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, 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 in visible light is actually a less massive companion, while the fainter, dimmer star is the dying, hot central star that has shed its outer layers to form the nebula. This 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. 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,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



“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. 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>.&nbsp;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 formed from 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, though it is partially visible in the Northern Hemisphere as well. 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...

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Luminous galaxy NGC 3783 and a blue giant star

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



The gas that fuels <a href="https://www.earth.com/news/black-hole-is-starving-its-host-galaxy-of-star-forming-fuel/" target="_blank" rel="noreferrer noopener">star formation</a> can be used up, or it can be heated and pushed out of galaxies by supernovae or black holes, reducing the galaxy's ability to form new stars.



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



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



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



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



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



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



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



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



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NGC 1792: A galactic powerhouse 

Today's Image of the Day from the European Space Agency features the galaxy I Zwicky 18, which was captured in remarkable detail by the James Webb Space Telescope.



I Zwicky 18 is a blue compact dwarf <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">galaxy</a> located approximately 59 million light-years away in the constellation Ursa Major.&nbsp;



<h2 class="wp-block-heading" id="h-star-formation-in-i-zwicky-18">Star formation in I Zwicky 18</h2>



The galaxy is notable for its relatively young appearance and the fact that it contains very few heavy elements. These characteristics indicate that it has experienced little <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> compared to other galaxies of similar age.



“The galaxy was first identified by Swiss astronomer Fritz Zwicky in the 1930’s and resides roughly 59 million light-years from Earth,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>. “This galaxy has gone through several sudden bursts of star formation.” 



According to ESA, I Zwicky 18 is typical of the kinds of galaxies that inhabited the early universe and is much smaller than our <a href="https://www.earth.com/news/runaway-star-j1249-36-spotted-trying-to-escape-our-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



<h2 class="wp-block-heading" id="h-webb-telescope-image-of-the-galaxy">Webb telescope image of the galaxy</h2>



“Two major starburst regions are embedded in the heart of the galaxy. The wispy brown filaments surrounding the central starburst region are bubbles of gas that have been heated by stellar winds and intense ultraviolet radiation unleashed by hot, young stars,” noted ESA.



“A companion galaxy resides nearby to the dwarf galaxy, which can be seen at the bottom of the wider-field image. The companion may be interacting with the dwarf galaxy and may have triggered that galaxy's recent star formation.”&nbsp;



ESA explained that the “orange blobs” surrounding the galaxy are the dim glow from ancient fully formed galaxies at much larger distances.



<h2 class="wp-block-heading" id="h-key-characteristics-of-i-zwicky-18">Key characteristics of I Zwicky 18</h2>



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



As previously mentioned, the galaxy has a very low abundance of elements heavier than hydrogen and helium, suggesting that it has not undergone significant stellar processing.



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



Despite its old age, I Zwicky 18 contains many young, hot stars. This suggests that it might have experienced a burst of <a href="https://www.earth.com/news/hubble-detects-awe-inspiring-newborn-star/" target="_blank" rel="noreferrer noopener">star formation</a> relatively recently in its history.



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



The galaxy has a high density of gas, which is a prime ingredient for star formation. This gas is mostly in the form of hydrogen.



<h3 class="wp-block-heading" id="h-unusual-characteristics">Unusual characteristics</h3>



Its characteristics are more typical of primordial galaxies found in the early universe, making it a valuable object of study for understanding galaxy formation and evolution.



Ultimately, I Zwicky 18 provides insights into the conditions and processes that might have been prevalent in the early universe.



<h3 class="wp-block-heading" id="h-life-cycles-of-stars-and-dust">Life cycles of stars and dust</h3>



The image was captured as part of a Webb program to study the life cycle of dust in I Zw 18.&nbsp;



“Scientists are now building off of previous research with Hubble obtained at optical wavelengths, studying individual dusty stars in detail with Webb’s equivalent spatial resolution and sensitivity at infrared wavelengths.”&nbsp;



ESA noted that this galaxy is of particular interest as its content of elements heavier than helium is one of the lowest of all known <a href="https://www.earth.com/news/early-galaxy-formation-occurred-much-faster-than-we-thought/" target="_blank" rel="noreferrer noopener">galaxies</a> in the local universe.&nbsp;



“Such conditions are thought to be similar to those in some of the first star-forming galaxies at high redshift, so the Webb study of I Zw 18 should shed light on the life-cycle of stars and dust in the early universe.”



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



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Dwarf galaxy I Zwicky 18: A glimpse of the early universe

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



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



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



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



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



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



The polar cap is dynamic and changes over time. It becomes more prominent during the summer season of each pole. As Uranus moves along its orbit, the cap's appearance transforms, with the haze becoming thicker and brighter when the pole is in continuous sunlight.



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



Image Credit: NASA, ESA, CSA, STScI



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The ice giant Uranus in stunning detail

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

Today's Image of the Day from NASA Earth Observatory features a plume of Saharan dust pouring off the coast of southern Morocco.



The Sahara Desert is the world's biggest source of <a href="https://www.earth.com/news/dust-is-an-understudied-contributor-to-climate-change/" target="_blank" rel="noreferrer noopener">airborne dust</a>. Each year, it releases hundreds of millions of tons of mineral dust that are lifted into the atmosphere and transported across vast distances up to thousands of miles.&nbsp;



<h2 class="wp-block-heading" id="h-saharan-air-layer-nbsp">Saharan Air Layer&nbsp;</h2>



The transport of Saharan dust is primarily driven by the trade winds and atmospheric phenomena such as the Saharan Air Layer (SAL). This dry air mass often accompanies tropical storms across the Atlantic, sometimes even influencing the development and intensity of <a href="https://www.earth.com/news/saharan-dust-can-intensify-hurricanes/" target="_blank" rel="noreferrer noopener">hurricanes</a>.&nbsp;



“From late spring to early fall, it is common for the dry, dusty Saharan Air Layer to carry the particles westward across the Atlantic Ocean high in the atmosphere. With different wind patterns in the winter and spring, dust emerging from North Africa can drift over the United Kingdom and western Europe at relatively low altitudes,” said <a href="https://earthobservatory.nasa.gov/images/153246/dust-pours-off-the-moroccan-coast" target="_blank" rel="noreferrer noopener">NASA</a>.



