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. This 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

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

Today's Image of the Day from the European Space Agency features NGC 6744 - a large, barred spiral galaxy located approximately 30 million light-years away in the constellation Pavo.&nbsp;



The galaxy is often considered a close analog to the <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a> due to its similar structure and size, spanning about 175,000 light-years across.&nbsp;



<h2 class="wp-block-heading" id="h-euclid-space-mission-nbsp">Euclid space mission&nbsp;</h2>



The image was captured by the <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid</a> space telescope. NGC 6744 stands out as a prime example of the galaxies currently forming the majority of stars in the nearby universe, making it an ideal subject for study with the Euclid mission.&nbsp;



Euclid’s extensive field-of-view allows it to capture the entire galaxy, showcasing not only its large-scale spiral structure but also revealing intricate details on smaller scales across various wavelengths. These details include feather-like dust lanes, known as “spurs,” emerging from the spiral arms.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-6744">Star formation in NGC 6744</h2>



Euclid's observations enable scientists to count individual stars within NGC 6744, trace the distribution of stars and dust throughout the galaxy, and map the dust associated with the gas that fuels the development of new stars. 



<a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">Star formation</a> is a key process in the growth of galaxies, making these studies crucial for understanding galaxy evolution.



Researchers are utilizing Euclid’s data to explore the relationship between dust, gas, and star formation; to map the distribution of different stellar populations and identify regions of active star formation; and to investigate the underlying physics of spiral galaxy structures.&nbsp;



Spiral arms play a significant role in star formation by compressing gas, yet the precise mechanisms behind this process are still unclear. The presence of “spurs” along NGC 6744’s spiral arms offers valuable insights into the dynamics of star formation within these structures.



<h2 class="wp-block-heading" id="h-discovering-new-dwarf-galaxies-nbsp">Discovering new dwarf galaxies&nbsp;</h2>



Additionally, Euclid's dataset will help scientists identify clusters of old stars (globular clusters) and discover new dwarf galaxies around NGC 6744. Remarkably, Euclid has already identified a new dwarf satellite galaxy of NGC 6744 - a surprising discovery given that the galaxy has been studied extensively.



With Euclid’s detailed observations, scientists are gaining a deeper understanding of the processes shaping galaxies, providing essential clues to the evolution and appearance of the <a href="https://www.earth.com/news/universes-expansion-rate-hubble-tension-puzzles-astronomers/" target="_blank" rel="noreferrer noopener">universe</a>.



<h2 class="wp-block-heading" id="h-more-about-ngc-6744">More about NGC 6744</h2>



NGC 6744's disk is rich in star-forming regions and contains numerous young, bright blue stars. The galaxy's nucleus is slightly elongated and has a bar structure, which influences the motion of the stars and gas within it.&nbsp;



The spiral arms of NGC 6744 are well-defined and extend outward, wrapping around the central bar. Additionally, NGC 6744 has a smaller companion galaxy, NGC 6744A, which is interacting with it, adding to the complexity and interest of this distant system.&nbsp;



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



<a href="https://www.earth.com/news/the-mesmerizing-beauty-of-spiral-galaxies/" target="_blank" rel="noreferrer noopener">Spiral galaxies</a> are one of the most common types of galaxies in the universe, characterized by their distinct, spiral-shaped structure.&nbsp;



The galaxies typically consist of a flat, rotating disk containing stars, gas, and dust, along with a central concentration of stars known as the bulge. This bulge is often surrounded by a halo of older stars.&nbsp;



The spiral arms, which extend from the central bulge, are regions of active star formation and are rich in young, hot stars, giving them a bright, bluish appearance.&nbsp;



These arms are also sites where interstellar gas and dust are concentrated, leading to the formation of new stars.&nbsp;



Spiral galaxies are classified into different types based on the tightness of their spirals and the size of their central bulge, with classifications ranging from tightly wound arms in Sa galaxies to more loosely wound arms in Sc galaxies. The <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</a>, our home galaxy, is a prime example of a spiral galaxy.



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



Pavo, which means "peacock" in Latin, is a constellation in the southern sky. It was named by the Dutch astronomer Petrus Plancius in the late 16th century, based on observations made during the Dutch explorations of the southern hemisphere. 



Pavo is one of the 12 constellations created by Plancius from the records of explorers Pieter Dirkszoon Keyser and Frederick de Houtman. 



The constellation is known for its distinctive shape, resembling a peacock with a long, curved tail. Pavo is not visible from most of the northern hemisphere, but it can be seen from the southern hemisphere, particularly during the winter months.



The constellation contains several interesting celestial objects, including the star Peacock, also known as Alpha Pavonis, which is the brightest star in the constellation. This star is a blue-white subgiant located about 179 light-years from Earth.



Image Credit: <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>/Euclid/Euclid Consortium/NASA&nbsp;



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Spiral galaxy NGC 6744 in the constellation Pavo

Today's Image of the Day from NASA Earth Observatory features the Costa Atlántica Reserve stretching along the Atlantic coast in Argentina.



<h2 class="wp-block-heading" id="h-a-refuge-for-migratory-birds-nbsp">A refuge for migratory birds&nbsp;</h2>



“At the far southern reaches of South America, a stretch of tidal flats, shoals, and beaches serves as a refuge for migratory shorebirds and copious aquatic life,” said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



“The Costa Atlántica Reserve in Argentina extends for 220 kilometers (140 miles) along the eastern shore of Tierra del Fuego. The area was designated a Ramsar site in 1995 and a provincial nature reserve in 1998." 



According to NASA, the reserve is the southernmost site both on the Ramsar list and in the Western Hemisphere Shorebird Reserve Network.



<h2 class="wp-block-heading" id="h-significance-of-the-costa-atlantica-reserve">Significance of the Costa Atlántica Reserve</h2>



The Costa Atlántica Reserve is an important conservation site that signifies Argentina's commitment to preserving its rich <a href="https://www.earth.com/news/human-induced-changes-in-ocean-salinity-threaten-biodiversity-and-marine-ecosystems/" target="_blank" rel="noreferrer noopener">coastal biodiversity</a>. 



This vast expanse of protected area serves as a sanctuary for many species, ranging from migratory birds to marine mammals and diverse plant life.



“Tidal habitats along the coast support some 135 species of birds, while crustaceans, mollusks, fish, and cetaceans feed in the productive coastal waters,” said NASA.&nbsp;



“The topography inland of Costa Atlántica, stretching into Chile to the west, is blanketed in shrubs and grassland vegetation adapted to dry conditions - part of a semiarid ecosystem known as the Fuegian steppe.”



