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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, 11 Nov 2026 22:13:18 +0000</lastBuildDate>
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        <item>
            <title><![CDATA[The Ice Giants' Magnetic Fields are Very Strange Compared to Earth's]]></title>
            <link>https://www.universetoday.com/articles/the-ice-giants-magnetic-fields-are-very-strange-compared-to-earths</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-ice-giants-magnetic-fields-are-very-strange-compared-to-earths</guid>
            <pubDate>Wed, 11 Nov 2026 22:09:35 +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/ChiYan-Primary-Art-1-1536x864_20261111_184441.jpg" alt="These images show the Uranus-like (left) and Neptune-like (right) dynamo models for the ice giants. The tubes represent the magnetic fields, and the small gold arrows indicate the local field direction. Image Credit: Yan et al. 2026" width="1280" height="720" /></p><p>Uranus and Neptune, the Solar System's ice giants, have interiors unlike the other planets. As a result, they also have magnetic fields unlike the others. They're messy and tilted, and Voyager 2, the only spacecraft to even flyby them, showed us how messy they are. New research uses models to try to understand what's going on with the pair of planets and their weird fields, and found that it's likely they change on very short timescales. They could already be much different than when Voyager 2 visited in the late 1980s.</p>]]></description>
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            <title><![CDATA[Asteroid Mining Will Crash the Platinum Market, But That’s Good News for Earth]]></title>
            <link>https://www.universetoday.com/articles/asteroid-mining-will-crash-the-platinum-market-but-thats-good-news-for-earth</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/asteroid-mining-will-crash-the-platinum-market-but-thats-good-news-for-earth</guid>
            <pubDate>Wed, 11 Nov 2026 17:06:51 +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/PIA21275_-_Psyche_Artists_Concept_20261111_170620.jpg" alt="Artist's concept of a spacecraft flying by Psyche, the most famous M-type asteroid. Credit - NASA / JPL-Caltech" width="1280" height="720" /></p><p>Science fiction authors have been dreaming of robotic spacecraft harvesting fortunes from asteroids for decades. Humanity is slowly getting closer to that reality. But if you ask asteroid mining skeptics, they will usually ask one specific question - what happens to the prices of all those rare materials once someone actually brings them back? A pair of system dynamicists from MIT directly tackled that question with a new paper titled Will AstroForge Collapse the PGM Market?</p>]]></description>
        </item>
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            <title><![CDATA[The Chandra X-Ray Observatory Unmasks a Supernova Impostor]]></title>
            <link>https://www.universetoday.com/articles/the-chandra-x-ray-observatory-unmasks-a-supernova-impostor</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-chandra-x-ray-observatory-unmasks-a-supernova-impostor</guid>
            <pubDate>Wed, 11 Nov 2026 16:41:55 +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/at2016blu_labeled_20261111_140315.jpg" alt="This is a composite NASA Chandra X-ray and Sloan Digital Sky Survey (SDSS) optical image of the galaxy NGC 4559 located about 30 million light-years from Earth. The Chandra data shows X-ray point sources represented in purple, and the SDSS data shows the galaxy and foreground and background objects in red and blue. The luminous blue variable and supernova impostor AT 2016blu is in the middle of the small square. Image Credit: X-ray: NASA/CXC/Univ. of Virginia/M. Aghakhanloo et al.; Optical: SDSS; Image Processing: NASA/CXC/SAO/P. Edmonds" width="1280" height="720" /></p><p>Some stars, called Luminous Blue Variables, can be confused with supernovae explosions. They exhibit similar outbursts, but unlike supernovae, which explode once and then are gone forever, these stars have periodic outbursts. New research found that one of these 'supernova impostors' is in a binary relationship with a black hole or a neutron star, and that explains its periodic outbursts.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[Planets Don't Just Disappear, But They Can Wobble Out of Sight if Their Neighbour is Close Enough]]></title>
            <link>https://www.universetoday.com/articles/planets-dont-just-disappear-but-they-can-wobble-out-of-sight-if-their-neighbour-is-close-enough</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/planets-dont-just-disappear-but-they-can-wobble-out-of-sight-if-their-neighbour-is-close-enough</guid>
