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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

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

Today's Image of the Day from NASA Earth Observatory features an active landslide zone that has been shifting for decades on the Palos Verdes Peninsula in Los Angeles County.



This area, particularly in Portuguese Bend, experiences ongoing ground movement, with land sliding toward the ocean at varying rates of up to several feet per year. 



The instability is largely due to weak, water-saturated bedrock and the effects of <a href="https://www.earth.com/news/rising-seas-sinking-cities-land-subsidence-on-the-east-coast/">human activity</a>, including road construction and irrigation, which have exacerbated the natural movement.



<h2 class="wp-block-heading" id="h-analysis-of-the-landslide-zone">Analysis of the landslide zone</h2>



According to a recent report from NASA, the landslide zone on the Palos Verdes Peninsula has expanded.&nbsp;



“Researchers at NASA’s Jet Propulsion Laboratory in Southern California used data from an airborne radar to measure the movement of the slow-moving landslides on the Palos Verdes Peninsula in Los Angeles County,” the <a href="https://earthobservatory.nasa.gov/images/153893/los-angeles-area-landslide-expands">report</a> stated.



“The analysis determined that, during a four-week period in the fall of 2024, land in the residential area slid toward the ocean by as much as 4 inches (10 centimeters) per week."



“Portions of the peninsula, which juts into the Pacific Ocean just south of the city of Los Angeles, are part of an ancient complex of landslides that has been moving for at least the past six decades, affecting hundreds of buildings in local communities.”&nbsp;



NASA noted that the motion accelerated and the active area expanded following record-breaking rainfall in Southern California in 2023 and heavy <a href="https://www.earth.com/news/rainfall-is-increasingly-unpredictable-due-to-climate-change/" target="_blank" rel="noreferrer noopener">precipitation</a> in early 2024.



<h2 class="wp-block-heading" id="h-visualization-of-the-landslide-zone">Visualization of the landslide zone</h2>



To create the image, the Advanced Rapid Imaging and Analysis (ARIA) team used data from four flights of NASA’s Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR) collected between September 18 and October 17, 2024.&nbsp;



“The UAVSAR instrument was mounted to a Gulfstream III jet flown out of NASA’s Armstrong Flight Research Center in Edwards, California, and the four flights were planned to estimate the speed and direction of the landslides in three dimensions,” explained NASA.



“In the image above, colors indicate how fast parts of the landslide complex were moving in late September and October, with the darkest reds indicating the highest speeds." 



"The arrows represent the direction of horizontal motion. The white solid lines are the boundaries of the active landslide area as defined in 2007 by the California Geological Survey.”



<h2 class="wp-block-heading" id="h-accelerating-land-movement-and-risks">Accelerating land movement and risks</h2>



Alexander Handwerger is a landslide scientist at the Jet Propulsion Laboratory who performed the analysis. “In effect, we’re seeing that the footprint of land experiencing significant impacts has expanded, and the speed is more than enough to put human life and infrastructure at risk,” said Handwerger.&nbsp;



The landslide activity in this region dates back to the 1950s, when road construction projects disturbed the already <a href="https://www.earth.com/news/two-billion-people-are-threatened-by-land-subsidence/">unstable terrain</a>, accelerating movement.&nbsp;



Since then, shifting ground has led to significant damage to infrastructure, including cracked roads, broken utility lines, and distorted buildings. The instability has made it difficult for the city to maintain roads and essential services in the affected areas.



Despite efforts to slow the movement, including drainage improvements and engineering solutions, the land continues to shift. Homeowners and city officials have had to adapt, with some structures built to withstand slow movement, while others have been abandoned.&nbsp;



The situation remains a challenge, with scientists monitoring the landslide to better understand its <a href="https://www.earth.com/news/landslide-predictions-could-become-94-percent-more-accurate/">behavior</a> and explore potential mitigation strategies.



Portuguese Bend is a well-known example of a continuously active landslide, highlighting the complex interaction between geology, human development, and environmental forces.



Image Credit: NASA Earth Observatory&nbsp;



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Landslide zone in Los Angeles County is expanding

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

Today's Image of the Day from the European Space Agency features a pair of interacting spiral galaxies known as the Antennae Galaxies. They are located approximately 45 million light-years away in the constellation Corvus.&nbsp;



<h2 class="wp-block-heading" id="h-antennae-galaxies-in-a-deadly-embrace">Antennae Galaxies in a deadly embrace </h2>



“The NASA/ESA Hubble Space Telescope has snapped the best ever image of the Antennae Galaxies. Hubble has released images of these stunning galaxies twice before, once using observations from its Wide Field and Planetary Camera 2 (WFPC2) in 1997, and again in 2006 from the Advanced Camera for Surveys (ACS),” noted <a href="https://esahubble.org/images/potw1345a/" target="_blank" rel="noreferrer noopener">ESA</a>.



“The galaxies - also known as NGC 4038 and NGC 4039 - are locked in a deadly embrace. Once normal, sedate spiral galaxies like the Milky Way, the pair have spent the past few hundred million years sparring with one another.”



According to ESA, the clash of the Antennae Galaxies is so violent that stars have been ripped from their host <a href="https://www.earth.com/news/galaxy-collision-2-million-mph-stephans-quintet-captured-unprecedented-detail/" target="_blank" rel="noreferrer noopener">galaxies</a> to form a streaming arc between the two.&nbsp;



The name of the galaxy pair comes from this long stream of stars and gas, which resembles insect antennae.



<h2 class="wp-block-heading" id="h-intense-bursts-of-star-formation-nbsp">Intense bursts of star formation&nbsp;</h2>



The collision has triggered intense bursts of star formation, making the Antennae Galaxies one of the nearest and most dramatic examples of a starburst galaxy.&nbsp;



Many of the newly formed stars are concentrated in massive star clusters, some of which are expected to evolve into globular clusters over millions of years.



“This new image of the Antennae Galaxies shows obvious signs of chaos. Clouds of gas are seen in bright pink and red, surrounding the bright flashes of blue star-forming regions - some of which are partially obscured by dark patches of dust,” explained ESA.



“The rate of star formation is so high that the Antennae Galaxies are said to be in a state of starburst, a period in which all of the gas within the galaxies is being used to form stars.”&nbsp;



“This cannot last forever and neither can the separate galaxies; eventually the nuclei will coalesce, and the galaxies will begin their retirement together as one large elliptical galaxy.”



<h2 class="wp-block-heading" id="h-significance-of-the-antennae-galaxies">Significance of the Antennae Galaxies</h2>



The Antennae Galaxies are one of the most well-studied examples of galaxy collisions - offering insight into the processes that shape galaxies over time.