<h2 class="wp-block-heading" id="h-maintaining-ecological-balance-nbsp">Maintaining ecological balance&nbsp;</h2>



Established to safeguard the delicate ecosystems of dunes, estuaries, and <a href="https://www.earth.com/news/coastal-lagoons-have-high-loads-of-microplastics/" target="_blank" rel="noreferrer noopener">coastal lagoons</a>, the reserve plays a crucial role in maintaining ecological balance.&nbsp;



It provides critical habitats for numerous threatened species, including the <a href="https://www.earth.com/news/southern-right-whales-have-shifted-their-foraging-grounds/" target="_blank" rel="noreferrer noopener">Southern Right Whale</a>, which finds refuge in these waters during its breeding season.&nbsp;



<h2 class="wp-block-heading" id="h-costa-atlantica-reserve-a-living-laboratory-nbsp">Costa Atlántica Reserve: A living laboratory&nbsp;</h2>



The Costa Atlántica Reserve is not only a refuge for wildlife but also a living laboratory for scientific research. Conservationists and researchers work within its bounds to monitor ecosystems, study species behaviors, and develop strategies for sustainable management.&nbsp;



This ongoing research is pivotal in understanding the impacts of climate change on <a href="https://www.earth.com/news/coastal-river-deltas-face-major-threats-beyond-climate-change/" target="_blank" rel="noreferrer noopener">coastal environments</a> and in devising measures to mitigate these effects.



Furthermore, the reserve illustrates the importance of community involvement in conservation efforts. Local communities are engaged in sustainable tourism and educational programs. 



Through <a href="https://www.earth.com/news/how-bird-photographers-improve-nesting-success/" target="_blank" rel="noreferrer noopener">eco-tourism</a> initiatives, visitors can experience the natural beauty of the reserve while contributing to its preservation.



<h2 class="wp-block-heading" id="h-tierra-del-fuego-archipelago">Tierra del Fuego archipelago</h2>



According to NASA, the broader landscape of the Tierra del Fuego archipelago was shaped by glaciers.&nbsp;



“Ice advanced over the mountains and lowlands during cold climatic periods between the mid-Pleistocene, about 1 million years ago, and the Last Glacial Maximum, about 20,000 years ago. San Sebastián Bay formed in a tectonic depression that was deepened by glacial erosion," noted NASA. 



“Further evidence of glaciation, including hummocky moraines and fields of glacial erratics, appears around the bay, though it is too small to be visible in this image.”



“Partially enclosed by a long, sandy peninsula, San Sebastián Bay attracts copious migratory birds, some of which shuttle seasonally between the Northern and Southern Hemispheres.”



“Large populations of the Hudsonian godwit, white-rumped sandpiper, and other long-distance flyers congregate in the vast intertidal zones. This part of the reserve, however, is vulnerable to the impact of oil and gas extraction from onshore and offshore deposits.”



The image was captured on February 20, 2024 by the <a href="https://landsat.gsfc.nasa.gov/satellites/landsat-9/landsat-9-instruments/oli-2-design/" target="_blank" rel="noreferrer noopener">OLI-2</a> (Operational Land Imager-2) on Landsat 9.



Image Credit: NASA Earth Observatory&nbsp;



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Costa Atlántica Reserve in Argentina

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

Today's Image of the Day from the European Space Agency features Messier 82, a starburst galaxy located in the constellation Ursa Major. This galaxy is actively forming new stars at a rate ten times that of the Milky Way.



In a study using the <a href="https://webb.nasa.gov/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> (JWST), an international team of astronomers has taken an unprecedented look at Messier 82 (M82), revealing intricate details about its frenzied star formation. 



<h2 class="wp-block-heading" id="h-the-power-of-nircam-and-infrared-observations">The power of NIRCam and infrared observations</h2>



The study, led by Alberto Bolatto, utilized Webb’s Near-Infrared Camera (NIRCam) to penetrate the thick dust and gas covering the galaxy's core, a region critical to understanding <a href="https://www.earth.com/news/baby-stars-release-sneezes-of-gas-and-dust-as-they-develop/" target="_blank" rel="noreferrer noopener">star formation</a>. 



"M82 has garnered a variety of observations over the years because it can be considered as the prototypical starburst galaxy," noted Bolatto. “With Webb’s size and resolution, we can look at this star-forming galaxy and see all of this beautiful new detail.”



Webb's NIRCam has proven crucial for observing areas like M82’s center, where layers of dust typically obscure the view in other wavelengths. The camera's ability to capture infrared light allows it to reveal the galaxy's core and its dynamic processes.&nbsp;



<h2 class="wp-block-heading" id="h-messier-82-image-shows-the-power-of-webb-nbsp">Messier 82 image shows the power of Webb&nbsp;</h2>



“This image shows the power of Webb. Every single white dot in this image is either a star or a star cluster. We can start to distinguish all of these tiny point sources, which enables us to acquire an accurate count of all the star clusters in this galaxy,” noted study co-author Rebecca Levy from the University of Arizona.



One of the NIRCam's innovative features is its mode that prevents bright sources from overwhelming the detector, which was particularly useful in studying the intensely active center of Messier 82.&nbsp;



In the image, dark brown tendrils of dust weave through the galaxy's glowing white core, interspersed with small green specks that represent concentrated areas of iron from <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> remnants. Red patches highlight regions where molecular hydrogen is illuminated by the radiation from nearby young stars.



<h2 class="wp-block-heading" id="h-insights-into-galactic-winds">Insights into galactic winds</h2>



The study also focused on understanding how <a href="https://www.earth.com/news/spin-of-a-new-black-hole-is-unlocking-galactic-mysteries/" target="_blank" rel="noreferrer noopener">galactic wind</a>, driven by the rapid rate of star formation and subsequent supernovae, influences M82’s environment. The NIRCam images showed clumpy streams of gas, appearing in red, which extend above and below the galaxy's plane, marking the path of this wind rushing out from the starburst's core.



A key revelation came from the NIRCam’s tracing of polycyclic aromatic hydrocarbons (PAHs), sooty chemical molecules that map out the structure of the galactic wind. To the surprise of researchers, the PAH emissions closely resembled the patterns of the hot, ionized gas, suggesting a more complex interaction within the wind than previously understood.&nbsp;



"It was unexpected to see the PAH emission resemble ionised gas," said Bolatto. "PAHs are not supposed to live very long when exposed to such a strong radiation field, so perhaps they are being replenished all the time. It challenges our theories and shows us that further investigation is required."



<h3 class="wp-block-heading" id="h-future-observations-of-messier-82">Future observations of Messier 82</h3>



The findings from Webb are just the beginning. The team plans to further analyze Messier 82 with additional data, including spectroscopic observations, to determine the ages of the <a href="https://www.earth.com/news/galaxy-collisions-hubble-spots-a-string-of-pearls-star-cluster/" target="_blank" rel="noreferrer noopener">star clusters</a> and the duration of each star formation phase within the starburst environment.&nbsp;



These observations will also assist in a broader understanding of similar processes in early <a href="https://www.earth.com/news/ceers-2112-ancient-galaxy-looks-strikingly-similar-to-ours/" target="_blank" rel="noreferrer noopener">galaxies</a>, which were common in the young universe.



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



Study co-author Torsten Böker of the <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">European Space Agency</a> emphasized the broader implications of these findings. 



“With these amazing Webb images, and our upcoming spectra, we can study how exactly the strong winds and shock fronts from young stars and supernovae can remove the very gas and dust from which new stars are forming,” explained Böker.&nbsp;



“A detailed understanding of this ‘feedback’ cycle is important for theories of how the early universe evolved, because compact starbursts such as the one in M82 were very common at high redshift.”



