Today's Image of the Day from the European Space Agency features NGC 1333, a reflection nebula located in the Perseus molecular cloud about 960 light-years away from Earth. The photo is a mosaic of images captured by the James Webb Space Telescope.



“Webb’s superb sensitivity allows astronomers to investigate young objects with extremely low masses. Some of the faintest ‘stars’ in the picture are in fact newly born free-floating brown dwarfs with masses comparable to those of giant planets,” noted <a href="https://www.esa.int/" target="_blank" rel="noreferrer noopener">ESA</a>.



The same cluster was featured in the 33rd anniversary image of the Hubble Space Telescope in April 2023.&nbsp;



According to ESA, Hubble’s image just scratched the surface of this region, because clouds of dust obscure much of the star formation process. 



"Observing with larger aperture and in the infrared part of the spectrum, Webb is capable of peering through the dusty veil to reveal newborn stars, brown dwarfs and planetary mass objects."



<h2 class="wp-block-heading" id="h-webb-s-view-of-ngc-1333">Webb’s view of NGC 1333</h2>



ESA noted that the center of the image presents a deep peek into the heart of the NGC 1333 cloud.&nbsp;



“Across the image we see large patches of orange, which represent gas glowing in the infrared. These so-called Herbig-Haro objects form when ionized material ejected from young stars collides with the surrounding cloud. They are hallmarks of a very active site of star formation."



The disks of gas and dust that surround the <a href="https://www.earth.com/news/newly-discovered-stars-milky-way-are-old-as-universe/" target="_blank" rel="noreferrer noopener">stars</a> in this image may eventually produce planetary systems.&nbsp;



<h2 class="wp-block-heading" id="h-stars-in-the-sun-s-birth-cluster">Stars in the Sun's birth cluster</h2>



“Similar to the young stars in this mosaic, our own Sun and planets formed inside a dusty molecular cloud, 4.6 billion years ago. Our Sun did not form in isolation but as part of a cluster, which was perhaps even more massive than NGC 1333,” explained ESA.



Over time, the stars in the Sun's birth cluster would have drifted apart due to gravitational interactions and the dispersion of gas in the region.



Astronomers have been studying certain clues, such as isotopic signatures in meteorites, that hint the Sun may have formed near massive stars. These stars likely produced supernovae, which could have influenced the early <a href="https://www.earth.com/news/mysterious-objects-spotted-in-the-outer-solar-system-beyond-pluto/" target="_blank" rel="noreferrer noopener">solar system</a> by injecting heavy elements like iron-60.



<h2 class="wp-block-heading" id="h-star-formation-in-ngc-1333">Star formation in NGC 1333</h2>



NGC 1333 is a vibrant example of a stellar nursery, where active <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 ongoing. It is known for its chaotic appearance, shaped by the interactions between newborn stars and the surrounding material.



Within NGC 1333, astronomers have observed a high level of turbulence, which makes the region dynamic and complex. 



The disturbances are caused by the outflows of young stars as they eject material into their surroundings, creating shock waves and influencing further star formation. 



These outflows are often seen as jets, which are visible in multiple wavelengths of light, especially infrared, as the surrounding dust absorbs visible light.



<h2 class="wp-block-heading" id="h-early-stages-of-planet-formation">Early stages of planet formation </h2>



NGC 1333 is also an area of interest for studying the early stages of star and <a href="https://www.earth.com/news/planet-formation-new-insights-mechanics-physics/" target="_blank" rel="noreferrer noopener">planet formation</a>, as many of the stars within the cluster are in their infancy.



These stars are still in the process of gathering material and developing protoplanetary disks.&nbsp;



In images, NGC 1333 is marked by bright patches of blue and red, representing reflection <a href="https://www.earth.com/news/six-rogue-worlds-discovered-inside-a-young-star-forming-nebula/" target="_blank" rel="noreferrer noopener">nebulae</a> and the ionized gas created by energetic young stars.&nbsp;



<h2 class="wp-block-heading" id="h-the-perseus-molecular-cloud-nbsp">The Perseus molecular cloud&nbsp;</h2>



The Perseus molecular cloud is a vast region of cold gas and dust located about 600 light-years away from Earth in the constellation <a href="https://www.earth.com/news/1500-billion-orphan-stars-discovered-in-the-perseus-galaxy-cluster/" target="_blank" rel="noreferrer noopener">Perseus</a>.&nbsp;



It is one of the most studied star-forming regions in our galaxy due to its relative proximity and the diversity of its young stellar objects. This cloud spans several hundred light-years and contains dense pockets of gas where new stars are actively forming.&nbsp;



These areas are often enshrouded in thick dust, which obscures them in visible light but allows astronomers to study them using infrared and radio wavelengths.



The Perseus molecular cloud is particularly interesting because of the chemistry taking place within it, including the formation of complex organic molecules that could be precursors to life.&nbsp;



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



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Stellar nursery shines in the Perseus cloud

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

Today's Image of the Day from the European Space Agency features Messier 78 (M78), a reflection nebula located in the constellation Orion about 1,350 light-years away from Earth.&nbsp;



This image was released as part of the initial series of observations from ESA's <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid" target="_blank" rel="noreferrer noopener">Euclid space mission</a>.&nbsp;



All data collected during these early observations, including a series of incredible <a href="https://www.esa.int/Science_Exploration/Space_Science/Euclid/Euclid_s_first_images_the_dazzling_edge_of_darkness" target="_blank" rel="noreferrer noopener">new views</a> of the nearby universe, is available to the public.&nbsp;



<h2 class="wp-block-heading" id="h-image-of-messier-78">Image of Messier 78</h2>



Messier 78 is a dynamic region of star formation that is obscured by cosmic dust in this high-resolution image captured by the Euclid space telescope.