            <pubDate>Wed, 11 Nov 2026 13:02:29 +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/image_7543-Hot-Jupiter_20261110_222441.jpg" alt="This artist's illustration shows a hot Jupiter, a giant planet very close to its star with a very short orbital period. TESS watched one hot Jupiter transit its star for seven years, until it wasn't visible anymore. New research says that another nearby giant planet is responsible for tugging the hot Jupiter out of view. Image Credit: C. Carreau / ESA." width="1280" height="720" /></p><p>TESS watched an exoplanet about 1,000 light years away as it repeatedly transited in front of its star for seven years. But astronomers were surprised to find that the hot Jupiter disappeared. Of course, planets don't just disappear. Something interrupted its transits from our point of view, and astronomers think they've figured out what happened. An unseen, nearby giant planet companion tugged on it until TESS couldn't see it anymore.</p>]]></description>
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        <item>
            <title><![CDATA[Automated Assembly in Space is the Future and NOM4D is Showing the Way]]></title>
            <link>https://www.universetoday.com/articles/automated-assembly-in-space-is-the-future-and-nom4d-is-showing-the-way</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/automated-assembly-in-space-is-the-future-and-nom4d-is-showing-the-way</guid>
            <pubDate>Tue, 10 Nov 2026 19:52:32 +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/program-darpa-nom4d-phase-3_20261110_173344.jpg" alt="This artist's illustration shows what the future of in-space assembly might look like with NOM4D (Novel Orbital and Moon Manufacturing, Materials and Mass-efficient Design.) The inset image shows a liquid monomer being heated and forming a hardened polymer. It's a self-propagating reaction that can create long structural tubes. The larger image shows a robotic arm manipulating the tube into position to create a larger support structure. Though NOM4D hasn't yet performed this process, a recent test saw it assemble individual components manufactured on the ground into a truss structure. Image Credit: University of Illinois Urbana-Champaign" width="1280" height="720" /></p><p>The ability to build large structures in space is maturing. The ISS, Mir, and Tiangong were built in space from pre-constructed modules, but a new program called NOM4D is taking space construction to the next level. It recently showed that a simple robot can create truss-like structures in space from premade components. Is the sky the limit for NOM4D?</p>]]></description>
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            <title><![CDATA[ALMA Reveals a Jet of Cool Gas from a Microquasar]]></title>
            <link>https://www.universetoday.com/articles/alma-reveals-a-jet-of-cool-gas-from-a-microquasar</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/alma-reveals-a-jet-of-cool-gas-from-a-microquasar</guid>
            <pubDate>Tue, 10 Nov 2026 19:39:42 +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/LMC_P3_Within_Remnant_DEM_L241-1024x575_20261110_193137.jpg" alt="This object, called LMC P3, emits gamma-ray signals but also has smoking gun proof of a cool jet streaming away from it. Credit: Chandra X-ray Observatory Center/NASA’s Goddard Space Flight Center" width="1280" height="720" /></p><p>There's a strange gamma-ray emitter in the Large Magellanic Cloud that has astronomers stumped about its source. It lies within the ashes left behind by a supernova that created a compact object that's part of the system. The supernova remnant provides some evidence for the emissions, but not the whole story.</p>]]></description>
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            <title><![CDATA[First Direct Measurement of Cosmic Hydrogen Could Change How We Map the Universe]]></title>
            <link>https://www.universetoday.com/articles/breakthrough-cosmic-hydrogen-measurement-could-transform-our-view-of-the-universe</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/breakthrough-cosmic-hydrogen-measurement-could-transform-our-view-of-the-universe</guid>
            <pubDate>Tue, 10 Nov 2026 19:01:00 +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/demo_sky_image_20261110_185831.png" alt="Visualization of the distribution of matter in the cosmic web. Credit: MeerKLASS" width="1280" height="720" /></p><p>The MeerKLASS international collaboration achieves the first direct measurement of the large-scale clustering of cosmic hydrogen in the Universe.</p>]]></description>
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            <title><![CDATA[Why Aging Stars Suffer A Sudden Luminosity Dip]]></title>
            <link>https://www.universetoday.com/articles/why-aging-stars-suffer-a-sudden-luminosity-dip</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/why-aging-stars-suffer-a-sudden-luminosity-dip</guid>
