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        <title><![CDATA[Universe Today]]></title>
        <description><![CDATA[Space and Astronomy News from Universe Today]]></description>
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        <lastBuildDate>Fri, 24 Jul 2026 09:43:36 +0000</lastBuildDate>
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            <title><![CDATA[Spin-Reversing Comet May Face Self-Destruction]]></title>
            <link>https://www.universetoday.com/articles/spin-reversing-comet-may-face-self-destruction</link>
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            <pubDate>Fri, 24 Jul 2026 02:52:49 +0000</pubDate>
            <dc:creator><![CDATA[Laurence Tognetti, MSc]]></dc:creator>
            <author>Laurence Tognetti, MSc (https://www.universetoday.com/authors/laurencetognetti)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/STScI-01KKH8ZMJNEDZ0VG0TN1HS3VQQ.jpg_750_20260724_024608.jpg" alt="Artist’s illustration of comet 41P, measured at about 1 kilometer (0.6 miles) in diameter, depicted approaching the Sun, resulting in outgassing from the evaporating ice. (Illustration Credit: NASA, ESA, CSA, Ralf Crawford (STScI)" width="1280" height="720" /></p><p>Comets are known for providing breathtaking observations of their long and shiny tails when they travel too close to the Sun. This happens because comets are made of ice and primarily orbit far from the Sun, but as their icy core heats up it evaporates, resulting in the aforementioned breathtaking observations. But while evaporating comets make for great public photos, scientists who study comets are focused on these snowballs of gas and dust and how they are remnants of the origins of the solar system about 4.6 billion years ago.</p>]]></description>
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        <item>
            <title><![CDATA[Should Scientists Have Research "Reserves" on the Moon?]]></title>
            <link>https://www.universetoday.com/articles/should-scientists-have-research-reserves-on-the-moon</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/should-scientists-have-research-reserves-on-the-moon</guid>
            <pubDate>Fri, 24 Jul 2026 02:14:17 +0000</pubDate>
            <dc:creator><![CDATA[Carolyn Collins Petersen]]></dc:creator>
            <author>Carolyn Collins Petersen (https://www.universetoday.com/authors/cc-petersen)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/Far_side_of_the_Moon_20260724_014558.png" alt="The Lunar Far Side offers a pristine and welcoming environment for multi-messenger observatories due to its lack of light pollution and radio interference from Earth. Can we keep it that way for future scientists to use? Courtesy of Artemis 1 mission." width="1280" height="720" /></p><p>The worlds of the Solar System offer up exciting and (so far) mostly pristine places for planetary scientists to study. As space missions continue to travel to Mars, Europa, asteroids, and other worlds, questions keep coming up about keeping them safe for continued exploration and observations.</p>]]></description>
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        <item>
            <title><![CDATA[Hubble Discovers the First "Missing" Black Hole in this Famous Star Cluster]]></title>
            <link>https://www.universetoday.com/articles/hubble-discovers-the-first-missing-black-hole-in-this-famous-star-cluster</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/hubble-discovers-the-first-missing-black-hole-in-this-famous-star-cluster</guid>
            <pubDate>Fri, 24 Jul 2026 00:34:38 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/STScI-01KW2HRNXWCFJ07B2CEN49KTFP_20260724_003434.jpg" alt="Astronomers found Omega Centauri’s first stellar-mass black hole, which has a visible star companion that is shown in greater detail. Credit: ESA/NASA/MPIA/STScI" width="1280" height="720" /></p><p>Combining over 20 years of archival data from Hubble with new data from the James Webb Space Telescope, a team of astronomers has found the first of the "missing" black holes.</p>]]></description>
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        <item>
            <title><![CDATA[The First Confirmed Exo-satellite Challenges Our Definitions of Planets and Moons]]></title>
            <link>https://www.universetoday.com/articles/the-first-confirmed-exo-satellite-challenges-our-definitions-of-planets-and-moons</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-first-confirmed-exo-satellite-challenges-our-definitions-of-planets-and-moons</guid>
            <pubDate>Thu, 23 Jul 2026 16:20:58 +0000</pubDate>
            <dc:creator><![CDATA[Brian Koberlein]]></dc:creator>
            <author>Brian Koberlein (https://www.universetoday.com/authors/brian)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/eso2610a_20260723_161917.jpg" alt="This illustration shows the system around the star CD-35 2722, with the newly found moon-like object at the center. Credit: ESO/M. Kornmesser" width="1280" height="720" /></p><p>What do you call a Jupiter-like object that orbits the brown dwarf companion of a star? Is it a planet, a moon, or something new?</p>]]></description>