This specific view highlights how young stars generate winds of charged particles, carving out “cavities” in the molecular clouds around them.&nbsp;



The blue hues in the image represent ionized atomic hydrogen, which is a primary component of the cloud, while the red indicates the absorption and scattering of light by dust particles.



The image captures hundreds of stars varying in brightness, illuminating their nebulous, purple surroundings. A dark, arch-like structure stretches from the upper left to the bottom right of the frame, merging into the densest, darkest clouds at the image’s base.



<h2 class="wp-block-heading" id="h-active-site-of-star-formation-nbsp">Active site of star formation&nbsp;</h2>



Messier 78 is not just a single nebula but part of a larger complex of stars and nebulous regions in <a href="https://www.earth.com/news/orion-nebula-destroys-an-oceans-worth-of-water-every-month/" target="_blank" rel="noreferrer noopener">Orion</a>, which includes various other objects like dark nebulae that are visible as patches blocking light from behind.



This region is an active site of star formation, featuring many young stars and protostars, which are stars in the early stages of formation.&nbsp;



<h2 class="wp-block-heading" id="h-viewing-messier-78">Viewing Messier 78</h2>



M78 is easily observable with small telescopes, and it appears as a hazy patch of light with two prominent stars near its center, which illuminate the surrounding dust.&nbsp;



The nebula is also a favorite among amateur astronomers for its beauty and relatively bright appearance.



<h2 class="wp-block-heading" id="h-subject-of-scientific-interest-nbsp">Subject of scientific interest&nbsp;</h2>



Messier 78 is fascinating not only for its visual beauty but also for its scientific interest, particularly in the study of <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> and interstellar matter.&nbsp;



The nebula consists of dense, cold gas and dust, which are essential ingredients for the birth of new stars.&nbsp;



The intense blue light that characterizes M78 is due to the reflection of starlight off these dust particles - a process known as scattering.



<h2 class="wp-block-heading" id="h-region-surrounding-messier-78-nbsp">Region surrounding Messier 78&nbsp;</h2>



The region surrounding M78 includes several other interesting features. For instance, there are Herbig-Haro objects within it, which are small patches of nebulosity associated with <a href="https://www.earth.com/news/new-molecule-detected-in-space-where-stars-are-born/" target="_blank" rel="noreferrer noopener">newly born stars</a>.&nbsp;



These objects are formed when gas ejected by young stars collides with clouds of gas and dust at high speeds, creating shock waves that glow brightly.



<h2 class="wp-block-heading" id="h-earliest-stages-of-star-development-nbsp">Earliest stages of star development&nbsp;</h2>



Additionally, infrared observations of M78 have revealed much about the dust and colder objects in the area, which are not visible in optical light.&nbsp;



The observations have helped astronomers identify numerous young stars and brown dwarfs (objects that are too large to be planets and too small to be stars) within the nebula.&nbsp;



This makes M78 a critical area for studying the earliest stages of star development and the properties of the interstellar medium.



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



The <a href="https://www.earth.com/news/new-batch-of-brilliant-images-from-the-euclid-mission-live-up-to-the-hype/" target="_blank" rel="noreferrer noopener">Euclid space mission</a> is designed to study the dark universe, particularly focusing on dark energy and dark matter. These components are believed to drive the accelerating expansion of the universe and shape its large-scale structure. 



The mission aims to map the geometry of the dark universe and better understand the physics of the cosmos.



<h3 class="wp-block-heading" id="h-observing-billions-of-galaxies-nbsp">Observing billions of galaxies&nbsp;</h3>



Euclid uses two primary scientific instruments: a visible light camera (VIS) and a near-infrared spectrometer and photometer (NISP).&nbsp;



These instruments will allow Euclid to measure the shapes and redshifts of galaxies at distances of up to 10 billion light-years. By surveying more than a third of the sky, the mission is expected to observe several billion galaxies.



<h3 class="wp-block-heading" id="h-studying-the-dark-universe-nbsp">Studying the dark universe&nbsp;</h3>



The data collected will help astronomers in studying the effects of dark matter and dark energy in depth, testing cosmological models, and exploring new theories about the nature of the universe.&nbsp;



The mission, named after the ancient Greek mathematician Euclid, seeks to address key questions related to the structure of the universe and the fundamental laws of physics governing its evolution and expansion.



Image Credit: European Space Agency&nbsp;



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Messier 78: Young stars shine through dense dust

Today's Image of the Day from the European Space Agency showcases the striking beauty of the planetary nebula NGC 2899, which resembles a moth in flight. The photo was captured by the Hubble Space Telescope.



“The planetary nebula NGC 2899 is shaped like a single macaroni noodle, with its edges pointed up, but its edge-on central torus is semi-transparent in the middle,” noted <a href="https://www.esa.int/ESA_Multimedia/Images" target="_blank" rel="noreferrer noopener">ESA</a>.



“The top and bottom edges are thick and orange. The center is semi-transparent blue and green. The wider central region looks roughly like a moth, also filled with semi-transparent blue and green.”



