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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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Young, massive stars in the Triangulum Galaxy

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

Today's Image of the Day from NASA Earth Observatory features the Ruki River in the Democratic Republic of the Congo (DRC). It is a tributary of the Congo River, one of the largest rivers in the world by discharge and depth.&nbsp;



The Ruki River, previously known as the Busira, merges with the Momboyo River near the town of Basankusu to become the Lulonga River, which eventually flows into the Congo River at the town of Lisala.



<h2 class="wp-block-heading" id="h-dark-waters-of-the-ruki-river">Dark waters of the Ruki River</h2>



"If the appearance of the muddy Amazon River evokes a coffee cut with cream, the Ruki River, coursing gently through the Congo Basin, is like a dark tea," said <a href="https://earthobservatory.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA</a>.



"On its slow path through mostly untouched lowland rainforest in the Democratic Republic of Congo (DRC), the water leaches organic material from vegetation, prompting some researchers to think it is one of the darkest blackwater rivers on Earth."



According to NASA, scientists are finding that the dissolved material in this distinctive water offers clues about the carbon cycle of tropical forests.



<h2 class="wp-block-heading" id="h-organic-compounds-in-the-ruki-river">Organic compounds in the Ruki River</h2>



In a recent study, researchers measured the chemical <a href="https://www.earth.com/news/warmer-rivers-keep-antimicrobial-resistant-genes-at-bay/" target="_blank" rel="noreferrer noopener">composition</a> and flow of the Ruki for the first time.&nbsp;



"The study reported that, as the water color suggests, the Ruki is rich in dissolved organic carbon compounds," said NASA.



"It contains four times as much organic carbon as the Congo River and 1.5 times as much as the Rio Negro, the world’s largest blackwater river and a major tributary of the Amazon."



Due to this heavy carbon load, the researchers concluded that tropical forests like those around the Ruki might not accumulate quite as much carbon as we once thought.



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



The river is vital for the livelihoods of local communities. <a href="https://www.earth.com/news/fishing-communities-cooperate-to-survive-climate-change/" target="_blank" rel="noreferrer noopener">Fishing</a> is a crucial activity, with many people depending on it for sustenance and income. The river also supports agriculture along its banks, where communities grow crops.



In many parts of the DRC, <a href="https://www.earth.com/news/rivers-are-warming-up-and-losing-oxygen-faster-than-oceans/" target="_blank" rel="noreferrer noopener">rivers</a> like the Ruki are crucial transportation corridors due to the challenging and often nonexistent road infrastructure. 



The river enables the movement of people and goods, facilitating trade and access to markets, health care, and education.



<h2 class="wp-block-heading" id="h-wildlife-of-the-ruki-river">Wildlife of the Ruki River </h2>



The region around the Ruki River is home to diverse wildlife. It is part of the Congo Basin, the second-largest tropical rainforest area in the world, which is a critical habitat for endangered species.



Among the most notable species are elephants and <a href="https://www.earth.com/news/study-mean-chimpanzees-fare-better-in-life-than-nice-ones/" target="_blank" rel="noreferrer noopener">chimpanzees</a>, whose populations thrive in the surrounding forests. Other primates such as bonobos also live in this region, making it a critical area for primate conservation.



The river itself is home to various species of fish that are crucial to local livelihoods. Hippopotamuses and crocodiles are often found in the water.



Birds like kingfishers, herons, and egrets frequent the riverbanks - making it a haven for birdwatchers.



The Ruki River also supports several species of reptiles and amphibians - some of which are unique to the region.



<h2 class="wp-block-heading" id="h-managing-the-river-s-resources">Managing the river's resources </h2>



The region faces several challenges, including <a href="https://www.earth.com/news/global-deforestation-directly-linked-to-atmospheric-mercury-emissions/" target="_blank" rel="noreferrer noopener">deforestation</a>, overfishing, and environmental degradation, which threaten its ecological balance and the livelihoods of people who depend on it. 



Efforts to manage and conserve the river's resources are vital for sustainable development.



Understanding and protecting the Ruki River and its surroundings are crucial for the DRC's environmental sustainability, economic development, and the well-being of its communities.



<h2 class="wp-block-heading" id="h-landscapes-of-the-drc">Landscapes of the DRC</h2>



The Democratic Republic of Congo (DRC) boasts some of the most diverse and breathtaking landscapes in Africa, reflecting its vast size and ecological richness. Dominated by the Congo Basin, the country is a haven for biodiversity.



Beyond its rainforests, the DRC's landscapes shift dramatically. In the east, the terrain rises into rugged mountains, including the Virunga and Rwenzori ranges, where snow-capped peaks like Mount Stanley pierce the sky. 



This region is also marked by active volcanoes such as Mount Nyiragongo, which harbors one of the world’s largest lava lakes, creating a dramatic and otherworldly spectacle.



To the south and west, the country transitions to expansive savannas with rolling grasslands and scattered trees. These areas contrast sharply with the lushness of the forests, providing vital habitats for species like lions and antelope. 



Rivers like the Ruki are a dominant feature, with the mighty Congo River coursing through the heart of the country. Its tributaries shape the lives of millions.



The image was captured by the OLI (Operational Land Imager) on Landsat 8.



Image Credit: NASA Earth Observatory&nbsp;



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Ruki River in the Democratic Republic of the Congo

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

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA, ESA, and STScI



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Hubble captures a stunning stellar nursery

Today's Image of the Day from the European Space Agency features the Southern Ring Nebula, also known as NGC 3132.



The nebula is located about 2,000 light-years away from Earth in the constellation Vela. This remarkably detailed image was created using data from Webb’s Near-Infrared Camera (NIRCam).



The Southern Ring Nebula is one of the more famous examples of planetary nebulae. It is often studied for its beauty and valuable insights into the end stages of stellar evolution.



<h2 class="wp-block-heading" id="h-stars-power-the-southern-ring-nebula-nbsp">Stars power the Southern Ring Nebula&nbsp;</h2>



The <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a> is powered by two central stars in a binary system. The brighter star is actually a less massive companion. The fainter, dimmer star is the dying, hot central star that has shed its outer layers to form the nebula. 



The dimmer star is a white dwarf and is responsible for the ionization of the gas in the nebula, causing it to glow.



“The bright star at the center of NGC 3132, while prominent when viewed by NASA’s Webb Telescope in near-infrared light, plays a supporting role in sculpting the surrounding nebula," noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



"A second star, barely visible at lower left along one of the bright star’s diffraction spikes, is the nebula’s source. It has ejected at least eight layers of gas and dust over thousands of years.” 



“But the bright central star visible here has helped ‘stir’ the pot, changing the shape of this planetary nebula’s highly intricate rings by creating turbulence." 



ESA explained that the pair of stars are locked in a tight orbit, which leads the dimmer star to spray ejected material in a range of directions as they orbit one another, resulting in these jagged rings.



<h2 class="wp-block-heading" id="h-key-characteristics-of-the-southern-ring-nebula-nbsp">Key characteristics of the Southern Ring Nebula&nbsp;</h2>



The Southern Ring Nebula displays a complex structure with multiple layers of gas and dust. 



The outer shells of the nebula consist of hydrogen and other elements that were ejected from the dying star in previous stages of its <a href="https://www.earth.com/news/young-stellar-objects-observing-the-early-lives-of-stars/" target="_blank" rel="noreferrer noopener">evolution</a>. These layers are illuminated by ultraviolet radiation from the central white dwarf.



