Archaeology sometimes feels like detective work with a very long timeline. Every chip of flint or shard of bone builds a narrative of how early humans used tools to feed themselves, cooperated, and thought about the places they called home. 



Fresh finds from two sites just northeast of today’s Tel Aviv - Jaljulia and Qesem Cave - add an eye-opening chapter to that story. 



They point to a moment, roughly 400,000 years ago, when hunters in the Levant not only pivoted to new prey but also <a href="https://www.earth.com/news/stone-tools-in-south-africa-reveal-early-human-communication/" target="_blank" rel="noreferrer noopener">redesigned their tools</a> and, perhaps, their beliefs.



The discoveries revolve around a specialized flint implement known as a Quina scraper. 



At first glance the artifact looks modest - smaller than a modern smartphone. Its scalloped edge, though, is razor-sharp, built for slicing through muscle and hide with an efficiency that would have impressed any butcher.



<h2 class="wp-block-heading" id="h-flint-tools-and-shifting-appetites">Flint tools and shifting appetites</h2>



For nearly a million years, large game dominated dinner menus here - especially elephants that roamed plains stretching from Africa into Eurasia. 



When those giants dwindled, hunting parties had to recalibrate. 



The speedier, leaner fallow deer offered far less meat per kill, so hunters needed to process many more carcasses to match the calories once supplied by a single elephant. That change forced a rethink of both <a href="https://www.earth.com/news/stone-tool-discovery-challenges-entire-theory-of-human-evolution/" target="_blank" rel="noreferrer noopener">strategy and gear</a>.



Fallow deer thrived in mixed woodlands along what are now the Samarian highlands. Their bones fill layers in Jaljulia and Qesem Cave, signaling a dietary shift that mirrors broader environmental turnover during the late Lower Paleolithic.



<h2 class="wp-block-heading" id="h-tools-carved-with-flint-for-venison">Tools carved with flint for venison</h2>



Enter the Quina scraper. Unlike earlier, more rudimentary scrapers, this one features a stepped, scale-like working edge that holds a keen bevel. 



Microscopic wear marks reveal repeated motions suited to neatly removing skin and sinew. The <a href="https://www.earth.com/news/prehistoric-homo-sapiens-stone-tools-preserved-volcanic-ash-grotta-di-castelcivita/" target="_blank" rel="noreferrer noopener">stone tool design</a> likely spared hunters valuable time at the kill site, reducing exposure to scavengers and rival predators that could steal a hard-won carcass.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/stone-tools_400000-years-old_Quina-like_credit-Tel-Aviv_2.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/stone-tools_400000-years-old_Quina-like_credit-Tel-Aviv_2s.webp" alt="A Quina scraper from Qesem Cave. Residue and use-wear analyses showed that the scraper was wrapped with organic material and used for scraping a dry hide (after Zupancich 2020)" class="wp-image-1970089"/></a><figcaption class="wp-element-caption">A Quina scraper from Qesem Cave. Residue and use-wear analyses showed that the scraper was wrapped with organic material and used for scraping a dry hide (after Zupancich 2020). Click image to enlarge. Credit: Tel Aviv University</figcaption></figure>



Modern experiments with replicas confirm that the tool excels at producing long, clean strips of hide - ideal for lashing shelters, wrapping meat, or even tailoring early garments. 



A single scraper could be resharpened several times, making it a portable workhorse on multi-day forays.



<h2 class="wp-block-heading" id="h-stone-from-sacred-hills">Stone from sacred hills</h2>



The most unexpected twist lies not in the tool’s shape but in its raw material. Quina scrapers at both sites were made of flint hauled roughly 12.4 miles from the western slopes of the Samarian mountains, bypassing closer outcrops. 



That same upland served as a calving ground for fallow deer. Hunters, then, were linking an essential resource - flint - to the very landscape that provided their new staple food.



The study’s lead authors - Vlad Litov and Prof. Ran Barkai of <a href="https://english.tau.ac.il/" target="_blank" rel="noreferrer noopener">Tel Aviv University</a> - spell out what that pairing means. 



"In this study we tried to understand why <a href="https://www.earth.com/news/stone-tool-flint-discovery-challenges-theory-of-human-cultural-evolution/" target="_blank" rel="noreferrer noopener">stone tools changed</a> during prehistoric times, with a focus on a technological change in scrapers in the Lower Paleolithic, about 400,000 years ago," Litov explained. 



<h2 class="wp-block-heading" id="h-forced-to-hunt-smaller-animals">Forced to hunt smaller animals</h2>



We found a dramatic change in the human diet during this period, probably resulting from a change in the available fauna: the large game, <a href="https://www.earth.com/news/how-ancient-humans-hunted-elephants-with-stone-tools/" target="_blank" rel="noreferrer noopener">particularly elephants</a>, had disappeared, and humans were forced to hunt smaller animals, especially fallow deer.



Clearly, butchering a large elephant is one thing, and processing a much smaller and more delicate fallow deer is quite a different challenge. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/stone-tools_400000-years-old_Quina-like_credit-Tel-Aviv_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/stone-tools_400000-years-old_Quina-like_credit-Tel-Aviv_1s.webp" alt="Examples of scrapers shaped by Quina-like retouch from the Late Acheulian Jaljulia: Déjeté scraper (a); transverse scraper (b); Single scrapers (c, d); Convergent scraper fragment (e)" class="wp-image-1970087"/></a><figcaption class="wp-element-caption">Examples of scrapers shaped by Quina-like retouch from the Late Acheulian Jaljulia: Déjeté scraper (a); transverse scraper (b); Single scrapers (c, d); Convergent scraper fragment (e). Click image to enlarge. Credit: Tel Aviv University</figcaption></figure>



Systematic processing of numerous fallow deer to compensate for a single elephant was a complex and demanding task that required the development of new implements. 



"Consequently, we see the emergence of the new Quina scrapers, with a better-shaped, sharper, more uniform working edge compared to the simple scrapers used previously," Litov added.



<h2 class="wp-block-heading" id="h-tech-advancement-shown-in-flint-tools">Tech advancement shown in flint tools</h2>



Prof. Barkai explains that the study reveals “links between technological developments and changes in the fauna hunted and consumed by early humans.” 



While previous theories credited <a href="https://www.earth.com/news/from-nature-to-knapping-the-surprising-origins-of-stone-tools/" target="_blank" rel="noreferrer noopener">advancements in stone tools</a> to biological evolution, he and his team suggest a “double connection, both practical and perceptual.”



Practically, tool sophistication evolved to meet the demands of hunting smaller, faster prey. Perceptually, Barkai points to a symbolic association between specific locations and resources. 



“We found a connection between the plentiful source of fallow deer and the source of flint used to butcher them,” he notes. 



<a href="https://www.earth.com/news/early-humans-used-interesting-technique-hunt-big-animals-clovis-points/" target="_blank" rel="noreferrer noopener">Prehistoric hunters</a> seemed to favor flint from the same region where the deer roamed - Mounts Ebal and Gerizim - suggesting a deep-rooted awareness of the landscape and its significance.



“This behavior,” he adds, “is familiar from many other places worldwide and is still widely practiced by native hunter-gatherer communities.”



<h2 class="wp-block-heading" id="h-why-does-any-of-this-matter">Why does any of this matter?</h2>



According to Litov, the <a href="https://en.wikipedia.org/wiki/Samaria" target="_blank" rel="noreferrer noopener">Mountains of Samaria</a> held deep significance for prehistoric people living at Qesem Cave and Jaljulia. 



“We believe that the Mountains of Samaria were sacred to the prehistoric people… because that’s where the fallow deer came from,” he says.



As elephant populations declined, early humans in the region shifted their focus to fallow deer. Tools made from a variety of local stones have been found at Jaljulia, but something unique occurred when they began sourcing both their prey and tool-making materials from the Samarian highlands.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/05/stone-tools_400000-years-old_Quina-like_credit-Tel-Aviv_3m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/05/stone-tools_400000-years-old_Quina-like_credit-Tel-Aviv_3s.webp" alt="A close look at a Quina-like scraper from Jaljulia. Credit: Tel Aviv University" class="wp-image-1970091"/></a><figcaption class="wp-element-caption">A close look at a Quina-like scraper from Jaljulia. Click image to enlarge. Credit: Tel Aviv University</figcaption></figure>



“Identifying the deer's plentiful source, they began to develop the unique scrapers in the same place,” Litov explains. 



These specialized tools - first appearing in Jaljulia around 500,000 years ago - later spread more broadly, showing up at Qesem Cave between 400,000 and 200,000 years ago.



Archaeological evidence, including fallow deer bones from Mount Gerizim and other sites, suggests that the area supported deer populations well into the Holocene. 



“Apparently, the Mountains of Samaria gained a prominent or even sacred status as early as the Paleolithic period,” Litov concludes, “and retained their unique cultural position for hundreds of thousands of years.”



<h2 class="wp-block-heading" id="h-prehistoric-man-was-smarter-than-we-thought">Prehistoric man was smarter than we thought</h2>



Pairing a resource with a place crops up again and again in human history, from obsidian quarries in the American Southwest to jade rivers in ancient China. 



The Jaljulia and <a href="https://en.wikipedia.org/wiki/Qesem_cave" target="_blank" rel="noreferrer noopener">Qesem Cave</a> findings push that behavior deep into the past, showing that meaning and material were already intertwined long before written lore. Technology did not change in a vacuum; it mirrored environmental stress and social imagination.



Understanding how early communities adapted to shrinking megafauna offers a cautionary parallel for modern ecosystems losing key species. Innovation can soften the blow, but it also reshapes culture in ways that echo far beyond survival. 



A humble flint scraper, carried miles across rugged ground, reminds us that tools are never just tools. They are signatures of what people value, where they find sustenance, and how they make sense of their world.



The full study was published in the journal&nbsp;<a href="https://link.springer.com/article/10.1007/s11759-024-09493-w" target="_blank" rel="noreferrer noopener">Archaeologies</a>.



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Stone tools created 400,000 years show technological advancement of early humans

Archaeology sometimes feels like detective work with a very long timeline. Every chip of flint or shard of bone builds a narrative of how early humans used tools to feed themselves, cooperated, and thought about the places they called home. Fresh finds from two sites just northeast of today’s Tel Aviv - Jaljulia and Qesem Cave - add an eye-opening chapter to that story. They point to a moment, roughly 400,000 years ago, when hunters in the Levant not only pivoted to new prey but also redesigned...

Throughout history, humanity has chased the elusive promise of eternal youth. From mythical fountains to today's anti-aging creams, the pursuit of staying forever young remains constant. But beneath this superficial search lies a deeper scientific exploration into cellular aging.



Recently, a team of researchers at <a href="https://www.osaka-u.ac.jp/en" target="_blank" rel="noreferrer noopener">Osaka University</a> in Japan might have brought us closer to genuinely reversing the aging process at a cellular level.



<h2 class="wp-block-heading" id="h-understanding-cellular-aging">Understanding cellular aging</h2>



Our bodies naturally <a href="https://www.earth.com/news/random-dna-mutations-shape-biological-aging/" target="_blank" rel="noreferrer noopener">age</a> as cells gradually become less active, transitioning into a state known as senescence. Senescent cells are not just older; they are distinctly larger and characterized by thicker stress fibers. 



These stress fibers play a crucial role in how cells move and interact with their surrounding environment. However, why these older cells maintain such an unusually large size has puzzled scientists for years.



"We still don't understand how these senescent cells can maintain their huge size," noted study lead author Pirawan Chantachotikul. 



"One intriguing clue is that stress fibers are much thicker in senescent cells than in young cells, suggesting that proteins within these fibers help support their size."



<h2 class="wp-block-heading" id="h-promoting-cellular-rejuvenation">Promoting cellular rejuvenation </h2>



In their quest for answers, researchers pinpointed a specific protein, AP2A1 (Adaptor Protein Complex 2, Alpha 1 Subunit), which seems crucial to this cellular phenomenon. 



