Kasijy Reserve is a 19,800 hectares (49,000 acres) wildlife reserve in the Betsiboka region of <a href="https://www.earth.com/video/madagascar-from-space/" target="_blank" rel="noopener">Madagascar</a>. Nearly half of the species of plants and animals recorded within the reserve are endemic to Madagascar and <a href="https://www.birdlife.org/" target="_blank" rel="noopener">BirdLife International</a> have listed the reserve as an Important Bird Area.
Kasijy Reserve is 20 kilometres (12 mi) north-west of Bemonto in the Betsiboka region of Madagascar. Access is difficult because of the poor roads and there is no accommodation or Park Office in the reserve. The nearest accommodation is in the port of Mahajanga, to the north. There are two outcrops of karst, the Kasijy massif and the smaller Analamajera massif; both are covered in forest.
The Kasijy Reserve covers 19,800 hectares (49,000 acres), of which 14,931 hectares (36,900 acres) are savannah and 4,394 hectares (10,860 acres) tropical rainforest. There is also swamp and open water on the reserve. The site is bordered by three rivers; in the north is the Andranomaitso River, the Mahavavy River in the east and the Mahiarere River to the south. The climate is harsh with a dry season from April to November when the rivers run dry, and the reserve is closed to visitors in the wet season which runs from December to April. Annual rainfall is 1,679 millimetres (66.1 in) and temperatures can reach 38 °C (100 °F).
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Credit: Wikipedia

The Kasijy Reserve in Northwestern Madagascar

Today's Image of the Day from the European Space Agency features the barred spiral galaxy NGC 3783, which is located about 130 million light-years away in the constellation Centaurus. NGC 3783 is also the most prominent of a galaxy group (by the same name) that contains 47 galaxies. 



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



“Like galaxy clusters, galaxy groups are aggregates of gravitationally bound galaxies. Galaxy groups, however, are less massive and contain fewer members than <a href="https://www.earth.com/news/titanic-galaxy-cluster-collision-defies-all-current-understanding-of-the-universe/" target="_blank" rel="noreferrer noopener">galaxy clusters</a> do: where galaxy clusters can contain hundreds or even thousands of constituent galaxies, galaxy groups do not typically include more than 50,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The Milky Way is actually part of a galaxy group, known as the Local Group, which contains two other large galaxies (Andromeda and the Triangulum galaxy), as well as several dozen satellite and dwarf galaxies.”



<h2 class="wp-block-heading" id="h-hd-101274-a-blue-giant-star">HD 101274: A blue giant star</h2>



The bright object that appears to the right of the galaxy is the star HD 101274. “The perspective in this image makes the star and the galaxy look like close companions, but this is an illusion. HD 101274 lies only about 1,530 light-years from Earth, meaning it is about 85 thousand times closer than NGC 3783,” explained ESA.&nbsp;



The star is part of the NGC 3766 cluster, which is sometimes referred to as the Pearl Cluster, an open cluster known for its richness in bright stars and its relatively young age.



HD 101274 is categorized as a blue giant star, characterized by its high temperature and luminosity. 



Blue giants are massive stars that have left the main sequence phase of stellar evolution and are burning helium or heavier elements in their cores. These stars are known for their short lifespans relative to smaller stars due to their rapid consumption of nuclear fuel.



<h2 class="wp-block-heading" id="h-significance-of-blue-giants">Significance of blue giants</h2>



<a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">Stars</a> like HD 101274 are important for astronomers because they help in studying the properties of stellar populations in clusters and the dynamics of stellar evolution in different environments. 



The spectral and photometric observations of such stars can provide valuable insights into the characteristics of their atmospheres, internal structures, and the processes occurring within and around them.



<h2 class="wp-block-heading" id="h-bright-central-region-of-ngc-3783">Bright central region of NGC 3783</h2>



One of the most interesting aspects of NGC 3783 is that it harbors an active galactic nucleus, meaning its central region is exceptionally luminous, likely due to the presence of a supermassive black hole. This black hole is actively accreting material, which emits a substantial amount of radiation as it spirals inward and heats up.



The galaxy is particularly known for its bright central region and has been studied extensively in the ultraviolet and X-ray light spectra to understand better the properties of the accretion disk around the black hole and the complex dynamics of the material surrounding it. These studies are crucial for understanding the physics of active galactic nuclei and the role they play in <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxy evolution</a>.



According to ESA, NGC 3783 is a&nbsp;Type I Seyfert galaxy. “In this image it is recorded by Hubble in incredible detail, from its glowing central bar to its narrow, winding arms and the dust threaded through them, thanks to five separate images taken in different wavelengths of light," noted ESA.



“In fact, the galactic center is bright enough to Hubble that it exhibits diffraction spikes, normally only seen on stars such as HD 101274.”



<h2 class="wp-block-heading" id="h-more-about-the-ngc-3783-galaxy-group">More about the NGC 3783 galaxy group</h2>



The NGC 3783 group is part of the larger Hydra-Centaurus Supercluster, which itself is a massive collection of <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">galaxies</a> and galaxy clusters located primarily in the constellations of Hydra and Centaurus.



The NGC 3783 group consists of several galaxies that are gravitationally bound and interact with each other. These interactions can influence the galaxies' evolution through mechanisms like tidal forces and merger events, which can trigger star formation, fuel central black holes, and reshape the galaxies' structures.



Studying groups like the NGC 3783 group helps astronomers understand how <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a> evolve together in a common gravitational environment, offering insights into the dynamics and evolution of structures on cosmic scales. 



Image Credit: ESA/Hubble &amp; NASA



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Luminous galaxy NGC 3783 and a blue giant star

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

Today's Image of the Day from NASA Earth Observatory features a 9.5-mile section of Pangong Lake on the western end of the Tibetan Plateau. The image was captured on by a crew member onboard the International Space Station.&nbsp;



“In this winter scene, a sheet of cracked ice tops part of the lake,” noted <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>. “On the left side, open water appears blue. Shallow water offshore of a delta, formed by a small, winding river, appears green."



"Parallel lines along the coastlines of bays are visible in the high-resolution version of this image. These lines indicate raised beaches, which formed in the past when lake levels were higher.”



NASA pointed out that several roads cut across the landscape, including one with switchbacks that ascends a steep slope. "These roads facilitate tourist travel from both India and China.”&nbsp;



<h2 class="wp-block-heading" id="h-migratory-birds-at-pangong-lake-nbsp">Migratory birds at Pangong Lake&nbsp;</h2>



Pangong Lake and its surroundings are home to numerous bird species, particularly <a href="https://www.earth.com/news/migratory-birds-burn-unexpected-amounts-of-protein/" target="_blank" rel="noreferrer noopener">migratory birds</a>. Visitors can spot various waterfowl and waders that are rarely seen elsewhere.



“During the summer, species such as bar-headed geese and Brahminy ducks attract bird watchers to the lake, which is a major breeding ground for migrating birds,” said NASA.



Pangong Lake is one of the few places in India where the endangered black-necked crane is found during its breeding season. 



Ruddy shelduck and brown-headed <a href="https://www.earth.com/news/gulls-are-shifting-their-habitats-to-urban-areas/" target="_blank" rel="noreferrer noopener">gulls</a> are also frequently spotted around the lake. The ruddy shelduck is known for its striking orange-brown body and creamy white head, while the brown-headed gulls are often seen flying or swimming in the lake.



<h2 class="wp-block-heading" id="h-pangong-lake-nbsp">Pangong Lake&nbsp;</h2>



Pangong Lake is a stunning high-altitude lake situated in the <a href="https://www.earth.com/news/temperatures-are-rising-unexpectedly-fast-on-the-tibetan-plateau/" target="_blank" rel="noreferrer noopener">Himalayas</a>, extending from India to the Tibetan Autonomous Region of China. It is renowned for its mesmerizing beauty and dramatic setting, with the lake lying at an elevation of about 4,350 meters.



One of the most distinctive features of Pangong Lake is its changing colors, ranging from shades of blue to green and even red, influenced by the sky's reflection and the lake's mineral content.



This saline water lake is approximately 134 kilometers long and 5 kilometers wide at its broadest point. Despite its considerable size, Pangong Lake is relatively shallow. 



The lake gained additional popularity after being featured in several Indian films - most notably the Bollywood hit "3 Idiots." Its remote location requires a permit for visitors, especially due to its proximity to the Line of Actual Control between India and China.



Despite the geopolitical sensitivities surrounding its location, Pangong Lake remains a favorite among tourists for its unparalleled natural beauty and serene environment.



<h2 class="wp-block-heading" id="h-high-altitude-lakes">High-altitude lakes</h2>



High-altitude lakes are unique bodies of water found at elevations typically above 3,000 meters (about 10,000 feet) in mountain ranges like the <a href="https://www.earth.com/news/himalayan-glaciers-retreating-threat-is-much-worse-than-previously-believed/" target="_blank" rel="noreferrer noopener">Himalayas</a>, Andes, and Rockies. 



These lakes are formed either by glacial activity, where glaciers erode the earth to create depressions that fill with melted snow and rainwater, or when natural dams created by landslides or moraines trap water in valleys.



<h3 class="wp-block-heading" id="h-extreme-environments">Extreme environments</h3>



The conditions at high altitudes make these lakes distinct in several ways. The climate is typically colder and harsher, with significant temperature variations between day and night. 



This extreme environment affects both the physical characteristics of the <a href="https://www.earth.com/news/alarming-study-most-of-the-worlds-largest-lakes-are-quickly-losing-water/" target="_blank" rel="noreferrer noopener">lakes</a> and the types of ecosystems they support. For example, due to lower atmospheric pressure, the boiling point of water is reduced, which can affect the type of life that can survive in these regions.



<h3 class="wp-block-heading" id="h-critical-habitats">Critical habitats</h3>



Biologically, high-altitude lakes often have limited biodiversity because only certain types of plants and animals can tolerate the cold temperatures and lower oxygen levels in the water. 