<h2 class="wp-block-heading" id="h-defining-features-of-the-planetary-nebula">Defining features of the planetary nebula</h2>



The nebula features a bipolar, cylindrical outflow of gas extending diagonally, driven by intense radiation and stellar winds from a central <a href="https://www.earth.com/news/white-dwarf-planets-are-more-habitable-than-we-thought/" target="_blank" rel="noreferrer noopener">white dwarf</a> with a scorching temperature of nearly 22,000 degrees Celsius.&nbsp;



“In fact, there may be two companion stars that are interacting and sculpting the nebula, which is pinched in the middle by a fragmented ring or torus - looking like a half-eaten donut,” said ESA.



Streams of gaseous “pillars” extend outward, all pointing back toward the central source of energy. The vibrant colors in the image come from glowing hydrogen and oxygen gases.&nbsp;



<h2 class="wp-block-heading" id="h-discovery-and-significance-of-ngc-2899">Discovery and significance of NGC 2899</h2>



NGC 2899 was discovered by British astronomer John Herschel on March 2, 1835, during his survey of the southern skies from the Cape of Good Hope in South Africa. Herschel cataloged many deep-sky objects in the southern hemisphere, contributing significantly to the New General Catalogue (NGC) compiled later by John Louis Emil Dreyer.



NGC 2899 is located approximately 4,500 light-years from Earth in the southern constellation Vela, which is part of the larger Vela-Puppis-Carina region of the Milky Way known for its rich <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">star-forming activity</a> and remnants of past stellar explosions.&nbsp;



Vela, whose name means "sails" in Latin, represents the sails of the ancient Greek mythological ship Argo Navis. This region of the sky is particularly abundant in nebulae, star clusters, and other deep-sky objects, making it a focal point for astronomical observations.&nbsp;



The nebula’s distance places it well within our galaxy, offering astronomers a valuable glimpse into the later stages of stellar evolution and the processes that sculpt and illuminate planetary nebulae.



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



Nebulae are vast clouds of gas and dust in space, often serving as the birthplaces or remnants of stars.&nbsp;



They come in various types, including emission nebulae that glow due to ionized gases energized by nearby stars, reflection nebulae that shine by scattering starlight, and dark nebulae that obscure light from background <a href="https://www.earth.com/news/runaway-star-may-be-dragging-a-planet-along-with-it/" target="_blank" rel="noreferrer noopener">stars</a>.&nbsp;



Planetary nebulae form when dying stars shed their outer layers, creating colorful, often symmetrical shapes. Nebulae can span light-years across and are key to understanding the life cycles of stars and the structure of galaxies.



<h2 class="wp-block-heading" id="h-the-fate-of-dying-stars">The fate of dying stars</h2>



Not all dying stars become planetary nebulae. In fact, stars much more massive than the Sun follow a very different and far more violent path.&nbsp;



These massive stars end their lives in dramatic supernova explosions, releasing tremendous energy and scattering heavy elements into space, which enriches the interstellar medium.&nbsp;



What remains after the explosion depends on the star’s mass. The collapsed core can form a neutron star - an incredibly dense object composed mostly of neutrons. Or, if the star was even more massive, it may create a <a href="https://www.earth.com/news/astronomers-confirm-lone-black-hole-wandering-through-our-galaxy/" target="_blank" rel="noreferrer noopener">black hole</a>, where gravity is so intense that not even light can escape.



<h2 class="wp-block-heading" id="h-examples-of-winged-nebulae-nbsp">Examples of “winged” nebulae&nbsp;</h2>



Several well-known nebulae are noted for their "winged" or symmetrical, wing-like appearances, often earning them evocative nicknames.&nbsp;



One of the most famous is the Butterfly Nebula, located in the constellation Scorpius. This planetary <a href="https://www.earth.com/news/dragons-egg-nebula-is-a-truly-stunning-sight-to-behold/" target="_blank" rel="noreferrer noopener">nebula</a> displays two expansive lobes that resemble butterfly wings, shaped by fast stellar winds from a dying star.



The Omega Nebula (also known as the Swan Nebula) in the constellation Sagittarius is a bright star-forming region that has been said to resemble a swan in flight. It has broad, glowing "wings" formed by clouds of ionized hydrogen gas. 



Similarly, the Eagle Nebula has an overall shape reminiscent of a bird with outstretched wings, which inspired its name. It is located in the constellation Serpens and home to the iconic "Pillars of Creation."



Image Credit: ESA



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Planetary nebula with ethereal wings captured by Hubble

Today's Image of the Day from the European Space Agency features the vibrant colors of the Mawrth Vallis region of Mars. The image reveals a landscape abundant in iron, magnesium, and aluminum.&nbsp;



Mawrth Vallis lies just south of the dichotomy boundary, a ridge marking the divide between Mars' southern highlands and northern lowlands. Layered, clay-rich deposits found in this valley indicate prolonged interactions with water. 



Mawrth Vallis is considered a prime candidate for studying past habitability and the potential for preserved biosignatures. The region continues to captivate scientists due to its geological complexity and history of <a href="https://www.earth.com/news/mars-has-a-water-reservoir-two-miles-deep-enough-to-fill-earths-red-sea/" target="_blank" rel="noreferrer noopener">liquid water</a> flow. 