Found predominantly in senescent cells, particularly within the structural stress fibers, AP2A1 could be the key to understanding cellular aging.



To explore AP2A1’s function, researchers manipulated its presence in cells, observing significant effects. 



"The results were very intriguing," said Shinji Deguchi, senior author of the study. "Suppressing AP2A1 in older cells reversed senescence and promoted cellular rejuvenation, while AP2A1 overexpression in young cells advanced senescence."



<h2 class="wp-block-heading" id="h-understanding-collagen-the-basics">Understanding collagen - the basics</h2>



Collagen is like the glue that holds your body together - it keeps your skin firm, joints flexible, and hair and nails strong. 



But as you age, your body produces less collagen, leading to wrinkles, sagging skin, and achy joints. 



Starting in your mid-20s, collagen production naturally slows down, and by the time you hit your 40s and 50s, the decline becomes more noticeable. 



Sun exposure, smoking, poor diet, and stress can speed up collagen breakdown, making aging signs appear even faster. 



That’s why skincare and supplement industries are obsessed with collagen - it’s the key to keeping things youthful.



<h2 class="wp-block-heading" id="h-complex-collagen-scaffold">Complex collagen scaffold </h2>



Delving further into AP2A1, the researchers identified its close interaction with another vital protein, integrin β1. 



Integrin β1 is known for anchoring cells to their external surroundings, specifically to the extracellular matrix - a complex collagen scaffold providing structural support. 



Both AP2A1 and integrin β1 appear to traverse the stress fibers together, a process critical in cell structure and function.



Integrin β1’s role in strengthening adhesion between cells and their external environment could explain the enlarged and raised structure typical of senescent cells. This interaction likely helps older cells maintain their oversized physical characteristics.



<h2 class="wp-block-heading" id="h-potential-marker-for-cellular-aging">Potential marker for cellular aging</h2>



Given its strong correlation with senescent cells, AP2A1 presents itself as an exciting potential <a href="https://www.earth.com/news/muscles-defy-aging-with-remarkable-resilience/" target="_blank" rel="noreferrer noopener">biomarker</a> for aging. 



Identifying such markers is crucial in understanding aging at a molecular level and might eventually allow scientists to quantify aging more precisely.



Moreover, AP2A1 is not just a passive marker. Its active involvement in aging processes positions it as a promising target for medical interventions aimed at combating age-related diseases.



<h2 class="wp-block-heading" id="h-beyond-cosmetic-applications">Beyond cosmetic applications</h2>



This research is important beyond just improving how we look as we <a href="https://www.earth.com/news/beyond-genetics-the-biggest-factors-that-influence-health-and-aging/" target="_blank" rel="noreferrer noopener">age</a>. It targets the root cause of aging at the cellular level. 



Diseases linked to aging, such as heart disease, osteoporosis, and some cancers, may improve with therapies targeting proteins like AP2A1.



If scientists can reverse or slow cellular aging, people might live healthier, longer lives. Instead of treating symptoms after diseases appear, this approach prevents or delays their onset. 



Thus, understanding AP2A1 could lead to significant advances in medicine, benefiting overall human health, increasing lifespan, and enhancing quality of life.



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



The identification of a cellular process linked directly to aging offers exciting possibilities for future treatments. Current anti-aging methods usually mask aging symptoms rather than addressing their causes.



However, this new cellular discovery targets aging at its <a href="https://www.earth.com/news/aging-hotspot-found-in-the-brain-may-hold-the-key-to-longevity/" target="_blank" rel="noreferrer noopener">roots</a>, potentially reversing the process entirely. While the research is still evolving and requires further studies, its potential impact is significant. 



By understanding and controlling cellular mechanisms like the AP2A1 protein, medicine could effectively reverse aging, not just hide it.



Such advances promise genuine rejuvenation, significantly improving human health and extending lifespan. 



As science moves forward, these findings could lead to treatments combating various age-related diseases, from osteoporosis to heart disease.



Though practical applications are not yet available, the groundwork is promising. The ultimate goal is to help people maintain youthfulness at the cellular level, enhancing overall health and longevity.



The study is published in the journal <a href="https://www.sciencedirect.com/science/article/pii/S0898656825000294?via%3Dihub" target="_blank" rel="noreferrer noopener">Cellular Signalling</a>.



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Study: Protein discovered that can reverse cellular aging

Throughout history, humanity has chased the elusive promise of eternal...

Titanium leads the way in Japan’s most recent leap into renewable energy. The country has now unveiled the first solar panel that makes use of titanium - a technology that could potentially be 1000 times more powerful than traditional cells.



By harnessing the unique properties of titanium dioxide and selenium, this innovative approach not only boosts efficiency dramatically but also has the potential to transform the entire solar power generation sector. 



<h2 class="wp-block-heading" id="h-titanium-solar-panels-are-cheaper">Titanium solar panels are cheaper</h2>



Conventional solar panels use silicon-based materials whereas the new Japanese technology involves panels that use layers of titanium and selenium in the photovoltaic cells. 



The researchers found that they could enhance the adhesion between the layers of titanium oxide and selenium, which improved the energy conversion efficiency and allowed more electricity to be generated from the same amount of sunlight. 



They introduced this technology to the world in a publication in <a href="https://www.sciencedirect.com/science/article/abs/pii/S092702482400432X">Solar Energy Materials and Solar Cells.</a>



Titanium is a metal with exceptional strength and resistance to corrosion, making it useful for many engineering applications. However, its energy-intensive extraction process has always made it too costly to use extensively. 



<h2 class="wp-block-heading" id="h-solar-energy-and-titanium">Solar energy and titanium</h2>



Scientists from the <a href="https://www.u-tokyo.ac.jp/en/" target="_blank" rel="noreferrer noopener">University of Tokyo</a> have now designed a process of extraction that may finally break down the cost barrier of titanium and render it more accessible for numerous applications, including <a href="https://www.earth.com/news/harnessing-solar-power/" target="_blank" rel="noreferrer noopener">solar energy</a>. 



The results of this research, published in <a href="https://www.nature.com/articles/s41467-024-49085-4">Nature Communications</a>, have far-reaching implications, not just for the renewable energy industry, but also for other fields that make use of titanium, such as the aerospace industry and medical technologies.



“Industry mass-produces iron and aluminum metal - but not titanium metal, because of the expense of removing the oxygen from the ore,” explained Toru H. Okabe, lead author of the study. 



“We use an innovative technology based on rare-earth metals that removes oxygen from titanium to 0.02% on a per-mass basis.”



<h2 class="wp-block-heading" id="h-titanium-cost-no-longer-a-problem">Titanium cost no longer a problem </h2>



In order to remove oxygen from <a href="https://www.earth.com/news/titanium-is-a-promising-and-abundant-resource-for-carbon-capture/">titanium</a> ore and generate a purer metal, high energy input is needed. This has made titanium prohibitively expensive for many industrial applications. 



However, the new Japanese extraction process makes use of another rare element, namely yttrium. This metal is commonly used in a range of technologies, including LED screens and superconductors. 



The researchers reacted molten titanium with yttrium metal to produce a low-cost, solid, de-oxygenated titanium alloy.



Despite the fact that the new process is far more cost-effective, yttrium also comes with its drawbacks.



<h2 class="wp-block-heading" id="h-yttrium-is-a-blessing-and-a-curse">Yttrium is a blessing and a curse</h2>



Yttrium is clearly a huge asset when used to purify titanium, but a problem arises because the resulting product contains up to 1% yttrium, which could potentially affect the titanium's durability and resistance to corrosion.



These effects could pose a significant challenge to sectors like electronics and aerospace. 



Nonetheless, efforts are underway to resolve these issues and reduce the contamination by yttrium while still preserving the cost-saving benefits. In this way, countless additional applications for cheaper titanium could be unlocked.



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



This remarkable journey of scientific innovation doesn't just end here. The <a href="https://www.earth.com/news/renewable-energy-must-be-doubled-by-2030/" target="_blank" rel="noreferrer noopener">renewable energy</a> sector is poised for a dramatic transformation as we strive to harness greener resources even more effectively. 



Though the yttrium problem needs to be addressed, the overall outlook is upbeat. 



This is indeed a fertile terrain for future investments as continued research and development could lead to enhanced scalability and efficiency.



The key to realizing this technology's full potential lies in continuous investment and global cooperation. Success in this venture could herald a new age of solar power, making <a href="https://www.earth.com/news/clean-energy-biodiversity-wildlife-habitats-delicate-balancing-act/" target="_blank" rel="noreferrer noopener">clean energy</a> more potent, more accessible, and more affordable. 



With the advent of next-gen solar panels and more affordable titanium, the future of renewable energy has never been more exciting.



<h2 class="wp-block-heading" id="h-charting-the-course-ahead">Charting the course ahead</h2>



Japan's titanium solar panel breakthrough marks not just an evolution in solar technology, but a potential paradigm shift across multiple industries. 



As the world increasingly turns toward sustainable energy solutions, these innovation signal an era where advanced materials and smart engineering converge to redefine what's possible.



Beyond renewable energy, the success of titanium-based panels could catalyze the adoption of titanium innovations in other sectors, ranging from electronics to aerospace, while also driving down production costs and spurring economic growth.



Policymakers and industry leaders now have a unique opportunity to support these advances and pave the way for widespread implementation and further research investments.



In essence, this pioneering work is more than a scientific achievement; it represents a collective leap toward a future where clean, efficient energy is accessible to all. 



Details of this research were published in <a href="https://www.sciencedirect.com/science/article/abs/pii/S092702482400432X" target="_blank" rel="noreferrer noopener">Solar Energy Materials and Solar Cells</a>, and in <a href="https://www.nature.com/articles/s41467-024-49085-4" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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New solar panels are 1000 times more powerful with big tech breakthrough

Titanium leads the way in Japan’s most recent leap into...

Nearly a century ago, some astronomers proposed that we might be seeing only half the story of the universe's expansion. A lesser-known concept, called the “tired light” theory, proposed that photons could lose energy as they travel through space, causing what looks like expanding motion. 



Some experts have speculated that a possible spin of the universe could influence our perception of cosmic movement. However, the majority of experts support the Big Bang model, citing observations of galaxies moving away from us at rapid speeds.



<h2 class="wp-block-heading" id="h-our-perception-of-universe-expansion">Our perception of universe expansion </h2>



Lior Shamir, an associate professor at <a href="https://www.k-state.edu/" target="_blank" rel="noreferrer noopener">Kansas State University</a>, has brought this old theory back into focus. His recent work suggests that a fresh look at <a href="https://science.nasa.gov/mission/webb/multimedia/images/" target="_blank" rel="noreferrer noopener">JWST images</a> might offer a different perspective on what we perceive as the expansion of the universe.



Scientists have noted that JWST observations reveal galaxies that seem older than the universe itself, if based on traditional timelines. This contradicts the idea that everything condensed from a single point 13.8 billion years ago.



“The JWST provided deep images of the very early universe, but instead of showing an infant early universe…it showed large and mature galaxies,” said Professor Shamir.



Big Bang supporters are not all convinced to abandon their view. However, a portion of the astronomy community feels that such data call for a second glance at less conventional models. A few wonder whether our accepted view of cosmic expansion oversimplifies the story.



<h2 class="wp-block-heading" id="h-could-light-be-tricking-us">Could light be tricking us?</h2>



“The tired light theory was largely neglected, as astronomers adopted the Big Bang theory as the consensus model,” explained Professor Shamir. He has offered fresh <a href="https://www.mdpi.com/2571-712X/7/3/41" target="_blank" rel="noreferrer noopener">evidence</a> supporting the long-dismissed concept. 



