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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

[sendtonews key="oL4FnPTGCV-2384527-12187" type="single"] Today's Video of the Day from the European Space Agency 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...

This,Man-made,Vehicle,Reached,A,Record,Speed,Of,635,Thousand

NASA’s Parker Solar Probe is set to achieve its most dangerous feat yet tomorrow, December 24, 2024. After a six-year journey of spiraling closer to the star at the heart of our solar system, the spacecraft is expected to come within 3.8 million miles of the Sun’s surface. 



This tiny distance in cosmic terms lets scientists capture a new type of information, revealing secrets about solar winds, extreme heat, and magnetic fields.



<h2 class="wp-block-heading" id="h-solar-probe-on-the-sun-s-doorstep">Solar probe on the Sun's doorstep</h2>



Engineers have spent years carefully adjusting <a href="https://blogs.nasa.gov/parkersolarprobe/" target="_blank" rel="noreferrer noopener">Parker’s flight path</a> using multiple Venus gravity assists. These flybys reshape the spacecraft’s orbit and tighten its looping path around the Sun. “This is one example of NASA’s bold missions, doing something that no one else has ever done before to answer longstanding questions about our universe,” explained <a href="https://science.nasa.gov/people/dr-arik-posner/" target="_blank" rel="noreferrer noopener">Arik Posner</a>, Parker Solar Probe program scientist at NASA Headquarters, describing this mission’s significance.



Ever since the launch in 2018, Parker’s main goal has been to study the Sun’s outer atmosphere, known as the corona. Tomorrow’s approach, often called <a href="https://cneos.jpl.nasa.gov/glossary/perihelion.html" target="_blank" rel="noreferrer noopener">perihelion</a>, marks a new milestone in that quest. The probe moves at speeds around 430,000 miles per hour, faster than any other spacecraft. At such high velocity, it can swing around our star without getting swallowed. Even so, mission managers won’t receive immediate updates once Parker hits its closest point because signals cannot travel through the intense solar environment.



<h2 class="wp-block-heading" id="h-extreme-heat-and-lasting-protection">Extreme heat and lasting protection</h2>



What sets Parker apart is its resilient heat shield. This 4.5-inch-thick carbon-composite barrier enables the spacecraft’s instruments to continue functioning in an environment where temperatures can reach roughly 2,500 degrees Fahrenheit. Despite the harsh surroundings, the precious science instruments remain near room temperature, thanks to expert engineering by Johns Hopkins University Applied Physics Laboratory (<a href="https://parkersolarprobe.jhuapl.edu/" target="_blank" rel="noreferrer noopener">APL</a>).



During every close approach, Parker is pelted by gusts of solar wind and bathed in radiation. Still, it keeps sending back readings about magnetic fields, <a href="https://www.plasmacoalition.org/plasma_writeups/solar_plasmas.pdf" target="_blank" rel="noreferrer noopener">plasma</a> behavior, and energetic <a href="https://www.swpc.noaa.gov/phenomena/solar-radiation-storm#:~:text=Solar%20radiation%20storms%20occur%20when,of%20the%20speed%20of%20light." target="_blank" rel="noreferrer noopener">particles</a>. The probe’s data illuminates reasons behind the corona’s blazing heat, which can climb into the millions of degrees, significantly hotter than the visible surface of the Sun. Such puzzling behavior has fascinated scientists for decades.



<h2 class="wp-block-heading" id="h-chasing-the-solar-wind-s-origins">Chasing the solar wind’s origins</h2>



Solar wind, a stream of charged particles flowing away from the Sun at speeds topping one million miles per hour, plays a major role in <a href="https://science.nasa.gov/sun/what-is-the-solar-wind/">space weather</a>. 



By skimming through the corona, Parker records fresh evidence of how these particles speed up and scatter across the solar system. The answers may help experts forecast disturbances that affect satellites and astronaut safety. Surges of these charged particles can disable communication systems or even disrupt power grids on Earth.



For researchers, big questions remain. How does the <a href="https://science.nasa.gov/sun/what-is-the-solar-wind/">solar wind</a> pick up its pace so dramatically? Is there a specific region in the corona that triggers bursts of fast-moving particles? 



Parker’s measurements bring us closer to unraveling these mysteries. Officials at NASA say that by tomorrow’s approach, new layers of data will help them see patterns not possible to detect from a greater distance.



<h2 class="wp-block-heading" id="h-solar-probe-and-the-sun-s-active-cycle">Solar probe and the Sun's active cycle</h2>



The Sun moves through an 11-year activity cycle. Right now, it is in an active phase, meaning increased sunspots, <a href="https://www.earth.com/news/secondary-peak-extreme-geomagnetic-solar-storm-expected-today/" target="_blank" rel="noreferrer noopener">solar flares</a>, and <a href="https://www.swpc.noaa.gov/phenomena/coronal-mass-ejections" target="_blank" rel="noreferrer noopener">coronal mass ejections</a>. 



Researchers are tracking not only Parker’s journey but also the Sun’s changing patterns. Sometimes these outbursts interact with Earth’s magnetosphere and spark colorful auroras, even in places unused to such displays. And although most solar weather events are harmless for life on Earth, severe storms can interfere with GPS systems or satellites.



This is why Parker’s findings are so relevant. Gaining a better understanding of how energetic solar events begin could lead to timelier warnings, giving operators on Earth a heads-up to power down sensitive instruments or adjust satellite orbits.



<h2 class="wp-block-heading" id="h-paying-tribute-to-eugene-parker">Paying tribute to Eugene Parker</h2>



In 2017, NASA renamed the probe after <a href="https://news.uchicago.edu/story/eugene-parker-legendary-figure-solar-science-and-namesake-parker-solar-probe-1927-2022">Dr. Eugene N. Parker</a>, the first person to predict the solar wind in the 1950s. He introduced key ideas about how stars interact with their surroundings. The mission’s name honors his influential work. Dr. Parker passed away in 2022, but his legacy continues. 



The data this spacecraft is sending back not only expands knowledge of <a href="https://www.earth.com/news/tracing-solar-wind-directly-to-its-source-for-the-first-time/" target="_blank" rel="noreferrer noopener">solar physics</a> but also shows how correct Dr. Parker’s early theories were.



<h2 class="wp-block-heading" id="h-record-setting-solar-probe-flyby">Record-setting Solar Probe flyby</h2>



Mission operations expect Parker to reach perihelion at 6:53 a.m. EST on December 24. 



At that time, the spacecraft will run autonomously, and engineers at APL will wait until December 27 for a beacon tone confirming a safe passage around the Sun. “No human-made object has ever passed this close to a star, so Parker will truly be returning data from uncharted territory. We’re excited to hear back from the spacecraft when it swings back around the Sun,” explained <a href="https://parkersolarprobe.jhuapl.edu/News-Center/Show-Article.php?articleID=205" target="_blank" rel="noreferrer noopener">Nick Pinkine</a>, Parker Solar Probe mission operations manager. 



When that update arrives, scientists will study Parker’s recent measurements to identify potential clues about solar wind origins and coronal heating. Each orbit is another chance to witness the scorching conditions near our star. At the same time, the probe helps refine predictions about solar eruptions that might drive future storms toward Earth.



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



Beyond the scientific breakthroughs, Parker’s success can have practical benefits for technology we rely on every day. Our society depends on GPS signals and stable power systems, and <a href="https://www.earth.com/news/team-creates-video-showing-the-sun-in-gamma-rays-over-a-14-year-period/" target="_blank" rel="noreferrer noopener">major solar events</a> can disrupt both. By learning how to anticipate strong solar winds or flares, experts might one day keep satellites out of harm’s way or shield power grids from unexpected surges.



Tomorrow’s close approach continues a streak of remarkable achievements for NASA. As Parker zips through the corona, it gathers observations that no other mission could obtain. The craft appears ready for another sizzling pass, thanks to the robust thermal design and careful planning. 



Whether it’s helping forecast solar tempers or refining our knowledge of basic astrophysical processes, Parker remains on track to change the way we see the Sun.



Learn more about <a href="https://science.nasa.gov/mission/parker-solar-probe/" target="_blank" rel="noreferrer noopener">NASA's Parker Solar Probe here...</a>



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Spacecraft will fly through the Sun's atmosphere tomorrow for the first time ever

NASA’s Parker Solar Probe is set to achieve its most...

Bright,,Red-dark,Quasar,In,Deep,Space.,Elements,Of,This,Image

Astronomers have identified a remarkable water reservoir hidden in a corner of the cosmos, circling a quasar more than 12 billion light-years away.



At that distance, the light we see today began its journey not too long after the universe itself formed. 



The water supply in this distant place is huge, containing the equivalent of about 140 trillion times all the water in Earth’s oceans combined.



This supply is sitting near a supermassive black hole that is about 20 billion times more massive than our sun. 



<a href="https://www.earth.com/news/oldest-black-hole-ever-discovered-dates-back-to-the-dawn-of-time/" target="_blank" rel="noreferrer noopener">The black hole</a> is surrounded by a quasar named APM 08279+5255, which pumps out as much energy as a thousand trillion suns. 



This quasar, according to astronomers, holds the farthest and largest known reservoir of water anywhere in the universe.



<h2 class="wp-block-heading" id="h-quasar-apm-08279-5255-and-its-water">Quasar APM 08279+5255 and its water</h2>



Matt Bradford, a scientist at NASA’s <a href="https://www.jpl.nasa.gov/" target="_blank" rel="noreferrer noopener">Jet Propulsion Laboratory</a> in Pasadena, Calif., leads one of the teams involved in the observations.



“The environment around this quasar is very unique in that it’s producing this huge mass of water,” said Matt Bradford. “It’s another demonstration that water is pervasive throughout the universe, even at the very earliest times.”



Both Bradford’s group and a separate team of astronomers studied APM 08279+5255 and its <a href="https://www.earth.com/news/massive-black-hole-is-seen-taking-a-nap-after-eating-too-much/" target="_blank" rel="noreferrer noopener">black hole</a>, which sits at the center and draws matter inward. 