The study not only illuminates the specific mechanics of star formation in M82 but also enhances our general understanding of galactic evolution and the lifecycle of galaxies.&nbsp;



Image Credit: ESA/Webb, NASA &amp; CSA



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Messier 82: Unlocking the mysteries of star formation

Today's Image of the Day from NASA Earth Observatory features Tropical Storm Francine moving across the Gulf of Mexico on the afternoon of September 10, 2024. 



Just hours after the photo was captured by the Visible Infrared Imaging Radiometer Suite (VIIRS) on the NOAA-21 satellite, the storm intensified into <a href="https://www.earth.com/news/coastal-hurricanes-are-intensifying-faster-due-to-climate-change/">hurricane</a> strength.



By September 11, Francine had become a Category 2 hurricane, reaching wind speeds of 100 miles per hour. 



<h2 class="wp-block-heading" id="h-storms-fueled-by-rising-ocean-temperatures">Storms fueled by rising ocean temperatures</h2>



“Sea surface temperatures (SSTs) are a fair predictor of the readiness of the ocean to fuel and sustain storms. Meteorologists generally agree that SSTs should be above 82 degrees Fahrenheit to sustain and intensify hurricanes, cyclones, and typhoons,” noted <a href="https://earthobservatory.nasa.gov/images/153309/francine-bears-down-on-louisiana" target="_blank" rel="noreferrer noopener">NASA</a>.



“During the time of Francine’s development on September 8 to 10, temperatures in the southwestern Gulf were several degrees above that threshold and slightly above the 2003-2014 average for those dates, according to data from the Multiscale Ultrahigh Resolution Sea Surface Temperature (MUR SST) project.”



<h2 class="wp-block-heading" id="h-impacts-of-hurricane-francine">Impacts of Hurricane Francine</h2>



Louisiana was hit hardest by Francine, with coastal areas experiencing life-threatening storm surges up to 10 feet, heavy rainfall, and significant flooding. In Terrebonne Parish, where Francine made landfall, more than 200,000 residents lost power.&nbsp;



Southern regions of Texas also experienced heavy rainfall and <a href="https://www.earth.com/news/can-we-outrun-the-flood-risks-of-climate-change/" target="_blank" rel="noreferrer noopener">flooding</a>. Despite some weakening as Francine moved inland, Mississippi and other parts of the Gulf Coast still experienced flash flooding and strong winds as the system degraded into a tropical depression.



<h2 class="wp-block-heading" id="h-2024-atlantic-hurricane-season">2024 Atlantic hurricane season</h2>



The 2024 Atlantic hurricane season has been notably active, but with an unusual break in activity leading up to Hurricane Francine.&nbsp;



<h3 class="wp-block-heading" id="h-early-start-for-storms">Early start for storms</h3>



The season officially began on June 1, 2024. By early September, there had been five named storms, including three hurricanes, with one reaching Category 5 status - Hurricane Beryl in July.&nbsp;



Beryl set an early-season record as it intensified rapidly due to exceptionally warm sea surface <a href="https://www.earth.com/news/ocean-warming-has-nearly-doubled-in-the-last-decade/" target="_blank" rel="noreferrer noopener">temperatures</a>.



<h3 class="wp-block-heading" id="h-surprising-calm">Surprising calm</h3>



While the early part of the season saw significant activity, including Beryl's <a href="https://www.earth.com/news/what-causes-the-rapid-intensification-of-hurricanes/" target="_blank" rel="noreferrer noopener">explosive growth</a>, the basin has experienced a surprising calm since mid-August. 



From August 12 to September 3, there was no tropical activity, marking the quietest stretch in over 50 years. Experts attribute this inactivity to several factors, including cooling waters in parts of the Atlantic and shifts in atmospheric patterns over Africa that disrupted storm formation.



<h3 class="wp-block-heading" id="h-what-s-ahead">What's ahead</h3>



Looking ahead, forecasts are cautious but not pessimistic. Despite the quiet period, researchers still expect more activity, with potential for further storm development through September.



Predictions are pointing to up to 14 named storms - seven hurricanes, and three major hurricanes - by the end of the 2024 season.



<h2 class="wp-block-heading" id="h-hurricanes-in-the-gulf-of-mexico-nbsp">Hurricanes in the Gulf of Mexico&nbsp;</h2>



The location of the Gulf of Mexico makes it a hotspot for hurricane development and landfall. Warm sea surface temperatures, especially in late summer and early fall, provide the energy needed for these storms to grow in intensity.&nbsp;



When atmospheric conditions such as low wind shear and high moisture are favorable, hurricanes can rapidly intensify, becoming major threats to coastal regions.



<h3 class="wp-block-heading" id="h-little-time-for-preparation-nbsp">Little time for preparation&nbsp;</h3>



The Gulf of Mexico's geography also means that hurricanes have a relatively short distance to travel before making landfall, often allowing little time for preparation.&nbsp;



Communities in coastal states like Texas, Louisiana, Mississippi, Alabama, and Florida are frequently in the path of these storms.&nbsp;



<h3 class="wp-block-heading" id="h-devastating-impacts">Devastating impacts</h3>



Over the years, hurricanes like Katrina, Harvey, and Ida have highlighted the devastating impacts, from storm surges and flooding to wind damage and disruption of infrastructure.&nbsp;



Due to the Gulf's importance as an economic hub, especially for oil production and shipping, hurricanes can also have significant economic repercussions.



<h3 class="wp-block-heading" id="h-climate-change">Climate change</h3>



The region's vulnerability to hurricanes is compounded by climate change, which has led to warmer <a href="https://www.earth.com/news/extreme-ocean-heating-signals-alarm-for-a-3c-warmer-world/" target="_blank" rel="noreferrer noopener">ocean temperatures</a> and more intense storms. 



Predictions suggest that while the overall number of hurricanes may not increase, the number of major hurricanes (Category 3 and above) could rise. This will make the Gulf Coast an even more dangerous area during hurricane season, which typically lasts from June to November.



Image Credit: NASA Earth Observatory&nbsp;



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Hurricane Francine makes landfall in Louisiana 

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 brilliant remains of a massive star explosion

Spending almost five decades in deep space has not been easy on NASA's Voyager 1 spacecraft. Age-related issues are cropping up, including a recent clogging problem in its thrusters. 



Now is not the time for a space probe to get 'constipated.' It's got a job to do. But not to worry, NASA engineers have stepped in to resolve the situation.



<h2 class="wp-block-heading" id="h-voyager-1-s-thrusters-price-of-time">Voyager 1's thrusters price of time</h2>



Voyager 1's thrusters have <a href="https://www.earth.com/news/voyager-spacecraft-fighting-survival-cosmic-threats-outside-our-solar-system/" target="_blank" rel="noreferrer noopener">been active for 47 years</a>, during which they've gathered a byproduct of age: silicon dioxide.



