Today's Image of the Day from NASA Earth Observatory features the Corbassière glacier, a high-altitude glacier in Switzerland. The glacier originates on the northern slope of the Grand Combin, which is one of the highest peaks in the Pennine Alps.



Collectively, the <a href="https://www.earth.com/news/alpine-glaciers-will-lose-half-of-their-volume-by-2050/" target="_blank" rel="noreferrer noopener">alpine glaciers</a> of Switzerland have lost more than half of their volume since the 1930s.



<h2 class="wp-block-heading" id="h-natural-archives-of-past-climate">Natural archives of past climate </h2>



"Glaciers are natural archives of past climate. In their frozen layers lies evidence of Earth’s changing temperature and atmospheric composition. But as the climate warms, some of the longest records of our changing planet are melting away," said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"In just over two decades, Corbassière has shrunk in area and surface mass. The glacier was darker in 2023 due to lack of snow, and the glacier’s tongue had retreated."



<h2 class="wp-block-heading" id="h-ice-cores-from-the-corbassiere-glacier">Ice cores from the Corbassière glacier</h2>



To reconstruct past concentrations of atmospheric <a href="https://www.earth.com/news/how-do-aerosols-impact-the-climate/" target="_blank" rel="noreferrer noopener">aerosols</a>, a team of scientists analyzed ice cores that were collected from the Corbassière glacier in 2018 and 2020.&nbsp;



Aerosols are tiny airborne particles that are deposited in the ice. "Such information from glaciers around the world can provide clues about past environmental conditions thousands of years ago," noted NASA.



"Ice cores contain ammonium, nitrate, and sulfate ions - signatures of aerosols lacing the snow that’s deposited on glaciers year after year. Ion concentrations are lower in winter than in summer because less polluted air can rise from the valley when the air is cold."



When the researchers analyzed the ice core from 2018, they found seasonal fluctuations in the amount of ion deposits - which is what they expected to find.&nbsp;



"But when we went to core the glacier in 2020, we noticed melting on the surface right away,” said Margit Schwikowski, an environmental chemist at <a href="https://www.psi.ch/en" target="_blank" rel="noreferrer noopener">Paul Scherrer Institute</a> in Switzerland.&nbsp;



<h2 class="wp-block-heading" id="h-rapid-surface-melting-on-corbassiere-glacier">Rapid surface melting on Corbassière glacier</h2>



The experts determined that melting on the glacier's surface likely penetrated the glacier layers below and carried away the aerosol ions. 



"This melting rendered the core unusable in the team’s research, and other attempts to core the glacier had the same result. The valuable information stored in the ice was destroyed," explained NASA.



Schwikowski has joined a team of other experts in an effort to preserve cores from the last remaining glaciers. Led by the <a href="https://www.ice-memory.org/" target="_blank" rel="noreferrer noopener">Ice Memory Foundation</a>, the goal of the project is to obtain ice cores from 20 endangered glaciers around the world in 20 years and collect them in a global <a href="https://www.earth.com/news/antarcticas-ice-has-a-history-of-rapid-and-unexpected-changes/" target="_blank" rel="noreferrer noopener">climate archive</a>.



“Glaciers are retreating worldwide, and we may find similar issues at other sites,” said Schwikowski. She added that even at the highest altitudes in the Alps, "glaciers are on the verge of becoming unsuitable as natural paleo-archives."



<h2 class="wp-block-heading" id="h-features-of-the-corbassiere-glacier">Features of the Corbassière Glacier</h2>



The Corbassière Glacier is a captivating natural feature located in the Swiss Alps, part of the canton of Valais. 



The glacier stretches over approximately 9 kilometers, making it one of the significant glaciers in the region. It originates from the Grand Combin, an imposing mountain massif that reaches heights of over 4,300 meters, contributing greatly to the glacier's nourishment through snow and ice accumulation.



A distinct feature of the Corbassière Glacier is its accessibility and the dramatic scenery it offers, which attracts many hikers and nature enthusiasts. 



One of the most notable attractions near the <a href="https://www.earth.com/news/doomsday-glacier-seems-to-have-lost-its-ability-to-recover/" target="_blank" rel="noreferrer noopener">glacier</a> is the Corbassière footbridge, a 210-meter long suspension bridge that provides stunning views of the glacier and the surrounding peaks. 



This bridge not only enhances the experience for visitors but also serves as a crucial observation point for scientists studying glacier dynamics and the effects of climate change.



<h2 class="wp-block-heading">The Swiss Alps&nbsp;</h2>



The Swiss <a href="https://www.earth.com/news/snow-cover-in-the-alps-could-soon-be-cut-in-half/" target="_blank" rel="noreferrer noopener">Alps</a> are a majestic and expansive mountain range that stretches across the southern part of Switzerland, forming a part of the greater Alpine region that spreads across several countries in Europe.&nbsp;



Renowned for their stunning beauty and formidable peaks, the Swiss Alps are not just a geographical landmark but also a cultural symbol of Switzerland, epitomizing its identity as a nation of scenic landscapes and outdoor adventure.



The region is famous for its dramatic scenery, including towering mountains, pristine lakes, and picturesque valleys. Among these peaks are some of the highest in Europe, such as the Dufourspitze, part of the Monte Rosa massif, which is the highest point in Switzerland. 



The Matterhorn, perhaps the most iconic of all Swiss mountains, is celebrated for its unique, pyramid-like shape and is a magnet for climbers and tourists alike.



Image Credit: NASA Earth Observatory



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The Corbassière glacier in the Swiss Alps

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

Today's Image of the Day from NASA Earth Observatory features thick haze over Thailand during the fire season. The photograph was captured on March 16, 2024 by the Visible Infrared Imaging Radiometer Suite (VIIRS) on the Suomi NPP satellite.



<h2 class="wp-block-heading" id="h-waves-of-smoke-and-haze">Waves of smoke and haze</h2>



"Each year in January and February, satellites begin to detect waves of smoke and fire in Southeast Asia, particularly in highland forests in Cambodia, Laos, Myanmar, and Thailand. <a href="https://www.earth.com/image/intense-fire-season-in-mexico-is-part-of-a-worldwide-trend/" target="_blank" rel="noreferrer noopener">Fire activity</a> continues to increase through March and April, reaches a peak during the height of the dry season, and then fades in May with the start of the rainy season," noted <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"Individual fires are usually small and short-lived. But they are often so numerous that smoke, along with air pollution from rural and urban areas, mixes to produce thick layers of haze that blanket the landscape." 



According to NASA, the haze contains mixtures of small airborne particles called aerosols and gaseous pollutants such as nitrogen dioxide, sulfur dioxide, carbon monoxide, and ozone that degrade air quality.



<h2 class="wp-block-heading" id="h-haze-in-thailand-nbsp">Haze in Thailand&nbsp;</h2>



An international field campaign - the Airborne and Satellite Investigation of Asian Air Quality (ASIA-AQ) - was launched to investigate the haze in Thailand.



"During the last two weeks of March 2024, NASA’s DC-8 and Gulfstream III aircraft flew several flights over Chiang Mai, Bangkok, and rural areas surrounding the cities to sample air quality with several sensors. At the same time, satellites observed the haze from above," said NASA.



James Crawford, ASIA-AQ’s principal investigator, said the team is collaborating closely with national and local government entities in Thailand.



“The goal is to take as many simultaneous measurements of pollutants as possible from the ground, air, and space,” said Crawford. The team will use the data to gain a better understanding of how the haze forms, evolves chemically over time, and moves throughout the region.



<h2 class="wp-block-heading" id="h-haze-and-public-health-in-thailand">Haze and public health in Thailand </h2>



According to media reports, nearly 200,000 people have been hospitalized this year due to air quality in the region, with over 1.3 million people falling ill since January.&nbsp;



<h3 class="wp-block-heading" id="h-causes-of-the-haze">Causes of the haze</h3>



The root causes of the haze include agricultural burning, particularly of corn fields, as part of slash-and-burn practices to prepare land for the next planting cycle. This is exacerbated by the dry season when there's little rain to wash the pollutants away. 



The situation is worsened by industrial emissions and vehicle fumes, particularly in urban areas like Bangkok​.



<h3 class="wp-block-heading" id="h-sustainable-solutions-are-needed">Sustainable solutions are needed</h3>



Efforts to address the crisis have been complex, involving local and transboundary issues. Much of the agricultural burning occurs not only within Thailand but also in neighboring countries like Myanmar and Laos, contributing to the transboundary nature of the haze. 



Activists and local communities have called for sustainable solutions that do not exacerbate the poverty of smallholder farmers, emphasizing the need for affordable and realistic alternatives to burning​.



<h3 class="wp-block-heading" id="h-mitigation-measures-nbsp">Mitigation measures&nbsp;</h3>



The Thai government has implemented a no-burning rule until the end of April to combat wildfires and haze, but enforcement and effectiveness remain challenges​​. 



Some measures taken to mitigate the immediate effects of pollution in urban areas include spraying water and seeding clouds to encourage rain, although these have had limited success​​.



This ongoing environmental crisis has sparked widespread concern among citizens, who are increasingly using public interest litigation to hold companies and the government accountable for environmental commitments. 



With recent political changes, there is hope that the new administration will take more decisive action against the haze, possibly through more stringent regulations and international cooperation​​.



<h2 class="wp-block-heading" id="h-health-impacts-of-haze">Health impacts of haze</h2>



Haze poses several health hazards for those exposed to it, particularly when it contains fine particulate matter (PM2.5). Here are some of the main health risks associated with exposure to haze:



<h3 class="wp-block-heading" id="h-respiratory-problems">Respiratory problems</h3>



Haze can aggravate conditions such as asthma, bronchitis, and other chronic obstructive pulmonary diseases (COPD). The fine <a href="https://www.earth.com/news/heatwaves-and-air-pollution-may-double-fatal-heart-attack-risk/">particles</a> can penetrate deep into the lungs, causing inflammation and reducing lung function.