As it does, it warms the surrounding gas and dust, forming an area filled with molecules that have never before been detected at such an immense distance.



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



Quasars were first noticed more than half a century ago when telescopes revealed puzzling sources of intense brightness in <a href="https://www.earth.com/news/hubble-took-the-closest-ever-image-of-a-quasar-and-captured-some-weird-things/" target="_blank" rel="noreferrer noopener">distant areas of space</a>. 



These objects are unlike any ordinary star. They shine brightly from the center of distant galaxies, outshining all their galaxy’s stars combined.



At their heart sit supermassive black holes, millions or billions of times heavier than our sun. As gas and dust spiral in toward one of these black holes, the swirling material heats up and <a href="https://www.earth.com/news/black-hole-jet-crashes-into-an-unidentified-object/" target="_blank" rel="noreferrer noopener">releases energy</a>. 



This energy blasts out across all kinds of wavelengths, making quasars some of the brightest, most energetic phenomena ever seen.



Observing quasars helps astronomers understand what the universe looked like long ago, since the light we see now began its journey billions of years in the past. 



Quasars can show how galaxies formed, how matter spread out, and how the earliest structures in the cosmos came together.



They can even help map the distribution of matter between galaxies, shining light on the regions that would otherwise remain unseen. 



Some quasars also launch <a href="https://www.earth.com/news/black-hole-jets-are-like-million-light-year-long-jedi-lightsabers/" target="_blank" rel="noreferrer noopener">huge jets of high-speed particles</a> that stretch across enormous distances. These jets can affect how stars form, influencing entire neighborhoods of cosmic material.



<h2 class="wp-block-heading" id="h-strange-place-to-find-water">Strange place to find water</h2>



Astronomers observed that water vapor is present in this quasar’s environment. It occupies a region spanning hundreds of light-years, with one light-year at around six trillion miles. 



Although the gas is thin by Earth standards, it is surprisingly warm and dense compared to what is typical in places like our <a href="https://www.earth.com/news/milky-ways-black-hole-formed-through-a-merger/" target="_blank" rel="noreferrer noopener">Milky Way</a>.



The temperature hovers around minus 63 degrees Fahrenheit, and the gas is roughly 300 trillion times less dense than Earth’s atmosphere. 



Still, it is about five times hotter and tens to hundreds of times denser than the gas seen in normal galaxies. With its unusual conditions, this region stands out as an unexpected find.



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



<a href="https://www.earth.com/news/oceans-of-water-vapor-may-be-involved-in-planet-formation/" target="_blank" rel="noreferrer noopener">Water vapor</a> is not just a molecule. Its presence here suggests that the quasar is bathing its environment in radiation that keeps the gas relatively warm. 



Astronomers also spotted other molecules, like carbon monoxide, hinting that there is an abundance of raw material that can feed the black hole as it continues to grow.



They estimate that there is enough gas for the <a href="https://www.earth.com/news/largest-map-of-supermassive-black-holes-unveiled/" target="_blank" rel="noreferrer noopener">black hole</a> to increase in size by about six times, although what actually happens next is not certain. 



Some of this gas may form new stars, while some might be thrown out into space instead. Either way, these measurements open a window into what conditions were like when the universe was still young.



<h2 class="wp-block-heading" id="h-quasars-water-and-life-s-building-blocks">Quasars, water, and life's building blocks</h2>



Detecting water vapor in such a distant quasar expands our knowledge of how <a href="https://www.earth.com/news/did-the-building-blocks-of-life-replicate-on-their-own/" target="_blank" rel="noreferrer noopener">building blocks</a> appear across vast stretches of time and space. 



Water is essential for life as we know it, and its presence billions of years ago suggests that the elements needed for life have been around for a very long time.



Beyond that, water plays a key role in shaping how stars and galaxies evolve. When gas clouds cool, water helps by allowing those clouds to collapse more easily, leading to star birth. 



By spotting it this far back, astronomers get new clues about how galaxies changed as the universe aged and matured.



<h2 class="wp-block-heading" id="h-how-they-found-the-water-quasar">How they found the water quasar</h2>



Bradford’s team began collecting data in 2008 with an instrument called Z-Spec at the California Institute of Technology’s Submillimeter Observatory (<a href="https://www.cso.caltech.edu/" target="_blank" rel="noreferrer noopener">CSO</a>). 



This 33-foot telescope sits near the summit of Mauna Kea in Hawaii. They later confirmed their findings using the Combined Array for Research in Millimeter-Wave Astronomy (<a href="https://www.mmarray.org/" target="_blank" rel="noreferrer noopener">CARMA</a>), a set of radio dishes located high in the Inyo Mountains of Southern California.



Meanwhile, another group led by Dariusz Lis, senior research associate in physics at Caltech and deputy director of the Caltech Submillimeter Observatory, used the Plateau de Bure Interferometer in the French Alps. 



In 2010, Lis’s team found hints of water in this quasar by detecting a single signature, while Bradford’s team uncovered multiple signals that revealed the massive amount of water present.



<h2 class="wp-block-heading" id="h-where-do-we-go-from-here">Where do we go from here?</h2>



To sum it all up, this discovery shows that even at a time when the universe was young, water formed and gathered in places we never would have guessed. 



Instead of seeing just cold, empty darkness out there, astronomers have spotted a real treasure -- an enormous reservoir of water swirling around a quasar more than 12 billion light-years away. 



This water vapor, along with the intense radiation from the black hole at the quasar’s center, paints a picture of an environment that is far denser, warmer, and more active than ordinary parts of the cosmos.



By studying this distant quasar, scientists can learn how the earliest galaxies came together and evolved. They can see how matter spread out, how black holes grew, and how even tiny molecules like water played a role in shaping the universe. 



Every new detail uncovered by these long-ago signals traveling through time and space helps make sense of the vast cosmic story we are all a part of.



***



Other authors on the Bradford paper, "The water vapor spectrum of APM 08279+5255," include Hien Nguyen, Jamie Bock, Jonas Zmuidzinas and Bret Naylor of JPL; Alberto Bolatto of the University of Maryland, College Park; Phillip Maloney, Jason Glenn and Julia Kamenetzky of the University of Colorado, Boulder; James Aguirre, Roxana Lupu and Kimberly Scott of the University of Pennsylvania, Philadelphia; Hideo Matsuhara of the Institute of Space and Astronautical Science in Japan; and Eric Murphy of the Carnegie Institute of Science, Pasadena. Funding for Z-Spec was provided by the <a href="https://www.nsf.gov" target="_blank" rel="noreferrer noopener">National Science Foundation</a>, <a href="https://www.nasa.gov" target="_blank" rel="noreferrer noopener">NASA</a>, the Research Corporation and the partner institutions.



The full study was published in the <a href="https://iopscience.iop.org/article/10.1088/2041-8205/738/1/L6/meta" target="_blank" rel="noreferrer noopener">Astrophysical Journal Letters</a>.



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Enough water to fill trillions of Earth's oceans found in deep space circling a black hole

Astronomers have identified a remarkable water reservoir hidden in a...

Cosmic rays are high-speed particles that move through space and crash into our atmosphere from every direction. These energetic particles, mostly atomic nuclei stripped of their electrons, have puzzled scientists for decades.



They hit Earth from different places with a wide range of energies. Some arrive at moderate levels, while others carry so much punch that researchers use special detectors stretching over vast areas to understand their true nature.



<h2 class="wp-block-heading" id="h-cosmic-rays-above-5-eev">Cosmic rays above 5 EeV</h2>



Particles carrying more than about five <a href="https://pwg.gsfc.nasa.gov/Education/wenpart1.html" target="_blank" rel="noreferrer noopener">exa-electronvolts</a> (EeV) of energy stand out because they mark a turning point. 



At lower energies, cosmic rays often show a smoother distribution, and are strongly influenced by magnetic fields in our own galaxy.



Once they cross the 5 EeV threshold, however, their behavior and properties change. They begin to show patterns that cannot be explained by local sources alone. 



Instead of originating mostly from within the Milky Way, they appear to come from distant corners of the cosmos that lie far beyond our familiar galactic neighborhood.



Studies indicate that at these energies, called <a href="https://arxiv.org/pdf/2412.05974" target="_blank" rel="noreferrer noopener">the ankle region</a>, the usual mixture of mostly light nuclei, like protons, gradually gives way to heavier particles that are less scrambled by <a href="https://ui.adsabs.harvard.edu/abs/2013pss5.book..641B/abstract" target="_blank" rel="noreferrer noopener">galactic magnetic fields</a>.



According to <a href="https://www.researchgate.net/profile/Jonathan-Biteau" target="_blank" rel="noreferrer noopener">Jonathan Biteau</a>, from the Academic Institute of France's <a href="https://www.auger.org/collaboration/" target="_blank" rel="noreferrer noopener">Pierre Auger Collaboration</a>, this energy range represents a step into a more revealing territory.



<h2 class="wp-block-heading" id="h-observing-signs-in-the-data">Observing signs in the data</h2>



Changes in the large-scale patterns of cosmic rays <a href="https://www.earth.com/news/cosmic-rays-help-archaeologists-determine-age-discoveries-prehistoric-settlements/" target="_blank" rel="noreferrer noopener">seen across the sky</a> start to stand out and offer clues to their sources. 



This is where the cosmic ray story moves beyond a random spray of particles and hints at something else: extragalactic origins with distinct characteristics.



"Cosmic rays begin to reveal their secrets at energies above 5 EeV," said Biteau.



Measurements gathered over many years at facilities like the Pierre Auger Observatory show that once energies climb past this point, a pattern emerges in the shape of the energy spectrum.



Distinct features, known as the ankle near 5 EeV, the instep at about 15 EeV, and the toe around 45 EeV, mark noticeable shifts in the composition of the flux.



<h2 class="wp-block-heading" id="h-clues-to-sources-of-cosmic-rays">Clues to sources of cosmic rays</h2>



Observations <a href="https://arxiv.org/abs/2008.06486" target="_blank" rel="noreferrer noopener">indicate</a> that heavier nuclei start dominating the picture at higher energies. These changes tell researchers that different acceleration processes and astrophysical environments might be at play.



