Crater Lake National Park, Oregon

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 the European Space Agency...

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...

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA



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Rosetta Nebula: Sculpted by starlight over millions of years

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 new health-assessment method, called the Health Octo Tool, uses eight measures drawn from physical exams and routine lab tests to calculate a person’s biological age. 



The tool may predict an individual’s risk of disability and death more accurately than existing health predictors.



<h2 class="wp-block-heading" id="h-new-tool-to-measure-aging">New tool to measure aging </h2>



The research team, led by Shabnam Salimi from the <a href="https://www.uwmedicine.org/school-of-medicine" target="_blank" rel="noreferrer noopener">University of Washington School of Medicine</a>, believes the tool could uncover new factors that shape the aging <a href="https://www.earth.com/news/defying-time-three-ways-to-slow-biological-aging/">process</a> and help design interventions to extend lifespan. Salimi is a physician-scientist and acting instructor in the Department of Anesthesiology &amp; Pain Medicine. 



According to Salimi, existing health-assessment methods focus on the effects of individual diseases. However, they fail to take into consideration the interactions among diseases and how minor disorders affect overall health.



“An aging-based framework offers a new path to discover <a href="https://www.earth.com/news/alzheimers-disease-earliest-biomarker-protein-psd-95-identified/" target="_blank" rel="noreferrer noopener">biomarkers</a> and therapeutics that target organ-specific or whole-body aging, rather than individual diseases,” she explained.



The tool is built around the concept of “health entropy,” which refers to the accumulation of molecular and cellular damage over time and its impact on how well the body’s organs and systems function. 



In short, health entropy can be viewed as an indicator of a person’s general physical condition and can be translated into a measure of how quickly or slowly someone is aging.



<h2 class="wp-block-heading" id="h-data-from-major-aging-studies"><a></a>Data from major aging studies</h2>



To develop and test the Health Octo Tool, the researchers analyzed data from the <a href="https://www.blsa.nih.gov/" target="_blank" rel="noreferrer noopener">Baltimore Longitudinal Study on Aging</a>, one of the world’s longest-running aging studies. They used participants’ medical histories, physical exam results, and lab test outcomes. 



To confirm their findings, they then tested the method on two additional large datasets covering over 45,000 adults. The team first created what they called a Body Organ Disease Number. 



This score reflects how many organ systems - such as the cardiovascular, respiratory, and nervous systems - are affected by disease and whether a person has had <a href="https://www.earth.com/news/ai-is-the-next-frontier-in-cancer-treatment/" target="_blank" rel="noreferrer noopener">cancer</a> or a stroke. The score ranges from 1 to 14, depending on the extent of organ system involvement.



<h2 class="wp-block-heading" id="h-a-detailed-picture-of-biological-age">A detailed picture of biological age </h2>



“Our findings demonstrated that organ systems age at different rates, prompting us to develop a Bodily System-Specific Age metric to reflect the aging rate of each organ system and the Bodily-Specific Clock to represent each organ system’s intrinsic biological age,” Salimi said.



“Extending this concept to the whole body, we define the Body Clock as a composite measure of overall intrinsic age and Body Age as the corresponding rate of aging.”



Since not all people of the same biological age experience the same level of physical decline, the team also created additional metrics. These include the Speed-Body Clock and Speed-Body Age, which describe how biological age affects walking speed - often used as a simple test of older adults’ <a href="https://www.earth.com/news/biological-age-or-chronological-age-which-is-more-important/" target="_blank" rel="noreferrer noopener">functional capacity</a>.



<h2 class="wp-block-heading" id="h-measuring-disability-risks">Measuring disability risks</h2>



The team also introduced the Disability-Body Clock and Disability-Body Age, designed to estimate how aging influences the risk of developing cognitive or physical disabilities.



“Collectively, these eight metrics - Body Clock, Body Age, system-specific clocks and rates, Speed- and Disability-based clocks - offer a way to view an individual’s aging process with information gathered from their medical history, physical exam, and test results alone,” Salimi said.



One key takeaway from the study is that even relatively minor health conditions, if left untreated early in life, can significantly influence biological aging later on. 



For example, untreated high blood pressure during youth may greatly accelerate aging down the line. This suggests that early treatment of such conditions could have a meaningful impact on lifelong health.



<h2 class="wp-block-heading" id="h-looking-ahead-a-digital-aging-tracker"><a></a>Looking ahead: A digital aging tracker</h2>



The research team is now working on a digital app that will allow individuals and their healthcare providers to calculate their body’s and organs’ biological ages. The tool will let people track how quickly they are aging and measure the effects of lifestyle changes or treatments.



“Whether someone is adopting a new <a href="https://www.earth.com/news/dietary-restriction-slows-brain-aging-and-increases-lifespan/" target="_blank" rel="noreferrer noopener">diet</a>, exercise routine or taking longevity-targeting drugs, they will be able to visualize how their body - and each organ system - is responding,” Salimi explained.



By combining clinical data with detailed biological models, the Health Octo Tool offers a promising new way to track aging, tailor treatments, and potentially improve long-term health outcomes.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-58819-x" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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How old are you, really? New tool measures aging from the inside out

A new health-assessment method, called the Health Octo Tool, uses...

Healthy smiles often require more than simply brushing and flossing. People can develop stubborn buildup on their teeth that leads to discoloration and unpleasant odors.



One approach involves using a citrus drink that some believe can help remove this buildup. This method is supported by <a href="https://www.researchgate.net/scientific-contributions/Sealomita-Rizka-Apritama-2295981427" target="_blank" rel="noreferrer noopener">Dr. Sealomita Rizka Apritama</a>, who is affiliated with the Department of Public Health at the Institute for Advanced Health Science and Technology in Indonesia.



<h2 class="wp-block-heading" id="h-understanding-tartar">Understanding tartar</h2>



Tartar is a hardened layer that forms when plaque stays on tooth surfaces for too long. It can appear yellowish or brownish and might lead to serious problems if ignored.



This buildup can cause <a href="https://www.ncbi.nlm.nih.gov/books/NBK557422/" target="_blank" rel="noreferrer noopener">gingivitis</a>, a form of gum inflammation, and it can also pave the way for <a href="https://www.ncbi.nlm.nih.gov/books/NBK554590/" target="_blank" rel="noreferrer noopener">periodontitis</a>, which may damage deeper tissues. It often contributes to <a href="https://www.ncbi.nlm.nih.gov/books/NBK534859/" target="_blank" rel="noreferrer noopener">halitosis</a> by creating a cozy environment for odor-causing bacteria.