Despite this, these lakes are crucial habitats for some unique species of fish, birds, and other wildlife. They also serve as important indicators of climate change, as variations in their water levels and temperatures can reflect environmental shifts.



<h3 class="wp-block-heading" id="h-significance-of-high-altitude-lakes">Significance of high-altitude lakes </h3>



Lakes at high altitudes are often clear and pristine, due to the low density of human populations in these areas and minimal industrial activity, making them significant for ecological studies and attractive for tourism. 



However, they are sensitive ecosystems, and increased tourist activity brings challenges like pollution and habitat disruption.



High-altitude lakes are not only beautiful and scientifically significant but also hold cultural importance for local communities, often considered sacred and associated with historical and spiritual significance.



Image Credit: NASA Earth Observatory&nbsp;



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Pangong Lake on the Tibetan Plateau

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

Today's Image of the Day from the European Space Agency features the aftermath of devastating floods in the Valencia region of Eastern Spain.&nbsp;



On October 29, 2024, torrential rainfall unleashed nearly a year’s worth of precipitation in just eight hours, leading to catastrophic flash floods that affected a vast area from Málaga to Valencia. 



<h2 class="wp-block-heading" id="h-flash-floods-in-valencia">Flash floods in Valencia </h2>



<a href="https://www.earth.com/news/flash-floods-are-set-to-become-much-more-common-in-the-u-s/">Floodwaters</a> submerged entire neighborhoods and agricultural lands. Many roads and infrastructure were overwhelmed almost instantly, stranding vehicles and prompting widespread evacuations. Water levels rose faster than emergency services could respond.



One resident of Paiporta, near Valencia, told the BBC that when the water started to rise it was "like a tsunami wave."



“In a matter of minutes, flash floods caused by heavy downpours in eastern Spain swept away everything in their path. With no time to react, people were trapped in vehicles, homes and businesses,” reported the Associated Press.



More than 200 people were killed and thousands of people were rescued. According to SOS Desaparecidos, as many as 1,300 people remained unaccounted for on Friday, three days after the floods.



<h2 class="wp-block-heading" id="h-magnitude-of-the-tragedy-nbsp">Magnitude of the tragedy&nbsp;</h2>



Ángel Víctor Torres, the Minister for Territorial Policy and Democratic Memory, said: “The fact that we can’t give a number of the missing persons indicates the magnitude of the tragedy.”&nbsp;



Some areas, including the Spanish town of Alfafar, are completely cut off from communication.&nbsp;



Juan Ramón Adsuara, the mayor of Alfafar, said the aid isn't nearly enough for residents trapped in an "extreme situation."



"There are people living with corpses at home. It's very sad. We are organizing ourselves, but we are running out of everything," Adsuara told reporters. "We go with vans to Valencia, we buy and we come back, but here we are totally forgotten."



<h2 class="wp-block-heading" id="h-government-warning-was-not-issued-in-time">Government warning was not issued in time</h2>



On Tuesday morning, Spain's meteorological agency Aemet warned that torrential rains were forecast for the region of Valencia, before issuing a&nbsp; "maximum red alert.”



Carlos Mazon, Valencia’s regional president, said the government sent out an SMS alert reserved for the “worst possible scenario.” But according to a report from CNN, that alert was sent hours too late.



“By 5 p.m., Valencia’s emergency services were swamped by hundreds of pleas for help throughout the region,” wrote Atika Shubert, a CNN Senior International Correspondent.



“It was at 8 p.m. that cell phones finally buzzed with the public alert telling residents to stay indoors. Much too little, much too late, even for those downstream of the raging water who might otherwise have had time to prepare.”



The BBC also noted that many people have questioned the timing of the government's warning, which arrived more than 12 hours after Aemet issued its first red alert.



<h2 class="wp-block-heading" id="h-extreme-weather-in-a-warming-climate">Extreme weather in a warming climate</h2>



The deadly floods in Valencia were primarily caused by an extreme weather event that brought record-breaking <a href="https://www.earth.com/news/extreme-rainfall-events-are-interconnected-around-the-globe/">rainfall</a>. The intense downpour was fueled by unusually warm Mediterranean Sea temperatures, which increased moisture in the atmosphere and intensified the rainfall.&nbsp;



Climate experts link this phenomenon to climate change, as warmer seas lead to more frequent, severe storms. The combination of heavy rain and the region's limited drainage capacity led to flash flooding, overwhelming local <a href="https://www.earth.com/news/predicting-floods-its-not-just-about-rainfall/">infrastructure</a>.



Rising ocean temperatures are largely driven by increased greenhouse gases that trap more heat in the atmosphere. Oceans absorb about 90% of this excess heat, leading to warmer waters, especially near the surface.&nbsp;



This warming disrupts marine ecosystems, contributing to coral bleaching and altering habitats for species like fish and marine mammals.



With the <a href="https://www.earth.com/news/can-we-outrun-the-flood-risks-of-climate-change/">climate crisis</a> intensifying, experts warn that warmer ocean temperatures will heighten the risk of rapid, destructive rainfall events.



<h2 class="wp-block-heading" id="h-second-deadliest-flood-in-europe-this-century-nbsp">Second-deadliest flood in Europe this century&nbsp;</h2>



Prime Minister Pedro Sanchez said the disaster was the second-deadliest flood in Europe this century and that Spain was carrying out its largest deployment of army and security force personnel in peacetime. The country was sending 5,000 soldiers and 5,000 police officers to the eastern region of Valencia on Saturday.



Four days after the devastating floods, rescuers are still searching for bodies. Thousands of volunteers are helping to clean up the thick mud that covers streets, homes, and businesses in the hardest-hit towns.&nbsp;



Prime Minister Sanchez responded to people who expressed they feel abandoned with no help or communication in the days following the tragic flooding.



“I am aware the response is not enough, there are problems and severe shortages… towns buried by mud, desperate people searching for their relatives.”



"For those who at this moment are still looking for their loved ones, the whole of Spain weeps with you."



According to <a href="https://www.esa.int/">ESA</a>, the Copernicus Emergency Rapid Mapping Service has been activated to provide satellite imagery that can support rescue and recovery efforts.



Image Credit: USGS, processed by ESA&nbsp;



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Valencia floods: A tragedy fueled by extreme weather

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

Today's Image of the Day from the European Southern Observatory (ESO) features the Dark Wolf Nebula, located around 5,300 light-years from Earth in the constellation Scorpius.



According to ESO, this image of the dark <a href="https://www.earth.com/news/scientists-reveal-the-ring-nebula-as-it-has-never-been-seen-before/" target="_blank" rel="noreferrer noopener">nebula</a> creates the illusion of a wolf-like silhouette against a colorful cosmic backdrop. 



“This image takes up an area in the sky equivalent to four full Moons, but is actually part of an even larger nebula called Gum 55. If you look closely, the wolf could even be a werewolf, its hands ready to grab unsuspecting bystanders,” noted <a href="https://www.eso.org/public/" target="_blank" rel="noreferrer noopener">ESO</a>.



<h2 class="wp-block-heading" id="h-dark-nebulae-nbsp">Dark nebulae&nbsp;</h2>



Dark nebulae are dense regions in space filled with gas and dust that absorb visible light, making them appear as dark patches against brighter backgrounds.&nbsp;



Unlike emission or reflection nebulae, dark nebulae do not glow on their own. Instead, they obstruct and obscure the light from stars and other objects lying behind them.&nbsp;



This characteristic makes them challenging to observe using visible-light telescopes, as they absorb and scatter light rather than reflecting or emitting it.&nbsp;



However, when viewed in infrared, where their obscuring effect is reduced, dark nebulae reveal intricate details about the <a href="https://www.earth.com/news/building-blocks-of-life-found-in-the-perseus-cloud/" target="_blank" rel="noreferrer noopener">molecular clouds</a> they contain.



According to ESO, astronomers study these clouds of frozen dust because they often contain new stars in the making.



<h2 class="wp-block-heading" id="h-dark-wolf-nebula-nbsp">Dark Wolf Nebula&nbsp;</h2>



The Dark Wolf Nebula is part of a larger complex known as the Lupus Molecular Cloud, one of several significant star-forming regions close to Earth.&nbsp;



Inside of dark nebulae, the conditions are prime for star formation. The dense gas and dust clump together under gravitational forces, and as the clouds contract, they heat up, eventually igniting nuclear fusion and forming <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">new stars</a>.



The Dark Wolf Nebula is known for revealing young, low-mass stars, or T Tauri stars, which are in the early stages of their evolution. These stars are still surrounded by disks of material that may eventually form new planets.



This nebula is typically studied in infrared, which allows scientists to look beyond the obscuring dust to observe the processes of star formation.&nbsp;



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



Scorpius is one of the most recognizable constellations in the sky. It resembles a scorpion with a long, curved tail and stinger.&nbsp;



Located in the southern sky, Scorpius is especially visible during the summer months in the Northern Hemisphere and winter in the Southern Hemisphere.&nbsp;



The constellation is often associated with the story of Orion in Greek mythology. According to legend, the scorpion was sent by the goddess Artemis to kill Orion, the great hunter, either as punishment for his arrogance or to protect her animals, depending on the version of the tale.&nbsp;



The gods later placed both <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a> and Scorpius in the sky, but in opposite parts of the heavens so they would never be seen together - as Scorpius rises in the east and Orion sets in the west.



Scorpius contains several notable stars and deep-sky objects. Its brightest star, Antares, is a red supergiant often referred to as the "Heart of the Scorpion" due to its reddish hue and central position.&nbsp;



Antares is one of the largest visible stars in the sky and has a luminosity tens of thousands of times greater than that of our Sun.&nbsp;



Scorpius is located close to the core of the Milky Way, making it a rich region for star clusters and nebulae. Among these are the Butterfly Cluster and the Ptolemy Cluster, both of which are visible to the naked eye under dark skies.