As energies increase, the sky coverage reveals that some directions supply more cosmic rays than others. This nonuniformity, known as anisotropy, has become more apparent.



Over the past decade, scientists have reported that the pattern of cosmic-ray arrival directions changes in a way that strongly suggests extragalactic sources. 



<a href="https://www.science.org/doi/10.1126/science.aan4338" target="_blank" rel="noreferrer noopener">Research</a> shows a large-scale anisotropy above a few EeV rising to a significance of about 7 σ above 8 EeV.



<h2 class="wp-block-heading" id="h-one-step-closer">One step closer</h2>



Pinpointing the birthplaces of these high-energy particles has proved challenging, but scientists continue to gather clues. 



As cosmic rays push into these higher energy realms, they are less scattered by magnetic fields, making it easier to identify their original directions.



Emerging <a href="https://arxiv.org/abs/1612.07155" target="_blank" rel="noreferrer noopener">evidence</a> supports the idea that many of these ultra-high-energy rays are launched by extragalactic sources like star-forming galaxies or other intense astrophysical sites.



The data hint that active regions far beyond our galaxy could be connected to the observed arrival patterns.



Researchers also notice that certain sky regions, like those associated with clusters of nearby galaxies, line up better with the arrival directions than a purely uniform spread would allow.



<h2 class="wp-block-heading" id="h-shifts-in-cosmic-rays-composition">Shifts in cosmic rays' composition</h2>



Stepping above 5 EeV not only shines a light on extragalactic origins but also shows that the “stuff” hitting us at these energies is different.



Instead of mostly light nuclei like hydrogen and helium, many cosmic rays are heavier, involving atoms like carbon or oxygen.



This suggests that whatever "engines" are producing them, they must either selectively accelerate heavier particles or conditions in their environment alter the mix by the time they reach Earth.



The surprising scarcity of lighter elements runs counter to earlier guesses and requires fresh thinking from theorists.



<h2 class="wp-block-heading" id="h-what-holds-the-key-to-their-birthplaces">What holds the key to their birthplaces?</h2>



As these rays travel huge distances, their paths bend slightly in <a href="https://www.earth.com/news/powerful-magnetic-fields-may-be-key-features-of-black-holes/">magnetic fields</a> along the way. Even tiny bends can shuffle their directions enough to complicate efforts to pinpoint sources.



To address this, scientists model how nuclei of different masses respond to magnetic fields. If the rays still show a pattern that points to certain neighborhoods in space, that strengthens the argument that those regions contain the engines fueling these incredible energies.



<h2 class="wp-block-heading" id="h-no-single-culprit-yet">No single culprit yet</h2>



Many questions remain. Some experts suggest star-forming galaxies as prime suspects since these environments can host energetic events that might whip particles up to extreme energies.



Others consider whether active galactic nuclei, powered by <a href="https://astronomy.swin.edu.au/cosmos/S/Supermassive+Black+Hole" target="_blank" rel="noreferrer noopener">supermassive black holes</a>, might do the trick.



Current evidence favors the idea that star-forming galaxies provide a better match to the observed patterns than other candidates, but that does not slam the door on other possibilities.



<h2 class="wp-block-heading" id="h-bridging-theory-and-observations">Bridging theory and observations</h2>



The unusual composition and the changing patterns seen above 5 EeV push theorists to re-examine old ideas. 



Traditional models that relied on smooth distributions of particle energies and the presence of light nuclei are under pressure.



New models must explain the sharp transitions, the heavy nuclei, and the hints of extragalactic origins. As measurements improve, scientists hope to confirm or refute certain types of sources. 



If future data link cosmic rays more closely to certain types of galaxies or astrophysical conditions, it would be a major step forward in understanding how the universe’s most energetic particles are made.



<h2 class="wp-block-heading" id="h-ongoing-upgrades-and-the-future">Ongoing upgrades and the future</h2>



As detectors improve and more data are collected, the community expects to refine the energy calibration, measure more showers, and achieve better accuracy. Each improvement adds detail to this cosmic jigsaw puzzle.



If a tighter correlation with certain galaxy groups emerges, that could finally close in on the actual sources. Until then, each new measurement, each new analysis, and each new insight keeps the hunt alive.



The research paper was published in the <a href="https://journals.aps.org/prd/abstract/10.1103/PhysRevD.102.062005" target="_blank" rel="noreferrer noopener">Physical Review Journals</a>.



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Strange, high-energy cosmic rays: Did something outside our galaxy send them here?

Cosmic rays are high-speed particles that move through space and...

Humanity faces an urgent need for change to prevent biodiversity loss and the continued destruction of our planet. The UN biodiversity expert panel's latest "transformative change" report highlights the dire need for radical societal shifts.



Released Wednesday by the Intergovernmental Science-Policy Platform on Biodiversity and Ecosystem Services (IPBES), the report calls for immediate action to address overconsumption, wealth concentration, and humanity's growing disconnection from nature.



"It is not just governments. It is not just business. It is not just civil society. It is all of us. We all need to work together," said Arun Agrawal, one of the report’s lead authors.



While transformative action may seem challenging, the report emphasizes that it is achievable. Here’s a closer look at three inspiring examples of successful transformations from around the world.



<h2 class="wp-block-heading" id="h-reviving-marine-ecosystems-os-minarzos-model">Reviving marine ecosystems: "Os Minarzos" model</h2>



In 2002, Spain suffered a severe ecological disaster when the Prestige oil tanker broke apart, spilling massive amounts of oil into the Atlantic Ocean. 



This environmental catastrophe devastated Galicia's coastline, causing significant <a href="https://www.earth.com/news/polar-light-sustains-biodiversity-over-millions-of-years/" target="_blank" rel="noreferrer noopener">biodiversity</a> loss and severely affecting marine life and the livelihoods of local fishing communities.



In response, the communities in Galicia decided to adopt a new approach to marine reserve management, called the "Os Minarzos" model.



<h2 class="wp-block-heading" id="h-advantages-of-the-model">Advantages of the model</h2>



This innovative strategy brought together fishers, scientists, and local authorities to collaboratively restore and protect the marine ecosystem. 



The model emphasized sustainable fishing practices, scientific guidance, and community involvement - promoting cooperation among all stakeholders.



Although the transition faced challenges, including initial disagreements and tensions, the initiative became a long-term success. 



Over time, the "Os Minarzos" model led to healthier marine ecosystems, improved fishing practices, and increased <a href="https://www.earth.com/news/new-solutions-for-the-climate-and-biodiversity-crisis/" target="_blank" rel="noreferrer noopener">biodiversity</a>. Local fishers also experienced higher incomes, while trust and cooperation within the community strengthened significantly.



The model’s impact extended far beyond Galicia. It inspired international guidelines for sustainable marine management and influenced networks of over 20 million fishers across Europe and the Americas. 



<h2 class="wp-block-heading" id="h-technology-to-prevent-biodiversity-loss">Technology to prevent biodiversity loss</h2>



In China, the Ant Forest mobile application has become a <a href="https://www.earth.com/news/urban-biodiversity-is-not-a-luxury-it-is-attainable-for-everyone/" target="_blank" rel="noreferrer noopener">powerful tool</a> for promoting eco-friendly habits and environmental restoration. 



Launched in 2016, this innovative app encourages users to adopt sustainable behaviors, such as walking or cycling instead of driving, and cutting down on plastic and paper usage. 



For every eco-friendly action, users earn "green energy points" in the app, which accumulate to grow a virtual tree. Each virtual tree is then matched with the planting of a real tree.



The initiative has made a significant impact. Since its inception, Ant Forest has planted an astounding 548 million trees across 13 provinces in China. This reforestation effort not only helps combat climate change but also addresses environmental degradation in vulnerable areas.



Beyond its environmental benefits, the project has also provided economic opportunities. It has created jobs in eco-agriculture and ecotourism, particularly in rural regions struggling with environmental challenges. 



<h2 class="wp-block-heading" id="h-community-led-conservation">Community-led conservation</h2>



The <a href="https://www.nashulai.com" target="_blank" rel="noreferrer noopener">Nashulai Maasai Conservancy</a> in Kenya is a pioneering example of how traditional knowledge and community engagement can drive effective <a href="https://www.earth.com/news/what-are-the-biggest-drivers-of-biodiversity-loss/" target="_blank" rel="noreferrer noopener">conservation</a>. 



This initiative blends the wisdom of indigenous practices with modern approaches to tackle multiple challenges, including species protection, income generation, and climate change mitigation.



The conservancy adopts a holistic strategy by establishing community-managed protected areas. These areas not only safeguard wildlife and combat biodiversity loss but also involve local communities in activities like river cleaning and tree planting. 



Such efforts improve environmental health while addressing the needs of the people living in the region.



This collaborative approach has transformed Nashulai into a thriving habitat where both humans and wildlife coexist harmoniously. By empowering local communities and integrating ecological restoration with socio-economic benefits, Nashulai exemplifies how conservation can work in harmony with human development.



"Over a very short period of time, biodiversity reappeared," said Karen O’Brien, another lead author of the report. "The power of community, again and again in our examples, is important."



<h2 class="wp-block-heading" id="h-addressing-biodiversity-loss">Addressing biodiversity loss</h2>



The <a href="https://www.un.org/en/" target="_blank" rel="noreferrer noopener">UN</a> report highlights the interconnectedness of ecological, social, and economic challenges - offering a blueprint for action.



Addressing biodiversity loss and ecosystem collapse requires collective effort. "It is all of us. We all need to work together," said Agrawal.



These stories from Galicia, China, and Kenya show that transformation is not only possible but can yield tangible benefits. 



Whether through community-driven conservation, innovative technology, or collaborative governance, humanity has the tools to make a <a href="https://www.earth.com/news/animal-tracking-is-crucial-for-preserving-biodiversity/" target="_blank" rel="noreferrer noopener">difference</a>. The question is whether or not we will rise to the challenge.



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UN report calls for global change to stop biodiversity loss

Humanity faces an urgent need for change to prevent biodiversity...