Some people notice that tartar makes their teeth look dull. Others experience gum bleeding or sensitivity if they neglect proper cleaning.



Professional cleanings are the most reliable way to remove large amounts of buildup. Regular checkups help address early signs and reduce the need for complicated procedures.



<h2 class="wp-block-heading" id="h-why-lemon-stands-out">Why lemon stands out</h2>



Researchers have observed that lemon contains citric acid, which seems to discourage bacterial growth on teeth. They note that even moderate amounts may help reduce plaque deposits on tooth surfaces.



Lemon’s acidity can assist in removing surface stains, and making enamel brighter. It also leaves a refreshing scent that helps with bad breath.



Some people find this home remedy appealing because it is easy to prepare. Others like that it may address multiple concerns with minimal effort.



Dentists suggest being careful about using any highly acidic substance on teeth. Overuse can lead to enamel erosion and sensitivity.



<h2 class="wp-block-heading" id="h-easy-steps-to-get-started">Easy steps to get started</h2>



A basic citrus drink involves mixing half a squeezed lemon with about eight ounces (240 milliliters) of water. People often swish it around their mouths for around half a minute, though a few prefer gentle brushing with the solution.



Experts recommend rinsing with plain water right after to reduce <a href="https://www.ada.org/resources/ada-library/oral-health-topics/dental-erosion" target="_blank" rel="noreferrer noopener">acidity</a>. This practice helps protect the enamel from weakening.



Most individuals limit this step to once or twice a week. Excessive repetition might strain tooth surfaces, so moderation is key.



Combining this approach with daily brushing and flossing preserves a healthy foundation. Nobody wants to trade tartar problems for enamel issues.



<h2 class="wp-block-heading" id="h-extra-details-to-remember">Extra details to remember</h2>



Healthcare providers discourage replacing standard oral hygiene with lemon alone. They view this drink as a small addition rather than a full substitute.



It is wise to talk with a dentist if you have sensitive teeth before trying acidic gargles. For some, mild enamel flaws can worsen under frequent contact with strong acids.



Special caution is also advised when combining lemon with other products like baking soda. That mixture can make your teeth feel gritty or lead to further irritation.



Anyone who notices continued discoloration or sore gums should seek professional guidance. Timely dental advice can prevent bigger issues down the road.



<h2 class="wp-block-heading" id="h-keeping-a-balanced-routine">Keeping a balanced routine</h2>



The researchers noted that oral health is often considered to be on par with physical wellness. This perspective motivates many to brush and floss carefully, aiming to mitigate the effects of harmful bacteria.



Sugary snacks can speed up plaque formation because they feed those bacteria. Rinsing with water after sweet treats may help decrease leftover residues in the mouth.



High water intake helps keep the mouth moist and washes away stray particles. Dryness can lead to faster bacterial buildup, making it crucial to stay hydrated.



Tobacco use also worsens oral problems by discoloring teeth and increasing gum-related risks. Many smokers end up with more frequent tartar and unwanted stains.



<h2 class="wp-block-heading" id="h-smart-additions-for-better-results">Smart additions for better results</h2>



People might consider drinking water throughout the day to keep debris from clinging to teeth. Fruit and vegetable snacks can also stimulate saliva flow, which contributes to cleaning.



Some find that using fluoride toothpaste guards against decay and boosts enamel strength. Others benefit from mouthwash with antibacterial agents that can target hidden spots.



Routine cleanings by an oral hygienist can spot early warning signs that home methods cannot address. Dentists can detect whether a particular lemon rinse or other technique is suitable.



Balanced diets and regular checkups remain fundamental steps toward a strong smile. Lemon water might enhance results, but it works best alongside proven strategies.



<h2 class="wp-block-heading" id="h-final-thoughts">Final thoughts</h2>



A lemon-based rinse may help remove light stains and reduce certain odor-causing bacteria. It fits into a broader plan of brushing, flossing, and paying attention to diet.



This approach should not replace professional care. Dentists remain the best resource when stubborn tartar calls for a deeper cleaning.



The study is published in the <a href="https://www.ijahst.org/index.php/ijahst/article/view/402" target="_blank" rel="noreferrer noopener">International Journal of Advanced Health Science and Technology</a>.



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Say goodbye to stains and bad breath: the citrus drink that helps remove tartar and whitens teeth

Healthy smiles often require more than simply brushing and flossing....

Young,Amazed,Male,Kid,School,Boy,5-6,Years,Old,In

New research reveals that children as young as five already have the brain systems in place to support map-based navigation. For years, it’s been assumed that children don’t develop the brain systems for navigating large spaces - like towns or neighborhoods - until they’re around 12 years old.



But that idea may need some serious rethinking after this surprising discover from <a href="https://www.emory.edu/home/index.html" target="_blank" rel="noreferrer noopener">Emory University</a>.



<h2 class="wp-block-heading" id="h-studying-mental-maps-in-children">Studying mental maps in children</h2>



Using brain scans and a fun, virtual environment called “Tiny Town,” the scientists designed experiments to see whether young kids could mentally map a town and navigate its streets. 



The results showed that even five-year-olds were able to use the retrosplenial complex (RSC), a brain region involved in <a href="https://www.earth.com/news/how-our-brains-build-mental-maps-of-the-world/" target="_blank" rel="noreferrer noopener">spatial navigation</a>, to get around a virtual world.



“While large-scale navigation abilities certainly continue to develop throughout childhood, our findings show that the underlying neural system is established remarkably early,” said Yaelan Jung, first author and postdoctoral fellow in Emory’s Department of Psychology.



“Rather than taking a decade or more, map-based navigation is underway in half that time,” noted Daniel Dilks, associate professor of psychology and senior author of the study.



“Five-year-olds have the brain system enabling them to find their way around a tiny, virtual town. They not only know that the ice cream store in the mountain region is different than the ice cream store in the lake region, they know how to navigate the streets to get to each of them.”



<h2 class="wp-block-heading" id="h-building-maps-in-the-brain">Building maps in the brain</h2>



Understanding how the brain helps us recognize places and navigate the world is a key focus for researchers. One major tool for exploring these questions is <a href="https://www.earth.com/news/brain-imaging-method-will-unravel-mysteries-of-neural-processes/" target="_blank" rel="noreferrer noopener">functional magnetic resonance imaging</a> (fMRI). This noninvasive technique tracks changes in blood flow in the brain to identify which regions are active during different tasks.