If <a href="https://www.energy.gov/science/doe-explainsphotons" target="_blank" rel="noreferrer noopener">photons</a> gradually lose energy, the <a href="https://www.earth.com/news/largest-structure-in-universe-is-1-4-billion-light-years-long-quipu-superstructure/" target="_blank" rel="noreferrer noopener">universal</a> timeline we use might be off. That helps explain why galaxies appear so developed at early stages. Light might not always be a perfect gauge of distance if it changes subtly on the way.



Recent <a href="https://ui.adsabs.harvard.edu/abs/1988CeMec..45...31B/abstract" target="_blank" rel="noreferrer noopener">data</a> shows that almost all galaxies in the early universe displayed by JWST appear to rotate in the same direction. Shamir’s analysis found up to 50% more galaxies swirling one way, a difference that can even be seen by a non-expert scanning the images. 



He suggests this anomaly could mean the universe was “born” spinning or that we might live inside a colossal black hole.



Professor Shamir also noted that this rotational imbalance might be due to the Earth’s own motion. Because of <a href="https://courses.lumenlearning.com/suny-physics/chapter/6-1-rotation-angle-and-angular-velocity/" target="_blank" rel="noreferrer noopener">rotational velocity</a>, galaxies moving the opposite way relative to the Milky Way may appear brighter, so we see more of them.



Shamir’s team measured redshift in over 30,000 galaxies and found that the gap becomes larger at greater distances.



<h2 class="wp-block-heading" id="h-does-the-universe-spin">Does the universe spin?</h2>



The "axis of evil" in cosmology refers to unexpected alignments in the cosmic microwave background (CMB) radiation, suggesting a preferred direction in the universe. 



This is at odds with the widely accepted cosmological principle, which states that the universe should appear isotropic (the same in all directions) on large scales.



Some researchers speculate that this alignment could be a statistical fluke, an artifact of our observational methods, or even an indication of new physics beyond the standard model of cosmology. Others propose that it might hint at a deeper structure in the universe, challenging the assumption of uniformity.



Another theory entertains the possibility of a <a href="https://research.kuleuven.be/portal/en/project/3E230655" target="_blank" rel="noreferrer noopener">holographic universe</a>, pointing out that if the universe does have a giant spin, it is not unlike a black hole’s interior. 



This concept, commonly referred to as black hole cosmology, has circulated in physics circles for years, and Professor Shamir’s research brings it back into focus.



<h2 class="wp-block-heading" id="h-distance-measurements-may-shift">Distance measurements may shift</h2>



Shamir’s work also suggests that measurements of galaxies have overlooked the Milky Way’s rotational speed. If galaxies rotating opposite to the Milky Way show stronger brightness due to <a href="https://www.grc.nasa.gov/www/k-12/airplane/doppler.html" target="_blank" rel="noreferrer noopener">Doppler effects</a>, the difference could alter assumptions about how far away they are.



“Because the rotational velocity of the Earth relative to the galaxies is constant, the reason for the difference can be the distance of the galaxies from Earth,” noted Professor Shamir.



If that holds up, we may have to recalibrate large portions of existing data, which could reconcile other mysteries such as the mismatch in expansion rates and sightings of hefty <a href="https://www.earth.com/news/powerful-forces-have-made-the-structure-of-the-universe-messier/" target="_blank" rel="noreferrer noopener">galaxies</a> in early epochs.



<h2 class="wp-block-heading" id="h-gaps-in-the-big-bang-theory">Gaps in the Big Bang theory</h2>



Not everyone is ready to rewrite the textbooks, but some scientists see these observations as a nudge to keep an open mind. 



A few have always <a href="https://vernbender.com/key-points-about-criticisms-of-the-big-bang-theory-2/" target="_blank" rel="noreferrer noopener">contended</a> that the Big Bang theory left unexplained gaps, suggesting that light from distant galaxies may have simply lost energy over time. Shamir’s study echoes that question.&nbsp;



“If the Big Bang happened as scientists initially believed, these galaxies are older than the universe itself,” said Shamir. 



To him, that’s one more signal that alternative routes in cosmology deserve attention. An increasing number of researchers are questioning whether we made a basic error about universal expansion.



Whether or not the Big Bang needs a full overhaul is up for debate. But the evidence keeps stacking up that current distance yardsticks might be incomplete. 



Ultimately, the research indicates that we may yet discover hidden nuances in redshift data or find that the cosmos has had a built-in spin from the start.



The study is published in <a href="https://academic.oup.com/mnras/article/538/1/76/8019798" target="_blank" rel="noreferrer noopener">Monthly Notices of the Royal Astronomical Society</a>.



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Is the universe spinning? Strange galaxy motion suggests that it is

Nearly a century ago, some astronomers proposed that we might...

Space is filled with breathtaking sights and hidden processes that shape stars and planets. One of these fascinating places is Lynds 483 (L483), a massive cloud of gas and dust where two young stars are forming.



The twin stars are growing, constantly changing, and shaping their surroundings. NASA’s <a href="https://science.nasa.gov/mission/webb/" target="_blank" rel="noreferrer noopener">James Webb Space Telescope</a> has captured an incredibly detailed image of their stellar nursery, giving us a rare chance to witness its evolution.



For thousands of years, the young <a href="https://www.earth.com/news/fluffy-molecular-clouds-may-change-our-understanding-of-star-formation/" target="_blank" rel="noreferrer noopener">stars</a> have been throwing out streams of material. These jets collide, spread, and form glowing patterns in space. 



What looks like twin flames in the image are actually energetic bursts from the forming stars, creating a scene that shifts and transforms over time.



<h2 class="wp-block-heading" id="h-intense-ejections-of-gas-and-dust">Intense ejections of gas and dust</h2>



Over time, the young stars have periodically expelled gas and dust into <a href="https://www.earth.com/news/planet-forming-disks-surrounding-stars-often-last-much-longer-than-expected/" target="_blank" rel="noreferrer noopener">space</a>. Some ejections emerge as tight, fast jets, while others spread more slowly. 



When the young stars throw out gas and dust, the new bursts crash into older ones that were already there. Since some areas are thicker and some are thinner, the material spreads in different ways, creating unique patterns in space.



These collisions also cause chemical reactions. The energy from the crashes makes atoms and molecules mix and change. 



This leads to the formation of new substances like carbon monoxide, methanol, and other organic molecules. These chemicals could later help in the formation of planets and other space objects.



After approximately a million years, the stars will complete their formation. The intense ejections will stop, and the luminous gas and dust structures will fade, leaving behind a much clearer scene.



<h2 class="wp-block-heading" id="h-thick-dust-hides-the-twin-stars">Thick dust hides the twin stars</h2>



At the heart of the image, a thin, vertical cloud forms an hourglass-like structure. The stars responsible for this dramatic display remain shrouded in an opaque disk of cold gas and dust. 



Surrounding this disk, where the dust is thinner, the stars' light escapes, illuminating the surrounding material in brilliant shades of orange, blue, and purple.



The contrast between illuminated and shadowed areas is striking. Some regions appear empty, but they actually contain dense clouds that block most of the starlight. 



In these areas, Webb's sensitive near-infrared camera has detected distant <a href="https://www.earth.com/image/messier-82-unlocking-the-mysteries-of-star-formation/" target="_blank" rel="noreferrer noopener">stars</a> as faint, orange pinpoints shining through the thick dust. Where the dust is less obstructive, stars appear in bright white and shades of blue.



<h2 class="wp-block-heading" id="h-stellar-jets-and-star-evolution">Stellar jets and star evolution</h2>



The stars' ejections have created complex and sometimes twisted structures. Toward the top right of the image, a prominent orange arc marks a shock front, where the expelled material has encountered denser gas, slowing its movement. 



Just below this arc, orange and pink regions intertwine, forming a tangled pattern that astronomers are eager to study further.



The lower section of the image appears denser, with thick gas and dust. Tiny purple pillars emerge from this region, pointing toward the central <a href="https://www.earth.com/news/stunning-images-of-baby-planets-reveal-surprising-growth-spurts/" target="_blank" rel="noreferrer noopener">stars</a>. These pillars have resisted the force of stellar winds because their material is dense enough to remain intact. 



Due to the sheer size of L483, the image only captures part of the lower section, with the upper regions fully visible.



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



Astronomers continue to piece together the history of these stellar ejections. By refining their models, they aim to explain the patterns of symmetry and asymmetry observed in the clouds. 



Researchers will also determine how much material the stars have expelled, identify the molecules formed through these collisions, and measure the density of different regions.



In the distant future, these twin stars may each reach a mass similar to our Sun. Their powerful outflows will have dispersed the surrounding material, leaving behind a small disk of gas and dust. This remnant may eventually give rise to planets, shaping the next chapter of this celestial story.



<h2 class="wp-block-heading" id="h-honoring-beverly-t-lynds">Honoring Beverly T. Lynds</h2>



L483 bears the name of American astronomer <a href="https://skyandtelescope.org/astronomy-news/beverly-turner-lynds-1929-2024/" target="_blank" rel="noreferrer noopener">Beverly T. Lynds</a>, whose meticulous work in the early 1960s mapped dense dust clouds where stars form. 



Her extensive catalogs of dark and bright nebulae provided essential resources for astronomers long before digital imaging and online databases became available.



Such contributions continue to guide modern research, enabling <a href="https://www.earth.com/news/star-formation-reignited-in-the-galaxy-leo-p-after-billions-of-years/" target="_blank" rel="noreferrer noopener">discoveries</a> like the stunning imagery captured by the James Webb Space Telescope.



Image Credit: NASA, ESA, CSA, STScI



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Webb reveals the fiery birth of twin stars in stunning detail

Space is filled with breathtaking sights and hidden processes that...

Scientists have been investigating how certain common medications might hold back the movement of cancer cells. Many years of observational research has hinted that daily low-dose aspirin use could curb the spread of certain cancers, including breast and prostate tumors, which caught the attention of clinicians.



One question lingered: how exactly does aspirin slow or stop this hidden process that sends <a href="https://www.earth.com/news/cancer-cells-collaborate-to-survive-challenging-conditions/" target="_blank" rel="noreferrer noopener">cancer</a> cells drifting around the body? Experts at the <a href="https://www.cam.ac.uk/" target="_blank" rel="noreferrer noopener">University of Cambridge</a> say they have found a critical clue.



<h2 class="wp-block-heading" id="h-cancer-spread-and-immune-defense">Cancer spread and immune defense</h2>



When a tumor stays in one spot, doctors often have a chance to remove or treat it. Trouble emerges when the cancer cells slip into the bloodstream and lodge in other areas, creating <a href="https://www.cancer.gov/types/metastatic-cancer" target="_blank" rel="noreferrer noopener">metastatic growths</a> that are much harder to manage.



Small, lone cancer cells traveling through the body might be more open to immune system attacks than large <a href="https://www.earth.com/news/video-games-could-accelerate-discoveries-in-cancer-research/" target="_blank" rel="noreferrer noopener">tumors</a>. The Cambridge team tested this idea by looking for the factors that shrink or boost immune defense.



Their work drew attention to thromboxane A2, often called TXA2, which is produced by platelets. The team showed that TXA2 triggers a pathway in <a href="https://www.cancer.gov/publications/dictionaries/cancer-terms/def/t-cell" target="_blank" rel="noreferrer noopener">T cells</a> involving a protein called ARHGEF1, limiting the ability of these T cells to attack cancer.



Aspirin blocks the enzyme that leads to the creation of TXA2. When TXA2 levels drop, T cells seem to have more energy to find and eliminate microscopic <a href="https://www.earth.com/news/our-lifetime-cancer-risk-may-be-established-before-we-are-born/" target="_blank" rel="noreferrer noopener">cancer threats</a>.



<h2 class="wp-block-heading" id="h-aspirin-boosts-immunity-against-cancer">Aspirin boosts immunity against cancer</h2>



“It was a Eureka moment when we found TXA2 was the molecular signal that activates this suppressive effect on T cells,” said Dr. Jie Yang, a researcher in the Department of Pathology.



