The Universe contains many types of massive formations that shape our understanding of how stars and galaxies group together. Astronomers have long studied these sprawling patterns, which give valuable clues about where matter gathers and where it remains thinly spread. 



These features define how cosmic evolution unfolds and guide current theories of how the universe expands.



Recently, a team of experts announced a giant find. This collection of galaxy clusters surpasses previous giants by orders of magnitude.



This study adds fresh insights by demonstrating that our <a href="https://www.earth.com/news/interstellar-tunnel-found-that-connects-our-solar-system-to-other-stars/" target="_blank" rel="noreferrer noopener">cosmic neighborhood</a> can still surprise us with unexpected details about how matter arranges itself across unimaginable distances.



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



Hans Böhringer from the Max Planck Institute for Extraterrestrial Physics (<a href="https://www.mpe.mpg.de/main" target="_blank" rel="noreferrer noopener">MPE</a>) coordinated the effort in collaboration with the Max Planck Institute for Physics (<a href="https://www.mpp.mpg.de/en/" target="_blank" rel="noreferrer noopener">MPP</a>) and teams in Spain and South Africa. 



Their work relied on the ROSAT X-ray satellite’s survey, which singled out clusters of galaxies by detecting the energetic radiation these huge clusters emit. 



These data allowed the researchers to build a three-dimensional map of our cosmic vicinity.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/quipo_superstructure_3D-model_credit-MPE_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/quipo_superstructure_3D-model_credit-MPE_1s.webp" alt="Three-dimensional representation of the Quipu superstructure. Credit: MPE" class="wp-image-1960534"/></a><figcaption class="wp-element-caption">Three-dimensional representation of the Quipu superstructure. Credit: MPE</figcaption></figure>



“If you look at the distribution of the galaxy clusters in the sky in a spherical shell with a distance of 416 to 826 million light-years, you immediately notice a huge structure that stretches from high northern latitudes to almost the southern end of the sky,” explains Böhringer.



By tracing each cluster’s position in space, his team pinpointed how matter spreads out in swirling patterns of galaxies.



<h2 class="wp-block-heading" id="h-the-quipu-superstructure">The Quipu superstructure</h2>



The researchers named this discovery “Quipu,” taking inspiration from the knotted string recording system once used by the Incas. 



Observed as a long strand with smaller threads branching off, the Quipu superstructure contains 68 galaxy clusters with a combined mass of about 2.4 × 10^17 solar masses. 



Its size of roughly 1.4 billion light-years makes Quipu the largest superstructure ever accurately measured, surpassing the Sloan Great Wall’s 1.1 billion light-years.



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/quipo_superstructure_illustration_credit-MPE_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/quipo_superstructure_illustration_credit-MPE_1s.webp" alt="Distribution of galaxies (color coding) and galaxy clusters (black dots) in a spherical shell with a distance of 416 to 826 million light years surrounding us. The five superstructures are marked: 1 Quipu, 2 Shapley, 3 Serpens-Corona Borealis and Hercules (overlapping in the sky), 4 Sculptor-Pegasus. The area enclosed by white lines is shadowed by the disk of the Milky Way. Credit: MPE" class="wp-image-1960536"/></a><figcaption class="wp-element-caption">Distribution of galaxies (color coding) and galaxy clusters (black dots) in a spherical shell with a distance of 416 to 826 million light years surrounding us. The five superstructures are marked: 1 Quipu, 2 Shapley, 3 Serpens-Corona Borealis and Hercules (overlapping in the sky), 4 Sculptor-Pegasus. The area enclosed by white lines is shadowed by the disk of the Milky Way. Credit: MPE</figcaption></figure>



“This breaks the size record of all reliably measured cosmic structures,” note the researchers who compared the finding with other known formations. 



“The Quipu superstructure, end to end, is slightly longer than the <a href="https://www.researchgate.net/figure/SDSS-3D-Universe-Map-Credit-Sloan-Digital-Sky-Survey-Team-NASA-NSF-DOE_fig2_357328983" target="_blank" rel="noreferrer noopener">Sloan Great Wall</a>,” says J. Richard Gott III at Princeton University, who helped discover the Sloan Great Wall. “Congratulations to them for finding it.” 



The name also reflects a connection to Chile, where many distance measurements took place, and where ancient quipus are showcased in Santiago.



<h2 class="wp-block-heading" id="h-quipu-and-cosmological-principle">Quipu and cosmological principle</h2>



Across extremely large distances, matter is believed to spread out nearly evenly. At smaller scales of about a billion light-years, it collects in superclusters and leaves behind voids. 



This balance underpins the <a href="https://www.earth.com/news/cosmic-order-or-chaos-universe-expansion-may-follow-a-hidden-pattern/" target="_blank" rel="noreferrer noopener">cosmological principle</a>, which suggests that if we look far enough, the universe should appear uniform in every direction. 



Some experts argue these huge arrangements question that principle’s validity, with past findings triggering debates. 



<figure class="wp-block-image aligncenter size-full"><a href="https://www.earth.com/wp-content/uploads/2025/02/great-sloan-wall_superstructure_SDSS_credit-MIT_1m.jpg" target="_blank" rel="noreferrer noopener"><img src="https://www.earth.com/wp-content/uploads/2025/02/great-sloan-wall_superstructure_SDSS_credit-MIT_1s.webp" alt="Sloan Great Wall of galaxies. SDSS 3D Universe Map Credit: Sloan Digital Sky Survey Team, NASA, NSF, DOE." class="wp-image-1960531"/></a><figcaption class="wp-element-caption">Sloan Great Wall of galaxies is 1.1 billion light years long. SDSS 3D Universe Map Credit: Sloan Digital Sky Survey Team, NASA, NSF, DOE.</figcaption></figure>



“Making observations in too small a part of the universe, which has been done earlier on, can be misleading,” says Böhringer. 



Another point comes from an ambiguous definition of the principle. “There is not yet one definition of the cosmological principle that every cosmologist agrees on,” says Alexia Lopez at the <a href="https://www.uclan.ac.uk/" target="_blank" rel="noreferrer noopener">University of Central Lancashire</a> in the UK. 



Meanwhile, Seshadri Nadathur at the <a href="https://www.port.ac.uk/" target="_blank" rel="noreferrer noopener">University of Portsmouth</a> notes that “some of those galaxies may drift apart from each other instead of collapsing in on themselves, in which case, according to some interpretations, it’s not really a bound structure.”



<h2 class="wp-block-heading" id="h-cosmic-measurements-and-consequences">Cosmic measurements and consequences</h2>



Quipu’s existence highlights how vast formations can shape calculations of cosmic expansion rates and the properties of primordial radiation left over from the early universe. 