<h2 class="wp-block-heading" id="h-the-colors-of-mars">The colors of Mars</h2>



<a href="https://www.earth.com/news/air-samples-from-mars-could-reveal-fascinating-secrets/" target="_blank" rel="noreferrer noopener">Mars</a> gets its distinctive red color from iron oxides, or rust, on its surface. The Martian soil and dust are rich in iron minerals, which oxidize when exposed to the small amounts of oxygen present in the Martian atmosphere.&nbsp;



This oxidation process gives the planet its reddish hue, similar to how iron objects on Earth develop rust. 



The scattering of sunlight by these iron oxide particles further enhances the reddish appearance when viewed from a distance. However, the human eye can only perceive a fraction of Mars' <a href="https://www.earth.com/news/mars-captured-in-true-color-like-youve-never-seen-the-red-planet-before/" target="_blank" rel="noreferrer noopener">true color</a> palette.&nbsp;



<h2 class="wp-block-heading" id="h-striking-colors-revealed">Striking colors revealed</h2>



The European Colour and Stereo Surface Imaging System (CaSSIS) aboard the ExoMars Trace Gas Orbiter (TGO) offers a more detailed view, showcasing a striking diversity of colors.&nbsp;



This CaSSIS <a href="https://www.esa.int/ESA_Multimedia/Images/2024/06/Metallic_Mars_landscape" target="_blank" rel="noreferrer noopener">image</a> reveals yellow layers rich in iron and magnesium clays, overlain by white and blue layers abundant in aluminum.&nbsp;



The area is draped by a dark, heavily eroded layer, illustrating a vibrant, metallic landscape formed around 3.6 billion years ago.



<h2 class="wp-block-heading" id="h-upcoming-rosalind-franklin-mission">Upcoming Rosalind Franklin mission</h2>



The Rosalind Franklin mission is a joint mission by the European Space Agency (ESA) and Roscosmos aimed at exploring the surface of Mars to search for signs of past or present life. 



The mission is named after Rosalind Franklin, the pioneering British scientist whose work was crucial in the discovery of DNA's structure.



The rover is designed to drill up to two meters below the Martian surface, where it is believed any signs of life may be better preserved, away from the harsh surface radiation. 



The Rosalind Franklin rover was originally scheduled to launch in 2020, but technical delays and the COVID-19 pandemic pushed the launch window to 2028. 



Once on Mars, the rover will collaborate with other missions like NASA's Perseverance and Curiosity rovers to advance our understanding of the Red Planet's habitability and history.



<h2 class="wp-block-heading" id="h-studying-mars-ancient-past">Studying Mars’ ancient past</h2>



While Rosalind Franklin prepares for its mission, the TGO remains in orbit, conducting crucial research to unravel Mars' ancient past and assess its potential <a href="https://www.earth.com/news/secrets-of-mars-seismic-discoveries-and-the-quest-for-past-life/" target="_blank" rel="noreferrer noopener">habitability</a>.&nbsp;



Since beginning its full science mission in 2018, TGO has not only captured stunning images but also provided a comprehensive inventory of Mars' atmospheric gases and mapped water-rich locations on the planet's surface.



For six years, CaSSIS has delivered breathtaking views of Mars in vivid color, documenting features ranging from volcanic landscapes to active dust devils and immense sand dunes.&nbsp;



Understanding Mars' water history and its implications for past <a href="https://www.earth.com/news/mars-is-letting-out-mysterious-methane-burps-but-why/" target="_blank" rel="noreferrer noopener">life</a> remains a core focus of ESA’s ExoMars missions.



<h2 class="wp-block-heading" id="h-metals-on-mars">Metals on Mars</h2>



Mars is rich in various metals that contribute to its geological and mineralogical diversity. 



While iron is the most prominent, magnesium is also abundant. It is often found in the form of clays, contributing to the planet's diverse mineral composition. 



Aluminum is another significant metal present on Mars, commonly found in layered deposits and sediments. 



<h2 class="wp-block-heading" id="h-major-changes-over-time">Major changes over time</h2>



The metals are not evenly distributed but are found in various concentrations across the Martian surface. 



For instance, regions like Mawrth Vallis exhibit a complex layering of different metal-rich minerals, including iron and magnesium-rich clays overlain by aluminium-rich layers.&nbsp;



This diversity indicates a rich geological history involving water activity, volcanic processes, and sedimentary deposition.



The presence of these metals suggests that Mars has undergone significant chemical and physical processes over billions of years, shaping its current landscape.&nbsp;



Understanding the distribution and composition of metals on Mars helps scientists piece together the planet's history and assess its past potential for habitability.



Image Credit: ESA/TGO/CaSSIS



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Metallic Mars: The diverse colors of the Red Planet

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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



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



The Antennae Galaxies provide a glimpse into the future of our <a href="https://www.earth.com/news/uma3-u1-faintest-star-system-found-orbiting-milky-way-galaxy/" target="_blank" rel="noreferrer noopener">Milky Way</a>, which is expected to eventually merge with the Andromeda Galaxy - our closest spiral galaxy neighbor.



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



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



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



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



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



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



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



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



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



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



Image Credit: ESA/Hubble &amp; NASA



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Violent clash of the Antennae Galaxies  

By 2030, more than a billion adolescents aged 10 to 24 will still be growing up in countries where basic health risks remain widespread. 



Issues like HIV/AIDS, early pregnancy, unsafe sex, poor mental health, malnutrition, and injury are expected to continue threatening adolescent well-being - despite being largely preventable or treatable.



