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        <title><![CDATA[Universe Today]]></title>
        <description><![CDATA[Space and Astronomy News from Universe Today]]></description>
        <link>https://www.universetoday.com</link>
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        <lastBuildDate>Wed, 22 Jul 2026 22:43:52 +0000</lastBuildDate>
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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>
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            <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>
        </item>
        <item>
            <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>
            <guid isPermaLink="true">https://www.universetoday.com/articles/electrically-charged-mars-storms-threaten-future-exploration</guid>
            <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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        <item>
            <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>
            <guid isPermaLink="true">https://www.universetoday.com/articles/800-million-years-ago-a-catastrophic-asteroid-breakup-rained-fire-on-the-inner-solar-system</guid>
            <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>
            <guid isPermaLink="true">https://www.universetoday.com/articles/catch-comet-10p-tempel-while-you-can</guid>
            <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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            <title><![CDATA[Finding Venus Zone Planets with PLATO Will Show Us How Habitable Planets Evolve]]></title>
            <link>https://www.universetoday.com/articles/finding-venus-zone-planets-with-plato-will-show-us-how-habitable-planets-evolve</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/finding-venus-zone-planets-with-plato-will-show-us-how-habitable-planets-evolve</guid>
            <pubDate>Mon, 20 Jul 2026 18:16:14 +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/1280px-Venus_globe_20260720_160647.jpg" alt="Though this image is coloured to highlight Venus' surface features, it does a good job of presenting the planet's runaway greenhouse hellscape. In order to understand exoplanets in habitable zones, scientists need to find large numbers of Venus-like planets. The ESA's PLATO will help. Image Credit: By NASA/JPL - http://photojournal.jpl.nasa.gov/catalog/PIA00104, Public Domain, https://commons.wikimedia.org/w/index.php?curid=11826" width="1280" height="720" /></p><p>While simply finding exoplanets was an important first step in exoplanet science, more ambitious goals await. The ESA will launch PLATO in 2027 to search for rocky planets. But it will also find planets in the Venus Zone, a region bounded on its outer edge by a runaway greenhouse climate and on the inner edge by loss of atmosphere due to stellar flux. Understanding these planets will help scientists understand how Earth's path led to sustained habitability, while Venus, its sister planet, ended up with a runaway greenhouse climate.</p>]]></description>
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            <title><![CDATA[A Star Orbiting Our Galaxy's Supermassive Black Hole Tests the Limits of Relativity]]></title>
            <link>https://www.universetoday.com/articles/a-star-orbiting-our-galaxys-supermassive-black-hole-tests-the-limits-of-relativity</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/a-star-orbiting-our-galaxys-supermassive-black-hole-tests-the-limits-of-relativity</guid>
            <pubDate>Mon, 20 Jul 2026 17:53:51 +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/eso1644a_20260720_174825.jpg" alt="Illustration of a sunlike star passing very close to a supermassive black hole. Credit: ESO, ESA/Hubble, M. Kornmesser" width="1280" height="720" /></p><p>A Sun-like star orbits the supermassive black hole in our Milky Way so closely that it comes within the distance of Neptune's orbit of the Sun. It has a top speed of more than 8% of light speed. With such extreme motion the star gives astronomers the opportunity to test the limits of general relativity.</p>]]></description>
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            <title><![CDATA[Chandrasekhar and the Limits of Physics, Part 1: Triumph]]></title>
            <link>https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-1-triumph</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/chandrasekhar-and-the-limits-of-physics-part-1-triumph</guid>
            <pubDate>Mon, 20 Jul 2026 15:38:00 +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/helix_20260714_155103.jpg" alt="The Helix Nebula, the glowing shell thrown off by a dying star, with a hot white dwarf at its heart. White dwarfs, and the 1.4 solar mass limit that governs them, were Chandrasekhar's breakthrough. Credit: NASA/JPL-Caltech / Wikimedia Commons (public domain)." width="1280" height="720" /></p><p>The story of Subrahmanyan Chandrasekhar, who as a teenager on an ocean voyage worked out that white dwarf stars have a maximum mass of 1.4 Suns. A tour of degeneracy pressure, the relativistic insight everyone else missed, and the number that would define his life.</p>]]></description>