“Saharan Air Layer activity subsides after mid-August, according to NOAA, making it less likely that the plume shown here is bound for a transoceanic journey. Instead, it arcs to the north after blowing out over the ocean. Earlier in the summer, however, several clouds of fine dust from the Sahara reached the United States, creating hazy skies over Texas.”



<h2 class="wp-block-heading" id="h-impacts-of-saharan-dust-nbsp">Impacts of Saharan dust&nbsp;</h2>



Saharan dust plays a crucial role in global climate and environmental systems. For example, Saharan dust can affect weather patterns by absorbing and scattering sunlight, influencing temperature and cloud formation. It also plays a role in fertilizing ecosystems, such as the Amazon rainforest, by providing essential nutrients like iron and phosphorus.&nbsp;



However, Saharan dust also has more complex impacts. It can reduce air quality, leading to respiratory issues in people living downwind of the dust. In addition, the dust impacts <a href="https://www.earth.com/news/atmospheric-dust-plays-surprisingly-crucial-role-in-stabilizing-ocean-ecosystems/" target="_blank" rel="noreferrer noopener">ocean</a> health by contributing to algae blooms, which can create dead zones in marine environments.



<h2 class="wp-block-heading" id="h-dust-clouds-and-human-health">Dust clouds and human health</h2>



In a recent study from Texas A&amp;M University, researchers explored the potential health impacts of <a href="https://www.earth.com/news/sahara-desert-dust-storms-carry-harmful-bacteria-and-fungi-around-the-globe/" target="_blank" rel="noreferrer noopener">bacteria and fungi</a> that travel within dust plumes.&nbsp;



The team found traces of several pathogens known to cause disease in humans, as listed by the World Health Organization (WHO).



Study co-author Dr. Daniel Spalink noted that while the DNA of several pathogenic bacteria and fungi were identified in African dust, it is not yet known if they can infect us and make us sick.&nbsp;



<h2 class="wp-block-heading" id="h-summertime-dust-events">Summertime dust events</h2>



“Scientists are interested in summertime Saharan dust events in part because of the influence they can have on large storm systems. 



Dry, stable, dust-laden air can inhibit tropical cyclone formation in the North Atlantic. And in a new study, researchers found that dust can modulate the amount of rainfall brought by these storms,” noted NASA.



“Using a machine-learning model based on meteorological data, NASA’s IMERG (Integrated Multi-Satellite Retrievals for GPM) precipitation estimates, and other satellite measurements, the study’s authors found that dust optical depth - a measure of how much light filters through a dusty plume - was a key predictor of rainfall from tropical cyclones.”



The researchers concluded that smaller amounts of dust particles promote the formation of rain clouds, while the sunlight-blocking effects of large dust clouds ultimately suppress precipitation.



<h2 class="wp-block-heading" id="h-saharan-dust-storms">Saharan dust storms</h2>



Dust storms in the Sahara Desert are some of the most far-reaching in the world. These storms, also known as haboobs, occur when strong winds lift large quantities of sand and <a href="https://www.earth.com/news/arctic-warming-impacts-dust-levels-on-a-global-scale/" target="_blank" rel="noreferrer noopener">dust</a> from the desert's surface into the atmosphere.&nbsp;



Saharan dust storms vary in intensity, with some being relatively mild while others are severe, reducing visibility to almost zero and creating hazardous conditions. 



They often happen in the spring and early summer when the temperature difference between the desert and the surrounding regions creates strong pressure gradients, fueling powerful winds.



Ultimately, these dust storms are a natural part of life. They shape the landscape over time by eroding rock formations and redistributing sand dunes. 



Despite their destructive potential, they are also a reminder of the dynamic and interconnected nature of Earth's climate systems.



The image was captured on August 24, 2024 by the VIIRS (Visible Infrared Imaging Radiometer Suite) on the Suomi NPP satellite.



Image Credit: NASA Earth Observatory&nbsp;



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Saharan dust launches off the Moroccan coast

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

These mixtures of male horses and female donkeys are slightly smaller than horses, and they have thicker fur coats. They also cannot reproduce on their own, making them very difficult to obtain. Photo Credit: Wikimedia

Hinny

New research by scientists from South Africa and Brazil reveals that rival plants may compete for space on pollinators, with pollen grains vying for the chance to be carried to the next flower.&nbsp;



The study, published in the journal <a href="http://dx.doi.org/10.1086/732797" target="_blank" rel="noreferrer noopener">The American Naturalist</a>, suggests that <a href="https://www.earth.com/news/new-twist-in-the-evolution-of-plant-pollinator-relationships/" target="_blank" rel="noreferrer noopener">plants</a> have developed sophisticated mechanisms to manipulate pollen placement on pollinators, similar to how some animals manipulate sperm during reproduction.



<h2 class="wp-block-heading" id="h-plants-and-competitive-pollen-removal-nbsp">Plants and competitive pollen removal&nbsp;</h2>



Unlike animals, where mating involves direct contact, plants rely on <a href="https://www.earth.com/news/pollinators-face-extinction-risk-due-to-climate-change/%C3%B9" target="_blank" rel="noreferrer noopener">pollinators</a> such as birds and insects to transport pollen from one flower to another. In this context, plants need to find ways to ensure their pollen makes it to the pollinator and, eventually, to the next flower. 



According to the study’s lead author, professor Bruce Anderson of <a href="http://www.sun.ac.za/english" target="_blank" rel="noreferrer noopener">Stellenbosch University</a>, the strategy plants have developed can be compared to male-male competition in animals.



“Flowers visited by <a href="https://www.earth.com/news/hummingbirds-have-an-amazing-sense-of-touch-for-precise-navigation/" target="_blank" rel="noreferrer noopener">hummingbirds</a> deposit their pollen on the hummingbird bills, but there is very little place for the pollen to be deposited,” Anderson explained. 



“Flowers have evolved a catapult mechanism where pollen is shot at the bill of the hummingbird. The force of the ballistic grains dislodges previously deposited grains from rival plants, allowing the flower to place its own grains onto a cleaner bill, thus increasing its chances of reproductive success.”