Previous research had shown that three areas in the <a href="https://www.earth.com/news/how-the-human-brain-processes-visual-information/" target="_blank" rel="noreferrer noopener">visual cortex</a> specialize in handling scenes and navigation. The parahippocampal place area, or PPA, helps us recognize and categorize places. 



The retrosplenial complex, or RSC, allows us to map places within a larger space and figure out how to travel from one location to another. Meanwhile, the occipital place area, or OPA, helps us move through spaces without bumping into obstacles.



“Two fundamental questions in neuroscience are how knowledge is organized in the brain and the origins of that knowledge,” said Dilks. “In other words, what knowledge are you born with and how does knowledge develop as you grow?”



“We can’t fix most neurological problems right now. But by continuing to learn more about how the brain develops and functions normally, we keep moving closer to being able to repair it when something goes wrong.”



<h2 class="wp-block-heading" id="h-when-walking-is-harder-than-mapping">When walking is harder than mapping</h2>



Interestingly, the same research team previously found that the brain system responsible for helping kids walk around and avoid obstacles doesn’t mature until age 8.



“It seems counterintuitive,” says Dilks. “Most children can walk before the age of two. And yet the brain system helping you walk around your immediate surroundings doesn’t start appearing adultlike until relatively late.”



That puzzling timeline led the researchers to wonder if the brain might support more advanced map-like navigation skills in children earlier than previously thought. 



After all, children often experience the world through strollers, car rides, or being carried, helping them form <a href="https://www.earth.com/news/mental-maps-help-the-brain-remember-places-and-paths/" target="_blank" rel="noreferrer noopener">mental maps</a> even before they’re mobile themselves. To test this idea, the team designed a special experiment for five-year-olds.



<h2 class="wp-block-heading" id="h-welcome-to-tiny-town">Welcome to Tiny Town</h2>



The experiment began with a virtual environment called Neuralville, which featured eight buildings and a town square. However, the team soon realized it was too complex for young children. 



So, they simplified it, creating a triangular map called Tiny Town for the children to explore. Each corner of Tiny Town had a unique setting - a mountain, a tree, or a lake - to help kids orient themselves. 



The town had six buildings in total, including two each of fire stations, playgrounds, and ice cream stores. The goal was to make science approachable and fun for the kids.



“We want to get at the scientific questions that we’re trying to answer,” explained Jung, “but it’s also important that a child who participates in a study has a good time. We want them to leave with a good impression of science.”



The kids first explored Tiny Town on a computer, using arrow keys to “walk” through the streets. Then came the tests. Researchers showed them still images of buildings and asked if they had seen them before, or whether they were located in specific areas of the town.



Most of the children passed with ease. They then advanced to the next stage: learning how to stay still inside a brain scanner.



<h2 class="wp-block-heading" id="h-turning-brain-scans-into-a-game">Turning brain scans into a game</h2>



To prepare the kids for the scanner, the research team turned the training into a playful challenge. An adult would yell “Freeze!” and the child had to stay perfectly still - just like in the real scanner.



“The kids loved it! They especially liked to freeze the adults in the room,” said Jung. “They’d point at one of us and say, ‘It’s your turn now!’”



The children were told that the scanner was like a camera, and that staying still was necessary to get a clear photo while they performed tasks inside. To make it cozy, they were given a pillow and blanket and told they’d be watching a movie in their own private theater.



Inside the scanner, kids were shown images from Tiny Town and asked to push a button if certain combinations were accurate - for example, matching a fire station with the correct landscape setting. They practiced this task beforehand in a mock scanner to feel comfortable.



The brain scans revealed something remarkable: the five-year-olds were using their RSC to navigate, just like adults do. The children were building maps in their minds and using them to figure out where things were located.



<h2 class="wp-block-heading" id="h-moving-forward-children-building-maps">Moving forward: Children building maps</h2>



Beyond the scientific insight, the experiment was a joy for everyone involved. “It was really fun to work with the children,” noted Jung. “I learned that the age of five is a magical time to scan a child. They don’t tend to be afraid of new things.”



The research team is now planning a new project involving toddlers. That’s proven to be a bit trickier.



“Between the ages of two and three, children basically don’t listen to you,” said Jung, who is also the mother of a three-year-old.



To help the toddlers feel comfortable, the researchers are experimenting with cardboard scanners, cartoons, and Cheerios. The ultimate goal is to understand how the brain’s navigation system grows from infancy to adulthood - and how it might differ in children with <a href="https://www.earth.com/news/virtual-reality-will-unlock-mysteries-of-developmental-disorders/" target="_blank" rel="noreferrer noopener">developmental conditions</a>.



“It’s fascinating to explore how humans use different parts of the brain for complex behaviors and how that changes with age and experiences,” said Jung. “We’re laying the groundwork for clinical applications, including getting a better understanding of typical versus atypical neural development.”



The full study was published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2503569122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



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Children have the brainpower to navigate maps at a very young age

New research reveals that children as young as five already...

Colorful,Parrotfish,Feeding,On,A,Tropical,Coral,Reef

Coral reefs are among the most dazzling ecosystems on Earth. When viewed from above, they display intricate structures and colors. But many reefs also show curious rings of bare sand encircling them. These circles, called grazing halos, appear in satellite images as pale outlines around patches of coral.



The origin of grazing halos has long puzzled scientists. Why do they form in some places and not others? Why do they vary in size? And most importantly - do they reveal something about the health of the reef?



A new study published in The American Naturalist suggests a surprising answer. It’s not just fear that creates these halos - it’s also the way <a href="https://www.earth.com/news/breaks-in-ancient-coral-growth-reveal-earths-climate-past/" target="_blank" rel="noreferrer noopener">coral</a> shelter is arranged.



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



One widely accepted theory to explain grazing halos involves fear. Fish like parrotfish and other herbivores leave the safety of coral reefs to feed on algae or seagrass.



However, they do not venture far because predators like sharks lurk in the open. To avoid becoming prey, these fish tend to graze close to shelter.



Their grazing creates visible halos - barren rings where the vegetation has been eaten. The behavior aligns with what ecologists call the “landscape of fear.”



According to this idea, prey animals avoid open areas and concentrate activity near shelter, which alters the way that <a href="https://www.earth.com/news/coral-reefs-may-be-more-resilient-than-we-thought/" target="_blank" rel="noreferrer noopener">ecosystems</a> look.