The experts found that the protein ARHGEF1 makes T cells weaker, so they don’t fight cancer as well. When they stopped ARHGEF1 from doing this, the T cells stayed strong and attacked cancer more effectively. As a result, fewer cancer cells spread in the mice they tested.



In simple terms, the aspirin pathway stifles TXA2 production, which then allows T cells to keep doing their job without being put to sleep by that clotting factor. 



The researchers suspect that, in many people, this added boost could stand between remission and a devastating cancer comeback.



<h2 class="wp-block-heading" id="h-new-target-for-cancer-treatment">New target for cancer treatment </h2>



Rahul Roychoudhuri is a professor of cancer immunology and immunotherapy at the University of Cambridge. 



"Despite advances in <a href="https://www.earth.com/news/breakthrough-cancer-cells-have-a-molecular-switch-that-could-be-rewired-to-behave-normally/" target="_blank" rel="noreferrer noopener">cancer</a> treatment, many patients with early stage cancers receive treatments, such as surgical removal of the tumor, which have the potential to be curative," said Professor Roychoudhuri.



"We hope that therapies that target this window of vulnerability will have tremendous scope in preventing recurrence."



<h2 class="wp-block-heading" id="h-aspirin-s-potential-for-cancer-prevention">Aspirin’s potential for cancer prevention</h2>



Experts warn that aspirin is not without risks. A small portion of people can experience dangerous bleeding or <a href="https://www.nhs.uk/conditions/stomach-ulcer/" target="_blank" rel="noreferrer noopener">stomach ulcers</a>, so it is vital to speak with a doctor before making any changes to your routine.



On the bright side, the cost of low-dose aspirin is modest compared to many expensive antibody-based cancer drugs. Scientists believe this might mean broader global access if clinical trials confirm the results.



The <a href="https://www.addaspirintrial.org/" target="_blank" rel="noreferrer noopener">Add-Aspirin</a> clinical trial is investigating whether aspirin might keep some early tumors from returning. Scientists hope these new findings will guide them on how to personalize aspirin use and avoid giving it to people who will not benefit.



New <a href="https://www.nature.com/articles/s41571-018-0134-8" target="_blank" rel="noreferrer noopener">anti-metastatic</a> treatments could also be designed to target the TXA2 and ARHGEF1 pathway with more precision. This may ultimately become a useful strategy to reduce side effects and keep T cells motivated for the long run.



<h2 class="wp-block-heading" id="h-translating-findings-into-patient-care">Translating findings into patient care</h2>



Researchers agree that it is still early in the process, especially for establishing the safest dose or identifying who is likely to gain the most. But the potential payoff could be significant if these steps lead to lower rates of advanced <a href="https://www.earth.com/news/ai-is-the-next-frontier-in-cancer-treatment/" target="_blank" rel="noreferrer noopener">cancer</a> diagnoses.



Everything points to a greater role for the immune system in halting cancers before they get out of hand. Aspirin may enhance this defense, making it a key focus of cancer research.



The study is published in the journal <a href="https://www.nature.com/articles/s41586-025-08626-7" target="_blank" rel="noreferrer noopener">Nature</a>.



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Aspirin may prevent cancer from moving to other parts of the body

Scientists have been investigating how certain common medications might hold...

We don't give much thought to what happens to our eyes when we sleep. Our eyelids close, and the world around us recedes into darkness. But below those closed lids, a lot more is happening than you might think.



Researchers have found that the size of our pupils changes constantly while we sleep - sometimes expanding, sometimes contracting, and sometimes switching back and forth in a matter of seconds.



Researchers at <a href="https://ethz.ch/en.html" target="_blank" rel="noreferrer noopener">ETH Zurich</a> have been investigating these changes, and their research undermines a widely accepted assumption regarding sleep.



“These dynamics reflect the state of arousal, or the level of brain activation in regions that are responsible for sleep-wake regulation. These observations contradict the previous assumption that, essentially, the level of arousal during sleep is low," said Caroline Lustenberger, one of the researchers involved in the study.



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



Many assume that sleep is a low-energy state, but this study challenges that notion. The researchers found that even in resting states, our brains fluctuate between different levels of activation.



This is similar to what other studies have found in rodents, which also show slow shifts in activation levels while <a href="https://www.earth.com/news/humans-brains-can-subconsciously-respond-to-verbal-communication-while-sleeping/" target="_blank" rel="noreferrer noopener">asleep</a>.



To measure these changes, the scientists developed a new method for observing pupil movements in sleeping individuals. 



Since the brain regions that regulate activation levels are deep within the brainstem, they have been difficult to measure directly. 



Pupil size is known to reflect activation levels when we’re awake, so it serves as a useful marker for activity in these deep brain areas during different states of consciousness.



<h2 class="wp-block-heading" id="h-pupil-size-and-brain-activity">Pupil size and brain activity</h2>



Measuring <a href="https://www.earth.com/news/pupil-size-during-sleep-decides-if-new-or-old-memories-are-replayed/" target="_blank" rel="noreferrer noopener">pupil</a> movement in sleeping people is tricky - after all, our eyes naturally close when we drift off.



To address this, the researchers devised an unusual approach. They used a special adhesive technique with a transparent plaster to keep the test subjects’ <a href="https://www.earth.com/news/eyes-serve-as-an-early-warning-system-for-stroke-risk/" target="_blank" rel="noreferrer noopener">eyes</a> open for several hours while they slept.



“Our main concern was that the test subjects would be unable to sleep with their eyes open. But in a dark room, most people forget that their eyes are still open and they are able to sleep,” explained study lead author Manuel Carro Domínguez.



The data collected from these experiments showed a strong connection between <a href="https://www.earth.com/news/pupil-size-reveals-hidden-cognitive-fatigue/" target="_blank" rel="noreferrer noopener">pupil size</a> and different sleep stages. 



The researchers found that changes in pupil size corresponded with specific patterns of brain activity, such as sleep spindles and deep sleep waves - both of which play key roles in memory consolidation and sleep stability.



Interestingly, they also discovered that the brain’s response to sounds varies in intensity depending on the level of activation reflected in the pupil.



<h2 class="wp-block-heading" id="h-pupil-changes-and-brain-activity">Pupil changes and brain activity</h2>



One of the brain regions believed to regulate these changes is the locus coeruleus, a tiny area in the brainstem. In animals, this structure is known to help control <a href="https://www.earth.com/news/sleep-reboots-the-brain-making-room-for-new-memories/" target="_blank" rel="noreferrer noopener">sleep stages</a> and wakefulness.



While the researchers could not directly prove that the locus coeruleus is responsible for the pupil changes they observed, they suspect it plays a role.



“We are simply observing pupil changes that are related to the level of brain activation and heart activity,” said Lustenberger.



To investigate this further, the team plans to conduct follow-up studies using medication to influence the activity of the locus coeruleus. 



This will help them determine whether it directly controls pupil dynamics during sleep and how these shifts in activation impact sleep quality and function.



<h2 class="wp-block-heading" id="h-pupils-and-sleep-disorders">Pupils and sleep disorders</h2>



Beyond basic research, understanding how pupils change during sleep could have practical applications.



The researchers believe these findings could help in diagnosing and treating sleep disorders and other conditions linked to brain arousal dysfunctions.



The experts are particularly interested in whether pupil changes during sleep might indicate disorders such as insomnia, post-traumatic stress disorder, or even Alzheimer’s disease.



“These are just hypotheses that we want to investigate in the future,” said Lustenberger.



Another potential application is in hospital settings, where this method could be used to monitor wakefulness in coma patients or to improve the accuracy of sleep disorder diagnoses. 



By using the pupil as a “window” into brain activity, this approach could open new doors in sleep medicine and neuroscience.



The study highlights an important truth: sleep is far from a passive state. Even as we rest, our brains are busy regulating activity levels - something we can now see reflected in the ever-changing size of our pupils.



The full study was published in the journal <a href="https://www.nature.com/articles/s41467-025-57289-5" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Pupils reveal how active the brain is - even during sleep

We don't give much thought to what happens to our...

Earth has faced many climate challenges, but none compare to the catastrophe that unfolded 250 million years ago. The End-Permian Event (EPE) stands as the most severe extinction in history, wiping out more than 80% of marine species and devastating life on land. 



Scientists have extensively studied its effects on ocean ecosystems, but the impact of mass extinction on forests remains less clear.



A team of researchers from University College Cork (<a href="https://www.ucc.ie/en/" target="_blank" rel="noreferrer noopener">UCC</a>), the <a href="https://uconn.edu" target="_blank" rel="noreferrer noopener">University of Connecticut</a>, and the <a href="https://www.nhm-wien.ac.at" target="_blank" rel="noreferrer noopener">Natural History Museum</a> of Vienna has uncovered how plants responded to this crisis. 



Their findings reveal that ecosystem recovery was slow, complex, and shaped by extreme climate swings. 



By studying fossilized plants and rocks from the Sydney Basin in Australia, the team reconstructed a multi-million-year journey of forest <a href="https://www.earth.com/news/natures-climate-solutions-mixed-forests-store-more-carbon/" target="_blank" rel="noreferrer noopener">survival</a>, extinction, and eventual regrowth.



<h2 class="wp-block-heading" id="h-worst-mass-extinction-in-history">Worst mass extinction in history</h2>



The End-Permian Event, which occurred around 252.3 to 251.9 million years ago, caused the collapse of gymnosperm-supported ecosystems. 



Over 80% of ocean species vanished, making it the most severe mass extinction ever recorded. While its effects on marine life are well documented, its impact on land <a href="https://www.earth.com/news/forests-play-an-overlooked-role-in-the-climate-system/" target="_blank" rel="noreferrer noopener">ecosystems</a> has remained unclear.



Researchers examined fossilized plants and rocks from eastern Australia’s Sydney Basin, a region that was once located near the South Pole (∼70°S). 



Using sedimentology, biostratigraphy, and stable carbon isotope analysis, they traced the timing and sequence of gymnosperm reestablishment across different latitudes. 



The results of the analysis highlight the staggered nature of recovery, rather than a smooth, uninterrupted process.



<h2 class="wp-block-heading" id="h-cooler-temperatures-helped-forests-recover">Cooler temperatures helped forests recover</h2>



After the End-Permian Event, the first plants to return were peltasperm seed ferns. They managed to build stable ecosystems, holding on for about 200,000 years. 



But <a href="https://www.earth.com/news/forests-are-still-fighting-climate-change-against-all-odds/" target="_blank" rel="noreferrer noopener">nature</a> didn’t stand still. Over time, voltzialean conifers took over, spreading across the land and thriving for an impressive 1.5 million years.



Then, disaster struck again. Around 250.3 to 249.6 million years ago, global temperatures soared during the "Late Smithian Thermal Maximum."



The heat was too much for the conifer forests, and they collapsed. Their disappearance left space for a new kind of survivor - pleuromeian lycophytes. These plants were tough. They didn’t need much to grow, making them perfect for harsh conditions.



For 800,000 years, these small, shrubby plants dominated the land. But nothing lasts forever. 



As temperatures finally began to drop during the "Smithian-Spathian Event" around 249.6 to 249.2 million years ago, the environment shifted once again, opening the door for a new wave of plant life to reshape the world.



<h2 class="wp-block-heading" id="h-forests-recover-but-extinction-is-forever">Forests recover, but extinction is forever</h2>



The SSE brought much-needed relief to struggling <a href="https://www.earth.com/news/forests-rich-tree-diversity-adapt-better-changing-climate/" target="_blank" rel="noreferrer noopener">ecosystems</a>. 



As the climate cooled, a new kind of plant took over - umkomasialean seed ferns. These plants thrived and spread across the high-latitude forests of Gondwana, shaping the landscapes of the Middle and Late Triassic. They helped stabilize ecosystems that had been in chaos for millions of years.



But recovery didn’t happen the same way everywhere. In many parts of the world, pleuromeian lycophytes - a type of tough, shrubby plant - quickly spread after the End-Permian Event. However, in the polar south, this process was much slower.