Astronomers pay close attention to features like superclusters because they alter light paths and influence how we determine important parameters such as the <a href="https://www.earth.com/news/unknown-factors-are-accelerating-the-expansion-of-the-universe/" target="_blank" rel="noreferrer noopener">Hubble constant</a>. 



Small discrepancies can add up when researchers aim for precise numbers in modern cosmological studies.



“Even if these are only corrections of a few percent, they become increasingly important as the accuracy of cosmological observations increases,” emphasizes Gayoung Chon from the Max Planck Institute for Physics. 



This structure offers a reminder that the cosmos presents patterns on many scales. Those patterns appear to affect how we interpret data on the universe’s origin and shape the <a href="https://www.earth.com/news/massive-galactic-explosion-provides-clues-about-galaxy-evolution/" target="_blank" rel="noreferrer noopener">evolution of galaxies</a> in our vicinity and beyond.



<h2 class="wp-block-heading" id="h-quipu-and-the-incas">Quipu and the Incas</h2>



The Incas once managed vast territories using quipus, a system of knotted strings that helped track resources and information. 



Each knot arrangement acted like a code, revealing essential data in a form that required no written script.



Quipu’s naming borrowed that image of intertwined threads. 



Researchers see it as a nod to humanity’s long history of gathering knowledge, whether through knotted strings or advanced telescopes that trace the distribution of galaxies across cosmic depths.



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



The discovery underscores how ongoing surveys might uncover more structures. 



Scientists are keen to see if similar patterns exist in parts of the sky that remain less charted, which could either confirm current theories or reveal new gaps in our understanding.



Future maps will rely on technology to gather clearer data from remote regions. 



These efforts reflect a human wish to capture our place in the universe, searching for the patterns that connect everything from particles to vast congregations of galaxies.



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Featured image: The open cluster Westerlund 1 is located roughly 12,000 light-years away in the southern constellation Ara (the Altar) where it resides behind a huge interstellar cloud of gas and dust. Credit: <a href="https://www.esa.int" target="_blank" rel="noreferrer noopener">ESA</a>



The full study was published in the journal <a href="https://arxiv.org/abs/2501.19236" target="_blank" rel="noreferrer noopener">Astronomy and Astrophysics</a>.



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Largest structure ever found in the universe is 1.4 billion light years long

The Universe contains many types of massive formations that shape our understanding of how stars and galaxies group together. Astronomers have long studied these sprawling patterns, which give valuable clues about where matter gathers and where it remains thinly spread. These features define how cosmic evolution unfolds and guide current theories of how the universe expands. Recently, a team of experts announced a giant find. This collection of galaxy clusters surpasses previous giants by orders of magnitude. This study adds fresh insights by demonstrating that our cosmic...

As apex <a href="https://www.earth.com/news/clash-of-the-top-predators-wolves-are-eating-sea-otters/">predators</a>, large carnivores such as lions or wolves play crucial roles in their ecosystems. However, their numbers have significantly declined over the past decades, giving rise to efforts of relocating several species – including reintroduction of species to areas where they had been exterminated or reinforcing an existing population to increase its viability – to support their conservation. To date though, there has been little information about what factors determine whether such rewilding programs are successful or not.



Now, a team of researchers led by the <a href="https://www.ox.ac.uk/">University of Oxford</a> has analyzed data from nearly 300 animal relocations that took place between 2007 and 2021, spanning 22 countries on five continents, and involving 18 different large carnivore species, such as wolves, bears, hyenas, wild dogs, and big cats.



The analysis revealed that two thirds (66 percent) of the relocations were successful and that success rates for large carnivore relocations have increased substantially since 2007. According to the experts, for wild-born carnivores, success rates increased from 53 percent (pre-2007) to 70 percent, and for captive-born animals, success rates doubled from 32 percent to 64 percent. The species with the highest success rates were maned wolves, pumas, and ocelots (100 percent success rate), while those with the lowest success rate (approximately 50 percent) were African lions, cheetahs, brown hyenas, Iberian lynxes, and wolves.



“Soft-release” methods – involving acclimatizing the animals to the new environments before fully releasing them – appeared to me most successful. At the same time, releasing young animals (one or two years of age) also increased success rates, due to their greater behavioral plasticity to adapt to new environments. Compared to animals born in the wild, the success rate of animals released from captivity decreased by 1.5-fold. Unfortunately, just over a third (37 percent) of the relocated animals could find a mate and/or raise a cub in their new habitats.



Although the fact that most relocated animals survived is highly encouraging, their low mating success show the ongoing challenges rewilding efforts face and highlight the importance of protecting already existing habitats.



“In the last 15 years we have become more successful at translocating and reintroducing large carnivores. This allows us to be optimistic for the future of rebuilding damaged ecosystems around the globe, but we must remember that it is always more important to protect large carnivore populations where they are now before we lose them. Even as we have grown to be more successful, 34 percent of individual translocations fail and they cannot be seen as a replacement for immediate conservation action to save these populations,” concluded lead author Seth Thomas, a biologist at Oxford.



The study is published in the journal <a href="http://dx.doi.org/10.1016/j.biocon.2023.109909">Biological Conservation</a>.&nbsp;&nbsp;



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Rewilding programs have become increasingly successful

As apex predators, large carnivores such as lions or wolves...

Baby kangaroo feces could provide an unlikely solution to cow-produced methane, according to a new study from <a href="https://wsu.edu/">Washington State University</a>.



<a href="https://www.earth.com/video/wetlands-are-a-major-source-of-methane-emissions/">Methane</a> is the second largest greenhouse gas contributor and is 30 times more potent than carbon dioxide. More than half of the methane released into the atmosphere is thought to come from the agricultural sector. Ruminant animals, such as cattle and goats, are the most significant contributors.



Using a cow stomach simulator, the researchers discovered that methane production can be inhibited by a microbial culture developed from baby kangaroo feces.



“Methane emissions from cows are a major contributor to greenhouse gases, and at the same time, people like to eat red meat,” said study co-author Birgitte Ahring.



To reduce methane, researchers have tried changing cows’ diets and developing vaccines, but there are too many varieties of the methane-producing bacteria. These interventions can also negatively affect biological processes.



The WSU researchers had previously designed an artificial rumen, the largest stomach compartment, to simulate cow digestion. Ahring said that among the enzymes that are able to break down natural materials, rumens have “amazing abilities."



Ahring learned that kangaroos have acetic acid-producing, instead of methane-producing, bacteria in their foregut. The specialized acetic acid-producing process only occurred in baby kangaroos – not in adults. Unlike methane, acetic acid benefits cows by supporting muscle growth.&nbsp;



After reducing the methane-producing bacteria in their reactor with a specialized chemical, the acetic acid bacteria were able to replace the methane-producing microbes for several months.