This finding supports the idea of competitive pollen removal, where flowers actively remove rival pollen from pollinators before securing a spot for their own pollen.



<h2 class="wp-block-heading" id="h-explosive-pollen-placement-in-action">Explosive pollen placement in action</h2>



To demonstrate this mechanism, the researchers conducted experiments with Hypenea macrantha, a red flower native to Brazil. Using slow-motion video footage, they captured the flower’s explosive pollen placement mechanism in action.&nbsp;



The flower essentially “catapults” its pollen onto the bill of a hummingbird, dislodging the pollen of competing plants in the process.



This mechanism, known as explosive pollen placement, is not new in the plant kingdom, but this study marks the first time researchers have provided empirical evidence of its effectiveness.&nbsp;



By labeling <a href="https://www.earth.com/news/pollen-alters-cloud-formation-and-changes-weather-patterns/" target="_blank" rel="noreferrer noopener">pollen</a> with quantum dots and counting how much was displaced by the explosion, the team was able to confirm the success of the mechanism.



<div class="wp-block-sendtonews-playerselector">[sendtonews key="ZwJf9SY4md-3926185-12187" type="single"]</div>



<h2 class="wp-block-heading" id="h-a-new-perspective-on-floral-competition">A new perspective on floral competition</h2>



Traditionally, floral explosion has been viewed as a strategy to help plants efficiently place their pollen on pollinators or to startle pollinators into flying to other plants, thereby dispersing the pollen over greater distances.&nbsp;



However, this new research shows that explosive pollen placement may serve an additional function: removing rival pollen to improve a plant’s reproductive success.



“Our data suggest, however, that this mechanism may actually displace pollen from previous flowers, enhancing male reproductive success by increasing competition for space on the pollinators’ bodies,” said co-author Vinícius Brito, a botanist at the <a href="https://ufu.br/" target="_blank" rel="noreferrer noopener">Federal University of Uberlândia</a> in Brazil.



<h2 class="wp-block-heading" id="h-plant-reproduction-and-pollen-rivalry">Plant reproduction and pollen rivalry</h2>



The research highlights a previously unrecognized form of competition between plants. In contrast to animals, where males may use physical structures to remove rival sperm from females, plants must manipulate the placement of their pollen on pollinators before it reaches the next flower. 



As Anderson explained, “until recently, no one has ever thought of looking for these kinds of structures in plants.”



This form of competition occurs on the pollinator’s body. When a pollinator, such as a hummingbird, arrives at a flower, it may already be covered in pollen from previously visited plants.&nbsp;



This makes it challenging for the new flower to place its pollen, as space is limited. Even if the flower does manage to place its pollen, it must then compete with rival pollen grains for access to the ovules of the next flower.



<h2 class="wp-block-heading" id="h-implications-for-understanding-plant-evolution">Implications for understanding plant evolution</h2>



This discovery offers new insights into how plants may compete with one another for reproductive success in ways that were previously unimagined. Anderson and his colleagues suggest that plants may evolve strategies akin to those in animals, where physical adaptations aid in removing rival sperm.



As the researchers continue to explore this phenomenon, their findings could reshape our understanding of how plants have <a href="https://www.earth.com/news/insects-boost-plant-evolution-in-surprising-ways/" target="_blank" rel="noreferrer noopener">evolved</a> complex mechanisms to increase their chances of reproductive success. 



By manipulating pollen on the bodies of pollinators, flowers may be competing in a hidden but highly effective battle for space and, ultimately, for the continuation of their species.



In conclusion, this study adds a fascinating new dimension to our understanding of plant reproduction and competition. As Brito points out, these discoveries highlight the importance of further research into how plants interact with their environment, pollinators, and even each other in their quest for survival.



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Pollen wars: Plants compete for space on pollinators

New research by scientists from South Africa and Brazil reveals...

A new study has revealed an intriguing phenomenon that could be contributing to the increasing consumption of plastic waste by whales. 



It all starts within the mysterious depths of the ocean where sunlight does not venture. This is where the likes of <a href="https://www.earth.com/news/where-have-the-sperm-whales-gulf-gone-gulf-jumbo-squid-scientists-think-they-know/" target="_blank" rel="noreferrer noopener">sperm whales</a> and goose-beaked whales forage for food, relying on their intricate soundwave-based navigation system to find their next meal.



But there seems to be a hitch - a torn plastic party balloon can sound remarkably similar to a delicious squid in these lightless depths.



A recent study has found a potential reason why whales might mistake plastic for prey – they sound the same underwater.



<h2 class="wp-block-heading" id="h-acoustic-signatures-in-the-deep-sea">Acoustic signatures in the deep sea</h2>



What exactly are these acoustic signatures? Well, when a <a href="https://www.earth.com/news/blue-whales-continue-their-battle-for-survival/" target="_blank" rel="noreferrer noopener">whale</a> sends out clicks and buzzes from a vocal cord-like structure near their blowholes, the sounds bounce off objects in the water. 



The sounds that return carry information about the size, shape, and nature of those objects. This is how the whales "see" and interpret their surroundings. And to their acoustic perception, their favorite squid sounds eerily similar to a plastic bag.



"There are hundreds of types of plastic, and the various material properties including polymer (chemical) composition, additives, shape, size, age/weathering, and degree of fouling likely play a role in the frequency-specific responses observed," noted the study authors.



<h2 class="wp-block-heading" id="h-plastic-pollution-and-whales">Plastic pollution and whales </h2>



Now, it's crucial to mention that the whales' sound-based navigation system is not a new kid on the evolutionary block. This sophisticated system has been helping whales find food in the pitch-dark ocean depths for the past 25 million years.



However, plastic pollution is a relatively new challenge faced by whales, and according to Merrill's findings, it's messing with their ultrasonic grocery shopping.



<h2 class="wp-block-heading" id="h-plastic-debris-around-whales">Plastic debris around whales</h2>



Merrill and his team collected typical plastic trash items like shopping bags, ropes, bottles, and balloons from beaches in Beaufort and Atlantic Beach, North Carolina.