<h2 class="wp-block-heading" id="h-image-of-the-dark-wolf-nebula">Image of the Dark Wolf Nebula </h2>



“This image shows in spectacular detail how the dark wolf stands out against the glowing star-forming clouds behind it,” noted ESO.



“The colorful clouds are built up mostly of hydrogen gas and glow in reddish tones excited by the intense UV radiation from the newborn stars within them.”



The picture was created from images taken at different times. Each of the images has a filter that makes a different color of light visible.&nbsp;



Observations of the Dark Wolf Nebula provide astronomers with valuable information about the <a href="https://www.earth.com/news/massive-star-redefines-our-understanding-of-stellar-evolution/" target="_blank" rel="noreferrer noopener">evolution of stars</a> and the environments in which they form.



The image was captured by the VLT Survey Telescope (VST) at ESO’s Paranal Observatory in Chile.



Image Credit: ESO/VPHAS+ team



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Dark Wolf Nebula in the constellation Scorpius

Today's Image of the Day from the European Southern Observatory...

Today's Image of the Day from the European Space Agency features an incredible new image of the Crab Nebula in bright neon colors. 



“The unusual image was produced by combining data from telescopes spanning nearly the entire electromagnetic spectrum, from radio waves to X-rays,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>. 



Colored in red, the Karl G. Jansky Very Large Array (VLA) provided information about the nebula gathered in the radio regime.



NASA’s Spitzer Space Telescope took infrared images, which appear yellow, while the NASA/ESA <a href="https://www.earth.com/news/hubble-captures-another-cosmic-masterpiece-in-galaxy-ngc-2217/" target="_blank" rel="noreferrer noopener">Hubble</a> Space Telescope provided images made in optical wavelengths, colored in green.&nbsp;



Blue colors represent ultraviolet observations made by ESA’s XMM-Newton telescope, and the purple colors are X-ray radiation data from NASA’s Chandra X-ray Observatory.



<h2 class="wp-block-heading" id="h-about-the-crab-nebula-nbsp">About the Crab Nebula&nbsp;</h2>



The Crab Nebula, located in the constellation Taurus, contains the remnants of a <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova explosion</a> first observed on Earth in 1054 AD. This explosion was recorded by Chinese astronomers and possibly by Native American rock art.&nbsp;



The nebula spans about 11 light-years across and lies approximately 6,500 light-years away from Earth. It is one of the most <a href="https://www.earth.com/news/unraveling-the-mysterious-origins-of-the-crab-nebula/" target="_blank" rel="noreferrer noopener">studied objects</a> in the sky, largely due to its status as a bright and dynamic supernova remnant.&nbsp;



<h2 class="wp-block-heading" id="h-the-crab-pulsar">The Crab Pulsar</h2>



The Crab Nebula contains a pulsar at its center, which is a rapidly rotating <a href="https://www.earth.com/news/slow-spinning-neutron-star-completely-defies-our-expectations/" target="_blank" rel="noreferrer noopener">neutron star</a> that emits pulses of radiation. This pulsar, known as the Crab Pulsar, spins about 30 times per second and is a significant source of gamma rays and other forms of high-energy radiation.&nbsp;



The nebula itself is a complex structure of filaments and synchrotron radiation. The filaments are remnants of the original star's outer layers, while the synchrotron radiation emerges from electrons spiraling in the magnetic fields produced by the pulsar.



“Surrounding the pulsar lies a mix of material; some of it was originally expelled from the star before it went supernova, and the rest was ejected during the explosion itself,” explained ESA.&nbsp;



“Fast-moving winds of particles fly off from the neutron star, energizing the dust and gas around it. These different layers and intricacies of the nebula can be observed in all of the different wavelengths of light.”



<h2 class="wp-block-heading" id="h-crab-nebula-observation-nbsp">Crab Nebula observation&nbsp;</h2>



Throughout its history, the Crab Nebula has provided critical insights into the processes of stellar death, the behavior of <a href="https://www.earth.com/news/pulsars-are-helping-astronomers-pinpoint-dark-matter/" target="_blank" rel="noreferrer noopener">pulsars</a>, and the mechanics of supernova remnants.&nbsp;



Its continuous observation has revealed changes over time, such as the expansion of its filaments and variations in its brightness, offering a dynamic laboratory for astrophysical studies.



Overall, the Crab Nebula is a highly energetic and object, providing valuable insights into the processes following a supernova explosion.



<h2 class="wp-block-heading" id="h-fascinating-facts-about-nebulae">Fascinating facts about nebulae</h2>



Nebulae are some of the most breathtaking and intriguing structures in the universe. They are vast clouds of gas and dust, often considered stellar nurseries where new stars are born. 



<h3 class="wp-block-heading" id="h-colors-of-nebulae">Colors of nebulae </h3>



One of the most fascinating aspects of nebulae is their ability to glow in different colors. This occurs because they either reflect the light of nearby stars or emit light due to the ionization of gases within them, particularly hydrogen. 



Some nebulae, like the famous Orion Nebula, are visible to the naked eye and serve as one of the nearest regions of active star formation.



<h3 class="wp-block-heading" id="h-planetary-nebulae">Planetary nebulae </h3>



Stars are born in dense regions of nebulae, and when they die, some will expel their outer layers, creating stunning structures known as planetary nebulae. The colorful clouds left behind can shine brightly for thousands of years. 



<h3 class="wp-block-heading" id="h-massive-size">Massive size</h3>



Another amazing fact is that some nebulae are so vast that light can take years to travel from one side to the other, stretching across hundreds of light-years.



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



Perhaps even more mind-boggling is the fact that nebulae are the remnants of previous generations of stars. Supernova explosions of massive stars can create these glowing clouds of gas and dust, seeding the cosmos with the elements necessary for the formation of new stars and planets.



Image Credit: NASA, ESA, G. Dubner (IAFE, CONICET-University of Buenos Aires) et al.; A. Loll et al.; T. Temim et al.; F. Seward et al.; VLA/NRAO/AUI/NSF; Chandra/CXC; Spitzer/JPL-Caltech; XMM-Newton/ESA; and Hubble/STScI



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Crab Nebula: The remains of a massive star explosion

Today's Image of the Day from the European Space Agency features the star-forming region NGC 604, which is located 2.73 million light-years away from Earth in the Triangulum Galaxy (M33). The image was captured by the James Webb Space Telescope.



By studying regions like NGC 604, astronomers can gain insights into the complex interactions between stars and the interstellar medium, as well as the conditions that lead to the birth of stars. This, in turn, helps in understanding the evolution of <a href="https://www.earth.com/news/galaxies-like-our-own-milky-way-are-not-unique/" target="_blank" rel="noreferrer noopener">galaxies</a> and the universe as a whole.



<h2 class="wp-block-heading" id="h-massive-stars-of-ngc-604">Massive stars of NGC 604</h2>



"Sheltered among NGC 604’s dusty envelopes of gas are more than 200 of the hottest, most massive kinds of stars, all in the early stages of their lives," said <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"These types of stars are known as B-types and O-types, the latter of which can be more than 100 times the mass of our own Sun. It’s quite rare to find this concentration of them in the nearby universe. In fact, there’s no similar region within our own Milky Way galaxy."



According to ESA, this concentration of massive stars, combined with its relatively close distance, means NGC 604 gives astronomers an opportunity to study these objects at a fascinating time early in their life.



<h2 class="wp-block-heading" id="h-gigantic-region-of-ionized-hydrogen">Gigantic region of ionized hydrogen</h2>



NGC 604 is one of the largest known regions of ionized hydrogen, also known as an H II region. This nebula is significantly larger than the Orion Nebula, which is one of the most well-known H II regions in our own <a href="https://www.earth.com/news/large-amount-of-dark-matter-may-be-missing-from-the-milky-way/" target="_blank" rel="noreferrer noopener">Milky Way galaxy</a>.&nbsp;



NGC 604 spans about 1,500 light-years across, making it one of the largest H II regions in the Local Group of galaxies. This group includes the Milky Way, the Andromeda Galaxy, and about 54 other smaller galaxies. 



<h2 class="wp-block-heading" id="h-ngc-604-starburst-phenomenon">NGC 604 starburst phenomenon </h2>



Within NGC 604, there are hundreds of young, hot, massive <a href="https://www.earth.com/news/stars-at-the-edge-of-our-milky-way-galaxy-travel-more-slowly/" target="_blank" rel="noreferrer noopener">stars</a>. These stars have ionized the surrounding gas, causing it to glow and creating the nebula. The region is a prime example of a starburst phenomenon, where stars form at a much higher rate than in typical galactic conditions.



“The bright orange streaks in this image signify the presence of carbon-based molecules known as polycyclic aromatic hydrocarbons, or PAHs," explained ESA.



"As you travel further from the immediate cavities of dust where the star is forming, the deeper red signifies molecular hydrogen. This cooler gas is a prime environment for star formation. Ionized hydrogen from ultraviolet radiation appears as a white and blue ghostly glow."



<h2 class="wp-block-heading" id="h-more-about-star-formation">More about star formation </h2>



Star formation is crucial for the evolution of galaxies and the synthesis of heavy elements. In the cores of stars, elements heavier than helium are created.



The elements are spread throughout the <a href="https://www.earth.com/news/ancient-stars-shakti-shiva-shaped-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">galaxy</a> when stars reach the end of their lives and expel their material - either gently through winds or violently via supernova explosions. This enriching process allows for the formation of new stars and planets, and ultimately, the potential for life.



<h3 class="wp-block-heading">Cloud collapse</h3>



The process begins when part of a molecular cloud becomes unstable and starts to collapse under its own gravity. This can be triggered by events like shock waves from nearby <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernovae</a>, galactic collisions, or the influence of other massive stars.



<h3 class="wp-block-heading">Formation of a protostar</h3>



As the cloud collapses, it fragments into smaller clumps. Each clump will eventually form one or more stars. 