Astronomers study the Antennae Galaxies using a range of telescopes across different wavelengths, including visible light, infrared, and X-rays.&nbsp;



Observations in X-rays have revealed evidence of supernovae and <a href="https://www.earth.com/news/black-holes-may-talk-to-galaxies-through-energetic-winds/" target="_blank" rel="noreferrer noopener">black holes</a>, while infrared studies highlight regions of dust and star formation.&nbsp;



<h2 class="wp-block-heading" id="h-the-milky-way-s-collision-course-nbsp">The Milky Way's collision course&nbsp;</h2>



The Antennae Galaxies provide a glimpse into the future of our <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>, which is expected to eventually merge with the Andromeda Galaxy - our closest spiral galaxy neighbor.



The cosmic collision course of the Milky Way and Andromeda will reshape both galaxies over billions of years.&nbsp;



This event is expected to occur in about 4.5 billion years. Both galaxies are part of the Local Group, a cluster of galaxies bound together by gravity. Their mutual gravitational pull is drawing them closer at a speed of approximately 110 kilometers per second.



<h2 class="wp-block-heading" id="h-the-birth-of-an-elliptical-galaxy-nbsp">The birth of an elliptical galaxy&nbsp;</h2>



When the two galaxies collide, their individual stars will largely avoid direct collisions due to the vast distances between them. However, the gravitational forces involved will create dramatic effects.&nbsp;



These forces will distort the galaxies' <a href="https://www.earth.com/news/shapes-of-one-million-galaxies-hint-at-the-universes-origins/" target="_blank" rel="noreferrer noopener">shapes</a>, triggering intense bursts of star formation as gas clouds collide and compress. Over time, the galaxies will settle into a new, larger elliptical galaxy often referred to as "Milkomeda" or "Milkdromeda" by astronomers.



<h2 class="wp-block-heading" id="h-galaxy-merger-and-the-solar-system">Galaxy merger and the solar system</h2>



Despite the seemingly destructive nature of the collision, the solar system is unlikely to face direct harm. Our Sun may find itself flung into a new orbit within the merged galaxy or even cast into intergalactic space.&nbsp;



The merger will also significantly alter the night sky, with the Andromeda Galaxy becoming increasingly prominent before blending into the unified structure.



This event is part of the natural <a href="https://www.earth.com/news/galaxies-are-much-bigger-than-we-originally-believed-gas-clouds/" target="_blank" rel="noreferrer noopener">evolution of galaxies</a> and serves as a fascinating reminder of the dynamic and ever-changing nature of the universe. 



While the collision is still billions of years away, studying it helps astronomers understand galactic interactions and the long-term future of our cosmic neighborhood.



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

Today's Image of the Day from the European Space Agency features the star-forming region NGC 604. The nebula is located 2.73 million light-years away from Earth in the Triangulum Galaxy (M33). 



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 that 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.&nbsp;



<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 NASA Earth Observatory features dust streaming off the coast of Iran in January 2025.



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Dust rises from the Jazmurian Basin in Iran

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Glowing spiral galaxy in the constellation Reticulum

Incredibly, a pack of wolverines appeared to be thriving in Mount Rainier National Park! A mom and her two kits suddenly appeared during a routine recording inspection. And this was a huge deal. No one had witnessed a wolverine in the park in over a century. Photo credit: NPS/CASCADES CARNIVORE PROJECT, FLICKR // CC BY 2.0

A Century Wait

Ancient fish once roamed the waters with features that preceded human elbows and knees. Scientists have revealed that our flexible joints can be traced to the earliest jawed fish, bridging the distant past with our daily movements.



Research on ancient fossils has shown that skeleton flexibility is not a modern trait. Jawless species do not appear to share this structural hallmark, signaling a major shift in <a href="https://www.earth.com/news/coelacanth-ngamugawi-wirngarri-new-species-living-fossil-fish-survived-over-400-million-years/" target="_blank" rel="noreferrer noopener">vertebrate history</a>.



Neelima Sharma of <a href="https://www.uchicago.edu/" target="_blank" rel="noreferrer noopener">The University of Chicago</a> is part of the team that investigated fossil evidence and living examples to see where these joints first emerged.



Sharma's <a href="https://journals.plos.org/plosbiology/article?id=10.1371/journal.pbio.3002990" target="_blank" rel="noreferrer noopener">work</a> reveals that these articulated connections, once believed unique to bony species on land, appeared in ancient aquatic creatures long before limbs evolved.



<h2 class="wp-block-heading" id="h-exploring-flexible-connections">Exploring flexible connections</h2>



Synovial joints are typically found in <a href="https://www.earth.com/news/ice-age-art-discovery-reveals-15800-year-old-fishing-secrets/" target="_blank" rel="noreferrer noopener">creatures</a> that require movement with reduced friction. They appear as spaces, or cavities, between bones or cartilage, lubricated by a thin fluid.



This arrangement provides a blend of strength and range. It is more complex than joints that simply fuse or cartilaginous links that have limited motion.



<h2 class="wp-block-heading" id="h-what-sets-synovial-joints-apart">What sets synovial joints apart</h2>



Bone surfaces involved in this flexible setup often show specialized cells and proteins. These features help maintain smooth motion and prevent harmful rubbing.



Scientists once thought that this design was mostly found in land vertebrates. That assumption is now questioned by new analyses on certain fish skeletons.



<a href="https://www.glfc.org/sea-lamprey.php" target="_blank" rel="noreferrer noopener">Sea lampreys</a>, which belong to a lineage without jaws, do not display synovial cavities. Their skeletal elements meet in ways that lack the lubricated space.



Bamboo sharks and little skates, both cartilaginous fish, present a different picture. Joints in these species have the layered tissues and proteins that connect to the type of architecture previously linked to synovial structures.



<h2 class="wp-block-heading" id="h-fossil-scans-reveal-ancient-fish-joints">Fossil scans reveal ancient fish joints</h2>



The team used advanced imaging techniques to study a fossil fish known as Bothriolepis. This specimen exhibited a cavity between skeletal components - a trait places it among the oldest <a href="https://www.earth.com/news/mayan-civilization-may-have-been-shaped-by-ingenious-fisheries/" target="_blank" rel="noreferrer noopener">creatures</a> with a documented synovial joint.



Cartilaginous fish from modern times share some of these patterns with the fossil. Researchers see this as a sign that their common ancestor had joints that could bend with less wear.