These items were then suspended underwater and subjected to sonar transponder tests on Duke Marine Lab's ship, the R/V Shearwater. 



The team performed acoustic testing on these items at three varying sonar frequencies that span the range of 'clicks' emitted by different species of deep-diving <a href="https://www.earth.com/news/how-a-warming-climate-will-change-the-humpback-whales-diet/" target="_blank" rel="noreferrer noopener">whales</a>.



The sounds of real squid (albeit deceased ones) and pieces of squid beak were also recorded for comparison.



<h2 class="wp-block-heading" id="h-whales-mistake-plastic-for-prey">Whales mistake plastic for prey</h2>



The results were as alarming as they were surprising. The plastic debris almost always sounded like food, especially plastic films and fragments, which are among the most commonly found items in the stomachs of deceased whales.



Merrill suggests that we could consider re-engineering some plastics to not have an acoustic signature. But he also warns of potential risks. 



For instance, if fishing net and fishing line became "acoustically invisible," that could lead to increased entanglements where whales wouldn't be able to identify and avoid these threats.



For this pioneering study, Merrill collaborated with scientists from neighboring marine labs operated by NOAA, NC State University, and UNC – Chapel Hill.



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



The findings from Merrill's study have profound implications for marine conservation strategies aimed at protecting whales. 



Traditional approaches have largely focused on reducing the amount of plastic that enters the oceans - a task vital to the health of marine ecosystems.



However, understanding that plastic can acoustically resemble prey to whales suggests that addressing the challenge could require innovative solutions within the manufacturing sector as well. 



This could involve developing materials that emit distinct acoustic signatures detectable by marine life without posing any risk of ingestion. 



Such multidisciplinary cooperation between conservationists and material scientists could pave the way for groundbreaking strategies to safeguard these majestic creatures.



<h2 class="wp-block-heading" id="h-addressing-the-plastic-crisis">Addressing the plastic crisis</h2>



In light of these revelations, there is an urgent need to collectively address the plastic pollution crisis. Reducing our reliance on harmful plastics and advancing research into safer alternatives is paramount.



Moreover, stringent regulations on plastic manufacturing could play a crucial role in mitigating this crisis. By innovating responsibly and enforcing global standards, we can not only protect marine biodiversity but also ensure a healthier planet. 



While technological innovations and alternatives to plastic are critical in addressing this issue of <a href="https://www.earth.com/news/worlds-rarest-whale-found-on-new-zealand-beach/" target="_blank" rel="noreferrer noopener">whales</a>, perhaps the more immediate and straightforward action we can all take is responsible disposal of our waste.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0025326X24010464?via%3Dihub" target="_blank" rel="noreferrer noopener">Marine Pollution Bulletin</a>.



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Plastic trash sounds just like food to deep-diving whales

A new study has revealed an intriguing phenomenon that could...

This week, the October sky is treating us to a brilliant display that you won't want to miss -- the Hunter's supermoon, a rare comet, and the Orionids meteor shower. 



Comet C/2023 A3 Tsuchinshan-ATLAS is a rare comet making its journey past Earth, offering a unique opportunity to witness its tail of icy particles glistening against the dark canvas of space.



In addition, this week features the biggest supermoon of the year, Hunter's supermoon, which will illuminate the night with a breathtaking orangish glow.



Since Tuesday, the moon has looked larger than usual, and it’ll keep that appearance through Friday. By Thursday morning, as people head out for their morning commute. Depending on the weather in your area, Thursday night being the best time to see the full Hunter's supermoon..



And let's not forget the dazzling Orionids meteor shower, where you can catch glimpses of shooting stars streaking across the sky, resulting from debris left by Halley's Comet.



There's truly something for everyone in this celestial display. So, grab a warm jacket, perhaps a pair of binoculars for a closer look.



<h2 class="wp-block-heading" id="h-80-000-year-old-time-traveler">80,000-year-old time traveler</h2>



Meet <a href="https://www.earth.com/news/most-anticipated-comet-of-2024-returns-this-weekend-after-80000-years/" target="_blank" rel="noreferrer noopener">Comet C/2023 A3 Tsuchinshan-ATLAS</a>, a celestial wanderer that's been on an 80,000-year long odyssey. 



From the outermost regions of our solar system, this comet embarks on an interminable journey around the sun. The last time it paid us a visit, our ancestors were just crafting civilizations.



Although its closest Earth pass was on October 12, it remains visible for the remainder of the month. 



So, how do you spot it? An hour into the sunset, turn your sight to where the sun has sunk and voila. The elusive comet, while difficult to sight with the naked eye, could be seen with a pair of binoculars. 



Don't miss this rare chance to witness a phenomenon that won't return for another 80,000 years.



<h2 class="wp-block-heading" id="h-hunter-s-supermoon">Hunter's Supermoon</h2>



Next up...mark your calendars for October 17, 2024. The night sky is all set to parade the Hunter's Moon, but this year it's not just a full moon -- <a href="https://www.earth.com/news/hunters-supermoon-prepares-to-illuminate-the-october-skies/" target="_blank" rel="noreferrer noopener">it's a supermoon</a>! 



This phenomenon occurs when the moon is at its closest to Earth during its full phase, making it larger and brighter.



The Hunter’s Moon got its name from the historical practice of hunters utilizing the bright moonlight to track game and gather food in preparation for winter. This full moon rises soon after sunset, extending the period of illumination more than usual.



As it ascends, the Hunter’s Moon appears particularly large and orange, a visual effect produced by its lower position on the horizon and the scattering of light in the atmosphere.



This lunar phase holds cultural significance across various traditions, representing a time for preparation and gathering, underscoring the importance of readiness for the impending colder months.



The Hunter’s Moon is generally in October -- although once every four years it makes an appearance in November.



While contemporary life may not depend on this extra light to hunt or complete outdoor tasks, the Hunter’s Moon remains a fascinating reminder of nature’s rhythms and the cyclical changes of the seasons.