It took around 1.7 million years for these plants to finally establish themselves. This delay reveals that recovery from mass extinction wasn’t simple or predictable. Some places rebounded faster than others, while some struggled for much longer.



Even though forests eventually grew dense again, they were not the same. The plants that filled these new <a href="https://www.earth.com/news/trees-are-relocating-in-a-race-against-global-warming/" target="_blank" rel="noreferrer noopener">ecosystems</a> were completely different from those that had dominated before the extinction. Nature rebuilt itself, but in a way no one could have expected.



“The term ‘recovery’ can be misleading. Forests recover eventually, but extinction is forever," said Dr. Chris Mays, leader of the Mass Extinction Group at University College Cork.



<h2 class="wp-block-heading" id="h-lessons-from-ancient-forest-extinction">Lessons from ancient forest extinction</h2>



Studying how ancient ecosystems recovered from extreme climate shifts gives us clues about what might happen to plants today. The way they adapted back then can help scientists predict how modern plant life will respond to environmental changes.



Plants do much more than just grow. They form the foundation of nature’s balance, providing food for animals and humans alike. 



They also help regulate the Earth's climate by absorbing carbon dioxide and producing oxygen. When plants thrive, ecosystems stay stable. When they struggle, the entire planet feels the impact.



“This research highlights how crucial plants are, not just as the base of land food chains, but also as natural carbon sinks that stabilize Earth’s climate,” explained UCC researcher Marcos Amores, the study’s lead author.



“The disruption of these systems can have impacts lasting hundreds of thousands of years, so protecting today’s <a href="https://www.earth.com/news/forests-face-rising-damage-risks-as-their-diversity-dwindles/" target="_blank" rel="noreferrer noopener">ecosystems</a> is more important than ever.”



Earth’s past reveals a clear lesson: nature can recover, but it takes time. The resilience of plant life has shaped the world we know today, making conservation efforts essential for the future of our ecosystems.



The study is published in the journal <a href="https://pubs.geoscienceworld.org/gsa/gsabulletin/article-abstract/doi/10.1130/B38017.1/652555/Age-controlled-south-polar-floral-trends-show-a?redirectedFrom=fulltext" target="_blank" rel="noreferrer noopener">Geological Society of America Bulletin</a>.



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How forests rose again after the planet’s most extreme extinction

Earth has faced many climate challenges, but none compare to...

Smokers and e-cigarette advocates often believe that vaping helps people to quit the use of tobacco. However, new research provides strong evidence contradicting this belief, challenging the widely held assumption.



The research was conducted by a team of scientists at the Herbert Wertheim School of Public Health and Human Longevity Science, and at Moores Cancer Center at the <a href="https://ucsd.edu/" target="_blank" rel="noreferrer noopener">University of California, San Diego</a>.



Their significant results have recently been published in the Journal of the American Medical Association (JAMA).



<h2 class="wp-block-heading" id="h-vaping-vs-smoking">Vaping vs. smoking</h2>



“Most smokers think vaping will help you quit <a href="https://www.earth.com/news/quitting-smoking-at-any-age-brings-big-and-immediate-health-benefits/" target="_blank" rel="noreferrer noopener">smoking</a>,” stated John P. Pierce, Ph.D., Distinguished Professor in the Herbert Wertheim School of Public Health (<a href="https://hwsph.ucsd.edu/" target="_blank" rel="noreferrer noopener">HWSPH</a>), and one of the study's co-authors.



“However, this belief is not supported by science to date. While some researchers have suggested that smokers who switch to daily vaping will be more successful in quitting smoking, we studied quitting success among both daily and non-daily vapers and came up with a quite definitive answer.”



More than 6,000 U.S. smokers took part in the study, of which 943 were also smokers who vaped.



One striking finding from this study was that quitting smoking was less successful among vapers than among <a href="https://www.earth.com/news/smokers-have-weaker-hearts-that-pump-less-blood/" target="_blank" rel="noreferrer noopener">smokers</a> who didn't vape. 



Daily vape users were 4.1% less successful at quitting smoking, and occasional vape users were 5.3% less successful.



<h2 class="wp-block-heading" id="h-misleading-perception-of-vaping">Misleading perception of vaping</h2>



The Centers for Disease Control and Prevention (CDC) states that close to one out of every five Americans consumes <a href="https://www.earth.com/news/tobacco-bans-could-help-prevent-1-2-million-lung-cancer-deaths/" target="_blank" rel="noreferrer noopener">tobacco</a> products. 



Most tobacco consumers are cigarette smokers although, in recent times, there has been a shift towards vaping, mostly because people feel that it is safer than smoking cigarettes.



This perception of safety reinforces the illusion that vaping can aid a smoker to get weaned off <a href="https://www.earth.com/news/smoking-cigarettes-accelerates-aging/" target="_blank" rel="noreferrer noopener">cigarettes</a>.



Interestingly, researchers took note of the potential dangers of vaping, and asserted that e-cigarettes are not benign.



“The adverse health effects of cigarette smoking become obvious after people have smoked for 20 years. While vapes generally don’t contain the same harmful chemicals as cigarette smoke, they have other risks, and we just don’t yet know what the health consequences of vaping over 20 to 30 years will be,” shared Pierce.



<h2 class="wp-block-heading" id="h-smoking-and-vaping-definitive-study">Smoking and vaping - definitive study</h2>



One particular strength of the research is its capacity to adjust for a large number of variables that are understood to impact the cessation of smoking.



The scientists carefully controlled for variables such as smoking frequency, levels of interest in quitting, having a smoke-free household, and socioeconomic status.



This way, they were able to ensure that what they found wasn't confounded by outside factors, and therefore the conclusions drawn would be stronger.



“For example, if a smoker is already very interested in quitting, has a smoke-free home, and does not smoke daily, they are much more likely to successfully quit, regardless of whether they vape or not,” said senior author Karen Messer, Ph.D., professor of biostatistics at the Herbert Wertheim School of Public Health.



“We matched each smoker/vaper on such characteristics. You have to make very sure you’re comparing like with like, and that’s why this analysis is so definitive.”



According to the researchers, previous studies that failed to account for these confounding factors have contributed to the persistent misconception that vaping aids smoking cessation. 



<h2 class="wp-block-heading" id="h-informing-public-health-policy">Informing public health policy</h2>



The findings also have significant implications for public health policy, particularly in connection with the marketing of <a href="https://www.earth.com/news/e-cigarettes-linked-to-increased-risk-of-heart-failure/" target="_blank" rel="noreferrer noopener">e-cigarettes</a>.



Young people are often the target of marketing campaigns and may find themselves using e-cigarettes as a stepping stone to nicotine addiction.



“There’s still a lot we don’t know about the impact of vaping on people,” commented Natalie Quach, &nbsp;a third-year&nbsp;biostatistics Ph.D.&nbsp;student at the Herbert Wertheim School of Public Health, and the study’s first author.



“But what we do know is that the idea that vaping helps people quit isn’t actually true. It is more likely that it keeps them addicted to nicotine.”



Messer emphasized the importance of rigorous research in shaping public health strategies. 



“As the public health community continues to grapple with the complexities of tobacco control, it is essential that we rely on rigorous scientific evidence to inform our policies and interventions,” she stated.



“Our research shows that misleading associations between vaping and smoking cessation routinely occur unless confounding characteristics are carefully accounted for.”



<h2 class="wp-block-heading" id="h-why-this-study-matters">Why this study matters</h2>



These findings highlight the importance of evidence-based policymaking, particularly as e-cigarette use continues to increase.



Without careful consideration of the full range of influences on smoking behavior, the public may continue to be misled about the role of vaping in tobacco cessation.



The full study was published in the <a href="https://jamanetwork.com/journals/jamanetworkopen/fullarticle/2831011" target="_blank" rel="noreferrer noopener">JAMA</a>.



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Does vaping help people stop smoking cigarettes? New study has answers

Smokers and e-cigarette advocates often believe that vaping helps people...

Meandering,Bends,Of,The,Lower,Padma,River.,The,Lower,Portion

Rivers, lava, and ice carve through landscapes in twisting, meandering channels. At first glance, their bends appear similar. 



However, a recent study from researchers at <a href="https://www.utexas.edu" target="_blank" rel="noreferrer noopener">The University of Texas</a> at Austin reveals that rivers form curves differently than lava or ice channels.



The exact forces shaping these channels remain unclear. However, past research suggests that the interaction between the fluid and the surrounding terrain plays a crucial role. 



This study builds on those ideas by analyzing thousands of bends formed by different <a href="https://www.earth.com/news/shanay-timpishka-river-amazon-rainforest-is-so-hot-that-it-literally-boils-destroying-nearby-biodiversity/" target="_blank" rel="noreferrer noopener">natural processes</a>.



<h2 class="wp-block-heading" id="h-science-behind-the-river-bends">Science behind the river bends</h2>



In <a href="https://www.earth.com/news/what-amount-of-water-do-earths-rivers-hold/" target="_blank" rel="noreferrer noopener">rivers</a>, centrifugal force plays a major role. Water moves faster along the outer edges of a curve and slows down along the inner edges. 



This causes erosion on the outer banks while depositing sediment on the inner banks, which gradually intensifies the bends.



Volcanic and ice channels, however, behave differently. These channels erode through melting rather than by carrying and depositing sediments. 



Because of this, erosion occurs mainly on the outer edge of a bend, resulting in smaller curves when compared to rivers.



“This distinction sets up a great natural experiment for us to see if the shape, or size, of bends in rivers is distinct from those in volcanic or ice channels,” said Tim Goudge, a co-author on the study and an assistant professor at the <a href="https://www.jsg.utexas.edu" target="_blank" rel="noreferrer noopener">Jackson School of Geosciences</a>, Department of Earth and Planetary Sciences.



<h2 class="wp-block-heading" id="h-implications-beyond-earth">Implications beyond Earth</h2>



This research could help scientists analyze sinuous <a href="https://www.earth.com/news/atmospheric-rivers-are-shifting-with-global-climate-impacts/" target="_blank" rel="noreferrer noopener">channels</a> on other planets and moons, where the origin of fluids remains uncertain. Without direct access to these channels, their shapes may provide clues about their formation.



The study, published in Geology, was led by Juan Vazquez, who completed his undergraduate degree at the Jackson School in 2024. 



He worked alongside Goudge to analyze thousands of bends in rivers on Earth, volcanic channels on the Moon, and ice channels on glaciers.



Vazquez initially believed he had made an error when analyzing the data. However, he soon realized that river bends were significantly more extreme than those of lava and ice.



“It wasn’t until the parameters for the code we had set for the volcanic channels on the Moon kept failing for the rivers on Earth that we realized, ‘Oh, that’s not a fault of the code. It’s an intrinsically different amplitude,’” Vazquez related.



<h2 class="wp-block-heading" id="h-identifying-channel-origins">Identifying channel origins</h2>



The study also found that volcanic and ice channels tend to have a higher proportion of downstream-accentuated bends compared to rivers. 



This pattern could help distinguish different types of <a href="https://www.earth.com/news/planning-for-an-uncertain-future-in-the-colorado-river-basin/" target="_blank" rel="noreferrer noopener">channels</a> on planetary bodies like Titan, Saturn’s largest moon.



On Earth, scientists can observe the fluids or study geological evidence to determine a channel’s origin. 



However, on Titan, liquid ethane and methane carve through ice, making it difficult to determine whether channels form like rivers or through melting and dissolution.



Mars presents a similar challenge. Several billion years ago, the planet had flowing rivers and active volcanoes. 



Today, sinuous channels appear on the sides of Martian volcanoes. Some scientists believe these formed from lava, while others argue that melting snow created them.



“There are these sinuous channels on the sides of Martian volcanos. Some people have interpreted them as volcanic channels, and some people have interpreted them as rivers that formed when maybe snowpack on the top of the volcano melted,” said Goudge. 