These are the findings of a new report from the second Lancet Commission on Adolescent Health and Well-being. The researchers concluded that the world is making slow, uneven progress - and many young people are at risk of being left behind.



“The health and well-being of adolescents worldwide is at a tipping point,” said Professor Sarah Baird of <a href="https://www.gwu.edu/" target="_blank" rel="noreferrer noopener">George Washington University</a>.



<h2 class="wp-block-heading" id="h-mixed-gains-for-teen-health">Mixed gains for teen health</h2>



The new report updates a landmark 2016 Commission by examining changes over the past ten years. It shows some positive signs. 



<a href="https://www.earth.com/news/smoking-cigarettes-accelerates-aging/">Smoking</a> and <a href="https://www.earth.com/news/alcohol-and-depression-study-challenges-self-medication-theory/" target="_blank" rel="noreferrer noopener">alcohol</a> use among adolescents are down. More young people are finishing high school and attending college. But these gains are overshadowed by rising problems. 



In some parts of Africa and Asia, adolescent obesity rates have jumped eightfold. Mental health issues are becoming more severe and widespread.



Even more concerning is how little has changed in key areas. In 2016, about 1 billion adolescents lived in what the Commission terms “multi-burden countries” - places where young people face multiple, daily health threats. That number has now grown to nearly 1.1 billion. Projections show that without urgent action, it will still top a billion by 2030.



Investing in young people's health and well-being is essential to securing our shared future. “We must prioritize investment in adolescent health and wellbeing through initiatives including those that strengthen schools to promote health and wellbeing and to ensure universal access to healthcare for adolescents,” said Baird.



<h2 class="wp-block-heading" id="h-growing-health-risks-for-adolescents">Growing health risks for adolescents</h2>



One of the most alarming trends is the state of adolescent <a href="https://www.earth.com/news/mental-health-the-hidden-casualty-of-climate-change/" target="_blank" rel="noreferrer noopener">mental health</a>. In countries with data, mental health among young people has worsened over the last 30 years. 



The COVID-19 pandemic made things even harder. By 2030, mental illness and suicide will cost adolescents 42 million healthy life years - 2 million more than in 2015.



Another issue is anemia, especially among girls. Nearly one in three adolescent girls could be anaemic by 2030. The condition is linked to fatigue, poor growth, and - in severe cases - organ damage. Yet progress in addressing it has been slow.



<a href="https://www.earth.com/news/obesity-is-linked-to-32-cancer-types-that-could-drive-40-of-cases/">Obesity</a> is also increasing at a worrying pace. By 2030, one-third of adolescents in high-income countries, Latin America, and the Middle East may exceed recommended weight. Global numbers will rise to 464 million, up from 321 million in 2015.



<h2 class="wp-block-heading" id="h-demographic-shifts-and-global-progress">Demographic shifts and global progress </h2>



Professor Alex Ezeh of Drexel University noted that demographic shifts will continue to drive global progress - or lack thereof - in adolescent health and well-being.



“Africa’s share of global adolescents will increase from under 25% currently to more than 46% by 2100," said Professor Ezeh.



"Consequently, progress in improving the health and well-being of adolescents in Africa will increasingly determine progress in improving the health and well-being of adolescents globally.”



<h2 class="wp-block-heading" id="h-the-challenge-of-climate-change">The challenge of climate change</h2>



The Commission points to two emerging issues that will shape adolescent health in the decades to come: climate change and <a href="https://www.earth.com/news/how-does-digital-technology-influence-our-sense-of-self/" target="_blank" rel="noreferrer noopener">digital technology</a>.



Climate change is already impacting today’s youth. For the first time, a generation will grow up with global temperatures consistently 0.5°C above pre-industrial levels. 



By 2100, that could rise to 2.8°C. This increase brings serious risks - heat-related illnesses, reduced food and water supplies, and mental health problems linked to climate trauma.



A new review by the Commission shows both sudden disasters (like hurricanes) and slower events (like long-term food insecurity) are harming adolescents' mental health. Conditions like PTSD, anxiety, and depression are on the rise.



<h2 class="wp-block-heading" id="h-social-media-and-mental-health">Social media and mental health </h2>



Digital life is another double-edged sword. On the one hand, it gives adolescents access to new learning, work, and health tools. On the other, it replaces many in-person experiences with online ones. 



Though research is limited, concern is growing over social media’s impact on mental health. The Commission calls for balance - early protective steps without harsh restrictions that could isolate young people further.



<h2 class="wp-block-heading" id="h-adolescent-aid-is-underfunded">Adolescent aid is underfunded</h2>



Despite the scale of these challenges, funding has not kept pace. Adolescents make up 25% of the world’s population and face 9% of the global disease burden. Yet only 2.4% of global aid is directed toward their health and wellbeing.



The Commission argues this is a poor investment strategy. Spending on adolescents yields results equal to or greater than investing in early childhood. 



But funding often goes to adults or younger children, partly because adolescent health lacks strong leadership and coordination at both global and national levels.



<h2 class="wp-block-heading" id="h-strategies-to-protect-adolescent-health">Strategies to protect adolescent health</h2>



Dr. Aaron Jenkins of the University of Sydney said that he is profoundly encouraged by our Second Lancet Commission on adolescent health and well-being, which embraces the ecological foundations of human well-being.