<h3 class="wp-block-heading" id="h-cardiovascular-issues-and-haze">Cardiovascular issues and haze</h3>



Exposure to fine particulate matter can also affect the cardiovascular system, leading to increased risk of heart attacks, strokes, and high blood pressure. Particles can affect blood vessel function and promote the formation of blood clots.



<h3 class="wp-block-heading" id="h-eye-irritation">Eye irritation</h3>



Haze can cause eye irritation, leading to conditions such as conjunctivitis (pink eye) or exacerbated symptoms in people with existing eye conditions.



<h3 class="wp-block-heading" id="h-skin-problems">Skin problems</h3>



For some people, exposure to <a href="https://www.earth.com/news/air-pollution-will-increase-dramatically-in-a-hotter-climate/">polluted air</a> can cause skin irritation or exacerbate skin conditions like eczema or psoriasis.



<h3 class="wp-block-heading" id="h-reduced-immune-function">Reduced immune function</h3>



There is evidence to suggest that prolonged exposure to polluted air can weaken the immune system, making individuals more susceptible to infections.



<h3 class="wp-block-heading" id="h-impact-on-mental-health">Impact on mental health</h3>



There are growing concerns about the impact of air pollution on <a href="https://www.earth.com/news/air-pollution-linked-to-multiple-chronic-health-conditions/">mental health</a>, with studies suggesting a link between exposure to polluted air and an increased risk of depression and anxiety.



<h3 class="wp-block-heading" id="h-pregnant-women-and-children">Pregnant women and children</h3>



Pregnant women, children, and the elderly are particularly vulnerable to the effects of haze. There may be increased risks of preterm birth and low birth weight in babies, and children may experience delayed development and reduced lung function.



The health impacts of haze can be mitigated by staying indoors on days when <a href="https://www.earth.com/news/twenty-years-of-air-quality-improvement-erased-by-wildfires/" target="_blank" rel="noreferrer noopener">air quality</a> is particularly poor, using air purifiers, wearing masks designed to filter out fine particles, and following local health advisories.



Image Credit: NASA Earth Observatory



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<h3 class="wp-block-heading" id="h-nbsp">&nbsp;</h3>

Haze pollution is an environmental crisis in Thailand

Today's Image of the Day from NASA Webb Images features an extraordinary view of Uranus, the seventh planet from the sun in our solar system.&nbsp;



The photo reveals the rings, moons, and extreme seasons of the ice giant Uranus in unprecedented detail.&nbsp;



<h2 class="wp-block-heading" id="h-dynamic-north-polar-cap-nbsp">Dynamic north polar cap&nbsp;</h2>



“The Webb image exquisitely captures Uranus’s seasonal north polar cap, including the bright, white, inner cap and the dark lane in the bottom of the polar cap,” noted NASA.



Unlike Earth, where polar ice caps are formed by the freezing of water, Uranus's polar caps are thought to be primarily composed of a dense concentration of haze in the atmosphere.&nbsp;



The polar cap's haze is likely composed of methane particles. Methane in Uranus's atmosphere condenses into ice particles, which then create a thick haze that scatters sunlight, giving the polar cap its distinct bright appearance in visible and infrared light.



The polar cap is dynamic and changes over time. It becomes more prominent during the summer season of each pole. 



As Uranus moves along its orbit, the cap's appearance transforms, with the haze becoming thicker and brighter when the pole is in continuous sunlight.



<h2 class="wp-block-heading" id="h-the-zeta-ring-nbsp">The Zeta ring&nbsp;</h2>



The inner and outer rings of Uranus are visible in the image, including Zeta - the innermost ring which is the faintest and most difficult to observe.



The <a href="https://www.earth.com/news/stunning-photo-of-uranus-and-its-rings-and-moons-captured-by-the-webb-telescope/" target="_blank" rel="noreferrer noopener">rings of Uranus</a> are primarily composed of narrow bands of particles, likely made of water ice mixed with a dark material. These rings are distinct from those of Saturn in that they are much darker and narrower.



The faintness and characteristics of the Zeta ring make it a subject of interest in studies related to the dynamics and composition of planetary ring systems.



<h2 class="wp-block-heading" id="h-moons-of-uranus-nbsp">Moons of Uranus&nbsp;</h2>



The <a href="https://science.nasa.gov/mission/webb/multimedia/images/" target="_blank" rel="noreferrer noopener">Webb</a> photo also features nine of the planet’s <a href="https://www.earth.com/news/nasa-four-uranus-moons-may-have-oceans-that-are-miles-deep/" target="_blank" rel="noreferrer noopener">moons</a>, which appear as blue dots surrounding the rings.&nbsp;



“Clockwise starting at 2 o’clock, they are: Rosalind, Puck, Belinda, Desdemona, Cressida, Bianca, Portia, Juliet, and Perdita. The orbits of these moons share the 98-degree tilt of their parent planet relative to the plane of the solar system,” noted NASA.



Uranus has 27 known moons, and they are divided into three main groups based on their orbits: the inner moons, the major moons, and the irregular moons.



The <a href="https://www.earth.com/news/uranus-moon-ariel-may-have-a-hidden-ocean/" target="_blank" rel="noreferrer noopener">moons</a> of Uranus are unique because they are named after characters from the works of William Shakespeare and Alexander Pope, rather than being named after figures from classical mythology, as is common for the moons of other planets.



<h2 class="wp-block-heading" id="h-the-ice-giant-uranus-nbsp">The ice giant Uranus&nbsp;</h2>



Uranus is classified as an "ice giant" because, unlike the gas giants Jupiter and Saturn, which are primarily composed of hydrogen and helium, Uranus has a significant proportion of "ices" in its composition.&nbsp;



In astronomical terms, ices refer to volatile substances like water, ammonia, and methane, which exist in solid or liquid forms at the low temperatures found in the outer solar system.



Uranus has a thick atmosphere of hydrogen and helium, but beneath that, it contains a large, dense mantle composed of these ices, along with rock and other heavier elements.&nbsp;



The term <a href="https://www.earth.com/news/diamond-rain-may-be-common-on-giant-icy-planets/" target="_blank" rel="noreferrer noopener">ice giant</a> differentiates Uranus (and Neptune, the other ice giant) from the larger gas giants, emphasizing the different chemical compositions and internal structures of these planets.



<h2 class="wp-block-heading" id="h-climate-of-uranus-nbsp">Climate of Uranus&nbsp;</h2>



Uranus has a unique and extreme climate, largely influenced by its unusual tilt, which causes the planet to rotate almost on its side. This tilt leads to extreme seasonal variations, with each pole experiencing 42 years of continuous sunlight followed by 42 years of darkness.&nbsp;



Even though it is closer to the sun than Neptune, Uranus is the coldest planet in the solar system, with temperatures plunging to as low as -224°C (-371°F). The reason for this is not fully understood, but it might be due to an internal heat distribution anomaly.



Despite these frigid conditions, Uranus experiences intense weather patterns, including powerful storms and winds that can reach speeds of up to 900 kilometers per hour. These winds blow in the same direction as the planet’s rotation and are some of the fastest in the solar system.



Storms on Uranus are driven by its internal heat and the interaction of its <a href="https://www.earth.com/news/uranus-is-more-gassy-less-icy-than-we-ever-imagined/" target="_blank" rel="noreferrer noopener">atmospheric gases</a>. Observations have shown that these storms can be quite large, sometimes comparable in size to the Earth, and can last for several years.&nbsp;



The planet’s extreme axial tilt also means that the storms and weather patterns are highly variable, depending on the season. During equinoxes, when the Sun is directly over the equator, Uranus exhibits more storm activity compared to when the poles are pointed towards the Sun or away from it.



<h2 class="wp-block-heading" id="h-observations-of-uranus">Observations of Uranus</h2>



“One day on Uranus is about 17 hours, so the planet’s rotation is relatively quick. This makes it supremely difficult for observatories with a sharp eye like Webb to capture one simple image of the entire planet - storms and other atmospheric features, and the planet’s moons, move visibly within minutes,” explained NASA.



“This image combines several longer and shorter exposures of this dynamic system to correct for those slight changes throughout the observing time.”



The first recorded observations of Uranus were made by John Flamsteed on December 13, 1690. However, Flamsteed mistakenly identified the planet as a star, which he named “34 Tauri."&nbsp;



It wasn't until March 13, 1781, that Uranus was officially identified as a planet by William Herschel. He initially thought he had discovered a comet, but further observations and calculations by other astronomers confirmed that it was a new planet, making Uranus the first planet discovered in modern history with the aid of a telescope.



Image Credit: NASA, ESA, CSA, STScI



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The ice giant Uranus in stunning detail

Today's Image of the Day from NASA Webb Images features...

Today's Image of the Day from NASA Earth Observatory features a strong extratropical cyclone, which struck the Pacific Northwest on November 19, 2024.



“The storm knocked over trees and left nearly 600,000 people without power in Washington state on November 20, according to news reports,” noted <a href="https://search.app?link=https%3A%2F%2Fearthobservatory.nasa.gov%2Fimages%2F153605%2Fextratropical-cyclone-whips-over-the-pacific-northwest&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">NASA</a>. “This image shows the storm system at 1:50 p.m. Pacific Time on November 19.” 



According to NASA, mature extratropical cyclones like this often feature comma-shaped cloud patterns that are the product of ‘conveyor belt’ circulation. “Heavy precipitation is often present near the low-pressure head of the comma.”



<h2 class="wp-block-heading" id="h-impacts-of-the-extratropical-cyclone-nbsp">Impacts of the extratropical cyclone&nbsp;</h2>



The “bomb cyclone” brought <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fhow-much-does-climate-change-influence-extreme-weather-events%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">severe weather</a>, including strong winds exceeding 70 mph, heavy rainfall, and snow in higher elevations. These conditions led to significant disruptions, including downed trees and hazardous travel conditions.