<h2 class="wp-block-heading" id="h-flexible-joints-helped-fish-move-better">Flexible joints helped fish move better</h2>



Changing from rigid junctions to more mobile connections offered new avenues in feeding and locomotion. Evolving jaws was one major step, but flexible joints around those jaws opened even more possibilities.



Joint evolution also affected survival. Fish that could maneuver more freely had advantages in escaping predators or capturing prey.



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



“The origin of mobile joints in our fish ancestors enabled them to move about and feed in new ways. This study shows that the developmental processes that are responsible for these joints arose deep within the fish evolutionary tree,” said Sharma.



There is ongoing interest in how other fossil groups fit into the timeline. Scientists aim to look at additional specimens, hoping to see exactly when these structural traits appeared in different <a href="https://www.earth.com/news/tiktaalik-fossil-discovery-sheds-light-on-how-fish-walked-onto-land/" target="_blank" rel="noreferrer noopener">fish branches</a>.



<h2 class="wp-block-heading" id="h-clues-from-embryonic-development">Clues from embryonic development</h2>



Developing embryos often hold secrets about evolutionary history. The researchers found that the <a href="https://www.nature.com/articles/s41586-023-05868-1" target="_blank" rel="noreferrer noopener">little skate embryo</a> forms joints in a way similar to tetrapods. <a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC21740/" target="_blank" rel="noreferrer noopener">Specific proteins</a> appear during development, signaling joint formation in ways that match land vertebrates.



Muscle activity also plays a crucial role. When scientists temporarily paralyzed developing little skates, their joints failed to form properly. This suggests that movement itself is key in shaping these structures, much like in zebrafish and tetrapods.



<h2 class="wp-block-heading" id="h-what-this-means-for-human-joints">What this means for human joints</h2>



Understanding where our synovial joints originated could help scientists explore joint disorders. Conditions like <a href="https://www.niams.nih.gov/health-topics/osteoarthritis" target="_blank" rel="noreferrer noopener">osteoarthritis</a> involve the breakdown of joint cartilage, leading to pain and stiffness. 



Studying how these joints evolved may offer insights into preventing or treating such diseases.



The research also has implications for regenerative medicine. If scientists understand how these joints first formed, they may uncover ways to encourage cartilage repair.



Future studies could look at whether some of the ancient joint-forming proteins could be used in therapies for joint damage.



The study is published in the journal <a href="https://journals.plos.org/plosbiology/article?id=10.1371/journal.pbio.3002990" target="_blank" rel="noreferrer noopener">PLOS Biology</a>.



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Ancient fish had flexible joints like humans

Ancient fish once roamed the waters with features that preceded...

Eilat is the southernmost city of Israel, located on the Gulf of Aqaba in the Red Sea. It is known for its warm climate, coral reefs, and vibrant tourism industry.



Each year in March and April, visitors to Eilat can witness a stunning spectacle. The shores turn pink due to millions of tiny crustaceans with large eyes. These organisms, identified as amphipods, belong to the order Amphipoda.



A recent study provides new insight into this unusual phenomenon. The research was led by Professor Tamar Guy-Haim from Israel Oceanographic and Limnological Research (<a href="https://www.ocean.org.il/en/" target="_blank" rel="noreferrer noopener">IOLR</a>), in collaboration with Dr. Bracha Farstey from the <a href="https://iui-eilat.ac.il" target="_blank" rel="noreferrer noopener">Interuniversity Institute for Marine Sciences</a> in Eilat.



<h2 class="wp-block-heading" id="h-pink-shores-on-the-red-sea">Pink shores on the Red Sea</h2>



The pink color of amphipods comes from carotenoid pigments that they obtain through their diet.



The researchers used an integrative taxonomy approach, combining genetic analysis with morphological identification, to classify these creatures. 



The team also examined environmental factors contributing to their mass mortality, which happens yearly during the same months.



"Like in a detective mystery, we tested several hypotheses," explained Professor Guy-Haim. "Many amphipods exhibit a unique reproductive strategy known as semelparity, where reproduction occurs only once in their lifetime, after which the females die, often simultaneously."



"However, our analyses showed an almost equal ratio of males to females, along with individuals of different sizes, allowing us to rule out semelparity as the root cause."



<h2 class="wp-block-heading" id="h-environmental-stressors-and-amphipod-mortality">Environmental stressors and amphipod mortality</h2>



Climate change and marine heat waves have caused mass die-offs in the past. In the summer of 2017, sea temperatures in Eilat rose by over 4°C in just two and a half days, leading to mass coral reef fish deaths. 



However, the researchers found no unusual temperature spikes during the amphipod mortality events.



"Sometimes, environmental stressors increase susceptibility to parasites and pathogens," noted Professor Guy-Haim. "This has been observed in reef fish and the long-spined sea urchin in Eilat. However, we found no supporting evidence for this hypothesis either."



<h2 class="wp-block-heading" id="h-a-possible-natural-cycle">A possible natural cycle</h2>



To dig deeper, the researchers reviewed scientific literature and discovered a similar event from March 1977. Back then, amphipods covered the shores of Aqaba in large numbers, suggesting this phenomenon might be part of a natural cycle.



Previous studies in the Gulf of Aqaba have documented ocean currents known as eddies. These circular currents can either bring deep, nutrient-rich waters to the surface (upwelling) or push surface water downward (downwelling).



<h2 class="wp-block-heading" id="h-amphipods-in-strong-ocean-currents">Amphipods in strong ocean currents</h2>



In the Northern Hemisphere, cyclonic eddies rotate counterclockwise, pulling deep waters to the surface. In the northern Gulf of Aqaba, these currents strengthen between November and April, becoming up to ten times faster than normal surface currents.



"We hypothesize that the amphipods were trapped in a cyclonic eddy in the northern Gulf and transported by the currents toward the shore," explained Professor Guy-Haim.



"In Hawaii, a mass mortality event of the same amphipod species was documented following the formation of a cyclonic eddy." 



"This is currently our leading hypothesis, but further research is needed to better understand the relationship between current dynamics and such phenomena in the Gulf of Aqaba and other marine systems worldwide."



<h2 class="wp-block-heading" id="h-amphipods-role-in-marine-ecosystems">Amphipods' role in marine ecosystems</h2>



Amphipods hold an essential place in marine food webs. They serve as a food source for fish, seabirds, and even whales. Understanding their life cycle and movement patterns helps researchers study larger ecological processes in marine environments.



This ongoing research could reveal more about the natural forces shaping marine life. Future studies may offer deeper insight into how ocean currents influence marine species worldwide.