"For the first time, we are identifying and encouraging interventions that simultaneously advance adolescent health, ecological integrity, biodiversity conservation, climate change mitigation, and social justice.”



<h2 class="wp-block-heading" id="h-a-youth-led-push-for-change">A youth-led push for change</h2>



The research stands out for how it involved young people. Ten youth commissioners aged 23 to 35 helped lead the work, representing diverse sectors like academia, civil society, and international organizations. Their experiences and <a href="https://www.earth.com/news/employees-win-empowered-trust/" target="_blank" rel="noreferrer noopener">leadership</a> shaped the final recommendations. 



In addition, more than 200 adolescents from 36 countries participated in Youth Solution Labs to identify top priorities and solutions.



“Young people are navigating a rapidly changing world, and through this Commission we’ve heard the diverse and alarming concerns adolescents have about their health,” said Youth Commissioner Dr. Shakira Choonara. 



“However, there are also opportunities - and we've seen firsthand and through the Commission findings how adolescents are already stepping up as active citizens and powerful agents of change.”



“I am deeply inspired by the change youth leaders are bringing to their communities and to the global landscape. Investing in and engaging with our generation will build a healthier, more empowered, and better-equipped generation of future leaders.”



The full study was published in the journal <a href="https://www.thelancet.com/journals/lancet/article/PIIS0140-6736(25)00503-3/abstract" target="_blank" rel="noreferrer noopener">The Lancet</a>.



<blockquote class="wp-block-quote">
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Over a billion adolescents face a major health crisis by 2030

By 2030, more than a billion adolescents aged 10 to...

A walk in the forest often brings peace, calm, and a deep sense of renewal. From ancient times to modern therapy practices, forests have stood as symbols of balance and healing. But not all forests heal equally. 



As cities grow and public health concerns rise, scientists are uncovering how the design and structure of forests matter. The health benefits we get from <a href="https://www.earth.com/news/cities-in-the-global-south-have-far-less-green-space/" target="_blank" rel="noreferrer noopener">green spaces</a>, especially forests, depend not just on their presence, but on what they are made of.



A new study from the University of Surrey and the <a href="https://www.ugent.be/en" target="_blank" rel="noreferrer noopener">University of Ghent</a> sheds light on this. Working with partners across Europe, the research team explored how specific features of forests influence human health. 



The findings mark a major step in understanding the complex links between ecological structure and wellbeing.



<h2 class="wp-block-heading" id="h-forest-traits-and-human-health-benefits">Forest traits and human health benefits </h2>



The study, which is part of the larger Dr. Forest research project, included 164 forests across five European countries. The researchers focused on seven ecological characteristics and their <a href="https://www.earth.com/news/urban-green-spaces-are-urgently-needed-across-the-global-south/" target="_blank" rel="noreferrer noopener">influence</a> on various health outcomes.



The forests were not selected at random. They varied in structure, species mix, and density, allowing researchers to draw comparisons. This wide range of forest types provided a rare opportunity to explore how real-world differences affect human experiences and health.



The goal was not to judge forests as good or bad, but to understand how their differences shaped people’s health responses. What emerged was a nuanced view. Forests benefit health, but their structure can amplify or limit those effects.



<h2 class="wp-block-heading" id="h-the-power-of-tree-diversity">The power of tree diversity</h2>



One of the key traits studied was tree species diversity. The findings showed that more diverse forests offered modest but positive health <a href="https://www.earth.com/news/urban-tree-layout-influences-human-health-and-mortality-rates/" target="_blank" rel="noreferrer noopener">outcomes</a>. These effects were not dramatic, but they were consistent enough to support the idea that diversity is beneficial.



Tree diversity does not just matter for human health. It also supports broader biodiversity, helping insects, birds, and mammals thrive. This makes it a safe, low-risk strategy for forest managers aiming to enhance public health while improving ecosystem resilience.



More tree species create different textures, shapes, and colors, making forests more visually stimulating and ecologically stable. These aspects can subtly influence how people feel and behave when they visit such areas. 



While the direct health impacts may be limited, the indirect ones, through enhanced engagement and ecosystem strength, are valuable.



<h2 class="wp-block-heading" id="h-canopy-structure-a-major-influence">Canopy structure: A major influence</h2>



Among the ecological features studied, canopy structure had the strongest impact. Dense canopies reduce heat by offering shade and help regulate the forest's internal climate. They also provide larger leaf surfaces, which trap fine particulate matter and improve air quality.



These benefits are especially important in urban settings, where heatwaves and pollution are on the rise. In such contexts, a well-structured canopy becomes more than a luxury. It is a necessity. The cooling effect alone can reduce heat stress and the risk of heat-related illnesses.



Yet, there are trade-offs. Denser canopies create more humid conditions. While that is good for moisture-loving plants, it also creates ideal habitats for ticks, which carry Lyme disease. 



In addition, less sunlight reaches the forest floor. This limits the growth of medicinal plants, reducing some of the forest's potential healing properties.



<h2 class="wp-block-heading" id="h-mental-health-gains-beyond-structure">Mental health gains beyond structure</h2>



Perhaps the most consistent finding across the study was the benefit of simply being in a forest. Regardless of structure or biodiversity, spending time in a forest improved mental wellbeing. People reported lower anxiety and stress, along with more positive <a href="https://www.earth.com/news/surprising-mental-health-benefits-of-living-near-green-spaces/" target="_blank" rel="noreferrer noopener">emotions</a>.