Mars,Inner,Structure.,Elements,Of,This,Image,Furnished,By,Nasa

A fresh look inside Mars suggests that what lurks far beneath its dusty surface might change how we think about water on the Red Planet.



Evidence emerging from <a href="https://www.pnas.org/doi/10.1073/pnas.2409983121" target="_blank" rel="noreferrer noopener">research</a> published in the Proceedings of the National Academy of Sciences indicates that liquid water is sequestered deep under the Red Planet's surface, locked in cracks and pores.



Scientists say there could be enough of it to blanket the entire planet under about a mile of ocean. This revelation challenges the old assumption that most of Mars water vanished into space billions of years ago.



Instead, a substantial portion of it may never have left at all -- remaining present deep underground.



<h2 class="wp-block-heading" id="h-subterranean-secrets">Subterranean secrets</h2>



Deep beneath the barren landscape, seismic readings gathered by NASA’s <a href="https://science.nasa.gov/mission/insight" target="_blank" rel="noreferrer noopener">InSight mission</a> support the idea of an immense, hidden reservoir. 



Researchers from the <a href="https://www.berkeley.edu/" target="_blank" rel="noreferrer noopener">University of California, Berkeley</a>, and <a href="https://ucsd.edu/" target="_blank" rel="noreferrer noopener">UC San Diego</a> honed in on signals from Mars's quakes, meteor strikes, and volcanic murmurs to map what lies below.



By interpreting how these waves traveled through different layers, the team found that the presence of water-soaked rock best explains the data.



The <a href="https://www.forbes.com/sites/roberthart/2024/08/12/scientists-discover-oceans-worth-of-liquid-water-on-mars-and-a-potential-home-for-alien-life-but-theres-one-big-catch/">findings</a> suggest that liquid is trapped in tiny fissures deep underground. According to Manga, a hidden water supply far below the Martian surface is hardly an inhospitable zone.



“I don't see why [the underground water] is not a habitable environment,” said <a href="https://eps.berkeley.edu/people/michael-manga" target="_blank" rel="noreferrer noopener">Michael Manga</a>, a professor of earth and planetary science at UC Berkeley.



<h2 class="wp-block-heading" id="h-mars-water-and-potential-for-life">Mars water and potential for life</h2>



No direct biosignatures have ever emerged from Mars, yet the notion of a suitable habitat underground tempts the imagination. 



Organisms on Earth survive at crushing depths and in pitch-black caverns. Similar conditions might exist beneath Mars’s crust.



“We haven't found any evidence for <a href="https://www.earth.com/news/insights-alien-life-mars-water-sulfur-discovered-gained-studying-extreme-life-earth/">life on Mars</a>, but at least we have identified a place that should, in principle, be able to sustain life,” Manga explained.



Even so, confirming anything alive down there is a tall order, and any future attempt to reach these elusive waters would stretch engineering know-how to its limit.



<h2 class="wp-block-heading" id="h-deep-drilling-and-tough-odds">Deep drilling and tough odds</h2>



Though the newfound reservoir might hold riches of scientific interest, it also resides at depths of about 7 to 13 miles (11 to 21 kilometers). 



On Earth, drilling down that far is beyond current engineering capabilities. The <a href="https://www.theguardian.com/world/2023/jun/06/china-begins-drilling-one-of-worlds-deepest-holes-in-hunt-for-discoveries-deep-inside-the-earth" target="_blank" rel="noreferrer noopener">Kola Superdeep Borehole</a> in Russia, the deepest hole ever created by humans, reached just over 7.6 miles (12 kilometers).



Tapping the <a href="https://www.earth.com/news/mars-has-a-water-reservoir-two-miles-deep-enough-to-fill-earths-red-sea/" target="_blank" rel="noreferrer noopener">Martian water supply</a>, which sits deeper, looks virtually impossible with the technology we have today. 



This puts a damper on visions of settlers using these waters as a resource anytime soon. Mars may be water-rich underground, but those riches are locked away.



<h2 class="wp-block-heading" id="h-clues-from-the-past">Clues from the past</h2>



Long ago, Mars likely resembled a wetter place. Orbital imaging and rover missions have <a href="https://www.nasa.gov/news-release/nasa-confirms-evidence-that-liquid-water-flows-on-todays-mars/" target="_blank" rel="noreferrer noopener">revealed</a> surface features that point to a time when rivers and lakes carved out the terrain. 



Geological evidence indicates that liquid water helped <a href="https://www.earth.com/news/freya-castle-rock-with-black-and-white-stripes-found-on-mars-has-nasa-excited/">form certain minerals</a>.



Scientists have struggled to explain what happened when Mars lost its thick atmosphere, which once prevented surface water from vaporizing into space. 



These new findings hint that large portions of the planet’s original water supply did not vanish entirely. Instead, it may have seeped deep into the planet's crust, remaining there ever since.



<h2 class="wp-block-heading" id="h-window-into-martian-history">Window into Martian history</h2>



Wright, who contributed to understanding Mars’s current water distribution, stressed the significance of knowing how much and where liquid exists today.&nbsp;



“Understanding the Martian water cycle is critical for understanding the evolution of the climate, surface and interior. 



A useful starting point is to identify where water is and how much is there,” said <a href="https://vwright.scrippsprofiles.ucsd.edu/" target="_blank" rel="noreferrer noopener">Vashan Wright</a>, assistant professor at UC San Diego’s <a href="https://scripps.ucsd.edu/" target="_blank" rel="noreferrer noopener">Scripps Institution of Oceanography</a>.



Peering into this underground reservoir offers a rare glimpse into ancient processes that shaped the Red Planet. It may explain why Mars shifted from a wet environment to a cold, dry world.



<h2 class="wp-block-heading" id="h-water-on-mars-and-future-study">Water on Mars and future study</h2>



The InSight mission, which ended in 2022, recorded seismic activity long enough to provide a wealth of clues about <a href="https://www.earth.com/news/mars-gravity-map-exposes-ancient-structures-and-volcanic-activity/">Mars’s structure</a>. Its readings have now sparked a different perspective on where the Red Planet stashed its water.



Reaching and analyzing these underground stores remain a distant dream, but simply knowing they exist changes how scientists think about Mars as a potentially habitable place. 



Perhaps the mysteries of these deep waters will inspire novel tools and missions in future.



Until then, human curiosity and imagination will keep this buried reservoir near the top of must-explore questions as we continue to study the planet’s past and puzzle over its <a href="https://www.earth.com/news/nasa-may-have-finally-discovered-life-on-mars/">potential for supporting life</a>.



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Buried water found on Mars sparks new hopes and headaches

A fresh look inside Mars suggests that what lurks far...

Have you ever wondered how malignancies like cancer grow, evolve, and, most importantly, how we can stop them? The answer may be hidden within the microscopic world of our cells.



This year, the World Health Organization has reported that cancer afflicted over 20 million people and claimed nearly 10 million lives. The search for an effective cure is a race against time, and two bright minds from Texas A&amp;M University have brought us a step closer to the finish line.



<h2 class="wp-block-heading" id="h-environment-around-cancer-cells">Environment around cancer cells</h2>



Graduate students Samere Zade and Ting-Ching Wang from <a href="https://www.tamu.edu" target="_blank" rel="noreferrer noopener">Texas A&amp;M University</a>, working under the guidance of the Lele Lab, have uncovered valuable insights into <a href="https://www.earth.com/news/ai-is-the-next-frontier-in-cancer-treatment/" target="_blank" rel="noreferrer noopener">cancer’s progression</a>.



The research, published in the journal Nature Communications, reveals how the stiffening of a tumor cell’s environment influences the structure and function of its nucleus. This offers a new perspective on why cancer cells proliferate so aggressively.



“Cancer has proven to be a difficult disease to treat. It is extremely complex, and the molecular mechanisms that enable tumor progression are not understood,” explained Dr. Tanmay Lele, a joint faculty member in biomedical and chemical engineering. 



“Our findings shed new light into how the stiffening of tumor tissue can promote tumor cell proliferation.”



<h2 class="wp-block-heading" id="h-stiffness-and-cancer-cell-proliferation">Stiffness and cancer cell proliferation</h2>



The study highlights how tumor <a href="https://www.earth.com/news/the-cooking-oils-in-your-diet-may-be-linked-to-cancer/" target="_blank" rel="noreferrer noopener">cells</a> respond to stiff surroundings. The nuclear lamina, which is like a support structure for the cell's nucleus, becomes smoother and tighter when the cell interacts with a stiff environment. 



This happens because the cell spreads out on the rigid surface, causing changes in the nucleus's structure.



As a result, a specific protein called yes-associated protein (YAP) moves into the nucleus. YAP plays a crucial role in controlling how cells multiply. Once inside the nucleus, YAP activates processes that make the <a href="https://www.earth.com/news/molecular-fingerprints-could-be-key-to-early-cancer-detection/" target="_blank" rel="noreferrer noopener">cancer</a> cells grow and divide more rapidly, contributing to the aggressive spread of the tumor.



“The ability of stiff matrices to influence nuclear tension and regulate YAP localization could help explain how tumors become more aggressive and perhaps even resistant to treatment in stiffened tissues,” said Zade.



<h2 class="wp-block-heading" id="h-structural-integrity-of-the-cell-nucleus">Structural integrity of the cell nucleus</h2>



This discovery expands on earlier research by the Lele Lab, which showed that the cell nucleus acts similarly to a liquid droplet. Just like a droplet maintains its shape due to surface tension, the nucleus relies on a protein called lamin A/C in its nuclear lamina to preserve its structural integrity.



In the new study, researchers found that lamin A/C not only helps maintain the nucleus shape but also plays a key role in regulating cancer cell <a href="https://www.earth.com/news/simple-lifestyle-changes-could-prevent-half-of-all-cancer-deaths/" target="_blank" rel="noreferrer noopener">growth</a>.



When lamin A/C levels are reduced, it disrupts the ability of the yes-associated protein (YAP) to move into the nucleus. 



Since YAP is responsible for promoting cell multiplication, this reduction in lamin A/C limits YAP activity in the nucleus, slowing down the rapid proliferation of cancer cells. This finding suggests that lamin A/C could be a potential target for cancer treatments.