<h2 class="wp-block-heading" id="h-potential-impacts-on-marine-biodiversity">Potential impacts on marine biodiversity</h2>



When large numbers of amphipods die, it can affect the ocean ecosystem in different ways.



If too many amphipods disappear, animals that eat them - like fish and seabirds - might struggle to find enough food. This could change how these animals feed and survive.



Scientists are studying whether these deaths harm local marine life or if animals have adapted to this cycle over time. If this happens regularly, some species might rely on these seasonal die-offs as a food source.



<h2 class="wp-block-heading" id="h-further-research-on-amphipods">Further research on amphipods</h2>



Understanding amphipod population dynamics in the Red Sea can help scientists monitor broader ecological trends. 



Researchers plan to continue tracking amphipod movements and mortality patterns in the Gulf of Aqaba. They aim to determine whether these events are purely natural or if human activities and climate shifts play a role.



Future studies could focus on how amphipods respond to environmental stress and whether their deaths influence marine food webs. With better data, scientists can predict changes in marine ecosystems and protect species affected by shifting ocean conditions.



The study is published in the journal <a href="https://onlinelibrary.wiley.com/doi/10.1002/ece3.70949" target="_blank" rel="noreferrer noopener">Ecology and Evolution</a>.



Image Credit: Omri Amosi, Israel Nature and Parks Authority



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Why the shores of the Red Sea turn pink every year

Eilat is the southernmost city of Israel, located on the...

Scientists have long suspected that unusually rapid changes in our DNA might hold the key to brain evolution.



Researchers have now <a href="https://www.nature.com/articles/s41586-025-08622-x" target="_blank" rel="noreferrer noopener">found</a> that certain stretches of our <a href="https://www.genome.gov/genetics-glossary/Chromosome" target="_blank" rel="noreferrer noopener">chromosomes</a> changed more rapidly over time than seen during typical evolution, which may have influenced how our brain’s nerve cells form <a href="https://www.earth.com/news/subtle-dna-changes-shaped-human-brain-evolution/" target="_blank" rel="noreferrer noopener">complex connections</a>. 



The research was led by Professor Yin Shen from the <a href="https://weill.ucsf.edu/" target="_blank" rel="noreferrer noopener">UCSF Weill Institute for Neurosciences</a> and the UCSF Institute for Human Genetics. Her team performed experiments on artificial brain cells from humans and chimpanzees to see which genetic features set us apart.



<h2 class="wp-block-heading" id="h-fast-evolving-dna-and-brain-development">Fast-evolving DNA and brain development</h2>



Fast-changing chromosomal regions, known as human accelerated regions (<a href="https://www.science.org/doi/10.1126/science.abm1696" target="_blank" rel="noreferrer noopener">HARs</a>), differ significantly between people and chimpanzees. Experts believe these areas might have helped shape the advanced thinking and language skills that define our species.



Some of these regions appear to influence how neurons send and receive signals. Shen’s group used cutting-edge genetic approaches to find out why these DNA stretches, HARs, had such a strong effect on <a href="https://qbi.uq.edu.au/brain/brain-anatomy/what-neuron" target="_blank" rel="noreferrer noopener">neuron</a> function.



The team noted that small edits within these regions might have caused a big jump in brain complexity, which could explain the advent of human creativity and problem-solving. It also raises questions about whether these gains come with possible trade-offs in mental health.



<h2 class="wp-block-heading" id="h-neurite-connections-and-complexity">Neurite connections and complexity</h2>



The researchers noticed that human nerve cells grow multiple <a href="https://www.sciencedirect.com/topics/neuroscience/neurite" target="_blank" rel="noreferrer noopener">neurites</a>, which are tiny branches that help with communication between cells. Chimpanzee neurons in the same setting grew fewer branches, which suggests a more streamlined network.



“More neurites during development could mean more complexity in our neural networks. These networks facilitate the transmission of signals in the nervous system and support our higher cognitive functions,” explained Shen.



The investigations revealed that tweaking chimp cells to include human HARs triggered more <a href="https://royalsocietypublishing.org/doi/10.1098/rsif.2023.0265" target="_blank" rel="noreferrer noopener">branching</a>. The differences hint that our ancestors’ DNA picked up precise mutations that amped up the <a href="https://www.nature.com/articles/s41586-024-07558-y" target="_blank" rel="noreferrer noopener">neuronal wiring</a> of the brain.



<h2 class="wp-block-heading" id="h-benefits-and-risks-of-rapid-brain-evolution">Benefits and risks of rapid brain evolution</h2>



Researchers point out that advanced wiring may come at a cost. Some HARs appear to link with genes that show up in certain mental conditions, suggesting that our unique cognitive edge might also come paired with vulnerability to certain mental illnesses. 



Genes like <a href="https://pubmed.ncbi.nlm.nih.gov/16172381/" target="_blank" rel="noreferrer noopener">NPAS3</a> have been tied to <a href="https://www.earth.com/news/how-time-and-space-interact-in-the-brain/" target="_blank" rel="noreferrer noopener">brain development</a> and mental health conditions. Subtle changes in HARs near NPAS3 could shift how much of the gene gets turned on or off in early stages of neuron growth.



The group also examined regions that influence <a href="https://pubmed.ncbi.nlm.nih.gov/12368809/" target="_blank" rel="noreferrer noopener">SOCS2</a>, which is connected to neurite outgrowth. Variations in these areas might change how nerve cells shape themselves, possibly swinging the balance between boosting intelligence and elevating the odds of neurological disorders.



<h2 class="wp-block-heading" id="h-beyond-the-1-difference">Beyond the 1% difference</h2>



<a href="https://www.nature.com/articles/s41586-025-08622-x" target="_blank" rel="noreferrer noopener">Studies</a> have estimated that humans and chimpanzees share about 98-99% of their DNA. That small gap includes HARs, which set the stage for distinctive thought processes, social behavior, and more advanced language skills.



This shift in our <a href="https://www.genome.gov/human-genome-project" target="_blank" rel="noreferrer noopener">genomic blueprint</a> is believed to have unfolded relatively fast in evolutionary time. Slight tweaks in just a few spots can have outsized impacts on neuron structure and brain wiring.



Shen’s experiments used modern genetic engineering to introduce human HARs into chimp cells. Watching those <a href="https://www.ncbi.nlm.nih.gov/search/research-news/1912/" target="_blank" rel="noreferrer noopener">lab-grown neurons</a> form new branches helped confirm how these DNA elements shape connectivity.