<h3 class="wp-block-heading" id="h-what-puts-the-super-in-the-supermoon">What puts the 'super' in the supermoon?</h3>



So, you might ask, "What's so super about the supermoon?" As Anna Gammon-Ross, a seasoned astronomer from the <a href="https://www.rmg.co.uk/" target="_blank" rel="noreferrer noopener">Royal Museums Greenwich</a> explains, a supermoon occurs when a full moon is nearest to Earth in its orbit. 



This cosmic alignment results in a moon that's roughly 14% larger and 30% brighter than usual. On seeing the radiant orb hanging low in the sky, you'd agree that the supermoon does indeed earn its name.



<h2 class="wp-block-heading" id="h-shooting-stars-orionids-meteor-shower">Shooting stars: Orionids meteor shower</h2>



The Orionids meteor shower is one of the highlights of the October night sky. These meteors are actually tiny bits of dust left behind by <a href="https://www.earth.com/news/orionids-meteor-shower-peaks-this-weekend-heres-what-to-expect/" target="_blank" rel="noreferrer noopener">Halley's Comet</a> as it travels through the solar system. 



When Earth passes through this trail of debris, the particles slam into our atmosphere at incredible speeds -- up to 148,000 miles per hour! As they burn up, they create those bright streaks of light we love to watch.



What's cool about the Orionids is that they're known for their fast and bright meteors, often leaving glowing trails that last for a few seconds. 



The best time to catch them is in the early morning hours before dawn, when the <a href="https://www.earth.com/news/betelgeuse-one-of-our-brightest-stars-will-vanish-from-sight-next-week/" target="_blank" rel="noreferrer noopener">constellation Orion</a> (which gives the meteor shower its name) is high in the sky. 



Just find a comfy spot away from city lights, let your eyes adjust to the darkness, and enjoy the show -- no special equipment needed.



<h2 class="wp-block-heading" id="h-skywatching-101">Skywatching 101</h2>



All set to behold these cosmic spectacles? Here are some tips to enhance your experience:



<ul class="wp-block-list">
<li>Search for a location far from city lights to escape light pollution. </li>



<li>Always check the weather. Clear skies are your best pals for skywatching. </li>



<li>Bring your binoculars. For the supermoon, they are optional, but they'll help with the comet and make meteor watching more fun. </li>



<li>Comfort is key. Dress warmly and consider bringing a blanket or a chair. </li>



<li>Patience is a virtue. Allow around 20 minutes for your eyes to adjust to the darkness.</li>
</ul>



These celestial showstoppers make for some spectacular photography opportunities. 



For the supermoon, a camera with manual settings, plus a tripod for steadiness, can help capture stunning shots. 



For the meteors, a wide-angle lens with a long exposure setting can help you nab a shooting star.



<h2 class="wp-block-heading" id="h-more-wonders-to-watch">More wonders to watch</h2>



October's skywatching doesn't end with the comet, supermoon, and meteor shower. 



Throughout the month, Venus brightly greets morning risers, while Saturn and Jupiter are earlier night visitors. 



Mars is a bit elusive but worth seeking out. Several constellations, such as Cassiopeia and Perseus, also adorn the night sky. 



If you're a novice stargazer, a smartphone app can help you navigate the starry expanse.



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Hunter's supermoon, a comet, and Orionids meteors are sharing the sky tonight

This week, the October sky is treating us to a...

The Europa Clipper is headed toward Jupiter’s moon, Europa, with a mission to search for signs of life.



The <a href="https://www.earth.com/news/send-your-name-to-jupiters-ocean-moon-as-europa-clipper-mission-searches-for-life/" target="_blank" rel="noreferrer noopener">spacecraft</a> is beginning an incredible 1.8 billion-mile (2.9 billion-kilometer) journey, using gravity assists for propulsion.



Clipper will make its first stop at Mars in four months, followed by a return to Earth in 2026 for an additional gravity boost.



The spacecraft is scheduled to begin orbiting <a href="https://www.earth.com/news/alien-life-on-europa-co2-discovery-by-webb-increases-the-odds/" target="_blank" rel="noreferrer noopener">Jupiter</a> in April 2030 and is estimated to fly past the moon Europa 49 times, collecting valuable data during each pass.



<h2 class="wp-block-heading" id="h-europa-clipper-mission">Europa Clipper mission</h2>



The Europa Clipper is NASA's largest spacecraft built for a planetary mission and the first dedicated to studying an ocean world beyond Earth.



"Congratulations to our Europa Clipper team for beginning the first journey to an ocean world <a href="https://www.earth.com/news/key-compound-suggests-that-life-beyond-earth-could-be-common/" target="_blank" rel="noreferrer noopener">beyond Earth</a>," said NASA Administrator Bill Nelson. 



"NASA leads the world in exploration and discovery, and the Europa Clipper mission is no different. By exploring the unknown, Europa Clipper will help us better understand whether there is the potential for life not just within our solar system, but among the billions of moons and planets beyond our Sun."



<h2 class="wp-block-heading" id="h-searching-for-habitable-worlds-beyond-earth">Searching for habitable worlds beyond Earth</h2>



Five minutes after launch, Europa Clipper emerged as the rocket’s nose cone opened. An hour later, it separated from the rocket, with ground controllers confirming its status and establishing communication through NASA’s Deep Space Network.



<div class="wp-block-sendtonews-playerselector">[sendtonews key="GF2ZEZQycs-3925933-12187" type="single"]</div>



Dr. Nicky Fox is the Associate Administrator (AA) for the Science Mission Directorate at NASA Headquarters in Washington.



"We could not be more excited for the incredible and unprecedented science NASA’s Europa Clipper mission will deliver in the generations to come," said Dr. Fox. 



"Europa Clipper’s scientific discoveries will build upon the legacy created by our other missions exploring Jupiter - including Juno, Galileo, and Voyager - in our search for habitable worlds beyond our home planet."



<h2 class="wp-block-heading" id="h-an-ocean-world-with-intriguing-possibilities">An ocean world with intriguing possibilities</h2>



The mission’s primary goal is to determine whether Europa has the conditions to support life.



While Europa is similar in size to our Moon, its interior composition sets it apart. Data from NASA’s Galileo mission in the 1990s revealed that beneath Europa's icy shell is a vast, salty ocean, possibly holding more water than all of Earth’s oceans combined. 