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            <title><![CDATA[The Case of the Sun's Missing Silver]]></title>
            <link>https://www.universetoday.com/articles/the-case-of-the-suns-missing-silver</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-case-of-the-suns-missing-silver</guid>
            <pubDate>Mon, 20 Jul 2026 05:15:18 +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/highresolutionsolarspectrum1200w_20260720_051306.jpg" alt="The Sun's spectrum, crossed by dark Fraunhofer lines where atoms in its outer layers absorb light at specific wavelengths, the fingerprint astronomers use to work out what a star is made of (Credit : NASA)" width="1280" height="720" /></p><p>Astronomers have solved a decades old puzzle about the Sun's missing silver, not by finding something new, but by modelling something old far more accurately. A revised, more realistic model of the Sun's atmosphere reveals it actually contains 55 per cent more silver than previously calculated, finally matching what meteorites have been telling us all along. It's a quiet reminder that some of the biggest revelations in astronomy come not from new data, but from asking familiar questions with sharper tools.</p>]]></description>
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            <title><![CDATA[The First Breath of Another World]]></title>
            <link>https://www.universetoday.com/articles/the-first-breath-of-another-world</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-first-breath-of-another-world</guid>
            <pubDate>Mon, 20 Jul 2026 04:58:02 +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/1280px-Artists_impression_of_the_super-Earth_exoplanet_LHS_1140b_20260720_045400.jpg" alt="Artist's impression of the planet LHS 1140 b and its host star (Credit : ESO/spaceengine.org)" width="1280" height="720" /></p><p>Astronomers have detected an atmosphere around a rocky planet in another star's habitable zone for the very first time. It’s a milestone that brings us a step closer to answering whether life could exist beyond our Solar System. Predicted by a mathematical model before it was ever observed, and confirmed using a rare planetary alignment 48 light years away, this discovery does more than identify one intriguing world, it provides us with a whole new way to search for others like it.</p>]]></description>
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            <title><![CDATA[NASA's Perseverance Rover Uncovers Evidence of 4 Billion Year Old Impacts]]></title>
            <link>https://www.universetoday.com/articles/nasas-perseverance-rover-uncovers-evidence-of-4-billion-year-old-impacts</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasas-perseverance-rover-uncovers-evidence-of-4-billion-year-old-impacts</guid>
            <pubDate>Sun, 19 Jul 2026 20:00:11 +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_-_PIA26574_-_Selfie_20260719_160426.jpg" alt="NASA’s Perseverance took this selfie at “Witch Hazel Hill” on Jezero Crater’s rim on May 10th, 2025. Credit: NASA/JPL-Caltech/MSSS" width="1280" height="720" /></p><p>Old rocks exposed on the rim of Jezero Crater preserve a roughly 4-billion-year-old cosmic “weather report” from the solar system’s most dynamic era.</p>]]></description>
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            <title><![CDATA[NASA’s Artemis III Lander Test Will be a "Dress Rehearsal" for Returning to the Moon!]]></title>
            <link>https://www.universetoday.com/articles/nasas-artemis-iii-lander-test-will-be-a-dress-rehearsal-for-returning-to-the-moon</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasas-artemis-iii-lander-test-will-be-a-dress-rehearsal-for-returning-to-the-moon</guid>
            <pubDate>Sun, 19 Jul 2026 02:41:29 +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/11_03_24_artemis_3_on_surfacelarge_20260718_225352.jpg" alt="Artist's impression of the Starship and Blue Moon Human Landing System (HLS) concepts on the lunar surface. Credit: SpaceX/Blue Origin" width="1280" height="720" /></p><p>Before Artemis astronauts land on the Moon’s surface in 2028, NASA will conduct the Artemis III demonstration mission in 2027, allowing teams on Earth and in orbit to practice rendezvous and docking operations between commercial human landing systems and the Orion spacecraft. Data from that mission, along with future uncrewed demonstration missions at the Moon,</p>]]></description>
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