<h2 class="wp-block-heading" id="h-future-research-on-dna-and-brain-function">Future research on DNA and brain function</h2>



The scientists are excited about exploring whether changes in these regions hold clues to unexplored cognitive abilities. They want to see whether specific HAR variants spread more quickly than others among early humans.



The researchers are also investigating whether certain DNA shifts might drive differences in brain development across various populations. This could reveal why some communities have increased or decreased risks of suffering brain-related conditions.



Further work will likely look at how HAR-based alterations influence gene interactions in living brains. That might help scientists pinpoint when these genetic quirks first appeared and how they spread in human ancestors.



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



This laboratory approach offers a peek at how subtle DNA changes can rewrite the instructions for assembling our brains. By comparing the DNA in human and chimpanzee cells, scientists can help map our evolutionary path.



The researchers hope that these findings may guide therapies for disorders linked to abnormal neuron connections. Understanding which DNA sites boost or hamper neurite growth might open opportunities to target them in conditions like autism and related syndromes.



The real excitement lies in how these studies bridge the gap between basic biology and the possibility of medical advances. If scientists can pinpoint how these fast-evolving regions shape neurons, they might uncover ways to preserve healthy <a href="https://www.earth.com/news/your-brain-literally-changes-based-on-daily-activities-and-lifestyle/" target="_blank" rel="noreferrer noopener">brain networks</a>.



<h2 class="wp-block-heading" id="h-dna-research-may-shape-brain-health">DNA research may shape brain health</h2>



Researchers envision a time when analyzing HARs becomes routine in identifying early risk markers for certain developmental issues. A single genetic misstep in these areas might cause a ripple effect on how brain cells wire to each other.



The next steps may include testing potential treatments that regulate the expression of crucial genes tied to neuron branching. That might reduce the impact of disruptions that hamper normal growth or communication in the brain.



The research also encourages us to consider our species' rapid rise in intelligence. Speedy edits in a small stretch of code may have set us on a path to become the tool-making, idea-sharing beings we are today.



The study, which was funded by the National Institutes of Health, is published in the journal <a href="https://www.nature.com/articles/s41586-025-08622-x" target="_blank" rel="noreferrer noopener">Nature</a>.



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DNA changes supercharged the human brain - but at a cost

Scientists have long suspected that unusually rapid changes in our...

The past century has witnessed a dramatic increase in wildfires, particularly in the western regions of the United States, where once-seasonal blazes have escalated into year-round occurrences.



Just within the past decade, raging flames have devoured millions of acres, destroyed communities, and released staggering amounts of carbon into the atmosphere - exacerbating the very conditions that fuel more fires.



The increasing number of wildfires is not just an act of nature. The fires are the result of a lethal cocktail of factors including global warming, drought, and well-intentioned but deficient fire suppression efforts.



These factors have collectively spawned a real-life monster - a "fire deficit." This is brought on by an alarming imbalance in which excess dead wood and dry vegetation build up over time and create dangerously combustible conditions.



<h2 class="wp-block-heading" id="h-scientific-approach-to-wildfire-prevention">Scientific approach to wildfire prevention</h2>



Well-regarded for its advanced research initiatives, <a href="https://www.fau.edu/" target="_blank" rel="noreferrer noopener">Florida Atlantic University</a> has taken on this growing problem. 



A team of scientists at the institution has been exploring how the strategic removal of dead wood - one of the primary fuels driving intense wildfires - can not only mitigate fire risk but also enhance carbon storage, creating a win-win scenario for both forest health and climate resilience.



The research looks into the intricate balance between reducing <a href="https://www.earth.com/news/extreme-wildfires-have-doubled-in-the-last-20-years/" target="_blank" rel="noreferrer noopener">fire hazards</a> and maintaining ecological integrity, as they search for interventions that are both effective and sustainable.



The study focuses particularly on the Sierra Nevada region, a biodiversity hotspot where <a href="https://www.earth.com/news/how-persistent-droughts-will-impact-wildlife-in-the-u-s/" target="_blank" rel="noreferrer noopener">prolonged droughts</a> and rising temperatures have exacerbated fire risks. In this region, both natural ecosystems and nearby communities are threatened.



<h2 class="wp-block-heading" id="h-indigenous-inspired-forest-management">Indigenous-inspired forest management</h2>



The scientists found inspiration in the practices of the Indigenous Peoples of the Western U.S. For thousands of years, these communities have ingeniously <a href="https://www.earth.com/news/indigenous-forests-prevent-15-million-yearly-cases-of-disease/" target="_blank" rel="noreferrer noopener">managed forests</a>, using methods such as controlled, low-severity burns and harvesting non-timber forest products.



This rich heritage of forest management has shaped ecosystems and has provided a solid basis for modern techniques that the team at Florida Atlantic University have been exploring.



The researchers tested the efficacy of several different forest management strategies. Eight different treatments were tested for their potential effects on <a href="https://www.earth.com/news/wildfire-risks-not-commonly-disclosed-by-u-s-companies/" target="_blank" rel="noreferrer noopener">wildfire risks</a>. They were juxtaposed with a "control" scenario that included only wildfire.



The treatments ranged from thinning vegetation to physical removal of surface fuel and prescribed burning, either alone or in combination.



<h2 class="wp-block-heading" id="h-dead-wood-removal-and-forest-resilience">Dead wood removal and forest resilience </h2>



The results of the study are quite promising. They suggest that combining physical removal of dead wood with thinning of vegetation can reduce risks like tree mortality and crown fires significantly.



This proactive approach could, in theory, decrease carbon emissions and aid in carbon storage through the creation of biochar, a charcoal produced from organic material in a low-oxygen environment.



"In our increasingly warming world with frequent dangerous fire weather, more people and structures at risk in the wildland-urban interface, health risks from exposure to smoke, and need to enhance carbon sequestration to mitigate global warming, scientists need to examine effective alternative management actions," said study co-author Dr. Scott H. Markwith.



"By combining physical harvesting with thinning – removing smaller or fire-vulnerable trees – evidence from this research suggests we can help restore healthy, resilient forests."



<h2 class="wp-block-heading" id="h-fire-prevention-and-carbon-storage">Fire prevention and carbon storage</h2>



The team at Florida Atlantic University emphasized the potential advantages of this approach which, apart from reducing smoke and wildfire severity, could also generate carbon credits.



"Over time, repeated fuel reduction treatments, such as prescribed burns, can emit more carbon than a single wildfire in an untreated forest. However, by harvesting dead wood and converting it into biochar – a stable form of carbon – emissions can be reduced," noted study lead author Dr. Rabindra Parajuli.