This resultant from a rubber diaphragm in the spacecraft's fuel tank has had the audacity to clog the fuel tubes in the thrusters, impacting their efficiency. But the <a href="https://science.nasa.gov/mission/voyager/" target="_blank" rel="noreferrer noopener">team at NASA</a> was not about to be defeated by some clogged tubes.



<h2 class="wp-block-heading" id="h-efficiency-of-voyager-1-s-thrusters">Efficiency of Voyager 1's thrusters</h2>



The thrusters operate on liquid hydrazine that, once turned into gas, is released in short puffs to direct the spacecraft's antenna towards Earth. 



If the Voyager 1's thrusters were in prime condition, about 40 of these puffs would be enough to do the job in a day. 



They are vital, you might say, for the spacecraft to <a href="https://www.earth.com/news/voyager-1-resumes-sending-data-to-earth-from-interstellar-space/" target="_blank" rel="noreferrer noopener">interact with Earth</a> -- to receive commands, send engineering data, and unload the precious scientific data it has been collecting in its journey.



<h2 class="wp-block-heading" id="h-choices-ahead-with-voyager-1-thrusters">Choices ahead with Voyager 1 thrusters</h2>



Voyager 1 is endowed with three sets of thrusters, two being attitude propulsion thrusters and one set being trajectory correction maneuver thrusters. In its younger years, during planetary flybys, all types were actively used. 



But now, as Voyager 1 boldly goes where no human-made object has gone before -- out of our solar system -- the needs are simpler. Any thruster can be used to pivot the craft towards Earth.



In 2002, engineers at NASA's Jet Propulsion Laboratory (<a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">JPL</a>) noticed clogging in the fuel tubes in use for pointing the spacecraft towards our home planet.



The solution was to switch to the second branch of attitude thrusters. Sixteen years later, in 2018, they had to switch again as the second branch also showed signs of clogging. 



The choice? The trajectory correction maneuver thrusters.



<h2 class="wp-block-heading" id="h-dilemma-of-cold-and-power">Dilemma of cold and power</h2>



Switching Voyager 1's thrusters isn’t as simple as it used to be in the spacecraft due to the advanced age of the spacecraft and the resultant decrease in its power supply. 



Along those lines, non-essential systems have been deactivated to conserve power, including some heaters, leading to the spacecraft getting colder. Operating the cold thrusters could risk damaging them beyond repair.



The solution? Turning on non-essential heaters to warm up the thrusters. But there's a catch. 



Power is so limited that turning on these heaters would require shutting off something else, and everything currently in operation is essential.



<h2 class="wp-block-heading" id="h-power-puzzle-of-voyager-1-s-thrusters">Power puzzle of Voyager 1's thrusters </h2>



After ruling out switching off an operating science instrument, the engineers decided to temporarily turn off one of the spacecraft's main heaters to provide enough electricity for the non-essential heater. And it worked. 



The thrusters returned to action, as confirmed on Aug. 27, successfully guiding Voyager 1 towards Earth.



"All the decisions we will have to make going forward are going to require a lot more analysis and caution than they once did," confessed Suzanne Dodd, Voyager's project manager at the Jet Propulsion Laboratory.



<h2 class="wp-block-heading" id="h-resilience-of-voyager-1-s-legacy">Resilience of Voyager 1's legacy</h2>



Voyager 1's journey has not only been a <a href="https://www.earth.com/news/voyager-1-resumes-messages-to-earth-from-15-billion-miles-away/" target="_blank" rel="noreferrer noopener">testament to the scientific and engineering prowess</a> of the late 20th century but also a marvel of the resilience embedded in legacy technology. 



Constructed with materials and systems that predate modern advancements, Voyager 1 continues to function beyond expectations. 



Its durability demonstrates the foresight of its initial design, which has allowed it to withstand the harsh conditions of space for decades.



This legacy technology, while appearing antiquated by today's standards, showcases a robustness that modern systems strive to emulate. 



The mission's success is a reminder of the value of meticulous engineering and the enduring quest for exploration.



<h2 class="wp-block-heading" id="h-looking-to-the-future">Looking to the future</h2>



As Voyager 1 and its thrusters continue its solitary voyage through interstellar space, it carries with it the hopes and aspirations of humanity. 



The data it transmits back to Earth provides invaluable insights into the universe's broader realms and conditions far beyond our solar system. 



With each <a href="https://www.earth.com/news/nasa-lost-contact-with-voyager-2-spacecraft-12-billion-miles-away/" target="_blank" rel="noreferrer noopener">transmission</a>, scientists gain a deeper understanding of cosmic phenomena, feeding curiosity and inspiration across generations.



Although the spacecraft's operational future is limited by its diminishing power supply, the legacy of its mission will influence future endeavors. 



Lessons learned from Voyager 1 fuel the ambition to explore deeper into space, forever pushing the boundaries of what is possible.



<h2 class="wp-block-heading" id="h-treading-the-uncharted-voyager-1-s-thrusters">Treading the uncharted Voyager 1's thrusters</h2>



Voyager 1 is now in the realm of interstellar space, far beyond the protective bubble of particles and magnetic fields created by our sun – it's uncharted territory. 



The mission isn't over yet. The team aims to keep Voyager going as long as possible, continuing to reveal the mysteries of the interstellar environment. 



How will it fare? Only time will tell. The universe is watching and so are we.



On the path of continuous discovery, the Voyager 1's and its thrusters journey stands as an epitome of the resolute human spirit, overcoming challenges and advancing knowledge in pursuit of the unfathomable cosmos. It truly is a remarkable journey.



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Voyager 1 team accomplishes tricky thruster swap from 15 billion miles away

Spending almost five decades in deep space has not been...

On World Ozone Day, we celebrate global efforts to protect and restore the ozone layer, a vital shield that protects life on Earth from harmful ultraviolet (UV) radiation.&nbsp;



World Ozone Day was established by the United Nations General Assembly in 1994. This occasion highlights the <a href="https://www.earth.com/news/decline-in-ozone-depleting-chemicals-is-an-encouraging-trend/" target="_blank" rel="noreferrer noopener">success</a> of the Montreal Protocol, an international treaty adopted in 1987, which has been instrumental in phasing out the production and use of ozone-depleting substances.&nbsp;



<h2 class="wp-block-heading" id="h-climate-action-on-world-ozone-day-nbsp">Climate action on World Ozone Day&nbsp;</h2>



World Ozone Day is an important reminder of the link between <a href="https://www.earth.com/news/wildfires-threaten-the-recovery-of-the-ozone-layer/" target="_blank" rel="noreferrer noopener">ozone protection</a> and climate action. The phasing out of ozone-depleting chemicals has greatly contributed to reducing greenhouse gas emissions and slowing global warming.



<div class="wp-block-sendtonews-playerselector">[sendtonews key="iO1Qd1FFM1-3858489-12187" type="single"]</div>



“The theme for this year's World Ozone Day (WOD) is Montreal Protocol: Advancing Climate Action. This theme underscores the critical role the Montreal Protocol plays in not only restoring the stratospheric ozone layer but also in mitigating climate change,” noted James Curlin, head of the <a href="https://www.unep.org/node" target="_blank" rel="noreferrer noopener">UNEP</a> Law Division’s OzonAction Branch.