            <pubDate>Tue, 10 Nov 2026 17:22:37 +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/STScI-01J1X25A66FJK08ZQSZP6TH1GZ_20260723_230143.jpg" alt="This Hubble image shows the well-known Omega Centauri globular cluster. Most of the orange and yellow stars are RGB stars. These stars exhibit a dip in luminosity called the RGB luminosity bump, which has puzzled astrophysicists. New research may have an explanation. Image Credit: ESA/Hubble, NASA, Maximilian Häberle (MPIA)" width="1280" height="720" /></p><p>When low-mass stars like our Sun age, they leave the main sequence and follow the Red Giant Branch. As they ascend this branch, their luminosity steadily increases. But there's a sort of hiccup in the path called the RGB luminosity bump, where their luminosity suddenly dips. Astrophysicists have struggle to explain this, but one astrophysicist might have the answer.</p>]]></description>
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            <title><![CDATA[Tiny Solar Whirlpools May Hold the Secret to the Sun’s Blistering Corona]]></title>
            <link>https://www.universetoday.com/articles/tiny-solar-whirlpools-may-hold-the-secret-to-the-suns-blistering-corona</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/tiny-solar-whirlpools-may-hold-the-secret-to-the-suns-blistering-corona</guid>
            <pubDate>Tue, 10 Nov 2026 14:07:10 +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/kh-waves-on-sun_20261110_140634.jpg" alt="Image of KH waves on the Sun. Credit - NSF/NSO/AURA/MPS/Inouye Tel" width="1280" height="720" /></p><p>For the second time in a few weeks, we’re writing about research into the temperature gap between the Sun’s surface and its corona. More and more data from various missions continue to feed this wave of discovery. A new paper by Katariina Nykyri of Embry-Riddle, recently published in The Astrophysical Journal Letters, adds to this growing body of work. She argues that millions of tiny whirlpools scattered across the Sun’s surface could be the energetic engine driving that temperature difference.</p>]]></description>
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            <title><![CDATA[Using Vibrations and AI, Future Robotic Missions Could Handle Buried Rocks Autonomously]]></title>
            <link>https://www.universetoday.com/articles/virginia-tech-researchers-use-vibrations-and-ai-to-estimate-depth-of-buried-objects-for-future-lunar</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/virginia-tech-researchers-use-vibrations-and-ai-to-estimate-depth-of-buried-objects-for-future-lunar</guid>
            <pubDate>Mon, 09 Nov 2026 21:44:00 +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/subsurfacewater_Mars-1024x768_20261109_211716.jpg" alt="Artist's impression of a cutaway showing Mars' subsurface layers. Credit: ESA/Medialab" width="1280" height="720" /></p><p>Mechanical engineering assistant professor Erik Komendera developed a method that combines vibrations and AI to determine how deeply a rock is buried, helping robots clear terrain more efficiently.</p>]]></description>
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            <title><![CDATA[Mars' Molten Heart is Long Gone, but Some Magma Chambers May Persist]]></title>
            <link>https://www.universetoday.com/articles/mars-molten-heart-is-long-gone-but-some-magma-chambers-may-persist</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/mars-molten-heart-is-long-gone-but-some-magma-chambers-may-persist</guid>
            <pubDate>Mon, 09 Nov 2026 21:25:39 +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/Alba-Mons-HCl_20261109_210137.jpg" alt="We've known about HCl in Mars' atmosphere for some time, thanks to the Trace Gas Orbiter. They were attributed to atmospheric interactions due to warmth during perihelion. But the same chemical has been detected at aphelion, and researchers think it may be venting into the atmosphere from underground magma chambers. If that's true, then Mars isn't as dormant as thought. Image Credit: MEX/HRSC global color mosaic, ESA/DLR/FU Berlin, G. Michael. Inset: Blended MOLA-HRSC digital elevation model, Fergason et al 2018" width="1280" height="720" /></p><p>Mars may be more volcanically active than we thought, according to new research. The Trace Gas Orbiter detected HCl, a chemical associated with magma, at a time of year that's difficult except by volcanic origins. The new research also identified new surface fissures on Mars that could be the source of the chemical.</p>]]></description>
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            <title><![CDATA[A Perseverance Experiment Could Help Astronauts Prepare for Dust Storms on Mars]]></title>
            <link>https://www.universetoday.com/articles/a-perseverance-experiment-could-help-astronauts-prepare-for-dust-storms-on-mars</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/a-perseverance-experiment-could-help-astronauts-prepare-for-dust-storms-on-mars</guid>
            <pubDate>Mon, 09 Nov 2026 19:56:35 +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/resizepia26520-perseverance-and-sherlocs-calibration-target-1200x700_20261109_194634.jpg" alt="The rover Perseverance carries swatches of spacesuit material to test the impacts of Martian dust. Image: NASA/JPL-Caltech" width="1280" height="720" /></p><p>Researchers at Washington University examined how dust interacts with the spacesuit swatches on the Perseverance Rover. Future missions to Mars require that planners account for the effects of dust exposure on humans and materials.</p>]]></description>