The researchers agree on the necessity of continued, long-term research, including simulation modeling and field experiments, to evaluate the effectiveness of the approach across various forest types and over time.



These efforts represent a strategic investment in our planet's future - a route towards restoring historic wildfire regimes and enhancing the health and resilience of forests in the western United States and beyond.



The full study was published in the journal <a href="https://www.sciencedirect.com/science/article/abs/pii/S0301479725005110?via%3Dihub" target="_blank" rel="noreferrer noopener">Journal of Environmental Management</a>.



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Dead wood removal can save forests from future wildfires

The past century has witnessed a dramatic increase in wildfires,...

A cutting-edge artificial intelligence system promises to help protect elephants in Malaysia from illegal hunting. 



By blending predictive analytics with insights into elephant behavior, the technology aims to shield these animals from escalating threats that have long jeopardized their survival.



Developed through a collaborative effort at <a href="https://www.cardiff.ac.uk/" target="_blank" rel="noreferrer noopener">Cardiff University</a>, PoachNet combines <a href="https://www.earth.com/news/deep-learning-can-help-track-changes-in-forest-cover/" target="_blank" rel="noreferrer noopener">deep learning</a>, GPS-based data, and ecological insights to gauge and mitigate poaching hazards.&nbsp;



The tool has been designed specifically to forecast where elephants are most likely to be found and then assess each location’s risk level, offering a proactive approach that goes beyond routine surveillance.



Scientists from the School of Computer Science and Informatics and the School of Biosciences worked together to construct a platform capable of learning from historical elephant movement patterns and detecting threats in near-real time.&nbsp;



By applying advanced machine-learning techniques, the research team can predict where <a href="https://www.earth.com/news/african-elephants-have-drastically-declined-in-the-last-50-years/">elephants</a> are headed, identify hazardous zones, and assist on-the-ground teams in allocating resources effectively.



<h2 class="wp-block-heading" id="h-a-better-way-to-protect-elephants-nbsp">A better way to protect elephants&nbsp;</h2>



Central to PoachNet’s operation is a knowledge graph that compiles diverse information about elephant movements and known risk factors. This structured repository is linked to a specialized machine-learning model that interprets data from elephant GPS trackers.&nbsp;



“Elephant GPS data is analyzed with a special type of AI - a sequential neural network - to predict their movements," explained study lead author Naeima Hamed, a PhD student at Cardiff.



"These predictions are added to the knowledge graph in a meaningful way - then PoachNet uses a rule-based system to apply poaching rules and detect hidden patterns in the data." 



The platform’s predictive ability sets it apart from more conventional methods of wildlife protection.&nbsp;



“We found that, when tested, PoachNet was more accurate than other leading methods, consistently performing better. By handling the complexity of time and space data and turning predictions into practical rules, PoachNet offers a big improvement in tracking and protecting elephants,” said Hamed.



<h2 class="wp-block-heading" id="h-predicting-poaching-before-it-happens">Predicting poaching before it happens</h2>



Before PoachNet, strategies to curb poaching often relied on single approaches - such as analyzing ranger patrol logs or examining evidence captured by camera traps.&nbsp;



However, these methods do not always account for the dynamic ways elephants move or the full spectrum of human impacts on their habitats. 



PoachNet integrates broader knowledge of <a href="https://www.earth.com/news/covid-lockdowns-had-unexpected-impacts-on-wildlife-behavior/" target="_blank" rel="noreferrer noopener">wildlife behavior</a>, enabling the system to recognize emergent patterns that may indicate an imminent poaching threat.



The project’s designers hope that by identifying where elephants are most at risk, authorities in Sabah can mobilize anti-poaching patrols and camera traps in the most vulnerable areas.&nbsp;



This targeted response could lead to more efficient use of conservation resources, focusing on regions where illegal activity is statistically more likely to occur.



<h2 class="wp-block-heading" id="h-broader-implications-for-conservation">Broader implications for conservation</h2>



Study co-author Omer Rana from Cardiff’s School of Computer Science and Informatics highlighted the system’s potential to extend beyond elephant conservation in Malaysia.&nbsp;



“PoachNet is a unique software tool that integrates semantically modeled regional data sources with emerging machine learning algorithms and semantic reasoning. PoachNet addresses a challenge that continues to affect communities supporting endangered species,” said Rana.



“Both climate change and economics are leading to significant impact across this interface between human activity and natural habitats. The data-driven approach adopted in PoachNet can also be generalized to support other similar localities and national parks - enabling more efficient use of law enforcement and government resources.”



While PoachNet is currently attuned to Bornean elephants, the underlying architecture could be adapted to protect various endangered species worldwide, as each instance might require only modest adjustments in the knowledge graph and relevant predictive models.



<h2 class="wp-block-heading" id="h-urgent-need-to-protect-elephants">Urgent need to protect elephants</h2>



Efforts to shield Bornean elephants from poaching have never been more critical. As habitat areas shrink and the illegal ivory trade persists, these animals face a grim reality.&nbsp;



According to co-author Benoit Goossens, a scientist at Cardiff University’s School of Biosciences and director of the <a href="https://www.danaugirang.com.my/" target="_blank" rel="noreferrer noopener">Danau Girang Field Center</a>, “<a href="https://www.earth.com/news/koalas-face-critical-threats-from-disease-and-habitat-loss/" target="_blank" rel="noreferrer noopener">habitat loss</a>, human-elephant conflict, and poaching threaten Bornean elephants.&nbsp;



“Despite global anti-poaching efforts, the illegal ivory trade continues to drive poaching, reducing the population to fewer than 1500. We hope that PoachNet can assist in poaching prevention methods, therefore helping to ensure the safety of the elephant population in Sabah for the future.”



Given that traditional mechanisms to combat poaching must constantly evolve, there is an urgent need for innovative solutions like PoachNet that incorporate modern technologies and up-to-date ecological knowledge.&nbsp;



By matching predictive models with ground-level patrolling and international regulatory measures, the system could help reverse some of the most destructive trends endangering these elephants.



<h2 class="wp-block-heading" id="h-the-future-of-wildlife-protection">The future of wildlife protection </h2>



In the long term, the research team plans to enhance PoachNet by introducing additional data sources. 



This could involve tapping into acoustic sensors that detect gunshots or vehicle noises, as well as using satellite imagery to keep track of land-use changes and growing human activities. 



Such expansions would feed the system with even more contextual information, improving its predictive power and enabling faster, more decisive responses.