“It serves as a powerful reminder of our collective responsibility to continue and intensify our efforts to fight climate change through any means possible, be it through the phase out of hydrochlorofluorocarbons (HCFCs) and other ozone depleting substances, or through the phase down of hydrofluorocarbons (HFCs).”&nbsp;



“By doing so, we can significantly reduce both the direct and indirect emissions of gases that heat our planet, contribute to the broader goals of climate action, and build a sustainable future for all.”



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



<a href="https://www.earth.com/news/burning-up-of-satellites-severely-harms-ozone-recovery/" target="_blank" rel="noreferrer noopener">Ozone depletion</a> refers to the gradual thinning of the Earth’s ozone layer in the stratosphere. This phenomenon is primarily caused by the release of ozone-depleting chemicals containing gaseous chlorine or bromine from industrial and consumer products.&nbsp;



<h3 class="wp-block-heading" id="h-contributing-factors">Contributing factors</h3>



The most significant contributors are chlorofluorocarbons (CFCs), halons, and other related <a href="https://www.earth.com/news/monsoons-launch-ozone-depleting-substances-into-the-stratosphere/" target="_blank" rel="noreferrer noopener">substances</a>.&nbsp;



When these chemicals are released into the atmosphere, they eventually reach the stratosphere, where ultraviolet (UV) radiation breaks them down, releasing chlorine and bromine atoms.&nbsp;



These atoms then react with ozone (O3) molecules, causing the ozone to break apart into oxygen molecules (O2) and single oxygen atoms, thus depleting the ozone layer.



<h3 class="wp-block-heading" id="h-impacts-of-ozone-depletion">Impacts of ozone depletion</h3>



The depletion of the ozone layer has significant environmental and health impacts.&nbsp;



A thinner ozone layer allows more harmful UV-B radiation to reach the Earth’s surface, which can lead to an increase in skin cancers, cataracts, and other health issues.&nbsp;



Ozone depletion also affects ecosystems, particularly marine life, as increased <a href="https://www.earth.com/news/antarctic-ozone-hole-exposes-wildlife-to-harmful-uv-radiation/" target="_blank" rel="noreferrer noopener">UV radiation</a> can harm phytoplankton, the base of the marine food web.



<h2 class="wp-block-heading" id="h-success-of-the-montreal-protocol-nbsp">Success of the Montreal Protocol&nbsp;</h2>



As we celebrate the success of the Montreal Protocol, we must recognize the need to address ongoing environmental threats.&nbsp;



Hydrofluorocarbons (HFCs) are chemicals that were introduced as replacements for ozone-depleting substances like chlorofluorocarbons (CFCs).



However, despite their ozone-friendly nature, HFCs have a global warming potential (GWP) that can be hundreds to thousands of times greater than carbon dioxide.&nbsp;



Recognizing this issue, the Kigali Amendment to the Montreal Protocol, adopted in 2016, was created to phase down the production and use of HFCs. This amendment aims to reduce the use of HFCs and minimize their impact on global warming, while maintaining the protection of the ozone layer.



<h2 class="wp-block-heading" id="h-international-cooperation-on-world-ozone-day-nbsp">International cooperation on World Ozone Day&nbsp;</h2>



World Ozone Day is also a celebration of international cooperation, as nations across the globe have united to tackle a major environmental threat.&nbsp;



The progress in healing the ozone layer shows how collective action can address global challenges.&nbsp;



“At a time when multilateralism is under severe strain, the Montreal Protocol to help protect the ozone layer stands out as a powerful symbol of hope.&nbsp; It is a reminder that when countries show political resolve for the common good, change is possible,” said UN Secretary-General António Guterres.



“In uniting the world to phase out the consumption and production of different ozone depleting substances, the Protocol has also contributed to shielding carbon sinks, protecting humanity’s health and avoiding economic losses.”



“On this World Ozone Day, let’s commit to making peace with our planet. Let’s commit to build on the success of the Montreal Protocol to show what international cooperation at its best can achieve.”



Video Credit: Ozone Secretariat



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World Ozone Day 2024: Advancing climate action

On World Ozone Day, we celebrate global efforts to protect...

Scientists have recently discovered an important control circuit involved in swallowing food. The study has shown that fly larvae have special receptors in their esophagus which are triggered as the insect swallows something.&nbsp;



This leads to the release of <a href="https://www.earth.com/news/serotonin-expedite-learning-process/" target="_blank" rel="noreferrer noopener">serotonin</a>, a messenger substance that is frequently referred to as the “feel-good hormone.” The release of serotonin ensures that the larva continues to eat. 



Although the study focused on flies, the experts argue that humans may also have a similar control circuit.&nbsp;



<h2 class="wp-block-heading" id="h-swallowing-food-makes-you-want-more-nbsp">Swallowing food makes you want more&nbsp;</h2>



Imagine you're sitting in a restaurant, feeling hungry, with a delicious pizza in front of you. Its irresistible aroma fills the air.&nbsp;



You take a bite, savor the flavor as you chew, and the moment you swallow, a wave of satisfaction hits you: Wow, that was amazing! Without hesitation, you reach for another slice and eagerly take another bite.



While the pizza’s smell and taste motivate you to begin eating, it is the pleasurable feeling you have after <a href="https://www.earth.com/news/cane-toads-swallow-their-tongue-when-they-eat/" target="_blank" rel="noreferrer noopener">swallowing</a> which is responsible for you continuing to eat. 



“But how exactly does this process work? Which neural circuits are responsible? Our study has provided an answer to these questions,” said Michael Pankratz, an expert in life and medical sciences at the <a href="https://www.uni-bonn.de/en/" target="_blank" rel="noreferrer noopener">University of Bonn</a>.



<h2 class="wp-block-heading" id="h-neurons-communicate-with-the-digestive-system-nbsp">Neurons communicate with the digestive system&nbsp;</h2>



The study was focused on the larvae of the <a href="https://www.earth.com/news/fruit-fly-smell/" target="_blank" rel="noreferrer noopener">fruit fly</a> Drosophila, which have from 10,000 to 15,000 nerve cells - a manageable number compared to the 100 billion nerve cells in the human brain. 



However, these 15,000 nerve cells form a highly complex network, with every neuron having branching projections through which it contacts dozens or even hundreds of other neurons.



“We wanted to gain a detailed understanding of how the <a href="https://www.earth.com/news/healthy-humans-have-shockingly-different-digestive-systems/" target="_blank" rel="noreferrer noopener">digestive system</a> communicates with the brain when consuming food,” Pankratz said. 



“In order to do this, we had to understand which neurons are involved in this flow of information and how they are triggered.”&nbsp;



<h2 class="wp-block-heading" id="h-an-activated-network-of-neurons">An activated network of neurons</h2>



The scientists investigated not just the paths of all of the nerve fibers in the fruit fly larvae but also the connections between neurons.&nbsp;



To do this, they cut a larva into thousands of very thin slices and photographed them under an electron microscope.