“It is a very good culture. I have no doubt it is promising,” Ahring said. “It could be really interesting to see if that culture could run for an extended period of time, so we would only have to inhibit the methane production from time to time. Then, it could actually be a practice.”



The research is published in the journal <a href="http://dx.doi.org/10.1016/j.bcab.2022.102526">Biocatalysis and Agricultural Biotechnology</a>.



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By <a href="mailto:katherinebucko@gmail.com">Katherine Bucko</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Kangaroos could help reduce methane emissions from cattle

Baby kangaroo feces could provide an unlikely solution to cow-produced...

The preferred <a href="https://www.earth.com/news/male-spiders-transfer-more-sperm-when-mating-with-cannibals/">mating</a> strategy of the eastern Australian humpback whale has shifted from singing to fighting in recent years, according to a new study led by Professor Rebecca Dunlop from <a href="https://www.uq.edu.au/">The University of Queensland</a>.



While analyzing nearly two decades of data, the researchers found that male whales along Australia’s eastern seaboard have given up singing to attract mates. Instead, they are battling it out with other male competitors.&nbsp;



"The eastern Australian humpback whale population was whaled almost to extinction in the 1960s (~200 whales) and has recovered to pre-whaling numbers (&gt;20,000 whales). Using an 18-year dataset, where the population increased from approximately 3,700 to 27,000 whales, we found that as male density increased over time, the use of mating tactics shifted towards more males engaging in non-singing physical competition over singing," wrote the study authors.



The experts noted that while singing was the more successful mating strategy in earlier post-whaling years, non-singing behavior became the more successful tactic in later years.



“In 1997, a singing male whale was almost twice as likely to be seen trying to breed with a female when compared to a non-singing male,” said Dr. Dunlop. “But by 2015 it had flipped, with non-singing males almost five times more likely to be recorded trying to breed than singing males."



“It’s quite a big change in behavior so humans aren’t the only ones subject to big social changes when it comes to mating rituals.”



According to the researchers, the transition in mating behavior happened progressively as whale populations recovered from low numbers.



Study co-author Dr. Celine Frere noted that previous work by UQ Professor Michael Noad found that the whale population increased from approximately 3,700 whales to 27,000 between 1997 and 2015.



“We used this rich dataset, collected off Queensland’s Peregian Beach, to explore how this big change in whale social dynamics could lead to changes in their mating behavior,” said Dr. Frere. “We tested the hypothesis that whales may be less likely to use singing as a mating tactic when the population size is larger, to avoid attracting other males to their potential mate.”



“If competition is fierce, the last thing the male wants to do is advertise that there is a female in the area, because it might attract other males which could out-compete the singer for the female,” explained Dr. Dunlop. “By switching to non-singing behavior, males may be less likely to attract competition and more likely to keep the female.



“If other males do find them, then they either compete, or leave. With humpbacks, physical aggression tends to express itself as ramming, charging, and trying to head slap each other. This runs the risk of physical injury, so males must weigh up the costs and benefits of each tactic.”



“It will be fascinating to see how whale mating behavior continues to be shaped in the future.”



The study is published in the journal <a href="http://dx.doi.org/10.1038/s42003-023-04509-7">Communications Biology</a>.



Image Credit: The Cetacean Ecology Group, University of Queensland.



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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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Whales changed their mating tactic from singing to fighting

The preferred mating strategy of the eastern Australian humpback whale...

The <a href="https://www.earth.com/news/thwaites-glacier-underground-lakes/">Thwaites Glacier</a> is one of the fastest changing glaciers in Antarctica, with its grounding zone - the point where it meets the seafloor – retreating 14 kilometers since the 1990s. Since much of this glacier’s ice sheet lies below the sea level and is susceptible to rapid, irreversible loss, global sea levels could rise by over half a meter within centuries if melting continues at such rates.



However, according to two new recent studies published in the journal <a href="https://www.nature.com/">Nature</a>, although melting has increased beneath the floating ice shelf, the current rate of melting is slower than several computer models have estimated.&nbsp;



By collecting data from ocean measurements through deep boreholes at six different locations underneath the ice shelf over a nine-month period, a team of researchers led by the <a href="https://www.bas.ac.uk/">British Antarctic Survey</a> (BAS) and <a href="https://www.cornell.edu/">Cornell University</a> has found that the rapid retreat of this glacier is driven by different processes under the ice shelf. According to the scientists, while melting beneath much of the ice shelf is weaker than expected, melting in cracks and crevices is much faster.



“Our results are a surprise but the glacier is still in trouble,” said Peter Davis, an oceanographer at BAS and lead author of <a href="https://www.nature.com/articles/s41586-022-05586-0">one of the studies</a>. “If an ice shelf and a glacier is in balance, the ice coming off the continent will match the amount of ice being lost through melting and iceberg calving. What we have found is that despite small amounts of melting there is still rapid glacier retreat, so it seems that it doesn’t take a lot to push the glacier out of balance.”



Thus, although the vertical melting along the base of the ice shelf was less than expected, melting along sloped ice in cracks and terraces is much higher and could be a major factor in ice loss across this massive glacier, particularly as large rifts are progressing along the ice shelf and may become the primary trigger for ice shelf collapse.



“These new ways of observing the glacier allow us to understand that it’s not just how much melting is happening, but&nbsp;how&nbsp;and&nbsp;where&nbsp;it is happening that matters in these very warm parts of Antarctica. We see crevasses, and probably terraces, across warming glaciers like Thwaites.&nbsp;Warm water is getting into the cracks, helping wear down the glacier at its weakest points,” explained Britney Schmidt, an associate professor of Planetary Science at Cornell and lead author of the <a href="https://www.nature.com/articles/s41586-022-05691-0">second study</a>.&nbsp;



“Our results demonstrate that the canonical model of ice-shelf basal melting used to generate sea-level projections cannot reproduce observed melt rates beneath this critically important glacier, and that rapid and possibly unstable grounding-line retreat may be associated with relatively modest basal melt rates,” the experts concluded.



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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What is causing the rapid retreat of the Thwaites Glacier?

The Thwaites Glacier is one of the fastest changing glaciers...

By examining data spanning nine billions of years, a team of scientists led by the&nbsp;<a href="https://manoa.hawaii.edu/">University of Hawaiʻi at Mānoa</a> has found the first observational evidence that <a href="https://www.earth.com/news/earths-closest-black-hole-has-been-discovered/">black holes</a> contain cores of dark energy, a mysterious force driving the accelerating expansion of the universe. Thus, instead of dark energy being spread out across spacetime, as many scientists have previously assumed, the new findings suggest that this energy was created and remains inside the (increasingly larger) black holes that formed in the crushing forces of collapsing stars.