“The protein lamin A/C plays a key role here - reducing it made cells less responsive to environmental stiffness, particularly affecting the localization of a key regulatory protein (YAP) to the nucleus,” Zade explained.



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



The implications of this research extend beyond academic understanding. By uncovering how matrix stiffness drives nuclear changes and regulates pathways like YAP signaling, the findings open the door to innovative cancer treatments.



“Uncovering how matrix stiffness drives nuclear changes and regulates key pathways, like YAP signaling, opens the door to developing therapies that target these mechanical pathways,” said Zade. 



“Drugs or treatments could be designed to soften the tumor environment, disrupting the physical cues that help cancer cells thrive. Lamin A/C and related nuclear mechanics could become targets for cancer treatments.”



<h2 class="wp-block-heading" id="h-future-research-directions">Future research directions</h2>



The <a href="https://lelelab.org" target="_blank" rel="noreferrer noopener">Lele Lab</a> plans to expand its research by investigating the extent to which these findings apply to tumors derived from patients. This step could bridge the gap between lab-based discoveries and practical treatments, bringing hope to millions affected by <a href="https://www.earth.com/news/ketogenic-diet-may-help-the-body-kill-cancer-cells/" target="_blank" rel="noreferrer noopener">cancer</a>.



This work was supported by the National Institutes of Health, the Cancer Prevention and Research Institute of Texas, and the National Science Foundation. The Texas A&amp;M Engineering Experiment Station administered the funding, highlighting the institution’s commitment to innovative cancer research.



Through their meticulous study of nuclear mechanics and tumor stiffness, the researchers at the Lele Lab have paved the way for new avenues in cancer treatment. 



The findings highlight the importance of targeting the physical microenvironment of cancer cells, offering a fresh perspective in the fight against one of humanity’s most challenging diseases.



The study is published in the journal <a href="https://www.nature.com/articles/s41467-024-54577-4" target="_blank" rel="noreferrer noopener">Nature Communications</a>.



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Microscopic discovery reveals how cancer cells grow faster

Have you ever wondered how malignancies like cancer grow, evolve,...

Ever thought that saving trees was as simple as stopping deforestation? Think again. A new study from Ecuador's Amazon reveals a more complicated story, where the survival of trees depends on a delicate dance between plants and animals - and this dance is falling apart.



Research from the Universidad de las Américas (UDLA) in Ecuador, led by Dr. Juan Ernesto Guevara-Andino and Dr. María-José Endara, has revealed some startling numbers.



About 14% of tree species in the Ecuadorian Amazon are critically endangered, while almost half (47%) could go extinct if things don't change.



<h2 class="wp-block-heading" id="h-trees-with-smaller-fruits">Trees with smaller fruits</h2>



Size matters in the Amazon, but not in the way you'd expect. Trees with smaller fruits are having an especially tough time. These <a href="https://www.earth.com/news/more-than-one-third-of-the-worlds-trees-face-extinction/" target="_blank" rel="noreferrer noopener">trees</a> rely on specific animals to spread their seeds, and those animals are becoming harder to find.



It's like a restaurant losing its delivery drivers - the food's ready to go, but there's no way to get it where it needs to be.



<h2 class="wp-block-heading" id="h-threats-to-amazonian-trees">Threats to Amazonian trees</h2>



While most of us think of logging when we hear about threats to the Amazon, the reality is far more complex.



<a href="https://www.earth.com/news/the-worlds-largest-living-organism-consists-of-47000-trees/" target="_blank" rel="noreferrer noopener">Trees</a> don't live in isolation - they are part of a community that includes insects, birds, and mammals. Each species plays its role, whether it's pollinating flowers or spreading seeds.



"Thus, our results highlight the importance of incorporating meaningful ecological traits in extinction risk estimates, such as those related to reproduction and life history strategies," explained Dr. Endara.



Her words point to a crucial fact: we can't save trees without understanding their relationships with other species.



<h2 class="wp-block-heading" id="h-protected-areas-not-as-safe-as-we-thought">Protected areas: Not as safe as we thought</h2>



One may think trees in protected areas would be safe. However, the study found otherwise. Even in Yasuní National Park, Ecuador's crown jewel of conservation, <a href="https://www.earth.com/news/resilient-trees-can-help-safeguard-cities-from-climate-change/" target="_blank" rel="noreferrer noopener">trees are in trouble</a>.



"For example, we found that some endemic tree species populations are experiencing high levels of threat by deforestation inside the Yasuní National Park, the biggest and most iconic protected area in the Ecuadorian Amazon," noted Dr. Guevara-Andino.



<h2 class="wp-block-heading" id="h-new-approach-to-protecting-amazon-trees">New approach to protecting Amazon trees</h2>



The old way of protecting trees mainly focused on stopping deforestation. But this study shows we need to think bigger. 



We need to protect not just the trees, but the entire system that they are part of - including the animals that help them reproduce and spread.



This means conservation plans need to consider things like which animals disperse each tree's seeds, how different species depend on each other, and what happens when one species disappears from the system.



<h2 class="wp-block-heading" id="h-looking-beyond-ecuador">Looking beyond Ecuador</h2>



What's happening in Ecuador isn't just Ecuador's problem. The <a href="https://www.udla.cl" target="_blank" rel="noreferrer noopener">UDLA</a> study gives us clues about what might be happening in other rainforests around the world. 



When we lose one species, it affects many others - like pulling one thread and watching a whole sweater unravel.



The good news is that understanding these connections gives us new ways to help. By protecting both trees and the animals they depend on, we have a better chance of <a href="https://www.earth.com/news/trees-are-relocating-in-a-race-against-global-warming/" target="_blank" rel="noreferrer noopener">keeping these forests alive</a> for future generations.



<h2 class="wp-block-heading" id="h-saving-the-amazon-s-trees">Saving the Amazon's trees</h2>



The numbers from this study - 14% critically endangered tree species and and 47% threatened - should wake us up.



But they also point the way forward. We can't just focus on stopping chainsaws. We need to protect the whole forest community - from the smallest pollinator to the largest seed-dispersing animal.



The path ahead isn't simple, but it's clear. To save the Amazon's trees, we need to think about forests differently. They're not just collections of trees - they're complex communities where every species plays a vital role. And just like any community, they are stronger when all of their members are healthy and present.



The research does more than just raise alarms. It shows us that saving trees means saving relationships - between <a href="https://www.earth.com/news/trees-have-an-amazing-ability-to-adapt-to-new-climates/" target="_blank" rel="noreferrer noopener">plants</a> and animals, between species and their environment, and ultimately, between humans and nature. The question now is whether we'll act on this knowledge in time to make a difference.



The trees of Ecuador's Amazon face many threats, but perhaps the biggest one is our own limited understanding of how forests really work. This study helps fix that problem. Now it's up to us to use this knowledge to protect not just the <a href="https://www.earth.com/news/city-greening-predicting-the-cooling-effects-of-trees/" target="_blank" rel="noreferrer noopener">trees</a>, but the entire web of life they're part of.



The study is published in the journal <a href="https://nph.onlinelibrary.wiley.com/doi/10.1002/ppp3.10606" target="_blank" rel="noreferrer noopener">Plants People Planet</a>.



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Amazon trees are critically endangered, even in protected areas

Ever thought that saving trees was as simple as stopping...

For many decades, scientists have documented how burning fossil fuels releases greenhouse gases that trap heat near Earth’s surface, driving a gradual - but consistent - warming trend.&nbsp;



Recently, however, the world has experienced an extraordinary surge in temperatures, catapulting the climate system into uncharted territory and confounding some of the best climate models available.&nbsp;



This abrupt, persistent streak of unprecedented warmth over the past two years has shattered temperature records, raising urgent questions: Why is it so much hotter than expected right now, and does it signal a more profound transformation underway?



<h2 class="wp-block-heading" id="h-a-remarkable-and-persistent-heat-surge">A remarkable and persistent heat surge</h2>



After decades of steadily rising temperatures, 2023 saw a dramatic jump in <a href="https://www.earth.com/news/mapping-2024s-record-heat-unveiling-earths-climate-danger-zones/" target="_blank" rel="noreferrer noopener">global heat</a> - enough for it to become the hottest year in recorded history. But the extraordinary nature of this uptick did not stop there.&nbsp;



By 2024, average sea-surface and air temperatures had shot up again, setting new records that far exceeded previous benchmarks.&nbsp;



According to the <a href="https://wmo.int/" target="_blank" rel="noreferrer noopener">World Meteorological Organization</a>, the temperature anomalies between June 2023 and September 2024 were so far beyond typical year-to-year variability that experts called it an “unprecedented streak,” with 2024 now on track to be the warmest year ever documented.



“Warming in 2023 was head-and-shoulders above any other year, and 2024 will be as well,” said Gavin Schmidt, director of the <a href="https://www.giss.nasa.gov/" target="_blank" rel="noreferrer noopener">NASA Goddard Institute for Space Studies</a>. "I wish I knew why, but I don’t. We’re still in the process of assessing what happened and if we are seeing a shift in how the climate system operates.”



While all scientists agree that <a href="https://www.earth.com/news/greenhouse-gas-emissions-reach-another-all-time-high/" target="_blank" rel="noreferrer noopener">greenhouse gases</a> from fossil fuel use remain the primary driver of Earth’s overall warming trend, they are still debating how to explain this short-term explosion in global temperatures.&nbsp;



Changes in cloud patterns, air pollution, and the planet’s capacity to store carbon are among the suspected contributors, but experts believe it may take at least another year or two to fully untangle the puzzle.



<h2 class="wp-block-heading" id="h-uncharted-territory-in-climate-records">“Uncharted territory” in climate records</h2>



Climate specialists characterize the past two years as pushing the planet “well into uncharted territory,” a phrase used by Richard Allan, a climate scientist from the University of Reading in the UK.&nbsp;



The magnitude of recent warming has tested established climate models, placing it, according to climatologist Sonia Seneviratne at ETH Zurich, “at the limit of what we would expect based on existing climate models.”&nbsp;



At the same time, Seneviratne emphasized that rising fossil fuel emissions make long-term warming trends wholly unsurprising.



