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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, 26 Aug 2026 08:48:23 +0000</lastBuildDate>
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            <title><![CDATA[New Simulations Show How Galactic Centers Grow Together]]></title>
            <link>https://www.universetoday.com/articles/new-simulations-show-how-galactic-centers-grow-together</link>
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            <pubDate>Wed, 26 Aug 2026 01:28:39 +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/Portrait_of_the_Great_Barred_Spiral_20260825_233846.jpg" alt="NGC 1365 imaged by the Cerro Tololo Inter-American Observatory. Credit:DES/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA" width="1280" height="720" /></p><p>Using a state-of-the-art galaxy simulation, a team led by scientists from the Leibniz Institute for Astrophysics Potsdam (AIP) gained new insights into the processes shaping galactic centres across the Universe and the formation history of the Milky Way.</p>]]></description>
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        <item>
            <title><![CDATA[Surface Chemistry Shows Which Massive Stars Have Gained Mass from Binary Companions]]></title>
            <link>https://www.universetoday.com/articles/surface-chemistry-shows-which-massive-stars-have-gained-mass-from-binary-companions</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/surface-chemistry-shows-which-massive-stars-have-gained-mass-from-binary-companions</guid>
            <pubDate>Tue, 25 Aug 2026 19:39:00 +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/hpWRQLtpMVDH23PGbNyxdU-750-80_20260825_191700.jpg" alt="This artist's illustration shows a blue star gaining mass from its red giant companion. Mass transfer is common in massive stars, most of which are in binary relationships. A pair of researchers have developed a way to identify stars that have gained mass, even if the transfer happened a long time ago. Image Credit: NASA/ESA, A. Feild (STScI))" width="1280" height="720" /></p><p>Most stars, including massive ones, are in binary pairs. Astronomers think that about 70% of them have gained mass from their companions, but there's been no way to determine which ones have done so. Now, researchers have found a way.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[A Distant Stream of Stars May Offer New Clues to Dark Matter]]></title>
            <link>https://www.universetoday.com/articles/a-distant-stream-of-stars-may-offer-new-clues-to-dark-matter</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/a-distant-stream-of-stars-may-offer-new-clues-to-dark-matter</guid>
            <pubDate>Tue, 25 Aug 2026 18:53:39 +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/Kuglehobestr_m_1100x600_20260825_183618.jpg" alt="A Hubble Space Telescope view of the ultra-diffuse galaxy UGC9050-Dw1 and a stream of stars from an associated globular cluster. The stream is shaped by the influence of dark matter. Credit: STScI, Holm, et al." width="1280" height="720" /></p><p>Dark matter continues to challenge astronomers as they work to solve the mystery of this so-far-unseen material that permeates the Universe. It's not that the stuff doesn't exist. It does, but we just can't see it. The only way it can be detected is by its gravitational effects on ordinary matter. A team of researchers led by University of Copenhagen PhD student Julie Kiel Holm has found a stream of stars stretching out more than 3,000 light-years from a globular cluster that appears to have been shaped by dark matter in a distant galaxy.</p>]]></description>
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            <title><![CDATA[Comet 220P McNaught Puts On An Encore Performance]]></title>
            <link>https://www.universetoday.com/articles/comet-220p-mcnaught-puts-on-an-encore-performance</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/comet-220p-mcnaught-puts-on-an-encore-performance</guid>
            <pubDate>Tue, 25 Aug 2026 17:27:00 +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/55480209808_493f7548c5_c_20260825_153738.jpg" alt="Comet 220P McNaught from August 22nd. Credit: Frank Astro." width="1280" height="720" /></p><p>It has been a busy month for astronomy. In the midst of an eclipse season bookended by the total solar eclipse on August 12th and the deep partial lunar eclipse coming right up this week on August 28th, an outbound comet hanging high in the dawn sky just refuses to die: 220P/McNaught.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[NASA Starshade Would Enable Astronomers To Directly Image Rocky Exoworlds]]></title>