In urban and rural areas, damage to infrastructure and properties was substantial, with emergency responders and utility crews working around the clock to restore services.&nbsp;



Additionally, mountain passes faced dangerous blizzard conditions, with up to 20 inches of snow accumulating in some areas, severely affecting travel.



<h2 class="wp-block-heading" id="h-rapid-pace-of-acceleration">Rapid pace of acceleration</h2>



Chris Dolce is a meteorologist at The Weather Channel. He noted that on the evening of November 19, the storm’s central pressure dropped to levels on par with a storm in October 2021, which saw the lowest pressure in about 50 years of records for that region.



“The pace of the storm’s intensification was more than double the criteria for bombogenesis - a popular term that describes a midlatitude cyclone that rapidly intensifies into a ‘bomb cyclone,’” said NASA.



The rapidly dropping atmospheric pressure at the center of the <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fcoastal-hurricanes-are-intensifying-faster-due-to-climate-change%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">storm</a> caused winds to intensify quickly. According to the National Weather Service in Seattle, wind gusts reached up to 77 miles per hour in the mountains southeast of the city.



“The cyclone kicked off a long-duration atmospheric river that forecasters expect will park over Northern California and southern Oregon through November 22. The National Weather Service estimates that these areas could see rainfall totals of 12 to 16 inches over the duration of the storm,” noted NASA.



<h2 class="wp-block-heading" id="h-what-is-an-extratropical-cyclone">What is an extratropical cyclone?</h2>



An extratropical cyclone is a large-scale weather system that forms outside the tropics, typically between 30° and 60° latitude, and is associated with areas of low pressure.&nbsp;



<h3 class="wp-block-heading" id="h-energy-source">Energy source</h3>



These cyclones obtain their energy from the contrast in temperature between air masses, such as cold polar air and warm subtropical air. This contrast creates instability and drives atmospheric circulation.



<h3 class="wp-block-heading" id="h-development-of-extratropical-cyclones-nbsp">Development of extratropical cyclones&nbsp;</h3>



Extratropical cyclones usually have well-defined warm and cold fronts. They often develop along the polar front, where cold and warm air masses meet.



A common area for their development is the mid-latitudes, particularly in regions like the North Atlantic and North Pacific.



<h3 class="wp-block-heading" id="h-weather-conditions">Weather conditions</h3>



Extratropical cyclones can bring a variety of <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fhuman-activity-is-rapidly-changing-weather-in-north-america%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">weather conditions</a>, including heavy rain, snow, strong winds, and severe storms. They are responsible for much of the day-to-day weather in mid-latitude regions.



<h3 class="wp-block-heading" id="h-tropical-vs-extratropical-cyclones-nbsp">Tropical vs. extratropical cyclones&nbsp;</h3>



While <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Ffast-moving-tropical-cyclones-are-becoming-more-powerful%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">tropical cyclones</a> derive energy from warm ocean waters and have a warm core, extratropical cyclones gain energy from temperature contrasts and have a cold core.



Tropical cyclones typically lack fronts, whereas extratropical cyclones are defined by them.



These systems are essential in distributing heat and energy across the planet, playing a critical role in the Earth's climate system.



<h2 class="wp-block-heading" id="h-caught-off-guard-by-the-weather">Caught off guard by the weather</h2>



The bomb cyclone in the Pacific Northwest highlights the importance of <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Fnew-era-in-forecasting-ai-will-improve-extreme-weather-warnings%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">preparedness</a>, as residents were urged to secure loose outdoor items, stock emergency supplies, and avoid unnecessary travel.



The fire department in Bellevue, east of Seattle, posted a Severe Weather Safety alert on Facebook: “It’s severe out there. Trees are coming down all over the city, with multiple falling onto homes. If you are able, head to the lowest floor you can and stay away from windows. Do not go outside if you can avoid it.”



The image was captured by the VIIRS (Visible Infrared Imaging Radiometer Suite) on NOAA’s JPSS-1 (Joint Polar Satellite System-1).



Image Credit: NASA Earth Observatory



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Bomb cyclone rapidly intensified in the Pacific Northwest

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 little-observed southern constellation Reticulum. The image was captured by the James Webb Space Telescope.&nbsp;



<h2 class="wp-block-heading" id="h-fuel-for-star-formation">Fuel for star formation </h2>



"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 ionised 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 studying stellar evolution and the lifecycle of stars.



The structure of NGC 1559 includes well-defined spiral arms that are rich in 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>.



The galaxy’s central bar is believed to play a role in driving gas towards the core, fueling both the star formation and the activity around its nucleus.



<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 NGC 1559 is a loner in outer space

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

Today's Image of the Day from the European Space Agency features NGC 1792, a spiral galaxy located in the constellation Columba, about 43 million light-years away from Earth.&nbsp;



This galaxy, discovered by British astronomer James Dunlop in 1826, is part of the larger NGC 1808 group of galaxies.&nbsp;



<h2 class="wp-block-heading" id="h-intimate-view-of-ngc-1792">Intimate view of NGC 1792</h2>



“An orange glow radiates from the center of NGC 1792, the heart of this stellar forge. Captured by the NASA/ESA Hubble Space Telescope, this intimate view of NGC 1792 gives us some insight into this galactic powerhouse,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The vast swathes of tell-tale blue seen throughout the galaxy indicate areas that are full of young, hot stars, and it is in the shades of orange, seen nearer the center, that the older, cooler stars reside.”



<h2 class="wp-block-heading" id="h-vigorous-star-formation-nbsp">Vigorous star formation&nbsp;</h2>



NGC 1792 is notable for its vigorous star formation, classifying it as a starburst galaxy. This high rate of star formation is thought to be triggered by gravitational interactions with neighboring galaxies, though the exact cause is still under study.



“Nestled in the constellation of Columba (The Dove), NGC 1792 is both a spiral galaxy, and a starburst galaxy,” said ESA. “Within starburst galaxies, stars are forming at comparatively exorbitant rates. The rate of star formation can be more than 10 times faster in a starburst galaxy than in the Milky Way.”



<h2 class="wp-block-heading" id="h-fierce-bursts-of-star-formation">Fierce bursts of star formation</h2>



ESA noted that when galaxies have a large reservoir of gas, like NGC 1792, these short-lived starburst phases can be sparked by galactic events such as mergers and tidal interactions.&nbsp;



“One might think that these starburst galaxies would easily consume all of their gas in a large forming event. However, supernova explosions and intense stellar winds produced in these powerful starbursts can inject energy into the gas and disperse it.”&nbsp;



“This halts the star formation before it can completely deplete the galaxy of all its fuel. Scientists are actively working to understand this complex interplay between the dynamics that drive and quench these fierce bursts of star formation.”



Due to its distance and brightness, NGC 1792 can be observed with medium-sized telescopes under favorable conditions.



<h2 class="wp-block-heading" id="h-galaxy-evolution">Galaxy evolution</h2>



Galaxy evolution refers to the process by which galaxies form and change over time. It begins in the early universe, shortly after the <a href="https://www.earth.com/news/new-observations-disprove-big-bang-theory-universe-began-tired-light-theory/" target="_blank" rel="noreferrer noopener">Big Bang</a>, when small density fluctuations in the primordial gas led to the collapse of matter into the first galaxies. 



<h3 class="wp-block-heading" id="h-galaxy-mergers">Galaxy mergers</h3>



These early galaxies were small and irregular, composed mostly of gas and dark matter. Over billions of years, galaxies grew larger by merging with one another and by accreting gas from the surrounding space.&nbsp;



These interactions often triggered bursts of star formation, and collisions between galaxies sometimes led to the creation of new, more massive galaxies.



<h3 class="wp-block-heading" id="h-structural-changes">Structural changes</h3>



As galaxies evolve, their morphology - their shape and structure - can change. Early galaxies were often irregular or disk-shaped, but over time, many galaxies formed into the elliptical or spiral shapes we see today.&nbsp;



<h3 class="wp-block-heading" id="h-star-formation">Star formation</h3>



Star formation is a key driver of galaxy evolution, but it gradually slows down as galaxies age. 



The gas that fuels <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> can be used up, or it can be heated and pushed out of galaxies by supernovae or black holes, reducing the galaxy's ability to form new stars.



<h3 class="wp-block-heading" id="h-galaxy-environment-nbsp">Galaxy environment&nbsp;</h3>



The environment in which a galaxy resides also plays a role in its evolution. Galaxies in dense clusters are more likely to interact with their neighbors, which can alter their shape or trigger bursts of star formation.&nbsp;



In contrast, galaxies in more isolated regions of space evolve more slowly and without as many dramatic interactions.



<h3 class="wp-block-heading" id="h-dark-matter">Dark matter</h3>



Dark matter also plays a crucial role in galaxy evolution. It provides the gravitational framework that holds galaxies together and influences their interactions with one another.&nbsp;



Supermassive <a href="https://www.earth.com/search-results/?search=Galaxies%20merge&amp;start=0" target="_blank" rel="noreferrer noopener">black holes</a>, found at the centers of most large galaxies, can also affect their evolution by releasing energy that impacts star formation and the movement of gas within the galaxy.



Overall, galaxy evolution is a complex and ongoing process driven by interactions between stars, gas, <a href="https://www.earth.com/news/study-dark-matter-does-not-exist-and-the-universe-is-27-billion-years-old/" target="_blank" rel="noreferrer noopener">dark matter</a>, and black holes, and shaped by both internal processes and external influences.