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        <item>
            <title><![CDATA[Chandrasekhar and the Limits of Physics, Part 4: Vindication]]></title>
            <link>https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-4-vindication</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-4-vindication</guid>
            <pubDate>Thu, 23 Jul 2026 15:41:00 +0000</pubDate>
            <dc:creator><![CDATA[Paul Sutter]]></dc:creator>
            <author>Paul Sutter (https://www.universetoday.com/authors/pmsutter)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/header_20260714_152954.jpg" alt="The remnant of Tycho's supernova, a Type Ia explosion, in X-ray light. Such blasts happen when a white dwarf reaches the Chandrasekhar limit. Credit: NASA / Wikimedia Commons (public domain)." width="1280" height="720" /></p><p>The collapsing stars Eddington swore couldn't exist turned out to be everywhere, and half a century later the world handed Chandrasekhar his Nobel. How the 1.4 solar mass limit became one of the most important numbers in modern astronomy.</p>]]></description>
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        <item>
            <title><![CDATA[The Red Potato Galaxy and its Stifling Neighbour]]></title>
            <link>https://www.universetoday.com/articles/the-red-potato-galaxy-and-its-stifling-neighbour</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-red-potato-galaxy-and-its-stifling-neighbour</guid>
            <pubDate>Thu, 23 Jul 2026 15:14:21 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/redpotato_20260722_212641.jpg" alt="This image the red potato galaxy inside its cloud of gas, coloured red in this image. The blue gas contains another galaxy, and the extended blue region is the x-ray jet from the galaxy's AGN. The red potato is quiescent, despite being surrounded by gas, and researchers think it's because of the jet from the neighbouring galaxy. Image Credit: X-ray: NASA/CXC/Univ. Milano-Bicocca/W. Wang et al.; Infrared: NASA/ESA/CSA/STScI; Radio: ESO/NRAO/NAOJ/ALMA; Image processing: NASA/CXC/SAO/N. Wolk &amp; P. Edmonds" width="1280" height="720" /></p><p>Galaxies attract cold gas from the intergalactic medium and turn it into stars. But the JWST has found galaxies that aren't forming stars in the early Universe, long before they should've become quiescent. In at least one instance involving the Red Potato Galaxy, an AGN jet from a neighbouring galaxy is the likely culprit.</p>]]></description>
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            <title><![CDATA[Probing the Universe's Missing Matter With Mysterious Fast Radio Bursts]]></title>
            <link>https://www.universetoday.com/articles/probing-the-universes-missing-matter-with-mysterious-fast-radio-bursts</link>
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            <pubDate>Thu, 23 Jul 2026 15:12:54 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/eso2317a_1_20260722_191706.jpg" alt="This illustration shows a Fast Radio Burst form a distant galaxy reaching Earth. In new work, researchers used thousands of FRBs to probe the Universe for its missing matter. Image Credit: ESO/M. Kornmesser" width="1280" height="720" /></p><p>Astronomers aren't certain where Fast Radio Bursts come from. But they still have utility. They can use them to find the Universe's "missing matter."</p>]]></description>
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            <title><![CDATA[The Milky Way Flipped its Disk Billions of Years Ago]]></title>
            <link>https://www.universetoday.com/articles/the-milky-way-flipped-its-disk-billions-of-years-ago</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-milky-way-flipped-its-disk-billions-of-years-ago</guid>
            <pubDate>Wed, 22 Jul 2026 17:33:53 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/nik8496-cc_20260722_162042.jpg" alt="The Milky Way in the sky over the ESO's La Silla Observatory in Chile's Atacama Desert. The Milky Way's thick disk is full of older stars and rotates more slowly than its thin disk, which is full of younger stars. New research says a cosmic flip is responsible for this puzzling arrangement. Image Credit: ESO/B. Tafreshi (twanight.org)" width="1280" height="720" /></p><p>The Milky Way has two disks, the thin disk where most of the stars dwell, and the thick disk, populated by much older stars. The ESA's Gaia mission showed us that the thick disk rotates more slowly than the thin disk. The culprit, according to powerful simulations, was a disk flip in the MW's past, driven by a merger.</p>]]></description>
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            <title><![CDATA[Chandrasekhar and the Limits of Physics, Part 3: Exile and Beauty]]></title>