“We’re saying that because volcanic channel bends are so distinct, you can measure those channels to find out.”



<h2 class="wp-block-heading" id="h-future-research-on-river-bend-patterns">Future research on river bend patterns</h2>



Goudge cautions that this research should not be seen as a strict rule for identifying the origin of <a href="https://www.earth.com/news/international-day-of-action-for-rivers-lifelines-of-our-planet/" target="_blank" rel="noreferrer noopener">channels</a>. 



Natural channels, whether formed by rivers, lava, or ice, can vary widely due to different environmental conditions. Because of this variability, the method may not always provide clear answers.



Before scientists can confidently use these findings to determine whether a channel was created by water, lava, or ice, more data needs to be collected. 



Further studies and analysis of additional channels are necessary to confirm the reliability of this approach.



By refining this research, scientists may unlock a new way to study planetary surfaces, helping them to decode the histories of distant worlds.



The study is published in the journal <a href="https://pubs.geoscienceworld.org/gsa/geology/article-abstract/doi/10.1130/G52706.1/652506/Upstream-bend-skewing-in-alluvial-meandering?redirectedFrom=fulltext" target="_blank" rel="noreferrer noopener">Geology</a>.



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Discovery about Earth's rivers could help us find water on other planets

Rivers, lava, and ice carve through landscapes in twisting, meandering...

The Kuiper belt, a distant region of icy bodies beyond Neptune, is home to many celestial wonders. Among them, one particular trio of space rocks has recently caught the attention of scientists.



Cosmic systems involving three orbiting bodies have always challenged astronomers as it is difficult to predict the paths of the three gravitationally bound objects. 



Interactions between the gravitational fields of the three bodies tend to lead to chaotic dynamics, which has given rise to the "<a href="https://www.earth.com/news/finding-order-in-the-chaos-of-the-three-body-problem/" target="_blank" rel="noreferrer noopener">three-body problem</a>."



The discovery that a previously identified binary system in the Kuiper belt may actually involve three bodies could reshape our understanding of how objects in the Kuiper belt form and evolve.



The research team that have identified the system claim to have found a stable group of three bodies, which is highly unusual but not entirely unheard of. This would marking a significant breakthrough in planetary science.



<h2 class="wp-block-heading" id="h-what-astronomers-found">What astronomers found</h2>



Researchers from the <a href="https://www.byu.edu/" target="_blank" rel="noreferrer noopener">Brigham Young University</a> in Provo, Utah, believe they've uncovered the second trio of space rocks ever identified in the Kuiper belt. 



If verified, this suggest that there may be other three body systems present. It adds credence to a unique theory on the history of our solar system and the formation of Kuiper belt objects (KBOs).



"The universe is filled with a range of three-body systems, including the closest stars to Earth, the Alpha Centauri star system, and we're finding that the Kuiper belt may be no exception," says the study's lead author, Maia Nelsen, a physics and astronomy graduate of BYU.



<h2 class="wp-block-heading" id="h-what-are-kuiper-belt-objects">What are Kuiper Belt objects?</h2>



Catalogued in 1992, KBOs are primordial icy remains from the very beginnings of our solar system. The belt where these objects are found lies well beyond Neptune's orbit.



To date, scientists have recorded over 3,000 KBOs and predict a possible number in the hundreds of thousands if they include those bigger than 10 miles (16 kilometers) in diameter.



Dwarf planet <a href="https://www.earth.com/news/pluto-may-not-be-real-planet-but-has-real-big-ocean/" target="_blank" rel="noreferrer noopener">Pluto</a> ranks as the biggest KBO.



<h2 class="wp-block-heading" id="h-formation-of-kuiper-belt-objects">Formation of Kuiper belt objects</h2>



The new Hubble breakthrough offers key insights into a <a href="https://www.earth.com/news/space-snowman-arrokoth-celestial-objects-become-ice-bombs/" target="_blank" rel="noreferrer noopener">KBO formation</a> theory in which the three small, rocky bodies would not have formed as the result of collision in the busy Kuiper belt, but rather from the gravitational collapse of matter in the disk of material surrounding the newly formed Sun.



This likely happened around 4.5 billion years ago.



By comparison, stars are known to form by the gravitational collapse of gas, often in pairs or triples. 



The notion that celestial bodies in the Kuiper belt form similarly is a fascinating concept that is currently under review.



<h2 class="wp-block-heading" id="h-insights-into-the-altjira-system">Insights into the Altjira system</h2>



Located in the outer realms of our solar system, some 44 times the distance between Earth and the Sun, the Altjira System is the subject of this compelling research. 



Though two KBOs were seen in Hubble images of this system, scientists now believe the inner object is, in fact, a pair of bodies that appears as one due to their close proximity and their great distance from observers on Earth. 



The scientists explain that differentiating the two tiny bodies at such a great distance requires non-imaging methods. 



The team monitored the Altjira system over a 17-year period, observing the unique co-orbital movement of the outer object. Over time, they noticed subtle shift in orbit that was not expected.



<h2 class="wp-block-heading" id="h-multiple-hypotheses-for-the-altjira-system">Multiple hypotheses for the Altjira system</h2>



In analyzing the Hubble footage, the team found that the strongest evidence supported the idea of a triple system.



They also considered that the inner object could be a contact binary (two separate bodies so close that they touch each other) or an irregularly flat object reminiscent of a pancake.



Currently, the researchers estimate there are around 40 <a href="https://www.earth.com/news/mors-somnus-provides-clues-neptune-evolution/" target="_blank" rel="noreferrer noopener">binary objects</a> in the Kuiper belt.



With the discovery of a potential second triple system, it is possible that these systems are not single eccentricities but rather examples of an entire population of three-body systems formed under similar conditions.



Historically, the only KBOs studied in detail are Pluto and the smaller object Arrokoth, which were explored by NASA's New Horizons missions in 2015 and 2019, respectively.



Arrokoth is a contact binary, a pair of objects that have moved ever closer to each other and assumed a peanut shape.



<h2 class="wp-block-heading" id="h-what-happens-next">What happens next?</h2>



The team describes Altjira as a close relative of Arrokoth, as it hails from the same Kuiper belt group.



They estimate Altjira to be approximately ten times larger though, with a diameter of 124 miles (200 kilometers).



Even though there's no planned mission to see Altjira as closely as Arrokoth was observed, the researchers gleefully await an upcoming opportunity for further study. 



Over the next decade, they will get the chance to observe the outer body passing in front of the central body, which will give them a chance to learn more about this intriguing system and other aspects of the <a href="http://arth.com/news/webb-telescope-confirms-hubble-constant-our-understanding-of-universe-expansion-very-wrong/">universe</a>



In addition, NASA’s James Webb Space Telescope will join the study in its upcoming Cycle 3 observations, and it will add new evidence about these three frosted cosmic bodies.



The study was published in <a href="https://iopscience.iop.org/article/10.3847/PSJ/ad864d">The Planetary Science Journal</a>.



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'Streaming instability' hypothesis: What is it and how is Hubble involved?

The Kuiper belt, a distant region of icy bodies beyond...

For centuries, Mars has captivated human curiosity, from early astronomers to modern scientists. The Red Planet remains a source of mystery, and with the possibility of human exploration on the horizon, understanding its environment is more crucial than ever.



While its mountains and valleys get much attention, the atmosphere of Mars is just as interesting and complex.



Recent research, including contributions from the <a href="https://www.u-tokyo.ac.jp/en/" target="_blank" rel="noreferrer noopener">University of Tokyo</a>, has shed new light on how Mars' atmosphere behaves. Scientists have discovered that atmospheric gravity waves play a crucial role in shaping latitudinal air currents, particularly in the middle and upper layers of the planet’s atmosphere.



This discovery helps us understand <a href="https://www.earth.com/news/nasa-seeks-a-faster-way-to-bring-mars-samples-to-earth/" target="_blank" rel="noreferrer noopener">Mars</a>' weather better and may also improve climate predictions on Earth.



<h2 class="wp-block-heading" id="h-behavior-of-mars-atmosphere">Behavior of Mars' atmosphere </h2>



To grasp the significance of these findings, it is important to understand how Mars' atmosphere differs from our own. 



Earth has a thick atmosphere full of nitrogen and oxygen, making it suitable for life. <a href="https://www.earth.com/news/detecting-life-on-mars-a-breakthrough-in-space-research/" target="_blank" rel="noreferrer noopener">Mars</a>, on the other hand, has very thin air, mostly made of carbon dioxide. This major difference causes Mars' atmosphere to behave in unique ways.



Even though they are different, both planets have air movements caused by their rotation and heat from the Sun. 



"On Earth, large-scale atmospheric waves caused by the planet’s rotation, known as Rossby waves, are the primary influence on the way air circulates in the stratosphere, or the lower part of the middle atmosphere," said Professor Kaoru Sato from the Department of Earth and Planetary Science. 



"But our study shows that on Mars, gravity waves (GWs) have a dominant effect at the mid and high latitudes of the middle atmosphere."



“Rossby waves are large-scale atmospheric waves, or resolved waves, whereas GWs are unresolved waves, meaning they are too fine to be directly measured or modeled and must be estimated by more indirect means.”



<h2 class="wp-block-heading" id="h-what-are-gravity-waves">What are gravity waves?</h2>



Gravity waves are a type of movement in the air. They happen when air moves up and down like waves in the ocean because of differences in air pressure and buoyancy. These waves are different from gravitational waves, which come from space events like black hole collisions.



Since gravity waves are small and hard to see directly, scientists have struggled to measure their effects in Mars' atmosphere. 



To solve this problem, Professor Sato and her team used a special dataset called the Ensemble Mars Atmosphere Reanalysis System (<a href="https://www.datacommons.psu.edu/download/meteorology/greybush/emars-1p0/a_landing_page.html#:~:text=EMARS%20uses%20the%20Local%20Ensemble,Sounder%20(MCS)%20temperature%20retrievals." target="_blank" rel="noreferrer noopener">EMARS</a>). This dataset combines information collected from spacecraft over many years, helping researchers study how these waves influence Mars’ weather and climate.



<h2 class="wp-block-heading" id="h-new-perspective-on-mars-atmosphere">New perspective on Mars' atmosphere</h2>



The study revealed that gravity waves transport angular momentum rapidly, affecting north-south circulation patterns in Mars’ middle atmosphere.



"We found something interesting, that GWs facilitate the rapid vertical transfer of angular momentum, significantly influencing the meridional, or north-south, in the middle atmosphere circulations on Mars," said graduate student Anzu Asumi. 



"It’s interesting because it more closely resembles the behavior seen in Earth’s mesosphere rather than in our stratosphere. This suggests existing <a href="https://www.earth.com/news/nasa-collects-26th-rock-sample-on-mars-plans-to-bring-them-all-to-earth-for-study/" target="_blank" rel="noreferrer noopener">Martian</a> atmospheric circulation models may need to be refined to better incorporate these wave effects, potentially improving future climate and weather simulations."



This discovery challenges previous assumptions about <a href="https://www.earth.com/news/wave-ripples-discovered-mars-surface-indicate-liquid-water-present-4-billion-years-ago/" target="_blank" rel="noreferrer noopener">Mars</a>’ atmospheric circulation and highlights the need for updated models. If researchers can refine simulations based on these findings, future climate predictions for Mars will be more accurate.



<h2 class="wp-block-heading" id="h-improving-weather-predictions-on-earth">Improving weather predictions on Earth</h2>



Studying Mars helps scientists learn more about how <a href="https://www.earth.com/news/new-year-on-mars-avalanches-icy-explosions-and-the-arrival-of-spring/" target="_blank" rel="noreferrer noopener">weather</a> works on different planets. 



Mars and Earth have some similarities, like how fast they spin and how they tilt as they orbit the Sun. These similarities make Mars a useful place to study how atmospheres behave.