Image Credit: ESA/Hubble &amp; NASA, J. Lee



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NGC 1792: A galactic powerhouse 

Burn Scars and Late-Season Fires in Kazakhstan. Therefore This true-color image from the Moderate Resolution Imaging Spectroradiometer (MODIS) on the <a href="https://en.wikipedia.org/wiki/Aqua_(satellite)">Aqua satellite</a> shows several large fires burning. And in the steppes of <a href="http://www.earth.com/image/kazakhstans-alakol-lake/">Kazakhstan</a> (bottom and center) as well as smaller, scattered agricultural fires (top). All active fires are marked with red dots (or outlines in the high-resolution images). The image was acquired on September 21, 2002. Although The Fires shown on the satellite can show various fires across the country. It has done massive damage. Due to high wind storms.

Credit: Image courtesy Jacques Descloitres, MODIS Rapid Response Team at NASA GSFC

Burn Scars and Late-Season Fires in Kazakhstan

The ESA-led Solar Orbiter mission is currently observing and studying the Sun with six different imaging instruments, allowing the spacecraft to peel away the Sun's many layers and reveal its diverse faces.



<h2 class="wp-block-heading" id="h-high-resolution-views-of-the-sun">High-resolution views of the Sun</h2>



Recently, the mission released the highest-resolution full views to date of the Sun's visible surface, known as the photosphere.&nbsp;



The images were assembled from data captured by the spacecraft's Polarimetric and Helioseismic Imager (PHI).&nbsp;



This instrument not only photographs the Sun in visible light but also measures the direction of the <a href="https://search.app?link=https%3A%2F%2Fwww.earth.com%2Fnews%2Forigin-of-the-suns-magnetic-field-discovered-after-400-years%2F&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">magnetic field</a> and maps the speed and direction in which different parts of the surface are moving.



PHI's measurements of the photosphere can be directly compared to a new image of the Sun's outer atmosphere, the corona.&nbsp;



This image is essentially a mosaic assembled from high-resolution images taken by the Extreme Ultraviolet Imager (EUI) instrument on the same day in March 2023. The EUI captures images of the Sun in ultraviolet light.



<div class="wp-block-sendtonews-playerselector">[sendtonews key="wWscNjX6hZ-4055472-12187" type="single"]</div>



Daniel Müller, Solar Orbiter's Project Scientist, noted that the Sun's <a href="https://www.earth.com/news/solar-dynamo-sun-magnetic-field-origin-generated-near-surface/" target="_blank" rel="noreferrer noopener">magnetic field</a> is key to understanding the dynamic nature of our home star from the smallest to the largest scales.&nbsp;



“These new high-resolution maps from Solar Orbiter's PHI instrument show the beauty of the Sun's surface magnetic field and flows in great detail,” said Miller.



“At the same time, they are crucial for inferring the magnetic field in the Sun's hot corona, which our EUI instrument is imaging.”&nbsp;



The image release builds upon one from two years ago when the mission shared full images of the Sun taken by the spacecraft's EUI and Spectral Imaging of the Coronal Environment (SPICE) instruments on March 7, 2022.



<h2 class="wp-block-heading" id="h-sunspots-and-a-chaotic-magnetic-field">Sunspots and a chaotic magnetic field</h2>



Zooming into PHI's detailed visible light images reveals the Sun's “surface” for what it truly is: a constantly moving layer of glowing, hot plasma (charged gas). 



This layer emits almost all the Sun's radiation and has a temperature between 4,500 and 6,000°C. 



Beneath it lies the convection zone, where hot, dense plasma churns similarly to magma in Earth's mantle. This turbulent movement gives the Sun's surface its grainy appearance.



The most striking features in the images are the <a href="https://www.earth.com/news/sun-solar-cycle-25-highest-number-sunspots-activity-seen-since-2001/" target="_blank" rel="noreferrer noopener">sunspots</a>. In the visible light images, these appear as dark spots or holes on the otherwise smooth surface. Sunspots are cooler than their surroundings, emitting less light as a result.



PHI's magnetic map, or “magnetogram," shows that the Sun's magnetic field is concentrated in the sunspot regions, pointing either outward (red) or inward (blue) where the sunspots lie.&nbsp;



The strong magnetic field explains why plasma inside sunspots is cooler. Normally, convection moves heat from inside the Sun to its surface, but this process is disrupted as charged particles are forced to follow the dense magnetic field lines in and around the sunspots.



<h2 class="wp-block-heading" id="h-mapping-movement-on-the-surface">Mapping movement on the surface</h2>



The speed and direction of material movement on the Sun's surface are displayed in PHI's velocity map, also known as a “tachogram.”&nbsp;



In this map, blue indicates movement toward the spacecraft, while red signifies movement away. The map reveals that while the plasma on the Sun's surface generally rotates with the Sun's overall spin around its axis, it is pushed outward around the sunspots.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/11/Solar-Orbiter_3-views-of-Sun_lenses_ESA_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/Solar-Orbiter_3-views-of-Sun_lenses_ESA_1s.webp" alt="The three views of the Sun's surface shown here are based on measurements taken on March 22, 2023 by the ESA-led Solar Orbiter mission. From left to right, you see the Sun in visible light, a magnetic map of the Sun, and a map of the line-of-sight speed and direction of movement of material at the Sun's visible surface. Credit: ESA" class="wp-image-1951400"/></a><figcaption class="wp-element-caption">The three views of the Sun's surface shown here are based on measurements taken on March 22, 2023 by the ESA-led Solar Orbiter mission. From left to right, you see the Sun in visible light, a magnetic map of the Sun, and a map of the line-of-sight speed and direction of movement of material at the Sun's visible surface. Credit: ESA</figcaption></figure>



Finally, EUI's image of the Sun's <a href="https://www.earth.com/news/why-is-the-suns-corona-hotter-than-its-surface/" target="_blank" rel="noreferrer noopener">corona</a> shows what happens above the photosphere. Above the active sunspot regions, glowing plasma protrudes outward. 



This million-degree plasma follows magnetic field lines extending from the Sun, often connecting neighboring sunspots.



<h2 class="wp-block-heading" id="h-piecing-together-the-sun-s-mosaic">Piecing together the Sun's mosaic</h2>



The images were captured when the Solar Orbiter was less than 74 million kilometers from the Sun.&nbsp;



Being so close meant that each high-resolution image taken by PHI and EUI covered only a small portion of the Sun. To image the entire face, the spacecraft had to be tilted and rotated after each individual image was taken.



To create the full-disc images presented, all individual images were stitched together like a mosaic. Both the PHI and EUI mosaics consist of 25 images each, captured over more than four hours.&nbsp;



The resulting mosaics have a diameter of nearly 8,000 pixels, revealing an astonishing amount of detail.



The image processing required to produce the PHI mosaics was new and challenging. 



Now that it has been accomplished once, future data processing and mosaic assembly will be faster. The PHI team expects to provide such high-resolution mosaics twice a year.



<h2 class="wp-block-heading" id="h-advancing-our-understanding-of-the-sun">Advancing our understanding of the Sun</h2>



The new images not only showcase the beauty of our star but also enhance our understanding of its complex magnetic fields and dynamic processes.&nbsp;



By comparing data from different instruments, scientists can gain deeper insights into how the Sun's magnetic field influences phenomena from the smallest to the largest scales.



With continued efforts from missions like Solar Orbiter, we are peeling back the layers of the Sun to better comprehend its impact on our Solar System.



Video/ Image Credit: European Space Agency&nbsp;



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Solar Orbiter spacecraft sees the Sun through three different lenses

The ESA-led Solar Orbiter mission is currently observing and studying...

You probably know at least a little bit about ocean circulation around the world, also known as currents. In fact, you may have felt smaller currents yourself on a day at the beach.



But have you heard bout the "great global ocean conveyor belt," which is a vast network of currents that constantly moves water around the entire planet?



This massive system helps distribute heat around the world, influencing everything from temperatures to rainfall. Unfortunately, it's slowing down and on the verge of total collapse.



Scientists have been studying this phenomenon, and according to recent research published in <a href="https://www.nature.com/articles/s41561-024-01568-1" target="_blank" rel="noreferrer noopener">Nature Geoscience</a>, it's a bigger deal than we thought. 



<h2 class="wp-block-heading" id="h-ocean-circulation-and-the-amoc">Ocean circulation and the AMOC?</h2>



The Atlantic Meridional Overturning Circulation, or AMOC, is like a massive ocean conveyor belt that moves warm and cold water around the <a href="https://www.earth.com/news/why-the-atlantic-ocean-may-ultimately-vanish/" target="_blank" rel="noreferrer noopener">Atlantic Ocean</a>. 



It starts in the Gulf of Mexico, where warm, salty water flows northward along the eastern coast of the United States and across the Atlantic towards Europe. 



As this warm water reaches the North Atlantic, it cools down, becomes denser, and sinks deep into the ocean. 



This sinking process pulls more warm water north to replace it, creating a continuous loop that helps <a href="https://www.earth.com/news/collapse-of-major-ocean-system-would-cause-weather-chaos/" target="_blank" rel="noreferrer noopener">regulate the climate</a> by distributing heat across the planet. 



Thanks to the AMOC, regions like Western Europe enjoy milder winters than they would otherwise.



Humans rely on the AMOC in several important ways. By regulating global temperatures, it helps maintain stable weather patterns, which are crucial for agriculture, ecosystems, and our daily lives. 



Researchers point out that the Atlantic Meridional Overturning Circulation (AMOC) is now weaker than at any other time in the past 1,000 years.



The research team from several leading universities explains that global warming is behind this slowdown. 



Their new modeling suggests that meltwater from the <a href="https://www.earth.com/news/greenlands-melting-icebergs-may-not-be-threat-to-ocean-currents-amoc/" target="_blank" rel="noreferrer noopener">Greenland ice sheet</a> and Canadian glaciers could be the missing piece of the puzzle.