<h3 class="wp-block-heading" id="h-coloration">Coloration</h3>



The colors seen in the Southern Ring Nebula come from the different gases present. For example, hydrogen emits red light, while oxygen emits blue-green light. 



These colors help astronomers study the composition and dynamics of the nebula.



<h3 class="wp-block-heading" id="h-size-and-shape">Size and shape</h3>



The nebula spans about half a light-year in diameter. Its intricate, symmetrical structure provides valuable insights into the late stages of <a href="https://www.earth.com/news/star-collapse-black-hole-instead-of-supernova-vanish-from-sky/" target="_blank" rel="noreferrer noopener">stellar evolution</a>, especially the processes involved in the shedding of outer layers by dying stars.



<h2 class="wp-block-heading" id="h-spotlights-from-the-bright-star">Spotlights from the bright star</h2>



ESA noted that hundreds of straight, brightly-lit lines pierce through the rings of gas and dust. “These ‘spotlights’ emanate from the bright star and stream through holes in the nebula like sunlight through gaps in a cloud."



“But not all of the starlight can escape. The density of the central region, set off in teal, is reflected by how transparent or opaque it is. Areas that are a deeper teal indicate that the gas and dust are denser - and light is unable to break free.”



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



According to ESA, this is not only a crisp image of a planetary nebula - it also shows us objects in the vast distances of space behind it. The transparent red sections of the nebula are filled with distant <a href="https://www.earth.com/news/galaxies-have-hearts-and-lungs-that-help-them-live-longer/" target="_blank" rel="noreferrer noopener">galaxies</a>.



“Look for the bright angled line at the upper left. It is not starlight - it is a faraway galaxy seen edge-on. Distant spirals, of many shapes and colors, also dot the scene. Those that are farthest away - or very dusty - are small and red,” said ESA.



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



Vela is a southern constellation that represents the sails of a ship. It was once part of a larger constellation called Argo Navis, which depicted the ship of the mythological hero Jason and the Argonauts. 



In the 18th century, Argo Navis was divided into three separate constellations: Vela (the sails), Carina (the keel), and Puppis (the stern).



Vela is notable for containing several interesting astronomical features. One of its most prominent stars is Gamma Velorum, also known as Suhail or Regor, which is a bright, massive star system consisting of multiple stars.&nbsp;



The constellation also hosts the Vela Supernova Remnant, the remains of a <a href="https://www.earth.com/news/supernova-explosions-could-damage-distant-planets/" target="_blank" rel="noreferrer noopener">supernova</a> explosion that occurred about 11,000 years ago. 



This remnant is associated with the Vela Pulsar, a neutron star that formed during the supernova explosion, which is one of the brightest pulsars in the sky.



Vela is best observed in the Southern Hemisphere, where it can be seen in the summer months. Its position along the Milky Way makes it a popular region for both amateur and professional astronomers to explore.



Image Credit: NASA, ESA, CSA, STScI



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Southern Ring Nebula in the constellation Vela 

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 the European Space Agency features the Little Dumbbell Nebula, also known as Messier 76, located in the constellation Perseus 3,400 light-years away from Earth.



Astronomers captured this image of the Little Dumbbell Nebula to commemorate the 34th anniversary of the Hubble Space Telescope, a joint venture between NASA and the European Space Agency (<a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>).



The snapshot provides not only a breathtaking view but also deep insights into the life cycle of <a href="https://www.earth.com/news/dark-stars-scientists-discover-a-new-type-of-star-powered-by-dark-matter/" target="_blank" rel="noreferrer noopener">stars</a> and the dynamic processes within nebulae.



<h2 class="wp-block-heading" id="h-understanding-messier-76">Understanding Messier 76</h2>



Messier 76 is categorized as a planetary nebula - a term which refers to its round, planet-like appearance when viewed through early, low-power telescopes. 



However, the term is somewhat misleading as planetary nebulae have no connection to actual <a href="https://www.earth.com/news/nasa-finds-17-exoplanets-that-have-oceans-and-possibly-alien-life/" target="_blank" rel="noreferrer noopener">planets</a>. 



Instead, they represent an expansive shell of luminous gases expelled by a dying red giant star, which subsequently collapses into a dense, hot white dwarf. 



This transformation marks the late stages of stellar evolution for medium to low-mass stars.



<h2 class="wp-block-heading" id="h-structure-of-messier-76">Structure of Messier 76</h2>



The structure of Messier 76 is particularly notable. It includes a central ring, giving the appearance of a bar-like feature, with two distinct lobes emanating from either side. 



This formation is believed to be the result of materials ejected by the star during its red giant phase, possibly sculpted by interactions with a companion star. 



Although this binary companion is not visible in current Hubble images, its presence is inferred from the thick disk of dust and gas aligned with its orbital plane. 



The phenomenon of the companion star potentially being absorbed by the primary star, a process akin to stellar cannibalism, is a captivating aspect of the nebula's history.



<h2 class="wp-block-heading" id="h-the-dynamic-environment-of-the-nebula">The dynamic environment of the nebula</h2>



At the core of the nebula, the primary star, now collapsing into a <a href="https://www.earth.com/news/white-dwarf-stars-may-be-billions-of-years-older-than-estimated/" target="_blank" rel="noreferrer noopener">white dwarf</a>, reaches extreme temperatures. This heat is estimated to be 120,000 degrees Celsius - about 24 times hotter than the surface of our Sun. 



This intensely hot remnant is visible as a small, bright point at the center of the nebula. Directly below this, another star can be seen; however, it is merely aligned with the nebula by chance and is not a part of it.



<h2 class="wp-block-heading" id="h-powerful-glow-of-messier-76">Powerful glow of Messier 76</h2>



The dynamics within Messier 76 are driven by powerful forces. The central disk seems to constrict the material, creating two lobes of gas escaping along the rotational axis of the star, perpendicular to the disk.&nbsp;



The lobes are propelled outward by a potent stellar wind, moving at a staggering two million miles per hour. This rapid movement is sufficient to travel the distance from Earth to the <a href="https://www.earth.com/news/timeless-mystery-solved-scientists-uncover-what-is-inside-the-moons-core/" target="_blank" rel="noreferrer noopener">Moon</a> in just over seven minutes.&nbsp;



The collision of the fast-moving gas with older, slower-moving material ejected during the star’s red giant phase results in the stunning glowing effect seen in the nebula. 



The glow, ignited by the ultraviolet radiation from the white dwarf, is a spectacle of colors with red emanating from nitrogen and blue from oxygen.



<h2 class="wp-block-heading" id="h-a-cosmic-moment-in-time">A cosmic moment in time</h2>



Despite its current brilliance, the existence of the Little Dumbbell Nebula is fleeting on a cosmological scale. It is expected to last only about 15,000 years - a mere moment in the lifespan of the <a href="https://www.earth.com/news/dark-energy-is-ripping-the-universe-apart-but-we-arent-sure-how/" target="_blank" rel="noreferrer noopener">universe</a>. 



This brief period highlights the transient nature of such cosmic phenomena, which, while short-lived, provide crucial insights into the mechanics of stellar evolution and the complex interactions within these celestial sculptures.



<h2 class="wp-block-heading" id="h-more-about-messier-76">More about Messier 76</h2>



Messier 76 was discovered by Pierre Méchain in 1780. It was later cataloged by Charles Messier, who included it in his famous list of nebulous objects.



The nebula's faintness and small size require a good telescope to be observed effectively, with larger telescopes able to reveal more of its fine details and structure.