            <link>https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-3-exile-and-beauty</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-3-exile-and-beauty</guid>
            <pubDate>Wed, 22 Jul 2026 15:40:00 +0000</pubDate>
            <dc:creator><![CDATA[Paul Sutter]]></dc:creator>
            <author>Paul Sutter (https://www.universetoday.com/authors/pmsutter)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/header_20260714_152900.jpg" alt="An artist's impression of Sirius A and its faint white dwarf companion, Sirius B. White dwarfs were Chandrasekhar's signature subject. Credit: NASA/ESA / Wikimedia Commons (public domain)." width="1280" height="720" /></p><p>Driven from Europe by the feud, Chandrasekhar rebuilt his life in America and turned mastery-and-move-on into an art form. On his conviction that beautiful physics is true physics, and the two students he drove through blizzards to teach.</p>]]></description>
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            <title><![CDATA[The Milky Way's Most Powerful Particle Accelerator]]></title>
            <link>https://www.universetoday.com/articles/the-milky-ways-most-powerful-particle-accelerator</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-milky-ways-most-powerful-particle-accelerator</guid>
            <pubDate>Wed, 22 Jul 2026 04:32:02 +0000</pubDate>
            <dc:creator><![CDATA[Mark Thompson]]></dc:creator>
            <author>Mark Thompson (https://www.universetoday.com/authors/mark)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/English_Release_Lead_Image_500x375_0_20260722_042255.png" alt="Gamma ray observations from NASA's Fermi Space Telescope reveal the extended emission region around LHAASO J1912+1014u, now confirmed as a proton PeVatron. The dashed circle shows the Moon's size for scale (Credit : Tsunefumi Mizuno et al.)" width="1280" height="720" /></p><p>Astronomers have conclusively identified a source of the highest energy cosmic ray protons in the Milky Way, solving a long standing puzzle near the star Altair. By combining gamma ray, radio, and X-ray data from three separate observatories, a Hiroshima University led team ruled out competing explanations and confirmed the object as a genuine “PeVatron”. These natural particle accelerators are far more powerful than anything humans have ever built and helps us in the hunt for similar sources across the Galaxy.</p>]]></description>
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            <title><![CDATA[Electrically Charged Mars Storms Threaten Future Exploration]]></title>
            <link>https://www.universetoday.com/articles/electrically-charged-mars-storms-threaten-future-exploration</link>
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            <pubDate>Wed, 22 Jul 2026 02:45:46 +0000</pubDate>
            <dc:creator><![CDATA[Laurence Tognetti, MSc]]></dc:creator>
            <author>Laurence Tognetti, MSc (https://www.universetoday.com/authors/laurencetognetti)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/image_20260722_023817.jpg" alt="Orbital image of the global dust storm occurring in Martian Year 34 (mid-2018), which enveloped the entire Red Planet. (Credit: NASA/ESU)" width="1280" height="720" /></p><p>Martian dust storms are some of the most fascinating and mysterious planetary surface processes ever observed, as Earth, Mars, and Saturn’s moon Titan are the only known planetary bodies to have active dust storms. However, the major difference for Mars is its dust storms can blanket the entire planet at once, resulting in the surface becoming completely unobservable and blocking out sunlight, with the scientific community concerned this might hinder robotic, and even human, space exploration. But what if covering the surface and blocking sunlight wasn’t the only issue Martian global dust storms pose for future missions?</p>]]></description>
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            <title><![CDATA[NASA's Psyche Spacecraft Captured a Time-Lapse Video of its Mars Flyby]]></title>
            <link>https://www.universetoday.com/articles/nasas-psyche-spacecraft-captured-a-time-lapse-video-of-its-mars-flyby</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasas-psyche-spacecraft-captured-a-time-lapse-video-of-its-mars-flyby</guid>
            <pubDate>Tue, 21 Jul 2026 21:28:35 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/Psyche_Mars_20260721_210127.jpg" alt="In May, NASA's Psyche spacecraft performed a gravity-assist maneuver that sent in on its way to its target, the metal-rich asteroid 16 Psyche. The flyby was also an opportunity to test the spacecraft's instruments, including its multispectral camera. NASA has released a time-lapse video of the encounter. Image Credit: NASA/JPL" width="1280" height="720" /></p><p>NASA's Psyche mission used a gravity assist maneuver at Mars to gain velocity and adjust its trajectory to its eventual target. The asteroid 16 Psyche is a metal-rich asteroid that may be the remnant rocky core of a protoplanet. The flyby not only shepherded the spacecraft on to its target, it was also an opportunity to test Psyche's science instruments and cameras. NASA has released a timelapse of the flyby.</p>]]></description>