Evidence also suggests that Europa may contain organic compounds and energy sources beneath its surface. 



If Europa proves to be habitable, it could indicate that there are more life-supporting worlds in our universe than we previously imagined.



<h2 class="wp-block-heading" id="h-europa-clipper-will-deliver-mind-blowing-science">Europa Clipper will deliver mind-blowing science</h2>



"We’re ecstatic to send Europa Clipper on its way to explore a potentially <a href="https://www.earth.com/news/nasa-confirms-an-ocean-on-europa-may-be-habitable/" target="_blank" rel="noreferrer noopener">habitable ocean world</a>, thanks to our colleagues and partners who’ve worked so hard to get us to this day," said Laurie Leshin, director of <a href="https://www.jpl.nasa.gov/news/liftoff-nasas-europa-clipper-sails-toward-ocean-moon-of-jupiter/" target="_blank" rel="noreferrer noopener">NASA’s Jet Propulsion Laboratory</a> in Southern California. 



"Europa Clipper will undeniably deliver mind-blowing science. While it's always bittersweet to send something we’ve labored over for years off on its journey, we know this remarkable team and spacecraft will expand our knowledge of our solar system and inspire future exploration."



<h2 class="wp-block-heading" id="h-a-closer-look-at-europa-clipper">A closer look at Europa Clipper</h2>



By 2031, Europa Clipper will begin flybys of Europa, using advanced instruments powered by NASA to study the moon’s surface and interior. Notably, over 4,000 people have contributed to the mission since 2015.



"As Europa Clipper embarks on its journey, I’ll be thinking about the countless hours of dedication, innovation, and teamwork that made this moment possible," said Jordan Evans, project manager at NASA JPL. 



"This launch isn’t just the next chapter in our exploration of the solar system; it’s a leap toward uncovering the mysteries of another ocean world, driven by our shared curiosity and continued search to answer the question, ‘are we alone?’"



Embarking on this exciting mission, the Europa Clipper's three main science objectives are to determine the thickness of the moon’s icy shell and its interactions with the ocean below, investigate its composition, and to characterize its geology.



These detailed explorations will greatly expand our understanding of the astrobiological potential for <a href="https://www.earth.com/news/habitable-worlds-new-strategy-to-identify-planets-that-may-host-life/" target="_blank" rel="noreferrer noopener">habitable worlds beyond our planet</a>, offering new insights into where life might exist elsewhere in the universe.



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Europa Clipper will search for signs of life on Jupiter's icy moon

The Europa Clipper is headed toward Jupiter’s moon, Europa, with...

The global invasion of microplastics is an unfortunate reality that we are facing. These microscopic <a href="https://www.earth.com/news/hotspots-of-microplastic-pollution-found-in-the-north-sea/" target="_blank" rel="noreferrer noopener">plastic contaminants</a> have become an unwelcomed guest, trespassing into the bodies of numerous creatures worldwide.



Food ingestion is the most common way that microplastics enter the bodies of both humans and wildlife.



For us humans, and even rodents, researchers have established a disturbing connection between these invasive particles and adverse health impacts. The culprits? Oxidative stress and inflammation, to name a couple.



<h2 class="wp-block-heading" id="h-to-breathe-or-not-to-breathe">To breathe or not to breathe?</h2>



While ingesting contaminated food isn't exactly "fine dining," another potential exposure method lurks in the shadows - inhalation. Although notorious among humans, this path has been quite neglected in wildlife research. 



But now, experts have discovered that bottlenose dolphins are exhaling microplastic particles, indicating that inhalation may be a relevant route of exposure for wildlife.



<h2 class="wp-block-heading" id="h-microplastics-in-dolphin-breath">Microplastics in dolphin breath</h2>



Our quest for knowledge leads us to two places - Sarasota Bay, Florida, and Barataria Bay, Louisiana. Here, Miranda Dziobak of the <a href="https://charleston.edu" target="_blank" rel="noreferrer noopener">College of Charleston</a> and her team have been busy gathering samples.



Their subjects? Five bottlenose dolphins from Sarasota and six of their kin in Barataria. And the object of interest? Air, or more specifically, the air they exhale.



Here's an unexpected shocker. The analysis revealed every single one of these 11 dolphins was "breathing plastic." The team discovered suspected <a href="https://www.earth.com/news/microplastic-pollution-is-everywhere-even-in-newborns-and-getting-worse/" target="_blank" rel="noreferrer noopener">microplastic particles</a> in the exhaled air of each dolphin.



The microplastics came in the forms of both fibers and fragments and included several plastic polymers: polyethylene terephthalate (PET), polyester, polyamide, polybutylene terephthalate, and poly(methyl methacrylate), also known as PMMA.



<h2 class="wp-block-heading" id="h-evaluating-microplastics-exposure-in-dolphins">Evaluating microplastics exposure in dolphins</h2>



To ensure the study's credibility, the researchers also sampled the surrounding air. This step reinforced the stark reality that microplastics were not just passersby in the ambient air but residents in the dolphins' exhaled breath. 



The findings fuel the suspicion that inhalation, like ingestion, is another high-priority exposure route for dolphins. However, everyone loves a good mystery, and the researchers emphasize that these results are preliminary. 



The scientific community must roll up its collective sleeves and dive deeper into evaluating the degree of various microplastic inhalations among bottlenose dolphins.



<h2 class="wp-block-heading" id="h-long-term-implications">Long-term implications </h2>



Also, what are the longer-term implications of this <a href="https://www.earth.com/news/new-process-converts-microplastics-into-valuable-graphene-wonder-material/" target="_blank" rel="noreferrer noopener">exposure</a>? Lung damage? It's time to find out. 



“We know that microplastics are floating around in the air, so we suspected that we would find microplastics in breath samples," noted the researchers.



"We are concerned by what we are seeing because dolphins have a large lung capacity and take really deep breaths, so we are worried about what these plastics could be doing to their lungs."



<h2 class="wp-block-heading" id="h-microplastics-and-dolphin-health">Microplastics and dolphin health</h2>



Going forward, the experts aim to scrutinize the comprehensive impact of microplastics on marine mammal health.