The material within these clumps continues to fall inward, heating up as it does so, eventually forming a warm core called a protostar. At this stage, the protostar is not yet hot enough for nuclear fusion (the process that powers stars) to occur.



<h3 class="wp-block-heading">Accretion disk</h3>



Around the protostar, material from the surrounding cloud continues to fall inward, forming a rotating disk. This material slowly accretes onto the protostar, increasing its mass.



<h3 class="wp-block-heading">Nuclear fusion begins</h3>



Once the core of the protostar reaches a high enough temperature and pressure, hydrogen atoms begin to fuse into helium, releasing energy in the process. This marks the transition from a protostar to a main sequence star, like our sun.



<h3 class="wp-block-heading">Main sequence and beyond</h3>



The star will spend the majority of its life in the main sequence stage, where it balances the gravitational forces trying to collapse it and the outward pressure from nuclear fusion. 



Eventually, the star will exhaust its hydrogen fuel. Its subsequent evolution will depend on its initial mass, leading to various end stages such as red giants, supernovae, neutron stars, or black holes.



Image Credit: NASA/ESA/CSA James Webb Space Telescope



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Young, massive stars in the Triangulum Galaxy

Today's Image of the Day from the European Space Agency features a false-color radar depiction of central Ethiopia.



According to ESA, the photograph is a blend of multiple Sentinel-1 images from spring, summer and autumn 2023, which have been overlaid to create this single image.



“Radar images capture surface texture rather than reflected light so they are naturally black and white but here images from each season have been assigned a different color: red, green and blue respectively,” explained <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“When the images are combined, the different colors reveal variations that occurred in the different seasons.”



<h2 class="wp-block-heading" id="h-rugged-terrain-of-central-ethiopia-nbsp">Rugged terrain of central Ethiopia&nbsp;</h2>



ESA noted that Ethiopia’s terrain is one of the most rugged in Africa. The landscape is primarily characterized by highlands and plateaus.&nbsp;



The Ethiopian Highlands, also known as the Roof of Africa, dominate this region and include some of the highest peaks in Africa, such as Ras Dashen. The terrain features steep escarpments, deep valleys, and numerous rivers.&nbsp;



The central part of the country is also home to the Great Rift Valley, which runs through Ethiopia and includes a series of lakes and volcanic mountains. The region's varied topography contributes to its rich biodiversity and distinct climate zones.



<h2 class="wp-block-heading" id="h-lakes-of-central-ethiopia-nbsp">Lakes of central Ethiopia&nbsp;</h2>



According to ESA, water bodies appear dark in this image because flat water surfaces reflect the radar signal away from the satellite. “The various colors visible in some lakes are due either to the changing surface currents and sediments from rivers or to variations in water level.”



Lake Ziway is one of the largest <a href="https://www.earth.com/news/africas-flamingos-at-risk-due-to-rising-lake-levels/" target="_blank" rel="noreferrer noopener">lakes</a> in the region. It is located about 160 kilometers south of Addis Ababa, the capital of Ethiopia.&nbsp;



The lake is known for its rich bird diversity, including large populations of pelicans, cormorants, and herons. Lake Ziway also supports local fishing communities.



Lake Shala is the deepest lake in the Ethiopian Rift Valley and is known for its volcanic origins. It has a maximum depth of 266 meters and is surrounded by hot springs and steep, rocky cliffs.



<h2 class="wp-block-heading" id="h-climate-of-central-ethiopia-nbsp">Climate of central Ethiopia&nbsp;</h2>



Central Ethiopia features a diverse climate, primarily influenced by its elevation and geographical location within the tropics.



<h3 class="wp-block-heading" id="h-highland-climate">Highland climate</h3>



Much of central Ethiopia consists of highlands, with elevations ranging from 1,500 to over 3,000 meters above sea level. These highlands experience a temperate climate, with cooler <a href="https://www.earth.com/news/temperatures-in-africa-are-rising-above-levels-that-rhinoceros-can-tolerate/" target="_blank" rel="noreferrer noopener">temperatures</a> compared to the lowlands.&nbsp;



The average temperatures range from 50 to 68 degrees Fahrenheit. The higher elevations, such as those found in the Ethiopian Highlands, can experience temperatures that are close to freezing at night.



<h3 class="wp-block-heading" id="h-rainy-seasons">Rainy seasons</h3>



Central Ethiopia has two main rainy seasons. The primary rainy season, known as the "Kiremt," occurs from June to September and brings the majority of the annual rainfall.&nbsp;



The "Belg," or short rainy season, occurs from March to May. The rainfall during these periods supports agriculture, which is a key part of the region's economy.



<h3 class="wp-block-heading" id="h-dry-season">Dry season</h3>



The <a href="https://www.earth.com/news/africas-wet-forests-have-seen-an-alarming-rise-in-wildfires/" target="_blank" rel="noreferrer noopener">dry season</a>, known as the "Bega," spans from October to February.&nbsp;During this time, the region experiences significantly less rainfall, and the weather tends to be sunny and dry. 



<h2 class="wp-block-heading" id="h-culture-of-central-ethiopia-nbsp">Culture of central Ethiopia&nbsp;</h2>



The <a href="https://www.earth.com/news/humans-are-not-the-only-animals-that-create-their-own-culture/" target="_blank" rel="noreferrer noopener">culture</a> of central Ethiopia is a dynamic blend of ancient traditions and modern influences. This culture is characterized by a strong sense of community and a profound connection to the region's historical and spiritual roots.



The Amhara people have played a significant role in the cultural and political life of central Ethiopia. The Amhara are known for their rich heritage, which includes the Amharic language, a Semitic tongue that serves as one of the country's official languages.



Orthodox Christianity is a key aspect of central Ethiopian culture, particularly among the Amhara and other highland communities.&nbsp;



This part of East Africa is also known for its traditional music and dance, which reflect the region's historical depth and cultural diversity.&nbsp;



The cuisine of central Ethiopia is another significant cultural aspect, with injera (a spongy flatbread made from teff) being a staple food.&nbsp;Injera is typically served with a variety of stews (wats) and salads.



The communal eating experience, where meals are shared from a single large plate, emphasizes the importance of community and togetherness.



Image Credit: ESA&nbsp;



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The vibrant seasons of central Ethiopia

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

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

Heavy snow and cloud cover in the Alps

Monitoring Earth Changes with MODIS

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

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

A frozen Lake Erie in February

Aqua Earth Observing Satellite

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

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

Super Typhoon Noru in the Pacific Ocean

Incredible Images of Earth from Space

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

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

Northern Italy from the Space Station

Photos from the International Space Station

A comprehensive review study has recently investigated the vital connections between marine biodiversity conservation, human health, and well-being. According to the experts, marine protected areas (MPAs) not only support ecological balance but also provide tangible benefits for people, underscoring their dual importance.



<h2 class="wp-block-heading" id="h-marine-protected-areas-nbsp">Marine protected areas&nbsp;</h2>



Marine protected areas are legally designated sections of the ocean recognized for their conservation value. These areas are protected by laws that restrict human activities, aiming to allow ecosystems to thrive without significant interference. 



Depending on the specific regulations of an <a href="https://www.earth.com/news/marine-protected-areas-fall-short-on-2030-biodiversity-targets/" target="_blank" rel="noreferrer noopener">MPA</a>, activities like fishing, building, or oil drilling may be prohibited or limited. The overarching goal is to create a space where marine life can flourish and, in turn, contribute to ecological and human welfare.



<h2 class="wp-block-heading" id="h-expanding-ocean-protection">Expanding ocean protection</h2>



With global plans to extend MPAs as part of the UN's “30x30” initiative - seeking to protect 30% of the world's oceans and land by 2030 - understanding the impact of these areas on both people and nature has become increasingly important.&nbsp;



The new study, conducted by the <a href="https://www.worldwildlife.org/" target="_blank" rel="noreferrer noopener">World Wide Fund for Nature</a>, <a href="https://www.harvard.edu/" target="_blank" rel="noreferrer noopener">Harvard University</a>’s School of Public Health, and <a href="https://duke.edu/" target="_blank" rel="noreferrer noopener">Duke University</a>’s marine laboratory, led by Daniel Viana, reviewed data from over 200 scientific articles published since 1973.



The team discovered that in 234 MPAs worldwide, more than 60% reported improvements in both conservation outcomes and <a href="https://www.earth.com/news/world-environment-day-the-critical-role-of-nature-in-human-well-being/" target="_blank" rel="noreferrer noopener">human well-being</a>. This finding suggests that well-managed MPAs can simultaneously support nature and the communities that depend on marine resources.



<h2 class="wp-block-heading" id="h-protected-areas-and-local-communities-nbsp">Protected areas and local communities&nbsp;</h2>



The study also included MPAs that permit sustainable use through controlled <a href="https://www.earth.com/news/sustainable-fishing-gets-a-boost-from-genomics-roadmap/" target="_blank" rel="noreferrer noopener">fishing</a> practices that avoid harming delicate ecosystems. These measures, such as using hook-and-line methods or fish traps, minimize damage to coral reefs and other sensitive habitats. 



The research suggests that investing in MPAs often results in benefits for local communities, particularly in terms of fishing yields and food access.



MPAs play an essential role in small island nations like Bonaire, Palau, and the Cook Islands. These regions, where over 95% of fish catches are tied to area-based conservation, illustrate how marine protection can drive both ecological and economic gains.&nbsp;



However, the study noted that despite the evident link between MPAs and improved food access, few studies have measured the direct nutritional impact on local communities.&nbsp;



Only one research project in the Philippines established a connection between enhanced fish access and better health outcomes, finding reduced rates of childhood stunting.