But this explanation has gaps. Some reefs that are full of predators lack halos. Others, where predator populations have collapsed due to overfishing, still show clear halos. 



Something else must be shaping these patterns - something embedded in the landscape itself.



<h2 class="wp-block-heading" id="h-reef-shelter-layout-and-halo-formation">Reef shelter layout and halo formation</h2>



The new study points to the layout of coral shelters as a missing piece of the puzzle. The researchers examined how the spatial distribution of reef <a href="https://www.earth.com/news/coral-reefs-may-not-adapt-quickly-enough-to-survive-climate-change/" target="_blank" rel="noreferrer noopener">structures</a> influences halo formation. Do halos behave differently when coral is clustered tightly versus scattered widely?



The team used Heron Island on Australia’s Great Barrier Reef to test their ideas. This site is a hub for reef science and faces ongoing threats from climate change, including coral bleaching, storm damage, and ocean acidification.



The study explored how coral shelter layout affects where herbivores graze. Some corals are clustered closely together and provide tightly packed shelter, while others are more dispersed. 



The scattered corals create more distance between safe zones. The team predicted that these differences would shape how halos appear - or disappear - across the seascape.



<h2 class="wp-block-heading" id="h-models-predict-halo-shapes-on-reefs">Models predict halo shapes on reefs</h2>



To explore this, the researchers built two mathematical models. The first was geometric. It examined how simple circular shapes - representing coral patches - overlap on the seafloor. This helped predict how much vegetation should remain in areas around the patches, depending on how the shelters are arranged.



Study lead author Theresa Ong is an assistant professor of environmental studies at Dartmouth.



“If the shelter <a href="https://www.earth.com/news/coral-reefs-could-vanish-if-temperatures-continue-to-rise/" target="_blank" rel="noreferrer noopener">habitat</a> is tightly packed in one space, then there’s not much room for nervous prey to explore and less vegetation to eat. But if shelter is more evenly distributed, the halos carve out more empty space in the landscape and their distinctive patterns disappear into one another as they overlap," noted Professor Ong.



The geometric model revealed that clustered coral leads to clearer, more distinct halos. Scattered coral causes the rings to overlap and blur, making them harder to detect. This may explain why halos vary across reefs - even when predator presence remains constant.



<h2 class="wp-block-heading" id="h-grazing-patterns-change-over-time">Grazing patterns change over time</h2>



Geometry only tells part of the story. Grazing patterns change over time as vegetation regrows and fish populations fluctuate. So, the team developed a second model - one that added time and movement into the equation.



The dynamic model showed two scenarios. When coral patches are dispersed, fish must travel further to feed. This can lead to overgrazing - vegetation disappears, fish numbers drop, vegetation returns, and the cycle begins again. Halos may vanish and reappear in a rhythmic pattern.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/coral-reef_grazing-halos_great-barrier-reef_credit-Google-Earth_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/coral-reef_grazing-halos_great-barrier-reef_credit-Google-Earth_1s.webp" alt="Overview view of Heron Island on the Great Barrier Reef, Australia, and close-up view of a selected reef region (box in overview) where macroalgae cover is dense and coral halos (vegetation-free space surrounding coral patch reefs) are prevalent. Example 1X-scale plots (47 × 47 m) are indicated by arrows to illustrate increasing dispersion in coral patch distributions. Credit: Google Earth Pro" class="wp-image-1968578"/></a><figcaption class="wp-element-caption">Overview of Heron Island on the Great Barrier Reef, Australia, and close-up view of a selected reef region (box in overview) where macroalgae cover is dense and coral halos (vegetation-free space surrounding coral patch reefs) are prevalent. Example 1X-scale plots (47 × 47 m) are indicated by arrows to illustrate increasing dispersion in coral patch distributions. Click image to enlarge. Credit: Google Earth Pro</figcaption></figure>



When coral is clustered, grazing remains more localized and consistent. This leads to more stable halo patterns. 



The models suggest that both stable and cyclic halos can exist on <a href="https://www.earth.com/news/restored-coral-reefs-can-bounce-back-in-just-four-years/" target="_blank" rel="noreferrer noopener">healthy reefs</a> - and both tell stories about how the ecosystem is functioning.



<h2 class="wp-block-heading" id="h-not-all-changes-are-alarming">Not all changes are alarming</h2>



A major insight from the study is that halo patterns - whether stable or oscillating - are not in themselves signs of reef health or decline. What matters more is how those patterns change over time.



“Oscillating halos are not necessarily a sign of overfishing or poor reef health,” said Ong. “What’s more concerning is if static halos suddenly start cycling or if cyclic halos suddenly become static, which could indicate a major shift in system health and resilience.”



In other words – it’s not the presence or size of the halo that reveals the truth, but whether its behavior shifts in ways that suggest underlying ecological change.



<h2 class="wp-block-heading" id="h-using-satellites-for-reef-surveillance">Using satellites for reef surveillance</h2>



Studying coral reefs directly is expensive and difficult. That’s where satellite imagery offers a powerful advantage. Researchers can quickly scan large areas and assess general patterns - even from space.



“There are a lot of endemic species on reefs, especially on the <a href="https://www.earth.com/news/great-barrier-reef-is-on-the-brink-of-extinction/" target="_blank" rel="noreferrer noopener">Great Barrier Reef</a>, which we could easily lose due to the compounding effects of climate change and overfishing,” noted Professor Ong.



“So gaining a better understanding of how halo patterns reflect reef community dynamics may be useful in reef conservation efforts.”



Halos might become an early warning system. Their changes could alert scientists to shifts in predator numbers, herbivore behavior, or coral shelter integrity - all of which influence reef resilience.



<h2 class="wp-block-heading" id="h-halo-dynamics-beyond-reefs">Halo dynamics beyond reefs</h2>



The models developed by the team aren’t limited to coral reefs. They apply to any system where grazing happens near shelter. 



Think of cattle grazing near trees, or deer feeding near forest edges. The same logic - of safety shaping movement - plays out across many ecosystems.



Still, <a href="https://www.earth.com/news/coral-reefs-could-vanish-if-temperatures-continue-to-rise/" target="_blank" rel="noreferrer noopener">coral reefs</a> are especially fragile. Climate change is heating the oceans, acidifying waters, and disrupting food webs. Even subtle changes in reef structure can lead to major ecological shifts.