<h2 class="wp-block-heading" id="h-why-should-we-care-about-this">Why should we care about this?</h2>



"Our results show the Atlantic overturning circulation is likely to become a third weaker than it was 70 years ago at 2°C of global warming," says the research team. 



"This would bring big changes to the <a href="https://www.earth.com/news/the-arctic-is-melting-fast-but-a-slowing-ocean-current-could-help/" target="_blank" rel="noreferrer noopener">climate and ecosystems</a>, including faster warming in the southern hemisphere, harsher winters in Europe, and weakening of the northern hemisphere's tropical monsoons."



Think about that for a second. A weaker ocean current could mean colder winters in Europe and shifts in rainfall patterns that affect millions of people. It's not just about the ocean; <a href="https://www.earth.com/news/disastrous-climate-changes-of-the-last-ice-age-could-happen-again/" target="_blank" rel="noreferrer noopener">it's about our daily lives</a>.



<h2 class="wp-block-heading" id="h-meltwater-and-ocean-circulation">Meltwater and ocean circulation</h2>



The Earth has already warmed 1.5ºC since the industrial revolution. And get this: the Arctic has been heating up nearly four times faster than the rest of the planet. 



All that heat is melting Arctic sea ice, glaciers, and the Greenland ice sheet.



"Since 2002, Greenland lost 5,900 billion tons (gigatons) of ice," notes the research team. "To put that into perspective, imagine if the entire state of Texas was covered in ice 26 feet thick."



All this fresh meltwater flowing into the subarctic ocean is lighter than salty seawater, so it doesn't sink as much. 



That messes with the southward flow of deep, cold waters from the Atlantic and <a href="https://www.earth.com/news/climate-change-will-impact-the-gulf-stream-more-than-we-thought/" target="_blank" rel="noreferrer noopener">weakens the Gulf Stream</a> -- the same current that gives Britain its mild winters.



<h2 class="wp-block-heading" id="h-ripple-effects-around-the-globe">Ripple effects around the globe</h2>



So, what's the big deal with the Gulf Stream slowing down? Well, for starters, Europe could face harsher winters. 



<a href="https://www.earth.com/news/climate-paradox-ocean-current-collapse-could-plunge-europe-into-cold/" target="_blank" rel="noreferrer noopener">Places like Britain</a> might start feeling more like their chilly counterparts at the same latitude, such as parts of Canada.



<figure class="wp-block-image aligncenter size-full is-resized"><a href="https://www.earth.com/wp-content/uploads/2024/11/Atlantic-Meridional-Overturning-Circulation_AMOC_collapsing_Nature-Geoscience_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/Atlantic-Meridional-Overturning-Circulation_AMOC_collapsing_Nature-Geoscience_1s.webp" alt="The addition of meltwater in the North Atlantic leads to localised cooling in the subpolar North Atlantic and warming in the South Atlantic. Credit: Nature Geoscience (2024)." class="wp-image-1951410" style="width:300px;height:auto"/></a><figcaption class="wp-element-caption">The addition of meltwater in the North Atlantic leads to localised cooling in the subpolar North Atlantic and warming in the South Atlantic. Credit: Nature Geoscience (2024).</figcaption></figure>



"Our new research shows meltwater from the Greenland ice sheet and Arctic glaciers in Canada is the missing piece in the climate puzzle," the researchers explain. 



When they included this meltwater in their simulations, the slowing of the oceanic circulation made sense.



The study confirms that the Atlantic overturning circulation has been slowing down since the mid-20th century. It also gives us a sneak peek into <a href="https://www.earth.com/news/atlantic-and-arctic-mixing-is-crucial-for-earths-climate-stability/" target="_blank" rel="noreferrer noopener">what's coming next</a>.



<h2 class="wp-block-heading" id="h-northern-and-southern-oceans-connected">Northern and Southern oceans connected</h2>



"Our new research also shows the North and South Atlantic oceans are more connected than previously thought," the team states. 



Changes in one part of the ocean can quickly affect distant regions. When the oceanic circulation is strong, it transfers a lot of heat to the <a href="https://www.earth.com/news/antarctic-warming-triggers-rising-north-atlantic-sea-levels/" target="_blank" rel="noreferrer noopener">North Atlantic</a>. 



But when it weakens, the surface of the ocean south of Greenland doesn't warm up as much, leading to what's called a "warming hole." Meanwhile, the South Atlantic ends up storing more heat and salt.



<h2 class="wp-block-heading" id="h-time-is-not-on-our-side">Time is not on our side</h2>



"Our simulations show changes in the far North Atlantic are felt in the South Atlantic Ocean in less than two decades," the researchers reveal. This means the effects of the slowdown are spreading faster than we thought.



Climate projections have suggested the Atlantic overturning circulation will weaken by about 30% by 2060. But hold on -- that's without considering all that extra meltwater.



"The Greenland ice sheet will continue melting over the coming century, possibly raising global sea level by about 4 inches," the study notes. 



"If this additional meltwater is included in climate projections, the overturning circulation will weaken faster. It could be 30% weaker by 2040. That's 20 years earlier than initially projected."



<h2 class="wp-block-heading" id="h-what-can-we-do">What can we do?</h2>



Such a rapid decrease in the overturning circulation will shake things up. 



Europe might see colder winters, the northern tropics could get drier, and places like the southern United States might experience warmer, wetter summers.



"Our climate has changed dramatically over the past 20 years," the researchers warn. "More rapid melting of the ice sheets will accelerate further disruption of the climate system."



So, what does this all mean for us? It means we have even less time to get our act together. Reducing emissions isn't just a good idea -- it's crucial.



Our planet's systems are interconnected in ways we're only beginning to understand. If we want to keep things from getting worse, we need to act now. Every little bit counts, and the clock is ticking.



The full study was published in the journal <a href="https://www.nature.com/articles/s41561-024-01568-1" target="_blank" rel="noreferrer noopener">Nature Geoscience</a>.



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Collapse of Earth's main ocean water circulation system is already happening

You probably know at least a little bit about ocean...

A,Vintage,World,Globe,Tilted,And,Standing,On,A,Central

Picture this: every time you use water from your tap, you're inadvertently influencing our Earth's rotational tilt and climate change. Strange, and not a good thing, but true.



Our planet is a dynamic entity, constantly shifting and adapting. Believe it or not, something as seemingly insignificant as our water usage can cause Earth's physical orientation to deviate. 



Over less than two decades, our groundwater pumping has tilted the <a href="https://www.earth.com/news/earth-days-getting-longer-rotation-slows-climate-change/" target="_blank" rel="noreferrer noopener">Earth</a> by 31.5 inches. To put this into perspective, this water redistribution equates to approximately 0.24 inches of sea-level rise.



“Our study shows that among climate-related causes, the redistribution of groundwater actually has the largest impact on the drift of the rotational pole,” said Ki-Weon Seo, a geophysicist at <a href="https://en.snu.ac.kr/index.html" target="_blank" rel="noreferrer noopener">Seoul National University</a>.



So, before you dismiss the power of your water usage, remember, even the smallest actions have consequences.



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



Groundwater is the water that sits beneath the Earth's surface, filling up the spaces in soil, sand, and rock formations. 



It comes from rain and other precipitation that soaks into the ground, gradually making its way down to <a href="https://www.earth.com/news/millions-of-people-in-the-u-s-rely-on-contaminated-groundwater/" target="_blank" rel="noreferrer noopener">underground reservoirs</a> called aquifers. 



Unlike the water you see in rivers and lakes, groundwater is hidden away, acting like nature’s hidden water bank. 



It plays a crucial role in the water cycle, providing a steady supply of water even during dry spells when surface water might be scarce.



Humans rely on groundwater for a <a href="https://www.earth.com/news/groundwater-has-a-vital-role-in-ecosystem-survival/" target="_blank" rel="noreferrer noopener">variety of essential needs</a>. Many people use it as their primary source of drinking water, especially in rural areas where surface water isn't readily available. 



Farmers depend on groundwater for irrigating crops, ensuring that food production can continue even when there's not enough rain. Additionally, industries use groundwater for manufacturing processes and cooling systems. 



<h2 class="wp-block-heading" id="h-groundwater-s-role-in-earth-s-tilt">Groundwater's role in Earth's tilt</h2>



The study, which included data from 1993 through 2010, showed that pumping as much as 2,150 gigatons of groundwater has caused a shift in the Earth's tilt. 



These figures are hard to comprehend, but they reflect our intense water consumption for irrigation and human use.



We may not think about where our water goes after we use it, but most of it ends up being transported to the oceans. 



“Observing changes in Earth’s rotational pole is useful for understanding continent-scale water storage variations,” said Seo.



Linking these variations to water movement, particularly from western North America and northwestern India, shows how our everyday actions can impact the <a href="https://www.earth.com/news/earths-rotation-is-shifting-toward-a-25-hour-day/" target="_blank" rel="noreferrer noopener">Earth</a> on a global scale.



<h2 class="wp-block-heading" id="h-rotational-pole-drift">Rotational pole drift</h2>



Alongside influencing our planet's tilt and rotation, groundwater pumping paints an alarming picture for the <a href="https://www.earth.com/news/groundwater-temperatures-may-rise-due-to-climate-change/" target="_blank" rel="noreferrer noopener">consequences of climate change</a>.



“I’m very glad to find the unexplained cause of the rotation pole drift. On the other hand, as a resident of Earth and a father, I’m concerned and surprised that pumping groundwater is another source of sea-level rise,” said Seo.



These findings might seem overwhelming, especially considering the challenges we already face in combating climate change. 



However, understanding the impact of groundwater pumping on Earth's tilt and climate is a step in the right direction.



This knowledge can potentially guide conservationists toward effective strategies to mitigate further sea-level rise and other climate issues.