The ultimate objective is to give conservation authorities an advanced tool capable of anticipating illegal activities, thereby reducing the risk to Bornean elephants and potentially other species in peril.&nbsp;



By blending scientific rigor, state-of-the-art AI, and on-the-ground intelligence, PoachNet represents a considerable step forward in wildlife protection strategies.



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



As poaching incidents continue to imperil elephant populations, the hope is that this novel system will allow for data-driven vigilance, pinpointing threats before they escalate into irreversible harm.&nbsp;



With more accurate forecasts and the flexibility to adapt to new conditions, PoachNet may well serve as a blueprint for conservation efforts aimed at preserving some of Earth’s most iconic and vulnerable animals.



Details of this system appear in the research paper, “PoachNet: Predicting Poaching Using an Ontology-Based Knowledge Graph,” published in the journal <a href="https://www.mdpi.com/1424-8220/24/24/8142" target="_blank" rel="noreferrer noopener">Sensors</a>.&nbsp;



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New era in wildlife conservation: How AI will help protect elephants

A cutting-edge artificial intelligence system promises to help protect elephants...

The ocean isn’t just a vast expanse of blue - it’s alive, constantly shifting, breathing, churning, and now weakening in critical ways. The Atlantic Meridional Overturning Circulation (AMOC), a colossal conveyor belt of warm and cold water, keeps weather patterns in check, stabilizes temperatures, and even dictates rainfall in distant corners of the world.



But now, this large system of currents in the Atlantic Ocean is weakening and slowing down. And that could spell disaster.



<h2 class="wp-block-heading" id="h-a-delicate-balancing-act">A delicate balancing act</h2>



Think of the AMOC as Earth’s natural <a href="https://www.earth.com/news/critical-ocean-current-may-be-more-stable-than-previously-thought/" target="_blank" rel="noreferrer noopener">climate regulator</a>. It moves warm water from the tropics up toward Europe, keeping winters there milder than they otherwise would be. 



Meanwhile, colder water flows back south, helping maintain equilibrium. This system is ancient, powerful, and - until recently -remarkably reliable. Now, something is shifting. 



<h2 class="wp-block-heading" id="h-unsettling-signs-of-weakening-ocean-currents">Unsettling signs of weakening ocean currents </h2>



Scientists have observed an unusual cooling area in the North Atlantic, often called a "cold blob." This is unexpected because, as the planet warms, <a href="https://www.earth.com/news/collapse-of-main-atlantic-ocean-circulaton-current-amoc-is-already-happening/" target="_blank" rel="noreferrer noopener">ocean</a> temperatures should generally rise, not drop.



This cold patch suggests a deeper problem linked to the Gulf Stream, which is a key part of the AMOC. The Gulf Stream normally carries warm water northward, but if it slows down or weakens, less warm water reaches the region, causing unexpected cooling.



The effects of this disruption go beyond the ocean. It can change wind patterns, shift where and how much rain falls, and make extreme weather - like storms, droughts, and heatwaves - more frequent and severe. 



These changes can impact agriculture, infrastructure, and daily life worldwide.



<h2 class="wp-block-heading" id="h-price-of-a-weakening-amoc">Price of a weakening AMOC</h2>



A team of researchers from the University of Hamburg's Cluster of Excellence for Climate Research (<a href="https://www.cliccs.uni-hamburg.de" target="_blank" rel="noreferrer noopener">CLICCS</a>) and the <a href="https://mpimet.mpg.de/en/homepage" target="_blank" rel="noreferrer noopener">Max Planck Institute for Meteorology</a> has taken a closer look at the potential consequences. 



Their conclusion? The economic toll of a weakened AMOC could run into trillions of euros by the end of the century.



This isn’t just about changes in <a href="https://www.earth.com/news/atlantic-current-system-may-collapse-by-2037/" target="_blank" rel="noreferrer noopener">ocean temperature</a>. A sluggish AMOC means more heatwaves, longer droughts, fiercer storms. Infrastructure will buckle, food systems will strain, and insurance costs will skyrocket.



<h2 class="wp-block-heading" id="h-science-behind-ocean-current-weakening">Science behind ocean current weakening</h2>



The AMOC relies on the sinking of dense, salty water in the North Atlantic to keep its cycle going. 



But as Arctic ice melts, massive amounts of freshwater pour into the ocean. This dilutes the salt levels, making the water less dense. When that happens, the sinking slows, and so does the AMOC.



And it’s not just about the ocean’s movement. With less water being pulled into the depths, more carbon dioxide lingers in the atmosphere. That means more heat trapped leading to more <a href="https://www.earth.com/news/atlantic-and-arctic-mixing-is-crucial-for-earths-climate-stability/" target="_blank" rel="noreferrer noopener">climate chaos</a>.



<h2 class="wp-block-heading" id="h-flawed-assumptions-costly-mistakes">Flawed assumptions, costly mistakes</h2>



For years, some economic models suggested that a weaker AMOC might actually help cool the Northern Hemisphere, acting as a counterweight to global warming. That assumption no longer holds.



"Our findings indicate that previous studies on AMOC weakening most likely underestimated the economic impacts," noted Felix Schaumann, a climate economist and co-author of the study.



In other words, what seemed like a potential silver lining is, in reality, another storm cloud forming on the horizon.



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



To understand what’s coming, the researchers used climate and economic models to simulate different scenarios. They compared a world where the AMOC stays strong to one where it weakens at various rates.



The results weren’t encouraging. The weaker the AMOC, the less carbon the ocean absorbs, and the faster climate change accelerates. The cost of inaction? Staggering.



<h2 class="wp-block-heading" id="h-chain-reaction-of-consequences">Chain reaction of consequences</h2>



A weakened AMOC doesn’t just affect temperatures. It throws entire ecosystems off balance.



Fisheries that rely on predictable ocean currents could collapse. Crops accustomed to steady rainfall patterns may wither under unexpected droughts. Coastal communities will face rising sea levels, while storms become more violent and erratic.



Each of these effects compounds the next. The economy, already under pressure from rising global temperatures, will strain even further.



<h2 class="wp-block-heading" id="h-a-crossroads-for-policy">A crossroads for policy</h2>



There’s no easy fix. But there are choices to be made.



Slowing carbon emissions is the most immediate step. Investing in renewable energy, strengthening coastal defenses, and improving climate resilience in vulnerable regions are no longer optional - they’re essential.



The AMOC has existed for thousands of years, shaping life as we know it. If it falters, the world will feel the consequences. The question now is whether we act before it's too late.