From overlapping rings of sand to predictive models and satellite imagery - this work reveals that coral reefs are writing their own story in patterns we can now begin to understand. We just have to learn how to read the halos.



The study is published in the journal <a href="https://www.journals.uchicago.edu/doi/10.1086/735688" target="_blank" rel="noreferrer noopener">The American Naturalist</a>.



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What 'grazing halos' and parrotfish reveal about coral reef health

Coral reefs are among the most dazzling ecosystems on Earth....

The Step Pyramid rises taller than a 20‑story building on the edge of Egypt’s desert plateau, about 15 miles south of the modern sprawl of Giza. Built roughly 4,650 years ago, it was the first gigantic structure ever assembled entirely from carved stone blocks. 



Yet for all its fame, scholars have long puzzled over how its builders coaxed more than 11 million cubic feet of limestone into perfectly symmetrical positions with the tools of their day.



A fresh study now hints that the secret may have flowed through channels and pools rather than up crumbling earthen ramps. 



By tracing <a href="https://www.earth.com/news/egypts-pyramids-were-built-along-a-buried-branch-of-the-nile-river/" target="_blank" rel="noreferrer noopener">ancient watercourses</a> visible in satellite radar images and matching them with clues cut into bedrock, researchers suggest that water power - a type of hydraulic elevator - did most of the work of raising the pyramid, tier by tier.



<h2 class="wp-block-heading" id="h-king-djoser-s-step-pyramid">King Djoser's Step Pyramid</h2>



Half a century before the better‑known pyramids at Giza, Pharaoh Djoser ordered his chief architect, Imhotep, to design a tomb like no other -- The Step Pyramid of Djoser.



The result was a six‑stepped monument that still stands between 197 ft and 203 ft tall. 



Instead of a single-level structure, Imhotep stacked six <a href="https://www.earth.com/news/3800-year-old-hexagonal-pyramid-discovered-possibly-a-royal-tomb/" target="_blank" rel="noreferrer noopener">layers of stone</a>, creating a striking staircase to the heavens. For the first time, Egyptian builders used large, carved limestone blocks.



In the decades that followed, the know‑how refined at Saqqara sparked a construction sprint in the region. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser_Saqqara-plateau_water-course_Volcano-hydraulic-lift_Paleotechnic_PLOS-One_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser_Saqqara-plateau_water-course_Volcano-hydraulic-lift_Paleotechnic_PLOS-One_1s.webp" alt="Map of the Saqqara plateau showing the water course from the Gisr el-Mudir dam to the water treatment facility near Djoser pyramid. The water is then transferred to the pyramid's network of pipes to power the hydraulic elevator. Credit: Paleotechnic of Paris, France" class="wp-image-1968267"/></a><figcaption class="wp-element-caption">Map of the Saqqara plateau showing the water course from the Gisr el-Mudir dam to the water treatment facility near Djoser pyramid. The water is then transferred to the pyramid's network of pipes to power the hydraulic elevator. Click image to enlarge. Credit: Paleotechnic of Paris, France</figcaption></figure>



Stones ballooned in size from 660 pounds apiece to more than 5,000 pounds, and roughly 28 million tons of masonry went into building just seven royal pyramids.



Surrounding the pyramid was an elaborate complex of courtyards, temples, and ceremonial spaces, all designed to serve the pharaoh in the afterlife. 



These spaces weren’t just symbolic - they were functional parts of a belief system that saw the king as a god on Earth.



<h2 class="wp-block-heading" id="h-finding-clues-etched-in-stone">Finding clues etched in stone</h2>



Leading the latest push towards unraveling this mystery is Dr. Xavier Landreau of the <a href="https://www.cea.fr/english/Pages/Welcome.aspx" target="_blank" rel="noreferrer noopener">CEA Paleotechnic Institute</a>. 



His French team combed through decades of excavation notes and paired them with high‑resolution radar scenes. 



“Satellite imagery clearly shows that a rectangular stone enclosure known as <a href="https://en.wikipedia.org/wiki/Gisr_el-Mudir" target="_blank" rel="noreferrer noopener">Gisr el‑Mudir</a>, located west of the Saqqara necropolis, has all the technical characteristics of a check dam," explains Dr. Landreau. 



"This feature would have been used to control the flow of flash floods and capture heavy objects coming from upriver.”



<h2 class="wp-block-heading" id="h-vanished-lake-purpose-built-moat">Vanished lake, purpose‑built moat</h2>



On the lee side of the dam, the landscape bows into a shallow basin. Soil chemistry there hints at a lake that swelled during seasonal Nile surges. 



When the water dropped, channels funneled the remaining flow into a rock‑cut trench now nicknamed the Dry Moat ringing the pyramid precinct. 



Its southern arm contains a line of chambers whose stepped floors resemble today’s sedimentation basins at municipal water plants.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser-complex_North-Saqqara_water-course-map_credit-Airbus_PLOS-ONE_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser-complex_North-Saqqara_water-course-map_credit-Airbus_PLOS-ONE_1s.webp" alt="North Saqqara map showing the relation between the Abusir water course and the Step Pyramid construction process (Inset). The arrows figuring the flow directions are approximate and given for illustrative purposes based on the Franco-Egyptian SFS/IGN survey. Satellite image: Airbus Pléiades" class="wp-image-1968271"/></a><figcaption class="wp-element-caption">North Saqqara map showing the relation between the Abusir water course and the Step Pyramid construction process (Inset). The arrows figuring the flow directions are approximate and given for illustrative purposes based on the Franco-Egyptian SFS/IGN survey. Click image to enlarge. Satellite image: Airbus Pléiades</figcaption></figure>



“Together, the Gisr el‑Mudir and the Dry Moat’s inner south section work as a unified hydraulics system that improves water quality and regulates flow for practical purposes and human needs,” the authors write. 



The cleaned runoff, they argue, arrived just in time to solve a pressing construction headache.



<h2 class="wp-block-heading" id="h-water-and-the-step-pyramid-stones">Water and the Step Pyramid stones</h2>



Inside the pyramid, stone corridors angle upward from a central shaft. Their shape and wear patterns nudge the imagination toward a liquid‑powered lift. 



“The <a href="https://www.earth.com/news/ancient-buildings-used-passive-cooling-methods-to-reduce-heat-with-out-air-conditioning/" target="_blank" rel="noreferrer noopener">ancient architects</a> likely raised the stones from the pyramid center in a volcano fashion using the sediment‑free water from the Dry Moat’s south section,” the authors write. 