“We used a high-performance computer to create three-dimensional images from these photographs,” Pankratz explained.&nbsp;



Next, project assistants Andreas Schoofs and Anton Miroschnikow analyzed how all these nerve cells are connected to one another.



<h2 class="wp-block-heading" id="h-detecting-food-quality-while-swallowing-nbsp">Detecting food quality while swallowing&nbsp;</h2>



The investigation helped the researchers identify what they called a “stretch receptor” in the esophagus that is wired to a cluster of six neurons in the larva’s brain which can produce serotonin, the “feel-good hormone” ensuring that we feel rewarded for certain actions.



The serotonin-releasing neurons receive new information about what the fly has just swallowed.&nbsp;



“They can detect whether it is food or not and also evaluate its quality,” Schoofs explained. “They only produce serotonin if good quality food is detected, which in turn ensures that the larva continues to eat.”



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



The scientists believe that this fundamental mechanism most likely also exists in humans, and, when defective, it could lead to eating disorders such as anorexia or <a href="https://www.earth.com/news/binge-eating-linked-to-a-specific-set-of-brain-cells/" target="_blank" rel="noreferrer noopener">binge eating</a>. 



Thus, the results of this study might also have implications for the treatment of such disorders.&nbsp;



“But we don’t know enough at this stage about how the control circuit in humans actually works.There is still years of research required in this area,” Pankratz cautioned.



<h2 class="wp-block-heading" id="h-food-swallowing-in-mammals">Food swallowing in mammals</h2>



The study authors noted that serotonin signaling has been implicated in motor function in the mammalian esophagus as well.



“The human esophagus also has distinct regions, with a proximal striated muscle region that is mainly controlled by motor neurons in the brainstem and a distal smooth muscle region that is controlled by central neurons in the medulla oblongata and peripheral neurons of the myenteric plexus.”&nbsp;



The researchers concluded that, despite the differences in the number of cell types as compared with the fly, it would be interesting to see if serotonin also monitors the completion of a biologically meaningful action such as swallowing or other vital activities in mammals.



The study is published in the journal <a href="http://dx.doi.org/10.1016/j.cub.2024.08.025" target="_blank" rel="noreferrer noopener">Current Biology</a>.



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Swallowing food triggers ‘feel-good hormones’

Scientists have recently discovered an important control circuit involved in...

Have you ever thought about the role your home and office heating and cooling systems play during climate change? If your answer is no, you are not alone. Most of us don't. 



We are amusingly oblivious that the warm air we so much enjoy during winters and the cool breeze we desire in hot summers have a tiny part to contribute to the global climate. 



It's time to focus on urban microclimates -- a fascinating yet overlooked aspect of climate change. The mundane <a href="https://www.earth.com/news/rising-sea-levels-threaten-groundwater-global-cities-underground-infrastructure/" target="_blank" rel="noreferrer noopener">city infrastructure</a> we interact with daily can significantly alter local climates and eventually our beloved globe.



It's like throwing a tiny stone in a pond. The ripples may start small, but they grow larger, affecting a much wider area than the stone's initial impact.



<h2 class="wp-block-heading" id="h-heating-and-cooling-systems-in-cities">Heating and cooling systems in cities</h2>



Leading the pack in this research is the <a href="https://illinois.edu" target="_blank" rel="noreferrer noopener">University of Illinois Urbana-Champaign</a>. Under the stewardship of civil and environmental engineering professor Lei Zhao, the team has been investigating the effects of city-level waste heat from our beloved residential and commercial buildings.



“The heat generated from heating and cooling systems is a substantial part of the total heat generated within urban areas,” Zhao said. 



“These systems generate a lot of heat that is released into the atmosphere within cities, making them hotter and further increasing the demand for indoor cooling systems, which feeds even more heat into local climates.”



Think of these systems as the culprits that release a lot of heat into the <a href="https://www.earth.com/news/2024-is-likely-the-hottest-year-in-recorded-history/" target="_blank" rel="noreferrer noopener">city's atmosphere</a>, making it uncomfortably hot and thereby increasing everyone's demand for cooling systems.



That, my friends, is a classic example of a positive physical feedback loop. As we insist on cooling our spaces, we inadvertently feed more and more heat into local climates. Isn't that a bit counterproductive?



<h2 class="wp-block-heading" id="h-negative-loops-to-polarized-demand">Negative loops to polarized demand</h2>



However, the plot thickens. Zhao and his team also discovered an antagonist to this boiling story -- the negative feedback loop.



With rising temperatures under climate change, it's plausible that people would require less heating during winter months. 



Translated to city scales, less heating use would mean less heat being released into the city atmosphere, leading to less <a href="https://www.earth.com/news/scorching-summer-of-2024-could-make-it-the-hottest-year-on-record/" target="_blank" rel="noreferrer noopener">warming</a>.



But don't get too comfy just yet. "This process forms a negative physical feedback loop that may dampen the heating demand decrease. But it does not by any means cancel out the positive feedback loop effect," Zhao warns. 



The team's model hints at a potential polarization of seasonal electricity demand that could unravel a unique set of challenges requiring careful planning.



<h2 class="wp-block-heading" id="h-feedback-loops-of-heating-and-cooling-systems">Feedback loops of heating and cooling systems</h2>



The team, led by Zhao, includes experts from various fields. Zhao is part of the <a href="https://sustainability.illinois.edu/" target="_blank" rel="noreferrer noopener">Institute for Sustainability, Energy, and Environment</a>. He also works with the National Center for Supercomputing Applications and the <a href="https://giesbusiness.illinois.edu/" target="_blank" rel="noreferrer noopener">Gies College of Business</a> at Illinois.



The team used a hybrid modeling framework to study global urban heating and cooling energy demand. This framework combines dynamic Earth system modeling with machine learning techniques. Their research addresses the effects of climate change, considering variability and uncertainties.



Their mission? To integrate the effects of positive and negative physical feedback loops into energy projections and ultimately lay the groundwork for more comprehensive <a href="https://www.earth.com/news/climate-change-earth-energy-imbalance-temperature-rise/" target="_blank" rel="noreferrer noopener">climate impact assessment</a>, science-based policymaking and coordination on climate-sensitive energy planning.



<h2 class="wp-block-heading" id="h-moving-forward">Moving forward </h2>



Supported by the National Science Foundation (<a href="https://www.nsf.gov/" target="_blank" rel="noreferrer noopener">NSF</a>) and iSEE at the University of Illinois Urbana-Champaign, the team is embarking on another exciting journey. 



They plan on introducing variables like humidity, building materials, and future climate-mitigating efforts into their models to refine energy-demand projections further.



As we move forward, the importance of such research becomes more evident. The in-depth understanding it provides will play a crucial role in shaping our sustainable energy planning for the future.



<h2 class="wp-block-heading" id="h-using-heating-and-cooling-systems">Using heating and cooling systems</h2>



If there's one thing to take away from this deep dive, it's this -- every action matters. The way we cool or heat our spaces today might seem insignificant in the larger picture of climate change, but remember the ripples.



Unseen to the eye, these ripples are expanding in the form of local microclimates. The way we plan our cities, consume energy, and mitigate climate impacts can either create ripples of problems or waves of sustainable solutions.