So how is it that temperatures became so anomalous? Early theories focus on how natural climate variability has intersected with human-driven warming.&nbsp;



One factor is the unusually strong shift from a rare, three-year La Niña - which generally cools the planet by sending additional heat into the deep oceans - to a warming El Niño event that started in mid-2023, releasing stored energy back into the atmosphere.&nbsp;



While this helps explain some portion of the spike, temperatures remained persistently high even after <a href="https://www.earth.com/news/el-nino-event-may-push-earth-towards-its-hottest-year-ever/" target="_blank" rel="noreferrer noopener">El Niño</a> peaked in January.



“It is difficult to explain this at the moment,” said Robert Vautard, a member of the <a href="https://www.ipcc.ch/" target="_blank" rel="noreferrer noopener">Intergovernmental Panel on Climate Change</a> (IPCC). “We lack a bit of perspective. If temperatures do not drop more sharply in 2025, we will really have to ask ourselves questions about the cause.”



<h2 class="wp-block-heading" id="h-factors-contributing-to-the-heat-surge">Factors contributing to the heat surge</h2>



Amid these extraordinary conditions, scientists have zeroed in on multiple theories that go beyond El Niño.



<h3 class="wp-block-heading" id="h-shifts-in-airborne-pollution">Shifts in airborne pollution</h3>



A global shift to cleaner shipping fuels around 2020 might have slashed emissions of sulfur compounds that ordinarily create reflective, mirror-like clouds in shipping lanes.&nbsp;



With fewer sulfur aerosols, more sunlight could be reaching the Earth’s surface, potentially accelerating warming.



<h3 class="wp-block-heading" id="h-reduction-in-low-lying-clouds-nbsp">Reduction in low-lying clouds&nbsp;</h3>



A peer-reviewed study proposed that a global decline in low-lying clouds might have allowed extra solar radiation to heat the surface, but establishing consistent data across the planet remains challenging.



<h3 class="wp-block-heading" id="h-weakening-of-carbon-sinks-nbsp">Weakening of carbon sinks&nbsp;</h3>



Forests and oceans, traditionally known to absorb much of humanity’s carbon emissions, showed signs of stress in 2023. Scientists described this as an “unprecedented weakening” of Earth’s <a href="https://www.earth.com/news/mountains-both-carbon-sinks-and-carbon-sources/" target="_blank" rel="noreferrer noopener">carbon sinks</a>, suggesting the planet’s ability to store CO₂ might be faltering.&nbsp;



If sinks become less effective at capturing carbon, warming could speed up beyond current estimates.



<h3 class="wp-block-heading" id="h-arctic-tundra-emissions-nbsp">Arctic tundra emissions&nbsp;</h3>



In December, the <a href="https://www.noaa.gov/" target="_blank" rel="noreferrer noopener">U.S. National Oceanic and Atmospheric Administration</a> reported that Arctic tundra, which has locked away carbon dioxide for millennia, has begun releasing more CO₂ than it captures.&nbsp;



Such a shift, scientists warn, might tip the balance of the global carbon cycle, further feeding into accelerated warming.



None of these hypotheses alone fully accounts for the heat surge, prompting climate experts to suspect the convergence of multiple factors.&nbsp;



“We cannot exclude that some other factors also further amplified the temperatures... the verdict is still out,” said Seneviratne.



<h2 class="wp-block-heading" id="h-at-odds-with-climate-models">At odds with climate models</h2>



Climate models, which have reliably simulated broad, decades-long warming trends, appear to have underestimated just how extreme and enduring this recent heat streak would be.&nbsp;



“What occurred was at the limit of what we would expect based on existing climate models,” Seneviratne said. Some experts worry that if any key feedbacks or phenomena were missing from these models, the planet could be approaching a threshold of more profound, potentially less reversible changes.



Johan Rockström, director of the <a href="https://www.pik-potsdam.de/en/home" target="_blank" rel="noreferrer noopener">Potsdam Institute for Climate Impact Research</a>, voiced concerns about rapidly warming oceans, which have long served as massive heat and carbon sinks.&nbsp;



“Oceans are warming at a rate scientists cannot fully explain,” he said last month. “Could this be a first sign of a planet starting to show a loss of resilience? We cannot exclude it.”



<h2 class="wp-block-heading" id="h-a-warning-for-what-may-lie-ahead">A warning for what may lie ahead</h2>



Record-high temperatures in 2023 and 2024 offer a stark reminder of the fragility of Earth’s climate system.&nbsp;



Although some interplay of El Niño, cloud cover, and carbon sink changes may explain part of the observed heat, the fundamental driver remains human emissions of greenhouse gases from fossil fuels.&nbsp;



Even if the dramatic peak fades in coming months, the possibility persists that Earth’s temperature baseline has permanently ratcheted up, edging us closer to thresholds that portend more dangerous extremes.



For many climate experts, these heat surges serve as yet another clarion call to reduce emissions swiftly, to develop robust adaptation strategies, and to keep monitoring the climate system’s every nuance. 



If the current anomalies hint at hidden processes at work - like a weakening Arctic tundra sink or oceanic shifts - policy decisions made now to cut emissions and preserve resilience could become all the more consequential.



Vautard emphasized that if the climate doesn’t cool off more sharply in 2025, it would prompt scientists to reevaluate their assumptions about the interplay of natural and human-driven factors - perhaps indicating a more profound shift in how our climate operates.&nbsp;



In this uncertain scenario, building deeper scientific understanding becomes ever more urgent.



<h2 class="wp-block-heading" id="h-building-resilience-against-future-heat-surges">Building resilience against future heat surges</h2>



Although the short-term temperature surge has challenged existing forecasts, the broader climate consensus remains intact: Earth is warming at an alarming rate, primarily due to carbon dioxide and other greenhouse gases.&nbsp;



This abrupt heat wave may be a harbinger of future extremes, or possibly just a short-lived but jarring deviation from expected patterns.&nbsp;



Determining which is the case will likely require another year or two of data, plus renewed efforts to bolster climate observation networks, refine models, and capture nuanced processes in the oceans, atmosphere, and polar regions.



No matter the final explanation, the world’s experience over the last two years underscores the climate’s capacity to surprise - sometimes by margins that drastically shift our sense of what is “normal.”&nbsp;



For policymakers, this event highlights both the urgency of emission cuts and the importance of resilience-building measures against more frequent or severe heat surges.&nbsp;



For scientists, the anomaly reveals how much is still left to learn about the planet’s complex interplay of feedbacks and stresses.



“We’re still in the process of assessing what happened and if we are seeing a shift in how the climate system operates,” Schmidt said.&nbsp;



Whether this remarkable episode proves to be a short detour or a glimpse of a new reality, it adds fresh impetus to the effort to better predict, manage, and mitigate the precarious path Earth is on.



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Puzzling heat surge pushes Earth’s climate to new extremes

For many decades, scientists have documented how burning fossil fuels...

Honey, often described as “liquid gold,” has captivated civilizations for millennia. Long prized for its sweetness, it has also been used in diverse cultures and traditions to soothe sore throats, support wound healing, and even address infections.&nbsp;



While honey’s anti-inflammatory, antioxidant, and antimicrobial properties have earned it a place in both kitchens and home remedies, questions remain about the science behind these claims.&nbsp;



What exactly gives honey its therapeutic potential, and how do the microorganisms within it influence its benefits and safety?



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



When people think of honey, they usually picture a sticky, golden sweetener ready to drizzle on toast or stir into tea. Yet behind this simplicity lies a rich microbial community.&nbsp;



Honey carries a variety of <a href="https://www.earth.com/news/microbes-laid-the-foundation-for-early-life-on-earth/" target="_blank" rel="noreferrer noopener">microorganisms</a> that together create a microscopic ecosystem. This local microbiome in honey prompts inquiries about its safety, particularly regarding how honey is produced, whether it’s consumed raw or pasteurized, and the risks it may pose for certain individuals, such as infants.



Honey primarily consists of sugars (mainly fructose and glucose), water, and organic compounds produced by <a href="https://www.earth.com/news/bees-are-making-less-honey-and-five-decades-of-data-reveals-why/" target="_blank" rel="noreferrer noopener">bees</a>. While the western honeybee, Apis mellifera, is the dominant species in large-scale honey production, at least eight other bee species - including Apis cerana and Apis nigrocincta - are also known to produce honey.&nbsp;



Each species, along with environmental and floral variations, can influence the composition of the honey they create.



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



Bees generate honey through a multifaceted process involving the collection of nectar and honeydew from flowers and subsequent enzymatic transformations within the hive.&nbsp;



During this process, microorganisms - such as Bacillus, Saccharomyces, and Aspergillus - are introduced to the honey via the bees’ digestive tracts and from external sources like air, soil, and plant matter.



Some microbes, particularly lactic acid bacteria like Lactobacillus and Bifidobacterium, are beneficial. They can contribute to honey’s acidity and preserve it against spoilage.&nbsp;



Conversely, certain yeasts, such as Candida and Saccharomyces, may thrive in honey that has excessive moisture, potentially causing fermentation or spoilage. Thus, honey’s microbial profile is shaped by the floral environment, geographic location, bee health, and other situational elements.



The <a href="https://www.earth.com/news/honey-bees-face-a-multitude-of-complex-stressors-in-the-field/" target="_blank" rel="noreferrer noopener">honeybee</a> gut microbiome itself plays a critical part in shaping honey’s characteristics. In addition to lactic acid bacteria, microbes like Enterobacter and Klebsiella help maintain bee health.&nbsp;



If this beneficial microbial community becomes unbalanced - due to factors such as disease or environmental stress - bees can become susceptible to infections, including fungal pathogens like Aspergillus fumigatus.&nbsp;



This fungus can harm both immunocompromised humans and bee larvae, emphasizing the shared health interests of bees and humans.