<h2 class="wp-block-heading" id="h-nutrient-contributions-of-protected-areas-nbsp">Nutrient contributions of protected areas&nbsp;</h2>



The world’s waters - rivers, seas, lakes, and floodplains - are rich in edible plants and animals that offer essential vitamins, minerals, and <a href="https://www.earth.com/news/insects-provide-essential-fatty-acids-to-other-animals/" target="_blank" rel="noreferrer noopener">fatty acids</a>. These nutrients, particularly when harvested sustainably, can significantly bolster the diets of coastal populations. 



The study quantified the nutrient contributions from foods within MPAs, revealing that even with just 8% of the oceans under protection, these areas contribute 14% of the global supply of six key micronutrients from marine sources.



By fostering healthy marine environments, MPAs enhance fish populations that can spill over into adjacent areas, leading to more robust catches, increased income from fishing, and better access to nutritious food.



<h2 class="wp-block-heading" id="h-challenges-and-complexities">Challenges and complexities</h2>



While MPAs offer considerable benefits, implementing them effectively is not without challenges. The study found that many MPAs lack effective management, which can limit their success.&nbsp;



Additionally, while MPAs help support marine life and nearby human communities, they do not directly address significant threats like <a href="https://www.earth.com/news/marine-protected-areas-were-not-designed-for-climate-resilience/" target="_blank" rel="noreferrer noopener">climate change</a> and pollution that require broader action.



<a href="https://www.earth.com/news/aquaculture-impacts-wild-fish-much-more-than-we-thought/" target="_blank" rel="noreferrer noopener">Aquaculture</a>, or the farming of aquatic organisms, is growing as a supplement to wild harvests to meet the increasing demand for aquatic food. Although it provides more than half of the aquatic food consumed globally, aquaculture must continue to advance in sustainability practices. 



The study also emphasized that in many developing coastal nations, wild-harvested food remains a critical source of nutrition for millions.



<h2 class="wp-block-heading" id="h-marine-protected-areas-and-global-health">Marine protected areas and global health</h2>



Linking marine conservation to human health presents promising opportunities but also reveals research gaps. While MPAs can contribute to better health outcomes by boosting fish availability and nutrient intake, questions remain about the equitable distribution of these benefits.&nbsp;



For instance, in the Maldives, the majority of fish caught from reefs are consumed by tourists rather than local residents, illustrating potential disparities.



Despite these challenges, the study underscores the potential of MPAs to promote a regenerative relationship between people and the environment.&nbsp;



By managing fisheries to support nutritional health rather than merely maximizing profits, a “nutrition-sensitive” approach to marine conservation could help address global food security.



In conclusion, while MPAs cannot tackle all threats alone, their role in sustaining both marine ecosystems and human communities represents a promising path toward a balanced, health-focused future.



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How marine protected areas boost human health

A comprehensive review study has recently investigated the vital connections...

Recent studies on the Thwaites Glacier, infamously known as the “Doomsday Glacier,” have fueled discussions on potential solutions to mitigate climate change impacts, including controversial geoengineering approaches.&nbsp;



The glacier’s stability is pivotal because its collapse could lead to catastrophic sea level rise, threatening millions.



<h2 class="wp-block-heading" id="h-accelerated-melting-of-doomsday-glacier">Accelerated melting of Doomsday Glacier </h2>



One key <a href="https://dx.doi.org/10.1073/pnas.2404766121" target="_blank" rel="noreferrer noopener">study</a>, led by researchers from the <a href="https://uci.edu/" target="_blank" rel="noreferrer noopener">University of California Irvine</a> and <a href="https://uwaterloo.ca/" target="_blank" rel="noreferrer noopener">University of Waterloo</a> and published in May, highlighted how warming <a href="https://www.earth.com/news/ocean-warming-is-subtly-changing-the-tides/" target="_blank" rel="noreferrer noopener">tidal currents</a> are accelerating Thwaites' melting faster than many models anticipated. 



Situated along the marine edge of the West Antarctic Ice Sheet (WAIS), the <a href="https://www.earth.com/news/doomsday-glacier-may-collapse-sooner-than-we-thought/" target="_blank" rel="noreferrer noopener">Thwaites Glacier</a> acts as a critical barrier. The glacier's retreat, fueled by climate change, already contributes to 4% of global sea level rise, losing about 50 billion tons of ice annually.



The WAIS itself, a vast ice sheet sitting below sea level, could raise sea levels by nearly 11 feet if it collapses. This would have dire implications for major coastal cities and vulnerable island nations.&nbsp;



The potential breaching of Thwaites represents a tipping point - a situation where crossing a critical climate threshold leads to rapid, potentially irreversible changes.



<h2 class="wp-block-heading" id="h-doomsday-glacier-stability">Doomsday Glacier stability</h2>



Amid these concerning findings, a more recent <a href="https://dx.doi.org/10.1126/sciadv.ado7794" target="_blank" rel="noreferrer noopener">study</a> led by <a href="https://home.dartmouth.edu/" target="_blank" rel="noreferrer noopener">Dartmouth College</a> and the <a href="https://www.ed.ac.uk/" target="_blank" rel="noreferrer noopener">University of Edinburgh</a> offered a glimmer of hope. This study suggests that Thwaites may be less prone to a process known as marine ice cliff instability (MICI) than previously believed. 



The MICI theory proposes that tall, retreating ice cliffs are inherently unstable and likely to collapse, leading to accelerated glacier loss.&nbsp;



However, the researchers found that thinning ice may, in fact, slow the calving process, potentially stabilizing ice cliffs. This discovery underscores the need for refined models to improve predictions about WAIS behavior.



<h2 class="wp-block-heading" id="h-solutions-to-slow-glacial-retreat">Solutions to slow glacial retreat</h2>



The potential risks associated with Thwaites’ rapid melting have pushed scientists to consider geoengineering as a possible <a href="https://www.earth.com/news/should-we-risk-geoengineering-to-reverse-climate-change/" target="_blank" rel="noreferrer noopener">intervention</a>. 



Geoengineering involves altering the environment through technological and structural means to slow down or stop glacial retreat, even in the face of rising <a href="https://www.earth.com/news/global-temperatures-increase-scientists-plan-slow-down-rising-heat/" target="_blank" rel="noreferrer noopener">global temperatures</a>.



A <a href="https://climateengineering.uchicago.edu/wp-content/uploads/2024/05/Glacial-Climate-Intervention_A-Research-Vision.pdf" target="_blank" rel="noreferrer noopener">report</a> from the <a href="https://www.uchicago.edu/en" target="_blank" rel="noreferrer noopener">University of Chicago</a>’s Climate Systems Engineering Initiative, published in July, called for further research into glacier geoengineering as a response to the severe threats posed by rapidly receding glaciers. 



John Moore, an Arctic Center professor and co-author of the report, stressed the challenges faced by such approaches: “it will take 15 to 30 years for us to understand enough to recommend or rule out any [glacier geoengineering] interventions.”



<h2 class="wp-block-heading" id="h-radical-geoengineering-proposals">Radical geoengineering proposals</h2>



Among the proposed geoengineering strategies are large-scale interventions, such as constructing submarine curtains to block warm tidal currents from reaching glacier ice.&nbsp;



These curtains could be crafted from durable fabrics or created through a network of pipes releasing air bubbles to act as a barrier.



Gernot Wagner, a climate economist at the Columbia Climate School, highlighted the potential of such interventions when executed correctly.&nbsp;



“For some polar <a href="https://www.earth.com/news/can-we-still-prevent-critical-climate-tipping-points/" target="_blank" rel="noreferrer noopener">tipping points</a> like Arctic sea ice and the WAIS, glacial geoengineering seems to be the only way for us to more or less guarantee that we can address these tipping points,” he said.



<h2 class="wp-block-heading" id="h-concerns-about-geoengineering-solutions">Concerns about geoengineering solutions</h2>



Despite the potential benefits, geoengineering has drawn criticism from glaciologists and climate experts who question its feasibility and warn that it may divert attention from critical emission-reduction efforts.&nbsp;



Concerns are that reliance on geoengineering could foster complacency, overshadowing the immediate need to reduce carbon emissions.



Wagner himself expressed mixed feelings, acknowledging that while the idea of using submarine curtains initially seemed "crazy," it could also serve as a wake-up call.&nbsp;



“You can use it as a push to say, ‘wait, if serious people are talking about [using curtains] as a solution, maybe we should be taking it more seriously and cutting emissions much more.’”



<h2 class="wp-block-heading" id="h-urgent-need-for-emission-reductions">Urgent need for emission reductions</h2>



Geoengineering, as Wagner succinctly put it, is not a cure-all. “When we talk about glacial geoengineering, we need to tell the truth, which is that it’s not a solution to climate change - at best, it’s a painkiller.”&nbsp;



This approach, while potentially buying time to stave off the most severe impacts, must be paired with aggressive measures to curb <a href="https://www.earth.com/news/global-carbon-dioxide-emissions-hit-a-record-high-in-2023/" target="_blank" rel="noreferrer noopener">global emissions</a>.



As research continues and new studies emerge, the fate of the Thwaites Glacier serves as a stark reminder of the delicate balance needed in addressing climate challenges.&nbsp;



While innovative solutions may offer temporary relief, the ultimate focus must remain on long-term strategies that promote sustainability and prevent reaching critical climate tipping points.



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Can geoengineering save the Doomsday Glacier?

Recent studies on the Thwaites Glacier, infamously known as the...

As plastic pollution reaches alarming levels in ecosystems worldwide, a new study traces this crisis back to decades of industrial growth.



The research, led by an interdisciplinary team of Penn State researchers, explores the rise of microplastics in freshwater environments and links it to a global increase in plastic production since the 1950s.



<h2 class="wp-block-heading" id="h-tracking-freshwater-microplastics">Tracking freshwater microplastics </h2>



The exports tracked microplastic levels in freshwater sediment back to the mid-20th century. They uncovered a clear link between rising microplastic concentrations and the global surge in plastic manufacturing.