The choice, as always, is ours.



So next time you adjust your thermostat on the heating or cooling systems, take a moment to think - "What ripple am I creating?".



The study is published in the journal <a href="https://dx.doi.org/10.1038/s41558-024-02108-w" target="_blank" rel="noreferrer noopener">Nature Climate Change</a>.



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Indoor heating and cooling systems affect city temperatures

Have you ever thought about the role your home and...

Rapa Nui, also known as Easter Island or Te Pito o Te Henua (the navel of the world), is one of the most remote inhabited locations on Earth, situated over 1,900 km from the nearest Polynesian island and 3,700 km from South America.&nbsp;



<h2 class="wp-block-heading" id="h-biggest-mysteries-of-easter-island-nbsp">Biggest mysteries of Easter Island&nbsp;</h2>



Despite extensive study by archaeologists, anthropologists, and geneticists, two central aspects of Rapa Nui’s history remain controversial.



The first contentious topic is the theory of Easter Island's population collapse due to “ecocide” or environmental mismanagement.



The second debate centers around whether the Polynesian ancestors of the Rapanui people had contact with Indigenous Americans before European arrival in 1722.



<h2 class="wp-block-heading" id="h-new-clues-in-easter-island-remains">New clues in Easter Island remains</h2>



A new study published in the journal <a href="https://dx.doi.org/10.1038/s41586-024-07881-4" target="_blank" rel="noreferrer noopener">Nature</a> examines the genomes of 15 Rapanui individuals who lived between 1670 and 1950.&nbsp;



The remains from Easter Island, housed in the Musée de l'Homme in Paris, were analyzed by an international team of scientists, including assistant professor Víctor Moreno-Mayar from the <a href="https://www.ku.dk/english/" target="_blank" rel="noreferrer noopener">University of Copenhagen</a> and researchers from institutions across Europe, the U.S., Chile, and Rapa Nui itself.&nbsp;



The study sheds light on both the ecocide theory and the possibility of transpacific contact.



<h2 class="wp-block-heading" id="h-a-cautionary-tale">A cautionary tale</h2>



For many years, the story of Rapa Nui has been used as a cautionary tale of <a href="https://www.earth.com/news/biodiversity-loss-can-lead-to-total-ecosystem-collapse/" target="_blank" rel="noreferrer noopener">ecological collapse</a>. After the island was settled by Polynesians around 1250, its landscape dramatically transformed.&nbsp;



The famous moai statues were constructed, and the once-lush forests, particularly palm trees, disappeared by the 1600s.&nbsp;



According to the “ecocide” hypothesis, the environmental changes were triggered by a growing population of over 15,000 people, leading to resource depletion, warfare, famine, and even cannibalism, which ultimately caused a catastrophic population collapse.



<h2 class="wp-block-heading" id="h-easter-island-population-was-surprisingly-stable">Easter Island population was surprisingly stable</h2>



However, the new genetic study challenges this narrative. The researchers expected to find signs of a sudden population decline in the genomes of ancient Rapanui individuals, but their analysis showed no such genetic evidence.&nbsp;



Study co-author Bárbara Sousa da Mota is a researcher at the <a href="https://www.unil.ch/central/en/home.html" target="_blank" rel="noreferrer noopener">University of Lausanne</a>.



“Our genetic analysis shows a stably growing population from the 13th century through to European contact in the 18th century. This stability is critical because it directly contradicts the idea of a dramatic pre-contact population collapse,” said Sousa da Mota.



The study illustrates the resilience of the Rapanui population in adapting to environmental changes, suggesting that the real disruptions came with <a href="https://www.earth.com/news/blue-antelope-hippotragus-leucophaeus-extinction-caused-european-colonization/" target="_blank" rel="noreferrer noopener">European colonial activity</a> after 1722.



<h2 class="wp-block-heading" id="h-settling-a-long-debate">Settling a long debate</h2>



Another long-debated topic is whether the Polynesian ancestors of the Rapanui reached the Americas before European arrival.&nbsp;



Despite previous studies rejecting the possibility of such contact, the new research paints a different picture.&nbsp;



By generating high-quality ancient genomes, the researchers discovered that around ten percent of the Rapanui gene pool has Indigenous American origins.&nbsp;



More importantly, the team found that this contact likely occurred before European arrival.



<h2 class="wp-block-heading" id="h-distribution-of-ancient-dna">Distribution of ancient DNA</h2>



Study lead author Víctor Moreno-Mayar is an assistant professor at the University of Copenhagen’s Globe Institute.



“We looked into how the <a href="https://www.earth.com/news/native-american-civilization-cahokia-50000-people-vanished-600-years-ago/" target="_blank" rel="noreferrer noopener">Indigenous American</a> DNA was distributed across the Polynesian genetic background of the Rapanui. This distribution is consistent with a contact occurring between the 13th and the 15th centuries,” explained Moreno-Mayar.



While the study cannot pinpoint where this contact took place, the findings suggest that the ancestors of the Rapanui may have reached the Americas before <a href="https://www.earth.com/news/vikings-landed-in-the-americas-500-years-before-columbus/" target="_blank" rel="noreferrer noopener">Columbus</a>. This could mean that Polynesians undertook even more formidable voyages than previously thought.



<h2 class="wp-block-heading" id="h-challenging-the-narratives-of-easter-island-nbsp">Challenging the narratives of Easter Island&nbsp;</h2>



The new findings challenge longstanding narratives about Easter Island and the potential collapse of its population.&nbsp;



“Personally, I believe the idea of the ecocide is part of a colonial narrative,” said Moreno-Mayar. “The notion that these supposedly primitive people could not manage their resources and almost destroyed themselves is not supported by the genetic evidence.”&nbsp;



“While we must acknowledge that human arrival dramatically altered the ecosystem, there is no evidence of a population collapse before Europeans came. So we can put those ideas to rest now.”



<h2 class="wp-block-heading" id="h-formidable-voyages-across-the-pacific-nbsp">Formidable voyages across the Pacific&nbsp;</h2>



Likewise, the study debunks the idea that Indigenous American genetic ancestry in modern-day Rapanui is solely due to European colonial activity. Instead, it points to earlier interactions between Rapanui and Indigenous American populations.&nbsp;



“We believe this means that Rapanui were capable of even more formidable voyages across the Pacific than previously established,” noted Sousa da Mota.



The research team engaged directly with the Rapanui community, including the “Comisión Asesora de Monumentos Nacionales” (CAMN), to ensure the study addressed questions of interest to both scientists and the islanders.&nbsp;



<h2 class="wp-block-heading" id="h-genetic-revelations-nbsp">Genetic revelations&nbsp;</h2>



One key outcome of these discussions was confirmation that the ancient Rapanui individuals studied are most closely related to the modern-day population of Rapa Nui.



“We have seen that museum archives contain mistakes and mislabels. Now that we have established that these 15 individuals were in fact Rapanui, we know they belong back on the island,” said Moana Gorman Edmunds, an archaeologist from Rapa Nui and co-author of the study.