What enhanced these effects was how natural and biodiverse the forest felt to the visitor. Forests that looked wild, vibrant, and untamed tended to offer more psychological relief. This suggests that human perception plays a key role in shaping forest-based experiences.



“Our study shows that forests generally provide a mental health benefit, reducing anxiety and stress, regardless of their biodiversity or structure. As one in six people in England experience anxiety and depression each week, this research suggests that simply being in a forest can improve mental health,” noted Dr. Melissa Marselle, a lecturer in environmental psychology at the <a href="https://www.surrey.ac.uk" target="_blank" rel="noreferrer noopener">University of Surrey</a>.



“For the UK, this means preserving urban forests so people can easily access forests where they live, work and play for their mental wellbeing. Contact with forests could be prescribed by the NHS, as research shows that NHS nature prescriptions are effective at improving mental health.” 



<h2 class="wp-block-heading" id="h-designing-healthier-cities-with-forests">Designing healthier cities with forests </h2>



The study points to a pressing need in urban planning. It is not enough to plant trees and call it a forest. The structure, layout, and biodiversity of these spaces must be considered. Urban forests should reduce heat, absorb pollution, and offer mental rest.



This involves difficult trade-offs. Canopy density must balance between cooling the environment and letting in enough light. Species choices should consider both ecological function and visual appeal. Forests must feel natural to the human eye while also being safe and accessible.



Planners and health professionals can now use this evidence to shape better public spaces. Health services could integrate forest access into mental health treatments. Parks could be designed not just for recreation but also for healing. In a time when stress-related disorders are rising, these changes could make a meaningful difference.



<h2 class="wp-block-heading" id="h-forests-are-essential-tools-for-public-health">Forests are essential tools for public health</h2>



This research redefines the role of forests. No longer just natural assets or scenic spots, they emerge as powerful contributors to public health. But their power lies in their details. Forests must be built, preserved, and managed with intention.



Tree diversity adds depth and life. Canopy structure shapes the microclimate and air. Visitor perceptions tie it all together. Forests that feel alive and balanced bring calm and strength to those who enter them.



Nature has always played a quiet role in healing. Now, with evidence in hand, we have the chance to shape that role more deliberately. Managed well, forests can support both ecosystems and the people who rely on them for peace and mental clarity.



The study is published in the journal <a href="https://www.nature.com/articles/s41893-025-01547-3" target="_blank" rel="noreferrer noopener">Nature Sustainability</a>.



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Forests provide different health benefits based on their structure

A walk in the forest often brings peace, calm, and...

Our memories define us. They help us learn, shape our identities, and guide decisions. While the psychology of memory has long been explored, the biological roots remain a complex puzzle. Now, a breakthrough study from Linköping University (LiU) in Sweden sheds new light on how molecules in our brain might hold a kind of memory themselves.



Published in the journal Nature Communications, this work explores a special ion channel called CaV2.1, crucial for communication between brain <a href="https://www.earth.com/news/memory-isnt-only-stored-in-our-brains-other-cells-can-remember-too/" target="_blank" rel="noreferrer noopener">cells</a>. This molecular machine does more than just transmit signals. It appears to "remember" them, laying the groundwork for long-term changes in the brain.



The discovery has implications not only for understanding memory formation but also for treating rare neurological diseases linked to genetic variations in these channels.



<h2 class="wp-block-heading" id="h-how-brain-molecules-support-memory">How brain molecules support memory</h2>



The <a href="https://www.earth.com/news/secrets-of-learning-how-our-brains-neurons-make-and-retrieve-memories/" target="_blank" rel="noreferrer noopener">brain</a> uses electrical pulses to send messages across networks of neurons. At the end of these neurons are specialized junctions called synapses, where neurotransmitters pass the message forward. Calcium ion channels such as CaV2.1 sit at these junctions and regulate when neurotransmitters are released.



When a neuron fires, the CaV2.1 channel opens briefly, allowing calcium to enter. The calcium influx triggers neurotransmitter release into the synapse, reaching the next neuron. These brief openings seem simple, but they are essential for how we learn and adapt.



However, the channel does not stay fully responsive after repeated stimulation. If neurons fire continuously, fewer CaV2.1 channels remain ready to open. This leads to weaker signals at the synapse. Until now, scientists did not know how this "dampening" occurred on a molecular level.



“I want to uncover the secret lives of these ion channel molecules,” said Antonios Pantazis, associate professor at the Department of Biomedical and Clinical Sciences at LiU, who led the study.



“Calcium ion channels have very important functions in the body - by opening and closing, they regulate, among other things, nerve-to-nerve signaling. But beyond that, these molecules also have a kind of memory of their own, and can remember previous nerve signals.”



<h2 class="wp-block-heading" id="h-brain-molecules-hold-traces-of-memories">Brain molecules hold traces of memories</h2>



The study dives into the structure of CaV2.1 channels, revealing that they are made up of multiple parts called voltage-sensor domains or VSDs. These domains sense electrical <a href="https://www.earth.com/news/deep-sleep-how-slow-waves-boost-memory-formation/" target="_blank" rel="noreferrer noopener">changes</a> and help the channel open or close. Each VSD plays a different role.



VSD-I, in particular, emerged as the central player. It responds to brief electrical signals and undergoes a dramatic transformation after repeated activation. The researchers found that this domain could switch between two different operating modes. 