This pursuit involves deploying more sophisticated analytical techniques to pinpoint not only the presence but also the concentrations of various microplastic polymers specific to <a href="https://www.earth.com/news/ocean-microplastics-are-here-to-stay-so-what-can-we-do-now/" target="_blank" rel="noreferrer noopener">different environmental contexts</a>. 



The need for collaborative ventures among marine biologists, ecologists, and material scientists grows urgent, as these efforts could unveil critical insights into mitigating the risks plastic particles pose to the delicate balance of marine ecosystems.



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



The experts noted that further research is also needed to understand health implications following inhaled microplastic exposure, especially among vulnerable populations experiencing adverse pulmonary impacts.



"A systematic assessment of particle exhalation in Sarasota Bay dolphins is planned to examine life history influences on exposure and associations with health impacts in the well-studied Sarasota Bay dolphin community."



<h2 class="wp-block-heading" id="h-engaging-the-public">Engaging the public</h2>



Addressing microplastics exposure among marine creatures like dolphins transcends the realm of scientific inquiry - it calls for widespread public awareness and action.



Leveraging educational campaigns can play a pivotal role in informing communities, policy makers, and industries about the pervasive nature and adverse effects of microplastics. 



Such efforts should advocate for reduced plastic consumption, enhanced waste management practices, and the development of biodegradable alternatives. 



Empowering individuals and institutions to make environmentally responsible choices is vital, as these collective actions could substantially reduce the microplastic <a href="https://www.earth.com/news/microplastics-pose-a-greater-threat-to-some-ocean-animals/" target="_blank" rel="noreferrer noopener">load in our oceans</a>, ultimately fostering a healthier environment for dolphins and other marine inhabitants.



The study is published in the journal <a href="https://journals.plos.org/plosone/article?id=10.1371/journal.pone.0309377" target="_blank" rel="noreferrer noopener">PLoS ONE</a>.



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Microplastics found in dolphin breath

The global invasion of microplastics is an unfortunate reality that...

Plant life is the fundamental fabric of our planet, and it's astonishing to realize that about one-third of all known plant species have made islands their home. 



Despite representing a little more than 5% of Earth's land surface, islands are the embodiment of rich biodiversity. How did this happen?



<h2 class="wp-block-heading" id="h-plant-species-dwelling-on-islands">Plant species dwelling on islands</h2>



Dr. Julian Schrader from <a href="https://www.mq.edu.au/faculty-of-science-and-engineering/departments-and-schools/school-of-natural-sciences" target="_blank" rel="noreferrer noopener">Macquarie University’s School of Natural Sciences</a>, along with an international team of researchers, analyzed data from around 304,103 plants – which essentially sums up all species known to science. The results highlight the incredible biodiversity existing on islands.



Out of 94,052 species that were identified as natives of <a href="https://www.earth.com/news/how-the-amazon-became-a-biodiversity-hotspot/" target="_blank" rel="noreferrer noopener">islands</a>, the team found that a whopping 63,280 are endemic. In layman's terms, these plant species can only be found on their home islands.



This means that 21% of global plant diversity is tucked away on islands across our planet. The research marks the first-ever comprehensive examination of vascular plants native to marine islands worldwide.



<h2 class="wp-block-heading" id="h-native-and-endemic-plants">Native and endemic plants</h2>



A native plant is one that grows naturally on an <a href="https://www.earth.com/news/effective-conservation-efforts-key-to-saving-biodiversity/" target="_blank" rel="noreferrer noopener">island</a>, while an endemic plant species takes it one step further. They're exclusive to a specific island or a group of islands. 



Among these are vascular plants, a diverse group that includes trees, shrubs, herbs, ferns and grasses. They are distinctive from their non-vascular counterparts (like mosses and liverworts), thanks to their circulatory system.



“This is the first time we have had such a complete understanding of which species are where, globally,” noted Dr. Schrader.



“We can now explore the conservation status of some of our rarest plants and come up with distinct strategies to conserve them, such as identifying botanical gardens that could host rescue populations.”



It also allows researchers to strategize ways of protecting and preserving these unique species. For example, botanical gardens can help by hosting rescue populations.



<h2 class="wp-block-heading" id="h-island-plant-paradox">Island plant paradox </h2>



While islands are bursting at the seams with species diversity, it's alarming to note that only 6% of islands with endemic species are making the cut for a UN goal to protect 30% of land and sea areas by 2030. 



The research also shines a spotlight on top centers of <a href="https://www.earth.com/news/plant-life-on-islands-loses-diversity-when-humans-arrive/" target="_blank" rel="noreferrer noopener">plant</a> endemism. These regions are large, tropical islands shaped by a complex terrain and a long history of isolation.



The stars of the show are Madagascar with 9,318 endemic plant species, followed by New Guinea with 8,793 species, Borneo with 5,765, Cuba with 2,679, and New Caledonia with 2,493.



According to Dr Schrader, it's all about the geography. The physical distance, coupled with unique climates and environments, fuels the evolutionary process, leading to new species creation or "speciation."



<h2 class="wp-block-heading" id="h-threats-to-island-biodiversity">Threats to island biodiversity</h2>



However, isolation can be a double-edged sword. Many plant species that have evolved uniquely in such isolated ecosystems may find it hard to compete with non-native species. 



Climate change adds another layer of complexity to this situation. The threat is particularly grave for low-lying islands that are susceptible to rising sea levels and extreme weather events.



In this light, the study offers a critical baseline for monitoring changes in islands and <a href="https://www.earth.com/news/tree-islands-can-counteract-biodiversity-loss-in-oil-palm-plantations/" target="_blank" rel="noreferrer noopener">plant communities</a> over time. Think of it as a roadmap for prioritizing protection efforts. It's about the survival of these unique species that dot our planet's islands, each with their own tale of evolution, adaptation and survival.



“In French Polynesia, I was trying to find one of the rarest plants in the world, the flowering shrub called tiare apetahi (Sclerotheca raiateensis), with only a few individuals left in the wild,” said Dr. Schrader.