Studying Messier 76 helps astronomers understand the life cycle of stars and the processes that occur during the late stages of stellar evolution. 



The materials expelled by planetary nebulae like Messier 76 eventually contribute to the interstellar medium, from which new stars and planetary systems may form.



Image Credit: ESA Space Agency&nbsp;



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Secrets of the Little Dumbbell Nebula  

St. Patrick Bay Ice Caps Nearly Fully Melted. The dome-shaped glaciers, or ice caps, on <a href="http://www.earth.com/image/lake-st-clair-of-the-u-s-and-canada/">Canada’</a>s Hazen Plateau started to form about five thousand years ago. After several periods of growth and retreat over the millennia, these ice caps have become fragile and could disappear completely within a few decades.

Two of these ice caps are located north of St. Patrick Bay, on Ellesmere Island in Nunavut, Canada, about 65 kilometers (40 miles) south of Alert. These images of the St. Patrick Bay ice caps — standing amidst the darker tundra were acquired with the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite. The top image shows their extent on July 12, 2004; the second image is from August 4, 2015. Turn on the image comparison tool to see the retreat.

[caption id="attachment_2388755" align="alignleft" width="150"]<a href="http://cff1.greenatom.net/uploads/2016/03/23203452/st-patrick-bay-ice-cap-july2004_1-2big_aster_nasa.jpg"><img class="wp-image-2388755 size-thumbnail" src="http://cff1.greenatom.net/uploads/2016/03/23203452/st-patrick-bay-ice-cap-july2004_1-2big_aster_nasa-150x150.jpg" alt="St. Patrick's Bay ice cap, July 2004" width="150" height="150" /></a> St. Patrick's Bay ice cap, July 2004[/caption]

In 1959, aerial and ground-based surveyors estimated the size of the larger ice cap at 7.5 square kilometers (3 square miles). The extent of both caps from that year is marked with a yellow line. The two ASTER images show significant shrinking in just a decade, and by 2015, the larger ice cap had shrunk to just 7 percent of its 1959 area; the smaller cap stood at just 6 percent.

Mark Serreze, director of the National Snow &amp; Ice Data Center (NSIDC), described his time spent studying the ice caps in the early 1980s. “While I’ve been to a lot of interesting places since 1983, a day has rarely gone by that I haven’t thought about my early adventures on the St. Patrick Bay ice caps,” he said in an NSIDC story. “To think that they are likely to die before I do blows my mind.”

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<a href="http://www.nasa.gov" target="_blank" rel="noopener noreferrer">NASA</a>

St. Patrick Bay Ice Caps Nearly Fully Melted

Researchers recently revealed a stunning new species of sea slug glowing in the ocean's darkest depths. Known as the "mystery mollusk" or&nbsp;Bathydevius caudactylus, this nudibranch inhabits the ocean's midnight zone, one of Earth's least-explored realms.



This discovery is more than just a new name on a species list - it's an illuminating dive into our planet's vast, hidden ecosystems.



<h2 class="wp-block-heading" id="h-mystery-mollusk-in-the-midnight-zone">Mystery mollusk in the midnight zone</h2>



The "mystery mollusk," Bathydevius caudactylus as the scientists officially named it, inhabits the <a href="https://www.earth.com/news/highly-unusual-bacteria-discovered-in-deep-sea-corals/" target="_blank" rel="noreferrer noopener">ocean's deep abyss</a>, also known as the midnight zone.



But this isn't just about a new species - it's about an exciting lifeline into understanding our planet's largest habitat in more depth.



Monterey Bay Aquarium Research Institute (<a href="https://www.mbari.org" target="_blank" rel="noreferrer noopener">MBARI</a>) Senior Scientist Bruce Robison steered this explorative venture.



“Thanks to MBARI’s advanced underwater technology, we were able to prepare the most comprehensive description of a deep-sea animal ever made," noted Robison.



"We've invested more than 20 years in understanding the natural history of this fascinating species of nudibranch. Our discovery is a new piece of the puzzle that can help better understand the largest habitat on Earth."



<h2 class="wp-block-heading" id="h-identifying-the-mystery-mollusk">Identifying the mystery mollusk</h2>



This unusual sea creature was first spotted in the year 2000, during an expedition using the institute's remotely operated vehicle (ROV) named Tiburon. It was found gliding through the waters offshore of Monterey Bay at a depth of 2,614 meters (8,576 feet).



Confusion arose when the team initially struggled to identify this creature due to its anomalous appearance - a voluminous hood, a flat tail fringed with numerous, finger-like projections, and a set of colorful internal organs.



But after years of research and countless ROV sightings, the <a href="https://www.earth.com/news/sea-pigs-unicumbers-strange-stunning-creatures-discovered-abyssal-plains-ccz/" target="_blank" rel="noreferrer noopener">mystery</a> was solved - this strange creature is, in fact, a nudibranch or sea slug.



<div class="wp-block-sendtonews-playerselector">[sendtonews key="rLItWTv9qr-4019991-12187" type="single"]</div>



<h2 class="wp-block-heading" id="h-a-nudibranch-unlike-any-other">A nudibranch unlike any other</h2>



The mystery mollusk isn't your ordinary nudibranch. It's the first of its kind known to dwell in the immense open waters of the bathypelagic zone, a region 1,000 to 4,000 meters (3,300 to 13,100 feet) below the ocean surface.



Also, the sightings of this fascinating creature span the Pacific coast of North America, from Oregon to as far south as Southern California. Plus, similar creatures spotted by NOAA researchers in the Mariana Trench hint at the mollusk's potentially widespread existence.



<h2 class="wp-block-heading" id="h-survival-techniques-of-the-sea-slug">Survival techniques of the sea slug</h2>



Surviving in such harsh environments is no easy feat. How does the mystery mollusk manage? Interestingly, it has evolved unique survival strategies.



For instance, unlike most sea slugs that feed by rasping prey off the <a href="https://www.earth.com/news/ocean-life-100-new-sea-creatures-found-in-chile/" target="_blank" rel="noreferrer noopener">seafloor</a>, it uses its cavernous hood to trap crustaceans, much like a Venus flytrap plant would do.



Moreover, to avoid predators, it has a clear body that blends with the surrounding waters and can emit a bright bioluminescence to deter and distract hungry predators. 



“When we first filmed it glowing with the ROV, everyone in the control room let out a loud ‘Oooooh!’ at the same time. We were all enchanted by the sight,” said MBARI senior scientist Steven Haddock.



“Only recently have cameras become capable of filming bioluminescence in high-resolution and in full color. MBARI is one of the only places in the world where we have taken this new technology into the deep ocean, allowing us to study the luminous behavior of deep-sea animals in their natural habitat.”



<h2 class="wp-block-heading" id="h-nudibranch-family-tree-expands">Nudibranch family tree expands</h2>



Beyond its captivating appearance and survival tactics, what really stood out during the research was the mollusc's genetic uniqueness. 



Detailed examination of specific gene sequences emphasized that the mystery mollusk is distinct enough from other known nudibranchs to merit the creation of a new family, Bathydeviidae.



"What is exciting to me about the mystery mollusk is that it exemplifies how much we are learning as we spend more time in the deep sea, particularly below 2,000 meters," said Haddock.



"For there to be a relatively large, unique, and glowing animal that is in a previously unknown family really underscores the importance of using new technology to catalog this vast environment. The more we learn about deep-sea communities, the better we will be at ocean decision-making and stewardship.”