However, Mars is also very different. Its air is much thinner than Earth's and mostly made of carbon dioxide. It also has extreme seasons that change the planet’s weather in unusual ways. These differences give scientists a chance to see how various factors shape a planet’s climate.



By comparing Mars and Earth, researchers can improve their understanding of how atmospheres work in general. This knowledge might even help improve weather predictions and climate models for Earth. 



As scientists develop better ways to study planetary weather, their findings could be useful for both space exploration and life on our own planet.



<h2 class="wp-block-heading" id="h-exploring-the-role-of-dust-storms">Exploring the role of dust storms</h2>



“Looking ahead, we plan to investigate the impact of <a href="https://www.earth.com/news/did-mars-once-host-life-we-finally-know-where-to-look/" target="_blank" rel="noreferrer noopener">Martian</a> dust storms on atmospheric circulation. So far, our analysis has focused on years without major dust storms,” said Sato. 



“However, these storms dramatically alter atmospheric conditions, and we suspect they may intensify the role of GWs in circulation. Our research lays the groundwork for forecasting Martian weather, which will be essential for ensuring the success of future Mars missions."



Future studies will examine how these storms on Mars reshape global atmospheric patterns. If scientists can predict these changes with precision, mission planners will be able to prepare astronauts for the planet’s extreme weather. 



With each new breakthrough, the dream of reliable <a href="https://www.earth.com/news/mars-has-spectacular-glowing-clouds-at-sunset/" target="_blank" rel="noreferrer noopener">Martian</a> weather forecasting moves closer to reality.



The study is published in the <a href="https://doi.org/10.1029/2023JE008137" target="_blank" rel="noreferrer noopener">Journal of Geophysical Research Planets</a>.



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Secrets of Mars' atmosphere may improve weather predictions

For centuries, Mars has captivated human curiosity, from early astronomers...

Blood,Moon,-,This,Is,A,Photo,Of,The,Moon

March’s night sky is alive with motion - planets shift, the Moon changes, and Mercury makes a fleeting appearance before disappearing again. 



Whether or not you're an avid <a href="https://www.earth.com/news/january-2025-stargazing-a-parade-of-bright-planets/" target="_blank" rel="noreferrer noopener">stargazer</a>, March has something extraordinary in store. Some of this month's astronomical events will last weeks - others just minutes. 



With skywatching tips from <a href="https://science.nasa.gov/solar-system/skywatching/whats-up-march-2025-skywatching-tips-from-nasa/" target="_blank" rel="noreferrer noopener">NASA</a>, you'll know just what to look for.



The universe keeps changing, whether we watch or not. But if you do take the time, March's night sky will reward you.



<h2 class="wp-block-heading" id="h-mercury-at-sunset">Mercury at sunset</h2>



<a href="https://www.earth.com/news/bepicolombo-spacecraft-captures-high-definition-images-of-mercury-during-close-flyby/" target="_blank" rel="noreferrer noopener">Mercury</a> is a tricky planet to see because it stays close to the Sun. Most of the time, the Sun's brightness hides it, making it one of the hardest planets to spot without a telescope. 



However, for a few days in early March, you have a rare chance to see it with your own eyes.



To find Mercury, look towards the western sky about 30 minutes after sunset. It will appear as a tiny bright dot just below <a href="https://www.earth.com/news/venus-was-never-capable-of-supporting-life-as-we-know-it/" target="_blank" rel="noreferrer noopener">Venus</a>. 



But don’t wait too long - each night, Mercury moves lower and gets harder to see. By mid-March, it will sink into the Sun’s glare and won’t be visible for months in the night sky.



For the best view, go to a place with a clear horizon, like a beach, an open field, or a hilltop. Trees, buildings, and city lights can block your view, making it even harder to spot. 



If you do manage to see Mercury before it disappears, enjoy the moment - because it won’t last long.



<h2 class="wp-block-heading" id="h-the-planetary-shuffle">The planetary shuffle</h2>



While Mercury will be tricky to spot, the other planets will have their own stories to tell in March’s night sky.



Venus, the unmistakable “evening star,” will start the month low in the western sky. But its time will be short. Venus will sink lower each night and by mid-March, it will be gone.



Mars, however, will hold its ground. High in the east after sunset, it will linger late into the night, not setting until around 3 a.m. If you stay up past midnight, you will still see its reddish glow overhead.



Jupiter, the giant of our solar system, will dominate the western <a href="https://www.earth.com/news/four-planets-will-align-this-week-during-a-rare-nighttime-spectacle-heres-how-to-see-them/" target="_blank" rel="noreferrer noopener">sky</a> once night falls. Its bright, steady light will make it one of the easiest planets to spot, even in light-polluted areas.



But like Venus, it will eventually fade, setting around 1 a.m. And when that happens, the morning sky will be planet-free for the first time in a year.



<h2 class="wp-block-heading" id="h-blood-red-moon-in-the-march-sky">Blood-red Moon in the March sky</h2>



And then, there’s the main event - the total lunar eclipse on the <a href="https://www.earth.com/news/venus-mars-and-bodes-galaxy-will-light-up-februarys-night-sky/" target="_blank" rel="noreferrer noopener">night</a> of March 13th into the 14th.



Unlike a solar eclipse, which requires protective eyewear, this event is safe to watch with your own eyes. No equipment is needed - just step outside, find the Moon, and enjoy the show.



At first, you’ll notice a shadow creeping across its surface, like a slow-moving bite taken out of a cookie. As the eclipse deepens, the Moon won’t vanish - it will turn an eerie, deep red. This crimson is the Earth’s atmosphere at work.



If you were standing on the Moon during the eclipse, you’d see something incredible - a fiery ring around Earth, made up of all the sunrises and sunsets happening at that moment.



That reddish light bends through Earth’s air and spills onto the Moon, giving it the signature blood-red hue.



Then, just as it appeared, the shadow slowly retreats. The deep red hue fades, the darkened edge shrinks, and the Moon regains its usual glow. 



Another cycle ends, and another celestial event is etched into the ever-changing story of March's night sky.



<h2 class="wp-block-heading" id="h-what-s-on-the-dark-side-of-the-moon">What’s on the dark side of the Moon?</h2>



The phrase “dark side of the Moon” is a bit misleading. It makes it sound like there’s a half of the Moon that never sees sunlight - an eternal night locked in place. But that’s not the case.



The Moon does have a far side, the part we never see from Earth. This happens because it’s tidally locked, meaning one side always faces us. 



But just like Earth, the Moon rotates. Every part of its surface gets bathed in sunlight at some point. There’s no permanent darkness, only the changing light of the lunar day.



The far side of the Moon only faces Earth when the Moon is new. That’s when the Moon is positioned between us and the Sun - so close to the Sun’s light that we can’t see it at all. Unless, of course, there’s a solar eclipse.



<h2 class="wp-block-heading" id="h-optimal-view-of-march-s-night-sky">Optimal view of March's night sky</h2>



March 29th marks the new moon - a night of darkness, and a golden opportunity for stargazers.



Without the Moon’s glare washing out the sky, faint celestial objects suddenly become visible. The Milky Way stretches across the heavens. Distant galaxies, usually hidden, start to emerge. 



<a href="https://esahubble.org/wordbank/nebula/" target="_blank" rel="noreferrer noopener">Nebulae</a>, those swirling clouds of cosmic dust and gas, become easier to photograph.



If you own a telescope, now’s the time to use it. If you don’t, all you really need is a clear, dark sky. Find a spot far from city lights and let your eyes adjust. 



March reminds us that the sky is always changing. Mercury appears briefly, then vanishes.



Venus fades away, followed by Jupiter. The Moon transforms into a deep red during the eclipse, only to return to its usual glow. And with the new moon, the night sky reveals sights you may have never noticed before.



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March 2025 stargazing: A red moon and a vanishing planet

March’s night sky is alive with motion - planets shift,...

Scientists are transforming chocolate into a functional food by infusing it with probiotics and prebiotics, aiming to create a treat that satisfies cravings while supporting gut health. 



The challenge lies in maintaining chocolate's beloved texture and flavor while adding health benefits.



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Probiotics - beneficial microbes that balance gut bacteria and aid digestion - are typically fragile and can be destroyed by stomach acid or processing. 



Prebiotics act as food for these microbes, helping them thrive. Together, they form "synbiotics," a powerful health combination.



Researchers Smriti Gaur and Shubhi Singh from India's Jaypee Institute of Information Technology took an innovative approach, using natural prebiotics like corn and honey instead of complex processing methods. 



They created five chocolate varieties: a control and four synbiotic versions containing different combinations of prebiotics, probiotics (Lactobacillus strains), and flavor enhancers (cinnamon or orange).



Laboratory simulations of human digestion showed the probiotics remained viable for over five hours, suggesting they could survive long enough to benefit gut health.



Taste tests were positive, with researchers particularly enjoying the orange-flavored variety, describing it as having "vibrant citrus notes" complementing the "rich cocoa" with a "luxurious" texture.



This research represents just the beginning. With further refinement of strains, textures, and flavors, chocolate could evolve beyond mere indulgence to become a functional food that nourishes while it delights.



The study is published in the journal <a href="https://pubs.acs.org/doi/10.1021/acsfoodscitech.4c00741" target="_blank" rel="noreferrer noopener">ACS Food Science &amp; Technology</a>.

Is chocolate the next nutritional powerhouse?

Scientists are transforming chocolate into a functional food by infusing...

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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



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

Flu viruses are more flexible than expected

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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



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

Designing crops that can beat the heat

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Today’s Video of the Day from the <a href="https://www.acs.org/">American Chemical Society</a> explores the ability of salt to transform the way that foods and beverages taste. Salt is known to cover up undesirable flavors, such as bitterness in coffee or beer, but how exactly does sodium chloride change the taste of other compounds?



One previous study showed that, not only does salt suppress bitterness, but also enhances sweetness and sourness. Another study revealed that bitterness reduction by salt seems to be happening at the tongue receptor level as well as in the brain.&nbsp;



While it is known that salt taste is mediated by the presence of sodium channels in the form of taste buds, experts believe that there is also an unknown receptor responsible for how we taste salt that has not yet been identified.&nbsp;



Video Credit: ACS Reactions



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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.

How does salt makes things taste better?

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Santiago, the capital city of Chile. The city is located in the center of the Santiago Metropolitan Region, which has a population of about eight million people.&nbsp;



'The weather of Santiago resembles the Mediterranean climate with dry and warm summers with temperatures reaching up to 35°C (from October to March) and cool and humid winters that can drop to 0°C (from April to September)."



"The city lies in the centre of the country’s central valley around 80 km from the Pacific Ocean to the west and borders Argentina to the east. A tiny part of Argentina is visible in the top-right corner of the image where the mountain crest of the Andes Mountains acts as a divider between the two countries," says ESA.



Video/ Image Credit: ESA



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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.

Santiago, Chile in South America

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Spiral,Galaxy,,Illustration,Of,Milky,Way

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Astronomers at <a href="https://www.jhu.edu/">Johns Hopkins University</a> have created an interactive map of the universe, including the actual position and real colors of 200,000 galaxies. The map allows the public to access data that was previously only available to scientists.



The map was developed using data collected by the Sloan Digital Sky Survey. For over two decades, a telescope in New Mexico was aimed at slightly different locations to capture the night sky.&nbsp;



"Growing up I was very inspired by astronomy pictures, stars, nebulae and galaxies, and now it's our time to create a new type of picture to inspire people," said map creator Brice Ménard, a professor at Johns Hopkins. "Astrophysicists around the world have been analyzing this data for years, leading to thousands of scientific papers and discoveries. But nobody took the time to create a map that is beautiful, scientifically accurate, and accessible to people who are not scientists. Our goal here is to show everybody what the universe really looks like."



"In this map, we are just a speck at the very bottom, just one pixel. And when I say we, I mean our galaxy, the Milky Way which has billions of stars and planets. We are used to seeing astronomical pictures showing one galaxy here, one galaxy there or perhaps a group of galaxies. But what this map shows is a very, very different scale."