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            <title><![CDATA[An Artificial CORTEX to Guide Satellite Rescue Missions]]></title>
            <link>https://www.universetoday.com/articles/an-artificial-cortex-to-guide-satellite-rescue-missions</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/an-artificial-cortex-to-guide-satellite-rescue-missions</guid>
            <pubDate>Mon, 09 Nov 2026 18:36:51 +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/Debris_objects_in_low-Earth_orbit_LEO-media-9a2dd926-query2x.1b400515_20261109_183647.jpg" alt="This illustration is exaggerated and isn't to scale, but it highlights the growing space debris problem. Some of the debris isn't really junk; it's zombie satellites. Researchers are developing an autonomous framework called CORTEX for guiding servicing satellites to dock with these zombies and revive them. Image Credit: ESA" width="1280" height="720" /></p><p>Thousands of so-called zombie satellites orbit Earth in the critical Low-Earth Orbit regime. They're either inactive or have stopped alerting other satellites to their presence. Researchers are building a system called CORTEX that can guide a repair satellite to autonomously dock with these zombies.</p>]]></description>
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            <title><![CDATA[A Common Food Emulsifier Could Solve One of Rocketry’s Oldest Fuel Problems]]></title>
            <link>https://www.universetoday.com/articles/a-common-food-emulsifier-could-solve-one-of-rocketrys-oldest-fuel-problems</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/a-common-food-emulsifier-could-solve-one-of-rocketrys-oldest-fuel-problems</guid>
            <pubDate>Mon, 09 Nov 2026 17:22:56 +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/new-gel-fuel-could-mak_20261109_172122.jpg" alt="Graphic of the chemical process of fuel creation. Credit - P. Mudaliar &amp; J. John" width="1280" height="720" /></p><p>In propulsion system design, engineers have long faced a trade-off between solid and liquid rocket fuels. Each has advantages and disadvantages, and in an effort to try to min/max the efficacy of different types of fuel, researchers have long placed an emphasis on a hybrid between solids and liquids - in other words they’ve been working with gels. Unfortunately, gels have their own sets of problems to deal with. But a new paper published by Pranay Mudaliar and Jerin John of Concordia in the journal Langmuir uses an uncommon ingredient to elegantly solve some of those problems, but which is typically used in a completely different area of human activity - lecithin.</p>]]></description>
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            <title><![CDATA[A Stellar Odd Couple at an Unusual Stage of Evolution]]></title>
            <link>https://www.universetoday.com/articles/a-stellar-odd-couple-at-an-unusual-stage-of-evolution</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/a-stellar-odd-couple-at-an-unusual-stage-of-evolution</guid>
            <pubDate>Mon, 09 Nov 2026 14:39:00 +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/Figura2_20261109_162512.jpg" alt="Artist's impression of the binary system NGC 362d. On the left, the millisecond pulsar draws material from its white dwarf companions, and emits beams of radio waves; on the right, the young white dwarf is surrounded by material leftover from the previous mass transfer. Image Credit: INAF (Image generated using artificial intelligence.)" width="1280" height="720" /></p><p>Millisecond pulsars are fascinating objects that serve as natural clocks in the Universe. They form by drawing material and angular momentum from a companion. This mass transfer can rapidly accelerate the companion's evolution to a white dwarf. Astronomers have detected a millisecond pulsar's white dwarf companion that appears to be observed just as the mass transfer completed. They can still see some of the debris.</p>]]></description>
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            <title><![CDATA[Nearby Dwarf Galaxies Show Surprising Lack Of Oxygen, Says Paper]]></title>
            <link>https://www.universetoday.com/articles/nearby-dwarf-galaxies-show-surprising-lack-of-oxygen-says-paper</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nearby-dwarf-galaxies-show-surprising-lack-of-oxygen-says-paper</guid>
            <pubDate>Mon, 09 Nov 2026 08:11:11 +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/STScI-01M4RST3TGWT2T53FVXQBSP75D_1_20261109_080246.jpg" alt="Image from NASA’s Hubble Space Telescope of NGC 4449, one of the dwarf galaxies in the Galaxies Losing Oxygen via Winds (GLOW) study. Researchers found that dwarf galaxies can hold onto only a small fraction of the oxygen made by their stars. 