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            <title><![CDATA[Astronomers Are Still Trying to Understand How a Galaxy's Spiral Arms Form]]></title>
            <link>https://www.universetoday.com/articles/astronomers-are-still-trying-to-understand-how-a-galaxys-spiral-arms-form</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/astronomers-are-still-trying-to-understand-how-a-galaxys-spiral-arms-form</guid>
            <pubDate>Tue, 21 Jul 2026 19:38:46 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/m51-and-companion_0-jpg_20260721_163524.jpg" alt="The Whirlpool Galaxy (M51) is the classic grand design spiral galaxy. It was the first object recognized as a spiral, though at the time astronomers thought they were nebulae. Astronomers have been pondering spiral galaxies for a long time, trying to understand how their spiral arms persist. New research has at least a partial answer. Image Credit: NASA, ESA, S. Beckwith (STScI) and the Hubble Heritage Team (STScI/AURA)" width="1280" height="720" /></p><p>Spiral galaxies, including grand spirals like the Whirlpool galaxy, are plentiful. But it's still a mystery how their spiral arms form and persist for hundreds of millions of years, and why some galaxies have one, two, or three or more arms. New research based on Euclid data finds links between galaxy mass, star formation rate, and number of arms, and hints at their formation.</p>]]></description>
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            <title><![CDATA[Astronomers Catch a "Dark Comet" Red-Handed]]></title>
            <link>https://www.universetoday.com/articles/astronomers-catch-a-dark-comet-red-handed</link>
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            <pubDate>Tue, 21 Jul 2026 19:10:24 +0000</pubDate>
            <dc:creator><![CDATA[Andy Tomaswick]]></dc:creator>
            <author>Andy Tomaswick (https://www.universetoday.com/authors/andy-tomaswick)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/1-pia21259_20260721_191018.webp" alt="Artist's depiction of a near-Earth asteroid with an elongated orbit. Credit - NASA/JPL-Caltech" width="1280" height="720" /></p><p>Our ability to track and visualize small rocks in space is still improving. And occasionally we’ll find a space rock that will remind us of that fact. One such rock is detailed in a new paper, led by Davide Farnocchia of NASA’s Jet Propulsion Laboratory, and recently published in Nature Astronomy, where the research team discovered what they thought was a normal, run of the mill asteroid, was actually a “dark comet”.</p>]]></description>
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            <title><![CDATA[800 Million Years Ago, a Catastrophic Asteroid Breakup Rained Fire on the Inner Solar System]]></title>
            <link>https://www.universetoday.com/articles/800-million-years-ago-a-catastrophic-asteroid-breakup-rained-fire-on-the-inner-solar-system</link>
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            <pubDate>Tue, 21 Jul 2026 16:13:54 +0000</pubDate>
            <dc:creator><![CDATA[Andy Tomaswick]]></dc:creator>
            <author>Andy Tomaswick (https://www.universetoday.com/authors/andy-tomaswick)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/cosmic-collisions_20260721_161338.jpg" alt="Artist's depicion of the cause and consequnece of the Eulalia asteroid catastrophe. Credit - SwRI/Don Davis" width="1280" height="720" /></p><p>On Earth, it’s hard to track events that reshape its surface, as the surface itself is being reshaped constantly by weather and tectonic or volcanic upheavals. However, the Moon is much more static, and scientists have been slowly unraveling a pattern that is noticeable in its craters - that something dramatic happened around 800 million years ago. A new paper by researchers at the Southwest Research Institute (SwRI), led by Dr. William F. Bottke, and accepted for publication in the Planetary Science Journal, suggests they might have found a culprit - the parent body of a family of asteroids now known as Eulalia.</p>]]></description>
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            <title><![CDATA[Catch Comet 10P Tempel While You Can]]></title>
            <link>https://www.universetoday.com/articles/catch-comet-10p-tempel-while-you-can</link>
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            <pubDate>Tue, 21 Jul 2026 16:01:00 +0000</pubDate>
            <dc:creator><![CDATA[David Dickinson]]></dc:creator>