“Ours is one of the first to track microplastic levels in freshwater sediment from before the 1950s to today, showing that concentrations rise in line with <a href="https://www.earth.com/news/plastic-production-increases-create-identical-plastic-pollution-increase/" target="_blank" rel="noreferrer noopener">plastic production</a>," said Nathaniel Warner, associate professor of civil and environmental engineering at Penn State.



<h2 class="wp-block-heading" id="h-focus-of-the-research">Focus of the research </h2>



Microplastics are minute particles of plastic that range from one hundredth the width of a human hair to roughly the size of a pencil eraser.



The study was primarily focused on sediment cores from four watersheds in Pennsylvania: Kiskiminetas River, Blacklick Creek, Raystown Lake, and Darby Creek. 



Interestingly, the team discovered that regardless of the population density or land use, high levels of microplastics could be found.



<h2 class="wp-block-heading" id="h-the-recycling-landscape-and-plastic-build-up">The recycling landscape and plastic build-up</h2>



Lisa Emili, associate professor of physical geography and environmental studies at Penn State Altoona, explained how the findings differed from previous studies.



“Based on other findings in the literature, what we thought would be important turned out not to be driving forces in microplastic variation across sites, notably the percentage of microplastics related to developed area and population density," said Emili.



The researchers found a decrease in microplastic accumulation from 2010 to 2020, a timeline that seems to align with increased <a href="https://www.earth.com/news/u-s-plastic-recycling-dropped-under-six-percent-in-2021/" target="_blank" rel="noreferrer noopener">recycling</a> efforts. 



Observations from the U.S. Environmental Protection Agency support this finding. The agency reported substantial expansion in plastic recycling efforts from 1980 to 2010.



<h2 class="wp-block-heading" id="h-the-mystery-of-missing-plastic">The mystery of missing plastic </h2>



Raymond Najjar, professor of oceanography at Penn State, believes this study can clarify the "<a href="https://www.earth.com/news/ocean-interior-has-accumulated-missing-plastics/" target="_blank" rel="noreferrer noopener">missing plastics</a>" paradox. This refers to the disparity between the estimated amounts of plastic waste entering the ocean annually and the visible amount that can be found floating on the ocean's surface.



Professor Najjar suggested that estuaries, particularly tidal marshes, could be trapping river-borne plastics preventing them from reaching the ocean. 



"This could explain why there is far less plastic floating around in the surface ocean compared to how much is expected to be there given the input to the ocean from rivers," said Professor Najjar.



<h2 class="wp-block-heading" id="h-need-to-reduce-plastic-consumption">Need to reduce plastic consumption </h2>



The research team predicts continued growth of microplastic concentrations in both water and sediment.



"<a href="https://www.earth.com/news/contamination-crisis-microplastics-found-in-88-of-protein-sources/" target="_blank" rel="noreferrer noopener">Humans are ingesting plastic when they eat</a> and drink and inhaling it when they breathe, and the long-term impacts are just beginning to be studied," said Warner. 



"However, we need to figure out how to release less plastic into the environment and how to reduce consumption and exposure.”



<h2 class="wp-block-heading" id="h-study-implications-and-future-research-directions">Study implications and future research directions</h2>



Bringing together an interdisciplinary team from three campuses, five colleges, and five disciplines, Emili highlighted the significance of this collaboration. 



“We brought together complementary skillsets from our fields of chemistry, engineering, hydrology, oceanography and soil science."



Emili also mentioned that the research project was initially funded with an Institute of Energy and the Environment seed grant, which "served as an ‘incubator’ for a continuation and expansion of our work exploring the fate and transport of microplastics in freshwater environments, with a particular focus on <a href="https://www.earth.com/news/coastal-lagoons-have-high-loads-of-microplastics/" target="_blank" rel="noreferrer noopener">coastal locations</a>.”



Going forward, Professor Warner hopes to investigate how the composition and types of microplastics have evolved over time. He also wants to assess how the associated health risks have unfolded.



The research was supported by the U.S. National Science Foundation, Penn State’s Commonwealth Campus Center Nodes (C3N) Program, and the Institute of Energy and the Environment.



Ultimately, the study aims to expand our understanding of the land-to-sea pathway of microplastics and inspire long-term solutions to reduce pollution and its associated health risks.



The study is published in the journal <a href="https://linkinghub.elsevier.com/retrieve/pii/S0048969724067755" target="_blank" rel="noreferrer noopener">Science of The Total Environment</a>.



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Microplastics are steadily increasing in freshwater environments

As plastic pollution reaches alarming levels in ecosystems worldwide, a...

Not long ago, the common belief was that only a subset of media consumers - often less educated and highly biased - would let their political allegiance override the truth. They would believe the news that favors their political inclinations, even if it wasn't authentic.



Then some intriguing studies emerged which indicated quite the opposite. The research suggested that media consumers across the spectrum value truth over partisanship.



The studies proclaimed that the authenticity of news was more influential than its alignment with a consumer's political views by more than four times.



However, as we stand on the brink of a national election fraught with misinformation, a fresh study shakes this understanding to its core.



<h2 class="wp-block-heading" id="h-news-and-political-views">News and political views</h2>



The research, led by top psychology scholars at Stanford University, suggests that the masses tend to prioritize partisanship over truth when <a href="https://www.earth.com/news/political-views-change-our-perception-of-the-past-and-future/" target="_blank" rel="noreferrer noopener">consuming news</a>.



Quite unexpectedly, this behavioral pattern spans across all political orientations, educational backgrounds, and reasoning capabilities.



Study lead author Michael Schwalbe is a postdoctoral scholar in the Department of Psychology at the School of Humanities and Sciences at <a href="http://www.stanford.edu/" target="_blank" rel="noreferrer noopener">Stanford University</a>.



"We saw an effect of people being more influenced by political alignment than truth," said Schwalbe. 



"We saw it on both political sides and even among people who scored well on a reasoning test. We were a bit surprised to see how widespread this tendency was. People were engaging in a lot of resistance to inconvenient truths."



<h2 class="wp-block-heading" id="h-pervasive-problem-across-political-parties">Pervasive problem across political parties</h2>



The researchers unearthed intriguing ways in which political views and partisanship can impact the analysis of news. 



In one measure of bias, people's beliefs about the impartiality of their political side compared to their rivals were assessed. Ironically, those who were most confident in their side's neutrality were the most biased.



Furthermore, partisanship seemed to have a more robust effect on <a href="https://www.earth.com/news/climate-change-opinions-swing-voting-and-elections-in-the-u-s/" target="_blank" rel="noreferrer noopener">processing real news</a> than fake news. People demonstrated a higher propensity to reject true information that challenged their political views and accept false information that supported their ideological stances.



"Everyone thinks it's the other person who is the problem," said Geoffrey L. Cohen, the James G. March Professor of Organizational Studies in Education and Business, professor of psychology in H&amp;S, and senior author of the study. 



"People say, 'Not me!' But it turns out, like with a lot of social psychological research, it's actually a pretty pervasive problem across political parties and up and down the educational ladder. The problem isn't just misinformation but the filters of our own mind - perhaps more so."



<h2 class="wp-block-heading" id="h-news-sources-and-political-beliefs">News sources and political beliefs</h2>



The study is based on research conducted on a sample of the voting-age U.S. population, matched to the demographics of the census. This group included supporters and opponents of former President Donald Trump.



A distinctive aspect of this research is its deviation in methodology from previous studies. According to Cohen, this could be why the findings contradict them. While the other studies used existing news headlines, this research involved fabricated ones.



Also, in prior investigations, subjects could see the news sources, which may have influenced their acceptance or rejection of the information, whereas this study focused on the headlines alone.



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



The research team conjured fake headlines like "Trump Beats Grandmaster Chess Champion" and "Trump Attended Private Halloween Gala with Sex Orgies Dressed as the Pope." 



Surprisingly, the experts discovered that Trump's supporters and opponents were more likely to believe headlines that aligned with their views than to accept <a href="https://www.earth.com/news/cities-are-largely-unprepared-for-the-effects-of-climate-change/" target="_blank" rel="noreferrer noopener">true headlines</a> that opposed their beliefs.



The researchers suggest that one contributing factor for this situation is the increased consumption of partisan media. 



"We found that the strongest predictors of bias include extreme views of Trump, a one-sided media diet, and belief in the objectivity and lack of bias of a person's own political side relative to the other side," Schwalbe said.



<h2 class="wp-block-heading" id="h-growing-concern-about-news-consumption">Growing concern about news consumption </h2>



The findings of this study underscore concerns about news consumption in the 21st century, especially with the advent of social media and the constant availability of political news. 



Gaining access to one-sided information has become easier, which can reinforce beliefs in personal objectivity and lead to deepened polarization over time.



<h2 class="wp-block-heading" id="h-possible-paths-to-improvement">Possible paths to improvement</h2>



Having identified the problem, the next logical step is to propose interventions. A measure suggested by Cohen, known as "pre-bunking," involves proactive fact-checking where media sources warn of potential misinformation, or people independently learn to recognize manipulation tactics.



However, Cohen and Schwalbe emphasized that the solution doesn't solely lie in policy changes focused on fake news; people are also biased in their disbelief of true news.



Accordingly, they highlight the significance of promoting intellectual humility, wherein media consumers acknowledge the fallibility of their minds and learn to question their perceptions.



"There's still much more to do to understand the problem," said Schwalbe. So, while this study forms a solid foundation for further exploration, there's no denying that we're only at the beginning of this investigative journey.



The study is published in the <a href="https://psycnet.apa.org/fulltext/2025-33892-004.html" target="_blank" rel="noreferrer noopener">Journal of Experimental Psychology: General</a>. 



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People trust news that matches their political views, even when it's fake

Not long ago, the common belief was that only a...

The cooperative behavior of bees, resembling a singular "superorganism," is something uniquely remarkable in the world of nature.



It is not uncommon for thousands of worker bees to function collectively to protect the colony, feed it, and look after the offspring. This intricate social conduct unifies their individual actions into a concerted effort.