"From this speck at the bottom, we are able to map out galaxies across the entire universe, and that says something about the power of science."



The <a href="https://mapoftheuniverse.net/">interactive map</a> is available online, where it can be downloaded for free.



Video Credit: Johns Hopkins&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.

Interactive map of the universe includes 200,000 galaxies

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Today's Video of the Day from <a href="https://www.nasa.gov/goddard">NASA Goddard</a> describes the first comprehensive estimate of carbon density in the Saharan, Sahel, and Sudanian zones of Africa. In an effort to measure the amount of carbon stored across these drylands, a team of scientists used high-resolution satellite images and artificial intelligence to map nearly 10 billion individual trees. 



"The high spatial resolution (50 cm) combined with AI and field measurements used in this study is key to improving tree inventories in drylands," said Pierre Hiernaux, a French researcher working for NASA. "The ever-increasing availability of very high-resolution satellite imagery will make it possible to assess carbon pools and their dynamics at the individual tree level on a global scale."



"This study is exceptional because it is pioneering a type of approach that will revolutionize the monitoring of trees and forests on a global scale: in the short term, it will be possible to map the world's trees from the centre of the Amazon to our schoolyards," said <a href="https://www.inrae.fr/en">INRAE</a> researcher Jean-Pierre Wigneron.



"Many fields of application will become much more efficient and accurate, such as tracking carbon stocks, biodiversity, monitoring logging and protection against illegal forest degradation, in near real time.”



Video Credit: NASA Goddard&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.

Remote sensing will revolutionize the way we monitor trees

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Today's Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Dublin, the capital and largest city of Ireland. Beyond its pub culture, Dublin is known as a modern culinary destination and a UNESCO City of Literature.



"Dublin is located near the midpoint of Ireland’s east coast in the province of Leinster. The city, which covers an area of around 115 square kilometers, is bordered by the Dublin Mountains, a low mountain range to the south, and is surrounded by flat farmland to the north and west," says ESA.



"The city straddles the River Liffey, which rises in the Wicklow Mountains and flows around 80 kilometers eastwards through the city of Dublin, in which it is canalised and bordered with quays. It then empties into Dublin Bay, an arm of the Irish Sea."



Dublin has an abundance of green spaces, including one of the largest enclosed public parks in any European capital city. Phoenix Park, which was originally formed as a royal hunting park in the 1660s, includes 707 hectares of green space.



Video Credit: ESA&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.

The city of Dublin on Ireland's east coast

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Today's Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features the province of Zaragoza in northeast Spain. The image was captured by the Copernicus Sentinel-2 mission.



"Together with the provinces of Huesca and Teruel, Zaragoza formed the old kingdom of Aragon. Its capital, also called Zaragoza (not visible in this image) is home to around half of Aragon’s population," says ESA.



"The Ebro River can be seen winding its way through the province from west to east in this image. Between its source in the Cantabrian Mountains in the northwest and its delta on the Mediterranean coast, the Ebro River is fed by more than 200 tributaries as it flows 910 km across much of northern Spain."



Since rainfall is very scarce in this region, irrigation in the Ebro basin is critically important. In the valleys surrounding the Ebro River, many fields are used for growing crops such as corn, wheat, and barley.



Video/ Image Credit: ESA



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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.

The province of Zaragoza in northeast Spain

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Today's Video of the Day from <a href="https://www.nasa.gov/goddard">NASA Goddard</a> features a visual dataset of.methane emissions from wetlands across the globe. Atmospheric methane levels have reached record highs in recent years, and wetlands are a major source of these emissions.&nbsp;



"Methane is an important greenhouse gas that contributes substantially to global warming. On a molecule by molecule basis, methane is much more efficient at trapping heat than carbon dioxide, the main driver of warming," says NASA.



"Though human activities, including agriculture, oil and natural gas production and use, and waste disposal, collectively contribute the majority of methane to the atmosphere, about a third of total methane emissions comes from wetlands."&nbsp;



According to NASA, understanding methane emissions from wetlands and other natural sources is critically important for scientists and policymakers who are working to combat climate change by reducing emissions from human activities.



Video Credit: NASA Goddard



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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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Wetlands are a major source of methane emissions

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Today’s Video of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> reveals the evolution of the Columbia Glacier in southeastern Alaska. Columbia is among the fastest shrinking glaciers in the world, and the video documents its rapid retreat over the years.&nbsp;



Columbia Glacier is a large, multi-branched calving glacier that flows out of the Chugach Mountains to the Prince William Sound.&nbsp;



According to USGS, Columbia had a long history of stability prior to 1980, with a length 41 miles, and small, short-lived advances or retreats.



In the years since 1980, however, satellite images have captured Columbia’s alarming retreat. By using false-color images, scientists can distinguish between snow and ice, open water, vegetation, and rocky debris on the glacier’s surface.



The series of false-color images featured in today's video were acquired over the span of 35 years. You can see that by 2021, the glacier’s main branch had retreated about 15 miles from its initial position.



The Columbia Glacier has also lost more than 50 percent of its volume, mostly due to calving. <a href="https://www.earth.com/video/nasa-reveals-3d-visual-of-an-atmospheric-river/">NASA</a> reports that while climate change likely started the retreat, mechanical processes kept the disintegration going.



The NASA images are provided by Jesse Allen, Robert Simmon, Joshua Stevens, and Lauren Dauphin using data from Landsat satellites, from the U.S. Geological Survey, and data from MODIS on NASA’s Terra satellite. The structure of Columbia’s moraine played a large role in the stability of the glacier before 1980. 



Like other tidewater glaciers, the Columbia built up a moraine over time, and the mixture of ice and rock functioned like a dam keeping out the sea. It was supported on one end by the shoreline and by the underwater terminal moraine at the other.



Video Credit: NASA Earth Observatory/&nbsp; NASA’s Scientific Visualization Studio



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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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The rapid retreat of the Columbia Glacier

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features the Pyrenees Mountains, which form a natural boundary between France and Spain in southwest Europe.



The mountain range is 430 kilometers in length. It stretches from the Mediterranean Sea on the east to the Atlantic Ocean on the west.



At an elevation of 3404 meters, Pico de Aneto is the highest mountain peak in the Pyrenees, and the third-highest peak in Spain. Pico de Aneto is located in the Posets-Maladeta Natural Park, which spans more than 82,000 acres.&nbsp;



"Geological studies have revealed that the Pyrenees Mountains have been around for longer than the Alps, with their sediments first deposited in coastal basins during the Paleozoic and Mesozoic eras," reports ESA.



"The entire mountain range formed due to the upwelling of large sedimentary rocks by the collision of the Iberian and the Eurasian plate around 100 to 150 million years ago, followed by intense erosion from ice and water."



The western Pyrenees receive more precipitation due to moisture blowing in from the Atlantic Ocean. The mountain range contains many lakes, several small glaciers, and some of the highest waterfalls in Europe.



Video &amp; Image Credit: ESA



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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.

The Pyrenees Mountains in southwest Europe

[sendtonews key="6HyfrAJTBI-1831843-12187" type="single"] Today’s Video of the Day from the...

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Today’s Video of the Day from <a href="https://www.stowers.org/">Stowers Institute for Medical Research</a> describes why experts are studying zebrafish to gain a better understanding of how the immune system responds to injury. Zebrafish have the ability to repair and regenerate organs.



“Organ regeneration offers an exciting opportunity for studying the immune system and to inquire why some species can regenerate organs like the heart or missing limbs while others like humans cannot,” explained Dr. Tatjana Piotrowski.



Zebrafish sensory organ hair cells are an ideal system to investigate the pathways and cell types involved in regeneration since they are easily destroyed with antibiotics and begin regenerating within five hours. This enabled the researchers to identify the exact timing and genetic programs for each anti-inflammatory macrophage activation state.&nbsp;



“Our hypothesis is that human macrophages do not receive the proper chemical activation 'cocktail' to instruct pro-regenerative processes,” said Dr. Nicolas Denans. “Identifying the molecular recipe of macrophage activation in zebrafish may one day enable us to design regenerative immunotherapies in humans.”&nbsp;&nbsp;&nbsp;



“The new evidence is a valuable resource for comparative studies on the genetic programs involved in macrophage-mediated repair and regeneration. In other words, different types of injuries may induce different kinds of inflammatory responses. We want to decipher whether this 'language' is universal or if there are a variety of dialects."



Video Credit: Stowers Institute for Medical Research&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.

How the immune system responds to injury

[sendtonews key="0dEcERCq61-2283382-12187" type="single"] Today’s Video of the Day from Stowers...

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Today's Video of the Day from <a href="https://www.nasa.gov/goddard">NASA Goddard</a> describes how record-breaking heat expressed itself around the world in 2022.



Scientists have determined that 2022 was the 5th warmest year since 1880. Furthermore, the last nine consecutive years have been the warmest on record.



From devastating floods and wildfires to natural disasters like Hurricane Ian, 2022 showed us yet again how a warming climate affects people across the globe.&nbsp;



"As we look back at 20:22 and years past, we see that each year we better understand the challenges we face and how important it is to meet them," says NASA.



Video/ Image Credit: NASA Goddard



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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.

2022 illustrated the consequences of a warming climate

[sendtonews key="3UUsNkFOuS-2487333-12187" type="single"] Today's Video of the Day from NASA...

Earth,Like,Exoplanet,3d,Render

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Today's Video of the Day from <a href="https://www.nasa.gov/goddard">NASA Goddard</a> describes two exoplanets that are orbiting a star 218 light-years away. A team of researchers led by the University of Montreal has found evidence that these planets are "water worlds."



The experts used data from NASA’s Hubble and Spitzer Space Telescopes. They discovered that exoplanets Kepler-138 c and Kepler-138 could be composed largely of water.



"We previously thought that planets that were a bit larger than Earth were big balls of metal and rock, like scaled-up versions of Earth, and that's why we called them super-Earths," explained study co-author Björn Benneke.&nbsp;



"However, we have now shown that these two planets, Kepler-138 c and d, are quite different in nature and that a big fraction of their entire volume is likely composed of water. It is the best evidence yet for water worlds, a type of planet that was theorized by astronomers to exist for a long time."



Video Credit: NASA Goddard



Image Credit: NASA, ESA, and Leah Hustak (STScI)



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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.

Two distant planets may be "water worlds"

[sendtonews key="QIoVYJqRBi-2434608-12187" type="single"] Today's Video of the Day from NASA...

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Satellites reveal how Earth's systems are interconnected Today’s Video of the Day from <a href="https://www.nasa.gov/goddard">NASA Goddard</a> describes Earth’s interconnected systems, and how this network is affected by rising temperatures.&nbsp;



During 2020, average global temperatures matched the hottest year on record. The hurricane season was also record-breaking, with many of the storms intensifying at extraordinary speeds. Hot water in the ocean is fuel for hurricanes. The satellite data shows that it's all one interconnected system showing how Satellites reveal how Earth's systems are interconnected.



According to NASA, dust swept up from Northern Africa plays a major role in the formation of hurricanes, and is also a key source of fertilization in the Amazon rainforest. As a result of<a href="https://www.earth.com/news/seagrass-wasting-disease-is-fueled-by-climate-change/"> climate</a> change, dust plumes are expected to decline, which will have an effect on vegetation far away.&nbsp;



Images from Earth-observing satellites show how the world’s plant life is affected by natural disasters, fires, and deforestation. Satellites also reveal how widespread changes in vegetation impact waterways,&nbsp; the climate, air quality. Satellites communicate by using radio waves to send signals to the antennas on the Earth. "Earth From Space" is a groundbreaking two-hour special that reveals a spectacular new space-based vision of our planet. 



Video Credit: NASA Goddard&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.

Satellites reveal how Earth's systems are interconnected

[sendtonews key="JbW4VsY53O-1632195-12187" type="single"] Satellites reveal how Earth's systems are interconnected...

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