<h2 class="wp-block-heading" id="h-wealth-of-deep-sea-discoveries">Wealth of deep-sea discoveries</h2>



This discovery is just one exciting piece in the puzzle of <a href="https://www.earth.com/news/new-species-of-deep-sea-squid-discovered-that-broods-giant-eggs/" target="_blank" rel="noreferrer noopener">deep-sea exploration</a>. MBARI's state-of-the-art technology has unveiled over 250 previously unknown deep-sea species to date, encouraging us to plunge deeper into these fascinating, otherworldly realms.



“Deep-sea animals capture the imagination. These are our neighbors that share our blue planet. Each new discovery is an opportunity to raise awareness about the deep sea and inspire the public to protect the amazing animals and environments found deep beneath the surface,” said Robison.



Indeed, each new discovery brings us one step closer to fully understanding and protecting our fascinating blue planet. And with this latest revelation of the mystery mollusk, we get to marvel at another fascinating dweller of the deep.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0967063724001845?via%3Dihub" target="_blank" rel="noreferrer noopener">Deep Sea Research</a>.



Image/ Video Credit: MBARI



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Mystery mollusk: Glowing creature found in the deep ocean

Researchers recently revealed a stunning new species of sea slug...

Across the globe, approximately 8.7 million different plant species exist, with around a quarter of them dwelling in the ocean.



For centuries, our understanding of these species, particularly those on land, has been largely shaped by their physical characteristics. 



The process of identifying species based on their morphological characteristics was first established by 18th-century scientist Carl Linnaeus.



However, new findings suggest that this method may not be as comprehensive as we once thought. The research suggests that DNA holds the key to uncovering the identities of plants. 



<h2 class="wp-block-heading" id="h-using-dna-to-identify-plant-species">Using DNA to identify plant species</h2>



While Linnaeus's method has guided our identification of species for centuries, advancements in technology have ushered in a new era of species identification - through <a href="https://www.earth.com/news/largest-ever-ocean-dna-study-uncovers-mysteries-of-marine-life/" target="_blank" rel="noreferrer noopener">DNA sequencing</a>. 



Over the last decade, biologists have begun to depend heavily on DNA sequencing to distinguish between species more accurately. This approach typically involves analyzing a single, species-specific site in the DNA, but it's not foolproof.



"There are times when different plant species are difficult to characterize from a small DNA sequence. But now DNA sequencing has taken several steps forward and we have been able to identify completely new species by analyzing a larger part of the genome," explained Zaynab Shaik, author of a doctoral thesis at the <a href="https://www.gu.se/en" target="_blank" rel="noreferrer noopener">University of Gothenburg</a>.



<h2 class="wp-block-heading" id="h-the-case-of-the-cryptic-daisies">The case of the cryptic daisies</h2>



Shaik's research zeroes in on a group of daisies in the Cape Province of her native South Africa. This collection comprises 66 recognized species, and the first of these species was described in 1753.



Despite their prevalence and commonality, some daisies in the region have puzzled botanists. These "cryptic" plants appear identical in leaf and flower structure, growth habit, and distribution, yet they boast significant <a href="https://www.earth.com/news/just-a-few-genetic-differences-tailor-flowers-to-specific-pollinators/" target="_blank" rel="noreferrer noopener">genetic differences</a>.



"It is important that we have a better understanding of plant relationships and <a href="https://www.earth.com/news/animal-tracking-is-crucial-for-preserving-biodiversity/" target="_blank" rel="noreferrer noopener">biodiversity</a> on Earth. It is easy to imagine how wrong it could be if we discover that a plant is suitable for use as a base in a drug, and then we pick another, similar, species instead, which may not have the same properties at all," said Shaik.



<h2 class="wp-block-heading" id="h-dna-reveals-new-plant-species">DNA reveals new plant species </h2>



Shaik's DNA analyses of these cryptic daisies have led to the unmasking of four new species. She noted that these species aren't new creations hidden in unexplored terrains. 



"When I'm asked about this, there's a bit of an anti-climax when I explain that it's not that I've found a new daisy in a remote location that no one has seen before. But these have been admired for a long time, but they have been mistaken for another species."



Shaik's identification method, known as integrative taxonomy, merges traditional observational techniques with modern DNA sequencing. 



This combination enhances our knowledge of species boundaries and is expected to ramp up the rate of new species discovery.



<h2 class="wp-block-heading" id="h-many-more-discoveries-to-be-made">Many more discoveries to be made</h2>



Shaik hints at a possible underestimation of the biodiversity in the Cape region and, by extension, other parts of the world. 



"In the Cape, it has been thought that only 1 percent of biodiversity remains to be discovered. My results suggest that it could be much more than that. And the same should reasonably apply to other areas of the globe."



Thus, <a href="https://www.earth.com/news/saving-parrots-in-the-illegal-wildlife-trade-with-dna-technology/" target="_blank" rel="noreferrer noopener">DNA technology</a>, progressing hand in hand with traditional methods, is undeniably reshaping our understanding of Earth's biodiversity. 



As we continue to unravel more secrets within the realm of genetics, the question arises: how much more of nature's mysteries are waiting to be unveiled?



<h2 class="wp-block-heading" id="h-technology-and-plant-species-discovery">Technology and plant species discovery</h2>



The integration of DNA sequencing with traditional taxonomy, known as integrative taxonomy, is becoming the cornerstone of modern biodiversity studies. 



Unlike conventional methods that rely solely on observable physical traits, this approach combines morphological analysis with molecular data, offering a multi-dimensional view of species identification. 



This hybrid method addresses limitations found in singular approaches and helps clarify ambiguities, particularly in species with minimal visible differences.



Integrative taxonomy is not only accelerating the pace of <a href="https://www.earth.com/news/mushroom-magic-new-species-discovered-in-africa/" target="_blank" rel="noreferrer noopener">species discovery</a> but also refining conservation strategies.



By identifying genetic differences that aren't apparent through morphology alone, researchers can better understand which populations may be at risk and develop more effective protection measures. 



This evolving field highlights the importance of embracing modern technology alongside traditional scientific practices to enrich our understanding of life on Earth.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/abs/pii/S025462992400320X?via%3Dihub" target="_blank" rel="noreferrer noopener">South African Journal of Botany</a>.



Image Credit: Zaynab Shaik



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DNA technology will accelerate the pace of plant species discovery

Across the globe, approximately 8.7 million different plant species exist,...

Who invented the wheel? This question has been a topic of debate for centuries. But because it predates recorded history, the exact inventor of the wheel has remained unknown.



Despite the wheel's undeniable importance in human history, its origins have been shrouded in mystery and speculation. What we do know is that the wheel likely evolved over time from simpler tools.



<h2 class="wp-block-heading" id="h-redefining-the-origins-of-the-wheel">Redefining the origins of the wheel</h2>



A new study on the evolution of the wheel has pushed the clock back by 6,000 years, offering new and compelling insights into this fascinating puzzle.



This discovery represents an exciting development that shatters the conventional timeline, moving it far beyond the previously accepted era of 4000 BC in ancient <a href="https://www.earth.com/news/mesopotamian-bricks-reveal-anomaly-in-earths-magnetic-field-3000-years-ago/" target="_blank" rel="noreferrer noopener">Mesopotamia</a>.