<h2 class="wp-block-heading" id="h-honey-s-remarkable-self-preservation-abilities">Honey’s remarkable self-preservation abilities</h2>



Despite harboring an assortment of microbes, honey naturally resists spoilage and pathogenic bacteria. One central reason lies in the enzyme glucose oxidase, which worker bees secrete from their hypopharyngeal glands.&nbsp;



When bees combine this enzyme with glucose in the nectar, it produces hydrogen peroxide (H₂O₂) and water. The resulting hydrogen peroxide remains encased in the honey, helping lower its pH to levels unfavorable for bacterial growth.



Additionally, honey’s high sugar content and minimal water availability (i.e., low moisture) create an osmotic environment hostile to many microorganisms. These traits together form a potent natural defense that helps honey avoid quick spoilage, even when stored at room temperature for extended periods.



Still, honey’s acidity can vary according to seasonal flora and the particular flowers the bees visit. More than 300 honey varieties exist around the world, each uniquely shaped by local botanical and environmental factors.&nbsp;



In the United States alone, one can find distinct honeys like buckwheat honey in the Midwest or citrus blossom honey in Florida and southern California.&nbsp;



Globally, the famed Manuka honey originates from Leptospermum scoparium flowers in New Zealand and Australia and is celebrated for its heightened antibacterial effects, often attributed to methylglyoxal (MGO).



<h2 class="wp-block-heading" id="h-medicinal-properties-of-honey">Medicinal properties of honey</h2>



Manuka honey is one of the most researched types, largely due to the presence of MGO, which is formed from dihydroxyacetone (DHA) in Manuka flower nectar.&nbsp;



Studies suggest that Manuka honey is more potent against certain bacteria, like Pseudomonas aeruginosa, than generic honeys. However, evidence shows that various constituents of Manuka honey, including hydrogen peroxide and an osmotic effect, work together to amplify its antimicrobial strength.



While Manuka honey has garnered attention for wound care and infection control, clinical research on its effectiveness for broader health issues - such as <a href="https://www.earth.com/news/new-tool-detects-changes-in-gut-health-to-help-prevent-disease/" target="_blank" rel="noreferrer noopener">gut health</a>, diabetes, or cancer - remains limited.&nbsp;



A few clinical trials point to Manuka honey’s potential to ease throat discomfort in chemotherapy patients, but these studies have not conclusively shown that honey surpasses existing treatments.&nbsp;



Further investigations are needed to determine whether honey’s properties can be harnessed reliably in mainstream healthcare.



<h2 class="wp-block-heading" id="h-balancing-benefits-and-safety">Balancing benefits and safety</h2>



One key distinction in honey is whether it’s raw or pasteurized. Raw honey undergoes minimal filtration and retains more of its natural microbes, including pollen particles and other hive components.&nbsp;



Some argue this confers extra health advantages, like enhanced antioxidant and probiotic qualities. However, raw honey also poses allergy risks to individuals sensitive to pollen or bee-derived proteins.



Pasteurized honey, processed at high temperatures to lower its microbial load, can be safer in terms of minimizing fermentation or spoilage. Yet pasteurization may also reduce honey’s beneficial enzymes and microbes, potentially lessening any therapeutic qualities.&nbsp;



Regardless of processing, improper honey storage - especially exposure to moisture, heat, or air - can trigger spoilage or microbial growth, underscoring the need for careful handling.



<h2 class="wp-block-heading" id="h-honey-consumption-risks">Honey consumption risks</h2>



While honey is generally considered safe, one well-known concern is the presence of Clostridium botulinum spores. Though relatively rare, these spores can produce a potent neurotoxin that induces botulism, a serious condition marked by muscle weakness and possible paralysis.&nbsp;



Infants under one year old are particularly vulnerable because their developing digestive tracts are ill-equipped to counteract C. botulinum spores. Consequently, pediatric and public health guidelines strongly advise against giving honey to infants less than 12 months of age.&nbsp;



Although botulism risk in older children and adults is minimal, the possibility of contamination underscores the importance of following storage and processing recommendations.



<h2 class="wp-block-heading" id="h-honey-s-role-in-health-and-research">Honey’s role in health and research</h2>



As scientists deepen their understanding of honey’s chemistry and the interplay of its microbial inhabitants, possibilities emerge for broader applications.&nbsp;



Honey’s mix of sugars, enzymes, and natural compounds could prove relevant in addressing <a href="https://www.earth.com/news/scientists-create-viruses-to-combat-antibiotic-resistant-bacteria/" target="_blank" rel="noreferrer noopener">antibiotic-resistant</a> infections, improving wound healing, and perhaps even aiding in metabolic or gastrointestinal disorders. However, robust, large-scale clinical trials remain necessary to confirm many of these potential benefits.



Still, anecdotal evidence and limited studies already support honey’s use in alleviating mild conditions, like sore throats or minor cuts. Traditional medicine in many cultures has leveraged honey’s soothing properties for centuries.&nbsp;



Modern science is now trying to define these uses more precisely, distinguishing home remedies from evidence-based healthcare solutions.



<h2 class="wp-block-heading" id="h-a-spectrum-of-varieties">A spectrum of varieties</h2>



Honey is incredibly diverse, owing to factors like bee species, local flora, and environmental conditions. Orange blossom honey from Florida, for example, differs not only in taste from avocado honey in California or buckwheat honey in New York, but also in antioxidant capacity and potential microbial composition.&nbsp;



Globally, Manuka honey remains the most studied, but dozens of specialty honeys in various regions hold cultural and medicinal significance, reflecting how nature’s subtleties shape each batch.



Understanding this variety can guide consumers seeking specific flavors or purported health benefits. It can also inform researchers studying how different nectar sources yield distinct antimicrobial or antioxidant properties in honey, potentially expanding its role in food science and medicine.



<h2 class="wp-block-heading" id="h-looking-ahead-honey-s-future-as-a-resource">Looking ahead: Honey’s future as a resource</h2>



Honey stands as an intriguing intersection of biology, chemistry, ecology, and culinary art. While marketed primarily as a sweetener, its composition reveals a wealth of complex interactions among sugars, enzymes, microbes, and floral compounds.&nbsp;



These interactions contribute to honey’s distinctive flavor profiles, antimicrobial resilience, and prospective therapeutic potential.



Ongoing research into honey’s properties - including how it fights certain <a href="https://www.earth.com/news/intestinal-bacteria-could-help-you-live-a-very-long-life/" target="_blank" rel="noreferrer noopener">bacteria</a>, whether it can bolster wound healing, and its broader impact on human health - reflects a growing recognition of nature’s capacity to inspire and innovate.&nbsp;



As studies become more rigorous, honey’s status in modern integrative medicine and food science may continue to rise, provided that researchers address the gaps and ensure consumer safety.



<h2 class="wp-block-heading" id="h-honey-as-a-natural-marvel-nbsp">Honey as a natural marvel&nbsp;</h2>



Honey’s enduring popularity stems not only from its sweet taste but also from the remarkable benefits attributed to it over centuries of traditional use.&nbsp;



Contemporary investigations highlight how honey’s microbial makeup, enzymatic processes, and sugar chemistry coalesce to create a product that is both delicious and potentially health-affirming.&nbsp;



Although definitive scientific consensus on many of honey’s medical applications remains elusive, its low-risk nature and storied past suggest that honey will continue to delight and possibly heal.



By bridging knowledge from microbiology, beekeeping, environmental science, and clinical research, scientists stand poised to uncover additional facets of honey’s significance.&nbsp;



Whether stirred into tea or considered for more formal therapeutic roles, honey’s multifaceted profile ensures that it remains a subject of fascination in culinary, cultural, and medical contexts.



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Nature's sweet remedy: Honey is a microbial marvel

Honey, often described as “liquid gold,” has captivated civilizations for...

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Today’s Video of the Day from the <a href="https://www.nsf.gov/">National Science Foundation</a> describes a big data study by experts at UT Austin that could revolutionize earthquake science.&nbsp;The research is focused on a massive rock called the Kumano Pluton, which is buried miles beneath the coast of southern Japan.&nbsp;



Based on 20 years of seismic data processed through one of the world's most powerful supercomputers, the scientists have developed the first complete, 3D visualization of Kumano Pluton.



The results of the analysis suggest that the mountain-sized rock now may be acting like a "lightning rod" that channels energy into the megaquakes seen in the this region.&nbsp;



While scientists have known about thy existence of Kumano Pluton for years, they were only aware of small sections of it. The UT Austin study provides a view of the entire rock formation. This will enable experts to study the pluton's effect on regional tectonics.&nbsp;



According to study co-author Shuichi Kodaira, director of the Japan Agency for Marine-Earth Science and Technology, the findings will provide critical information for a major new Japanese government-funded project to find out whether another major earthquake is building in the Nankai subduction zone, where the pluton is located.



"We cannot predict exactly when, where, or how large future earthquakes will be, but by combining our model with monitoring data, we can begin estimating near-future processes," said Kodaira, who was among the scientists who first discovered the Kumano Pluton in 2006. "That will provide very important data for the Japanese public to prepare for the next big earthquake."



"The fact that we can make such a large discovery in an area that is already well studied is, I think, eye opening to what might await at places that are less well monitored," said study lead author Adrien Arnulf, a research assistant professor at the University of Texas Institute for Geophysics.



Image/ Video Credit: National Science Foundation/ UT Austin&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

Kumano Pluton could be a magnet for megaquakes

[sendtonews key="xD9vsIXoKi-1905077-12187" type="single"] Today’s Video of the Day from the...

Astronomer,With,A,Telescope,Watching,At,The,Stars,And,Moon.

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Today’s Video of the Day from NASA's <a href="https://www.jpl.nasa.gov/">Jet Propulsion Laboratory</a> describes what you can get a glimpse of this month in the October sky. 



"Giant planets Jupiter and Saturn are visible throughout the night in October. Early in the evening, you'll find them to the southeast, moving slowly westward with the stars over the course of the night. They form a triangle with bright star Fomalhaut," says NASA.



"When observing this trio, note how the planets shine with a steady light, while the star twinkles. This can be an easy way to know if what you're looking at is a planet or a star."



Over the next few months, Mars will appear to change direction. This is called retrograde, and occurs when the apparent motion of a planet is in the opposite direction of other bodies within its system,



The Orionid meteor shower is active in October and November, and will peak on the night of October 20. At its peak, this shower usually produces 10 to 20 meteors per hour.