But how is this complex behavior encoded and inherited among generations of <a href="https://www.earth.com/news/honey-bees-spread-viruses-to-bumblebees-in-the-spring/" target="_blank" rel="noreferrer noopener">honey bees</a>? The answer lies in a special gene, as unveiled by a team of scientists.



The research was led by experts at Heinrich Heine University Düsseldorf (<a href="https://www.hhu.de/en/" target="_blank" rel="noreferrer noopener">HHU</a>), along with colleagues from Frankfurt/Main, Oxford, and Würzburg. The study has uncovered the genetic underpinnings of honey bee cooperation.



<h2 class="wp-block-heading" id="h-genes-behind-cooperative-bee-behavior">Genes behind cooperative bee behavior</h2>



The principal investigator and the head of the Institute of Evolutionary Genetics at Heinrich-Heine University, Dr. Martin Beye, and his team have made this breakthrough discovery. The research was focused on a gene called "doublesex" or "dsx."



"The behavioral repertoire of the individual bees and their function in the <a href="https://www.earth.com/news/honey-bee-colonies-are-collapsing-as-climate-change-progresses/" target="_blank" rel="noreferrer noopener">colony</a> are not learned, but rather inherited. Until now, it was not known how such complex behaviors were genetically encoded," said Dr. Beye.



The key discovery is that the dsx gene influences worker bee-specific behavior, noted study first author Dr. Vivien Sommer.



"The gene programs whether a worker bee takes up a task in the colony and for how long. This includes collective tasks such as caring for the larvae or foraging for food and social exchanges on food sources, for example," said Dr. Sommer. 



<h2 class="wp-block-heading" id="h-gene-editing-in-bees">Gene editing in bees</h2>



The team used the CRISPR/Cas9 gene-editing technique to modify the dsx gene in select bees, attaching a QR code to the manipulated bees.



Cameras inside the hive monitored the bees' behavior, and with the assistance of artificial intelligence, video sequences were analyzed to determine individual behavioral patterns.



"Our central question was whether and how the inherited behavioral patterns changed as a result of the gene modification. Such changes must be reflected in the nervous system of the worker bees where the specific behaviour is controlled," said Dr. Sommer.



Adding a twist, the researchers introduced a green fluorescent protein (GFP) into the dsx sequence to visualize the neuronal circuits. 



They found that the dsx gene plays a crucial role in creating specific neural pathways in the <a href="https://www.earth.com/news/study-explores-the-basis-of-social-behavior-in-the-insect-brain/" target="_blank" rel="noreferrer noopener">bee’s brain</a>, according to doctoral researcher Jana Seiler, who is also a co-author of the study.



<h2 class="wp-block-heading" id="h-new-chapter-in-bee-behavior">New chapter in bee behavior </h2>



"Our findings indicate a fundamental genetic program that determines the neuronal circuitry and behavior of worker bees," said Dr. Wolfgang Rössler, an expert in the Department of Behavioural Physiology and Sociobiology at the University of Würzburg.



The next challenge is to move from the individual honeybee to the whole bee colony and understand how the gene influences the “superorganism.” 



"We hope to find the link between individual programming and the coordinated behaviour of many individuals," said Alina Sturm, a doctoral researcher at HHU.



Revealing the genetic secret behind the collective behavior of honey bees is more than just a scientific breakthrough. It’s a tribute to the remarkable complexity of nature and its infinite capacity for surprise. 



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



The discovery of a gene that influences honey bee behavior has implications beyond the study of bees.



Understanding how a <a href="https://www.earth.com/news/a-single-gene-allows-cape-honey-bees-to-reproduce-asexually/" target="_blank" rel="noreferrer noopener">single gene</a> can shape complex social dynamics could inspire innovations in fields such as robotics and artificial intelligence.



For example, roboticists often look to nature for insights into building more efficient, cooperative systems. The hive’s "superorganism" structure could serve as a model for developing autonomous swarm robots designed to work together toward a shared goal.



Additionally, the study of bee cooperation offers valuable insights for ecology and conservation. 



Honey bees play a critical role in pollination. Identifying the genetic foundations of their social behavior could lead to better strategies for supporting bee populations amid environmental threats.



By shedding light on the inner workings of the hive, this research adds a new dimension to preserving biodiversity and maintaining the stability of ecosystems that rely heavily on <a href="https://www.earth.com/news/world-honey-bee-day-protecting-our-vital-pollinators/" target="_blank" rel="noreferrer noopener">pollinators</a>.



The study is published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adp3953?adobe_mc=MCMID%3D91765132952246405812279585398434020131%7CMCORGID%3D242B6472541199F70A4C98A6%2540AdobeOrg%7CTS%3D1730680771" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Bees do not learn to be cooperative - it is in their genes

The cooperative behavior of bees, resembling a singular "superorganism," is...

The Big Bang theory describes a mind-blowing event that took place around 14 billion years ago. The observable universe expanded from the size of a minuscule bacterium to the mammoth dimensions of the Milky Way, all within a fraction of a second. 



According to currently accepted theory, this early universe was a hot, dense environment. So, how do we know this massive <a href="https://www.earth.com/news/new-observations-disprove-big-bang-theory-universe-began-tired-light-theory/" target="_blank" rel="noreferrer noopener">cosmic event</a> actually happened?



Much of what we know comes from evidence collected in the last century. In the late 1920s, American astronomer Edwin Hubble found that galaxies are moving away from each other, leading to the idea that our universe is always expanding. 



If we <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">trace this expansion back</a>, we discover a universe that is as old as the oldest astronomical objects we see.



<h2 class="wp-block-heading" id="h-believers-and-skeptics-of-big-bang-theory">Believers and skeptics of Big Bang theory</h2>



Initially, this radical idea was met with skepticism. Interestingly, it was a skeptic, an Englishman named Fred Hoyle, who facetiously dubbed this hypothesis as the "Big Bang" during a <a href="https://www.bbc.com" target="_blank" rel="noreferrer noopener">BBC</a> radio interview in 1949.



The tune of skepticism began to change when, in 1964, Arno Penzias and Robert Wilson detected cosmic microwave background (CMB) radiation -- an afterglow of the Big Bang that filled all space.



This discovery, which earned them the 1978 Nobel Prize in Physics, opened a window into the hot, dense <a href="https://www.earth.com/news/gravitational-waves-dark-matter-big-bang-breakthrough/" target="_blank" rel="noreferrer noopener">beginning of our universe</a>.



<h2 class="wp-block-heading" id="h-first-moments-after-the-big-bang">First moments after the Big Bang</h2>



Over the years, experiments at particle accelerators like the <a href="https://www.earth.com/news/higgs-boson-god-particle-still-remains-quantum-mystery-after-12-years/" target="_blank" rel="noreferrer noopener">Large Hadron Collider</a> have shed light on <a href="https://www.earth.com/news/origins-of-matter-discovered-by-recreating-the-big-bang/" target="_blank" rel="noreferrer noopener">conditions that existed</a> closer to the time of the Big Bang.



Our understanding of physics at these high energies suggests that the four fundamental forces of physics we recognize now were initially unified as a single force.



What are these four forces? We know them as <a href="https://www.earth.com/news/theory-gravity-exists-without-mass-so-dark-matter-does-not-exist/" target="_blank" rel="noreferrer noopener">gravity</a>, <a href="https://www.earth.com/news/lightning-sparks-the-discovery-of-a-new-electromagnetic-wave/" target="_blank" rel="noreferrer noopener">electromagnetism</a>, and the strong and weak nuclear forces. 



As our universe expanded and cooled down, it underwent dramatic changes, known as phase transitions, splitting these forces.



Experiments suggest that a <a href="https://www.earth.com/news/microscopic-primordial-black-holes-may-explain-all-dark-matter-in-universe/" target="_blank" rel="noreferrer noopener">few billionths of a second</a> after the Big Bang, the breakdown of electroweak unification took place. 



This was when electromagnetism and the weak nuclear force separated, leading to all matter in the universe acquiring its mass.



<h2 class="wp-block-heading" id="h-universe-s-primordial-soup">Universe’s primordial soup</h2>



Our walk through the early universe reveals a world filled with a peculiar substance called quark-gluon plasma. 



As its name suggests, this 'primordial soup' consisted of <a href="https://www.earth.com/news/gluons-quarks-and-mystery-what-makes-proton-spin/" target="_blank" rel="noreferrer noopener">quarks and gluons</a>, sub-atomic particles responsible for the strong nuclear force. This plasma didn't last long, though.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/11/big-bang-theory_graphic-illustration_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/11/big-bang-theory_graphic-illustration_1s.jpg" alt="Infographic explaining the Big Bang theory and how it resulted in the universe that we see today." class="wp-image-1949475"/></a><figcaption class="wp-element-caption">Infographic explaining the Big Bang theory and how it resulted in the universe that we see today.</figcaption></figure>



A few millionths of a second post-Big Bang, as the <a href="https://www.earth.com/news/origins-of-matter-discovered-by-recreating-the-big-bang/" target="_blank" rel="noreferrer noopener">universe</a> expanded and cooled, quarks and gluons clumped together to form protons and neutrons, the building blocks of atoms. This event is referred to as quark confinement.



<h2 class="wp-block-heading" id="h-big-bang-nucleosynthesis">Big Bang nucleosynthesis</h2>



With fewer high energy photons in the universe, the process called <a href="https://www.earth.com/news/new-study-claims-our-universe-is-27-billion-years-old-double-the-current-age-estimate/" target="_blank" rel="noreferrer noopener">Big Bang nucleosynthesis</a> (BBN) kicked in. This was when the first atomic nuclei -- dense lumps of matter made from protons and neutrons -- formed.



Once, the higher amount of high energy photons would have quickly destroyed any <a href="https://www.earth.com/news/atomic-nucleus-made-of-quarks-and-gluons-reproduced-for-the-first-time/" target="_blank" rel="noreferrer noopener">atomic nuclei</a>, but with fewer of them around, BBN could take place. 