The existence of dark energy was first proposed in the 1990s when investigations of distant stars revealed that the expansion of the universe was accelerating. This strange phenomenon – given that gravity should be slowing the universe’s expansion – made scientists ponder what could drive the expansion faster and led them to postulate dark energy as an unknown, mysterious force working against gravity. However, its precise nature and origins have not yet been clearly understood. Now, by connecting this force to the evolution of black holes over extended periods of time, the researchers have managed to shed new light on the nature of our universe.&nbsp;



“We’re really saying two things at once: that there’s evidence the typical black hole solutions don’t work for you on a long, long timescale, and we have the first proposed astrophysical source for dark energy,'” said lead author Duncan Farrah, an astrophysicist at Hawai’i.



“What that means, though, is not that other people haven’t proposed sources for dark energy, but this is the first observational paper where we’re not adding anything new to the universe as a source for dark energy: black holes in Einstein’s theory of gravity are the dark energy.”



By comparing black hole masses in young galaxies, where stars are still forming, with black holes masses in old, so-called “dormant galaxies,” where no more stars are currently born, the scientists discovered that black holes in dormant galaxies are between seven to 20 times larger than expected, suggesting that black holes too are growing as the universe expands.



“Here’s a toy analogy. You can think of a coupled black hole like a rubber band, being stretched along with the universe as it expands,” explained co-author Kevin Croker, a cosmologist at Hawai’i. “As it stretches, its energy increases. Einstein’s&nbsp;E = mc2&nbsp;tells you that mass and energy are proportional, so the black hole mass increases, too.”



“The importance of this work is that it’s taken the theories about black holes with dark energy cores and linked them for the first time to tangible observations of the universe,” concluded co-author Chris Pearson, an astronomer at the research institute <a href="https://www.ralspace.stfc.ac.uk/Pages/home.aspx">RAL&nbsp;Space</a>&nbsp;in Oxfordshire. “These black holes are expected to grow in mass as the universe expands.”&nbsp;



The findings are synthetized in two articles published in <a href="https://iopscience.iop.org/article/10.3847/1538-4357/acac2e">The Astrophysical Journal</a>&nbsp;and&nbsp;<a href="https://iopscience.iop.org/article/10.3847/2041-8213/acb704">The Astrophysical Journal Letters</a>.



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Dark energy is created and contained in black holes

By examining data spanning nine billions of years, a team...

According to music psychology expert Michael Bonshor of the University of Sheffield, to create a happy song, <a href="https://www.earth.com/news/music-helps-dementia-patients-connect-with-caregivers/">music</a> artists should combine a major key, 7th chords, 137 BPM (beats per minute), strong beats, four beats in every bar, and a verse-chorus-verse-chorus structure. Moreover, happy songs should have a short intro, repeated riffs, bright tone, high volume, and a mix of predictability and surprise.



“Previous studies have found songs are perceived as happy if they are in a major key, with a sweet spot of approximately 137 beats per minute. We like ‘7th chords’ as they add interest; regular chords use three notes, whereas ‘7th chords’ add an extra note which provides a sense of musical ‘tension’ and ‘relief,’” Bonshor explained.



“Alongside this, cheery songs usually&nbsp;have a strong 1-2-1-2 beat to them, so that you can dance along – and a short introduction means the song kicks off with a bang straight away, and there’s not a long build up. We like high volume when it comes to how our happy songs are made, with notes played in a bright and bouncy way by instruments such as trumpets or electric guitars instead of mellower instruments. Finally, a repetitive rhythm or guitar riff that people can latch onto and becomes memorable is the cherry on the cake.”



According to Dr. Bonshor’s formula, the happiest song ever created and performed is “Good Vibrations” by The Beach Boys, followed by “I Got You” (I Feel Good) by James Brown, “House of Fun” by Madness, and “Get the Party Started” by P!nk. Moreover, this “happy formula” has now been turned by Jamie P and Oliver Price into a pitch-perfect track called “<a href="https://soundcloud.com/mullerlight/the-lighter-note?utm_source=clipboard&amp;utm_medium=text&amp;utm_campaign=social_sharing">The Lighter Note</a>.”



Here are the top 10 happiest songs according to Dr. Bonshor’s formula:



<ol><li>“Good Vibrations” by The Beach Boys</li><li>“I Got You” (I Feel Good) by James Brown</li><li>“House of Fun” by Madness</li><li>“Get the Party Started” by P!nk</li><li>“Uptown Girl” by Billy Joel</li><li>“Sun Is Shining” by Bob Marley</li><li>“I Get Around” by The Beach Boys</li><li>“YMCA” by Village People</li><li>“Waterloo” by ABBA</li><li>“September” by Earth, Wind &amp; Fire</li></ol>



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Which songs make people the happiest?

According to music psychology expert Michael Bonshor of the University...

Paleontology is usually associated with studying ancient bones, and most would imagine that brain study would be off the cards for creatures as ancient as <a href="https://www.earth.com/news/early-dinosaurs-benefited-from-changes-in-global-climate/">dinosaurs</a>. However, recent collaborative studies between the <a href="https://www.southampton.ac.uk/">University of Southampton</a> and Ohio University concern exactly that - the reconstruction of the brains of two spinosaurs based on fossils found at the Isle of Wight.&nbsp;



 The team studied Baryonyx fossils from Surrey and Ceratosuchops from the Isle of Wight, both of which contained the oldest braincase material known. The fossils are anticipated to be around 125 million years old, yet both specimens have been well preserved, which helped to facilitate the reconstruction.&nbsp;



The researchers conducted the study to learn more about the spinosaur brain and how these animals interacted with their environment. They were unusual species that had crocodile-like jaws, conical teeth, and lived an aquatic lifestyle of stalking riverbanks - behaviors which were very different from other theropods such as the Allosaurus or the Tyrannosaurus.



 The researchers noted that the creature's sense of smell would not have been very good due to the undeveloped nature of its olfactory bulbs. Furthermore, it was concluded that these animals would mostly only hear low frequencies, and that parts of the brain involved in developing head stability and a prey gaze were likely to be less developed than in more specialized dinosaurs.&nbsp;



“Despite their unusual ecology, it seems the brains and senses of these early spinosaurs retained many aspects in common with other large-bodied theropods – there is no evidence that their semi-aquatic lifestyles are reflected in the way their brains are organized,” explained study lead author Chris Barker.