Video Credit: NASA JPL



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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

October stargazing: Mars retrograde and the Orionid meteor shower

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Tenerife, the largest of the Canary Islands. The archipelago consists of eight main islands including Gran Canaria, Lanzarote and La Palma, as well as many small islands and islets. The Canary Islands make up the southernmost region of Spain in the Atlantic Ocean.&nbsp;



Tenerife is dominated by Mount Teide, the third largest volcano in the world. Teide National Park (a UNESCO World Heritage Site) is located in the center of the island. Tourists flock to the beaches of Tenerife, which have sand that ranges in color from golden yellow to black.&nbsp;



"Owing to the island’s diverse topography and unique climatic factors, Tenerife has multiple microclimates, which means that the weather can vary drastically from one part of the island to the other," says ESA.



"Weather and climate are heavily influenced by the trade winds blowing from the northeast for most of the year, bringing humidity and precipitation to the north of the island, as well as to the northern slopes of Mount Teide."&nbsp;



Video Credit: European Space Agency



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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

Tenerife in the Canary Islands

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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 data release from the Gaia observatory, which was launched in 2013. The observatory has been mapping our galaxy from Lagrange point 2, creating the most accurate and complete multi-dimensional map of the Milky Way.



"By now two full sets of data have been released, the first set in 2016 and a second one in 2018. These data contained stellar positions, distances, motions across the sky, and colour information, among others," says ESA.



On June 13, 2022 a third full data set was released. ESA said this data release contains even more and improved information about almost two billion stars, Solar System objects and extragalactic sources. 



"It also includes radial velocities for 33 million stars, a five-time increase compared to data release 2," explains ESA. "Another novelty in this data set is the largest catalog yet of binary stars in the Milky Way, which is crucial to understand stellar evolution."



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

Gaia is mapping the Milky Way in unprecedented detail

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features Fuerteventura and Lanzarote, part of the Canary Islands in the North Atlantic Ocean. The false-color image was captured by the Copernicus Sentinel-2 mission.



"The Canary Islands are a group of ocean island volcanoes that were formed by volcanic activity millions of years ago. The Spanish region and archipelago is located around 100 km off the north coast of Africa and 1,000 km from the Iberian Peninsula," says ESA.



"The eight main islands are (in order of largest to smallest in area) Tenerife, Fuerteventura, Gran Canaria, Lanzarote, La Palma, La Gomera, El Hierro and La Graciosa. The archipelago also includes many smaller islands and islets."



Lanzarote is the third most populous Canary Island, with a population of 150,000, and is also the easternmost island in the archipelago.



"Lanzarote has a long history of eruptions and is often referred to as the ‘Island of the 1000 volcanoes,' yet it is actually the least mountainous Canarian Island," reports ESA.



"The highest mountain is the volcano Peñas del Chache near Haría in the northern part of the island, which is 670 m above sea level. The Timanfaya National Park can be seen in the southwest part of the island and is entirely made up of volcanic soil."



Fuerteventura Island is the second largest of the Canaries. It is also the oldest, emerging between 12 and 20 million years ago.



"The island is fairly flat and has a desert landscape of sand and stones as well as long beaches," says ESA. "The center of the island is made up of a wide, elongated valley and, from north to south, is dissected by a series of extinct, eroded volcanoes. The west coast is dotted with rugged cliffs and small bays."



Video 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

Fuerteventura and Lanzarote of the Canary Islands

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> (ESA) reveals an image from the Copernicus Sentinel-3 mission which illustrates the extreme temperatures that struck Britain in August. Summer heatwaves also affected North Africa, Asia, and the United States.



"The image, captured on 12 August 2022, shows the United Kingdom’s previously green land appear brown (particularly in the southeast) amid the scorching conditions. The heatwave comes after months of extreme temperatures and low rainfall left the landscape parched. The dry conditions are also visible in parts of France, Belgium and the Netherlands," says ESA.



"The severe heatwaves experienced across Europe this summer are a harsh reminder of what is in store for our future.&nbsp; Extreme weather events will happen more frequently and intensely according to the Intergovernmental Panel on Climate Change (IPCC). This trend is set to worsen unless the rise in atmospheric greenhouse gas emissions caused by human activities is addressed."



Video 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

Impacts of UK heatwaves can be seen from space

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Today’s Video of the Day from the <a href="https://www.nsf.gov/">National Science Foundation</a> reveals that lizards could provide new insight into how species have evolved over centuries.  Understanding how environmental changes have affected animals in the past can help predict how they will be affected in the future.



A research team led by Dr. Melissa Kemp, a paleobiologist at the University of Texas at Austin, is studying lizards to find out more about a process called "adaptive radiation," or how organisms evolve to adapt to changing environments. The research is focused on lizards in the&nbsp; Caribbean.



"If we can gain any insights from past instances of extinction, it might be informative of what communities might look like in the future as these communities undergo future environmental changes," Dr. Kemp said in a profile piece by UT Austin.&nbsp;



Image/ Video Credit: National Science Foundation/ UT Austin&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

Lizards hold secrets of how animals evolve

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Milky,Way,In,The,Night,Sky

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Today’s Video of the Day from the <a href="https://www.jpl.nasa.gov/">NASA Jet Propulsion Laboratory</a> features some tips for skywatchers in August 2022. 



The morning quartet of planets will come to an end in August - with Venus and Saturn making their exits on opposite sides of the sky. Mars and Jupiter, however, will remain visible.&nbsp;



"The daily parade of four naked-eye planets in the mornings comes to an end this month. But there are still lots of great highlights, especially if you have access to binoculars," says NASA. "Plus, Saturn and Jupiter are returning to nighttime skies!"&nbsp;



"The outlook for the Perseid meteors isn't great due to a full moon on the peak night of August 12, but still it's worth keeping an eye out for early Perseids after midnight the week before. And August is a great month to learn an easy-to-spot constellation – Cygnus the swan."



Video Credit: NASA JPL



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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

NASA reveals what you can find in the August sky

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features the Great Lakes - Superior, Michigan, Huron, Erie, and Ontario - captured by the Copernicus Sentinel-3 mission.&nbsp;



According to ESA, the lakes represent the largest surface of freshwater in the world with a combined area of around 244,000 square kilometers, covering an area larger than the United Kingdom.



The lakes were formed around 100,000 years ago, when a massive ice sheet and giant glaciers transformed the landscape across most of Canada and part of the United States. As the ice melted, holes left behind from glaciers filled with meltwater and formed thousands of lakes. 



Huron is one of the five American great lakes and one of the largest freshwater lakes. It forms a natural border between the American state of Michigan and the Canadian province of Ontario.



Video 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

The Great Lakes of North America

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Today's Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features the Galápagos Islands, a volcanic archipelago in the Pacific Ocean. This region is one of the most famous places on the planet for viewing wildlife.



The Galápagos Islands are home to many native plants and animals that cannot be found anywhere else in the world, including giant tortoises and sea lions.&nbsp;



When Charles Darwin visited the islands in 1835, his wildlife observations inspired the theory of evolution by natural selection. In 1959, the Ecuadorian government made the entire archipelago a national park to protect its unique diversity.



The archipelago is made up of 13 major islands and several smaller islands and islets across 60,000 square kilometers of ocean. According to ESA, repeated volcanic eruptions and ongoing seismic activity have helped form the rugged mountain landscape of the islands. The most populated islands of Galapagos are San Cristóbal, Santa Cruz and Isabela.



The largest of the Galapagos Islands, Isabela, was formed from the joining of six shield volcanoes - Ecuador, Wolf, Darwin, Alcedo, Sierra Negra, and Cerro Azul. Volcanic activity persisted in the Galapagos for at least 20 million years, and possibly&nbsp; even longer. The archipelago is characterized by large contemporaneous volcanoes - some with plume magma sources, others from the asthenosphere. 



Video 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

The Galápagos Islands in the eastern Pacific

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

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> reveals a fascinating discovery from Gaia, a space observatory launched in 2013. The researchers have discovered that Gaia is capable of detecting starquakes – tiny motions on the surface of stars that change their shape. This is unexpected, considering that detecting starquakes is not something that Gaia was built for.  



"Previously, Gaia already found radial oscillations that cause stars to swell and shrink periodically, while keeping their spherical shape. But Gaia has now also spotted other vibrations that are more like large-scale tsunamis. These nonradial oscillations change the global shape of a star and are therefore harder to detect," says ESA.



"Nonradial oscillation modes cause a star's surface to move while it rotates, as shown in the animation. Dark patches are slightly cooler than bright patches, giving rise to periodic changes in the brightness of the star. The frequency of the rotating and pulsating stars was increased 8.6 million times to shift them into the audible range of humans."



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

Gaia spacecraft is capable of detecting starquakes

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Today’s Video of the Day from the <a href="https://www.esa.int/">European Space Agency</a> features the Italian city of Carrara, which is known around the world for its prestigious marble. Carrara is located on the Carrione River in northern Tuscany about 130 kilometers from Florence.&nbsp;



"The city is famous for its white or blue-grey marble, called Carrara, taken from nearby quarries in the Apuan Alps, a mountain range that stretches for approximately 55 kilometers and reaching around 2,000 meters high," reports ESA. "What appears as snow cover on the rugged mountains is actually bright white marble, contrasting with Tuscany’s lush green vegetation."



According to ESA, Carrara marble is one of the most prestigious marbles in the world, and its quarries produce more marble than any other place on Earth. The famous stone was formed by calcite-rich shells that were left behind by marine organisms after they died.&nbsp;



"When water bodies evaporate, the deposited remains form limestone, and when buried under multi-tonne layers of rock, the intense heat and pressure cause the limestone to metamorphose into marble," explains ESA.



"The special quality of the Carrara marble has made it a popular resource for many famous sculptures, including Michelangelo’s Pietà, and has been used for some of the most remarkable buildings in Ancient Rome, including the Pantheon and Trajan’s Column."



Video/ Image 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

Carrara, Italy and its world famous marble

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