Picture buoyant barges - or perhaps sealed sleds - nudged ever higher as fresh water flowed beneath them.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser-complex_subterranean-layout_credit-PLOS-One_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser-complex_subterranean-layout_credit-PLOS-One_1s.webp" alt="Overview of Djoser’s complex subterranean layout, focusing on the Latvian mission’s discoveries (orange parts)–courtesy of Monnier. Credit: PLOS One" class="wp-image-1968273"/></a><figcaption class="wp-element-caption">Overview of Djoser’s complex subterranean layout, focusing on the Latvian mission’s discoveries (orange parts)–courtesy of Monnier. Click image to enlarge. Credit: PLOS One</figcaption></figure>



Numbers support the idea. With a column of water roughly 30 ft deep, upward pressure could cancel out two‑thirds of a limestone block’s weight, leaving workers on terraced ledges to guide the payload into place. 



Such a system would sidestep the need for massive ramps long thought to encircle early pyramids yet never found in situ.



<h2 class="wp-block-heading" id="h-floods-first-droughts-later">Floods first, droughts later</h2>



“Before the Fourth Dynasty, there were more problems with floods than with a lack of water,” Dr. Landreau noted, highlighting why the Saqqara workforce might have embraced hydraulic engineering. 



Annual inundations could swallow work sites, rot timber, and strand supplies. Turning surplus water into a construction ally would have converted a hazard into free labor.



The shift paid off quickly. <a href="https://www.earth.com/news/solar-eclipse-may-have-changed-the-architecture-of-ancient-egypt-forever/" target="_blank" rel="noreferrer noopener">Stone sizes doubled</a> within a generation, and by the time Khufu’s Great Pyramid went up around 2550 B.C., individual blocks tipped the scales at more than 5 tons. 



Specialists calculate that hauling such loads up a mile‑long ramp would have required at least 4,000 men at any given moment. A water‑driven elevator could slash that headcount and keep quarry teams ahead of schedule.



<h2 class="wp-block-heading" id="h-all-of-that-work-for-what">All of that work for what?</h2>



Yet the Step Pyramid keeps one trick buried deep: its burial chamber is empty. No royal mummy, no treasure, no wall texts. 



Where is Pharaoh Djoser?



Some archaeologists have floated the idea that the hollow core acted less as a tomb and more as a pressure vessel, a technical heart that made the water lift possible. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser-complex_rock-cut-trench_workers_credit-PLOS-One_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/great-pyramids_Djoser-complex_rock-cut-trench_workers_credit-PLOS-One_1s.webp" alt="View of compartment-1 of the rock-cut deep trench (1943), 27m deep, 3m wide. a: View from the west; b: View from the east. The workers in the background provide a sense of the structure’s immense scale and technicity. Credit: PLOS One" class="wp-image-1968277"/></a><figcaption class="wp-element-caption">View of compartment-1 of the rock-cut deep trench (1943), 27m deep, 3m wide. a: View from the west; b: View from the east. The workers in the background provide a sense of the structure’s immense scale and technicity. Click image to enlarge. Credit: PLOS One</figcaption></figure>



The maze of tunnels, hinged stone doors, and drop‑block traps hint at mechanical ingenuity as sophisticated as any irrigation canal.



<h2 class="wp-block-heading" id="h-step-pyramid-and-modern-engineers">Step Pyramid and modern engineers</h2>



Today, Saqqara’s mastery of fluid dynamics may sound eerily familiar to civil engineers who harness controlled floods to build delta land in Louisiana or raise entire houses atop pneumatic lifts. 



If ancient builders truly manipulated water columns to float stones skyward, they pulled off a feat that resonates with modern efforts to work with natural forces rather than fight them.



The findings don't close every gap in the long saga of Egypt’s pyramids, but they do open an inviting corridor for future digs. 



Drill cores from the Dry Moat’s silt layers could confirm lake deposits; mineral stains on interior shafts might betray repeated wet cycles. 



Either way, the Step Pyramid is an engineering marvel that continues to teach us that even in antiquity, people were willing to tackle colossal challenges with solutions as fluid as the Nile itself.



The full study was published in the journal <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0306690" target="_blank" rel="noreferrer noopener">PLOS One</a>.



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Ancient high-tech machinery was used to build Egypt's pyramids, study claims

The Step Pyramid rises taller than a 20‑story building on...

Quantum computers promise faster solutions to certain problems, but proving those advantages has been tricky. A new study now points to a more concrete win in the area of approximate optimization.



Daniel Lidar from the University of Southern California (<a href="https://www.usc.edu" target="_blank" rel="noreferrer noopener">USC</a>) led the project. 



The team focused on showing how quantum hardware offers better scaling as problem sizes grow, especially when perfect solutions aren’t required.



<h2 class="wp-block-heading" id="h-quantum-annealing-breakthrough">Quantum annealing breakthrough</h2>



Scientists have long theorized that quantum <a href="https://docs.dwavequantum.com/en/latest/quantum_research/quantum_annealing_intro.html" target="_blank" rel="noreferrer noopener">annealing</a> could boost the search for near-optimal answers in difficult tasks. 



They define quantum annealing as a process where a specialized computer explores many possibilities at once by using qubits, the fundamental units of quantum <a href="https://www.earth.com/news/google-claims-commercial-quantum-computing-is-just-five-years-away/" target="_blank" rel="noreferrer noopener">information</a>.



This study aimed to verify whether such an approach truly beats top classical techniques, especially for solving bigger problems. 



It involved complex spin-based challenges, which are often used to measure the performance of advanced computing methods.



Many jobs in finance, logistics, and science do not demand a perfect outcome, but they do need good answers within a certain margin. 



Traditional supercomputers or large-scale servers often handle these tasks by relying on approximate algorithms.



Quantum teams suggest that if a specialized device can reach near-optimal solutions with less total time, it might save both money and computational resources.



That’s why the demonstration of a quantum setup that handles these approximate optimization tasks faster than classical methods caught many experts by surprise.



<h2 class="wp-block-heading" id="h-quantum-power-grows-with-spins">Quantum power grows with spins</h2>



One example involves <a href="https://arxiv.org/pdf/2302.04842" target="_blank" rel="noreferrer noopener">spin-glass systems</a>, which arise in physics when magnetic spins clash in ways that don’t stabilize easily. These setups represent real-world problems filled with conflicting interactions.