It was during that period when the wheel was first recognized as an essential tool, initially used in pottery-making and preceding the <a href="https://www.earth.com/news/bronze-age-teeth-discovery-highlight-the-evolution-of-the-human-diet/" target="_blank" rel="noreferrer noopener">Bronze Age</a> innovation of wheeled vehicles by centuries.



This newfound understanding prompts a reevaluation of how early humans harnessed rotational technology and its transformative impact on the trajectory of human civilization.



<h2 class="wp-block-heading" id="h-development-of-rotational-tools">Development of rotational tools</h2>



The spotlight is now shining on an archaeological discovery in Israel that has potentially rewritten this humble invention’s history and shifted our understanding of early human ingenuity.



Over a hundred perforated pebbles - primarily composed of limestone and bearing a circular shape with a central hole - were unearthed at the Nahal-Ein Gev II site, a location that has already provided valuable insights into <a href="https://www.earth.com/news/prehistoric-women-were-not-just-gatherers-they-were-hunters-too/" target="_blank" rel="noreferrer noopener">prehistoric</a> life.



This extraordinary find represents a key milestone in the development of rotational tools, including our beloved wheel, and emphasizes the sophisticated craftsmanship and resourcefulness of <a href="https://www.earth.com/news/kids-in-hunter-gatherer-stone-age-societies-had-better-parenting-than-modern-children/" target="_blank" rel="noreferrer noopener">early societies</a>.



It reveals not only the ingenuity behind these tools but also hints at the broader implications for the evolution of technology and innovation in human history.



<h2 class="wp-block-heading" id="h-invention-of-a-wheel-shaped-tool">Invention of a wheel-shaped tool</h2>



What's astonishing is that these ancient stones date back to approximately 12,000 years, far surpassing any previously known examples. 



Scholars from the <a href="https://en.huji.ac.il/" target="_blank" rel="noreferrer noopener">Hebrew University of Jerusalem</a> suggest that these stones served as spindle whorls - round weighted objects attached to a spindle stick.



This tool was instrumental in gathering fibers such as wool and spinning them into yarn, demonstrating the human use of rotation with a wheel-shaped tool.



<h2 class="wp-block-heading" id="h-the-first-wheels-in-form-and-function">The first wheels in form and function </h2>



Professor Leore Grosman emphasized the importance of these artifacts, describing them as early examples of wheel-shaped tools connected to a rotating axle.



"These perforated stones are actually the first wheels in form and function - a round object with a hole in the center connected to a rotating axle, used long before the appearance of the wheel for transportation purposes," said Professor Grosman.



This early use eventually paved the way for more advanced wheel-based rotational inventions, including the renowned potter's wheel and, later, the significantly useful cart wheel.



<h2 class="wp-block-heading" id="h-fingerprints-of-prehistoric-innovation">Fingerprints of prehistoric innovation</h2>



"The most important aspect of the study is how modern technology allows us to delve deep into touching the fingerprints of the prehistoric craftsman, then learn something new about them and their innovativeness, and at the same time, about our modern technology and how we're linked," noted the researchers.



Their study embodies the "wheel and axle" concept, a revolutionary mechanism that triggered technology's transformation from linear to rotary motion.



The paper concludes that the ancient origins tied to the carts' prominence during the Bronze Age now focus on a much-earlier wheel-shaped tool.



So, the next time you marvel at the complexity of modern machinery, remember its connection to these humble stones from 12,000 years ago, and appreciate the role of human innovation throughout the ages.



<h2 class="wp-block-heading" id="h-human-ingenuity-and-innovation">Human ingenuity and innovation</h2>



This discovery not only enriches our understanding of early <a href="https://www.earth.com/news/400000-year-old-stone-tools-show-technological-adaptations-of-prehistoric-humans/" target="_blank" rel="noreferrer noopener">technological advancements</a> but also illustrates the seamless progression from simple tools to complex mechanisms.



The spindle whorls unearthed at Nahal-Ein Gev II showcase the fundamental principles of rotational technology, a concept that would eventually lead to the wheel's application in pottery, transportation, and machinery.



By examining these early developments, researchers draw parallels between ancient creativity and modern technology, highlighting the continuous thread of human ingenuity through the ages.



The study is published in the journal <a href="https://search.app?link=https%3A%2F%2Fjournals.plos.org%2Fplosone%2Farticle%3Fid%3D10.1371%2Fjournal.pone.0312007&amp;utm_campaign=aga&amp;utm_source=agsadl2%2Csh%2Fx%2Fgs%2Fm2%2F4" target="_blank" rel="noreferrer noopener">Plos One</a>.



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Who invented the wheel? It all started with stones

Who invented the wheel? This question has been a topic...

THC, the main psychoactive ingredient in cannabis, is being used by more pregnant women as the legalization of recreational cannabis gains ground. Women who are expecting often use cannabis for morning sickness, lower back pain, or anxiety relief.



Recent figures indicate that up to 1 in 5 pregnant women in the U.S. now use cannabis. However, growing research suggests that THC exposure could pose significant risks to the developing fetus.



A recent study highlights how prenatal exposure to THC may increase the risk of opioid addiction later in life.



<h2 class="wp-block-heading" id="h-thc-rewires-the-fetal-brain">THC rewires the fetal brain</h2>



The preclinical animal study, led by researchers at the <a href="https://www.medschool.umaryland.edu/" target="_blank" rel="noreferrer noopener">University of Maryland School of Medicine</a> and published in the journal Science Advances, revealed that prenatal exposure to THC rewires the fetal brain.



According to the study, THC made certain <a href="https://www.earth.com/news/covid-19-makes-you-feel-moody-and-sad-by-depleting-dopamine/" target="_blank" rel="noreferrer noopener">dopamine</a> neurons hyperactive, resulting in a marked increase in dopamine release and an amplified response to reward-related cues, such as a signal indicating the availability of food or an opioid drug.



“Doctors are contending with an explosion of cannabis use, and the THC content has quadrupled from what it was a generation ago,” said Dr. Joseph Cheer, a professor of Neurobiology and Psychiatry at the University of Maryland School of Medicine.



“It demonstrates the enduring consequences that prenatal cannabis exposure exerts on the brain’s reward system, which ultimately results in a neurobiological vulnerability to <a href="https://www.earth.com/news/opioid-related-deaths-are-on-the-rise-among-young-people/" target="_blank" rel="noreferrer noopener">opioid</a> drugs.”



<h2 class="wp-block-heading" id="h-prenatal-exposure-to-thc">Prenatal exposure to THC</h2>



The study revealed that prenatal exposure to THC led to significant changes in the brain's reward system, particularly in male animals. 



These animals displayed an exaggerated surge in the "reward-seeking" brain chemical dopamine when exposed to opioid drugs during adolescence, compared to those not exposed to THC.



Even moderate doses of THC - equivalent to one to two joints per day in humans - altered how the fetal brain processed rewards, fostering behavior suggestive of increased opioid-seeking.



This behavior was confirmed by follow-up experiments where tiny sensors implanted in their brains detected heightened dopamine release and over-activation of neurons linked to reward-seeking behavior.



“These observations support the hypothesis of a hypersensitized ‘wanting’ system that develops in the brain after exposure to THC during <a href="https://www.earth.com/news/prenatal-cannabis-exposure-has-unexpected-effect-on-infant-language/" target="_blank" rel="noreferrer noopener">prenatal</a> development,“ said Dr. Cheer. 



"Interestingly, we found that this opioid-seeking phenotype occurs significantly more in males compared to females, and we are currently performing research with our colleagues at UMSOM to determine why this is the case.”