<h2 class="wp-block-heading" id="h-groundwater-pumping-and-polar-motion">Groundwater pumping and polar motion</h2>



The new revelations about <a href="https://www.earth.com/news/groundwater-depletion-is-accelerating-but-it-is-not-inevitable/" target="_blank" rel="noreferrer noopener">groundwater pumping</a> open new doors for our understanding of climate change and our capacity for action.



"They’ve quantified the role of groundwater pumping on polar motion, and it’s pretty significant," said Surendra Adhikari, a research scientist at NASA’s Jet Propulsion Laboratory (<a href="https://www.jpl.nasa.gov" target="_blank" rel="noreferrer noopener">JPL</a>).



The potential for change isn't exclusive to scientists and researchers. As individuals, we can adapt our habits and live more sustainably. 



This awareness around groundwater pumping's global impact should empower us to reconsider our everyday water usage.



<h2 class="wp-block-heading" id="h-future-research-and-policy-initiatives">Future research and policy initiatives </h2>



Given the significant findings of the study, future research and policy initiatives must prioritize sustainable groundwater management to mitigate its adverse impacts on Earth's rotation and climate change. 



It is imperative to balance human needs with environmental conservation, which requires innovative approaches to water usage, such as enhanced irrigation <a href="https://www.earth.com/news/our-moon-is-drifting-away-and-earth-will-never-be-the-same-without-it/" target="_blank" rel="noreferrer noopener">systems</a>, rainwater harvesting, and improved municipal water management. 



Furthermore, global cooperation among countries is essential to create comprehensive policies that address the equitable distribution and consumption of water resources. 



By encouraging multidisciplinary collaboration among geophysicists, climate scientists, policy-makers, and the public, we can develop a robust framework for more sustainable water management practices. 



Such initiatives not only hold promise for protecting Earth's rotational stability but also contribute to <a href="https://www.earth.com/news/climate-change-is-now-the-driving-force-behind-droughts/" target="_blank" rel="noreferrer noopener">broader climate change</a> mitigation efforts.



<h2 class="wp-block-heading" id="h-water-taps-tilting-the-earth">Water taps tilting the Earth</h2>



The journey towards understanding and combating climate change is a long and complex one. But in this struggle, knowledge is power. 



Understanding the impact of groundwater pumping is an invaluable tool in our arsenal.



As we look to the future, let's harness this knowledge and strive for a more sustainable world.



The study is published in the journal <a href="https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2023GL103509" target="_blank" rel="noreferrer noopener">Geophysical Research Letters</a>.



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Earth's rotation has tilted 31.5 inches, and humans are 100% to blame

Picture this: every time you use water from your tap,...

The alphabet holds a unique place in human history, and every new discovery about its origins can illuminate our past and challenge long-held beliefs. 



Its simplicity and adaptability transformed the way humans communicated, laying the foundation for countless languages and cultures. 



Each breakthrough brings us closer to understanding how early societies transitioned from complex symbols to accessible scripts.



<h2 class="wp-block-heading" id="h-oldest-alphabet-ever-found">Oldest alphabet ever found</h2>



A recent phenomenal finding has done just that - it’s reshaping what we know about the beginnings of alphabetic writing.



Our story begins in Syria, where a team from <a href="https://www.jhu.edu/" target="_blank" rel="noreferrer noopener">Johns Hopkins University</a> made an unexpected discovery.



The researchers unearthed finger-length clay cylinders from an ancient tomb, etched with what appears to be the oldest alphabet in known human history.



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



This incredible finding dates back to approximately 2400 BCE, which is a staggering 500 years older than any other known alphabetic scripts. 



This revelation is monumental as it overthrows previously held theories about the origins of alphabets, and how they were adopted by <a href="https://www.earth.com/news/ice-cores-show-that-early-societies-were-dominated-by-climate-events/" target="_blank" rel="noreferrer noopener">early societies</a>, changing their lifestyle and course of civilization.



Glenn Schwartz is a professor of archaeology at Johns Hopkins University and one of the lead researchers who discovered the clay cylinders.



"Alphabets revolutionized writing by making it accessible to people beyond royalty and the socially elite," said Professor Schwartz. 



"Alphabetic writing changed the way people lived, how they thought, how they communicated. And this new discovery shows that people were experimenting with new <a href="https://www.earth.com/news/quantum-holograms-future-of-secure-messaging-encryption-internet/" target="_blank" rel="noreferrer noopener">communication technologies</a> much earlier and in a different location than we had imagined before now."



<h2 class="wp-block-heading" id="h-digging-deeper-into-the-past">Digging deeper into the past</h2>



The story behind this discovery unfolds at Tell Umm-el Marra, an early urban center in Western Syria. A group of archaeologists, including experts from the University of Amsterdam, embarked on a 16-year excavation journey at this site.



The fruitful outcome of their dedication was the unearthing of tombs from the Early <a href="https://www.earth.com/news/bronze-age-teeth-discovery-highlight-the-evolution-of-the-human-diet/" target="_blank" rel="noreferrer noopener">Bronze Age</a>. Among these tombs, one stood out - the final resting place of six individuals, adorned with gold and silver jewelry, cookware, a spearhead, and intact <a href="https://www.earth.com/news/baltic-pottery-reveals-ancient-culinary-traditions/" target="_blank" rel="noreferrer noopener">pottery vessels</a>.



Interestingly, found next to the pottery were four lightly baked clay cylinders, etched with what seems to be alphabetic writing. 



"The cylinders were perforated, so I’m imagining a string tethering them to another object to act as a label. Maybe they detail the contents of a vessel, or maybe where the vessel came from, or who it belonged to. Without a means to translate the writing, we can only speculate," said Professor Schwartz. 



<h2 class="wp-block-heading" id="h-a-new-chapter-for-the-alphabet">A new chapter for the alphabet?</h2>



Thanks to advanced carbon-14 dating techniques, the researchers were able to confirm the ages of the tombs, the artifacts, and the writing. 



The discovery challenges existing theories about the birth of the alphabet. It shifts our understanding of the origins of alphabetic writing, hinting at an entirely different narrative, as Professor Schwartz explained.



"Previously, scholars thought the alphabet was invented in or around Egypt sometime after 1900 BCE,” said Schwartz. "But our <a href="https://www.earth.com/news/monkey-stone-tools-look-like-early-human-artifacts/" target="_blank" rel="noreferrer noopener">artifacts</a> are older and from a different area on the map, suggesting the alphabet may have an entirely different origin story than we previously thought.”



The research highlights the importance of continuous exploration in our endeavor to comprehend our past and understand its impact on our present and future.



<h2 class="wp-block-heading" id="h-broader-impact-of-alphabetic-discoveries">Broader impact of alphabetic discoveries</h2>



The discovery of the oldest known alphabet in Syria does more than just challenge existing theories - it offers a deeper understanding of how early societies communicated and evolved.



Alphabetic writing, unlike the pictograms and logograms used in earlier writing systems, simplified communication, making it more accessible to wider populations. 



This democratization of writing could have been a pivotal factor in advancing trade, governance, and cultural exchanges among early civilizations.



The implications of the ancient alphabet extend beyond archaeology. Linguists, historians, and even technology researchers could gain insights into the roots of structured communication systems.



Understanding the origins of the alphabet also helps contextualize its influence on modern languages and scripts, illustrating its role as a building block for contemporary literacy and education.



Image Credit: Glenn Schwartz, Johns Hopkins University



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Oldest known alphabet discovered in Syria

The alphabet holds a unique place in human history, and...

A recent NASA-funded study has deepened the enigma of why life uses molecules with specific orientations.&nbsp;



Researchers have discovered that RNA - a crucial molecule thought to have potentially carried life's instructions before DNA emerged - can favor making the building blocks of proteins in either left-handed or right-handed forms. This finding could provide valuable clues to the origin of life.



<h2 class="wp-block-heading" id="h-the-puzzle-of-life-s-molecular-orientation">The puzzle of life's molecular orientation</h2>



<a href="https://www.earth.com/news/how-life-begins-egg-sperm-and-a-covert-team-of-proteins/" target="_blank" rel="noreferrer noopener">Proteins</a> are essential molecules in all living organisms, serving functions from structural components like hair to enzymes that speed up or regulate chemical reactions. 



Similar to how the 26 letters of the alphabet combine to form countless words, life uses 20 different amino acids in a vast array of arrangements to create millions of different proteins.&nbsp;



Some amino acids exist in two mirror-image forms, like left and right hands, but life predominantly uses the left-handed variety - a phenomenon known as homochirality.&nbsp;



Scientists remain puzzled about why life chose left-handed amino acids over right-handed ones, especially since life based on right-handed <a href="https://www.earth.com/news/how-did-the-building-blocks-of-life-form/" target="_blank" rel="noreferrer noopener">amino acids</a> would presumably function just as well.



<h2 class="wp-block-heading" id="h-exploring-the-rna-world-hypothesis">Exploring the “RNA world” hypothesis</h2>



DNA holds the instructions for building and maintaining living organisms but is complex and specialized. It “subcontracts” the work of reading instructions to RNA molecules and building proteins to ribosomes.&nbsp;



Due to DNA's complexity, scientists theorize that a simpler molecule preceded it billions of years ago during early life evolution. RNA, capable of both storing genetic information and building proteins, is a leading candidate, giving rise to the “<a href="https://www.earth.com/news/rna-world-unraveling-mysteries-life-origin/" target="_blank" rel="noreferrer noopener">RNA world</a>” hypothesis.



If this proposition is correct, perhaps something about RNA caused it to favor building left-handed proteins over right-handed ones.&nbsp;



However, the new research did not support this idea, deepening the mystery of why life favored left-handed proteins.