Researchers used a family of spin-glass instances to test whether quantum annealing could find workable solutions faster. They specifically examined problems arranged in two dimensions, which creates a highly entangled network of spins.



Although some early quantum <a href="https://www.earth.com/news/baffling-quantum-entanglement-statistics-puzzle-finally-solved-advanced-technologies/" target="_blank" rel="noreferrer noopener">demonstrations</a> struggled to maintain consistent improvements as the problem size grew, this work showed promising scaling gains. 



The researchers targeted situations where the solution energy rested within a given range of the best answer.



By focusing on near solutions, the device found answers more quickly and consistently. This led to a scaling advantage once tasks became large enough to highlight the difference.



<h2 class="wp-block-heading" id="h-fixing-errors-with-quantum-annealing">Fixing errors with quantum annealing</h2>



These results hinged on another technique called quantum annealing <a href="https://arxiv.org/abs/1507.02658" target="_blank" rel="noreferrer noopener">correction</a>, which is designed to reduce errors. 



Noise can disrupt the fragile quantum states in a machine, so this procedure stabilizes important information by grouping qubits in special configurations.



The study showed that this protective layer helped the quantum hardware maintain a clear edge over classical algorithms. The improvements remained even as the size of the spin-glass grid expanded into the thousands of qubits.



The team relied on a <a href="https://www.dwavequantum.com/solutions-and-products/systems/" target="_blank" rel="noreferrer noopener">D-Wave Advantage</a> quantum annealer housed at USC’s Information Sciences Institute. This machine is built with superconducting circuits that implement the quantum interactions needed for annealing.



Other quantum computers take a gate-model approach, but specialized annealing devices often focus on optimization alone, using carefully designed hardware links.



<h2 class="wp-block-heading" id="h-quantum-computers-may-help-business">Quantum computers may help business</h2>



Workers in supply chain management, portfolio design, and scheduling might someday prefer a quantum system if it consistently hits good-enough targets in less time. 



Many large corporations already use advanced algorithms, but classical methods can require a huge amount of <a href="https://www.earth.com/news/new-quantum-states-found-in-crystal-layers-could-boost-computing/" target="_blank" rel="noreferrer noopener">processing</a> as problems grow.



Finding a flexible, hardware-based improvement could reduce operational bottlenecks. Even a marginal speedup at scale can lead to significant financial or resource savings.



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



<a href="https://www.earth.com/news/how-quantum-revolution-will-impact-all-aspects-of-society/" target="_blank" rel="noreferrer noopener">Quantum computers</a> still face practical hurdles, including cost and hardware reliability. Researchers are optimistic, though, that future refinements will further close the gap between labs and factories. 



They note that the D-Wave machine already handles complex inputs and quickly explores millions of potential solutions. The bigger question is how soon it will slot neatly into existing operations.



The paper’s authors hope to explore tougher scenarios, including more densely connected challenges. They suggest that expanding the dimensionality of these tasks may uncover even greater computational boosts.



It also raises the possibility of testing other quantum error-correction schemes. Those might produce even steadier results for a wide array of optimization tasks.



<h2 class="wp-block-heading" id="h-expanding-quantum-s-reach">Expanding quantum’s reach</h2>



Beyond the specialized setting of spin-glass problems, scientists anticipate a growing menu of real-world uses for quantum annealing. 



Some industries need only approximate solutions to multi-variable tasks, making them good matches for this style of <a href="https://www.earth.com/news/microsoft-announces-giant-leap-in-quantum-computing-majorana-1/" target="_blank" rel="noreferrer noopener">computing</a>.



“The way quantum annealing works is by finding low-energy states in quantum systems, which correspond to optimal or near-optimal solutions to the problems being solved,” said Lidar. 



He explained that quantum annealers excel when the search space is huge but the requirement is to stay within a small error margin.&nbsp;



<h2 class="wp-block-heading" id="h-next-generation-optimization-programs">Next-generation optimization programs</h2>



While hype often surrounds new computing claims, the team behind this project stressed measured excitement. They believe the real significance lies in consistent scaling gains, not just momentary jumps on small problems.



Their data show that quantum annealing’s advantage grows as complexities increase. That runs counter to older critiques that quantum improvements disappear for sizable tasks.



As hardware improves, it may handle more variables without losing accuracy. That opens doors to next-generation optimization programs.



Many see near-optimal solutions as a huge resource saver. They argue that the quest for absolute perfection can be too expensive or time-consuming in many fields.



<h2 class="wp-block-heading" id="h-industry-eyes-quantum-annealing-tools">Industry eyes quantum annealing tools</h2>



Several leading firms keep an eye on quantum annealing developments. For them, even a moderate performance gain could boost daily operations.



Success in one niche might transfer to broader industrial and academic use, especially if the cost of <a href="https://www.earth.com/news/google-claims-commercial-quantum-computing-is-just-five-years-away/" target="_blank" rel="noreferrer noopener">quantum machines</a> drops. Meanwhile, classical algorithms continue to improve, so the race won’t end soon.



Merging ideas from academia, government labs, and industry has sparked new forms of experimentation. The synergy in this study united specialized hardware with advanced theory.



Now that quantum annealing has shown a scaling advantage, more investigators will likely test it on other tough cases. Each new demonstration sheds light on how quantum logic can tackle deeply entangled puzzles.



The study is published in the journal <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.134.160601" target="_blank" rel="noreferrer noopener">Physical Review Letters</a>.



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Quantum computer defeats a supercomputer in a very crucial task for the first time

Quantum computers promise faster solutions to certain problems, but proving...

The icy fringe of our planet is sprouting new growth. Fast warming in the Arctic - now running at roughly four times the global average - is reshaping tundra landscapes and affecting shrubs and meadows that have looked the same since the last ice age.



A vast forty‑year experiment, spread across more than 2,000 research plots, shows that almost every facet of Arctic plant life is in flux. Scientists say the changes are an early sign that the wider <a href="https://www.earth.com/news/arctic-fjords-show-signs-of-struggle-in-a-warming-world/" target="_blank" rel="noreferrer noopener">Arctic</a> system, from wildlife to water supplies, will also shift.