“It’s surprising to see such ‘non-specialized’ brains…but the results are still significant. It’s exciting to get so much information on sensory abilities from British dinosaurs. Using cutting-edge technology, we basically obtained all the brain-related information we possibly could from these fossils,” said Dr. Darren Naish.



The researchers are anticipating that this study is just the start of a new research boom in dinosaur cognition, with several spinosaur studies already taking place in Britain over the last few years.&nbsp;



“This new research is just the latest in what amounts to a revolution in paleontology due to advances in CT-based imaging of fossils,” said Professor Lawrence M. Witmer. 



“This new study highlights the significant role British fossils have in our constantly evolving, fast-moving understanding of dinosaurs, and shows how the UK - and the University of Southampton in particular - is at the forefront of spinosaur research,” said Dr. Neil Gostling.



 The research is published in the <a href="http://dx.doi.org/10.1111/joa.13837">Journal of Anatomy</a>.&nbsp;



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By <a href="mailto:calumvaughan05@gmail.com">Calum Vaughan</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Spinosaur brains reveal how they interacted with their environment

Paleontology is usually associated with studying ancient bones, and most...

We cannot know exactly how Earth’s climate was in the past, nor how it will be in the future. However, it is very important for scientists to try and predict what changes may take place so that policy- and decision-makers can develop ways to reduce and mitigate against the destructive effects of a warming planet.&nbsp;



Scientists make use of climate system models to get a better idea of how weather patterns and climatic factors may change in the future. These are computer simulations that use real data on factors that drive the climate today to predict how <a href="https://www.earth.com/news/extreme-weather-is-becoming-more-difficult-to-predict/">weather</a> patterns may change under different conditions, such as increases in the levels of greenhouse gases.&nbsp;



Before using a climate model to predict what may happen in future, it is important that its accuracy in identifying past climatic conditions is assessed. This is done by comparing the model’s simulated conditions with climatic data derived from other sources, such as tree rings or pollen, or the stable isotope ratios in lake and ocean sediments or ice cores. These sources of data are known as proxies since they reflect past climatic conditions indirectly.&nbsp;



Interestingly, when climatic models are used to predict the Earth’s temperature during the Holocene Period (the past 12,000 years), the predictions disagree with the evidence obtained from proxy sources. The paleo-environmental proxy data, including evidence from ocean and lake sediments, indicate that temperature peaked at 6,500 years ago and then gradually cooled down until humans started burning fossil fuels around 200 years ago. In contrast, the climate models generally show global average temperatures increasing gradually throughout the Holocene Period.



The disagreement on climatic conditions during this time period is known as the Holocene temperature conundrum. A new review article, published in the journal <a href="http://dx.doi.org/10.1038/s41586-022-05536-w">Nature</a>, has now addressed this conflict between the findings of climate models and proxy evidence by analyzing a large quantity of available data on global temperature from the past 12,000 years.&nbsp;



The researchers included lead author Darrell Kaufman, a Regents’ professor in the School of Earth and Sustainability at <a href="https://nau.edu/">Northern Arizona University</a>, and University of Arizona postdoctoral researcher Ellie Broadman, a co-author who worked on the study while earning her Ph.D. at NAU. The team aimed to identify whether the global average temperature 6,500 years ago was warmer, as indicated by proxy evidence, or colder, as simulated by models, than the temperature in the late 19th&nbsp;century, when the Industrial Revolution led to a significant increase in human-caused warming.



This comprehensive and systematic assessment concludes that the global average temperature 6,500 years ago was likely warmer and was followed by a multi-millennial cooling trend that ended in the 1800s. This finding supports the data derived from numerous proxy sources, rather than the conclusions derived from current climate models. However, the authors cautioned that uncertainty still exists, despite recent studies that have claimed to have resolved the conundrum.



“Quantifying the average temperature of the earth during the past, when some places were warming while others were cooling, is challenging, and more research is needed to firmly resolve the conundrum,” Kaufman said.&nbsp;



“But tracing changes in global average temperature is important because it’s the same metric used to gauge the march of human-caused warming and to identify internationally negotiated targets to limit it. In particular, our review revealed how surprisingly little we know about slow-moving climate variability, including forces now set into motion by humans, that will play out as sea level rises and permafrost thaws over coming millennia.”



We know more about the climate of the Holocene, which began after the last major ice age ended, 12,000 years ago, than any other multi-millennial period. There are published studies from a variety of natural archives that store information about historical changes that occurred in the atmosphere, oceans, cryosphere and on land; studies that look at the forces that drove past climate changes, such as Earth’s orbit, solar irradiance, volcanic eruptions and greenhouse gases; and climate model simulations that translate those forces into changing global temperatures. All these types of studies were included in this review.



If the researchers are correct, and the proxy data gives a more accurate reflection of global temperature changes during this time, this implies deficiencies in the models and casts uncertainty on their use to forecast climatic conditions in the future. In particular, this would challenge climate scientists’ understanding of factors that naturally drive climate changes and feedbacks, and that are used in the development of climate models.&nbsp;



If the researchers are incorrect, then scientists need to improve their understanding of the way in which proxy records indicate past temperature information, and further develop analytical tools to capture these trends on a global scale.



What is a certainty, however, is that the change in global average temperature in the past 6,500 years, be it upwards or downwards, has been gradual and has been very small – less than 1oC (1.8oF). This is less than the warming already measured in the last 100 years alone, most of which is related to human activities.&nbsp;



Attempting to resolve the Holocene global temperature conundrum has been a priority for climate scientists in the last decade; Broadman remembers reading the initial paper on this topic when she started her Ph.D. in 2016. All the studies since then have added to the understanding of this issue. However, it is still not clear what factors might be driving a cooling climate in the past 6,500 years when levels of atmospheric greenhouse gases were slowly increasing and ice sheets were slowly retreating – both factors that would be expected to cause warming, not cooling.



The current review certainly highlights the fact that we don’t yet know the solution to this conundrum.



“One interesting takeaway is that our findings demonstrate the impact that regional&nbsp;changes can have on&nbsp;global&nbsp;average temperature. Environmental changes in some regions of the Earth, like declining Arctic sea ice or changing vegetation cover in what are now vast deserts, can cause feedbacks that influence the planet as a whole,” Broadman said.&nbsp;



“With current global warming, we already see some regions changing very quickly. Our work highlights that some of those regional changes and feedbacks are really important to understand and capture in climate models.”



Additionally, Kaufman said, accurately reconstructing the details of past temperature change offers insights into climate’s response to various causes of both natural and anthropogenic climate change. The responses serve as benchmarks to test how well climate models simulate the Earth’s climate system.