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



Th study offers significant new insights into Rapa Nui’s history, refuting the ecocide theory and providing evidence of pre-European contact between Rapanui and Indigenous Americans.&nbsp;



Moreover, it opens the door to discussions about repatriating the remains of Rapanui ancestors and preserving their legacy for future generations.



The Rapanui community, through CAMN, will also retain control over who has access to the genetic data of their ancestors and how it is used.



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Easter Island DNA proves the population did not collapse 

Rapa Nui, also known as Easter Island or Te Pito...

NOAA Warning: "Strong" solar storms and auroras expected today

Update -- September 16, 2024, 09:06 AM Eastern Time The...

A recent discovery slamming the fish world is drawing us deep into the abyss. The protagonist of our story is an ancient fish called a coelacanth. 



If you haven't heard of them, these large, less-than-attractive fish have been swimming around our planet for over 400 million years. Yet, they still have a few tricks up their fins.



Our adventure starts in the sun-soaked stretches of Western Australia, where an ancient, pristinely preserved new coelacanth species from the Devonian Period was <a href="https://www.earth.com/wp-content/uploads/2024/09/coelacanth_Ngamugawi-wirngarri_new-species_credit-Katrina-Kenny_1b.jpg">found poking through the sand</a>.



The story weaves between past and present, science and culture, tracing the evolution of coelacanths and the Earth itself.



<h2 class="wp-block-heading" id="h-coelacanths-a-fish-out-of-time">Coelacanths: A fish out of time</h2>



What makes these deep-sea dwellers so fascinating? Today, coelacanths are a rare spectacle observed off the coasts of eastern Africa and Indonesia. 



Reaching up to 2 meters (about 6.5 feet), they are known as "lobe-finned" fish. Their fin structure bears an uncanny <a href="https://www.earth.com/news/human-shoulders-evolved-from-the-jawbones-of-ancient-fish-called-placoderms/" target="_blank" rel="noreferrer noopener">resemblance to our arm bones</a>.



This particular quirk places them closer to lungfish and backboned animals -- frogs, emus, mice (and yes, dear reader, humans too) -- than most fish.



Over their 410-million-year tenure, coelacanths have bloomed into more than 175 species worldwide. One of their finer moments of diversification occurred during the <a href="https://www.earth.com/news/dinosaurs-were-not-the-only-animals-that-grew-fast-during-the-mesozoic/" target="_blank" rel="noreferrer noopener">Mesozoic Era</a>, the age of dinosaurs. 



But as the <a href="https://www.earth.com/news/extraordinary-dinosaur-fossils-discovered-from-the-end-of-cretaceous-era/" target="_blank" rel="noreferrer noopener">Cretaceous Period</a> (around 66 million years ago) rolled to a close under the impact of an asteroid, these mighty fish fell off our fossil radar.



In 1938, however, a group of South African fishermen pulled a Lazarus-like marvel from the ocean's depths -- a living, breathing coelacanth. 



This resurgence led to their infamous reputation as 'living fossils'. However, evidence is beginning to challenge this notion.



<h2 class="wp-block-heading" id="h-birth-of-ngamugawi-wirngarri">Birth of Ngamugawi wirngarri</h2>



This brings us to our ancient starlet, the newly discovered coelacanth called Ngamugawi wirngarri. This specimen comes from a time of heightened tectonic activity. 



These time periods were earth-shaking epochs when the terrestrial plates shifted and carved out new habitats.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2024/09/coelacanth_Ngamugawi-wirngarri_skull-discovery_credit-Katrina-Kenny_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2024/09/coelacanth_Ngamugawi-wirngarri_skull-discovery_credit-Katrina-Kenny_1s.webp" alt="Ngamugawi wirngarri, a new coelacanth species, skull bones after they were acid etched out of rock at Museum Victoria, 2009. Credit: Flinders University" class="wp-image-1944732"/></a><figcaption class="wp-element-caption">Ngamugawi wirngarri, a new coelacanth species, skull bones after they were acid etched out of rock at Museum Victoria, 2009. Credit: Flinders University</figcaption></figure>



Dr. Alice Clement, an evolutionary biologist and paleontologist from <a href="https://www.flinders.edu.au" target="_blank" rel="noreferrer noopener">Flinders University</a> in Australia, was part of the team that christened the fish in partnership with the Mimbi community.



"Our analyses found that tectonic plate activity had a profound influence on rates of coelacanth evolution," she revealed. 



"New species of coelacanth were more likely to evolve during periods of heightened tectonic activity as new habitats were divided and created."



<h2 class="wp-block-heading" id="h-gogo-sites-and-coelacanth-fish">Gogo sites and coelacanth fish</h2>



Ngamugawi wirngarri lived about 380 million years ago amidst the Devonian Period's tropical reefs, teeming with more than 50 species of fish. 



Today, this region is the rocky Gogo Formation on Gooniyandi Country in the Kimberley region of northern Western Australia.



John Long, a Flinders University Strategic Professor of Palaeontology, sheds light on the importance of the Gogo sites. 



"For more than 35 years, we have found several perfectly preserved 3D fish fossils from Gogo sites," he said, "which have yielded many significant discoveries, including mineralized soft tissues and the origins of complex sexual reproduction in vertebrates," he explained.



<h2 class="wp-block-heading" id="h-importance-of-ngamugawi-wirngarri">Importance of Ngamugawi wirngarri</h2>



The story of coelacanths takes a crucial turn as we dive deeper into their lineage. Many landmarks of human anatomy, such as our jaws, teeth, and chambered hearts, can trace their <a href="https://www.earth.com/news/ancient-rays-were-more-diverse-than-previously-thought/" target="_blank" rel="noreferrer noopener">roots to early fishes</a> in the <a href="https://www.earth.com/news/giant-swamp-creature-found-in-namibia-was-an-ambush-predator/" target="_blank" rel="noreferrer noopener">Early Palaeozoic</a> (540-350 million years ago).



Although coelacanths' evolution has dramatically slowed since the dinosaur era, they're not static entities fossilized in time. 



Richard Cloutier, a vertebrate paleontologist at the <a href="https://www.uqar.ca" target="_blank" rel="noreferrer noopener">University of Quebec</a> in Rimouski and a study co-author, offers unique insight.



"While most early forms remain poorly known, our study allows us to start understanding how living coelacanth species of Latimeria might not deserve the enigmatic title of 'living fossils,'" he explained.



The discovery of Ngamugawi wirngarri brings to light the intricate interplay between biology and geology that has shaped life on our planet. 



It's more than just a fish tale -- it's a story about the profound influence of Earth's ever-changing skin on the dance of evolution.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-51238-4" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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'Living fossil' fish species has survived for over 400 million years

A recent discovery slamming the fish world is drawing us...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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

Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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Detecting mercury contamination with the tap of a finger

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

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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...

James went into his garage and brought out a shovel. If this plastic bag was the cause of this strange phenomenon, he needed to remove it. He dug into his beloved grass one shovel at a time until he reached the culprit. He reached his hand in and tried to pull it out again. But even though the plastic bag looked like it had been there for years, it was still as tough as nails.

The First Dig