The Atlantic Meridional Overturning Circulation isn’t just another <a href="https://www.earth.com/news/disastrous-climate-changes-of-the-last-ice-age-could-happen-again/" target="_blank" rel="noreferrer noopener">climate variable</a>. It’s the backbone of the planet’s climate system. If AMOC weakens, the effects will be widespread, costly, and potentially irreversible.



The study is published in the journal <a href="https://www.pnas.org/doi/10.1073/pnas.2419543122" target="_blank" rel="noreferrer noopener">Proceedings of the National Academy of Sciences</a>.



Image Credit: CEN Climate Visualization Laboratory



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Weakening ocean currents could cost trillions of dollars

The ocean isn’t just a vast expanse of blue -...

Flowers do more than brighten gardens and decorate tables. Their scent - sweet, musky, or sometimes citrusy - isn’t just for human enjoyment. It’s a luring message, a chemical whisper meant for pollinators.



For years, scientists have tried to crack the genetic code behind floral fragrance, and now, a research team has found a crucial piece of the puzzle.



Led by Professor Alexander Vainstein at <a href="https://en.huji.ac.il" target="_blank" rel="noreferrer noopener">The Hebrew University</a> of Jerusalem, the study reveals that a single gene, PhDEF, pulls double duty. It doesn’t just shape the <a href="https://www.earth.com/news/flowers-as-food-how-ultrasound-makes-it-possible/" target="_blank" rel="noreferrer noopener">petals</a>; it also controls the flower’s scent. 



This discovery could reshape agriculture, horticulture, and even biotechnology.



<h2 class="wp-block-heading" id="h-linking-petal-shape-and-scent-in-flowers">Linking petal shape and scent in flowers</h2>



The study flips the script on what we thought PhDEF did. This gene was always known for defining petal identity, but researchers discovered another, unexpected function - it helps flowers <a href="https://www.earth.com/news/corpse-flowers-amorphophallus-titanum-smell-like-death-but-thousands-rush-to-see-them-bloom/" target="_blank" rel="noreferrer noopener">produce scent</a>.



And not just at any time. PhDEF kicks in later in flower development, orchestrating the release of compounds that attract pollinators.



Using genetic analysis and viral-induced gene silencing, the research team tested what would happen if PhDEF was turned off.



The result? A dramatic drop in floral fragrance. Petunias that once filled the air with their scent suddenly became undetectable, their chemical signals lost.



"Our findings show that PhDEF is not just responsible for defining petal identity but also for coordinating the production of scent compounds critical for pollination," said Professor Vainstein. 



"This dual functionality suggests that petunia flowers have evolved an integrated regulatory mechanism to optimize their attraction to pollinators."



<h2 class="wp-block-heading" id="h-scent-production-in-flowers">Scent production in flowers</h2>



PhDEF does not act alone in controlling floral scent. The experts identified it as a key regulator that activates two other important genetic regulators, EOBI and EOBII. These regulators then control a set of genes responsible for producing and releasing floral scent compounds.



Think of PhDEF as a master switch. When it is active, it triggers a chain reaction. First, it turns on EOBI and EOBII, which then activate other genes involved in scent production. This process leads to the creation and emission of molecules like methyl benzoate and benzyl alcohol - compounds that give flowers their characteristic fragrance.



To test PhDEF’s role, the scientists silenced it in petunias. The result was striking: the <a href="https://www.earth.com/news/some-bees-value-quality-over-quantity-in-flower-selection/" target="_blank" rel="noreferrer noopener">flowers</a> lost most of their scent, but their petal shape remained unchanged. This proved that scent production and petal formation, though both controlled by PhDEF, are separate processes.



The discovery suggests that floral fragrance can be modified through genetic changes without altering the flower’s physical appearance.



<h2 class="wp-block-heading" id="h-what-this-means-for-flowers-and-crops">What this means for flowers and crops</h2>



Imagine flowers bred for beauty but stripped of their fragrance, such as roses that look stunning but smell like nothing.



Many commercial varieties have suffered this fate. But now, with PhDEF in the spotlight, scientists might be able to bring scent back to flowers bred for aesthetics.



The implications extend beyond ornamental plants. Many crops depend on pollinators, and enhancing floral scent could increase their attractiveness to bees and other essential pollinators. Stronger scents might mean better yields, more reliable pollination, and greater stability for <a href="https://www.earth.com/news/tree-of-life-created-for-flowering-plants-using-400-million-specimens/" target="_blank" rel="noreferrer noopener">agriculture</a>.



The fragrance industry, too, could benefit. By tweaking PhDEF and its related pathways, bioengineers could craft flowers with specific scent profiles, creating natural perfumes tailored to human preferences.



<h2 class="wp-block-heading" id="h-nature-s-fine-tuned-balance">Nature’s fine-tuned balance</h2>



This discovery adds another layer to our understanding of plant biology. It shows how nature optimizes every detail, ensuring that flowers not only look appealing but also produce the right chemical signals at the right time. 



The genetic link between petal formation and scent production reveals a carefully balanced system - one that could have applications far beyond what we see today.



"This discovery advances our knowledge of plant biology and offers potential applications for breeding more resilient and pollinator-friendly crops," said Professor Vainstein.



Science continues to pull back the curtain on nature’s secrets. With every breakthrough, we move closer to harnessing these intricate systems - whether to create more fragrant flowers, improve pollination, or develop new scents for industry.



The more we learn, the more we realize that nothing in nature is accidental. It’s all part of a finely tuned symphony, playing out in every garden, field, and greenhouse.



The study is published in the journal <a href="https://academic.oup.com/plcell/article/37/2/koaf027/8003630" target="_blank" rel="noreferrer noopener">The Plant Cell</a>.



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Flowers get their shape and scent from a single gene

Flowers do more than brighten gardens and decorate tables. Their...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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Detecting mercury contamination with the tap of a finger

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

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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Kainji Lake in north central Nigeria

[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...

Regardless of their hiding skills, razor-sharp claws, and super strength, wolverines had also been no match for humans’ traps and weaponry. They&#8217;d gone the way of the fishers, it seemed. Then CCP video cameras picked up something stunning. Photo credit: Reference / Daniel J Cox Getty Images

A Need For Protection

It's a good job, too, as wolverines can sense weakness. They're opportunistic scavengers, which means they have the sensory skills and intelligence to selectively take down large prey with a physical disadvantage, such as an injury. And while no animal should be hunted to extinction, the lack of wolverines around Mount Rainier definitely made it a safer place for the other critters living there. Photo credit: Youtube / AnimalLogic

A Need For Protection

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