“Climate models are the only source of detailed quantitative climate predictions, so their fidelity is critical for planning the most effective strategies to mitigate and adapt to climate change,” said Kaufman. “Our review suggests that climate models are underestimating important climate feedbacks that can amplify global warming.”



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By <a href="mailto:bosman@truewan.co.za">Alison Bosman</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Was Earth heating up or cooling down before global warming?

We cannot know exactly how Earth’s climate was in the...

A new study led by the <a href="https://www.cam.ac.uk/">University of Cambridge</a> has found that there is a significant lack of awareness among both U.S. and UK populations regarding the possibility and effects of a “nuclear winter” – the potential for long-term environmental and public health consequences from any exchange of nuclear weapons.



According to the experts, detonations from nuclear exchanges would throw vast amounts of debris into the stratosphere, blocking out much of the sun for over a decade, and thus causing global drops in temperature, mass crop failure, and widespread famine. Combined with radiation fall-out, such consequences would lead to the death of millions of people in the wake of a <a href="https://www.earth.com/news/canada-wildfire-smoke-nuclear-war/">nuclear war</a>, including many far outside of any blast zone.



To assess their awareness of such a scenario, the researchers asked 3,000 participants in an online survey (half from the U.S. and half from the UK) to self-report on a sliding scale how much they felt they knew about a nuclear winter, and if they heard about such a possibility from contemporary media/culture, recent academic studies, or Cold War era beliefs and memories.&nbsp;



The analysis revealed that only 3.2 and 7.5 percent of the participants (from UK and US, respectively) were familiar with such a phenomenon from media or culture, 1.6 percent (UK) and 5.2 percent (U.S.) from academic studies, and 5.4 percent (UK) and 9 percent (U.S.) from Cold War memories. In the event of a hypothetical Russian nuclear attack on Ukraine, fewer than one in five participants from both countries supported in-kind retaliation, with men more likely than women to back nuclear reprisal - 20.7 percent (U.S.) and 24.4 percent (UK) of men compared to 14.1 percent (US) and 16.1 percent (UK) of women.



“In 2023 we find ourselves facing a risk of nuclear conflict greater than we’ve seen since the early eighties. Yet there is little in the way of public knowledge or debate of the unimaginably dire long-term consequences of nuclear war for the planet and global populations,” said study lead author Paul Ingram, a senior research associate at University of Cambridge’s <a href="https://www.cser.ac.uk/">Center for the Study of Existential Risk</a> (CSER).



“Ideas of nuclear winter are predominantly a lingering cultural memory, as if it is the stuff of history, rather than a horribly contemporary risk. Of course, it is distressing to consider large-scale catastrophes, but decisions need to account for all potential consequences, to minimize the risk. Any stability within nuclear deterrence is undermined if it is based on decisions that are ignorant of the worst consequences of using nuclear weapons.”&nbsp;



“There is an urgent need for public education within all nuclear-armed states that is informed by the latest research. We need to collectively reduce the temptation that leaders of nuclear-armed states might have to threaten or even use such weapons in support of military operations,” he concluded.



The findings are published in a report on CSER’s <a href="https://www.cser.ac.uk/news/opinion-poll-survey-public-awareness-nuclear-winte/">website</a>.



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Risk of nuclear winter underestimated by most people

A new study led by the University of Cambridge has...

While coastal populations all over the world are already bracing for rising sea levels, planning for measures to mitigate flooding and other possible damages has been quite difficult. This is because the latest climate projections disagree on how rapidly the world’s largest ice sheets will respond to global warming.&nbsp;



Now, a study published in the journal <a href="http://dx.doi.org/10.1038/s41467-023-36051-9">Nature Communications</a> argues that an irreversible loss of the West Antarctic and Greenland ice sheets, along with a rapid acceleration of <a href="https://www.earth.com/news/sea-level-rise-will-cause-widespread-impacts-sooner-than-expected/">sea level rise</a>, will be imminent if global temperatures rise more than 1.8°C above pre-industrial levels.



Although melting ice sheets are likely the largest contributor to sea level rise, their behavior has been hardest to predict since the physics governing their temperature-related changes is highly complex.&nbsp;



“Moreover, computer models that simulate the dynamics of the ice sheets in Greenland and Antarctica often do not account for the fact that ice sheet melting will affect ocean processes, which, in turn, can feed back onto the ice sheet and the atmosphere,”&nbsp;said study lead author Jun Young Park, a doctoral student in Climate Sciences at the <a href="https://ibsclimate.org/">IBS Center for Climate Physics</a> and the <a href="https://www.pusan.ac.kr/eng/Main.do">Pusan National University</a> in South Korea.



By using a groundbreaking computer model that captures the complex relations among ice sheets, icebergs, ocean, and atmosphere, the scientists discovered that a rapid acceleration of ice sheet melting and sea level rise could only be prevented if the world reaches net zero emissions by 2060.



“If we miss this emission goal, the ice sheets will disintegrate and melt at an accelerated pace, according to our calculations. If we don’t take any action, retreating ice sheets would continue to increase sea level by at least 100 cm within the next 130 years. This would be on top of other contributions, such as the thermal expansion of ocean water,” explained study co-author Axel Timmermann, the director of the IBS Center.



While in previous studies scientists have mainly stressed the importance of subsurface ocean melting, sea ice and atmospheric circulation changes around Antarctica also play major roles in controlling the amount of ice sheet melting and subsequent sea level rise. Thus, more complex earth system models that can capture the interactions between different climate components are urgently needed, along with new observational programs.



“One of the key challenges in simulating ice sheets is that even small-scale processes can play a crucial role in the large-scale response of an ice sheet and for the corresponding sea-level projections. Not only do we have to include the coupling of all components, as we did in our current study, but we also need to simulate the dynamics at the highest possible spatial resolution using some of the fastest supercomputers,”&nbsp;Timmermann concluded.



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Rapid acceleration of sea level rise may be unavoidable

While coastal populations all over the world are already bracing...

A new study led by the <a href="https://www.shh.mpg.de/en">Max Planck Institute for the Science of Human History</a> has found that dogs and humans who have the strongest relationships have similar <a href="https://www.earth.com/news/people-select-their-dogs-according-to-their-own-personality/">personalities</a>, matching on features such as levels of warmth, enjoyment of spending time outdoors, and selflessness with their possessions. However, according to the experts, owners who are overly attached to their pups may give rise to dysfunctional human-animal relationships.



The scientists reviewed 29 published articles on dog-owner relationships to clarify what personality traits lead to positive interspecies connections.&nbsp;



The analysis revealed that canine personality traits associated with functional and fulfilling dog-owner relationships included energy, affection, openness, intelligence, agreeableness, and responsiveness to training. By contrast, antisocial, territorial, and destructive dogs were linked to problematic relationships with their owners.