            <link>https://www.universetoday.com/articles/nasa-starshade-would-enable-astronomers-to-directly-image-rocky-exoworlds</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasa-starshade-would-enable-astronomers-to-directly-image-rocky-exoworlds</guid>
            <pubDate>Mon, 24 Aug 2026 07:16:54 +0000</pubDate>
            <dc:creator><![CDATA[Bruce Dorminey]]></dc:creator>
            <author>Bruce Dorminey (https://www.universetoday.com/authors/bruce)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/Starshade_Artists_Concept_2_PIA20911_20260122_162947.jpg" alt="An artist's concept of a generic starshade.  Credit:  Public Domain" width="1280" height="720" /></p><p>Innovative NASA-funded orbital starshade could help capture first direct images from extrasolar earths.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[Astronomers Use Rare Ultra-Magnetic Star to Crack a Quantum Mystery]]></title>
            <link>https://www.universetoday.com/articles/astronomers-use-rare-ultra-magnetic-star-to-crack-a-quantum-mystery</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/astronomers-use-rare-ultra-magnetic-star-to-crack-a-quantum-mystery</guid>
            <pubDate>Sun, 23 Aug 2026 22:19:31 +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/cq5dam.web.2560.1440_20260823_214012.jpeg" alt="A Swinburne astronomer may have just confirmed one of the quirkiest aspects of quantum mechanics: that seemingly empty space can alter the behavior of light. Credit: NASA." width="1280" height="720" /></p><p>An international team observed a magnetar known as 1E 1547.0–5408 using NASA’s Imaging X-ray Polarimetry Explorer (IXPE), leading to what could be the first detection of vacuum birefringence taking place in the magnetar’s ultra-strong magnetic field. These findings could potentially resolve a long-standing mystery quantum mechanics.</p>]]></description>
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            <title><![CDATA[NASA Highlights Next-Gen Cargo Landers Paving the Way for a Moon Base]]></title>
            <link>https://www.universetoday.com/articles/nasa-highlights-next-gen-cargo-landers-paving-the-way-for-a-moon-base</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasa-highlights-next-gen-cargo-landers-paving-the-way-for-a-moon-base</guid>
            <pubDate>Sun, 23 Aug 2026 13:01:35 +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/moon-base-update-slate_20260823_130110.webp" alt="Artist's depiction of a NASA moon based, along with it's update imagery. Credit - NASA" width="1280" height="720" /></p><p>NASA and its commercial partners are making progress on their way to a permanent human presence on the Moon. As part of that, a recent press release and accompanying YouTube video hints they may be looking to provide regular updates to the progress of those efforts - and, at least for this first one, that progress looks pretty good.</p>]]></description>
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            <title><![CDATA[White Dwarf-Red Dwarf Binaries Power Cosmic Lasers]]></title>
            <link>https://www.universetoday.com/articles/synchronized-stars-power-cosmic-radio-laser</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/synchronized-stars-power-cosmic-radio-laser</guid>
            <pubDate>Sat, 22 Aug 2026 23:02:54 +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/WD_MD.original_20260822_182847.png" alt="Artwork of a white dwarf–M dwarf binary stars. The white dwarf's magnetic field lines, which are stronger than those from the M dwarf, play a key role in creating long-period bursts of radio emission observed from binary stars like these. Credit: Elias Most (AI-generated)" width="1280" height="720" /></p><p>Researchers have helped unravel the mystery of why certain pairs of stars pulse with regular, long-period bursts of radio waves. The particular class of objects they observed come in pairs that always include a compact dead star, called a white dwarf, locked in orbit with an M dwarf, a red star smaller than our Sun.</p>]]></description>
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            <title><![CDATA[Dry Martian Meteorite Reveals Early Water in Mars's Crust]]></title>
            <link>https://www.universetoday.com/articles/dry-martian-meteorite-reveals-early-water-in-marss-crust</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/dry-martian-meteorite-reveals-early-water-in-marss-crust</guid>