<h2 class="wp-block-heading" id="h-advancing-research-and-guidance">Advancing research and guidance </h2>



Dr. Cheer and his colleague, Dr. Mary Kay Lobo, co-direct the Center for Substance Use in Pregnancy at the University of Maryland School of Medicine’s Kahlert Institute for Addiction Medicine. 



Their ongoing research aims to further understand the long-term impact of <a href="https://www.earth.com/news/prenatal-thc-exposure-linked-to-life-long-health-risks/" target="_blank" rel="noreferrer noopener">drug exposure during pregnancy</a>.



“We need to more fully understand the enduring effects of THC exposure in the womb and whether we can reverse some of the deleterious effects through CRISPR-based gene therapies or repurposed drugs," said study co-author Dr. Dean Mark T. Gladwin.



"We also need to provide better advice to pregnant patients, many of whom are using cannabis to help control anxiety because they think this drug is safer for their baby than traditional anti-anxiety medications.”



<h2 class="wp-block-heading" id="h-cannabis-use-during-pregnancy">Cannabis use during pregnancy </h2>



The findings suggest that there is a need for more exhaustive public health programs to educate pregnant women on the long-term effects that coincide with <a href="https://www.earth.com/news/record-number-of-americans-are-high-on-marijuana-at-work/" target="_blank" rel="noreferrer noopener">marijuana</a> exposure during pregnancy. 



Previous studies on cannabis use during pregnancy have also raised significant concerns about its potential impacts on fetal development and maternal health.



For example, studies have linked prenatal cannabis exposure to deficits in attention, memory, and executive functioning in children. 



Furthermore, cannabis use during pregnancy is associated with an increased risk of low birth weight, which can lead to complications such as developmental delays and long-term health issues.



Guidelines on pregnancy and provision of adequate resources for pregnant women could be created and harmonized in collaboration between healthcare providers, researchers, and policymakers.



Investments in supplemental research, which would include human studies, may also clarify how exposures to THC impact the fetal brain in its developing state. 



The study is published in the journal <a href="https://www.science.org/doi/10.1126/sciadv.adq5652" target="_blank" rel="noreferrer noopener">Science Advances</a>.



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Cannabis use during pregnancy rewires the fetal brain

THC, the main psychoactive ingredient in cannabis, is being used...

Usually, we see ants forming a single file, following a scent trail to a food source and returning back to their nest. However, what happens when there are multiple food sources available? 



Well, the ants in this scenario create a network of trails connecting their nest to all the available food sources. This is the conclusion of a fascinating new study from Florida State University.



Bhargav Karamched, an assistant professor of mathematics at Florida State University (FSU), is the lead researcher.



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



"Social insect behavior has fascinated the biological community for a long time. The collective behavior of insects can be used to achieve more complicated outcomes than possible for individuals," noted the researchers.



"This is especially important for ant species that rely on communication via pheromone to coordinate activity."



Working in <a href="https://www.fsu.edu" target="_blank" rel="noreferrer noopener">FSU</a>’s Institute of Molecular Biophysics, Karamched and his team have created a pioneering model that explains the phenomenon of trail formation to multiple food sources.



<h2 class="wp-block-heading" id="h-ants-with-multiple-food-sources">Ants with multiple food sources</h2>



"The power of mathematics is that we can devise models that reproduce experimentally observed data and make concrete predictions about what will happen next," Karamched noted.



“In this case, we uncovered something that hasn’t been described well by other models: if an ant has access to multiple food sources from its nest, it will initially make multiple trails to each of the sources.”



The research has unveiled how ants, when presented with multiple food sources, initially make multiple trails to <a href="https://www.earth.com/news/ants-are-now-using-cars-to-travel-spread-to-new-locations/" target="_blank" rel="noreferrer noopener">each source</a>.



Graduate student and study lead author Sean Hartman expressed his lifelong interest in mathematics which led him to pursue research in this field.



“I was intrigued by ant trail research that Dr. Karamched shared with me and became interested in pursuing further research on it and creating models based on this previous work,” he said.



<h2 class="wp-block-heading" id="h-secret-behind-the-ants-food-hunt">Secret behind the ants' food hunt</h2>



For ants, foraging is not just a daily activity, it's a necessity for their survival. They use chemical pheromones for self-organization. 



Once a food source is detected, the ant secretes these chemicals as a trail marker for its fellow <a href="https://www.earth.com/news/climate-change-is-destabilizing-ant-plant-relationships/" target="_blank" rel="noreferrer noopener">ants</a>. 



Karamched's team factored this behavior into their computational simulations which also showed that ants eventually prefer the food source closer to their nest in an environment with multiple sources.



The researchers divided <a href="https://www.earth.com/news/larger-ant-colonies-drove-the-evolution-of-worker-castes/" target="_blank" rel="noreferrer noopener">ants</a> into two groups: foragers who wander in search of food, and returners who head straight for the nest after finding food. 



“These subpopulations behave differently, as foragers tend to wander around in search of food while returners always return directly to the nest after finding food, making their motion less stochastic or random," Karamched explained.



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



The research team considered the concentration of pheromones secreted by the ants - the higher the concentration, the stronger the scent trail for others to follow. 



Interestingly, ants returning from a food source close to the nest secrete fewer pheromones. Hartman's coding simulations produced insights into this pheromone-based decision-making process.



“Once my code was fully tested and accurate, multiple trail formations became distinct and were easily understandable,” Hartman said. 



“It was so cool to see how equidistant food sources could maintain multiple food trails as an equilibrium. If one food source was just slightly closer to the ants’ nest, the ants would eventually form one singular trail to the closest source. It was at this moment that it felt all our hard work finally paid off.”



<h2 class="wp-block-heading" id="h-using-chemical-signals-to-communicate">Using chemical signals to communicate</h2>



The model devised by Karamched's team isn't just limited to <a href="https://www.earth.com/news/ant-queens-turn-to-cannibalism-recycle-bodies-for-colony-disease-control/" target="_blank" rel="noreferrer noopener">ants</a>. Its simplicity and focus on pheromone gradients make it applicable to other organisms and biological systems that communicate using pheromones. 



This could include bacteria, slime molds, other insects, fish, and even some reptiles and mammals.



According to Karamched, the fundamental pheromone concentration gradient is the underpinning factor that analyzes collective behavior. 



“From a microbial level to complex organisms, using this chemical signaling to communicate allows certain organisms to coordinate activity on huge spatial scales, which is fascinating.”



The seemingly simple act of ants foraging for food, decoded with mathematics and simulations, offers new insights into the world of these hardworking insects.



The study is published in the <a href="https://link.springer.com/article/10.1007/s00285-024-02136-2" target="_blank" rel="noreferrer noopener">Journal of Mathematical Biology</a>. 



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Ants create chemical trails to guide their friends to food

Usually, we see ants forming a single file, following a...

"Go outside and play!" - a phrase many of us heard growing up and one that is echoing through the halls of schools across Quebec, with an unexpected twist. It's not just playtime that is being taken outdoors, but actual class time.



This approach was backed by research showing that spending time in natural settings bolsters mental health in children. This one-of-a-kind initiative is transforming the way we see education and childhood development.



<h2 class="wp-block-heading" id="h-nature-as-a-teaching-tool">Nature as a teaching tool</h2>



This research was led by Sylvana Côté from the Observatoire pour l’éducation et la santé des enfants (<a href="https://www.observatoireenfants.ca/fr/" target="_blank" rel="noreferrer noopener">OPES</a>) and a group of dedicated researchers from McGill and Université de Montréal. 