“Openness and agreeableness of the dog could represent traits which enable them to facilitate these social interactions especially well.&nbsp;Particularly in cases where the owners do not possess these traits, they might benefit greatly from their presence in their dogs,” the authors explained.



Moreover, the researchers discovered that functional dog-owner relationships tend to be “complementary” – with both humans and animals being similarly friendly, but opposite in dominance/submissiveness traits. However, the combination of a dominant dog and a submissive owner was found to be challenging in practical ownership.



Finally, the investigation provided evidence that highly attached owners characterized by a “humanistic orientation towards the dog” could often give rise to mental issues in their pet, such as increased separation anxiety.&nbsp;



“That highly attached owners often owned dogs with separation related problems might be because the owners themselves are very worried about the imminent spatial separation, which in turn creates a negative feeling in the dogs,” the authors wrote.



“While many studies have reported that cuteness and general appearance are among the most important purchase motives of owners, this review suggests that future owners should focus more on personality and attachment aspects in the acquisition process instead. Compatibility between owners and their dogs may help unfold advantages of dog ownership, and prevent canine behavioral problems and their adverse consequences,” they concluded.



The study is published in the journal <a href="https://doi.org/10.1016/j.applanim.2023.105857">Applied Animal Behavior Science</a>.



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By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Dogs and their humans often share similar personalities

A new study led by the Max Planck Institute for...

A new study led by the <a href="https://www.ucla.edu/">University of California, Los Angeles</a> (UCLA) has found that global atmospheric <a href="https://www.earth.com/news/dust-asteroid-ice-age/">dust</a> (microscopic airborne particles from desert dust storms) has a small, yet significant cooling effect on our planet, which has hidden the full amount of warming caused by greenhouse gas emissions. According to the experts, the amount of desert dust has grown by 55 percent since the mid-19th century, thus increasing its cooling effect.



While some of the effects of atmospheric dust contribute to global warming, others counteract it - for instance, by scattering sunlight back into space and dissipating high clouds that warm the planet. Overall, the researchers estimate that dust has a cooling effect.



“We show desert dust has increased, and most likely slightly counteracted greenhouse warming, which is missing from current climate models,” said study lead author Jasper Kok, an atmospheric physicist at UCLA. “The increased dust hasn’t caused a whole lot of cooling - the climate models are still close - but our findings imply that greenhouses gases alone could cause even more climate warming than models currently predict.”



Besides its atmospheric interactions with sunlight and cloud cover, when dust falls back on the Earth’s surface, it can darken snow and ice, making them absorb more heat. In addition, dust also cools the planet by depositing nutrients such as phosphorous or iron into the oceans, which support the growth of phytoplankton that absorbs CO2 from the atmosphere, thereby causing a net cooling effect.



“We want climate projections to be as accurate as possible, and this dust increase could have masked up to eight percent of the greenhouse warming,” Kok explained. “By adding the increase in desert dust, which accounts for over half of the atmosphere’s mass of particulate matter, we can increase the accuracy of climate model predictions. This is of tremendous importance because better predictions can inform better decisions of how to mitigate or adapt to climate change.”



Although atmospheric desert dust levels have increased since the pre-industrial period, this trend has not been steady, and, since there are so many natural and human-caused variables which can cause dust levels to increase or decline, scientists cannot accurately project how the amount of dust will change during the following decades. Moreover, while the increase in atmospheric dust has somewhat masked the full potential of greenhouse gases to warm the climate, the findings do not show that existing climate models are wrong.



“The climate models are very useful in predicting future climate change, and this finding could further improve their usefulness,” Kok concluded.



The study is published in the journal <a href="https://www.nature.com/articles/s43017-022-00379-5">Nature Reviews Earth &amp; Environment</a>.



—



By <a href="mailto:andrei.ionescu5891@gmail.com">Andrei Ionescu</a>, <a href="https://www.earth.com/staff/">Earth.com</a> Staff Writer



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Atmospheric dust has been masking greenhouse warming

A new study led by the University of California, Los...

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



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



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



Video/ Image Credit: ESA



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

Nushagak Bay in southwest Alaska

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



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



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



Video/ Image Credit: American Chemical Society&nbsp;



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



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Flu viruses are more flexible than expected

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

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



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



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



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



Video/Image Credit: ESA&nbsp;



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

Lake Trasimeno in Central Italy

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



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



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



Video Credit: American Chemical Society&nbsp;



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



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Detecting mercury contamination with the tap of a finger

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

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Today’s Video of the Day from the <a href="https://www.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



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How does salt makes things taste better?

[sendtonews key="X0f6OHYoI4-2310561-12187" type="single"] Today’s Video of the Day from the...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features 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



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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



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Interactive map of the universe includes 200,000 galaxies

[sendtonews key="e4ZG0Jawp3-2374785-12187" type="single"] Astronomers at Johns Hopkins University have created...

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Lesotho: Africa's "Kingdom in the Sky" Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features northwest Lesotho in South Africa.



According to ESA, Lesotho is the only nation in the world that lies completely above 1,000 m in elevation. The country is famous for its tall mountains and narrow valleys, and is known as Africa's "Kingdom in the Sky."



Out of a population of around two million people, about 80 percent live in rural areas. More than 75 percent of these people are engaged in <a href="https://www.earth.com/news/climate-change-will-have-a-global-impact-on-agriculture/">agriculture</a>, including rainfed cereal production and animal grazing.&nbsp;



ESA reports that the country’s agricultural system faces a growing number of issues, with climate-related vulnerabilities such as drought, floods and extreme temperatures occurring more frequently. 



Diamonds are amongst the minerals found in the mountains. Indeed, Lesotho can truly be called the Kingdom in the Sky. Beautiful, culturally rich, safe, affordable, and easily accessible from Durban and Johannesburg, mountainous Lesotho is a vastly underrated travel destination. the Kingdom of Lesotho (Sotho: 'Muso oa Lesotho) is an enclaved country in southern Africa. It is just over 30,000 km2 (11,583 sq mi) in size and has a population of around 2 million.



Video Credit: ESA&nbsp;&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> Staff Writer 



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Lesotho: Africa's "Kingdom in the Sky"

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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



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The city of Dublin on Ireland's east coast

[sendtonews key="qjvhBOBnY8-2426650-12187" type="single"] Today's Video of the Day from the...

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Today's Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features 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



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The province of Zaragoza in northeast Spain

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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

[sendtonews key="0879czfG3k-1785905-12187" type="single"] Today’s Video of the Day from NASA...