Credit:  NASA, ESA, Hubble Heritage–ESA/Hubble Collaboration, Alessandra Aloisi (STScI, ESA)" width="1280" height="720" /></p><p>A new study of more than three dozen dwarf galaxies has surprised researchers with just how little oxygen they have been able to retain over cosmic time.  The results reveal that we still have major gaps in our understanding of galaxy evolution.</p>]]></description>
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            <title><![CDATA[Our Sun’s Undiscovered Stellar Nemesis Is Still Out There, Says Physicist]]></title>
            <link>https://www.universetoday.com/articles/our-suns-undiscovered-stellar-nemesis-is-still-out-there-says-physicist</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/our-suns-undiscovered-stellar-nemesis-is-still-out-there-says-physicist</guid>
            <pubDate>Sat, 07 Nov 2026 08:47:00 +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/Comet_2021_A1_Leonard_20261107_091553.jpg" alt="The long period Oort Cloud Comet Leonard as seen in 2021.  Credit:  Wikipedia" width="1280" height="720" /></p><p>The decades old idea that our solar system’s Oort Cloud is continually perturbed by a heretofore undetected low mass Red Dwarf star remains the best explanation for periodicities found in Earth’s impact record.  Or so says a well known physicist who has long championed this idea.</p>]]></description>
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        <item>
            <title><![CDATA[The ELT Can Probe Ultra-Diffuse Galaxies and Their Dark Matter Mysteries]]></title>
            <link>https://www.universetoday.com/articles/the-elt-can-probe-ultra-diffuse-galaxies-and-their-dark-matter-mysteries</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-elt-can-probe-ultra-diffuse-galaxies-and-their-dark-matter-mysteries</guid>
            <pubDate>Fri, 06 Nov 2026 20:34:10 +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-NGC_1052-DF2_a_ghostly_galaxy_lacking_dark_matter_20261106_190049.jpg" alt="This is NGC 1052-DF2, and Ultra-Diffuse Galaxy. These galaxies have a small number of stars spread over a wide area. Their dark matter halos are puzzling, and UDGs don't seem to follow &quot;regular&quot; galaxy formation models. Studying them could reveal a lot about dark matter halos and the Lambda-CDM model. Image Credit: By ESA/Hubble, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=67837884" width="1280" height="720" /></p><p>Ultra-Diffuse Galaxies are strange because they're as large as the Milky Way, but have far fewer stars. It's as if they're puffed up for some reason. Determining what's going on with them could help confirm the Lambda-CDM model. A new proposed instrument for the Extremely Large Telescope could give astronomers their best look yet at these strange galaxies.</p>]]></description>
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            <title><![CDATA[NASA's Twin Spacecraft Will Execute Powered Slingshot Maneuvers on Their Way to Mars]]></title>
            <link>https://www.universetoday.com/articles/nasas-twin-spacecraft-will-execute-powered-slingshot-maneuvers-on-their-way-to-mars</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/nasas-twin-spacecraft-will-execute-powered-slingshot-maneuvers-on-their-way-to-mars</guid>
            <pubDate>Fri, 06 Nov 2026 16:35:09 +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/8hQwfNsWcwXixNayQBuQy6-750-80_20261106_143237.jpg" alt="NASA's ESCAPADE mission is a pair of identical twin spacecraft that will orbit in formation over Mars. They're about to perform powered slingshot maneuvers around Earth to increase their speed. Once they reach Mars, they'll study how the solar wind interacts with Mars' remnant magnetic fields. Image Credit: NASA." width="1280" height="720" /></p><p>NASA's ESCAPADE mission features a pair of identical spacecraft on their way to Mars. They launched outside of the normal launch window, so they'll perform powered slingshot maneuvers to boost their speed. Once there, they'll "fly" in formation and study how the solar wind interacts with what remains of Mars ancient magnetosphere.</p>]]></description>
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            <title><![CDATA[Earth's Gravity May Have Kept the Early Moon's Volcanic Heart Beating]]></title>
            <link>https://www.universetoday.com/articles/earths-gravity-may-have-kept-the-early-moons-volcanic-heart-beating</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/earths-gravity-may-have-kept-the-early-moons-volcanic-heart-beating</guid>
            <pubDate>Fri, 06 Nov 2026 14:42:30 +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/PIA14011_fig1_20261106_144229.jpg" alt="Image of the volcanic lunar mare from LRO. Credit - NASA Science" width="1280" height="720" /></p><p>We typically think of the Moon as a static, floating object that has remained the same for basically its entire lifetime, with an occasional asteroid impact serving as an exception. That understanding is grounded in physics - the Moon should have cooled rapidly after forming when a huge protoplanet hit the early Earth around 4.5 billion years ago. But, some lunar material returned from the Chang’e-5 mission was notably formed only around two billion years ago, yet appeared to be volcanic in origin. So how did a world that was supposed to have settled down without volcanism remain hot enough to create these materials more than two billion years after its violent birth? A new paper from Miao Chen of the Chengdu University of Technology and his colleagues, and recently published in the journal Planet, offers an explanation - tidal heating.</p>]]></description>
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