This plant holds cultural significance to the local community but is grappling with overharvesting and predation. The solution may lie in botanical gardens, but figuring out how to grow the species outside its natural habitat is the challenge at hand.



The story of island biodiversity is a tale of enchantment, intrigue, and urgent rescue efforts. It's a narrative that highlights the need for collective action, careful stewardship, and informed conservation strategies.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-024-08036-1" target="_blank" rel="noreferrer noopener">Nature</a>.



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Islands are home to one-third of all known plants

Plant life is the fundamental fabric of our planet, and...

An international team of scientists has completely transformed our understanding of meteorites and their origins.



The experts have successfully demonstrated that 70% of all known meteorite falls originate from just three young asteroid families.



The study was led by researchers from the CNRS, the European Southern Observatory (ESO, Europe), and <a href="https://cuni.cz/UKEN-1.html" target="_blank" rel="noreferrer noopener">Charles University</a> (Czech Republic).



<h2 class="wp-block-heading" id="h-mysterious-origins-of-meteorites">Mysterious origins of meteorites</h2>



Traditionally, meteorites have fueled our <a href="https://www.earth.com/news/two-meteor-showers-delta-aquarids-alpha-capricornids-light-up-night-skies-august-2024/" target="_blank" rel="noreferrer noopener">curiosity about the cosmos</a>. They serve as tangible pieces of the universe that we can observe, analyze, and learn from without leaving our home planet.



The international research team concluded that of all known meteorite falls, the majority can be traced back to three young <a href="https://www.earth.com/news/two-large-asteroids-will-pass-near-earth-this-week/" target="_blank" rel="noreferrer noopener">asteroid</a> families - Karin, Koronis, and Massalia.



These families were born from collisions in the main asteroid belt about 5.8, 7.5, and roughly 40 million years ago. Most noteworthy among these families, the Massalia family has been identified as the source of 37% of known meteorites.



While it's true that we have records of more than 70,000 meteorites, only 6% had been clearly identified by their composition. These "achondrites" are known to come from the Moon, Mars, or Vesta (one of the largest asteroids in the main belt).



The origin of the other 94% of meteorites, the majority of which are ordinary "chondrites," had remained a puzzle.



<h2 class="wp-block-heading" id="h-life-cycle-of-asteroid-families">Life cycle of asteroid families</h2>



But why are the three young asteroid families such prolific contributors to meteorite falls? The answer lies in the life cycle of asteroid families.



Young families are defined by an abundance of small fragments left over from collisions. This abundance, coupled with the fragments' high mobility, increases the risk of collisions that can lead to escape from the belt, possibly hurtling towards Earth. 



In contrast, asteroid families produced by older collisions are "depleted" sources of meteorites. Over time, the abundance of small fragments naturally erodes and eventually disappears, paving the way for new sources of meteorites from more recent collisions.



<h2 class="wp-block-heading" id="h-breakthrough-in-meteorite-origins">Breakthrough in meteorite origins</h2>



The monumental discovery was made possible by a telescopic survey of the composition of all the major asteroid families in the main belt, bolstered by state-of-the-art computer simulations.



This method was extended to all meteorite families, unveiling the primary sources of carbonaceous chondrites and achondrites, adding to those from the Moon, Mars, and Vesta. 



Consequently, the origin of more than 90% of meteorites has now been identified - a significant leap in our understanding.



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



This research has also enabled scientists to trace the origin of asteroids that are large enough to pose a threat to life on Earth. 



For instance, it turns out that the asteroids Ryugu and Bennu - recently sampled by the Hayabusa2 (Japanese Aerospace Exploration Agency JAXA) and OSIRIS-REx (NASA) missions and studied in laboratories around the world - are derived from the same parent asteroid as the Polana family.



Even after this remarkable breakthrough, the origin of the remaining 10 percent of known meteorites remains uncharted. Undeterred, the team is already gearing up for their next mission - to characterize all young families formed less than 50 million years ago.



<h2 class="wp-block-heading" id="h-significance-of-meteorite-origins-research">Significance of meteorite origins research</h2>



As we advance our comprehension of meteorite origins, the implications for both scientific inquiry and <a href="https://www.earth.com/news/dart-mission-debris-will-create-a-human-made-meteor-shower/" target="_blank" rel="noreferrer noopener">practical applications</a> become increasingly compelling. 



Future research prospects include a more detailed analysis of less-studied asteroid families, potentially identifying their contribution to the remaining 10% of uncharted meteorite origins. 



The emphasis on innovative observational methods and computational models holds the promise of refining our understanding of the cosmic processes that govern the distribution and descent of meteorites. 



These efforts are supported by ongoing and future space missions tasked with bringing back direct samples from asteroids.



Further research will improve our understanding of the meteorites themselves, as well as the formation and evolution of our solar system.



<h2 class="wp-block-heading" id="h-intersection-of-space-research">Intersection of space research</h2>



The knowledge gained from meteorite studies extends beyond academic curiosity, offering valuable applications in fields ranging from geology to planetary defense.



Understanding the composition and behavior of meteorites can help experts draw parallels with Earth's geological history, providing clues to the early conditions and processes of our planet.



This research also helps to inform the development of planetary defense strategies, as the ability to predict and mitigate potential impacts from space debris is enhanced.



Moreover, meteorite-oriented discoveries fuel advancements in material science, potentially leading to the development of novel materials or understanding natural occurrences in extreme environments. 



As our grasp of these cosmic visitors strengthens, we stand better equipped not only to unravel the mysteries of our own planet but also to anticipate and navigate the challenges of space exploration and habitation.



The study is published in the journal <a href="https://www.aanda.org/articles/aa/full_html/2024/09/aa50532-24/aa50532-24.html" target="_blank" rel="noreferrer noopener">Astronomy and Astrophysics</a>.



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Most meteorites can be traced to three asteroid families

An international team of scientists has completely transformed our understanding...

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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



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

Detecting mercury contamination with the tap of a finger

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



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



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



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



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



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



Video/ Image Credit: European Space Agency&nbsp;



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



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

Kainji Lake in north central Nigeria

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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



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Designing crops that can beat the heat

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