The fascinating study reveals that merely two hours of class time spent outdoors significantly reduces emotional distress among children aged 10-12 who previously struggled with <a href="https://www.earth.com/news/supportive-adults-help-protect-children-from-mental-health-issues/" target="_blank" rel="noreferrer noopener">mental health</a> concerns.



These findings could not be more timely, considering a recent UNICEF report which emphasized the importance of green spaces for child development.



<h2 class="wp-block-heading" id="h-impact-of-outdoor-classes">Impact of outdoor classes</h2>



The researchers studied the effects of <a href="https://www.earth.com/news/world-environment-day-the-critical-role-of-nature-in-human-well-being/" target="_blank" rel="noreferrer noopener">nature time on the behavior</a> and mental health symptoms of over 500 Quebec schoolchildren in Spring 2023.



The transformation seen in children post-intervention confirm that nature operates as a unique form of therapy. 



The students who benefited the most were those grappling with severe issues earlier, including anxiety, depression, aggressivity, impulsivity, and social interaction problems.



<h2 class="wp-block-heading" id="h-calmness-and-attentiveness">Calmness and attentiveness </h2>



After the intervention, teachers noticed a pronounced calmness and attentiveness in their students, hinting at nature's role as a catalyst for mental quietude and focus.



Study senior author Marie-Claude Geoffroy is an associate professor in the McGill Department of Psychiatry and Canada Research Chair in Youth Mental Health and Suicide Prevention at the Douglas Research Centre.



"Children with higher mental health symptoms at baseline showed greater reductions in symptoms following the intervention," said Professor Geoffrey.



<h2 class="wp-block-heading" id="h-outdoor-classes-improve-mental-health">Outdoor classes improve mental health</h2>



"Nature-based programs may offer targeted benefits for children with higher levels of mental health vulnerabilities and potentially act as an equalizer of mental health among school-age children," noted Côté.



First, a randomized controlled trial was used to depict the genuine advantages children experience from spending time <a href="https://www.earth.com/news/mental-health-the-hidden-casualty-of-climate-change/" target="_blank" rel="noreferrer noopener">amidst nature</a>. Over a thousand children, ranging in age from 10 to 12 and from diverse socio-economic backgrounds, participated with a control group in the mix.



According to Professor Geoffery, the motivation for this project arose during the height of the pandemic, when concerns regarding children's health risks from being confined indoors were soaring.



This prompted the idea of an intervention where school children could spend time in nature, with effects measured on their mood and behavior.



<h2 class="wp-block-heading" id="h-monitoring-changes-after-outdoor-classes">Monitoring changes after outdoor classes</h2>



Over a three-month period, changes in the behaviors of both the nature-intervention and control groups were evaluated using quick questionnaires. The goal was to gauge children's emotional and behavioral difficulties and their strengths.



The children were not merely frolicking in the park for two hours. Teachers conducted regular classes such as math, languages, or science outdoors.



A short, 10-15 minute activity designed to boost mental health was also integrated into these sessions using resources provided by the research team.



<h2 class="wp-block-heading" id="h-potential-impact-on-education-systems">Potential impact on education systems</h2>



<a href="https://www.umontreal.ca/en/" target="_blank" rel="noreferrer noopener">Université de Montréal</a> post-doctoral fellow Tianna Loose, the paper's first author, emphasizes the relevance of their results for educators, policy-makers, and mental health professionals. 



"The intervention was low-cost, well-received, and posed no risks, making it a promising strategy for schools with access to greenspaces," she said.



The research team is excited about designing a follow-up study on outdoor classes involving teenagers that will co-design an intervention in nature to enhance well-being, reduce climate anxiety, and promote a deeper <a href="https://www.earth.com/news/natural-biodiversity-areas-have-greater-mental-health-impact/" target="_blank" rel="noreferrer noopener">connection to nature</a>.



This transformation in classroom dynamics has opened up a new avenue not just in education but also in mental health interventions. It adds credence to the phrase "the best classroom is roofed only by the sky." 



As societies, we need to reevaluate and appreciate the boundless potential of nature, especially in nurturing the mental health of our younger generations. 



The study is published in the journal <a href="https://jamanetwork.com/journals/jamanetworkopen/fullarticle/2826214" target="_blank" rel="noreferrer noopener">JAMA Network Open</a>.



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Outdoor classes improve children's mental health

"Go outside and play!" - a phrase many of us...

Dogs have moved from kennels to the coziest corners of our homes, carving out an irreplaceable role in our hearts. They are no longer "just pets"- dogs are friends, family, guardians, and even considered children to some. 



Recent research from the Department of Ethology at Eötvös Loránd University (ELTE) examines these relationships, shining a light on how societal trends and personal owner profiles shape the care provided to dogs.



<h2 class="wp-block-heading" id="h-human-dog-relationships">Human-dog relationships</h2>



In Western cultures, the shift in human-dog relationships is remarkable. The <a href="https://www.earth.com/news/dogs-can-feel-our-emotions-through-our-heart-rate/" target="_blank" rel="noreferrer noopener">pooch</a> has ascended the status ladder to become man's best friend, a cherished family member, or even a furry dog child. 



This change is so pronounced that up to two-thirds of dog owners affirm their dog to be more important than any human in their lives.



Why has humanity's friendship with dogs strengthened so intensely? 



A considerable factor could be the demographic transition of the last few decades, evident through smaller families and declining birth rates. 



As people feel increasingly lonely and socially isolated, dogs have emerged as comforting companions, filling a void left by human contact. But how does this trend affect the daily lives of dogs? That's exactly the question for which ELTE researchers sought answers.



<h2 class="wp-block-heading" id="h-what-makes-dogs-so-lovable">What makes dogs so lovable?</h2>



In their quest to identify why dogs are so treasured, <a href="https://www.elte.hu/en/" target="_blank" rel="noreferrer noopener">ELTE</a> researchers analyzed questionnaire data from approximately 800 dog owners. 



The results? A resounding 97.6% of owners relished the physical contact with their <a href="https://www.earth.com/news/dogs-are-evolving-to-fit-the-modern-lives-of-humans/" target="_blank" rel="noreferrer noopener">dogs</a>, while 93.7% preferred the unconditional love their canines provided, and 88.4% admired the aesthetics of their four-legged friends. 



However, the percentages varied when it came to social interactions generated by dogs, with 24.3% of owners not finding it beneficial.



<h2 class="wp-block-heading" id="h-roles-of-dogs-in-families-and-beyond">Roles of dogs in families and beyond</h2>



The study allowed owners to assign numerous roles to their dogs - friend, family member, child, colleague, domesticated animal, or security guard.



"We found three distinct profiles of owners whose dogs played diverse social and practical roles," said Laura Gillet, PhD student at the Department of Ethology and lead author of the study.



For example, some owners saw their dogs in dual roles - as colleagues and security guards, and as their most cherished companions.



<h2 class="wp-block-heading" id="h-dog-parents-and-companion-dogs">Dog parents and companion dogs</h2>



Another group of owners, tagged "dog parents," saw their dogs in human-like roles without any practical functions. There was also a group of owners who kept dogs primarily for companionship, albeit having a greater <a href="https://www.earth.com/news/how-human-speech-changes-when-we-talk-to-dogs/" target="_blank" rel="noreferrer noopener">emotional distance</a> from their pets.