            <author>David Dickinson (https://www.universetoday.com/authors/david-dickinson)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/Jaeger-Rehmann_20260721_152547.jpg" alt="Comet 10P/Tempel from July 17th, 2026, with the orbital dust trail prominent as a bright streak across the image. Credit: Michael Jaeger/Gerald Rhemann." width="1280" height="720" /></p><p>A low-number periodic comet is stalking our fair planet this summer, and putting on its best show of several generations. We’re talking about Comet 10P/Tempel. The comet is currently loitering in the early dawn sky, presenting a good target for large binoculars or a small telescope. But act fast, as the comet is taking the plunge southward in August, post-perihelion.</p>]]></description>
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            <title><![CDATA[Chandrasekhar and the Limits of Physics, Part 2: Humiliation]]></title>
            <link>https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-2-humiliation</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-2-humiliation</guid>
            <pubDate>Tue, 21 Jul 2026 15:39:00 +0000</pubDate>
            <dc:creator><![CDATA[Paul Sutter]]></dc:creator>
            <author>Paul Sutter (https://www.universetoday.com/authors/pmsutter)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/ring_20260714_155156.jpg" alt="The Ring Nebula, another dying star's cast-off shell, lit from within by the hot white dwarf now forming at its center. Credit: NASA/ESA / Wikimedia Commons (public domain)." width="1280" height="720" /></p><p>In 1935 the most eminent astronomer alive stood up in a packed room and called Chandrasekhar's discovery "stellar buffoonery." The story of Arthur Eddington's years-long campaign against a result that everyone privately knew was correct.</p>]]></description>
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            <title><![CDATA[Researchers Narrow Down the Type of Meteorite that Killed the Dinosaurs]]></title>
            <link>https://www.universetoday.com/articles/researchers-narrow-down-the-type-of-meteorite-that-killed-the-dinosaurs</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/researchers-narrow-down-the-type-of-meteorite-that-killed-the-dinosaurs</guid>
            <pubDate>Mon, 20 Jul 2026 23:50:28 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/1-newanalysiso-1024x819_20260720_234314.jpg" alt="Artistic rendition of the Chicxulub impactor striking ancient Earth, with a Pterosaur observing. Credit: NASA" width="1280" height="720" /></p><p>An international team of Earth scientists has narrowed down the class of impactor that caused the Cretaceous-Paleogene extinction event. According to their findings, it was a rare type of rock that originated in the outer Solar System.</p>]]></description>
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            <title><![CDATA[Astronomers Determine that Exoplanets Around Barnard's Star are Extremely Uninhabitable]]></title>
            <link>https://www.universetoday.com/articles/astronomers-determine-that-exoplanets-around-barnards-star-are-extremely-uninhabitable</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/astronomers-determine-that-exoplanets-around-barnards-star-are-extremely-uninhabitable</guid>
            <pubDate>Mon, 20 Jul 2026 22:49:54 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/noirlab2510a_dp.jpg_20260720_214642.webp" alt="Artist’s illustration of exoplanets orbiting Barnard’s Star. Credit: [International Gemini Observatory/NOIRLab/NSF/AURA/P. Marenfeld](https://www.gemini.edu/gallery/images/noirlab2510a/)" width="1280" height="720" /></p><p>Scientists have painted the most detailed portrait yet of the planetary system orbiting Barnard’s Star. Unfortunately, the picture is not encouraging, as all four planets appear to be "extremely uninhabitable."</p>]]></description>
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            <title><![CDATA[Meet Our Newest Stellar Neighbours That Hid in the Glare of Other Stars]]></title>
            <link>https://www.universetoday.com/articles/meet-our-newest-stellar-neighbours-that-hid-in-the-glare-of-other-stars</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/meet-our-newest-stellar-neighbours-that-hid-in-the-glare-of-other-stars</guid>
            <pubDate>Mon, 20 Jul 2026 21:34:25 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/pce-binary-2-credit-mark-a.-garlick-university-of-warwick_20260720_212043.jpg" alt="This artist's illustration shows a white dwarf and its much larger red dwarf binary companion. Astronomers have four more of these binary stars in the Sun's neighborhood. They're called post-common-envelope binaries, and they're hard to detect because the bright red dwarf hides the white dwarf from telescopes. Image Credit: Mark A. Garlick/University of Warwick" width="1280" height="720" /></p><p>Astronomers have found four new white dwarfs within about 65 light years. Even though the sky has been studied thoroughly, these escaped detection. That's because they're tight binaries with red dwarf partners, and the much brighter red dwarfs hide the white dwarfs. The binaries used to share common envelopes.</p>]]></description>
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