistance, suggesting that their bodies are still better wired for independent repair. 



This contrast points to an evolutionary gap between our biological abilities and the environments we've built to support them.



<h2 class="wp-block-heading" id="h-new-research-on-human-skin-healing">New research on human skin healing</h2>



Additional insights from comparative biology might identify subtle differences that set human skin apart. Continued experiments may reveal fresh angles on how hair follicles, sweat glands, and immune responses interplay.



Clues from ancient fossils hint that humans have coped with injuries for centuries. Groups likely shared information about wound treatments, shaping our medical traditions.



The study is published in <a href="https://royalsocietypublishing.org/doi/10.1098/rspb.2025.0233" target="_blank" rel="noreferrer noopener">Proceedings of the Royal Society B: Biological Sciences</a>.



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Medical oddity: Human skin heals three times slower than our primate relatives

Many people believe that small skin injuries heal quickly. Recent...

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



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



<figure class="wp-block-embed aligncenter is-type-video is-provider-youtube wp-block-embed-youtube wp-embed-aspect-16-9 wp-has-aspect-ratio"><div class="wp-block-embed__wrapper">
https://youtu.be/Ug657J67iEo?si=w96YjGMsg939LD_3
</div></figure>



Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



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



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



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



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



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



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



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

Is chocolate the next nutritional powerhouse?

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

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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