<h2 class="wp-block-heading" id="h-the-role-of-evolutionary-pressures-nbsp">The role of evolutionary pressures&nbsp;</h2>



The experiment tested RNA molecules that act like enzymes to build proteins, called ribozymes.&nbsp;



“The experiment demonstrated that ribozymes can favor either left- or right-handed amino acids, indicating that RNA worlds, in general, would not necessarily have a strong bias for the form of amino acids we observe in biology now,” said corresponding author Irene Chen, a scientist at the <a href="https://www.ucla.edu/" target="_blank" rel="noreferrer noopener">University of California, Los Angeles</a> (UCLA) Samueli School of Engineering.



In simulating potential early-Earth conditions of the RNA world, researchers incubated a solution containing ribozymes and amino acid precursors to observe the relative percentages of right-handed and left-handed phenylalanine amino acids produced.&nbsp;



They tested 15 different ribozyme combinations and found that ribozymes can favor either left-handed or right-handed amino acids. This lack of inherent preference challenges the notion that early life was predisposed to select left-handed amino acids, which dominate in modern proteins.



“The findings suggest that life’s eventual homochirality might not be a result of chemical determinism but could have emerged through later evolutionary pressures,” said co-author Alberto Vázquez-Salazar, a UCLA postdoctoral scholar and member of Chen’s research group.



<h2 class="wp-block-heading" id="h-implications-for-understanding-life-s-origins">Implications for understanding life's origins</h2>



Earth's prebiotic history predates the oldest fossil records, which have been erased by plate tectonics - the slow movement of Earth's crust.&nbsp;



During that time, the planet was likely bombarded by <a href="https://www.earth.com/news/what-would-happen-small-asteroid-hit-earth-nasa-ai-simulation-found-out/" target="_blank" rel="noreferrer noopener">asteroids</a>, which may have delivered some of life's building blocks, such as amino acids. Alongside chemical experiments, other origin-of-life researchers are examining molecular evidence from meteorites and asteroids.



Study co-author Jason Dworkin is a senior scientist for astrobiology at NASA’s <a href="https://www.nasa.gov/goddard/" target="_blank" rel="noreferrer noopener">Goddard Space Flight Center</a> in Greenbelt, Maryland, and director of <a href="https://science.gsfc.nasa.gov/691/analytical/" target="_blank" rel="noreferrer noopener">Goddard’s Astrobiology Analytical Laboratory</a>.



Dworkin is also the project scientist on NASA’s OSIRIS-REx mission - which extracted samples from the asteroid Bennu and delivered them to Earth.



“Understanding the chemical properties of life helps us know what to look for in our search for life across the solar system,” said Dworkin.&nbsp;



“We are analyzing OSIRIS-REx samples for the chirality (handedness) of individual amino acids, and in the future, samples from Mars will also be tested in laboratories for evidence of life including ribozymes and proteins.”



<h2 class="wp-block-heading" id="h-the-search-for-life-s-molecular-secrets">The search for life's molecular secrets</h2>



This discovery adds complexity to our understanding of life's molecular orientations, suggesting that homochirality might not have resulted from initial chemical conditions but could have developed due to evolutionary factors.&nbsp;



The findings prompt further research into the <a href="https://www.earth.com/news/new-clues-about-the-origins-of-life-on-earth/" target="_blank" rel="noreferrer noopener">origins of life</a> and may influence how scientists search for life beyond Earth.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-52362-x" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



Image Credit: NASA



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Life’s molecular orientation: New discovery deepens the mystery

A recent NASA-funded study has deepened the enigma of why...

For the past two months, a small asteroid named 2024 PT5 has been keeping Earth company, acting as a temporary "mini-moon." This week, it's set to drift away, pulled by the stronger gravity of the sun.



Richard Binzel, an astronomer at the Massachusetts Institute of Technology (<a href="https://www.mit.edu" target="_blank" rel="noreferrer noopener">MIT</a>), has been following these kinds of celestial visitors for years. 



"These happen more often than we think, but they're small and tough to spot," Binzel explained. "Only lately have our telescopes become powerful enough to catch them regularly."



In August, a team of astronomers from the <a href="https://www.ucm.es/english" target="_blank" rel="noreferrer noopener">Complutense University</a> of Madrid detected 2024 PT5 using a powerful telescope in Sutherland, South Africa. 



They weren't the only ones watching; NASA's Asteroid Terrestrial-impact Last Alert System (<a href="https://fallingstar.com/home.php" target="_blank" rel="noreferrer noopener">ATLAS</a>) at Haleakala Observatory in Hawaii first noticed the asteroid on August 7, 2024.



This discovery has excited astronomers, offering a rare chance to learn more about <a href="https://www.earth.com/news/nasa-test-simulation-shows-earth-not-prepared-prevent-large-asteroid-strike/" target="_blank" rel="noreferrer noopener">near-Earth objects</a>. But what exactly is 2024 PT5, and why does it matter?



<h2 class="wp-block-heading" id="h-2024-pt5-tiny-asteroid-big-role">2024 PT5: Tiny asteroid, big role</h2>



<a href="https://www.earth.com/news/its-official-earth-now-has-two-moons-captured-asteroid-2024-pt5/" target="_blank" rel="noreferrer noopener">Earth occasionally captures small asteroids</a> like 2024 PT5, placing them into temporary orbits around our planet. 



While most asteroids orbit the sun on regular paths, some come close enough for Earth's gravity to grab them for a brief visit. 



These cosmic hitchhikers stay with us for a short time -- typically a few weeks or months -- before breaking free and continuing their journey around the sun.



"All mini-moons are unique in their own way," said William Blackmore, Planetarium Director and Astronomy Instructor at <a href="https://www.mhcc.edu/" target="_blank" rel="noreferrer noopener">Mt. Hood Community College</a>. "This one isn't different from others except that it's the most recent."



<h2 class="wp-block-heading" id="h-comparing-2024-pt5-to-the-moon">Comparing 2024 PT5 to the Moon</h2>



To put things into perspective, 2024 PT5 is about 37 feet across. In contrast, <a href="https://www.earth.com/news/how-did-earth-get-its-moon-a-new-theory-has-emerged/" target="_blank" rel="noreferrer noopener">Earth's main moon</a> stretches a massive 2,159 miles in diameter. 



That makes our moon over 300,000 times wider than this tiny asteroid. Knowing it's up there is pretty exciting, even if we can't see it without some serious telescopic equipment.



"These temporary captures are natural cosmic laboratories," Binzel mentioned. "They help us understand the small bodies that <a href="https://www.earth.com/news/27500-hidden-near-earth-asteroids-discovered-using-google-cloud/" target="_blank" rel="noreferrer noopener">come close to Earth</a> and could be important for future space missions."



<h2 class="wp-block-heading" id="h-how-2024-pt5-became-a-mini-moon">How 2024 PT5 became a mini-moon</h2>



Understanding how 2024 PT5 became Earth's temporary companion involves a bit of <a href="https://www.earth.com/news/finding-order-in-the-chaos-of-the-three-body-problem/" target="_blank" rel="noreferrer noopener">orbital mechanics</a>. 



Blackmore explained, "It's moving along with us in our orbit around the sun. It's part of a group of asteroids called the Arjuna asteroids, which move at about the same pace as Earth."



He added an analogy to make it clearer: 



"Imagine a skateboarder dropping into a skate park. They ride the curves, adding energy as they go. That's like the asteroid getting caught in <a href="https://www.earth.com/news/dart-mission-debris-will-create-a-human-made-meteor-shower/" target="_blank" rel="noreferrer noopener">Earth's gravitational field</a>, riding the curve before moving on."



<h2 class="wp-block-heading" id="h-spotting-mini-moons-like-2024-pt5">Spotting mini-moons like 2024 PT5</h2>



Catching sight of mini-moons is no easy task. 



They're incredibly small and faint, often just a few dozen feet across, which means they don't reflect much sunlight. This makes them nearly invisible against the dark backdrop of space.



Astronomers use powerful telescopes equipped with <a href="https://www.earth.com/news/gaia-reveals-moons-around-hundreds-of-asteroids/" target="_blank" rel="noreferrer noopener">sensitive detectors and smart software</a> to find them. 



Projects like the ATLAS system scan the skies every night, searching for any objects that weren't there before. 



When they spot something moving in a way that suggests it's close to Earth, they alert other astronomers to help confirm the find.



"It's a collaborative effort," Blackmore said. "Combining technology and teamwork helps us spot these elusive cosmic visitors."



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



While 2024 PT5 doesn't pose any threat to Earth, <a href="https://www.earth.com/news/is-there-a-fifth-force-of-nature-asteroids-provide-new-clues/" target="_blank" rel="noreferrer noopener">studying it is crucial</a>. 



"It's important to analyze how it moves and interacts with Earth's gravitational pull," Blackmore noted. "This helps us refine our techniques for tracking objects that could cross our path again."



Another expert, Todd, highlighted the practical applications of this knowledge. 



"We need to understand how to intercept an asteroid at a distance and change its direction," he said. "This could be vital in <a href="https://www.earth.com/news/nasa-dart-mission-proves-humanity-can-be-saved-from-asteroid-collision/" target="_blank" rel="noreferrer noopener">preventing potential impacts</a> in the future."



<h2 class="wp-block-heading" id="h-challenges-in-observing-2024-pt5">Challenges in observing 2024 PT5</h2>



For those eager to see this mini-moon, experts warn that it would be extremely difficult. 



"You'd need a telescope with a diameter of at least 30 inches," Blackmore mentioned. "That's beyond what most amateur astronomers have."



Todd agreed, adding, "It won't be visible to the naked eye. Being 33 feet wide and so far away, you'd need a very large telescope."



<h2 class="wp-block-heading" id="h-inspiration-for-future-space-missions">Inspiration for future space missions</h2>



Blackmore envisioned future missions that could take advantage of these temporary visitors. 



"It would be fascinating if we had missions ready to send small satellites or probes to these objects when they come close," he mused. "Imagine building a network of sensors or cameras traveling along with us, like space webcams."