            <pubDate>Sat, 22 Aug 2026 04:37:04 +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/MarsMeteorite-NWA7034-716969main_black_beauty_full.jpg_750_20260822_042904.jpg" alt="Meteorite Northwest Africa 7034 (NWA 7034) aka Black beauty. (Credit: NASA)" width="1280" height="720" /></p><p>Billions of years ago, Mars was hypothesized to have been a habitable world with flowing liquid water and the potential for life. But directly studying its ancient past is currently limited to orbiters and rovers, as scientists have yet to obtain direct samples from Mars. However, meteorites have been found on Earth to have potentially originated from Mars during large impacts that flung chunks of the Red Planet into space, eventually being grabbed by Earth’s gravity and crashing into the Earth’s surface.</p>]]></description>
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            <title><![CDATA[The CosmoCube Satellite Will Listen to the Early Universe From the Far Side of the Moon]]></title>
            <link>https://www.universetoday.com/articles/the-cosmoquest-satellite-will-listen-to-the-early-universe-from-the-far-side-of-the-moon</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-cosmoquest-satellite-will-listen-to-the-early-universe-from-the-far-side-of-the-moon</guid>
            <pubDate>Fri, 21 Aug 2026 23:33:00 +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/CosmoCube_CREDIT_Surrey_Space_Technology_Ltd.jpg_20260821_223505.webp" alt="None" width="1280" height="720" /></p><p>A tiny UK-developed satellite, roughly the size of a small carry-on suitcase, could help answer one of the biggest questions in cosmology: what happened in the roughly 150 million years of cosmic dark ages, before the universe’s first stars appeared?</p>]]></description>
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        <item>
            <title><![CDATA[Strange Signals Called Long-period Radio Transits Come From Cataclysmic Variables]]></title>
            <link>https://www.universetoday.com/articles/strange-signals-called-long-period-radio-transits-come-from-cataclysmic-variables</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/strange-signals-called-long-period-radio-transits-come-from-cataclysmic-variables</guid>
            <pubDate>Fri, 21 Aug 2026 19:59:01 +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/ASKAP-Rose-WD-e1780465074367_20260820_225651.jpg" alt="This iullustration shows a white dwarf star accreting material from its companion. New research says that this can explain at least one of the puzzling Long Period Radio Transients, mysterious radio signals that repeat with periods ranging from a few minutes to a few hours. Image Credit: Carl Knox (OzGrav, Swinburne University of Technology) and Joshua Preston Pritchard (CSIRO)." width="1280" height="720" /></p><p>Long-period Radio Transients are sources that emit repeating radio and x-ray signals. The signals are polarized and coherent, and are similar to pulsars in some respects. But the type of astrophysical object responsible for them has been vigorously debated. New research says that at least one of them comes from a cataclysmic variable, a binary star where a white dwarf and a red dwarf orbit closely.</p>]]></description>
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            <title><![CDATA[New Solar System Models Show Earth Is No Fluke]]></title>
            <link>https://www.universetoday.com/articles/new-solar-system-models-show-earth-is-no-fluke</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/new-solar-system-models-show-earth-is-no-fluke</guid>
            <pubDate>Fri, 21 Aug 2026 07:12:12 +0000</pubDate>
            <dc:creator><![CDATA[Bruce Dorminey]]></dc:creator>
            <author>Bruce Dorminey (https://www.universetoday.com/authors/bruce)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/The_Blue_Marble_AS17-148-22727_20260821_070011.jpg" alt="The Blue Marble Credit: Harrison Schmitt / Apollo 17" width="1280" height="720" /></p><p>Astrobiologists use new starting points to produce ‘organic’ models of our solar system’s formation.</p>]]></description>
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            <title><![CDATA[NASA's Lunar Reconnaissance Orbiter Images Falcon 9 Crater on Moon, With Some Help From a Korean Spacecraft]]></title>
            <link>https://www.universetoday.com/articles/nasas-lunar-reconnaissance-orbiter-images-falcon-9-crater-on-moon-with-some-help-from-a-korean-space</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasas-lunar-reconnaissance-orbiter-images-falcon-9-crater-on-moon-with-some-help-from-a-korean-space</guid>