<h2 class="wp-block-heading" id="h-summers-lengthen-arctic-shrubs-thrive">Summers lengthen, Arctic shrubs thrive</h2>



Researchers have spent decades tracking the low carpets of <a href="https://www.earth.com/news/planting-moss-helps-restore-land-damaged-by-oil-and-gas-exploration/" target="_blank" rel="noreferrer noopener">mosses</a>, grasses, and dwarf shrubs that dominate mountains and polar plains. They found that almost six in ten plots have already lost some long‑standing species or gained new arrivals.



No single winner or loser stands out everywhere. Local soil moisture, shelter from wind, and the number of frost‑free days all tip the balance in different directions. Yet the pattern is unmistakable: taller, woodier <a href="https://www.earth.com/news/shrubs-play-a-dual-role-in-forest-recovery-following-wildfires/" target="_blank" rel="noreferrer noopener">shrubs</a> thrive when summers lengthen, shading out species that hug the ground.



“Changes in vegetation are an early warning signal that the entire ecosystem will change, with consequential effects on wildlife, humanity, and Earth's natural ability to store <a href="https://www.earth.com/news/carbon-storage-mystery-emerges-in-the-southern-ocean/" target="_blank" rel="noreferrer noopener">carbon</a>,” said co-author Anne Bjorkman, a researcher in plant ecology at the <a href="https://www.gu.se/en" target="_blank" rel="noreferrer noopener">University of Gothenburg</a>.



<h2 class="wp-block-heading" id="h-shrubs-stretch-higher-meadows-shrink"><a></a>Shrubs stretch higher, meadows shrink</h2>



Investigators see the biggest gains among evergreen stragglers such as lingonberry and crowberry, along with fast‑growing willow bushes that keep their leaves only for the warm season. These plants once clung to the Arctic <a href="https://www.earth.com/news/warming-climate-turns-tundra-from-carbon-sink-to-source/" target="_blank" rel="noreferrer noopener">tundra</a> only where snow melted early.



Now they push onto windswept ridges because snow lies for fewer days each year. Where they thicken, their leaves intercept sunlight that formerly bounced off pale lichens or was absorbed by low moss mats. Tall stems also sling snow into drifts that insulate soils, letting roots stay active later in autumn.



“The change in what grows on a site is extensive, with new species appearing and/or existing species disappearing on almost 60% of the experimental plots. There are many factors that determine how plant life changes at a particular Arctic site, such as how wet the soil is, or how windy it is. This affects the microclimate that plants experience,” said Robert Bjork, a researcher at the University of Gothenburg.



“In general, we see that shrubs benefit from a longer growing season, they simply steal the sunlight from species with a low growth habit.”



<h2 class="wp-block-heading" id="h-impacts-of-arctic-shrubs">Impacts of Arctic shrubs </h2>



On open ridges where dwarf birch and willow take hold, <a href="https://www.earth.com/news/how-plant-diversity-can-help-combat-climate-change/" target="_blank" rel="noreferrer noopener">plant diversity</a> often drops. The low‑lying herbs and sedges that fuel summer pollinators can no longer compete.



South of the tree line, mountain birch saplings work upslope, nibbling away at alpine meadows soaked in brief bursts of meltwater. Once those meadows vanish, the displaced flora has no colder niche to retreat to.



“But where the shrubs take over, biodiversity will decrease, and then the question is where the outcompeted species will go. There are no colder regions than the Arctic, and some species may disappear completely from large areas,” Bjorkman said.



Shrub lines affect more than flowers. Dark leaves absorb solar energy, warming surface layers and melting permafrost ice that holds ancient carbon. 



When that carbon leaks as methane or carbon dioxide, regional warming accelerates. Taller plants also trap snow that would otherwise reflect sunlight and delay spring thaw, another feedback that adds heat.



<h2 class="wp-block-heading" id="h-ripples-through-animals-people-and-water"><a></a>Ripples through animals, people, and water</h2>



“Changes in vegetation obviously also affect <a href="https://www.earth.com/news/forest-biodiversity-benefits-from-large-herbivores-like-elephants-and-moose/" target="_blank" rel="noreferrer noopener">herbivorous animals</a>. Reindeer husbandry cannot have the same grazing areas in the valleys as today, perhaps they can find new ones on the bare mountains,” Bjork explained.



“Then tourism will be affected when mountain birches and shrubs take over on the mountains and the alpine meadows with beautiful wildflowers disappear. And it will be difficult to get hold of drinkable water when the glaciers and the late snowfields melt away.”



Reindeer and caribou herds already follow thinner green waves in sprinting summers. The loss of valley forage may force animals higher, straining age‑old herding routes. 



Visitors who come for wide carpets of summer color may find thickets instead. Local communities could face water stress as shrinking glaciers feed fewer melt streams during late summer.



<h2 class="wp-block-heading" id="h-radical-changes-ahead">Radical changes ahead</h2>



Scientists at the Latnjajaure field camp near Abisko, Sweden, witness these shifts in real time. Birches creep onto formerly barren slopes. 



Moss mats turn patchy under rising shrubs. Streams surge earlier in spring and dwindle sooner in August. Yet no one can plot the exact timetable for the next leap.



“We are in the midst of climate change and will reach certain thresholds where the flora will change radically, but we don't know when it will happen. Or how it will happen,”  Bjorkman warned.



<h2 class="wp-block-heading" id="h-the-future-of-arctic-shrubs">The future of Arctic shrubs</h2>



More data will refine forecasts, but the direction is set. Open alpine meadows will contract as shrub lands will expand. Carbon and energy flows between ground and sky will alter, pushing feedback loops that amplify <a href="https://www.earth.com/news/frequent-heatwaves-have-become-the-norm-in-the-arctic-ocean/" target="_blank" rel="noreferrer noopener">Arctic heat</a>.



For conservationists, the lesson is urgent: protect refuges where cold‑loving plants might survive and plan for landscapes that will not stay as they were such as the Arctic. For everyone else, the message is simpler.



The quiet creep of shrubs in the far north is one more sign that climate change is coming. It is here, and it is rewriting the map from the top downward.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-025-08946-8" target="_blank" rel="noreferrer noopener">Nature</a>.



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Arctic plant alert: Rising shrubs and vanishing meadows

The icy fringe of our planet is sprouting new growth....

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

[sendtonews key="0ynNMYkMKa-2340414-12187" type="single"] Today’s Video of the Day from the...

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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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

[sendtonews key="LvS8v8bp9z-2564889-12187" type="single"] Today's Video of the Day from the...

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Today’s Video of the Day from the <a href="https://www.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



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Kainji Lake in north central Nigeria

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