Todd also saw potential in <a href="https://www.earth.com/news/asteroid-named-psyche-is-worth-10000-quadrillion-for-whoever-can-extract-minerals/" target="_blank" rel="noreferrer noopener">asteroid mining</a> and scientific discovery. 



"There might be materials on these asteroids that we can't find on Earth," he said. "They could solve problems in medicine or technology. But we need to weigh the benefits carefully."



<h2 class="wp-block-heading" id="h-brief-visit-with-a-lasting-impact">Brief visit with a lasting impact</h2>



The short stay of asteroid 2024 PT5 serves as a reminder of the dynamic nature of our solar system. While it didn't stick around long, its presence offered valuable opportunities for learning and exploration.



As technology advances, we'll likely spot more of these mini-moons. Each one gives us a chance to understand our cosmic environment better and prepare for the future.



The full study was published in the&nbsp;<a href="https://iopscience.iop.org/article/10.3847/2515-5172/ad781f" target="_blank" rel="noreferrer noopener">journal IOPscience</a>.



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Earth has lost its mini-moon, which may have come from our main Moon

For the past two months, a small asteroid named 2024...

In the world of science, we often focus on what we see. We examine what is visible, tangible, and easy to perceive with our own two eyes. But what about the sounds of the past - more specifically, the sounds of dinosaurs?



How can we possibly know what a creature from millions of years ago sounded like? Well, this can be answered using paleoacoustics.



Before we dive into the how, let's take a moment to consider what we are talking about. Picture the Parasaurolophus - a duck-billed <a href="https://www.earth.com/news/rare-triassic-fossil-gondwanax-paraisensis-may-rewrite-history-of-dinosaurs/" target="_blank" rel="noreferrer noopener">dinosaur</a> with a unique crest.



This huge creature, standing around 16 feet tall and weighing between 6,000 to 8,000 pounds, dominated the landscapes some 70 million to 80 million years ago. It has been named in many science fiction films and dinosaur-themed games.



<h2 class="wp-block-heading" id="h-decoding-dinosaur-sounds">Decoding dinosaur sounds</h2>



Sound is essentially vibrations traveling through the air. These vibrations hit our eardrums, get converted into electrical signals, and are interpreted by our brains. 



But for creatures like the Parasaurolophus, with unique physical attributes, their sounds would have been produced and resonated differently.



The starting point to understanding how the Parasaurolophus might have sounded is through mathematical modeling. 



Sounds a bit strange, doesn't it? But it's not just number crunching. Math is a universal language that is able to represent complex physical phenomena in a way that can be computed, simulated, and even visualized.



<h2 class="wp-block-heading" id="h-exploring-what-dinosaurs-sounded-like">Exploring what dinosaurs sounded like</h2>



Enter our scientist, Hongjun Lin, a researcher at <a href="https://www.nyu.edu" target="_blank" rel="noreferrer noopener">New York University</a> who is on a mission to decode the sounds of the past.



He presented his research on the acoustic characteristics of a physical model of the Parasaurolophus' crest at the 187th Meeting of the Acoustical Society of America in November 2024.



"I've been fascinated by giant animals ever since I was a kid. I'd spend hours reading books, watching movies, and imagining what it would be like if <a href="https://www.earth.com/news/carnian-pluvial-episode-one-million-years-of-rain-triggered-dinosaur-takeover-of-earth/" target="_blank" rel="noreferrer noopener">dinosaurs</a> were still around today," said Lin.



But a realization in college sparked a new direction for Lin's passion. "It wasn't until college that I realized the sounds we hear in movies and shows - while mesmerizing - are completely fabricated using sounds from modern animals."



"That's when I decided to dive deeper and explore what dinosaurs might have actually sounded like."



<h2 class="wp-block-heading" id="h-creating-dinosaur-sounds">Creating dinosaur sounds</h2>



To bring mathematics into the tangible realm, Lin created a physical setup - affectionately named the "Linophone." It is made of tubes that resemble the resonance chambers used in musical instruments.



This theoretical model, despite its simplicity, was pivotal in approximating what was happening acoustically inside the Parasaurolophus' crest.



The Linophone isn’t a perfect replica of the Parasaurolophus, but it's a stepping stone - a means to verify the mathematical framework.



Lin's initial findings suggest that the Parasaurolophus' crest was used for resonance, a phenomenon not unfamiliar to us - it’s the same principle that gives birds their unique songs.



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



The journey has just begun. Lin's research is far from complete, and the mathematical model is still a work in progress. 



But the implications of this study extend beyond just dinosaurs. This research paves the way for studying animals with similar vocal structures, leading to a deeper understanding of Earth's ancient inhabitants.



The idea doesn't stop there. Lin shares his plan for the future - an accessible plug-in for people to experiment with and even incorporate dinosaur sounds into music. Can you imagine rock and roll with a dash of Parasaurolophus?



"Once we have a working model, we'll move toward using&nbsp;fossil&nbsp;scans," Lin said. "My ultimate goal is to re-create the sound of the Parasaurolophus."



<h2 class="wp-block-heading" id="h-understanding-how-dinosaurs-communicated">Understanding how dinosaurs communicated</h2>



Understanding how dinosaurs communicated provides insights into their social structures and behaviors. The Parasaurolophus, with its crest capable of producing distinctive sounds, is a fascinating subject to explore these <a href="https://www.earth.com/news/qunkasaura-pintiquiniestra-new-sauropod-dinosaur-discovered-in-spain/" target="_blank" rel="noreferrer noopener">dynamics</a>. 



This anatomical feature may have allowed it to generate low-frequency calls, which could travel across long distances - a valuable adaptation for herd communication over expansive territories.



Such communication would have played a pivotal role in coordinating movement, warning of approaching predators, or even engaging in mating rituals. 



As research progresses, scientists hope to unravel whether these sounds were unique to each species, locality, or even individual, offering a more nuanced picture of dinosaur life.



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



While Lin's work has primarily focused on recreating the sounds of the Parasaurolophus, the broader implications of paleoacoustic research are vast. 



By refining techniques and understanding, scientists can apply these methods to other <a href="https://www.earth.com/news/nadir-crater-second-massive-asteroid-impact-discovered-dinosaur-extinction/" target="_blank" rel="noreferrer noopener">prehistoric animals</a>, providing a comprehensive soundtrack of the past. These innovations bolster educational tools, allowing students and enthusiasts worldwide to engage more deeply with Earth's history through sound. 



The field also enriches other disciplines, such as paleontology, biology, and acoustics - promoting interdisciplinary collaboration and innovative thinking.



As the boundaries of current research continue to expand, so too does our capacity to connect with the ancient world, transforming silent fossils into a symphony of prehistory.



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What did dinosaurs sound like?

In the world of science, we often focus on what...

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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



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

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



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

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



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

Kainji Lake in north central Nigeria

[sendtonews key="iuA5mpp3jv-1641775-12187" type="single"] Today’s Video of the Day from the...

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Today’s Video of the Day from <a href="https://www.igb.illinois.edu/">Carl R. Woese Institute for Genomic Biology</a> reveals how scientists can modify common crops like soybean, rice, and wheat to protect them from heat stress.



“We need to double crop production by 2050 to feed a growing global population, and not only are we not on track to do that, but climate change is further complicating things,” said Amanda Cavanagh, a lecturer at the University of Essex. 



The study is part of Realizing Increased Photosynthetic Efficiency (RIPE), an international research project that aims to develop food crops that turn the sun’s energy into food more efficiently.



“Using an engineering approach we designed multiple alternative metabolic pathways to photorespiration. Testing them in the field showed increases in productivity which led Amanda to significantly move the project forward by showing our engineered plants can withstand pretty extreme temperature stress,” said study co-author and RIPE researcher Paul South.&nbsp;



“As the climate changes and temperature stresses increase the pressure on our global food supply, farmers will need every tool available including engineering approaches like the synthetic biology used here to maintain safe and productive harvests.”



The experts tested plants modified to have more efficient photorespiration to see if they were better adapted to warmer temperatures.&nbsp;



The team found that the engineered plants produced 26 percent more biomass than the wild-type plants exposed to the same temperatures, and had 15 percent less yield loss under the higher temperatures.



Video Credit: Amanda Nguyen/University of Illinois



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



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

Designing crops that can beat the heat

[sendtonews key="QGPzYnXEtN-1712599-12187" type="single"] Today’s Video of the Day from Carl...

Hurricane Isidore hammers the Yucatan Peninsula. There as though even as it moves westward into the <a href="https://en.wikipedia.org/wiki/Gulf_of_Mexico">Gulf of Mexico.</a>  Also begins eyeing the Gulf Coast of the <a href="https://www.earth.com/video/the-eastern-united-states-from-space/">United States</a>. In this true-color Moderate Resolution Imaging Spectroradiometer (MODIS) image from the Aqua satellite. Therefore large atmospheric circulation associated with the storm is easily seen. If the storm were centered in the Gulf, it would fill it completely. This iamge was acquired on September 22, 2002.
Credit: <a href="https://visibleearth.nasa.gov/view.php?id=61834">Jacques Descloitres, MODIS Land Rapid Response Team, NASA/GSFC</a>

Hurricane Isidore over Yucatan Peninsula

Tropical Storm Isidore. Therefore with the maximum sustained winds approaching 125 mph (205 km/hr). Also this Hurricane Isidore is just skirting the coast of the Yucatan <a href="http://www.earth.com/image/the-yucatan-peninsula-from-space/">Peninsula</a>. The eye is clearly visible in this image and has an approximate diameter of 20 nautical miles. Isidore is expected to continue on a westward path for the next 24 hours.

Credit: <a href="https://earthobservatory.nasa.gov/images/10202/tropical-storm-isidore">Image courtesy Jacques Descloitres, MODIS Land Rapid Response Team at NASA GSFC</a>