            <pubDate>Thu, 20 Aug 2026 21:16:02 +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/no_crater_crater_20260820_211152.jpg" alt="These images from NASA's Lunar Reconnaissance Orbiter show the Falcon upper-stage's crash site on the Moon. The left image is before the crash, the right image is after, showing the impact crater. Image Credit: NASA Goddard/Intuitive Machines" width="1280" height="720" /></p><p>A SpaceX Falcon upper stage crashed into the Moon on August 5th. NASA's Lunar Reconnaissance Orbiter captured images of the crash site from different viewing angles and with different sunlight angles. The images showed that the crater is about 18 meters wide and about 3 meters deep. SpaceX says the crash was an accident.</p>]]></description>
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            <title><![CDATA[Mars's Funky Moon Deimos was Shaped by an Impact]]></title>
            <link>https://www.universetoday.com/articles/marss-funky-moon-deimos-was-shaped-by-an-impact</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/marss-funky-moon-deimos-was-shaped-by-an-impact</guid>
            <pubDate>Thu, 20 Aug 2026 19:21:06 +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/Deimos_with_crater_20260820_172124.jpg" alt="This illustration shows Mars' moon Deimos and its distinctive south pole depression. Thought the moon's surface appears smoother than its sibling Phobos, it's still been battered by impacts. One major impact created the south pole crater, and also spread a layer of regolith on the moon's surface. Image Credit: NASA Eyes on the Solar System." width="1280" height="720" /></p><p>Mars' moon Deimos has a large crater on its southern pole. It's also covered by a layer of regolith so deep it buries many other, smaller craters. New research shows that an impact is responsible for both, and that the moon is rather fragile and porous, like a rubble pile asteroid.</p>]]></description>
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            <title><![CDATA[How Gas Filaments and Interfilaments Feed Star Formation in Monoceros R2]]></title>
            <link>https://www.universetoday.com/articles/how-gas-filaments-and-interfilaments-feed-star-formation-in-monoceros-r2</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/how-gas-filaments-and-interfilaments-feed-star-formation-in-monoceros-r2</guid>
            <pubDate>Thu, 20 Aug 2026 16:50:20 +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/20260_Hwang_Fig.1-2_20260819_192055.jpg" alt="This illustration shows dense gas (green arrows) moving along filaments into a star forming hub. It also shows less dense (blue arrows) gas flowing through the interfilament regions. Observations show that the dense gas moves more quickly than the gas in the interfilament regions. But the less dense gas also plays an important role. It moves more slowly and sideways into the filaments, replenishing their supply. Image Credit: Jihye Hwang/Kyushu University." width="1280" height="720" /></p><p>Researchers studied gas flows in the Monoceros R2 star forming region to understand how gas is channeled into star forming hubs. By tracing the flow of carbon monoxide, they found that a system of hub-filaments and interfilaments are responsible for feeding gas into star-forming locations. The filaments move most of the gas, but the interfilaments play a role too, especially by feeding more gas into the main filaments.</p>]]></description>
        </item>
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            <title><![CDATA[Catching An 'Almost Total' Lunar Eclipse on August 28th]]></title>
            <link>https://www.universetoday.com/articles/catching-an-almost-total-lunar-eclipse-on-august-28th</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/catching-an-almost-total-lunar-eclipse-on-august-28th</guid>
            <pubDate>Thu, 20 Aug 2026 15:21:00 +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/Screenshot_2026-08-19_130300_20260819_174721.png" alt="A fine view of the March 14th 2025 lunar eclipse. Credit: Marion Haligowski." width="1280" height="720" /></p><p>So, did you miss the August 12th total solar eclipse? Like lots of humanity, we sat out the celestial drama of this month's solar eclipse, both total and partial. But the good news is, a large swath of the world can still catch the eclipse season spirit, with a deep, nearly total partial lunar eclipse next week. The event is the last eclipse of four (two lunar and two solar) for 2026. This also marks the current end of the second eclipse season for 2026, which began with the total solar eclipse on August 12th.</p>]]></description>
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            <title><![CDATA[What Can We Actually Find on an Exoplanet? Part 4: Looking For Us]]></title>