The fusion reactions stopped just a few minutes after the Big Bang, but their effects are observable to this day.



<h2 class="wp-block-heading" id="h-big-bang-theory-and-the-singularity">Big Bang theory and the singularity</h2>



Penetrating further into our cosmic past, we reach an intriguing period where there's no evidence for what existed before the breakdown of electroweak unification. 



The energy density at this point was so high that our mathematical equations fumble and become nonsensical. This period is known as a singularity.



In the 1960s, two British theoretical physicists, Stephen Hawking and Roger Penrose, presented a series of mathematical theorems suggesting that the universe's spacetime must end at a singularity in the past -- the Big Bang singularity.



While Penrose received the Nobel Prize in 2020, Hawking, who passed away in 2018, was not eligible for this posthumous honor.



According to these theories, <a href="https://www.earth.com/news/matter-spacetime-gravitational-waves-fabric-of-the-universe/" target="_blank" rel="noreferrer noopener">space and time</a> appear at the Big Bang singularity, suggesting there is no 'before' the Big Bang. So, in scientific terms, the Big Bang is the dawn of time.



<h2 class="wp-block-heading" id="h-quantum-quandary-of-big-bang-theory">Quantum quandary of Big Bang theory</h2>



Despite its accuracy in a vast majority of cases, the theory of <a href="https://www.earth.com/news/radical-new-theory-finally-unites-gravity-spacetime-and-the-quantum-realm/" target="_blank" rel="noreferrer noopener">general relativity</a> fails to describe <a href="https://www.earth.com/news/impossible-quantum-effects-observed-atoms-positioned-closely-together/" target="_blank" rel="noreferrer noopener">atoms</a>, <a href="https://www.earth.com/news/t-coronae-borealis-nova-explosion-nearby-star-light-up-earths-skies/" target="_blank" rel="noreferrer noopener">nuclear fusion</a>, or radioactivity. These phenomena are instead explained by quantum theory.



Quantum theory differs from its classical counterparts, such as relativity, by being probabilistic. While classical theories are deterministic and predict a definite outcome from certain initial conditions, quantum theory assigns a probability to <a href="https://www.earth.com/news/quantum-entanglement-a-simple-way-to-grasp-this-impossible-concept-carl-kocher/" target="_blank" rel="noreferrer noopener">multiple possible outcomes</a>.



Gravity is one such area where the classical description falls short, especially when spacetime curvature is extreme, near a singularity. 



During these extreme conditions, the <a href="https://www.earth.com/news/central-theory-of-quantum-gravity-is-modeled-in-the-laboratory/" target="_blank" rel="noreferrer noopener">quantum nature of gravity</a> surfaces, making spacetime more like the fibers and threads of a carpet seen up close -- gnarly, not smooth.



Close to the Big Bang singularity, the structure of spacetime ceases to be smooth. Mathematical theorems suggest that spacetime is overwhelmed by gnarly features, or spacetime foam. 



In spacetime foam, causality does not apply, making the question "why did the Big Bang occur?" meaningless. Events do not need a cause to occur.



<h2 class="wp-block-heading" id="h-universe-born-out-of-chaos">Universe born out of chaos</h2>



To understand the physics at a singularity like the Big Bang, we need a theory explaining the <a href="https://www.earth.com/news/quantum-particles-solution-gravitational-wave-mystery-bose-einstein-condensate/" target="_blank" rel="noreferrer noopener">quantum behavior of gravity</a>. 



But efforts to formulate one, such as loop quantum gravity and <a href="https://www.earth.com/news/consciousness-may-stem-from-unseen-dimensions-beyond-our-reality/" target="_blank" rel="noreferrer noopener">string theory</a>, are still in their infancy, rendering spacetime foam an enigma.



However, the theory of cosmic inflation, introduced by Alexei Starobinsky and Alan Guth, might provide some answers. 



Inflation is a period of accelerated expansion in the early universe. As difficult as it may be to comprehend, it explains why our universe is large, uniform, and spatially flat.



"I usually describe inflation as a theory of the 'bang' of the Big Bang: It describes the propulsion mechanism that we call the Big Bang," explained Alan Guth.



<h2 class="wp-block-heading" id="h-what-does-all-of-this-mean">What does all of this mean?</h2>



To sum it all up, according to a well-accepted theory called the Big Bang, the story of our universe begins with a cataclysmic explosion roughly 14 billion years ago. 



This explosion kickstarted a period of explosive expansion, called <a href="https://www.earth.com/news/nasa-telescope-will-reveal-the-universe-in-more-than-100-colors/" target="_blank" rel="noreferrer noopener">cosmic inflation</a>. The events before inflation remain a mystery. Is it a spacetime singularity, or is it spacetime foam? The answer is still largely unknown.



We know, or at least what we think we know, is that our universe was born from <a href="https://www.earth.com/news/visible-matter-dark-matter-evolved-together-big-bang/" target="_blank" rel="noreferrer noopener">chaos</a> and has evolved over billions of years into the organized cosmos we see today. 



We still have a lot to learn, but we've come a very long way in a relatively short period of time. 



Rather than beat ourselves up that we still don't know the "why" part of the question, let's just enjoy the ride and never stop seeking the answer to the ultimate question: How did it all begin?



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If the Big Bang theory is correct, what exactly happened?

The Big Bang theory describes a mind-blowing event that took...

Ever wondered about the fish you see leaping across rivers with a furious determination? These diligent creatures, including salmon and similar species, have one thing in common. They all face a significant life decision early on - whether to stay in the river or migrate to the sea and then return to procreate.



This choice is about survival and it's a tough one, as both paths come with their unique set of challenges.



<h2 class="wp-block-heading" id="h-salmon-migrating-to-the-open-sea">Salmon migrating to the open sea</h2>



Salmon-like fish, known as salmonids, often choose to either stick around in their birthplace or adapt to the seawater of the open sea, returning to the river to lay their eggs later. 



This branching of strategies impacts how these <a href="https://www.earth.com/news/large-fish-swarms-attract-predators-making-them-an-easy-target/" target="_blank" rel="noreferrer noopener">fish communities</a> evolve over time, especially when we factor in their interplay with environmental conditions. 



This complex interaction could potentially shape individual traits, leading to a shift in the proportion of fish adopting the different pathways.



Such strategic divergences are not exceptional in the animal kingdom. However, how this sort of divergence affects population evolution is not entirely understood. So, researchers are diving into this topic to unravel the mysteries beneath these aquatic decisions.



<h2 class="wp-block-heading" id="h-residents-or-migrants">Residents or migrants?</h2>



To investigate, a team of researchers led by Jun-nosuke Horita from the Japan Weather Association, and Yuuya Tachiki, an assistant professor at <a href="https://www.tmu.ac.jp/english/index.html" target="_blank" rel="noreferrer noopener">Tokyo Metropolitan University</a>, developed a mathematical model.



The model incorporates known traits of a specific salmonid, the female masu salmon, and explores how populations evolve over time given the availability of alternative strategies.



Female masu salmon have three strategies to choose from. They can remain in the river where they were born (residents), migrate to the sea after a year (early migrants), or venture out into the sea at a later stage of their lives (late migrants). 



For simplicity, the research team modeled the salmon to be either resident or early migrants.



<h2 class="wp-block-heading" id="h-salmon-size-in-open-sea">Salmon size in open sea</h2>



An intriguing aspect of the model was the inclusion of size distributions. Young salmon that are smaller are more prone to choose migrating over staying put. 



This study built upon known features of salmon demographics, including the number of eggs per individual and their survival rate. 



<h2 class="wp-block-heading" id="h-predicting-the-migratory-paths">Predicting the migratory paths</h2>



The results of the study were significant. The research team observed that under a broad range of parameters, a stable population was maintained. 



Interestingly, they also identified set conditions under which alternative strategies could be triggered. It was found that a river environment unfavorable for survival, coupled with a fertile sea environment, increased the likelihood of salmon migrating. 



When the survival rate of the arduous migration process plunges below a certain threshold, there is a sudden switch which leads to entire <a href="https://www.earth.com/news/fish-find-new-ways-to-reproduce-in-response-to-predators/" target="_blank" rel="noreferrer noopener">populations</a> opting to stay home and become residents.



<h2 class="wp-block-heading" id="h-survival-evolution-and-environmental-changes">Survival, evolution, and environmental changes </h2>



The ability to predict how populations choose different migratory strategies is crucial for understanding eco-evolution.



This knowledge can help us comprehend how changes in our environment can impact the survival of these organisms. The team is hopeful that their work could be applied to assess and forecast how human-induced changes can affect animal populations.



So, the next time you spot a salmon leaping across the river, remember, it's not just a <a href="https://www.earth.com/news/ai-illuminates-fish-interactions-in-coral-reefs/" target="_blank" rel="noreferrer noopener">fish</a> going against the flow; it's an individual caught in the intricate web of survival, evolution, and environmental changes.



<h2 class="wp-block-heading" id="h-salmon-evolving-in-seas">Salmon evolving in seas</h2>



The research has provided some valuable insights into the world of salmonids and their struggle between migrating and staying put. But it also raises questions about the impact of environmental changes on these aquatic beings.



"This model provides several insights into the eco-evolutionary response of the population to environmental change. For example, the increase in survivorship during migration increased the population size and the fraction of migrants as an ecological and evolutionary response, respectively," noted the researchers.



As we continue our journey of exploration and understanding, let's remember that the decisions we make and the actions we take today have a ripple effect on these fragile ecosystems. 



The study is published in the journal <a href="https://esj-journals.onlinelibrary.wiley.com/doi/10.1002/1438-390X.12196" target="_blank" rel="noreferrer noopener">Population Ecology</a>.



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How do salmon decide whether to venture out to sea?

Ever wondered about the fish you see leaping across rivers...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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...