The researchers also factored in the type of dogs owned. For instance, dogs with dual roles were from breeds known for their working abilities, such as Border Collie, Belgian Shepherd Dog, and German Shepherd Dog. 



Owners keeping dogs for companionship preferred the Mudi, the English Cocker Spaniel, and the Labrador Retriever breeds, and were generally older. 



"Dog parents," on the other hand, preferred Border collies, Vizsla, Boxer, and Dachshund, and were more likely to house their dogs indoors only.



<h2 class="wp-block-heading" id="h-should-dogs-be-part-of-family">Should dogs be part of family?</h2>



The researchers also collected data about the behavioral problems in dogs, often seen as indicators of canine welfare. 



However, no matter the roles owners attributed to their dogs, no association was found between these roles and the perceived behavioral problems in dogs.



This finding suggests that attributing human-like roles to dogs had no negative impact on their well-being.



<h2 class="wp-block-heading" id="h-changing-dynamics-of-dogs-and-owners">Changing dynamics of dogs and owners</h2>



The bottom line? Dogs can assume various roles in our lives, offering distinct benefits. This unique research methodology unravels the intricacies of the dog-human bond and the implications it might have on the <a href="https://www.earth.com/news/this-simple-technique-instantly-reduces-heat-stress-in-dogs/" target="_blank" rel="noreferrer noopener">dogs' daily lives</a>. 



Younger owners, in particular, appear to forge stronger emotional ties with their dogs and more commonly refer to them as their children than the older generations. 



This generational shift in how we perceive our relationship with dogs demands more exhaustive research, not just for the well-being of our four-legged friends, but to understand what it says about our evolving families and societies.



Dogs have indeed become more to us than mere pets. They've become companions that walk with us through life's highs and lows, offering comfort and joy. 



As we unravel the dog-human dynamic further, it's clear that our furry friends are here to stay, not just in our homes, but also in the deepest corners of our hearts.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0169809524005398?via%3Dihub" target="_blank" rel="noreferrer noopener">Atmospheric Research</a>.&nbsp;



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Friends, family members, and guardians: Dogs are more than just pets

Dogs have moved from kennels to the coziest corners of...

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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

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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...

Huge burn scar from the California Sand Fire. The Sand Fire, in the <a href="https://www.earth.com/image/huge-burn-scar-from-the-california-sand-fire/">Santa Clarita</a> area northwest of Los Angeles, has burned more than 41,000 acres, destroyed 18 houses and caused one fatality. By August 1, 2016, when the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on <a href="https://en.wikipedia.org/wiki/NASA">NASA’s</a> Terra spacecraft acquired this image, the fire was more than 90 percent contained. The fire began July 22 in a brushy area near Highway 14. It grew explosively to thousands of acres, driven by high winds and temperatures over 100 degrees Fahrenheit (38 degrees Celsius).
At one time, more than 10,000 homes were evacuated. In this image, vegetation is displayed in red, and the burn area is the irregularly shaped dark area in the middle of the image. The image covers an area of 16.4 by 19.4 miles (26.4 by 31.3 kilometers) and is located at 34.4 degrees north, 118.3 degrees west. Therefore the Huge burn scar from the California Sand Fire has causes a lot of damage tot he area and terrain. Also seen in the image above the fire spread so far causing the damage to be a wide range.
Credit: <a href="http://www.nasa.gov" target="_blank" rel="noopener noreferrer">NASA</a>/METI/AIST/Japan Space Systems, and U.S./Japan ASTER Science Team

Huge burn scar from the California Sand Fire

In July 2016, a massive and mysterious avalanche sent glacial ice and rock spilling down a valley in the Aru Range of Tibet. Leading glaciologists were baffled by what might have caused the ice avalanche in Tibet, which killed nine people. In the months before, temperatures had been normal, and there was nothing out of the ordinary about the rainfall. Most surprisingly, the part of the glacier that collapsed sat on fairly flat terrain.

In September 2016, the story got even stranger. A second massive avalanche occurred just a few kilometers to the south of the first. “Even one of these gigantic glacier avalanches is very unusual,” said Andreas Kääb, a glaciologist at the University of Oslo. “Two of them within close geographical and temporal vicinity is, to our best knowledge, unprecedented.”

Several Earth-observing satellites have acquired imagery of these twin avalanches. In the set of images at the top of the page, the June 24 image shows the area before either avalanche occurred; the July 21 image shows the first avalanche; the September 24 image shows the area after both avalanches. The June 24 and July 21 natural-color images were acquired by Landsat 8 and Sentinel-2, respectively. A synthetic aperture radar (SAR) on the Sentinel-1A satellite captured the September 24 image.

Notice that the older avalanche appears significantly darker than the newer one in the SAR image. The brightness of a radar image varies based on the “roughness” of the surface and how much moisture it contains. Rougher surfaces and those with low water content appear brighter. The first avalanche either had a smoother and/or wetter surface than the newer avalanche, most likely because ice on the surface of the older avalanche has been exposed longer and had time to partially melt. Distinguishing between wetness and surface roughness based on this satellite imagery is not possible.

[caption id="attachment_90208" align="alignleft" width="150"]<img class="size-thumbnail wp-image-90208" src="http://www.earth.com/wp-content/uploads/2016/10/tibet-ice-avalanche-062416-092416_1big_aster_nasa-150x150.jpg" alt="Tibet ice avalanche images, June 24, July 21, September 24, 2016" width="150" height="150" /> Tibet ice avalanche images, June 24, July 21, September 24, 2016[/caption]

Below, an image from the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite shows both avalanches in false color. This image was acquired on October 4, 2016.

Ever since the first avalanche, scientists affiliated with the International Association of Cryospheric Sciences and the International Permafrost Association have been racing to understand what caused it. While analyzing optical and radar data from satellites for the months prior to the collapse, they noticed a distinctive pattern of crevasses on the glacier surface, as well as changes in the height. Both suggested that it was in the process of surging—a term glaciologists use to describe the unusually rapid flow of ice from the upper part of a glacier to the lower part.

Though ice in a surging glacier can flow 10 to 100 times faster than usual, there have been no documented cases of surging glaciers causing abrupt and violent collapses. However, in the case of the Tibet glaciers, observations made by Sentinel and other satellites suggest that the surging process may have primed the glaciers for collapse. The first glacier started to surge by at least September 2015, but then stalled a few months later as the flow reached a narrow valley. Computer simulations conducted by a team of Swiss scientists suggest that the blockage caused extra water to build up beneath and inside the glacier, and that the extra lubrication made the glacier more likely to collapse. The pooling of melt water (light blue) on the glacier surface in the lower third of the ASTER image provides another line of evidence that excess lubrication was part of the collapse.

While avalanches are difficult to predict, the scientists detected clues that a second avalanche was poised to happen. Seeing the same telltale crevasses and changes in elevation that preceded the first collapse, the team warned Chinese scientists and government officials on September 21, 2016, that a second avalanche appeared to be imminent to the south. The warning turned out to be just a little too late. Just a few hours before the warning arrived, the second glacier had already collapsed in spectacular fashion, sending another huge load of ice spilling toward Aru Co.

The search for the precise causes of the avalanches continues. Despite their close proximity, Kääb says there is no evidence of a direct physical connection between the glaciers or their collapse. The similarities between the two events imply that shared factors—such as short-term weather conditions, longer term climate change, and the underlying geological or topographic environment—may have played a role.

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Credit: <a href="http://www.nasa.gov" target="_blank">NASA</a>