            <link>https://www.universetoday.com/articles/what-can-we-actually-find-on-an-exoplanet-part-4-looking-for-us</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/what-can-we-actually-find-on-an-exoplanet-part-4-looking-for-us</guid>
            <pubDate>Thu, 20 Aug 2026 10:19:00 +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_20260814_095912.jpg" alt="Earth at night, its city lights tracing the footprint of human civilization. Industry leaves atmospheric technosignatures an alien astronomer might detect. Credit: NASA (public domain)." width="1280" height="720" /></p><p>Some signs of an alien civilization are easier to spot than signs of life itself. On technosignatures, from CFCs and industrial gases to the pandemic dip in pollution, and why Earth's most detectable moment might be right now.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[Webb Captures the Treasure Chest at the Heart of the Carina Nebula]]></title>
            <link>https://www.universetoday.com/articles/webb-captures-the-treasure-chest-at-the-heart-of-the-carina-nebula</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/webb-captures-the-treasure-chest-at-the-heart-of-the-carina-nebula</guid>
            <pubDate>Wed, 19 Aug 2026 21:37:46 +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/2000x960_20260819_203003.jpg" alt="Hubble image of the Carina Nebula (NGC 3372), which lies just 7500 light-years away in the constellation Carina (the Keel). Credit: NASA/ESA/UC Berkeley/STScI/NOAO/AURA/NSF" width="1280" height="720" /></p><p>This NASA/ESA/CSA James Webb Space Telescope Picture of the Month takes us to a fantastical realm within our home galaxy, where piercing starlight and billowing winds sculpt dust clouds into inventive shapes. This scene is from the Carina Nebula, which lies just 7500 light-years away in the constellation Carina (the Keel).</p>]]></description>
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            <title><![CDATA[Pluto Planetary Science is the Gift that Keeps on Giving]]></title>
            <link>https://www.universetoday.com/articles/pluto-planetary-science-is-the-gift-that-keeps-on-giving</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/pluto-planetary-science-is-the-gift-that-keeps-on-giving</guid>
            <pubDate>Wed, 19 Aug 2026 20:12:54 +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/Pluto-01_Stern_03_Pluto_Color_TXT_20260812_215944.jpg" alt="Pluto as seen by New Horizons during its 2015 flyby. Sputnik Planitia is a heart-shaped region that appears to be resurfaced by upwelling liquid nitrogen from below. That action creates what look like convection cells outlined by darker lines that could be flow channels. Credit: NASA/JHU/APL/New Horizons mission" width="1280" height="720" /></p><p>Something's wetting the surface of dwarf planet Pluto along the northern edge of Sputnik Planitia, and planetary scientists have found a good explanation for it. A recent study of new Horizons images taken during the 2015 flyby revealed evidence that liquid nitrogen is rising up through cracks in Sputnik Planitia. That's the giant heart-shaped glacial basin we see in all the Pluto images taken by the spacecraft.</p>]]></description>
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            <title><![CDATA[The Fastest Star in the Milky Way Will Test Relativity]]></title>
            <link>https://www.universetoday.com/articles/the-fastest-star-in-the-milky-way-will-test-relativity</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-fastest-star-in-the-milky-way-will-test-relativity</guid>
            <pubDate>Wed, 19 Aug 2026 18:30:57 +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/eso2612a_20260819_172156.jpg" alt="These panels are Very Large Telescope images of the star S301 orbiting the Milky Way's SMBH, SgrA*. S301 is the fastest moving S star ever found, and also the closest to the black hole. The star can be used to measure the black hole's spin. S301's orbit is shown with an elliptical curve. In each frame, the solid curve shows the path that the star has already completed up to that point, whereas the dashed one marks the path it will follow afterwards. Image Credit: ESO/GRAVITY collaboration" width="1280" height="720" /></p><p>Astronomers have discovered another S star, the population of stars that orbits the Milky Way's SMBH. This one is the fastest of them all, and also comes closest to the SMBH. It will let astronomers test relativity, especially the Lense-Thirring effect.</p>]]></description>
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