In one mode, it allows the channel to open. In the other, it effectively shuts the channel down. This switch doesn’t happen instantly. It’s a slow process that builds with repeated neural activity.



This behavior is strikingly similar to memory itself. Brief experiences can lead to long-term consequences. In this case, short bursts of neural activity reshape the channel, leaving a molecular trace of that experience.



<h2 class="wp-block-heading" id="h-brain-channels-shift-to-record-memory">Brain channels shift to record memory</h2>



Through voltage-clamp fluorometry and kinetic modeling, the researchers showed that CaV2.1 channels can adopt nearly 200 different conformations. These shifts depend on both the intensity and duration of electrical <a href="https://www.earth.com/news/breathing-rhythms-help-strengthen-memories-during-sleep/" target="_blank" rel="noreferrer noopener">signals</a>. It’s a level of molecular complexity far greater than previously imagined.



“We believe that during sustained electrical nerve signaling, an important part of the molecule disconnects from the channel gate, similar to the way the clutch in a car breaks the connection between the engine and the wheels,” said Pantazis.



“The ion channel can then no longer be opened. When hundreds of signals occur over long enough time, they can convert most channels into this ‘declutched memory state’ for several seconds.”



This state change is not just a quirk. It acts like a short-term memory at the molecular level. Although the channels stay shut for only a few seconds, this effect can accumulate across many neurons. 



The result is a long-term weakening of certain synapses, which over time may be pruned altogether. This is how the brain refines its networks.



<h2 class="wp-block-heading" id="h-short-brain-events-lasting-memory">Short brain events, lasting memory</h2>



One might wonder how a <a href="https://www.earth.com/news/human-brains-create-three-copies-of-every-memory-we-make/" target="_blank" rel="noreferrer noopener">memory</a> that lasts only seconds in one molecule could matter. But the answer lies in scale. In a brain with billions of neurons, such subtle changes can shape entire circuits. The researchers propose that the transition of VSD-I into its inactive mode contributes to a broader memory process.



“In this way, a ‘memory’ that lasts for a few seconds in a single molecule can make a small contribution to a person’s memory that lasts for a lifetime,” said Pantazis.



The timing here is crucial. A single neural spike lasts only milliseconds, but the channel’s inactive state can persist for seconds. That mismatch acts as a biological filter, allowing the brain to decide which signals are important enough to encode. 



Over time, repeated exposure to certain signals strengthens or weakens specific pathways, forming the basis of learning and memory.



<h2 class="wp-block-heading" id="h-molecular-shape-and-neural-function">Molecular shape and neural function </h2>



The research also uncovered how each of the four voltage-sensor domains behaves. VSD-II stood out as unresponsive to voltage, acting as a kind of bystander. VSD-III and VSD-IV, on the other hand, activated at more negative voltages and were sensitive to the brain’s resting state.



These domains help the channel prepare for incoming signals or fine-tune its response. However, only VSD-I showed a direct link to inactivation. This distinction helps researchers understand which part of the molecule could be targeted by future drugs.



The visual data, particularly the structural maps on pages 3 to 6 of the paper, illustrate how these domains shift under different conditions. These figures bring clarity to the idea that molecular shape affects neural function.



<h2 class="wp-block-heading" id="h-potential-for-new-treatments">Potential for new treatments</h2>



There’s more than curiosity at stake. The CACNA1A gene, which encodes the CaV2.1 channel, has many variants linked to rare but serious brain diseases. 



These include episodic ataxia and some forms of migraine. By pinpointing the regions responsible for the channel’s memory-like behavior, researchers can now identify where new drugs might act.



“Our work pinpoints which part of the protein should be targeted when developing new drugs,” noted Pantazis.



Understanding the exact shape and function of VSD-I, especially how it switches states, gives drug developers a precise target. Instead of broadly affecting the brain, a medication could focus on restoring proper function in only the channels that malfunction.



<h2 class="wp-block-heading" id="h-brain-molecules-support-flexible-memory">Brain molecules support flexible memory</h2>



At rest, the CaV2.1 channel is a picture of complexity. It can be open, closed, or inactivated. Its VSDs can exist in different states depending on the history of electrical activity. 



According to the models in the study, especially those on page 9, the greatest diversity in channel shape occurs at the brain's resting voltage. This allows the brain to stay flexible, ready to respond or to reset depending on context.



Depolarization, an electrical event, pushes VSDs into active positions. But only VSD-I directly causes the channel to open. That makes it the trigger point for neurotransmitter release and memory encoding.



Pantazis and colleagues suggest a term for this kind of behavior: syntasic. This means the VSD and pore open together, like gears meshing. The idea captures the elegance of how voltage, shape, and function all interconnect.



<h2 class="wp-block-heading" id="h-a-molecular-basis-for-memory">A molecular basis for memory</h2>



The study reveals that the molecules behind neural communication are not just passive players. They process information, adapt, and even remember. The CaV2.1 channel’s VSD-I acts as a gatekeeper, shaping how neurons communicate based on past activity.



In the grand theater of the brain, even the smallest parts play starring roles. By understanding these roles in detail, science moves closer to answering one of its oldest questions: how do we remember?



The study is published in the journal <a href="https://www.nature.com/articles/s41467-025-58884-2" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Brain molecules unexpectedly store their own memory

Our memories define us. They help us learn, shape our...

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