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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

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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...

Today’s Video of the Day from the <a href="https://welcome.miami.edu/">University of Miami</a> Rosenstiel School of Marine and Atmospheric Science explores how changes in water temperatures have affected tiger shark habitats and movements in the North Atlantic Ocean. The study reveals that rising temperatures have caused the sharks to shift toward the poles over the past 40 years.



“Tiger shark annual migrations have expanded poleward, paralleling rising water temperatures,” explained study lead author Neil Hammerschlag. “These results have consequences for tiger shark conservation, since shifts in their movements outside of marine protected areas may leave them more vulnerable to commercial fishing.”



The researchers analyzed nine years of tracking data from satellite-tagged tiger sharks, combined with four decades of conventional tag and recapture data provided by National Oceanic and Atmospheric Administration (NOAA) Cooperative Shark Tagging Program.



The experts found that during the last decade of record heat, for every one-degree Celsius increase in water temperatures, tiger sharks migrated further poleward by over 400 kilometers. They also migrated two weeks earlier than usual to waters off the northeastern coast of the United States.



“Given their role as apex predators, these changes to tiger shark movements may alter predator-prey interactions, leading to ecological imbalances, and more frequent encounters with humans,” concluded Professor Hammerschlag.



Video Credit: University of Miami Rosenstiel School of Marine and Atmospheric Science



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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.

Tiger sharks are shifting poleward as temperatures rise

Today’s Video of the Day from the University of Miami...

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> is focused on the melt ponds that emerge during the spring and summer on the Greenland Ice Sheet, which is the largest ice mass in the northern hemisphere.



"Melt ponds are vast pools of open water that form on both sea ice and ice sheets and are visible as turquoise-blue pools of water in this Copernicus Sentinel-2 image," says ESA.



"When snow and ice melts atop glaciers, water flows in channels and streams and collects in depressions on the surface. These melt ponds can speed up the melting of the surrounding ice since they greatly reduce the ice’s ability to reflect sunlight."



"This can create a positive feedback where an increasing number of melt ponds absorb more heat which causes ice cover to melt even faster."



According to ESA, Greenland has been hit with a late-season heatwave that began in early September. This caused the type of melt event that usually occurs in the middle of summer.



"In a recent paper published in Nature Climate Change, scientists found that major sea-level rise from the melting of the Greenland ice cap is now ‘inevitable’ even if the burning of fossil fuels were to halt overnight," says ESA. "Using satellite observations of Greenland ice loss and ice cap from 2000 to 2019, the team found the losses will lead to a minimum rise of 27 cm regardless of climate change."



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.

Melt ponds on the Greenland Ice Sheet

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> describes a new map of Mars that is providing insight into the planet’s watery past. The map also reveals where future missions could safely land on Mars.&nbsp;



The map has been created over the last decade using observations of water-rich rocks and mineral deposits. The images were captured by ESA’s Mars Express and NASA’s Mars Reconnaissance Orbiter.



"A big surprise is the prevalence of these minerals, with the map revealing hundreds of thousands of water-affected locations in the oldest parts of the planet," says ESA. "The new data will help answer exciting questions about Mars’ climate history, whether water was globally persistent or confined to short, intense episodes, and whether the conditions were ever suitable for life."



"Specifically, the map shows the locations and abundances of aqueous minerals. These are from rocks that have been chemically altered by the action of water in the past, and have typically been transformed into clays and salts."



According to John Carter of the Institut d’Astrophysique Spatiale (IAS), our collective understanding of Mars has been oversimplified. He explained that planetary scientists have tended to think that only a few types of clay minerals on Mars were created during its wet period, then as the water gradually dried up, salts were produced across the planet.



The new map shows that the composition of Mars is much more complicated than what we thought. For example, while many salts formed after Martian clays, there are some salts that are presumed to be older than some of the clays.&nbsp;



“The evolution from lots of water to no water is not as clear cut as we thought, the water didn’t just stop overnight. We see a huge diversity of geological contexts, so that no one process or simple timeline can explain the evolution of the mineralogy of Mars. That’s the first result of our study. The second is that if you exclude life processes on Earth, Mars exhibits a diversity of mineralogy in geological settings just as Earth does,” said Carter.



Video 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 history of Mars is much more complex than we thought

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Today's Video of the Day from the <a href="https://www.stowers.org/">Stowers Institute for Medical Research</a> describes how cavefish adapted to a sedentary lifestyle over tens of thousands of years. 



The experts found that the muscle metabolism of cavefish has been genetically reprogrammed over time. As a result, the animals have experienced major changes in their morphology and behavior. Despite these changes, however, the cavefish remain healthy and fit.



The research may provide new clues about the evolutionary consequences of prolonged physical inactivity in humans.&nbsp;



“It’s no surprise that people are moving less and less as technology has advanced,” said Rohner. “With cavefish, we have a unique system where we can study what might happen if people remained couch potatoes over very, very long periods of time.”



Video Credit: Stowers Institute for Medical Research



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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.

Cavefish are healthy despite their sedentary lifestyle

[sendtonews key="vpljfR2VBX-2560867-12187" type="single"] Today's Video of the Day from the...

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Today’s Video of the Day from <a href="https://earthobservatory.nasa.gov/">NASA Earth Observatory</a> some of the most incredible waves in the world, as seen by Landsat satellites.



"With more than 370,000 miles of coastline on Earth, there are plenty of places where epic waves build up, curl over, and hurtle toward the shore.- much to the thrill of surfers," says NASA. "There are some places where these waves are so magnificent that they can be seen from space."



"With the broad perspective of satellites, we can see how these iconic waves develop into the world’s tallest, longest, fastest, and heaviest."



Video Credit: NASA Earth Observatory&nbsp;



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



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Satellites capture the world's biggest and fastest waves

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> describes why satellite images and measurements of our planet have become "essential to our survival, offering a new outlook of our world."&nbsp;



Rising sea levels pose one of the biggest societal threats associated with climate change. According to ESA, satellite altimeter missions such as Copernicus Sentinel-6 are essential in monitoring global and regional changes in sea level.



"Unbeknown to many, the island of Crete, Greece, plays an important role in the Copernicus satellite altimetry constellation and on an international stage," reports ESA.



"Satellite altimetry data have to be continuously monitored at the ESA’s Permanent Facility for Altimetry Calibration where different techniques have pioneered the use of transponders to provide the best measurements to validate satellite altimeters in space soon after launch."



Dr. Craig Donlon explains that, by understanding planet Earth through satellite measurements, we are able to find evidence of change.&nbsp;



Video Credit: European Space Agency&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

Satellites have become essential to our survival

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